1 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed toward the Earth. This orbit is for an extended mission approved by NASA HQ. | |||||||
---|---|---|---|---|---|---|---|---|
2 | The period has been defined as a week before perijove to a week before the subsequent perijove, unlike the mission-planning definition, which extends from a day before the perijove to a day after the perijove. | |||||||
3 | Period: Orbit 76-EXT [GRAV] (2025 Sept 7 - 2025 Oct 6?) | |||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | ||
5 | Observations requested. | |||||||
6 | Observations planned / granted time | |||||||
7 | Observations successful | |||||||
8 | ||||||||
9 | ||||||||
10 | ||||||||
11 | ||||||||
12 | ||||||||
13 | ||||||||
14 | ||||||||
15 | ||||||||
16 | ||||||||
17 | ||||||||
18 | ||||||||
19 | Scheduled observations by Juno. | |||||||
20 | ||||||||
21 | Perijove is approximately 2025 Sept 14 23:42 SCET ( = UTC - light time). System-III longitude = 91.5°W | |||||||
22 | ||||||||
23 | Period: Orbit 76-EXT [GRAV] (2025 Sept 7 - 2025 Oct 6?) | |||||||
24 | Instrument | Description | ||||||
25 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||
26 | MWR | |||||||
27 | UVS | |||||||
28 | JunoCam | |||||||
29 | JIRAM |
1 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed toward the Earth. This orbit is for an extended mission approved by NASA HQ. | |||||||
---|---|---|---|---|---|---|---|---|
2 | The period has been defined as a week before perijove to a week before the subsequent perijove, unlike the mission-planning definition, which extends from a day before the perijove to a day after the perijove. | |||||||
3 | Period: Orbit 75-EXT [GRAV] (2025 August 6 - 2025 Sept 7) | |||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | ||
5 | Observations requested. | |||||||
6 | Observations planned / granted time | |||||||
7 | Observations successful | |||||||
8 | ||||||||
9 | ||||||||
10 | ||||||||
11 | ||||||||
12 | ||||||||
13 | ||||||||
14 | ||||||||
15 | ||||||||
16 | ||||||||
17 | ||||||||
18 | ||||||||
19 | Scheduled observations by Juno. | |||||||
20 | ||||||||
21 | Perijove is approximately 2025 Aug 13 7:06 SCET ( = UTC - light time). System-III longitude = 73.4°W | |||||||
22 | ||||||||
23 | Period: Orbit 75-EXT [GRAV] (2025 August 6 - 2025 Sept 7) | |||||||
24 | Instrument | Description | ||||||
25 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||
26 | MWR | |||||||
27 | UVS | |||||||
28 | JunoCam | |||||||
29 | JIRAM |
1 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed toward the Earth. This orbit is for an extended mission approved by NASA HQ. | |||||||
---|---|---|---|---|---|---|---|---|
2 | The period has been defined as a week before perijove to a week before the subsequent perijove, unlike the mission-planning definition, which extends from a day before the perijove to a day after the perijove. | |||||||
3 | Period: Orbit 74-EXT [GRAV] (2025 July 4 - 2025 August 6) | |||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | ||
5 | Observations requested. | |||||||
6 | Observations planned / granted time | |||||||
7 | Observations successful | |||||||
8 | ||||||||
9 | ||||||||
10 | ||||||||
11 | ||||||||
12 | ||||||||
13 | ||||||||
14 | ||||||||
15 | ||||||||
16 | ||||||||
17 | ||||||||
18 | ||||||||
19 | Scheduled observations by Juno. | |||||||
20 | ||||||||
21 | Perijove is approximately 2025 July 11 13:40 SCET ( = UTC - light time). System-III longitude = 24.5°W | |||||||
22 | ||||||||
23 | Period: Orbit 74-EXT [GRAV] (2025 July 4 - 2025 August 6) | |||||||
24 | Instrument | Description | ||||||
25 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||
26 | MWR | |||||||
27 | UVS | |||||||
28 | JunoCam | |||||||
29 | JIRAM |
1 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed toward the Earth. This orbit is for an extended mission approved by NASA HQ. | |||||||
---|---|---|---|---|---|---|---|---|
2 | The period has been defined as a week before perijove to a week before the subsequent perijove, unlike the mission-planning definition, which extends from a day before the perijove to a day after the perijove. | |||||||
3 | Period: Orbit 73-EXT [GRAV] (2025 June 1 - 2025 July 4) | |||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | ||
5 | Observations requested. | |||||||
6 | Observations planned / granted time | |||||||
7 | Observations successful | |||||||
8 | ||||||||
9 | ||||||||
10 | ||||||||
11 | ||||||||
12 | ||||||||
13 | ||||||||
14 | ||||||||
15 | ||||||||
16 | ||||||||
17 | ||||||||
18 | ||||||||
19 | Scheduled observations by Juno. | |||||||
20 | ||||||||
21 | Perijove is approximately 2025 June 8 20:30 SCET ( = UTC - light time). System-III longitude = 346°W | |||||||
22 | ||||||||
23 | Period: Orbit 73-EXT [GRAV] (2025 June 1 - 2025 July 4) | |||||||
24 | Instrument | Description | ||||||
25 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||
26 | MWR | |||||||
27 | UVS | |||||||
28 | JunoCam | |||||||
29 | JIRAM |
1 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed toward the Earth. This orbit is for an extended mission approved by NASA HQ. | |||||||
---|---|---|---|---|---|---|---|---|
2 | The period has been defined as a week before perijove to a week before the subsequent perijove, unlike the mission-planning definition, which extends from a day before the perijove to a day after the perijove. | |||||||
3 | Period: Orbit 72-EXT [GRAV] (2025 April 30 - 2025 June 1) | |||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | ||
5 | Observations requested. | |||||||
6 | Observations planned / granted time | |||||||
7 | Observations successful | |||||||
8 | ||||||||
9 | ||||||||
10 | ||||||||
11 | ||||||||
12 | ||||||||
13 | ||||||||
14 | ||||||||
15 | ||||||||
16 | ||||||||
17 | ||||||||
18 | ||||||||
19 | Scheduled observations by Juno. | |||||||
20 | ||||||||
21 | Perijove is approximately 2025 May 7 3:01 SCET ( = UTC - light time). System-III longitude = 295.3°W | |||||||
22 | ||||||||
23 | Period: Orbit 72-EXT [GRAV] (2025 April 30 - 2025 June 1) | |||||||
24 | Instrument | Description | ||||||
25 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||
26 | MWR | |||||||
27 | UVS | |||||||
28 | JunoCam | |||||||
29 | JIRAM |
1 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed toward the Earth. This orbit is for an extended mission approved by NASA HQ. | |||||||
---|---|---|---|---|---|---|---|---|
2 | The period has been defined as a week before perijove to a week before the subsequent perijove, unlike the mission-planning definition, which extends from a day before the perijove to a day after the perijove. | |||||||
3 | Period: Orbit 71-EXT [GRAV] (2025 March 28 - 2025 April 30) | |||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | ||
5 | Observations requested. | |||||||
6 | Observations planned / granted time | |||||||
7 | Observations successful | |||||||
8 | ||||||||
9 | ||||||||
10 | ||||||||
11 | ||||||||
12 | ||||||||
13 | ||||||||
14 | ||||||||
15 | ||||||||
16 | ||||||||
17 | ||||||||
18 | ||||||||
19 | Scheduled observations by Juno. | |||||||
20 | ||||||||
21 | Perijove is approximately 2025 April 4 9:30 SCET ( = UTC - light time). System-III longitude =243.9°W | |||||||
22 | ||||||||
23 | Period: Orbit 71-EXT [GRAV] (2025 March 28 - 2025 April 30) | |||||||
24 | Instrument | Description | ||||||
25 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||
26 | MWR | |||||||
27 | UVS | |||||||
28 | JunoCam | |||||||
29 | JIRAM |
1 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed toward the Earth. This orbit is for an extended mission approved by NASA HQ. | |||||||
---|---|---|---|---|---|---|---|---|
2 | The period has been defined as a week before perijove to a week before the subsequent perijove, unlike the mission-planning definition, which extends from a day before the perijove to a day after the perijove. | |||||||
3 | Period: Orbit 70-EXT [GRAV] (2025 Feb 23 - 2025 March 28) | |||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | ||
5 | Observations requested. | |||||||
6 | Observations planned / granted time | |||||||
7 | Observations successful | |||||||
8 | ||||||||
9 | ||||||||
10 | ||||||||
11 | ||||||||
12 | ||||||||
13 | ||||||||
14 | ||||||||
15 | ||||||||
16 | ||||||||
17 | ||||||||
18 | ||||||||
19 | Scheduled observations by Juno. | |||||||
20 | ||||||||
21 | Perijove is approximately 2025 March 2 16:04 SCET ( = UTC - light time). System-III longitude =195°W | |||||||
22 | ||||||||
23 | Period: Orbit 70-EXT [GRAV] (2025 Feb 23 - 2025 March 28) | |||||||
24 | Instrument | Description | ||||||
25 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||
26 | MWR | |||||||
27 | UVS | |||||||
28 | JunoCam | |||||||
29 | JIRAM |
1 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed toward the Earth. This orbit is for an extended mission approved by NASA HQ. | |||||||
---|---|---|---|---|---|---|---|---|
2 | The period has been defined as a week before perijove to a week before the subsequent perijove, unlike the mission-planning definition, which extends from a day before the perijove to a day after the perijove. | |||||||
3 | Period: Orbit 69-EXT [GRAV] (2025 Jan 21 - 2025 Feb 23) | |||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | ||
5 | Observations requested. | |||||||
6 | Observations planned / granted time | |||||||
7 | Observations successful | |||||||
8 | ||||||||
9 | ||||||||
10 | ||||||||
11 | ||||||||
12 | ||||||||
13 | ||||||||
14 | ||||||||
15 | ||||||||
16 | ||||||||
17 | ||||||||
18 | ||||||||
19 | Scheduled observations by Juno. | |||||||
20 | ||||||||
21 | Perijove is approximately 2025 Jan 28 23:05 SCET ( = UTC - light time). System-III longitude =162.4°W | |||||||
22 | ||||||||
23 | Period: Orbit 69-EXT [GRAV] (2025 Jan 21 - 2025 Feb 23) | |||||||
24 | Instrument | Description | ||||||
25 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||
26 | MWR | |||||||
27 | UVS | |||||||
28 | JunoCam | |||||||
29 | JIRAM |
1 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed toward the Earth. This orbit is for an extended mission approved by NASA HQ. | |||||||
---|---|---|---|---|---|---|---|---|
2 | The period has been defined as a week before perijove to a week before the subsequent perijove, unlike the mission-planning definition, which extends from a day before the perijove to a day after the perijove. | |||||||
3 | Period: Orbit 68-EXT [GRAV] (2024 Dec 20 - 2025 Jan 21) | |||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | ||
5 | Observations requested. | |||||||
6 | Observations planned / granted time | |||||||
7 | Observations successful | |||||||
8 | ||||||||
9 | ||||||||
10 | ||||||||
11 | ||||||||
12 | ||||||||
13 | ||||||||
14 | ||||||||
15 | ||||||||
16 | ||||||||
17 | ||||||||
18 | ||||||||
19 | Scheduled observations by Juno. | |||||||
20 | ||||||||
21 | Perijove is approximately 2024 Dec 27 5:22 SCET ( = UTC - light time). System-III longitude =103.6°W | |||||||
22 | ||||||||
23 | Period: Orbit 68-EXT [GRAV] (2024 Dec 20 - 2025 Jan 21) | |||||||
24 | Instrument | Description | ||||||
25 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||
26 | MWR | |||||||
27 | UVS | |||||||
28 | JunoCam | |||||||
29 | JIRAM |
1 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed toward the Earth. This orbit is for an extended mission approved by NASA HQ. | |||||||
---|---|---|---|---|---|---|---|---|
2 | The period has been defined as a week before perijove to a week before the subsequent perijove, unlike the mission-planning definition, which extends from a day before the perijove to a day after the perijove. | |||||||
3 | Period: Orbit 67-EXT [GRAV] (2024 Nov 17 - 2024 Dec 20) | |||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | ||
5 | Observations requested. | |||||||
6 | Observations planned / granted time | |||||||
7 | Observations successful | |||||||
8 | ||||||||
9 | ||||||||
10 | ||||||||
11 | ||||||||
12 | ||||||||
13 | ||||||||
14 | ||||||||
15 | ||||||||
16 | ||||||||
17 | ||||||||
18 | ||||||||
19 | Scheduled observations by Juno. | |||||||
20 | ||||||||
21 | Perijove is approximately 2024 Nov 24 13:05 SCET ( = UTC - light time). System-III longitude = 96.5°W | |||||||
22 | ||||||||
23 | Period: Orbit 67-EXT [GRAV] (2024 Nov 17 - 2024 Dec 20) | |||||||
24 | Instrument | Description | ||||||
25 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||
26 | MWR | |||||||
27 | UVS | |||||||
28 | JunoCam | |||||||
29 | JIRAM |
1 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed toward the Earth. This orbit is for an extended mission approved by NASA HQ. | |||||||
---|---|---|---|---|---|---|---|---|
2 | The period has been defined as a week before perijove to a week before the subsequent perijove, unlike the mission-planning definition, which extends from a day before the perijove to a day after the perijove. | |||||||
3 | Period: Orbit 66-EXT [GRAV] (2024 Oct 15 - 2024 Nov 17) | |||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | ||
5 | Observations requested. | |||||||
6 | Observations planned / granted time | |||||||
7 | Observations successful | |||||||
8 | ||||||||
9 | ||||||||
10 | ||||||||
11 | ||||||||
12 | ||||||||
13 | ||||||||
14 | ||||||||
15 | ||||||||
16 | ||||||||
17 | ||||||||
18 | ||||||||
19 | Scheduled observations by Juno. | |||||||
20 | ||||||||
21 | Perijove is approximately 2024 October 22 18:10 SCET ( = UTC - light time). System-III longitude = 354.3°W | |||||||
22 | ||||||||
23 | Period: Orbit 66-EXT [GRAV] (2024 Oct 16 - 2024 Nov 18) | |||||||
24 | Instrument | Description | ||||||
25 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||
26 | MWR | |||||||
27 | UVS | |||||||
28 | JunoCam | |||||||
29 | JIRAM |
1 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed toward the Earth. This orbit is for an extended mission approved by NASA HQ. | |||||||
---|---|---|---|---|---|---|---|---|
2 | The period has been defined as a week before perijove to a week before the subsequent perijove, unlike the mission-planning definition, which extends from a day before the perijove to a day after the perijove. | |||||||
3 | Period: Orbit 65-EXT [GRAV] (2024 Sept 13 - 2024 Oct 15) | |||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | ||
5 | mid IR | Fletcher | VLT / VISIR | Filtered radiometric imaging to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology. | Available in raw form in the ESO archive within 24 hours of acquisition; cylindrical maps within 1-2 days and reduced maps within a week. | Observations requested. | ||
6 | near-IR | Dahl | IRTF/SpeX | Imaging and scanning spectroscopy between 1.58 and 5.1 µm | Requested dates +/-3 days from PJ date | Before being archived, available upon request | Observations planned / granted time | |
7 | Observations successful | |||||||
8 | ||||||||
9 | ||||||||
10 | ||||||||
11 | ||||||||
12 | ||||||||
13 | ||||||||
14 | ||||||||
15 | ||||||||
16 | ||||||||
17 | ||||||||
18 | ||||||||
19 | Scheduled observations by Juno. | |||||||
20 | ||||||||
21 | Perijove is approximately 2024 September 20 2:28 SCET ( = UTC - light time). System-III longitude = 8.3°W | |||||||
22 | ||||||||
23 | Period: Orbit 65-EXT [GRAV] (2024 Sept 13 - 2024 Oct 16) | |||||||
24 | Instrument | Description | ||||||
25 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||
26 | MWR | |||||||
27 | UVS | |||||||
28 | JunoCam | |||||||
29 | JIRAM |
1 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed toward the Earth. This orbit is for an extended mission approved by NASA HQ. | |||||||
---|---|---|---|---|---|---|---|---|
2 | The period has been defined as a week before perijove to a week before the subsequent perijove, unlike the mission-planning definition, which extends from a day before the perijove to a day after the perijove. | |||||||
3 | Period: Orbit 64-EXT [GRAV] (2024 Aug 11 - 2024 Sept 13) | |||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | ||
5 | mid IR | Fletcher | VLT / VISIR | Filtered radiometric imaging to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology. | Available in raw form in the ESO archive within 24 hours of acquisition; cylindrical maps within 1-2 days and reduced maps within a week. | Observations requested. | ||
6 | near-IR | Dahl | IRTF/SpeX | Imaging and scanning spectroscopy between 1.58 and 5.1 µm | Requested dates +/-3 days from PJ date | Before being archived, available upon request | Observations planned / granted time | |
7 | Observations successful | |||||||
8 | ||||||||
9 | ||||||||
10 | ||||||||
11 | ||||||||
12 | ||||||||
13 | ||||||||
14 | ||||||||
15 | ||||||||
16 | ||||||||
17 | ||||||||
18 | ||||||||
19 | Scheduled observations by Juno. | |||||||
20 | ||||||||
21 | Perijove is approximately 2024 August 18 6:57 SCET ( = UTC - light time). System-III longitude = 243.4°W | |||||||
22 | ||||||||
23 | Period: Orbit 64-EXT [GRAV] (2024 Aug 11 - 2024 Sept 13) | |||||||
24 | Instrument | Description | ||||||
25 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||
26 | MWR | |||||||
27 | UVS | |||||||
28 | JunoCam | |||||||
29 | JIRAM |
1 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed toward the Earth. This orbit is for an extended mission approved by NASA HQ. | |||||||
---|---|---|---|---|---|---|---|---|
2 | The period has been defined as a week before perijove to a week before the subsequent perijove, unlike the mission-planning definition, which extends from a day before the perijove to a day after the perijove. | |||||||
3 | Period: Orbit 63-EXT [GRAV] (2024 July 9 - 2024 Aug 11) | |||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | ||
5 | near-IR | Dahl | IRTF/SpeX | Imaging and scanning spectroscopy between 1.58 and 5.1 µm | Requested dates +/-3 days from PJ date | Before being archived, available upon request | Observations requested. | |
6 | near-IR | Orton | Palomar/PHARO | near-iR imaging with AO stabilization | second half of the night on July 29 and 30 | Observations planned / granted time | ||
7 | mid IR | Fletcher | VLT / VISIR | Filtered radiometric imaging to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology. | Available in raw form in the ESO archive within 24 hours of acquisition; cylindrical maps within 1-2 days and reduced maps within a week. | Observations successful | ||
8 | mid IR | Orton | IRTF/MIRSI | mid-IR imaing with refurbished detector array | July 17-18 | Availale on request | ||
9 | ||||||||
10 | ||||||||
11 | ||||||||
12 | ||||||||
13 | ||||||||
14 | ||||||||
15 | ||||||||
16 | ||||||||
17 | ||||||||
18 | ||||||||
19 | Scheduled observations by Juno. | |||||||
20 | ||||||||
21 | Perijove is approximately2024 July 16 14:33 SCET ( = UTC - light time). System-III longitude = 232°W | |||||||
22 | ||||||||
23 | Period: Orbit 63-EXT [GRAV] (2024 July 10 - 2024 Aug 11) | |||||||
24 | Instrument | Description | ||||||
25 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||
26 | MWR | |||||||
27 | UVS | |||||||
28 | JunoCam | |||||||
29 | JIRAM |
1 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed toward the Earth. This orbit is for an extended mission approved by NASA HQ. | |||||||||
---|---|---|---|---|---|---|---|---|---|---|
2 | The period has been defined as a week before perijove to a week before the subsequent perijove, unlike the mission-planning definition, which extends from a day before the perijove to a day after the perijove. | |||||||||
3 | Period: Orbit 62-EXT [GRAV] (2024 June 6 - 2024 July 9) | Observations requested. | ||||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | Observations planned / granted time | |||
5 | ||||||||||
6 | Observations successful | |||||||||
7 | ||||||||||
8 | ||||||||||
9 | ||||||||||
10 | ||||||||||
11 | ||||||||||
12 | ||||||||||
13 | ||||||||||
14 | ||||||||||
15 | ||||||||||
16 | ||||||||||
17 | ||||||||||
18 | ||||||||||
19 | Scheduled observations by Juno. | |||||||||
20 | ||||||||||
21 | Perijove is approximately 2024 June 13 19:53 SCET ( = UTC - light time). System-III longitude = 139°W | |||||||||
22 | ||||||||||
23 | Period: Orbit 62-EXT [GRAV] (2024 June 7 - 2024 July 10) | |||||||||
24 | Instrument | Description | ||||||||
25 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||
26 | MWR | |||||||||
27 | UVS | |||||||||
28 | JunoCam | |||||||||
29 | JIRAM |
1 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed toward the Earth. This orbit is for an extended mission approved by NASA HQ. | |||||||||
---|---|---|---|---|---|---|---|---|---|---|
2 | The period has been defined as a week before perijove to a week before the subsequent perijove, unlike the mission-planning definition, which extends from a day before the perijove to a day after the perijove. | |||||||||
3 | Period: Orbit 61-EXT [GRAV] (2024 May 5 - 2024 June 6) | Observations requested. | ||||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | Observations planned / granted time | |||
5 | ||||||||||
6 | Observations successful | |||||||||
7 | ||||||||||
8 | ||||||||||
9 | ||||||||||
10 | ||||||||||
11 | ||||||||||
12 | ||||||||||
13 | ||||||||||
14 | ||||||||||
15 | ||||||||||
16 | ||||||||||
17 | ||||||||||
18 | ||||||||||
19 | Scheduled observations by Juno. | |||||||||
20 | ||||||||||
21 | Perijove is approximately 2024 May 12 3:38 SCET ( = UTC - light time). System-III longitude = 132.8 °W | |||||||||
22 | ||||||||||
23 | Period: Orbit 61-EXT [GRAV] (2024 May 5 - 2024 June 7) | |||||||||
24 | Instrument | Description | ||||||||
25 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||
26 | MWR | |||||||||
27 | UVS | |||||||||
28 | JunoCam | |||||||||
29 | JIRAM |
1 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed toward the Earth. This orbit is for an extended mission approved by NASA HQ. | |||||||||
---|---|---|---|---|---|---|---|---|---|---|
2 | The period has been defined as a week before perijove to a week before the subsequent perijove, unlike the mission-planning definition, which extends from a day before the perijove to a day after the perijove. | |||||||||
3 | Period: Orbit 60-EXT [GRAV] (2024 April 2 - 2024 May 5) | Observations requested. | ||||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | Observations planned / granted time | |||
5 | near-IR | Dahl | IRTF/SpeX | Imaging and scanning spectroscopy between 1.58 and 5.1 µm | Requested dates +/-3 days from PJ date | Before being archived, available upon request | ||||
6 | Observations successful | |||||||||
7 | ||||||||||
8 | ||||||||||
9 | ||||||||||
10 | ||||||||||
11 | ||||||||||
12 | ||||||||||
13 | ||||||||||
14 | ||||||||||
15 | ||||||||||
16 | ||||||||||
17 | ||||||||||
18 | ||||||||||
19 | Scheduled observations by Juno. | |||||||||
20 | ||||||||||
21 | Perijove is approximately 2024 April 9 8:48 SCET ( = UTC - light time). System-III longitude = 32.9°W | |||||||||
22 | ||||||||||
23 | Period: Orbit 60-EXT [GRAV] (2024 April 2 - 2024 May 5) | |||||||||
24 | Instrument | Description | ||||||||
25 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||
26 | MWR | |||||||||
27 | UVS | |||||||||
28 | JunoCam | |||||||||
29 | JIRAM |
1 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed toward the Earth. This orbit is for an extended mission approved by NASA HQ. | |||||||||
---|---|---|---|---|---|---|---|---|---|---|
2 | The period has been defined as a week before perijove to a week before the subsequent perijove, unlike the mission-planning definition, which extends from a day before the perijove to a day after the perijove. | |||||||||
3 | Period: Orbit 59-EXT [GRAV] (2024 Feb 29 - 2024 April 2) | Observations requested. | ||||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | Observations planned / granted time | |||
5 | near-IR | Dahl | IRTF/SpeX | Imaging and scanning spectroscopy between 1.58 and 5.1 µm | Requested dates +/-3 days from PJ date | Before being archived, available upon request | ||||
6 | Observations successful | |||||||||
7 | ||||||||||
8 | ||||||||||
9 | ||||||||||
10 | ||||||||||
11 | ||||||||||
12 | ||||||||||
13 | ||||||||||
14 | ||||||||||
15 | ||||||||||
16 | ||||||||||
17 | ||||||||||
18 | ||||||||||
19 | Scheduled observations by Juno. | |||||||||
20 | ||||||||||
21 | Perijove is approximately 2024 March 7 15:42 SCET ( = UTC - light time). System-III longitude = 32.9°W | |||||||||
22 | ||||||||||
23 | Period: Orbit 59-EXT [GRAV] (2024 Feb 29 - 2024 April 2) | |||||||||
24 | Instrument | Description | ||||||||
25 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||
26 | MWR | |||||||||
27 | UVS | |||||||||
28 | JunoCam | |||||||||
29 | JIRAM |
1 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed toward the Earth. This orbit is for an extended mission approved by NASA HQ. | |||||||||
---|---|---|---|---|---|---|---|---|---|---|
2 | The period has been defined as a week before perijove to a week before the subsequent perijove, unlike the mission-planning definition, which extends from a day before the perijove to a day after the perijove. | |||||||||
3 | Period: Orbit 58-EXT [GRAV] (2024 Jan 27 - 2024 Feb 29) | Observations requested. | ||||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | Observations planned / granted time | |||
5 | ||||||||||
6 | FUV | Retherford & Bagenal | Hubble+JWST | Large Program 17470: https://www.stsci.edu/cgi-bin/get-visit-status?id=17470&markupFormat=html&observatory=HST | Io Aurora: 1/31/2024 6:49:41, Feb 1, 2024 06:33:31, Feb 2, 2024 06:17:23. Io Surface: Feb 17, 2024 07:05:33 | Immediately | ||||
7 | ||||||||||
8 | visible/NUV/ near-IR | Wong (17275) | Hubble/ WFC3-UVIS | hi-resolution non-global snapshot | 2024 Feb 3 planned | Observations successful | ||||
9 | near-IR | Dahl | IRTF/SpeX | Imaging and scanning spectroscopy between 1.58 and 5.1 µm | First half of night on Feb. 4, 5 UT. Photmetric sky conditions. | Before being archived, available upon request | ||||
10 | near-IR | Orton | Keck-2/NIRC2 | near-IR imaging with AO stabilization | First quarter of the night on Feb 4 and 5. Some instabilithy in AO system and telescope control on Feb 4, obtaining only half of disk; Feb 5 was mostly successful | Available on request | ||||
11 | near-IR | Orton | Palomar/PHARO | near-iR imaging with AO stabilization | First half of the night on Feb 11 and 12 was schedled. Feb 11 lost fo melting snow on dome, most of Feb 12 half night was successful; AO was possible using Galilean satellites as wavefront sensors / "natural guide stars" | Available on request | ||||
12 | mid-IR | Orton | IRTF/MIRSI | mid-IR imaing with refurbished detector array | First half of the night on Feb 1 and 2. Very good data with photometric sky conditions. | Available on request | ||||
13 | ||||||||||
14 | ||||||||||
15 | ||||||||||
16 | ||||||||||
17 | ||||||||||
18 | ||||||||||
19 | Scheduled observations by Juno. | |||||||||
20 | ||||||||||
21 | Perijove is approximately 2024 February 3, 21:47 SCET ( = UTC - light time). System-III longitude = 290 °W | |||||||||
22 | ||||||||||
23 | Period: Orbit 58-EXT [GRAV] (2024 Jan 27 - 2024 Feb 29) | |||||||||
24 | Instrument | Description | ||||||||
25 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||
26 | MWR | |||||||||
27 | UVS | |||||||||
28 | JunoCam | |||||||||
29 | JIRAM | |||||||||
30 | SRU | Two images on Jupiter's nightside, 2024 Feb 3. At 21:42:36 61.3N, 281.4W, and at 22:07:37 1.2N, 315.6W |
1 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed toward the Earth. This orbit is for an extended mission approved by NASA HQ. | |||||||||
---|---|---|---|---|---|---|---|---|---|---|
2 | The period has been defined as a week before perijove to a week before the subsequent perijove, unlike the mission-planning definition, which extends from a day before the perijove to a day after the perijove. | |||||||||
3 | Period: Orbit 57-EXT [GRAV] (2023 Dec 24 - 2024 Jan 27) | Observations requested. | ||||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | Observations planned / granted time | |||
5 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | Nightly, weather permitting | https://doi.org/10.5281/zenodo.8342758 see also https://arxiv.org/abs/2403.03131 | ||||
6 | radio | Zarka, Cecconi, Lamy, Louis | Nançay Decameter Array (France) | coordinated measurement of 10-40 MHz cyclotron radio emission | every day, 8 hours around the transition to local meridian | https://maser.lesia.obspm.fr/task-1-data-collections/juno-ground-radio/juno-ground-radio-nancay-decameter.html?lang=en | Observations successful | |||
7 | Visible | Retherford & Bagenal | Hubble+JWST | Large Program 17470: https://www.stsci.edu/cgi-bin/get-visit-status?id=17470&markupFormat=html&observatory=HST | Io Surface Image Cube: Jan 15, 2024 07:57:37 | Immediately | ||||
8 | visible/NUV/ near-IR | Simon (17495) | Hubble/ WFC3-UVIS | two hi-resolution non-global snapshots over consecutive Jupiter rotations | 2023 Dec 27 and 28 planned | |||||
9 | near-IR | Dahl | IRTF/SpeX | Imaging and scanning spectroscopy between 1.58 and 5.1 µm | Dec 27 and 28 in photmetric skies and good to excellent seeing conditions | |||||
10 | near IR | Bjoraker | IRTF/iSHELL | 5 micron spectra | requested near Dec 29 | later | ||||
11 | mid-infrared | Orton | TEXES | global mapping, medium and low resolution spectroscopy | requested near Dec 31 | |||||
12 | mid-infrared | Sinclair | TEXES | mapping of auroral and non-auroral regions for temperature and chemsiry | requested near Dec - Jan | |||||
13 | mid-IR | Fletcher | VISIR | Filtered imaging and M-band lucky imaging | Near PJ | Upon request | ||||
14 | ||||||||||
15 | ||||||||||
16 | ||||||||||
17 | ||||||||||
18 | ||||||||||
19 | ||||||||||
20 | ||||||||||
21 | Scheduled observations by Juno. | |||||||||
22 | ||||||||||
23 | Perijove is approximately 2023 Dec 30, 12:36 SCET ( = UTC - light time). System-III longitude = 89°W | |||||||||
24 | ||||||||||
25 | Period: Orbit 57-EXT [GRAV] (2023 Dec 24 - 2024 Jan 27) | |||||||||
26 | Instrument | Description | ||||||||
27 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||
28 | MWR | |||||||||
29 | UVS | |||||||||
30 | JunoCam | |||||||||
31 | JIRAM | |||||||||
32 | ||||||||||
33 | ||||||||||
34 | ||||||||||
35 | ||||||||||
36 | ||||||||||
37 | ||||||||||
38 | ||||||||||
39 | ||||||||||
40 | ||||||||||
41 | ||||||||||
42 | ||||||||||
43 | ||||||||||
44 | ||||||||||
45 | ||||||||||
46 | ||||||||||
47 | ||||||||||
48 | ||||||||||
49 | ||||||||||
50 | ||||||||||
51 | ||||||||||
52 | ||||||||||
53 | ||||||||||
54 | ||||||||||
55 | Composite RGB global map from inbound JunoCam images, assembled by Gerald Eichstaedt, without labelled features. | |||||||||
56 | ||||||||||
57 | ||||||||||
58 | ||||||||||
59 | ||||||||||
60 | ||||||||||
61 | ||||||||||
62 | ||||||||||
63 | ||||||||||
64 | ||||||||||
65 | ||||||||||
66 | ||||||||||
67 | ||||||||||
68 | ||||||||||
69 | ||||||||||
70 | ||||||||||
71 | ||||||||||
72 | ||||||||||
73 | ||||||||||
74 | ||||||||||
75 | ||||||||||
76 | ||||||||||
77 | ||||||||||
78 | ||||||||||
79 | ||||||||||
80 | ||||||||||
81 | ||||||||||
82 | ||||||||||
83 | ||||||||||
84 | ||||||||||
85 | ||||||||||
86 | ||||||||||
87 | ||||||||||
88 | ||||||||||
89 | ||||||||||
90 | ||||||||||
91 | ||||||||||
92 | ||||||||||
93 | ||||||||||
94 | ||||||||||
95 | ||||||||||
96 | ||||||||||
97 | ||||||||||
98 | ||||||||||
99 | ||||||||||
100 | ||||||||||
101 | ||||||||||
102 | ||||||||||
103 | ||||||||||
104 | ||||||||||
105 | ||||||||||
106 | ||||||||||
107 | ||||||||||
108 | ||||||||||
109 | ||||||||||
110 | ||||||||||
111 | MWR footprints for the minimum emission angle at each spacecraft rotation +-40 minutes from perijove. The cross marks the location of the perijove. | |||||||||
112 | ||||||||||
113 |
1 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed toward the Earth. This orbit is for an extended mission approved by NASA HQ. | |||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|
2 | The period has been defined as a week before perijove to a week before the subsequent perijove, unlike the mission-planning definition, which extends from a day before the perijove to a day after the perijove. | |||||||||||
3 | Period: Orbit 56-EXT [GRAV] (2023 Nov 16 - Dec 23) | Observations requested. | ||||||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | Observations planned / granted time | |||||
5 | visible/NUV/ near-IR | Simon (16995) | Hubble/ WFC3-UVIS | two consecutive hi-resolution global maps | 2023 Nov 22 planned | https://archive.stsci.edu/prepds/opal/ https://doi.org/10.1016/j.icarus.2022.114994 | ||||||
6 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | Nightly, weather permitting | https://doi.org/10.5281/zenodo.8342758 see also https://arxiv.org/abs/2403.03131 | ||||||
7 | radio | Zarka, Cecconi, Lamy, Louis | Nançay Decameter Array (France) | coordinated measurement of 10-40 MHz cyclotron radio emission | every day, 8 hours around the transition to local meridian | https://maser.lesia.obspm.fr/task-1-data-collections/juno-ground-radio/juno-ground-radio-nancay-decameter.html?lang=en | Observations successful | |||||
8 | near-IR | Dahl | IRTF/SpeX | Imaging and scanning spectroscopy between 1.58 and 5.1 µm | ||||||||
9 | near IR | Bjoraker | IRTF/iSHELL | 5 micron spectra | requested near Nov 20-23 | later | ||||||
10 | mid-IR | Fletcher | VISIR | Filtered imaging and M-band lucky imaging | Near PJ | Upon request | ||||||
11 | ||||||||||||
12 | ||||||||||||
13 | ||||||||||||
14 | ||||||||||||
15 | ||||||||||||
16 | ||||||||||||
17 | ||||||||||||
18 | ||||||||||||
19 | Scheduled observations by Juno. | |||||||||||
20 | ||||||||||||
21 | Perijove is appoximately 2023 Nov 22, 12:17 SCET ( = UTC - light time). System-III longitude = 117°W | |||||||||||
22 | ||||||||||||
23 | Period: Orbit 56-EXT [GRAV] (2023 Nov 16 - Dec 23) | |||||||||||
24 | Instrument | Description | ||||||||||
25 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||||
26 | MWR | |||||||||||
27 | UVS | |||||||||||
28 | JunoCam | |||||||||||
29 | JIRAM | |||||||||||
30 | ||||||||||||
31 | ||||||||||||
32 | ||||||||||||
33 | ||||||||||||
34 | ||||||||||||
35 | ||||||||||||
36 | ||||||||||||
37 | ||||||||||||
38 | ||||||||||||
39 | ||||||||||||
40 | ||||||||||||
41 | ||||||||||||
42 | ||||||||||||
43 | ||||||||||||
44 | ||||||||||||
45 | ||||||||||||
46 | ||||||||||||
47 | ||||||||||||
48 | ||||||||||||
49 | ||||||||||||
50 | ||||||||||||
51 | ||||||||||||
52 | ||||||||||||
53 | ||||||||||||
54 | Composite RGB global map from JunoCam images, assembled by John Rogers and Gerald Eichstaedt, without labelled features. | |||||||||||
55 | ||||||||||||
56 | ||||||||||||
57 | ||||||||||||
58 | ||||||||||||
59 | ||||||||||||
60 | ||||||||||||
61 | ||||||||||||
62 | ||||||||||||
63 | ||||||||||||
64 | ||||||||||||
65 | ||||||||||||
66 | ||||||||||||
67 | ||||||||||||
68 | ||||||||||||
69 | ||||||||||||
70 | ||||||||||||
71 | ||||||||||||
72 | ||||||||||||
73 | ||||||||||||
74 | ||||||||||||
75 | ||||||||||||
76 | ||||||||||||
77 | ||||||||||||
78 | ||||||||||||
79 | ||||||||||||
80 | ||||||||||||
81 | ||||||||||||
82 | ||||||||||||
83 | ||||||||||||
84 | ||||||||||||
85 | ||||||||||||
86 | ||||||||||||
87 | ||||||||||||
88 | ||||||||||||
89 | ||||||||||||
90 | ||||||||||||
91 | ||||||||||||
92 | ||||||||||||
93 | ||||||||||||
94 | ||||||||||||
95 | ||||||||||||
96 | ||||||||||||
97 | ||||||||||||
98 | ||||||||||||
99 | ||||||||||||
100 | ||||||||||||
101 | ||||||||||||
102 | ||||||||||||
103 | ||||||||||||
104 | ||||||||||||
105 | ||||||||||||
106 | ||||||||||||
107 | ||||||||||||
108 | ||||||||||||
109 | ||||||||||||
110 | MWR footprints for the minimum emission angle at each spacecraft rotation +-40 minutes from perijove. The cross marks the location of the perijove. | |||||||||||
111 | ||||||||||||
112 |
1 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed toward the Earth. This orbit is for an extended mission approved by NASA HQ. | ||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|
2 | The period has been defined as a week before perijove to a week before the subsequent perijove, unlike the mission-planning definition, which extends from a day before the perijove to a day after the perijove. | ||||||||||||
3 | Period: Orbit 55-EXT [GRAV] (2023 Oct 9 - Nov15) | Observations requested. | |||||||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | Observations planned / granted time | ||||||
5 | visible/NUV/ near-IR | Wong (17275) | Hubble/ WFC3-UVIS | hi-resolution non-global snapshot | 2023 Oct 13 | future: https://archive.stsci.edu/hlsp/wfcj | |||||||
6 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | Nightly, weather permitting | https://doi.org/10.5281/zenodo.8342758 see also https://arxiv.org/abs/2403.03131 | |||||||
7 | near-IR | Dahl | IRTF/SpeX | Imaging and scanning spectroscopy between 1.58 and 5.1 µm | Oct 14-15. One of best nights ever. Totally photometric weather and seeing typially at 0.4-0.6". | ||||||||
8 | near IR | Bjoraker | IRTF/iSHELL | 5 micron spectra | Oct 16 | later | |||||||
9 | mid-infrared | Orton | TEXES | global mapping, medium and low resolution spectroscopy | About 4.5 hours on Oct 1-2 during bad weather, with 1.5 hours of very good observing on Oct 7. | ||||||||
10 | radio | Zarka, Cecconi, Lamy, Louis | Nançay Decameter Array (France) | coordinated measurement of 10-40 MHz cyclotron radio emission | every day, 8 hours around the transition to local meridian | https://maser.lesia.obspm.fr/task-1-data-collections/juno-ground-radio/juno-ground-radio-nancay-decameter.html?lang=en | |||||||
11 | mid-IR | Fletcher | VISIR | Filtered imaging and M-band lucky imaging | Near PJ | Upon request | |||||||
12 | Radio (mm/sub-mm) | Tseng | SMA | Ground-based radio observations of Io around 335-367GHz | requested 3 tracks from Sep to Oct | Collaboration is possible with the investigators. | |||||||
13 | |||||||||||||
14 | |||||||||||||
15 | |||||||||||||
16 | |||||||||||||
17 | |||||||||||||
18 | |||||||||||||
19 | Scheduled observations by Juno. | ||||||||||||
20 | |||||||||||||
21 | Perijove is approximately 2023 Oct 15, 10:53 SCET ( = UTC - light time). System-III longitude = 107°W | ||||||||||||
22 | |||||||||||||
23 | Period: Orbit 55-EXT [GRAV] (2023 Oct 9 - Nov15) | ||||||||||||
24 | Instrument | Description | |||||||||||
25 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | |||||||||||
26 | MWR | ||||||||||||
27 | UVS | ||||||||||||
28 | JunoCam | ||||||||||||
29 | JIRAM | ||||||||||||
30 | |||||||||||||
31 | |||||||||||||
32 | |||||||||||||
33 | |||||||||||||
34 | |||||||||||||
35 | |||||||||||||
36 | |||||||||||||
37 | |||||||||||||
38 | |||||||||||||
39 | |||||||||||||
40 | |||||||||||||
41 | |||||||||||||
42 | |||||||||||||
43 | |||||||||||||
44 | |||||||||||||
45 | |||||||||||||
46 | |||||||||||||
47 | |||||||||||||
48 | |||||||||||||
49 | |||||||||||||
50 | |||||||||||||
51 | |||||||||||||
52 | |||||||||||||
53 | |||||||||||||
54 | |||||||||||||
55 | |||||||||||||
56 | Composite RGB global map from JunoCam images, assembled by John Rogers and Gerald Eichstaedt, with various features labelled. | ||||||||||||
57 | |||||||||||||
58 | |||||||||||||
59 | |||||||||||||
60 | |||||||||||||
61 | |||||||||||||
62 | |||||||||||||
63 | |||||||||||||
64 | |||||||||||||
65 | |||||||||||||
66 | |||||||||||||
67 | |||||||||||||
68 | |||||||||||||
69 | |||||||||||||
70 | |||||||||||||
71 | |||||||||||||
72 | |||||||||||||
73 | |||||||||||||
74 | |||||||||||||
75 | |||||||||||||
76 | |||||||||||||
77 | |||||||||||||
78 | |||||||||||||
79 | |||||||||||||
80 | |||||||||||||
81 | |||||||||||||
82 | |||||||||||||
83 | |||||||||||||
84 | |||||||||||||
85 | |||||||||||||
86 | |||||||||||||
87 | |||||||||||||
88 | Composite RGB global map from ground-based images, assembled by Andy Casely, with various features labelled by John Rogers | ||||||||||||
89 | |||||||||||||
90 | |||||||||||||
91 | |||||||||||||
92 | |||||||||||||
93 | |||||||||||||
94 | |||||||||||||
95 | |||||||||||||
96 | |||||||||||||
97 | |||||||||||||
98 | |||||||||||||
99 | |||||||||||||
100 | |||||||||||||
101 | |||||||||||||
102 | |||||||||||||
103 | |||||||||||||
104 | |||||||||||||
105 | |||||||||||||
106 | |||||||||||||
107 | |||||||||||||
108 | |||||||||||||
109 | |||||||||||||
110 | |||||||||||||
111 | |||||||||||||
112 | |||||||||||||
113 | |||||||||||||
114 | |||||||||||||
115 | |||||||||||||
116 | |||||||||||||
117 | |||||||||||||
118 | |||||||||||||
119 | |||||||||||||
120 | |||||||||||||
121 | |||||||||||||
122 | |||||||||||||
123 | |||||||||||||
124 | |||||||||||||
125 | |||||||||||||
126 | |||||||||||||
127 | |||||||||||||
128 | |||||||||||||
129 | |||||||||||||
130 | |||||||||||||
131 | |||||||||||||
132 | |||||||||||||
133 | |||||||||||||
134 | |||||||||||||
135 | |||||||||||||
136 | |||||||||||||
137 | |||||||||||||
138 | |||||||||||||
139 | |||||||||||||
140 | MWR footprints for the minimum emission angle at each spacecraft rotation +-40 minutes from perijove. The cross marks the location of the perijove. | ||||||||||||
141 |
1 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed toward the Earth. This orbit is for an extended mission approved by NASA HQ. | |||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|
2 | The period has been defined as a week before perijove to a week before the subsequent perijove, unlike the mission-planning definition, which extends from a day before the perijove to a day after the perijove. | |||||||||||
3 | Period: Orbit 54-EXT [GRAV] (2023 Sep 1 - Oct 8) | Observations requested. | ||||||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | Observations planned / granted time | |||||
5 | visible/NUV/ near-IR | Wong (17275) | Hubble/ WFC3-UVIS | hi-resolution near-global map | 2023 Sept 9 | now: https://mast.stsci.edu/search/ui/#/hst/results?&proposal_id=16913 https://doi.org/10.3847/1538-4365/ab775f future: https://archive.stsci.edu/hlsp/wfcj | ||||||
6 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | Nightly, weather permitting | https://doi.org/10.5281/zenodo.8342758 see also https://arxiv.org/abs/2403.03131 | ||||||
7 | visible/nearIR | Alexander, Irwin | VLT/MUSE - IFU | spectroscopic imaging, 475-930 nm to determine cloud structure and albedo spectrum of particles. | Observations successful | |||||||
8 | near-IR | Stallard | JWST/NIRSPEC | spectroscopic IFU imaging between 3-5 micron, mapping the entire planetary limb | Requested 7 Sept, current range is 7-11 September | Propriatory period 12 months. Collaboration is possible with the investigators. | ||||||
9 | Near-IR | Schmit | Keck/NIRSpec | spectral slit scans, supporting regions covered by JWST and Juno occultations | 7 September | Propriatory period 6 months. Collaboration is possible with the investigators. | ||||||
10 | Near-IR | Knowles | IRTF/iSHELL | Spectral scans across the disk at Lp4 (3.8-4.1 micron) | One scan every two days for a month before September 6 | |||||||
11 | Radio (mm/sub-mm) | Tseng | SMA | Ground-based radio observations of Io around 335-367GHz | requested 3 tracks from Sep to Oct | Collaboration is possible with the investigators. | ||||||
12 | radio | Zarka, Cecconi, Lamy, Louis | Nançay Decameter Array (France) | coordinated measurement of 10-40 MHz cyclotron radio emission | every day, 8 hours around the transition to local meridian | https://maser.lesia.obspm.fr/task-1-data-collections/juno-ground-radio/juno-ground-radio-nancay-decameter.html?lang=en | ||||||
13 | ||||||||||||
14 | ||||||||||||
15 | Scheduled observations by Juno. | |||||||||||
16 | ||||||||||||
17 | Perijove is approximately 2023 Sep 7, 11:58 SCET ( = UTC - light time). System-III longitude = 186°W | |||||||||||
18 | ||||||||||||
19 | Period: Orbit 54-EXT [GRAV] (2023 Sep 1 - Oct 8) | |||||||||||
20 | Instrument | Description | ||||||||||
21 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||||
22 | MWR | |||||||||||
23 | UVS | |||||||||||
24 | JunoCam | |||||||||||
25 | JIRAM | |||||||||||
26 | ||||||||||||
27 | ||||||||||||
28 | ||||||||||||
29 | ||||||||||||
30 | ||||||||||||
31 | ||||||||||||
32 | ||||||||||||
33 | ||||||||||||
34 | ||||||||||||
35 | ||||||||||||
36 | ||||||||||||
37 | ||||||||||||
38 | ||||||||||||
39 | ||||||||||||
40 | ||||||||||||
41 | ||||||||||||
42 | ||||||||||||
43 | ||||||||||||
44 | ||||||||||||
45 | ||||||||||||
46 | ||||||||||||
47 | ||||||||||||
48 | ||||||||||||
49 | ||||||||||||
50 | ||||||||||||
51 | ||||||||||||
52 | Composite RGB global map from JunoCam images, assembled by John Rogers and Gerald Eichstaedt, with various features labelled. | |||||||||||
53 | ||||||||||||
54 | ||||||||||||
55 | ||||||||||||
56 | ||||||||||||
57 | ||||||||||||
58 | ||||||||||||
59 | ||||||||||||
60 | ||||||||||||
61 | ||||||||||||
62 | ||||||||||||
63 | ||||||||||||
64 | ||||||||||||
65 | ||||||||||||
66 | ||||||||||||
67 | ||||||||||||
68 | ||||||||||||
69 | ||||||||||||
70 | ||||||||||||
71 | ||||||||||||
72 | ||||||||||||
73 | ||||||||||||
74 | ||||||||||||
75 | ||||||||||||
76 | ||||||||||||
77 | ||||||||||||
78 | ||||||||||||
79 | ||||||||||||
80 | ||||||||||||
81 | ||||||||||||
82 | ||||||||||||
83 | ||||||||||||
84 | ||||||||||||
85 | ||||||||||||
86 | ||||||||||||
87 | ||||||||||||
88 | ||||||||||||
89 | ||||||||||||
90 | ||||||||||||
91 | ||||||||||||
92 | ||||||||||||
93 | ||||||||||||
94 | ||||||||||||
95 | ||||||||||||
96 | ||||||||||||
97 | ||||||||||||
98 | ||||||||||||
99 | ||||||||||||
100 | ||||||||||||
101 | ||||||||||||
102 | ||||||||||||
103 | ||||||||||||
104 | ||||||||||||
105 | ||||||||||||
106 | ||||||||||||
107 | ||||||||||||
108 | ||||||||||||
109 | ||||||||||||
110 | MWR footprints for the minimum emission angle at each spacecraft rotation +-40 minutes from perijove. The cross marks the location of the perijove. | |||||||||||
111 |
1 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed toward the Earth. This orbit is for an extended mission approved by NASA HQ. | ||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|
2 | The period has been defined as a week before perijove to a week before the subsequent perijove, unlike the mission-planning definition, which extends from a day before the perijove to a day after the perijove. | ||||||||||||
3 | Period: Orbit 53-EXT [GRAV] (2023 Jul 25 - Aug 31) | Observations requested. | |||||||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | Observations planned / granted time | ||||||
5 | visible/NUV/ near-IR | Wong (17275) | Hubble/ WFC3-UVIS | hi-resolution non-global snapshot | 2023 July 31 | now: https://mast.stsci.edu/search/ui/#/hst/results?&proposal_id=16913 https://doi.org/10.3847/1538-4365/ab775f future: https://archive.stsci.edu/hlsp/wfcj | |||||||
6 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | Nightly, weather permitting | https://doi.org/10.5281/zenodo.8342758 see also https://arxiv.org/abs/2403.03131 | |||||||
7 | visible/nearIR | Alexander, Irwin | VLT/MUSE - IFU | spectroscopic imaging, 475-930 nm to determine cloud structure and albedo spectrum of particles. | Observations successful | ||||||||
8 | near-IR | Dahl | IRTF/SpeX | Imaging and scanning spectroscopy between 1.58 and 5.1 µm | July 29, July 30 | ||||||||
9 | near IR (5 µm) | Wong | Gemini-N/NIRI | lucky imaging, 5-µm maps | 2023 July 29 and 31 | now: https://archive.gemini.edu/searchform/GN-2022B-Q-106 future: https://archive.stsci.edu/hlsp/wfcj | |||||||
10 | mid IR | Orton | IRTF/MIRSI | filtered radiometric imaging to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology and auroral heating and chemistry. | July 31 - August 1 | Collaboration is possible with the investigators. | |||||||
11 | mid IR | Orton, Greathouse, Giles | 5-25 micron spectral imaging using TEXES | Jupiter's thermal infrared temperatures, atmospheric haze, and hyrdrocarbon abundances | July 23-25, most complete observations on July 25; some observations on July 25 overlap with Juno occulation region | Collaboration is possible with the investigators. | |||||||
12 | radio | Zarka, Cecconi, Lamy, Louis | Nançay Decameter Array (France) | coordinated measurement of 10-40 MHz cyclotron radio emission | every day, 8 hours around the transition to local meridian | https://maser.lesia.obspm.fr/task-1-data-collections/juno-ground-radio/juno-ground-radio-nancay-decameter.html?lang=en | |||||||
13 | |||||||||||||
14 | |||||||||||||
15 | |||||||||||||
16 | |||||||||||||
17 | |||||||||||||
18 | |||||||||||||
19 | |||||||||||||
20 | |||||||||||||
21 | |||||||||||||
22 | Scheduled observations by Juno. | ||||||||||||
23 | |||||||||||||
24 | Perijove is approximately 2023 Jul 31, 9:05 SCET ( = UTC - light time). System-III longitude = 122°W | ||||||||||||
25 | |||||||||||||
26 | Period: Orbit 53-EXT [GRAV] (2023 Jul 25 - Aug 31) | ||||||||||||
27 | Instrument | Description | |||||||||||
28 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | |||||||||||
29 | MWR | ||||||||||||
30 | UVS | ||||||||||||
31 | JunoCam | ||||||||||||
32 | JIRAM | ||||||||||||
33 | Communication Antennas | Radio-occultation experiments were performed with INGRESS at 2023-JUL-31 09:11:26 SCET, 32 N / 107 W and EGRESS at 2023-JUL-31 09:15:49 SCET, 20.6 N / 109 W. Latitudes are planetocentric and longitudes are in System III. | |||||||||||
34 | |||||||||||||
35 | |||||||||||||
36 | |||||||||||||
37 | |||||||||||||
38 | |||||||||||||
39 | |||||||||||||
40 | |||||||||||||
41 | |||||||||||||
42 | |||||||||||||
43 | |||||||||||||
44 | |||||||||||||
45 | |||||||||||||
46 | |||||||||||||
47 | |||||||||||||
48 | |||||||||||||
49 | |||||||||||||
50 | |||||||||||||
51 | |||||||||||||
52 | |||||||||||||
53 | |||||||||||||
54 | |||||||||||||
55 | |||||||||||||
56 | |||||||||||||
57 | |||||||||||||
58 | |||||||||||||
59 | |||||||||||||
60 | |||||||||||||
61 | |||||||||||||
62 | Composite RGB global map from JunoCam images, assembled by John Rogers and Gerald Eichstaedt, with various features labelled. | ||||||||||||
63 | |||||||||||||
64 | |||||||||||||
65 | |||||||||||||
66 | |||||||||||||
67 | |||||||||||||
68 | |||||||||||||
69 | |||||||||||||
70 | |||||||||||||
71 | |||||||||||||
72 | |||||||||||||
73 | |||||||||||||
74 | |||||||||||||
75 | |||||||||||||
76 | |||||||||||||
77 | |||||||||||||
78 | |||||||||||||
79 | |||||||||||||
80 | |||||||||||||
81 | |||||||||||||
82 | |||||||||||||
83 | |||||||||||||
84 | |||||||||||||
85 | |||||||||||||
86 | |||||||||||||
87 | |||||||||||||
88 | |||||||||||||
89 | |||||||||||||
90 | |||||||||||||
91 | |||||||||||||
92 | |||||||||||||
93 | |||||||||||||
94 | |||||||||||||
95 | |||||||||||||
96 | |||||||||||||
97 | |||||||||||||
98 | |||||||||||||
99 | |||||||||||||
100 | |||||||||||||
101 | |||||||||||||
102 | |||||||||||||
103 | |||||||||||||
104 | |||||||||||||
105 | |||||||||||||
106 | |||||||||||||
107 | |||||||||||||
108 | |||||||||||||
109 | |||||||||||||
110 | MWR footprints for the minimum emission angle at each spacecraft rotation +-40 minutes from perijove. The cross marks the location of the perijove. | ||||||||||||
111 |
1 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed toward the Earth. This orbit is for an extended mission approved by NASA HQ. | ||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|
2 | The period has been defined as a week before perijove to a week before the subsequent perijove, unlike the mission-planning definition, which extends from a day before the perijove to a day after the perijove. | ||||||||||||
3 | Period: Orbit 52-EXT [GRAV] (2023 Jun 17 - Jul 24) | Observations requested. | |||||||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | Observations planned / granted time | ||||||
5 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | Nightly, weather permitting | https://doi.org/10.5281/zenodo.8342758 see also https://arxiv.org/abs/2403.03131 | |||||||
6 | visible/nearIR | Alexander, Irwin | VLT/MUSE - IFU | spectroscopic imaging, 475-930 nm to determine cloud structure and albedo spectrum of particles. | Observations successful | ||||||||
7 | near-IR | Dahl | IRTF/SpeX | Imaging and scanning spectroscopy between 1.58 and 5.1 µm, Several hours of good daytime seeing. | June 23-24 | ||||||||
8 | mid IR | Orton | IRTF/MIRSI | filtered radiometric imaging to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology and auroral heating and chemistry. Several hours of good daytime seeing. | June 21-22 | Collaboration is possible with the investigators. | |||||||
9 | mid IR | Orton, Greathouse, Giles | 5-25 micron spectral imaging using TEXES | Jupiter's thermal infrared temperatures, atmospheric haze, and hyrdrocarbon abundances | July 23-25, most complete observations on July 25; some observations on July 25 overlap with Juno occulation region | Collaboration is possible with the investigators. | |||||||
10 | radio | Zarka, Cecconi, Lamy, Louis | Nançay Decameter Array (France) | coordinated measurement of 10-40 MHz cyclotron radio emission | every day, 8 hours around the transition to local meridian | https://maser.lesia.obspm.fr/task-1-data-collections/juno-ground-radio/juno-ground-radio-nancay-decameter.html?lang=en | |||||||
11 | Radio (mm/sub-mm) | Tseng | SMA | Ground-based radio observations of Io around 335-367GHz | 26 June and 2 more tracks in July | Collaboration is possible with the investigators. | |||||||
12 | |||||||||||||
13 | |||||||||||||
14 | |||||||||||||
15 | |||||||||||||
16 | |||||||||||||
17 | |||||||||||||
18 | |||||||||||||
19 | |||||||||||||
20 | Scheduled observations by Juno. | ||||||||||||
21 | |||||||||||||
22 | Perijove is approximately 2023 Jun 23, 6:55 SCET ( = UTC - light time). System-III longitude = 83°W | ||||||||||||
23 | |||||||||||||
24 | Period: Orbit 52-EXT [GRAV] (2023 Jun 17 - Jul 24) | ||||||||||||
25 | Instrument | Description | |||||||||||
26 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | |||||||||||
27 | MWR | ||||||||||||
28 | UVS | ||||||||||||
29 | JunoCam | ||||||||||||
30 | JIRAM | ||||||||||||
31 | |||||||||||||
32 | |||||||||||||
33 | |||||||||||||
34 | |||||||||||||
35 | |||||||||||||
36 | |||||||||||||
37 | |||||||||||||
38 | |||||||||||||
39 | |||||||||||||
40 | |||||||||||||
41 | |||||||||||||
42 | |||||||||||||
43 | |||||||||||||
44 | |||||||||||||
45 | |||||||||||||
46 | |||||||||||||
47 | |||||||||||||
48 | |||||||||||||
49 | |||||||||||||
50 | |||||||||||||
51 | |||||||||||||
52 | |||||||||||||
53 | |||||||||||||
54 | |||||||||||||
55 | |||||||||||||
56 | Composite RGB global map from JunoCam images, assembled by John Rogers and Gerald Eichstaedt, with various features labelled. | ||||||||||||
57 | |||||||||||||
58 | |||||||||||||
59 | |||||||||||||
60 | |||||||||||||
61 | |||||||||||||
62 | |||||||||||||
63 | |||||||||||||
64 | |||||||||||||
65 | |||||||||||||
66 | |||||||||||||
67 | |||||||||||||
68 | |||||||||||||
69 | |||||||||||||
70 | |||||||||||||
71 | |||||||||||||
72 | |||||||||||||
73 | |||||||||||||
74 | |||||||||||||
75 | |||||||||||||
76 | |||||||||||||
77 | |||||||||||||
78 | |||||||||||||
79 | |||||||||||||
80 | |||||||||||||
81 | |||||||||||||
82 | |||||||||||||
83 | |||||||||||||
84 | |||||||||||||
85 | |||||||||||||
86 | |||||||||||||
87 | |||||||||||||
88 | |||||||||||||
89 | |||||||||||||
90 | |||||||||||||
91 | |||||||||||||
92 | |||||||||||||
93 | |||||||||||||
94 | |||||||||||||
95 | |||||||||||||
96 | |||||||||||||
97 | |||||||||||||
98 | |||||||||||||
99 | |||||||||||||
100 | |||||||||||||
101 | |||||||||||||
102 | |||||||||||||
103 | |||||||||||||
104 | |||||||||||||
105 | |||||||||||||
106 | |||||||||||||
107 | |||||||||||||
108 | |||||||||||||
109 | |||||||||||||
110 | MWR footprints for the minimum emission angle at each spacecraft rotation +-40 minutes from perijove. The cross marks the location of the perijove. | ||||||||||||
111 |
1 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed toward the Earth. This orbit is for an extended mission approved by NASA HQ. | ||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|
2 | The period has been defined as a week before perijove to a week before the subsequent perijove, unlike the mission-planning definition, which extends from a day before the perijove to a day after the perijove. | ||||||||||||
3 | Period: Orbit 51-EXT [GRAV] (2023 May 10 - Jun 16) | Observations requested. | |||||||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | Observations planned / granted time | ||||||
5 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | Nightly, weather permitting | https://doi.org/10.5281/zenodo.8342758 see also https://arxiv.org/abs/2403.03131 | |||||||
6 | visible/nearIR | Alexander, Irwin | VLT/MUSE - IFU | spectroscopic imaging, 475-930 nm to determine cloud structure and albedo spectrum of particles. | Observations successful | ||||||||
7 | near-IR | Dahl | IRTF/SpeX | Imaging and scanning spectroscopy between 1.58 and 5.1 µm | May 16-17, paritally clear / partially cloudy weather, with imaging done between clouds. Most successful imaging is at 5.1 microns. | ||||||||
8 | mid IR | Orton | IRTF/MIRSI | filtered radiometric imaging to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology and auroral heating and chemistry. | May 14-15. Mostly successful imagin, with seeing generally worse than 1" due to daytime conditions. | Collaboration is possible with the investigators. | |||||||
9 | radio | Zarka, Cecconi, Lamy, Louis | Nançay Decameter Array (France) | coordinated measurement of 10-40 MHz cyclotron radio emission | every day, 8 hours around the transition to local meridian | https://maser.lesia.obspm.fr/task-1-data-collections/juno-ground-radio/juno-ground-radio-nancay-decameter.html?lang=en | |||||||
10 | |||||||||||||
11 | |||||||||||||
12 | |||||||||||||
13 | |||||||||||||
14 | |||||||||||||
15 | |||||||||||||
16 | |||||||||||||
17 | |||||||||||||
18 | |||||||||||||
19 | Scheduled observations by Juno. | ||||||||||||
20 | |||||||||||||
21 | Perijove is approximately 2023 May 16, 7:31 SCET ( = UTC - light time). System-III longitude = 145°W | ||||||||||||
22 | |||||||||||||
23 | Period: Orbit 51-EXT [GRAV] (2023 May 10 - Jun 16) | ||||||||||||
24 | Instrument | Description | |||||||||||
25 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | |||||||||||
26 | MWR | ||||||||||||
27 | UVS | ||||||||||||
28 | JunoCam | ||||||||||||
29 | JIRAM | ||||||||||||
30 | |||||||||||||
31 | |||||||||||||
32 | |||||||||||||
33 | |||||||||||||
34 | |||||||||||||
35 | |||||||||||||
36 | |||||||||||||
37 | |||||||||||||
38 | |||||||||||||
39 | |||||||||||||
40 | |||||||||||||
41 | |||||||||||||
42 | |||||||||||||
43 | |||||||||||||
44 | |||||||||||||
45 | |||||||||||||
46 | |||||||||||||
47 | |||||||||||||
48 | |||||||||||||
49 | |||||||||||||
50 | |||||||||||||
51 | |||||||||||||
52 | Composite RGB global map from JunoCam images, assembled by John Rogers and Gerald Eichstaedt. | ||||||||||||
53 | |||||||||||||
54 | |||||||||||||
55 | |||||||||||||
56 | |||||||||||||
57 | |||||||||||||
58 | |||||||||||||
59 | |||||||||||||
60 | |||||||||||||
61 | |||||||||||||
62 | |||||||||||||
63 | |||||||||||||
64 | |||||||||||||
65 | |||||||||||||
66 | |||||||||||||
67 | |||||||||||||
68 | |||||||||||||
69 | |||||||||||||
70 | |||||||||||||
71 | |||||||||||||
72 | |||||||||||||
73 | |||||||||||||
74 | |||||||||||||
75 | |||||||||||||
76 | |||||||||||||
77 | |||||||||||||
78 | |||||||||||||
79 | |||||||||||||
80 | |||||||||||||
81 | |||||||||||||
82 | |||||||||||||
83 | |||||||||||||
84 | |||||||||||||
85 | |||||||||||||
86 | |||||||||||||
87 | |||||||||||||
88 | |||||||||||||
89 | |||||||||||||
90 | |||||||||||||
91 | |||||||||||||
92 | |||||||||||||
93 | |||||||||||||
94 | |||||||||||||
95 | |||||||||||||
96 | |||||||||||||
97 | |||||||||||||
98 | |||||||||||||
99 | |||||||||||||
100 | |||||||||||||
101 | |||||||||||||
102 | |||||||||||||
103 | |||||||||||||
104 | |||||||||||||
105 | |||||||||||||
106 | |||||||||||||
107 | |||||||||||||
108 | |||||||||||||
109 | |||||||||||||
110 | MWR footprints for the minimum emission angle at each spacecraft rotation +-40 minutes from perijove. The cross marks the location of the perijove. | ||||||||||||
111 | |||||||||||||
112 |
1 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed toward the Earth. This orbit is for an extended mission approved by NASA HQ. | |||||||||
---|---|---|---|---|---|---|---|---|---|---|
2 | No Earth-based observations are expected due to proximity to solar conjunction on April 11. | |||||||||
3 | The period has been defined as a week before perijove to a week before the subsequent perijove, unlike the mission-planning definition, which extends from a day before the perijove to a day after the perijove. | |||||||||
4 | Period: Orbit 50-EXT [GRAV] (2023 Apr 2 - May 9) | Observations requested. | ||||||||
5 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | Observations planned / granted time | |||
6 | radio | Zarka, Cecconi, Lamy, Louis | Nançay Decameter Array (France) | coordinated measurement of 10-40 MHz cyclotron radio emission | every day, 8 hours around the transition to local meridian | https://maser.lesia.obspm.fr/task-1-data-collections/juno-ground-radio/juno-ground-radio-nancay-decameter.html?lang=en | Observations successful | |||
7 | ||||||||||
8 | ||||||||||
9 | ||||||||||
10 | ||||||||||
11 | ||||||||||
12 | ||||||||||
13 | ||||||||||
14 | ||||||||||
15 | ||||||||||
16 | ||||||||||
17 | ||||||||||
18 | Scheduled observations by Juno. | |||||||||
19 | ||||||||||
20 | Perijove is approximatley 2023 Apr 8, 9:46 SCET ( = UTC - light time). System-III longitude = 267°W | |||||||||
21 | ||||||||||
22 | Period: Orbit 50-EXT [GRAV] (2023 Apr 2 - May 9) | |||||||||
23 | Instrument | Description | ||||||||
24 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||
25 | MWR | |||||||||
26 | UVS | |||||||||
27 | JunoCam | |||||||||
28 | JIRAM | |||||||||
29 | ||||||||||
30 | ||||||||||
31 | ||||||||||
32 | ||||||||||
33 | ||||||||||
34 | ||||||||||
35 | ||||||||||
36 | ||||||||||
37 | ||||||||||
38 | ||||||||||
39 | ||||||||||
40 | ||||||||||
41 | ||||||||||
42 | ||||||||||
43 | ||||||||||
44 | ||||||||||
45 | ||||||||||
46 | Composite RGB global map from JunoCam images, assembled by John Rogers and Gerald Eichstaedt, with various features labelled. | |||||||||
47 | ||||||||||
48 | ||||||||||
49 | ||||||||||
50 | ||||||||||
51 | ||||||||||
52 | ||||||||||
53 | ||||||||||
54 | ||||||||||
55 | ||||||||||
56 | ||||||||||
57 | ||||||||||
58 | ||||||||||
59 | ||||||||||
60 | ||||||||||
61 | ||||||||||
62 | ||||||||||
63 | ||||||||||
64 | ||||||||||
65 | ||||||||||
66 | ||||||||||
67 | ||||||||||
68 | ||||||||||
69 | ||||||||||
70 | ||||||||||
71 | ||||||||||
72 | ||||||||||
73 | ||||||||||
74 | ||||||||||
75 | ||||||||||
76 | ||||||||||
77 | ||||||||||
78 | ||||||||||
79 | ||||||||||
80 | ||||||||||
81 | ||||||||||
82 | ||||||||||
83 | ||||||||||
84 | ||||||||||
85 | ||||||||||
86 | ||||||||||
87 | ||||||||||
88 | ||||||||||
89 | ||||||||||
90 | ||||||||||
91 | ||||||||||
92 | ||||||||||
93 | ||||||||||
94 | ||||||||||
95 | ||||||||||
96 | ||||||||||
97 | ||||||||||
98 | ||||||||||
99 | ||||||||||
100 | ||||||||||
101 | ||||||||||
102 | ||||||||||
103 | ||||||||||
104 | ||||||||||
105 | ||||||||||
106 | MWR footprints for the minimum emission angle at each spacecraft rotation. The cross marks the location of the perijove. | |||||||||
107 | ||||||||||
108 |
1 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed toward the Earth. This orbit is for an extended mission approved by NASA HQ. | |||||||||
---|---|---|---|---|---|---|---|---|---|---|
2 | The period has been defined as a week before perijove to a week before the subsequent perijove, unlike the mission-planning definition, which extends from a day before the perijove to a day after the perijove. | |||||||||
3 | Period: Orbit 49-EXT [GRAV] (2023 Feb 23 - Apr 1) | Observations requested. | ||||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | Observations planned / granted time | |||
5 | Observations successful | |||||||||
6 | ||||||||||
7 | ||||||||||
8 | mid IR | Orton | IRTF/MIRSI | filtered radiometric imaging to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology and auroral heating and chemistry. | Feb 27: about two hours of useful data, Feb 28 no data obtained due to snowstorm | Collaboration is possible with the investigators. | s | |||
9 | near-IR | Dahl | IRTF/SpeX | Imaging and scanning spectroscopy between 1.58 and 5.1 µm | March 1, March 2: no data obtained due to snowstorm | |||||
10 | radio | Zarka, Cecconi, Lamy, Louis | Nançay Decameter Array (France) | coordinated measurement of 10-40 MHz cyclotron radio emission | every day, 8 hours around the transition to local meridian | https://maser.lesia.obspm.fr/task-1-data-collections/juno-ground-radio/juno-ground-radio-nancay-decameter.html?lang=en | ||||
11 | ||||||||||
12 | ||||||||||
13 | ||||||||||
14 | ||||||||||
15 | ||||||||||
16 | ||||||||||
17 | Scheduled observations by Juno. | |||||||||
18 | ||||||||||
19 | Perijove is 2023 Mar 1, 5:53:18 SCET ( = UTC - light time). System-III longitude = 165.8°W | |||||||||
20 | ||||||||||
21 | Period: Orbit 49-EXT [GRAV] (2023 Feb 23 - Apr 1) | |||||||||
22 | Instrument | Description | ||||||||
23 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||
24 | MWR | |||||||||
25 | UVS | |||||||||
26 | JunoCam | |||||||||
27 | JIRAM | |||||||||
28 | ||||||||||
29 | ||||||||||
30 | ||||||||||
31 | ||||||||||
32 | ||||||||||
33 | ||||||||||
34 | ||||||||||
35 | ||||||||||
36 | ||||||||||
37 | ||||||||||
38 | ||||||||||
39 | ||||||||||
40 | ||||||||||
41 | ||||||||||
42 | ||||||||||
43 | ||||||||||
44 | ||||||||||
45 | ||||||||||
46 | ||||||||||
47 | ||||||||||
48 | ||||||||||
49 | ||||||||||
50 | ||||||||||
51 | ||||||||||
52 | ||||||||||
53 | ||||||||||
54 | ||||||||||
55 | ||||||||||
56 | Composite RGB global map from JunoCam images, assembled by John Rogers and Gerald Eichstaedt, with various features labelled. | |||||||||
57 | ||||||||||
58 | ||||||||||
59 | ||||||||||
60 | ||||||||||
61 | ||||||||||
62 | ||||||||||
63 | ||||||||||
64 | ||||||||||
65 | ||||||||||
66 | ||||||||||
67 | ||||||||||
68 | ||||||||||
69 | ||||||||||
70 | ||||||||||
71 | ||||||||||
72 | ||||||||||
73 | ||||||||||
74 | ||||||||||
75 | ||||||||||
76 | ||||||||||
77 | ||||||||||
78 | ||||||||||
79 | ||||||||||
80 | ||||||||||
81 | ||||||||||
82 | ||||||||||
83 | ||||||||||
84 | ||||||||||
85 | ||||||||||
86 | ||||||||||
87 | ||||||||||
88 | ||||||||||
89 | ||||||||||
90 | ||||||||||
91 | ||||||||||
92 | ||||||||||
93 | ||||||||||
94 | ||||||||||
95 | ||||||||||
96 | ||||||||||
97 | ||||||||||
98 | ||||||||||
99 | ||||||||||
100 | ||||||||||
101 | ||||||||||
102 | ||||||||||
103 | ||||||||||
104 | ||||||||||
105 | ||||||||||
106 | ||||||||||
107 | ||||||||||
108 | ||||||||||
109 | ||||||||||
110 | MWR footprints for the minimum emission angle at each spacecraft rotation. The cross marks the location of the perijove. | |||||||||
111 |
1 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed toward the Earth. This orbit is for an extended mission approved by NASA HQ. | |||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
2 | The period has been defined as a week before perijove to a week before the subsequent perijove, unlike the mission-planning definition, which extends from a day before the perijove to a day after the perijove. | |||||||||||||
3 | Period: Orbit 48-EXT [GRAV] (2023 Jan 16 - Feb 22) | Observations requested. | ||||||||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | Observations planned / granted time | |||||||
5 | FUV | Bonfond | HST/STIS | Timetag imaging of northern aurora | Observations successful | |||||||||
6 | visible/NUV/ near-IR | Wong (17275) | Hubble/ WFC3-UVIS | hi-resolution non-global snapshot | 2023 Jan 22 | now: https://mast.stsci.edu/search/ui/#/hst/results?&proposal_id=16913 https://doi.org/10.3847/1538-4365/ab775f future: https://archive.stsci.edu/hlsp/wfcj | ||||||||
7 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | Nightly, weather permitting | https://doi.org/10.5281/zenodo.8342758 | ||||||||
8 | UV, VIS, near-IR | Sanchez-Lavega | Planetcam, 2.2m Calar Alto Observatory | Observing Jupiter with new detectors (0.35-1 micron) & (1-1.6 micron) | 20, 21, 22, 23 January | |||||||||
9 | visible/nearIR | Alexander, Irwin | VLT/MUSE - IFU | spectroscopic imaging, 475-930 nm to determine cloud structure and albedo spectrum of particles. | Dates near PJ48 requested. | Raw data publicly available to download from ESO portal this time next year. Standard calibration pipeline takes of the order of 1-3 days to complete. | ||||||||
10 | near IR | Orton | IRTF/SpeX | filtered imaging and scanning spectroscopy between 1.58 and 5.1µm | Jan 21 data partially acquired. Jan 23 observations lost to weather | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired. Reduced "quick-look" observations (geometrically but not radiometrically calibrated) will be available for immeduately use from the Juno-curated web site: http://junoirtf.space.swri.edu/ | s | |||||||
11 | mid IR | Orton | IRTF/MIRSI | filtered radiometric imaging and spectroscopy to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology and auroral heating and chemistry. | Jan 24 data partially acquired through variable sky conditions | Collaboration is possible with the investigators. | ||||||||
12 | radio | Zarka, Cecconi, Lamy, Louis | Nançay Decameter Array (France) | coordinated measurement of 10-40 MHz cyclotron radio emission | every day, 8 hours around the transition to local meridian | https://maser.lesia.obspm.fr/task-1-data-collections/juno-ground-radio/juno-ground-radio-nancay-decameter.html?lang=en | ||||||||
13 | ||||||||||||||
14 | ||||||||||||||
15 | ||||||||||||||
16 | ||||||||||||||
17 | ||||||||||||||
18 | Scheduled observations by Juno. | |||||||||||||
19 | ||||||||||||||
20 | Perijove is 2023 Jan 22, 5:43:28 SCET ( = UTC - light time). System-III longitude = 199.9°W | |||||||||||||
21 | ||||||||||||||
22 | Period: Orbit 48-EXT [GRAV] (2023 Jan 16 - Feb 22) | |||||||||||||
23 | Instrument | Description | ||||||||||||
24 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||||||
25 | MWR | |||||||||||||
26 | UVS | |||||||||||||
27 | JunoCam | |||||||||||||
28 | JIRAM | |||||||||||||
29 | ||||||||||||||
30 | ||||||||||||||
31 | ||||||||||||||
32 | ||||||||||||||
33 | ||||||||||||||
34 | ||||||||||||||
35 | ||||||||||||||
36 | ||||||||||||||
37 | ||||||||||||||
38 | ||||||||||||||
39 | ||||||||||||||
40 | ||||||||||||||
41 | ||||||||||||||
42 | ||||||||||||||
43 | ||||||||||||||
44 | ||||||||||||||
45 | ||||||||||||||
46 | ||||||||||||||
47 | ||||||||||||||
48 | ||||||||||||||
49 | ||||||||||||||
50 | ||||||||||||||
51 | ||||||||||||||
52 | ||||||||||||||
53 | Composite RGB global map from JunoCam images. Only the outbound images were useable due to a temperature-relatve anomaly in the instrument affecting the previous images. | |||||||||||||
54 | ||||||||||||||
55 | ||||||||||||||
56 | ||||||||||||||
57 | ||||||||||||||
58 | ||||||||||||||
59 | ||||||||||||||
60 | ||||||||||||||
61 | ||||||||||||||
62 | ||||||||||||||
63 | ||||||||||||||
64 | ||||||||||||||
65 | ||||||||||||||
66 | ||||||||||||||
67 | ||||||||||||||
68 | ||||||||||||||
69 | ||||||||||||||
70 | ||||||||||||||
71 | ||||||||||||||
72 | ||||||||||||||
73 | ||||||||||||||
74 | ||||||||||||||
75 | ||||||||||||||
76 | ||||||||||||||
77 | ||||||||||||||
78 | ||||||||||||||
79 | ||||||||||||||
80 | ||||||||||||||
81 | ||||||||||||||
82 | ||||||||||||||
83 | ||||||||||||||
84 | ||||||||||||||
85 | ||||||||||||||
86 | ||||||||||||||
87 | ||||||||||||||
88 | ||||||||||||||
89 | ||||||||||||||
90 | ||||||||||||||
91 | ||||||||||||||
92 | ||||||||||||||
93 | ||||||||||||||
94 | ||||||||||||||
95 | ||||||||||||||
96 | ||||||||||||||
97 | ||||||||||||||
98 | MWR footprints for the minimum emission angle at each spacecraft rotation. The cross marks the location of the perijove. | |||||||||||||
99 |
1 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed toward the Earth. This orbit is for an extended mission approved by NASA HQ. | |||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
2 | The period has been defined as a week before perijove to a week before the subsequent perijove, unlike the mission-planning definition, which extends from a day before the perijove to a day after the perijove. | |||||||||||||
3 | Period: Orbit 47-EXT [GRAV] (2022 Dec 7 - 2023 Jan 15) | Observations requested. | ||||||||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | Observations planned / granted time | |||||||
5 | FUV | Bonfond | HST/STIS | Timetag imaging of northern aurora | Observations successful | |||||||||
6 | visible/NUV | Wong | HST/WFC3 UVIS | hi-resolution map of perijove track, single orbit snapshot | Observations cancelled or unsuccessful | |||||||||
7 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | 20221208 20230104 20221209 20230105 20221210 20230108 20221211 20230109 20221217 20230111 20221222 20230113 20221223 20230114 20221224 | https://doi.org/10.5281/zenodo.8342758 | ||||||||
8 | near IR | Orton | IRTF/SpeX | filtered imaging and scanning spectroscopy between 1.58 and 5.1µm | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired. Reduced "quick-look" observations (geometrically but not radiometrically calibrated) will be available for immeduately use from the Juno-curated web site: http://junoirtf.space.swri.edu/ | |||||||||
9 | mid IR | Orton | IRTF/MIRSI | filtered radiometric imaging and spectroscopy to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology and auroral heating and chemistry. | Collaboration is possible with the investigators. | |||||||||
10 | Visible | Schmidt | Keck I HIRES | Io Na & K recovery post-eclipse (18:41- 19:55 visibility in shadow) Incident plasma conditions IPT structure and composition | 16 Dec, evening | immediately available on KOA public archive: https://koa.ipac.caltech.edu/cgi-bin/KOA/nph-KOAlogin | ||||||||
11 | visible/nearIR | Alexander, Irwin | VLT/MUSE - IFU | spectroscopic imaging, 475-930 nm to determine cloud structure and albedo spectrum of particles. | Dates near PJ47 requested. | Raw data publicly available to download from ESO portal this time next year. Standard calibration pipeline takes of the order of 1-3 days to complete. | ||||||||
12 | radio | Zarka, Cecconi, Lamy, Louis | Nançay Decameter Array (France) | coordinated measurement of 10-40 MHz cyclotron radio emission | every day, 8 hours around the transition to local meridian | https://maser.lesia.obspm.fr/task-1-data-collections/juno-ground-radio/juno-ground-radio-nancay-decameter.html?lang=en | ||||||||
13 | ||||||||||||||
14 | ||||||||||||||
15 | Scheduled observations by Juno. | |||||||||||||
16 | ||||||||||||||
17 | Perijove is 2022 Dec 15, 3:23:21 SCET ( = UTC - light time). System-III longitude = 170.1°W | |||||||||||||
18 | ||||||||||||||
19 | Period: Orbit 47-EXT [GRAV] (2022 Dec 7 - 2023 Jan 15) | |||||||||||||
20 | Instrument | Description | ||||||||||||
21 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||||||
22 | MWR | |||||||||||||
23 | UVS | |||||||||||||
24 | JunoCam | |||||||||||||
25 | JIRAM | |||||||||||||
26 | ||||||||||||||
27 | ||||||||||||||
28 | ||||||||||||||
29 | ||||||||||||||
30 | ||||||||||||||
31 | ||||||||||||||
32 | ||||||||||||||
33 | ||||||||||||||
34 | ||||||||||||||
35 | ||||||||||||||
36 | ||||||||||||||
37 | ||||||||||||||
38 | ||||||||||||||
39 | ||||||||||||||
40 | ||||||||||||||
41 | ||||||||||||||
42 | ||||||||||||||
43 | ||||||||||||||
44 | ||||||||||||||
45 | ||||||||||||||
46 | ||||||||||||||
47 | ||||||||||||||
48 | ||||||||||||||
49 | ||||||||||||||
50 | ||||||||||||||
51 | ||||||||||||||
52 | ||||||||||||||
53 | ||||||||||||||
54 | Composite of JIRAM M-band (5-micron) map. | |||||||||||||
55 | ||||||||||||||
56 | ||||||||||||||
57 | ||||||||||||||
58 | ||||||||||||||
59 | ||||||||||||||
60 | ||||||||||||||
61 | ||||||||||||||
62 | ||||||||||||||
63 | ||||||||||||||
64 | ||||||||||||||
65 | ||||||||||||||
66 | ||||||||||||||
67 | ||||||||||||||
68 | ||||||||||||||
69 | ||||||||||||||
70 | ||||||||||||||
71 | ||||||||||||||
72 | ||||||||||||||
73 | ||||||||||||||
74 | ||||||||||||||
75 | ||||||||||||||
76 | ||||||||||||||
77 | ||||||||||||||
78 | ||||||||||||||
79 | ||||||||||||||
80 | ||||||||||||||
81 | ||||||||||||||
82 | ||||||||||||||
83 | ||||||||||||||
84 | ||||||||||||||
85 | ||||||||||||||
86 | ||||||||||||||
87 | ||||||||||||||
88 | ||||||||||||||
89 | ||||||||||||||
90 | ||||||||||||||
91 | ||||||||||||||
92 | ||||||||||||||
93 | ||||||||||||||
94 | ||||||||||||||
95 | ||||||||||||||
96 | ||||||||||||||
97 | ||||||||||||||
98 | ||||||||||||||
99 | ||||||||||||||
100 | ||||||||||||||
101 | ||||||||||||||
102 | Plot of Microwave Radiometer (MWR) footprints for the minimum emission angle field of view vs time for each spin of the spacecraft. | |||||||||||||
103 | The cross marks the position of the perijove. | |||||||||||||
104 | ||||||||||||||
105 | ||||||||||||||
106 | ||||||||||||||
107 | ||||||||||||||
108 | ||||||||||||||
109 | ||||||||||||||
110 | ||||||||||||||
111 | ||||||||||||||
112 | ||||||||||||||
113 | ||||||||||||||
114 | ||||||||||||||
115 | ||||||||||||||
116 | ||||||||||||||
117 | ||||||||||||||
118 | ||||||||||||||
119 | ||||||||||||||
120 | ||||||||||||||
121 | ||||||||||||||
122 | ||||||||||||||
123 | ||||||||||||||
124 | ||||||||||||||
125 | ||||||||||||||
126 | ||||||||||||||
127 | ||||||||||||||
128 | ||||||||||||||
129 | ||||||||||||||
130 | ||||||||||||||
131 | ||||||||||||||
132 | Composite global RGB map from approach images, John Rogers, Gerald Eichstaedt | |||||||||||||
133 | ||||||||||||||
134 | ||||||||||||||
135 | ||||||||||||||
136 | ||||||||||||||
137 | ||||||||||||||
138 | ||||||||||||||
139 | ||||||||||||||
140 | ||||||||||||||
141 | ||||||||||||||
142 | ||||||||||||||
143 | ||||||||||||||
144 | ||||||||||||||
145 | ||||||||||||||
146 | ||||||||||||||
147 | ||||||||||||||
148 | ||||||||||||||
149 | Composite RGB map from perijove images, John Rogers, Gerald Eichstaedt | |||||||||||||
150 | ||||||||||||||
151 | ||||||||||||||
152 | ||||||||||||||
153 | ||||||||||||||
154 | ||||||||||||||
155 | ||||||||||||||
156 | ||||||||||||||
157 | ||||||||||||||
158 | ||||||||||||||
159 | ||||||||||||||
160 | Composite RGB map from perijove images, John Rogers, Gerald Eichstaedt |
1 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed toward the Earth. This orbit is for an extended mission approved by NASA HQ. | |||||||||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
2 | The period has been defined as a week before perijove to a week before the subsequent perijove, unlike the mission-planning definition, which extends from a day before the perijove to a day after the perijove. | |||||||||||||||||||
3 | Period: Orbit 46-EXT [GRAV] (2022 Oct 31 - 2022 Dec 7) | Observations requested. | ||||||||||||||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | Observations planned / granted time | |||||||||||||
5 | FUV | Bonfond | HST/STIS | Timetag imaging of northern aurora | Observations successful | |||||||||||||||
6 | FUV and NUV | Roth | HST / STIS and COS | Ganymede's aurora in eclipse, FUV imaging and NUV spectrum | 13 Nov, and 05 Dec | after 6 months proprietary period or contact PI | ||||||||||||||
7 | visible/NUV | Wong | HST/WFC3 UVIS | hi-resolution map of perijove track, single orbit snapshot | Observations cancelled or unsuccessful | |||||||||||||||
8 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | Nightly, weather permitting 20221101 20221117 20221103 20221118 20221105 20221119 20221106 20221120 20221108 20221121 20221109 20221122 20221110 20221127 20221111 20221128 20221112 20221129 20221113 20221130 20221114 20221201 20221115 20221202 20221116 20221203 | See Fall 2022 AGU poster SM42F-2232 and right for record of outbursts results from past 6 years. Publication planned soon | ||||||||||||||
9 | visible/nearIR | Alexander, Irwin | VLT/MUSE - IFU | spectroscopic imaging, 475-930 nm to determine cloud structure and albedo spectrum of particles. | Dates near PJ46 requested. | Raw data publicly available to download from ESO portal this time next year. Standard calibration pipeline takes of the order of 1-3 days to complete. | ||||||||||||||
10 | Visible | Schmidt | Keck I HIRES | Ganymede O I line ratios: H2O vs O2 vs O diagnostic, eclipse visibility Plasma structure and composition of IPT | 23 Nov, evening | |||||||||||||||
11 | Visible | Schmidt | Keck I HIRES | Ganymede O I line ratios: H2O vs O2 vs O diagnostic, 20:28-23:02 eclipse visibility Plasma structure and composition of IPT | 04 Dec, evening | weathered out | ||||||||||||||
12 | Near IR | Schmidt | Keck II NIRSPEC | Jovian Aurora H2/H3+ mapping, Pre-PJ46 @ 11:38 (maps of both hemispheres) | 05 Nov, evening | immediately available on KOA public archive: https://koa.ipac.caltech.edu/cgi-bin/KOA/nph-KOAlogin | ||||||||||||||
13 | near IR | Orton | IRTF/SpeX | filtered imaging and scanning spectroscopy between 1.58 and 5.1µm | IRTF observations cancelled due to mechanical problems with the dome shutter | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired. Reduced "quick-look" observations (geometrically but not radiometrically calibrated) will be available for immeduately use from the Juno-curated web site: http://junoirtf.space.swri.edu/ | ||||||||||||||
14 | near IR | Orton | Gemini-N/NIRI | filtered near-infrared imaging of Jupiter, often with Adaptive-Optics (AO) stabilization. | Gemini North observations canelled due to mechanical problems with the primary mirror | avalable on request | ||||||||||||||
15 | mid IR | Orton | IRTF/MIRSI | filtered radiometric imaging and spectroscopy to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology and auroral heating and chemistry. | IRTF observations cancelled due to mechanical problems with the dome shutter | Collaboration is possible with the investigators. | ||||||||||||||
16 | mid-IR | Fletcher | VLT/VISIR | Filtered imaging 5-20 µm. | Acquired on 2022-10-31 and 2022-11-16, desired global map could not be completed. | Available on request, example shown to the right. | ||||||||||||||
17 | radio | Zarka, Cecconi, Lamy, Louis | Nançay Decameter Array (France) | coordinated measurement of 10-40 MHz cyclotron radio emission | every day, 8 hours around the transition to local meridian | https://maser.lesia.obspm.fr/task-1-data-collections/juno-ground-radio/juno-ground-radio-nancay-decameter.html?lang=en | ||||||||||||||
18 | Radio | Lamy for the NenuFar ES07 team | NenuFAR (France) | coordinated measurements of 10-40 MHz cyclotron radio emission at high time/frequency resolution | 2022/11/06T15:02:00 - 02:32:00 2022/11/07T15:00:00 - 02:29:00 2022/11/08T15:00:00 - 02:24:00 | Data available on demand to laurent.lamy@obspm.fr | ||||||||||||||
19 | Radio (mm/sub-mm) | Tseng | SMA | Ground-based radio observations of Io around 335-367GHz | 11 Oct | Collaboration is possible with the investigators. | ||||||||||||||
20 | ||||||||||||||||||||
21 | ||||||||||||||||||||
22 | Scheduled observations by Juno. | |||||||||||||||||||
23 | ||||||||||||||||||||
24 | Perijove is 2022 Nov 6, 21:38:26 SCET ( = UTC - light time). System-III longitude = 1.4°W | |||||||||||||||||||
25 | s | |||||||||||||||||||
26 | Period: Orbit 46-EXT [GRAV] (2022 Oct 31 - 2022 Dec 7) | |||||||||||||||||||
27 | Instrument | Description | ||||||||||||||||||
28 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||||||||||||
29 | MWR | |||||||||||||||||||
30 | UVS | |||||||||||||||||||
31 | JunoCam | |||||||||||||||||||
32 | JIRAM | |||||||||||||||||||
33 | ||||||||||||||||||||
34 | ||||||||||||||||||||
35 | ||||||||||||||||||||
36 | ||||||||||||||||||||
37 | ||||||||||||||||||||
38 | ||||||||||||||||||||
39 | ||||||||||||||||||||
40 | ||||||||||||||||||||
41 | ||||||||||||||||||||
42 | ||||||||||||||||||||
43 | ||||||||||||||||||||
44 | ||||||||||||||||||||
45 | ||||||||||||||||||||
46 | ||||||||||||||||||||
47 | ||||||||||||||||||||
48 | ||||||||||||||||||||
49 | ||||||||||||||||||||
50 | ||||||||||||||||||||
51 | ||||||||||||||||||||
52 | ||||||||||||||||||||
53 | ||||||||||||||||||||
54 | ||||||||||||||||||||
55 | ||||||||||||||||||||
56 | ||||||||||||||||||||
57 | ||||||||||||||||||||
58 | ||||||||||||||||||||
59 | ||||||||||||||||||||
60 | ||||||||||||||||||||
61 | ||||||||||||||||||||
62 | Composite color map from JunoCam, combining low-resolution global observations from the perijove approach phase at low latitudes with high-resolution maps near perijove. | |||||||||||||||||||
63 | ||||||||||||||||||||
64 | ||||||||||||||||||||
65 | ||||||||||||||||||||
66 | ||||||||||||||||||||
67 | ||||||||||||||||||||
68 | ||||||||||||||||||||
69 | ||||||||||||||||||||
70 | ||||||||||||||||||||
71 | ||||||||||||||||||||
72 | ||||||||||||||||||||
73 | ||||||||||||||||||||
74 | ||||||||||||||||||||
75 | ||||||||||||||||||||
76 | ||||||||||||||||||||
77 | ||||||||||||||||||||
78 | ||||||||||||||||||||
79 | ||||||||||||||||||||
80 | ||||||||||||||||||||
81 | ||||||||||||||||||||
82 | ||||||||||||||||||||
83 | ||||||||||||||||||||
84 | ||||||||||||||||||||
85 | ||||||||||||||||||||
86 | ||||||||||||||||||||
87 | ||||||||||||||||||||
88 | ||||||||||||||||||||
89 | Composite of JIRAM M-band (5-micron) map. | |||||||||||||||||||
90 | ||||||||||||||||||||
91 | ||||||||||||||||||||
92 | ||||||||||||||||||||
93 | ||||||||||||||||||||
94 | ||||||||||||||||||||
95 | ||||||||||||||||||||
96 | ||||||||||||||||||||
97 | ||||||||||||||||||||
98 | ||||||||||||||||||||
99 | ||||||||||||||||||||
100 | ||||||||||||||||||||
101 | ||||||||||||||||||||
102 | ||||||||||||||||||||
103 | ||||||||||||||||||||
104 | ||||||||||||||||||||
105 | ||||||||||||||||||||
106 | ||||||||||||||||||||
107 | ||||||||||||||||||||
108 | ||||||||||||||||||||
109 | ||||||||||||||||||||
110 | ||||||||||||||||||||
111 | ||||||||||||||||||||
112 | ||||||||||||||||||||
113 | ||||||||||||||||||||
114 | ||||||||||||||||||||
115 | ||||||||||||||||||||
116 | ||||||||||||||||||||
117 | ||||||||||||||||||||
118 | ||||||||||||||||||||
119 | ||||||||||||||||||||
120 | ||||||||||||||||||||
121 | ||||||||||||||||||||
122 | ||||||||||||||||||||
123 | ||||||||||||||||||||
124 | ||||||||||||||||||||
125 | ||||||||||||||||||||
126 | ||||||||||||||||||||
127 | ||||||||||||||||||||
128 | ||||||||||||||||||||
129 | ||||||||||||||||||||
130 | ||||||||||||||||||||
131 | ||||||||||||||||||||
132 | ||||||||||||||||||||
133 | ||||||||||||||||||||
134 | ||||||||||||||||||||
135 | ||||||||||||||||||||
136 | ||||||||||||||||||||
137 | ||||||||||||||||||||
138 | ||||||||||||||||||||
139 | Plot of Microwave Radiometer (MWR) footprints for the minimum emission angle field of view vs time for each spin of the spacecraft. | |||||||||||||||||||
140 | The cross marks the position of the perijove. |
1 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed toward the Earth. This orbit is for an extended mission approved by NASA HQ. | |||||||||
---|---|---|---|---|---|---|---|---|---|---|
2 | Near this perijove, on September 29, the spacecraft will make a close approach of the Galilean satellite Europa. | |||||||||
3 | The period has been defined as a week before perijove to a week before the subsequent perijove, unlike the mission-planning definition, which extends from a day before the perijove to a day after the perijove. | |||||||||
4 | Period: Orbit 45-EXT [GRAV] (2022 Sep 20 - 2022 Oct 31) | Observations requested. | ||||||||
5 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | Observations planned / granted time | |||
6 | FUV | Roth | HST / STIS | Ganymede's aurora in eclipse, FUV imaging | 23 Oct, 30 Oct | after 6 months proprietary period or contact PI | ||||
7 | FUV | Bonfond | HST/STIS | Timetag imaging of northern aurora | Observations successful | |||||
8 | visible/NUV/ near-IR | Wong (16913) | Hubble/ WFC3-UVIS | hi-resolution non-global snapshot | 2022 Sept 29 | now: https://mast.stsci.edu/search/ui/#/hst/results?&proposal_id=16913 https://doi.org/10.3847/1538-4365/ab775f future: https://archive.stsci.edu/hlsp/wfcj | Observations cancelled or unsuccessful | |||
9 | near IR (5 µm) | Wong | Gemini-N/NIRI | lucky imaging, 5-µm maps | 2022 Sept 30 | now: https://archive.gemini.edu/searchform/GN-2022B-Q-106 future: https://archive.stsci.edu/hlsp/wfcj | ||||
10 | UV, VIS, near-IR | Sanchez-Lavega | Planetcam, 2.2m Calar Alto Observatory | Observing Jupiter with new detectors (0.35-1 micron) & (1-1.6 micron) | 29 September | |||||
11 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | Nightly, weather permitting 20220928 20221019 20221002 20221020 20221003 20221021 20221004 20221025 20221011 20221026 20221012 20221027 20221013 20221028 20221014 20221029 20221018 20221030 | |||||
12 | visible/nearIR | Alexander, Irwin | VLT/MUSE - IFU | spectroscopic imaging, 475-930 nm to determine cloud structure and albedo spectrum of particles. | 18/19th September | Raw data publicly available to download from ESO portal this time next year. Standard calibration pipeline takes of the order of 1-3 days to complete. | ||||
13 | Visible & Near IR | Schmidt | Keck I Hires & Keck II NIRSPEC | Europa sputtered Na and K atmosphere. Jupiter at opposition, Europa flyby near transit. Plasma structure and composition of IPT H2/H3+ mapping of Jovian Aurora: northern oval velocity + global temperature (PJ45 @ 7:11) | 28 Sept | immediately available on KOA public archive: https://koa.ipac.caltech.edu/cgi-bin/KOA/nph-KOAlogin | ||||
14 | near IR | Bjoraker | IRTF/iSHELL | 5 micron spectra | 30 Sept UT | later | ||||
15 | near IR | Orton | IRTF/SpeX | filtered imaging and scanning spectroscopy between 1.58 and 5.1µm | filtered imaging obtained on September 28, 30 at high resolution (0.6" or better) and photometric nights. Also on October 14 with 1" seeing and thin cirrus. | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired. Reduced "quick-look" observations (geometrically but not radiometrically calibrated) will be available for immeduately use from the Juno-curated web site: http://junoirtf.space.swri.edu/ | ||||
16 | near IR | Orton | Gemini-N/NIRI | filtered near-infrared imaging of Jupiter, often with Adaptive-Optics (AO) stabilization. | ||||||
17 | mid IR | Orton | IRTF/MIRSI | filtered radiometric imaging and spectroscopy to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology and auroral heating and chemistry. | Observations made on September 27 with good diffraction-limited seeing and photometric weather. | Collaboration is possible with the investigators. | ||||
18 | radio | Zarka, Cecconi, Lamy, Louis | Nançay Decameter Array (France) | coordinated measurement of 10-40 MHz cyclotron radio emission | every day, 8 hours around the transition to local meridian | https://maser.lesia.obspm.fr/task-1-data-collections/juno-ground-radio/juno-ground-radio-nancay-decameter.html?lang=en | ||||
19 | Radio | Lamy for the NenuFar ES07 team | NenuFAR (France) | coordinated measurements of 10-40 MHz cyclotron radio emission at high time/frequency resolution | 2022/09/28T17:44:00 - 05:27:00 2022/09/29T17:39:00 - 05:23:00 2022/09/30T17:36:00 - 05:18:00 | Data available on demand to laurent.lamy@obspm.fr | ||||
20 | Radio (mm/sub-mm) | Tseng | SMA | Ground-based radio observations of Io around 335-367GHz | 26 Oct | Collaboration is possible with the investigators. | ||||
21 | ||||||||||
22 | Scheduled observations by Juno. | |||||||||
23 | ||||||||||
24 | Perijove is 2022 Sep 29, 17:11:30 SCET ( = UTC - light time). System-III longitude = 240.0°W | |||||||||
25 | ||||||||||
26 | Period: Orbit 45-EXT [GRAV] (2022 Sep 20 - 2022 Oct 31) | |||||||||
27 | Instrument | Description | ||||||||
28 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||
29 | MWR | |||||||||
30 | UVS | |||||||||
31 | JunoCam | |||||||||
32 | JIRAM | |||||||||
33 | ||||||||||
34 | ||||||||||
35 | ||||||||||
36 | ||||||||||
37 | ||||||||||
38 | ||||||||||
39 | ||||||||||
40 | ||||||||||
41 | ||||||||||
42 | ||||||||||
43 | ||||||||||
44 | ||||||||||
45 | ||||||||||
46 | ||||||||||
47 | ||||||||||
48 | ||||||||||
49 | ||||||||||
50 | ||||||||||
51 | ||||||||||
52 | ||||||||||
53 | ||||||||||
54 | ||||||||||
55 | ||||||||||
56 | ||||||||||
57 | Mosaic of JunoCam images by J. Rogers and G. Eichstaedt | |||||||||
58 | ||||||||||
59 | ||||||||||
60 | ||||||||||
61 | ||||||||||
62 | ||||||||||
63 | ||||||||||
64 | ||||||||||
65 | ||||||||||
66 | ||||||||||
67 | ||||||||||
68 | ||||||||||
69 | ||||||||||
70 | ||||||||||
71 | ||||||||||
72 | ||||||||||
73 | ||||||||||
74 | ||||||||||
75 | ||||||||||
76 | ||||||||||
77 | ||||||||||
78 | ||||||||||
79 | ||||||||||
80 | ||||||||||
81 | ||||||||||
82 | ||||||||||
83 | ||||||||||
84 | ||||||||||
85 | Composite of JIRAM M-band (5-micron) map. | |||||||||
86 | ||||||||||
87 | ||||||||||
88 | ||||||||||
89 | ||||||||||
90 | ||||||||||
91 | ||||||||||
92 | ||||||||||
93 | ||||||||||
94 | ||||||||||
95 | ||||||||||
96 | ||||||||||
97 | ||||||||||
98 | ||||||||||
99 | ||||||||||
100 | ||||||||||
101 | ||||||||||
102 | ||||||||||
103 | ||||||||||
104 | ||||||||||
105 | ||||||||||
106 | ||||||||||
107 | ||||||||||
108 | ||||||||||
109 | ||||||||||
110 | ||||||||||
111 | ||||||||||
112 | ||||||||||
113 | ||||||||||
114 | ||||||||||
115 | ||||||||||
116 | ||||||||||
117 | ||||||||||
118 | ||||||||||
119 | ||||||||||
120 | ||||||||||
121 | ||||||||||
122 | ||||||||||
123 | ||||||||||
124 | ||||||||||
125 | ||||||||||
126 | ||||||||||
127 | ||||||||||
128 | ||||||||||
129 | ||||||||||
130 | ||||||||||
131 | ||||||||||
132 | ||||||||||
133 | ||||||||||
134 | ||||||||||
135 | ||||||||||
136 | ||||||||||
137 | ||||||||||
138 | ||||||||||
139 | ||||||||||
140 | ||||||||||
141 | MWR footprints for the minimum emission angle at each spacecraft rotation. The cross marks the location of the perijove. | |||||||||
142 | ||||||||||
143 |
1 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed toward the Earth. This orbit is for an extended mission approved by NASA HQ. | ||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|
2 | The period has been defined as a week before perijove to a week before the subsequent perijove, unlike the mission-planning definition, which extends from a day before the perijove to a day after the perijove. | ||||||||||||
3 | Period: Orbit 44-EXT [GRAV] (2022 Aug 11 - 2022 Sep 20) | Observations requested. | |||||||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | Observations planned / granted time | ||||||
5 | FUV | Bonfond | HST/STIS | Timetag imaging of northern aurora | Aug 17 (22.229) from 17:18 to 18:05 | Publicly on MAST as soon as released by STScI | Observations successful | ||||||
6 | visible/NUV/ near-IR | Wong (16913) | Hubble/ WFC3-UVIS | hi-resolution non-global snapshot | 2022 Aug 16 | now: https://mast.stsci.edu/search/ui/#/hst/results?&proposal_id=16913 https://doi.org/10.3847/1538-4365/ab775f future: https://archive.stsci.edu/hlsp/wfcj | |||||||
7 | near IR (5 µm) | Wong | Gemini-N/NIRI | lucky imaging, 5-µm maps | 2022 Aug 17 | now: https://archive.gemini.edu/searchform/GN-2022A-Q-111 future: https://archive.stsci.edu/hlsp/wfcj | |||||||
8 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | Nightly, weather permitting (horrible monsoon) 20220905 20220915 20220906 20220916 20220907 20220918 20220908 | ||||||||
9 | Visible | Schmidt | Keck I HIRES | Europa O I line ratios in eclipse (2:15-4:07 visible): H2O vs O2 vs O diagnostic Plasma structure and composition of IPT | 17 Aug, morning | immediately available on KOA public archive: https://koa.ipac.caltech.edu/cgi-bin/KOA/nph-KOAlogin | |||||||
10 | Visible | de Pater | Keck I Hires | Jupiter | UT Aug. 15 + 16 | Avaliable after publication of student thesis | |||||||
11 | visible/nearIR | Alexander, Irwin | VLT/MUSE - IFU | spectroscopic imaging, 475-930 nm to determine cloud structure and albedo spectrum of particles. | 27th July, also have 30th July focused on GRS | Raw data publicly available to download from ESO portal this time next year. Standard calibration pipeline takes of the order of 1-3 days to complete. | |||||||
12 | near IR | Bjoraker | IRTF/iSHELL | high-resolution spectroscopy in the 5-micron region | August 16 | ||||||||
13 | near IR | Orton | IRTF/SpeX | filtered imaging and scanning spectroscopy between 1.58 and 5.1µm | observations made on August 17-18 in very good seeing conditions and photometric skies. Short imaging sequences were made on September 3 and 7. | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired. Reduced "quick-look" observations (geometrically but not radiometrically calibrated) will be available for immeduately use from the Juno-curated web site: http://junoirtf.space.swri.edu/ | |||||||
14 | near IR & mid IR | Fletcher & Hammel | JWST NIRSpec, MIRI | imaging and spectroscopy of Great Red Spot | August 14/15 | data available from MAST immediately | |||||||
15 | near IR | Schmidt | Keck II NIRSPEC | H2/H3+ mapping of Jovian Aurora (intensity, density, temperature, velocity) | 16 Aug, morning | immediately available on KOA public archive: https://koa.ipac.caltech.edu/cgi-bin/KOA/nph-KOAlogin | |||||||
16 | 5-mu spectroscopy | de Pater | Keck II Nirspec | Jupiter | UT Aug. 15 + 16 | Avaliable after publication student thesis | |||||||
17 | Mid-IR | Fletcher | VISIR | Jupiter | August 8th 08:36-09:40UT | ||||||||
18 | mid IR | Orton | IRTF/MIRSI | filtered radiometric imaging and spectroscopy to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology and auroral heating and chemistry. | Observations were made on August 14-15. | Collaboration is possible with the investigators. | |||||||
19 | radio | Zarka, Cecconi, Lamy, Louis | Nançay Decameter Array (France) | coordinated measurement of 10-40 MHz cyclotron radio emission | every day, 8 hours around the transition to local meridian | https://maser.lesia.obspm.fr/task-1-data-collections/juno-ground-radio/juno-ground-radio-nancay-decameter.html?lang=en | |||||||
20 | Radio | Lamy for the NenuFar ES07 team | NenuFAR (France) | coordinated measurements of 10-40 MHz cyclotron radio emission at high time/frequency resolution | 2022/08/13T20:54:00 - 08:42:00 2022/08/15T20:45:00 - 08:42:00 2022/08/16T20:41:00 - 08:42:00 2022/08/17T20:41:00 - 08:38:00 2022/08/18T20:41:00 - 08:34:00 | Data available on demand to laurent.lamy@obspm.fr | |||||||
21 | |||||||||||||
22 | Scheduled observations by Juno. | ||||||||||||
23 | |||||||||||||
24 | Perijove is 2022 Aug 17, 14:45:30 SCET ( = UTC - light time). System-III longitude = 158.9°W | ||||||||||||
25 | |||||||||||||
26 | Period: Orbit 44-EXT [GRAV] (2022 Aug 11 - 2022 Sep 20) | ||||||||||||
27 | Instrument | Description | |||||||||||
28 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | |||||||||||
29 | MWR | Paper Published during this time frame: | |||||||||||
30 | UVS | ||||||||||||
31 | JunoCam | Title: Solar Wind Driven Changes in Jupiter’s Emission | |||||||||||
32 | JIRAM | Author(s): Matuszewska, K; Velusamy, T, et. al., Aug 2022 | |||||||||||
33 | Discipline(s): Planetary And Exoplanetary Atmospheres, Interstellar and Heliospheric Physics | ||||||||||||
34 | |||||||||||||
35 | |||||||||||||
36 | |||||||||||||
37 | |||||||||||||
38 | |||||||||||||
39 | |||||||||||||
40 | |||||||||||||
41 | |||||||||||||
42 | |||||||||||||
43 | |||||||||||||
44 | |||||||||||||
45 | |||||||||||||
46 | |||||||||||||
47 | |||||||||||||
48 | |||||||||||||
49 | |||||||||||||
50 | |||||||||||||
51 | |||||||||||||
52 | |||||||||||||
53 | |||||||||||||
54 | |||||||||||||
55 | |||||||||||||
56 | |||||||||||||
57 | Color mosaic of JunoCam images by J. Rogers and G. Eichstaedt | ||||||||||||
58 | |||||||||||||
59 | |||||||||||||
60 | |||||||||||||
61 | |||||||||||||
62 | |||||||||||||
63 | |||||||||||||
64 | |||||||||||||
65 | |||||||||||||
66 | |||||||||||||
67 | |||||||||||||
68 | |||||||||||||
69 | |||||||||||||
70 | |||||||||||||
71 | |||||||||||||
72 | |||||||||||||
73 | |||||||||||||
74 | |||||||||||||
75 | |||||||||||||
76 | |||||||||||||
77 | |||||||||||||
78 | |||||||||||||
79 | |||||||||||||
80 | |||||||||||||
81 | |||||||||||||
82 | |||||||||||||
83 | |||||||||||||
84 | |||||||||||||
85 | |||||||||||||
86 | Composite of JIRAM M-band (5-micron) map. | ||||||||||||
87 | |||||||||||||
88 | |||||||||||||
89 | |||||||||||||
90 | |||||||||||||
91 | |||||||||||||
92 | |||||||||||||
93 | |||||||||||||
94 | |||||||||||||
95 | |||||||||||||
96 | |||||||||||||
97 | |||||||||||||
98 | |||||||||||||
99 | |||||||||||||
100 | |||||||||||||
101 | |||||||||||||
102 | |||||||||||||
103 | |||||||||||||
104 | |||||||||||||
105 | |||||||||||||
106 | |||||||||||||
107 | |||||||||||||
108 | |||||||||||||
109 | |||||||||||||
110 | |||||||||||||
111 | |||||||||||||
112 | |||||||||||||
113 | |||||||||||||
114 | |||||||||||||
115 | |||||||||||||
116 | |||||||||||||
117 | |||||||||||||
118 | |||||||||||||
119 | |||||||||||||
120 | |||||||||||||
121 | |||||||||||||
122 | |||||||||||||
123 | |||||||||||||
124 | |||||||||||||
125 | |||||||||||||
126 | |||||||||||||
127 | |||||||||||||
128 | |||||||||||||
129 | |||||||||||||
130 | |||||||||||||
131 | |||||||||||||
132 | |||||||||||||
133 | |||||||||||||
134 | |||||||||||||
135 | |||||||||||||
136 | |||||||||||||
137 | |||||||||||||
138 | |||||||||||||
139 | |||||||||||||
140 | |||||||||||||
141 | |||||||||||||
142 | |||||||||||||
143 | |||||||||||||
144 | |||||||||||||
145 | |||||||||||||
146 | |||||||||||||
147 | |||||||||||||
148 | |||||||||||||
149 | |||||||||||||
150 | |||||||||||||
151 | |||||||||||||
152 | |||||||||||||
153 | |||||||||||||
154 | |||||||||||||
155 | MWR footprints for the minimum emission angle at each spacecraft rotation. The cross marks the location of the perijove. |
1 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed toward the Earth. This orbit is for an extended mission approved by NASA HQ. | |||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
2 | The period has been defined as a week before perijove to a week before the subsequent perijove, unlike the mission-planning definition, which extends from a day before the perijove to a day after the perijove. | |||||||||||||
3 | Period: Orbit 43-EXT [GRAV] (2022 June 28 - 2022 Aug 11) | Observations requested. | ||||||||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | Observations planned / granted time | |||||||
5 | FUV | Bonfond | HST/STIS | Timetag imaging of northern aurora | July 4 (22.185) 12:43 to 13:29 | Publicly on MAST as soon as released by STScI | Observations successful | |||||||
6 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | Nightly, weather permitting 20220706 20220707 (horrible monsoon!) | |||||||||
7 | Visible | Schmidt | Keck I HIRES | Ganymede O I line ratios: H2O vs O2 vs O diagnostic, 23:58-2:53 eclipse visibility Plasma structure and composition of IPT | 04 Aug, morning | immediately available on KOA public archive: https://koa.ipac.caltech.edu/cgi-bin/KOA/nph-KOAlogin | ||||||||
8 | visible/nearIR | Alexander, Irwin | VLT/MUSE - IFU | spectroscopic imaging, 475-930 nm to determine cloud structure and albedo spectrum of particles. | 29th June | Raw data publicly available to download from ESO portal this time next year. Standard calibration pipeline takes of the order of 1-3 days to complete. | ||||||||
9 | near IR | Orton | IRTF/SpeX | filtered imaging and scanning spectroscopy between 1.58 and 5.1µm | observations made on July 8-9 in very good seeing conditions and photometric skies. Short imaging sequences were made on July 25-26. | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired. Reduced "quick-look" observations (geometrically but not radiometrically calibrated) will be available for immeduately use from the Juno-curated web site: http://junoirtf.space.swri.edu/ | ||||||||
10 | near IR | Orton | Gemini-N/NIRI | filtered near-infrared imaging of Jupiter, often with Adaptive-Optics (AO) stabilization. | No data during this time frame due to weather / equipment problems | avalable on request | ||||||||
11 | visible/NUV/ near-IR | Wong (16913) | Hubble/ WFC3-UVIS | hi-resolution non-global snapshot | 2022 July 5 | now: https://mast.stsci.edu/search/ui/#/hst/results?&proposal_id=16913 https://doi.org/10.3847/1538-4365/ab775f future: https://archive.stsci.edu/hlsp/wfcj | ||||||||
12 | near IR (5 µm) | Wong | Gemini-N/NIRI | lucky imaging, 5-µm maps | 4x 40-min full-disk mosaics 05 Jul 12:00 (PJ + 2 hr) 05 Jul 13:45 (west of PJ) 07 Jul 12:00 (east of PJ) 07 Jul 13:20 (PJ + 2 days) | NIRI offline (fault, coldhead warmed on june 21, offline until 15 aug) | ||||||||
13 | near IR (0.7 - 2.5, 2.9 - 5.2 μm) | Cartwright | IRTF/SpeX: SXD (0.8" slit), LXD_short (0.3"), LXD_long (0.3"). LXD modes cover JIRAM order sorting filter gap | Reflectance spectroscopy of Europa (E), Ganymede (G), and Callisto (C). SXD native R ~750 at 2.2 μm, native R ~2500 in LXD modes | July 15 (E), July 18 (E and G), July 24 (E), July 26 (G and C), July 27 (E and C), July 29 (E) | Contact PI - interested in collaborating with teams using Juno instruments to observe moons (especially JIRAM) | ||||||||
14 | mid IR | Orton | IRTF/MIRSI | filtered radiometric imaging and spectroscopy to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology and auroral heating and chemistry. | Observations made on July 10-11. July 10 and 11 had good seeing, but only July 10 had clear skies. Images were obtained on July 11 but not with trustworthy photometry. | Collaboration is possible with the investigators. | ||||||||
15 | near IR & mid IR | Stansberry | JWST NIRCam, NIRSpec, NIRISS imaging and spectroscopy + MIRI spectral imaging for engineering test pusposes | imaging and spectroscopy as a part of tests of JWST capabilities | July 3,4,14 | Data ultimatly avaialble from MAST. | ||||||||
16 | near IR | Bjoraker | IRTF/iSHELL | high-resolution spectroscopy in the 5-micron region | August 2 | |||||||||
17 | Mid IR | Fletcher | VISIR | Imaging | July 6th 08:19-09:25UT | |||||||||
18 | near IR & mid IR | de Pater | JWST NIRSpec, MIRI | imaging and spectroscopy of South Polar Region | window is June 2 to Aug 15 | data available from MAST immediately | ||||||||
19 | radio | Zarka, Cecconi, Lamy, Louis | Nançay Decameter Array (France) | coordinated measurement of 10-40 MHz cyclotron radio emission | every day, 8 hours around the transition to local meridian | https://maser.lesia.obspm.fr/task-1-data-collections/juno-ground-radio/juno-ground-radio-nancay-decameter.html?lang=en | ||||||||
20 | Radio | Lamy for the NenuFar ES07 team | NenuFAR (France) | coordinated measurements of 10-40 MHz cyclotron radio emission at high time/frequency resolution | 2022/07/03T23:32:00 - 11:34:00 2022/07/04T23:28:00 - 11:30:00 2022/07/05T23:28:00 - 11:27:00 2022/07/07T23:28:00 - 11:20:00 | Data available on demand to laurent.lamy@obspm.fr | ||||||||
21 | radio | Kreuser-Jenkins | DSS13 | Ground based radio observations of Jupiter using DSS13 via the GAVRT Program | June 30, July 1, July 7, July 21, July 25, July 26, July 27, Aug 3 | Raw data available upon request | ||||||||
22 | Radio (mm/sub-mm) | Tseng | SMA | Ground-based radio observations of Io around 335-367GHz | 16, 24, 30 June | Collaboration is possible with the investigators. | ||||||||
23 | Scheduled observations by Juno. | |||||||||||||
24 | ||||||||||||||
25 | ||||||||||||||
26 | Perijove is 2022 July 5, 9:17:20 SCET ( = UTC - light time). System-III longitude = 327.6°W | |||||||||||||
27 | ||||||||||||||
28 | Period: Orbit 43-EXT [GRAV] (2022 June 28 - 2022 Aug 11) | |||||||||||||
29 | Instrument | Description | ||||||||||||
30 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||||||
31 | MWR | |||||||||||||
32 | UVS | |||||||||||||
33 | JunoCam | |||||||||||||
34 | JIRAM | |||||||||||||
35 | ||||||||||||||
36 | ||||||||||||||
37 | ||||||||||||||
38 | ||||||||||||||
39 | ||||||||||||||
40 | ||||||||||||||
41 | ||||||||||||||
42 | ||||||||||||||
43 | ||||||||||||||
44 | ||||||||||||||
45 | ||||||||||||||
46 | ||||||||||||||
47 | ||||||||||||||
48 | ||||||||||||||
49 | ||||||||||||||
50 | ||||||||||||||
51 | ||||||||||||||
52 | ||||||||||||||
53 | ||||||||||||||
54 | ||||||||||||||
55 | ||||||||||||||
56 | ||||||||||||||
57 | ||||||||||||||
58 | ||||||||||||||
59 | ||||||||||||||
60 | ||||||||||||||
61 | ||||||||||||||
62 | ||||||||||||||
63 | ||||||||||||||
64 | Planned coverage by JIRAM M-band. | |||||||||||||
65 | ||||||||||||||
66 | ||||||||||||||
67 | ||||||||||||||
68 | ||||||||||||||
69 | ||||||||||||||
70 | ||||||||||||||
71 | ||||||||||||||
72 | ||||||||||||||
73 | ||||||||||||||
74 | ||||||||||||||
75 | ||||||||||||||
76 | ||||||||||||||
77 | ||||||||||||||
78 | ||||||||||||||
79 | ||||||||||||||
80 | ||||||||||||||
81 | ||||||||||||||
82 | ||||||||||||||
83 | ||||||||||||||
84 | ||||||||||||||
85 | ||||||||||||||
86 | ||||||||||||||
87 | ||||||||||||||
88 | ||||||||||||||
89 | Color composite of JunoCam observations on PJ43 -John Rogers and Gerald Eichstaedt | |||||||||||||
90 | ||||||||||||||
91 | ||||||||||||||
92 | ||||||||||||||
93 | ||||||||||||||
94 | ||||||||||||||
95 | ||||||||||||||
96 | ||||||||||||||
97 | ||||||||||||||
98 | ||||||||||||||
99 | ||||||||||||||
100 | ||||||||||||||
101 | ||||||||||||||
102 | ||||||||||||||
103 | ||||||||||||||
104 | ||||||||||||||
105 | ||||||||||||||
106 | ||||||||||||||
107 | ||||||||||||||
108 | ||||||||||||||
109 | ||||||||||||||
110 | ||||||||||||||
111 | ||||||||||||||
112 | ||||||||||||||
113 | ||||||||||||||
114 | ||||||||||||||
115 | ||||||||||||||
116 | ||||||||||||||
117 | ||||||||||||||
118 | ||||||||||||||
119 | ||||||||||||||
120 | ||||||||||||||
121 | ||||||||||||||
122 | ||||||||||||||
123 | ||||||||||||||
124 | ||||||||||||||
125 | ||||||||||||||
126 | ||||||||||||||
127 | ||||||||||||||
128 | ||||||||||||||
129 | ||||||||||||||
130 | ||||||||||||||
131 | ||||||||||||||
132 | ||||||||||||||
133 | ||||||||||||||
134 | ||||||||||||||
135 | ||||||||||||||
136 | ||||||||||||||
137 | ||||||||||||||
138 | ||||||||||||||
139 | ||||||||||||||
140 | ||||||||||||||
141 | ||||||||||||||
142 | ||||||||||||||
143 | ||||||||||||||
144 | ||||||||||||||
145 | ||||||||||||||
146 | ||||||||||||||
147 | ||||||||||||||
148 | ||||||||||||||
149 | ||||||||||||||
150 | ||||||||||||||
151 | ||||||||||||||
152 | ||||||||||||||
153 | ||||||||||||||
154 | ||||||||||||||
155 | ||||||||||||||
156 | ||||||||||||||
157 | MWR footprints for the minimum emission angle at each spacecraft rotation. The cross marks the location of the perijove. | |||||||||||||
158 | ||||||||||||||
159 |
1 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed toward the Earth. This orbit is for an extended mission approved by NASA HQ. | |||||||||
---|---|---|---|---|---|---|---|---|---|---|
2 | The period has been defined as a week before perijove to a week before the subsequent perijove, unlike the mission-planning definition, which extends from a day before the perijove to a day after the perijove. | |||||||||
3 | Period: Orbit 42-EXT [GRAV] (2022 May 18 - 2022 June 28) | Observations requested. | ||||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | Observations planned / granted time | |||
5 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | Nightly, weather permitting 20220520 20220603 20220521 20220604 20220522 20220605 20220523 20220606 20220524 20220607 20220525 20220608 20220526 20220609 20220527 20220613 20220528 20220614 20220529 20220615 20220530 20220616 20220531 20220618 20220601 20220619 20220602 | |||||
6 | visible/NUV/ near-IR | Wong (16913) | Hubble/ WFC3-UVIS | hi-resolution non-global snapshot | 2022 May 21 | now: https://mast.stsci.edu/search/ui/#/hst/results?&proposal_id=16913 https://doi.org/10.3390/rs15030702 https://doi.org/10.3847/1538-4365/ab775f future: https://archive.stsci.edu/hlsp/wfcj | ||||
7 | visible/nearIR | Alexander, Irwin | VLT/MUSE - IFU | spectroscopic imaging, 475-930 nm to determine cloud structure and albedo spectrum of particles. | Dates near PJ42 requested. Unsuccessful due to tight scheduling constraints | Raw data publicly available to download from ESO portal this time next year. Standard calibration pipeline takes of the order of 1-3 days to complete. | ||||
8 | near IR | Orton | IRTF/SpeX. | Filtered imaging and scanning spectroscopy between 1.58 and 5.1µm. scanned spectral imaging. | Imaging and spectroscopic observations were taken on May 21-22, with short imaging sequences on June 11-12. | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired. Reduced "quick-look" observations (geometrically but not radiometrically calibrated) will be available for immeduately use from the Juno-curated web site: http://junoirtf.space.swri.edu/ | ||||
9 | near IR | Orton | Gemini-N/NIRI | filtered near-infrared imaging of Jupiter, often with Adaptive-Optics (AO) stabilization. | Observations obtained on June 4, 16 and 20. | avalable on request | ||||
10 | mid IR | Orton | IRTF/MIRSI | filtered radiometric imaging and spectroscopy to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology and auroral heating and chemistry. | IRTF is offering this instrument in "shared risk" mode. Observations on May 23-24 were successful. | Collaboration is possible with the investigators. | ||||
11 | near IR (5 µm) | Wong | Gemini-N/NIRI | lucky imaging, 5-µm maps | 2x 30-min full-disk mosaics 23 May 14:20 (PJ + 1 rot) 28 May 14:00 (PJ + 5 days) | now: https://archive.gemini.edu/searchform/GN-2021B-Q-110 https://doi.org/10.3390/rs15030702 https://doi.org/10.3847/1538-4365/ab775f future: https://archive.stsci.edu/hlsp/wfcj | ||||
12 | near IR & mid IR | Fletcher & Hammel | JWST NIRSpec, MIRI | imaging and spectroscopy of Great Red Spot | Partial images on June 27, replacement images made on Aug 15 | data available from MAST immediately | ||||
13 | near IR & mid IR | de Pater | JWST NIRSpec, MIRI | imaging and spectroscopy of South Polar Region | June 27 | data available from MAST immediately | ||||
14 | radio | Zarka, Cecconi, Lamy, Louis | Nançay Decameter Array (France) | coordinated measurement of 10-40 MHz cyclotron radio emission | every day, 8 hours around the transition to local meridian | https://maser.lesia.obspm.fr/task-1-data-collections/juno-ground-radio/juno-ground-radio-nancay-decameter.html?lang=en | ||||
15 | Radio | Lamy for the NenuFar ES07 team | NenuFAR (France) | coordinated measurements of 10-40 MHz cyclotron radio emission at high time/frequency resolution | 2022/05/23T02:05:00 - 09:00:00 2022/05/24T02:02:00 - 13:47:00 2022/05/25T02:00:00 - 13:44:00 | Data available on demand to laurent.lamy@obspm.fr | ||||
16 | radio | Kreuser-Jenkins | SMA | Ground based radio observations of Jupiter using DSS13 via the GAVRT Program | June 16, June 24 | Raw data available upon request | ||||
17 | radio (mm/sub-mm) | Tseng | ||||||||
18 | ||||||||||
19 | Scheduled observations by Juno. | |||||||||
20 | ||||||||||
21 | Perijove is 2022 May 23, 2:15:47 SCET ( = UTC - light time). System-III longitude = 80.0°W | |||||||||
22 | ||||||||||
23 | Period: Orbit 42-EXT [GRAV] (2022 May 18 - 2022 June 28) | |||||||||
24 | Instrument | Description | ||||||||
25 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||
26 | MWR | |||||||||
27 | UVS | |||||||||
28 | JunoCam | |||||||||
29 | JIRAM | |||||||||
30 | ||||||||||
31 | ||||||||||
32 | ||||||||||
33 | ||||||||||
34 | ||||||||||
35 | ||||||||||
36 | ||||||||||
37 | ||||||||||
38 | ||||||||||
39 | ||||||||||
40 | ||||||||||
41 | ||||||||||
42 | ||||||||||
43 | ||||||||||
44 | ||||||||||
45 | ||||||||||
46 | ||||||||||
47 | ||||||||||
48 | ||||||||||
49 | ||||||||||
50 | ||||||||||
51 | ||||||||||
52 | ||||||||||
53 | ||||||||||
54 | ||||||||||
55 | ||||||||||
56 | Color composite of JunoCam images at PJ42 by John Rogers and Gerald Eichstaedt | |||||||||
57 | ||||||||||
58 | ||||||||||
59 | ||||||||||
60 | ||||||||||
61 | ||||||||||
62 | ||||||||||
63 | ||||||||||
64 | ||||||||||
65 | ||||||||||
66 | ||||||||||
67 | ||||||||||
68 | ||||||||||
69 | ||||||||||
70 | ||||||||||
71 | ||||||||||
72 | ||||||||||
73 | ||||||||||
74 | ||||||||||
75 | ||||||||||
76 | ||||||||||
77 | ||||||||||
78 | ||||||||||
79 | ||||||||||
80 | ||||||||||
81 | ||||||||||
82 | ||||||||||
83 | ||||||||||
84 | ||||||||||
85 | ||||||||||
86 | ||||||||||
87 | ||||||||||
88 | ||||||||||
89 | ||||||||||
90 | ||||||||||
91 | ||||||||||
92 | ||||||||||
93 | ||||||||||
94 | ||||||||||
95 | ||||||||||
96 | ||||||||||
97 | ||||||||||
98 | ||||||||||
99 | ||||||||||
100 | ||||||||||
101 | ||||||||||
102 | ||||||||||
103 | ||||||||||
104 | ||||||||||
105 | ||||||||||
106 | ||||||||||
107 | ||||||||||
108 | ||||||||||
109 | ||||||||||
110 | ||||||||||
111 | ||||||||||
112 | ||||||||||
113 | ||||||||||
114 | ||||||||||
115 | ||||||||||
116 | ||||||||||
117 | ||||||||||
118 | ||||||||||
119 | ||||||||||
120 | ||||||||||
121 | ||||||||||
122 | ||||||||||
123 | ||||||||||
124 | ||||||||||
125 | ||||||||||
126 | MWR footprints for the minimum emission angle at each spacecraft rotation. The cross marks the location of the perijove. | |||||||||
127 | ||||||||||
128 |
1 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed toward the Earth. This orbit is for an extended mission approved by NASA HQ. | |||||||||
---|---|---|---|---|---|---|---|---|---|---|
2 | The period has been defined as a week before perijove to a week before the subsequent perijove, unlike the mission-planning definition, which extends from a day before the perijove to a day after the perijove. | |||||||||
3 | Period: Orbit 41-EXT [GRAV] (2022 Apr 2 - 2022 May 18) | Observations requested. | ||||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | Observations planned / granted time | |||
5 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | Nightly, weather permitting (too early in opposition) | |||||
6 | near infrared | Kim, Sang-Joon | Gemini-N/GNIRS | CH4 non-LTE aurora | 13:41-14:21 (UT) 30 May | |||||
7 | IRTF/SpeX | filtered imaging and scanning spectroscopy between 1.58 and 5.1µm | Filtered imaging and scanning spectroscopy between 1.58 and 5.1µm on April 8-9, with shorter imaging sequences on April 29-30 | filtered imaging and scanning spectroscopy between 1.58 and 5.1µm | Data obtained on 6-hour sequences on April 8 and 9, and ~45-min sequences on April 29 and 30. All were obtained in partially cloudy and overcast weather. | raw images avaialble immediate from IRTF web site; fully reduced images available wtihint a month or sooner, as desired. Reduced "quick-look" observations (geometrically but not radiometrically calibrated) will be availablefor immedate use from the Juno-curated web site: http://junoirtf.space.swri.edu/ | ||||
8 | mid IR | Orton | IRTF/MIRSI | filtered radiometric imaging and spectroscopy to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology and auroral heating and chemistry. | IRTF is offering this instrument in "shared risk" mode. Observations made on April 10-11 during non-ideal weather conditions. | Collaboration is possible with the investigators. | ||||
9 | radio | Zarka, Cecconi, Lamy, Louis | Nançay Decameter Array (France) | coordinated measurement of 10-40 MHz cyclotron radio emission | every day, 8 hours around the transition to local meridian | https://maser.lesia.obspm.fr/task-1-data-collections/juno-ground-radio/juno-ground-radio-nancay-decameter.html?lang=en | ||||
10 | Radio | Lamy for the NenuFar ES07 team | NenuFAR (France) | coordinated measurements of 10-40 MHz cyclotron radio emission at high time/frequency resolution | 2022/04/07T04:47:00 - 16:00:00 2022/04/08T04:44:00 - 15:57:00 2022/04/09T05:00:00 - 15:55:00 2022/04/10T04:38:00 - 15:52:00 2022/04/25T05:36:00 - 08:07:00 2022/05/16T07:51:00 - 12:18:00 2022/05/17T11:00:00 - 13:40:00 | Data available on demand to laurent.lamy@obspm.fr | ||||
11 | ||||||||||
12 | ||||||||||
13 | ||||||||||
14 | ||||||||||
15 | ||||||||||
16 | Scheduled observations by Juno. | |||||||||
17 | ||||||||||
18 | Perijove is 2022 Apr 9, 15:49:13 SCET ( = UTC - light time). System-III longitude = 68.5°W | |||||||||
19 | ||||||||||
20 | Period: Orbit 41-EXT [GRAV] (2022 Apr 2 - 2022 May 18) | |||||||||
21 | Instrument | |||||||||
22 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||
23 | MWR | |||||||||
24 | UVS | |||||||||
25 | JunoCam | |||||||||
26 | JIRAM | |||||||||
27 | ||||||||||
28 | ||||||||||
29 | ||||||||||
30 | ||||||||||
31 | ||||||||||
32 | ||||||||||
33 | ||||||||||
34 | ||||||||||
35 | ||||||||||
36 | ||||||||||
37 | ||||||||||
38 | ||||||||||
39 | ||||||||||
40 | ||||||||||
41 | ||||||||||
42 | ||||||||||
43 | ||||||||||
44 | ||||||||||
45 | ||||||||||
46 | ||||||||||
47 | ||||||||||
48 | ||||||||||
49 | ||||||||||
50 | ||||||||||
51 | ||||||||||
52 | ||||||||||
53 | ||||||||||
54 | ||||||||||
55 | ||||||||||
56 | ||||||||||
57 | ||||||||||
58 | ||||||||||
59 | Atmospheric coverage by the JIRAM M-band (5-micron channel) | |||||||||
60 | ||||||||||
61 | ||||||||||
62 | ||||||||||
63 | ||||||||||
64 | ||||||||||
65 | ||||||||||
66 | ||||||||||
67 | ||||||||||
68 | ||||||||||
69 | ||||||||||
70 | ||||||||||
71 | ||||||||||
72 | ||||||||||
73 | ||||||||||
74 | ||||||||||
75 | ||||||||||
76 | ||||||||||
77 | ||||||||||
78 | ||||||||||
79 | ||||||||||
80 | ||||||||||
81 | ||||||||||
82 | ||||||||||
83 | Composite of JunoCam coverage of Jupiter's atmosphere in cylindrical map form for PJ41 by John Rogers and Gerald Eichstaedt | |||||||||
84 | ||||||||||
85 | ||||||||||
86 | ||||||||||
87 | ||||||||||
88 | ||||||||||
89 | ||||||||||
90 | ||||||||||
91 | ||||||||||
92 | ||||||||||
93 | ||||||||||
94 | ||||||||||
95 | ||||||||||
96 | ||||||||||
97 | ||||||||||
98 | ||||||||||
99 | ||||||||||
100 | ||||||||||
101 | ||||||||||
102 | ||||||||||
103 | ||||||||||
104 | ||||||||||
105 | ||||||||||
106 | ||||||||||
107 | ||||||||||
108 | ||||||||||
109 | ||||||||||
110 | ||||||||||
111 | ||||||||||
112 | ||||||||||
113 | ||||||||||
114 | ||||||||||
115 | ||||||||||
116 | ||||||||||
117 | ||||||||||
118 | ||||||||||
119 | ||||||||||
120 | ||||||||||
121 | ||||||||||
122 | ||||||||||
123 | ||||||||||
124 | ||||||||||
125 | ||||||||||
126 | ||||||||||
127 | ||||||||||
128 | ||||||||||
129 | ||||||||||
130 | ||||||||||
131 | ||||||||||
132 | ||||||||||
133 | ||||||||||
134 | ||||||||||
135 | ||||||||||
136 | ||||||||||
137 | ||||||||||
138 | ||||||||||
139 | ||||||||||
140 | ||||||||||
141 | ||||||||||
142 | ||||||||||
143 | ||||||||||
144 | ||||||||||
145 | ||||||||||
146 | ||||||||||
147 | ||||||||||
148 | ||||||||||
149 | ||||||||||
150 | ||||||||||
151 | ||||||||||
152 | ||||||||||
153 | ||||||||||
154 | ||||||||||
155 | ||||||||||
156 | ||||||||||
157 | ||||||||||
158 | ||||||||||
159 | ||||||||||
160 | ||||||||||
161 | ||||||||||
162 | ||||||||||
163 | ||||||||||
164 | MWR footprints for the minimum emission angle at each spacecraft rotation. The cross marks the location of the perijove. | |||||||||
165 | ||||||||||
166 | ||||||||||
167 |
1 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed toward the Earth. This orbit is for an extended mission approved by NASA HQ. | |||||||||
---|---|---|---|---|---|---|---|---|---|---|
2 | The period has been defined as a week before perijove to a week before the subsequent perijove, unlike the mission-planning definition, which extends from a day before the perijove to a day after the perijove. | |||||||||
3 | Period: Orbit 40-EXT [GRAV] (2022 Feb 19 - 2022 Apr 2) | Observations requested. | ||||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | Observations planned / granted time | |||
5 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | Nightly, weather permitting (mechanical problems fixed!) but too early in opposition | |||||
6 | radio | Zarka, Cecconi, Lamy, Louis | Nançay Decameter Array (France) | coordinated measurement of 10-40 MHz cyclotron radio emission | every day, 8 hours around the transition to local meridian | https://maser.lesia.obspm.fr/task-1-data-collections/juno-ground-radio/juno-ground-radio-nancay-decameter.html?lang=en | ||||
7 | Radio | Lamy for the NenuFar ES07 team | NenuFAR (France) | coordinated measurements of 10-40 MHz cyclotron radio emission at high time/frequency resolution | 2022/02/23T07:16:00 - 17:53:00 2022/02/24T07:12:00 - 17:51:00 2022/02/25T07:09:00 - 10:00:00 2022/02/25T10:00:00 - 17:49:00 2022/02/26T07:06:00 - 17:47:00 2022/02/27T07:02:00 - 17:44:00 | Data available on demand to laurent.lamy@obspm.fr | ||||
8 | ||||||||||
9 | ||||||||||
10 | ||||||||||
11 | ||||||||||
12 | ||||||||||
13 | ||||||||||
14 | ||||||||||
15 | Scheduled observations by Juno. | |||||||||
16 | ||||||||||
17 | Perijove is 2022 Feb 25 1:58:52 SCET ( = UTC - light time). System-III longitude = 293.9°W | |||||||||
18 | ||||||||||
19 | Period: Orbit 40-EXT [GRAV] (2022 Feb 19 - 2022 Apr 2) | |||||||||
20 | Instrument | Description | ||||||||
21 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||
22 | MWR | |||||||||
23 | UVS | |||||||||
24 | JunoCam | |||||||||
25 | JIRAM | |||||||||
26 | ||||||||||
27 | ||||||||||
28 | ||||||||||
29 | ||||||||||
30 | ||||||||||
31 | ||||||||||
32 | ||||||||||
33 | ||||||||||
34 | ||||||||||
35 | ||||||||||
36 | ||||||||||
37 | ||||||||||
38 | ||||||||||
39 | ||||||||||
40 | ||||||||||
41 | ||||||||||
42 | ||||||||||
43 | ||||||||||
44 | ||||||||||
45 | ||||||||||
46 | ||||||||||
47 | ||||||||||
48 | ||||||||||
49 | ||||||||||
50 | ||||||||||
51 | ||||||||||
52 | ||||||||||
53 | ||||||||||
54 | ||||||||||
55 | ||||||||||
56 | ||||||||||
57 | ||||||||||
58 | ||||||||||
59 | Atmospheric coverage by the JIRAM M-band (5-micron channel) | |||||||||
60 | ||||||||||
61 | ||||||||||
62 | ||||||||||
63 | ||||||||||
64 | ||||||||||
65 | ||||||||||
66 | ||||||||||
67 | ||||||||||
68 | ||||||||||
69 | ||||||||||
70 | ||||||||||
71 | ||||||||||
72 | ||||||||||
73 | ||||||||||
74 | ||||||||||
75 | ||||||||||
76 | ||||||||||
77 | ||||||||||
78 | ||||||||||
79 | ||||||||||
80 | ||||||||||
81 | ||||||||||
82 | ||||||||||
83 | Composite of JunoCam coverage of Jupiter's atmosphere in cylindrical map form. by John Rogers and Gerald Eichstaedt | |||||||||
84 | ||||||||||
85 | ||||||||||
86 | ||||||||||
87 | ||||||||||
88 | ||||||||||
89 | ||||||||||
90 | ||||||||||
91 | ||||||||||
92 | ||||||||||
93 | ||||||||||
94 | ||||||||||
95 | ||||||||||
96 | ||||||||||
97 | ||||||||||
98 | ||||||||||
99 | ||||||||||
100 | ||||||||||
101 | ||||||||||
102 | ||||||||||
103 | ||||||||||
104 | ||||||||||
105 | ||||||||||
106 | ||||||||||
107 | ||||||||||
108 | ||||||||||
109 | ||||||||||
110 | ||||||||||
111 | ||||||||||
112 | ||||||||||
113 | ||||||||||
114 | ||||||||||
115 | ||||||||||
116 | ||||||||||
117 | ||||||||||
118 | ||||||||||
119 | ||||||||||
120 | ||||||||||
121 | ||||||||||
122 | ||||||||||
123 | ||||||||||
124 | ||||||||||
125 | ||||||||||
126 | ||||||||||
127 | ||||||||||
128 | ||||||||||
129 | ||||||||||
130 | ||||||||||
131 | ||||||||||
132 | ||||||||||
133 | ||||||||||
134 | ||||||||||
135 | ||||||||||
136 | ||||||||||
137 | ||||||||||
138 | ||||||||||
139 | ||||||||||
140 | ||||||||||
141 | ||||||||||
142 | ||||||||||
143 | ||||||||||
144 | ||||||||||
145 | ||||||||||
146 | ||||||||||
147 | ||||||||||
148 | ||||||||||
149 | ||||||||||
150 | ||||||||||
151 | ||||||||||
152 | ||||||||||
153 | ||||||||||
154 | ||||||||||
155 | ||||||||||
156 | ||||||||||
157 | ||||||||||
158 | ||||||||||
159 | ||||||||||
160 | ||||||||||
161 | ||||||||||
162 | ||||||||||
163 | ||||||||||
164 | ||||||||||
165 | ||||||||||
166 | ||||||||||
167 | ||||||||||
168 | ||||||||||
169 | ||||||||||
170 | ||||||||||
171 | ||||||||||
172 | ||||||||||
173 | ||||||||||
174 | ||||||||||
175 | ||||||||||
176 | ||||||||||
177 | ||||||||||
178 | MWR footprints for the minimum emission angle at each spacecraft rotation. The cross marks the location of the perijove. | |||||||||
179 |
1 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed toward the Earth. This orbit is for an extended mission approved by NASA HQ. | |||||||||
---|---|---|---|---|---|---|---|---|---|---|
2 | The period has been defined as a week before perijove to a week before the subsequent perijove, unlike the mission-planning definition, which extends from a day before the perijove to a day after the perijove. | |||||||||
3 | Period: Orbit 39-EXT [GRAV] (2022 Jan 7 - 2022 Feb 19) | Observations requested. | ||||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | Observations planned / granted time | |||
5 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | Mechanical problems | |||||
6 | near IR | Orton | IRTF/SpeX | filtered imaging and scanning spectroscopy between 1.58 and 5.1µm | Observations in support of PJ39, observed on Jan 13-14 with only partial success, due to proximity to sun, seeing and sky conditions | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired. Reduced "quick-look" observations (geometrically but not radiometrically calibrated) will be available for immeduately use from the Juno-curated web site: http://junoirtf.space.swri.edu/ | ||||
7 | near IR | Orton | Gemini-N/NIRI | filtered near-infrared imaging of Jupiter; adaptive-optics stabilization has been requested, if working. | observations requested near PJ39 | avalable on request | ||||
8 | ||||||||||
9 | radio | Zarka, Cecconi, Lamy, Louis | Nançay Decameter Array (France) | coordinated measurement of 10-40 MHz cyclotron radio emission | every day, 8 hours around the transition to local meridian | https://maser.lesia.obspm.fr/task-1-data-collections/juno-ground-radio/juno-ground-radio-nancay-decameter.html?lang=en | ||||
10 | Radio | Lamy for the NenuFar ES07 team | NenuFAR (France) | coordinated measurements of 10-40 MHz cyclotron radio emission at high time/frequency resolution | Jan. 11 16:15 - 19:48; Jan. 12 09:41 - 19:46; Jan. 13 09:38 - 19:43 | Data available on demand to laurent.lamy@obspm.fr | ||||
11 | ||||||||||
12 | ||||||||||
13 | ||||||||||
14 | ||||||||||
15 | Scheduled observations by Juno. | |||||||||
16 | ||||||||||
17 | Perijove is 2022 Jan 12, 10:32:56 SCET ( = UTC - light time). System-III longitude = 101.5°W | |||||||||
18 | ||||||||||
19 | Period: Orbit 39-EXT [GRAV] (2022 Jan 7 - 2022 Feb 19) | |||||||||
20 | Instrument | Description | ||||||||
21 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||
22 | MWR | |||||||||
23 | UVS | |||||||||
24 | JunoCam | |||||||||
25 | JIRAM | |||||||||
26 | ||||||||||
27 | ||||||||||
28 | ||||||||||
29 | ||||||||||
30 | ||||||||||
31 | ||||||||||
32 | ||||||||||
33 | ||||||||||
34 | ||||||||||
35 | ||||||||||
36 | ||||||||||
37 | ||||||||||
38 | ||||||||||
39 | ||||||||||
40 | ||||||||||
41 | ||||||||||
42 | ||||||||||
43 | ||||||||||
44 | ||||||||||
45 | ||||||||||
46 | ||||||||||
47 | ||||||||||
48 | ||||||||||
49 | Atmospheric coverage by the JIRAM M-band (5-micron channel) | |||||||||
50 | ||||||||||
51 | ||||||||||
52 | ||||||||||
53 | ||||||||||
54 | ||||||||||
55 | ||||||||||
56 | ||||||||||
57 | ||||||||||
58 | ||||||||||
59 | ||||||||||
60 | ||||||||||
61 | ||||||||||
62 | ||||||||||
63 | ||||||||||
64 | ||||||||||
65 | ||||||||||
66 | ||||||||||
67 | ||||||||||
68 | ||||||||||
69 | ||||||||||
70 | ||||||||||
71 | ||||||||||
72 | ||||||||||
73 | ||||||||||
74 | ||||||||||
75 | Composite of JunoCam coverage of Jupiter's atmosphere in cylindrical map form. by John Rogers and Gerald Eichstaedt | |||||||||
76 | ||||||||||
77 | ||||||||||
78 | ||||||||||
79 | ||||||||||
80 | ||||||||||
81 | ||||||||||
82 | ||||||||||
83 | ||||||||||
84 | ||||||||||
85 | ||||||||||
86 | ||||||||||
87 | ||||||||||
88 | ||||||||||
89 | ||||||||||
90 | ||||||||||
91 | ||||||||||
92 | ||||||||||
93 | ||||||||||
94 | ||||||||||
95 | ||||||||||
96 | ||||||||||
97 | ||||||||||
98 | ||||||||||
99 | ||||||||||
100 | ||||||||||
101 | ||||||||||
102 | ||||||||||
103 | ||||||||||
104 | ||||||||||
105 | ||||||||||
106 | ||||||||||
107 | ||||||||||
108 | ||||||||||
109 | ||||||||||
110 | ||||||||||
111 | ||||||||||
112 | ||||||||||
113 | ||||||||||
114 | ||||||||||
115 | ||||||||||
116 | ||||||||||
117 | ||||||||||
118 | ||||||||||
119 | ||||||||||
120 | ||||||||||
121 | ||||||||||
122 | ||||||||||
123 | ||||||||||
124 | ||||||||||
125 | ||||||||||
126 | ||||||||||
127 | ||||||||||
128 | ||||||||||
129 | ||||||||||
130 | ||||||||||
131 | ||||||||||
132 | ||||||||||
133 | ||||||||||
134 | ||||||||||
135 | ||||||||||
136 | ||||||||||
137 | ||||||||||
138 | ||||||||||
139 | ||||||||||
140 | ||||||||||
141 | ||||||||||
142 | ||||||||||
143 | MWR footprints for the minimum emission angle at each spacecraft rotation. The cross marks the location of the perijove. | |||||||||
144 |
1 | Note: On this orbit the spacecraft orientation will be turned by 30 degrees to accomodate extensive mapping by the JIRAM instrument, which will benefit remote sensing in general. This orbit is for an extended mission approved by NASA HQ. | ||||||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
2 | The period has been defined as a week before perijove to a week before the subsequent perijove, unlike the mission-planning definition, which extends from a day before the perijove to a day after the perijove. | ||||||||||||||||
3 | Period: Orbit 38-EXT [GRAV] (2021 Nov 22 - 2022 Jan 7) | Observations requested. | |||||||||||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | Observations planned / granted time | ||||||||||
5 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | Mechanical problems | ||||||||||||
6 | Visible/near IR | Alexander/Irwin | VLT/MUSE - IFU | spectroscopic imaging, 465-930 nm to determine cloud structure and albedo spectrum of particles. | 14/15th December | Raw data publicly available to download from ESO portal. | |||||||||||
7 | near IR | Orton | IRTF/SpeX | filtered imaging and scanning spectroscopy between 1.58 and 5.1µm | Observations in support of PJ38 on Nov 30 - Dec 1 were wiped out comletely by bad weather. Short sequences of imaging on December 17 and 18 were successful but amid high humidity, clouds and fog. | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired. Reduced "quick-look" observations (geometrically but not radiometrically calibrated) will be available for immeduately use from the Juno-curated web site: http://junoirtf.space.swri.edu/ | |||||||||||
8 | near IR | Orton | Gemini-N/NIRI | filtered near-infrared imaging of Jupiter; adaptive-optics stabilization has been requested, if working. | Observations scheduled near PJ38 were successful only on December 10. | available on request | |||||||||||
9 | mid-IR | Fletcher | VLT/VISIR | Filtered imaging 5-20 µm, including lucky imaging at 5 µm. | Acquired northern and southern maps, plus M-band burst, 2021-11-26 | Available on request. | |||||||||||
10 | radio | Imai | Long Wavelength Array station 1 (LWA-1), LWA-Sevilleta (LWA-SV) | Jupiter's decametric auroral radio observations | November 22, 23 December 10, 16, 17, 23, 24 | Low-resolution LWA1 data are freely accessible via Autoplot (http://autoplot.org) by accepting the data usage policy (http://space.physics.uiowa.edu/earth/datapolicy.html) More information can be found at http://space.physics.uiowa.edu/earth/ | |||||||||||
11 | Radio | Kreuser-Jenkins | DSS-13 | ground based radio observations of Jupiter using DSS13 via the GAVRT Program | 11/22/2021, 11/29/2021, 12/2/2021 | Raw data available upon request | |||||||||||
12 | radio | Zarka, Cecconi, Lamy, Louis | Nançay Decameter Array (France) | coordinated measurement of 10-40 MHz cyclotron radio emission | every day, 8 hours around the transition to local meridian | https://maser.lesia.obspm.fr/task-1-data-collections/juno-ground-radio/juno-ground-radio-nancay-decameter.html?lang=en | |||||||||||
13 | Radio | Lamy for the NenuFar ES07 team | NenuFAR (France) | coordinated measurements of 10-40 MHz cyclotron radio emission at high time/frequency resolution | Nov. 28 12:45 - 22:00; Nov. 29 12:42 - 21:57; Nov. 30 12:39 - 21:53; Nov. 30 13:04 - 16:11; Nov. 30 14:51 - 16:11; Nov. 30 16:19 - 21:53 | Data available on demand to laurent.lamy@obspm.fr | |||||||||||
14 | |||||||||||||||||
15 | Scheduled observations by Juno. | ||||||||||||||||
16 | |||||||||||||||||
17 | Perijove is 2021 Nov 29, 14:13:26 SCET ( = UTC - light time). System-III longitude = 91.7°W | ||||||||||||||||
18 | |||||||||||||||||
19 | Period: Orbit 38-EXT [GRAV] (2021 Nov 22 - 2022 Jan 7) | ||||||||||||||||
20 | Instrument | Description | |||||||||||||||
21 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | |||||||||||||||
22 | MWR | ||||||||||||||||
23 | UVS | ||||||||||||||||
24 | JunoCam | ||||||||||||||||
25 | JIRAM | Aided by a spacecraft turn, all longitudes of Jupiter were mapped at latitude around and north of 45 deg S (see figure). | |||||||||||||||
26 | |||||||||||||||||
27 | |||||||||||||||||
28 | |||||||||||||||||
29 | |||||||||||||||||
30 | |||||||||||||||||
31 | |||||||||||||||||
32 | |||||||||||||||||
33 | |||||||||||||||||
34 | |||||||||||||||||
35 | |||||||||||||||||
36 | |||||||||||||||||
37 | |||||||||||||||||
38 | |||||||||||||||||
39 | |||||||||||||||||
40 | |||||||||||||||||
41 | |||||||||||||||||
42 | |||||||||||||||||
43 | Atmospheric coverage by the JIRAM M-band (5-micron channel) | ||||||||||||||||
44 | |||||||||||||||||
45 | |||||||||||||||||
46 | |||||||||||||||||
47 | |||||||||||||||||
48 | |||||||||||||||||
49 | |||||||||||||||||
50 | |||||||||||||||||
51 | |||||||||||||||||
52 | |||||||||||||||||
53 | |||||||||||||||||
54 | |||||||||||||||||
55 | |||||||||||||||||
56 | |||||||||||||||||
57 | |||||||||||||||||
58 | |||||||||||||||||
59 | |||||||||||||||||
60 | |||||||||||||||||
61 | |||||||||||||||||
62 | |||||||||||||||||
63 | |||||||||||||||||
64 | |||||||||||||||||
65 | |||||||||||||||||
66 | Composite of JunoCam images during PJ38, reduced by Gerald Eichstaedt and assembled by John Rogers | ||||||||||||||||
67 | |||||||||||||||||
68 | |||||||||||||||||
69 | |||||||||||||||||
70 | |||||||||||||||||
71 | |||||||||||||||||
72 | |||||||||||||||||
73 | |||||||||||||||||
74 | |||||||||||||||||
75 | |||||||||||||||||
76 | |||||||||||||||||
77 | |||||||||||||||||
78 | |||||||||||||||||
79 | |||||||||||||||||
80 | |||||||||||||||||
81 | |||||||||||||||||
82 | |||||||||||||||||
83 | |||||||||||||||||
84 | |||||||||||||||||
85 | |||||||||||||||||
86 | |||||||||||||||||
87 | |||||||||||||||||
88 | |||||||||||||||||
89 | |||||||||||||||||
90 | |||||||||||||||||
91 | |||||||||||||||||
92 | |||||||||||||||||
93 | |||||||||||||||||
94 | |||||||||||||||||
95 | |||||||||||||||||
96 | |||||||||||||||||
97 | |||||||||||||||||
98 | |||||||||||||||||
99 | |||||||||||||||||
100 | |||||||||||||||||
101 | |||||||||||||||||
102 | |||||||||||||||||
103 | |||||||||||||||||
104 | |||||||||||||||||
105 | |||||||||||||||||
106 | |||||||||||||||||
107 | |||||||||||||||||
108 | |||||||||||||||||
109 | |||||||||||||||||
110 | |||||||||||||||||
111 | |||||||||||||||||
112 | |||||||||||||||||
113 | |||||||||||||||||
114 | |||||||||||||||||
115 | |||||||||||||||||
116 | |||||||||||||||||
117 | |||||||||||||||||
118 | |||||||||||||||||
119 | |||||||||||||||||
120 | |||||||||||||||||
121 | |||||||||||||||||
122 | |||||||||||||||||
123 | |||||||||||||||||
124 | |||||||||||||||||
125 | |||||||||||||||||
126 | |||||||||||||||||
127 | |||||||||||||||||
128 | |||||||||||||||||
129 | |||||||||||||||||
130 | |||||||||||||||||
131 | |||||||||||||||||
132 | |||||||||||||||||
133 | |||||||||||||||||
134 | MWR footprints for the minimum emission angle at each spacecraft rotation. The cross marks the location of the perijove. | ||||||||||||||||
135 | |||||||||||||||||
136 |
1 | - | ||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|
2 | The period has been defined as a week before perijove to a week before the subsequent perijove, unlike the mission-planning definition, which extends from a day before the perijove to a day after the perijove. | ||||||||||||
3 | Period: Orbit 37-EXT [GRAV] (2021 Oct 9 - 2021 Nov 19) | Observations requested. | |||||||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | Observations planned / granted time | ||||||
5 | X-ray | Caitriona Jackman | Chandra HRC-I | Explore timing and morphology of jovian X-rays when Juno is close to perijove (crossing current sheet) and during perijove | Successful Chandra-HRC-I Observations.. 3 x 1-jovian-rotation (36 ks): ObsID 23373, 36 ks, start 2021-10-11 22:46:17; ObsID 23374, 36 ks, start 2021-10-13 08:10:50; ObsID 23375, 36 ks, start 2021-10-17 11:08:26 | Publicly available on the Chandra Data Archive: https://cda.harvard.edu/chaser/ | |||||||
6 | Visible/NIR | Alexander/Irwin | VLT/MUSE - IFU | spectroscopic imaging, 465-930 nm to determine cloud structure and albedo spectrum of particles. | 7/8th Nov (focused on PJ longitude) 8/9th Nov (focus on GRS) | Raw data publicly available to download from ESO portal. | |||||||
7 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | 20211002 20211020 20211003 20211021 20211009 20211022 20211010 20211023 20211011 20211024 20211013 20211025 20211014 20211026 20211015 20211027 20211016 20211028 20211017 20211029 20211019 | ||||||||
8 | near IR | Kim, Sang-joon | Gemini-N/GNIRS | 3.31 - 3.41 micron | 07:50-08:18 (UT) 7 Oct | ||||||||
9 | near IR | Orton | IRTF/SpeX | filtered imaging and scanning spectroscopy between 1.58 and 5.1µm | Observations obtained during short sequences on Nov 3,4 | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired. Reduced "quick-look" observations (geometrically but not radiometrically calibrated) will be available for immeduately use from the Juno-curated web site: http://junoirtf.space.swri.edu/ | |||||||
10 | near IR (5 µm) | Wong | Gemini-N/NIRI | lucky imaging, 5-µm maps | 2021 June 7 and 9 | now: https://archive.gemini.edu/searchform/GN-2021B-Q-110 future: https://archive.stsci.edu/hlsp/wfcj | |||||||
11 | Radio | Kreuser-Jenkins | DSS-13 | ground based radio observations of Jupiter using DSS13 via the GAVRT Program | 10/25/2021, 10/27/2021, 11/1/2021, 11/3/2021, 11/17/2021, 11/18/2021 | raw data available upon request | |||||||
12 | near IR | Orton | Gemini-N/NIRI | filtered near-infrared imaging of Jupiter; adaptive-optics stabilization has been requested, if working. | observations obtained on Oct 10, 11 and 15. | available on request | |||||||
13 | mid-IR | Fletcher | VLT/VISIR | Filtered imaging 5-20 µm, including lucky imaging at 5 µm. | Global map acquired between November 9th and November 19th, under varying seeing conditions. | Available on request, example shown to the right. | |||||||
14 | mid-IR | Orton | IRTF/MIRSI | Filtered imaging 5-18 µm | Observations made on Nov 11-12 in quasi-engineering run. | Substantial processing must be done with new instrument. | |||||||
15 | radio | Imai | Long Wavelength Array station 1 (LWA-1), LWA-Sevilleta (LWA-SV) | Jupiter's decametric auroral radio observations | October 7, 8, 14, 15 November 2, 8, 9, 15, 16 | Low-resolution LWA1 data are freely accessible via Autoplot (http://autoplot.org) by accepting the data usage policy (http://space.physics.uiowa.edu/earth/datapolicy.html) More information can be found at http://space.physics.uiowa.edu/earth/ | |||||||
16 | radio | Zarka, Cecconi, Lamy, Louis | Nançay Decameter Array (France) | coordinated measurement of 10-40 MHz cyclotron radio emission | every day, 8 hours around the transition to local meridian | https://maser.lesia.obspm.fr/task-1-data-collections/juno-ground-radio/juno-ground-radio-nancay-decameter.html?lang=en | |||||||
17 | Radio | Lamy for the NenuFar ES07 team | NenuFAR (France) | coordinated measurements of 10-40 MHz cyclotron radio emission at high time/frequency resolution | Oct. 15 15:10 - Oct. 16 00:36; Oct. 16 15:06 - Oct. 17 00:32; Oct. 17 15:02 - Oct. 18 00:28; Nov. 02 14:00 - 16:30 | Data available on demand to laurent.lamy@obspm.fr | |||||||
18 | |||||||||||||
19 | Scheduled observations by Juno. | ||||||||||||
20 | |||||||||||||
21 | Perijove is 2021 October 16, 17:13:28 SCET ( = UTC - light time). System-III longitude = 57.5°W | ||||||||||||
22 | |||||||||||||
23 | Period: Orbit 37-EXT [GRAV] (2021 Oct 9 - 2021 Nov 19) | ||||||||||||
24 | Instrument | Description | |||||||||||
25 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | |||||||||||
26 | MWR | ||||||||||||
27 | UVS | ||||||||||||
28 | JunoCam | ||||||||||||
29 | JIRAM | ||||||||||||
30 | |||||||||||||
31 | |||||||||||||
32 | |||||||||||||
33 | |||||||||||||
34 | |||||||||||||
35 | |||||||||||||
36 | |||||||||||||
37 | |||||||||||||
38 | |||||||||||||
39 | |||||||||||||
40 | |||||||||||||
41 | |||||||||||||
42 | |||||||||||||
43 | |||||||||||||
44 | |||||||||||||
45 | |||||||||||||
46 | |||||||||||||
47 | |||||||||||||
48 | |||||||||||||
49 | |||||||||||||
50 | |||||||||||||
51 | |||||||||||||
52 | |||||||||||||
53 | |||||||||||||
54 | |||||||||||||
55 | |||||||||||||
56 | |||||||||||||
57 | |||||||||||||
58 | |||||||||||||
59 | |||||||||||||
60 | |||||||||||||
61 | |||||||||||||
62 | Atmospheric coverage by the JIRAM M-band (5-micron channel) | ||||||||||||
63 | |||||||||||||
64 | |||||||||||||
65 | |||||||||||||
66 | |||||||||||||
67 | |||||||||||||
68 | |||||||||||||
69 | |||||||||||||
70 | |||||||||||||
71 | |||||||||||||
72 | |||||||||||||
73 | |||||||||||||
74 | |||||||||||||
75 | |||||||||||||
76 | |||||||||||||
77 | |||||||||||||
78 | |||||||||||||
79 | |||||||||||||
80 | |||||||||||||
81 | |||||||||||||
82 | |||||||||||||
83 | |||||||||||||
84 | |||||||||||||
85 | |||||||||||||
86 | |||||||||||||
87 | |||||||||||||
88 | |||||||||||||
89 | |||||||||||||
90 | |||||||||||||
91 | |||||||||||||
92 | |||||||||||||
93 | |||||||||||||
94 | |||||||||||||
95 | |||||||||||||
96 | |||||||||||||
97 | |||||||||||||
98 | |||||||||||||
99 | |||||||||||||
100 | |||||||||||||
101 | |||||||||||||
102 | |||||||||||||
103 | |||||||||||||
104 | |||||||||||||
105 | |||||||||||||
106 | |||||||||||||
107 | |||||||||||||
108 | |||||||||||||
109 | |||||||||||||
110 | |||||||||||||
111 | |||||||||||||
112 | |||||||||||||
113 | |||||||||||||
114 | |||||||||||||
115 | |||||||||||||
116 | |||||||||||||
117 | |||||||||||||
118 | |||||||||||||
119 | |||||||||||||
120 | |||||||||||||
121 | |||||||||||||
122 | |||||||||||||
123 | |||||||||||||
124 | |||||||||||||
125 | |||||||||||||
126 | |||||||||||||
127 | |||||||||||||
128 | |||||||||||||
129 | |||||||||||||
130 | |||||||||||||
131 | |||||||||||||
132 | MWR footprints for the minimum emission angle at each spacecraft rotation. The cross marks the location of the perijove. | ||||||||||||
133 | |||||||||||||
134 | |||||||||||||
135 | |||||||||||||
136 | |||||||||||||
137 | |||||||||||||
138 | |||||||||||||
139 | |||||||||||||
140 | |||||||||||||
141 | |||||||||||||
142 | |||||||||||||
143 | |||||||||||||
144 | |||||||||||||
145 | |||||||||||||
146 | |||||||||||||
147 | |||||||||||||
148 | |||||||||||||
149 | |||||||||||||
150 | |||||||||||||
151 | |||||||||||||
152 | |||||||||||||
153 | |||||||||||||
154 | |||||||||||||
155 | |||||||||||||
156 | |||||||||||||
157 | |||||||||||||
158 | |||||||||||||
159 | |||||||||||||
160 | |||||||||||||
161 | Composite cylindrical map from JunoCam images by John Rogers and Gerald Eichstaedt |
1 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed toward the Earth. This orbit is for an extended mission approved by NASA HQ. | |||||||||
---|---|---|---|---|---|---|---|---|---|---|
2 | The period has been defined as a week before perijove to a week before the subsequent perijove, unlike the mission-planning definition, which extends from a day before the perijove to a day after the perijove. | |||||||||
3 | Period: Orbit 36-EXT [GRAV] (2021 Aug 27 - 2021 Oct 1) | Observations requested. | ||||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | Observations planned / granted time | |||
5 | X-ray | Caitriona Jackman | Chandra HRC-I | Explore timing and morphology of jovian X-rays when Juno is close to perijove (crossing current sheet) and during perijove | 1 long (144 ks ) Chandra HRC-I observation made ObsID 23369, 144 ks, start 2021-09-15 12:32:16 | Publicly available on the Chandra Data Archive: https://cda.harvard.edu/chaser/ | ||||
6 | FUV | Bonfond | HST/STIS | Timetag imaging of northern aurora | 3 successful HST orbits on August 30, Sept. 1 and 3 | Publicly available on HST's MAST archive | Observations successful | |||
7 | Radio | Kreuser-Jenkins | DSS-13 | ground based radio observations of Jupiter using DSS13 via the GAVRT Program | 9/2/2021, 9/3/2021 | raw data available upon request | ||||
8 | visible/NUV | Simon | HST/WFC3 UVIS | hi-resolution maps of Jupiter at all longitudes and several filters with a repeat. Part of the Outer Planet Atmospheric Legacy (OPAL) program. | 4 September | https://archive.stsci.edu/prepds/opal/ https://doi.org/10.1016/j.icarus.2022.114994 | Observations cancelled or unsuccessful | |||
9 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | 20210909 20210920
20210914 20210921 20210915 20210922 20210916 20210929 20210919 | |||||
10 | near IR | Orton | IRTF/SpeX | filtered imaging and scanning spectroscopy between 1.58 and 5.1µm | Images and scanning spectra were obtained on Sep 4-5 with good seeing and clear skies or light cirrus. Seeing was 0.6-1.0". Some images were virtually simultaneous with WFC3/UVIS observations. Images on Sep 20-21 were made in 0.55-0.65" seeing. | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired. Reduced "quick-look" observations (geometrically but not radiometrically calibrated) will be available for immeduately use from the Juno-curated web site: http://junoirtf.space.swri.edu/ | ||||
11 | near IR | Orton | Gemini-N/NIRI | filtered near-infrared imaging of Jupiter; adaptive-optics stabilization has been requested, if working. | observations near PJ36 not made | NIRI is off the telescope until October | ||||
12 | mid-IR | Fletcher | VLT/VISIR | Filtered imaging 5-20 µm, including lucky imaging at 5 µm. | Within a week of PJ36, acquiring a global map, subject to recommissioning of VISIR. | Observations not made, with VISIR still off the VLT. | ||||
13 | radio | Zarka, Cecconi, Lamy, Louis | Nançay Decameter Array (France) | coordinated measurement of 10-40 MHz cyclotron radio emission | every day, 8 hours around the transition to local meridian | https://maser.lesia.obspm.fr/task-1-data-collections/juno-ground-radio/juno-ground-radio-nancay-decameter.html?lang=en | ||||
14 | Radio | Lamy for the NenuFar ES07 team | NenuFAR (France) | coordinated measurements of 10-40 MHz cyclotron radio emission at high time/frequency resolution | Sep. 02 18:07 - Sep. 03 03:43; Sep. 03 18:02 - Sep. 04 03:38; Sep. 24 16:34-19:30; Sep. 25 17:48-20:52; Oct. 01 16:06-20:14; Oct. 02 19:30-21:36 | Data available on demand to laurent.lamy@obspm.fr | ||||
15 | ||||||||||
16 | ||||||||||
17 | Scheduled observations by Juno. | |||||||||
18 | ||||||||||
19 | Perijove is 2021 Sep 2, 22:42:43 SCET ( = UTC - light time). System-III longitude = 113.5°W | |||||||||
20 | ||||||||||
21 | Period: Orbit 36-EXT [GRAV] (2021 Aug 27 - 2021 Oct 1) | |||||||||
22 | Instrument | Description | ||||||||
23 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||
24 | MWR | |||||||||
25 | UVS | |||||||||
26 | JunoCam | |||||||||
27 | JIRAM | area covered is shown in the figure below | ||||||||
28 | ||||||||||
29 | ||||||||||
30 | ||||||||||
31 | ||||||||||
32 | ||||||||||
33 | ||||||||||
34 | ||||||||||
35 | ||||||||||
36 | ||||||||||
37 | ||||||||||
38 | ||||||||||
39 | ||||||||||
40 | ||||||||||
41 | ||||||||||
42 | ||||||||||
43 | ||||||||||
44 | ||||||||||
45 | ||||||||||
46 | ||||||||||
47 | ||||||||||
48 | ||||||||||
49 | ||||||||||
50 | ||||||||||
51 | ||||||||||
52 | ||||||||||
53 | ||||||||||
54 | ||||||||||
55 | JIRAM coverage of Jupiter's atmosphere with the M-band (5 microns) | |||||||||
56 | ||||||||||
57 | ||||||||||
58 | ||||||||||
59 | ||||||||||
60 | ||||||||||
61 | ||||||||||
62 | ||||||||||
63 | ||||||||||
64 | ||||||||||
65 | ||||||||||
66 | ||||||||||
67 | ||||||||||
68 | ||||||||||
69 | ||||||||||
70 | ||||||||||
71 | ||||||||||
72 | ||||||||||
73 | ||||||||||
74 | ||||||||||
75 | ||||||||||
76 | Composite of JunoCam coverage of Jupiter's atmosphere in cylindrical map form. by Gerald Eichstaedt | |||||||||
77 | ||||||||||
78 | ||||||||||
79 | ||||||||||
80 | ||||||||||
81 | ||||||||||
82 | ||||||||||
83 | ||||||||||
84 | ||||||||||
85 | ||||||||||
86 | ||||||||||
87 | ||||||||||
88 | ||||||||||
89 | ||||||||||
90 | ||||||||||
91 | ||||||||||
92 | ||||||||||
93 | ||||||||||
94 | ||||||||||
95 | ||||||||||
96 | ||||||||||
97 | ||||||||||
98 | ||||||||||
99 | ||||||||||
100 | ||||||||||
101 | ||||||||||
102 | ||||||||||
103 | ||||||||||
104 | ||||||||||
105 | ||||||||||
106 | ||||||||||
107 | ||||||||||
108 | ||||||||||
109 | ||||||||||
110 | ||||||||||
111 | ||||||||||
112 | ||||||||||
113 | ||||||||||
114 | ||||||||||
115 | ||||||||||
116 | ||||||||||
117 | ||||||||||
118 | ||||||||||
119 | ||||||||||
120 | ||||||||||
121 | ||||||||||
122 | ||||||||||
123 | ||||||||||
124 | ||||||||||
125 | ||||||||||
126 | ||||||||||
127 | ||||||||||
128 | ||||||||||
129 | MWR footprints for the minimum emission angle at each latitude. The cross marks the location of the perijove. | |||||||||
130 | ||||||||||
131 | MWR footprints for the minimum emission angle at each spacecraft rotation. The cross marks the location of the perijove. | |||||||||
132 |
1 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed toward the Earth. This orbit is for an extended mission approved by NASA HQ. | |||||||||
---|---|---|---|---|---|---|---|---|---|---|
2 | The period has been defined as a week before perijove to a week before the subsequent perijove, unlike the mission-planning definition, which extends from a day before the perijove to a day after the perijove. | |||||||||
3 | Period: Orbit 35-EXT [GRAV] (2021 Jul 15 - 2021 Aug 26) | Observations requested. | ||||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | Observations planned / granted time | |||
5 | X-ray | Caitriona Jackman | Chandra HRC-I | Explore timing and morphology of jovian X-rays when Juno is close to perijove (crossing current sheet) and during perijove | Successful Chandra-HRC-I Observations.. 3 x 1-jovian-rotation (36 ks). 1 x long observation (144 ks): ObsID 23370, 36 ks, start 2021-07-16 14:02:24; ObsID 23368, 144 ks, start 2021-07-22 02:38:26; ObsID 23371, 36 ks, start 2021-07-17 09:35:32; ObsID 23372, 36 ks, start 2021-07-19 16:36:47 | Publicly available on the Chandra Data Archive: https://cda.harvard.edu/chaser/ | ||||
6 | FUV | Bonfond | HST/STIS | Timetag imaging of northern aurora | Out of 4 HST orbits, only the one on July 19th was successful | Publicly available on HST's MAST | Observations successful | |||
7 | Radio | Kreuser-Jenkins | DSS-13 | ground based radio observations of Jupiter using DSS13 via the GAVRT Program | 8/25/2021, 8/26/2021 | raw data available upon request | ||||
8 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | 20210805 20210823 20210820 20210824 20210822 20210826 (horrible monsoon season) | |||||
9 | Visible | de Pater | Keck | HIRES | July 20 (July 21 was weathered out) | This is part of a student's PhD thesis. | ||||
10 | Visible + Near IR (0.38-1.7 micron) | Sanchez-Lavega & Antuñano | 2.2m Calar Alto | lucky imaging | 20-24 July, with extraordinarily good seeing | |||||
11 | near IR | Orton | IRTF/SpeX | filtered imaging and scanning spectroscopy between 1.58 and 5.1µm | Images only were made in 6 hour sessions on 20-21 July. We were dodging clouds on both nights, although it cleared up toward the end of the 21 July sesssion and a photometric standard G-type star was observed. | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired. Reduced "quick-look" observations (geometrically but not radiometrically calibrated) will be available for immeduately use from the Juno-curated web site: http://junoirtf.space.swri.edu/ | ||||
12 | near IR | Orton | Gemini-N/NIRI | filtered near-infrared imaging of Jupiter | Images obtaine on July 10 and August 10 without AO stabilization | avalable on request | ||||
13 | 3.31 - 3.41 micron | Kim, Sang-joon | Gemini-N/GNIRS | high spectral resolution, auroral mapping | July 17 | See below for details | ||||
14 | near IR | de Pater | Keck | 5-micron spectroscopy | July 20 (July 21 was weathered out) | This is part of a student's PhD thesis | ||||
15 | near IR (0.7 - 2.5, 2.9 - 5.2 μm) | Cartwright | IRTF/SpeX: SXD (0.8" slit), LXD_short (0.3"), LXD_long (0.3"). LXD modes cover JIRAM order sorting filter gap | Reflectance spectroscopy of Europa (E), Ganymede (G), and Callisto (C). SXD native R ~750 at 2.2 μm, native R ~2500 in LXD modes | July 17 (G and C), July 18 (E and G), July 28 (E and G) | Contact PI - interested in collaborating with teams using Juno instruments to observe moons (especially JIRAM) | ||||
16 | radio | Zarka, Cecconi, Lamy, Louis | Nançay Decameter Array (France) | coordinated measurement of 10-40 MHz cyclotron radio emission | every day, 8 hours around the transition to local meridian | https://maser.lesia.obspm.fr/task-1-data-collections/juno-ground-radio/juno-ground-radio-nancay-decameter.html?lang=en | ||||
17 | radio | Lamy for the NenuFar ES07 team | NenuFAR (France) | coordinated measurements of 10-40 MHz cyclotron radio emission at high time/frequency resolution | Jul. 20 21:09-Jul. 21 01:00; Jul. 21 03:00-07:05 Jul. 21 21:05-Jul. 22 07:00; Jul. 22 21:01-Jul. 23 06:57; | Data available on demand to laurent.lamy@obspm.fr | ||||
18 | Scheduled observations by Juno. | |||||||||
19 | ||||||||||
20 | Perijove is 2021 Jul 21 08:14:53 SCET ( = UTC - light time). System-III longitude = 316.4°W | |||||||||
21 | ||||||||||
22 | Period: Orbit 35-EXT [GRAV] (2021 Jul 15 - 2021 Aug 26) | |||||||||
23 | Instrument | Description | ||||||||
24 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||
25 | MWR | |||||||||
26 | UVS | |||||||||
27 | JunoCam | |||||||||
28 | JIRAM | |||||||||
29 | ||||||||||
30 | ||||||||||
31 | ||||||||||
32 | ||||||||||
33 | ||||||||||
34 | ||||||||||
35 | ||||||||||
36 | ||||||||||
37 | ||||||||||
38 | ||||||||||
39 | ||||||||||
40 | ||||||||||
41 | ||||||||||
42 | ||||||||||
43 | ||||||||||
44 | ||||||||||
45 | ||||||||||
46 | ||||||||||
47 | ||||||||||
48 | ||||||||||
49 | ||||||||||
50 | ||||||||||
51 | ||||||||||
52 | ||||||||||
53 | ||||||||||
54 | ||||||||||
55 | ||||||||||
56 | JIRAM coverage of Jupiter's atmosphere with the M-band (5 microns) | |||||||||
57 | ||||||||||
58 | ||||||||||
59 | ||||||||||
60 | ||||||||||
61 | ||||||||||
62 | ||||||||||
63 | ||||||||||
64 | ||||||||||
65 | ||||||||||
66 | ||||||||||
67 | ||||||||||
68 | ||||||||||
69 | ||||||||||
70 | ||||||||||
71 | ||||||||||
72 | ||||||||||
73 | ||||||||||
74 | ||||||||||
75 | ||||||||||
76 | ||||||||||
77 | ||||||||||
78 | ||||||||||
79 | ||||||||||
80 | Composite of JunoCam coverage of Jupiter's atmosphere in cylindrical map form. by John Rogers and Gerald Eichstaedt | |||||||||
81 | ||||||||||
82 | ||||||||||
83 | ||||||||||
84 | ||||||||||
85 | ||||||||||
86 | ||||||||||
87 | ||||||||||
88 | ||||||||||
89 | ||||||||||
90 | ||||||||||
91 | ||||||||||
92 | ||||||||||
93 | ||||||||||
94 | ||||||||||
95 | ||||||||||
96 | ||||||||||
97 | ||||||||||
98 | ||||||||||
99 | ||||||||||
100 | ||||||||||
101 | ||||||||||
102 | ||||||||||
103 | ||||||||||
104 | ||||||||||
105 | ||||||||||
106 | ||||||||||
107 | ||||||||||
108 | ||||||||||
109 | ||||||||||
110 | ||||||||||
111 | ||||||||||
112 | ||||||||||
113 | ||||||||||
114 | ||||||||||
115 | ||||||||||
116 | ||||||||||
117 | ||||||||||
118 | ||||||||||
119 | ||||||||||
120 | ||||||||||
121 | ||||||||||
122 | ||||||||||
123 | ||||||||||
124 | ||||||||||
125 | ||||||||||
126 | ||||||||||
127 | ||||||||||
128 | ||||||||||
129 | ||||||||||
130 | ||||||||||
131 | ||||||||||
132 | ||||||||||
133 | ||||||||||
134 | ||||||||||
135 | ||||||||||
136 | ||||||||||
137 | ||||||||||
138 | ||||||||||
139 | ||||||||||
140 | ||||||||||
141 | ||||||||||
142 | ||||||||||
143 | ||||||||||
144 | ||||||||||
145 | ||||||||||
146 | ||||||||||
147 | ||||||||||
148 | ||||||||||
149 | ||||||||||
150 | MWR footprints for the minimum emission angle at each spacecraft rotation. The cross marks the location of the perijove. | |||||||||
151 | ||||||||||
152 |
1 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed toward the Earth. This is the first orbit of an extended mission approved by NASA HQ. | |||||||||
---|---|---|---|---|---|---|---|---|---|---|
2 | The period has been defined as a week before perijove to a week before the subsequent perijove, unlike the mission-planning definition, which extends from a day before the perijove to a day after the perijove. | |||||||||
3 | Shortly before perijove on Jun 7, the spacraft will make a close approach to the Galilean satellite Ganymede. | |||||||||
4 | Period: Orbit 34-EXT [GRAV] (2021 Jun 1 - 2021 Jul 14) | Observations requested. | ||||||||
5 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | Observations planned / granted time | |||
6 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | 20210607 20210616 20210608 20210617 20210609 20210618 20210610 20210621 20210611 20210622 20210612 20210625 20210613 20210709 20210614 | |||||
7 | 3.31 - 3.41 micron | Kim, Sang-joon | Gemini-N/GNIRS | high spectral resolution, auroral mapping | June 30 | See below for details | ||||
8 | Visible + Near IR (0.38-1.7 micron) | Sanchez-Lavega | PlanetCam 2.2m Calar Alto | lucky imaging | July 20-23 with extraordinarily good seeing | |||||
9 | near IR (5 µm) | Wong | Gemini-N/NIRI | lucky imaging, 5-µm maps | 7, 9, 13, 14, 16, 23 June; 13-23 June dedicated to GRS | now: https://archive.gemini.edu/searchform/GN-2020B-Q-101 https://doi.org/10.1016/j.icarus.2022.114994 future: https://archive.stsci.edu/hlsp/wfcj | ||||
10 | near IR | Orton | IRTF/SpeX | filtered imaging and scanning spectroscopy between 1.58 and 5.1µm | Images at one longitude were obtained on May 26-27 with generally clear skies and 0.5-0.9" seeing. More were made on June 7-8 over nearly all longitudes in clear weather and 0.7-0.9" seeing on June 7 and 0.55-0.6" seeing on June 8, with scanning spectroscopy performed, as well. Images were obtained on June 24-25 at one longitude in clear weather and seeing varying between 0.3 and 0.9". | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired. Reduced "quick-look" observations (geometrically but not radiometrically calibrated) will be available for immeduately use from the Juno-curated web site: http://junoirtf.space.swri.edu/ | ||||
11 | near IR | Orton | Gemini-N/NIRI | filtered near-infrared imaging of Jupiter, often with Adaptive-Optics (AO) stabilization. | 6 June, 12 June, 23 June. AO stabilization was available for 12 June and 28 June. 6 June imaging targetted the GRS. | avalable on request | ||||
12 | near IR | Bjoraker | IRTF/iSHELL | 5-micron spectroscopy | UT June 6 and June 9 | available on request | ||||
13 | Visible + Near IR (0.38-1.7 micron) | Antuñano | PlanetCam 2.2m Calar Alto | lucky imaging | 4-7 June | |||||
14 | near IR (0.7 - 2.5, 2.9 - 5.2 μm) | Cartwright | IRTF/SpeX: SXD (0.8" slit), LXD_short (0.3"), LXD_long (0.3"). LXD modes cover JIRAM order sorting filter gap | Reflectance spectroscopy of Europa (E), Ganymede (G), and Callisto (C). SXD native R ~750 at 2.2 μm, native R ~2500 in LXD modes | June 12 (G), June 17 (G), June 21 (G), June 22 (G and C), June 25 (C) | Contact PI - interested in collaborating with teams using Juno instruments to observe moons (especially JIRAM) | ||||
15 | mid-infrared | Antuñano | TEXES | global mapping, medium and low resolution spectroscopy | 26 and 27 June | |||||
16 | mid-infrared | Sinclair | TEXES | high spectral resolution, auroral mapping | 28 and 29 June | |||||
17 | radio | Zarka, Cecconi, Lamy, Louis | Nançay Decameter Array (France) | coordinated measurement of 10-40 MHz cyclotron radio emission | every day, 8 hours around the transition to local meridian | https://maser.lesia.obspm.fr/task-1-data-collections/juno-ground-radio/juno-ground-radio-nancay-decameter.html?lang=en | ||||
18 | Radio | Lamy for the NenuFar ES07 team | NenuFAR (France) | coordinated measurements of 10-40 MHz cyclotron radio emission at high time/frequency resolution | Jun. 07 00:03-08:01; Jun. 08 00:00-10:00; Jun. 08 23:57-04:00; Jun. 09 05:00-09:58; Jun. 09 23:53-09:00 | Data available on demand to laurent.lamy@obspm.fr | ||||
19 | Scheduled observations by Juno. | |||||||||
20 | ||||||||||
21 | Perijove is 2021 Jun 8 07:46:00 SCET ( = UTC - light time). System-III longitude = 306.6°W | |||||||||
22 | ||||||||||
23 | Period: Orbit 34-EXT [GRAV] (2021 Jun 1 - 2021 Jul 14) | |||||||||
24 | Instrument | Description | ||||||||
25 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||
26 | MWR | |||||||||
27 | UVS | |||||||||
28 | JunoCam | |||||||||
29 | JIRAM | |||||||||
30 | ||||||||||
31 | ||||||||||
32 | Sang-joon Kim | As of 6/7/21, a paper "Morphological Variations and Energetics of the 3-micorn Jovian Northern Aurorae" is being prepared based on 2020 data. | ||||||||
33 | ||||||||||
34 | ||||||||||
35 | ||||||||||
36 | ||||||||||
37 | ||||||||||
38 | ||||||||||
39 | ||||||||||
40 | ||||||||||
41 | ||||||||||
42 | ||||||||||
43 | ||||||||||
44 | ||||||||||
45 | ||||||||||
46 | ||||||||||
47 | ||||||||||
48 | ||||||||||
49 | ||||||||||
50 | ||||||||||
51 | ||||||||||
52 | ||||||||||
53 | ||||||||||
54 | ||||||||||
55 | ||||||||||
56 | ||||||||||
57 | ||||||||||
58 | ||||||||||
59 | ||||||||||
60 | ||||||||||
61 | ||||||||||
62 | ||||||||||
63 | JIRAM coverage of Jupiter's atmosphere with the M-band (5 microns) | |||||||||
64 | ||||||||||
65 | ||||||||||
66 | ||||||||||
67 | ||||||||||
68 | ||||||||||
69 | ||||||||||
70 | ||||||||||
71 | ||||||||||
72 | ||||||||||
73 | ||||||||||
74 | ||||||||||
75 | ||||||||||
76 | ||||||||||
77 | ||||||||||
78 | ||||||||||
79 | ||||||||||
80 | ||||||||||
81 | ||||||||||
82 | ||||||||||
83 | ||||||||||
84 | ||||||||||
85 | Composite of JunoCam coverage of Jupiter's atmosphere in cylindrical map form. by John Rogers and Gerald Eichstaedt | |||||||||
86 | ||||||||||
87 | Composite of JunoCam coverage of Jupiter's atmosphere in cylindrical map form. by John Rogers and Gerald Eichstaedt | |||||||||
88 | ||||||||||
89 | ||||||||||
90 | ||||||||||
91 | ||||||||||
92 | ||||||||||
93 | ||||||||||
94 | ||||||||||
95 | ||||||||||
96 | ||||||||||
97 | ||||||||||
98 | ||||||||||
99 | ||||||||||
100 | ||||||||||
101 | ||||||||||
102 | ||||||||||
103 | ||||||||||
104 | ||||||||||
105 | ||||||||||
106 | ||||||||||
107 | ||||||||||
108 | ||||||||||
109 | ||||||||||
110 | ||||||||||
111 | ||||||||||
112 | ||||||||||
113 | ||||||||||
114 | Composite of JIRAM M-band (5-micron) map. | |||||||||
115 | ||||||||||
116 | ||||||||||
117 | ||||||||||
118 | ||||||||||
119 | ||||||||||
120 | ||||||||||
121 | ||||||||||
122 | ||||||||||
123 | ||||||||||
124 | ||||||||||
125 | ||||||||||
126 | ||||||||||
127 | ||||||||||
128 | ||||||||||
129 | ||||||||||
130 | ||||||||||
131 | ||||||||||
132 | ||||||||||
133 | ||||||||||
134 | ||||||||||
135 | ||||||||||
136 | ||||||||||
137 | ||||||||||
138 | ||||||||||
139 | ||||||||||
140 | ||||||||||
141 | ||||||||||
142 | ||||||||||
143 | ||||||||||
144 | ||||||||||
145 | ||||||||||
146 | ||||||||||
147 | ||||||||||
148 | ||||||||||
149 | ||||||||||
150 | ||||||||||
151 | ||||||||||
152 | ||||||||||
153 | ||||||||||
154 | ||||||||||
155 | ||||||||||
156 | ||||||||||
157 | MWR footprints for the minimum emission angle at each spacecraft rotation. The cross marks the location of the perijove. | |||||||||
158 | ||||||||||
159 | ||||||||||
160 | ||||||||||
161 | ||||||||||
162 | ||||||||||
163 | ||||||||||
164 | ||||||||||
165 | ||||||||||
166 | ||||||||||
167 | ||||||||||
168 | ||||||||||
169 | ||||||||||
170 | ||||||||||
171 | ||||||||||
172 | ||||||||||
173 | ||||||||||
174 | ||||||||||
175 | ||||||||||
176 | ||||||||||
177 | ||||||||||
178 | ||||||||||
179 | ||||||||||
180 | ||||||||||
181 | ||||||||||
182 | ||||||||||
183 |
1 | Note: On this orbit the spacecraft orientation optimizes gravity mapping (GRAV) with the antenna pointed toward the Earth continuously. | |||||||
---|---|---|---|---|---|---|---|---|
2 | ||||||||
3 | Period: Orbit 33 [GRAV] (2021 Apr 15 - 2021 Jun 6) | Observations requested. | ||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | Observations planned / granted time | |
5 | FUV | Bonfond | HST/STIS | Timetag imaging of northern aurora | April 12-15 | Observations successful | ||
6 | Radio | Kreuser-Jenkins | DSS-13 | ground based radio observations of Jupiter using DSS13 via the GAVRT Program | 4/27/2021, 5/12/2021 | Raw data available upon request | Observations cancelled or unsuccessful | |
7 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | 20210430 20210517 20210503 20210518 20210504 20210519 20210505 20210520 20210506 20210523 20210507 20210524 20210508 20210525 20210509 20210526 20210510 20210528 20210511 20210529 20210512 20210530 20210513 20210531 20210514 20210604 20210515 20210605 20210516 20210606 | |||
8 | Visible/near IR | Alexander/Irwin | VLT/MUSE - IFU | spectroscopic imaging, 465-930 nm to determine cloud structure and albedo spectrum of particles. | 2021-04-16, 2021-05-10 | Raw data publicly available to download from ESO portal. Additional geometric calibration is needed to calibrate these observations on top of the standard calibration pipeline. | ||
9 | Visible + Near IR (0.38-1.7 micron) | Sanchez-Lavega | 2.2m Calar Alto | lucky imaging | June 4-7 | |||
10 | 3.31 - 3.41 micron | Kim, Sang-joon | Gemini-N/GNIRS | high spectral resolution, auroral mapping | May 30 | See below for details | ||
11 | near IR | Orton | IRTF/SpeX | filtered imaging and scanning spectroscopy between 1.58 and 5.1µm | April 12-13 daytime observationsL April 12 observations not made due to IRTF dome closure due to icing. April 13 observations successful, with seeing variable from 0.6-2.0 arcsec FWHM. One spectral scan ~0.8-2.5 microns and three sets of imaging observations with calibration during photometric sky conditions. May 5-6 observations largely washed out by bad weather. | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired. Reduced "quick-look" observations (geometrically but not radiometrically calibrated) will be available for immeduately use from the Juno-curated web site: http://junoirtf.space.swri.edu/ | ||
12 | radio | Zarka, Cecconi, Lamy, Louis | Nançay Decameter Array (France) | coordinated measurement of 10-40 MHz cyclotron radio emission | every day, 8 hours around the transition to local meridian | https://maser.lesia.obspm.fr/task-1-data-collections/juno-ground-radio/juno-ground-radio-nancay-decameter.html?lang=en | ||
13 | Radio | Lamy for the NenuFar ES07 team | NenuFAR (France) | coordinated measurements of 10-40 MHz cyclotron radio emission at high time/frequency resolution | Apr. 15 03:18-13:01; Apr. 16 03:15-12:58; Jun. 06 00:08-10:08 | Data available on demand to laurent.lamy@obspm.fr | ||
14 | Scheduled observations by Juno. | |||||||
15 | ||||||||
16 | Perijove is 2021 Apr 15 13:36:23 UTC. System-III longitude = 298.0°W | |||||||
17 | ||||||||
18 | Period: Orbit 33 [GRAV] (2021 Apr 15 - 2021 Jun 6) | |||||||
19 | Instrument | Description | ||||||
20 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||
21 | MWR | |||||||
22 | UVS | |||||||
23 | JunoCam | |||||||
24 | JIRAM | |||||||
25 | ||||||||
26 | ||||||||
27 | ||||||||
28 | ||||||||
29 | ||||||||
30 | ||||||||
31 | ||||||||
32 | ||||||||
33 | ||||||||
34 | ||||||||
35 | ||||||||
36 | ||||||||
37 | ||||||||
38 | ||||||||
39 | ||||||||
40 | ||||||||
41 | ||||||||
42 | ||||||||
43 | ||||||||
44 | ||||||||
45 | ||||||||
46 | ||||||||
47 | ||||||||
48 | ||||||||
49 | ||||||||
50 | ||||||||
51 | ||||||||
52 | ||||||||
53 | ||||||||
54 | ||||||||
55 | ||||||||
56 | ||||||||
57 | ||||||||
58 | Coverage of Jupiter's atmosphere by JIRAM at M-band (5 microns) | |||||||
59 | ||||||||
60 | ||||||||
61 | ||||||||
62 | ||||||||
63 | ||||||||
64 | ||||||||
65 | ||||||||
66 | ||||||||
67 | ||||||||
68 | ||||||||
69 | ||||||||
70 | ||||||||
71 | ||||||||
72 | ||||||||
73 | ||||||||
74 | ||||||||
75 | ||||||||
76 | ||||||||
77 | ||||||||
78 | ||||||||
79 | ||||||||
80 | ||||||||
81 | ||||||||
82 | ||||||||
83 | Composite of JunoCam coverage of Jupiter's atmosphere in cylindrical map form. by John Rogers and Gerald Eichstaedt | |||||||
84 | ||||||||
85 | ||||||||
86 | ||||||||
87 | ||||||||
88 | ||||||||
89 | ||||||||
90 | ||||||||
91 | ||||||||
92 | ||||||||
93 | ||||||||
94 | ||||||||
95 | ||||||||
96 | ||||||||
97 | ||||||||
98 | ||||||||
99 | ||||||||
100 | ||||||||
101 | ||||||||
102 | ||||||||
103 | ||||||||
104 | ||||||||
105 | ||||||||
106 | ||||||||
107 | ||||||||
108 | ||||||||
109 | Composite of JIRAM M-band (5-micron) map. | |||||||
110 | ||||||||
111 | ||||||||
112 | ||||||||
113 | ||||||||
114 | ||||||||
115 | ||||||||
116 | ||||||||
117 | ||||||||
118 | ||||||||
119 | ||||||||
120 | ||||||||
121 | ||||||||
122 | ||||||||
123 | ||||||||
124 | ||||||||
125 | ||||||||
126 | ||||||||
127 | ||||||||
128 | ||||||||
129 | ||||||||
130 | ||||||||
131 | ||||||||
132 | ||||||||
133 | ||||||||
134 | ||||||||
135 | ||||||||
136 | ||||||||
137 | ||||||||
138 | ||||||||
139 | ||||||||
140 | ||||||||
141 | ||||||||
142 | ||||||||
143 | ||||||||
144 | ||||||||
145 | ||||||||
146 | ||||||||
147 | ||||||||
148 | ||||||||
149 | ||||||||
150 | ||||||||
151 | ||||||||
152 | ||||||||
153 | ||||||||
154 | ||||||||
155 | ||||||||
156 | ||||||||
157 | ||||||||
158 | ||||||||
159 | ||||||||
160 | ||||||||
161 | ||||||||
162 | ||||||||
163 | ||||||||
164 | ||||||||
165 | ||||||||
166 | ||||||||
167 | ||||||||
168 | ||||||||
169 | ||||||||
170 | ||||||||
171 | ||||||||
172 | ||||||||
173 | ||||||||
174 | ||||||||
175 | ||||||||
176 | ||||||||
177 | ||||||||
178 | ||||||||
179 | ||||||||
180 | ||||||||
181 | ||||||||
182 | MWR footprints for the minimum emission angle at each spacecraft rotation. The cross marks the location of the perijove. | |||||||
183 | ||||||||
184 |
1 | Note: On this orbit the spacecraft orientation optimizes gravity mapping (GRAV) with the antenna pointed toward the Earth continuously. | |||||||
---|---|---|---|---|---|---|---|---|
2 | ||||||||
3 | Period: Orbit 32 [GRAV] (2021 Feb 21 - 2021 Apr 14) | Observations requested. | ||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | Observations planned / granted time | |
5 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | Nightly, weather permitting as Jupiter becomes available | Observations successful | ||
6 | near IR | Orton | IRTF/SpeX | filtered imaging and scanning spectroscopy between 1.58 and 5.1µm | requested dates near PJ32 for daytime observing No time granted | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired. Reduced "quick-look" observations (geometrically but not radiometrically calibrated) will be available for immeduately use from the Juno-curated web site: http://junoirtf.space.swri.edu/ | ||
7 | radio | Kreuser-Jenkins/Huffine | DSS-13 | Ground based radio observations of Jupiter using DSS-13 via the GAVRT Program | 2021 February 23, 25 2021 March 3, 4, 8, 9, 11, 15, 16, 18 | raw data available upon request | ||
8 | radio | Zarka, Cecconi, Lamy, Louis | Nançay Decameter Array (France) | coordinated measurement of 10-40 MHz cyclotron radio emission | every day, 8 hours around the transition to local meridian | https://maser.lesia.obspm.fr/task-1-data-collections/juno-ground-radio/juno-ground-radio-nancay-decameter.html?lang=en | ||
9 | Radio | Lamy for the NenuFar ES07 team | NenuFAR (France) | coordinated measurements of 10-40 MHz cyclotron radio emission at high time/frequency resolution | Feb. 21 06:20-15:30; Feb. 22 06:16-15:27; Mar. 12 05:16-09:20; Mar. 13 08:30-10:40; Mar. 21 07:14-09:00; Apr. 14 03:23-13:05 | Data available on demand to laurent.lamy@obspm.fr | ||
10 | ||||||||
11 | ||||||||
12 | ||||||||
13 | ||||||||
14 | ||||||||
15 | ||||||||
16 | Scheduled observations by Juno. | |||||||
17 | ||||||||
18 | Perijove is 2021 Feb 21 17:40:27 UTC. System-III longitude = 27.7°W | |||||||
19 | ||||||||
20 | Period: Orbit 32 [GRAV] (2021 Feb 21 - 2021 Apr 14) | |||||||
21 | Instrument | Description | ||||||
22 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||
23 | MWR | |||||||
24 | UVS | |||||||
25 | JunoCam | |||||||
26 | JIRAM | |||||||
27 | ||||||||
28 | ||||||||
29 | ||||||||
30 | ||||||||
31 | ||||||||
32 | ||||||||
33 | ||||||||
34 | ||||||||
35 | ||||||||
36 | ||||||||
37 | ||||||||
38 | ||||||||
39 | ||||||||
40 | ||||||||
41 | ||||||||
42 | ||||||||
43 | ||||||||
44 | ||||||||
45 | ||||||||
46 | ||||||||
47 | ||||||||
48 | ||||||||
49 | ||||||||
50 | ||||||||
51 | ||||||||
52 | ||||||||
53 | ||||||||
54 | ||||||||
55 | ||||||||
56 | Composite of JunoCam images in cylindrical map form by John Rogers and Gerald Eichstaedt | |||||||
57 | ||||||||
58 | ||||||||
59 | ||||||||
60 | ||||||||
61 | ||||||||
62 | ||||||||
63 | ||||||||
64 | ||||||||
65 | ||||||||
66 | ||||||||
67 | ||||||||
68 | ||||||||
69 | ||||||||
70 | ||||||||
71 | ||||||||
72 | ||||||||
73 | ||||||||
74 | ||||||||
75 | ||||||||
76 | ||||||||
77 | ||||||||
78 | ||||||||
79 | ||||||||
80 | ||||||||
81 | ||||||||
82 | ||||||||
83 | ||||||||
84 | ||||||||
85 | ||||||||
86 | Composite of JIRAM M-band (5-micron) map. | |||||||
87 | ||||||||
88 | ||||||||
89 | ||||||||
90 | ||||||||
91 | ||||||||
92 | ||||||||
93 | ||||||||
94 | ||||||||
95 | ||||||||
96 | ||||||||
97 | ||||||||
98 | ||||||||
99 | ||||||||
100 | ||||||||
101 | ||||||||
102 | ||||||||
103 | ||||||||
104 | ||||||||
105 | ||||||||
106 | ||||||||
107 | ||||||||
108 | ||||||||
109 | ||||||||
110 | ||||||||
111 | ||||||||
112 | ||||||||
113 | ||||||||
114 | ||||||||
115 | ||||||||
116 | ||||||||
117 | ||||||||
118 | ||||||||
119 | ||||||||
120 | ||||||||
121 | ||||||||
122 | ||||||||
123 | ||||||||
124 | ||||||||
125 | ||||||||
126 | ||||||||
127 | ||||||||
128 | ||||||||
129 | ||||||||
130 | ||||||||
131 | ||||||||
132 | ||||||||
133 | ||||||||
134 | ||||||||
135 | ||||||||
136 | ||||||||
137 | ||||||||
138 | ||||||||
139 | ||||||||
140 | ||||||||
141 | ||||||||
142 | ||||||||
143 | ||||||||
144 | ||||||||
145 | ||||||||
146 | ||||||||
147 | ||||||||
148 | ||||||||
149 | ||||||||
150 | ||||||||
151 | ||||||||
152 | ||||||||
153 | ||||||||
154 | ||||||||
155 | ||||||||
156 | ||||||||
157 | ||||||||
158 | MWR footprints for the minimum emission angle at each spacecraft rotation. The cross marks the location of the perijove. | |||||||
159 |
1 | Note: On this orbit the spacecraft orientation optimizes gravity mapping (GRAV) with the antenna pointed toward the Earth continuously. | ||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|
2 | |||||||||||
3 | Period: Orbit 31 [GRAV] (2020 Dec 30 - 2021 Feb 20) | Observations requested. | |||||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | Observations planned / granted time | ||||
5 | Observations successful | ||||||||||
6 | X-ray | Wibisono | XMM-Newton | ~340 ks of time-tagged spectra during Juno AJ, approach and PJ | 10-12 May, 2-3 June, 5-7 June (may be able to change to 7-9 June) | Propietary for 1 year then in the XMM public archive. I'm happy to share and collaborate, please just email me at affelia.wibisono.18@ucl.ac.uk | Observations cancelled or unsuccessful | ||||
7 | near IR | Orton | IRTF/MIRSI, repaced by SpeX observations in the near infrared | filtered imaging at several wavelengths between 5 and 18 µm | Dec 22-23, 13:00-16:00 HST | raw images available from IRTF web site; fully reduced images available within a month or sooner, as desired. MIRSI not available; SpeX observations will be made instead. | |||||
8 | radio | Zarka, Cecconi, Lamy, Louis | Nançay Decameter Array (France) | coordinated measurement of 10-40 MHz cyclotron radio emission | every day, 8 hours around the transition to local meridian | https://maser.lesia.obspm.fr/task-1-data-collections/juno-ground-radio/juno-ground-radio-nancay-decameter.html?lang=en | |||||
9 | radio | Louis/Jackman | LOFAR | ground-based radio observations of Jupiter with the LOFAR ground-based radio telescope | December 31st | will be analysed by team at Dublin Institute for Advanced Studies - contact corentin.louis@dias.ie and cjackman@cp.dias.ie directly to discuss | |||||
10 | radio | Kreuser-Jenkins/Huffine | DSS-13 | ground-based radio obervations of Jupiter using DSS13 via the GAVRT Program | 2021 January 12, 14, 19, 21 | raw data available upon request | |||||
11 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | 20201130 20201206 20201201 20201207 20201202 20201208 20201203 20201209 20201204 20201212 20201205 20201213 | ||||||
12 | Radio | Lamy for the NenuFar ES07 team | NenuFAR (France) | coordinated measurements of 10-40 MHz cyclotron radio emission at high time/frequency resolution | 2020 Dec. 30 09:15-17:30; 2020 Dec. 31 09:11-17:30; 2021 Feb. 20 06:23-15:33 | Data available on demand to laurent.lamy@obspm.fr | |||||
13 | |||||||||||
14 | |||||||||||
15 | |||||||||||
16 | |||||||||||
17 | Scheduled observations by Juno. | ||||||||||
18 | |||||||||||
19 | Perijove is 2020 Dec 30 21:45:08 UTC. System-III longitude = 117.7°W | ||||||||||
20 | |||||||||||
21 | Period: Orbit 31 [GRAV] (2020 Dec 30 - 2021 Feb 20) | ||||||||||
22 | Instrument | Description | |||||||||
23 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | |||||||||
24 | MWR | ||||||||||
25 | UVS | ||||||||||
26 | JunoCam | ||||||||||
27 | JIRAM | ||||||||||
28 | |||||||||||
29 | |||||||||||
30 | |||||||||||
31 | |||||||||||
32 | |||||||||||
33 | |||||||||||
34 | |||||||||||
35 | |||||||||||
36 | |||||||||||
37 | |||||||||||
38 | |||||||||||
39 | |||||||||||
40 | |||||||||||
41 | |||||||||||
42 | |||||||||||
43 | |||||||||||
44 | |||||||||||
45 | |||||||||||
46 | |||||||||||
47 | |||||||||||
48 | |||||||||||
49 | |||||||||||
50 | |||||||||||
51 | |||||||||||
52 | |||||||||||
53 | |||||||||||
54 | |||||||||||
55 | |||||||||||
56 | |||||||||||
57 | Composite JunoCam map | John Rogers & Gerald Eichstaedt | |||||||||
58 | |||||||||||
59 | |||||||||||
60 | |||||||||||
61 | |||||||||||
62 | |||||||||||
63 | |||||||||||
64 | |||||||||||
65 | |||||||||||
66 | |||||||||||
67 | |||||||||||
68 | |||||||||||
69 | |||||||||||
70 | |||||||||||
71 | |||||||||||
72 | |||||||||||
73 | |||||||||||
74 | |||||||||||
75 | |||||||||||
76 | |||||||||||
77 | |||||||||||
78 | |||||||||||
79 | |||||||||||
80 | |||||||||||
81 | |||||||||||
82 | |||||||||||
83 | |||||||||||
84 | |||||||||||
85 | |||||||||||
86 | |||||||||||
87 | |||||||||||
88 | |||||||||||
89 | Composite of JIRAM M-band (5-micron) map. | ||||||||||
90 | |||||||||||
91 | |||||||||||
92 | |||||||||||
93 | |||||||||||
94 | |||||||||||
95 | |||||||||||
96 | |||||||||||
97 | |||||||||||
98 | |||||||||||
99 | |||||||||||
100 | |||||||||||
101 | |||||||||||
102 | |||||||||||
103 | |||||||||||
104 | |||||||||||
105 | |||||||||||
106 | |||||||||||
107 | |||||||||||
108 | |||||||||||
109 | |||||||||||
110 | |||||||||||
111 | |||||||||||
112 | |||||||||||
113 | |||||||||||
114 | |||||||||||
115 | |||||||||||
116 | |||||||||||
117 | |||||||||||
118 | |||||||||||
119 | |||||||||||
120 | |||||||||||
121 | |||||||||||
122 | |||||||||||
123 | |||||||||||
124 | |||||||||||
125 | |||||||||||
126 | |||||||||||
127 | |||||||||||
128 | |||||||||||
129 | |||||||||||
130 | |||||||||||
131 | |||||||||||
132 | |||||||||||
133 | |||||||||||
134 | |||||||||||
135 | |||||||||||
136 | |||||||||||
137 | |||||||||||
138 | |||||||||||
139 | |||||||||||
140 | |||||||||||
141 | |||||||||||
142 | |||||||||||
143 | |||||||||||
144 | |||||||||||
145 | |||||||||||
146 | |||||||||||
147 | |||||||||||
148 | |||||||||||
149 | |||||||||||
150 | |||||||||||
151 | |||||||||||
152 | |||||||||||
153 | |||||||||||
154 | MWR footprints for the minimum emission angle at each spacecraft rotation. The cross marks the location of the perijove. | ||||||||||
155 | |||||||||||
156 |
1 | Note: On this orbit the spacecraft orientation optimizes gravity mapping (GRAV) with the antenna pointed toward the Earth continuously. | |||||||
---|---|---|---|---|---|---|---|---|
2 | Observations requested. | |||||||
3 | Period: Orbit 30 [GRAV] (2020 Nov 8 - 2020 Dec 29) | Observations planned / granted time | ||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | Observations successful | |
5 | FUV | Bonfond | HST/STIS | Timetag imaging of northern aurora | November 8 | MAST and video snapshots on Youtube | ||
6 | near IR (5 µm) | Wong | Gemini-N/NIRI | lucky imaging, 5-µm maps | observaion cancelled due to extended telescope repair period | Observations cancelled or unsuccessful | ||
7 | near IR | Orton | IRTF/SpeX | filtered imaging and scanning spectroscopy between 1.58 and 5.1µm | Nov 5-6 14:00-19:30HST | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired. Reduced "quick-look" observations (geometrically but not radiometrically calibrated) will be available for immeduately use from the Juno-curated web site: http://junoirtf.space.swri.edu/ | ||
8 | near IR | Orton | Gemini-N/NIRI | near-infrared imaging of reflected sunlight between 1.58 and 2.27 microns (adaptive-optics system is broken but will be requested if repaired in time for this observation) | observaion cancelled due to extended telescope repair period | avalable on request | ||
9 | near IR | Orton | IRTF/MIRSI originally scheduled, but SpeX substituted for MIRSI. Imaging and scanning spectroscopy were performed at near-infrared wavelengths successfully. | filtered imaging at several wavelengths between 7 and 18 µm | Nov 7-8 14:00-19:30 HST | raw images available from IRTF web site; fully reduced images available within a month or sooner, as desired. If MIRSI is not available; SpeX observations will be made instead. | ||
10 | near IR | Sinclair | IRTF/MIRSI | filtered imaging at several wavelengths between 7 and 14 µm; MIRSI was unavaialble, so imaging and scanning spectroscopy were performed of Jupiter instead, along with similar observations on Saturn. | Nov 9-10 14:00-20:00 | raw images available from IRTF web site; fully reduced images available within a month or sooner, as desired. If MIRSI is not available; SpeX observations will be made instead. | ||
11 | radio | Zarka, Cecconi, Lamy, Louis | Nançay Decameter Array (France) | coordinated measurement of 10-40 MHz cyclotron radio emission | every day, 8 hours around the transition to local meridian | https://maser.lesia.obspm.fr/task-1-data-collections/juno-ground-radio/juno-ground-radio-nancay-decameter.html?lang=en | ||
12 | radio | Imai | Long Wavelength Array station 1 (LWA-1), LWA-Sevilleta (LWA-SV) | Jupiter's decametric auroral radio observations | November 8-13 December 24-30 | Low-resolution LWA1 data are freely accessible via Autoplot (http://autoplot.org) by accepting the data usage policy (http://space.physics.uiowa.edu/earth/datapolicy.html) More information can be found at http://space.physics.uiowa.edu/earth/ | ||
13 | Radio | Levin et al. | GAVRT | 2.3 GHz measurements using DSSN13, 34-m DSN radio telescope | Nov 9-10 Nov 12 | |||
14 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | 20201109 20201130 20201111 20201201 20201112 20201202 20201118 20201203 20201119 20201204 20201120 20201205 20201121 20201206 20201122 20201207 20201124 20201208 20201125 20201209 20201126 20201212 20201127 20201213 20201128 20201214 20201129 | |||
15 | Radio | Lamy for the NenuFar ES07 team | NenuFAR (France) | coordinated measurements of 10-40 MHz cyclotron radio emission at high time/frequency resolution | Nov. 08 12:52-20:16; Dec. 09 11:00-18:49; Dec. 16 10:00-18:30; Dec. 21 13:34-18:15; Dec. 28 09:21-17:30; Dec. 29 09:18-17:30 | Data available on demand to laurent.lamy@obspm.fr | ||
16 | ||||||||
17 | Scheduled observations by Juno. | |||||||
18 | ||||||||
19 | Perijove is 2020 Nov 8 01:49:34 UTC. System-III longitude = 207.7°W | |||||||
20 | ||||||||
21 | Period: Orbit 30 (2020 Nov 8 - 2020 Dec 29) | |||||||
22 | Instrument | Description | ||||||
23 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||
24 | MWR | |||||||
25 | UVS | |||||||
26 | JunoCam | |||||||
27 | JIRAM | |||||||
28 | ||||||||
29 | ||||||||
30 | ||||||||
31 | ||||||||
32 | ||||||||
33 | ||||||||
34 | ||||||||
35 | ||||||||
36 | ||||||||
37 | ||||||||
38 | ||||||||
39 | ||||||||
40 | ||||||||
41 | ||||||||
42 | ||||||||
43 | ||||||||
44 | ||||||||
45 | ||||||||
46 | ||||||||
47 | ||||||||
48 | ||||||||
49 | ||||||||
50 | ||||||||
51 | ||||||||
52 | ||||||||
53 | ||||||||
54 | ||||||||
55 | ||||||||
56 | ||||||||
57 | ||||||||
58 | ||||||||
59 | ||||||||
60 | ||||||||
61 | ||||||||
62 | ||||||||
63 | ||||||||
64 | ||||||||
65 | ||||||||
66 | ||||||||
67 | ||||||||
68 | ||||||||
69 | ||||||||
70 | ||||||||
71 | ||||||||
72 | ||||||||
73 | ||||||||
74 | ||||||||
75 | ||||||||
76 | ||||||||
77 | ||||||||
78 | ||||||||
79 | ||||||||
80 | ||||||||
81 | ||||||||
82 | Diagram of JIRAM M-band imaging coverage. | |||||||
83 | ||||||||
84 | ||||||||
85 | ||||||||
86 | ||||||||
87 | ||||||||
88 | ||||||||
89 | ||||||||
90 | ||||||||
91 | ||||||||
92 | ||||||||
93 | ||||||||
94 | ||||||||
95 | ||||||||
96 | ||||||||
97 | ||||||||
98 | ||||||||
99 | ||||||||
100 | ||||||||
101 | ||||||||
102 | ||||||||
103 | ||||||||
104 | ||||||||
105 | ||||||||
106 | ||||||||
107 | ||||||||
108 | Composite of JunoCam images in cylindrical map form by John Rogers & Gerald Eichstaedt | |||||||
109 | ||||||||
110 | ||||||||
111 | ||||||||
112 | ||||||||
113 | ||||||||
114 | ||||||||
115 | ||||||||
116 | ||||||||
117 | ||||||||
118 | ||||||||
119 | ||||||||
120 | ||||||||
121 | ||||||||
122 | ||||||||
123 | ||||||||
124 | ||||||||
125 | ||||||||
126 | ||||||||
127 | ||||||||
128 | ||||||||
129 | ||||||||
130 | ||||||||
131 | ||||||||
132 | ||||||||
133 | ||||||||
134 | ||||||||
135 | ||||||||
136 | ||||||||
137 | Composite of JIRAM M-band (5-micron) map. | |||||||
138 | ||||||||
139 | ||||||||
140 | ||||||||
141 | ||||||||
142 | ||||||||
143 | ||||||||
144 | ||||||||
145 | ||||||||
146 | ||||||||
147 | ||||||||
148 | ||||||||
149 | ||||||||
150 | ||||||||
151 | ||||||||
152 | ||||||||
153 | ||||||||
154 | ||||||||
155 | ||||||||
156 | ||||||||
157 | ||||||||
158 | ||||||||
159 | ||||||||
160 | ||||||||
161 | ||||||||
162 | ||||||||
163 | ||||||||
164 | ||||||||
165 | ||||||||
166 | ||||||||
167 | ||||||||
168 | ||||||||
169 | ||||||||
170 | ||||||||
171 | ||||||||
172 | ||||||||
173 | ||||||||
174 | ||||||||
175 | ||||||||
176 | ||||||||
177 | ||||||||
178 | ||||||||
179 | ||||||||
180 | ||||||||
181 | ||||||||
182 | ||||||||
183 | ||||||||
184 | ||||||||
185 | ||||||||
186 | ||||||||
187 | ||||||||
188 | ||||||||
189 | ||||||||
190 | ||||||||
191 | ||||||||
192 | ||||||||
193 | ||||||||
194 | ||||||||
195 | ||||||||
196 | ||||||||
197 | ||||||||
198 | ||||||||
199 | ||||||||
200 | ||||||||
201 | ||||||||
202 | ||||||||
203 | ||||||||
204 | ||||||||
205 | ||||||||
206 | MWR footprints for the minimum emission angle at each latitude. The cross marks the location of the perijove. | |||||||
207 | ||||||||
208 | ||||||||
209 |
1 | Note: On this orbit the spacecraft orientation optimizes gravity mapping (GRAV) with the antenna pointed toward the Earth continuously. | |||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|
2 | Observations requested. | |||||||||||
3 | Period: Orbit 29 [GRAV] (2020 Sept 16 - 2020 Nov 8) | Observations planned / granted time | ||||||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | Observations successful | |||||
5 | visible/NUV | Wong (16074) | HST/WFC3 UVIS | hi-resolution map of perijove track, single orbit snapshot | September 15, 16:33-17:11 UT | https://archive.stsci.edu/prepds/wfcj/ https://doi.org/10.3847/1538-4365/ab775f https://doi.org/10.3390/rs15030702 | Observations cancelled or unsuccessful | |||||
6 | Visible | Dahl | APO 3.5-m / NAIC | Hyperspectral image cubes from 470-950 nm | Night of Sept. 15th, covering crossing longitude | TBD | ||||||
7 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | 20200916 20200930 20200917 20201001 20200918 20201002 20200919 20201003 20200920 20201004 20200921 20201005 20200922 20201006 20200923 20201007 20200924 20201008 20200925 20201009 20200926 20201010 20200927 20201011 20200928 20200929 | |||||||
8 | Visible, near IR (0.4-1.0) and Short-Wave IR (1.0-1.7 microns) | Sánchez-Lavega et al. | PlanetCam at Calar Alto 2.2m telescope | Photometric and high-resolution observations in multiple filters | Oct 30, 31 and November 1, 2 | Available upon request. Images have been pipelined and can be photometrically calibrated. High-resolution versions are also available. | ||||||
9 | near IR (5 µm) | Wong | Gemini-N/NIRI | lucky imaging, 5-µm maps | Sept 17, 07:51-08:24 | https://archive.stsci.edu/prepds/wfcj/ https://doi.org/10.3847/1538-4365/ab775f | ||||||
10 | near IR | Orton | IRTF/SpeX | filtered imaging and scanning spectroscopy between 1.58 and 5.1µm | Sep 20 18:45-23:00; Sep 2118:45-20:00; Oct 2-3 18:35-19:20 HST, Oct. 14,15 18:35-19:20 HST | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired. Reduced "quick-look" observations (geometrically but not radiometrically calibrated) will be available for immeduately use from the Juno-curated web site: http://junoirtf.space.swri.edu/ | ||||||
11 | near IR | Orton | Gemini-N/NIRI | near-infrared imaging of reflected sunlight between 1.58 and 2.27 microns (adaptive-optics system is broken but will be requested if repaired in time for this observation) | observations requested on dates near PJ29 and in mid-August and mid-October to monitor variability of the 3D structure of clouds and haze associated with the Great Red Spot. PJ29 dates are Sep 19, 20 UT. | avalable on request | ||||||
12 | mid IR | Fletcher | VLT / VISIR | filtered radiometric imaging to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology. M-band burst mode mapping. | Two hours of service time at perijove awarded, exact timing TBD. Aim to capture the PJ longitude within a week of the encounter. | Almost surely to be cancelled due to ongoing concerns about the pandemic to ESO staff | ||||||
13 | mid IR | Orton | IRTF/MIRSI now scheduled for IRTF / SpeX | filtered imaging at several wavelengths between 7 and 18 µm | Sep 16-17, 18:15-23:00; Spectroscopy and imaging with SpeX (near-infrared) on the first shift with photometry possible (we were observing among some clouds). Imaging only on the second shift with reduced transparency; we were observing through variable cirrus. Oct 8 18:00-21:00. High-resolution imaging of Jupiter but no spectroscopy. | raw images available from IRTF web site; fully reduced images available within a month or sooner, as desired. If MIRSI is not available; SpeX observations will be made instead. | Jupiter at 5.1 microns, Oct 9 UT | |||||
14 | mid IR | Antunano | 5-25 micron spectral imaging using TEXES | Jupiter's thermal infrared temperatures and atmospheric haze and hyrdrocarbon abundances | Sep 4-5, 18:15-23:00 HST | cancelled due to State of Hawaii quarantiine requirements | ||||||
15 | mid-IR | Sinclair | IRTF/TEXES | TEXES high-resolution spectroscopy of CH3, CH4, C2H2, C2H4, C2H6, H2 S(1) emission from mid-to-high latitudes. Retrieval analysis of CH3, CH4 and H2 S(1) emission will allow constraints on CH4 homopause altitude | September 14-15 18:15-23:00 | Cancelled due to quarantine requirements by the State of Hawaii | ||||||
16 | mid-IR | Sinclair | IRTF/TEXES | TEXES high-resolution spectroscopy of CH3, CH4, C2H2, C2H4, C2H6, H2 S(1) emission from mid-to-high latitudes. Retrieval analysis of CH3, CH4 and H2 S(1) emission will allow constraints on CH4 homopause altitude | September 14-15 18:15-23:00 | Cancelled due to quarantine requirements by the State of Hawaii | ||||||
17 | radio | Zarka, Cecconi, Lamy, Louis | Nançay Decameter Array (France) | coordinated measurement of 10-40 MHz cyclotron radio emission | every day, 8 hours around the transition to local meridian | https://maser.lesia.obspm.fr/task-1-data-collections/juno-ground-radio/juno-ground-radio-nancay-decameter.html?lang=en | ||||||
18 | radio | Imai | Long Wavelength Array station 1 (LWA-1), LWA-Sevilleta (LWA-SV) | Jupiter's decametric auroral radio observations | September 17-21 November 2-8 | Low-resolution LWA1 data are freely accessible via Autoplot (http://autoplot.org) by accepting the data usage policy (http://space.physics.uiowa.edu/earth/datapolicy.html) More information can be found at http://space.physics.uiowa.edu/earth/ | ||||||
19 | Radio | Leven et al. | GAVRT | 2.3 GHz measurements using DSSN13, 34-m DSN radio telescope, Ops; Newsome HS, FL | Sep 16. 23:48-6:03 | |||||||
20 | Radio | Leven et al. | GAVRT | 2.3 GHz measurements using DSSN13, 34-m DSN radio telescope | Oct 29-30 Nov 4-6 | |||||||
21 | Radio | Lamy for the NenuFar ES07 team | NenuFAR (France) | coordinated measurements of 10-40 MHz cyclotron radio emission at high time/frequency resolution | Sep. 16 15:18-23:23; Sep. 17 15:16-23:21; Sep. 29 14:30-22:36; Nov. 06 13:00-20:22; Nov. 07 12:56-20:19; Nov. 08 12:52-20:16 | Data available on demand to laurent.lamy@obspm.fr | ||||||
22 | Scheduled observations by Juno. | |||||||||||
23 | ||||||||||||
24 | Perijove is 2020 Sept 16 02:10:43 UTC. System-III longitude = 162.7°W | |||||||||||
25 | ||||||||||||
26 | Period: Orbit 29 (2020 Sept 16 - 2020 Nov 8) | |||||||||||
27 | Instrument | Description | ||||||||||
28 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||||
29 | MWR | |||||||||||
30 | UVS | |||||||||||
31 | JunoCam | |||||||||||
32 | JIRAM | |||||||||||
33 | ||||||||||||
34 | ||||||||||||
35 | ||||||||||||
36 | ||||||||||||
37 | ||||||||||||
38 | ||||||||||||
39 | ||||||||||||
40 | ||||||||||||
41 | ||||||||||||
42 | ||||||||||||
43 | ||||||||||||
44 | ||||||||||||
45 | ||||||||||||
46 | ||||||||||||
47 | ||||||||||||
48 | ||||||||||||
49 | ||||||||||||
50 | ||||||||||||
51 | ||||||||||||
52 | ||||||||||||
53 | ||||||||||||
54 | ||||||||||||
55 | ||||||||||||
56 | ||||||||||||
57 | ||||||||||||
58 | ||||||||||||
59 | ||||||||||||
60 | ||||||||||||
61 | ||||||||||||
62 | ||||||||||||
63 | ||||||||||||
64 | ||||||||||||
65 | ||||||||||||
66 | ||||||||||||
67 | ||||||||||||
68 | ||||||||||||
69 | ||||||||||||
70 | ||||||||||||
71 | ||||||||||||
72 | ||||||||||||
73 | ||||||||||||
74 | ||||||||||||
75 | ||||||||||||
76 | ||||||||||||
77 | ||||||||||||
78 | ||||||||||||
79 | ||||||||||||
80 | ||||||||||||
81 | ||||||||||||
82 | ||||||||||||
83 | ||||||||||||
84 | ||||||||||||
85 | ||||||||||||
86 | ||||||||||||
87 | ||||||||||||
88 | ||||||||||||
89 | ||||||||||||
90 | ||||||||||||
91 | Diagram of JIRAM M-band imaging coverage on PJ29. | |||||||||||
92 | ||||||||||||
93 | ||||||||||||
94 | ||||||||||||
95 | ||||||||||||
96 | ||||||||||||
97 | ||||||||||||
98 | ||||||||||||
99 | ||||||||||||
100 | ||||||||||||
101 | ||||||||||||
102 | ||||||||||||
103 | ||||||||||||
104 | ||||||||||||
105 | ||||||||||||
106 | ||||||||||||
107 | ||||||||||||
108 | ||||||||||||
109 | ||||||||||||
110 | ||||||||||||
111 | ||||||||||||
112 | ||||||||||||
113 | ||||||||||||
114 | ||||||||||||
115 | ||||||||||||
116 | ||||||||||||
117 | ||||||||||||
118 | ||||||||||||
119 | Composite of JIRAM M-band (5-micron) map. | |||||||||||
120 | ||||||||||||
121 | ||||||||||||
122 | ||||||||||||
123 | ||||||||||||
124 | ||||||||||||
125 | ||||||||||||
126 | ||||||||||||
127 | ||||||||||||
128 | ||||||||||||
129 | ||||||||||||
130 | ||||||||||||
131 | ||||||||||||
132 | ||||||||||||
133 | ||||||||||||
134 | ||||||||||||
135 | ||||||||||||
136 | ||||||||||||
137 | ||||||||||||
138 | ||||||||||||
139 | ||||||||||||
140 | ||||||||||||
141 | ||||||||||||
142 | ||||||||||||
143 | ||||||||||||
144 | ||||||||||||
145 | ||||||||||||
146 | ||||||||||||
147 | ||||||||||||
148 | ||||||||||||
149 | ||||||||||||
150 | ||||||||||||
151 | ||||||||||||
152 | ||||||||||||
153 | ||||||||||||
154 | ||||||||||||
155 | ||||||||||||
156 | ||||||||||||
157 | ||||||||||||
158 | ||||||||||||
159 | ||||||||||||
160 | ||||||||||||
161 | ||||||||||||
162 | ||||||||||||
163 | ||||||||||||
164 | ||||||||||||
165 | ||||||||||||
166 | ||||||||||||
167 | ||||||||||||
168 | ||||||||||||
169 | ||||||||||||
170 | ||||||||||||
171 | ||||||||||||
172 | ||||||||||||
173 | ||||||||||||
174 | ||||||||||||
175 | ||||||||||||
176 | ||||||||||||
177 | ||||||||||||
178 | ||||||||||||
179 | ||||||||||||
180 | ||||||||||||
181 | ||||||||||||
182 | ||||||||||||
183 | ||||||||||||
184 | ||||||||||||
185 | ||||||||||||
186 | ||||||||||||
187 | ||||||||||||
188 | ||||||||||||
189 | ||||||||||||
190 | ||||||||||||
191 | ||||||||||||
192 | MWR footprints for the minimum emission angle at each latitude. The cross marks the location of the perijove. | |||||||||||
193 | ||||||||||||
194 | ||||||||||||
195 | ||||||||||||
196 | ||||||||||||
197 | ||||||||||||
198 | ||||||||||||
199 | ||||||||||||
200 | ||||||||||||
201 | ||||||||||||
202 | ||||||||||||
203 | ||||||||||||
204 | ||||||||||||
205 | ||||||||||||
206 | ||||||||||||
207 | ||||||||||||
208 | ||||||||||||
209 | ||||||||||||
210 | ||||||||||||
211 | ||||||||||||
212 | ||||||||||||
213 | ||||||||||||
214 | ||||||||||||
215 | ||||||||||||
216 | ||||||||||||
217 | ||||||||||||
218 | ||||||||||||
219 | ||||||||||||
220 | ||||||||||||
221 | ||||||||||||
222 | ||||||||||||
223 | ||||||||||||
224 | ||||||||||||
225 | ||||||||||||
226 | ||||||||||||
227 | ||||||||||||
228 | ||||||||||||
229 | ||||||||||||
230 | ||||||||||||
231 | ||||||||||||
232 | ||||||||||||
233 | ||||||||||||
234 | ||||||||||||
235 | ||||||||||||
236 | ||||||||||||
237 | ||||||||||||
238 | ||||||||||||
239 | ||||||||||||
240 |
1 | ||||||||||
---|---|---|---|---|---|---|---|---|---|---|
2 | Observations requested. | |||||||||
3 | Period: Orbit 28 [GRAV] (2020 Jul 25 - 2020 Sept 15) | Observations planned / granted time | ||||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | Observations successful | |||
5 | Observations cancelled or unsuccessful | |||||||||
6 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | 20200726 20200820 20200728 20200821 20200729 20200822 20200730 20200825 20200731 20200826 20200801 20200827 20200804 20200902 20200806 20200903 20200808 20200904 20200809 20200905 20200810 20200907 20200811 20200908 20200818 20200910 20200819 20200915 | |||||
7 | Visible | Dahl | APO 3.5-m / NAIC | Hyperspectral image cubes from 470-950 nm | plus/minus 2 nights and PJ, covering crossing longitude | Observations not obtained due to inclement weather. | ||||
8 | Visible and near IR | Sánchez-Lavega | Calar Alto2.2m/PlanetCam | Lucky imaging observations from 0.4 to 1.7 microns | 27-30 August (re-scheduled from previously cancelled observations) | available on request | ||||
9 | visible/NUV/ near-IR | de Pater (16053) | Hubble Space Telescope / WFC3-UVIS | hi-resolution global maps | 2020 July 22–25 | Part of student's PhD thesis. Also: https://archive.stsci.edu/prepds/wfcj/ https://doi.org/10.3847/1538-4365/ab775f https://doi.org/10.3390/rs15030702 | ||||
10 | visible/IR | de Pater | Keck 1, 2 | visible HIRESR and 5 micron spectroscopy | July 24 and 25, quarters 2 and 3. Few NIRSPEC 5-mu spectra obtained July 24; none July 25. HIRES went well. | Raw data avalaible a yr after they have been taken. This is part of a student's PhD thesis. | ||||
11 | near IR | Bjoraker | IRTF/iSHELL | 5-micron spectroscopy | July 24, 27 UT | available on request | ||||
12 | near IR | Orton | Gemini-N/NIRI | adaptive-optics-stabilized imaging of reflected sunlight. Adaptive-optics hardware was not working. | observations obtained on July 25 - 26. Plus correlated with Subaru COMICS observations on July 29 and July 31. Additional observatiosn were made of the NTB upwelling on August 28 UT. | avalable on request | ||||
13 | near IR | Orton | IRTF/SpeX | filtered imaging at several wavelengths between 1.58 and 5.1µm | Aug 14-15 22:45-23:45 HST. Part of Augsut 14 observations suffered from inclement weather, but images in some filters were obtained. A full set of images were obtained on Aug. 15 in photometric weather and good seeing. Additional observations were made on Sept 16-21. | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired. Reduced "quick-look" observations (geometrically but not radiometrically calibrated) will be available for immeduately use from the Juno-curated web site: http://junoirtf.space.swri.edu/ | Jupiter at Brackett Gamma (2.16 microns), September 21 | |||
14 | mid IR | Antunano | 5-25 micron spectral imaging using TEXES | Jupiter's thermal infrared temperatures and atmospheric haze and hyrdrocarbon abundances | Sep 4-5, 18:15-23:00 HST | cancelled due to State of Hawaii quarantiine requirements | ||||
15 | mid IR | Sinclair | IRTF TEXES | mapping of auroral-related stratospheric heating | Sep 14-15 15:18-23:00 | cancelled due to State of Hawaii quarantiine requirements | ||||
16 | near IR (5 µm) | Wong | Gemini-N/NIRI | lucky imaging, 5-µm maps | July 23, 24, 25 | https://archive.stsci.edu/prepds/wfcj/ https://doi.org/10.3847/1538-4365/ab775f https://doi.org/10.1016/j.icarus.2022.114994 | ||||
17 | mid IR | Kasaba | Subaru / COMICS | filtered radiometric imaging and spectroscopy to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology and auroral heating and chemistry. | Mid-infrared imaging and spectroscopy July 28, 30 (full nights). This is the last semester COMICS will be made available. | Collaboration is possible with the investigators. | ||||
18 | mid IR | Fletcher | VLT / VISIR | filtered radiometric imaging to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology. M-band burst mode mapping. | Two hours of service time at perijove awarded, exact timing TBD. Aim to capture the PJ longitude within a week of the encounter. | VLT is still not operational due to COVID-related issues. | ||||
19 | microwave | Moeckel | VLA | radio, X and Ku bands | 4 nights, 2 on July 24, 25; 2 others 3 days earlier or later. | Observations not obtained due to equipment problems. | ||||
20 | radio | Zarka, Cecconi, Lamy, Louis | Nançay Decameter Array (France) | coordinated measurement of 10-40 MHz cyclotron radio emission | every day, 8 hours around the transition to local meridian | https://maser.lesia.obspm.fr/task-1-data-collections/juno-ground-radio/juno-ground-radio-nancay-decameter.html?lang=en | ||||
21 | radio | Imai | Long Wavelength Array station 1 (LWA-1), LWA-Sevilleta (LWA-SV) | Jupiter's decametric auroral radio observations | July 25-29 September 11-15 | Low-resolution LWA1 data are freely accessible via Autoplot (http://autoplot.org) by accepting the data usage policy (http://space.physics.uiowa.edu/earth/datapolicy.html) More information can be found at http://space.physics.uiowa.edu/earth/ | ||||
22 | Radio | Levin et al. | GAVRT | 2.3 GHz measurements using DSSN13, 34-m DSN radio telescope, Ops; Newsome HS, FL | Jul 24. 3:51-08:27 Jul 25. 4:07-08:24 Jul 26. 3:58-08:23 | |||||
23 | Radio | Lamy for the NenuFar ES07 team | NenuFAR (France) | coordinated measurements of 10-40 MHz cyclotron radio emission at high time/frequency resolution | Jul. 24 19:07- Jul. 25 03:10; Jul. 25 19:02 - Jul. 26 03:06; Jul. 26 18:58 - Jul. 27 03:01; Sep. 15 15:22 - 23:27 | Data available on demand to laurent.lamy@obspm.fr | ||||
24 | Scheduled observations by Juno. | |||||||||
25 | ||||||||||
26 | Perijove is 2020 Jul 25 06:15:14 UTC. System-III longitude = 252.8°W | |||||||||
27 | ||||||||||
28 | Period: Orbit 28 (2020 Jul 25 - 2020 Sept 16) | |||||||||
29 | Instrument | Description | ||||||||
30 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||
31 | MWR | |||||||||
32 | UVS | |||||||||
33 | JunoCam | |||||||||
34 | JIRAM | |||||||||
35 | ||||||||||
36 | ||||||||||
37 | ||||||||||
38 | ||||||||||
39 | ||||||||||
40 | ||||||||||
41 | ||||||||||
42 | ||||||||||
43 | ||||||||||
44 | ||||||||||
45 | ||||||||||
46 | ||||||||||
47 | ||||||||||
48 | ||||||||||
49 | ||||||||||
50 | ||||||||||
51 | ||||||||||
52 | ||||||||||
53 | ||||||||||
54 | ||||||||||
55 | ||||||||||
56 | ||||||||||
57 | ||||||||||
58 | ||||||||||
59 | ||||||||||
60 | ||||||||||
61 | ||||||||||
62 | ||||||||||
63 | ||||||||||
64 | ||||||||||
65 | ||||||||||
66 | ||||||||||
67 | ||||||||||
68 | ||||||||||
69 | ||||||||||
70 | ||||||||||
71 | ||||||||||
72 | ||||||||||
73 | ||||||||||
74 | ||||||||||
75 | ||||||||||
76 | ||||||||||
77 | ||||||||||
78 | ||||||||||
79 | ||||||||||
80 | ||||||||||
81 | ||||||||||
82 | ||||||||||
83 | ||||||||||
84 | ||||||||||
85 | ||||||||||
86 | ||||||||||
87 | Composite of JunoCam images in cylindrical format, with identification of specific features without the MWR footprints. | John Regers & Gerald Eichstaedt | ||||||||
88 | ||||||||||
89 | ||||||||||
90 | ||||||||||
91 | ||||||||||
92 | ||||||||||
93 | ||||||||||
94 | ||||||||||
95 | ||||||||||
96 | ||||||||||
97 | ||||||||||
98 | ||||||||||
99 | ||||||||||
100 | ||||||||||
101 | ||||||||||
102 | ||||||||||
103 | ||||||||||
104 | ||||||||||
105 | ||||||||||
106 | ||||||||||
107 | ||||||||||
108 | ||||||||||
109 | ||||||||||
110 | ||||||||||
111 | ||||||||||
112 | ||||||||||
113 | ||||||||||
114 | ||||||||||
115 | ||||||||||
116 | ||||||||||
117 | ||||||||||
118 | ||||||||||
119 | ||||||||||
120 | Composite of JIRAM M-band (5-micron) map. | |||||||||
121 | ||||||||||
122 | ||||||||||
123 | ||||||||||
124 | ||||||||||
125 | ||||||||||
126 | ||||||||||
127 | ||||||||||
128 | ||||||||||
129 | ||||||||||
130 | ||||||||||
131 | ||||||||||
132 | ||||||||||
133 | ||||||||||
134 | ||||||||||
135 | ||||||||||
136 | ||||||||||
137 | ||||||||||
138 | ||||||||||
139 | ||||||||||
140 | ||||||||||
141 | ||||||||||
142 | ||||||||||
143 | ||||||||||
144 | ||||||||||
145 | ||||||||||
146 | ||||||||||
147 | ||||||||||
148 | ||||||||||
149 | ||||||||||
150 | ||||||||||
151 | ||||||||||
152 | ||||||||||
153 | ||||||||||
154 | ||||||||||
155 | ||||||||||
156 | ||||||||||
157 | ||||||||||
158 | ||||||||||
159 | ||||||||||
160 | ||||||||||
161 | ||||||||||
162 | ||||||||||
163 | ||||||||||
164 | ||||||||||
165 | ||||||||||
166 | ||||||||||
167 | ||||||||||
168 | ||||||||||
169 | ||||||||||
170 | ||||||||||
171 | ||||||||||
172 | ||||||||||
173 | ||||||||||
174 | ||||||||||
175 | ||||||||||
176 | ||||||||||
177 | ||||||||||
178 | ||||||||||
179 | ||||||||||
180 | ||||||||||
181 | ||||||||||
182 | ||||||||||
183 | ||||||||||
184 | ||||||||||
185 | ||||||||||
186 | ||||||||||
187 | ||||||||||
188 | ||||||||||
189 | ||||||||||
190 | ||||||||||
191 | MWR footprints for the minimum emission angle at each latitude. The cross marks the location of the perijove. | |||||||||
192 | ||||||||||
193 |
1 | Note: On this orbit the spacecraft orientation optimizes gravity mapping (GRAV) with the antenna pointed toward the Earth continuously. | |||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|
2 | See also PJ28 for observations that include July 24. | Observations requested. | ||||||||||
3 | Period: Orbit 27 [GRAV] (2020 Jun 2 - 2020 Jul 24) | Observations planned / granted time | ||||||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | Observations successful | |||||
5 | Observations cancelled or unsuccessful | |||||||||||
6 | visible/NUV/ near-IR | Wong (16074) | Hubble/ WFC3-UVIS | hi-resolution non-global snapshot | 2 June UT 00:39 | https://archive.stsci.edu/prepds/wfcj/ https://doi.org/10.3847/1538-4365/ab775f https://doi.org/10.1016/j.icarus.2022.114994 | ||||||
7 | Visible | Dahl | APO 3.5-m / NAIC | Hyperspectral image cubes from 470-950 nm | cancelled due to COVID-19. | TBD | ||||||
8 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | 20200603 20200623 20200604 20200624 20200605 20200625 20200606 20200626 20200607 20200627 20200608 20200629 20200609 20200630 20200610 20200701 20200611 20200702 20200612 20200704 20200613 20200705 20200614 20200706 20200615 20200707 20200616 20200708 20200617 20200709 20200618 20200711 20200619 20200713 20200620 20200714 20200621 20200716 20200622 20200720 | |||||||
9 | Visible and near IR | Sánchez-Lavega | Calar Alto2.2m/PlanetCam | Lucky imaging observations from 0.4 to 1.7 microns | Cancelled due to COVID-19. Rescheduled for 27-30 August | available on request | ||||||
10 | near IR | Orton | Gemini-N/NIRI | adaptive-optics-stabilized imaging of reflected sunlight | observations obtained on June 21 and June 26. Adaptive-optics capability not available. | Originally scheduled June 4 and 6 observations cancelled due to helium leak in the NIRI instrument. | ||||||
11 | near IR (5 µm) | Wong | Gemini-N/NIRI | lucky imaging, 5-µm maps | June 2 observation cancelled due to helium leak in NIRI instrument | |||||||
12 | near IR | Bjoraker | IRTF/iSHELL | 5-micron spectroscopy | June 2 and June 4 UT | available on request | ||||||
13 | mid IR | Orton (Keck exchange time) | Subaru / COMICS | filtered radiometric imaging and spectroscopy to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology and auroral heating and chemistry. | Mid-infrared imaging was performed on June 2 with interruption from weather and equipment problems, but with excellent seeing. Images were also obtained with no problems on June 3 of the opposite hemisphere but additional coverage of the PJ27 track. | Collaboration is possible with the investigators. | ||||||
14 | mid IR | Antunano | 5-25 micron spectral imaging using TEXES/IRTF | Jupiter's thermal infrared temperatures and atmospheric haze and hyrdrocarbon abundances | Observations were cancelled due to COVID-19-related travel restrictions to Hawaii required for operation of the TEXES instrument. | Observations were replaced in the IRTF schedule with near-infrared imaging of Jupiter using the SpeX facility instrument on July 3 and 4. | ||||||
15 | mid IR | Fletcher | VLT / VISIR | filtered radiometric imaging to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology. M-band burst mode mapping. | Service-time observations were cancelled due to COVID-19. | available in raw form in the ESO archive within 24 hours of acquisition; cylindrical maps within 1-2 days and reduced maps within a week | ||||||
16 | radio | Zarka, Cecconi, Lamy, Louis | Nançay Decameter Array (France) | coordinated measurement of 10-40 MHz cyclotron radio emission | every day, 8 hours around the transition to local meridian | https://maser.lesia.obspm.fr/task-1-data-collections/juno-ground-radio/juno-ground-radio-nancay-decameter.html?lang=en | ||||||
17 | radio | Imai | Long Wavelength Array station 1 (LWA-1), LWA-Sevilleta (LWA-SV) | Jupiter's decametric auroral radio observations | June 2-5 July 20-24 | Low-resolution LWA1 data are freely accessible via Autoplot (http://autoplot.org) by accepting the data usage policy (http://space.physics.uiowa.edu/earth/datapolicy.html) More information can be found at http://space.physics.uiowa.edu/earth/ | ||||||
18 | Radio | Leven et al. | GAVRT | 2.3 GHz measurements using DSSN13, 34-m DSN radio telescope, Ops | Jul 24. 3:51-08:27 | |||||||
19 | Radio | Lamy for the NenuFar ES07 team | NenuFAR (France) | coordinated measurements of 10-40 MHz cyclotron radio emission at high time/frequency resolution | Jun. 02 22:56-06:58 Jul. 22 19:16-03:19 Jul. 24 19:07- Jul. 25 03:10 | Data available on demand to laurent.lamy@obspm.fr | ||||||
20 | ||||||||||||
21 | Scheduled observations by Juno. | |||||||||||
22 | ||||||||||||
23 | Perijove is 2020 Jun 2 10:19:47 UTC. System-III longitude = 342.9°W | |||||||||||
24 | ||||||||||||
25 | Period: Orbit 27 (2020 Jun 2 - 2020 Jul 25) | |||||||||||
26 | Instrument | Description | ||||||||||
27 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||||
28 | MWR | |||||||||||
29 | UVS | |||||||||||
30 | JunoCam | |||||||||||
31 | JIRAM | |||||||||||
32 | ||||||||||||
33 | ||||||||||||
34 | ||||||||||||
35 | ||||||||||||
36 | ||||||||||||
37 | ||||||||||||
38 | ||||||||||||
39 | ||||||||||||
40 | ||||||||||||
41 | ||||||||||||
42 | ||||||||||||
43 | ||||||||||||
44 | ||||||||||||
45 | ||||||||||||
46 | ||||||||||||
47 | ||||||||||||
48 | ||||||||||||
49 | ||||||||||||
50 | ||||||||||||
51 | ||||||||||||
52 | ||||||||||||
53 | ||||||||||||
54 | ||||||||||||
55 | ||||||||||||
56 | ||||||||||||
57 | ||||||||||||
58 | ||||||||||||
59 | ||||||||||||
60 | ||||||||||||
61 | ||||||||||||
62 | ||||||||||||
63 | ||||||||||||
64 | ||||||||||||
65 | ||||||||||||
66 | ||||||||||||
67 | ||||||||||||
68 | ||||||||||||
69 | ||||||||||||
70 | ||||||||||||
71 | ||||||||||||
72 | ||||||||||||
73 | ||||||||||||
74 | ||||||||||||
75 | ||||||||||||
76 | ||||||||||||
77 | ||||||||||||
78 | ||||||||||||
79 | ||||||||||||
80 | ||||||||||||
81 | ||||||||||||
82 | ||||||||||||
83 | ||||||||||||
84 | ||||||||||||
85 | ||||||||||||
86 | ||||||||||||
87 | ||||||||||||
88 | ||||||||||||
89 | ||||||||||||
90 | Composite of JunoCam images in cylindrical format, with identification of specific features without the MWR footprints. | John Rogers & Gerald Eichstaedt | ||||||||||
91 | ||||||||||||
92 | ||||||||||||
93 | ||||||||||||
94 | ||||||||||||
95 | ||||||||||||
96 | ||||||||||||
97 | ||||||||||||
98 | ||||||||||||
99 | ||||||||||||
100 | ||||||||||||
101 | ||||||||||||
102 | ||||||||||||
103 | ||||||||||||
104 | ||||||||||||
105 | ||||||||||||
106 | ||||||||||||
107 | ||||||||||||
108 | ||||||||||||
109 | ||||||||||||
110 | ||||||||||||
111 | ||||||||||||
112 | ||||||||||||
113 | ||||||||||||
114 | ||||||||||||
115 | ||||||||||||
116 | ||||||||||||
117 | ||||||||||||
118 | ||||||||||||
119 | ||||||||||||
120 | ||||||||||||
121 | ||||||||||||
122 | ||||||||||||
123 | ||||||||||||
124 | ||||||||||||
125 | ||||||||||||
126 | ||||||||||||
127 | ||||||||||||
128 | ||||||||||||
129 | ||||||||||||
130 | ||||||||||||
131 | ||||||||||||
132 | ||||||||||||
133 | ||||||||||||
134 | JIRAM fields of view. | |||||||||||
135 | The dates reported (both in UTC and in hours from PJ) on the top are referred to the last acquisition with the M filter of the whole plan for the given JM | |||||||||||
136 | The # field, is the estimated number of the acquisition of the whole plan, | |||||||||||
137 | (Ignore the percentage field.) | |||||||||||
138 | The light blue area, enclosed by dark blue lines, represented the FoVs of Imager M projected on Jupiter. Dark blue areas that you can see in some positions are created | |||||||||||
139 | by more projected FoV overlapping at close distance; i.e. these zones are created by multi FoV edges ( dark blue lines) that plot each close to the other create these graphic artefacts | |||||||||||
140 | The background cloud rendition is for general orientation; the position of the Great Red Spot does not indicate its actual position during these observations. | |||||||||||
141 | ||||||||||||
142 | ||||||||||||
143 | ||||||||||||
144 | ||||||||||||
145 | ||||||||||||
146 | ||||||||||||
147 | ||||||||||||
148 | ||||||||||||
149 | ||||||||||||
150 | ||||||||||||
151 | ||||||||||||
152 | ||||||||||||
153 | ||||||||||||
154 | ||||||||||||
155 | ||||||||||||
156 | ||||||||||||
157 | ||||||||||||
158 | ||||||||||||
159 | ||||||||||||
160 | ||||||||||||
161 | ||||||||||||
162 | ||||||||||||
163 | ||||||||||||
164 | ||||||||||||
165 | ||||||||||||
166 | ||||||||||||
167 | ||||||||||||
168 | ||||||||||||
169 | ||||||||||||
170 | ||||||||||||
171 | ||||||||||||
172 | ||||||||||||
173 | ||||||||||||
174 | ||||||||||||
175 | Composite of JIRAM M-band (5-micron) map. | |||||||||||
176 | ||||||||||||
177 | ||||||||||||
178 | ||||||||||||
179 | ||||||||||||
180 | ||||||||||||
181 | ||||||||||||
182 | ||||||||||||
183 | ||||||||||||
184 | ||||||||||||
185 | ||||||||||||
186 | ||||||||||||
187 | ||||||||||||
188 | ||||||||||||
189 | ||||||||||||
190 | ||||||||||||
191 | ||||||||||||
192 | ||||||||||||
193 | ||||||||||||
194 | ||||||||||||
195 | ||||||||||||
196 | ||||||||||||
197 | ||||||||||||
198 | ||||||||||||
199 | ||||||||||||
200 | ||||||||||||
201 | ||||||||||||
202 | ||||||||||||
203 | ||||||||||||
204 | ||||||||||||
205 | ||||||||||||
206 | ||||||||||||
207 | ||||||||||||
208 | ||||||||||||
209 | ||||||||||||
210 | ||||||||||||
211 | ||||||||||||
212 | ||||||||||||
213 | ||||||||||||
214 | ||||||||||||
215 | ||||||||||||
216 | ||||||||||||
217 | ||||||||||||
218 | ||||||||||||
219 | ||||||||||||
220 | ||||||||||||
221 | ||||||||||||
222 | ||||||||||||
223 | ||||||||||||
224 | ||||||||||||
225 | ||||||||||||
226 | ||||||||||||
227 | ||||||||||||
228 | ||||||||||||
229 | ||||||||||||
230 | ||||||||||||
231 | ||||||||||||
232 | ||||||||||||
233 | ||||||||||||
234 | MWR footprints for the minimum emission angle at each latitude. The cross marks the location of the perijove. | |||||||||||
235 |
1 | ||||||||
---|---|---|---|---|---|---|---|---|
2 | Observations requested. | |||||||
3 | Period: Orbit 26 [OAA] (2020 Apr 10 - 2020 Jun 1) | Observations planned / granted time | ||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | Observations successful | |
5 | FUV | Grodent | HST/COS | Io Eclipse Spectroscopy | 26 April UT | Data publically archived: HST GO # 15638 | Observations cancelled or unsuccessful | |
6 | visible/NUV/ near-IR | Wong (16074) | Hubble/ WFC3-UVIS | hi-resolution non-global snapshot | 10 Apr UT 23:48 | https://archive.stsci.edu/prepds/wfcj/ https://doi.org/10.3847/1538-4365/ab775f https://doi.org/10.1016/j.icarus.2022.114994 | ||
7 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | 20200410 20200504 20200411 20200505 20200413 20200506 20200414 20200507 20200415 20200508 20200416 20200512 20200417 20200513 20200418 20200514 20200419 20200515 20200420 20200516 20200421 20200517 20200422 20200518 20200423 20200519 20200424 20200520 20200425 20200521 20200426 20200522 20200427 20200523 20200428 20200524 20200429 20200525 20200430 20200526 20200502 20200527 20200503 20200528 20200529 | |||
8 | Visible | Schmidt | Keck / HIRES | Io Eclipse Spectroscopy | April 26 UT | cancelled due to COVID-19 related Keck closure of operations | ||
9 | near IR | Orton | Gemini-N/NIRI | adaptive-optics-stabilized imaging of reflected sunlight | observations requested on dates near PJ26 when Galilean satellites are available as wave-front sensors: April 10, 14:47-15:30 at the PJ26 longitude, a complementary longitude on April 4. Also on April 22, May 11 and May 28 to track the evolution of 3D structure of clouds and haze associated with the Great Red Spot at high resolutioj. | avalable on request (note April and some May dates are cancelled due to COVID-19-related closure of telescope operations) | ||
10 | near IR (5 µm) | Wong | Gemini-N/NIRI | lucky imaging, 5-µm maps | April 10 UT 14:00 | cancelled due to COVID-19-related Gemini N closure of operations | ||
11 | near IR | Bjoraker | IRTF/iSHELL | 5-micron spectroscopy | April 15 and April 22 UT | cancelled due to COVID-19 related Keck closure of operations | ||
12 | mid IR | Fletcher | VLT / VISIR | filtered radiometric imaging to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology. M-band burst mode mapping. | Six hours of service time at perijove awarded to cover all longitudes, exact timing TBD. | candelled due to COVID-19-related Very Large Telescope closure of operations | ||
13 | mid IR | Antunano | 5-25 micron spectral imaging using TEXES | Jupiter's thermal infrared temperatures and atmospheric haze and hyrdrocarbon abundances | April 8-10th (3.5 hours each night) | Observations Cancelled due to Corona Virus Pandemic | ||
14 | radio | Zarka, Cecconi, Lamy, Louis | Nançay Decameter Array (France) | coordinated measurement of 10-40 MHz cyclotron radio emission | every day, 8 hours around the transition to local meridian | https://maser.lesia.obspm.fr/task-1-data-collections/juno-ground-radio/juno-ground-radio-nancay-decameter.html?lang=en | ||
15 | radio | Imai | Long Wavelength Array station 1 (LWA-1), LWA-Sevilleta (LWA-SV) | Jupiter's decametric auroral radio observations | April 10-13 May 26-29 | Low-resolution LWA1 data are freely accessible via Autoplot (http://autoplot.org) by accepting the data usage policy (http://space.physics.uiowa.edu/earth/datapolicy.html) More information can be found at http://space.physics.uiowa.edu/earth/ | ||
16 | Radio | Levin et al. | GAVRT | 2.3 GHz measurements using DSSN13, 34-m DSN radio telescope, Ops; Newsome, FL High School Students + 4 additional schools; El Dorado Library | May 7 May 19 Jun 1. 8:37-13:22 | |||
17 | Radio | Lamy for the NenuFar ES07 team | NenuFAR (France) | coordinated measurements of 10-40 MHz cyclotron radio emission at high time/frequency resolution | Apr. 10 02:25-10:25; Apr. 11 02:21-10:21; May 10 03:04-05:54; Jun. 01 00:00-07:07; Jun. 01 23:00-07:02 | Data available on demand to laurent.lamy@obspm.fr | ||
18 | Scheduled observations by Juno. | |||||||
19 | ||||||||
20 | Perijove is 2020 Apr 10 13:47:11 UTC. System-III longitude = 50.5°W | |||||||
21 | ||||||||
22 | Period: Orbit 26 (2020 Apr 10 - 2020 Jun 2) | |||||||
23 | Instrument | Description | ||||||
24 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. See figures below for track through magnetic coordinates. | ||||||
25 | MWR | Coverage is shown on the figure below | ||||||
26 | UVS | |||||||
27 | JunoCam | Coverage is shown in the figure below. | ||||||
28 | JIRAM | Coverage is shown in the figure below. | ||||||
29 | ||||||||
30 | ||||||||
31 | ||||||||
32 | ||||||||
33 | ||||||||
34 | ||||||||
35 | ||||||||
36 | ||||||||
37 | ||||||||
38 | ||||||||
39 | ||||||||
40 | ||||||||
41 | ||||||||
42 | ||||||||
43 | ||||||||
44 | ||||||||
45 | ||||||||
46 | ||||||||
47 | ||||||||
48 | ||||||||
49 | ||||||||
50 | ||||||||
51 | ||||||||
52 | ||||||||
53 | ||||||||
54 | ||||||||
55 | ||||||||
56 | ||||||||
57 | ||||||||
58 | ||||||||
59 | ||||||||
60 | ||||||||
61 | ||||||||
62 | ||||||||
63 | ||||||||
64 | ||||||||
65 | ||||||||
66 | ||||||||
67 | ||||||||
68 | ||||||||
69 | ||||||||
70 | ||||||||
71 | ||||||||
72 | ||||||||
73 | ||||||||
74 | ||||||||
75 | ||||||||
76 | ||||||||
77 | ||||||||
78 | ||||||||
79 | ||||||||
80 | ||||||||
81 | ||||||||
82 | ||||||||
83 | Composite of JunoCam images in cylindrical format, with identification of specific features overlain by the MWR footprints. | John Rogers & Gerald Eichstaedt | ||||||
84 | ||||||||
85 | ||||||||
86 | ||||||||
87 | ||||||||
88 | ||||||||
89 | ||||||||
90 | ||||||||
91 | ||||||||
92 | ||||||||
93 | ||||||||
94 | ||||||||
95 | ||||||||
96 | ||||||||
97 | ||||||||
98 | ||||||||
99 | ||||||||
100 | ||||||||
101 | ||||||||
102 | ||||||||
103 | ||||||||
104 | ||||||||
105 | ||||||||
106 | ||||||||
107 | ||||||||
108 | ||||||||
109 | ||||||||
110 | ||||||||
111 | Composite of JunoCam images in cylindrical format, with identification of specific features without the MWR footprints. | John Rogers & Gerald Eichstaedt | ||||||
112 | ||||||||
113 | ||||||||
114 | ||||||||
115 | ||||||||
116 | ||||||||
117 | ||||||||
118 | ||||||||
119 | ||||||||
120 | ||||||||
121 | ||||||||
122 | ||||||||
123 | ||||||||
124 | ||||||||
125 | ||||||||
126 | ||||||||
127 | ||||||||
128 | ||||||||
129 | ||||||||
130 | ||||||||
131 | ||||||||
132 | ||||||||
133 | ||||||||
134 | ||||||||
135 | ||||||||
136 | ||||||||
137 | ||||||||
138 | ||||||||
139 | ||||||||
140 | ||||||||
141 | ||||||||
142 | ||||||||
143 | ||||||||
144 | ||||||||
145 | Composite of JIRAM M-band (5-micron) map. | |||||||
146 | ||||||||
147 | ||||||||
148 | ||||||||
149 | ||||||||
150 | ||||||||
151 | ||||||||
152 | ||||||||
153 | ||||||||
154 | ||||||||
155 | ||||||||
156 | ||||||||
157 | ||||||||
158 | ||||||||
159 | ||||||||
160 | ||||||||
161 | ||||||||
162 | ||||||||
163 | ||||||||
164 | ||||||||
165 | ||||||||
166 | ||||||||
167 | ||||||||
168 | ||||||||
169 | ||||||||
170 | ||||||||
171 | ||||||||
172 | ||||||||
173 | ||||||||
174 | ||||||||
175 | ||||||||
176 | ||||||||
177 | ||||||||
178 | ||||||||
179 | ||||||||
180 | ||||||||
181 | JIRAM fields of view. | |||||||
182 | The dates reported (both in UTC and in hours from PJ) on the top are referred to the last acquisition with the M filter of the whole plan for the given JM | |||||||
183 | The # field, is the estimated number of the acquisition of the whole plan, | |||||||
184 | (Ignore the percentage field.) | |||||||
185 | The light blue area, enclosed by dark blue lines, represented the FoVs of Imager M projected on Jupiter. Dark blue areas that you can see in some positions are created | |||||||
186 | by more projected FoV overlapping at close distance; i.e. these zones are created by multi FoV edges ( dark blue lines) that plot each close to the other create these graphic artefacts | |||||||
187 | The background cloud rendition is for general orientation; the position of the Great Red Spot does not indicate its actual position during these observations. | |||||||
188 | ||||||||
189 | ||||||||
190 | ||||||||
191 | ||||||||
192 | ||||||||
193 | ||||||||
194 | ||||||||
195 | ||||||||
196 | ||||||||
197 | ||||||||
198 | ||||||||
199 | ||||||||
200 | ||||||||
201 | ||||||||
202 | ||||||||
203 | ||||||||
204 | ||||||||
205 | ||||||||
206 | ||||||||
207 | ||||||||
208 | ||||||||
209 | ||||||||
210 | ||||||||
211 | ||||||||
212 | ||||||||
213 | ||||||||
214 | ||||||||
215 | ||||||||
216 | ||||||||
217 | ||||||||
218 | ||||||||
219 | ||||||||
220 | ||||||||
221 | ||||||||
222 | ||||||||
223 | ||||||||
224 | ||||||||
225 | ||||||||
226 | ||||||||
227 | ||||||||
228 | ||||||||
229 | ||||||||
230 | ||||||||
231 | ||||||||
232 | ||||||||
233 | ||||||||
234 | ||||||||
235 | ||||||||
236 | ||||||||
237 | ||||||||
238 | ||||||||
239 | ||||||||
240 | ||||||||
241 | ||||||||
242 | ||||||||
243 | ||||||||
244 | ||||||||
245 | ||||||||
246 | ||||||||
247 | ||||||||
248 | ||||||||
249 | ||||||||
250 | ||||||||
251 | ||||||||
252 | MWR footprints for the minimum emission angle at each latitude. The cross marks the location of the perijove. |
1 | Note: On this orbit the spacecraft orientation optimizes gravity mapping (GRAV) with the antenna pointed toward the Earth continuously. | ||||||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
2 | |||||||||||||||||
3 | Period: Orbit 25 [GRAV] (2020 Feb 17 - 2020 Apr 9) | ||||||||||||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | Observations requested. | ||||||||||
5 | Observations planned / granted time | ||||||||||||||||
6 | Observations successful | ||||||||||||||||
7 | Observations cancelled or unsuccessful | ||||||||||||||||
8 | Visible | Schmidt | Apache Point / ARCES | Io Eclipse Spectroscopy | March 27 UT | cancelled due to closure of APO operations due to COVID-19 | |||||||||||
9 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | 20200324 20200402 20200325 20200403 20200326 20200404 20200328 20200405 20200329 20200407 20200330 20200408 20200331 20200409 | ||||||||||||
10 | radio | Imai | Long Wavelength Array station 1 (LWA-1), LWA-Sevilleta (LWA-SV) | Jupiter's decametric auroral radio observations | February 17-22 April 5-9 | Low-resolution LWA1 data are freely accessible via Autoplot (http://autoplot.org) by accepting the data usage policy (http://space.physics.uiowa.edu/earth/datapolicy.html) More information can be found at http://space.physics.uiowa.edu/earth/ | |||||||||||
11 | Radio | Leven et al. | GAVRT | 2.3 GHz measurements using DSSN13, 34-m DSN radio telescope, Ops; Newport MS, PA; Cardinal Gibbons, NC; Newsome, FL High School Students | Feb 25. 15:12-17:25 Feb 27 Mar 3 Mar 11 Mar 31 Apr 2 Apr 7. 12:07-12:37 Apr 8. 12:08-15:30 Apr 9. 11:52-16:24 | ||||||||||||
12 | radio | Zarka, Cecconi, Lamy, Louis | Nançay Decameter Array (France) | coordinated measurement of 10-40 MHz cyclotron radio emission | every day, 8 hours around the transition to local meridian | https://maser.lesia.obspm.fr/task-1-data-collections/juno-ground-radio/juno-ground-radio-nancay-decameter.html?lang=en | |||||||||||
13 | Radio | Lamy for the NenuFar ES07 team | NenuFAR (France) | coordinated measurements of 10-40 MHz cyclotron radio emission at high time/frequency resolution | Feb. 17 05:27-13:09 Feb. 18 05:23-10:30 Apr. 01 05:59-09:01 | Data available on demand to laurent.lamy@obspm.fr | |||||||||||
14 | |||||||||||||||||
15 | Scheduled observations by Juno. | ||||||||||||||||
16 | |||||||||||||||||
17 | Perijove is 2020 Feb 17 17:51:42 UTC. System-III longitude = 140.6°W | ||||||||||||||||
18 | |||||||||||||||||
19 | Period: Orbit 25 (2020 Feb 17 - 2020 Apr 10) | ||||||||||||||||
20 | Instrument | Description | |||||||||||||||
21 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | |||||||||||||||
22 | MWR | ||||||||||||||||
23 | UVS | ||||||||||||||||
24 | JunoCam | ||||||||||||||||
25 | JIRAM | ||||||||||||||||
26 | |||||||||||||||||
27 | |||||||||||||||||
28 | |||||||||||||||||
29 | |||||||||||||||||
30 | |||||||||||||||||
31 | |||||||||||||||||
32 | |||||||||||||||||
33 | |||||||||||||||||
34 | |||||||||||||||||
35 | |||||||||||||||||
36 | |||||||||||||||||
37 | |||||||||||||||||
38 | |||||||||||||||||
39 | |||||||||||||||||
40 | |||||||||||||||||
41 | |||||||||||||||||
42 | |||||||||||||||||
43 | |||||||||||||||||
44 | |||||||||||||||||
45 | |||||||||||||||||
46 | |||||||||||||||||
47 | |||||||||||||||||
48 | |||||||||||||||||
49 | |||||||||||||||||
50 | |||||||||||||||||
51 | |||||||||||||||||
52 | |||||||||||||||||
53 | |||||||||||||||||
54 | |||||||||||||||||
55 | |||||||||||||||||
56 | |||||||||||||||||
57 | |||||||||||||||||
58 | |||||||||||||||||
59 | |||||||||||||||||
60 | |||||||||||||||||
61 | |||||||||||||||||
62 | |||||||||||||||||
63 | |||||||||||||||||
64 | |||||||||||||||||
65 | |||||||||||||||||
66 | |||||||||||||||||
67 | |||||||||||||||||
68 | |||||||||||||||||
69 | |||||||||||||||||
70 | |||||||||||||||||
71 | |||||||||||||||||
72 | MWR footprints for the minimum emission angle at each latitude. | ||||||||||||||||
73 | |||||||||||||||||
74 | |||||||||||||||||
75 | |||||||||||||||||
76 | |||||||||||||||||
77 | |||||||||||||||||
78 | |||||||||||||||||
79 | |||||||||||||||||
80 | |||||||||||||||||
81 | |||||||||||||||||
82 | |||||||||||||||||
83 | |||||||||||||||||
84 | |||||||||||||||||
85 | |||||||||||||||||
86 | |||||||||||||||||
87 | |||||||||||||||||
88 | |||||||||||||||||
89 | |||||||||||||||||
90 | |||||||||||||||||
91 | |||||||||||||||||
92 | |||||||||||||||||
93 | |||||||||||||||||
94 | |||||||||||||||||
95 | |||||||||||||||||
96 | |||||||||||||||||
97 | |||||||||||||||||
98 | |||||||||||||||||
99 | |||||||||||||||||
100 | |||||||||||||||||
101 | |||||||||||||||||
102 | MWR footprints for the minimum emission angle at each longitude. | ||||||||||||||||
103 | |||||||||||||||||
104 | |||||||||||||||||
105 | |||||||||||||||||
106 | |||||||||||||||||
107 | |||||||||||||||||
108 | |||||||||||||||||
109 | |||||||||||||||||
110 | |||||||||||||||||
111 | |||||||||||||||||
112 | |||||||||||||||||
113 | |||||||||||||||||
114 | |||||||||||||||||
115 | |||||||||||||||||
116 | |||||||||||||||||
117 | |||||||||||||||||
118 | |||||||||||||||||
119 | |||||||||||||||||
120 | |||||||||||||||||
121 | |||||||||||||||||
122 | |||||||||||||||||
123 | |||||||||||||||||
124 | |||||||||||||||||
125 | |||||||||||||||||
126 | |||||||||||||||||
127 | |||||||||||||||||
128 | |||||||||||||||||
129 | |||||||||||||||||
130 | |||||||||||||||||
131 | |||||||||||||||||
132 | |||||||||||||||||
133 | |||||||||||||||||
134 | |||||||||||||||||
135 | JIRAM fields of view. | ||||||||||||||||
136 | The dates reported (both in UTC and in hours from PJ) on the top are referred to the last acquisition with the M filter of the whole plan for the given JM | ||||||||||||||||
137 | The # field, is the estimated number of the acquisition of the whole plan, | ||||||||||||||||
138 | (Ignore the percentage field.) | ||||||||||||||||
139 | The light blue area, enclosed by dark blue lines, represented the FoVs of Imager M projected on Jupiter. Dark blue areas that you can see in some positions are created | ||||||||||||||||
140 | by more projected FoV overlapping at close distance; i.e. these zones are created by multi FoV edges ( dark blue lines) that plot each close to the other create these graphic artefacts | ||||||||||||||||
141 | The background cloud rendition is for general orientation; the position of the Great Red Spot does not indicate its actual position during these observations. | ||||||||||||||||
142 | |||||||||||||||||
143 | |||||||||||||||||
144 | |||||||||||||||||
145 | |||||||||||||||||
146 | |||||||||||||||||
147 | |||||||||||||||||
148 | |||||||||||||||||
149 | |||||||||||||||||
150 | |||||||||||||||||
151 | |||||||||||||||||
152 | |||||||||||||||||
153 | |||||||||||||||||
154 | |||||||||||||||||
155 | |||||||||||||||||
156 | |||||||||||||||||
157 | |||||||||||||||||
158 | |||||||||||||||||
159 | |||||||||||||||||
160 | |||||||||||||||||
161 | |||||||||||||||||
162 | |||||||||||||||||
163 | |||||||||||||||||
164 | |||||||||||||||||
165 | |||||||||||||||||
166 | |||||||||||||||||
167 | |||||||||||||||||
168 | |||||||||||||||||
169 | |||||||||||||||||
170 | Composite of JIRAM M-band (5-micron) map. | ||||||||||||||||
171 | |||||||||||||||||
172 | |||||||||||||||||
173 | |||||||||||||||||
174 | |||||||||||||||||
175 | |||||||||||||||||
176 | |||||||||||||||||
177 | |||||||||||||||||
178 | |||||||||||||||||
179 | |||||||||||||||||
180 | |||||||||||||||||
181 | |||||||||||||||||
182 | |||||||||||||||||
183 | |||||||||||||||||
184 | |||||||||||||||||
185 | |||||||||||||||||
186 | |||||||||||||||||
187 | |||||||||||||||||
188 | |||||||||||||||||
189 | |||||||||||||||||
190 | |||||||||||||||||
191 | |||||||||||||||||
192 | |||||||||||||||||
193 | |||||||||||||||||
194 | |||||||||||||||||
195 | |||||||||||||||||
196 | |||||||||||||||||
197 | |||||||||||||||||
198 | Composite of JunoCam images in cylindrical format, with identification of specific features. | John Rogers & Gerald Eichstaedt |
1 | Note: On this orbit the spacecraft orientation optimizes gravity mapping (GRAV) with the antenna pointed toward the Earth continuously. | |||||||
---|---|---|---|---|---|---|---|---|
2 | ||||||||
3 | Period: Orbit 24 [GRAV] (2019 Dec 26 - 2020 Feb 16) | Observations requested. | ||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | Observations planned / granted time | |
5 | Observations successful | |||||||
6 | Observations cancelled or unsuccessful | |||||||
7 | near IR | Orton | IRTF/SpeX | filtered imaging at several wavelengths between 1.58 and 5.1µm and spectral scanning in the 2- and 5-µm regions | Observations 3-5 days prior to the PJ25 perijove (Feb 17) | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired. Reduced "quick-look" observations (geometrically but not radiometrically calibrated) will be available for immeduately use from the Juno-curated web site: http://junoirtf.space.swri.edu/ | ||
8 | radio | Imai | Long Wavelength Array station 1 (LWA-1), LWA-Sevilleta (LWA-SV) | Jupiter's decametric auroral radio observations | February 13-16 | Low-resolution LWA1 data are freely accessible via Autoplot (http://autoplot.org) by accepting the data usage policy (http://space.physics.uiowa.edu/earth/datapolicy.html) More information can be found at http://space.physics.uiowa.edu/earth/ | ||
9 | Radio | Leven et al. | GAVRT | 2.3 GHz measurements using DSSN13, 34-m DSN radio telescope, Australian HS students | Jan 28 Feb 6. 15:51-18:05 | |||
10 | radio | Zarka, Cecconi, Lamy, Louis | Nançay Decameter Array (France) | coordinated measurement of 10-40 MHz cyclotron radio emission | every day, 8 hours around the transition to local meridian | https://maser.lesia.obspm.fr/task-1-data-collections/juno-ground-radio/juno-ground-radio-nancay-decameter.html?lang=en | ||
11 | Radio | Lamy for the NenuFar ES07 team | NenuFAR (France) | coordinated measurements of 10-40 MHz cyclotron radio emission at high time/frequency resolution | Dec. 26 08:05-15:47; Dec. 27 10:00-15:44; Feb. 16 05:30-13:12 | Data available on demand to laurent.lamy@obspm.fr | ||
12 | ||||||||
13 | ||||||||
14 | ||||||||
15 | ||||||||
16 | Scheduled observations by Juno. | |||||||
17 | ||||||||
18 | Perijove is 2019 Dec 26 17:35:57 UTC. System-III longitude = 73.3°W. Note this is virually coincident with solar conjunction and few Earth-based supporting observations are expected. | |||||||
19 | ||||||||
20 | Period: Orbit 24 (2019 Dec 26 - 2020 Feb 17) | |||||||
21 | Instrument | Description | ||||||
22 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||
23 | MWR | |||||||
24 | UVS | |||||||
25 | JunoCam | |||||||
26 | JIRAM | |||||||
27 | ||||||||
28 | ||||||||
29 | ||||||||
30 | ||||||||
31 | ||||||||
32 | ||||||||
33 | ||||||||
34 | ||||||||
35 | ||||||||
36 | ||||||||
37 | ||||||||
38 | ||||||||
39 | ||||||||
40 | ||||||||
41 | ||||||||
42 | ||||||||
43 | ||||||||
44 | ||||||||
45 | ||||||||
46 | ||||||||
47 | ||||||||
48 | ||||||||
49 | ||||||||
50 | ||||||||
51 | ||||||||
52 | ||||||||
53 | ||||||||
54 | ||||||||
55 | ||||||||
56 | ||||||||
57 | ||||||||
58 | ||||||||
59 | ||||||||
60 | ||||||||
61 | ||||||||
62 | ||||||||
63 | ||||||||
64 | ||||||||
65 | ||||||||
66 | ||||||||
67 | ||||||||
68 | ||||||||
69 | ||||||||
70 | ||||||||
71 | ||||||||
72 | ||||||||
73 | ||||||||
74 | ||||||||
75 | ||||||||
76 | ||||||||
77 | ||||||||
78 | ||||||||
79 | ||||||||
80 | ||||||||
81 | ||||||||
82 | ||||||||
83 | ||||||||
84 | ||||||||
85 | ||||||||
86 | ||||||||
87 | ||||||||
88 | ||||||||
89 | MWR footprints at the minimum emission angle of each latitude. | |||||||
90 | ||||||||
91 | ||||||||
92 | ||||||||
93 | ||||||||
94 | ||||||||
95 | ||||||||
96 | ||||||||
97 | ||||||||
98 | ||||||||
99 | ||||||||
100 | ||||||||
101 | ||||||||
102 | ||||||||
103 | ||||||||
104 | ||||||||
105 | ||||||||
106 | ||||||||
107 | ||||||||
108 | ||||||||
109 | ||||||||
110 | ||||||||
111 | ||||||||
112 | ||||||||
113 | ||||||||
114 | ||||||||
115 | ||||||||
116 | ||||||||
117 | ||||||||
118 | ||||||||
119 | ||||||||
120 | ||||||||
121 | ||||||||
122 | ||||||||
123 | ||||||||
124 | ||||||||
125 | JIRAM fields of view | |||||||
126 | The dates reported (both in UTC and in hours from PJ) on the top are referred to the last acquisition with the M filter of the whole plan for the given JM | |||||||
127 | The # field, is the estimated number of the acquisition of the whole plan, | |||||||
128 | (Ignore the percentage field.) | |||||||
129 | The light blue area, enclosed by dark blue lines, represented the FoVs of Imager M projected on Jupiter. Dark blue areas that you can see in some positions are created | |||||||
130 | by more projected FoV overlapping at close distance; i.e. these zones are created by multi FoV edges ( dark blue lines) that plot each close to the other create these graphic artefacts | |||||||
131 | The background cloud rendition is for general orientation; the position of the Great Red Spot does not indicate its actual position during these observations. | |||||||
132 | ||||||||
133 | ||||||||
134 | ||||||||
135 | ||||||||
136 | ||||||||
137 | ||||||||
138 | ||||||||
139 | ||||||||
140 | ||||||||
141 | ||||||||
142 | ||||||||
143 | ||||||||
144 | ||||||||
145 | ||||||||
146 | ||||||||
147 | ||||||||
148 | ||||||||
149 | ||||||||
150 | ||||||||
151 | ||||||||
152 | ||||||||
153 | ||||||||
154 | ||||||||
155 | ||||||||
156 | ||||||||
157 | ||||||||
158 | ||||||||
159 | ||||||||
160 | Composite of JIRAM M-band (5-micron) map. | |||||||
161 | ||||||||
162 | ||||||||
163 | ||||||||
164 | ||||||||
165 | ||||||||
166 | ||||||||
167 | ||||||||
168 | ||||||||
169 | ||||||||
170 | ||||||||
171 | ||||||||
172 | ||||||||
173 | ||||||||
174 | ||||||||
175 | ||||||||
176 | ||||||||
177 | ||||||||
178 | ||||||||
179 | ||||||||
180 | ||||||||
181 | ||||||||
182 | ||||||||
183 | ||||||||
184 | ||||||||
185 | ||||||||
186 | ||||||||
187 | ||||||||
188 | Composite JunoCam map with features labeled. Note that zero degrees longitude West in System III is at the center of this map. -John Rogers and Gerald Eichstaedt |
1 | Note: On this orbit the spacecraft orientation optimizes gravity mapping (GRAV) with the antenna pointed toward the Earth continuously. | |||||||
---|---|---|---|---|---|---|---|---|
2 | ||||||||
3 | Period: Orbit 23 [GRAV] (2019 Nov 3 - 2019 Dec 26) | Observations requested. | ||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | Observations planned / granted time | |
5 | Observations successful | |||||||
6 | Observations cancelled or unsuccessful | |||||||
7 | ||||||||
8 | near IR | Orton | IRTF/SpeX | filtered imaging at several wavelengths between 1.58 and 5.1µm and spectral scanning in the 2- and 5-µm regions | Nov 5, 12:15-18:35 HST; Nov 6, 13:45-18:35 HST. No observations were made on Nov 5 due to the SpeX guide-camera filter motor failure. On Nov 6, the iSHELL guide camera was used but heavy cloud cover prevailed all the time, so only flat-field data were obtained from sky and mirror-cover-closed observations. | |||
9 | mid IR | Orton | IRTF/MIRSI IRTF/SpeX | filtered radiometric imaging to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology. | Nov 3-4, 12:15-18:35 HST. MIRSI was unavailable. SpeX was used instead. Some results with not particularly good (but typical daytime) seeing, mostly at 5.1 microns. We were also just observing between holes in clouds. Toward the end of Nov 4, the guide-camera filter motor died and the filter moved manually to the J-filter setting. It will remain there until SpeX can be warmed up and the motor repaired or replaced. | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired. Reduced "quick-look" observations (geometrically but not radiometrically calibrated) will be available for immeduately use from the Juno-curated web site: http://junoirtf.space.swri.edu/ | ||
10 | Radio | Leven et al. | GAVRT | 2.3 GHz measurements using DSSN13, 34-m DSN radio telescope, Japanese HS students | 29 Oct Nov 1. 20:23-23:23 | |||
11 | radio | Zarka, Cecconi, Lamy, Louis | Nançay Decameter Array (France) | coordinated measurement of 10-40 MHz cyclotron radio emission | every day, 8 hours around the transition to local meridian | https://maser.lesia.obspm.fr/task-1-data-collections/juno-ground-radio/juno-ground-radio-nancay-decameter.html?lang=en | ||
12 | Radio | Lamy for the NenuFar ES07 team | NenuFAR (France) | coordinated measurements of 10-40 MHz cyclotron radio emission at high time/frequency resolution | Nov. 03 12:35-18:30; Nov. 04 12:15-18:40; Dec. 25 08:08-15:49; Dec. 26 08:05-15:47 | Data available on demand to laurent.lamy@obspm.fr | ||
13 | ||||||||
14 | Scheduled observations by Juno. | |||||||
15 | ||||||||
16 | Perijove is 2019 Nov 3 22:18:14 UTC. System-III longitude = 186.2°W | |||||||
17 | ||||||||
18 | Period: Orbit 23 (2019 Nov 3 - 2019 Dec 26) | |||||||
19 | Instrument | Description | ||||||
20 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||
21 | MWR | |||||||
22 | UVS | |||||||
23 | JunoCam | |||||||
24 | JIRAM | |||||||
25 | ||||||||
26 | ||||||||
27 | ||||||||
28 | ||||||||
29 | ||||||||
30 | ||||||||
31 | ||||||||
32 | ||||||||
33 | ||||||||
34 | ||||||||
35 | ||||||||
36 | ||||||||
37 | ||||||||
38 | ||||||||
39 | ||||||||
40 | ||||||||
41 | ||||||||
42 | ||||||||
43 | ||||||||
44 | ||||||||
45 | ||||||||
46 | ||||||||
47 | ||||||||
48 | ||||||||
49 | ||||||||
50 | ||||||||
51 | ||||||||
52 | ||||||||
53 | ||||||||
54 | ||||||||
55 | ||||||||
56 | ||||||||
57 | ||||||||
58 | ||||||||
59 | ||||||||
60 | ||||||||
61 | ||||||||
62 | ||||||||
63 | ||||||||
64 | ||||||||
65 | ||||||||
66 | ||||||||
67 | ||||||||
68 | ||||||||
69 | ||||||||
70 | ||||||||
71 | ||||||||
72 | ||||||||
73 | ||||||||
74 | ||||||||
75 | ||||||||
76 | ||||||||
77 | ||||||||
78 | ||||||||
79 | ||||||||
80 | ||||||||
81 | ||||||||
82 | ||||||||
83 | ||||||||
84 | ||||||||
85 | ||||||||
86 | ||||||||
87 | ||||||||
88 | ||||||||
89 | ||||||||
90 | ||||||||
91 | MWR footprints at the minimum emission angle of each latitude | |||||||
92 | ||||||||
93 | ||||||||
94 | ||||||||
95 | ||||||||
96 | ||||||||
97 | ||||||||
98 | ||||||||
99 | ||||||||
100 | ||||||||
101 | ||||||||
102 | ||||||||
103 | ||||||||
104 | ||||||||
105 | ||||||||
106 | ||||||||
107 | ||||||||
108 | ||||||||
109 | ||||||||
110 | ||||||||
111 | ||||||||
112 | ||||||||
113 | ||||||||
114 | ||||||||
115 | ||||||||
116 | ||||||||
117 | ||||||||
118 | ||||||||
119 | ||||||||
120 | ||||||||
121 | ||||||||
122 | ||||||||
123 | ||||||||
124 | ||||||||
125 | ||||||||
126 | ||||||||
127 | JIRAM fields of view | |||||||
128 | The dates reported (both in UTC and in hours from PJ) on the top are referred to the last acquisition with the M filter of the whole plan for the given JM | |||||||
129 | The # field, is the estimated number of the acquisition of the whole plan, | |||||||
130 | (Ignore the percentage field.) | |||||||
131 | The light blue area, enclosed by dark blue lines, represented the FoVs of Imager M projected on Jupiter. Dark blue areas that you can see in some positions are created | |||||||
132 | by more projected FoV overlapping at close distance; i.e. these zones are created by multi FoV edges ( dark blue lines) that plot each close to the other create these graphic artefacts | |||||||
133 | The background cloud rendition is for general orientation; the position of the Great Red Spot does not indicate its actual position during these observations. | |||||||
134 | ||||||||
135 | ||||||||
136 | ||||||||
137 | ||||||||
138 | ||||||||
139 | ||||||||
140 | ||||||||
141 | ||||||||
142 | ||||||||
143 | ||||||||
144 | ||||||||
145 | ||||||||
146 | ||||||||
147 | ||||||||
148 | ||||||||
149 | ||||||||
150 | ||||||||
151 | ||||||||
152 | ||||||||
153 | ||||||||
154 | ||||||||
155 | ||||||||
156 | ||||||||
157 | ||||||||
158 | ||||||||
159 | ||||||||
160 | ||||||||
161 | ||||||||
162 | ||||||||
163 | ||||||||
164 | Composite of JIRAM M-band (5-micron) map. |
1 | Note: On this orbit the spacecraft orientation optimizes gravity mapping (GRAV) with the antenna pointed toward the Earth continuously. | Observations requested. | |||||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
2 | Observations planned / granted time | ||||||||||||||||
3 | Period: Orbit 22 [GRAV] (2019 Sept 12 - 2019 Nov 3) | Observations successful | |||||||||||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | Observations cancelled or unsuccessful | ||||||||||
5 | X Ray | Gladstone/Dunn | Chandra | XMM | 11 hours (Joint Observation, Dunn XMM) | ||||||||||||
6 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | 20190920 20191009 20190921 20191010 20190927 20191011 20190928 20191013 20190929 20191014 20190930 20191018 20191001 20191019 20191002 20191020 20191003 20191021 20191005 20191022 20191006 20191023 20191007 20191024 20191008 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | Jan 15 to Jul 3, near continuous observations | Major Sodium outburst Jan -- Jun (Morgenthaler et al. 2019 ApJL) | ||||||
7 | CCD | Irwin | VLT/MUSE - IFU | spectroscopic imaging, 475-930 nm to determine cloud structure and albedo spectrum of particles. | 7th and 8th of October | Raw data publicly available to download from ESO portal this time next year. Standard calibration pipeline takes of the order of 1-3 days to complete. | |||||||||||
8 | near IR | Orton | IRTF/SpeX | filtered imaging at several wavelengths between 1.58 and 5.1µm | Sep 18-20 18:45-19:45 HST; Oct 28, 17:15-18:35 | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired. Reduced "quick-look" observations (geometrically but not radiometrically calibrated) will be available for immeduately use from the Juno-curated web site: http://junoirtf.space.swri.edu/ | |||||||||||
9 | near IR | Orton | IRTF/SpeX | filtered imaging at several wavelengths between 1.58 and 5.1µm and spectral scanning in the 2- and 5-µm regions | Oct 29, 15:345-18:35 HST. Near-infrared imaging was partially successful, often through thin cirrus or short holes between clouds. No time was available for scanning spectroscopy. | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired. Reduced "quick-look" observations (geometrically but not radiometrically calibrated) will be available for immeduately use from the Juno-curated web site: http://junoirtf.space.swri.edu/ | |||||||||||
10 | mid IR | Orton | IRTF/MIRSI | filtered radiometric imaging to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology. | Oct 30-31, 15:15-18:35 HST. MIRSI was not ready for observing. Near-infrared imaging with SpeX was done instead, often through thin cirrus or short holes between clouds | TBD | |||||||||||
11 | FUV | Grodent (HST GO-15638) | HST/STIS | Jupiter FUV aurora | North Aurora: 2019.246 (09/04/2019) 12:38 2019.247 (09/05/2019) 07:41 2019.249 (09/07/2019) 10:30 2019.250 (09/08/2019) 15:07 XMM 2019.251 (09/08/2019) 16:43 XMM 2019.252 (09/(09/2019) 11:46 XMM 2019.253 (09/10/2019) 08:26 2019.255 (09/12/2019) 09:41 PJ+6h (03:41) 2019.256 (09/13/2019) 04:43 XMM 2019.256 (09/13/2019) 14:16 XMM South Aurora: 2019.253 (09/10/2019) 05:15 Chandra (23:00-06:00) | No proprietary period. Check out preview movies at https://www.lpap.uliege.be/cms/c_3478756/en/lpap-hst-campaign | |||||||||||
12 | radio | Zarka, Cecconi, Lamy, Louis | Nançay Decameter Array (France) | coordinated measurement of 10-40 MHz cyclotron radio emission | every day, 8 hours around the transition to local meridian | https://maser.lesia.obspm.fr/task-1-data-collections/juno-ground-radio/juno-ground-radio-nancay-decameter.html?lang=en | |||||||||||
13 | Radio | Lamy for the NenuFar ES07 team | NenuFAR (France) | coordinated measurements of 10-40 MHz cyclotron radio emission at high time/frequency resolution | Nov. 03 12:35-18:30 | Data available on demand to laurent.lamy@obspm.fr | |||||||||||
14 | visible/NUV/ near-IR | Wong (14661) | Hubble/ WFC3-UVIS | hi-resolution non-global snapshot marked "failed" because wrong (non-Juno) longitude was observed | 2019 Sept 12 | https://archive.stsci.edu/prepds/wfcj/ https://doi.org/10.3847/1538-4365/ab775f https://doi.org/10.1016/j.icarus.2022.114994 | |||||||||||
15 | |||||||||||||||||
16 | Scheduled observations by Juno. | ||||||||||||||||
17 | |||||||||||||||||
18 | Perijove is 2019 Sept 12 03:40:47 UTC. System-III longitude = 323.3°W | ||||||||||||||||
19 | |||||||||||||||||
20 | Period: Orbit 22 (2019 Sept 12 - 2019 Nov 3) | ||||||||||||||||
21 | Instrument | Description | |||||||||||||||
22 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | |||||||||||||||
23 | MWR | ||||||||||||||||
24 | UVS | ||||||||||||||||
25 | JunoCam | ||||||||||||||||
26 | JIRAM | ||||||||||||||||
27 | |||||||||||||||||
28 | |||||||||||||||||
29 | |||||||||||||||||
30 | |||||||||||||||||
31 | |||||||||||||||||
32 | |||||||||||||||||
33 | |||||||||||||||||
34 | |||||||||||||||||
35 | |||||||||||||||||
36 | |||||||||||||||||
37 | |||||||||||||||||
38 | |||||||||||||||||
39 | |||||||||||||||||
40 | |||||||||||||||||
41 | |||||||||||||||||
42 | |||||||||||||||||
43 | |||||||||||||||||
44 | |||||||||||||||||
45 | |||||||||||||||||
46 | |||||||||||||||||
47 | |||||||||||||||||
48 | |||||||||||||||||
49 | |||||||||||||||||
50 | |||||||||||||||||
51 | |||||||||||||||||
52 | |||||||||||||||||
53 | |||||||||||||||||
54 | |||||||||||||||||
55 | |||||||||||||||||
56 | |||||||||||||||||
57 | |||||||||||||||||
58 | |||||||||||||||||
59 | |||||||||||||||||
60 | |||||||||||||||||
61 | |||||||||||||||||
62 | |||||||||||||||||
63 | |||||||||||||||||
64 | |||||||||||||||||
65 | |||||||||||||||||
66 | |||||||||||||||||
67 | |||||||||||||||||
68 | |||||||||||||||||
69 | |||||||||||||||||
70 | |||||||||||||||||
71 | |||||||||||||||||
72 | |||||||||||||||||
73 | |||||||||||||||||
74 | |||||||||||||||||
75 | |||||||||||||||||
76 | |||||||||||||||||
77 | |||||||||||||||||
78 | |||||||||||||||||
79 | |||||||||||||||||
80 | |||||||||||||||||
81 | |||||||||||||||||
82 | |||||||||||||||||
83 | |||||||||||||||||
84 | |||||||||||||||||
85 | |||||||||||||||||
86 | |||||||||||||||||
87 | |||||||||||||||||
88 | |||||||||||||||||
89 | |||||||||||||||||
90 | |||||||||||||||||
91 | MWR footprints for the minimum emisison angle at each spin of the spacecraft. The perijove position is given by the cross. | ||||||||||||||||
92 | |||||||||||||||||
93 | |||||||||||||||||
94 | |||||||||||||||||
95 | |||||||||||||||||
96 | |||||||||||||||||
97 | |||||||||||||||||
98 | |||||||||||||||||
99 | |||||||||||||||||
100 | |||||||||||||||||
101 | |||||||||||||||||
102 | |||||||||||||||||
103 | |||||||||||||||||
104 | |||||||||||||||||
105 | |||||||||||||||||
106 | |||||||||||||||||
107 | |||||||||||||||||
108 | |||||||||||||||||
109 | |||||||||||||||||
110 | |||||||||||||||||
111 | |||||||||||||||||
112 | |||||||||||||||||
113 | |||||||||||||||||
114 | |||||||||||||||||
115 | |||||||||||||||||
116 | |||||||||||||||||
117 | |||||||||||||||||
118 | |||||||||||||||||
119 | |||||||||||||||||
120 | |||||||||||||||||
121 | |||||||||||||||||
122 | |||||||||||||||||
123 | |||||||||||||||||
124 | |||||||||||||||||
125 | |||||||||||||||||
126 | |||||||||||||||||
127 | JIRAM fields of view | ||||||||||||||||
128 | The dates reported (both in UTC and in hours from PJ) on the top are referred to the last acquisition with the M filter of the whole plan for the given JM | ||||||||||||||||
129 | The # field, is the estimated number of the acquisition of the whole plan, | ||||||||||||||||
130 | (Ignore the percentage field.) | ||||||||||||||||
131 | The light blue area, enclosed by dark blue lines, represented the FoVs of Imager M projected on Jupiter. Dark blue areas that you can see in some positions are created | ||||||||||||||||
132 | by more projected FoV overlapping at close distance; i.e. these zones are created by multi FoV edges ( dark blue lines) that plot each close to the other create these graphic artefacts | ||||||||||||||||
133 | The background cloud rendition is for general orientation; the position of the Great Red Spot does not indicate its actual position during these observations. | ||||||||||||||||
134 | |||||||||||||||||
135 | |||||||||||||||||
136 | |||||||||||||||||
137 | |||||||||||||||||
138 | |||||||||||||||||
139 | |||||||||||||||||
140 | |||||||||||||||||
141 | |||||||||||||||||
142 | |||||||||||||||||
143 | |||||||||||||||||
144 | |||||||||||||||||
145 | |||||||||||||||||
146 | |||||||||||||||||
147 | |||||||||||||||||
148 | |||||||||||||||||
149 | |||||||||||||||||
150 | |||||||||||||||||
151 | |||||||||||||||||
152 | |||||||||||||||||
153 | |||||||||||||||||
154 | |||||||||||||||||
155 | |||||||||||||||||
156 | |||||||||||||||||
157 | |||||||||||||||||
158 | |||||||||||||||||
159 | |||||||||||||||||
160 | |||||||||||||||||
161 | |||||||||||||||||
162 | Composite of JIRAM M-band (5-micron) map. | ||||||||||||||||
163 |
1 | Note: On this orbit the spacecraft orientation optimizes gravity mapping (GRAV) with the antenna pointed toward the Earth continuously. | ||||||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
2 | Observations requested. | ||||||||||||||||
3 | Period: Orbit 21 [GRAV] (2019 July 21 - 2019 Sept 12) | Observations planned / granted time | |||||||||||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | Observations successful | ||||||||||
5 | X Ray | Gladstone/Dunn | Chandra | Time tagged and high spatial resolution | Sept 9 23:00 - 06:00 | Observations cancelled or unsuccessful | |||||||||||
6 | X-ray | W. Dunn | XMM-Newton | ~120 hours of time-tagged spectra during Juno approach and PJ | 8 Sept @ 08:25 - 10 Sept @ 02:21; 10 Sept @ 08:17 - 12 Sept @ 02:09; 12 Sept @ 08:08 - 14 Sept @ 03:16 | Propietary for 1 year then in the XMM public archive. However, I'm always very happy to share and collaborate, so just let me know if you'd like access to it - Will (w.dunn@ucl.ac.uk) | |||||||||||
7 | FUV | Grodent (HST GO-15638) | HST/STIS | Jupiter FUV aurora | North Aurora: 07/14/2019 19:35 07/15/2019 14:44 07/15/2019 16:15 07/16/2019 11:19 07/19/2019 18:46 07/18/2019 14:08 07/19/2019 09:13 07/20/2019 13:50 07/21/2019 10:29 | No proprietary period. Check out preview movies at https://www.lpap.uliege.be/cms/c_3478756/en/lpap-hst-campaign | |||||||||||
8 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | 20190721 20190818 20190722 20190819 20190812 20190820 20190813 20190821 20190814 20190822 20190816 20190827 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | Jan 15 to Jul 3, near continuous observations | Major Sodium outburst Jan -- Jun (Morgenthaler et al. 2019 ApJL) | ||||||
9 | Visible and Near IR (0.4-1.7 microns) | Sánchez-Lavega | Calar Alto / PlanetCam | Lucky-imaging high-resolution observations with stars for calibration. PJ20 longitudes on one night and images of the GRS from one limb to the other on 2 nights. | July 17-21 | partially successfull due to weather conditions. Reduction of the data is complex and generally requires one to two weeks after the observations. | |||||||||||
10 | CCD | Braude/Irwin | VLT/MUSE - IFU | spectroscopic imaging, 475-930 nm to determine cloud structure and albedo spectrum of particles. | 29 August | Raw data publicly available to download from ESO portal this time next year. Standard calibration pipeline takes of the order of 1-3 days to complete. Observation meant to coincide with PJ22 but taken 2 weeks early | |||||||||||
11 | visible/NUV/ near-IR | Wong (14661) | Hubble/ WFC3-UVIS | hi-resolution non-global snapshot | 2019 July 21 | https://archive.stsci.edu/prepds/wfcj/ https://doi.org/10.3847/1538-4365/ab775f | |||||||||||
12 | near IR | Chowdhury | IRTF/iSHELL | high-resolution spectroscopy of H3+ | Jul 21, 4:42-11:00 UTC | Observations cancelled as a result of anti-TMT protesters, who blocked all access to telescopes at Maunakea. | |||||||||||
13 | near IR | Rathburn | IRTF/SpeX | imaging of Io’s Jupiter-facing hemisphere while in eclipse to determine the brightnesses of volcanoes | Jul 27, 6:20-7:50 UTC | Observations cancelled as a result of anti-TMT protesters, who blocked all access to telescopes at Maunakea. | |||||||||||
14 | near IR | Rathburn | IRTF/SpeX | imaging of Io to determine if any major eruptions are occurring | Jul 31, 4:55-5:25 UTC | Observations cancelled as a result of anti-TMT protesters, who blocked all accesss to telescopes at Maunakea. | |||||||||||
15 | near IR | Orton | IRTF/SpeX | filtered imaging at several wavelengths between 1.58 and 5.1µm | Aug 1, 18:55-19:55 HST; Aug 2, 19:35-20:35 - telescope unavailable due to anti-TMT protesters, who blocked all access totelescopes at Maunakea; Aug 27-28 18:10-19:10 HST | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired. Reduced "quick-look" observations (geometrically but not radiometrically calibrated) will be available for immeduately use from the Juno-curated web site: http://junoirtf.space.swri.edu/ | |||||||||||
16 | near IR | Orton | IRTF/MIRSI IRTF/SpeX | filtered imaging at several wavelengths between 7 and 25 µm (First scientific application of refurbished instrument.) | Sep 9-10, 14:45-20:30 HST; MIRSI was not available, so images were taken using SpeX through partly cloudy skies | raw images available from IRTF web site; fully reduced images available within a month or sooner, as desired. MIRSI not available; SpeX observations will be made instead. | |||||||||||
17 | radio | Zarka, Cecconi, Lamy, Louis | Nançay Decameter Array (France) | coordinated measurement of 10-40 MHz cyclotron radio emission | every day, 8 hours around the transition to local meridian | https://maser.lesia.obspm.fr/task-1-data-collections/juno-ground-radio/juno-ground-radio-nancay-decameter.html?lang=en | |||||||||||
18 | Radio | Lamy for the NenuFar ES07 team | NenuFAR (France) | coordinated measurements of 10-40 MHz cyclotron radio emission at high time/frequency resolution | Sep. 11 14:36-20:20; Sep. 12 14:33-20:17 | Data available on demand to laurent.lamy@obspm.fr | |||||||||||
19 | |||||||||||||||||
20 | Scheduled observations by Juno. | ||||||||||||||||
21 | |||||||||||||||||
22 | Perijove is 2019 July 21 04:02:44 UTC. System-III longitude = 278.6°W | ||||||||||||||||
23 | |||||||||||||||||
24 | Period: Orbit 21 (2019 July 21 - 2019 Sept 12) | ||||||||||||||||
25 | Instrument | Description | |||||||||||||||
26 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | |||||||||||||||
27 | MWR | ||||||||||||||||
28 | UVS | ||||||||||||||||
29 | JunoCam | ||||||||||||||||
30 | JIRAM | ||||||||||||||||
31 | |||||||||||||||||
32 | |||||||||||||||||
33 | |||||||||||||||||
34 | |||||||||||||||||
35 | |||||||||||||||||
36 | |||||||||||||||||
37 | |||||||||||||||||
38 | |||||||||||||||||
39 | |||||||||||||||||
40 | |||||||||||||||||
41 | |||||||||||||||||
42 | |||||||||||||||||
43 | |||||||||||||||||
44 | |||||||||||||||||
45 | |||||||||||||||||
46 | |||||||||||||||||
47 | |||||||||||||||||
48 | |||||||||||||||||
49 | |||||||||||||||||
50 | |||||||||||||||||
51 | |||||||||||||||||
52 | |||||||||||||||||
53 | |||||||||||||||||
54 | |||||||||||||||||
55 | |||||||||||||||||
56 | |||||||||||||||||
57 | |||||||||||||||||
58 | |||||||||||||||||
59 | |||||||||||||||||
60 | |||||||||||||||||
61 | |||||||||||||||||
62 | |||||||||||||||||
63 | |||||||||||||||||
64 | |||||||||||||||||
65 | |||||||||||||||||
66 | |||||||||||||||||
67 | |||||||||||||||||
68 | |||||||||||||||||
69 | |||||||||||||||||
70 | |||||||||||||||||
71 | |||||||||||||||||
72 | |||||||||||||||||
73 | |||||||||||||||||
74 | |||||||||||||||||
75 | |||||||||||||||||
76 | |||||||||||||||||
77 | |||||||||||||||||
78 | |||||||||||||||||
79 | |||||||||||||||||
80 | |||||||||||||||||
81 | |||||||||||||||||
82 | |||||||||||||||||
83 | |||||||||||||||||
84 | |||||||||||||||||
85 | |||||||||||||||||
86 | |||||||||||||||||
87 | |||||||||||||||||
88 | |||||||||||||||||
89 | |||||||||||||||||
90 | |||||||||||||||||
91 | |||||||||||||||||
92 | |||||||||||||||||
93 | |||||||||||||||||
94 | |||||||||||||||||
95 | |||||||||||||||||
96 | |||||||||||||||||
97 | |||||||||||||||||
98 | MWR footprints for the minimum emission angle at each latitude. | ||||||||||||||||
99 | |||||||||||||||||
100 | |||||||||||||||||
101 | |||||||||||||||||
102 | |||||||||||||||||
103 | |||||||||||||||||
104 | |||||||||||||||||
105 | |||||||||||||||||
106 | |||||||||||||||||
107 | |||||||||||||||||
108 | |||||||||||||||||
109 | |||||||||||||||||
110 | |||||||||||||||||
111 | |||||||||||||||||
112 | |||||||||||||||||
113 | |||||||||||||||||
114 | |||||||||||||||||
115 | |||||||||||||||||
116 | |||||||||||||||||
117 | |||||||||||||||||
118 | |||||||||||||||||
119 | |||||||||||||||||
120 | |||||||||||||||||
121 | |||||||||||||||||
122 | |||||||||||||||||
123 | |||||||||||||||||
124 | |||||||||||||||||
125 | |||||||||||||||||
126 | |||||||||||||||||
127 | |||||||||||||||||
128 | |||||||||||||||||
129 | JIRAM fields of view | ||||||||||||||||
130 | The dates reported (both in UTC and in hours from PJ) on the top are referred to the last acquisition with the M filter of the whole plan for the given JM | ||||||||||||||||
131 | The # field, is the estimated number of the acquisition of the whole plan, | ||||||||||||||||
132 | (Ignore the percentage field.) | ||||||||||||||||
133 | The light blue area, enclosed by dark blue lines, represented the FoVs of Imager M projected on Jupiter. Dark blue areas that you can see in some positions are created | ||||||||||||||||
134 | by more projected FoV overlapping at close distance; i.e. these zones are created by multi FoV edges ( dark blue lines) that plot each close to the other create these graphic artefacts | ||||||||||||||||
135 | The background cloud rendition is for general orientation; the position of the Great Red Spot does not indicate its actual position during these observations. | ||||||||||||||||
136 | |||||||||||||||||
137 | |||||||||||||||||
138 | |||||||||||||||||
139 | |||||||||||||||||
140 | |||||||||||||||||
141 | |||||||||||||||||
142 | |||||||||||||||||
143 | |||||||||||||||||
144 | |||||||||||||||||
145 | |||||||||||||||||
146 | |||||||||||||||||
147 | |||||||||||||||||
148 | |||||||||||||||||
149 | |||||||||||||||||
150 | |||||||||||||||||
151 | |||||||||||||||||
152 | |||||||||||||||||
153 | |||||||||||||||||
154 | |||||||||||||||||
155 | |||||||||||||||||
156 | |||||||||||||||||
157 | |||||||||||||||||
158 | |||||||||||||||||
159 | |||||||||||||||||
160 | |||||||||||||||||
161 | |||||||||||||||||
162 | |||||||||||||||||
163 | |||||||||||||||||
164 | |||||||||||||||||
165 | |||||||||||||||||
166 | Composite of JIRAM M-band (5-micron) map. |
1 | Note: On this orbit the spacecraft orientation is planned to be off Earth-axis in order to improve remote-sensing observations. | |||||||
---|---|---|---|---|---|---|---|---|
2 | Observations requested. | |||||||
3 | Period: Orbit 20 [GRAV] (2019 May 29 – 2019 July 21) | Observations planned / granted time | ||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | Observations successful | |
5 | X ray | Gladstone | Chandra | DDT | 2019 May 29 03:28 – 14:03 in ObsID 22159 | Observations cancelled or unsuccessful | ||
6 | X-ray | W. Dunn | Chandra High Resolution Camera | 5 x 7hour time-tagged spatially resolved observations while Juno is approaching Jupiter for PJ 21 | July 13 01:30 - 09:00 July 13 21:00 - July 14 - 04:00 July 15 13:00 - 20:00 July 16 09:00 - 16:00 July 18 20:00 - July 19th 04:00 | Propietary for 1 year then in the Chandra public archive. However, I'm always very happy to share and collaborate, so just let me know if you'd like access to it - Will (w.dunn@ucl.ac.uk) | ||
7 | FUV | Grodent (HST GO-15638) | HST/STIS | Jupiter FUV aurora | Visit 23 19.142 (May 22) 21:58 Visit 25 19.143 (May 23) 17:03 Visit 22 19.145 (May 25) 13:32 Visit 27 19.146 (May 26) 14:57 Visit 24 19.146 (May 26) 21:18 Visit 26 19.147 (May 27) 17:58 Visit 28 19.148 (May 28) 20:59 Visit 29 19.149 (May 29) 12:52 Visit 30 19.150 (May 30) 17:28 | No proprietary period. Check out preview movies at https://www.lpap.uliege.be/cms/c_3478756/en/lpap-hst-campaign | ||
8 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | 20190529, 20190530, 20190531, 20190601, 20190602, 20190603, 20190606, 20190607, 20190609, 20190611, 20190612, 20190613, 20190614, 20190615, 20190616, 20190617, 20190618, 20190619, 20190620, 20190621, 20190622, 20190623, 20190624, 20190625, 20190626, 20190627, 20190628, 20190702, 20190703, 20190704, 20190705, 20190709, 20190710, 20190716, 20190717, 20190720, 20190721 | |||
9 | visible | Dahl | APO/NAIC | Hyperspectral image cubes, 470-950 nm | Nights of May 27, 28 | TBD | ||
10 | visible | Machado | VLT/ESPRESSO | Seismology and Doppler Velocimetry by studying reflected light on Jupiter's cloud tops | June 4th. | TBD | ||
11 | visible | Machado | Calar Alto/CARMENES | Doppler velocimetry | May-29 | TBD | ||
12 | Visible and Near IR (0.4-1.7 microns) | Sánchez-Lavega | Calar Alto / PlanetCam | Lucky-imaging high-resolution observations with stars for calibration. PJ20 longitudes on one night and images of the GRS from one limb to the other on 2 nights. | May 27-30 | partially successfull due to weather conditions. Reduction of the data is complex and generally requires one to two weeks after the observations. | ||
13 | CCD | Braude/Irwin | VLT/MUSE - IFU | spectroscopic imaging, 475-930 nm to determine cloud structure and albedo spectrum of particles. | 8 June, 9 July | Raw data publicly available to download from ESO portal this time next year. Standard calibration pipeline takes of the order of 1-3 days to complete. 9 July observation to coincide with PJ21 obtained 2 weeks prematurely | ||
14 | near IR | Giles | Gemini-N/NIRI | adaptive-optics-stabilized imaging of reflected sunlight | June 11, June 20 and July 6 | reduced and avalable on request | ||
15 | near IR (5 µm) | Wong | Gemini-N/NIRI | lucky imaging, 5-µm maps | 2019 May 29 | https://archive.stsci.edu/prepds/wfcj/ https://doi.org/10.3847/1538-4365/ab775f | ||
16 | mid IR | Livengood | IRTF / iSHELL | High-res spectroscopy of H3+ at 4 microns and images at 3.4 and 4 microns | June 5,7 UT clear; June 6 clouded out | |||
17 | mid IR | Orton (Keck exchange time and direct Subaru time), Kasaba | Subaru / COMICS | filtered radiometric imaging and spectroscopy to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology and auroral heating and chemistry. | Mid-infrared imaging of Jupiter was performed for the second half of May 25 and May 26. (May 26 & 27, UT). PJ20 longitudes were covered on May 25/26 althogh at moderately high emission angles. Very good images were obtained of Oval BA and the Great Red Spot on May 26/27. | Collaboration is possible with the investigators. | ||
18 | near IR | Bjoraker | IRTF/iSHELL | high-resolution 5-micron spectroscopy of Jupiter | May 28, 9:00-16:05 UTC May 31, 8:00-13:30 UTC | |||
19 | near IR | Chowdhury | IRTF/iSHELL | high-resolution spectroscopy of H3+ | May 29, 8:35-16:05 UTC | |||
20 | near IR | Bjoraker | IRTF/iSHELL | imaging at 1.58, 2.1, & 5 microns | June 10-11 10:56-11:35 UTC | |||
21 | near IR | Rathbun | IRTF/SpeX | imaging of Io’s Jupiter-facing hemisphere while in eclipse to determine the brightnesses of volcanoes | Jun 18, 8:40-10:10 UTC Jun 25, 10:10-11:50 UTC Jul 4, 6:30-8:00 UTC Jul 11, 8:15-6:00 UTC Jul 20, 4:30-6:00 UTC | |||
22 | near IR | Rathbun | IRTF/SpeX | imaging of Io to determine if any major eruptions are occurring | Jun 9, 11:10-11:40 UTC Jun 28, 9:40-10:10 UTC Jul 1, 0:00-0:30 UTC Jul 8, 6:30-7:00 UTC Jul 14, 8:55-9:25 UTC | |||
23 | radio | Zarka, Cecconi, Lamy, Louis | Nançay Decameter Array (France) | coordinated measurement of 10-40 MHz cyclotron radio emission | every day, 8 hours around the transition to local meridian | https://maser.lesia.obspm.fr/task-1-data-collections/juno-ground-radio/juno-ground-radio-nancay-decameter.html?lang=en | ||
24 | Radio | Lamy for the NenuFar ES07 team | NenuFAR (France) | coordinated measurements of 10-40 MHz cyclotron radio emission at high time/frequency resolution | Jul. 11 21:31-21:36 | Data available on demand to laurent.lamy@obspm.fr | ||
25 | Scheduled observations by Juno. | |||||||
26 | ||||||||
27 | Perijove is May 29 2019 08:08:14 UTC. System-III longitude = 9.1°W | |||||||
28 | ||||||||
29 | Period: Orbit 20 (2019 May 29 – 2019 July 21) | |||||||
30 | Instrument | Description | ||||||
31 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||
32 | MWR | |||||||
33 | UVS | |||||||
34 | JunoCam | |||||||
35 | JIRAM | |||||||
36 | ||||||||
37 | ||||||||
38 | ||||||||
39 | ||||||||
40 | ||||||||
41 | ||||||||
42 | ||||||||
43 | ||||||||
44 | ||||||||
45 | ||||||||
46 | ||||||||
47 | ||||||||
48 | ||||||||
49 | ||||||||
50 | ||||||||
51 | ||||||||
52 | ||||||||
53 | ||||||||
54 | ||||||||
55 | ||||||||
56 | ||||||||
57 | ||||||||
58 | ||||||||
59 | ||||||||
60 | ||||||||
61 | ||||||||
62 | ||||||||
63 | ||||||||
64 | ||||||||
65 | ||||||||
66 | ||||||||
67 | ||||||||
68 | ||||||||
69 | ||||||||
70 | ||||||||
71 | ||||||||
72 | ||||||||
73 | ||||||||
74 | ||||||||
75 | ||||||||
76 | ||||||||
77 | ||||||||
78 | ||||||||
79 | ||||||||
80 | ||||||||
81 | ||||||||
82 | ||||||||
83 | ||||||||
84 | ||||||||
85 | ||||||||
86 | ||||||||
87 | ||||||||
88 | ||||||||
89 | ||||||||
90 | ||||||||
91 | ||||||||
92 | ||||||||
93 | ||||||||
94 | ||||||||
95 | ||||||||
96 | ||||||||
97 | ||||||||
98 | ||||||||
99 | MWR footprints for the minimum emission angle at each rotation of the spacecraft. The perijove position is shown by the cross. | |||||||
100 | ||||||||
101 | ||||||||
102 | ||||||||
103 | ||||||||
104 | ||||||||
105 | ||||||||
106 | ||||||||
107 | ||||||||
108 | ||||||||
109 | ||||||||
110 | ||||||||
111 | ||||||||
112 | ||||||||
113 | ||||||||
114 | ||||||||
115 | ||||||||
116 | ||||||||
117 | ||||||||
118 | ||||||||
119 | ||||||||
120 | ||||||||
121 | ||||||||
122 | ||||||||
123 | ||||||||
124 | ||||||||
125 | ||||||||
126 | ||||||||
127 | ||||||||
128 | ||||||||
129 | ||||||||
130 | ||||||||
131 | ||||||||
132 | ||||||||
133 | ||||||||
134 | JIRAM fields of view | |||||||
135 | The dates reported (both in UTC and in hours from PJ) on the top are referred to the last acquisition with the M filter of the whole plan for the given JM | |||||||
136 | The # field, is the estimated number of the acquisition of the whole plan, | |||||||
137 | (Ignore the percentage field.) | |||||||
138 | The light blue area, enclosed by dark blue lines, represented the FoVs of Imager M projected on Jupiter. Dark blue areas that you can see in some positions are created | |||||||
139 | by more projected FoV overlapping at close distance; i.e. these zones are created by multi FoV edges ( dark blue lines) that plot each close to the other create these graphic artefacts | |||||||
140 | The background cloud rendition is for general orientation; the position of the Great Red Spot does not indicate its actual position during these observations. | |||||||
141 | ||||||||
142 | ||||||||
143 | ||||||||
144 | ||||||||
145 | ||||||||
146 | ||||||||
147 | ||||||||
148 | ||||||||
149 | ||||||||
150 | ||||||||
151 | ||||||||
152 | ||||||||
153 | ||||||||
154 | ||||||||
155 | ||||||||
156 | ||||||||
157 | ||||||||
158 | ||||||||
159 | ||||||||
160 | ||||||||
161 | ||||||||
162 | ||||||||
163 | ||||||||
164 | ||||||||
165 | ||||||||
166 | ||||||||
167 | ||||||||
168 | ||||||||
169 | Composite of JIRAM M-band (5-micron) map. | |||||||
170 | ||||||||
171 | ||||||||
172 | ||||||||
173 | ||||||||
174 | ||||||||
175 | ||||||||
176 | ||||||||
177 | ||||||||
178 | ||||||||
179 | ||||||||
180 | ||||||||
181 | ||||||||
182 | ||||||||
183 | ||||||||
184 | ||||||||
185 | ||||||||
186 | ||||||||
187 | ||||||||
188 | ||||||||
189 | ||||||||
190 | ||||||||
191 | ||||||||
192 | ||||||||
193 | ||||||||
194 | ||||||||
195 | ||||||||
196 | ||||||||
197 | ||||||||
198 | ||||||||
199 | ||||||||
200 | ||||||||
201 | ||||||||
202 | ||||||||
203 | ||||||||
204 | ||||||||
205 | ||||||||
206 | ||||||||
207 | ||||||||
208 | ||||||||
209 | ||||||||
210 | ||||||||
211 | ||||||||
212 | ||||||||
213 | ||||||||
214 | ||||||||
215 | ||||||||
216 | ||||||||
217 | ||||||||
218 | ||||||||
219 |
1 | Note: On this orbit the spacecraft orientation will be made in order to enable the MWR experiment to create a cross-track map and get the first center-to-limb observations in the zonal direction. | ||||||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
2 | Observations requested. | ||||||||||||||||
3 | Period: Orbit 19 [MWR X-track] (2019 April 6 – 2019 May 28) | Observations planned / granted time | |||||||||||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | Observations successful | ||||||||||
5 | FUV | Grodent (HST GO-15638) | HST/COS/G130M | Io eclipse spectroscopy (Visit 52) | 2019-04-29 16:21 18:26 2019-04-29 16:04 16:12 (failed, HOPR requested) 2019-04-30 03:19 03:58 | No proprietary period | Observations cancelled or unsuccessful | ||||||||||
6 | FUV | Grodent (HST GO-15638) | HST/STIS | Jupiter FUV aurora | Visit 11 19.087 (Mar 28) 21:30-22:15 Visit 12 19.088 (Mar 29) 18:09-18:55 Visit 13 19.089 (Mar 30) 22:45-23:30 Visit 14 19.090 (Mar 31) 19:25-20:10 Visit 15 19.091 (Apr 1) 16:04-16:50 Visit 16 19.092 (Apr 2) 01:36-02;21 Visit 17 19.093 (Apr 3) 17:19-18:05 Visit 18 19.095 (Apr 5) 18:34-19:20 Visit 19 19.096 (Apr 6) 13:38-14:24 Visit 20 19.096 (Apr 6) 23:11-23:56 | No proprietary period. Check out preview movies at https://www.lpap.uliege.be/cms/c_3478756/en/lpap-hst-campaign | |||||||||||
7 | Visible and Near IR | Sánchez-Lavega | Calar Alto / PlanetCam | 27,28,29,30 May | |||||||||||||
8 | visible/NUV/ near-IR | Wong, de Pater (14661, 15159, 15665) | Hubble/ WFC3-UVIS | hi-resolution global maps | 2019 Apr 6–9 | https://archive.stsci.edu/prepds/wfcj/ https://doi.org/10.3847/1538-4365/ab775f https://doi.org/10.1126/science.abf1015 https://doi.org/10.1016/j.icarus.2022.114994 | |||||||||||
9 | visible | Veillet | LBT / PEPSI | Io eclipse spectroscopy | April 24 | TBD | |||||||||||
10 | visible | Dahl | APO/NAIC | Hyperspectral image cubes, 470-950 nm | April 4-5 | TBD | |||||||||||
11 | CCD | Braude/Irwin | VLT/MUSE - IFU | spectroscopic imaging, 475-930 nm to determine cloud structure and albedo spectrum of particles. | April 13 and 29, May 18 | Raw data publicly available to download from ESO portal this time next year. Standard calibration pipeline takes of the order of 1-3 days to complete. Although our proposed observation to coincide with PJ19 was rejected, we obtained an observation of the GRS on the 13th of April (which may have had some light contamination around 860nm) and an observation of BA on the 29th. We also obtained an observation of the PJ20 longitude obtained 11 days prematurely. | |||||||||||
12 | CCD | Braude/Irwin | VLT/MUSE - IFU | spectroscopic imaging, 460-930 nm to determine cloud structure and albedo spectrum of particles. | May 18 | Trial observation using MUSE's new AO-E mode, observing down to 460nm (instead of 480nm as with previous observations) and making use of adaptive optics, with GRS observed close to terminator. Unfortunately, observing conditions and standard are poor, and second-order contamination is present above approximately 0.88 microns | |||||||||||
13 | near IR | Giles | Gemini-N/NIRI | adaptive-optics-stabilized imaging of reflected sunlight | No AO opportunities involving Galilean satellites during this period | ||||||||||||
14 | near IR (5 µm) | Wong | Gemini-N/NIRI | lucky imaging, 5-µm maps | 2019 Apr 6–8 | https://archive.stsci.edu/prepds/wfcj/ https://doi.org/10.3847/1538-4365/ab775f https://doi.org/10.1126/science.abf1015 | |||||||||||
15 | near IR | de Pater | Keck/NIRSPEC | high-resolution spectroscopy of Jupiter in the 5-µm window. NIRSPEC upgrade worked well. SCAM now yields M-prime images. | April 5 and 6, 10:24-15:23 UTC | TBD | |||||||||||
16 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | 20190406, 20190407, 20190408, 20190409, 20190410, 20190411, 20190413, 20190414, 20190415, 20190416, 20190418, 20190419, 20190420, 20190421, 20190422, 20190423, 20190424, 20190425, 20190426, 20190427, 20190428, 20190429, 20190430, 20190501, 20190502, 20190504, 20190505, 20190506, 20190508, 20190509, 20190514, 20190515, 20190516, 20190517, 20190518, 20190521, 20190522, 20190524, 20190525, 20190526, 20190527, 20190528 | Major Sodium outburst Jan -- Jun (Morgenthaler et al. 2019 ApJL) | |||||||||||
17 | near IR | de Pater | Keck NIRSPEC+NIRC2 | observations of Io successfully acquired | April 6-7, ~15 UTC; April 14 11-15 UT | ||||||||||||
18 | near IR | Bjoraker | IRTF/iSHELL | high-res 5-micron spectroscopy of Jupiter. Good data both nights. | Apr 3, 12:10-16:10 UTC Apr 8, 12:10-16:10 UTC | ||||||||||||
19 | near IR | Chowdhury | IRTF/iSHELL | high-resolution spectroscopy of H3+ with strategic 5.1-micron imaging requested by Orton | Apr 6, 9:10-16:10 UTC | ||||||||||||
20 | near IR | Rathbun | IRTF/SpeX | imaging of Io’s Jupiter-facing hemisphere while in eclipse to determine the brightnesses of volcanoes | May 1, 11:50-13:20 UTC May 8, 13:35-15:05 UTC May 17, 9:45-11:15 UTC May 24, 11:30-13:00 UTC May 31, 13:30-15:00 UTC | ||||||||||||
21 | near IR | Rathbun | IRTF/SpeX | imaging of Io to determine if any major eruptions are occurring | Apr 4, 14:50-15:10 UTC Apr 5, 15:40-16:10 UTC Apr 10, 15:40-16:10 UTC Apr 11, 15:40-16:10 UTC Apr 26 15:40-16:10 UTC Apr 29 15:40-16:10 UTC May 3 15:35-16:05 UTC May 14, 11:00-11:30 UTC May 18, 11:45-12:15 UTC May 20, 9:15-9:45 UTC May 24, 11:30-13:00 UTC | ||||||||||||
22 | mid IR | Greathouse | IRTF TEXES | mapping of quasi-quadrennial oscillation | Apr 15,23,24 | ||||||||||||
23 | mid IR | Sinclair | IRTF TEXES | mapping of auroral-related stratospheric heating | Apr 15,16,21,23,24 | ||||||||||||
24 | mid IR | Antunano | IRTF TEXES | mapping of EZ Disturbance | Apr 17, 13:15-18:00 UTC Apr 18, 13:15-18:00 UTC | ||||||||||||
25 | microwave | de Pater | VLA | X and Ku band | Apr. 6 and 7, 2019 | ||||||||||||
26 | K band | Apr. 8 and 9, 2019 | |||||||||||||||
27 | radio | Zarka, Cecconi, Lamy, Louis | Nançay Decameter Array (France) | coordinated measurement of 10-40 MHz cyclotron radio emission | every day, 8 hours around the transition to local meridian | https://maser.lesia.obspm.fr/task-1-data-collections/juno-ground-radio/juno-ground-radio-nancay-decameter.html?lang=en | |||||||||||
28 | Radio | Lamy for the NenuFar ES07 team | NenuFAR (France) | coordinated measurements of 10-40 MHz cyclotron radio emission at high time/frequency resolution | Apr. 06 00:29-08:30; Apr. 07 00:25-08:27; Apr. 16 01:49-03:31 | Data available on demand to laurent.lamy@obspm.fr | |||||||||||
29 | Scheduled observations by Juno. | ||||||||||||||||
30 | |||||||||||||||||
31 | Perijove is April 6 2019 12:14:00 UTC. System-III longitude = 99.7°W | ||||||||||||||||
32 | |||||||||||||||||
33 | Period: Orbit 19 (2019 April 6 – 2019 May 28) | ||||||||||||||||
34 | Instrument | Description | |||||||||||||||
35 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | |||||||||||||||
36 | MWR | Thhe MWR will scan perpendicular to the orbit track ("cross-track"), thus observing more area but at a single emission angle. | |||||||||||||||
37 | UVS | no data, due to the unusual spacecraft orientation | |||||||||||||||
38 | JunoCam | no data, due to the unusual spacecraft orientation | |||||||||||||||
39 | JIRAM | no data, due to the unusual spacecraft orientation | |||||||||||||||
40 | |||||||||||||||||
41 | |||||||||||||||||
42 | |||||||||||||||||
43 | |||||||||||||||||
44 | |||||||||||||||||
45 | |||||||||||||||||
46 | |||||||||||||||||
47 | |||||||||||||||||
48 | |||||||||||||||||
49 | |||||||||||||||||
50 | |||||||||||||||||
51 | |||||||||||||||||
52 | |||||||||||||||||
53 | |||||||||||||||||
54 | |||||||||||||||||
55 | |||||||||||||||||
56 | |||||||||||||||||
57 | |||||||||||||||||
58 | |||||||||||||||||
59 | |||||||||||||||||
60 | |||||||||||||||||
61 | |||||||||||||||||
62 | |||||||||||||||||
63 | |||||||||||||||||
64 | |||||||||||||||||
65 | |||||||||||||||||
66 | |||||||||||||||||
67 | |||||||||||||||||
68 | |||||||||||||||||
69 | |||||||||||||||||
70 | |||||||||||||||||
71 | |||||||||||||||||
72 | |||||||||||||||||
73 | |||||||||||||||||
74 | |||||||||||||||||
75 | |||||||||||||||||
76 | |||||||||||||||||
77 | |||||||||||||||||
78 | |||||||||||||||||
79 | |||||||||||||||||
80 | |||||||||||||||||
81 | |||||||||||||||||
82 | |||||||||||||||||
83 | |||||||||||||||||
84 | |||||||||||||||||
85 | |||||||||||||||||
86 | |||||||||||||||||
87 | |||||||||||||||||
88 | |||||||||||||||||
89 | |||||||||||||||||
90 | |||||||||||||||||
91 | |||||||||||||||||
92 | |||||||||||||||||
93 | |||||||||||||||||
94 | |||||||||||||||||
95 | MWR coverage in "cross-track" attitide. Visual image of Jupiter is for orientation only and does not correspond to Jupiter's actual cloud morphology during this perijove. | ||||||||||||||||
96 | |||||||||||||||||
97 | |||||||||||||||||
98 | |||||||||||||||||
99 | |||||||||||||||||
100 | |||||||||||||||||
101 | |||||||||||||||||
102 | |||||||||||||||||
103 | |||||||||||||||||
104 | |||||||||||||||||
105 | |||||||||||||||||
106 | |||||||||||||||||
107 | |||||||||||||||||
108 | |||||||||||||||||
109 | |||||||||||||||||
110 | |||||||||||||||||
111 | |||||||||||||||||
112 | |||||||||||||||||
113 | |||||||||||||||||
114 | |||||||||||||||||
115 | |||||||||||||||||
116 | |||||||||||||||||
117 | |||||||||||||||||
118 | |||||||||||||||||
119 | |||||||||||||||||
120 | |||||||||||||||||
121 | |||||||||||||||||
122 | |||||||||||||||||
123 | |||||||||||||||||
124 | |||||||||||||||||
125 | |||||||||||||||||
126 | MWR coverage in "cross-track" attitide in mercator projection. Areas in gray denote coverage in which the fields of view are entirely on the planet. | ||||||||||||||||
127 | |||||||||||||||||
128 | |||||||||||||||||
129 | |||||||||||||||||
130 | |||||||||||||||||
131 | |||||||||||||||||
132 | |||||||||||||||||
133 | |||||||||||||||||
134 | |||||||||||||||||
135 | |||||||||||||||||
136 | |||||||||||||||||
137 | |||||||||||||||||
138 | |||||||||||||||||
139 | |||||||||||||||||
140 | |||||||||||||||||
141 | |||||||||||||||||
142 | |||||||||||||||||
143 | |||||||||||||||||
144 | |||||||||||||||||
145 | |||||||||||||||||
146 | |||||||||||||||||
147 | |||||||||||||||||
148 | |||||||||||||||||
149 | |||||||||||||||||
150 | |||||||||||||||||
151 | |||||||||||||||||
152 | |||||||||||||||||
153 | |||||||||||||||||
154 | |||||||||||||||||
155 | |||||||||||||||||
156 | |||||||||||||||||
157 | |||||||||||||||||
158 | |||||||||||||||||
159 | |||||||||||||||||
160 | |||||||||||||||||
161 | |||||||||||||||||
162 | |||||||||||||||||
163 | |||||||||||||||||
164 | |||||||||||||||||
165 | |||||||||||||||||
166 | |||||||||||||||||
167 | |||||||||||||||||
168 | |||||||||||||||||
169 | |||||||||||||||||
170 | |||||||||||||||||
171 | |||||||||||||||||
172 | |||||||||||||||||
173 | |||||||||||||||||
174 | |||||||||||||||||
175 | |||||||||||||||||
176 | |||||||||||||||||
177 | |||||||||||||||||
178 | |||||||||||||||||
179 | |||||||||||||||||
180 | |||||||||||||||||
181 | |||||||||||||||||
182 | |||||||||||||||||
183 | |||||||||||||||||
184 | |||||||||||||||||
185 | |||||||||||||||||
186 | |||||||||||||||||
187 | JIRAM fields of view | ||||||||||||||||
188 | The dates reported (both in UTC and in hours from PJ) on the top are referred to the last acquisition with the M filter of the whole plan for the given JM | ||||||||||||||||
189 | The # field, is the estimated number of the acquisition of the whole plan, | ||||||||||||||||
190 | (Ignore the percentage field.) | ||||||||||||||||
191 | The light blue area, enclosed by dark blue lines, represented the FoVs of Imager M projected on Jupiter. Dark blue areas that you can see in some positions are created | ||||||||||||||||
192 | by more projected FoV overlapping at close distance; i.e. these zones are created by multi FoV edges ( dark blue lines) that plot each close to the other create these graphic artefacts | ||||||||||||||||
193 | The background cloud rendition is for general orientation; the position of the Great Red Spot does not indicate its actual position during these observations. | ||||||||||||||||
194 | |||||||||||||||||
195 | |||||||||||||||||
196 | |||||||||||||||||
197 | |||||||||||||||||
198 | |||||||||||||||||
199 | |||||||||||||||||
200 | |||||||||||||||||
201 | |||||||||||||||||
202 | |||||||||||||||||
203 | |||||||||||||||||
204 | |||||||||||||||||
205 | |||||||||||||||||
206 | |||||||||||||||||
207 | |||||||||||||||||
208 | |||||||||||||||||
209 | |||||||||||||||||
210 | |||||||||||||||||
211 | |||||||||||||||||
212 | |||||||||||||||||
213 | |||||||||||||||||
214 | |||||||||||||||||
215 | |||||||||||||||||
216 | |||||||||||||||||
217 | |||||||||||||||||
218 | |||||||||||||||||
219 | |||||||||||||||||
220 | |||||||||||||||||
221 | |||||||||||||||||
222 | |||||||||||||||||
223 | |||||||||||||||||
224 | Composite of JIRAM M-band (5-micron) map. | ||||||||||||||||
225 |
1 | ||||||||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
2 | ||||||||||||||||||
3 | Period: Orbit 18 [GRAV] (2019 February 12 – 2019 April 5) | |||||||||||||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | Observations requested. | |||||||||||
5 | Observations planned / granted time | |||||||||||||||||
6 | Visible | Veillet | LBT / PEPSI | Io eclipse spectroscopy | March 16, April 1 | TBD | Observations successful | |||||||||||
7 | Visible | Schmidt | Keck / HIRES | Io eclipse spectroscopy | Feb 12 pre-PJ18 | Cancelled (ice) | Observations cancelled or unsuccessful | |||||||||||
8 | visible/NUV/ near-IR | Wong (14661) | Hubble/ WFC3-UVIS | hi-resolution non-global snapshot | 2019 Feb 12 | https://archive.stsci.edu/prepds/wfcj/ https://doi.org/10.3847/1538-4365/ab775f https://doi.org/10.1016/j.icarus.2022.114994 | ||||||||||||
9 | near IR | Giles | Gemini-N/NIRI | adaptive-optics-stabilized imaging of reflected sunlight | observations requested several times during this period | TBD | ||||||||||||
10 | X-ray | Dunn | XMM-Newton | ~20 hours of continuous spectral, spatial and temporal resolution of Jupiter planned for start of April | start of April, dates to be confirmed, with some flexibility to plan around other observations at this time - contact w.dunn@ucl.ac.uk, if you think we might be able to do some valuable science by scheduling simultaneity | |||||||||||||
11 | FUV | Grodent (HST GO-15638) | HST/STIS | Jupiter northern FUV aurora | Northern hemisphere 19.040 (Feb 9) 18:01-18:50 19.042 (Feb 11) 00:13-01:01 19.042 (Feb 11) 19:18-20:05 19.044 (Feb 13) 01:29-02:19 19.044 (Feb 13) 20:35-21:20 Southern hemisphere 19.041 (Feb 10) 00:24-01:11 19.041 (Feb 10) 21:03-21:50 19.043 (Feb 12) 01:40-02:26 There should be two additional orbits in the north near apojove (early March). | No proprietary period. Check out preview movies at https://www.lpap.uliege.be/cms/c_3478756/en/lpap-hst-campaign | ||||||||||||
12 | FUV | Grodent | HST/STIS/G140L | Io's FUV airglow wake region around the ~1" Io disk when Io is at orbital longitude close to 90 deg (visit 51) | Feb 14 (19.045) 20:27-21:10 Feb 14 (19.045) 21:58-22:45 | |||||||||||||
13 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | 20190212, 20190217, 20190218, 20190224, 20190225, 20190226, 20190301, 20190304, 20190305, 20190306, 20190307, 20190309, 20190314, 20190316, 20190318, 20190319, 20190320, 20190321, 20190322, 20190323, 20190325, 20190326, 20190404, 20190405 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | Jan 15 to Jul 3, near continuous observations | Major Sodium outburst Jan -- Jun (Morgenthaler et al. 2019 ApJL) | |||||||
14 | near IR | Rathbun | IRTF/SpeX | imaging of Io’s Jupiter-facing hemisphere while in eclipse to determine the brightnesses of volcanoes, with strategic 5.1-micron imaging of Jupiter requested by Orton | Feb 28, 13:40-15:10 UTC Mar 7, 15:35-17:05 UTC Mar 23, 13:50-15:20 UTC Mar 30, 15:40-17:10 UTC | |||||||||||||
15 | near IR | Rathbun | IRTF/SpeX | imaging of Io to determine if any major eruptions are occurring | Mar 4, 15:50-16:20 UTC Mar 5, 15:50-16:20 UTC Mar 11, 15:50-16:20 UTC Mar 12, 15:50-16:20 UTC Mar 18, 15:50-16:20 UTC Mar 20, 15:50-16:20 UTC Mar 28 14:50-15:20 UTC Mar 21, 14:50-16:20 UTC | |||||||||||||
16 | mid IR | Greathouse | IRTF TEXES | mapping of quasi-quadrennial oscillation | Feb 9, 15:15-21:00 UTC Feb 10, 15:15-21:00 UTC | |||||||||||||
17 | mid IR | Sinclair | IRTF TEXES | mapping of auroral-related stratospheric heating | Feb 11, 15:30-20:00 UTC Feb 12, 15:15-20:00 UTC | |||||||||||||
18 | mid IR | Antunano | IRTF TEXES | mapping of EZ Disturbance | Feb 13, 15:00-20:00 UTC Feb 14, 15:00-20:00 UTC | |||||||||||||
19 | radio | Zarka, Cecconi, Lamy, Louis | Nançay Decameter Array (France) | coordinated measurement of 10-40 MHz cyclotron radio emission | every day, 8 hours around the transition to local meridian | https://maser.lesia.obspm.fr/task-1-data-collections/juno-ground-radio/juno-ground-radio-nancay-decameter.html?lang=en | ||||||||||||
20 | Radio | Lamy for the NenuFar ES07 team | NenuFAR (France) | coordinated measurements of 10-40 MHz cyclotron radio emission at high time/frequency resolution | Apr. 05 00:33-08:34 | Data available on demand to laurent.lamy@obspm.fr | ||||||||||||
21 | ||||||||||||||||||
22 | ||||||||||||||||||
23 | ||||||||||||||||||
24 | Scheduled observations by Juno. | |||||||||||||||||
25 | ||||||||||||||||||
26 | Perijove is February 12 2019 17:34:16 UTC. System-III longitude = 235.3°W | |||||||||||||||||
27 | ||||||||||||||||||
28 | Period: Orbit 18 (2019 February 12 – 2019 April 5) | |||||||||||||||||
29 | Instrument | Description | ||||||||||||||||
30 | MAG, JADE, JEDI, WAVES | |||||||||||||||||
31 | MWR | |||||||||||||||||
32 | UVS | |||||||||||||||||
33 | JunoCam | |||||||||||||||||
34 | JIRAM | |||||||||||||||||
35 | ||||||||||||||||||
36 | ||||||||||||||||||
37 | ||||||||||||||||||
38 | ||||||||||||||||||
39 | ||||||||||||||||||
40 | ||||||||||||||||||
41 | ||||||||||||||||||
42 | ||||||||||||||||||
43 | ||||||||||||||||||
44 | ||||||||||||||||||
45 | ||||||||||||||||||
46 | ||||||||||||||||||
47 | ||||||||||||||||||
48 | ||||||||||||||||||
49 | ||||||||||||||||||
50 | ||||||||||||||||||
51 | ||||||||||||||||||
52 | ||||||||||||||||||
53 | ||||||||||||||||||
54 | ||||||||||||||||||
55 | ||||||||||||||||||
56 | ||||||||||||||||||
57 | ||||||||||||||||||
58 | ||||||||||||||||||
59 | ||||||||||||||||||
60 | ||||||||||||||||||
61 | ||||||||||||||||||
62 | ||||||||||||||||||
63 | ||||||||||||||||||
64 | ||||||||||||||||||
65 | ||||||||||||||||||
66 | ||||||||||||||||||
67 | ||||||||||||||||||
68 | ||||||||||||||||||
69 | ||||||||||||||||||
70 | ||||||||||||||||||
71 | ||||||||||||||||||
72 | ||||||||||||||||||
73 | ||||||||||||||||||
74 | ||||||||||||||||||
75 | ||||||||||||||||||
76 | ||||||||||||||||||
77 | ||||||||||||||||||
78 | ||||||||||||||||||
79 | ||||||||||||||||||
80 | ||||||||||||||||||
81 | ||||||||||||||||||
82 | ||||||||||||||||||
83 | ||||||||||||||||||
84 | ||||||||||||||||||
85 | ||||||||||||||||||
86 | ||||||||||||||||||
87 | ||||||||||||||||||
88 | ||||||||||||||||||
89 | MWR footprints for the minimum emission angle at each latitude. | |||||||||||||||||
90 | ||||||||||||||||||
91 | ||||||||||||||||||
92 | ||||||||||||||||||
93 | ||||||||||||||||||
94 | ||||||||||||||||||
95 | ||||||||||||||||||
96 | ||||||||||||||||||
97 | ||||||||||||||||||
98 | ||||||||||||||||||
99 | ||||||||||||||||||
100 | ||||||||||||||||||
101 | ||||||||||||||||||
102 | ||||||||||||||||||
103 | ||||||||||||||||||
104 | ||||||||||||||||||
105 | ||||||||||||||||||
106 | ||||||||||||||||||
107 | ||||||||||||||||||
108 | ||||||||||||||||||
109 | ||||||||||||||||||
110 | ||||||||||||||||||
111 | ||||||||||||||||||
112 | ||||||||||||||||||
113 | ||||||||||||||||||
114 | ||||||||||||||||||
115 | ||||||||||||||||||
116 | ||||||||||||||||||
117 | ||||||||||||||||||
118 | ||||||||||||||||||
119 | ||||||||||||||||||
120 | ||||||||||||||||||
121 | ||||||||||||||||||
122 | ||||||||||||||||||
123 | ||||||||||||||||||
124 | ||||||||||||||||||
125 | ||||||||||||||||||
126 | ||||||||||||||||||
127 | JIRAM fields of view | |||||||||||||||||
128 | The dates reported (both in UTC and in hours from PJ) on the top are referred to the last acquisition with the M filter of the whole plan for the given JM | |||||||||||||||||
129 | The # field, is the estimated number of the acquisition of the whole plan, | |||||||||||||||||
130 | (Ignore the percentage field.) | |||||||||||||||||
131 | The light blue area, enclosed by dark blue lines, represented the FoVs of Imager M projected on Jupiter. Dark blue areas that you can see in some positions are created | |||||||||||||||||
132 | by more projected FoV overlapping at close distance; i.e. these zones are created by multi FoV edges ( dark blue lines) that plot each close to the other create these graphic artefacts | |||||||||||||||||
133 | The background cloud rendition is for general orientation; the position of the Great Red Spot does not indicate its actual position during these observations. | |||||||||||||||||
134 | ||||||||||||||||||
135 | ||||||||||||||||||
136 | ||||||||||||||||||
137 | ||||||||||||||||||
138 | ||||||||||||||||||
139 | ||||||||||||||||||
140 | ||||||||||||||||||
141 | ||||||||||||||||||
142 | ||||||||||||||||||
143 | ||||||||||||||||||
144 | ||||||||||||||||||
145 | ||||||||||||||||||
146 | ||||||||||||||||||
147 | ||||||||||||||||||
148 | ||||||||||||||||||
149 | ||||||||||||||||||
150 | ||||||||||||||||||
151 | ||||||||||||||||||
152 | ||||||||||||||||||
153 | ||||||||||||||||||
154 | ||||||||||||||||||
155 | ||||||||||||||||||
156 | ||||||||||||||||||
157 | ||||||||||||||||||
158 | ||||||||||||||||||
159 | ||||||||||||||||||
160 | ||||||||||||||||||
161 | ||||||||||||||||||
162 | ||||||||||||||||||
163 | ||||||||||||||||||
164 | ||||||||||||||||||
165 | ||||||||||||||||||
166 | Composite of JIRAM M-band (5-micron) map. |
1 | ||||||||
---|---|---|---|---|---|---|---|---|
2 | ||||||||
3 | Period: Orbit 17 [GRAV] (2018 December 21 – 2019 February 11) | Observations requested. | ||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | Observations planned / granted time | |
5 | Observations successful | |||||||
6 | Observations cancelled or unsuccessful | |||||||
7 | near IR | Giles | Gemini-N/NIRI | adaptive-optics-stabilized imaging of reflected sunlight | observations requested several times during this period | TBD | ||
8 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | 20190209 20190211 | |||
9 | mid-IR | Orton | IRTF/MIRSI (instrument not available, replaced by IRTF/SpeX) | filtered imaging at several wavelengths between 1.58 and 5.1 microns | Six hours on two sequentional days: 2019 Jan 16 and 17 | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired. Reduced "quick-look" observations (geometrically but not radiometrically calibrated) will be available for immeduately use from the Juno-curated web site: http://junoirtf.space.swri.edu/ | ||
10 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | Jan 15 to Jul 3, near continuous observations | Major Sodium outburst Jan -- Jun (Morgenthaler et al. 2019 ApJL) | ||
11 | radio | Zarka, Cecconi, Lamy, Louis | Nançay Decameter Array (France) | coordinated measurement of 10-40 MHz cyclotron radio emission | every day, 8 hours around the transition to local meridian | https://maser.lesia.obspm.fr/task-1-data-collections/juno-ground-radio/juno-ground-radio-nancay-decameter.html?lang=en | ||
12 | ||||||||
13 | ||||||||
14 | ||||||||
15 | ||||||||
16 | ||||||||
17 | Scheduled observations by Juno. | |||||||
18 | ||||||||
19 | Perijove is December 21 2018 17:00:27 UTC. System-III longitude = 157.0°W | |||||||
20 | ||||||||
21 | Period: Orbit 17 (2018 December 21 – 2019 February 11) | |||||||
22 | Instrument | Description | ||||||
23 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||
24 | MWR | |||||||
25 | UVS | |||||||
26 | JunoCam | |||||||
27 | JIRAM | |||||||
28 | ||||||||
29 | ||||||||
30 | ||||||||
31 | ||||||||
32 | ||||||||
33 | ||||||||
34 | ||||||||
35 | ||||||||
36 | ||||||||
37 | ||||||||
38 | ||||||||
39 | ||||||||
40 | ||||||||
41 | ||||||||
42 | ||||||||
43 | ||||||||
44 | ||||||||
45 | ||||||||
46 | ||||||||
47 | ||||||||
48 | ||||||||
49 | ||||||||
50 | ||||||||
51 | ||||||||
52 | ||||||||
53 | ||||||||
54 | ||||||||
55 | ||||||||
56 | ||||||||
57 | ||||||||
58 | ||||||||
59 | ||||||||
60 | ||||||||
61 | ||||||||
62 | ||||||||
63 | ||||||||
64 | ||||||||
65 | ||||||||
66 | ||||||||
67 | ||||||||
68 | ||||||||
69 | ||||||||
70 | ||||||||
71 | ||||||||
72 | ||||||||
73 | ||||||||
74 | ||||||||
75 | ||||||||
76 | ||||||||
77 | ||||||||
78 | ||||||||
79 | ||||||||
80 | ||||||||
81 | ||||||||
82 | ||||||||
83 | MWR footprints for the minimum emission angle at each spacecraft rotation. Periove position is given by the cross. | |||||||
84 | ||||||||
85 | ||||||||
86 | ||||||||
87 | ||||||||
88 | ||||||||
89 | ||||||||
90 | ||||||||
91 | ||||||||
92 | ||||||||
93 | ||||||||
94 | ||||||||
95 | ||||||||
96 | ||||||||
97 | ||||||||
98 | ||||||||
99 | ||||||||
100 | ||||||||
101 | ||||||||
102 | ||||||||
103 | ||||||||
104 | ||||||||
105 | ||||||||
106 | ||||||||
107 | ||||||||
108 | ||||||||
109 | ||||||||
110 | ||||||||
111 | ||||||||
112 | ||||||||
113 | ||||||||
114 | ||||||||
115 | ||||||||
116 | ||||||||
117 | JIRAM fields of view | |||||||
118 | The dates reported (both in UTC and in hours from PJ) on the top are referred to the last acquisition with the M filter of the whole plan for the given JM | |||||||
119 | The # field, is the estimated number of the acquisition of the whole plan, | |||||||
120 | (Ignore the percentage field.) | |||||||
121 | The light blue area, enclosed by dark blue lines, represented the FoVs of Imager M projected on Jupiter. Dark blue areas that you can see in some positions are created | |||||||
122 | by more projected FoV overlapping at close distance; i.e. these zones are created by multi FoV edges ( dark blue lines) that plot each close to the other create these graphic artefacts | |||||||
123 | The background cloud rendition is for general orientation; the position of the Great Red Spot does not indicate its actual position during these observations. | |||||||
124 | ||||||||
125 | ||||||||
126 | ||||||||
127 | ||||||||
128 | ||||||||
129 | ||||||||
130 | ||||||||
131 | ||||||||
132 | ||||||||
133 | ||||||||
134 | ||||||||
135 | ||||||||
136 | ||||||||
137 | ||||||||
138 | ||||||||
139 | ||||||||
140 | ||||||||
141 | ||||||||
142 | ||||||||
143 | ||||||||
144 | ||||||||
145 | ||||||||
146 | ||||||||
147 | ||||||||
148 | ||||||||
149 | ||||||||
150 | ||||||||
151 | Composite of JIRAM M-band (5-micron) map. | |||||||
152 |
1 | Note: On this orbit the spacecraft orientation is planned to be off Earth-axis in order to improve remote-sensing observations. Jupiter is very close to solar conjunction during this period. | |||||||
---|---|---|---|---|---|---|---|---|
2 | ||||||||
3 | Period: Orbit 16 [GRAV] (2018 October 29 – 2018 December 20) | |||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | ||
5 | near IR | Orton | IRTF/SpeX | filtered imaging at several wavelengths between 1.58 and 5.1µm in ~3-hour daytime boserving program, using Director Discretionary time. Observations to be made of the PJ16 longitude ~20 hours after PJ16 overflight. | Oct 27, 20:30-23:30 UTC; December 17, 22:00-23:30 UTC (the December dates are closer to PJ17) | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired. Reduced "quick-look" observations (geometrically but not radiometrically calibrated) will be available for immeduately use from the Juno-curated web site: http://junoirtf.space.swri.edu/ | ||
6 | radio | Zarka, Cecconi, Lamy, Louis | Nançay Decameter Array (France) | coordinated measurement of 10-40 MHz cyclotron radio emission | every day, 8 hours around the transition to local meridian | https://maser.lesia.obspm.fr/task-1-data-collections/juno-ground-radio/juno-ground-radio-nancay-decameter.html?lang=en | Observations requested. | |
7 | Observations planned / granted time | |||||||
8 | Scheduled observations by Juno. | Observations successful | ||||||
9 | Observations cancelled or unsuccessful | |||||||
10 | Perijove is October 29 2018 21:06:17 UTC. System-III longitude = 247.6°W | |||||||
11 | ||||||||
12 | Period: Orbit 16 (2018 October 29 – 2018 December 20) | |||||||
13 | Instrument | Description | ||||||
14 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||
15 | MWR | |||||||
16 | UVS | |||||||
17 | JunoCam | |||||||
18 | JIRAM | |||||||
19 | ||||||||
20 | ||||||||
21 | ||||||||
22 | ||||||||
23 | ||||||||
24 | ||||||||
25 | ||||||||
26 | ||||||||
27 | ||||||||
28 | ||||||||
29 | ||||||||
30 | ||||||||
31 | ||||||||
32 | ||||||||
33 | ||||||||
34 | ||||||||
35 | ||||||||
36 | ||||||||
37 | ||||||||
38 | ||||||||
39 | ||||||||
40 | ||||||||
41 | ||||||||
42 | ||||||||
43 | ||||||||
44 | ||||||||
45 | ||||||||
46 | ||||||||
47 | ||||||||
48 | ||||||||
49 | ||||||||
50 | ||||||||
51 | ||||||||
52 | ||||||||
53 | ||||||||
54 | ||||||||
55 | ||||||||
56 | ||||||||
57 | ||||||||
58 | ||||||||
59 | ||||||||
60 | ||||||||
61 | ||||||||
62 | ||||||||
63 | ||||||||
64 | ||||||||
65 | ||||||||
66 | ||||||||
67 | ||||||||
68 | ||||||||
69 | ||||||||
70 | ||||||||
71 | ||||||||
72 | ||||||||
73 | ||||||||
74 | ||||||||
75 | ||||||||
76 | MWR footprints for the minimum emission angle at each latitude. | |||||||
77 | ||||||||
78 | ||||||||
79 | ||||||||
80 | ||||||||
81 | ||||||||
82 | ||||||||
83 | ||||||||
84 | ||||||||
85 | ||||||||
86 | ||||||||
87 | ||||||||
88 | ||||||||
89 | ||||||||
90 | ||||||||
91 | ||||||||
92 | ||||||||
93 | ||||||||
94 | ||||||||
95 | ||||||||
96 | ||||||||
97 | ||||||||
98 | ||||||||
99 | ||||||||
100 | ||||||||
101 | ||||||||
102 | ||||||||
103 | ||||||||
104 | ||||||||
105 | ||||||||
106 | ||||||||
107 | ||||||||
108 | ||||||||
109 | JIRAM fields of view | |||||||
110 | The dates reported (both in UTC and in hours from PJ) on the top are referred to the last acquisition with the M filter of the whole plan for the given JM | |||||||
111 | The # field, is the estimated number of the acquisition of the whole plan, | |||||||
112 | (Ignore the percentage field.) | |||||||
113 | The light blue area, enclosed by dark blue lines, represented the FoVs of Imager M projected on Jupiter. Dark blue areas that you can see in some positions are created | |||||||
114 | by more projected FoV overlapping at close distance; i.e. these zones are created by multi FoV edges ( dark blue lines) that plot each close to the other create these graphic artefacts | |||||||
115 | The background cloud rendition is for general orientation; the position of the Great Red Spot does not indicate its actual position during these observations. | |||||||
116 | ||||||||
117 | ||||||||
118 | ||||||||
119 | ||||||||
120 | ||||||||
121 | ||||||||
122 | ||||||||
123 | ||||||||
124 | ||||||||
125 | ||||||||
126 | ||||||||
127 | ||||||||
128 | ||||||||
129 | ||||||||
130 | ||||||||
131 | ||||||||
132 | ||||||||
133 | ||||||||
134 | ||||||||
135 | ||||||||
136 | ||||||||
137 | ||||||||
138 | ||||||||
139 | ||||||||
140 | ||||||||
141 | ||||||||
142 | ||||||||
143 | ||||||||
144 | ||||||||
145 | Composite of JIRAM M-band (5-micron) map. |
1 | Note: On this orbit the spacecraft orientation optimizes gravity mapping (GRAV) with the antenna pointed toward the Earth continuously. | ||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|
2 | |||||||||||
3 | Period: Orbit 15 [GRAV] (2018 September 6 – 2018 October 28) | Observations requested. | |||||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | Observations planned / granted time | ||||
5 | X-ray | Gladstone | Chandra | ~10 hours of HRC-I observations of Jupiter | 09/06/2018 20:40 - 09/07/2018 08:35 | publicly available after 1 year | Observations successful | ||||
6 | X-ray | Dunn | XMM-Newton | spectral, spatial and time-tagged X-ray observations of Jupiter | 8/27/2018 15:27:02 - 2018-08-28 04:43:42 | Dunn happy to share data | Observations cancelled or unsuccessful | ||||
7 | FUV | Grodent | HST/STIS | Jupiter FUV aurora (last observations of this HST program 14634) | start time (~45 min exp) 09/03/2018 02:36:00 09/04/2018 08:48:00 09/05/2018 03:52:00 09/06/2018 05:17:00 09/07/2018 05:07:00 | https://www.lpap.uliege.be/cms/c_3478756/en/lpap-hst-campaign | |||||
8 | CCD | Irwin/Braude | VLT/MUSE - IFU | spectroscopic imaging, 475-930 nm to determine cloud structure and albedo spectrum of particles. | 11 Sep 2018 | Raw data publicly available to download from ESO portal this time next year. Standard calibration pipeline takes of the order of 1-3 days to complete. Calibration is a bit iffy due to poor standard. | |||||
9 | visible/NUV | Wong | HST/WFC3 UVIS | hi-resolution map of perijove track, single orbit snapshot | PJ | https://archive.stsci.edu/prepds/wfcj/ https://dx.doi.org/10.1016/j.icarus.2017.06.007 | |||||
10 | near IR | Orton | IRTF/SpeX | filtered imaging at several wavelengths between 1.58 and 5.1µm in ~40-min program, using Director Discretionary time. Observations were made of the PJ15 longitude ~20 hours before PJ15 overflight. | Sept 6, 16:20-16:50 UTC. | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired. Reduced "quick-look" observations (geometrically but not radiometrically calibrated) will be available for immeduately use from the Juno-curated web site: http://junoirtf.space.swri.edu/ | |||||
11 | near IR | Giles | Gemini-N/NIRI | adaptive-optics-stabilized imaging of reflected sunlight | observations requested several times during this period | TBD | |||||
12 | near IR (5 µm) | Wong | Gemini-N/NIRI | lucky imaging, 5-µm maps | PJ15 | ||||||
13 | mid-IR | Fletcher | VLT/VISIR | filtered radiometric imaging to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology. | 3.3 hrs awarded | available in raw form in the ESO archive within 24 hours of acquisition; cylindrical maps within 1-2 days and reduced maps within a week | |||||
14 | radio | Zarka, Cecconi, Lamy, Louis | Nançay Decameter Array (France) | coordinated measurement of 10-40 MHz cyclotron radio emission | every day, 8 hours around the transition to local meridian | https://maser.lesia.obspm.fr/task-1-data-collections/juno-ground-radio/juno-ground-radio-nancay-decameter.html?lang=en | |||||
15 | |||||||||||
16 | |||||||||||
17 | Scheduled observations by Juno. | ||||||||||
18 | |||||||||||
19 | Perijove is September 7 2018 01:11:57 UTC. System-III longitude = 338.2°W | ||||||||||
20 | |||||||||||
21 | Period: Orbit 15 (2018 September 7 – 2018 October 28) | ||||||||||
22 | Instrument | Description | |||||||||
23 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | |||||||||
24 | MWR | ||||||||||
25 | UVS | ||||||||||
26 | JunoCam | ||||||||||
27 | JIRAM | ||||||||||
28 | |||||||||||
29 | |||||||||||
30 | |||||||||||
31 | |||||||||||
32 | |||||||||||
33 | |||||||||||
34 | |||||||||||
35 | |||||||||||
36 | |||||||||||
37 | |||||||||||
38 | |||||||||||
39 | |||||||||||
40 | |||||||||||
41 | |||||||||||
42 | |||||||||||
43 | |||||||||||
44 | |||||||||||
45 | |||||||||||
46 | |||||||||||
47 | |||||||||||
48 | |||||||||||
49 | |||||||||||
50 | |||||||||||
51 | |||||||||||
52 | |||||||||||
53 | |||||||||||
54 | |||||||||||
55 | |||||||||||
56 | MWR footprints for the minimum emission angle at each latitude. | ||||||||||
57 | |||||||||||
58 | |||||||||||
59 | |||||||||||
60 | |||||||||||
61 | |||||||||||
62 | |||||||||||
63 | |||||||||||
64 | |||||||||||
65 | |||||||||||
66 | |||||||||||
67 | |||||||||||
68 | |||||||||||
69 | |||||||||||
70 | |||||||||||
71 | |||||||||||
72 | |||||||||||
73 | |||||||||||
74 | |||||||||||
75 | |||||||||||
76 | |||||||||||
77 | |||||||||||
78 | |||||||||||
79 | |||||||||||
80 | |||||||||||
81 | |||||||||||
82 | |||||||||||
83 | |||||||||||
84 | |||||||||||
85 | |||||||||||
86 | |||||||||||
87 | |||||||||||
88 | |||||||||||
89 | |||||||||||
90 | |||||||||||
91 | |||||||||||
92 | |||||||||||
93 | |||||||||||
94 | |||||||||||
95 | |||||||||||
96 | JIRAM fields of view | ||||||||||
97 | The dates reported (both in UTC and in hours from PJ) on the top are referred to the last acquisition with the M filter of the whole plan for the given JM | ||||||||||
98 | The # field, is the estimated number of the acquisition of the whole plan, | ||||||||||
99 | (Ignore the percentage field.) | ||||||||||
100 | The light blue area, enclosed by dark blue lines, represented the FoVs of Imager M projected on Jupiter. Dark blue areas that you can see in some positions are created | ||||||||||
101 | by more projected FoV overlapping at close distance; i.e. these zones are created by multi FoV edges ( dark blue lines) that plot each close to the other create these graphic artefacts | ||||||||||
102 | The background cloud rendition is for general orientation; the position of the Great Red Spot does not indicate its actual position during these observations. | ||||||||||
103 | |||||||||||
104 | |||||||||||
105 | |||||||||||
106 | |||||||||||
107 | |||||||||||
108 | |||||||||||
109 | |||||||||||
110 | |||||||||||
111 | |||||||||||
112 | |||||||||||
113 | |||||||||||
114 | |||||||||||
115 | |||||||||||
116 | |||||||||||
117 | |||||||||||
118 | |||||||||||
119 | |||||||||||
120 | |||||||||||
121 | |||||||||||
122 | |||||||||||
123 | |||||||||||
124 | |||||||||||
125 | |||||||||||
126 | |||||||||||
127 | |||||||||||
128 | |||||||||||
129 | |||||||||||
130 | |||||||||||
131 | |||||||||||
132 | |||||||||||
133 | |||||||||||
134 | |||||||||||
135 | Composite of JIRAM M-band (5-micron) map. | ||||||||||
136 |
1 | ||||||||||
---|---|---|---|---|---|---|---|---|---|---|
2 | Note: On this orbit the spacecraft orientation optimizes gravity mapping (GRAV) with the antenna pointed toward the Earth continuously. | Observations requested. | ||||||||
3 | Observations planned / granted time | |||||||||
4 | Period: Orbit 14 [GRAV] (2018 July 16 – 2018 September 5) | Observations successful | ||||||||
5 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | Observations cancelled or unsuccessful | |||
6 | X-ray | Gladstone | Chandra | ~10 hours of HRC-I observations of Jupiter | 07/15/2018 23:45 - 07/16/2018 11:24 | publicly available after 1 year | ||||
7 | X-ray | Dunn | XMM-Newton | spectral, spatial and time-tagged X-ray observations of Jupiter on 16 July 03:06-09:06 and 17:38 16 July to 07:01 on 17 july | on 16 July 03:06-09:06 and 17:38 16 July to 07:01 on 17 july | Dunn is happy to share data | ||||
8 | FUV | Grodent | HST/STIS | Io Spectroscopy: 5 consecutive HST orbits to observe the evolution of Io's oxygen aurora in parallel with Juno/UVS views of the footprint and Hisaki monitoring of the Io torus and volcanic activity | 1K STIS/CCD STIS/FUV-MAMA 2 Jul 16, 2018 05:43:24 Jul 16, 2018 08:16:26 1L STIS/CCD STIS/FUV-MAMA 2 Jul 16, 2018 09:11:29 Jul 16, 2018 11:27:08 1Y STIS/CCD STIS/FUV-MAMA 1 Jul 16, 2018 12:17:48 Jul 16, 2018 12:58:19 | |||||
9 | FUV | Grodent | HST/STIS | Jupiter northern FUV aurora | 1M STIS/FUV-MAMA Jul 14, 2018 04:26:29 Jul 14, 2018 05:26:52 1T STIS/FUV-MAMA Jul 15, 2018 10:34:39 Jul 15, 2018 11:35:47 1U STIS/FUV-MAMA Jul 13, 2018 09:18:50 Jul 13, 2018 10:17:58 | |||||
10 | CCD | Irwin/Braude | VLT/MUSE - IFU | spectroscopic imaging, 475-930 nm to determine cloud structure and albedo spectrum of particles. | 7/12/2018 | Raw data publicly available to download from ESO portal this time next year. Standard calibration pipeline takes of the order of 1-3 days to complete. Off from PJ14 sub-observer longitude by about 30 degrees | ||||
11 | visible/NUV | Wong | HST/WFC3 UVIS | hi-resolution map of perijove track, single orbit snapshot | PJ14 | https://archive.stsci.edu/prepds/wfcj/ https://dx.doi.org/10.1016/j.icarus.2017.06.007 | ||||
12 | near IR | Orton | IRTF/SpeX | filtered imaging at several wavelengths between 1.58 and 5.1µm and spectral scanning over 2-µm and 5-µm ranges | 6-hour shifts on July 21 and 22 UT with marginal weather, but some images were obtained with useful SNR. 6-hour shift on July 23 UT obtained many good images but with ~0.8" seeing, and good spectroscopic scans at 0.7-2.5 microns and 4.3-5.2 microns covering the whole disk. Short sequences were obtained on August 19 through clear skies with 0.7" seeing and on August 20 through moderate cirrus with 1.0" seeing. | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired. Reduced "quick-look" observations (geometrically but not radiometrically calibrated) will be available for immeduately use from the Juno-curated web site: http://junoirtf.space.swri.edu/ | ||||
13 | near IR (5 µm) | Wong | Gemini-N/NIRI | lucky imaging, 5-µm maps | PJ14 | |||||
14 | near IR | Schmidt | IRTF/iSHELL | Io Spectroscopy | July 30th | |||||
15 | mid IR | Fletcher | VLT / VISIR | filtered radiometric imaging to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology. | 4.3 hours of observations in service time | available in raw form in the ESO archive within 24 hours of acquisition; cylindrical maps within 1-2 days and reduced maps within a week | ||||
16 | mid-IR | Melin | IRTF/TEXES | scanned spectral maps of Jupiter's disk at ten key spectral settings to derive upper-tropospheric and stratospheric temperatures, aerosol/cloud distributions, and distribution of tropospheric NH3 and PH3, and stratospheric C2H2 and C2H6. | one global map obtained for each of several key spectral settings near Sep 7 | raw data available almost immediately, calibrated files with geometry within a month, and retrieved properties potentially available within 1-2 weeks (subject to any unforeseen issues) | ||||
17 | mid IR | Greathouse | IRTF/TEXES | scanned high- and medium-resolution spectral maps of Jupiter's disk at key CH4- and H2-absorbing wavelengths to determine temperatures in the upper troposphere and stratosphere to determine the structure of non-seasonal thermal waves associated with the Quasi-Quadrennial Oscillation (QQO) | Two half nights at the start and again at the end of a dedicated TEXES run.sometime in Aug/Sep. | TBD | ||||
18 | mid IR | Sinclair | Subaru/COMICS | mosaicked images of Jupiter in discrete filters between 7 and 25 microns | Observations made during a ~30-min interval prior to thermal images of Saturn (post-Cassini support) on August 19/20 and 20/21 | requested through Keck exchange time | ||||
19 | mid-IR | Fletcher | VLT/VISIR | filtered radiometric imaging (as well as 'any time' M-band lucky imaging) to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology. | 4.3 hrs awarded | available in raw form in the ESO archive within 24 hours of acquisition; cylindrical maps within 1-2 days and reduced maps within a week | ||||
20 | radio | Zarka, Cecconi, Lamy, Louis | Nançay Decameter Array (France) | coordinated measurement of 10-40 MHz cyclotron radio emission | every day, 8 hours around the transition to local meridian | https://maser.lesia.obspm.fr/task-1-data-collections/juno-ground-radio/juno-ground-radio-nancay-decameter.html?lang=en | ||||
21 | ||||||||||
22 | Scheduled observations by Juno. | |||||||||
23 | ||||||||||
24 | Perijove is 07/16/2018 05:17:39 UTC. System-III longitude = 68.7 W | |||||||||
25 | ||||||||||
26 | Period: Orbit 14 [GRAV] (2018 July 16 – 2018 September 6) | |||||||||
27 | Instrument | Description | ||||||||
28 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||
29 | MWR | MWR will obtain oblique observations of Jupiter's atmosphere. Footprints of the lowest-emission-angle observations are shown in the figure below, with the perijove shown as the cross. | ||||||||
30 | UVS | |||||||||
31 | JunoCam | JunoCam will obtain images of polar regions and oblique views of lower latitudes. | ||||||||
32 | JIRAM | JIRAM will obtain imaging and spectroscopy of polar regions. | ||||||||
33 | ||||||||||
34 | ||||||||||
35 | ||||||||||
36 | ||||||||||
37 | ||||||||||
38 | ||||||||||
39 | ||||||||||
40 | ||||||||||
41 | ||||||||||
42 | ||||||||||
43 | ||||||||||
44 | ||||||||||
45 | ||||||||||
46 | ||||||||||
47 | ||||||||||
48 | ||||||||||
49 | ||||||||||
50 | ||||||||||
51 | ||||||||||
52 | ||||||||||
53 | ||||||||||
54 | ||||||||||
55 | ||||||||||
56 | ||||||||||
57 | ||||||||||
58 | ||||||||||
59 | ||||||||||
60 | ||||||||||
61 | ||||||||||
62 | ||||||||||
63 | ||||||||||
64 | ||||||||||
65 | MWR footprints for the minimum emission angle at each latitude. | |||||||||
66 | ||||||||||
67 | ||||||||||
68 | ||||||||||
69 | ||||||||||
70 | ||||||||||
71 | ||||||||||
72 | ||||||||||
73 | ||||||||||
74 | ||||||||||
75 | ||||||||||
76 | ||||||||||
77 | ||||||||||
78 | ||||||||||
79 | ||||||||||
80 | ||||||||||
81 | ||||||||||
82 | ||||||||||
83 | ||||||||||
84 | ||||||||||
85 | ||||||||||
86 | ||||||||||
87 | ||||||||||
88 | ||||||||||
89 | ||||||||||
90 | ||||||||||
91 | ||||||||||
92 | ||||||||||
93 | ||||||||||
94 | ||||||||||
95 | ||||||||||
96 | ||||||||||
97 | ||||||||||
98 | ||||||||||
99 | ||||||||||
100 | ||||||||||
101 | ||||||||||
102 | ||||||||||
103 | ||||||||||
104 | ||||||||||
105 | ||||||||||
106 | ||||||||||
107 | ||||||||||
108 | ||||||||||
109 | ||||||||||
110 | ||||||||||
111 | ||||||||||
112 | ||||||||||
113 | ||||||||||
114 | link to BAA report on PJ 14: | https://britastro.org/node/15050 | ||||||||
115 | ||||||||||
116 | ||||||||||
117 | ||||||||||
118 | ||||||||||
119 | ||||||||||
120 | ||||||||||
121 | ||||||||||
122 | ||||||||||
123 | ||||||||||
124 | ||||||||||
125 | ||||||||||
126 | ||||||||||
127 | ||||||||||
128 | ||||||||||
129 | ||||||||||
130 | ||||||||||
131 | ||||||||||
132 | ||||||||||
133 | ||||||||||
134 | ||||||||||
135 | ||||||||||
136 | ||||||||||
137 | ||||||||||
138 | ||||||||||
139 | ||||||||||
140 | ||||||||||
141 | ||||||||||
142 | ||||||||||
143 | ||||||||||
144 | ||||||||||
145 | ||||||||||
146 | ||||||||||
147 | ||||||||||
148 | ||||||||||
149 | JIRAM fields of view | |||||||||
150 | The dates reported (both in UTC and in hours from PJ) on the top are referred to the last acquisition with the M filter of the whole plan for the given JM | |||||||||
151 | The # field, is the estimated number of the acquisition of the whole plan, | |||||||||
152 | (Ignore the percentage field.) | |||||||||
153 | The light blue area, enclosed by dark blue lines, represented the FoVs of Imager M projected on Jupiter. Dark blue areas that you can see in some positions are created | |||||||||
154 | by more projected FoV overlapping at close distance; i.e. these zones are created by multi FoV edges ( dark blue lines) that plot each close to the other create these graphic artefacts | |||||||||
155 | The background cloud rendition is for general orientation; the position of the Great Red Spot does not indicate its actual position during these observations. | |||||||||
156 | ||||||||||
157 | ||||||||||
158 | ||||||||||
159 | ||||||||||
160 | ||||||||||
161 | ||||||||||
162 | ||||||||||
163 | ||||||||||
164 | ||||||||||
165 | ||||||||||
166 | ||||||||||
167 | ||||||||||
168 | ||||||||||
169 | ||||||||||
170 | ||||||||||
171 | ||||||||||
172 | ||||||||||
173 | ||||||||||
174 | ||||||||||
175 | ||||||||||
176 | ||||||||||
177 | ||||||||||
178 | ||||||||||
179 | ||||||||||
180 | ||||||||||
181 | ||||||||||
182 | ||||||||||
183 | ||||||||||
184 | ||||||||||
185 | Composite of JIRAM M-band (5-micron) map. |
1 | Note: On this orbit the spacecraft orientation optimizes gravity mapping (GRAV) with the antenna pointed toward the Earth continuously. | |||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|
2 | Observations requested. | |||||||||||
3 | Period: Orbit 13 [GRAV] (2018 May 24 – 2018 July 15) | Observations planned / granted time | ||||||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | Observations successful | |||||
5 | X-ray | Gladstone | Chandra | ~10 hours of HRC-I observations of Jupiter | 05/24/2018 00:01 - 05/24/2018 11:49 | publicly available after 1 year | Observations cancelled or unsuccessful | |||||
6 | FUV | Grodent | HST/STID | Jupiter northern FUV aurora | Visit 1O 05/22/2018 (18.142) from 16:17 to 17:04 Visit 1P 05/23/2018 (18.143) from 12:56 to 13:44 Visit 1Q 05/24/2018 (18.144) from 08:00 to 08:49 Visit 1S 05/24/2018 (18.144) from 09:36 to 10:24 | |||||||
7 | visible/NUV | Wong | HST/WFC3 UVIS | hi-resolution map of perijove track, single orbit snapshot | PJ13 | https://archive.stsci.edu/prepds/wfcj/ https://dx.doi.org/10.1016/j.icarus.2017.06.007 | ||||||
8 | visible/NUV | Simon | HST/WFC3 UVIS | Multiple-filtered imaging, 275-885 nm; global map pair (Outer Planet Atmospheric Legacy [OPAL] program) | opposition | https://archive.stsci.edu/prepds/opal/ | ||||||
9 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | Jan 15 to Jul 3, near continuous observations | Major Sodium outburst Jan -- Jun (Morgenthaler et al. 2019 ApJL) | ||||||
10 | Visible and Near IR (0.4-1.7 microns) | Sánchez-Lavega | Calar Alto / PlanetCam | Lucky-imaging high-resolution observations with star calibration | May 21-24 | Reduction of the data is complex and generally requires one to two weeks after the observations. | ||||||
11 | Visible and Near IR (0.4-1.7 microns) | Sánchez-Lavega | Calar Alto / PlanetCam | Lucky-imaging high-resolution observations with star calibration. Good data for the GRS sector in one night. Data for the rest of the planet is worse. | June 26-27 | Example shows a raw image from the automatic pipeline. Final images are generally much better but imply non-automatic image processing for the different filters and sequences. | ||||||
12 | CCD | Irwin/Braude | VLT/MUSE - IFU | spectroscopic imaging, 475-930 nm to determine cloud structure and albedo spectrum of particles. | May 25 | Raw data publicly available to download from ESO portal this time next year. Standard calibration pipeline takes of the order of 1-3 days to complete. Observation directly above GRS, a set of observations closer to PJ13 longitude was obtained on the 18th of May | ||||||
13 | CCD (Visible) | Dahl & Chanover | APO | Hyperspectral image cubes, 470-950 nm | May 23 and 24 | |||||||
14 | near IR | Kim | Gemini/N | group of observations / 3 micron CH4 aurora variability. | June 29 | obtained spectra of the north polar 8-micron hot spot and a standard star. | ||||||
15 | Near IR | Spencer | IRTF/SpeX | Io Eclipse and sunlit imaging | June 6 | Significant brightening of Loki since May 23, probably onset of typical months-long periodic brightening event | ||||||
16 | Near IR | Spencer | IRTF/SpeX | Io Eclipse and sunlit imaging | June 15, 22, 29, July 1 | Mostly Jupiter-facing hemisphere | ||||||
17 | near IR | Orton | IRTF/SpeX | filtered imaging at several wavelengths between 1.58 and 5.1µm and spectral scanning over 2-µm and 5-µm ranges | One 6-hour shift as close as possible to the perijove epoch and covering the perijove longitude. One 6-hour shift on the preceding or following date to cover complemenary longitudes. June 4,5,29,30. | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired. Reduced "quick-look" observations (geometrically but not radiometrically calibrated) will be available for immeduately use from the Juno-curated web site: http://junoirtf.space.swri.edu/ | ||||||
18 | near IR | Bjoraker | IRTF/iSHELL | 5-micron spectroscopy | May 25-26 UT | attached images at 5.1 and 1.58 mu at longitude of PJ13 | ||||||
19 | near IR | Orton | Gemini-N/NIRI | adaptive-optics-stabilized imaging of reflected sunlight | observations requested any time during this period | TBD | ||||||
20 | near IR (5 µm) | Wong | Gemini-N/NIRI | lucky imaging, 5-µm maps | 26 May UT (earliest NIRI availability) | |||||||
21 | mid IR | Fletcher | VLT / VISIR | filtered radiometric imaging to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology. full south/majority north polar map, addition of 5 N-band filters further constraining vertical NH3 profile | four half-nights of observations near perijove (full visitor mode) | available in raw form in the ESO archive within 24 hours of acquisition; cylindrical maps within 1-2 days and reduced maps within a week | ||||||
22 | mid IR | Kasaba, Orton (Keck exchange time and direct Subaru time | Subaru / COMICS | filtered radiometric imaging and spectroscopy to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology and auroral heating and chemistry. | Mid-infrared imaging and of Jupiter obtained during the first half of May 24 and the second half of May 25. | Kasaba would like to see agreement in place with Juno science team first and discussed at the workshop, but willing to share. Orton will share immediately. | ||||||
23 | submillimeter / millimeter | de Pater | Atacama Large Millimeter Array (ALMA) | Bands 5 and 6 | 16 May | Student thesis | ||||||
24 | radio | Zarka, Cecconi, Lamy, Louis | Nançay Decameter Array (France) | coordinated measurement of 10-40 MHz cyclotron radio emission | every day, 8 hours around the transition to local meridian | https://maser.lesia.obspm.fr/task-1-data-collections/juno-ground-radio/juno-ground-radio-nancay-decameter.html?lang=en | ||||||
25 | Scheduled observations by Juno. | |||||||||||
26 | ||||||||||||
27 | Perijove is 05/24/2018 5:39:50 UTC. System-III longitude = 24 W | |||||||||||
28 | ||||||||||||
29 | Period: Orbit 13 [GRAV] (2018 May 24 – 2018 July 15) | |||||||||||
30 | Instrument | Description | ||||||||||
31 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||||
32 | MWR | MWR will obtain oblique observations of Jupiter's atmosphere. Footprints of the lowest-emission-angle observations are shown below, with the perijove location shown by the cross. | ||||||||||
33 | UVS | |||||||||||
34 | JunoCam | |||||||||||
35 | JIRAM | |||||||||||
36 | ||||||||||||
37 | link to BAA report on PJ 13: | https://britastro.org/node/14425 | ||||||||||
38 | ||||||||||||
39 | ||||||||||||
40 | ||||||||||||
41 | ||||||||||||
42 | ||||||||||||
43 | ||||||||||||
44 | ||||||||||||
45 | ||||||||||||
46 | ||||||||||||
47 | ||||||||||||
48 | ||||||||||||
49 | ||||||||||||
50 | ||||||||||||
51 | ||||||||||||
52 | ||||||||||||
53 | ||||||||||||
54 | ||||||||||||
55 | ||||||||||||
56 | ||||||||||||
57 | ||||||||||||
58 | ||||||||||||
59 | ||||||||||||
60 | ||||||||||||
61 | ||||||||||||
62 | ||||||||||||
63 | ||||||||||||
64 | ||||||||||||
65 | ||||||||||||
66 | ||||||||||||
67 | ||||||||||||
68 | ||||||||||||
69 | ||||||||||||
70 | ||||||||||||
71 | ||||||||||||
72 | ||||||||||||
73 | MWR footprints for the minimum emission angle at each rotation of the spacecraft. Perijove position is marked by the cross. | |||||||||||
74 | ||||||||||||
75 | ||||||||||||
76 | ||||||||||||
77 | ||||||||||||
78 | ||||||||||||
79 | ||||||||||||
80 | ||||||||||||
81 | ||||||||||||
82 | ||||||||||||
83 | ||||||||||||
84 | ||||||||||||
85 | ||||||||||||
86 | ||||||||||||
87 | ||||||||||||
88 | ||||||||||||
89 | ||||||||||||
90 | ||||||||||||
91 | ||||||||||||
92 | ||||||||||||
93 | ||||||||||||
94 | ||||||||||||
95 | ||||||||||||
96 | ||||||||||||
97 | ||||||||||||
98 | ||||||||||||
99 | ||||||||||||
100 | ||||||||||||
101 | ||||||||||||
102 | ||||||||||||
103 | ||||||||||||
104 | ||||||||||||
105 | ||||||||||||
106 | ||||||||||||
107 | JIRAM fields of view | |||||||||||
108 | The dates reported (both in UTC and in hours from PJ) on the top are referred to the last acquisition with the M filter of the whole plan for the given JM | |||||||||||
109 | The # field, is the estimated number of the acquisition of the whole plan, | |||||||||||
110 | (Ignore the percentage field.) | |||||||||||
111 | The light blue area, enclosed by dark blue lines, represented the FoVs of Imager M projected on Jupiter. Dark blue areas that you can see in some positions are created | |||||||||||
112 | by more projected FoV overlapping at close distance; i.e. these zones are created by multi FoV edges ( dark blue lines) that plot each close to the other create these graphic artefacts | |||||||||||
113 | The background cloud rendition is for general orientation; the position of the Great Red Spot does not indicate its actual position during these observations. | |||||||||||
114 | ||||||||||||
115 | ||||||||||||
116 | ||||||||||||
117 | ||||||||||||
118 | Composite of JIRAM M-band (5-micron) map. | |||||||||||
119 | ||||||||||||
120 | ||||||||||||
121 | ||||||||||||
122 | ||||||||||||
123 | ||||||||||||
124 | ||||||||||||
125 | ||||||||||||
126 | ||||||||||||
127 | ||||||||||||
128 | ||||||||||||
129 | ||||||||||||
130 | ||||||||||||
131 | ||||||||||||
132 | ||||||||||||
133 | ||||||||||||
134 | ||||||||||||
135 | ||||||||||||
136 | ||||||||||||
137 | ||||||||||||
138 | ||||||||||||
139 | ||||||||||||
140 | ||||||||||||
141 | ||||||||||||
142 | ||||||||||||
143 | ||||||||||||
144 | Composite of JIRAM M-band (5-micron) map. | |||||||||||
145 | ||||||||||||
146 | ||||||||||||
147 | ||||||||||||
148 | ||||||||||||
149 | ||||||||||||
150 | ||||||||||||
151 | ||||||||||||
152 | ||||||||||||
153 | ||||||||||||
154 | ||||||||||||
155 | ||||||||||||
156 | ||||||||||||
157 | ||||||||||||
158 | ||||||||||||
159 | ||||||||||||
160 | ||||||||||||
161 | ||||||||||||
162 | ||||||||||||
163 | ||||||||||||
164 | ||||||||||||
165 | ||||||||||||
166 | ||||||||||||
167 | ||||||||||||
168 | ||||||||||||
169 | ||||||||||||
170 | ||||||||||||
171 | ||||||||||||
172 | ||||||||||||
173 | ||||||||||||
174 | ||||||||||||
175 | ||||||||||||
176 | ||||||||||||
177 | ||||||||||||
178 | ||||||||||||
179 | ||||||||||||
180 | ||||||||||||
181 | ||||||||||||
182 | ||||||||||||
183 |
1 | Note: On this orbit the spacecraft orientation is turned off Earth in order to optimize access to low emission-angle observations. | ||||||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
2 | |||||||||||||||||
3 | Period: Orbit 12 [MWR] (2018 March 31 – 2018 May 23) | Observations requested. | |||||||||||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | Observations planned / granted time | ||||||||||
5 | X-ray | Gladstone | Chandra | ~10 hours of HRC-I observations of Jupiter | 03/31/2018 23:12 - 04/01/2018 10:39 | publicly available after 1 year | Observations successful | ||||||||||
6 | X-ray | Kraft | Chandra | ~10 hours of HRC-I observations of Jupiter | 04/01/2018 10:39 - 04/01/2018 22:00 | publicly available after 1 year | Observations cancelled or unsuccessful | ||||||||||
7 | FUV | Schmidt | HST/COS | Io Spectroscopy | April 25 and May 17 | Publicly archived | |||||||||||
8 | CCD | Irwin/Braude | VLT/MUSE - IFU | spectroscopic imaging, 475-930 nm to determine cloud structure and albedo spectrum of particles. | April 9 | Raw data publicly available to download from ESO portal this time next year. Standard calibration pipeline takes of the order of 1-3 days to complete. Observation at PJ12 longitude, with GRS in view. | |||||||||||
9 | CCD | Irwin/Braude | VLT/MUSE - IFU | spectroscopic imaging, 475-930 nm to determine cloud structure and albedo spectrum of particles. | April 14 | Raw data publicly available to download from ESO portal this time next year. Standard calibration pipeline takes of the order of 1-3 days to complete. Two sets of observations, one with Oval BA at nadir and the other at 211W sub-observer longitude (III) | |||||||||||
10 | CCD | Irwin/Braude | VLT/MUSE - IFU | spectroscopic imaging, 475-930 nm to determine cloud structure and albedo spectrum of particles. | May 18 | Raw data publicly available to download from ESO portal this time next year. Standard calibration pipeline takes of the order of 1-3 days to complete. This observation was obtained at 52W central longitude (III) and was originally scheduled to coincide with PJ13 but was obtained a week early. | |||||||||||
11 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | Jan 15 to Jul 3, near continuous observations | Major Sodium outburst Jan -- Jun (Morgenthaler et al. 2019 ApJL) | |||||||||||
12 | visible/NUV | Wong | HST/WFC3 UVIS | hi-resolution map of PJ12 perijove track, global map pair | PJ | https://archive.stsci.edu/prepds/wfcj/ https://dx.doi.org/10.1016/j.icarus.2017.06.007 | |||||||||||
13 | CCD (Visible) | Dahl & Chanover | APO | Hyperspectral image cubes, 470-950 nm | March 31, April 1 | Mostly non-photometric; one cube at photometric conditions | |||||||||||
14 | Visible and Near IR (0.4-1.7 microns) | Sánchez-Lavega | Calar Alto / PlanetCam | Lucky-imaging high-resolution observations with star calibration | April 2-5 | Reduction of the data is complex and generally requires one to two weeks after the observations. | |||||||||||
15 | near IR | Bjoraker, de Pater | Keck/NIRSPEC | 5-micron spectra | March 31, April 3 No obervations were made due to weather and weather-related adverse conditions. | N/A | |||||||||||
16 | Near IR | Spencer | IRTF/SpeX | Io Eclipse and sunlit imaging | April 12, 19, 22, 23, 24, 26, May 5, 10, 12, 14, 21, 23 | Loki faint, bright eruption S of Pele May 10 | |||||||||||
17 | near IR | Kim | Gemini/N | group of obervations / 3 micron CH4 aurora variability | May 14 | we missed the north polar 8-micron hot spot and instead we obtained spectra of an equatorial region and a standard star. | |||||||||||
18 | near IR | Bjoraker, Momary | IRTF/SpeX | filtered imaging 1.58-5.1 microns | March 31 successful, April 3 clouded out | TBD | |||||||||||
19 | near IR | Orton | IRTF/SpeX | filtered imaging at several wavelengths between 1.58 and 5.1µm in ~45-min programs | April 7-8 clouded out. April 23-24 successful. | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired. Reduced "quick-look" observations (geometrically but not radiometrically calibrated) will be available for immeduately use from the Juno-curated web site: http://junoirtf.space.swri.edu/ | |||||||||||
20 | near IR | Orton | IRTF/SpeX | filtered imaging at several wavelengths between 1.58 and 5.1µm and spectral scanning over 2-µm, 4-µm and 5-µm ranges | May 11-12 scheduled. | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired. Reduced "quick-look" observations (geometrically but not radiometrically calibrated) will be available for immeduate use from the Juno-curated web site: http://junoirtf.space.swri.edu/ | |||||||||||
21 | near IR | Moore | Keck/NIRSPEC | auroral spectral scans near 2 µm, focused on constraining neutral and ion winds | 2nd half March 31 unsucessful due to dome closure; 1st half May 23 | TBD | |||||||||||
22 | near IR | Melin | IRTF/iSHELL | N polar mapping of H3+ emissions between 3-4 µm | ~10-14 UT on Apr 1; some context imaging as well as spectroscopy | ||||||||||||
23 | near IR | O'Donoghue | Keck/NIRSPEC | global mapping of H3+ emissions between 3-4 µm | ~7-14 UT on May 1; ~8-15 UT on May 2 | ||||||||||||
24 | near IR | O'Donoghue | IRTF/iShell | global mapping of H3+ emissions between 3-4 µm | 6, 7 & 8 May; Full nights (4-16 UT) | ||||||||||||
25 | Orton | Gemini-N/NIRI | adaptive-optics-stabilized imaging of reflected sunlight | no observations made due to weather | no observations were made due to persistent adverse weather conditions | ||||||||||||
26 | near IR (5 µm) | Wong | Gemini-N/NIRI | lucky imaging, 5-µm maps | Apr 1, contemporaneous with PJ12 covering the overflight track. May 2-3 scheduled. | ||||||||||||
27 | mid IR | Fletcher | VLT / VISIR | filtered radiometric imaging to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology. | Six hours of service time at perijove awarded. March 25: (UT08:03-09:33) 8-12μm spectra including Mband burst mode imaging CMLIII ~110 March 27: (UT08:16-09:05) Full imaging including Mband (std imaging) CMLIII ~45 (largely missed PJ longitudes) | available in raw form in the ESO archive within 24 hours of acquisition; cylindrical maps within 1-2 days and reduced maps within a week | |||||||||||
28 | mid IR | Kasaba, Orton | Subaru / COMICS | filtered radiometric imaging and spectroscopy to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology and auroral heating and chemistry. | Mid-infrared imaging of Jupiter on April 1, 10-14 UT including observations close to PJ12 epoch, covering the overflight track. Scheduled April 2 observations clouded out. | Kasaba would like to see agreement in place with Juno science team first and discussed at the workshop, but willing to share. | |||||||||||
29 | radio | Zarka, Cecconi, Lamy, Louis | Nançay Decameter Array (France) | coordinated measurement of 10-40 MHz cyclotron radio emission | every day, 8 hours around the transition to local meridian | https://maser.lesia.obspm.fr/task-1-data-collections/juno-ground-radio/juno-ground-radio-nancay-decameter.html?lang=en | |||||||||||
30 | radio | Imai | Long Wavelength Array 1 (LWA1) | Jupiter's decametric auroral radio observations | March 31-April 9 | Low-resolution LWA1 data are freely accessible via Autoplot (http://autoplot.org) by accepting the data usage policy (http://space.physics.uiowa.edu/earth/datapolicy.html) More information can be found at http://space.physics.uiowa.edu/earth/ | |||||||||||
31 | FUV | Grodent | HST/STIS | Jupiter northern FUV aurora. 1 orbit | April 1, 2018 10:16-10:57 | http://www.lpap.uliege.be/cms/c_4082676/en/hst-juno-orbit-12 | |||||||||||
32 | FUV | Grodent | HST/COS | Ganymede aurora spectroscopy. 2 orbits | April 4, 2018 14:31-16:48 | ||||||||||||
33 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | Jan 15 to Jul 3, near continuous observations | Major Sodium outburst Jan -- Jun (Morgenthaler et al. 2019 ApJL) | |||||||||||
34 | |||||||||||||||||
35 | |||||||||||||||||
36 | |||||||||||||||||
37 | Scheduled observations by Juno. | ||||||||||||||||
38 | |||||||||||||||||
39 | Perijove is 04/01/2018 09:45:43 UTC. System-III longitude = 114.6 W | ||||||||||||||||
40 | |||||||||||||||||
41 | Period: Orbit 12 [MWR XTk] (2018 April 1 – 2018 May 23) | ||||||||||||||||
42 | Instrument | Description | |||||||||||||||
43 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | |||||||||||||||
44 | MWR | MWR will obtain oblique observations of Jupiter's atmosphere. Footprints of the lowest-emission-angle observations are shown below; the perijove position is shown by the cross. | |||||||||||||||
45 | UVS | ||||||||||||||||
46 | JunoCam | JunoCam will obtain observations of the poles, with oblique observations at lower latitudes. | |||||||||||||||
47 | JIRAM | JIRAM will obtain images and spectra of polar regions. | |||||||||||||||
48 | |||||||||||||||||
49 | link to BAA report on PJ 12: | https://britastro.org/node/13011 | |||||||||||||||
50 | |||||||||||||||||
51 | |||||||||||||||||
52 | |||||||||||||||||
53 | |||||||||||||||||
54 | |||||||||||||||||
55 | |||||||||||||||||
56 | |||||||||||||||||
57 | |||||||||||||||||
58 | |||||||||||||||||
59 | |||||||||||||||||
60 | |||||||||||||||||
61 | |||||||||||||||||
62 | |||||||||||||||||
63 | |||||||||||||||||
64 | |||||||||||||||||
65 | |||||||||||||||||
66 | |||||||||||||||||
67 | |||||||||||||||||
68 | |||||||||||||||||
69 | |||||||||||||||||
70 | |||||||||||||||||
71 | |||||||||||||||||
72 | |||||||||||||||||
73 | |||||||||||||||||
74 | |||||||||||||||||
75 | |||||||||||||||||
76 | |||||||||||||||||
77 | |||||||||||||||||
78 | MWR map of footprints at the minimum emission angle at each spaceraft rotation. The periove position is given by the cross. | ||||||||||||||||
79 | |||||||||||||||||
80 | |||||||||||||||||
81 | |||||||||||||||||
82 | |||||||||||||||||
83 | |||||||||||||||||
84 | |||||||||||||||||
85 | |||||||||||||||||
86 | |||||||||||||||||
87 | |||||||||||||||||
88 | |||||||||||||||||
89 | |||||||||||||||||
90 | |||||||||||||||||
91 | |||||||||||||||||
92 | |||||||||||||||||
93 | |||||||||||||||||
94 | |||||||||||||||||
95 | |||||||||||||||||
96 | |||||||||||||||||
97 | |||||||||||||||||
98 | |||||||||||||||||
99 | |||||||||||||||||
100 | |||||||||||||||||
101 | |||||||||||||||||
102 | |||||||||||||||||
103 | |||||||||||||||||
104 | |||||||||||||||||
105 | |||||||||||||||||
106 | |||||||||||||||||
107 | |||||||||||||||||
108 | |||||||||||||||||
109 | |||||||||||||||||
110 | |||||||||||||||||
111 | |||||||||||||||||
112 | |||||||||||||||||
113 | |||||||||||||||||
114 | |||||||||||||||||
115 | |||||||||||||||||
116 | |||||||||||||||||
117 | |||||||||||||||||
118 | |||||||||||||||||
119 | |||||||||||||||||
120 | |||||||||||||||||
121 | |||||||||||||||||
122 | |||||||||||||||||
123 | |||||||||||||||||
124 | |||||||||||||||||
125 | |||||||||||||||||
126 | |||||||||||||||||
127 | |||||||||||||||||
128 | |||||||||||||||||
129 | |||||||||||||||||
130 | |||||||||||||||||
131 | JIRAM fields of view | ||||||||||||||||
132 | The dates reported (both in UTC and in hours from PJ) on the top are referred to the last acquisition with the M filter of the whole plan for the given JM | ||||||||||||||||
133 | The # field, is the estimated number of the acquisition of the whole plan, | ||||||||||||||||
134 | (Ignore the percentage field.) | ||||||||||||||||
135 | The light blue area, enclosed by dark blue lines, represented the FoVs of Imager M projected on Jupiter. Dark blue areas that you can see in some positions are created | ||||||||||||||||
136 | by more projected FoV overlapping at close distance; i.e. these zones are created by multi FoV edges ( dark blue lines) that plot each close to the other create these graphic artefacts | ||||||||||||||||
137 | The background cloud rendition is for general orientation; the position of the Great Red Spot does not indicate its actual position during these observations. | ||||||||||||||||
138 | |||||||||||||||||
139 | |||||||||||||||||
140 | |||||||||||||||||
141 | |||||||||||||||||
142 | |||||||||||||||||
143 | |||||||||||||||||
144 | |||||||||||||||||
145 | |||||||||||||||||
146 | |||||||||||||||||
147 | |||||||||||||||||
148 | |||||||||||||||||
149 | |||||||||||||||||
150 | |||||||||||||||||
151 | |||||||||||||||||
152 | |||||||||||||||||
153 | |||||||||||||||||
154 | |||||||||||||||||
155 | |||||||||||||||||
156 | |||||||||||||||||
157 | |||||||||||||||||
158 | |||||||||||||||||
159 | |||||||||||||||||
160 | |||||||||||||||||
161 | |||||||||||||||||
162 | |||||||||||||||||
163 | |||||||||||||||||
164 | |||||||||||||||||
165 | |||||||||||||||||
166 | |||||||||||||||||
167 | |||||||||||||||||
168 | |||||||||||||||||
169 | Composite of JIRAM M-band (5-micron) map. | ||||||||||||||||
170 | |||||||||||||||||
171 | |||||||||||||||||
172 | |||||||||||||||||
173 | |||||||||||||||||
174 | |||||||||||||||||
175 | |||||||||||||||||
176 | |||||||||||||||||
177 | |||||||||||||||||
178 | |||||||||||||||||
179 | |||||||||||||||||
180 | |||||||||||||||||
181 | |||||||||||||||||
182 | |||||||||||||||||
183 | |||||||||||||||||
184 | |||||||||||||||||
185 | |||||||||||||||||
186 | |||||||||||||||||
187 | |||||||||||||||||
188 | |||||||||||||||||
189 | |||||||||||||||||
190 | |||||||||||||||||
191 | |||||||||||||||||
192 | |||||||||||||||||
193 | |||||||||||||||||
194 | |||||||||||||||||
195 | |||||||||||||||||
196 | |||||||||||||||||
197 | |||||||||||||||||
198 | |||||||||||||||||
199 | |||||||||||||||||
200 | |||||||||||||||||
201 | |||||||||||||||||
202 | |||||||||||||||||
203 | |||||||||||||||||
204 | |||||||||||||||||
205 | |||||||||||||||||
206 | |||||||||||||||||
207 | |||||||||||||||||
208 | |||||||||||||||||
209 | |||||||||||||||||
210 | |||||||||||||||||
211 | |||||||||||||||||
212 | |||||||||||||||||
213 | |||||||||||||||||
214 | |||||||||||||||||
215 | |||||||||||||||||
216 | |||||||||||||||||
217 | |||||||||||||||||
218 | |||||||||||||||||
219 | |||||||||||||||||
220 | |||||||||||||||||
221 | |||||||||||||||||
222 | |||||||||||||||||
223 | |||||||||||||||||
224 | |||||||||||||||||
225 | |||||||||||||||||
226 | |||||||||||||||||
227 | |||||||||||||||||
228 | |||||||||||||||||
229 | |||||||||||||||||
230 | |||||||||||||||||
231 | |||||||||||||||||
232 | |||||||||||||||||
233 | |||||||||||||||||
234 | |||||||||||||||||
235 | |||||||||||||||||
236 | |||||||||||||||||
237 | |||||||||||||||||
238 | |||||||||||||||||
239 | |||||||||||||||||
240 | |||||||||||||||||
241 |
1 | Note: On this orbit the spacecraft orientation optimizes gravity mapping (GRAV) with the antenna pointed toward the Earth continuously. | Observations requested. | ||||||||
---|---|---|---|---|---|---|---|---|---|---|
2 | Observations planned / granted time | |||||||||
3 | Period: Orbit 11 [GRAV] (2018 February 7 – 2018 March 30) | Observations successful | ||||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | Observations cancelled or unsuccessful | |||
5 | visible/NUV | de Pater | HST/WFC3 UVIS | hi-resolution map of perijove track, single global map (4 orbits) | covering PJ longitude and VLA track on 2018-02-07 | |||||
6 | visible/NUV | Wong | HST/WFC3 UVIS | hi-resolution map of perijove track, single orbit snapshot | *2 rotations earlier than actual PJ pass* reason: HST observations precisely at PJ (see de Pater PI below) are gyro-only due to lunar separation of 5°. to offset risk, single orbit snapshot will be taken 2 orbits prior to perijove | https://archive.stsci.edu/prepds/wfcj/ https://dx.doi.org/10.1016/j.icarus.2017.06.007 | Caution: lunar separation angle of only ~5° (from earth) at time of perijove | |||
7 | Visible | Ates | TUG (Turkish National Observatory) / T100 | Lucky imaging, UBVRI | observations obtaind on March 23 at 11:50-02:23 UT and March 27 aat 00>09-02:01 UT | Processed and raw data will be forwarded to interested parties http://www.tug.tubitak.gov.tr/projeler/t100/t100_proje_tahsis.htm | ||||
8 | CCD (Visible) | Dahl & Chanover | APO | Hyperspectral image cubes, 470-950 nm | Feb 6-7 | observed both nights, conditions were non-photometric | ||||
9 | Visible | Schmidt | Perkins/RIPS | Io Spectroscopy | March 9-15 | Raw data March 14 only | ||||
10 | Visible | Schmidt | APO/DIS | Io Plasma Torus Spectroscopy | March 9, 20, 22, 27, 30 | Calibrated data available upon request March 9, 20, 22, and 30. | ||||
11 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | Jan 15 to Jul 3, near continuous observations | Major Sodium outburst Jan -- Jun (Morgenthaler et al. 2019 ApJL) | ||||
12 | Near IR | Schmidt | IRTF/iSHELL | Io Eclipse Spectroscopy | Feb 16 | Cloudy. No observations. | ||||
13 | Near IR | Spencer | IRTF/SpeX | Io Eclipse and sunlit imaging | March 18, 22 | No major volcanic activity | ||||
14 | near IR | Orton | IRTF/SpeX | filtered imaging at several wavelengths between 1.58 and 5.1µm and spectral scanning over 2-µm, 4-µm and 5-µm ranges | One 6-hour shift each on February 14 and 15 covering opposite hemispheres of Jupiter. Uncalibrated images were obtained on Feb 14 through small openings between clouds. Imaging and one stellar calibration, as well as a single calibrated 0.8-2.5 micron spectral scale were obtained on Feb 15 before high winds and fog forced closure. Observations during short shifts on Feb 24 and 25 were prevented by adverse weather. Observations scheduled on 6-hour shifts on March 25 and 26 were similarly cancelled due to snowstorm preventing access to the IRTF. | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired. Reduced "quick-look" observations (geometrically but not radiometrically calibrated) will be available for immeduately use from the Juno-curated web site: http://junoirtf.space.swri.edu/ | ||||
15 | near IR | Moore | Keck/NIRSPEC | auroral spectral scans near 2 µm, focused on constraining neutral and ion winds | 2nd half Feb 5, March 31; 1st half May 23 | March 31 weathered out | ||||
16 | near IR | Orton | Gemini-N/NIRI | adaptive-optics-stabilized imaging of reflected sunlight | no observations made due to weather | no observations were made due to persistent adverse weather conditions | ||||
17 | near IR (5 µm) | Wong | Gemini-N/NIRI | lucky imaging, 5-µm maps | 9 Feb UT (earliest NIRI availability) | no observations were made due to weather conditions | ||||
18 | near IR | de Pater,Bjoraker | Keck/NIRSPEC | Keck/NIRSPEC; 5-micron spectrospcopy | Feb 6-7 | lost both nights to snow | ||||
19 | near IR | Kim | Gemini/N | observe 3 micron CH4 aurora variability. | March 15 | Using this offset method, on March 15, we obtained good 3-micron data on the 8-micron hot spot and a standard star, and these data are now under data reduction/calibration. | ||||
20 | mid IR | Fletcher | VLT / VISIR | filtered radiometric imaging to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology. | Six hours of service time at perijove awarded. | No observations were made as a result of weather conditions near perijove. One high-resolution M-band image was obtained on Feb 19. | ||||
21 | mid IR | Sinclair | IRTF / TEXES | Emission spectra of CH4, C2H2, C2H4, C2H6 and H2 S(1) measured at Jupiter's high latitudes | Measurements taken on February 9 12:30 - 19:30 and February 11 12:30 - 14:40 UT | Reduced, calibrated spectra and retrieved temperature maps avaiable from Sinclair upon request. | ||||
22 | radio | de Pater | VLA | microwave synthetic imaging in Ku and X bands, probably in a mixed A and B configuration | 8h on 2/7/2018 | |||||
23 | radio | Ries | DSN/GAVRT | unresolved continuum observations at 2.245 GHz (mostly S-Band) | 2018-02: 7,8,26,27,28; 2018-03: 1,2,6,13,14, 15, 16, 19, 22, 23, 27,28, 29, 30 | Calibrated data available from Ries upon request | ||||
24 | radio | Zarka, Cecconi, Lamy, Louis | Nançay Decameter Array (France) | coordinated measurement of 10-40 MHz cyclotron radio emission | every day, 8 hours around the transition to local meridian | https://maser.lesia.obspm.fr/task-1-data-collections/juno-ground-radio/juno-ground-radio-nancay-decameter.html?lang=en | ||||
25 | radio | Imai | Long Wavelength Array 1 (LWA1) | Jupiter's decametric auroral radio observations | February 7-12 | Low-resolution LWA1 data are freely accessible via Autoplot (http://autoplot.org) by accepting the data usage policy (http://space.physics.uiowa.edu/earth/datapolicy.html) More information can be found at http://space.physics.uiowa.edu/earth/ | ||||
26 | ||||||||||
27 | ||||||||||
28 | Scheduled observations by Juno. | |||||||||
29 | ||||||||||
30 | Perijove is 02/07/2018 13:51:30 UTC. System-III longitude = 205.1 W | |||||||||
31 | ||||||||||
32 | Period: Orbit 11 [GRAV] (2018 February 7 – 2018 March 31) | |||||||||
33 | Instrument | Description | ||||||||
34 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||
35 | MWR | |||||||||
36 | UVS | |||||||||
37 | JunoCam | |||||||||
38 | JIRAM | |||||||||
39 | ||||||||||
40 | ||||||||||
41 | link to BAA report on PJ 11: | https://britastro.org/node/12580 | ||||||||
42 | ||||||||||
43 | ||||||||||
44 | ||||||||||
45 | ||||||||||
46 | ||||||||||
47 | ||||||||||
48 | ||||||||||
49 | ||||||||||
50 | ||||||||||
51 | ||||||||||
52 | ||||||||||
53 | ||||||||||
54 | ||||||||||
55 | ||||||||||
56 | ||||||||||
57 | ||||||||||
58 | ||||||||||
59 | ||||||||||
60 | ||||||||||
61 | ||||||||||
62 | ||||||||||
63 | ||||||||||
64 | ||||||||||
65 | ||||||||||
66 | ||||||||||
67 | ||||||||||
68 | ||||||||||
69 | ||||||||||
70 | ||||||||||
71 | MWR footprints for the minimum emission angle at each latitude. | |||||||||
72 | ||||||||||
73 | ||||||||||
74 | ||||||||||
75 | ||||||||||
76 | ||||||||||
77 | ||||||||||
78 | ||||||||||
79 | ||||||||||
80 | ||||||||||
81 | ||||||||||
82 | ||||||||||
83 | ||||||||||
84 | ||||||||||
85 | ||||||||||
86 | ||||||||||
87 | ||||||||||
88 | ||||||||||
89 | ||||||||||
90 | ||||||||||
91 | ||||||||||
92 | ||||||||||
93 | ||||||||||
94 | ||||||||||
95 | ||||||||||
96 | ||||||||||
97 | ||||||||||
98 | ||||||||||
99 | ||||||||||
100 | ||||||||||
101 | ||||||||||
102 | ||||||||||
103 | ||||||||||
104 | JIRAM fields of view | |||||||||
105 | The dates reported (both in UTC and in hours from PJ) on the top are referred to the last acquisition with the M filter of the whole plan for the given JM | |||||||||
106 | The # field, is the estimated number of the acquisition of the whole plan, | |||||||||
107 | (Ignore the percentage field.) | |||||||||
108 | The light blue area, enclosed by dark blue lines, represented the FoVs of Imager M projected on Jupiter. Dark blue areas that you can see in some positions are created | |||||||||
109 | by more projected FoV overlapping at close distance; i.e. these zones are created by multi FoV edges ( dark blue lines) that plot each close to the other create these graphic artefacts | |||||||||
110 | The background cloud rendition is for general orientation; the position of the Great Red Spot does not indicate its actual position during these observations. | |||||||||
111 | ||||||||||
112 | ||||||||||
113 | ||||||||||
114 | ||||||||||
115 | ||||||||||
116 | ||||||||||
117 | ||||||||||
118 | ||||||||||
119 | ||||||||||
120 | ||||||||||
121 | ||||||||||
122 | ||||||||||
123 | ||||||||||
124 | ||||||||||
125 | ||||||||||
126 | ||||||||||
127 | ||||||||||
128 | ||||||||||
129 | ||||||||||
130 | ||||||||||
131 | ||||||||||
132 | ||||||||||
133 | ||||||||||
134 | ||||||||||
135 | ||||||||||
136 | ||||||||||
137 | ||||||||||
138 | ||||||||||
139 | ||||||||||
140 | Composite of JIRAM M-band (5-micron) map. | |||||||||
141 | ||||||||||
142 | ||||||||||
143 | ||||||||||
144 | ||||||||||
145 | ||||||||||
146 | ||||||||||
147 | ||||||||||
148 | ||||||||||
149 | ||||||||||
150 | ||||||||||
151 | ||||||||||
152 | ||||||||||
153 | ||||||||||
154 | ||||||||||
155 | ||||||||||
156 | ||||||||||
157 | ||||||||||
158 | ||||||||||
159 | ||||||||||
160 | ||||||||||
161 | ||||||||||
162 | ||||||||||
163 | ||||||||||
164 | ||||||||||
165 | ||||||||||
166 | ||||||||||
167 | ||||||||||
168 | ||||||||||
169 | ||||||||||
170 | ||||||||||
171 | ||||||||||
172 | ||||||||||
173 | ||||||||||
174 | ||||||||||
175 | ||||||||||
176 | ||||||||||
177 | ||||||||||
178 | ||||||||||
179 | ||||||||||
180 |
1 | Note: On this orbit the spacecraft orientation optimizes gravity mapping (GRAV) with the antenna pointed toward the Earth continuously. | ||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|
2 | Observations requested. | ||||||||||
3 | Period: Orbit 10 [GRAV] (2017 December 16 – 2018 February 6) | Observations planned / granted time | |||||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | Observations successful | ||||
5 | FUV | Grodent | HST-FUV/MAMA | high spatial and temporal resolution FUV observations of magnetosphere and ultraviolet auroras. Current sheet crossings 30-40 RJ | Feb 4 14:28-15:17 (northern aurora) Feb 5 20:40-21:28 (northern aurora) Feb 6 15:44-16:32 (northern aurora) | http://www.stsci.edu/hst/confirm-charts/14634/ | Observations cancelled or unsuccessful | ||||
6 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | Jan 15 to Jul 3, near continuous observations | Major Sodium outburst Jan -- Jun (Morgenthaler et al. 2019 ApJL) | |||||
7 | Near IR | Spencer | IRTF/SpeX | Io Eclipse and sunlit imaging | Dec 16, 30, Jan 3, 6, 8, 13, 15 | No major volcanic activity. Loki faint | |||||
8 | near IR | Orton | IRTF/SpeX | filtered imaging at several wavelengths between 1.58 and 5.1µm and spectral scanning over 2-µm and 5-µm ranges | Dec 17-18, 06:30-13:00 HST. All observations weathered out. | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired. Reduced "quick-look" observations (geometrically but not radiometrically calibrated) will be available for immeduately use from the Juno-curated web site: http://junoirtf.space.swri.edu/ | |||||
9 | near IR | Orton | IRTF/iSHELL | filtered imaging at several wavelengths between 1.58 and 5.1µm, nominally in service time | 45-minute intervals on Jan 7, 8; 14, 15. Jan 7-8 observations were very successful with 0.5-0.6" seeing but no time for stellar calibration. Other dates were weathered out. SpeX was not available, so the guide camera for iSHELL was used. | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired. Reduced "quick-look" observations (geometrically but not radiometrically calibrated) will be available for immeduately use from the Juno-curated web site: http://junoirtf.space.swri.edu/ | |||||
10 | near IR | Spencer | IRTF/Spex | filtered imaging of Io at several wavelengths | Dec 22 5:35-6:20 HST, Dec 23 7:20-8:50, Dec 27 5:20-6:05 | TBD | |||||
11 | near IR | Moore | Keck/NIRSPEC | auroral spectral scans near 2 µm, focused on constraining neutral and ion winds | 2nd half Feb 5, March 31; 1st half May 23 | Feb 5 weathered out | |||||
12 | radio | de Pater | VLA | Ku and X bands | 8h on 16 Dec, 2017 | student thesis | |||||
13 | radio | Kita | GMRT | L-band | 16 Dec / 07:00-13:00 (IST) 17 Dec / 07:00-13:00 (IST) | reduced data will be available upon request | |||||
14 | radio | Zarka, Cecconi, Lamy, Louis | Nançay Decameter Array (France) | coordinated measurement of 10-40 MHz cyclotron radio emission | every day, 8 hours around the transition to local meridian | https://maser.lesia.obspm.fr/task-1-data-collections/juno-ground-radio/juno-ground-radio-nancay-decameter.html?lang=en | |||||
15 | radio | Imai | Long Wavelength Array 1 (LWA1) | Jupiter's decametric auroral radio observations | December 16-20 February 2-6 | Low-resolution LWA1 data are freely accessible via Autoplot (http://autoplot.org) by accepting the data usage policy (http://space.physics.uiowa.edu/earth/datapolicy.html) More information can be found at http://space.physics.uiowa.edu/earth/ | |||||
16 | radio | Ryabov / Zakharenko | UTR-2 (Ukraine) GURT (Ukraine) | Decametric emissions Spectrograms (8-33 MHz) Waveforms (8-33 MHz) Spectrograms (8-80 MHz) | December (16)-(17) 4:50(16)-10:00(16) UTC 4:59(17)-10:00(17) UTC 4:50(16)-6:30(16) UTC 3:45(16)-11:01(16) UTC 2:30(17)-10:55(17) UTC | The data will be available upon request to V. Ryabov. | |||||
17 | |||||||||||
18 | Scheduled observations by Juno. | ||||||||||
19 | |||||||||||
20 | Perijove is 12/16/2017 17:56:59 UTC. System-III longitude = 295.3 W | ||||||||||
21 | |||||||||||
22 | Period: Orbit 10 [GRAV] (2017 December 16 – 2018 February 6) | ||||||||||
23 | Instrument | Description | |||||||||
24 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | |||||||||
25 | MWR | ||||||||||
26 | UVS | ||||||||||
27 | JunoCam | ||||||||||
28 | JIRAM | ||||||||||
29 | |||||||||||
30 | |||||||||||
31 | |||||||||||
32 | |||||||||||
33 | |||||||||||
34 | |||||||||||
35 | |||||||||||
36 | |||||||||||
37 | |||||||||||
38 | |||||||||||
39 | |||||||||||
40 | |||||||||||
41 | |||||||||||
42 | |||||||||||
43 | |||||||||||
44 | |||||||||||
45 | |||||||||||
46 | |||||||||||
47 | |||||||||||
48 | |||||||||||
49 | |||||||||||
50 | |||||||||||
51 | |||||||||||
52 | |||||||||||
53 | |||||||||||
54 | |||||||||||
55 | |||||||||||
56 | |||||||||||
57 | MWR footprints for the minimum emission angle at each latitude. | ||||||||||
58 | |||||||||||
59 | |||||||||||
60 | |||||||||||
61 | |||||||||||
62 | |||||||||||
63 | |||||||||||
64 | |||||||||||
65 | |||||||||||
66 | |||||||||||
67 | |||||||||||
68 | |||||||||||
69 | |||||||||||
70 | |||||||||||
71 | |||||||||||
72 | |||||||||||
73 | |||||||||||
74 | |||||||||||
75 | |||||||||||
76 | |||||||||||
77 | |||||||||||
78 | |||||||||||
79 | |||||||||||
80 | |||||||||||
81 | |||||||||||
82 | |||||||||||
83 | |||||||||||
84 | |||||||||||
85 | |||||||||||
86 | |||||||||||
87 | |||||||||||
88 | |||||||||||
89 | JIRAM fields of view | ||||||||||
90 | The dates reported (both in UTC and in hours from PJ) on the top are referred to the last acquisition with the M filter of the whole plan for the given JM | ||||||||||
91 | The # field, is the estimated number of the acquisition of the whole plan, | ||||||||||
92 | (Ignore the percentage field.) | ||||||||||
93 | The light blue area, enclosed by dark blue lines, represented the FoVs of Imager M projected on Jupiter. Dark blue areas that you can see in some positions are created | ||||||||||
94 | by more projected FoV overlapping at close distance; i.e. these zones are created by multi FoV edges ( dark blue lines) that plot each close to the other create these graphic artefacts | ||||||||||
95 | The background cloud rendition is for general orientation; the position of the Great Red Spot does not indicate its actual position during these observations. | ||||||||||
96 | |||||||||||
97 | |||||||||||
98 | |||||||||||
99 | |||||||||||
100 | |||||||||||
101 | |||||||||||
102 | |||||||||||
103 | |||||||||||
104 | |||||||||||
105 | |||||||||||
106 | |||||||||||
107 | |||||||||||
108 | |||||||||||
109 | |||||||||||
110 | |||||||||||
111 | |||||||||||
112 | |||||||||||
113 | |||||||||||
114 | |||||||||||
115 | |||||||||||
116 | |||||||||||
117 | |||||||||||
118 | |||||||||||
119 | |||||||||||
120 | |||||||||||
121 | |||||||||||
122 | |||||||||||
123 | |||||||||||
124 | |||||||||||
125 | Composite of JIRAM M-band (5-micron) map. | ||||||||||
126 | |||||||||||
127 | |||||||||||
128 | |||||||||||
129 | |||||||||||
130 | |||||||||||
131 | |||||||||||
132 | |||||||||||
133 | |||||||||||
134 | |||||||||||
135 | |||||||||||
136 | |||||||||||
137 | |||||||||||
138 | |||||||||||
139 | |||||||||||
140 | |||||||||||
141 | |||||||||||
142 | |||||||||||
143 | |||||||||||
144 | |||||||||||
145 | |||||||||||
146 | |||||||||||
147 | |||||||||||
148 | |||||||||||
149 | |||||||||||
150 | |||||||||||
151 | |||||||||||
152 | |||||||||||
153 | |||||||||||
154 | |||||||||||
155 | |||||||||||
156 | |||||||||||
157 | |||||||||||
158 | |||||||||||
159 | |||||||||||
160 | |||||||||||
161 | |||||||||||
162 | |||||||||||
163 | |||||||||||
164 | |||||||||||
165 |
1 | Note: On this orbit the spacecraft orientation optimizes MWR sensing with the antenna pointed to achieve nadir or near-nadir observations and the spacecraft is tilted to optimize the MWR getting coincident fields of view over all channels. At perijove, Jupiter is 2 degrees from the Sun. Few, if any, Earth-based observations are anticipated. | ||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|
2 | No Earth-based observations are expected near perijove, when Jupiter is only 2 degrees from the sun. | ||||||||||
3 | Period: Orbit 9 [MWR tilt] (2017 October 23 – 2017 December 15) | ||||||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | |||||
5 | radio | Zarka, Cecconi, Lamy, Louis | Nançay Decameter Array (France) | coordinated measurement of 10-40 MHz cyclotron radio emission | every day, 8 hours around the transition to local meridian | https://maser.lesia.obspm.fr/task-1-data-collections/juno-ground-radio/juno-ground-radio-nancay-decameter.html?lang=en | |||||
6 | radio | Imai | Long Wavelength Array 1 (LWA1) | Jupiter's decametric auroral radio observations | December 12-15 | Low-resolution LWA1 data are freely accessible via Autoplot (http://autoplot.org) by accepting the data usage policy (http://space.physics.uiowa.edu/earth/datapolicy.html) More information can be found at http://space.physics.uiowa.edu/earth/ | |||||
7 | radio | Ryabov / Zakharenko | UTR-2 (Ukraine) GURT (Ukraine) | Decametric emissions Spectrograms (8-33 MHz) Spectrograms (8-80 MHz) | October (24)-(25) 5:20(24)-13:09(24) UTC 5:30(25)-13:37(25) UTC 5:14(24)-11:47(24) UTC | The data will be available upon request to V. Ryabov. | |||||
8 | Observations requested. | ||||||||||
9 | Observations planned / granted time | ||||||||||
10 | Observations successful | ||||||||||
11 | Observations cancelled or unsuccessful | ||||||||||
12 | |||||||||||
13 | |||||||||||
14 | |||||||||||
15 | |||||||||||
16 | Scheduled observations by Juno. | ||||||||||
17 | |||||||||||
18 | Perijove is 2017 October 24, 17:42:31 UTC. System-III longitude = 228.4°W | ||||||||||
19 | |||||||||||
20 | Period: Orbit 9 [MWR tilt] (2017 October 23 – 2017 December 15) | ||||||||||
21 | Instrument | Description | |||||||||
22 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | |||||||||
23 | MWR | ||||||||||
24 | UVS | ||||||||||
25 | JunoCam | ||||||||||
26 | JIRAM | ||||||||||
27 | |||||||||||
28 | |||||||||||
29 | |||||||||||
30 | |||||||||||
31 | |||||||||||
32 | |||||||||||
33 | |||||||||||
34 | |||||||||||
35 | |||||||||||
36 | |||||||||||
37 | |||||||||||
38 | |||||||||||
39 | |||||||||||
40 | |||||||||||
41 | |||||||||||
42 | |||||||||||
43 | |||||||||||
44 | |||||||||||
45 | |||||||||||
46 | |||||||||||
47 | |||||||||||
48 | |||||||||||
49 | |||||||||||
50 | |||||||||||
51 | |||||||||||
52 | |||||||||||
53 | |||||||||||
54 | |||||||||||
55 | MWR footprints for the minimum emission angle at each rotation of the spacecraft. The perijove position is given by the cross. | ||||||||||
56 | |||||||||||
57 | |||||||||||
58 | |||||||||||
59 | |||||||||||
60 | |||||||||||
61 | |||||||||||
62 | |||||||||||
63 | |||||||||||
64 | |||||||||||
65 | |||||||||||
66 | |||||||||||
67 | |||||||||||
68 | |||||||||||
69 | |||||||||||
70 | |||||||||||
71 | |||||||||||
72 | |||||||||||
73 | |||||||||||
74 | |||||||||||
75 | |||||||||||
76 | |||||||||||
77 | |||||||||||
78 | |||||||||||
79 | |||||||||||
80 | |||||||||||
81 | |||||||||||
82 | |||||||||||
83 | |||||||||||
84 | |||||||||||
85 | |||||||||||
86 | Composite of JIRAM M-band (5-micron) map. | ||||||||||
87 | |||||||||||
88 | |||||||||||
89 | |||||||||||
90 | |||||||||||
91 | |||||||||||
92 | |||||||||||
93 | |||||||||||
94 | |||||||||||
95 | |||||||||||
96 | |||||||||||
97 | |||||||||||
98 | |||||||||||
99 | |||||||||||
100 | |||||||||||
101 | |||||||||||
102 | |||||||||||
103 | |||||||||||
104 | |||||||||||
105 | |||||||||||
106 | |||||||||||
107 | |||||||||||
108 | |||||||||||
109 | |||||||||||
110 | |||||||||||
111 | |||||||||||
112 | |||||||||||
113 | |||||||||||
114 | |||||||||||
115 | |||||||||||
116 | |||||||||||
117 | |||||||||||
118 | |||||||||||
119 | |||||||||||
120 | |||||||||||
121 | |||||||||||
122 | |||||||||||
123 | |||||||||||
124 | |||||||||||
125 | |||||||||||
126 |
1 | Note: On this orbit the spacecraft orientation optimizes gravity mapping (GRAV) with the antenna pointed toward the Earth continuously. | Observations requested. | |||||||||
---|---|---|---|---|---|---|---|---|---|---|---|
2 | Observations planned / granted time | ||||||||||
3 | Period: Orbit 8 [GRAV] (2017 August 30 – 2017 October 22) | Observations successful | |||||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | Observations cancelled or unsuccessful | ||||
5 | Hard X-ray | Mori | NuSTAR | Approved GO program. Hard X-ray (>2 keV) coverage. | 130 ks covering the September 1 Perijove. Likely will match the XMM observations. | ||||||
6 | near IR | Orton | IRTF/SpeX guide camera | filtered imaging at several near-infrared wavelengths, including H3+ emission at 3.14µm and thermal emission at 5.1 µm. | Two 8-hour runs on Sept 2 and 3, during dayime hours, 10:30-18:30 HST (20:30-4:30 UTC). Observations were made but had predominantly poor seeing for the first several hours. Except for the beginning of Sep 3, weather was photometric. Seeing was better toward the end of the run, and we managed to get scanned spectroscopic observations completed each night. Short observations were also obtained at the beginning of runs scheduled for Cassini-supporting Saturn observations Sept 9 and 10, starting at 15:30 HST; these also had moderate seeing conditions at best, being in late-afternoon daylight. | raw images available immediately from IRTF web site. Reduced "quick-look" observations (geometrically but not radiometrically calibrated) will be available for immeduately use from the Juno-curated web site: http://junoirtf.space.swri.edu/ | |||||
7 | mid IR | Sinclair, Orton | Subaru / COMICS | filtered radiometric imaging and spectroscopy to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology and auroral heating and chemistry. | Mid-infrared imaging of Jupiter on September 6 and 7 UTC (Sinclair, Subaru Keck-exchange time), early observations during a run mostly dedicated to Saturn imaging and spectroscopy. Images at high airmass, seeing 1" or worse, but 7.8, 8.7, 10.3, 17.8, 18.7, 20.3, 24.5 microns. Observations of the PJ8 longitude near the central meridian were made on September 7. | Data can be shareed immediately with collaborative partners. | |||||
8 | radio | Zarka, Cecconi, Lamy, Louis | Nançay Decameter Array (France) | coordinated measurement of 10-40 MHz cyclotron radio emission | every day, 8 hours around the transition to local meridian | https://maser.lesia.obspm.fr/task-1-data-collections/juno-ground-radio/juno-ground-radio-nancay-decameter.html?lang=en | |||||
9 | radio | Imai | Long Wavelength Array 1 (LWA1) | Jupiter's decametric auroral radio observations | August 30 September 1-7 | Low-resolution LWA1 data are freely accessible via Autoplot (http://autoplot.org) by accepting the data usage policy (http://space.physics.uiowa.edu/earth/datapolicy.html) More information can be found at http://space.physics.uiowa.edu/earth/ | |||||
10 | radio | Ryabov / Zakharenko | UTR-2 (Ukraine) GURT (Ukraine) URAN2 (Ukraine) | Decametric emissions Spectrograms (8-33 MHz) Waveforms (8-33 MHz) Spectrograms (8-80 MHz) Spectrograms (8-33 MHz) | September (1)-(2) 9:00(1)-16:00(1) UTC 9:00(2)-15:55(2) UTC 10:25(1)-10:45(1) UTC 13:30(2)-15:55(2) UTC 14:00(1)-20:00(1) UTC 10:00(2)-16:00(2) UTC 8:55(1)-16:00(1) UTC 8:55(2)-13:00(2) UTC 13:30(2)-16:00(2) UTC | The data will be available upon request to V. Ryabov. Time resolution 10 ms Time resolution 10 ms Time resolution 2 ms | |||||
11 | |||||||||||
12 | Scheduled observations by Juno. | ||||||||||
13 | |||||||||||
14 | Perijove is 2017 September 1, 21:48:50 UTC. System-III longitude = 319°W | ||||||||||
15 | Instrument | Description | |||||||||
16 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | |||||||||
17 | MWR | N/S scans near perijove longitude, not centered on nadir. The figure below shows footprints at MWR's minimum emission angles. | |||||||||
18 | UVS | TBD | |||||||||
19 | JunoCam | E/PO observations targeting features voted on by public. | |||||||||
20 | JIRAM | TBD | |||||||||
21 | |||||||||||
22 | |||||||||||
23 | |||||||||||
24 | |||||||||||
25 | |||||||||||
26 | |||||||||||
27 | |||||||||||
28 | |||||||||||
29 | |||||||||||
30 | |||||||||||
31 | |||||||||||
32 | |||||||||||
33 | |||||||||||
34 | |||||||||||
35 | |||||||||||
36 | |||||||||||
37 | |||||||||||
38 | |||||||||||
39 | |||||||||||
40 | |||||||||||
41 | |||||||||||
42 | |||||||||||
43 | |||||||||||
44 | |||||||||||
45 | |||||||||||
46 | MWR footprints for the minimum emission angle at each latitude. | ||||||||||
47 | |||||||||||
48 | |||||||||||
49 | |||||||||||
50 | |||||||||||
51 | |||||||||||
52 | |||||||||||
53 | |||||||||||
54 | |||||||||||
55 | |||||||||||
56 | |||||||||||
57 | |||||||||||
58 | |||||||||||
59 | |||||||||||
60 | |||||||||||
61 | |||||||||||
62 | |||||||||||
63 | |||||||||||
64 | |||||||||||
65 | |||||||||||
66 | |||||||||||
67 | |||||||||||
68 | |||||||||||
69 | |||||||||||
70 | |||||||||||
71 | |||||||||||
72 | |||||||||||
73 | |||||||||||
74 | |||||||||||
75 | |||||||||||
76 | |||||||||||
77 | |||||||||||
78 | |||||||||||
79 | |||||||||||
80 | |||||||||||
81 | |||||||||||
82 | |||||||||||
83 | |||||||||||
84 | |||||||||||
85 | |||||||||||
86 | |||||||||||
87 | |||||||||||
88 | |||||||||||
89 | |||||||||||
90 | |||||||||||
91 | |||||||||||
92 | |||||||||||
93 | |||||||||||
94 | |||||||||||
95 | |||||||||||
96 | |||||||||||
97 | |||||||||||
98 | |||||||||||
99 | |||||||||||
100 | |||||||||||
101 | |||||||||||
102 | |||||||||||
103 | |||||||||||
104 | |||||||||||
105 | |||||||||||
106 | |||||||||||
107 | |||||||||||
108 | |||||||||||
109 | |||||||||||
110 | |||||||||||
111 | |||||||||||
112 | |||||||||||
113 | |||||||||||
114 | |||||||||||
115 | |||||||||||
116 | |||||||||||
117 | |||||||||||
118 | |||||||||||
119 | |||||||||||
120 | |||||||||||
121 | Composite of JIRAM M-band (5-micron) map. | ||||||||||
122 | |||||||||||
123 | |||||||||||
124 | |||||||||||
125 | |||||||||||
126 | |||||||||||
127 | |||||||||||
128 | |||||||||||
129 | |||||||||||
130 | |||||||||||
131 | |||||||||||
132 | |||||||||||
133 | |||||||||||
134 | |||||||||||
135 | |||||||||||
136 | |||||||||||
137 | |||||||||||
138 | |||||||||||
139 | |||||||||||
140 | |||||||||||
141 | |||||||||||
142 | |||||||||||
143 | |||||||||||
144 | |||||||||||
145 | |||||||||||
146 | |||||||||||
147 | |||||||||||
148 | |||||||||||
149 | |||||||||||
150 | |||||||||||
151 | |||||||||||
152 | |||||||||||
153 | |||||||||||
154 | |||||||||||
155 | |||||||||||
156 | |||||||||||
157 | |||||||||||
158 | |||||||||||
159 | |||||||||||
160 | |||||||||||
161 | |||||||||||
162 |
1 | Note: On this orbit the spacecraft orientation optimizes MWR sensing with the antenna pointed to achieve nadir or near-nadir observations. An overflight was made through the center of the Great Red Spot. | |||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
2 | Observations requested. | |||||||||||||
3 | Period: Orbit 7 [MWR tilt] (2017 July 10 – 2017 August 30) | Observations planned / granted time | ||||||||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | Observations successful | |||||||
5 | Hard X-ray | Mori | NuSTAR | Approved GO program. Hard X-ray (>2 keV) coverage. | 2017-Jul-10 to 2017-Jul-12. | Observations cancelled or unsuccessful | ||||||||
6 | X-ray | Caitriona Jackman | Chandra | 36 ks (10 hours) continuous observation by Chandra near apojove | Start 2017:218:02:08:23.288 August 6th 2017 36 ks (10-hour) observation with Chandra. No overlap with any other remote campaigns and alignment with Juno activities will be a priority. Visibility was heavily skewed toward the north, with few counts from the southern pole. | Request to Jackman. Keen to collaborate with Juno team as contemporaneous in situ data will help to constrain the X-ray drivers thought to map to this region | ||||||||
7 | X-ray | Dunn | XMM-Newton | 40 hours of continuous spatial, spectral and temporal resolution on PJ 7, 30 hours on 16-17 July | 2017-07-10 18:49:10 -- 2017-07-10 18:49:10, 2017-07-16 18:26:32 -- 2017-07-17 22:13:08, 2017-06-18 19:45:25 -- 2017-06-19 23:48:45 | |||||||||
8 | X-ray | Gladstone | Chandra | ~10 hours of HRC-I observations of Jupiter | 07/10/2017 21:12 - 07/11/2017 09:00 | publicly available after 1 year | ||||||||
9 | FUV | Grodent | HST/FUV-MAMA | high spatial and temporal resolution FUV observations of magnetosphere and ultraviolet auroras | 2017-07-08 05:13:19 to 2017-07-08 05:54:43 2017-07-09 01:50:36 to 2017-07-09 02:32:00 2017-07-10 23:55:23 to 2017-07-11 00:36:47 2017-07-11 06:32:07 to 2017-07-11 06:58:55 2017-07-11 01:31:19 to 2017-07-11 02:12:43 2017-07-11 07:52:45 to 2017-07-11 08:34:09 2017-07-11 23:46:17 to 2017-07-12 00:27:41 2017-07-11 06:15:04 to 2017-07-11 06:19:33 2017-07-13 21:51:32 to 2017-07-13 22:32:56 2017-07-14 01:02:15 to 2017-07-14 01:43:39 2017-07-14 05:48:18 to 2017-07-14 06:29:42 2017-07-14 07:23:40 to 2017-07-14 08:05:04 2017-07-15 00:52:33 to 2017-07-15 01:33:57 2017-07-15 02:27:54 to 2017-07-15 03:09:18 2017-07-15 04:03:16 to 2017-07-15 04:44:40 EUROPA-ACQ 2017-07-16 21:20:11 to 2017-07-16 21:24:24 GANYMEDE-TRANSIT 2017-07-16 21:36:58 to 2017-07-16 22:03:48 GANYMEDE-TRANSIT 2017-07-16 22:53:43 to 2017-07-16 23:39:02 2017-07-16 02:18:14 to 2017-07-16 02:59:38 2017-07-18 03:34:19 to 2017-07-18 04:15:43 | |||||||||
10 | CCD | Irwin | VLT/MUSE - IFU | spectroscopic imaging, 475-930 nm to determine cloud structure and albedo spectrum of particles. | spectral images of Jupiter obtained on July 20, July 26 and August 15/16. GRS only clearly present far from terminator in August 15/16 images, and even then, seeing is relatively poor. | Raw data publicly available to download from ESO portal. Standard calibration pipeline takes of the order of 1-3 days to complete. 20 July observations not photometric due to poor weather conditions. | ||||||||
11 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | 2017-07-12 to date | |||||||||
12 | visible/NUV | Wong | HST/WFC3 UVIS | hi-resolution map of perijove track, single orbit snapshot | Start time: 2017-Jul-11 09:25:44 UT, End time: 2017-Jul-11 09:59:03 UT | https://archive.stsci.edu/prepds/wfcj/ https://dx.doi.org/10.1016/j.icarus.2017.06.007 | ||||||||
13 | CCD / near IR | Sanchez-Lavega | Calar Alto 2.2-m telescope / PlanetCam | 0.38-1.7 micron imaging | July 10 | Generally available within two weeks (photometric version). High-resolution versions available later on. Calibrated data also available upon request. | ||||||||
14 | near IR | Orton | IRTF/SpeX | filtered imaging at several wavelengths between 1.58 and 5.1µm and spectral scanning over 2-µm and 5-µm ranges | successful on July 10 @ 13:30-16:30 HST, July 11, but July 12 @ 13:30 - 16:30 HST obervations weathered out. July 11 observations were unphotometric images only, through afternoon seeing and variable cirrus. A single set of observations through each filter was made on July 18 in partly cloudy weather conditions with sub-optimal seeing. July 25, 26 date were taken in clear skies but ~1" seeing. | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired. Reduced "quick-look" observations (geometrically but not radiometrically calibrated) will be available for immeduately use from the Juno-curated web site: http://junoirtf.space.swri.edu/. Data on Jul 10 and 11 are radiometrically uncalibrated, due to cirrus clouds across the sky obviating reliable comparisons with standard stars. | ||||||||
15 | near-IR | Orton | IRTF/SpeX | filtered imaging at several wavelengths between 1.58 and 5.1µm and spectral scanning over 2-µm and 5-µm ranges | Brief sets of observations were made on August 7, 8, and 29. August 28 was weathered out. None of these are photmetric, as we were looking close to the sun. | Raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired. Reduced "quick-look" observations (geometrically but not radiometrically calibrated) will be available for immeduately use from the Juno-curated web site: http://junoirtf.space.swri.edu/. | ||||||||
16 | near IR (5 µm) | Wong | Gemini-N/NIRI | lucky imaging, 5-µm maps | Start time: 2017-Jul-09 07:00:07 UT, End time: 2017-Jul-09 08:16:55 UT. Start time: 2017-Jul-10 06:17:08 UT, End time: 2017-Jul-10 07:12:27 UT. | |||||||||
17 | mid-IR | Fletcher | IRTF/TEXES | scanned spectral maps of Jupiter's disk at ten key spectral settings to derive upper-tropospheric and stratospheric temperatures, aerosol/cloud distributions, and distribution of tropospheric NH3 and PH3, and stratospheric C2H2 and C2H6. | obtained July 9, 4:00-7:00 UT with cirrus (focusing on 5-micron observations); July 11, 3:30-7:30 UT; July 15, 3:00-6:00 UT | raw data available almost immediately, calibrated files with geometry within a month, and retrieved properties potentially available within 1-2 weeks (subject to any unforeseen issues) | ||||||||
18 | mid IR | Fletcher | VLT / VISIR | Filtered radiometric imaging to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology. | July 06: (UT00:04-01:00) 8-12μm spectra of PJ longitudes CMLIII ~32 July 13: (UT22:34-23:38) Full imaging including Mband (std imaging) CMLIII ~82 July 18: (UT00:28-01:36) Full imaging including Mband (std imaging) CMLIII ~36 July 20: (UT00:07-01:52) 8-12μm spectra including Mband burst mode imaging CMLIII ~337 July 20/21: (UT23:39-00:32) Full imaging (std) observations CMLIII ~91 | Available in raw form in the ESO archive within 24 hours of acquisition; cylindrical maps within 1-2 days and reduced maps within a week. | ||||||||
19 | mid IR | Greathouse | IRTF/TEXES | scanned high- and medium-resolution spectral maps of Jupiter's disk at key CH4- and H2-absorbing wavelengths to determine temperatures in the upper troposphere and stratosphere to determine the structure of non-seasonal thermal waves associated with the Quasi-Quadrennial Oscillation (QQO) | obtained Jul 8, 4:00-6:30 UT; additional supporting medium-resolution maps on July 15, 17, 18 | TBD | ||||||||
20 | mid IR | Sinclair | IRTF/TEXES | scanned high-resolution spectral maps of Jupiter's disk at six key spectral settings to derive stratospheric temperatures and 3-dimensional distribution of stratospheric C2H2, C2H4, C2H6 and H3+ in auroral regions. | obtained July 13, 4:00-7:30 UT; July 16, 3:00-7:30 UT; July 17, 4:00-7:00 UT (medium-resolution); July 18, 3:00-7:00 UT (medium-resolution). No scheduled high-resolution observations were made due to pervasive cirrus in order to compensate for poor sky transmission and variabiity. | Spectra available from Sinclair upon request. Retrieval analysis in progress. | ||||||||
21 | mid IR | Fletcher | VLT / VISIR | filtered radiometric imaging to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology. | observations obtained in service time on July 13 , 18 and 20 | available in raw form in the ESO archive within 24 hours of acquisition; cylindrical maps within 1-2 days and reduced maps within a week | ||||||||
22 | radio | Zarka, Cecconi, Lamy, Louis | Nançay Decameter Array (France) | coordinated measurement of 10-40 MHz cyclotron radio emission | every day, 8 hours around the transition to local meridian | https://maser.lesia.obspm.fr/task-1-data-collections/juno-ground-radio/juno-ground-radio-nancay-decameter.html?lang=en | ||||||||
23 | radio | Imai | Long Wavelength Array 1 (LWA1) | Jupiter's decametric auroral radio observations | July 10-17 August 28-29 | Low-resolution LWA1 data are freely accessible via Autoplot (http://autoplot.org) by accepting the data usage policy (http://space.physics.uiowa.edu/earth/datapolicy.html) More information can be found at http://space.physics.uiowa.edu/earth/ | ||||||||
24 | radio | Kita | GMRT (India) | L-band | 10Jul2017 14:00-20:00 IST | Reduced data will be available upon request. | ||||||||
25 | radio | Ryabov / Zakharenko | UTR-2 (Ukraine) GURT(Ukraine) | Decametric emissions Spectrograms (8-33 MHz) Waveforms (8-33 MHz) Spectrograms (8-80 MHz) | July (10)-(11) 14:00(10)-20:00(10) UTC 10:00(11)-16:00(11) UTC 14:30(11)-16:00(11) UTC 14:00(10)-20:00(10) UTC 10:00(11)-16:00(11) UTC | The data will be available upon request to V. Ryabov. | ||||||||
26 | CCD (Visible) | Chanover | APO | Hyperspectral image cubes, 470-950 nm | July 10-11 | At least one cube under photometric conditions | ||||||||
27 | ||||||||||||||
28 | Scheduled observations by Juno. | |||||||||||||
29 | ||||||||||||||
30 | Perijove is 2017 July 11, 1:54:42 UTC. System-III longitude = 49.4°W | |||||||||||||
31 | ||||||||||||||
32 | Period: Orbit 7 (2017 July 10 – 2017 August 29) | |||||||||||||
33 | Instrument | Description | ||||||||||||
34 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||||||
35 | MWR | N/S scans near perijove longitude, not centered on nadir. | ||||||||||||
36 | UVS | TBD | ||||||||||||
37 | JunoCam | E/PO observations targeting features voted on by public. | ||||||||||||
38 | JIRAM | polar regions, hot spots. no observations of the GRS or its environment | ||||||||||||
39 | ||||||||||||||
40 | ||||||||||||||
41 | ||||||||||||||
42 | ||||||||||||||
43 | ||||||||||||||
44 | ||||||||||||||
45 | ||||||||||||||
46 | ||||||||||||||
47 | ||||||||||||||
48 | ||||||||||||||
49 | ||||||||||||||
50 | ||||||||||||||
51 | ||||||||||||||
52 | ||||||||||||||
53 | ||||||||||||||
54 | ||||||||||||||
55 | ||||||||||||||
56 | ||||||||||||||
57 | ||||||||||||||
58 | ||||||||||||||
59 | ||||||||||||||
60 | ||||||||||||||
61 | ||||||||||||||
62 | MWR footprints for the minimum emission angle at each rotation of the spacecraft. The periojove position is given by the cross. | |||||||||||||
63 | ||||||||||||||
64 | ||||||||||||||
65 | ||||||||||||||
66 | ||||||||||||||
67 | ||||||||||||||
68 | ||||||||||||||
69 | ||||||||||||||
70 | ||||||||||||||
71 | ||||||||||||||
72 | ||||||||||||||
73 | ||||||||||||||
74 | ||||||||||||||
75 | ||||||||||||||
76 | ||||||||||||||
77 | ||||||||||||||
78 | ||||||||||||||
79 | ||||||||||||||
80 | ||||||||||||||
81 | ||||||||||||||
82 | ||||||||||||||
83 | ||||||||||||||
84 | ||||||||||||||
85 | ||||||||||||||
86 | ||||||||||||||
87 | ||||||||||||||
88 | ||||||||||||||
89 | ||||||||||||||
90 | ||||||||||||||
91 | ||||||||||||||
92 | ||||||||||||||
93 | ||||||||||||||
94 | ||||||||||||||
95 | ||||||||||||||
96 | ||||||||||||||
97 | ||||||||||||||
98 | ||||||||||||||
99 | ||||||||||||||
100 | ||||||||||||||
101 | ||||||||||||||
102 | ||||||||||||||
103 | ||||||||||||||
104 | ||||||||||||||
105 | ||||||||||||||
106 | ||||||||||||||
107 | ||||||||||||||
108 | ||||||||||||||
109 | ||||||||||||||
110 | ||||||||||||||
111 | ||||||||||||||
112 | ||||||||||||||
113 | ||||||||||||||
114 | ||||||||||||||
115 | ||||||||||||||
116 | ||||||||||||||
117 | ||||||||||||||
118 | ||||||||||||||
119 | ||||||||||||||
120 | ||||||||||||||
121 | ||||||||||||||
122 | ||||||||||||||
123 | ||||||||||||||
124 | ||||||||||||||
125 | ||||||||||||||
126 | ||||||||||||||
127 | ||||||||||||||
128 | ||||||||||||||
129 | ||||||||||||||
130 | ||||||||||||||
131 | ||||||||||||||
132 | ||||||||||||||
133 | ||||||||||||||
134 | ||||||||||||||
135 | ||||||||||||||
136 | ||||||||||||||
137 | ||||||||||||||
138 | ||||||||||||||
139 | ||||||||||||||
140 | ||||||||||||||
141 | ||||||||||||||
142 | ||||||||||||||
143 | ||||||||||||||
144 | ||||||||||||||
145 | ||||||||||||||
146 | ||||||||||||||
147 | ||||||||||||||
148 | ||||||||||||||
149 | ||||||||||||||
150 | ||||||||||||||
151 | ||||||||||||||
152 | ||||||||||||||
153 | ||||||||||||||
154 | ||||||||||||||
155 | ||||||||||||||
156 | Above are various reconstructions of the visual morhpology of Jupiter's clouds from the JunoCam instrument. | John Rogers and Gerald Eichstaedt | ||||||||||||
157 | ||||||||||||||
158 | ||||||||||||||
159 | ||||||||||||||
160 | ||||||||||||||
161 | ||||||||||||||
162 | ||||||||||||||
163 | ||||||||||||||
164 | ||||||||||||||
165 | ||||||||||||||
166 | ||||||||||||||
167 | ||||||||||||||
168 | ||||||||||||||
169 | ||||||||||||||
170 | ||||||||||||||
171 | ||||||||||||||
172 | ||||||||||||||
173 | ||||||||||||||
174 | ||||||||||||||
175 | ||||||||||||||
176 | ||||||||||||||
177 | ||||||||||||||
178 | ||||||||||||||
179 | ||||||||||||||
180 | ||||||||||||||
181 | ||||||||||||||
182 | ||||||||||||||
183 | ||||||||||||||
184 | ||||||||||||||
185 | ||||||||||||||
186 | ||||||||||||||
187 | ||||||||||||||
188 | ||||||||||||||
189 | ||||||||||||||
190 | ||||||||||||||
191 | Composite of JIRAM M-band (5-micron) map. | |||||||||||||
192 | ||||||||||||||
193 | ||||||||||||||
194 | ||||||||||||||
195 | ||||||||||||||
196 | ||||||||||||||
197 | ||||||||||||||
198 | ||||||||||||||
199 | ||||||||||||||
200 | ||||||||||||||
201 | ||||||||||||||
202 | ||||||||||||||
203 | ||||||||||||||
204 | ||||||||||||||
205 | ||||||||||||||
206 | ||||||||||||||
207 | ||||||||||||||
208 | ||||||||||||||
209 | ||||||||||||||
210 | ||||||||||||||
211 | ||||||||||||||
212 | ||||||||||||||
213 | ||||||||||||||
214 | ||||||||||||||
215 | ||||||||||||||
216 | ||||||||||||||
217 | ||||||||||||||
218 | ||||||||||||||
219 | ||||||||||||||
220 | ||||||||||||||
221 | ||||||||||||||
222 | ||||||||||||||
223 | ||||||||||||||
224 | ||||||||||||||
225 | ||||||||||||||
226 | ||||||||||||||
227 | ||||||||||||||
228 | ||||||||||||||
229 | ||||||||||||||
230 | ||||||||||||||
231 | ||||||||||||||
232 | ||||||||||||||
233 | ||||||||||||||
234 | ||||||||||||||
235 | ||||||||||||||
236 | ||||||||||||||
237 | ||||||||||||||
238 | ||||||||||||||
239 | ||||||||||||||
240 | ||||||||||||||
241 | ||||||||||||||
242 |
1 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed directly at the Earth. | |||||||||
---|---|---|---|---|---|---|---|---|---|---|
2 | Observations requested. | |||||||||
3 | Observations planned / granted time | |||||||||
4 | Period: Orbit 6 [GRAV] (2017 May 18 – 2017 July 9) | Observations successful | ||||||||
5 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | Observations cancelled or unsuccessful | |||
6 | X-ray | Gladstone | Chandra | ~10 hours of HRC-I observations of Jupiter | 05/19/2017 00:28-12:21 | publicly available after 1 year | ||||
7 | X-ray | W. Dunn | XMM-Newton | 30 hours continuous spectral, spatial and temporal resolution on Juno Apojove June 18-19 | 2017-06-18 19:45:25 -- 2017-06-19 23:48:45 | W. Dunn happy to share data | ||||
8 | X-ray | Caitriona Jackman | Chandra | 36 ks (10 hours) continuous observation by Chandra at Juno apojove | Obs #1: Start: 2017:169:18:39:05 -> End: 2017:170:05:31:25 Coincident with XMM 2017-Jun-18 (DoY 169) T20:29:60 to 2017-Jun-19 (DoY 170) T20:06:40 (85 ks)) and with HST nd NuStar | Request of Jackman. Keen to collaborate with Juno team as contemporaneous in situ data will help to constrain the X-ray drivers thought to map to this region | ||||
9 | Hard X-ray | Jackman (collaboration with Mori, Dunn, Branduardi-Raymont, Gladstone etc.) | NuSTAR | Long observation to cover interval around Juno apojove, coincident with: Chandra, XMM, HST | 2017:169:06:40:16 to 2017:171:18:05:00 | Request of Jackman and Mori | ||||
10 | Hard X-ray | Mori | NuSTAR | 130 ks overlapping with the Chandra obesrvation | TBD, but will span the Chandra observation on 2017-May-19 | Public after 1 year | ||||
11 | FUV | Grodent | HST/FUV-MAMA | high spatial and temporal resolution FUV observations of magnetosphere and ultraviolet auroras | 2017-05-0906:42:14 to 2017-05-09 07:23:38 2017-05-10 11:19:00 to 2017-05-10 12:00:24 2017-05-10 06:32:53 to 2017-05-10 07:14:17 2017-05-10 12:53:48 to 2017-05-10 13:35:12 2017-05-11 07:58:51 to 2017-05-11 08:40:15 2017-05-13 09:15:18 to 2017-05-13 09:56:42 2017-05-13 10:50:40 to 2017-05-13 11:32:04 2017-05-15 12:06:56 to 2017-05-15 12:48:20 2017-05-16 07:11:14 to 2017-05-16 07:52:38 2017-05-17 03:50:54 to 2017-05-17 04:32:18 2017-05-18 08:27:19 to 2017-05-18 09:08:43 2017-05-18 10:02:40 to 2017-05-18 10:44:04 2017-05-19 11:28:19 to 2017-05-19 12:09:43 2017-05-19 01:56:13 to 2017-05-19 02:37:37 2017-05-19 03:31:34 to 2017-05-19 04:12:58 2017-05-19 05:06:55 to 2017-05-19 05:48:19 2017-05-19 06:42:17 to 2017-05-19 07:23:41 2017-05-19 09:52:59 to 2017-05-19 10:34:23 2017-05-19 08:26:31 to 2017-05-19 08:58:53 2017-05-19 08:15:19 to 2017-05-19 08:19:48 2017-05-20 01:46:31 to 2017-05-20 02:27:55 2017-05-21 06:22:53 to 2017-05-21 07:04:17 2017-05-24 04:18:33 to 2017-05-24 04:59:57 2017-05-24 23:22:50 to 2017-05-25 00:04:14 2017-05-25 00:58:12 to 2017-05-25 01:39:36 2017-05-26 05:34:44 to 2017-05-26 06:16:08 2017-05-27 00:39:08 to 2017-05-27 01:20:32 2017-05-27 02:14:30 to 2017-05-27 02:55:54 2017-05-27 21:18:55 to 2017-05-27 22:00:19 2017-06-18 19:27:33 to 2017-06-18 19:27:33 2017-06-18 09:55:28 to 2017-06-18 10:36:52 2017-07-04 02:38:03 to 2017-07-04 03:19:27 2017-07-05 08:50:08 to 2017-07-05 09:31:32 2017-07-06 02:19:12 to 2017-07-06 03:00:36 2017-07-06 10:16:03 to 2017-07-06 10:57:27 2017-07-07 00:34:21 to 2017-07-07 01:15:45 2017-07-08 06:46:16 to 2017-07-08 07:27:40 | Times may change by re-scheduling on the part of HST | ||||
12 | visible/NUV | Wong | HST/WFC3 UVIS | hi-resolution map of perijove track, single orbit snapshot | Start time: 2017-May-19 14:38:23 UT, End time: 2017-May-19 15:16:17 UT | https://archive.stsci.edu/prepds/wfcj/ https://dx.doi.org/10.1016/j.icarus.2017.06.007 | ||||
13 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | 2017-05-20 2017-05-21 2017-05-22 2017-05-27 2017-05-28 2017-05-29 2017-06-02 2017-06-03 2017-06-04 2017-06-05 2017-06-06 2017-07-01 2017-07-02 2017-07-05 2017-07-06 2017-07-07 2017-07-08 | |||||
14 | Visible | Schmidt | Apache Point Observatory / Dual Imaging Spectrograph (DIS) | Long-slit visible spectroscopy of both sides of the Io torus to determine S+, S++, O+ composition and electron density | May 19 | Calibrated data products available upon request | ||||
15 | CCD | Sanchez-Lavega | Aulo EspaZio Gela, Bilbao, Spain / 28-cm telescope and 36-cm telescope at Calar Alto | continuous imaging survey, 0.38-0.9 microns | images 28cm telescope: May 19,20, 23, 24 31 and Jun 18; images 36 cm telescope : May 18 and June 1 | Images have been procssed and are available upon request. | ||||
16 | CCD | Colas, Hueso | Pic du Midi T1m | lucky imaging in the visible (RVB, IR650 and 890 nm) | June 9-11 | Data available at PVOL2. No calibrated data but images have very high spatial resolution | ||||
17 | CCD / near IR | Sanchez-Lavega | Calar Alto 2.2-m telescope / PlanetCam | 0.38-1.7 micron imaging | Imaging on June 12, 13, 14, 15 | Photometric and procssed images with different degree of quality for each night area avaialble upon request. | ||||
18 | CCD / near IR | Sanchez-Lavega | Calar Alto 2.2-m telescope / PlanetCam | 0.38-1.7 micron imaging | July 9 (high quality data on July 9) | Generally available within two weeks (photometric version). High-resolution versions available later on. Calibrated data also available upon request. | ||||
19 | CCD | Irwin | VLT/MUSE - IFU | spectroscopic imaging, 480-930 nm to determine cloud structure and albedo spectrum of particles. | May 28 | Raw data publicly available to download from ESO portal. Standard calibration pipeline takes of the order of 1-3 days to complete. Oval BA is present in these observations, though its annulus is difficult to resolve from its core. | ||||
20 | near IR | Skrutskie | Fan Mountain / 31" FanCam | Io H and K band flux, disk integrated | TBD | |||||
21 | near IR | Johnson | IRTF/iSHELL | imaging and high-resolution spectroscopy of H3+ emission | obtained May 18, May 31 June 1, June 1, June 9, June 29 | TBD | ||||
22 | near IR | Bjoraker | IRTF/iSHELL | high-resoution spectroscopy of Jupiter in the 5-µm window to determine NH3, H2O abundances and propeties of water clouds at similar locations and nearly the same time as Juno | Taken May 17, 18:15 - May 18, 0:15 HST; and same time on May 20-21 HST; May 18:excellent seeing (0.3 arcsec) and low humidity (10%), May 21:0.6arcsec seeing and 20% humidity | fully reduced spectra available in 2 months | ||||
23 | near IR | Orton | IRTF/SpeX | filtered imaging at several wavelengths between 1.58 and 5.1µm and spectral scanning over 2-µm and 5-µm ranges | obtained on May 18, 22:00-01:30 HST; May 19, 18:15- May 20, 1:15 HST; June 7, 18:20-19:20 HST; June 18, 19:00-19:45 HST; June 19, 21:20-22:00 HST (poor seeing); June 25, 18:20-19:35 HST (poor seeing) | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired. Reduced "quick-look" observations (geometrically but not radiometrically calibrated) will be available for immeduately use from the Juno-curated web site: http://junoirtf.space.swri.edu/ | ||||
24 | near IR | Orton | Gemini-N/NIRI | AO-stabilized imaging of Jupiter at several wavelengths | images obtained on service time May 18, May 26, May 31, Jule 1, June 2, June 9, June 29, July 4 (one wavelength), July 6 UT | TBD | ||||
25 | near IR | Orton | IRTF/SpeX guide camera | filtered imaging at several near-infrared wavelengths, including H3+ emission at 3.14µm and thermal emission at 5.1 µm. | obtained on July 9 @ 19:30-20:10 HST | raw images available immediately from IRTF web site. Reduced "quick-look" observations (geometrically but not radiometrically calibrated) will be available for immeduately use from the Juno-curated web site: http://junoirtf.space.swri.edu/ | ||||
26 | near IR | Chudczer | Gemini N/GIRS | Spectroscopic polar mapping of auroral H3+ emission | successful observations on May 19 | Maps of the 2.04 and 2.09 microns reduced and available. We also obtained the first maps of He I at 2.058 micron. The spectra in two regions of K and L bands are being analysed. Looking for a collaborator - expert in the He I emissions. | ||||
27 | near IR (5 µm) | Wong | Gemini-N/NIRI | lucky imaging, 5-µm maps | Start time: 2017-May-21 05:34:34 UT, End time: 2017-May-21 06:59:22 UT. | |||||
28 | mid IR | Greathouse | IRTF/TEXES | scanned high- and medium-resolution spectral maps of Jupiter's disk at key CH4- and H2-absorbing wavelengths to determine temperatures in the upper troposphere and stratosphere to determine the structure of non-seasonal thermal waves associated with the Quasi-Quadrennial Oscillation (QQO) | obtaiendMay 27-28, 17:15 - 23:00 HST | TBD | ||||
29 | mid IR | Kasaba Orton | Subaru / COMICS | filtered radiometric imaging and spectroscopy to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology and auroral heating and chemistry. | Mid-infrared imaging and spectroscopy of Jupiter on May 17-18 (Orton, Subaru Keck-exchange time), May 19-20 (Kasaba, Subaru direct time) 05:00-10:00 UT. May 17: two full sets of filters and 8-14 micron scanned spectroscopy of Oval BA and adjacent latitude. May 18: three full sets of filtered images and 8-14 micron scanned spectroscopy of GRS, NEB with slit parallel to the equator, and of the PJ6 longitude with slit parallel to the rotation axis. May 19: one single-hemisphere set of images 1.5 hours before PJ9 and three subsequent full images at all wavelengths, plus scans of NEB; May 20: three sets of images, spectral scans of: south polar aurora, GRS and wake, and PJ9 longitude. Seeing on May 17-19 was 0.3-0.5" at 10 microns; May 20 degraded to 0.6". | Kasaba would like to see agreement in place with Juno science team first and discussed at the workshop, but willing to share. Orton will share immediately. An image with the GRS at the central meridian is scheduled for a Subaru public release, 2017 June 30. | ||||
30 | mid IR | Sinclair | IRTF/TEXES | scanned high-resolution spectral maps of Jupiter's disk at six key spectral settings to derive stratospheric temperatures and 3-dimensional distribution of stratospheric C2H2, C2H4, C2H6 and H3+ in auroral regions. | May 30 - 31, 17:15 - 21:45 HST | Good quality data. Spectra, retrieved temperatures and abundances of C2H2, C2H4 and C2H6 are available from Sinclair upon request. | ||||
31 | mid IR | Fouchet | IRTF/TEXES | scanned high-resolution spectral maps of Jupiter's disk to make methyl as a function of latitude | June 1, 3:00 - 5:15 HST | TBD | ||||
32 | radio | Zarka, Cecconi, Lamy, Louis | Nançay Decameter Array (France) | coordinated measurement of 10-40 MHz cyclotron radio emission | every day, 8 hours around the transition to local meridian | https://maser.lesia.obspm.fr/task-1-data-collections/juno-ground-radio/juno-ground-radio-nancay-decameter.html?lang=en | ||||
33 | radio | Imai | Long Wavelength Array 1 (LWA1) | Jupiter's decametric auroral radio observations | May 10-17 July 4-5, 7-9 | Low-resolution LWA1 data are freely accessible via Autoplot (http://autoplot.org) by accepting the data usage policy (http://space.physics.uiowa.edu/earth/datapolicy.html) More information can be found at http://space.physics.uiowa.edu/earth/ | ||||
34 | radio | Kita | GMRT (India) | L-band | 18May2017 18:00-24:00 IST | Reduced data will be available upon request. | ||||
35 | radio | Ryabov / Zakharenko | UTR-2 (Ukraine) GURT(Ukraine) | Decametric emissions Spectrograms (8-33 MHz) Waveforms (8-33 MHz) Spectrograms (8-80 MHz) | May (18)-(19) 16:30(18)-00:09(19) UTC 12:43(18)-21:00(18) UTC 16:30(18)-19:20(18) UTC 17:00(18)-00:07(19) UTC 13:00(19)-21:00(19) UTC | The data will be available upon request to V. Ryabov. | ||||
36 | CCD (Visible) | Chanover | APO | Hyperspectral image cubes, 470-950 nm | May 20-21 | Photometric conditions | ||||
37 | ||||||||||
38 | Scheduled observations by Juno. | |||||||||
39 | ||||||||||
40 | Perijove is 2017 May 19, 6:00:47 UTC at Juno. System-III longitude = 139.8°W | |||||||||
41 | ||||||||||
42 | Period: Orbit 6 [GRAV] (2017 May 18 – 2017 July 9) | |||||||||
43 | Instrument | Description | ||||||||
44 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||
45 | MWR | N/S scans near perijove longitude, not centered on nadir. | ||||||||
46 | UVS | TBD | ||||||||
47 | JunoCam | E/PO observations targeting features voted on by public. | ||||||||
48 | JIRAM | TBD | ||||||||
49 | ||||||||||
50 | ||||||||||
51 | ||||||||||
52 | ||||||||||
53 | ||||||||||
54 | ||||||||||
55 | ||||||||||
56 | ||||||||||
57 | ||||||||||
58 | ||||||||||
59 | ||||||||||
60 | ||||||||||
61 | ||||||||||
62 | ||||||||||
63 | ||||||||||
64 | ||||||||||
65 | ||||||||||
66 | ||||||||||
67 | ||||||||||
68 | ||||||||||
69 | ||||||||||
70 | ||||||||||
71 | ||||||||||
72 | ||||||||||
73 | MWR footprints for the minimum emission angles at each latitude | |||||||||
74 | ||||||||||
75 | ||||||||||
76 | ||||||||||
77 | ||||||||||
78 | ||||||||||
79 | ||||||||||
80 | ||||||||||
81 | ||||||||||
82 | ||||||||||
83 | ||||||||||
84 | ||||||||||
85 | ||||||||||
86 | ||||||||||
87 | ||||||||||
88 | ||||||||||
89 | ||||||||||
90 | ||||||||||
91 | ||||||||||
92 | ||||||||||
93 | ||||||||||
94 | ||||||||||
95 | ||||||||||
96 | ||||||||||
97 | ||||||||||
98 | ||||||||||
99 | ||||||||||
100 | ||||||||||
101 | ||||||||||
102 | ||||||||||
103 | ||||||||||
104 | ||||||||||
105 | ||||||||||
106 | ||||||||||
107 | ||||||||||
108 | ||||||||||
109 | ||||||||||
110 | ||||||||||
111 | ||||||||||
112 | ||||||||||
113 | ||||||||||
114 | ||||||||||
115 | ||||||||||
116 | ||||||||||
117 | ||||||||||
118 | ||||||||||
119 | ||||||||||
120 | ||||||||||
121 | ||||||||||
122 | ||||||||||
123 | ||||||||||
124 | ||||||||||
125 | ||||||||||
126 | ||||||||||
127 | ||||||||||
128 | ||||||||||
129 | ||||||||||
130 | ||||||||||
131 | ||||||||||
132 | ||||||||||
133 | ||||||||||
134 | ||||||||||
135 | ||||||||||
136 | ||||||||||
137 | ||||||||||
138 | ||||||||||
139 | ||||||||||
140 | ||||||||||
141 | ||||||||||
142 | ||||||||||
143 | ||||||||||
144 | ||||||||||
145 | ||||||||||
146 | ||||||||||
147 | ||||||||||
148 | ||||||||||
149 | ||||||||||
150 | ||||||||||
151 | ||||||||||
152 | ||||||||||
153 | ||||||||||
154 | ||||||||||
155 | ||||||||||
156 | ||||||||||
157 | ||||||||||
158 | ||||||||||
159 | ||||||||||
160 | ||||||||||
161 | ||||||||||
162 | ||||||||||
163 | Composite of JIRAM M-band (5-micron) map. | |||||||||
164 | ||||||||||
165 | ||||||||||
166 | ||||||||||
167 | ||||||||||
168 | ||||||||||
169 | ||||||||||
170 | ||||||||||
171 | ||||||||||
172 | ||||||||||
173 | ||||||||||
174 | ||||||||||
175 | ||||||||||
176 | ||||||||||
177 | ||||||||||
178 | ||||||||||
179 | ||||||||||
180 | ||||||||||
181 | ||||||||||
182 | ||||||||||
183 | ||||||||||
184 | ||||||||||
185 | ||||||||||
186 | ||||||||||
187 | ||||||||||
188 | ||||||||||
189 | ||||||||||
190 | ||||||||||
191 | ||||||||||
192 | ||||||||||
193 | ||||||||||
194 | ||||||||||
195 | ||||||||||
196 | ||||||||||
197 | ||||||||||
198 | ||||||||||
199 | ||||||||||
200 | ||||||||||
201 | ||||||||||
202 | ||||||||||
203 | ||||||||||
204 |
1 | ||||||||||
---|---|---|---|---|---|---|---|---|---|---|
2 | Observations requested. | |||||||||
3 | Period: Orbit 5 [MWR/tilt] (2017 March 27 – 2017 May 17) | Observations planned / granted time | ||||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | Observations successful | |||
5 | X-ray | Gladstone | Chandra | ~3 hours of HRC-I observations of Jupiter | 03/27/2017 08:32-11:39 | publicly available 3/28/2018 | Observations cancelled or unsuccessful | |||
6 | FUV | Grodent | HST/FUV-MAMA | high spatial and temporal resolution FUV observations of magnetosphere and ultraviolet auroras | 2017-03-28 03:45:30 2017-03-28 11:42:24 2017-03-28 13:17:40 2017-03-29 08:22:00 2017-03-30 03:26:22 2017-03-30 05:01:44 2017-03-31 09:38:20 2017-04-01 06:18:07 2017-04-19 19:27:01 2017-04-23 14:00:08 2017-05-09 06:42:14 | Times may change by re-scheduling on the part of HST | ||||
7 | visible/NUV | Wong | HST/WFC3 UVIS | hi-resolution map of perijove track, single orbit snapshot | Start time: 2017-Mar-27 07:23:38 UT, End time: 2017-Mar-27 07:41:51 UT | https://archive.stsci.edu/prepds/wfcj/ https://dx.doi.org/10.1016/j.icarus.2017.06.007 | ||||
8 | visible/NUV | Simon | HST/WFC3 UVIS | Multiple-filtered imaging, 275-885 nm; global map pair (Outer Planet Atmospheric Legacy [OPAL] program) | Start time: 2017-Apr-03 01:11:24 UT, End time: 2017-Apr-03 22:25:13 UT | https://archive.stsci.edu/prepds/opal/ | ||||
9 | CCD | Sanchez-Lavega | Aulo EspaZio Gela, Bilbao, Spain / 28-cm telescope | continuous imaging survey, 0.38-0.9 microns (U (ultraviolet), 890 nm (methane), R610, R685, R,G,B, 727 nm (methane)) | 04/07, 04/08, 04/11, 04/12, 04/21, 04/22, 04/23 | Images available at PVOL2 and Aula EspaZio web page. | ||||
10 | CCD | Sanchez-Lavega | Aula EspaZio Gela 36-cm telescope at Calar Alta Observatory | continuous imaging survey, Wavelengths: R, V, B, IR, R610, 890nm (methane), R610 | 03/30, 04/08, 04/09, 04/10, 04/12, 05/03 | Images available at PVOL2 and Aula EspaZio web page. | ||||
11 | CCD (Visible) | Chanover | APO | Hyperspectral image cubes, 470-950 nm | March 26-27 | Photometric conditions | ||||
12 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | 2017-03-07 2017-03-08 2017-03-09 2017-03-12 2017-03-13 2017-03-14 2017-03-15 2017-03-17 2017-04-14 2017-04-15 2017-04-16 2017-04-18 2017-04-19 2017-04-20 2017-04-21 2017-04-24 2017-04-26 2017-04-27 2017-04-28 2017-05-01 2017-05-02 2017-05-03 2017-05-04 | |||||
13 | Visible | Schmidt | Apache Point Observatory / Dual Imaging Spectrograph (DIS) | Long-slit visible spectroscopy of both sides of the Io torus to determine S+, S++, O+ composition and electron density | 3/31/2017, 5/11/2017 | Calibrated data products available upon request | Q | |||
14 | CCD | Irwin | VLT/MUSE - IFU | spectroscopic imaging, 475-930 nm to determine cloud structure and albedo spectrum of particles. | May 15 | Raw data publicly available to download from ESO portal. Standard calibration pipeline takes of the order of 1-3 days to complete. | ||||
15 | CCD / near IR | Sanchez-Lavega | Calar Alto 2.2-m telescope / PlanetCam | 0.38-1.7 micron imaging Wavelengths: From 0.38 to 1.7 microns in a large number of spectral bands (see Mendikoa et al., PASP. 2016) | 03/28, 03/29, 03/29-30, 03/30-31 | Photometric versions available within two weeks. Processed images will be available later. | ||||
16 | near IR | Skrutskie | Fan Mountain / 31" FanCam | Io H and K band flux, disk integrated | ||||||
17 | Bjoraker | IRTF/iSHELL | high-resoution spectroscopy of Jupiter in the 5-µm window to determine NH3, H2O abundances and propeties of water clouds at similar locations and nearly the same time as Juno | Taken Mar 28, 0:30-6:30 HST good seeing & low humidity cover longitude of new PJ5: 187 System III | fully reduced spectra available in 2 months | |||||
18 | near IR | Orton | IRTF/SpeX | filtered imaging at several wavelengths between 1.58 and 5.1µm and spectral scanning over 2-µm and 5-µm ranges | obtained on Mar 27, 01:30-6:30 HST; Mar 28, 21:30-Mar 29 03:30 HST | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired. Reduced "quick-look" observations (geometrically but not radiometrically calibrated) will be available for immeduately use from the Juno-curated web site: http://junoirtf.space.swri.edu/ | ||||
19 | near IR | Johnson | IRTF/iSHELL | Scans of the southern auroral H3+ emission at ~3.4µm. Simultaneous to JIRAM, MAG, JADE and JEDI measurements. | Data obtained on Mar 26th 20:30 - 01:30 HST --> clear skies, successful guiding. Several sucessful scans were taken of the northern aurora just after perijove. Images taken main in the H3+ filter, some taken with 5.1 filter near to end of observing. Extra iSHELL time: 20th April 21:20 - 00:20 HST scanning the northern aurora, H3+ and 5.1 micron images & 21st April 22:20 - 01:20 HST scanning the southern aurora H3+ and 5.1 images. | Data reduction in process. | ||||
20 | near IR | Moore | IRTF/iSHELL | E-W spectral scans of Jupiter’s northern auroral region – rough cut of spectral images obtained, will ultimately yield a series of auroral H3+ temperature/density/radiance maps, one every ~30 min | 4/26/2017 and 4/28/2017 | Data reduction in process. Rough spectral images obtained. | ||||
21 | near IR | Orton | IRTF/SpeX guide camera | filtered imaging at several near-infrared wavelengths, including H3+ emission at 3.14µm and thermal emission at 5.1 µm. | Mar 30, 3:00-3:40 HST; Mar 31 | raw images available immediately from IRTF web site. Reduced "quick-look" observations (geometrically but not radiometrically calibrated) will be available for immeduately use from the Juno-curated web site: http://junoirtf.space.swri.edu/ | ||||
22 | sub-mm | Roth / Sanchez Monge | IRAM NOEMA | Io SO2 atmosphere | Successful observations on, April 6 and April 29 | TBD, reqeust to Roth | Q | |||
23 | radio | Zarka, Cecconi, Lamy, Louis | Nançay Decameter Array (France) | coordinated measurement of 10-40 MHz cyclotron radio emission | every day, 8 hours around the transition to local meridian | https://maser.lesia.obspm.fr/task-1-data-collections/juno-ground-radio/juno-ground-radio-nancay-decameter.html?lang=en | ||||
24 | radio | Imai | Long Wavelength Array 1 (LWA1) | Jupiter's decametric auroral radio observations | Mar 28-30, Apr 1 | Low-resolution LWA1 data are freely accessible via Autoplot (http://autoplot.org) by accepting the data usage policy (http://space.physics.uiowa.edu/earth/datapolicy.html) More information can be found at http://space.physics.uiowa.edu/earth/ | ||||
25 | radio | Kita | GMRT (India) | L-band | 25Mar2017 22-1 (IST) 26Mar2017 21-1 (IST) | Reduced data will be available upon request. | ||||
26 | radio | Ryabov / Zakharenko | UTR-2 (Ukraine) GURT(Ukraine) | Decametric emissions Spectrograms (8-33 MHz) Spectrograms (8-80 MHz) | Mar (26)-(27) 20:00(26)-03:05(27) UTC 17:49(27)-20:00(27) UTC 20:00(26)-04:20(27) UTC 17:49(27)-20:00(27) UTC | The data will be available upon request to V. Ryabov. | ||||
27 | ||||||||||
28 | Scheduled observations by Juno. | |||||||||
29 | ||||||||||
30 | Perijove 5 on is 2017 March 27, 8:51:52 UTC at Juno. System-III longitude = 184.9°W | |||||||||
31 | ||||||||||
32 | Period: Orbit 5 [MWR/tilt] (2017 March 26 – 2017 May 17) | |||||||||
33 | Instrument | Description | ||||||||
34 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||
35 | MWR | N/S scans near perijove longitude, not centered on nadir. | ||||||||
36 | UVS | TBD | ||||||||
37 | JunoCam | E/PO observations targeting features voted on by public. | ||||||||
38 | JIRAM | TBD | ||||||||
39 | ||||||||||
40 | ||||||||||
41 | ||||||||||
42 | ||||||||||
43 | ||||||||||
44 | ||||||||||
45 | ||||||||||
46 | ||||||||||
47 | ||||||||||
48 | ||||||||||
49 | ||||||||||
50 | ||||||||||
51 | ||||||||||
52 | ||||||||||
53 | ||||||||||
54 | ||||||||||
55 | ||||||||||
56 | ||||||||||
57 | ||||||||||
58 | ||||||||||
59 | ||||||||||
60 | ||||||||||
61 | ||||||||||
62 | ||||||||||
63 | MWR footprints for the minimum emission angles at each latitude | |||||||||
64 | ||||||||||
65 | ||||||||||
66 | ||||||||||
67 | ||||||||||
68 | ||||||||||
69 | ||||||||||
70 | ||||||||||
71 | ||||||||||
72 | ||||||||||
73 | ||||||||||
74 | ||||||||||
75 | ||||||||||
76 | ||||||||||
77 | ||||||||||
78 | ||||||||||
79 | ||||||||||
80 | ||||||||||
81 | ||||||||||
82 | ||||||||||
83 | ||||||||||
84 | ||||||||||
85 | ||||||||||
86 | ||||||||||
87 | ||||||||||
88 | ||||||||||
89 | ||||||||||
90 | ||||||||||
91 | ||||||||||
92 | ||||||||||
93 | ||||||||||
94 | ||||||||||
95 | ||||||||||
96 | ||||||||||
97 | ||||||||||
98 | ||||||||||
99 | ||||||||||
100 | ||||||||||
101 | ||||||||||
102 | ||||||||||
103 | ||||||||||
104 | ||||||||||
105 | ||||||||||
106 | ||||||||||
107 | ||||||||||
108 | ||||||||||
109 | ||||||||||
110 | ||||||||||
111 | ||||||||||
112 | ||||||||||
113 | ||||||||||
114 | ||||||||||
115 | ||||||||||
116 | ||||||||||
117 | ||||||||||
118 | ||||||||||
119 | Composite of JIRAM M-band (5-micron) map. | |||||||||
120 | ||||||||||
121 | ||||||||||
122 | ||||||||||
123 | ||||||||||
124 | ||||||||||
125 | ||||||||||
126 | ||||||||||
127 | ||||||||||
128 | ||||||||||
129 | ||||||||||
130 | ||||||||||
131 | ||||||||||
132 | ||||||||||
133 | ||||||||||
134 | ||||||||||
135 | ||||||||||
136 | ||||||||||
137 | ||||||||||
138 | ||||||||||
139 | ||||||||||
140 | ||||||||||
141 | ||||||||||
142 | ||||||||||
143 | ||||||||||
144 | ||||||||||
145 | ||||||||||
146 | ||||||||||
147 | ||||||||||
148 | ||||||||||
149 | ||||||||||
150 | ||||||||||
151 | ||||||||||
152 | ||||||||||
153 | ||||||||||
154 | ||||||||||
155 | ||||||||||
156 | ||||||||||
157 | ||||||||||
158 | ||||||||||
159 |
1 | Observations requested. | ||||||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
2 | Period: Orbit 4 [MWR] (2017 February 1 – 2017 March 26) | Observations planned / granted time | |||||||||||||||
3 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | Observations successful | ||||||||||
4 | X-ray | Caitriona Jackman | Chandra | 72 ks (20 hours) continuous observation by Chandra HRC-I around apojove | 02/28/2017 12:40 - 03/01/2017 09:18 | Request to Jackman. Keen to collaborate with Juno team as contemporaneous in situ data will help to constrain the X-ray drivers thought to map to this region | Observations cancelled or unsuccessful | ||||||||||
5 | X-ray | Gladstone | Chandra | ~10 hours of HRC-I observations of Jupiter | 02/02/2017 09:58-19:42 | publicly available 2/8/2018 | |||||||||||
6 | HST FUV | Grodent | HST STIS | UV aurora | HST/UT start time mm/dd/yyyy hh:mm:ss Exp. time ~ 47min 02/01/2017 12:20:26 02/02/2017 09:13:40 02/02/2017 10:31:21 02/02/2017 09:01:03 02/02/2017 13:46:13 02/02/2017 15:21:35 02/02/2017 16:57:53 01/31/2017 07:43:57 02/03/2017 08:50:35 02/03/201713:36:40 02/04/2017 08:41:03 02/04/2017 10:16:26 02/05/2017 06:56:14 02/06/2017 11:32:56 03/01/2017 15:54:00 03/05/2017 18:26:00 03/17/2017 08:36:00 03/18/2017 14:50:00 03/19/2017 09:54:00 03/20/2017 16:06:00 03/21/2017 11:11:00 03/21/2017 12:46:00 03/22/2017 07:51:00 03/23/2017 12:27:00 03/23/2017 14:03:00 03/24/2017 09:07:00 03/25/2017 05:47:00 03/26/2017 15:10:00 03/27/2017 03:53:00 03/27/2017 05:28:00 03/27/2017 07:03:00 03/27/2017 08:39:00 03/27/2017 10:14:00 03/27/2017 11:49:00 03/27/2017 13:25:00 | As of Feb 15, 2017 Times may change by re-scheduling on the part of HST | |||||||||||
7 | visible/NUV | Wong | HST/WFC3 UVIS | hi-resolution map of perijove track, global map pair | Start time: 2017-Feb-01 15:28:47 UT, End time: 2017-Feb-02 12:53:50 UT | https://archive.stsci.edu/prepds/wfcj/ https://dx.doi.org/10.1016/j.icarus.2017.06.007 | |||||||||||
8 | CCD | Irwin | VLT/MUSE - IFU | spectroscopic imaging, 465-930 nm to determine cloud structure and albedo spectrum of particles. | 24/25 March 2017 | Raw data publicly available to download from ESO portal. Additional geometric calibration is needed to calibrate these observations on top of the standard calibration pipeline. | |||||||||||
9 | CCD (Visible) | Chanover | APO | Hyperspectral image cubes, 470-950 nm | Feb 2-3 | Some photometric cubes | |||||||||||
10 | VIS (R,G,B), >720nm,889nm | S. Poshyachinda, C. Go and T. Santikunaporn | Thailand National Observatory 2.4m and 0.7m Telescopes | Imaging in Visible Light, Near IR and Methand Band for PJ3. Jan 31-Feb 1 with the 2.4m and on Feb 2 with the 0.7m. Imaging the region 10hrs before and 10hrs after PJ3. | Jan 31, Feb 1 and Feb 2 | ||||||||||||
11 | Visible | Schmidt | Apache Point Observatory / Dual Imaging Spectrograph (DIS) | Long-slit visible spectroscopy of both sides of the Io torus to determine S+, S++, O+ composition and electron density | 2/12/2017, 3/09/2017, 3/23/2017, 3/24/2017 | Calibrated data products available upon request | Q | ||||||||||
12 | near IR | O’Donoghue | Keck / NIRSpec | high-resolution scanning spectroscopy of H3+ auroral emission for temperature mapping. | Feb 1: Good observations obtained. | Building up long-term dataset of Jupiter's northern and southern aurorae | |||||||||||
13 | near IR | Johnson | IRTF/iSHELL | imaging and high-resolution spectroscopy of H3+ emission | Taken Feb 2, 3:30-9:00 HST --> clear skies, successful guiding. Several sucessful scans were taken of the southern aurora simultaneously with Juno. Images taken in varies filters. | Data reduction in process | |||||||||||
14 | near IR | Kita | IRTF/iSHELL | imaging and high-resolution spectroscopy of H3+ emission | Mar 11, 23:00-3:00; Mar. 13, 23:59-04:00; Mar 16, 21:45-1:45; Mar. 18, 23:00-03:00; Mar. 21 1:00-5:00; Mar 23, 23:00 - 3:00 (Cloudy) | Reduced data will be available upon request. | Q | ||||||||||
15 | near IR | de Pater, Bjoraker | Keck/NIRSPEC; joint observations with Hubble Space Telescope Feb 1-2 | 5-µm spectra of NH3,H2O | Taken on Feb, 4, 5, 6 Feb 4 &6 data cover the longitude of PJ4 (277 degrees System III) | fully reduced spectra available in 2 months | |||||||||||
16 | near IR | Bjoraker | IRTF/iSHELL | high-resoution spectroscopy of Jupiter in the 5-µm window to determine NH3, H2O abundances and propeties of water clouds at similar locations and nearly the same time as Juno | Taken Mar 26 0:30-6:30 HST; good seeing & low humidity cover longitude of new PJ5: 187 System III | fully reduced spectra available in 2 months | |||||||||||
17 | near IR (5 µm) | Wong | Gemini-N/NIRI | lucky imaging, 5-µm maps | Start time: 2017-Feb-01 15:40:31 UT, End time: 2017-Feb-01 16:36:48 UT. Start time: 2017-Feb-05 14:12:48 UT, End time: 2017-Feb-05 16:15:43 UT. | ||||||||||||
18 | near IR | Orton | Gemini-N/NIRI | AO-stabilized imaging of Jupiter at several wavelengths | images obtained on service time Jan 30, Feb 5 | TBD | |||||||||||
19 | near IR | Orton | IRTF/SpeX | filtered imaging at several wavelengths between 1.58 and 5.1µm and spectral scanning over 2-µm and 5-µm ranges | Feb 2, 01:30-3:30 HST; Feb 3, 1:30-6:30 HST | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired. Reduced "quick-look" observations (geometrically but not radiometrically calibrated) will be available for immeduately use from the Juno-curated web site: http://junoirtf.space.swri.edu/ | |||||||||||
20 | near IR | Orton | IRTF/SpeX guide camera | filtered imaging at several near-infrared wavelengths, including H3+ emission at 3.14µm and thermal emission at 5.1 µm. | obtained on Feb 15, 3:20-4:00 HST; Feb 16, 05:30-6:30 HST; Feb 23, 4:50-5:30 HST; Feb 24, 3:20-4:00 HST; Mar 15, 2:00-2:45 HST; Mar 16 5:40-6:30 HST; Mar 22, 3:45-4:30 HST | raw images available immediately from IRTF web site. Reduced "quick-look" observations (geometrically but not radiometrically calibrated) will be available for immeduately use from the Juno-curated web site: http://junoirtf.space.swri.edu/ | |||||||||||
21 | mid IR | Fletcher | VLT / VISIR | filtered radiometric imaging to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology. | Observed Feb 5th (08:33-09:29UT) and Feb 6th (04:36-05:34UT). We have a northern and southern OB (100 minutes total), in addition to a single burst-mode M-band OB (20 minutes), totalling 120 minutes. | available in raw form in the ESO archive within 24 hours of acquisition; cylindrical maps within 1-2 days and reduced maps within a week | |||||||||||
22 | mid IR | Fletcher | VLT / VISIR | filtered radiometric imaging to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology. | Observed Mar 16, 3:34 -5:47 UT. | available in raw form in the ESO archive within 24 hours of acquisition; cylindrical maps within 1-2 days and reduced maps within a week | |||||||||||
23 | near IR | O’Donoghue | Keck / NIRSpec | high-resolution scanning spectroscopy of H3+ auroral emission for temperature mapping. | Mar 16: Good observations obtained. | Building up long-term dataset of Jupiter's northern and southern aurorae | |||||||||||
24 | mid IR | Flecher | Gemini N / TEXES | scanned spectral maps of Jupiter's disk at ten key spectral settings to derive upper-tropospheric and stratospheric temperatures, aerosol/cloud distributions, and distribution of tropospheric NH3 and PH3, and stratospheric C2H2 and C2H6. | scans of Jupiter completed, March 11-13 | raw data available almost immediately, calibrated files with geometry within a month, and retrieved properties potentially available within 1-2 weeks (subject to any unforeseen issues) | |||||||||||
25 | mid IR | Greathouse | Gemini N / TEXES | scanned high- and medium-resolution spectral maps of Jupiter's disk at key CH4- and H2-absorbing wavelengths to determine temperatures in the upper troposphere and stratosphere to determine the structure of non-seasonal thermal waves associated with the Quasi-Quadrennial Oscillation (QQO) | scans of Jupiter obtained in the March 10-21 time frame; initiated March 13 | raw data available in 2-3 days, reduced and remapped to lat/lon in 1 month (could be done faster if requested) | |||||||||||
26 | mid IR | Sinclair | Gemini N / TEXES | scanned high-resolution spectral maps of Jupiter's disk at six key spectral settings to derive stratospheric temperatures and 3-dimensional distribution of stratospheric C2H2, C2H4, C2H6 and H3+ in auroral regions. | scans of Jupiter obtained in the March 10-21 time frame; initiated March 13 (March 17, 18, 19) | Spectra of H2 S(1), CH4, C2H2, C2H4 and C2H6 obtained on March 17, 18, 19 providing nearly completely spatial coverage. Spectra and retrieved temperatures/abundances available from Sinclair upon request. Results are in preparation for publication. | |||||||||||
27 | sub-mm | Roth / Sanchez-Monge | IRAM NOEMA | Io SO2 atmosphere | One 5-h track obtained on Feb 11. Bad conditions, analysis ongoing. Additional observation on March14. | Request to Lorenz Roth | |||||||||||
28 | microwave | de Pater | Very Large Array (VLA) | Probably D configuration in D band 1.3 cm | Feb 1-2 | MWR PI Janssen is a Co-Investigator | |||||||||||
29 | radio | Zarka, Cecconi, Lamy, Louis | Nançay Decameter Array (France) | coordinated measurement of 10-40 MHz cyclotron radio emission | every day, 8 hours around the transition to local meridian | https://maser.lesia.obspm.fr/task-1-data-collections/juno-ground-radio/juno-ground-radio-nancay-decameter.html?lang=en | |||||||||||
30 | radio | Kita | GMRT (India) | L-band | Feb. 08 2:00-8:00IST | Reduced data will be available upon request. | |||||||||||
31 | radio | Imai | Long Wavelength Array 1 (LWA1) | Jupiter's decametric auroral radio observations | Feb 1-7, Mar 17-27 | Low-resolution LWA1 data are freely accessible via Autoplot (http://autoplot.org) by accepting the data usage policy (http://space.physics.uiowa.edu/earth/datapolicy.html) More information can be found at http://space.physics.uiowa.edu/earth/ | |||||||||||
32 | radio | Ryabov / Zakharenko | UTR-2 (Ukraine) GURT(Ukraine) URAN-2 (Ukraine) UTR-2 (Ukraine) GURT (Ukraine) | Decametric emissions Spectrograms Waveforms (8-33 MHz) Spectrograms (8-80 MHz) Spectrograms (8-33 MHz) Spectrograms (8-33 MHz) Waveforms (8-33 MHz) Spectrograms (8-80 MHz) | Feb (1)-(2) 23:00(1)-05:58(2) UTC 01:34-02:07(2) UTC 23:00(1)-06:47(2) UTC 06:08(2)-07:00(2) UTC Feb (2)-(3) 22:20(2)-5:50(3) UTC 00:12(3)-02:05(3) UTC 22:42(2)-01:50(3) UTC | The data will be available upon request to V. Ryabov. | |||||||||||
33 | |||||||||||||||||
34 | Scheduled observations by Juno. | ||||||||||||||||
35 | |||||||||||||||||
36 | Perijove is 2017 February 2, 12:57:09 UTC. System-III longitude = 274.9°W | ||||||||||||||||
37 | |||||||||||||||||
38 | Period: Orbit 4 [MWR] (2017 February 1 - March 26) | ||||||||||||||||
39 | Instrument | Description | |||||||||||||||
40 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | |||||||||||||||
41 | MWR | N/S scans near perijove longitude, centered on nadir. | |||||||||||||||
42 | UVS | TBD | |||||||||||||||
43 | JunoCam | E/PO observations targeting features voted on by public. | |||||||||||||||
44 | JIRAM | TBD | |||||||||||||||
45 | |||||||||||||||||
46 | Note: On this next orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed directly at the Earth. | ||||||||||||||||
47 | |||||||||||||||||
48 | |||||||||||||||||
49 | |||||||||||||||||
50 | |||||||||||||||||
51 | |||||||||||||||||
52 | |||||||||||||||||
53 | |||||||||||||||||
54 | |||||||||||||||||
55 | |||||||||||||||||
56 | |||||||||||||||||
57 | |||||||||||||||||
58 | |||||||||||||||||
59 | |||||||||||||||||
60 | |||||||||||||||||
61 | |||||||||||||||||
62 | |||||||||||||||||
63 | |||||||||||||||||
64 | |||||||||||||||||
65 | |||||||||||||||||
66 | |||||||||||||||||
67 | MWR footprints for the minimum emission angles at each latitude | ||||||||||||||||
68 | |||||||||||||||||
69 | |||||||||||||||||
70 | |||||||||||||||||
71 | |||||||||||||||||
72 | |||||||||||||||||
73 | |||||||||||||||||
74 | |||||||||||||||||
75 | |||||||||||||||||
76 | |||||||||||||||||
77 | |||||||||||||||||
78 | |||||||||||||||||
79 | |||||||||||||||||
80 | |||||||||||||||||
81 | |||||||||||||||||
82 | |||||||||||||||||
83 | |||||||||||||||||
84 | |||||||||||||||||
85 | |||||||||||||||||
86 | |||||||||||||||||
87 | |||||||||||||||||
88 | |||||||||||||||||
89 | |||||||||||||||||
90 | |||||||||||||||||
91 | |||||||||||||||||
92 | |||||||||||||||||
93 | |||||||||||||||||
94 | |||||||||||||||||
95 | Composite of JunoCam coverage. -John Rogers and Gerald Eichstaedt. | ||||||||||||||||
96 | |||||||||||||||||
97 | |||||||||||||||||
98 | |||||||||||||||||
99 | |||||||||||||||||
100 | |||||||||||||||||
101 | |||||||||||||||||
102 | |||||||||||||||||
103 | |||||||||||||||||
104 | |||||||||||||||||
105 | |||||||||||||||||
106 | |||||||||||||||||
107 | |||||||||||||||||
108 | |||||||||||||||||
109 | |||||||||||||||||
110 | |||||||||||||||||
111 | |||||||||||||||||
112 | |||||||||||||||||
113 | |||||||||||||||||
114 | |||||||||||||||||
115 | |||||||||||||||||
116 | |||||||||||||||||
117 | |||||||||||||||||
118 | |||||||||||||||||
119 | |||||||||||||||||
120 | |||||||||||||||||
121 | |||||||||||||||||
122 | |||||||||||||||||
123 | |||||||||||||||||
124 | |||||||||||||||||
125 | Composite of JIRAM M-band (5-micron) map. | ||||||||||||||||
126 | |||||||||||||||||
127 | |||||||||||||||||
128 | |||||||||||||||||
129 | |||||||||||||||||
130 | |||||||||||||||||
131 | |||||||||||||||||
132 | |||||||||||||||||
133 | |||||||||||||||||
134 | |||||||||||||||||
135 | |||||||||||||||||
136 | |||||||||||||||||
137 | |||||||||||||||||
138 | |||||||||||||||||
139 | |||||||||||||||||
140 | |||||||||||||||||
141 | |||||||||||||||||
142 | |||||||||||||||||
143 | |||||||||||||||||
144 | |||||||||||||||||
145 | |||||||||||||||||
146 | |||||||||||||||||
147 | |||||||||||||||||
148 | |||||||||||||||||
149 | |||||||||||||||||
150 | |||||||||||||||||
151 | |||||||||||||||||
152 | |||||||||||||||||
153 | |||||||||||||||||
154 | |||||||||||||||||
155 | |||||||||||||||||
156 | |||||||||||||||||
157 | |||||||||||||||||
158 | |||||||||||||||||
159 | |||||||||||||||||
160 | |||||||||||||||||
161 | |||||||||||||||||
162 | |||||||||||||||||
163 | Graphic of JIRAM coverage of the M-band (5-micron) channel, color-coded by emission angle. | ||||||||||||||||
164 | |||||||||||||||||
165 | |||||||||||||||||
166 | |||||||||||||||||
167 | |||||||||||||||||
168 | |||||||||||||||||
169 | |||||||||||||||||
170 | |||||||||||||||||
171 | |||||||||||||||||
172 | |||||||||||||||||
173 |
1 | Observations requested. | ||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|
2 | Observations planned / granted time | ||||||||||||
3 | Observations successful | ||||||||||||
4 | Observations cancelled or unsuccessful | ||||||||||||
5 | Period: Early Orbit 3 (2016 December 10 – 2017 January 1) | ||||||||||||
6 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | |||||||
7 | FUV | Grodent | HST/FUV-MAMA | high spatial and temporal resolution FUV observations of magnetosphere and ultraviolet auroras | 12/10/2016 18:58:50 12/11/2016 17:14:00 12/11 2016 19:18:02 12/11/2016 20:24:44 12/12/2016 17:03:59 12/12/2016 15:29:12 12/13/2016 12:10:09 12/14/2016 16:45:51 12/15/2016 08:39:04 | Times may change by re-scheduling on the part of HST. Animations of all visits are posted on http://www.lpap.ulg.ac.be/Juno/HST/PJ03.html. | |||||||
8 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | Continuous | ||||||||
9 | visible/NUV | Wong | HST/WFC3 UVIS | hi-resolution map of perijove track, global map pair | Start time: Dec 11 08:00:24 UT, End time: Dec 12 09:49:14 UT | https://archive.stsci.edu/prepds/wfcj/ https://dx.doi.org/10.1016/j.icarus.2017.06.007 | |||||||
10 | CCD | Sanchez-Lavega | Aulo EspaZio Gela, Bilbao, Spain | continuous imaging survey, 0.38-0.9 microns | continuous | TBD | |||||||
11 | CCD | Irwin | VLT/MUSE - IFU | spectroscopic imaging, 465-930 nm to determine cloud structure and albedo spectrum of particles. | 30-minute observation sequence requested of Jupiter close the time of perijove passage that includes the perijove longitude | “reductions to photometrically-calibrated cubes can be done in a day or two if there is sufficient motivation!” | |||||||
12 | CCD (Visible) | Chanover | APO | Hyperspectral image cubes, 470-950 nm | Dec 14-16 | Majority non-photometric conditions | |||||||
13 | near IR | Orton | IRTF/SpeX guide camera | filtered imaging at 5 strategic wavelengths, including 5.1µm and 3.4µm (H3+ auroral emission); additional wavelengths imaged between 1.58 and 2.3 µm | obtained at high airmass Dec 13, PJ3 longitudes on the Earth-facing hemisphere; Dec 22 on opposite hemisphere with good seeing. | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired. Reduced "quick-look" observations (geometrically but not radiometrically calibrated) are available for immeduately use from the Juno-curated web site: http://junoirtf.space.swri.edu/ | |||||||
14 | near IR | Orton | IRTF/SpeX guide camera | filtered imaging at 9 strategic wavelengths, including 5.1µm and 3.4µm (H3+ auroral emission). | Dec 24 05:15-06:15; Dec 31 05:15-06:15, Jan 2 05:30-06:30, Jan 3 05:30-06:30, Jan 5 04:30-06:30 | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired | |||||||
15 | near IR | Johnson | IRTF/iSHELL | imaging and high-resolution spectroscopy of H3+ emission | Dec 11 03:15-09:15 --> no observations taken because of snow storm at Mauna Kea; Dec 28 04:15-10:15 (daylight observing) --> took H3+ spectra of the southern and northern aurora. Took some scans but no off-axis star was available and therefore the telescope drifted significantly. The weather was quite good, with some clouds quickly passing over the summit. | Data reduction in process | |||||||
16 | near IR | Bjoraker | IRTF/iSHELL | high-resoution spectroscopy of Jupiter in the 5-µm window to determine NH3, H2O abundances and propeties of water clouds at similar locations and nearly the same time as Juno | scheduled Dec 13 04:30-10:30 (daylight obs) | weathered out | |||||||
17 | near IR | Bjoraker | IRTF/iSHELL | high-resoution spectroscopy of Jupiter in the 5-µm window to determine NH3, H2O abundances and propeties of water clouds | good data obtained Dec 27 04:30-10:30, Dec 29 04:30-10:30 | fully reduced spectra 2 months after iSHELL_Tool data reduction package is released | |||||||
18 | near IR | Skrutskie | Fan Mountain / 31" FanCam | Io H and K band flux, disk integrated | Dec 22 9:10-10:20; Dec 29 11:10-12:10 | TBD | Q | ||||||
19 | near IR (5 µm) | Wong | Gemini-N/NIRI | lucky imaging, 5-µm maps | Start time: 2016-Dec-14 14:21:52 UT, End time: 2016-Dec-14 16:20:48 | ||||||||
20 | near IR (5 µm) | Wong | Gemini-N/NIRI | lucky imaging, 5-µm maps, near-global coverage | 1.5 hr each 27, 28, 29 Dec. | full maps available on junocam planning site within 2 weeks | |||||||
21 | near IR (1-2 µm) | Orton | Gemini-N/NIRI | AO-stabilized imaging of Jupiter at several wavelengths | moderately good data Dec 24 of longitudes east of the Great Red Spot; excellent data on Dec 28 of GRS environmenet and nominal PJ3 System III longitude. | TBD | |||||||
22 | mid IR | Fletcher | VLT / VISIR | filtered radiometric imaging to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology. | Observations acquired on Dec15: a northern and southern OB (100 minutes total), in addition to several M-band images without burst mode in early dawn twilight; repeated with full imaging on Dec 17 including M-band burst mode observations obtained with some GRS coverage but not PJ3 longitude; and M-band burst mode images acquired on Dec 18 | available in raw form in the ESO archive within 24 hours of acquisition; cylindrical maps within 1-2 days and reduced maps within a week. | |||||||
23 | mid IR | Fletcher | IRTF/TEXES | scanned spectral maps of Jupiter's disk at ten key spectral settings to derive upper-tropospheric and stratospheric temperatures, aerosol/cloud distributions, and distribution of tropospheric NH3 and PH3, and stratospheric C2H2 and C2H6. | obtained Dec 16 and 17, covering opposite hemispheres, but not in the best seeing conditions | raw data available almost immediately, calibrated files with geometry within a month, and retrieved properties potentially available within 1-2 weeks (subject to any unforeseen issues) | |||||||
24 | mid IR | Greathouse | IRTF/TEXES | scanned high- and medium-resolution spectral maps of Jupiter's disk at key CH4- and H2-absorbing wavelengths to determine temperatures in the upper troposphere and stratosphere to determine the structure of non-seasonal thermal waves associated with the Quasi-Quadrennial Oscillation (QQO) | awarded Dec 19 03:00-11:30, Dec 20 03:00-11:30 (both daylight observing) | TBD | |||||||
25 | mid IR | Encrenaz | IRTF/TEXES | scanned medium-resolution spectral maps of Jupiter's disk at key wavelengths to determine the distributions of gaseous NH3 and PH3 in Jupiter's troposphere | awarded Dec 16 11:30-14:30, Dec 17 11:30-14:30, Dec 21 15:00-19:30, Dec 22 15:00-19:30 (all daylight observing) | ||||||||
26 | mid IR | Sinclair | IRTF/TEXES | scanned high-resolution spectral maps of Jupiter's disk at six key spectral settings to derive stratospheric temperatures and 3-dimensional distribution of stratospheric C2H2, C2H4, C2H6 and H3+ in auroral regions. | awarded Dec 15 03:30-11:30, Dec 16 03:00-06:30. Daylight observing on Dec 15; Jan | Bad weather/high winds on December 15-16: data is very noisy | |||||||
27 | sub-mm | Roth / Sanchez-Monge | IRAM NOEMA | Io SO2 atmosphere | One 5-h track successdfully obtained on Dec 11. SO2 line detected | Request to Lorenz Roth | Q | ||||||
28 | microwave | de Pater | Very Large Array (VLA) | A configuration in X band (8-10 GHz) | observations successful on Dec 11 | MWR PI Janssen is a Co-Investigator | |||||||
29 | radio | Zarka, Cecconi, Lamy, Louis | Nançay Decameter Array (France) | coordinated measurement of 10-40 MHz cyclotron radio emission | every day, 8 hours around the transition to local meridian | https://maser.lesia.obspm.fr/task-1-data-collections/juno-ground-radio/juno-ground-radio-nancay-decameter.html?lang=en | |||||||
30 | radio | Imai | Long Wavelength Array 1 (LWA1) | Jupiter's decametric auroral radio observations | Dec 10-19 | Low-resolution LWA1 data are freely accessible via Autoplot (http://autoplot.org) by accepting the data usage policy (http://space.physics.uiowa.edu/earth/datapolicy.html) More information can be found at http://space.physics.uiowa.edu/earth/ | |||||||
31 | radio | Ryabov / Zakharenko | UTR-2 (Ukraine) | Decametric emissions Spectrograms Waveforms Spectrograms Waveforms (8-33 MHz) | Dec 11 01:08-10:00 UTC 01:08-05:49 UTC Dec 12 00:00-07:00 UTC 05:20-07:10 UTC | The data will be available upon request to V. Ryabov. | |||||||
32 | |||||||||||||
33 | Scheduled observations by Juno. | ||||||||||||
34 | |||||||||||||
35 | Perijove is 2016 December 11, 17:03:41 UTC. System-III longitude = 5.5°W | ||||||||||||
36 | |||||||||||||
37 | Period: Orbit 3 [GRAV] (2016 December 10 – 2017 January 31) | ||||||||||||
38 | Instrument | Description | |||||||||||
39 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | |||||||||||
40 | MWR | N/S scans near perijove longitude, not centered on nadir. | |||||||||||
41 | UVS | Scans of Jupiter’s aurora | |||||||||||
42 | JIRAM | No JIRAM data were taken during this period until a full sofware patch was created and tested in order to avoid the circumstances causing the safing event on PJ2. | |||||||||||
43 | JunoCam | No continuous imaging of Jupiter up to perijove. Close-up observations +-2 hours of perijove. Voting for 1-3 individual regions by public from Nov 25 to Dec 1. All observations successful, with some issues tested on PJ1 clarified. All data available on Mission Juno web site. | |||||||||||
44 | |||||||||||||
45 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with continuous monitoring of the high-gain antenna, which is pointed at the Earth through the perijove pass | ||||||||||||
46 | |||||||||||||
47 | |||||||||||||
48 | |||||||||||||
49 | |||||||||||||
50 | |||||||||||||
51 | |||||||||||||
52 | |||||||||||||
53 | |||||||||||||
54 | |||||||||||||
55 | |||||||||||||
56 | |||||||||||||
57 | |||||||||||||
58 | |||||||||||||
59 | |||||||||||||
60 | |||||||||||||
61 | |||||||||||||
62 | |||||||||||||
63 | |||||||||||||
64 | |||||||||||||
65 | |||||||||||||
66 | |||||||||||||
67 | |||||||||||||
68 | |||||||||||||
69 | |||||||||||||
70 | |||||||||||||
71 | |||||||||||||
72 | |||||||||||||
73 | |||||||||||||
74 | |||||||||||||
75 | |||||||||||||
76 | |||||||||||||
77 | |||||||||||||
78 | |||||||||||||
79 | |||||||||||||
80 | |||||||||||||
81 | |||||||||||||
82 | |||||||||||||
83 | |||||||||||||
84 | |||||||||||||
85 | |||||||||||||
86 | |||||||||||||
87 | |||||||||||||
88 | |||||||||||||
89 | |||||||||||||
90 | |||||||||||||
91 | |||||||||||||
92 | |||||||||||||
93 | |||||||||||||
94 | |||||||||||||
95 | |||||||||||||
96 | |||||||||||||
97 | |||||||||||||
98 | |||||||||||||
99 | |||||||||||||
100 | |||||||||||||
101 | |||||||||||||
102 | |||||||||||||
103 | |||||||||||||
104 | |||||||||||||
105 | |||||||||||||
106 | |||||||||||||
107 | Period: late Orbit 3 (2017 January 1 - 31): observations supporting Juno's original Perijoves 8 and 9 that investigator teams decided to retain | ||||||||||||
108 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | |||||||
109 | FUV | Grodent | HST/FUV-MAMA | high spatial and temporal resolution FUV observations of magnetosphere and ultraviolet auroras | 01/07/2017 01:57:08 01/07/2017 03:32:30 01/22/2017 15:31:08 01/23/2017 20:07:50 01/24/2017 15:11:42 01/24/2017 16:47:04 01/26 2017 18:04:03 01/27/2017 13:08:24 01/28/2017 09:48:08 01/29/2017 14:24:36 01/29/2017 15:59:58 | ||||||||
110 | CCD | Sanchez-Lavega | Aulo EspaZio Gela, Bilbao, Spain / 28-cm telescope | continuous imaging survey, 0.38-0.9 microns | 01/01, 01/03, 01/04, 01/05, 01/06, 01/07, 01/08 | Images available at PVOL2 and Aula EspaZio web page. | |||||||
111 | CCD | Sanchez-Lavega | Aula EspaZio Gela 36-cm telescope at Calar Alta Observatory | continuous imaging survey, Wavelengths: R, V, B, IR, R610, 890nm (methane), R610 | 01/13, 01/18 | Images available at PVOL2 and Aula EspaZio web page. | |||||||
112 | CCD | Irwin | VLT/MUSE - IFU | spectroscopic imaging, 480-930 nm to determine cloud structure and albedo spectrum of particles. | 9/10 January 2017 | Raw data publicly available to download from ESO portal. Standard calibration pipeline takes of the order of 1-3 days to complete. | |||||||
113 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | 30-minute observation sequence requested of Jupiter close the time of the former perijove passage that maximizes overlap with other investigations. | ||||||||
114 | visible/NUV | Wong | HST/WFC3 UVIS | hi-resolution map of perijove track | raw data available immediately from STScI archive; reduced maps and zonal wind profiles available within one month or potentially sooner; co-Is from MWR and JIRAM teams | Q | |||||||
115 | CCD / near IR | Sanchez-Lavega | Calar Alto 2.2-m telescope / PlanetCam | 0.38-1.5 micron imaging | scheduled 2017 Jan 11-18 | TBD | |||||||
116 | near IR | Orton | IRTF/SpeX guide camera | filtered imaging at 5 strategic wavelengths, including 5.1µm and 3.4µm (H3+ auroral emission). | Taken on Jan 23, 26: 05:30-06:30 Also supports Keck spectroscopy | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired | |||||||
117 | near IR | Kita | IRTF/iSHELL | K-band imaging and high-resolution spectroscopy of H3+ emission | 1/07 01:00-07:00 HST 1/08 01:00-07:00 HST 1/09 01:00-07:00 HST 1/11 01:00-07:00 HST | Reduced data will be available upon request. | |||||||
118 | near IR | Davies | Keck / NIRC2 | AO-stabilized imaging of Io at several wavelengths | Jan 3, 4, 7, 8 | TBD | |||||||
119 | near IR | Skrutskie | Fan Mountain / 31" FanCam | Io H and K band flux, disk integrated | Jan 30 07:42-08:46 UT | TBD | |||||||
120 | near IR | Schmidt | DCT IGRINS | Io H and K spectra R~40000 | Jan 14 09:26-10:34 UT Jan 21 11:20-12:28 UT | All night cancelled. Bad weather | Q | ||||||
121 | near IR | O'Donoghue | Keck/NIRSPEC | H3+ spectra approx 3-4µm, R~25000, 24'' slit aligned N/S | Jan 25 10:00-16:00 UT; Feb 2; March 17 | Building up long-term dataset of Jupiter's northern and southern aurorae. Full auroral coverage (in H3+ temperature/density/radiance, and partial global coverage). Paper 1 of 2 published (open access: https://www.nature.com/articles/s41586-021-03706-w) | |||||||
122 | 5-micron spectra | Bjoraker; de Pater | Keck/NIRSPEC | spectra of NH3,H2O | Taken on Jan 11 & 12. | fully reduced spectra available in 2 months | |||||||
123 | 5-micron spectra | de Pater; Bjoraker | Keck/NIRSPEC | 5-mu spectra, H2O, NH3 | Taken on Jan. 23, 24 | TBD | |||||||
124 | visible/uv | de Pater; Wong | HST WFC3 observations | contextual observations, coincident with Keck and VLA observations | Taken on Jan 11 & 12. | TBD | |||||||
125 | near IR (5 µm) | Wong | Gemini-N/NIRI | lucky imaging, 5-µm maps, global coverage | 3 hr 11 Jan, 2 hr 12 Jan, 23 Jan | full maps available on junocam planning site within 2 weeks | |||||||
126 | mid IR | Fletcher | VLT / VISIR | filtered radiometric imaging to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology. | Observations in 10 filters, Jan 10 2017, 07:23-08:26UT, immediately east of GRS, including mid-SEB outbreak. | available in raw form in the ESO archive within 24 hours of acquisition; cylindrical maps within 1-2 days and reduced maps within a week | |||||||
127 | mid IR | Fletcher | VLT / VISIR | filtered radiometric imaging to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology. | Observations in 10 filters, Jan 11, 07:20-0830UT, including M-band burst mode. Immediately west of GRS. | available in raw form in the ESO archive within 24 hours of acquisition; cylindrical maps within 1-2 days and reduced maps within a week | |||||||
128 | mid IR | Fletcher | IRTF/TEXES | scanned spectral maps of Jupiter's disk at ten key spectral settings to derive upper-tropospheric and stratospheric temperatures, aerosol/cloud distributions, and distribution of tropospheric NH3 and PH3, and stratospheric C2H2 and C2H6. | scans of Jupiter requested close to the perijove epoch Observed Jan 16 08:30-09:30, Jan 17 01:00-09:30 (both daylight observing), Jan 18 01:00-06:30 | raw data available almost immediately, calibrated files with geometry within a month, and retrieved properties potentially available within 1-2 weeks (subject to any unforeseen issues) | |||||||
129 | mid IR | Kasaba Orton | Subaru / COMICS | filtered radiometric imaging and spectroscopy to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology and auroral heating and chemistry. | mid-infrared imaging of Jupiter requested using a full set of filters close to the original PJ8 with observations on an adjacent night to map the comlementary hemisphere. Imaging made through breaks in clouds Jan 10,11 | would like to see agreement in place with Juno science team first and discussed at the workshop, but willing to share. | |||||||
130 | mid IR | Orton | Keck exchange time to use Subaru / COMICS | filtered radiometric imaging and spectroscopy to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology and auroral heating and chemistry. | mid-infrared imaging of Jupiter requested using a full set of filters close to the perijove time with observations on an adjacent night to map the comlementary hemisphere. Imaging and spectroscopy obtained under ideal conditions, January 12,13. | reduced observations available within 1-2 months; quick-look observations sooner | |||||||
131 | mid IR | Greathouse | IRTF/TEXES | scanned high- and medium-resolution spectral maps of Jupiter's disk at key CH4- and H2-absorbing wavelengths to determine temperatures in the upper troposphere and stratosphere to determine the structure of non-seasonal thermal waves associated with the Quasi-Quadrennial Oscillation (QQO) | awarded Jan 14 03:30-09:30, Jan 15 01:00-09:30, Jan 16 01:00-08:30 (all daylight observing) | ||||||||
132 | mid IR | Sinclair | IRTF/TEXES | scanned high-resolution spectral maps of Jupiter's disk at six key spectral settings to derive stratospheric temperatures and 3-dimensional distribution of stratospheric C2H2, C2H4, C2H6 and H3+ in auroral regions. | scans of Jupiter's polar regions requested within 1-2 days of the perijove passage, awarded Jan 18 06:30-09:30, Jan 19 01:00-09:30 (both daylight observing) | TBD | Q | ||||||
133 | mid IR | Encrenaz | IRTF/TEXES | scanned medium-resolution spectral maps of Jupiter's disk at key wavelengths to determine the distributions of gaseous NH3 and PH3 in Jupiter's troposphere | awarded Jan 20 12:00-18:30, Jan 21 12:00-18:30 (both daylight observing) | ||||||||
134 | mid IR | Orton | SOFIA/EXES | spatially resolved spectra along the central meridian for high-altitude temperature profile and HCN distribution. | 120-130 min on Jan 19/20 and 20/21 flithts. HCN observed at full request. Strong CH4 bands at high resolution covered only partially due to telescope pointing s/w failure and recovery on first night and slit placement confusion on second night. | TBD | |||||||
135 | submillimeter / millimeter | de Pater | Atacama Large Millimeter Array (ALMA) | 1 and 3 mm continuum | acquired Jan 3, 4 | TBD | |||||||
136 | microwave | de Pater | Very Large Array (VLA) | X band (8-12 GHz), A-config | acquired 11 Jan., coincident with former PJ8 | MWR PI Janssen is a Co-Investigator | |||||||
137 | radio | Imai | Long Wavelength Array 1 (LWA1) | Jupiter's decametric auroral radio observations | Jan 21-26, Jan 28-31 | Request to M. Imai More information can be found at http://www-pw.physics.uiowa.edu/earth/ | |||||||
138 | radio | Kita | GMRT (India) | L-band | Jan. 25 1:00-6:00IST | Reduced data will be available upon request. | |||||||
139 | |||||||||||||
140 | also maps with gemini; PI: Wong | ||||||||||||
141 | |||||||||||||
142 | |||||||||||||
143 | |||||||||||||
144 | |||||||||||||
145 | |||||||||||||
146 | |||||||||||||
147 | |||||||||||||
148 | |||||||||||||
149 | |||||||||||||
150 | |||||||||||||
151 | |||||||||||||
152 | |||||||||||||
153 | |||||||||||||
154 | |||||||||||||
155 | |||||||||||||
156 | |||||||||||||
157 | |||||||||||||
158 | |||||||||||||
159 | |||||||||||||
160 | |||||||||||||
161 | |||||||||||||
162 | |||||||||||||
163 | |||||||||||||
164 | |||||||||||||
165 |
1 | |||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|
2 | Period: Orbit 2 (2016 October 18 – December 9) | ||||||||||||
3 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | |||||||
4 | FUV | Grodent | HST/FUV-MAMA | high spatial and temporal resolution FUV observations of magnetosphere and ultraviolet auroras | 11/30/2016 15:47:26 11/30/2016 17:22:48 12/01/2016 17:13:28 12/01/2016 18:48:52 12/02/2016 17:03:31 12/02/2016 18:38:54 12/03/2016 13:43:56 12/04 2016 13:34:28 12/05/2016 19:46:26 12/05/2016 21:21:49 12/06/2016 14:51:43 12/06/2016 16:25:38 12/06/2016 18:01:00 12/07/2016 16:16:40 12/08/2016 11:21:03 12/09/2016 12:46:53 | Animations are routinely posted on: http://www.lpap.ulg.ac.be/Juno/HST/PJ03.html. | |||||||
5 | Visible | Kagitani/ Yoneda | Tohoku Univ. Haleakala 40cm / 60cm | Quasi-continous imaging of sodium nebula originating from Io | continuous as Hisaki/ EXCEED (UV/EUV) & IPRT (Synchrotron) through 2016 December | ||||||||
6 | CCD | Jackson | Boise State 16-inch | visible imaging, U, B, G, R | TBD | TBD | |||||||
7 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | Continuous | ||||||||
8 | near IR | Orton | IRTF/SpeX guide camera | filtered imaging 1.58-5.1µm (SpeX) to determine structure and distribution of clouds and aerosols. | SpeX images obtained on Oct 18,19, with some vignetting of the telescope beam coincident with the planned PJ2 Juno observations. SpeX images obtained on Nov 1, 2. Also Nov 29 with Bjoraker et al. | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner. Reduced "quick-look" observations (geometrically but not radiometrically calibrated) are available for immeduately use from the Juno-curated web site: http://junoirtf.space.swri.edu/ | |||||||
9 | near IR (1-2 µm) | Orton | Gemini-N/NIRI | AO-stabilized imaging of Jupiter at several wavelengths | Dec 6, 2008 | Observations were not be taken due to severe weather conditions at Mauna Kea | |||||||
10 | near IR | Orton | IRTF/SpeX guide camera | filtered imaging 480-950 nm (MORIS); 1.58-5.1µm and spectral scans: 0.8-2.5µm, 2.5-5.1µm (SpeX) to determine structure and distribution of clouds and aerosols. | awarded Dec 5 05:00-06:15, Dec 6 05:00-06:15, Dec 9 05:15-06:15, Dec 10 05:15-06:15 | Observations were not be taken due to severe weather conditions at Mauna Kea | |||||||
11 | near IR | Johnson | IRTF/iSHELL | imaging and high-resolution spectroscopy of H3+ emission | Nov 16 04:00-06:30 (clear skies, took some random spectra), Nov 30 04:05-07:05 (some high clouds which dissappeared but icy fog kept rolling in. We got some observations in between the fog and managed to try out Lp2 and 4 with slit widths 0.375'' and 4''. Took random spectra and one scan of the northern aurora.) | Data reduction in progress | |||||||
12 | near IR | Bjoraker | IRTF/iSHELL | high-resoution spectroscopy of Jupiter in the 5-µm window to determine NH3, H2O abundances and propeties of water clouds at similar locations and nearly the same time as Juno | completed Nov 15 06:05-12:05 Nov 18 06:05-12:05, also Nov 29 with SpeX (imaging and moderate-resolution spectroscopy) 06:05-12:05. Daylight observing. Dec 2 observations not taken due to snow at Mauna Kea. | awaiting iSHELL_Tool data reduction package | |||||||
13 | near IR | Skrutskie | Fan Mountain / 31" FanCam | Io H and K band flux, disk integrated | Nov 13 11:00-12:00 | TBD. | |||||||
14 | microwave | de Pater | Very Large Array (VLA) | A configuration in X band (8-10 GHz) | Observations obtained on 19 Oct., coincident IRTF observations | MWR PI Janssen is a Co-Investigator | |||||||
15 | radio | Zarka, Cecconi, Lamy, Louis | Nançay Decameter Array (France) | coordinated measurement of 10-40 MHz cyclotron radio emission | every day, 8 hours around the transition to local meridian | https://maser.lesia.obspm.fr/task-1-data-collections/juno-ground-radio/juno-ground-radio-nancay-decameter.html?lang=en | |||||||
16 | radio | Imai | Long Wavelength Array 1 (LWA1) | Jupiter's decametric auroral radio observations | Dec 5-8 | Request to M. Imai More information can be found at http://space.physics.uiowa.edu/earth/ | |||||||
17 | radio | Santos-Costa | LOFAR | LOFAR observations of Jupiter's electron belt at 50-190 MHz coorinated with Juno's in-situe and/or remote observations during Juno's final apoproach phase and first three orbits | four observation windows between May and November 2016 | no sooner than six months after data collection to allow observers and Juno team members to present / publish some preliminary observation results. | |||||||
18 | radio | Ryabov / Zakharenko | UTR-2 (Ukraine) | Decametric emissions Spectrograms (8-33 MHz) | Oct 19 06:30-11:00 UTC 13:00-14:00 UTC | The data will be available upon request to V. Ryabov. | |||||||
19 | CCD (Visible) | Chanover | APO | Hyperspectral image cubes, 470-950 nm | Nov 14-17 | Observed in November, when original PJ was supposed to take place | |||||||
20 | Observations by Juno. | Observations requested. | |||||||||||
21 | Observations planned / granted time | ||||||||||||
22 | The Perijove Reduction Maneuver (PRM) was not performed, due to issues involving sticking valves in the main engine. Due to a safing event just before PJ, no Juno data were taken except for gravity mapping. | Observations successful | |||||||||||
23 | Observations cancelled or unsuccessful | ||||||||||||
24 | Period: Orbit 2 (2016 October 18 – December 9) | ||||||||||||
25 | Instrument | Description | |||||||||||
26 | MAG, JADE, JEDI, WAVES | Some measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | |||||||||||
27 | MWR | No observations. | |||||||||||
28 | UVS | No observations. | |||||||||||
29 | JunoCam | No observations. | |||||||||||
30 | JIRAM | No observations. | |||||||||||
31 | |||||||||||||
32 | |||||||||||||
33 | |||||||||||||
34 | MWR footprint plan, but not executed | ||||||||||||
35 | |||||||||||||
36 | |||||||||||||
37 | |||||||||||||
38 | |||||||||||||
39 | |||||||||||||
40 | |||||||||||||
41 | |||||||||||||
42 | |||||||||||||
43 | |||||||||||||
44 | |||||||||||||
45 | |||||||||||||
46 | |||||||||||||
47 | |||||||||||||
48 | |||||||||||||
49 | |||||||||||||
50 | |||||||||||||
51 | |||||||||||||
52 | |||||||||||||
53 | |||||||||||||
54 | |||||||||||||
55 | |||||||||||||
56 | |||||||||||||
57 | |||||||||||||
58 | |||||||||||||
59 | |||||||||||||
60 | |||||||||||||
61 | |||||||||||||
62 | |||||||||||||
63 | |||||||||||||
64 | |||||||||||||
65 | |||||||||||||
66 | |||||||||||||
67 | |||||||||||||
68 | |||||||||||||
69 | |||||||||||||
70 | |||||||||||||
71 | |||||||||||||
72 | |||||||||||||
73 | |||||||||||||
74 | |||||||||||||
75 | |||||||||||||
76 | |||||||||||||
77 | |||||||||||||
78 | |||||||||||||
79 | |||||||||||||
80 | |||||||||||||
81 | |||||||||||||
82 | |||||||||||||
83 | |||||||||||||
84 | |||||||||||||
85 | |||||||||||||
86 | |||||||||||||
87 | |||||||||||||
88 | |||||||||||||
89 | |||||||||||||
90 | |||||||||||||
91 |
1 | Note: Jupiter may be too close to the sun for Earth-based observations during much of this period, except for daytime-capable observatories. | Observations requested. | ||||||||
---|---|---|---|---|---|---|---|---|---|---|
2 | Observations planned / granted time | |||||||||
3 | Period: Orbit 1 [C Orbit] (2016 August 26 – 2016 October 17) | Observations successful | ||||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | Observations cancelled or unsuccessful | |||
5 | Visible | Kagitani/ Yoneda | Tohoku Univ. Haleakala 40cm / 60cm | Quasi-continous imaging of sodium nebula originating from Io | continuous as Hisaki/ EXCEED (UV/EUV) & IPRT (Synchrotron) through 2016 December | |||||
6 | near IR | Orton | IRTF/SpeX guide camera | filtered imaging 1.58-5.1µm to determine structure and distribution of clouds and aerosols. | 1. Aug 26 19:30 - Aug 27 01:30 UTC (including a time frame observing the PJ1 longitude ~12.5 hours before PJ1) 2. Aug 27 19:30 - Aug 28 01:30 UTC including a time frame observing the PJ1 longitude ~8.5 hours after PJ1). Best observations were at 5.1 microns during period (1). Observing conditions in period (2) were extremely difficult, with only a single, low-SNR image obtained. | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired. Images all available without radiometric calibration at http://junoirtf.space.swri.edu/ | ||||
7 | radio | Santos-Costa | LOFAR | LOFAR observations of Jupiter's electron belt at 50-190 MHz coordinated with Juno's in-situ and/or remote observations during Juno's final approach phase and first three orbits | Observations obtained on Aug 27. | no sooner than six months after data collection to allow observers and Juno team members to present / publish some preliminary observation results. | ||||
8 | radio* | Kita | GMRT (India) | Synchrotron radio emission at L-band | Aug 27 09:30-11:30 | reduced data will be available upon request. Data reduction requires several months. | ||||
9 | radio | Ryabov / Zakharenko | UTR-2 (Ukraine) GURT (Ukraine) | Decametric emissions Spectrograms (8-33 MHz) (8-80 MHz) | Aug 27 08:00-17:00 UTC | The data will be available upon request to V. Ryabov | ||||
10 | radio | Zarka, Cecconi, Lamy, Louis | Nançay Decameter Array (France) | coordinated measurement of 10-40 MHz cyclotron radio emission | every day, 8 hours around the transition to local meridian | https://maser.lesia.obspm.fr/task-1-data-collections/juno-ground-radio/juno-ground-radio-nancay-decameter.html?lang=en | ||||
11 | Scheduled observations by Juno. | |||||||||
12 | ||||||||||
13 | Perijove is 2016 August 27, 12:50:44 UTC. System-III longitude = 95.8°W. | |||||||||
14 | ||||||||||
15 | Period: Orbit 1 [C Orbit] (2016 August 26 – 2016 October 17) | |||||||||
16 | Instrument | Description | ||||||||
17 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||
18 | MWR | N/S scans near perijove longitude, not centered on nadir - similar to GRAV-orbit scans | ||||||||
19 | UVS | Scans of Jupiter’s aurora Aug 27, 1:51 - 15:51. | ||||||||
20 | JIRAM | Imaging and spectra of Jupiter Aug 25 - 27, with spatial resolutions ~560 km to tens of km. | ||||||||
21 | JunoCam | Continuous imaging of Jupiter throughout this period, every ~15 minutes | ||||||||
22 | ||||||||||
23 | ||||||||||
24 | ||||||||||
25 | ||||||||||
26 | ||||||||||
27 | ||||||||||
28 | ||||||||||
29 | ||||||||||
30 | ||||||||||
31 | ||||||||||
32 | ||||||||||
33 | ||||||||||
34 | ||||||||||
35 | ||||||||||
36 | ||||||||||
37 | ||||||||||
38 | ||||||||||
39 | \ | |||||||||
40 | ||||||||||
41 | ||||||||||
42 | ||||||||||
43 | ||||||||||
44 | ||||||||||
45 | ||||||||||
46 | ||||||||||
47 | ||||||||||
48 | ||||||||||
49 | ||||||||||
50 | ||||||||||
51 | ||||||||||
52 | ||||||||||
53 | ||||||||||
54 | ||||||||||
55 | ||||||||||
56 | ||||||||||
57 | ||||||||||
58 | ||||||||||
59 | ||||||||||
60 | ||||||||||
61 | ||||||||||
62 | ||||||||||
63 | ||||||||||
64 | ||||||||||
65 | ||||||||||
66 | ||||||||||
67 | ||||||||||
68 | ||||||||||
69 | ||||||||||
70 | ||||||||||
71 | ||||||||||
72 | ||||||||||
73 | ||||||||||
74 | ||||||||||
75 | ||||||||||
76 | ||||||||||
77 | ||||||||||
78 | ||||||||||
79 | ||||||||||
80 | ||||||||||
81 | ||||||||||
82 | ||||||||||
83 | MWR footprints for the minimum emission angle at each latitude. | |||||||||
84 | ||||||||||
85 | ||||||||||
86 | ||||||||||
87 | ||||||||||
88 | ||||||||||
89 | ||||||||||
90 | ||||||||||
91 | ||||||||||
92 | ||||||||||
93 | ||||||||||
94 | ||||||||||
95 | ||||||||||
96 | ||||||||||
97 | ||||||||||
98 | ||||||||||
99 | ||||||||||
100 | ||||||||||
101 | ||||||||||
102 | ||||||||||
103 | ||||||||||
104 | ||||||||||
105 | ||||||||||
106 | ||||||||||
107 | ||||||||||
108 | ||||||||||
109 | ||||||||||
110 | Coverage by the JIRAM insturment M-band (5-micron), coded by emission angle. |
1 | ||||||||||
---|---|---|---|---|---|---|---|---|---|---|
2 | Period: Orbit 0 (2016 July 4 [JOI-1d] – 2016 August 25) | |||||||||
3 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | ||||
4 | FUV | Nichols | HST/STIS | imaging and spectroscopy of Jupiter’s auroral regions | observations made Jul 11-18 | data made available to Juno team asap; many are already Co-Is | ||||
5 | Visible | Kagitani/ Yoneda | Tohoku Univ. Haleakala 40cm / 60cm | Quasi-continous imaging of sodium nebula originating from Io | continuous as Hisaki/ EXCEED (UV/EUV) & IPRT (Synchrotron) through 2016 December | |||||
6 | CCD | Ip | Lulin 1-m/35-cm | UVBRI and CH4 filters | a few observations in July | raw data available in a couple of weeks | ||||
7 | near IR | Orton | IRTF/SpeX guide camera | filtered imaging at 5 strategic wavelengths, including 5.1µm and 3.4µm (H3+ auroral emission). | obtained during 60 min intervals on Jul 22; July 23 observing completely weathered out. | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired | ||||
8 | mid IR | Fletcher | VLT / VISIR | filtered radiometric imaging to map the temperature, minor constituent, and cloud distribution defining climatology, together with auroral heating and chemistry | July 27, 28, 31; August 1 | available in raw form in the ESO archive within 24 hours of acquisition; cylindrical maps within 1-2 days and reduced maps within a week | ||||
9 | radio | Zarka, Cecconi, Lamy, Louis | Nançay Decameter Array, NenuFAR, LOFAR (Nançay, France) UTR2, GURT, URAN (Kharkov, Ukraine); Future University Hakodate (Japan) Iitate, Tohoku U.; Awara, Fukui Technical U.; Agawa, Kochi National Coll. of Technology (Japan) LWA1 (New Mexico, USA) | coordinated measurement of 10-40 MHz cyclotron radio emission. For more information see: http://maser.lesia.obspm.fr/outils-services/juno-ground-radio/ | Observations made on Jul 23, 29, 30; Aug 5. See the web site for more details. Observations made on Jul 5. UTR-2 07:30 - 11:00 UTC GURT 07:15 - 15:00 UTC | Most observers intend to have their data immediately public , but some (e.g. Ukrainian) prefer to set up a private server that will deliver data on request. Data availability should be a matter of weeks or less. | ||||
10 | ||||||||||
11 | Scheduled observations by Juno. | |||||||||
12 | ||||||||||
13 | Note: All instruments will be powered on July 10, 0:00 UTC | |||||||||
14 | ||||||||||
15 | Orbits start at perijove minus one day. | |||||||||
16 | ||||||||||
17 | Perijove 2016 July 5, 02:47:38 UTC, System-III longitude = 32.8°W | |||||||||
18 | ||||||||||
19 | Period: Orbit 0 (2016 July 4 [JOI-1d] – 2016 August 25) | |||||||||
20 | Instrument | Description | ||||||||
21 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||
22 | MWR | On July 6, the MWR collected unresolved observations of Jupiter at a low data rate. | ||||||||
23 | MWR | The MWR observed at full rate during three concentrated periods totalling about 100 hours to make careful maps of its antenna beams using Jupiter as a bright, unresolved source. | ||||||||
24 | UVS | Scans of Jupiter’s aurora July 22-Aug 25: (Calibration on July 16 at 00:00) July 25 at 14:00, July 29 at 10:00, August 8 at 14:00 | ||||||||
25 | JIRAM | Observations to calibrate pointing and spin phase | ||||||||
26 | JunoCam | Continuous imaging of Jupiter throughout this period, starting 2016 July 10, every ~15 minutes | ||||||||
27 | ||||||||||
28 | ||||||||||
29 | ||||||||||
30 | ||||||||||
31 | ||||||||||
32 | ||||||||||
33 | ||||||||||
34 | ||||||||||
35 | ||||||||||
36 | ||||||||||
37 | ||||||||||
38 | ||||||||||
39 | ||||||||||
40 | ||||||||||
41 | ||||||||||
42 | ||||||||||
43 | ||||||||||
44 | ||||||||||
45 | ||||||||||
46 | ||||||||||
47 | ||||||||||
48 | ||||||||||
49 | ||||||||||
50 | ||||||||||
51 | ||||||||||
52 | ||||||||||
53 | ||||||||||
54 | ||||||||||
55 | ||||||||||
56 | ||||||||||
57 | ||||||||||
58 | ||||||||||
59 | ||||||||||
60 | ||||||||||
61 | ||||||||||
62 | ||||||||||
63 | ||||||||||
64 | ||||||||||
65 | ||||||||||
66 | ||||||||||
67 | ||||||||||
68 | ||||||||||
69 | ||||||||||
70 | ||||||||||
71 | ||||||||||
72 | ||||||||||
73 | ||||||||||
74 | ||||||||||
75 | ||||||||||
76 | ||||||||||
77 | ||||||||||
78 |
1 | Earth-Based Juno-Supporting Observations of Jupiter and Its Environment: | ||||||
---|---|---|---|---|---|---|---|
2 | |||||||
3 | |||||||
4 | |||||||
5 | Please take note of the following formatting guidlines | ||||||
6 | Observations are coded as follows: contemplated, proposed, awarded, completed, cancelled | ||||||
7 | |||||||
8 | We have a newsletter about Juno-supporting observations and related information for contributing scientists. | ||||||
9 | Please contact | emma.k.dahl@jpl.nasa.gov | to be added or removed from the mailing list. | ||||
10 | |||||||
11 | Note: availability of all data are subject to appropriate collaborative agreements between the observers and Juno team members. | ||||||
12 | |||||||
13 | HELPFUL LINKS | ||||||
14 | Instruments list | ||||||
15 | Trajectory Information | ||||||
16 | |||||||
17 | CHANGELOG | ||||||
18 | 2017 March 16 | The table has been revised up to observations scheduled through 2019 September 11, with any information about PJ4- through PJ8-supporting observations. - GO | |||||
19 | 2017 June 19 | Due to performance issues each perijove now has its separate table. - FT | |||||
20 | Added MWR footprint plots to PJ3 - PJ6 - FT | ||||||
21 | 2017 June 21 | Added helpful links; added "pigtail" plots. -FT | |||||
22 | Expanded sheets to PJ14 | ||||||
23 | 2017 August 25 | Added timing of subsequent potential PJs up to PJ33 | |||||
24 | 2018 July 12 | Updated timing of subsequent PJs up to 23 and potential PJs up to PJ35 | |||||
25 | 2019 Feb 14 | Added spreadsheets and pigtail plots for PJs up to PJ30 | |||||
26 | 2021 Feb 18 | Added proposed EM trajectory PJ's 35-77, subject to revision | |||||
27 | 2024 Feb 23 | PJs 56-76 updated w/ info from Marty Brennan | |||||
28 | 2024 Apr | Added tabs for PJ67-76 | |||||
29 | |||||||
30 | |||||||
31 | |||||||
32 | The mission has been approved for 53-day orbits. Blocks must still be created for those opportunities. | ||||||
33 | For the interim, a summary of the subsequent orbit perjoves is as follows: | ||||||
34 | Perijove | Date | SCET (UTC) | PJ lat. (centric) | PJ long. (Sys. III) | comments | |
35 | 1 | 2016 August 27 | 12:50:44 | 3.8 | 95.8 | ||
36 | 2 | 2016 October 19 | 18:10:54 | 4.7 | 347.7 | ||
37 | 3 | 2016 December 11 | 17:03:41 | 5.6 | 5.5 | S/C safing event | |
38 | 4 | 2017 February 2 | 12:57:09 | 6.6 | 274.9 | MWR orbit | |
39 | 5 | 2017 March 27 | 8:51:52 | 7.5 | 184.9 | MWR tilt orbit | |
40 | 6 | 2017 May 19 | 6:00:47 | 8.5 | 139.8 | GRAV orbit | |
41 | 7 | 2017 July 11 | 1:54:42 | 9.5 | 49.4 | MWR orbit | |
42 | 8 | 2017 September 1 | 21:48:50 | 10.4 | 319 | GRAV orbit | |
43 | 9 | 2017 October 24 | 17:42:31 | 11.3 | 228.4 | MWR tilt orbit | |
44 | 10 | 2017 December 16 | 17:56:59 | 12.2 | 295.3 | GRAV orbit | |
45 | 11 | 2018 February 7 | 13:51:30 | 13.1 | 205.1 | GRAV orbit | |
46 | 12 | 2018 April 1 | 9:45:43 | 13.9 | 114.6 | partial turn orbit | |
47 | 13 | 2018 May 24 | 5:39:51 | 14.8 | 24 | GRAV orbit | |
48 | 14 | 2018 July 16 | 5:17:22 | 15.7 | 68.7 | GRAV orbit | |
49 | 15 | 2018 Septmber 7 | 1:11:41 | 16.6 | 338.2 | GRAV orbit | |
50 | 16 | 2018 October 29 | 21:06:00 | 17.4 | 247.6 | GRAV orbit | |
51 | 17 | 2018 December 21 | 16:59:48 | 18.1 | 157 | GRAV orbit | |
52 | 18 | 2019 February 12 | 17:34:31 | 18.9 | 235.3 | GRAV orbit | |
53 | 19 | 2019 April 6 | 12:14:22 | 19.7 | 99.7 | MWR cross-track orbit | |
54 | 20 | 2019 May 29 | 8:08:18 | 20.3 | 9.1 | partial turn orbit | |
55 | 21 | 2019 July 21 | 4:02:43 | 21 | 278.6 | GRAV orbit | |
56 | 22 | 2019 September 12 | 3:40:44 | 21.7 | 323.3 | GRAV orbit | |
57 | 23 | 2019 November 3 | 22:18:14 | 22.5 | 186.2 | GRAV orbit | |
58 | 24 | 2019 December 26 | 17:36:13 | 22.9 | 73.3 | GRAV orbit | |
59 | 25 | 2020 February 17 | 17:51:55 | 23.5 | 140.6 | GRAV orbit | |
60 | 26 | 2020 April 10 | 13:47:40 | 24.1 | 50.5 | orbit attitude adjustment | |
61 | 27 | 2020 June 2 | 10:19:47 | 24.7 | 342.9 | GRAV orbit | |
62 | 28 | 2020 July 25 | 6:15:14 | 25.3 | 252.8 | GRAV orbit | |
63 | 29 | 2020 September 16 | 2:10:43 | 25.9 | 162.7 | GRAV orbit | |
64 | 30 | 2020 November 8 | 1:49:34 | 26.6 | 207.7 | GRAV orbit | |
65 | 31 | 2020 December 30 | 21:45:08 | 27.3 | 117.7 | GRAV orbit | |
66 | 32 | 2021 February 21 | 17:40:27 | 28 | 27.7 | GRAV orbit | |
67 | 33 | 2021 April 15 | 13:36:23 | 28.8 | 298 | GRAV orbit | |
68 | 34 | 2021 June 7 | 9:32:00 | 29.5 | 208.1 | GRAV orbit | |
69 | 35 | 2021 July 30 | 4:32:45 | 30.5 | 85.1 | GRAV orbit | |
70 | |||||||
71 | Extended Mission (proposed trajectory, subject to revision) | ||||||
72 | 34 | 2021 June 8 | 7:46:00 | 28.3 | 306.6 | GRAV orbit | |
73 | 35 | 2021 July 21 | 8:14:53 | 29.1 | 316.4 | GRAV orbit | |
74 | 36 | 2021 September 2 | 22:42:43 | 29.9 | 113.5 | GRAV orbit | |
75 | 37 | 2021 October 16 | 17:13:28 | 30.7 | 57.5 | GRAV orbit | |
76 | 38 | 2021 November 29 | 14:13:26 | 31.5 | 91.7 | GRAV orbit | |
77 | 39 | 2022 January 12 | 10:32:56 | 32.3 | 101.5 | GRAV orbit | |
78 | 40 | 2022 February 25 | 1:58:52 | 33.1 | 293.9 | GRAV orbit | |
79 | 41 | 2022 April 9 | 15:49:13 | 34 | 68.5 | GRAV orbit | |
80 | 42 | 2022 May 23 | 2:15:47 | 34.9 | 80 | GRAV orbit | |
81 | 43 | 2022 July 5 | 9:17:20 | 35.7 | 327.6 | GRAV orbit | |
82 | 44 | 2022 August 17 | 14:45:30 | 36.6 | 158.9 | GRAV orbit | |
83 | 45 | 2022 September 29 | 17:11:30 | 37.4 | 240 | GRAV orbit | |
84 | 46 | 2022 November 6 | 21:38:26 | 38.3 | 1.4 | GRAV orbit | |
85 | 47 | 2022 December 15 | 3:23:21 | 39.1 | 170.1 | GRAV orbit | |
86 | 48 | 2023 January 22 | 5:43:28 | 40.1 | 215.1 | GRAV orbit | |
87 | 49 | 2023 March 1 | 5:53:18 | 41 | 181.4 | GRAV orbit | |
88 | 50 | 2023 April 8 | 9:46:25 | 41.9 | 282.6 | GRAV orbit | |
89 | 51 | 2023 May 16 | 7:31:53 | 42.8 | 161.7 | GRAV orbit | |
90 | 52 | 2023 June 23 | 6:55:03 | 43.7 | 99.8 | GRAV orbit | |
91 | 53 | 2023 July 31 | 9:05:42 | 44.5 | 139.2 | GRAV orbit | |
92 | 54 | 2023 September 7 | 11:58:02 | 45.4 | 203.9 | GRAV orbit | |
93 | 55 | 2023 October 15 | 10:53:00 | 46.2 | 125.1 | GRAV orbit | |
94 | 56 | 2023 November 22 | 12:17:18 | 47.1 | 117.6 | GRAV orbit | *2-23-24: PJs 56-76 updated by Emma Dahl w/ info from Marty Brennan |
95 | 57 | 2023 December 30 | 12:36:21 | 47.4 | 88.7 | GRAV orbit | |
96 | 58 | 2024 February 3 | 21:47:29 | 48.5 | 289.7 | GRAV orbit | |
97 | 59 | 2024 March 7 | 15:42:51 | 49.4 | 355.9 | GRAV orbit | |
98 | 60 | 2024 April 9 | 8:48:18 | 50.4 | 32.9 | GRAV orbit | |
99 | 61 | 2024 May 12 | 3:38:37 | 51.3 | 132.8 | GRAV orbit | |
100 | 62 | 2024 June 13 | 19:53:47 | 52.2 | 138.9 | GRAV orbit | |
101 | 63 | 2024 July 16 | 14:33:56 | 53.1 | 232.6 | GRAV orbit | |
102 | 64 | 2024 August 18 | 6:57:05 | 54 | 243.4 | GRAV orbit | |
103 | 65 | 2024 September 20 | 2:28:50 | 54.9 | 8.3 | GRAV orbit | |
104 | 66 | 2024 October 22 | 18:10:59 | 55.8 | 354.3 | GRAV orbit | |
105 | 67 | 2024 November 24 | 13:05:24 | 56.6 | 96.5 | GRAV orbit | |
106 | 68 | 2024 December 27 | 5:22:27 | 57.5 | 103.6 | GRAV orbit | |
107 | 69 | 2025 January 28 | 23:05:08 | 58.4 | 162.4 | GRAV orbit | |
108 | 70 | 2025 March 2 | 16:04:28 | 59.3 | 195 | GRAV orbit | |
109 | 71 | 2025 April 4 | 9:30:50 | 60.1 | 243.9 | GRAV orbit | |
110 | 72 | 2025 May 7 | 3:01:28 | 61 | 295.3 | GRAV orbit | |
111 | 73 | 2025 June 8 | 20:30:45 | 61.8 | 346 | GRAV orbit | |
112 | 74 | 2025 July 11 | 13:40:11 | 62.7 | 24.5 | GRAV orbit | |
113 | 75 | 2025 August 13 | 7:06:46 | 63.5 | 73.4 | GRAV orbit | |
114 | 76 | 2025 September 14 | 23:42:30 | 64.24 | 91.5 | GRAV orbit | |
115 | 77 | 2025 October 20 | 15:31:07 | 65 | 210.9 | GRAV orbit | ** this final orbit waasn't in Marty's sheet - is PJ77 not happening? |
116 | |||||||
117 | |||||||
118 | |||||||
119 | |||||||
120 | |||||||
121 | |||||||
122 | |||||||
123 | |||||||
124 | |||||||
125 | |||||||
126 | |||||||
127 | |||||||
128 | |||||||
129 | |||||||
130 | |||||||
131 | |||||||
132 | |||||||
133 | |||||||
134 | |||||||
135 | |||||||
136 | |||||||
137 | |||||||
138 | |||||||
139 | |||||||
140 | |||||||
141 | |||||||
142 | |||||||
143 | |||||||
144 | |||||||
145 | |||||||
146 | |||||||
147 | |||||||
148 | |||||||
149 | |||||||
150 | |||||||
151 | |||||||
152 | |||||||
153 | |||||||
154 | |||||||
155 | |||||||
156 | |||||||
157 | |||||||
158 | |||||||
159 | |||||||
160 | |||||||
161 | |||||||
162 | |||||||
163 | |||||||
164 | |||||||
165 | |||||||
166 | |||||||
167 | |||||||
168 | |||||||
169 | |||||||
170 | |||||||
171 | |||||||
172 | |||||||
173 | |||||||
174 | |||||||
175 | |||||||
176 | |||||||
177 | |||||||
178 | |||||||
179 | |||||||
180 | |||||||
181 | |||||||
182 | |||||||
183 | |||||||
184 | |||||||
185 | |||||||
186 | |||||||
187 | |||||||
188 | |||||||
189 | |||||||
190 | |||||||
191 | |||||||
192 | |||||||
193 | |||||||
194 | |||||||
195 | |||||||
196 | |||||||
197 | |||||||
198 | |||||||
199 | |||||||
200 | |||||||
201 | |||||||
202 | |||||||
203 | |||||||
204 | |||||||
205 | |||||||
206 | |||||||
207 | |||||||
208 | |||||||
209 | |||||||
210 | |||||||
211 | |||||||
212 | |||||||
213 | |||||||
214 | |||||||
215 | |||||||
216 | |||||||
217 | |||||||
218 | |||||||
219 | |||||||
220 | |||||||
221 | |||||||
222 | |||||||
223 | |||||||
224 | |||||||
225 | |||||||
226 | |||||||
227 | |||||||
228 | |||||||
229 | |||||||
230 | |||||||
231 | |||||||
232 | |||||||
233 | |||||||
234 | |||||||
235 | |||||||
236 | |||||||
237 | |||||||
238 | |||||||
239 | |||||||
240 | |||||||
241 | |||||||
242 | |||||||
243 | |||||||
244 | |||||||
245 | |||||||
246 | |||||||
247 | |||||||
248 | |||||||
249 | |||||||
250 | |||||||
251 | |||||||
252 | |||||||
253 | |||||||
254 | |||||||
255 | |||||||
256 | |||||||
257 | |||||||
258 | |||||||
259 | |||||||
260 | |||||||
261 | |||||||
262 | |||||||
263 | |||||||
264 | |||||||
265 | |||||||
266 | |||||||
267 | |||||||
268 | |||||||
269 | |||||||
270 | |||||||
271 | |||||||
272 | |||||||
273 | |||||||
274 | |||||||
275 | |||||||
276 | |||||||
277 | |||||||
278 | |||||||
279 | |||||||
280 | |||||||
281 | |||||||
282 | |||||||
283 | |||||||
284 | |||||||
285 | |||||||
286 | |||||||
287 | |||||||
288 | |||||||
289 | |||||||
290 | |||||||
291 | |||||||
292 | |||||||
293 | |||||||
294 | |||||||
295 | |||||||
296 | |||||||
297 | |||||||
298 | |||||||
299 | |||||||
300 | |||||||
301 | |||||||
302 | |||||||
303 | |||||||
304 | |||||||
305 | |||||||
306 | |||||||
307 | |||||||
308 | |||||||
309 | |||||||
310 | |||||||
311 | |||||||
312 | |||||||
313 | |||||||
314 | |||||||
315 | |||||||
316 | |||||||
317 | |||||||
318 | |||||||
319 | |||||||
320 | |||||||
321 | |||||||
322 | |||||||
323 | |||||||
324 | |||||||
325 | |||||||
326 | |||||||
327 | |||||||
328 | |||||||
329 | |||||||
330 | |||||||
331 | |||||||
332 | |||||||
333 | |||||||
334 | |||||||
335 | |||||||
336 | |||||||
337 | |||||||
338 | |||||||
339 | |||||||
340 | |||||||
341 | |||||||
342 | |||||||
343 | |||||||
344 | |||||||
345 | |||||||
346 | |||||||
347 | |||||||
348 | |||||||
349 | |||||||
350 | |||||||
351 | |||||||
352 | |||||||
353 | |||||||
354 | |||||||
355 | |||||||
356 | |||||||
357 | |||||||
358 | |||||||
359 | |||||||
360 | |||||||
361 | |||||||
362 | |||||||
363 | |||||||
364 | |||||||
365 | |||||||
366 | |||||||
367 | |||||||
368 | |||||||
369 | |||||||
370 | |||||||
371 | |||||||
372 | |||||||
373 | |||||||
374 | |||||||
375 | |||||||
376 | |||||||
377 | |||||||
378 | |||||||
379 | |||||||
380 | |||||||
381 | |||||||
382 | |||||||
383 | |||||||
384 | |||||||
385 | |||||||
386 | |||||||
387 | |||||||
388 | |||||||
389 | |||||||
390 | |||||||
391 | |||||||
392 | |||||||
393 | |||||||
394 | |||||||
395 | |||||||
396 | |||||||
397 | |||||||
398 | |||||||
399 | |||||||
400 | |||||||
401 | |||||||
402 | |||||||
403 | |||||||
404 | |||||||
405 | |||||||
406 | |||||||
407 | |||||||
408 | |||||||
409 | |||||||
410 | |||||||
411 | |||||||
412 | |||||||
413 | |||||||
414 | |||||||
415 | |||||||
416 | |||||||
417 | |||||||
418 | |||||||
419 | |||||||
420 | |||||||
421 | |||||||
422 | |||||||
423 | |||||||
424 | |||||||
425 | |||||||
426 | |||||||
427 | |||||||
428 | |||||||
429 | |||||||
430 | |||||||
431 | |||||||
432 | |||||||
433 | |||||||
434 | |||||||
435 | |||||||
436 | |||||||
437 | |||||||
438 | |||||||
439 | |||||||
440 | |||||||
441 | |||||||
442 | |||||||
443 | |||||||
444 | |||||||
445 | |||||||
446 | |||||||
447 | |||||||
448 | |||||||
449 | |||||||
450 | |||||||
451 | |||||||
452 | |||||||
453 | |||||||
454 | |||||||
455 | |||||||
456 | |||||||
457 | |||||||
458 | |||||||
459 | |||||||
460 | |||||||
461 | |||||||
462 | |||||||
463 | |||||||
464 | |||||||
465 | |||||||
466 | |||||||
467 | |||||||
468 | |||||||
469 | |||||||
470 | |||||||
471 | |||||||
472 | |||||||
473 | |||||||
474 | |||||||
475 | |||||||
476 | |||||||
477 | |||||||
478 | |||||||
479 | |||||||
480 | |||||||
481 | |||||||
482 | |||||||
483 | |||||||
484 | |||||||
485 | |||||||
486 | |||||||
487 | |||||||
488 | |||||||
489 | |||||||
490 | |||||||
491 | |||||||
492 | |||||||
493 | |||||||
494 | |||||||
495 | |||||||
496 | |||||||
497 | |||||||
498 | |||||||
499 | |||||||
500 | |||||||
501 | |||||||
502 | |||||||
503 | |||||||
504 | |||||||
505 | |||||||
506 | |||||||
507 | |||||||
508 | |||||||
509 | |||||||
510 | |||||||
511 | |||||||
512 | |||||||
513 | |||||||
514 | |||||||
515 | |||||||
516 | |||||||
517 | |||||||
518 | |||||||
519 | |||||||
520 | |||||||
521 | |||||||
522 | |||||||
523 | |||||||
524 | |||||||
525 | |||||||
526 | |||||||
527 | |||||||
528 | |||||||
529 | |||||||
530 | |||||||
531 | |||||||
532 | |||||||
533 | |||||||
534 | |||||||
535 | |||||||
536 | |||||||
537 | |||||||
538 | |||||||
539 | |||||||
540 | |||||||
541 | |||||||
542 | |||||||
543 | |||||||
544 | |||||||
545 | |||||||
546 | |||||||
547 | |||||||
548 | |||||||
549 | |||||||
550 | |||||||
551 | |||||||
552 | |||||||
553 | |||||||
554 | |||||||
555 | |||||||
556 | |||||||
557 | |||||||
558 | |||||||
559 | |||||||
560 | |||||||
561 | |||||||
562 | |||||||
563 | |||||||
564 | |||||||
565 | |||||||
566 | |||||||
567 | |||||||
568 | |||||||
569 | |||||||
570 | |||||||
571 | |||||||
572 | |||||||
573 | |||||||
574 | |||||||
575 | |||||||
576 | |||||||
577 | |||||||
578 | |||||||
579 | |||||||
580 | |||||||
581 | |||||||
582 | |||||||
583 | |||||||
584 | |||||||
585 | |||||||
586 | |||||||
587 | |||||||
588 | |||||||
589 | |||||||
590 | |||||||
591 | |||||||
592 | |||||||
593 | |||||||
594 | |||||||
595 | |||||||
596 | |||||||
597 | |||||||
598 | |||||||
599 | |||||||
600 | |||||||
601 | |||||||
602 | |||||||
603 | |||||||
604 | |||||||
605 | |||||||
606 | |||||||
607 | |||||||
608 | |||||||
609 | |||||||
610 | |||||||
611 | |||||||
612 | |||||||
613 | |||||||
614 | |||||||
615 | |||||||
616 | |||||||
617 | |||||||
618 | |||||||
619 | |||||||
620 | |||||||
621 | |||||||
622 | |||||||
623 | |||||||
624 | |||||||
625 | |||||||
626 | |||||||
627 | |||||||
628 | |||||||
629 | |||||||
630 | |||||||
631 | |||||||
632 | |||||||
633 | |||||||
634 | |||||||
635 | |||||||
636 | |||||||
637 | |||||||
638 | |||||||
639 | |||||||
640 | |||||||
641 | |||||||
642 | |||||||
643 | |||||||
644 | |||||||
645 | |||||||
646 | |||||||
647 | |||||||
648 | |||||||
649 | |||||||
650 | |||||||
651 | |||||||
652 | |||||||
653 | |||||||
654 | |||||||
655 | |||||||
656 | |||||||
657 | |||||||
658 | |||||||
659 | |||||||
660 | |||||||
661 | |||||||
662 | |||||||
663 | |||||||
664 | |||||||
665 | |||||||
666 | |||||||
667 | |||||||
668 | |||||||
669 | |||||||
670 | |||||||
671 | |||||||
672 | |||||||
673 | |||||||
674 | |||||||
675 | |||||||
676 | |||||||
677 | |||||||
678 | |||||||
679 | |||||||
680 | |||||||
681 | |||||||
682 | |||||||
683 | |||||||
684 | |||||||
685 | |||||||
686 | |||||||
687 | |||||||
688 | |||||||
689 | |||||||
690 | |||||||
691 | |||||||
692 | |||||||
693 | |||||||
694 | |||||||
695 | |||||||
696 | |||||||
697 | |||||||
698 | |||||||
699 | |||||||
700 | |||||||
701 | |||||||
702 | |||||||
703 | |||||||
704 | |||||||
705 | |||||||
706 | |||||||
707 | |||||||
708 | |||||||
709 | |||||||
710 | |||||||
711 | |||||||
712 | |||||||
713 | |||||||
714 | |||||||
715 | |||||||
716 | |||||||
717 | |||||||
718 | |||||||
719 | |||||||
720 | |||||||
721 | |||||||
722 | |||||||
723 | |||||||
724 | |||||||
725 | |||||||
726 | |||||||
727 | |||||||
728 | |||||||
729 | |||||||
730 | |||||||
731 | |||||||
732 | |||||||
733 | |||||||
734 | |||||||
735 | |||||||
736 | |||||||
737 | |||||||
738 | |||||||
739 | |||||||
740 | |||||||
741 | |||||||
742 | |||||||
743 | |||||||
744 | |||||||
745 | |||||||
746 | |||||||
747 | |||||||
748 | |||||||
749 | |||||||
750 | |||||||
751 | |||||||
752 | |||||||
753 | |||||||
754 | |||||||
755 | |||||||
756 | |||||||
757 | |||||||
758 | |||||||
759 | |||||||
760 | |||||||
761 | |||||||
762 | |||||||
763 | |||||||
764 | |||||||
765 | |||||||
766 | |||||||
767 | |||||||
768 | |||||||
769 | |||||||
770 | |||||||
771 | |||||||
772 | |||||||
773 | |||||||
774 | |||||||
775 | |||||||
776 | |||||||
777 | |||||||
778 | |||||||
779 | |||||||
780 | |||||||
781 | |||||||
782 | |||||||
783 | |||||||
784 | |||||||
785 | |||||||
786 | |||||||
787 | |||||||
788 | |||||||
789 | |||||||
790 | |||||||
791 | |||||||
792 | |||||||
793 | |||||||
794 | |||||||
795 | |||||||
796 | |||||||
797 | |||||||
798 | |||||||
799 | |||||||
800 | |||||||
801 | |||||||
802 | |||||||
803 | |||||||
804 | |||||||
805 | |||||||
806 | |||||||
807 | |||||||
808 | |||||||
809 | |||||||
810 | |||||||
811 | |||||||
812 | |||||||
813 | |||||||
814 | |||||||
815 | |||||||
816 | |||||||
817 | |||||||
818 | |||||||
819 | |||||||
820 | |||||||
821 | |||||||
822 | |||||||
823 | |||||||
824 | |||||||
825 | |||||||
826 | |||||||
827 | |||||||
828 | |||||||
829 | |||||||
830 | |||||||
831 | |||||||
832 | |||||||
833 | |||||||
834 | |||||||
835 | |||||||
836 | |||||||
837 | |||||||
838 | |||||||
839 | |||||||
840 | |||||||
841 | |||||||
842 | |||||||
843 | |||||||
844 | |||||||
845 | |||||||
846 | |||||||
847 | |||||||
848 | |||||||
849 | |||||||
850 | |||||||
851 | |||||||
852 | |||||||
853 | |||||||
854 | |||||||
855 | |||||||
856 | |||||||
857 | |||||||
858 | |||||||
859 | |||||||
860 | |||||||
861 | |||||||
862 | |||||||
863 | |||||||
864 | |||||||
865 | |||||||
866 | |||||||
867 | |||||||
868 | |||||||
869 | |||||||
870 | |||||||
871 | |||||||
872 | |||||||
873 | |||||||
874 | |||||||
875 | |||||||
876 | |||||||
877 | |||||||
878 | |||||||
879 | |||||||
880 | |||||||
881 | |||||||
882 | |||||||
883 | |||||||
884 | |||||||
885 | |||||||
886 | |||||||
887 | |||||||
888 | |||||||
889 | |||||||
890 | |||||||
891 | |||||||
892 | |||||||
893 | |||||||
894 | |||||||
895 | |||||||
896 | |||||||
897 | |||||||
898 | |||||||
899 | |||||||
900 | |||||||
901 | |||||||
902 | |||||||
903 | |||||||
904 | |||||||
905 | |||||||
906 | |||||||
907 | |||||||
908 | |||||||
909 | |||||||
910 | |||||||
911 | |||||||
912 | |||||||
913 | |||||||
914 | |||||||
915 | |||||||
916 | |||||||
917 | |||||||
918 | |||||||
919 | |||||||
920 | |||||||
921 | |||||||
922 | |||||||
923 | |||||||
924 | |||||||
925 | |||||||
926 | |||||||
927 | |||||||
928 | |||||||
929 | |||||||
930 | |||||||
931 | |||||||
932 | |||||||
933 | |||||||
934 | |||||||
935 | |||||||
936 | |||||||
937 | |||||||
938 | |||||||
939 | |||||||
940 | |||||||
941 | |||||||
942 | |||||||
943 | |||||||
944 | |||||||
945 | |||||||
946 | |||||||
947 | |||||||
948 | |||||||
949 | |||||||
950 | |||||||
951 | |||||||
952 | |||||||
953 | |||||||
954 | |||||||
955 | |||||||
956 | |||||||
957 | |||||||
958 | |||||||
959 | |||||||
960 | |||||||
961 | |||||||
962 | |||||||
963 | |||||||
964 | |||||||
965 | |||||||
966 | |||||||
967 | |||||||
968 | |||||||
969 | |||||||
970 | |||||||
971 | |||||||
972 | |||||||
973 | |||||||
974 | |||||||
975 | |||||||
976 | |||||||
977 | |||||||
978 | |||||||
979 | |||||||
980 | |||||||
981 | |||||||
982 | |||||||
983 | |||||||
984 | |||||||
985 | |||||||
986 | |||||||
987 | |||||||
988 | |||||||
989 | |||||||
990 | |||||||
991 | |||||||
992 | |||||||
993 | |||||||
994 | |||||||
995 | |||||||
996 | |||||||
997 | |||||||
998 | |||||||
999 | |||||||
1000 | |||||||
1001 | |||||||
1002 | |||||||
1003 | |||||||
1004 | |||||||
1005 | |||||||
1006 | |||||||
1007 |
1 | |||
---|---|---|---|
2 | |||
3 | This is the link to the edited video for the DPS 2023 Earth Observing Workshop: | ||
4 | please be patient, it takes a minute or two for the video to start streaming! | ||
5 | |||
6 | |||
7 | |||
8 | DPS 2023 Earth Observing Workshop | ||
9 | |||
10 | |||
11 | Chronological List of Speakers | ||
12 | Emma Dahl, Glenn Orton - hosts | ||
13 | |||
14 | Speaker | Title | |
15 | |||
16 | Scott Bolton | Welcome Intro | |
17 | Federico Tosi | Recent Updates on JIRAM Results Obtained at Jupiter's Moons | |
18 | Randy Gladstone | X-Ray Observations | |
19 | Björn Jónsson | Recent JunoCam Related Work | |
20 | Leigh Fletcher | Supporting Juno in the Mid-IR (JWST & Ground-Based) | |
21 | Kurt Retherford | HST + Webb - Juno Io Campaign: Connecting Volcanos to the Plasma Environment | |
22 | Jeff Morgenthaler | Trends in Material Flow into and out of Jupiter's Magnetosphere from Observations of the Io Plasma Torus by PSI's Io Input/Output Observatory (IoIO) | |
23 | John Rogers | Jupiter in 2022-23 as Viewed by Amateur Observers and by JunoCam | |
24 | Heidi Becker | Juno's Dark Side Perijoves & Multi-Instrument Lightning Campaign | |
25 | Tom Stallard | Simultaneous Observations of the Ionosphere from JWST, Juno PJ54, Keck, and IRTF | |
26 | Cheng Li | Juno MWR Results on Jupiter's Atmosphere | |
27 | Steve Levin | Juno Microwave Radiometer Non-Atmospheric Results | |
28 | Gerald Eichstädt | Behind the Obvious: In-situ Radiation Flux and Dose Data Collection with JunoCam | |
29 | " | JunoCam's Varying Linear White-Balancing Radiometric Factors | |
30 | J.D. Nichols | Hubble and Juno Observations of Jupiter's Auroras and Magnetospheric Dynamics during the Juno Extended Mission | |
31 | James Sinclair | Auroral-driven Enhanced Vertical Transport at Jupiter's Poles: Spatial and Temporal Variations in the CH4 Homopause Altitude | |
32 | Charlotte Alexander | Simplifying Cloud Models of Jupiter: Can We Have the Best of Both Worlds? | |
33 | Ramanakumar Sankar | Jovian Vortex Hunter: A Citizen Science Project to Study the Jovian Atmospheric Dynamics | |
34 | Carl Schmidt | Recent & Ongoing Keck Observations | |
35 | Paul Steffes | Radio Occultation Studies of Jupiter's Ionosphere and Atmosphere with the Juno Spacecraft | |
36 | Wanying Kang | What Can We Learn About an Icy Moon Ocean by Observing Its Ice Thickness Variation and Ice Drift Rate |
1 | ||||||||||
---|---|---|---|---|---|---|---|---|---|---|
2 | ||||||||||
3 | Period: Jupiter Approach (2015 November 1 – 2016 July 3 [JOI-2d] | |||||||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | ||||
5 | X-ray | Kraft | Chandra / HRC | GTO time awarded for approach science / Juno support | ~10hrs on May 24 and June 1 | |||||
6 | X-ray | Dunn | XMM | 160 ks (44.5 h) requested for approach science / Juno support | ~10hrs on May 17-18, and 24 | "very keen to partner with any willing Juno teams to share findings, enrich the analysis and inform what might cause any X-ray variations we observe" | ||||
7 | X-ray | Ezoe | Hitomi(Astro-H) | 100 ks during the Performance Verification phase | spacecraft anomaly leading to mission failure | no data | ||||
8 | FUV | Nichols | HST/STIS | imaging and spectroscopy of Jupiter’s auroral regions | observations acquired May 16, 17, 18, 18, 21, 22, 23, 24, 25, 26, 27, 28, 29, 30, 31; Jun 1, 2, 3, 4, 5, 6, 7, 22, 23, 24, 26, 27, 30 | data made available to Juno team asap; many are already Co-Is. Time-lapse images are available for download from ftp://ftp.ion.le.ac.uk/HST. | ||||
9 | FUV/ EUV | Kimura, Yoshikawa | Hisaki/ EXCEED | Spectroscopy of Jupiter UV aurura (total flux) and EUV spectrum of Io torus (spatially resolved) | continuous observations, 2015 Dec – 2016 Jun (except Mar 4 to Apr 21 and Apr 26 to May 4) 2016 Jan 21-31 2016 Feb 1-29 2016 Mar 1-3, 5-31 2016 Apr 13, 22-26 2016 May 4-31 2016 Jun 1-30 2016 Jul 1-8 | Data open to anyone joining that Hisaki team. Hisaki successfully observed EUV aurora and Io plasma torus during this phase, so any comparison with other data is welcomed. | ||||
10 | CCD | Simon | HST/WFC3 | Multiple-filtered imaging, 275-885 nm; two rotations of Jupiter to determine structure and properties of clouds and aerosols at high resolution, define atmospheric flow and search for waves. (Outer Planet Atmospheric Legacy [OPAL] program) | Images acquired on 2016 February 9-10 UTC. | |||||
11 | CCD | Irwin | VLT/MUSE - IFU | spectroscopic imaging, 480-930 nm to determine cloud structure and albedo spectrum of particles. | Spectral images acquired March 8-9 and March 31-April 2, providing global coverage of Jupiter | Calibration complete, raw data publicly available to download from ESO portal. First set of 31 March data obtained during cloudy conditions | ||||
12 | CCD | Sanchez-Lavega | Bilbao 11” Celestron with CCD | visible imaging, U, B, G, R + CH4 filters. Use “lucky imaging” to gain spatial resolution. | Observations made on April 18, 28, May 2, 3, 4, 9; June 7, 8, 20, 21, 27 | raw data available in 2-3 days, processed data available in a week if necessary (sooner if desired) | ||||
13 | CCD | Sanchez-Lavega | Calar Alto 2.2-m telescope, with PlanetCam camera | visible imaging, U, B, G, R + CH4 filters plus several bands between 1.0 and 1.7 microns, including J and H filterss. Use “lucky imaging” to gain spatial resolution. | good images from March 3/4, some images from March 6/7, good images from May 16/17, some images from 17/18 + 18/19 amid clouds, good images over the full spectral range May 19, 20; June 22, 23; July 1-4 | raw data available in 2-3 days, processed data available in a week if necessary (sooner if desired) | ||||
14 | CCD | Sanchez-Lavega | Calar Alto 2.2-m telescope, with Astralux camera | visible imaging, U, B, G, R + CH4 filters. Use “lucky imaging” to gain spatial resolution. | June 25, 26, 27 (bad seeing on June 27) | Raw data available in 2-3 days, processed data available in a week if necessary (sooner if desired), pending analysis to asses the results and quality (suspect nothing exceptional) | ||||
15 | CCD | Ip | Lulin 1-m/35-cm | UVBRI and CH4 filters | Apr 22, 23; Jun 17, 19, 21 | raw data available in a couple of weeks | ||||
16 | CCD | Chanover | Apache Point Observatory / Acoustical Optical Tunable Filter (APO/AOTF) | ~450-940 nm spatially resolved spectroscopy to determine cloud structure as linked to atmospheric dynamics. | one night successful during March 28-30 run | data being reduced | ||||
17 | CCD | Schneider | Apache Point Observatory / Dual Imaging Spectrograph (DIS) | Long-slit visible spectroscopy of both sides of the Io torus to determine S+, S++, O+ composition and electron density | acquired April 6, 14, 15. | calibrated data available on request | ||||
18 | CCD | Schmidt | McDonald Observatory IFU | Io's Neutral Na clouds, integral field echelle | acquired May 3, 4, 12 | available upon request | ||||
19 | CCD | Asada/Kagitani/Sakanoi | Tohoku Univ. Haleakala 60cm | Visible imaging, RGB, 750nm and CH4 filters | 24 Dec. 2015 - 30 May 2016, 20 Dec. 2016 - | |||||
20 | Visible | Kagitani/ Yoneda | Tohoku Univ. Haleakala 40cm / 60cm | Imaging observations of [SII](6716=6731A) emission in Io plasma torus with a 60-cm reflector. Sample data are on http://pparc.gp.tohoku.ac.jp/data/hal/qlMovie2.gif | continuous as Hisaki/ EXCEED (UV/EUV) & IPRT (Synchrotron) 2016 Jan 1, 4-5, 7-10 2016 Feb 5-6, 8-16, 18-28 2016 Mar 1-7, 9-22, 24-25, 28-31 2016 Apr 1-5, 7, 9-11 2016 May 12, 15-24, 27-30 2016 Jun 1-13, 16, 18-23, 26-29 2016 Jul 3, 5, 7-9 | |||||
21 | Visible | Kagitani/ Yoneda | Tohoku Univ. Haleakala 40cm / 60cm | Imaging observations of Na neublar originating from Io. Sample data are: http://pparc.gp/tohoku.ac.jp/data/hal/na_movie.gif | continuous as Hisaki/ EXCEED (UV/EUV) & IPRT (Synchrotron) observed on same nights as [SII] emission | |||||
22 | Visible | Kagitani/ Yoneda | Tohoku Univ. Haleakala 10cm attached to 40 cm | Quasi-continous imaging of sodium nebula originating from Io | Dec 23 2016 - July 2017 continuous as Hisaki/ EXCEED (UV/EUV) & IPRT (Synchrotron) observed on same nights as [SII] emission | |||||
23 | Near UV to Near IR | François Colas / JL Dauvergne / Marc Delcroix | Pic du Midi | T1M telescope | Several observations from 17 to 23 May | ASAP | ||||
24 | CCD + near IR | Sanchez-Lavega | Calar Alto 2.2m/ PlanetCam | Filtered imaging, 0.38 –1.7µm. Use “lucky imaging” to gain spatial resolution. | March 3/4 excellent seeing; good images covering the whole spectral range; March 6/7 bad seeing, some images available; May 16/17 - very good seeing with good images coveragin gthe whole spectral range; ay 17/18, 18/19 - partly cloudy with some imaging, May 19/20 excellent seeing with good images covering the whole spectral range | raw images available in a week, processed images in 2-3 weeks if necessary (sooner if desired, e.g. interesting targets, etc.) | ||||
25 | CCD + near IR | Sanchez-Lavega | Calar Alto 2.2m/ PlanetCam | Filtered imaging, 0.38 –1.7µm. Use “lucky imaging” to gain spatial resolution. | images acquired between 1.0 and 1.7 microns on July 1-4 | raw images available in a week, processed images in 2-3 weeks if necessary (sooner if desired, e.g. interesting targets, etc.) | ||||
26 | CCD + near IR | Orton | IRTF/MORIS, SpeX guide camera and spectrometer | filtered imaging 480-950 nm (MORIS); 1.58-5.1µm and spectral scans: 0.8-2.5µm, 2.5-5.1µm (SpeX) to determine structure and distribution of clouds and aerosols. | acquired: 2015 Nov 2-3, 2016 Jan 2-3 (no MORIS data) 2016 Feb 28-29 (with MORIS images on Feb 29) | raw data can be made available immediately; reduced images can be made available within a month (or sooner, as desired); reduced spectral scans available within 6 months (software for geometric reduction is under development) | ||||
27 | CCD+ near IR | Orton | IRTF/MORIS, SpeX guide camera and spectrometer | filtered imaging 480-950 nm (MORIS); 1.58-5.1µm and spectral scans: 0.8-2.5µm, 2.5-5.1µm (SpeX) to determine structure and distribution of clouds and aerosols. | SpeX imaging and scanned spectroscopy acquired on: 2016 May 11-12 UT. No MORIS data collected. Radiometrically uncalibrated images available on request. | raw data can be made available immediately; reduced images can be made available within a month (or sooner, as desired); reduced spectral scans available within 6 months (s/w for geometric reduction is under development) | ||||
28 | near IR | Orton | IRTF/SpeX guide camera | filtered imaging at: 1.58 µm (cloud albedo), 2.16 µm (upper-tropospheric particle field), 3.417 µm (H3+ auroral emission), 3.80 µm (mid-tropospheric particle field and H3+ auroral emission) and 5.10 µm (deep-tropospheric particle and gas distribution) | Images obtained and available from: Feb. 1, 4, 22, 23, 28, 29; Mar 2, 3, , 11, 12, 24; Apr 4, 25, 26; May 24, 25; Jun 4, 6, 18, 19 UT. | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired; images are scheduled to be uploaded and available on JSOC | ||||
29 | near IR | Orton | IRTF/SpeX guide camera | 3.8 and 5.1 micron imaging observations of Io | Feb 11, 22, 23 Mar 2, 3, 12 Apr 4 Jun 4, 6, 18, 19 | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired; images are available at http://junoirtf.space.swri.edu/. | ||||
30 | near IR | Johnson | IRTF /CSHELL | high-res. scanning spectroscopy of H3+ auroral emission. | observations obtained on February 3, 5, 10, 15, 17, 22, 27 and March 5. Good weather. | scanned images & possibly velocity maps, within 24 hrs; properly calibrated data will take longer; currently working on pipeline. | ||||
31 | near IR | Kita | IRTF / CSHELL | high-resolution spectroscopy of H3+ auroral emission for velocity-field measurements. | H3+ images and spectra obtained on April 22, 25; May 7, 9, 19, 21 Good weather. | would like to see agreement in place with Juno science team first and discussed at the workshop, but willing to share | ||||
32 | near IR | Kasaba Kita | Subaru / IRCS | AO-guided imaging/spectroscopy of H3+ emission with high spatial and spectral resolution. (using Galilean satellites as NGS) | K spectrum (H2 & H3+) on May 19, 21 H3+ image on May 19, 21, 24 BrAlpha image on May 24 | would like to see agreement in place with Juno science team first and discussed at the workshop, but willing to share. | ||||
33 | near IR | Kim | Gemini S/ Phoenix | 3-µm spectroscopy of auroral-related CH4, hydrocarbons. | No data on any of the nights granted for these observations between April 25 and May 20 were taken due to adverse weather conditions. | N/A | ||||
34 | near IR | O’Donoghue | Keck / NIRSpec | high-resolution scanning spectroscopy of H3+ auroral emission for temperature mapping. | Good observations obtained during the first half of April 13, 16, 19 and 22, with excellent coverage of the northern aurora. Some additional coverage of low-latitude ionosphere. | Data reduction pipeline built. Building up long-term dataset of Jupiter's northern and southern aurorae | ||||
35 | near IR | Bonfond | VLT / NACO | high spatial resolution imaging to determine detailed structure of H3+ emission, differentiating between the Io and Ganymede footprints, using Galilean satellites as NGS. | service observations successful on April 7 | will provide previews and preliminary results to Juno ASAP. Hard to commit to specific data products, but “I belong to the Juno science team.” | ||||
36 | near IR | Defrère | LBT / LMIRCAM + NOMIC (7.9 µm) | imaging of H2 and H3+ emission to identify the infrared counterpart of FUV auroral features, disentangle auroral precipitation effects from Joule-heating effects, and measure the short-timescale variability of polar-most emissions. | Feb 20: a few minutes of H- and K-band data; March 28: ~15 minutes of K and K band data of the north pole | “data available right away” | ||||
37 | near IR | de Kleer | Gemini N / NIRI+AO | near-IR imaging of volcanism on Io, 2–4µm | Observations have been collected on 31 nights using Kc-band and L'-band images, Jan 30; Feb 3, 4, 9, 11, 15-21, 23; Mar 11-14; Apr 30; May 1-4, 8-14, 16-20, 23-25, 27-28, 31; Jun15, 710, 12, 16-20, 24-25, 27. | observations are part of de Kleer’s thesis, but specific requests will be considered | ||||
38 | mid IR | Greathouse | IRTF / TEXES | scanning spectroscopy to determine structure of low-latitude vertical oscillations vs. time. | Acquired on 2015 Nov 11-14 and 2016 Jan 13 10:30-17:30 UT, Jan 14 10:30-17:30 UT, Jan 18 11:30-19:00 UT, Jan 19 9:30-18:00 UT, Jan 21 9:30-12:30 UT & 15:00-18:00 UT April 28 3:00-10:30 UT, April 29 2:00-10:30 UT, May 4 2:00-7:30 UT, May 7 2:00-8:30 UT | raw data available in 2-3 days, reduced and remapped to lat/lon in 1 month (could be done faster if requested) | ||||
39 | mid IR | Fletcher | IRTF / TEXES | scanning spectroscopy to determine temperature and minor-constituent distribution. | Global maps in multiple settings acquired as follows: 2015-Nov-16/18; 2016-Jan-16/17/20; 2016-Apr-30 to May-06 | raw data available almost immediately, calibrated files with geometry within a month, and retrieved properties potentially available within 1-2 weeks (subject to any unforeseen issues) | ||||
40 | mid IR | Encrenaz | IRTF / TEXES | scanning spectroscopy to determine PH3 and trace-constituent distribution (5 and 10 microns). | Acquired on 2015 Nov 16-18; 2016 Jan 15 16:30-17:30 UT, Jan 16 9:50-19:00 UT, Jan 17 9:50-17:50 UT, Jan 20 9:50-19:00 UT; April 30 2:00-3:30 UT, May 2 2:00-10:30 UT, May 3 2:00-10:30 UT, May 5 2:00-10:30 UT, May 6 2:00-10:30 UT | TBD | ||||
41 | mid IR | Retherford | IRTF / TEXES | Ionized Sulfur | Acquired 2016 Jan 15 10:00-16:00 UT, Jan 21 12:50-15:00 UT | |||||
42 | mid IR | Tsang | IRTF / TEXES | 19 micron SO2 monitoring of Io | Acquired 2016 April 30 3:30-10:30 UT | |||||
43 | mid IR | Kasaba Orton Sinclair | Subaru / COMICS | spectroscopy and imaging to map the stratospheric temperature and minor constituent distribution associated with polar auroral regions. | <done> 24-25 Jan 2016 | would like to see agreement in place with Juno science team first and discussed at the workshop, but willing to share; raw images available immediately & reduced images possibly within a month, depending on interest; raw spectra available quickly “on demand” | ||||
44 | mid IR | Fletcher | VLT / VISIR | filtered radiometric imaging to map the temperature, minor constituent, and cloud distribution defining climatology, together with auroral heating and chemistry | Global maps, 7-20 µm, on 2016 Feb 15-16, 2016 Mar 25-26. 5-µm lucky imaging test on 2016 Feb 26 with June 27 press release. Northern aurora in 8 filters 2016 May 19; global observations June 7-8/8-9. | available in raw form in the ESO archive within 24 hours of acquisition; cylindrical maps within 1-2 days and reduced maps within a week | ||||
45 | mid IR | Sinclair | IRTF / TEXES | spectroscopy to map the distribution of stratospheric temperatures and minor constituents associated with polar auroral regions. | data acquired during TEXES block: 2016 May 1 2:00-10:30 UT, May 4 7:30-10:30 UT | raw data available in 2-3 days, reduced and remapped to lat/lon in 1 month (could be done faster if requested); once that is done, existing software could produce results in 3-5 days. | ||||
46 | mid IR | Kostiuk | HIPWAC | ultra high-resolution spatially resolved spectroscopy of stratospheric emission lines in Jupiter’s polar regions | successful spatially resolved spectroscopy using HIPWAC at the IRTF: April 18-21 | TBD | ||||
47 | radio* | Lamy, Zarka, Cecconi | Nançay Decameter Array, NenuFAR, LOFAR (Nançay, France) UTR2 (Kharkov, Ukraine) Iitate, Tohoku U.; Awara, Fukui Technical U.; Agawa, Kochi National Coll. of Technology (Japan) LWA1 (New Mexico, USA) | coordinated measurement of 10-40 MHz cyclotron radio emission. NDA data are acquired 8 hours per day. For more information see: http://maser.lesia.obspm.fr/outils-services/juno-ground-radio/ | See the web site for more details. | Most observers intend to have their data immediately public , but some (e.g. Ukrainian) prefer to set up a private server that will deliver data only to Juno-related scientists. Data availability should be a matter of weeks or less. | ||||
48 | radio* | Imai | LWA1 (USA) NDA (France) UTR-2 (Kharkov, Ukraine) GURT (Kharkov, Ukraine) URAN-2 (Poltava, Ukraine) URAN-3 (Lviv, Ukraine) | Coordinated Jupiter's DAM emissions. More information can be found at: PDF: Coordinated LWA1-NDA-URAN2 Observations for Jupiter’s DAM Radiation https://drive.google.com/file/d/0B32DAVbuGRxGMGlYN24wNXZuVlU/view?usp=sharing * URAN3 has mostly participated in this campaign, while UTR-2 and GURT sometimes join. PDF: Coordinated NDA-URAN2 Observations for Jupiter’s DAM Radiation https://drive.google.com/file/d/0B32DAVbuGRxGWXg5ZjlpRmRBcGs/view?usp=sharing * This corresponds to NDA-UTR2-GURT-URAN Jupiter observation campaign. | Observations combining LWA1+NDA+URAN2 made on Jan 8, 9, 15, 16; Feb 10, 16, 17, 23, 24; Mar 20, 26, 27; Apr 2, 3, 15; May 3, 4, 10, 11; Jun 11, 12, 18, 20, 21. Observations combining NDA+UTR2+GURT+URAN made on Mar 18, 25; Apr 12, 13, 19, 20; May 10. | Reduced data will be available upon request. Data process requires several months. | ||||
49 | radio | Santos-Costa | LOFAR | LOFAR observations of Jupiter's electron belt at 50-190 MHz coordinated with Juno's in-situ and/or remote observations during Juno's final approach phase and first three orbits | Observations obtained on June 2, 15. | no sooner than six months after data collection to allow observers and Juno team members to present / publish some preliminary observation results. | ||||
50 | radio | Levin (contact point) | DSN | 2.3-GHz synchrotron radio emission | two continuous 24-hour observations desired, with actual allocation TBD, possibly “last-minute” | data availability TBD but likely within a few months, based on previous experience | ||||
51 | radio | Levin (contact point) | DSN | 2.3-GHz synchrotron radio emission | Jan 24, 17:10-02:45 Jan 27,18:30-02:45 Jan 31, 18:30-02:30 Feb 4, 18:45-01:00 Feb 6, 18:20-01:10 Feb 11, 20:00-01:45 Feb 13, 18:55-01:40 Feb 14, 20:00-01:20 Feb 18, 21:45-01:20 Feb 19, 20:20, 01:15 Feb 27, 17:50-23:35 Mar 1, 19:15-02:05 Mar 3, 21:40-00:25 Mar 11, 18:15-23:55 Mar 15, 19:30-23:25 Mar 17, 18:15-03:05 Apr 1, 16:35-22:30 Apr 23, 14:45-21:05 May 3, 20:00-00:00 May 7, 20:00-23:40 May 10, 19:35-23:30 May 15, 11:30-21:45 | data availability TBD but likely within a few months | ||||
52 | radio* | Levin (contact point) | GAVRT | 2.3-GHz synchrotron radio emission, monitored as public outreach by students | A query of GAVRT database tables shows that observations of Jupiter were made from DSS-13 on Apr 21, 27; May 4, 24, 25, 31; Jun 20, 29. Observations were made from DSS-28 on Apr 21, 27; May 4, 25, 31; Jun 2. There is no assurance that data from any date are useful for a particular purpose. They must be examined. | http://galileo.gavrt.org/seti/access/scan/dssData.php ; Raw data available to anyone who wants it. Processed data will eventually be available at the same website. Please acknowledge the GAVRT project if you use these data in a publication. | ||||
53 | radio* | Misawa Tsuchiya | Iitate Planetary radio Telescope (IPRT) | 325MHz (& 785MHz) synchrotron radio emission, continuous monitoring with a 31mx33m single dish telescope | Continuous !!! | data available by request | ||||
54 | radio* | Kita | GMRT (India) | Synchrotron radio emission at L-band | May 03 14:30-16:30 May 14 13:30-15:30 May 20 13:30-15:30 May 28 15:30-17:30 Jun 02 14:30-16:30 Jun 05 12:30-14:30 Jun 07 13:30-15:30 Jun 11 11:30-13:30 Jun 23 12:30-14:30 | Reduced data will be available upon request. Data reduction requires several months. | ||||
55 | radio | Horiuchi | DSN Canberra DSS43(70m) or DSS34/45(34m) | 2.3/8.4 GHz synchrotron and thermal radio emission | Jan 30 030 09:10-16:50 Feb 11 042 09:55-12:40 Feb 16 047 08:20-14:55 Feb 28 059 07:50-15:55 Feb 03 063 07:55-15:15 Feb 24 084 08:05-10:30 Feb 26 086 07:45-11:15 Feb 27 087 07:40-10:40 Feb 28 088 07:40-11:20 Feb 29 089 07:35-10:35 Mar 30 090 05:35-11:15 Apr 07 098 07:05-11:45 May 08 129 05:40-11:00 May 19 140 03:40-10:25 Jun 02 154 05:00-07:15 Jun 04 156 04:20-07:45 Jun 05 157 04:05-08:25 Jun 11 163 02:10-08:00 Jun 19 171 04:35-11:30 Jun 24 176 06:10-10:40 Jun 29 181 05:00-06:45 Jul 02 184 04:40-09:55 | TBD | ||||
56 | Optical | Acar, Ateş | İSTEK Belde Observatory 16" | Multi-color lucky imaging | 2017 Feb 2 Mar 27 May 18 Jul 10 Sep 2 Oct 25 | Processed frames will be uploaded to the ground base data collection server | ||||
57 | ||||||||||
58 | ||||||||||
59 | Instruments are listed at: https://voparis-juno.obspm.fr/juno/instruments/pub_json | |||||||||
60 | ||||||||||
61 | ||||||||||
62 | Period: Jupiter Approach (2015 November 1 – 2016 July 3 [JOI-2d] | |||||||||
63 | Instrument | Description | ||||||||
64 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period up to a few days before JOI. These sample properties of the solar wind impinging on Jupiter’s magnetosphere, starting from a distance of ~1AU up to sampling the magnetosphere itself. | ||||||||
65 | UVS | Scans of Jupiter’s aurora June 3-29: June 3 at 02:30, June 4 at 18:30, June 9 at 08:30, June 14 at 08:30, June 16 at 00:30, June 18 at 02:30, June 21 at 10:30, June 24 at 13:30, June 26 at 00:30, June 27 at 14:00 | ||||||||
66 | JunoCam | Continuous imaging of Jupiter June 12-29, every ~15 minutes to create an "approach movie". Some large features on Jupiter are resolvable, and the motions of Galilean satellites are prominent and striking. | ||||||||
67 | JIRAM | Observations of Jupiter in Band L and M were made on January 25 and February 9 | ||||||||
68 | MWR | Jupiter was observed during the approach phase at times when it passes through the spin plane of the MWR antennas (the great circle on the sky which is continuously scanned by the MWR antennas due to the rotation of the spacecraft). At these times the spacecraft is at a large distance from Jupiter, so it appears smaller that the MWR antenna beams and only the total emission from the planet and radiation belts is measured. These scans will confirm that the MWR antenna patterns have remained unchanged, and allow us to check our absolute radiometric calibrations by comparison with ground-based single-dish calibrated measurements of Jupiter's total flux. Consequently such observations are desired at frequencies comparable to the lowest three or four frequencies of the MWR (600 Mhz, 1.25, 2.6 and 5Ghz) around the times of MWR observations. | ||||||||
69 | ||||||||||
70 | ||||||||||
71 | ||||||||||
72 | ||||||||||
73 | ||||||||||
74 | ||||||||||
75 | ||||||||||
76 | ||||||||||
77 | ||||||||||
78 | ||||||||||
79 | ||||||||||
80 | ||||||||||
81 | ||||||||||
82 | ||||||||||
83 | ||||||||||
84 | ||||||||||
85 | ||||||||||
86 | ||||||||||
87 | ||||||||||
88 | ||||||||||
89 | ||||||||||
90 | ||||||||||
91 | ||||||||||
92 | ||||||||||
93 | ||||||||||
94 | ||||||||||
95 | ||||||||||
96 | ||||||||||
97 | ||||||||||
98 | ||||||||||
99 | ||||||||||
100 | ||||||||||
101 | ||||||||||
102 | ||||||||||
103 | ||||||||||
104 | ||||||||||
105 | ||||||||||
106 | ||||||||||
107 | ||||||||||
108 | ||||||||||
109 | ||||||||||
110 | ||||||||||
111 | ||||||||||
112 | ||||||||||
113 | ||||||||||
114 | ||||||||||
115 | ||||||||||
116 | ||||||||||
117 | ||||||||||
118 | ||||||||||
119 | ||||||||||
120 | ||||||||||
121 | ||||||||||
122 | ||||||||||
123 | ||||||||||
124 | ||||||||||
125 | ||||||||||
126 | ||||||||||
127 | ||||||||||
128 | ||||||||||
129 | ||||||||||
130 | ||||||||||
131 | ||||||||||
132 | ||||||||||
133 | ||||||||||
134 | ||||||||||
135 | ||||||||||
136 | ||||||||||
137 | ||||||||||
138 | ||||||||||
139 | ||||||||||
140 | ||||||||||
141 | ||||||||||
142 | ||||||||||
143 | ||||||||||
144 | ||||||||||
145 | ||||||||||
146 | ||||||||||
147 | ||||||||||
148 | ||||||||||
149 | ||||||||||
150 | ||||||||||
151 | ||||||||||
152 | ||||||||||
153 | ||||||||||
154 | ||||||||||
155 | ||||||||||
156 | ||||||||||
157 | ||||||||||
158 | ||||||||||
159 | ||||||||||
160 | ||||||||||
161 | ||||||||||
162 | ||||||||||
163 | ||||||||||
164 | ||||||||||
165 | ||||||||||
166 | ||||||||||
167 | ||||||||||
168 | ||||||||||
169 | ||||||||||
170 | ||||||||||
171 | ||||||||||
172 | ||||||||||
173 | ||||||||||
174 | ||||||||||
175 | ||||||||||
176 |
1 | Note: On this orbit the spacecraft orientation optimizes gravity mapping (GRAV) with the antenna pointed toward the Earth continuously. | |||||
---|---|---|---|---|---|---|
2 | ||||||
3 | Period: Orbit 8 [GRAV] (2017 August 30 – 2017 October 22) | |||||
4 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability |
5 | ||||||
6 | ||||||
7 | ||||||
8 | ||||||
9 | ||||||
10 | ||||||
11 | ||||||
12 | ||||||
13 | ||||||
14 | ||||||
15 | ||||||
16 | ||||||
17 | Scheduled observations by Juno. | |||||
18 | ||||||
19 | Perijove is 2017 July 11, 1:55:56 UTC. System-III longitude = 52°W | |||||
20 | ||||||
21 | Period: Orbit 8 (2017 July 10 – 2017 August 29) | |||||
22 | Instrument | Description | ||||
23 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||
24 | MWR | |||||
25 | UVS | |||||
26 | JunoCam | |||||
27 | JIRAM |
1 | |||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|
2 | Earth-Based Juno-Supporting Observations of Jupiter and Its Environment: | ||||||||||
3 | |||||||||||
4 | |||||||||||
5 | The table has been revised up to observations scheduled through 2019 September 11, with any information about PJ4- through PJ8-supporting observations. - Glenn Orton, 2017 March 16 | ||||||||||
6 | |||||||||||
7 | Observations are coded as follows: contemplated, proposed, awarded, completed, cancelled | ||||||||||
8 | |||||||||||
9 | Note: availability of all data are subject to appropriate collaborative agreements between the observers and Juno team members. | ||||||||||
10 | |||||||||||
11 | Period: Jupiter Approach (2015 November 1 – 2016 July 3 [JOI-2d] | ||||||||||
12 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | |||||
13 | X-ray | Kraft | Chandra / HRC | GTO time awarded for approach science / Juno support | ~10hrs on May 24 and June 1 | ||||||
14 | X-ray | Dunn | XMM | 160 ks (44.5 h) requested for approach science / Juno support | ~10hrs on May 17-18, and 24 | "very keen to partner with any willing Juno teams to share findings, enrich the analysis and inform what might cause any X-ray variations we observe" | |||||
15 | X-ray | Ezoe | Hitomi(Astro-H) | 100 ks during the Performance Verification phase | spacecraft anomaly leading to mission failure | no data | |||||
16 | FUV | Nichols | HST/STIS | imaging and spectroscopy of Jupiter’s auroral regions | observations acquired May 16, 17, 18, 18, 21, 22, 23, 24, 25, 26, 27, 28, 29, 30, 31; Jun 1, 2, 3, 4, 5, 6, 7, 22, 23, 24, 26, 27, 30 | data made available to Juno team asap; many are already Co-Is. Time-lapse images are available for download from ftp://ftp.ion.le.ac.uk/HST. | |||||
17 | FUV/ EUV | Kimura, Yoshikawa | Hisaki/ EXCEED | Spectroscopy of Jupiter UV aurura (total flux) and EUV spectrum of Io torus (spatially resolved) | continuous observations, 2015 Dec – 2016 Jun (except Mar 4 to Apr 21 and Apr 26 to May 4) 2016 Jan 21-31 2016 Feb 1-29 2016 Mar 1-3, 5-31 2016 Apr 13, 22-26 2016 May 4-31 2016 Jun 1-30 2016 Jul 1-8 | Data open to anyone joining that Hisaki team. Hisaki successfully observed EUV aurora and Io plasma torus during this phase, so any comparison with other data is welcomed. | |||||
18 | CCD | Simon | HST/WFC3 | Multiple-filtered imaging, 275-885 nm; two rotations of Jupiter to determine structure and properties of clouds and aerosols at high resolution, define atmospheric flow and search for waves. (Outer Planet Atmospheric Legacy [OPAL] program) | Images acquired on 2016 February 9-10 UTC. | ||||||
19 | CCD | Irwin | VLT/MUSE - IFU | spectroscopic imaging, 465-930 nm to determine cloud structure and albedo spectrum of particles. | Spectral images of Jupiter acquired March 8-9 and March 31-April 2 | Raw data publicly available to download from ESO portal. Standard calibration pipeline takes of the order of 1-3 days to complete, although this appears to lead to radiance values that are (15 +/- 5) % too high. It is therefore recommended to scale the radiance values down in post-processing. | |||||
20 | CCD | Sanchez-Lavega | Bilbao 11” Celestron with CCD | visible imaging, U, B, G, R + CH4 filters. Use “lucky imaging” to gain spatial resolution. | Observations made on April 18, 28, May 2, 3, 4, 9; June 7, 8, 20, 21, 27 | raw data available in 2-3 days, processed data available in a week if necessary (sooner if desired) | |||||
21 | CCD | Sanchez-Lavega | Calar Alto 2.2-m telescope, with PlanetCam camera | visible imaging, U, B, G, R + CH4 filters plus several bands between 1.0 and 1.7 microns, including J and H filterss. Use “lucky imaging” to gain spatial resolution. | good images from March 3/4, some images from March 6/7, good images from May 16/17, some images from 17/18 + 18/19 amid clouds, good images over the full spectral range May 19, 20; June 22, 23; July 1-4 | raw data available in 2-3 days, processed data available in a week if necessary (sooner if desired) | |||||
22 | CCD | Sanchez-Lavega | Calar Alto 2.2-m telescope, with Astralux camera | visible imaging, U, B, G, R + CH4 filters. Use “lucky imaging” to gain spatial resolution. | June 25, 26, 27 (bad seeing on June 27) | Raw data available in 2-3 days, processed data available in a week if necessary (sooner if desired), pending analysis to asses the results and quality (suspect nothing exceptional) | |||||
23 | CCD | Ip | Lulin 1-m/35-cm | UVBRI and CH4 filters | Apr 22, 23; Jun 17, 19, 21 | raw data available in a couple of weeks | |||||
24 | CCD | Chanover | Apache Point Observatory / Acoustical Optical Tunable Filter (APO/AOTF) | ~450-940 nm spatially resolved spectroscopy to determine cloud structure as linked to atmospheric dynamics. | one night successful during March 28-30 run | data being reduced | |||||
25 | CCD | Schneider | Apache Point Observatory / Dual Imaging Spectrograph (DIS) | Long-slit visible spectroscopy of both sides of the Io torus to determine S+, S++, O+ composition and electron density | acquired April 6, 14, 15. | calibrated data available on request | |||||
26 | CCD | Schmidt | McDonald Observatory IFU | Io's Neutral Na clouds, integral field echelle | acquired May 3, 4, 12 | available upon request | |||||
27 | CCD | Asada/Kagitani/Sakanoi | Tohoku Univ. Haleakala 60cm | Visible imaging, RGB, 750nm and CH4 filters | 24 Dec. 2015 - 30 May 2016, 20 Dec. 2016 - | ||||||
28 | Visible | Kagitani/ Yoneda | Tohoku Univ. Haleakala 40cm / 60cm | Imaging observations of [SII](6716=6731A) emission in Io plasma torus with a 60-cm reflector. Sample data are on http://pparc.gp.tohoku.ac.jp/data/hal/qlMovie2.gif | continuous as Hisaki/ EXCEED (UV/EUV) & IPRT (Synchrotron) 2016 Jan 1, 4-5, 7-10 2016 Feb 5-6, 8-16, 18-28 2016 Mar 1-7, 9-22, 24-25, 28-31 2016 Apr 1-5, 7, 9-11 2016 May 12, 15-24, 27-30 2016 Jun 1-13, 16, 18-23, 26-29 2016 Jul 3, 5, 7-9 | ||||||
29 | Visible | Kagitani/ Yoneda | Tohoku Univ. Haleakala 40cm / 60cm | Imaging observations of Na neublar originating from Io. Sample data are: http://pparc.gp/tohoku.ac.jp/data/hal/na_movie.gif | continuous as Hisaki/ EXCEED (UV/EUV) & IPRT (Synchrotron) observed on same nights as [SII] emission | ||||||
30 | Visible | Kagitani/ Yoneda | Tohoku Univ. Haleakala 10cm attached to 40 cm | Quasi-continous imaging of sodium nebula originating from Io | Dec 23 2016 - July 2017 continuous as Hisaki/ EXCEED (UV/EUV) & IPRT (Synchrotron) observed on same nights as [SII] emission | ||||||
31 | Near UV to Near IR | François Colas / JL Dauvergne / Marc Delcroix | Pic du Midi | T1M telescope | Several observations from 17 to 23 May | ASAP | |||||
32 | CCD + near IR | Sanchez-Lavega | Calar Alto 2.2m/ PlanetCam | Filtered imaging, 0.38 –1.7µm. Use “lucky imaging” to gain spatial resolution. | March 3/4 excellent seeing; good images covering the whole spectral range; March 6/7 bad seeing, some images available; May 16/17 - very good seeing with good images coveragin gthe whole spectral range; ay 17/18, 18/19 - partly cloudy with some imaging, May 19/20 excellent seeing with good images covering the whole spectral range | raw images available in a week, processed images in 2-3 weeks if necessary (sooner if desired, e.g. interesting targets, etc.) | |||||
33 | CCD + near IR | Sanchez-Lavega | Calar Alto 2.2m/ PlanetCam | Filtered imaging, 0.38 –1.7µm. Use “lucky imaging” to gain spatial resolution. | images acquired between 1.0 and 1.7 microns on July 1-4 | raw images available in a week, processed images in 2-3 weeks if necessary (sooner if desired, e.g. interesting targets, etc.) | |||||
34 | CCD + near IR | Orton | IRTF/MORIS, SpeX guide camera and spectrometer | filtered imaging 480-950 nm (MORIS); 1.58-5.1µm and spectral scans: 0.8-2.5µm, 2.5-5.1µm (SpeX) to determine structure and distribution of clouds and aerosols. | acquired: 2015 Nov 2-3, 2016 Jan 2-3 (no MORIS data) 2016 Feb 28-29 (with MORIS images on Feb 29) | raw data can be made available immediately; reduced images can be made available within a month (or sooner, as desired); reduced spectral scans available within 6 months (software for geometric reduction is under development) | |||||
35 | CCD+ near IR | Orton | IRTF/MORIS, SpeX guide camera and spectrometer | filtered imaging 480-950 nm (MORIS); 1.58-5.1µm and spectral scans: 0.8-2.5µm, 2.5-5.1µm (SpeX) to determine structure and distribution of clouds and aerosols. | SpeX imaging and scanned spectroscopy acquired on: 2016 May 11-12 UT. No MORIS data collected. Radiometrically uncalibrated images available on request. | raw data can be made available immediately; reduced images can be made available within a month (or sooner, as desired); reduced spectral scans available within 6 months (s/w for geometric reduction is under development) | |||||
36 | near IR | Orton | IRTF/SpeX guide camera | filtered imaging at: 1.58 µm (cloud albedo), 2.16 µm (upper-tropospheric particle field), 3.417 µm (H3+ auroral emission), 3.80 µm (mid-tropospheric particle field and H3+ auroral emission) and 5.10 µm (deep-tropospheric particle and gas distribution) | Images obtained and available from: Feb. 1, 4, 22, 23, 28, 29; Mar 2, 3, , 11, 12, 24; Apr 4, 25, 26; May 24, 25; Jun 4, 6, 18, 19 UT. | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired; images are scheduled to be uploaded and available on JSOC | |||||
37 | near IR | Orton | IRTF/SpeX guide camera | 3.8 and 5.1 micron imaging observations of Io | Feb 11, 22, 23 Mar 2, 3, 12 Apr 4 Jun 4, 6, 18, 19 | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired; images are available at http://junoirtf.space.swri.edu/. | |||||
38 | near IR | Johnson | IRTF /CSHELL | high-res. scanning spectroscopy of H3+ auroral emission. | observations obtained on February 3, 5, 10, 15, 17, 22, 27 and March 5. Good weather. | scanned images & possibly velocity maps, within 24 hrs; properly calibrated data will take longer; currently working on pipeline. | |||||
39 | near IR | Kita | IRTF / CSHELL | high-resolution spectroscopy of H3+ auroral emission for velocity-field measurements. | H3+ images and spectra obtained on April 22, 25; May 7, 9, 19, 21 Good weather. | would like to see agreement in place with Juno science team first and discussed at the workshop, but willing to share | |||||
40 | near IR | Kasaba Kita | Subaru / IRCS | AO-guided imaging/spectroscopy of H3+ emission with high spatial and spectral resolution. (using Galilean satellites as NGS) | K spectrum (H2 & H3+) on May 19, 21 H3+ image on May 19, 21, 24 BrAlpha image on May 24 | would like to see agreement in place with Juno science team first and discussed at the workshop, but willing to share. | |||||
41 | near IR | Kim | Gemini S/ Phoenix | 3-µm spectroscopy of auroral-related CH4, hydrocarbons. | No data on any of the nights granted for these observations between April 25 and May 20 were taken due to adverse weather conditions. | N/A | |||||
42 | near IR | O’Donoghue | Keck / NIRSpec | high-resolution scanning spectroscopy of H3+ auroral emission for temperature mapping. | Good observations obtained during the first half of April 13, 16, 19 and 22, with excellent coverage of the northern aurora. Some additional coverage of low-latitude ionosphere. | Data reduction pipeline built. Building up long-term dataset of Jupiter's northern and southern aurorae | |||||
43 | near IR | Bonfond | VLT / NACO | high spatial resolution imaging to determine detailed structure of H3+ emission, differentiating between the Io and Ganymede footprints, using Galilean satellites as NGS. | service observations successful on April 7 | will provide previews and preliminary results to Juno ASAP. Hard to commit to specific data products, but “I belong to the Juno science team.” | |||||
44 | near IR | Defrère | LBT / LMIRCAM + NOMIC (7.9 µm) | imaging of H2 and H3+ emission to identify the infrared counterpart of FUV auroral features, disentangle auroral precipitation effects from Joule-heating effects, and measure the short-timescale variability of polar-most emissions. | Feb 20: a few minutes of H- and K-band data; March 28: ~15 minutes of K and K band data of the north pole | “data available right away” | |||||
45 | near IR | de Kleer | Gemini N / NIRI+AO | near-IR imaging of volcanism on Io, 2–4µm | Observations have been collected on 31 nights using Kc-band and L'-band images, Jan 30; Feb 3, 4, 9, 11, 15-21, 23; Mar 11-14; Apr 30; May 1-4, 8-14, 16-20, 23-25, 27-28, 31; Jun15, 710, 12, 16-20, 24-25, 27. | observations are part of de Kleer’s thesis, but specific requests will be considered | |||||
46 | mid IR | Greathouse | IRTF / TEXES | scanning spectroscopy to determine structure of low-latitude vertical oscillations vs. time. | Acquired on 2015 Nov 11-14 and 2016 Jan 13 10:30-17:30 UT, Jan 14 10:30-17:30 UT, Jan 18 11:30-19:00 UT, Jan 19 9:30-18:00 UT, Jan 21 9:30-12:30 UT & 15:00-18:00 UT April 28 3:00-10:30 UT, April 29 2:00-10:30 UT, May 4 2:00-7:30 UT, May 7 2:00-8:30 UT | raw data available in 2-3 days, reduced and remapped to lat/lon in 1 month (could be done faster if requested) | |||||
47 | mid IR | Fletcher | IRTF / TEXES | scanning spectroscopy to determine temperature and minor-constituent distribution. | Global maps in multiple settings acquired as follows: 2015-Nov-16/18; 2016-Jan-16/17/20; 2016-Apr-30 to May-06 | raw data available almost immediately, calibrated files with geometry within a month, and retrieved properties potentially available within 1-2 weeks (subject to any unforeseen issues) | |||||
48 | mid IR | Encrenaz | IRTF / TEXES | scanning spectroscopy to determine PH3 and trace-constituent distribution (5 and 10 microns). | Acquired on 2015 Nov 16-18; 2016 Jan 15 16:30-17:30 UT, Jan 16 9:50-19:00 UT, Jan 17 9:50-17:50 UT, Jan 20 9:50-19:00 UT; April 30 2:00-3:30 UT, May 2 2:00-10:30 UT, May 3 2:00-10:30 UT, May 5 2:00-10:30 UT, May 6 2:00-10:30 UT | TBD | |||||
49 | mid IR | Retherford | IRTF / TEXES | Ionized Sulfur | Acquired 2016 Jan 15 10:00-16:00 UT, Jan 21 12:50-15:00 UT | ||||||
50 | mid IR | Tsang | IRTF / TEXES | 19 micron SO2 monitoring of Io | Acquired 2016 April 30 3:30-10:30 UT | ||||||
51 | mid IR | Kasaba Orton Sinclair | Subaru / COMICS | spectroscopy and imaging to map the stratospheric temperature and minor constituent distribution associated with polar auroral regions. | <done> 24-25 Jan 2016 | would like to see agreement in place with Juno science team first and discussed at the workshop, but willing to share; raw images available immediately & reduced images possibly within a month, depending on interest; raw spectra available quickly “on demand” | |||||
52 | mid IR | Fletcher | VLT / VISIR | filtered radiometric imaging to map the temperature, minor constituent, and cloud distribution defining climatology, together with auroral heating and chemistry | Global maps, 7-20 µm, on 2016 Feb 15-16, 2016 Mar 25-26. 5-µm lucky imaging test on 2016 Feb 26 with June 27 press release. Northern aurora in 8 filters 2016 May 19; global observations June 7-8/8-9. | available in raw form in the ESO archive within 24 hours of acquisition; cylindrical maps within 1-2 days and reduced maps within a week | |||||
53 | mid IR | Sinclair | IRTF / TEXES | spectroscopy to map the distribution of stratospheric temperatures and minor constituents associated with polar auroral regions. | data acquired during TEXES block: 2016 May 1 2:00-10:30 UT, May 4 7:30-10:30 UT | raw data available in 2-3 days, reduced and remapped to lat/lon in 1 month (could be done faster if requested); once that is done, existing software could produce results in 3-5 days. | |||||
54 | mid IR | Kostiuk | HIPWAC | ultra high-resolution spatially resolved spectroscopy of stratospheric emission lines in Jupiter’s polar regions | successful spatially resolved spectroscopy using HIPWAC at the IRTF: April 18-21 | TBD | |||||
55 | radio* | Lamy, Zarka, Cecconi | Nançay Decameter Array, NenuFAR, LOFAR (Nançay, France) UTR2 (Kharkov, Ukraine) Iitate, Tohoku U.; Awara, Fukui Technical U.; Agawa, Kochi National Coll. of Technology (Japan) LWA1 (New Mexico, USA) | coordinated measurement of 10-40 MHz cyclotron radio emission. NDA data are acquired 8 hours per day. For more information see: http://maser.lesia.obspm.fr/outils-services/juno-ground-radio/ | See the web site for more details. | Most observers intend to have their data immediately public , but some (e.g. Ukrainian) prefer to set up a private server that will deliver data only to Juno-related scientists. Data availability should be a matter of weeks or less. | |||||
56 | radio* | Imai | LWA1 (USA) NDA (France) UTR-2 (Kharkov, Ukraine) GURT (Kharkov, Ukraine) URAN-2 (Poltava, Ukraine) URAN-3 (Lviv, Ukraine) | Coordinated Jupiter's DAM emissions. More information can be found at: PDF: Coordinated LWA1-NDA-URAN2 Observations for Jupiter’s DAM Radiation https://drive.google.com/file/d/0B32DAVbuGRxGMGlYN24wNXZuVlU/view?usp=sharing * URAN3 has mostly participated in this campaign, while UTR-2 and GURT sometimes join. PDF: Coordinated NDA-URAN2 Observations for Jupiter’s DAM Radiation https://drive.google.com/file/d/0B32DAVbuGRxGWXg5ZjlpRmRBcGs/view?usp=sharing * This corresponds to NDA-UTR2-GURT-URAN Jupiter observation campaign. | Observations combining LWA1+NDA+URAN2 made on Jan 8, 9, 15, 16; Feb 10, 16, 17, 23, 24; Mar 20, 26, 27; Apr 2, 3, 15; May 3, 4, 10, 11; Jun 11, 12, 18, 20, 21. Observations combining NDA+UTR2+GURT+URAN made on Mar 18, 25; Apr 12, 13, 19, 20; May 10. | Reduced data will be available upon request. Data process requires several months. | |||||
57 | radio | Santos-Costa | LOFAR | LOFAR observations of Jupiter's electron belt at 50-190 MHz coordinated with Juno's in-situ and/or remote observations during Juno's final approach phase and first three orbits | Observations obtained on June 2, 15. | no sooner than six months after data collection to allow observers and Juno team members to present / publish some preliminary observation results. | |||||
58 | radio | Levin (contact point) | DSN | 2.3-GHz synchrotron radio emission | two continuous 24-hour observations desired, with actual allocation TBD, possibly “last-minute” | data availability TBD but likely within a few months, based on previous experience | |||||
59 | radio | Levin (contact point) | DSN | 2.3-GHz synchrotron radio emission | Jan 24, 17:10-02:45 Jan 27,18:30-02:45 Jan 31, 18:30-02:30 Feb 4, 18:45-01:00 Feb 6, 18:20-01:10 Feb 11, 20:00-01:45 Feb 13, 18:55-01:40 Feb 14, 20:00-01:20 Feb 18, 21:45-01:20 Feb 19, 20:20, 01:15 Feb 27, 17:50-23:35 Mar 1, 19:15-02:05 Mar 3, 21:40-00:25 Mar 11, 18:15-23:55 Mar 15, 19:30-23:25 Mar 17, 18:15-03:05 Apr 1, 16:35-22:30 Apr 23, 14:45-21:05 May 3, 20:00-00:00 May 7, 20:00-23:40 May 10, 19:35-23:30 May 15, 11:30-21:45 | data availability TBD but likely within a few months | |||||
60 | radio* | Levin (contact point) | GAVRT | 2.3-GHz synchrotron radio emission, monitored as public outreach by students | A query of GAVRT database tables shows that observations of Jupiter were made from DSS-13 on Apr 21, 27; May 4, 24, 25, 31; Jun 20, 29. Observations were made from DSS-28 on Apr 21, 27; May 4, 25, 31; Jun 2. There is no assurance that data from any date are useful for a particular purpose. They must be examined. | http://galileo.gavrt.org/seti/access/scan/dssData.php ; Raw data available to anyone who wants it. Processed data will eventually be available at the same website. Please acknowledge the GAVRT project if you use these data in a publication. | |||||
61 | radio* | Misawa Tsuchiya | Iitate Planetary radio Telescope (IPRT) | 325MHz (& 785MHz) synchrotron radio emission, continuous monitoring with a 31mx33m single dish telescope | Continuous !!! | data available by request | |||||
62 | radio* | Kita | GMRT (India) | Synchrotron radio emission at L-band | May 03 14:30-16:30 May 14 13:30-15:30 May 20 13:30-15:30 May 28 15:30-17:30 Jun 02 14:30-16:30 Jun 05 12:30-14:30 Jun 07 13:30-15:30 Jun 11 11:30-13:30 Jun 23 12:30-14:30 | Reduced data will be available upon request. Data reduction requires several months. | |||||
63 | radio | Horiuchi | DSN Canberra DSS43(70m) or DSS34/45(34m) | 2.3/8.4 GHz synchrotron and thermal radio emission | Jan 30 030 09:10-16:50 Feb 11 042 09:55-12:40 Feb 16 047 08:20-14:55 Feb 28 059 07:50-15:55 Feb 03 063 07:55-15:15 Feb 24 084 08:05-10:30 Feb 26 086 07:45-11:15 Feb 27 087 07:40-10:40 Feb 28 088 07:40-11:20 Feb 29 089 07:35-10:35 Mar 30 090 05:35-11:15 Apr 07 098 07:05-11:45 May 08 129 05:40-11:00 May 19 140 03:40-10:25 Jun 02 154 05:00-07:15 Jun 04 156 04:20-07:45 Jun 05 157 04:05-08:25 Jun 11 163 02:10-08:00 Jun 19 171 04:35-11:30 Jun 24 176 06:10-10:40 Jun 29 181 05:00-06:45 Jul 02 184 04:40-09:55 | TBD | |||||
64 | Optical | Acar, Ateş | İSTEK Belde Observatory 16" | Multi-color lucky imaging | 2017 Feb 2 Mar 27 May 18 Jul 10 Sep 2 Oct 25 | Processed frames will be uploaded to the ground base data collection server | |||||
65 | |||||||||||
66 | |||||||||||
67 | Instruments are listed at: https://voparis-juno.obspm.fr/juno/instruments/pub_json | ||||||||||
68 | |||||||||||
69 | |||||||||||
70 | Period: Jupiter Approach (2015 November 1 – 2016 July 3 [JOI-2d] | ||||||||||
71 | Instrument | Description | |||||||||
72 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period up to a few days before JOI. These sample properties of the solar wind impinging on Jupiter’s magnetosphere, starting from a distance of ~1AU up to sampling the magnetosphere itself. | |||||||||
73 | UVS | Scans of Jupiter’s aurora June 3-29: June 3 at 02:30, June 4 at 18:30, June 9 at 08:30, June 14 at 08:30, June 16 at 00:30, June 18 at 02:30, June 21 at 10:30, June 24 at 13:30, June 26 at 00:30, June 27 at 14:00 | |||||||||
74 | JunoCam | Continuous imaging of Jupiter June 12-29, every ~15 minutes to create an "approach movie". Some large features on Jupiter are resolvable, and the motions of Galilean satellites are prominent and striking. | |||||||||
75 | JIRAM | Observations of Jupiter in Band L and M were made on January 25 and February 9 | |||||||||
76 | MWR | Jupiter was observed during the approach phase at times when it passes through the spin plane of the MWR antennas (the great circle on the sky which is continuously scanned by the MWR antennas due to the rotation of the spacecraft). At these times the spacecraft is at a large distance from Jupiter, so it appears smaller that the MWR antenna beams and only the total emission from the planet and radiation belts is measured. These scans will confirm that the MWR antenna patterns have remained unchanged, and allow us to check our absolute radiometric calibrations by comparison with ground-based single-dish calibrated measurements of Jupiter's total flux. Consequently such observations are desired at frequencies comparable to the lowest three or four frequencies of the MWR (600 Mhz, 1.25, 2.6 and 5Ghz) around the times of MWR observations. | |||||||||
77 | |||||||||||
78 | |||||||||||
79 | |||||||||||
80 | |||||||||||
81 | |||||||||||
82 | |||||||||||
83 | |||||||||||
84 | |||||||||||
85 | |||||||||||
86 | |||||||||||
87 | |||||||||||
88 | |||||||||||
89 | |||||||||||
90 | |||||||||||
91 | |||||||||||
92 | |||||||||||
93 | |||||||||||
94 | |||||||||||
95 | |||||||||||
96 | |||||||||||
97 | |||||||||||
98 | |||||||||||
99 | |||||||||||
100 | |||||||||||
101 | |||||||||||
102 | |||||||||||
103 | |||||||||||
104 | |||||||||||
105 | |||||||||||
106 | |||||||||||
107 | |||||||||||
108 | |||||||||||
109 | |||||||||||
110 | |||||||||||
111 | |||||||||||
112 | |||||||||||
113 | |||||||||||
114 | |||||||||||
115 | |||||||||||
116 | |||||||||||
117 | |||||||||||
118 | |||||||||||
119 | |||||||||||
120 | |||||||||||
121 | |||||||||||
122 | |||||||||||
123 | |||||||||||
124 | |||||||||||
125 | |||||||||||
126 | |||||||||||
127 | |||||||||||
128 | |||||||||||
129 | |||||||||||
130 | |||||||||||
131 | |||||||||||
132 | |||||||||||
133 | |||||||||||
134 | |||||||||||
135 | |||||||||||
136 | |||||||||||
137 | |||||||||||
138 | |||||||||||
139 | |||||||||||
140 | |||||||||||
141 | |||||||||||
142 | |||||||||||
143 | |||||||||||
144 | |||||||||||
145 | |||||||||||
146 | |||||||||||
147 | |||||||||||
148 | |||||||||||
149 | |||||||||||
150 | |||||||||||
151 | |||||||||||
152 | |||||||||||
153 | |||||||||||
154 | |||||||||||
155 | |||||||||||
156 | |||||||||||
157 | |||||||||||
158 | |||||||||||
159 | |||||||||||
160 | |||||||||||
161 | |||||||||||
162 | |||||||||||
163 | |||||||||||
164 | |||||||||||
165 | |||||||||||
166 | |||||||||||
167 | |||||||||||
168 | |||||||||||
169 | |||||||||||
170 | |||||||||||
171 | |||||||||||
172 | |||||||||||
173 | |||||||||||
174 | |||||||||||
175 | |||||||||||
176 | |||||||||||
177 | |||||||||||
178 | |||||||||||
179 | |||||||||||
180 | |||||||||||
181 | |||||||||||
182 | |||||||||||
183 | |||||||||||
184 | |||||||||||
185 | |||||||||||
186 | |||||||||||
187 | |||||||||||
188 | Period: Orbit 0 (2016 July 4 [JOI-1d] – 2016 August 25) | ||||||||||
189 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | |||||
190 | FUV | Nichols | HST/STIS | imaging and spectroscopy of Jupiter’s auroral regions | observations made Jul 11-18 | data made available to Juno team asap; many are already Co-Is | |||||
191 | Visible | Kagitani/ Yoneda | Tohoku Univ. Haleakala 40cm / 60cm | Quasi-continous imaging of sodium nebula originating from Io | continuous as Hisaki/ EXCEED (UV/EUV) & IPRT (Synchrotron) through 2016 December | ||||||
192 | CCD | Ip | Lulin 1-m/35-cm | UVBRI and CH4 filters | a few observations in July | raw data available in a couple of weeks | |||||
193 | near IR | Orton | IRTF/SpeX guide camera | filtered imaging at 5 strategic wavelengths, including 5.1µm and 3.4µm (H3+ auroral emission). | obtained during 60 min intervals on Jul 22; July 23 observing completely weathered out. | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired | |||||
194 | mid IR | Fletcher | VLT / VISIR | filtered radiometric imaging to map the temperature, minor constituent, and cloud distribution defining climatology, together with auroral heating and chemistry | July 27, 28, 31; August 1 | available in raw form in the ESO archive within 24 hours of acquisition; cylindrical maps within 1-2 days and reduced maps within a week | |||||
195 | radio* | Zarka, Cecconi | Nançay Decameter Array, NenuFAR, LOFAR (Nançay, France) UTR2 (Kharkov, Ukraine) Iitate, Tohoku U.; Awara, Fukui Technical U.; Agawa, Kochi National Coll. of Technology (Japan) LWA1 (New Mexico, USA) | coordinated measurement of 10-40 MHz cyclotron radio emission. For more information see: http://maser.lesia.obspm.fr/outils-services/juno-ground-radio/ | Observations made on Jul 23, 29, 30; Aug 5. See the web site for more details. | Most observers intend to have their data immediately public , but some (e.g. Ukrainian) prefer to set up a private server that will deliver data only to Juno-related scientists. Data availability should be a matter of weeks or less. | |||||
196 | |||||||||||
197 | Scheduled observations by Juno. | ||||||||||
198 | |||||||||||
199 | Note: All instruments will be powered on July 10, 0:00 UTC | ||||||||||
200 | |||||||||||
201 | Orbits start at perijove minus one day. | ||||||||||
202 | |||||||||||
203 | Perijove 2016 July 5, 02:47:38 UTC, System-III longitude = 32.8°W | ||||||||||
204 | |||||||||||
205 | Period: Orbit 0 (2016 July 4 [JOI-1d] – 2016 August 25) | ||||||||||
206 | Instrument | Description | |||||||||
207 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | |||||||||
208 | MWR | On July 6, the MWR collected unresolved observations of Jupiter at a low data rate. | |||||||||
209 | MWR | The MWR observed at full rate during three concentrated periods totalling about 100 hours to make careful maps of its antenna beams using Jupiter as a bright, unresolved source. | |||||||||
210 | UVS | Scans of Jupiter’s aurora July 22-Aug 25: (Calibration on July 16 at 00:00) July 25 at 14:00, July 29 at 10:00, August 8 at 14:00 | |||||||||
211 | JIRAM | Observations to calibrate pointing and spin phase | |||||||||
212 | JunoCam | Continuous imaging of Jupiter throughout this period, starting 2016 July 10, every ~15 minutes | |||||||||
213 | |||||||||||
214 | |||||||||||
215 | |||||||||||
216 | |||||||||||
217 | |||||||||||
218 | |||||||||||
219 | |||||||||||
220 | |||||||||||
221 | |||||||||||
222 | |||||||||||
223 | |||||||||||
224 | |||||||||||
225 | |||||||||||
226 | |||||||||||
227 | |||||||||||
228 | |||||||||||
229 | |||||||||||
230 | |||||||||||
231 | |||||||||||
232 | |||||||||||
233 | |||||||||||
234 | |||||||||||
235 | |||||||||||
236 | |||||||||||
237 | |||||||||||
238 | |||||||||||
239 | |||||||||||
240 | |||||||||||
241 | |||||||||||
242 | |||||||||||
243 | |||||||||||
244 | |||||||||||
245 | |||||||||||
246 | |||||||||||
247 | |||||||||||
248 | |||||||||||
249 | |||||||||||
250 | |||||||||||
251 | |||||||||||
252 | Note: Jupiter may be too close to the sun for Earth-based observations during much of this period, except for daytime-capable observatories. | ||||||||||
253 | |||||||||||
254 | Period: Orbit 1 [C Orbit] (2016 August 26 – 2016 October 17) | ||||||||||
255 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | |||||
256 | Visible | Kagitani/ Yoneda | Tohoku Univ. Haleakala 40cm / 60cm | Quasi-continous imaging of sodium nebula originating from Io | continuous as Hisaki/ EXCEED (UV/EUV) & IPRT (Synchrotron) through 2016 December | ||||||
257 | near IR | Orton | IRTF/SpeX guide camera | filtered imaging 1.58-5.1µm to determine structure and distribution of clouds and aerosols. | 1. Aug 26 19:30 - Aug 27 01:30 UTC (including a time frame observing the PJ1 longitude ~12.5 hours before PJ1) 2. Aug 27 19:30 - Aug 28 01:30 UTC including a time frame observing the PJ1 longitude ~8.5 hours after PJ1). Best observations were at 5.1 microns during period (1). Observing conditions in period (2) were extremely difficult, with only a single, low-SNR image obtained. | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired. Images all available without radiometric calibration at http://junoirtf.space.swri.edu/ | |||||
258 | radio | Santos-Costa | LOFAR | LOFAR observations of Jupiter's electron belt at 50-190 MHz coordinated with Juno's in-situ and/or remote observations during Juno's final approach phase and first three orbits | Observations obtained on Aug 27. | no sooner than six months after data collection to allow observers and Juno team members to present / publish some preliminary observation results. | |||||
259 | radio* | Kita | GMRT (India) | Synchrotron radio emission at L-band | Aug 27 09:30-11:30 | reduced data will be available upon request. Data reduction requires several months. | |||||
260 | Scheduled observations by Juno. | ||||||||||
261 | |||||||||||
262 | Perijove is 2016 August 27, 12:51:20 UTC. System-III longitude = 96.1°W. | ||||||||||
263 | |||||||||||
264 | Period: Orbit 1 [C Orbit] (2016 August 26 – 2016 October 17) | ||||||||||
265 | Instrument | Description | |||||||||
266 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | |||||||||
267 | MWR | N/S scans near perijove longitude, not centered on nadir - similar to GRAV-orbit scans | |||||||||
268 | UVS | Scans of Jupiter’s aurora Aug 27, 1:51 - 15:51. | |||||||||
269 | JIRAM | Imaging and spectra of Jupiter Aug 25 - 27, with spatial resolutions ~560 km to tens of km. | |||||||||
270 | JunoCam | Continuous imaging of Jupiter throughout this period, every ~15 minutes | |||||||||
271 | |||||||||||
272 | |||||||||||
273 | |||||||||||
274 | |||||||||||
275 | |||||||||||
276 | |||||||||||
277 | |||||||||||
278 | |||||||||||
279 | |||||||||||
280 | |||||||||||
281 | |||||||||||
282 | |||||||||||
283 | |||||||||||
284 | |||||||||||
285 | |||||||||||
286 | |||||||||||
287 | |||||||||||
288 | |||||||||||
289 | |||||||||||
290 | |||||||||||
291 | |||||||||||
292 | |||||||||||
293 | |||||||||||
294 | Period: Orbit 2 (2016 October 18 – December 9) | ||||||||||
295 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | |||||
296 | X-ray | Gladstone | Chandra | 5-hour observation targeting the northern aurora | 30 November 2016 | ||||||
297 | FUV | Grodent | HST/FUV-MAMA | high spatial and temporal resolution FUV observations of magnetosphere and ultraviolet auroras | 11/30/2016 15:47:26 11/30/2016 17:22:48 12/01/2016 17:13:28 12/01/2016 18:48:52 12/02/2016 17:03:31 12/02/2016 18:38:54 12/03/2016 13:43:56 12/04 2016 13:34:28 12/05/2016 19:46:26 12/05/2016 21:21:49 12/06/2016 14:51:43 12/06/2016 16:25:38 12/06/2016 18:01:00 12/07/2016 16:16:40 12/08/2016 11:21:03 12/09/2016 12:46:53 | Animations are routinely posted on: http://www.lpap.ulg.ac.be/Juno/HST/PJ03.html. | |||||
298 | Visible | Kagitani/ Yoneda | Tohoku Univ. Haleakala 40cm / 60cm | Quasi-continous imaging of sodium nebula originating from Io | continuous as Hisaki/ EXCEED (UV/EUV) & IPRT (Synchrotron) through 2016 December | ||||||
299 | CCD | Jackson | Boise State 16-inch | visible imaging, U, B, G, R | TBD | TBD | |||||
300 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | Continuous | ||||||
301 | near IR | Orton | IRTF/SpeX guide camera | filtered imaging 1.58-5.1µm (SpeX) to determine structure and distribution of clouds and aerosols. | SpeX images obtained on Oct 18,19, with some vignetting of the telescope beam coincident with the planned PJ2 Juno observations. SpeX images obtained on Nov 1, 2. Also Nov 29 with Bjoraker et al. | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner. Reduced "quick-look" observations (geometrically but not radiometrically calibrated) are available for immeduately use from the Juno-curated web site: http://junoirtf.space.swri.edu/ | |||||
302 | near IR (1-2 µm) | Orton | Gemini-N/NIRI | AO-stabilized imaging of Jupiter at several wavelengths | Dec 6, 2008 | Observations were not be taken due to severe weather conditions at Mauna Kea | |||||
303 | near IR | Orton | IRTF/SpeX guide camera | filtered imaging 480-950 nm (MORIS); 1.58-5.1µm and spectral scans: 0.8-2.5µm, 2.5-5.1µm (SpeX) to determine structure and distribution of clouds and aerosols. | awarded Dec 5 05:00-06:15, Dec 6 05:00-06:15, Dec 9 05:15-06:15, Dec 10 05:15-06:15 | Observations were not be taken due to severe weather conditions at Mauna Kea | |||||
304 | near IR | Johnson | IRTF/iSHELL | imaging and high-resolution spectroscopy of H3+ emission | Nov 16 04:00-06:30 (clear skies, took some random spectra), Nov 30 04:05-07:05 (some high clouds which dissappeared but icy fog kept rolling in. We got some observations in between the fog and managed to try out Lp2 and 4 with slit widths 0.375'' and 4''. Took random spectra and one scan of the northern aurora.) | Data reduction in progress | |||||
305 | near IR | Bjoraker | IRTF/iSHELL | high-resoution spectroscopy of Jupiter in the 5-µm window to determine NH3, H2O abundances and propeties of water clouds at similar locations and nearly the same time as Juno | completed Nov 15 06:05-12:05 Nov 18 06:05-12:05, also Nov 29 with SpeX (imaging and moderate-resolution spectroscopy) 06:05-12:05. Daylight observing. Dec 2 observations not taken due to snow at Mauna Kea. | awaiting iSHELL_Tool data reduction package | |||||
306 | near IR | Skrutskie | Fan Mountain / 31" FanCam | Io H and K band flux, disk integrated | Nov 13 11:00-12:00 | TBD. | |||||
307 | microwave | de Pater | Very Large Array (VLA) | A configuration in X band (8-10 GHz) | Observations obtained on 19 Oct., coincident IRTF observations | MWR PI Janssen is a Co-Investigator | |||||
308 | radio | Imai | Long Wavelength Array 1 (LWA1) | Jupiter's decametric auroral radio observations | Dec 5-8 | Request to M. Imai More information can be found at http://www-pw.physics.uiowa.edu/earth/ | |||||
309 | radio | Santos-Costa | LOFAR | LOFAR observations of Jupiter's electron belt at 50-190 MHz coorinated with Juno's in-situe and/or remote observations during Juno's final apoproach phase and first three orbits | four observation windows between May and November 2016 | no sooner than six months after data collection to allow observers and Juno team members to present / publish some preliminary observation results. | |||||
310 | |||||||||||
311 | Observations by Juno. | ||||||||||
312 | |||||||||||
313 | The Perijove Reduction Maneuver (PRM) was not performed, due to issues involving sticking valves in the main engine. Due to a safing event just before PJ, no Juno data were taken except for gravity mapping. | ||||||||||
314 | |||||||||||
315 | Period: Orbit 2 (2016 October 18 – December 9) | ||||||||||
316 | Instrument | Description | |||||||||
317 | MAG, JADE, JEDI, WAVES | Some measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | |||||||||
318 | MWR | No observations. | |||||||||
319 | UVS | No observations. | |||||||||
320 | JunoCam | No observations. | |||||||||
321 | JIRAM | No observations. | |||||||||
322 | |||||||||||
323 | |||||||||||
324 | |||||||||||
325 | MWR footprint plan, but not executed | ||||||||||
326 | |||||||||||
327 | |||||||||||
328 | |||||||||||
329 | |||||||||||
330 | |||||||||||
331 | |||||||||||
332 | |||||||||||
333 | |||||||||||
334 | |||||||||||
335 | |||||||||||
336 | |||||||||||
337 | |||||||||||
338 | |||||||||||
339 | |||||||||||
340 | |||||||||||
341 | |||||||||||
342 | |||||||||||
343 | |||||||||||
344 | |||||||||||
345 | |||||||||||
346 | |||||||||||
347 | |||||||||||
348 | |||||||||||
349 | |||||||||||
350 | |||||||||||
351 | |||||||||||
352 | |||||||||||
353 | |||||||||||
354 | |||||||||||
355 | |||||||||||
356 | |||||||||||
357 | |||||||||||
358 | |||||||||||
359 | |||||||||||
360 | |||||||||||
361 | |||||||||||
362 | |||||||||||
363 | |||||||||||
364 | |||||||||||
365 | |||||||||||
366 | |||||||||||
367 | |||||||||||
368 | |||||||||||
369 | |||||||||||
370 | |||||||||||
371 | |||||||||||
372 | |||||||||||
373 | |||||||||||
374 | |||||||||||
375 | |||||||||||
376 | |||||||||||
377 | |||||||||||
378 | |||||||||||
379 | |||||||||||
380 | |||||||||||
381 | |||||||||||
382 | |||||||||||
383 | |||||||||||
384 | |||||||||||
385 | |||||||||||
386 | |||||||||||
387 | Period: Early Orbit 3 (2016 December 10 – 2017 January 1) | ||||||||||
388 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | |||||
389 | X-ray | Gladstone | Chandra | 5-hour observation for day of perijove only targeting the northern aurora | 14 December 2016 | ||||||
390 | FUV | Grodent | HST/FUV-MAMA | high spatial and temporal resolution FUV observations of magnetosphere and ultraviolet auroras | 12/10/2016 18:58:50 12/11/2016 17:14:00 12/11 2016 19:18:02 12/11/2016 20:24:44 12/12/2016 17:03:59 12/12/2016 15:29:12 12/13/2016 12:10:09 12/14/2016 16:45:51 12/15/2016 08:39:04 | Times may change by re-scheduling on the part of HST. Animations of all visits are posted on http://www.lpap.ulg.ac.be/Juno/HST/PJ03.html. | |||||
391 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | Continuous | ||||||
392 | visible/NUV | Wong | HST/WFC3 UVIS | hi-resolution map of perijove track | Start time: Dec 11 08:00:24 UT, End time: Dec 12 09:49:14 UT | raw data available immediately from STScI archive; reduced maps and zonal wind profiles available within one month or potentially sooner; co-Is from MWR and JIRAM teams | |||||
393 | CCD | Sanchez-Lavega | Aulo EspaZio Gela, Bilbao, Spain | continuous imaging survey, 0.38-0.9 microns | continuous | TBD | |||||
394 | CCD | Irwin | VLT/MUSE - IFU | spectroscopic imaging, 465-930 nm to determine cloud structure and albedo spectrum of particles. | 30-minute observation sequence requested of Jupiter close the time of perijove passage that includes the perijove longitude | “reductions to photometrically-calibrated cubes can be done in a day or two if there is sufficient motivation!” | |||||
395 | near IR | Orton | IRTF/SpeX guide camera | filtered imaging at 5 strategic wavelengths, including 5.1µm and 3.4µm (H3+ auroral emission); additional wavelengths imaged between 1.58 and 2.3 µm | obtained at high airmass Dec 13, PJ3 longitudes on the Earth-facing hemisphere; Dec 22 on opposite hemisphere with good seeing. | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired. Reduced "quick-look" observations (geometrically but not radiometrically calibrated) are available for immeduately use from the Juno-curated web site: http://junoirtf.space.swri.edu/ | |||||
396 | near IR | Orton | IRTF/SpeX guide camera | filtered imaging at 9 strategic wavelengths, including 5.1µm and 3.4µm (H3+ auroral emission). | Dec 24 05:15-06:15; Dec 31 05:15-06:15, Jan 2 05:30-06:30, Jan 3 05:30-06:30, Jan 5 04:30-06:30 | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired | |||||
397 | near IR | Johnson | IRTF/iSHELL | imaging and high-resolution spectroscopy of H3+ emission | Dec 11 03:15-09:15 --> no observations taken because of snow storm at Mauna Kea; Dec 28 04:15-10:15 (daylight observing) --> took H3+ spectra of the southern and northern aurora. Took some scans but no off-axis star was available and therefore the telescope drifted significantly. The weather was quite good, with some clouds quickly passing over the summit. | Data reduction in process | |||||
398 | near IR | Bjoraker | IRTF/iSHELL | high-resoution spectroscopy of Jupiter in the 5-µm window to determine NH3, H2O abundances and propeties of water clouds at similar locations and nearly the same time as Juno | scheduled Dec 13 04:30-10:30 (daylight obs) | weathered out | |||||
399 | near IR | Bjoraker | IRTF/iSHELL | high-resoution spectroscopy of Jupiter in the 5-µm window to determine NH3, H2O abundances and propeties of water clouds | good data obtained Dec 27 04:30-10:30, Dec 29 04:30-10:30 | fully reduced spectra 2 months after iSHELL_Tool data reduction package is released | |||||
400 | near IR | Skrutskie | Fan Mountain / 31" FanCam | Io H and K band flux, disk integrated | Dec 22 9:10-10:20; Dec 29 11:10-12:10 | TBD | Q | ||||
401 | near IR (5 µm) | Wong | Gemini-N/NIRI | lucky imaging, 5-µm maps, near-global coverage | 14 Dec | full maps available on junocam planning site within 2 weeks | |||||
402 | near IR (5 µm) | Wong | Gemini-N/NIRI | lucky imaging, 5-µm maps, near-global coverage | 1.5 hr each 27, 28, 29 Dec. | full maps available on junocam planning site within 2 weeks | |||||
403 | near IR (1-2 µm) | Orton | Gemini-N/NIRI | AO-stabilized imaging of Jupiter at several wavelengths | moderately good data Dec 24 of longitudes east of the Great Red Spot; excellent data on Dec 28 of GRS environmenet and nominal PJ3 System III longitude. | TBD | |||||
404 | mid IR | Fletcher | VLT / VISIR | filtered radiometric imaging to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology. | Observations acquired on Dec15: a northern and southern OB (100 minutes total), in addition to several M-band images without burst mode in early dawn twilight; repeated with full imaging on Dec 17 including M-band burst mode observations obtained with some GRS coverage but not PJ3 longitude; and M-band burst mode images acquired on Dec 18 | available in raw form in the ESO archive within 24 hours of acquisition; cylindrical maps within 1-2 days and reduced maps within a week. | |||||
405 | mid IR | Fletcher | IRTF/TEXES | scanned spectral maps of Jupiter's disk at ten key spectral settings to derive upper-tropospheric and stratospheric temperatures, aerosol/cloud distributions, and distribution of tropospheric NH3 and PH3, and stratospheric C2H2 and C2H6. | obtained Dec 16 and 17, covering opposite hemispheres, but not in the best seeing conditions | raw data available almost immediately, calibrated files with geometry within a month, and retrieved properties potentially available within 1-2 weeks (subject to any unforeseen issues) | |||||
406 | mid IR | Greathouse | IRTF/TEXES | scanned high- and medium-resolution spectral maps of Jupiter's disk at key CH4- and H2-absorbing wavelengths to determine temperatures in the upper troposphere and stratosphere to determine the structure of non-seasonal thermal waves associated with the Quasi-Quadrennial Oscillation (QQO) | awarded Dec 19 03:00-11:30, Dec 20 03:00-11:30 (both daylight observing) | TBD | |||||
407 | mid IR | Encrenaz | IRTF/TEXES | scanned medium-resolution spectral maps of Jupiter's disk at key wavelengths to determine the distributions of gaseous NH3 and PH3 in Jupiter's troposphere | awarded Dec 16 11:30-14:30, Dec 17 11:30-14:30, Dec 21 15:00-19:30, Dec 22 15:00-19:30 (all daylight observing) | ||||||
408 | mid IR | Sinclair | IRTF/TEXES | scanned high-resolution spectral maps of Jupiter's disk at six key spectral settings to derive stratospheric temperatures and 3-dimensional distribution of stratospheric C2H2, C2H4, C2H6 and H3+ in auroral regions. | awarded Dec 15 03:30-11:30, Dec 16 03:00-06:30. Daylight observing on Dec 15; Jan | TBD | |||||
409 | sub-mm | Roth / Sanchez-Monge | IRAM NOEMA | Io SO2 atmosphere | One 5-h track successdfully obtained on Dec 11. SO2 line detected | Request to Lorenz Roth | Q | ||||
410 | microwave | de Pater | Very Large Array (VLA) | A configuration in X band (8-10 GHz) | observations successful on Dec 11 | MWR PI Janssen is a Co-Investigator | |||||
411 | radio | Imai | Long Wavelength Array 1 (LWA1) | Jupiter's decametric auroral radio observations | Dec 10-19 | Request to M. Imai More information can be found at http://www-pw.physics.uiowa.edu/earth/ | |||||
412 | |||||||||||
413 | |||||||||||
414 | Scheduled observations by Juno. | ||||||||||
415 | |||||||||||
416 | Perijove is 2016 December 14, 14:49:58 UTC. System-III longitude = 16.3°W | ||||||||||
417 | |||||||||||
418 | Period: Orbit 3 [GRAV] (2016 December 10 – 2017 January 31) | ||||||||||
419 | Instrument | Description | |||||||||
420 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | |||||||||
421 | MWR | N/S scans near perijove longitude, not centered on nadir. | |||||||||
422 | UVS | Scans of Jupiter’s aurora | |||||||||
423 | JIRAM | No JIRAM data were taken during this period until a full sofware patch was created and tested in order to avoid the circumstances causing the safing event on PJ2. | |||||||||
424 | JunoCam | No continuous imaging of Jupiter up to perijove. Close-up observations +-2 hours of perijove. Voting for 1-3 individual regions by public from Nov 25 to Dec 1. All observations successful, with some issues tested on PJ1 clarified. All data available on Mission Juno web site. | |||||||||
425 | |||||||||||
426 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with continuous monitoring of the high-gain antenna, which is pointed at the Earth through the perijove pass | ||||||||||
427 | |||||||||||
428 | PJ3 MWR footprints | ||||||||||
429 | |||||||||||
430 | |||||||||||
431 | |||||||||||
432 | |||||||||||
433 | |||||||||||
434 | |||||||||||
435 | |||||||||||
436 | |||||||||||
437 | |||||||||||
438 | |||||||||||
439 | |||||||||||
440 | |||||||||||
441 | |||||||||||
442 | |||||||||||
443 | |||||||||||
444 | |||||||||||
445 | |||||||||||
446 | |||||||||||
447 | |||||||||||
448 | |||||||||||
449 | |||||||||||
450 | |||||||||||
451 | |||||||||||
452 | |||||||||||
453 | |||||||||||
454 | |||||||||||
455 | |||||||||||
456 | |||||||||||
457 | |||||||||||
458 | |||||||||||
459 | |||||||||||
460 | |||||||||||
461 | |||||||||||
462 | |||||||||||
463 | |||||||||||
464 | |||||||||||
465 | |||||||||||
466 | |||||||||||
467 | |||||||||||
468 | |||||||||||
469 | |||||||||||
470 | |||||||||||
471 | |||||||||||
472 | |||||||||||
473 | |||||||||||
474 | |||||||||||
475 | |||||||||||
476 | |||||||||||
477 | |||||||||||
478 | |||||||||||
479 | |||||||||||
480 | |||||||||||
481 | |||||||||||
482 | |||||||||||
483 | |||||||||||
484 | |||||||||||
485 | |||||||||||
486 | |||||||||||
487 | |||||||||||
488 | Period: late Orbit 3 (2017 January 1 - 31): observations supporting Juno's original Perijoves 8 and 9 that investigator teams decided to retain | ||||||||||
489 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | |||||
490 | FUV | Grodent | HST/FUV-MAMA | high spatial and temporal resolution FUV observations of magnetosphere and ultraviolet auroras | 01/07/2017 01:57:08 01/07/2017 03:32:30 01/22/2017 15:31:08 01/23/2017 20:07:50 01/24/2017 15:11:42 01/24/2017 16:47:04 01/26 2017 18:04:03 01/27/2017 13:08:24 01/28/2017 09:48:08 01/29/2017 14:24:36 01/29/2017 15:59:58 | ||||||
491 | CCD | Sanchez-Lavega | Aulo EspaZio Gela, Bilbao, Spain / 28-cm telescope | continuous imaging survey, 0.38-0.9 microns | 01/01, 01/03, 01/04, 01/05, 01/06, 01/07, 01/08 | Images available at PVOL2 and Aula EspaZio web page. | |||||
492 | CCD | Sanchez-Lavega | Aula EspaZio Gela 36-cm telescope at Calar Alta Observatory | continuous imaging survey, Wavelengths: R, V, B, IR, R610, 890nm (methane), R610 | 01/13, 01/18 | Images available at PVOL2 and Aula EspaZio web page. | |||||
493 | CCD | Irwin | VLT/MUSE - IFU | spectroscopic imaging, 465-930 nm to determine cloud structure and albedo spectrum of particles. | 9/10 January 2017 | “reductions to photometrically-calibrated cubes can be done in a day or two if there is sufficient motivation!” | |||||
494 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | 30-minute observation sequence requested of Jupiter close the time of the former perijove passage that maximizes overlap with other investigations. | ||||||
495 | visible/NUV | Wong | HST/WFC3 UVIS | hi-resolution map of perijove track | raw data available immediately from STScI archive; reduced maps and zonal wind profiles available within one month or potentially sooner; co-Is from MWR and JIRAM teams | Q | |||||
496 | CCD / near IR | Sanchez-Lavega | Calar Alto 2.2-m telescope / PlanetCam | 0.38-1.5 micron imaging | scheduled 2017 Jan 11-18 | TBD | |||||
497 | near IR | Orton | IRTF/SpeX guide camera | filtered imaging at 5 strategic wavelengths, including 5.1µm and 3.4µm (H3+ auroral emission). | Taken on Jan 23, 26: 05:30-06:30 Also supports Keck spectroscopy | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired | |||||
498 | near IR | Kita | IRTF/iSHELL | K-band imaging and high-resolution spectroscopy of H3+ emission | 1/07 01:00-07:00 HST 1/08 01:00-07:00 HST 1/09 01:00-07:00 HST 1/11 01:00-07:00 HST | Reduced data will be available upon request. | |||||
499 | near IR | Davies | Keck / NIRC2 | AO-stabilized imaging of Io at several wavelengths | Jan 3, 4, 7, 8 | TBD | |||||
500 | near IR | Skrutskie | Fan Mountain / 31" FanCam | Io H and K band flux, disk integrated | Jan 30 07:42-08:46 UT | TBD | |||||
501 | near IR | Schmidt | DCT IGRINS | Io H and K spectra R~40000 | Jan 14 09:26-10:34 UT Jan 21 11:20-12:28 UT | All night cancelled. Bad weather | Q | ||||
502 | near IR | O'Donoghue | Keck/NIRSPEC | H3+ spectra approx 3-4µm, R~25000, 24'' slit aligned N/S | Jan 25 10:00-16:00 UT; Feb 2; March 17 | Building up long-term dataset of Jupiter's northern and southern aurorae. Full auroral coverage (in H3+ temperature/density/radiance, and partial global coverage). Data reduction partially complete. | |||||
503 | 5-micron spectra | Bjoraker; de Pater | Keck/NIRSPEC | spectra of NH3,H2O | Taken on Jan 11 & 12. | fully reduced spectra available in 2 months | |||||
504 | 5-micron spectra | de Pater; Bjoraker | Keck/NIRSPEC | 5-mu spectra, H2O, NH3 | Taken on Jan. 23, 24 | TBD | |||||
505 | visible/uv | de Pater; Wong | HST WFC3 observations | contextual observations, coincident with Keck and VLA observations | Taken on Jan 11 & 12. | TBD | |||||
506 | near IR (5 µm) | Wong | Gemini-N/NIRI | lucky imaging, 5-µm maps, global coverage | 3 hr 11 Jan, 2 hr 12 Jan, 23 Jan | full maps available on junocam planning site within 2 weeks | |||||
507 | mid IR | Fletcher | VLT / VISIR | filtered radiometric imaging to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology. | Observations in 10 filters, Jan 10 2017, 07:23-08:26UT, immediately east of GRS, including mid-SEB outbreak. | available in raw form in the ESO archive within 24 hours of acquisition; cylindrical maps within 1-2 days and reduced maps within a week | |||||
508 | mid IR | Fletcher | VLT / VISIR | filtered radiometric imaging to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology. | Observations in 10 filters, Jan 11, 07:20-0830UT, including M-band burst mode. Immediately west of GRS. | available in raw form in the ESO archive within 24 hours of acquisition; cylindrical maps within 1-2 days and reduced maps within a week | |||||
509 | mid IR | Fletcher | IRTF/TEXES | scanned spectral maps of Jupiter's disk at ten key spectral settings to derive upper-tropospheric and stratospheric temperatures, aerosol/cloud distributions, and distribution of tropospheric NH3 and PH3, and stratospheric C2H2 and C2H6. | scans of Jupiter requested close to the perijove epoch Observed Jan 16 08:30-09:30, Jan 17 01:00-09:30 (both daylight observing), Jan 18 01:00-06:30 | raw data available almost immediately, calibrated files with geometry within a month, and retrieved properties potentially available within 1-2 weeks (subject to any unforeseen issues) | |||||
510 | mid IR | Kasaba Orton | Subaru / COMICS | filtered radiometric imaging and spectroscopy to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology and auroral heating and chemistry. | mid-infrared imaging of Jupiter requested using a full set of filters close to the original PJ8 with observations on an adjacent night to map the comlementary hemisphere. Imaging made through breaks in clouds Jan 10,11 | would like to see agreement in place with Juno science team first and discussed at the workshop, but willing to share. | |||||
511 | mid IR | Orton | Keck exchange time to use Subaru / COMICS | filtered radiometric imaging and spectroscopy to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology and auroral heating and chemistry. | mid-infrared imaging of Jupiter requested using a full set of filters close to the perijove time with observations on an adjacent night to map the comlementary hemisphere. Imaging and spectroscopy obtained under ideal conditions, January 12,13. | reduced observations available within 1-2 months; quick-look observations sooner | |||||
512 | mid IR | Greathouse | IRTF/TEXES | scanned high- and medium-resolution spectral maps of Jupiter's disk at key CH4- and H2-absorbing wavelengths to determine temperatures in the upper troposphere and stratosphere to determine the structure of non-seasonal thermal waves associated with the Quasi-Quadrennial Oscillation (QQO) | awarded Jan 14 03:30-09:30, Jan 15 01:00-09:30, Jan 16 01:00-08:30 (all daylight observing) | ||||||
513 | mid IR | Sinclair | IRTF/TEXES | scanned high-resolution spectral maps of Jupiter's disk at six key spectral settings to derive stratospheric temperatures and 3-dimensional distribution of stratospheric C2H2, C2H4, C2H6 and H3+ in auroral regions. | scans of Jupiter's polar regions requested within 1-2 days of the perijove passage, awarded Jan 18 06:30-09:30, Jan 19 01:00-09:30 (both daylight observing) | TBD | Q | ||||
514 | mid IR | Encrenaz | IRTF/TEXES | scanned medium-resolution spectral maps of Jupiter's disk at key wavelengths to determine the distributions of gaseous NH3 and PH3 in Jupiter's troposphere | awarded Jan 20 12:00-18:30, Jan 21 12:00-18:30 (both daylight observing) | ||||||
515 | mid IR | Orton | SOFIA/EXES | spatially resolved spectra along the central meridian for high-altitude temperature profile and HCN distribution. | 120-130 min on Jan 19/20 and 20/21 flithts. HCN observed at full request. Strong CH4 bands at high resolution covered only partially due to telescope pointing s/w failure and recovery on first night and slit placement confusion on second night. | TBD | |||||
516 | submillimeter / millimeter | de Pater | Atacama Large Millimeter Array (ALMA) | 1 and 3 mm continuum | acquired Jan 3, 4 | TBD | |||||
517 | microwave | de Pater | Very Large Array (VLA) | X band (8-12 GHz), A-config | acquired 11 Jan., coincident with former PJ8 | MWR PI Janssen is a Co-Investigator | |||||
518 | radio | Imai | Long Wavelength Array 1 (LWA1) | Jupiter's decametric auroral radio observations | Jan 21-26, Jan 28-31 | Request to M. Imai More information can be found at http://www-pw.physics.uiowa.edu/earth/ | |||||
519 | radio | Kita | GMRT (India) | L-band | Jan. 25 1:00-6:00IST | Reduced data will be available upon request. | |||||
520 | |||||||||||
521 | also maps with gemini; PI: Wong | ||||||||||
522 | |||||||||||
523 | |||||||||||
524 | |||||||||||
525 | |||||||||||
526 | |||||||||||
527 | |||||||||||
528 | |||||||||||
529 | |||||||||||
530 | |||||||||||
531 | |||||||||||
532 | |||||||||||
533 | |||||||||||
534 | |||||||||||
535 | |||||||||||
536 | |||||||||||
537 | |||||||||||
538 | |||||||||||
539 | |||||||||||
540 | |||||||||||
541 | |||||||||||
542 | |||||||||||
543 | |||||||||||
544 | |||||||||||
545 | |||||||||||
546 | Period: Orbit 4 [MWR] (2017 February 1 – 2017 March 26) | ||||||||||
547 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | |||||
548 | near IR | O’Donoghue | Keck / NIRSpec | high-resolution scanning spectroscopy of H3+ auroral emission for temperature mapping. | Feb 1: Good observations obtained. | Building up long-term dataset of Jupiter's northern and southern aurorae | |||||
549 | CCD imaging | Wong, de Pater | HST WFC3 observations | contextual observations, coincident with PJ4 | Feb 1 and Feb 2 | TBD | |||||
550 | CCD | Irwin | VLT/MUSE - IFU | spectroscopic imaging, 465-930 nm to determine cloud structure and albedo spectrum of particles. | 24/25 March 2017 | “reductions to photometrically-calibrated cubes can be done in a day or two if there is sufficient motivation!” | |||||
551 | VIS (R,G,B), >720nm,889nm | S. Poshyachinda, C. Go and T. Santikunaporn | Thailand National Observatory 2.4m and 0.7m Telescopes | Imaging in Visible Light, Near IR and Methand Band for PJ3. Jan 31-Feb 1 with the 2.4m and on Feb 2 with the 0.7m. Imaging the region 10hrs before and 10hrs after PJ3. | Jan 31, Feb 1 and Feb 2 | ||||||
552 | HST FUV | Grodent | HST STIS | UV aurora | HST/UT start time mm/dd/yyyy hh:mm:ss Exp. time ~ 47min 02/01/2017 12:20:26 02/02/2017 09:13:40 02/02/2017 10:31:21 02/02/2017 09:01:03 02/02/2017 13:46:13 02/02/2017 15:21:35 02/02/2017 16:57:53 01/31/2017 07:43:57 02/03/2017 08:50:35 02/03/201713:36:40 02/04/2017 08:41:03 02/04/2017 10:16:26 02/05/2017 06:56:14 02/06/2017 11:32:56 03/01/2017 15:54:00 03/05/2017 18:26:00 03/17/2017 08:36:00 03/18/2017 14:50:00 03/19/2017 09:54:00 03/20/2017 16:06:00 03/21/2017 11:11:00 03/21/2017 12:46:00 03/22/2017 07:51:00 03/23/2017 12:27:00 03/23/2017 14:03:00 03/24/2017 09:07:00 03/25/2017 05:47:00 03/26/2017 15:10:00 03/27/2017 03:53:00 03/27/2017 05:28:00 03/27/2017 07:03:00 03/27/2017 08:39:00 03/27/2017 10:14:00 03/27/2017 11:49:00 03/27/2017 13:25:00 | As of Feb 15, 2017 Times may change by re-scheduling on the part of HST | |||||
553 | CCD | Sanchez-Lavega | Aulo EspaZio Gela, Bilbao, Spain / 28-cm telescope | continuous imaging survey, 0.38-0.9 microns | continuous | TBD | |||||
554 | Visible | Schmidt | Apache Point Observatory / Dual Imaging Spectrograph (DIS) | Long-slit visible spectroscopy of both sides of the Io torus to determine S+, S++, O+ composition and electron density | 2/12/2017, 3/09/2017, 3/23/2017, 3/24/2017 | Calibrated data products available upon request | Q | ||||
555 | near IR | Johnson | IRTF/iSHELL | imaging and high-resolution spectroscopy of H3+ emission | Taken Feb 2, 3:30-9:00 HST --> clear skies, successful guiding. Several sucessful scans were taken of the southern aurora simultaneously with Juno. Images taken in varies filters. | Data reduction in process | |||||
556 | near IR | Kita | IRTF/iSHELL | imaging and high-resolution spectroscopy of H3+ emission | Mar 11, 23:00-3:00; Mar. 13, 23:59-04:00; Mar 16, 21:45-1:45; Mar. 18, 23:00-03:00; Mar. 21 1:00-5:00; Mar 23, 23:00 - 3:00 (Cloudy) | Reduced data will be available upon request. | Q | ||||
557 | near IR | de Pater, Bjoraker | Keck/NIRSPEC; joint observations with Hubble Space Telescope Feb 1-2 | 5-µm spectra of NH3,H2O | Taken on Feb, 4, 5, 6 Feb 4 &6 data cover the longitude of PJ4 (277 degrees System III) | fully reduced spectra available in 2 months | |||||
558 | near IR | Bjoraker | IRTF/iSHELL | high-resoution spectroscopy of Jupiter in the 5-µm window to determine NH3, H2O abundances and propeties of water clouds at similar locations and nearly the same time as Juno | Taken Mar 26 0:30-6:30 HST; good seeing & low humidity cover longitude of new PJ5: 187 System III | fully reduced spectra available in 2 months | |||||
559 | near IR (5 µm) | Wong | Gemini-N/NIRI | lucky imaging, 5-µm maps | service time; Feb 1 and Feb 5 | full maps available on junocam planning site within 2 weeks | |||||
560 | near IR | Orton | Gemini-N/NIRI | AO-stabilized imaging of Jupiter at several wavelengths | images obtained on service time Jan 30, Feb 5 | TBD | |||||
561 | near IR | Orton | IRTF/SpeX | filtered imaging at several wavelengths between 1.58 and 5.1µm and spectral scanning over 2-µm and 5-µm ranges | Feb 2, 01:30-3:30 HST; Feb 3, 1:30-6:30 HST | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired. Reduced "quick-look" observations (geometrically but not radiometrically calibrated) will be available for immeduately use from the Juno-curated web site: http://junoirtf.space.swri.edu/ | |||||
562 | near IR | Orton | IRTF/SpeX guide camera | filtered imaging at several near-infrared wavelengths, including H3+ emission at 3.14µm and thermal emission at 5.1 µm. | obtained on Feb 15, 3:20-4:00 HST; Feb 16, 05:30-6:30 HST; Feb 23, 4:50-5:30 HST; Feb 24, 3:20-4:00 HST; Mar 15, 2:00-2:45 HST; Mar 16 5:40-6:30 HST; Mar 22, 3:45-4:30 HST | raw images available immediately from IRTF web site. Reduced "quick-look" observations (geometrically but not radiometrically calibrated) will be available for immeduately use from the Juno-curated web site: http://junoirtf.space.swri.edu/ | |||||
563 | mid IR | Fletcher | VLT / VISIR | filtered radiometric imaging to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology. | Observed Feb 5th (08:33-09:29UT) and Feb 6th (04:36-05:34UT). We have a northern and southern OB (100 minutes total), in addition to a single burst-mode M-band OB (20 minutes), totalling 120 minutes. | available in raw form in the ESO archive within 24 hours of acquisition; cylindrical maps within 1-2 days and reduced maps within a week | |||||
564 | mid IR | Fletcher | VLT / VISIR | filtered radiometric imaging to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology. | Observed Mar 16, 3:34 -5:47 UT. | available in raw form in the ESO archive within 24 hours of acquisition; cylindrical maps within 1-2 days and reduced maps within a week | |||||
565 | near IR | O’Donoghue | Keck / NIRSpec | high-resolution scanning spectroscopy of H3+ auroral emission for temperature mapping. | Mar 16: Good observations obtained. | Building up long-term dataset of Jupiter's northern and southern aurorae | |||||
566 | mid IR | Flecher | Gemini N / TEXES | scanned spectral maps of Jupiter's disk at ten key spectral settings to derive upper-tropospheric and stratospheric temperatures, aerosol/cloud distributions, and distribution of tropospheric NH3 and PH3, and stratospheric C2H2 and C2H6. | scans of Jupiter completed, March 11-13 | raw data available almost immediately, calibrated files with geometry within a month, and retrieved properties potentially available within 1-2 weeks (subject to any unforeseen issues) | |||||
567 | mid IR | Greathouse | Gemini N / TEXES | scanned high- and medium-resolution spectral maps of Jupiter's disk at key CH4- and H2-absorbing wavelengths to determine temperatures in the upper troposphere and stratosphere to determine the structure of non-seasonal thermal waves associated with the Quasi-Quadrennial Oscillation (QQO) | scans of Jupiter obtained in the March 10-21 time frame; initiated March 13 | raw data available in 2-3 days, reduced and remapped to lat/lon in 1 month (could be done faster if requested) | |||||
568 | mid IR | Sinclair | Gemini N / TEXES | scanned high-resolution spectral maps of Jupiter's disk at six key spectral settings to derive stratospheric temperatures and 3-dimensional distribution of stratospheric C2H2, C2H4, C2H6 and H3+ in auroral regions. | scans of Jupiter obtained in the March 10-21 time frame; initiated March 13 (March 17, 18, 19) | TBD | |||||
569 | microwave | de Pater | Very Large Array (VLA) | Probably D configuration in D band 1.3 cm | Feb 1-2 | MWR PI Janssen is a Co-Investigator | |||||
570 | sub-mm | Roth / Sanchez-Monge | IRAM NOEMA | Io SO2 atmosphere | One 5-h track obtained on Feb 11. Bad conditions, analysis ongoing | Request to Lorenz Roth | Q | ||||
571 | radio | Kita | GMRT (India) | L-band | Feb. 08 2:00-8:00IST | Reduced data will be available upon request. | |||||
572 | radio | Imai | Long Wavelength Array 1 (LWA1) | Jupiter's decametric auroral radio observations | Feb 1-7, Mar 17-27 | Request to M. Imai | |||||
573 | X-ray | Caitriona Jackman | Chandra | 72 ks (20 hours) continuous observation by Chandra around apojove | 2017:059:12:54:07.255 for 72.0 ks | Request to Jackman. Keen to collaborate with Juno team as contemporaneous in situ data will help to constrain the X-ray drivers thought to map to this region | |||||
574 | X-ray | Gladstone | Chandra | ~10 hours of HRC observations of Jupiter | 02/02/2017 09:58-19:42 | publicly available 2/8/2018 | |||||
575 | |||||||||||
576 | Scheduled observations by Juno. | ||||||||||
577 | |||||||||||
578 | Perijove is 2017 February 2, 12:59:12 UTC. System-III longitude = 277°W | ||||||||||
579 | |||||||||||
580 | Period: Orbit 4 [MWR] (2017 February 1 - March 26) | ||||||||||
581 | Instrument | Description | |||||||||
582 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | |||||||||
583 | MWR | N/S scans near perijove longitude, centered on nadir. | |||||||||
584 | UVS | TBD | |||||||||
585 | JunoCam | E/PO observations targeting features voted on by public. | |||||||||
586 | JIRAM | TBD | |||||||||
587 | |||||||||||
588 | Note: On this next orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed directly at the Earth. | ||||||||||
589 | |||||||||||
590 | |||||||||||
591 | |||||||||||
592 | |||||||||||
593 | |||||||||||
594 | |||||||||||
595 | |||||||||||
596 | |||||||||||
597 | |||||||||||
598 | |||||||||||
599 | |||||||||||
600 | |||||||||||
601 | |||||||||||
602 | |||||||||||
603 | |||||||||||
604 | |||||||||||
605 | |||||||||||
606 | |||||||||||
607 | |||||||||||
608 | |||||||||||
609 | |||||||||||
610 | |||||||||||
611 | |||||||||||
612 | |||||||||||
613 | |||||||||||
614 | |||||||||||
615 | |||||||||||
616 | |||||||||||
617 | |||||||||||
618 | |||||||||||
619 | |||||||||||
620 | |||||||||||
621 | |||||||||||
622 | |||||||||||
623 | |||||||||||
624 | |||||||||||
625 | |||||||||||
626 | |||||||||||
627 | |||||||||||
628 | |||||||||||
629 | |||||||||||
630 | |||||||||||
631 | |||||||||||
632 | |||||||||||
633 | |||||||||||
634 | |||||||||||
635 | |||||||||||
636 | |||||||||||
637 | |||||||||||
638 | |||||||||||
639 | |||||||||||
640 | |||||||||||
641 | |||||||||||
642 | |||||||||||
643 | |||||||||||
644 | |||||||||||
645 | |||||||||||
646 | Period: Orbit 5 [MWR/tilt] (2017 March 27 – 2017 May 17) | ||||||||||
647 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | |||||
648 | FUV | Grodent | HST/FUV-MAMA | high spatial and temporal resolution FUV observations of magnetosphere and ultraviolet auroras | 2017-03-28 03:45:30 2017-03-28 11:42:24 2017-03-28 13:17:40 2017-03-29 08:22:00 2017-03-30 03:26:22 2017-03-30 05:01:44 2017-03-31 09:38:20 2017-04-01 06:18:07 2017-04-19 19:27:01 2017-04-23 14:00:08 2017-05-09 06:42:14 | Times may change by re-scheduling on the part of HST | |||||
649 | visible/CCD | Wong | HST/WFC3 | Multiple-filtered imaging, 275-885 nm; two rotations of Jupiter to determine structure and properties of clouds and aerosols at high resolution, define atmospheric flow and search for waves. (Outer Planet Atmospheric Legacy [OPAL] program) | "snapshot" images acquired close to March 27 perijove | raw data available immediately from STScI archive; reduced maps and zonal wind profiles available within one month or potentially sooner; co-Is from MWR and JIRAM teams | |||||
650 | CCD | Sanchez-Lavega | Aulo EspaZio Gela, Bilbao, Spain / 28-cm telescope | continuous imaging survey, 0.38-0.9 microns (U (ultraviolet), 890 nm (methane), R610, R685, R,G,B, 727 nm (methane)) | 04/07, 04/08, 04/11, 04/12, 04/21, 04/22, 04/23 | Images available at PVOL2 and Aula EspaZio web page. | |||||
651 | CCD | Sanchez-Lavega | Aula EspaZio Gela 36-cm telescope at Calar Alta Observatory | continuous imaging survey, Wavelengths: R, V, B, IR, R610, 890nm (methane), R610 | 03/30, 04/08, 04/09, 04/10, 04/12, 05/03 | Images available at PVOL2 and Aula EspaZio web page. | |||||
652 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | 2017-03-07 2017-03-08 2017-03-09 2017-03-12 2017-03-13 2017-03-14 2017-03-15 2017-03-17 2017-04-14 2017-04-15 2017-04-16 2017-04-18 2017-04-19 2017-04-20 2017-04-21 2017-04-24 2017-04-26 2017-04-27 2017-04-28 2017-05-01 2017-05-02 2017-05-03 2017-05-04 | ||||||
653 | Visible | Schmidt | Apache Point Observatory / Dual Imaging Spectrograph (DIS) | Long-slit visible spectroscopy of both sides of the Io torus to determine S+, S++, O+ composition and electron density | 3/31/2017, 5/11/2017 | Calibrated data products available upon request | Q | ||||
654 | CCD / near IR | Sanchez-Lavega | Calar Alto 2.2-m telescope / PlanetCam | 0.38-1.7 micron imaging Wavelengths: From 0.38 to 1.7 microns in a large number of spectral bands (see Mendikoa et al., PASP. 2016) | 03/28, 03/29, 03/29-30, 03/30-31 | Photometric versions available within two weeks. Processed images will be available later. | |||||
655 | near IR | Skrutskie | Fan Mountain / 31" FanCam | Io H and K band flux, disk integrated | |||||||
656 | Bjoraker | IRTF/iSHELL | high-resoution spectroscopy of Jupiter in the 5-µm window to determine NH3, H2O abundances and propeties of water clouds at similar locations and nearly the same time as Juno | Taken Mar 28, 0:30-6:30 HST good seeing & low humidity cover longitude of new PJ5: 187 System III | fully reduced spectra available in 2 months | ||||||
657 | near IR | Orton | IRTF/SpeX | filtered imaging at several wavelengths between 1.58 and 5.1µm and spectral scanning over 2-µm and 5-µm ranges | obtained on Mar 27, 01:30-6:30 HST; Mar 28, 21:30-Mar 29 03:30 HST | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired. Reduced "quick-look" observations (geometrically but not radiometrically calibrated) will be available for immeduately use from the Juno-curated web site: http://junoirtf.space.swri.edu/ | |||||
658 | near IR | Johnson | IRTF/iSHELL | Scans of the southern auroral H3+ emission at ~3.4µm. Simultaneous to JIRAM, MAG, JADE and JEDI measurements. | Data obtained on Mar 26th 20:30 - 01:30 HST --> clear skies, successful guiding. Several sucessful scans were taken of the northern aurora just after perijove. Images taken main in the H3+ filter, some taken with 5.1 filter near to end of observing. Extra iSHELL time: 20th April 21:20 - 00:20 HST scanning the northern aurora, H3+ and 5.1 micron images & 21st April 22:20 - 01:20 HST scanning the southern aurora H3+ and 5.1 images. | Data reduction in process. | |||||
659 | near IR | Moore | IRTF/iSHELL | E-W spectral scans of Jupiter’s northern auroral region – rough cut of spectral images obtained, will ultimately yield a series of auroral H3+ temperature/density/radiance maps, one every ~30 min | 4/26/2017 and 4/28/2017 | Data reduction in process. Rough spectral images obtained. | |||||
660 | near IR | Orton | IRTF/SpeX guide camera | filtered imaging at several near-infrared wavelengths, including H3+ emission at 3.14µm and thermal emission at 5.1 µm. | Mar 30, 3:00-3:40 HST; Mar 31 | raw images available immediately from IRTF web site. Reduced "quick-look" observations (geometrically but not radiometrically calibrated) will be available for immeduately use from the Juno-curated web site: http://junoirtf.space.swri.edu/ | |||||
661 | sub-mm | Roth / Sanchez Monge | IRAM NOEMA | Io SO2 atmosphere | 1 track, March 14-15, good conditions | TBD, reqeust to Roth | Q | ||||
662 | radio | Imai | Long Wavelength Array 1 (LWA1) | Jupiter's decametric auroral radio observations | Mar 28-30, Apr 1 | Request to M. Imai More information can be found at http://www-pw.physics.uiowa.edu/earth/ | |||||
663 | radio | Kita | GMRT (India) | L-band | 25Mar2017 22-1 (IST) 26Mar2017 21-1 (IST) | Reduced data will be available upon request. | |||||
664 | X-ray | Gladstone | Chandra | ~2 hours of HRC observations of Jupiter | 03/27/2017 08:32-11:39 | publicly available 3/28/2018 | |||||
665 | Scheduled observations by Juno. | ||||||||||
666 | |||||||||||
667 | Perijove 5 on is 2017 March 27, 8:53:20 UTC at Juno. System-III longitude = 187.0°W | ||||||||||
668 | |||||||||||
669 | Period: Orbit 5 [MWR/tilt] (2017 March 26 – 2017 May 17) | ||||||||||
670 | Instrument | Description | |||||||||
671 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | |||||||||
672 | MWR | N/S scans near perijove longitude, not centered on nadir. | |||||||||
673 | UVS | TBD | |||||||||
674 | JunoCam | E/PO observations targeting features voted on by public. | |||||||||
675 | JIRAM | TBD | |||||||||
676 | |||||||||||
677 | |||||||||||
678 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed directly at the Earth. | ||||||||||
679 | |||||||||||
680 | |||||||||||
681 | Period: Orbit 6 [GRAV] (2017 May 18 – 2017 July 9) | ||||||||||
682 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | |||||
683 | X-ray | Gladstone | Chandra | ~10 hours of HRC observations of Jupiter | 2017-May-19 01:43-11:43 | publicly available after 1 year | |||||
684 | X-ray | Caitriona Jackman | Chandra | 36 ks (10 hours) continuous observation by Chandra | Obs #1: June 12th-19th 2017 Possibly coincident with XMM 2017-Jun-18 (DoY 169) T20:29:60 to 2017-Jun-19 (DoY 170) T20:06:40 (85 ks)) and/or with HST 2017-Jun-18 (DoY 169) T20:29:60 to 2017-Jun-19 (DoY 170) T20:06:40 (85 ks) | Request of Jackman. Keen to collaborate with Juno team as contemporaneous in situ data will help to constrain the X-ray drivers thought to map to this region | |||||
685 | Hard X-ray | Jackman (collaboration with Mori, Dunn, Branduardi-Raymont, Gladstone etc.) | NuSTAR | Long observation to cover interval around Juno apojove, coincident with: Chandra, XMM, HST | 2017:169:06:40:16 to 2017:171:18:05:00 | Request of Jackman and Mori | |||||
686 | Hard X-ray | Mori | NuSTAR | 130 ks overlapping with the Chandra obesrvation | TBD, but will span the Chandra observation on 2017-May-19 | Public after 1 year | |||||
687 | FUV | Grodent | HST/FUV-MAMA | high spatial and temporal resolution FUV observations of magnetosphere and ultraviolet auroras | Times may change by re-scheduling on the part of HST | ||||||
688 | visible/NUV | Wong | HST/WFC3 UVIS | hi-resolution map of perijove track | one orbit (50 min obs.) ~1-3 hours before perijove pass if possible, otherwise within one rotation of pass | raw data available immediately from STScI archive; reduced maps and zonal wind profiles available within one month or potentially sooner; co-Is from MWR and JIRAM teams | |||||
689 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | Continuous | ||||||
690 | Visible | Schmidt | Apache Point Observatory / Dual Imaging Spectrograph (DIS) | Long-slit visible spectroscopy of both sides of the Io torus to determine S+, S++, O+ composition and electron density | May 19 | Calibrated data products available upon request | |||||
691 | CCD | Sanchez-Lavega | Aulo EspaZio Gela, Bilbao, Spain / 28-cm telescope | continuous imaging survey, 0.38-0.9 microns | continuous | TBD | |||||
692 | CCD / near IR | Sanchez-Lavega | Calar Alto 2.2-m telescope / PlanetCam | 0.38-1.7 micron imaging | scheduled 2017 Jun 12-15 | Generally available within two weeks (photometric version). High-resolution versions available later on. | |||||
693 | CCD | Irwin | VLT/MUSE - IFU | spectroscopic imaging, 465-930 nm to determine cloud structure and albedo spectrum of particles. | May 15 | “reductions to photometrically-calibrated cubes can be done in a day or two if there is sufficient motivation!” | |||||
694 | CCD | Irwin | VLT/MUSE - IFU | spectroscopic imaging, 465-930 nm to determine cloud structure and albedo spectrum of particles. | May 28 | ||||||
695 | near IR | Skrutskie | Fan Mountain / 31" FanCam | Io H and K band flux, disk integrated | TBD | ||||||
696 | near IR | Johnson | IRTF/iSHELL | imaging and high-resolution spectroscopy of H3+ emission | obtained May 18, 19:30-22:00 HST | TBD | |||||
697 | near IR | Bjoraker | IRTF/iSHELL | high-resoution spectroscopy of Jupiter in the 5-µm window to determine NH3, H2O abundances and propeties of water clouds at similar locations and nearly the same time as Juno | Taken May 17, 18:15 - May 18, 0:15 HST; and same time on May 20-21 HST; May 18:excellent seeing (0.3 arcsec) and low humidity (10%), May 21:0.6arcsec seeing and 20% humidity | fully reduced spectra available in 2 months | |||||
698 | near IR | Orton | IRTF/SpeX | filtered imaging at several wavelengths between 1.58 and 5.1µm and spectral scanning over 2-µm and 5-µm ranges | obtained on May 18, 22:00-01:30 HST; May 19, 18:15- May 20, 1:15 HST | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired. Reduced "quick-look" observations (geometrically but not radiometrically calibrated) will be available for immeduately use from the Juno-curated web site: http://junoirtf.space.swri.edu/ | |||||
699 | near IR | Orton | IRTF/SpeX guide camera | filtered imaging at several near-infrared wavelengths, including H3+ emission at 3.14µm and thermal emission at 5.1 µm. | scheduled for Jun 7 18:20-19:20 HST, Jun 18, 19:00-19:45 HST; Jun 19, 21:20-22:00 HST, Jun 25, 18:20-19:35 HST; Jul 9, 19:30-20:10 HST | raw images available immediately from IRTF web site. Reduced "quick-look" observations (geometrically but not radiometrically calibrated) will be available for immeduately use from the Juno-curated web site: http://junoirtf.space.swri.edu/ | |||||
700 | near IR | Chudczer | Gemini N/GIRS | Spectroscopic polar mapping of auroral H3+ emission | successful observations on May 19 | TBD | |||||
701 | mid IR | Greathouse | IRTF/TEXES | scanned high- and medium-resolution spectral maps of Jupiter's disk at key CH4- and H2-absorbing wavelengths to determine temperatures in the upper troposphere and stratosphere to determine the structure of non-seasonal thermal waves associated with the Quasi-Quadrennial Oscillation (QQO) | scheduled May 27-28, 17:15 - 23:00 HST | TBD | |||||
702 | mid IR | Kasaba Orton | Subaru / COMICS | filtered radiometric imaging and spectroscopy to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology and auroral heating and chemistry. | Mid-infrared imaging and spectroscopy of Jupiter scheduled May 17-18 (Orton, Subaru Keck-exchange time), May 19-20 (Kasaba, Subaru direct time) 05:00-10:00 UT. May 17: two full sets of filters and 8-14 micron scanned spectroscopy of Oval BA and adjacent latitude. May 18: three full sets of filtered images and 8-14 micron scanned spectroscopy of GRS, NEB with slit parallel to the equator, and of the PJ6 longitude with slit parallel to the rotation axis. May 19: one single-hemisphere set of images 1.5 hours before PJ9 and three subsequent full images at all wavelengths, plus scans of NEB; May 20: three sets of images, spectral scans of: south polar aurora, GRS and wake, and PJ9 longitude. Seeing on May 17-19 was 0.3-0.5" at 10 microns; May 20 degraded to 0.6". | Kasaba would like to see agreement in place with Juno science team first and discussed at the workshop, but willing to share. Orton will share immediately. | |||||
703 | mid IR | Sinclair | IRTF/TEXES | scanned high-resolution spectral maps of Jupiter's disk at six key spectral settings to derive stratospheric temperatures and 3-dimensional distribution of stratospheric C2H2, C2H4, C2H6 and H3+ in auroral regions. | scheduled May 30 - 31, 17:15 - 21:45 HST | TBD | |||||
704 | mid IR | Fouchet | IRTF/TEXES | scanned high-resolution spectral maps of Jupiter's disk to make methyl as a function of latitude | scheduled Jun 1, 3:00 - 5:15 HST | TBD | |||||
705 | radio | Imai | Long Wavelength Array 1 (LWA1) | Jupiter's decametric auroral radio observations | May 10, 11, 12, 13, 14, 16, 17 | Request to M. Imai More information can be found at http://www-pw.physics.uiowa.edu/earth/ | |||||
706 | radio | Kita | GMRT (India) | L-band | 18May2017 18:00-24:00 IST | Reduced data will be available upon request. | |||||
707 | |||||||||||
708 | Scheduled observations by Juno. | ||||||||||
709 | |||||||||||
710 | Perijove is 2017 May 19, 17:44:04 UTC at Juno. System-III longitude = 142°W | ||||||||||
711 | |||||||||||
712 | Period: Orbit 6 [GRAV] (2017 May 18 – 2017 July 9) | ||||||||||
713 | Instrument | Description | |||||||||
714 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | |||||||||
715 | MWR | N/S scans near perijove longitude, not centered on nadir. | |||||||||
716 | UVS | TBD | |||||||||
717 | JunoCam | E/PO observations targeting features voted on by public. | |||||||||
718 | JIRAM | TBD | |||||||||
719 | |||||||||||
720 | |||||||||||
721 | |||||||||||
722 | |||||||||||
723 | |||||||||||
724 | |||||||||||
725 | |||||||||||
726 | |||||||||||
727 | |||||||||||
728 | |||||||||||
729 | |||||||||||
730 | |||||||||||
731 | |||||||||||
732 | |||||||||||
733 | |||||||||||
734 | |||||||||||
735 | |||||||||||
736 | |||||||||||
737 | |||||||||||
738 | |||||||||||
739 | |||||||||||
740 | |||||||||||
741 | |||||||||||
742 | |||||||||||
743 | |||||||||||
744 | |||||||||||
745 | |||||||||||
746 | |||||||||||
747 | |||||||||||
748 | |||||||||||
749 | |||||||||||
750 | |||||||||||
751 | |||||||||||
752 | |||||||||||
753 | |||||||||||
754 | |||||||||||
755 | |||||||||||
756 | Note: On this orbit the spacecraft orientation optimizes MWR sensing with the antenna pointed to achieve nadir or near-nadir observations. Current (2016 Dec 28) drift rates show a close overflight of the Great Red Spot. | ||||||||||
757 | |||||||||||
758 | Period: Orbit 7 [MWR tilt] (2017 July 10 – 2017 August 30) | ||||||||||
759 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | |||||
760 | Hard X-ray | Mori | NuSTAR | Approved GO program. Hard X-ray (>2 keV) coverage. | Nominally 2017-Jul-10 to 2017-Jul-12, but will likely match the XMM schedule. | ||||||
761 | X-ray | Caitriona Jackman | Chandra | 36 ks (10 hours) continuous observation by Chandra | August 1st-7th 2017 36 ks (10-hour) observation with Chandra. No overlap with any other remote campaigns and alignment with Juno activities will be a priority. | Request to Jackman. Keen to collaborate with Juno team as contemporaneous in situ data will help to constrain the X-ray drivers thought to map to this region | |||||
762 | X-ray | Gladstone | Chandra | ~10 hours of HRC observations of Jupiter | 2017-Jul-10 21:44 - 2017-Jul-11 07:44 | publicly available after 1 year | |||||
763 | FUV | Grodent | HST/FUV-MAMA | high spatial and temporal resolution FUV observations of magnetosphere and ultraviolet auroras | Times may change by re-scheduling on the part of HST | ||||||
764 | CCD | Machado | UVES/VLT | Spectroscopic scan (visible to UV) in order to measure Doppler winds | raw data available in a couple of weeks | ||||||
765 | CCD | Ip | Lulin 1-m/35-cm | UVBRI and CH4 filters | raw data available in a couple of weeks | ||||||
766 | CCD | Irwin | VLT/MUSE - IFU | spectroscopic imaging, 465-930 nm to determine cloud structure and albedo spectrum of particles. | July 11 | “reductions to photometrically-calibrated cubes can be done in a day or two if there is sufficient motivation!” | |||||
767 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | |||||||
768 | visible/NUV | Wong | HST/WFC3 UVIS | hi-resolution map of perijove track | raw data available immediately from STScI archive; reduced maps and zonal wind profiles available within one month or potentially sooner; co-Is from MWR and JIRAM teams | ||||||
769 | CCD | Sanchez-Lavega | Aulo EspaZio Gela, Bilbao, Spain / 28-cm telescope | continuous imaging survey, 0.38-0.9 microns | continuous | TBD | |||||
770 | CCD / near IR | Sanchez-Lavega | Calar Alto 2.2-m telescope / PlanetCam | 0.38-1.7 micron imaging | Requested 4 nights around 11 July. Waiting for aproval from the observatory Time Allocation Comittee. | Generally available within two weeks (photometric version). High-resolution versions available later on. | |||||
771 | Fletcher | Fletcher | IRTF/TEXES | scanned spectral maps of Jupiter's disk at ten key spectral settings to derive upper-tropospheric and stratospheric temperatures, aerosol/cloud distributions, and distribution of tropospheric NH3 and PH3, and stratospheric C2H2 and C2H6. | scheduled Jul 14-15, 17:15 - 21:30 HST | raw data available almost immediately, calibrated files with geometry within a month, and retrieved properties potentially available within 1-2 weeks (subject to any unforeseen issues) | |||||
772 | mid IR | Greathouse | IRTF/TEXES | scanned high- and medium-resolution spectral maps of Jupiter's disk at key CH4- and H2-absorbing wavelengths to determine temperatures in the upper troposphere and stratosphere to determine the structure of non-seasonal thermal waves associated with the Quasi-Quadrennial Oscillation (QQO) | scheduled Jul 11-13,17:15 - 21:00 HST | TBD | |||||
773 | mid IR | Sinclair | IRTF/TEXES | scanned high-resolution spectral maps of Jupiter's disk at six key spectral settings to derive stratospheric temperatures and 3-dimensional distribution of stratospheric C2H2, C2H4, C2H6 and H3+ in auroral regions. | scheduled Jul 10, 17:15 - 21:30 HST; Jul 16, 17 17:15 - 20:30 HST | TBD | |||||
774 | mid IR | Fletcher | VLT / VISIR | filtered radiometric imaging to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology. | available in raw form in the ESO archive within 24 hours of acquisition; cylindrical maps within 1-2 days and reduced maps within a week | ||||||
775 | sub-mm | Roth / Sanchez Monge | IRAM NOEMA | Io SO2 atmosphere | 1 track, some tome in May/June | TBD. Request to Roth | |||||
776 | X-ray | Caitriona Jackman | Chandra | 36 ks (10 hours) continuous observation by Chandra | At or within a few days or apojove August 6th. | Request to Jackman. Keen to collaborate with Juno team as contemporaneous in situ data will help to constrain the X-ray drivers thought to map to this region | |||||
777 | radio | Kita | GMRT (India) | L-band | 10Jul2017 14:00-20:00 IST | Reduced data will be available upon request. | |||||
778 | |||||||||||
779 | Scheduled observations by Juno. | ||||||||||
780 | |||||||||||
781 | Perijove is 2017 July 11, 1:55:56 UTC. System-III longitude = 52°W | ||||||||||
782 | |||||||||||
783 | Period: Orbit 7 (2017 July 10 – 2017 August 29) | ||||||||||
784 | Instrument | Description | |||||||||
785 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | |||||||||
786 | MWR | N/S scans near perijove longitude, not centered on nadir. | |||||||||
787 | UVS | TBD | |||||||||
788 | JunoCam | E/PO observations targeting features voted on by public. | |||||||||
789 | JIRAM | TBD | |||||||||
790 | |||||||||||
791 | |||||||||||
792 | |||||||||||
793 | Note: On this orbit the spacecraft orientation optimizes gravity mapping (GRAV) with the antenna pointed toward the Earth continuously. | ||||||||||
794 | |||||||||||
795 | Period: Orbit 8 [GRAV] (2017 August 30 – 2017 October 22) | ||||||||||
796 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | |||||
797 | Hard X-ray | Mori | NuSTAR | Approved GO program. Hard X-ray (>2 keV) coverage. | 130 ks covering the September 1 Perijove. Likely will match the XMM observations. | ||||||
798 | CCD | Irwin | VLT/MUSE - IFU | spectroscopic imaging, 465-930 nm to determine cloud structure and albedo spectrum of particles. | September 1st | “reductions to photometrically-calibrated cubes can be done in a day or two if there is sufficient motivation!” | |||||
799 | near IR | Orton | IRTF/SpeX guide camera | filtered imaging at several near-infrared wavelengths, including H3+ emission at 3.14µm and thermal emission at 5.1 µm. | scheduled for Jul 18, 18:25-19:25; Jul 25 18:25-19:25 | raw images available immediately from IRTF web site. Reduced "quick-look" observations (geometrically but not radiometrically calibrated) will be available for immeduately use from the Juno-curated web site: http://junoirtf.space.swri.edu/ | |||||
800 | mid IR | Fletcher | VLT / VISIR | filtered radiometric imaging to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology. | available in raw form in the ESO archive within 24 hours of acquisition; cylindrical maps within 1-2 days and reduced maps within a week | ||||||
801 | |||||||||||
802 | |||||||||||
803 | Scheduled observations by Juno. | ||||||||||
804 | |||||||||||
805 | Perijove is 2017 September 1, 21:50:01 UTC. System-III longitude = 322°W | ||||||||||
806 | Instrument | Description | |||||||||
807 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | |||||||||
808 | MWR | N/S scans near perijove longitude, not centered on nadir. | |||||||||
809 | UVS | TBD | |||||||||
810 | JunoCam | E/PO observations targeting features voted on by public. | |||||||||
811 | JIRAM | TBD | |||||||||
812 | |||||||||||
813 | |||||||||||
814 | The mission has been approved for 53-day orbits. Blocks must still be created for those opportunities. | ||||||||||
815 | For the interim, a summary of the subsequent orbit perjoves is as follows: | ||||||||||
816 | Perijove | Date | SCET (UTC) | x-equatorial longitude (System III) | |||||||
817 | 9 | 2017 October 24 | 17:42:56 | 232 | |||||||
818 | 10 | 2017 December 16 | 17:57:39 | 300 | |||||||
819 | 11 | 2018 February 7 | 13:52:15 | 210 | |||||||
820 | 12 | 2018 April 1 | 9:46:15 | 120 | |||||||
821 | 13 | 2018 May 24 | 5:40:17 | 30 | |||||||
822 | 14 | 2018 July 16 | 5:17:35 | 75 | |||||||
823 | 15 | 2018 Septmber 7 | 1:12:38 | 345 | |||||||
824 | 16 | 2018 October 29 | 21:06:41 | 255 | |||||||
825 | 17 | 2018 December 21 | 17:00:44 | 165 | |||||||
826 | 18 | 2019 February 12 | 17:35:05 | 243 | |||||||
827 | 19 | 2019 April 6 | 13:29:05 | 153 | |||||||
828 | 20 | 2019 May 29 | 9:23:10 | 63 | |||||||
829 | 21 | 2019 July 21 | 5:57:35 | 333 | |||||||
830 | 22 | 2019 September 11 | 20:13:35 | 62 (deorbit) |
1 | ||||||||||
---|---|---|---|---|---|---|---|---|---|---|
2 | Earth-Based Juno-Supporting Observations of Jupiter and Its Environment: | |||||||||
3 | ||||||||||
4 | ALERT: THERE HAS BEEN A MAJOR CHANGE IN THE MISSION PERIJOVE TIMING. THE SCHEDULE OF JUNO PERIJOVES 3 AND 4 IS NOW LIKELY TO | |||||||||
5 | BE 2016 DEC 11 AT 14:36 SPACECRAFT EVENT TIME (SCET) OVER SYSTEM III LONGITUDE 277 DEG W, AND 2017 FEB 2 AT 10:30 SCET OVER LONGITUDE 187 DEG W. | |||||||||
6 | THIS DECISION WAS MADE FOLLOWING UNEXPECTED BEHAVIOR OF VALUES IN THE JUNO ENGINE VALVES. MORE DETAIL CAN BE FOUND AT THIS | |||||||||
7 | WEB SITE: http://www.jpl.nasa.gov/news/news.php?feature=6648. | |||||||||
8 | Observations are coded as follows: contemplated, proposed, awarded, completed | |||||||||
9 | ||||||||||
10 | Note: availability of all data are subject to appropriate collaborative agreements between the observers and Juno team members. | |||||||||
11 | ||||||||||
12 | Period: Jupiter Approach (2015 November 1 – 2016 July 3 [JOI-2d] | |||||||||
13 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | ||||
14 | X-ray | Kraft | Chandra / HRC | GTO time awarded for approach science / Juno support | ~10hrs on May 24 and June 1 | |||||
15 | X-ray | Dunn | XMM | 160 ks (44.5 h) requested for approach science / Juno support | ~10hrs on May 17-18, and 24 | "very keen to partner with any willing Juno teams to share findings, enrich the analysis and inform what might cause any X-ray variations we observe" | ||||
16 | X-ray | Ezoe | Hitomi(Astro-H) | 100 ks during the Performance Verification phase | spacecraft anomaly leading to mission failure | no data | ||||
17 | FUV | Nichols | HST/STIS | imaging and spectroscopy of Jupiter’s auroral regions | observations acquired May 16, 17, 18, 18, 21, 22, 23, 24, 25, 26, 27, 28, 29, 30, 31; Jun 1, 2, 3, 4, 5, 6, 7, 22, 23, 24, 26, 27, 30 | data made available to Juno team asap; many are already Co-Is. Time-lapse images are available for download from ftp://ftp.ion.le.ac.uk/HST. | ||||
18 | FUV/ EUV | Kimura, Yoshikawa | Hisaki/ EXCEED | Spectroscopy of Jupiter UV aurura (total flux) and EUV spectrum of Io torus (spatially resolved) | continuous observations, 2015 Dec – 2016 Jun (except Mar 4 to Apr 21 and Apr 26 to May 4) 2016 Jan 21-31 2016 Feb 1-29 2016 Mar 1-3, 5-31 2016 Apr 13, 22-26 2016 May 4-31 2016 Jun 1-30 2016 Jul 1-8 | Available to persons who are approved to join Hisaki Science Team | ||||
19 | CCD | Simon | HST/WFC3 | Multiple-filtered imaging, 275-885 nm; two rotations of Jupiter to determine structure and properties of clouds and aerosols at high resolution, define atmospheric flow and search for waves. (Outer Planet Atmospheric Legacy [OPAL] program) | Images acquired on 2016 February 9-10 UTC. | HST DD time specifies that unreduced data be available immediately; reduced observations to be made available ASAP. | ||||
20 | CCD | Irwin | VLT/MUSE - IFU | spectroscopic imaging, 465-930 nm to determine cloud structure and albedo spectrum of particles. | Spectral images of Jupiter acquired March 8-9; possibly more toward the end of March | “reductions to photometrically-calibrated cubes can be done in a day or two if there is sufficient motivation!” | ||||
21 | CCD | Sanchez-Lavega | Bilbao 11” Celestron with CCD | visible imaging, U, B, G, R + CH4 filters. Use “lucky imaging” to gain spatial resolution. | Observations made on April 18, 28, May 2, 3, 4, 9; June 7, 8, 20, 21, 27 | raw data available in 2-3 days, processed data available in a week if necessary (sooner if desired) | ||||
22 | CCD | Sanchez-Lavega | Calar Alto 2.2-m telescope, with PlanetCam camera | visible imaging, U, B, G, R + CH4 filters plus several bands between 1.0 and 1.7 microns, including J and H filterss. Use “lucky imaging” to gain spatial resolution. | good images from March 3/4, some images from March 6/7, good images from May 16/17, some images from 17/18 + 18/19 amid clouds, good images over the full spectral range May 19, 20; June 22, 23; July 1-4 | raw data available in 2-3 days, processed data available in a week if necessary (sooner if desired) | ||||
23 | CCD | Sanchez-Lavega | Calar Alto 2.2-m telescope, with Astralux camera | visible imaging, U, B, G, R + CH4 filters. Use “lucky imaging” to gain spatial resolution. | June 25, 26, 27 (bad seeing on June 27) | Raw data available in 2-3 days, processed data available in a week if necessary (sooner if desired), pending analysis to asses the results and quality (suspect nothing exceptional) | ||||
24 | CCD | Ip | Lulin 1-m/35-cm | UVBRI and CH4 filters | Apr 22, 23; Jun 17, 19, 21 | raw data available in a couple of weeks | ||||
25 | CCD | Chanover | Apache Point Observatory / Acoustical Optical Tunable Filter (APO/AOTF) | ~450-940 nm spatially resolved spectroscopy to determine cloud structure as linked to atmospheric dynamics. | one night successful during March 28-30 run | data being reduced | ||||
26 | CCD | Schneider | Apache Point Observatory / Dual Imaging Spectrograph (DIS) | Long-slit visible spectroscopy of both sides of the Io torus to determine S+, S++, O+ composition and electron density | acquired April 6, 14, 15. | calibrated data available on request | ||||
27 | CCD | Schmidt | McDonald Observatory IFU | Io's Neutral Na clouds, integral field echelle | acquired May 3, 4, 12 | data being reduced | ||||
28 | Visible | Kagitani/ Yoneda | Tohoku Univ. Haleakala 40cm / 60cm | Imaging observations of [SII](6716=6731A) emission in Io plasma torus with a 60-cm reflector. Sample data are on http://pparc.gp.tohoku.ac.jp/data/hal/qlMovie2.gif | continuous as Hisaki/ EXCEED (UV/EUV) & IPRT (Synchrotron) 2016 Jan 1, 4-5, 7-10 2016 Feb 5-6, 8-16, 18-28 2016 Mar 1-7, 9-22, 24-25, 28-31 2016 Apr 1-5, 7, 9-11 2016 May 12, 15-24, 27-30 2016 Jun 1-13, 16, 18-23, 26-29 2016 Jul 3, 5, 7-9 | |||||
29 | Visible | Kagitani/ Yoneda | Tohoku Univ. Haleakala 40cm / 60cm | Imaging observations of Na neublar originating from Io. Sample data are: http://pparc.gp/tohoku.ac.jp/data/hal/na_movie.gif | continuous as Hisaki/ EXCEED (UV/EUV) & IPRT (Synchrotron) observed on same nights as [SII] emission | |||||
30 | Visible | Kagitani/ Yoneda | Tohoku Univ. Haleakala 40cm / 60cm | Quasi-continous imaging of sodium nebula originating from Io | continuous as Hisaki/ EXCEED (UV/EUV) & IPRT (Synchrotron) observed on same nights as [SII] emission | |||||
31 | Near UV to Near IR | François Colas / JL Dauvergne / Marc Delcroix | Pic du Midi | T1M telescope | Several observations from 17 to 23 May | ASAP | ||||
32 | CCD + near IR | Sanchez-Lavega | Calar Alto 2.2m/ PlanetCam | Filtered imaging, 0.38 –1.7µm. Use “lucky imaging” to gain spatial resolution. | March 3/4 excellent seeing; good images covering the whole spectral range; March 6/7 bad seeing, some images available; May 16/17 - very good seeing with good images coveragin gthe whole spectral range; ay 17/18, 18/19 - partly cloudy with some imaging, May 19/20 excellent seeing with good images covering the whole spectral range | raw images available in a week, processed images in 2-3 weeks if necessary (sooner if desired, e.g. interesting targets, etc.) | ||||
33 | CCD + near IR | Sanchez-Lavega | Calar Alto 2.2m/ PlanetCam | Filtered imaging, 0.38 –1.7µm. Use “lucky imaging” to gain spatial resolution. | images acquired between 1.0 and 1.7 microns on July 1-4 | raw images available in a week, processed images in 2-3 weeks if necessary (sooner if desired, e.g. interesting targets, etc.) | ||||
34 | CCD + near IR | Orton | IRTF/MORIS, SpeX guide camera and spectrometer | filtered imaging 480-950 nm (MORIS); 1.58-5.1µm and spectral scans: 0.8-2.5µm, 2.5-5.1µm (SpeX) to determine structure and distribution of clouds and aerosols. | acquired: 2015 Nov 2-3, 2016 Jan 2-3 (no MORIS data) 2016 Feb 28-29 (with MORIS images on Feb 29) | raw data can be made available immediately; reduced images can be made available within a month (or sooner, as desired); reduced spectral scans available within 6 months (software for geometric reduction is under development) | ||||
35 | CCD+ near IR | Orton | IRTF/MORIS, SpeX guide camera and spectrometer | filtered imaging 480-950 nm (MORIS); 1.58-5.1µm and spectral scans: 0.8-2.5µm, 2.5-5.1µm (SpeX) to determine structure and distribution of clouds and aerosols. | SpeX imaging and scanned spectroscopy acquired on: 2016 May 11-12 UT. No MORIS data collected. Radiometrically uncalibrated images available on request. | raw data can be made available immediately; reduced images can be made available within a month (or sooner, as desired); reduced spectral scans available within 6 months (s/w for geometric reduction is under development) | ||||
36 | near IR | Orton | IRTF/SpeX guide camera | filtered imaging at: 1.58 µm (cloud albedo), 2.16 µm (upper-tropospheric particle field), 3.417 µm (H3+ auroral emission), 3.80 µm (mid-tropospheric particle field and H3+ auroral emission) and 5.10 µm (deep-tropospheric particle and gas distribution) | Images obtained and available from: Feb. 1, 4, 22, 23, 28, 29; Mar 2, 3, , 11, 12, 24; Apr 4, 25, 26; May 24, 25; Jun 4, 6, 18, 19 UT. | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired; images are scheduled to be uploaded and available on JSOC | ||||
37 | near IR | Orton | IRTF/SpeX guide camera | 3.8 and 5.1 micron imaging observations of Io | Feb 11, 22, 23 Mar 2, 3, 12 Apr 4 Jun 4, 6, 18, 19 | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired; images are scheduled to be uploaded and available on JSOC | ||||
38 | near IR | Johnson | IRTF /CSHELL | high-res. scanning spectroscopy of H3+ auroral emission. | observations obtained on February 3, 5, 10, 15, 17, 22, 27 and March 5. Good weather. | scanned images & possibly velocity maps, within 24 hrs; properly calibrated data will take longer; currently working on pipeline. | ||||
39 | near IR | Kita | IRTF / CSHELL | high-resolution spectroscopy of H3+ auroral emission for velocity-field measurements. | H3+ images and spectra obtained on April 22, 25; May 7, 9, 19, 21 Good weather. | would like to see agreement in place with Juno science team first and discussed at the workshop, but willing to share | ||||
40 | near IR | Kasaba Kita | Subaru / IRCS | AO-guided imaging/spectroscopy of H3+ emission with high spatial and spectral resolution. (using Galilean satellites as NGS) | K spectrum (H2 & H3+) on May 19, 21 H3+ image on May 19, 21, 24 BrAlpha image on May 24 | would like to see agreement in place with Juno science team first and discussed at the workshop, but willing to share. | ||||
41 | near IR | Kim | Gemini S/ Phoenix | 3-µm spectroscopy of auroral-related CH4, hydrocarbons. | No data on any of the nights granted for these observations between April 25 and May 20 were taken due to adverse weather conditions. | N/A | ||||
42 | near IR | O’Donoghue | Keck / NIRSpec | high-resolution scanning spectroscopy of H3+ auroral emission for temperature mapping. | Good observations obtained during the first half of April 13, 16, 19 and 22, with excellent coverage of the northern aurora. Some additional coverage of low-latitude ionosphere. | |||||
43 | near IR | Bonfond | VLT / NACO | high spatial resolution imaging to determine detailed structure of H3+ emission, differentiating between the Io and Ganymede footprints, using Galilean satellites as NGS. | service observations successful on April 7 | will provide previews and preliminary results to Juno ASAP. Hard to commit to specific data products, but “I belong to the Juno science team.” | ||||
44 | near IR | Defrère | LBT / LMIRCAM + NOMIC (7.9 µm) | imaging of H2 and H3+ emission to identify the infrared counterpart of FUV auroral features, disentangle auroral precipitation effects from Joule-heating effects, and measure the short-timescale variability of polar-most emissions. | Feb 20: a few minutes of H- and K-band data; March 28: ~15 minutes of K and K band data of the north pole | “data available right away” | ||||
45 | near IR | de Kleer | Gemini N / NIRI+AO | near-IR imaging of volcanism on Io, 2–4µm | Observations have been collected on 31 nights using Kc-band and L'-band images, Jan 30; Feb 3, 4, 9, 11, 15-21, 23; Mar 11-14; Apr 30; May 1-4, 8-14, 16-20, 23-25, 27-28, 31; Jun15, 710, 12, 16-20, 24-25, 27. | observations are part of de Kleer’s thesis, but specific requests will be considered | ||||
46 | mid IR | Greathouse | IRTF / TEXES | scanning spectroscopy to determine structure of low-latitude vertical oscillations vs. time. | Acquired on 2015 Nov 11-14 and 2016 Jan 13 10:30-17:30 UT, Jan 14 10:30-17:30 UT, Jan 18 11:30-19:00 UT, Jan 19 9:30-18:00 UT, Jan 21 9:30-12:30 UT & 15:00-18:00 UT April 28 3:00-10:30 UT, April 29 2:00-10:30 UT, May 4 2:00-7:30 UT, May 7 2:00-8:30 UT | raw data available in 2-3 days, reduced and remapped to lat/lon in 1 month (could be done faster if requested) | ||||
47 | mid IR | Fletcher | IRTF / TEXES | scanning spectroscopy to determine temperature and minor-constituent distribution. | Global maps in multiple settings acquired as follows: 2015-Nov-16/18; 2016-Jan-16/17/20; 2016-Apr-30 to May-06 | raw data available almost immediately, calibrated files with geometry within a month, and retrieved properties potentially available within 1-2 weeks (subject to any unforeseen issues) | ||||
48 | mid IR | Encrenaz | IRTF / TEXES | scanning spectroscopy to determine PH3 and trace-constituent distribution (5 and 10 microns). | Acquired on 2015 Nov 16-18; 2016 Jan 15 16:30-17:30 UT, Jan 16 9:50-19:00 UT, Jan 17 9:50-17:50 UT, Jan 20 9:50-19:00 UT; April 30 2:00-3:30 UT, May 2 2:00-10:30 UT, May 3 2:00-10:30 UT, May 5 2:00-10:30 UT, May 6 2:00-10:30 UT | TBD | ||||
49 | mid IR | Retherford | IRTF / TEXES | Ionized Sulfur | Acquired 2016 Jan 15 10:00-16:00 UT, Jan 21 12:50-15:00 UT | |||||
50 | mid IR | Tsang | IRTF / TEXES | 19 micron SO2 monitoring of Io | Acquired 2016 April 30 3:30-10:30 UT | |||||
51 | mid IR | Kasaba Orton Sinclair | Subaru / COMICS | spectroscopy and imaging to map the stratospheric temperature and minor constituent distribution associated with polar auroral regions. | <done> 24-25 Jan 2016 | would like to see agreement in place with Juno science team first and discussed at the workshop, but willing to share; raw images available immediately & reduced images possibly within a month, depending on interest; raw spectra available quickly “on demand” | ||||
52 | mid IR | Fletcher | VLT / VISIR | filtered radiometric imaging to map the temperature, minor constituent, and cloud distribution defining climatology, together with auroral heating and chemistry | Global maps, 7-20 µm, on 2016 Feb 15-16, 2016 Mar 25-26. 5-µm lucky imaging test on 2016 Feb 26 with June 27 press release. Northern aurora in 8 filters 2016 May 19; global observations June 7-8/8-9. | available in raw form in the ESO archive within 24 hours of acquisition; cylindrical maps within 1-2 days and reduced maps within a week | ||||
53 | mid IR | Sinclair | IRTF / TEXES | spectroscopy to map the distribution of stratospheric temperatures and minor constituents associated with polar auroral regions. | data acquired during TEXES block: 2016 May 1 2:00-10:30 UT, May 4 7:30-10:30 UT | raw data available in 2-3 days, reduced and remapped to lat/lon in 1 month (could be done faster if requested); once that is done, existing software could produce results in 3-5 days. | ||||
54 | mid IR | Kostiuk | HIPWAC | ultra high-resolution spatially resolved spectroscopy of stratospheric emission lines in Jupiter’s polar regions | successful spatially resolved spectroscopy using HIPWAC at the IRTF: April 18-21 | TBD | ||||
55 | radio* | Lamy, Zarka, Cecconi | Nançay Decameter Array, NenuFAR, LOFAR (Nançay, France) UTR2 (Kharkov, Ukraine) Iitate, Tohoku U.; Awara, Fukui Technical U.; Agawa, Kochi National Coll. of Technology (Japan) LWA1 (New Mexico, USA) | coordinated measurement of 10-40 MHz cyclotron radio emission. NDA data are acquired 8 hours per day. For more information see: http://maser.lesia.obspm.fr/outils-services/juno-ground-radio/ | See the web site for more details. | Most observers intend to have their data immediately public , but some (e.g. Ukrainian) prefer to set up a private server that will deliver data only to Juno-related scientists. Data availability should be a matter of weeks or less. | ||||
56 | radio* | Imai | LWA1 (USA) NDA (France) UTR-2 (Kharkov, Ukraine) GURT (Kharkov, Ukraine) URAN-2 (Poltava, Ukraine) URAN-3 (Lviv, Ukraine) | Coordinated Jupiter's DAM emissions. More information can be found at: PDF: Coordinated LWA1-NDA-URAN2 Observations for Jupiter’s DAM Radiation https://drive.google.com/file/d/0B32DAVbuGRxGMGlYN24wNXZuVlU/view?usp=sharing * URAN3 has mostly participated in this campaign, while UTR-2 and GURT sometimes join. PDF: Coordinated NDA-URAN2 Observations for Jupiter’s DAM Radiation https://drive.google.com/file/d/0B32DAVbuGRxGWXg5ZjlpRmRBcGs/view?usp=sharing * This corresponds to NDA-UTR2-GURT-URAN Jupiter observation campaign. | Observations combining LWA1+NDA+URAN2 made on Jan 8, 9, 15, 16; Feb 10, 16, 17, 23, 24; Mar 20, 26, 27; Apr 2, 3, 15; May 3, 4, 10, 11; Jun 11, 12, 18, 20, 21. Observations combining NDA+UTR2+GURT+URAN made on Mar 18, 25; Apr 12, 13, 19, 20; May 10. | Reduced data will be available upon request. Data process requires several months. | ||||
57 | radio | Santos-Costa | LOFAR | LOFAR observations of Jupiter's electron belt at 50-190 MHz coordinated with Juno's in-situ and/or remote observations during Juno's final approach phase and first three orbits | Observations obtained on June 2, 15. | no sooner than six months after data collection to allow observers and Juno team members to present / publish some preliminary observation results. | ||||
58 | radio | Levin (contact point) | DSN | 2.3-GHz synchrotron radio emission | two continuous 24-hour observations desired, with actual allocation TBD, possibly “last-minute” | data availability TBD but likely within a few months, based on previous experience | ||||
59 | radio | Levin (contact point) | DSN | 2.3-GHz synchrotron radio emission | Jan 24, 17:10-02:45 Jan 27,18:30-02:45 Jan 31, 18:30-02:30 Feb 4, 18:45-01:00 Feb 6, 18:20-01:10 Feb 11, 20:00-01:45 Feb 13, 18:55-01:40 Feb 14, 20:00-01:20 Feb 18, 21:45-01:20 Feb 19, 20:20, 01:15 Feb 27, 17:50-23:35 Mar 1, 19:15-02:05 Mar 3, 21:40-00:25 Mar 11, 18:15-23:55 Mar 15, 19:30-23:25 Mar 17, 18:15-03:05 Apr 1, 16:35-22:30 Apr 23, 14:45-21:05 May 3, 20:00-00:00 May 7, 20:00-23:40 May 10, 19:35-23:30 May 15, 11:30-21:45 | data availability TBD but likely within a few months | ||||
60 | radio* | Levin (contact point) | GAVRT | 2.3-GHz synchrotron radio emission, monitored as public outreach by students | A query of GAVRT database tables shows that observations of Jupiter were made from DSS-13 on Apr 21, 27; May 4, 24, 25, 31; Jun 20, 29. Observations were made from DSS-28 on Apr 21, 27; May 4, 25, 31; Jun 2. There is no assurance that data from any date are useful for a particular purpose. They must be examined. | data available by request through April, after which a “data access” website will be established, which will host raw data within 24 hours of collection; little data analysis will be done by the GAVRT team | ||||
61 | radio* | Misawa Tsuchiya | Iitate Planetary radio Telescope (IPRT) | 325MHz (& 785MHz) synchrotron radio emission, continuous monitoring with a 31mx33m single dish telescope | Continuous !!! | data available by request | ||||
62 | radio* | Kita | GMRT (India) | Synchrotron radio emission at L-band | May 03 14:30-16:30 May 14 13:30-15:30 May 20 13:30-15:30 May 28 15:30-17:30 Jun 02 14:30-16:30 Jun 05 12:30-14:30 Jun 07 13:30-15:30 Jun 11 11:30-13:30 Jun 23 12:30-14:30 | Reduced data will be available upon request. Data reduction requires several months. | ||||
63 | radio | Horiuchi | DSN Canberra DSS43(70m) or DSS34/45(34m) | 2.3/8.4 GHz synchrotron and thermal radio emission | Jan 30 030 09:10-16:50 Feb 11 042 09:55-12:40 Feb 16 047 08:20-14:55 Feb 28 059 07:50-15:55 Feb 03 063 07:55-15:15 Feb 24 084 08:05-10:30 Feb 26 086 07:45-11:15 Feb 27 087 07:40-10:40 Feb 28 088 07:40-11:20 Feb 29 089 07:35-10:35 Mar 30 090 05:35-11:15 Apr 07 098 07:05-11:45 May 08 129 05:40-11:00 May 19 140 03:40-10:25 Jun 02 154 05:00-07:15 Jun 04 156 04:20-07:45 Jun 05 157 04:05-08:25 Jun 11 163 02:10-08:00 Jun 19 171 04:35-11:30 Jun 24 176 06:10-10:40 Jun 29 181 05:00-06:45 Jul 02 184 04:40-09:55 | TBD | ||||
64 | ||||||||||
65 | ||||||||||
66 | Instruments are listed at: https://voparis-juno.obspm.fr/juno/instruments/pub_json | |||||||||
67 | ||||||||||
68 | ||||||||||
69 | Period: Jupiter Approach (2015 November 1 – 2016 July 3 [JOI-2d] | |||||||||
70 | Instrument | Description | ||||||||
71 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period up to a few days before JOI. These sample properties of the solar wind impinging on Jupiter’s magnetosphere, starting from a distance of ~1AU up to sampling the magnetosphere itself. | ||||||||
72 | UVS | Scans of Jupiter’s aurora June 3-29: June 3 at 02:30, June 4 at 18:30, June 9 at 08:30, June 14 at 08:30, June 16 at 00:30, June 18 at 02:30, June 21 at 10:30, June 24 at 13:30, June 26 at 00:30, June 27 at 14:00 | ||||||||
73 | JunoCam | Continuous imaging of Jupiter June 12-29, every ~15 minutes to create an "approach movie". Some large features on Jupiter are resolvable, and the motions of Galilean satellites are prominent and striking. | ||||||||
74 | JIRAM | Observations of Jupiter in Band L and M were made on January 25 and February 9 | ||||||||
75 | MWR | Jupiter was observed during the approach phase at times when it passes through the spin plane of the MWR antennas (the great circle on the sky which is continuously scanned by the MWR antennas due to the rotation of the spacecraft). At these times the spacecraft is at a large distance from Jupiter, so it appears smaller that the MWR antenna beams and only the total emission from the planet and radiation belts is measured. These scans will confirm that the MWR antenna patterns have remained unchanged, and allow us to check our absolute radiometric calibrations by comparison with ground-based single-dish calibrated measurements of Jupiter's total flux. Consequently such observations are desired at frequencies comparable to the lowest three or four frequencies of the MWR (600 Mhz, 1.25, 2.6 and 5Ghz) around the times of MWR observations. | ||||||||
76 | ||||||||||
77 | ||||||||||
78 | ||||||||||
79 | ||||||||||
80 | ||||||||||
81 | ||||||||||
82 | ||||||||||
83 | ||||||||||
84 | ||||||||||
85 | ||||||||||
86 | ||||||||||
87 | ||||||||||
88 | ||||||||||
89 | ||||||||||
90 | ||||||||||
91 | ||||||||||
92 | ||||||||||
93 | ||||||||||
94 | ||||||||||
95 | ||||||||||
96 | ||||||||||
97 | ||||||||||
98 | ||||||||||
99 | ||||||||||
100 | ||||||||||
101 | ||||||||||
102 | ||||||||||
103 | ||||||||||
104 | ||||||||||
105 | ||||||||||
106 | ||||||||||
107 | ||||||||||
108 | ||||||||||
109 | ||||||||||
110 | ||||||||||
111 | ||||||||||
112 | ||||||||||
113 | ||||||||||
114 | ||||||||||
115 | ||||||||||
116 | ||||||||||
117 | ||||||||||
118 | ||||||||||
119 | ||||||||||
120 | ||||||||||
121 | ||||||||||
122 | ||||||||||
123 | ||||||||||
124 | ||||||||||
125 | ||||||||||
126 | ||||||||||
127 | ||||||||||
128 | ||||||||||
129 | ||||||||||
130 | ||||||||||
131 | ||||||||||
132 | ||||||||||
133 | ||||||||||
134 | ||||||||||
135 | ||||||||||
136 | ||||||||||
137 | ||||||||||
138 | ||||||||||
139 | ||||||||||
140 | ||||||||||
141 | ||||||||||
142 | ||||||||||
143 | ||||||||||
144 | ||||||||||
145 | ||||||||||
146 | ||||||||||
147 | ||||||||||
148 | ||||||||||
149 | ||||||||||
150 | ||||||||||
151 | ||||||||||
152 | ||||||||||
153 | ||||||||||
154 | ||||||||||
155 | ||||||||||
156 | ||||||||||
157 | ||||||||||
158 | ||||||||||
159 | ||||||||||
160 | ||||||||||
161 | ||||||||||
162 | ||||||||||
163 | ||||||||||
164 | ||||||||||
165 | ||||||||||
166 | ||||||||||
167 | ||||||||||
168 | ||||||||||
169 | ||||||||||
170 | ||||||||||
171 | ||||||||||
172 | ||||||||||
173 | ||||||||||
174 | ||||||||||
175 | ||||||||||
176 | ||||||||||
177 | ||||||||||
178 | ||||||||||
179 | ||||||||||
180 | ||||||||||
181 | ||||||||||
182 | ||||||||||
183 | ||||||||||
184 | ||||||||||
185 | ||||||||||
186 | ||||||||||
187 | Period: Orbit 0 (2016 July 4 [JOI-1d] – 2016 August 25) | |||||||||
188 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | ||||
189 | FUV | Nichols | HST/STIS | imaging and spectroscopy of Jupiter’s auroral regions | scheduled for Jul 11-18 | data made available to Juno team asap; many are already Co-Is | ||||
190 | Visible | Kagitani/ Yoneda | Tohoku Univ. Haleakala 40cm / 60cm | Quasi-continous imaging of sodium nebula originating from Io | continuous as Hisaki/ EXCEED (UV/EUV) & IPRT (Synchrotron) through 2016 December | |||||
191 | CCD | Ip | Lulin 1-m/35-cm | UVBRI and CH4 filters | possible observations in July | raw data available in a couple of weeks | ||||
192 | near IR | Orton | IRTF/SpeX guide camera | filtered imaging at 5 strategic wavelengths, including 5.1µm and 3.4µm (H3+ auroral emission). | obtained during 60 min intervals on Jul 22; July 23 observing completely weathered out. | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired | ||||
193 | mid IR | Fletcher | VLT / VISIR | filtered radiometric imaging to map the temperature, minor constituent, and cloud distribution defining climatology, together with auroral heating and chemistry | July 27, 28, 31; August 1 | available in raw form in the ESO archive within 24 hours of acquisition; cylindrical maps within 1-2 days and reduced maps within a week | ||||
194 | radio* | Zarka, Cecconi | Nançay Decameter Array, NenuFAR, LOFAR (Nançay, France) UTR2 (Kharkov, Ukraine) Iitate, Tohoku U.; Awara, Fukui Technical U.; Agawa, Kochi National Coll. of Technology (Japan) LWA1 (New Mexico, USA) | coordinated measurement of 10-40 MHz cyclotron radio emission. For more information see: http://maser.lesia.obspm.fr/outils-services/juno-ground-radio/ | Observations scheduled on Jul 23, 29, 30; Aug 5. See the web site for more details. | Most observers intend to have their data immediately public , but some (e.g. Ukrainian) prefer to set up a private server that will deliver data only to Juno-related scientists. Data availability should be a matter of weeks or less. | ||||
195 | ||||||||||
196 | Scheduled observations by Juno. | |||||||||
197 | ||||||||||
198 | Note: All instruments will be powered on July 10, 0:00 UTC | |||||||||
199 | ||||||||||
200 | Orbits start at perijove minus one day. | |||||||||
201 | ||||||||||
202 | Perijove 2016 July 5, 02:47:38 UTC, System-III longitude = 32.8°W | |||||||||
203 | ||||||||||
204 | Period: Orbit 0 (2016 July 4 [JOI-1d] – 2016 August 25) | |||||||||
205 | Instrument | Description | ||||||||
206 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||
207 | MWR | On July 6, the MWR began to collect unresolved observations of Jupiter at a low data rate. | ||||||||
208 | MWR | The MWR will observe at full rate during three concentrated periods totalling about 100 hours to make careful maps of its antenna beams using Jupiter as a bright, unresolved source. | ||||||||
209 | UVS | Scans of Jupiter’s aurora July 22-Aug 25: (Calibration on July 16 at 00:00) July 25 at 14:00, July 29 at 10:00, August 8 at 14:00 | ||||||||
210 | JIRAM | Observations to calibrate pointing and spin phase | ||||||||
211 | JunoCam | Continuous imaging of Jupiter throughout this period, starting 2016 July 10, every ~15 minutes | ||||||||
212 | ||||||||||
213 | ||||||||||
214 | ||||||||||
215 | ||||||||||
216 | ||||||||||
217 | ||||||||||
218 | ||||||||||
219 | ||||||||||
220 | ||||||||||
221 | ||||||||||
222 | ||||||||||
223 | ||||||||||
224 | ||||||||||
225 | ||||||||||
226 | ||||||||||
227 | ||||||||||
228 | ||||||||||
229 | ||||||||||
230 | ||||||||||
231 | ||||||||||
232 | ||||||||||
233 | ||||||||||
234 | ||||||||||
235 | ||||||||||
236 | ||||||||||
237 | ||||||||||
238 | ||||||||||
239 | ||||||||||
240 | ||||||||||
241 | ||||||||||
242 | ||||||||||
243 | ||||||||||
244 | ||||||||||
245 | ||||||||||
246 | ||||||||||
247 | ||||||||||
248 | ||||||||||
249 | ||||||||||
250 | ||||||||||
251 | Note: Jupiter may be too close to the sun for Earth-based observations during much of this period, except for daytime-capable observatories. | |||||||||
252 | ||||||||||
253 | Period: Orbit 1 [C Orbit] (2016 August 26 – 2016 October 17) | |||||||||
254 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | ||||
255 | Visible | Kagitani/ Yoneda | Tohoku Univ. Haleakala 40cm / 60cm | Quasi-continous imaging of sodium nebula originating from Io | continuous as Hisaki/ EXCEED (UV/EUV) & IPRT (Synchrotron) through 2016 December | |||||
256 | near IR | Orton | IRTF/SpeX guide camera | filtered imaging 1.58-5.1µm to determine structure and distribution of clouds and aerosols. | 1. Aug 26 19:30 - Aug 27 01:30 UTC (including a time frame observing the PJ1 longitude ~12.5 hours before PJ1) 2. Aug 27 19:30 - Aug 28 01:30 UTC including a time frame observing the PJ1 longitude ~8.5 hours after PJ1). Best observations were at 5.1 microns during period (1). Observing conditions in period (2) were extremely difficult, with only a single, low-SNR image obtained. | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired | ||||
257 | radio | Santos-Costa | LOFAR | LOFAR observations of Jupiter's electron belt at 50-190 MHz coordinated with Juno's in-situ and/or remote observations during Juno's final approach phase and first three orbits | Observations obtained on Aug 27. | no sooner than six months after data collection to allow observers and Juno team members to present / publish some preliminary observation results. | ||||
258 | radio* | Kita | GMRT (India) | Synchrotron radio emission at L-band | Aug 27 09:30-11:30 | reduced data will be available upon request. Data reduction requires several months. | ||||
259 | Scheduled observations by Juno. | |||||||||
260 | ||||||||||
261 | Perijove is 2016 August 27, 12:51:20 UTC. System-III longitude = 96.1°W. | |||||||||
262 | ||||||||||
263 | Period: Orbit 1 [C Orbit] (2016 August 26 – 2016 October 17) | |||||||||
264 | Instrument | Description | ||||||||
265 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||
266 | MWR | N/S scans near perijove longitude, not centered on nadir - similar to GRAV-orbit scans | ||||||||
267 | UVS | Scans of Jupiter’s aurora Aug 27, 1:51 - 15:51. | ||||||||
268 | JIRAM | Imaging and spectra of Jupiter Aug 25 - 27, with spatial resolutions ~560 km to tens of km. | ||||||||
269 | JunoCam | Continuous imaging of Jupiter throughout this period, every ~15 minutes | ||||||||
270 | ||||||||||
271 | ||||||||||
272 | ||||||||||
273 | ||||||||||
274 | ||||||||||
275 | ||||||||||
276 | ||||||||||
277 | ||||||||||
278 | ||||||||||
279 | ||||||||||
280 | ||||||||||
281 | ||||||||||
282 | ||||||||||
283 | ||||||||||
284 | ||||||||||
285 | ||||||||||
286 | ||||||||||
287 | ||||||||||
288 | ||||||||||
289 | ||||||||||
290 | ||||||||||
291 | ||||||||||
292 | Note that Jupiter ranges from 18 degrees to 36 degrees from the sun during this period. | |||||||||
293 | Period: Orbit 2 [PRM] (2016 October 18 – 31) | |||||||||
294 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | ||||
295 | Visible | Kagitani/ Yoneda | Tohoku Univ. Haleakala 40cm / 60cm | Quasi-continous imaging of sodium nebula originating from Io | continuous as Hisaki/ EXCEED (UV/EUV) & IPRT (Synchrotron) through 2016 December | |||||
296 | CCD | Brian Jackson | Boise State 16-inch | visible imaging, U, B, G, R | TBD | TBD | ||||
297 | near IR | Orton | IRTF/SpeX guide camera | filtered imaging 480-950 nm (MORIS); 1.58-5.1µm and spectral scans: 0.8-2.5µm, 2.5-5.1µm (SpeX) to determine structure and distribution of clouds and aerosols. | Scheduled for Oct 18,19. Weather permitting, the IRTF will be able to make the observations with careful placement of both its upper and lower shutters to shield SpeX from direct sunlight. Jupiter is 16.7 degrees from the sun. Daylight observing. Oct 18 06:50-12:50 Hawaiian Standard Time (HST) Oct 19 06:50-12:50 | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired | ||||
298 | microwave | de Pater | Very Large Array (VLA) | A configuration in X band (8-12 GHz) | awarded 19 Oct., coincident with first spatially resolved MWR observations of Jupiter | MWR PI Janssen is a Co-Investigator | ||||
299 | ||||||||||
300 | Scheduled observations by Juno. | |||||||||
301 | ||||||||||
302 | This is the Perijove Reduction Maneuver (PRM) orbit. The Perijove is 2016 October 19, 18:11:07 UTC. System-III longitude = 347.9°W | |||||||||
303 | ||||||||||
304 | Period: Orbit 2 [PRM] (2016 October 18 – 31) | |||||||||
305 | Instrument | Description | ||||||||
306 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||
307 | MWR | 3D map partial maps of Jupiter covering ±70° latitude, centered near a System-III longitude of 340°W. This should capture a part of the turbulent region to the northwest of the Great Red Spot. | ||||||||
308 | UVS | Scans of Jupiter’s aurora Oct 28, 2:03 - 14:23. | ||||||||
309 | JunoCam | Continuous imaging of Jupiter throughout this period, every ~15 minutes, but not near the PRM on Oct 19. | ||||||||
310 | JIRAM | none | ||||||||
311 | ||||||||||
312 | ||||||||||
313 | ||||||||||
314 | ||||||||||
315 | ||||||||||
316 | ||||||||||
317 | ||||||||||
318 | ||||||||||
319 | ||||||||||
320 | ||||||||||
321 | ||||||||||
322 | ||||||||||
323 | ||||||||||
324 | ||||||||||
325 | ||||||||||
326 | ||||||||||
327 | ||||||||||
328 | ||||||||||
329 | ||||||||||
330 | ||||||||||
331 | ||||||||||
332 | ||||||||||
333 | ||||||||||
334 | ||||||||||
335 | ||||||||||
336 | ||||||||||
337 | ||||||||||
338 | ||||||||||
339 | ||||||||||
340 | ||||||||||
341 | ||||||||||
342 | ||||||||||
343 | ||||||||||
344 | ||||||||||
345 | ||||||||||
346 | ||||||||||
347 | ||||||||||
348 | ||||||||||
349 | ||||||||||
350 | ||||||||||
351 | ||||||||||
352 | ||||||||||
353 | ||||||||||
354 | ||||||||||
355 | ||||||||||
356 | ||||||||||
357 | ||||||||||
358 | ||||||||||
359 | ||||||||||
360 | ||||||||||
361 | ||||||||||
362 | ||||||||||
363 | ||||||||||
364 | ||||||||||
365 | ||||||||||
366 | ||||||||||
367 | ||||||||||
368 | ||||||||||
369 | ||||||||||
370 | ||||||||||
371 | Period: Orbit 3 [Cleanup] (2016 November 1 – 2016 November 14) | |||||||||
372 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | ||||
373 | Visible | Kagitani/ Yoneda | Tohoku Univ. Haleakala 40cm / 60cm | Quasi-continous imaging of sodium nebula originating from Io | continuous as Hisaki/ EXCEED (UV/EUV) & IPRT (Synchrotron) through 2016 December | |||||
374 | near IR | Orton | IRTF/SpeX guide camera | filtered imaging 480-950 nm (MORIS); 1.58-5.1µm and spectral scans: 0.8-2.5µm, 2.5-5.1µm (SpeX) to determine structure and distribution of clouds and aerosols. | Scheduled for Nov 1,2 (daytime observing) Nov 1 06:30-12:30 Nov 2 06:30 -12:30 | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired | ||||
375 | radio | Santos-Costa | LOFAR | LOFAR observations of Jupiter's electron belt at 50-190 MHz coorinated with Juno's in-situe and/or remote observations during Juno's final apoproach phase and first three orbits | four observation windows between May and November 2016 | no sooner than six months after data collection to allow observers and Juno team members to present / publish some preliminary observation results. | ||||
376 | ||||||||||
377 | Scheduled observations by Juno. | |||||||||
378 | ||||||||||
379 | Perijove is 2016 November 2, 17:52:29 UTC. System-III longitude = 284.1°W | |||||||||
380 | ||||||||||
381 | Period: Orbit 3 [Cleanup] (2016 November 1 – 2016 November 14) | |||||||||
382 | Instrument | Description | ||||||||
383 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||
384 | MWR | N/S scans near perijove longitude, not centered on nadir - similar to GRAV-orbit scans | ||||||||
385 | UVS | Scans of Jupiter’s aurora Nov 2, 7:52 - 19:52; Nov 13, 5:24 - 17:24. | ||||||||
386 | JunoCam | Continuous imaging of Jupiter throughout this period, every ~15 minutes. | ||||||||
387 | JIRAM | TBD | ||||||||
388 | ||||||||||
389 | ||||||||||
390 | Note: This is the first official science orbit, with the spacecraft orientation optimizing MWR and other remote-sensing observations. | |||||||||
391 | ||||||||||
392 | ||||||||||
393 | ||||||||||
394 | ||||||||||
395 | ||||||||||
396 | ||||||||||
397 | ||||||||||
398 | ||||||||||
399 | ||||||||||
400 | ||||||||||
401 | ||||||||||
402 | ||||||||||
403 | ||||||||||
404 | ||||||||||
405 | ||||||||||
406 | ||||||||||
407 | ||||||||||
408 | ||||||||||
409 | ||||||||||
410 | ||||||||||
411 | ||||||||||
412 | ||||||||||
413 | ||||||||||
414 | Period: Orbit 4 [MWR] (2016 November 15 – 2016 November 28) | |||||||||
415 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | ||||
416 | Visible | Kagitani/ Yoneda | Tohoku Univ. Haleakala 40cm / 60cm | Quasi-continous imaging of sodium nebula originating from Io | continuous as Hisaki/ EXCEED (UV/EUV) & IPRT (Synchrotron) through 2016 December | |||||
417 | near IR | Johnson | IRTF/iSHELL | imaging and high-resolution spectroscopy of H3+ emission | awarded Nov 16 04:00-06:30 (10 hours before perijove) | |||||
418 | near IR | Bjoraker | IRTF/iSHELL | high-resoution spectroscopy of Jupiter in the 5-µm window to determine NH3, H2O abundances and propeties of water clouds at similar locations and nearly the same time as Juno | awarded Nov 15 06:05-12:05 Nov 18 06:05-12:05 Daylight observing | |||||
419 | mid IR | Fletcher | VLT / VISIR | filtered radiometric imaging to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology. | mid-infrared imaging of Jupiter requested using a partial set of filters close to the perijove of the perijove longitude, awarded Nov 16 (30 minute run to capture just the high priority filters, possibly 17.6, 8.6, 10.8 and 7.9) | available in raw form in the ESO archive within 24 hours of acquisition; cylindrical maps within 1-2 days and reduced maps within a week | ||||
420 | ||||||||||
421 | Scheduled observations by Juno. | |||||||||
422 | ||||||||||
423 | Perijove is 2016 November 16, 16:54:46 UTC. System-III longitude = 196.7°W | |||||||||
424 | ||||||||||
425 | Period: Orbit 4 [MWR] (2016 November 15 – 2016 November 28) | |||||||||
426 | Instrument | Description | ||||||||
427 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||
428 | MWR | N/S scans near perijove longitude centered on nadir. | ||||||||
429 | UVS | TBD | ||||||||
430 | JunoCam | E/PO observations targeting features voted on by public. | ||||||||
431 | JIRAM | TBD | ||||||||
432 | ||||||||||
433 | Note: This is the second official science orbit, with the spacecraft orientation optimizing gravity sensing with the antenna pointed directly at the Earth. | |||||||||
434 | ||||||||||
435 | ||||||||||
436 | ||||||||||
437 | ||||||||||
438 | ||||||||||
439 | ||||||||||
440 | ||||||||||
441 | ||||||||||
442 | ||||||||||
443 | ||||||||||
444 | ||||||||||
445 | ||||||||||
446 | ||||||||||
447 | ||||||||||
448 | ||||||||||
449 | ||||||||||
450 | ||||||||||
451 | ||||||||||
452 | ||||||||||
453 | ||||||||||
454 | ||||||||||
455 | ||||||||||
456 | Period: Orbit 5 [GRAV] (2016 November 29 – 2016 December 12) | |||||||||
457 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | ||||
458 | X-ray | Gladstone | Chandra | 5-hour observation for day of perijove only targeting the northern aurora | 30 November 2016 | |||||
459 | FUV | Grodent | HST/FUV-MAMA | high spatial and temporal resolution FUV observations of magnetosphere and ultraviolet auroras | Nov 28 (northern aurora) Nov 29 (northern aurora) Nov 30 (northern aurora) Dec 01 (southern and southern aurora) Dec 07 (northern aurora) | Times may change by re-scheduling on the part of HST | ||||
460 | Visible | Kagitani/ Yoneda | Tohoku Univ. Haleakala 40cm / 60cm | Quasi-continous imaging of sodium nebula originating from Io | continuous as Hisaki/ EXCEED (UV/EUV) & IPRT (Synchrotron) through 2016 December | |||||
461 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | Continuous | |||||
462 | visible/NUV | Wong | HST/WFC3 UVIS | hi-resolution map of perijove track | one orbit (50 min obs.) ~1-3 hours before perijove pass if possible, otherwise within one rotation of pass | raw data available immediately from STScI archive; reduced maps and zonal wind profiles available within one month or potentially sooner; co-Is from MWR and JIRAM teams | ||||
463 | near IR | Orton | IRTF/SpeX guide camera | filtered imaging at 5 strategic wavelengths, including 5.1µm and 3.4µm (H3+ auroral emission). | awarded Dec 5 05:00-06:15, Dec 6 05:00-06:15 | |||||
464 | near IR | Orton | IRTF/iSHELL | imaging and high-resolution spectroscopy | awarded Dec 9 05:15-06:15, Dec 10 05:15-06:15 | |||||
465 | near IR | Johnson | IRTF/iSHELL | imaging and high-resolution spectroscopy of H3+ emission | requested near PJ5, awarded Nov 30 04:05-07:05 | TBD | ||||
466 | near IR | Bjoraker | IRTF/ISHELL | high-resoution spectroscopy of Jupiter in the 5-µm window to determine NH3, H2O abundances and propeties of water clouds at similar locations and nearly the same time as Juno | requested near PJ5, awarded Nov 29 06:05-12:05 (daylight observing), Dec 2 04:30-10:30 | fully reduced spectra available in 2 months | ||||
467 | mid IR | Fletcher | VLT / VISIR | filtered radiometric imaging to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology. | mid-infrared imaging of Jupiter requested using a partial set of filters close to the perijove of the perijove longitude, awarded Nov 30, 30 minute run to capture just the highest priority filters, possibly 17.6, 8.6, 10.8, 7.9 | available in raw form in the ESO archive within 24 hours of acquisition; cylindrical maps within 1-2 days and reduced maps within a week | ||||
468 | ||||||||||
469 | Scheduled observations by Juno. | |||||||||
470 | ||||||||||
471 | Perijove is 2016 November 30, 15:52:21 UTC. System-III longitude = 106.5°W | |||||||||
472 | ||||||||||
473 | Period: Orbit 5 [GRAV] (2016 November 29 – 2016 December 12) | |||||||||
474 | Instrument | Description | ||||||||
475 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||
476 | MWR | N/S scans near perijove longitude, not centered on nadir. | ||||||||
477 | UVS | TBD | ||||||||
478 | JunoCam | E/PO observations targeting poles and features voted on by public. | ||||||||
479 | JIRAM | TBD | ||||||||
480 | ||||||||||
481 | Note: On this orbit the spacecraft orientation optimizes MWR and other remote-sensing observations. | |||||||||
482 | ||||||||||
483 | ||||||||||
484 | ||||||||||
485 | ||||||||||
486 | ||||||||||
487 | ||||||||||
488 | ||||||||||
489 | ||||||||||
490 | ||||||||||
491 | ||||||||||
492 | ||||||||||
493 | ||||||||||
494 | ||||||||||
495 | ||||||||||
496 | ||||||||||
497 | ||||||||||
498 | ||||||||||
499 | ||||||||||
500 | ||||||||||
501 | ||||||||||
502 | ||||||||||
503 | ||||||||||
504 | ||||||||||
505 | Period: Orbit 6 [MWR] (2016 December 13 – 2016 December 26) | |||||||||
506 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | ||||
507 | X-ray | Gladstone | Chandra | 5-hour observation for day of perijove only targeting the northern aurora | 14 December 2016 | |||||
508 | FUV | Grodent | HST/FUV-MAMA | high spatial and temporal resolution FUV observations of magnetosphere and ultraviolet auroras | Dec 11 (nothern aurora) Dec 12 (northern aurora) Dec 13 (nothern aurora) Dec 14 (northern and southern aurora) Dec 15 (southern aurora) Dec 16 (northern aurora) Dec 21 (nothern aurora) | Times may change by re-scheduling on the part of HST | ||||
509 | Visible | Kagitani/ Yoneda | Tohoku Univ. Haleakala 40cm / 60cm | Quasi-continous imaging of sodium nebula originating from Io | continuous as Hisaki/ EXCEED (UV/EUV) & IPRT (Synchrotron) through 2016 December | |||||
510 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | Continuous | |||||
511 | visible/NUV | Wong | HST/WFC3 UVIS | hi-resolution global context maps | global maps: 1 pair near perijove 6 to establish early Juno epoch global wind field. 3 additional global maps near perijove 9 (best spatial resolution in first 5 atmospheric perijoves) to assess short term variability. | raw data available immediately from STScI archive; reduced maps and zonal wind profiles available within one month or potentially sooner; co-Is from MWR and JIRAM teams | ||||
512 | CCD | Irwin | VLT/MUSE - IFU | spectroscopic imaging, 465-930 nm to determine cloud structure and albedo spectrum of particles. | 30-minute observation sequence requested of Jupiter close the time of perijove passage that includes the perijove longitude | “reductions to photometrically-calibrated cubes can be done in a day or two if there is sufficient motivation!” | ||||
513 | near IR | Orton | IRTF/SpeX guide camera | filtered imaging at 5 strategic wavelengths, including 5.1µm and 3.4µm (H3+ auroral emission). | awarded Dec 22 05:30-06:30, Dec 24 05:15-06:15 | |||||
514 | near IR | Johnson | IRTF/iSHELL | imaging and high-resolution spectroscopy of H3+ emission | awarded Dec 14 03:15-09:15 (daylight observing) | |||||
515 | near IR | Davies | Keck / NIRC2 | AO-stabilized imaging of Io at several wavelengths | 1/4 night granted | TBD | ||||
516 | near IR | Bjoraker | IRTF/iSHELL | high-resoution spectroscopy of Jupiter in the 5-µm window to determine NH3, H2O abundances and propeties of water clouds at similar locations and nearly the same time as Juno | awarded Dec 13 04:30-10:30 (daylight obs) | fully reduced spectra available in 2 months | ||||
517 | near IR (5 µm) | Wong | Gemini-N/NIRI | lucky imaging, 5-µm maps, near-global coverage | 1 hr each 13, 14, 15 Dec. | full maps available on junocam planning site within 2 weeks | ||||
518 | mid IR | Fletcher | VLT / VISIR | filtered radiometric imaging to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology. | awarded Dec 14 Will have a northern and southern OB (100 minutes total), in addition to a single burst-mode M-band OB (20 minutes), totalling 120 minutes per perijove | available in raw form in the ESO archive within 24 hours of acquisition; cylindrical maps within 1-2 days and reduced maps within a week | ||||
519 | mid IR | Fletcher | IRTF/TEXES | scanned spectral maps of Jupiter's disk at ten key spectral settings to derive upper-tropospheric and stratospheric temperatures, aerosol/cloud distributions, and distribution of tropospheric NH3 and PH3, and stratospheric C2H2 and C2H6. | awarded Dec 16 06:30-11:30, Dec 17 03:00-11:30 (both daylight observing) | raw data available almost immediately, calibrated files with geometry within a month, and retrieved properties potentially available within 1-2 weeks (subject to any unforeseen issues) | ||||
520 | mid IR | Greathouse | IRTF/TEXES | scanned high- and medium-resolution spectral maps of Jupiter's disk at key CH4- and H2-absorbing wavelengths to determine temperatures in the upper troposphere and stratosphere to determine the structure of non-seasonal thermal waves associated with the Quasi-Quadrennial Oscillation (QQO) | awarded Dec 19 03:00-11:30, Dec 20 03:00-11:30 (both daylight observing) | |||||
521 | mid IR | Encrenaz | IRTF/TEXES | scanned medium-resolution spectral maps of Jupiter's disk at key wavelengths to determine the distributions of gaseous NH3 and PH3 in Jupiter's troposphere | awarded Dec 16 11:30-14:30, Dec 17 11:30-14:30, Dec 21 15:00-19:30, Dec 22 15:00-19:30 (all daylight observing) | |||||
522 | mid IR | Sinclair | IRTF/TEXES | scanned high-resolution spectral maps of Jupiter's disk at six key spectral settings to derive stratospheric temperatures and 3-dimensional distribution of stratospheric C2H2, C2H4, C2H6 and H3+ in auroral regions. | awarded Dec 15 03:30-11:30, Dec 16 03:00-06:30. Daylight observing on Dec 15. | TBD | ||||
523 | ||||||||||
524 | ||||||||||
525 | Scheduled observations by Juno. | |||||||||
526 | ||||||||||
527 | Perijove is 2016 December 14, 14:49:58 UTC. System-III longitude = 16.3°W | |||||||||
528 | ||||||||||
529 | Period: Orbit 6 [MWR] (2016 December 13 – 2016 December 26) | |||||||||
530 | Instrument | Description | ||||||||
531 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||
532 | MWR | TBD | ||||||||
533 | UVS | TBD | ||||||||
534 | JunoCam | E/PO observations targeting features voted on by public. | ||||||||
535 | JIRAM | TBD | ||||||||
536 | ||||||||||
537 | Note: On this orbit the spacecraft orientation optimizes MWR and other remote-sensing observations. | |||||||||
538 | ||||||||||
539 | ||||||||||
540 | ||||||||||
541 | ||||||||||
542 | ||||||||||
543 | ||||||||||
544 | ||||||||||
545 | ||||||||||
546 | ||||||||||
547 | ||||||||||
548 | ||||||||||
549 | ||||||||||
550 | ||||||||||
551 | ||||||||||
552 | ||||||||||
553 | ||||||||||
554 | ||||||||||
555 | ||||||||||
556 | ||||||||||
557 | ||||||||||
558 | ||||||||||
559 | ||||||||||
560 | ||||||||||
561 | ||||||||||
562 | ||||||||||
563 | ||||||||||
564 | ||||||||||
565 | ||||||||||
566 | ||||||||||
567 | ||||||||||
568 | ||||||||||
569 | ||||||||||
570 | ||||||||||
571 | ||||||||||
572 | ||||||||||
573 | ||||||||||
574 | ||||||||||
575 | ||||||||||
576 | ||||||||||
577 | ||||||||||
578 | ||||||||||
579 | ||||||||||
580 | ||||||||||
581 | ||||||||||
582 | ||||||||||
583 | ||||||||||
584 | ||||||||||
585 | ||||||||||
586 | ||||||||||
587 | ||||||||||
588 | ||||||||||
589 | ||||||||||
590 | ||||||||||
591 | ||||||||||
592 | ||||||||||
593 | ||||||||||
594 | ||||||||||
595 | ||||||||||
596 | ||||||||||
597 | ||||||||||
598 | Period: Orbit 7 [MWR] (2016 December 27 – 2017 January 9) | |||||||||
599 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | ||||
600 | FUV | Grodent | HST/FUV-MAMA | high spatial and temporal resolution FUV observations of magnetosphere and ultraviolet auroras | Dec 25 (northern aurora) Dec 26 (northern aurora) Dec 27 (northern aurora) Dec 28 (northern aurora) Dec 29 ( southern aurora) Dec 30 (southern aurora) Dec 31 (northern aurora) Jan 04 (northern aurora) | Times may change by re-scheduling on the part of HST | ||||
601 | CCD | Irwin | VLT/MUSE - IFU | spectroscopic imaging, 465-930 nm to determine cloud structure and albedo spectrum of particles. | 30-minute observation sequence requested of Jupiter close the time of perijove passage that includes the perijove longitude | “reductions to photometrically-calibrated cubes can be done in a day or two if there is sufficient motivation!” | ||||
602 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | Continuous | |||||
603 | visible/NUV | Wong | HST/WFC3 UVIS | hi-resolution map of perijove track | one orbit (50 min obs.) ~1-3 hours before perijove pass if possible, otherwise within one rotation of pass | raw data available immediately from STScI archive; reduced maps and zonal wind profiles available within one month or potentially sooner; co-Is from MWR and JIRAM teams | ||||
604 | near IR | Orton | IRTF/iSHELL | imaging and high-resolution spectroscopy | awarded Dec 31 05:15-06:15 | |||||
605 | near IR | Johnson | IRTF/iSHELL | imaging and high-resolution spectroscopy of H3+ emission | awarded Dec 28 04:15-10:15 (daylight observing) | |||||
606 | near IR | Orton | IRTF/SpeX guide camera | filtered imaging at 5 strategic wavelengths, including 5.1µm and 3.4µm (H3+ auroral emission). | awarded Jan 2 05:30-06:30, Jan 3 05:30-06:30, Jan 5 04:30-06:30 | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired | ||||
607 | near IR | Davies | Keck / NIRC2 | AO-stabilized imaging of Io at several wavelengths | 1/4 night granted | TBD | ||||
608 | near iR | Bjoraker | IRTF/iSHELL | high-resoution spectroscopy of Jupiter in the 5-µm window to determine NH3, H2O abundances and propeties of water clouds at similar locations and nearly the same time as Juno | awarded Dec 27 04:30-10:30, Dec 29 04:30-10:30 (both daylight observing) | fully reduced spectra available in 2 months | ||||
609 | near IR (5 µm) | Wong | Gemini-N/NIRI | lucky imaging, 5-µm maps, global coverage | 1.5 hr each 27, 28, 29 Dec. Proposal to be submitted mid-semester or for director discretionary time. | full maps available on junocam planning site within 2 weeks | ||||
610 | near IR | Conrad | Large Binocular Telescope/LBTI-LMIRCAM with simultaneous mid-IR observations at 7.8- and 8.7-microns with LBTI-NOMIC | high-resolution images of polar emissions from H2 at 2.1 microns and H3+ at 3.4 microns, plus maps of Jupiter's cloud layers from thermal emission at 5 microns | 1 hour requested with priority on PJ7 epoch | TBD | ||||
611 | mid IR | Fletcher | VLT / VISIR | filtered radiometric imaging to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology. | awarded Dec 28 Will have a northern and southern OB (100 minutes total), in addition to a single burst-mode M-band OB (20 minutes), totalling 120 minutes per perijove | available in raw form in the ESO archive within 24 hours of acquisition; cylindrical maps within 1-2 days and reduced maps within a week | ||||
612 | mid IR | Fletcher | IRTF/TEXES | scanned spectral maps of Jupiter's disk at ten key spectral settings to derive upper-tropospheric and stratospheric temperatures, aerosol/cloud distributions, and distribution of tropospheric NH3 and PH3, and stratospheric C2H2 and C2H6. | scans of Jupiter requested toward the end of the 10-day TEXES observing run starting at PJ6 | raw data available almost immediately, calibrated files with geometry within a month, and retrieved properties potentially available within 1-2 weeks (subject to any unforeseen issues) | ||||
613 | mid IR | Sinclair | IRTF/TEXES | scanned high-resolution spectral maps of Jupiter's disk at six key spectral settings to derive stratospheric temperatures and 3-dimensional distribution of stratospheric C2H2, C2H4, C2H6 and H3+ in auroral regions. | scans of Jupiter's polar regions requested within 1-2 days of the perijove passage | TBD | ||||
614 | ||||||||||
615 | ||||||||||
616 | ||||||||||
617 | ||||||||||
618 | Scheduled observations by Juno. | |||||||||
619 | ||||||||||
620 | Perijove is 2016 December 28, 13:47:59 UTC. System-III longitude = 286.0°W | |||||||||
621 | ||||||||||
622 | Period: Orbit 7 [MWR] (2016 December 27 – 2017 January 9) | |||||||||
623 | Instrument | Description | ||||||||
624 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||
625 | MWR | N/S scans near perijove longitude, not centered on nadir. | ||||||||
626 | UVS | TBD | ||||||||
627 | JunoCam | E/PO observations targeting features voted on by public. | ||||||||
628 | JIRAM | TBD | ||||||||
629 | ||||||||||
630 | ||||||||||
631 | Note: On this orbit the spacecraft orientation optimizes MWR and other remote-sensing observations. The spacecraft orientation is tilted in order to optimize the alignment of all MWR channel fields of view onto the same atmospheric positions. | |||||||||
632 | ||||||||||
633 | ||||||||||
634 | ||||||||||
635 | ||||||||||
636 | ||||||||||
637 | ||||||||||
638 | ||||||||||
639 | ||||||||||
640 | ||||||||||
641 | ||||||||||
642 | ||||||||||
643 | ||||||||||
644 | ||||||||||
645 | ||||||||||
646 | ||||||||||
647 | ||||||||||
648 | ||||||||||
649 | ||||||||||
650 | ||||||||||
651 | ||||||||||
652 | ||||||||||
653 | ||||||||||
654 | ||||||||||
655 | ||||||||||
656 | Period: Orbit 8 [MWR tilt] (2017 January 10 – 2017 January 23) | |||||||||
657 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | ||||
658 | FUV | Grodent | HST/FUV-MAMA | high spatial and temporal resolution FUV observations of magnetosphere and ultraviolet auroras | Jan 8 (northern aurora) Jan 10 (northern aurora) Jan 11 (Ganymede's aurora) Jan 12 ( southern and northern aurora) Jan 13 (northern aurora) Jan 18 (northern aurora) | Times may change by re-scheduling on the part of HST | ||||
659 | CCD | Irwin | VLT/MUSE - IFU | spectroscopic imaging, 465-930 nm to determine cloud structure and albedo spectrum of particles. | 30-minute observation sequence requested of Jupiter close the time of perijove passage that includes the perijove longitude | “reductions to photometrically-calibrated cubes can be done in a day or two if there is sufficient motivation!” | ||||
660 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | Continuous | |||||
661 | visible/NUV | Wong | HST/WFC3 UVIS | hi-resolution map of perijove track | one orbit (50 min obs.) ~1-3 hours before perijove pass if possible, otherwise within one rotation of pass | raw data available immediately from STScI archive; reduced maps and zonal wind profiles available within one month or potentially sooner; co-Is from MWR and JIRAM teams | ||||
662 | near IR | Orton | IRTF/SpeX guide camera | filtered imaging at 5 strategic wavelengths, including 5.1µm and 3.4µm (H3+ auroral emission). | awarded Jan 23 05:30-06:30 | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired | ||||
663 | near IR | Kita | IRTF/iSHELL | imaging and high-resolution spectroscopy of H3+ emission | Jan. 7 01:00 07:00 Jan. 8 01:00 07:00 Jan. 9 01:00 07:00 Jan.11 01:00 07:00 | Reduced data will be available upon request. | ||||
664 | near IR | Conrad | Large Binocular Telescope/LBTI-LMIRCAM with simultaneous mid-IR observations at 7.8- and 8.7-microns with LBTI-NOMIC | high-resolution images of polar emissions from H2 at 2.1 microns and H3+ at 3.4 microns, plus maps of Jupiter's cloud layers from thermal emission at 5 microns | 1 hour requested with PJ8 epoch given as 2nd priority | TBD | ||||
665 | near IR | Davies | Keck / NIRC2 | AO-stabilized imaging of Io at several wavelengths | 1/4 night granted | TBD | ||||
666 | 5-micron spectra | Bjoraker; de Pater | Keck/NIRSPEC & NIRC2 | spectra of NH3,H2O | Scheduled on Jan 11 & 12, contemporaneous with MWR observations of Jupiter. | fully reduced spectra available in 2 months | ||||
667 | CCD imaging | Bjoraker; de Pater | HST WFC3 observations | contextual observations, coincident with Keck observations | Scheduled on Jan 11 & 12, contemporaneous with MWR observations of Jupiter. | TBD | ||||
668 | near IR (5 µm) | Wong | Gemini-N/NIRI | lucky imaging, 5-µm maps, global coverage | 3 hr 11 Jan, 2 hr 12 Jan | full maps available on junocam planning site within 2 weeks | ||||
669 | mid IR | Fletcher | VLT / VISIR | filtered radiometric imaging to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology. | awarded Jan 11 Will have a northern and southern OB (100 minutes total), in addition to a single burst-mode M-band OB (20 minutes), totalling 120 minutes per perijove | available in raw form in the ESO archive within 24 hours of acquisition; cylindrical maps within 1-2 days and reduced maps within a week | ||||
670 | mid IR | Fletcher | IRTF/TEXES | scanned spectral maps of Jupiter's disk at ten key spectral settings to derive upper-tropospheric and stratospheric temperatures, aerosol/cloud distributions, and distribution of tropospheric NH3 and PH3, and stratospheric C2H2 and C2H6. | scans of Jupiter requested close to the perijove epoch awarded Jan 16 08:30-09:30, Jan 17 01:00-09:30 (both daylight observing), Jan 18 01:00-06:30 | raw data available almost immediately, calibrated files with geometry within a month, and retrieved properties potentially available within 1-2 weeks (subject to any unforeseen issues) | ||||
671 | mid IR | Kasaba Orton | Subaru / COMICS | filtered radiometric imaging and spectroscopy to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology and auroral heating and chemistry. | mid-infrared imaging of Jupiter requested using a full set of filters close to the perijove time with observations on an adjacent night to map the comlementary hemisphere. Scheduled on Jan 10,11 | would like to see agreement in place with Juno science team first and discussed at the workshop, but willing to share. | ||||
672 | mid IR | Orton | Keck exchange time to use Subaru / COMICS | filtered radiometric imaging and spectroscopy to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology and auroral heating and chemistry. | mid-infrared imaging of Jupiter requested using a full set of filters close to the perijove time with observations on an adjacent night to map the comlementary hemisphere. Scheduled on on January 12,13. | reduced observations available within 1-2 months; quick-look observations sooner | ||||
673 | microwave | de Pater | Very Large Array (VLA) | A configuration in X band (8-12 GHz) | awarded 11 Jan., coincident with PJ8 | MWR PI Janssen is a Co-Investigator | ||||
674 | radio | Kita | GMRT (India) | L-band | Jan 11 3:00-9:00 (IST) | Reduced data will be available upon request. | ||||
675 | mid IR | Greathouse | IRTF/TEXES | scanned high- and medium-resolution spectral maps of Jupiter's disk at key CH4- and H2-absorbing wavelengths to determine temperatures in the upper troposphere and stratosphere to determine the structure of non-seasonal thermal waves associated with the Quasi-Quadrennial Oscillation (QQO) | awarded Jan 14 03:30-09:30, Jan 15 01:00-09:30, Jan 16 01:00-08:30 (all daylight observing) | |||||
676 | mid IR | Sinclair | IRTF/TEXES | scanned high-resolution spectral maps of Jupiter's disk at six key spectral settings to derive stratospheric temperatures and 3-dimensional distribution of stratospheric C2H2, C2H4, C2H6 and H3+ in auroral regions. | scans of Jupiter's polar regions requested within 1-2 days of the perijove passage, awarded Jan 18 06:30-09:30, Jan 19 01:00-09:30 (both daylight observing) | TBD | ||||
677 | mid IR | Encrenaz | IRTF/TEXES | scanned medium-resolution spectral maps of Jupiter's disk at key wavelengths to determine the distributions of gaseous NH3 and PH3 in Jupiter's troposphere | awarded Jan 20 12:00-18:30, Jan 21 12:00-18:30 (both daylight observing) | |||||
678 | ||||||||||
679 | Scheduled observations by Juno. | |||||||||
680 | ||||||||||
681 | Perijove is 2017 January 11, 13:59:37 UTC. System-III longitude = 240.8°W | |||||||||
682 | ||||||||||
683 | Period: Orbit 8 [MWR] (2017 January 10 – 2017 January 23) | |||||||||
684 | Instrument | Description | ||||||||
685 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||
686 | MWR | N/S scans near perijove longitude, centered on nadir, with spacecraft tilted orientation to provide overlapping area coverage over mulitple-angles at all latitudes. | ||||||||
687 | UVS | TBD | ||||||||
688 | JunoCam | E/PO observations targeting features voted on by public. | ||||||||
689 | JIRAM | TBD | ||||||||
690 | ||||||||||
691 | Note: On this orbit the spacecraft orientation optimizes MWR and other remote-sensing observations. | |||||||||
692 | ||||||||||
693 | ||||||||||
694 | ||||||||||
695 | ||||||||||
696 | ||||||||||
697 | ||||||||||
698 | ||||||||||
699 | ||||||||||
700 | ||||||||||
701 | ||||||||||
702 | ||||||||||
703 | ||||||||||
704 | ||||||||||
705 | ||||||||||
706 | ||||||||||
707 | ||||||||||
708 | ||||||||||
709 | ||||||||||
710 | ||||||||||
711 | ||||||||||
712 | ||||||||||
713 | ||||||||||
714 | ||||||||||
715 | ||||||||||
716 | Period: Orbit 9 [MWR] (2017 January 24 – 2017 February 6) | |||||||||
717 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | ||||
718 | FUV | Grodent | HST/FUV-MAMA | high spatial and temporal resolution FUV observations of magnetosphere and ultraviolet auroras | Jan 22 (northern aurora) Jan 23 (northern aurora) Jan 24 (northern aurora) Jan 25 (northern aurora) Jan 25 (Ganymede's aurora) Jan 26 (southern aurora) Feb 01 (northern aurora) | Times may change by re-scheduling on the part of HST | ||||
719 | visible/NUV | Wong | HST/WFC3 UVIS | hi-resolution global context maps | global maps: 1 pair near perijove 6 to establish early Juno epoch global wind field. 3 additional global maps near perijove 9 (best spatial resolution in first 5 atmospheric perijoves) to assess short term variability. | raw data available immediately from STScI archive; reduced maps and zonal wind profiles available within one month or potentially sooner; co-Is from MWR and JIRAM teams | ||||
720 | CCD | Irwin | VLT/MUSE - IFU | spectroscopic imaging, 465-930 nm to determine cloud structure and albedo spectrum of particles. | 30-minute observation sequence requested of Jupiter close the time of perijove passage that includes the perijove longitude | “reductions to photometrically-calibrated cubes can be done in a day or two if there is sufficient motivation!” | ||||
721 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | Continuous | |||||
722 | near IR | Orton | IRTF/SpeX guide camera | filtered imaging at 5 strategic wavelengths, including 5.1µm and 3.4µm (H3+ auroral emission). | awarded Jan 26 05:30-06:30 | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired | ||||
723 | near IR | Moore | Keck / NIRSpec | high-resolution spectroscopy of polar auroral H3+ emissions between 2 and 5 microns. | 1 night requested near perijove | TBD | ||||
724 | near IR | Davies | Keck / NIRC2 | AO-stabilized imaging of Io at several wavelengths | 1/4 night granted | TBD | ||||
725 | 5-micron spectra | de Pater, Bjoraker | Keck/NIRSPEC & NIRC2; joint observations with Hubble Space Telescope also granted | spectra of NH3,H2O | Scheduled on Jan 24 & 25, contemporaneous with MWR observations of Jupiter. | fully reduced spectra available in 2 months | ||||
726 | CCD imaging | de Pater, Bjoraker | HST WFC3 observations | contextual observations, coincident with Keck observations | Scheduled on Jan 24 & 25, contemporaneous with MWR observations of Jupiter. | TBD | ||||
727 | near IR (5 µm) | Wong | Gemini-N/NIRI | lucky imaging, 5-µm maps, global coverage | 3 hr 25 Jan, 2 hr 26 Jan | full maps available on junocam planning site within 2 weeks | ||||
728 | mid IR | Fletcher | VLT / VISIR | filtered radiometric imaging to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology. | awarded Jan 25 Will have a northern and southern OB (100 minutes total), in addition to a single burst-mode M-band OB (20 minutes), totalling 120 minutes per perijove | available in raw form in the ESO archive within 24 hours of acquisition; cylindrical maps within 1-2 days and reduced maps within a week | ||||
729 | mid IR | Flecher | IRTF/TEXES | scanned spectral maps of Jupiter's disk at ten key spectral settings to derive upper-tropospheric and stratospheric temperatures, aerosol/cloud distributions, and distribution of tropospheric NH3 and PH3, and stratospheric C2H2 and C2H6. | scans of Jupiter requested toward the end of the 10-day TEXES observing run starting at PJ8 | raw data available almost immediately, calibrated files with geometry within a month, and retrieved properties potentially available within 1-2 weeks (subject to any unforeseen issues) | ||||
730 | mid IR | Greathouse | IRTF/TEXES | scanned high- and medium-resolution spectral maps of Jupiter's disk at key CH4- and H2-absorbing wavelengths to determine temperatures in the upper troposphere and stratosphere to determine the structure of non-seasonal thermal waves associated with the Quasi-Quadrennial Oscillation (QQO) | scans of Jupiter requested between Jan 10 and Jan 31 | raw data available in 2-3 days, reduced and remapped to lat/lon in 1 month (could be done faster if requested) | ||||
731 | mid IR | Encrenaz | IRTF/TEXES | scanned medium-resolution spectral maps of Jupiter's disk at key wavelengths to determine the distributions of gaseous NH3 and PH3 in Jupiter's troposphere | scans of Jupiter requested between Jan 1 and Jan 31 | TBD | ||||
732 | mid IR | Sinclair | IRTF/TEXES | scanned high-resolution spectral maps of Jupiter's disk at six key spectral settings to derive stratospheric temperatures and 3-dimensional distribution of stratospheric C2H2, C2H4, C2H6 and H3+ in auroral regions. | scans of Jupiter's polar regions requested within 1-2 days of the perijove passage | TBD | ||||
733 | mid IR | Orton | Keck exchange time to use Subaru / COMICS | filtered radiometric imaging and spectroscopy to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology and auroral heating and chemistry. | mid-infrared imaging of Jupiter requested using a full set of filters close to the perijove time with observations on an adjacent night to map the comlementary hemisphere. One half night granted on January 23. ... not awarded | reduced observations available within 1-2 months; quick-look observations sooner | ||||
734 | microwave | de Pater | Very Large Array (VLA) | A configuration in X band (8-12 GHz) | Requested 25 Jan., coincident with PJ9 | MWR PI Janssen is a Co-Investigator | ||||
735 | radio | Kita | GMRT (India) | L-band | Jan. 25 3:00-9:00 | Reduced data will be available upon request. | ||||
736 | ||||||||||
737 | Scheduled observations by Juno. | |||||||||
738 | ||||||||||
739 | Perijove is 2017 January 25, 12:57:12 UTC. System-III longitude = 150.6°W | |||||||||
740 | ||||||||||
741 | Period: Orbit 9 [MWR] (2017 January 24 – 2017 February 6) | |||||||||
742 | Instrument | Description | ||||||||
743 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||
744 | MWR | N/S scans near perijove longitude, centered on nadir. | ||||||||
745 | UVS | TBD | ||||||||
746 | JunoCam | E/PO observations targeting features voted on by public. | ||||||||
747 | JIRAM | TBD | ||||||||
748 | ||||||||||
749 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed directly at the Earth. | |||||||||
750 | ||||||||||
751 | ||||||||||
752 | ||||||||||
753 | ||||||||||
754 | ||||||||||
755 | ||||||||||
756 | ||||||||||
757 | ||||||||||
758 | ||||||||||
759 | ||||||||||
760 | ||||||||||
761 | ||||||||||
762 | ||||||||||
763 | ||||||||||
764 | ||||||||||
765 | ||||||||||
766 | ||||||||||
767 | ||||||||||
768 | ||||||||||
769 | ||||||||||
770 | ||||||||||
771 | ||||||||||
772 | ||||||||||
773 | ||||||||||
774 | Period: Orbit 10 [GRAV] (2017 February 7 – 2017 February 20) | |||||||||
775 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | ||||
776 | FUV | Grodent | HST/FUV-MAMA | high spatial and temporal resolution FUV observations of magnetosphere and ultraviolet auroras | Feb 05 (northern aurora) Feb 06 (northern aurora) Feb 07 (northern aurora) Feb 08 (northern and southern aurora) Feb 09 (southern aurora) Feb 14 (northern aurora) | Times may change by re-scheduling on the part of HST | ||||
777 | visible/NUV | Wong | HST/WFC3 UVIS | hi-resolution map of perijove track | one orbit (50 min obs.) ~1-3 hours before perijove pass if possible, otherwise within one rotation of pass | raw data available immediately from STScI archive; reduced maps and zonal wind profiles available within one month or potentially sooner; co-Is from MWR and JIRAM teams | ||||
778 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | continuous | |||||
779 | near IR | Orton | IRTF/SpeX guide camera | filtered imaging at 5 strategic wavelengths, including 5.1µm and 3.4µm (H3+ auroral emission). | to be requested during 30-min interval whenever SpeX is being used | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired | ||||
780 | mid IR | Fletcher | VLT / VISIR | filtered radiometric imaging to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology. | mid-infrared imaging of Jupiter requested using a full set of filters close to the perijove of all longitudes on PJ10, PJ11 or PJ12. Not awarded | available in raw form in the ESO archive within 24 hours of acquisition; cylindrical maps within 1-2 days and reduced maps within a week | ||||
781 | mid IR | Kasaba Orton | Subaru / COMICS | filtered radiometric imaging and spectroscopy to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology and auroral heating and chemistry. | mid-infrared imaging of Jupiter requested using a full set of filters close to the perijove time with observations on an adjacent night to map the comlementary hemisphere. Proposed to Feb 7-8 or 8-9. | would like to see agreement in place with Juno science team first and discussed at the workshop, but willing to share. | ||||
782 | radio | Kita | GMRT (India) | L-band | Feb. 8 3:00-9:00 | Reduced data will be available upon request. | ||||
783 | ||||||||||
784 | Scheduled observations by Juno. | |||||||||
785 | ||||||||||
786 | Perijove is 2017 February 8, 11:54:47 UTC. System-III longitude = 60.4°W | |||||||||
787 | ||||||||||
788 | Period: Orbit 10 [GRAV] (2017 February 7 – 2017 February 20) | |||||||||
789 | Instrument | Description | ||||||||
790 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||
791 | MWR | N/S scans near perijove longitude, not centered on nadir. | ||||||||
792 | UVS | TBD | ||||||||
793 | JunoCam | E/PO observations targeting features voted on by public. | ||||||||
794 | JIRAM | TBD | ||||||||
795 | ||||||||||
796 | ||||||||||
797 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed directly at the Earth. | |||||||||
798 | ||||||||||
799 | Period: Orbit 11 [GRAV] (2017 February 4 – 2017 March 6) | |||||||||
800 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | ||||
801 | X-ray | Gladstone | Chandra | 5-hour observation for day of perijove only targeting the northern aurora | 2/22/2017 check date | |||||
802 | FUV | Grodent | HST/FUV-MAMA | high spatial and temporal resolution FUV observations of magnetosphere and ultraviolet auroras. Current sheet crossings 30-40 RJ | Feb 4 14:28-15:17 (northern aurora) Feb 5 20:40-21:28 (northern aurora) | Times are confirmed 2-weeks prior observation | ||||
803 | visible/NUV | Wong | HST/WFC3 UVIS | hi-resolution map of perijove track | one orbit (50 min obs.) ~1-3 hours before perijove pass if possible, otherwise within one rotation of pass | raw data available immediately from STScI archive; reduced maps and zonal wind profiles available within one month or potentially sooner; co-Is from MWR and JIRAM teams | ||||
804 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | Continuous | |||||
805 | near IR | Orton | IRTF/SpeX guide camera | filtered imaging at 5 strategic wavelengths, including 5.1µm and 3.4µm (H3+ auroral emission). | to be requested during 30-min interval whenever SpeX is being used | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired | ||||
806 | near IR | Bjoraker | IRTF/iSHELL | Spectra at 5 microns covering longitude of PJ 11 to support MWR | Requested 2017 Feb 21 and Feb 23 (second half) | Raw data available on IRTF website, reduced data available after a few months. | ||||
807 | mid IR | Johnson | IRTF/iSHELL | Scans of the southern auroral H3+ emission at ~3.4µm. Simultaneous to JIRAM, MAG, JADE and JEDI measurements. | Proposed 22nd Feburary 2017 | Raw data available on IRTF website, reduced data available after a few months. | ||||
808 | ||||||||||
809 | Scheduled observations by Juno. | |||||||||
810 | ||||||||||
811 | Perijove is 2017 February 22, 10:52:21UTC. System-III longitude = 330.2°W | |||||||||
812 | ||||||||||
813 | Period: Orbit 11 [GRAV] (2017 February 21 – 2017 March 6) | |||||||||
814 | Instrument | Description | ||||||||
815 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||
816 | MWR | N/S scans near perijove longitude, not centered on nadir. | ||||||||
817 | UVS | TBD | ||||||||
818 | JunoCam | E/PO observations targeting features voted on by public. | ||||||||
819 | JIRAM | TBD | ||||||||
820 | ||||||||||
821 | ||||||||||
822 | ||||||||||
823 | ||||||||||
824 | ||||||||||
825 | ||||||||||
826 | ||||||||||
827 | ||||||||||
828 | ||||||||||
829 | ||||||||||
830 | ||||||||||
831 | ||||||||||
832 | ||||||||||
833 | ||||||||||
834 | ||||||||||
835 | ||||||||||
836 | ||||||||||
837 | ||||||||||
838 | ||||||||||
839 | ||||||||||
840 | ||||||||||
841 | ||||||||||
842 | ||||||||||
843 | ||||||||||
844 | ||||||||||
845 | ||||||||||
846 | ||||||||||
847 | ||||||||||
848 | ||||||||||
849 | ||||||||||
850 | ||||||||||
851 | ||||||||||
852 | ||||||||||
853 | ||||||||||
854 | ||||||||||
855 | ||||||||||
856 | ||||||||||
857 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed directly at the Earth. | |||||||||
858 | ||||||||||
859 | Period: Orbit 12 [GRAV] (2017 March 7 – 2017 March 20) | |||||||||
860 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | ||||
861 | FUV | Grodent | HST/FUV-MAMA | high spatial and temporal resolution FUV observations of magnetosphere and ultraviolet auroras | Mar 06 (southern aurora) Mar 07 (northern aurora) Mar 08 (Ganymede's aurora) Mar 08-09 (southern aurora) Mar 15 (southern aurora) | Times may change by re-scheduling on the part of HST | ||||
862 | CCD | Machado | UVES/VLT | Spectroscopic scan (visible to UV) in order to measure Doppler winds | Proposed for 2-4 March 2017 | raw data available in a couple of weeks | ||||
863 | CCD | Ip | Lulin 1-m/35-cm | UVBRI and CH4 filters | March-May 2017 | raw data available in a couple of weeks | ||||
864 | CCD | Irwin | VLT/MUSE - IFU | spectroscopic imaging, 465-930 nm to determine cloud structure and albedo spectrum of particles. | Three 30-minute observation sequences requested of Jupiter close the time of perijove passage that includes the perijove longitude, plus charactierzatio of the rest of the disc, on PJ10, PJ11 or PJ12. | “reductions to photometrically-calibrated cubes can be done in a day or two if there is sufficient motivation!” | ||||
865 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | Continuous | |||||
866 | visible/NUV | Wong | HST/WFC3 UVIS | hi-resolution map of perijove track | one orbit (50 min obs.) ~1-3 hours before perijove pass if possible, otherwise within one rotation of pass | raw data available immediately from STScI archive; reduced maps and zonal wind profiles available within one month or potentially sooner; co-Is from MWR and JIRAM teams | ||||
867 | near IR | Orton | IRTF/SpeX guide camera | filtered imaging at 5 strategic wavelengths, including 5.1µm and 3.4µm (H3+ auroral emission). | to be requested during 30-min interval whenever SpeX is being used | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired | ||||
868 | near IR | Kasaba Kita | Subaru / IRCS | AO-guided imaging/spectroscopy of H3+ emission with high spatial and spectral resolution. (using Galilean satellites as NGS) | PJ12: 5-6 March PJ14: 2-3 April PJ16: 30 April - 1 May | would like to see agreement in place with Juno science team first and discussed at the workshop, but willing to share. | ||||
869 | mid IR | Fletcher | VLT / VISIR | filtered radiometric imaging to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology. | mid-infrared imaging of Jupiter requested using a full set of filters close to the perijove of all longitudes on PJ10, PJ11 or PJ12. Not awarded | available in raw form in the ESO archive within 24 hours of acquisition; cylindrical maps within 1-2 days and reduced maps within a week | ||||
870 | mid IR | Kasaba Orton | Subaru / COMICS | filtered radiometric imaging and spectroscopy to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology and auroral heating and chemistry. | mid-infrared imaging of Jupiter requested using a full set of filters close to the perijove time with observations on an adjacent night to map the comlementary hemisphere. Proposed to Mar 7-8. | would like to see agreement in place with Juno science team first and discussed at the workshop, but willing to share. | ||||
871 | mid IR | Johnson | IRTF/iSHELL | Scans of the southern auroral H3+ emission at ~3.4µm. Simultaneous to JIRAM, MAG, JADE and JEDI measurements. | Proposed 8th March 2017 | Raw data available on IRTF website, reduced data available after a few months. | ||||
872 | Mid-IR | Livengood | IRTF/HIPWAC | high-resolution spectroscopy of C2H6 emission in auroral region stratosphere, 11.7 µm | Request 6 days straddling perijove to get 3 North aurora peaks, 3 south aurora peaks, midlatitudes in between peaks. | |||||
873 | ||||||||||
874 | Scheduled observations by Juno. | |||||||||
875 | ||||||||||
876 | Perijove is 2017 March 8, 9:12:44 UTC. System-III longitude = 217.5°W | |||||||||
877 | ||||||||||
878 | Period: Orbit 12 [GRAV] (2017 March 7 – 2017 March 20) | |||||||||
879 | Instrument | Description | ||||||||
880 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||
881 | MWR | N/S scans near perijove longitude, not centered on nadir. | ||||||||
882 | UVS | TBD | ||||||||
883 | JunoCam | E/PO observations targeting features voted on by public. | ||||||||
884 | JIRAM | TBD | ||||||||
885 | ||||||||||
886 | ||||||||||
887 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed directly at the Earth. | |||||||||
888 | ||||||||||
889 | Period: Orbit 13 [GRAV] (2017 March 21 – 2017 April 3) | |||||||||
890 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | ||||
891 | X-ray | Gladstone | Chandra | 5-hour observation for day of perijove only targeting the northern aurora | 22 March 2017 | |||||
892 | FUV | Grodent | HST/FUV-MAMA | high spatial and temporal resolution FUV observations of magnetosphere and ultraviolet auroras | Mar 20 ( northern aurora) Mar 21 (northern aurora) Mar 22 (northern aurora) Mar 22 (Ganymede's aurora) Mar 23 (southern aurora) Mar 29 (northern aurora) | Times may change by re-scheduling on the part of HST | ||||
893 | CCD | Ip | Lulin 1-m/35-cm | UVBRI and CH4 filters | March-May 2017 | raw data available in a couple of weeks | ||||
894 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | Continuous | |||||
895 | near IR | Orton | IRTF/SpeX guide camera | filtered imaging at 5 strategic wavelengths, including 5.1µm and 3.4µm (H3+ auroral emission). | to be requested during 30-min interval whenever SpeX is being used | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired | ||||
896 | visible/NUV | Wong | HST/WFC3 UVIS | hi-resolution map of perijove track | one orbit (50 min obs.) ~1-3 hours before perijove pass if possible, otherwise within one rotation of pass. ONLY IF NO OPAL DATA (PI SIMON) THIS PJ | raw data available immediately from STScI archive; reduced maps and zonal wind profiles available within one month or potentially sooner; co-Is from MWR and JIRAM teams | ||||
897 | Mid-IR | Livengood | IRTF/HIPWAC | high-resolution spectroscopy of C2H6 emission in auroral region stratosphere, 11.7 µm | Request 6 days straddling perijove to get 3 North aurora peaks, 3 south aurora peaks, midlatitudes in between peaks. | |||||
898 | ||||||||||
899 | Scheduled observations by Juno. | |||||||||
900 | ||||||||||
901 | Perijove is 2017 March 22, 8:10:19 UTC. System-III longitude = 127.2°W | |||||||||
902 | ||||||||||
903 | Period: Orbit 13 [GRAV] (2017 March 21 – 2017 April 3) | |||||||||
904 | Instrument | Description | ||||||||
905 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||
906 | MWR | N/S scans near perijove longitude, centered on nadir, with spacecraft tilted orientation to provide overlapping area coverage over mulitple angles at all latitudes. | ||||||||
907 | UVS | TBD | ||||||||
908 | JunoCam | E/PO observations targeting features voted on by public. | ||||||||
909 | JIRAM | TBD | ||||||||
910 | ||||||||||
911 | ||||||||||
912 | Note: On this orbit the spacecraft orientation optimizes remote sensing with the antenna pointed so that MWR and other instruments sense the nadir. The spacecraft will also be tilted to as to align better the full set of MWR channels at all emission angles. On 2017 April 4, Jupiter will be at opposition from the sun. All remote-sensing instruments are expected to be affected by radiation damage by this point except for the MWR, which may well continue through the end of the nominal (or extended) mission. If this is the case, the need for Earth-based observations for context will be particularly important as the mission continues. | |||||||||
913 | ||||||||||
914 | Period: Orbit 14 [MWR] (2017 April 4 – 2017 April 17) | |||||||||
915 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | ||||
916 | FUV | Grodent | HST/FUV-MAMA | high spatial and temporal resolution FUV observations of magnetosphere and ultraviolet auroras | Apr 02 (northern aurora) Apr 03 (northern aurora) Apr 04 (northern aurora) Apr 05 (southern aurora) Apr 06 (northern aurora) Apr 12 (northern aurora) | Times may change by re-scheduling on the part of HST | ||||
917 | CCD | Ip | Lulin 1-m/35-cm | UVBRI and CH4 filters | March-May 2017 | raw data available in a couple of weeks | ||||
918 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | Continuous | |||||
919 | near IR | Orton | IRTF/SpeX guide camera | filtered imaging at 5 strategic wavelengths, including 5.1µm and 3.4µm (H3+ auroral emission). | to be requested during 30-min interval whenever SpeX is being used | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired | ||||
920 | near IR | Kasaba Kita | Subaru / IRCS | AO-guided imaging/spectroscopy of H3+ emission with high spatial and spectral resolution. (using Galilean satellites as NGS) | PJ12: 5-6 March PJ14: 2-3 April PJ16: 30 April - 1 May | would like to see agreement in place with Juno science team first and discussed at the workshop, but willing to share. | ||||
921 | visible/NUV | Wong | HST/WFC3 UVIS | hi-resolution map of perijove track | one orbit (50 min obs.) ~1-3 hours before perijove pass if possible, otherwise within one rotation of pass. ONLY IF NO OPAL DATA (PI SIMON) THIS PJ | raw data available immediately from STScI archive; reduced maps and zonal wind profiles available within one month or potentially sooner; co-Is from MWR and JIRAM teams | ||||
922 | visible/NUV | Simon | HST/WFC3 UVIS | hi-resolution global context maps | global maps: 1 pair near opposition (7 April; near perijove 14). Scheduling window is ±20 days, so actual observations might be closer to perijove 13 or 15. | raw data available immediately from STScI archive; reduced maps and zonal wind profiles available within one month or potentially sooner | ||||
923 | near IR | de Pater; Bjoraker | Keck/NIRSPEC | Spectra at 5 microns covering longitude of PJ 14 to support MWR | Requested UT 2017 Apr 4-6 (3 half nights 9PM Apr 3-5 to 3AM Apr 4-6 HST) | Raw data available on Keck website, reduced data available after a few months. | ||||
924 | mid IR | Kasaba Orton | Subaru / COMICS | filtered radiometric imaging and spectroscopy to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology and auroral heating and chemistry. | mid-infrared imaging of Jupiter requested using a full set of filters close to the perijove time with observations on an adjacent night to map the comlementary hemisphere. Proposed to Apr 3-4. | would like to see agreement in place with Juno science team first and discussed at the workshop, but willing to share. | ||||
925 | Mid-IR | Livengood | IRTF/HIPWAC | high-resolution spectroscopy of C2H6 emission in auroral region stratosphere, 11.7 µm | Request 6 days straddling perijove to get 3 North aurora peaks, 3 south aurora peaks, midlatitudes in between peaks. | |||||
926 | ||||||||||
927 | ||||||||||
928 | Scheduled observations by Juno. | |||||||||
929 | ||||||||||
930 | Perijove is 2017 April 5, 7:07:53 UTC. System-III longitude = 37.0°W | |||||||||
931 | ||||||||||
932 | Period: Orbit 14 [MWR] (2017 April 4 – 2017 April 17) | |||||||||
933 | Instrument | Description | ||||||||
934 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||
935 | MWR | N/S scans near perijove longitude, not centered on nadir. | ||||||||
936 | UVS | TBD | ||||||||
937 | JunoCam | E/PO observations targeting features voted on by public. | ||||||||
938 | JIRAM | TBD | ||||||||
939 | ||||||||||
940 | ||||||||||
941 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed directly at the Earth. | |||||||||
942 | ||||||||||
943 | Period: Orbit 15 [GRAV] (2017 April 18 – 2017 May 1) | |||||||||
944 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | ||||
945 | FUV | Grodent | HST/FUV-MAMA | high spatial and temporal resolution FUV observations of magnetosphere and ultraviolet auroras | Apr 17 (northern aurora) Apr 18 (northern aurora) Apr 19 (northern aurora) Apr 19 (Europa's aurora) | Times may change by re-scheduling on the part of HST | ||||
946 | CCD | Ip | Lulin 1-m/35-cm | UVBRI and CH4 filters | March-May 2017 | raw data available in a couple of weeks | ||||
947 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | Continuous | |||||
948 | near IR | Orton | IRTF/SpeX guide camera | filtered imaging at 5 strategic wavelengths, including 5.1µm and 3.4µm (H3+ auroral emission). | to be requested during 30-min interval whenever SpeX is being used | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired | ||||
949 | visible/NUV | Wong | HST/WFC3 UVIS | hi-resolution map of perijove track | one orbit (50 min obs.) ~1-3 hours before perijove pass if possible, otherwise within one rotation of pass. ONLY IF NO OPAL DATA (PI SIMON) THIS PJ | raw data available immediately from STScI archive; reduced maps and zonal wind profiles available within one month or potentially sooner; co-Is from MWR and JIRAM teams | ||||
950 | visible/NUV | Simon | HST/WFC3 UVIS | hi-resolution global context maps | global maps: 1 pair near opposition (7 April; near perijove 14). Scheduling window is ±20 days, so actual observations might be closer to perijove 13 or 15. | raw data available immediately from STScI archive; reduced maps and zonal wind profiles available within one month or potentially sooner | ||||
951 | Thermal-IR | Fletcher | VLT/VISIR | High-resolution imaging 5, 8.6, 10.8, 12.3, 13.0, 17.6, 18.7, 19.5 µm. | Global image of the whole planet in all filters to coincide with Jupiter opposition. | Raw data available immediately, reduced and spatially mapped images within a few weeks. | ||||
952 | ||||||||||
953 | Scheduled observations by Juno. | |||||||||
954 | ||||||||||
955 | Perijove is 2017 April 19, 6:05:27 UTC. System-III longitude = 306.8°W | |||||||||
956 | ||||||||||
957 | Period: Orbit 15 [GRAV] (2017 April 18 – 2017 May 1) | |||||||||
958 | Instrument | Description | ||||||||
959 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||
960 | MWR | N/S scans near perijove longitude, not centered on nadir. | ||||||||
961 | UVS | TBD | ||||||||
962 | JunoCam | TBD | ||||||||
963 | JIRAM | TBD | ||||||||
964 | ||||||||||
965 | ||||||||||
966 | ||||||||||
967 | ||||||||||
968 | ||||||||||
969 | ||||||||||
970 | ||||||||||
971 | ||||||||||
972 | ||||||||||
973 | ||||||||||
974 | ||||||||||
975 | ||||||||||
976 | ||||||||||
977 | ||||||||||
978 | ||||||||||
979 | ||||||||||
980 | ||||||||||
981 | ||||||||||
982 | ||||||||||
983 | ||||||||||
984 | ||||||||||
985 | ||||||||||
986 | ||||||||||
987 | ||||||||||
988 | ||||||||||
989 | ||||||||||
990 | ||||||||||
991 | ||||||||||
992 | ||||||||||
993 | ||||||||||
994 | ||||||||||
995 | ||||||||||
996 | ||||||||||
997 | ||||||||||
998 | ||||||||||
999 | ||||||||||
1000 | ||||||||||
1001 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed directly at the Earth. | |||||||||
1002 | ||||||||||
1003 | Period: Orbit 16 [GRAV] (2017 May 2 – 2017 May 15) | |||||||||
1004 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | ||||
1005 | FUV | Grodent | HST/FUV-MAMA | high spatial and temporal resolution FUV observations of magnetosphere and ultraviolet auroras | May 01 (northern aurora) May 02 (northern aurora) May 03 (southern aurora) May 03 (Ganymede aurora) May 04 (northern aurora) | Times may change by re-scheduling on the part of HST | ||||
1006 | CCD | Ip | Lulin 1-m/35-cm | UVBRI and CH4 filters | March-May 2017 | raw data available in a couple of weeks | ||||
1007 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | Continuous | |||||
1008 | visible/NUV | Wong | HST/WFC3 UVIS | hi-resolution map of perijove track | one orbit (50 min obs.) ~1-3 hours before perijove pass if possible, otherwise within one rotation of pass. | raw data available immediately from STScI archive; reduced maps and zonal wind profiles available within one month or potentially sooner; co-Is from MWR and JIRAM teams | ||||
1009 | near IR | Orton | IRTF/SpeX guide camera | filtered imaging at 5 strategic wavelengths, including 5.1µm and 3.4µm (H3+ auroral emission). | to be requested during 30-min interval whenever SpeX is being used | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired | ||||
1010 | near IR | Kasaba Kita | Subaru / IRCS | AO-guided imaging/spectroscopy of H3+ emission with high spatial and spectral resolution. (using Galilean satellites as NGS) | PJ12: 5-6 March PJ14: 2-3 April PJ16: 30 April - 1 May | would like to see agreement in place with Juno science team first and discussed at the workshop, but willing to share. | ||||
1011 | mid IR | Orton | Subaru / COMICS via Keck exchange time | filtered radiometric imaging and spectroscopy to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology and auroral heating and chemistry. | mid-infrared imaging of Jupiter requested using a full set of filters close to the perijove time with observations on an adjacent night to map the comlementary hemisphere. Proposed for May 2-3. | available for collaboration, subject to consent from collaborators | ||||
1012 | Mid-IR | Livengood | IRTF/HIPWAC | high-resolution spectroscopy of C2H6 emission in auroral region stratosphere, 11.7 µm | Request 6 days straddling perijove to get 3 North aurora peaks, 3 south aurora peaks, midlatitudes in between peaks. | |||||
1013 | Thermal-IR | Fletcher | VLT/VISIR | High-resolution imaging 5, 8.6, 10.8, 12.3, 13.0, 17.6, 18.7, 19.5 µm. | Imaging of perijove longitude within ±36 hours of flyby. | Raw data available immediately, reduced and spatially mapped images within a few weeks. | ||||
1014 | ||||||||||
1015 | Scheduled observations by Juno. | |||||||||
1016 | ||||||||||
1017 | Perijove is 2017 May 3, 6:17:26 UTC. System-III longitude = 261.5°W | |||||||||
1018 | ||||||||||
1019 | Period: Orbit 16 [GRAV] (2017 May 2 – 2017 May 15) | |||||||||
1020 | Instrument | Description | ||||||||
1021 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||
1022 | MWR | N/S scans near perijove longitude, not centered on nadir. | ||||||||
1023 | UVS | TBD | ||||||||
1024 | JunoCam | TBD | ||||||||
1025 | JIRAM | TBD | ||||||||
1026 | ||||||||||
1027 | ||||||||||
1028 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed directly at the Earth. | |||||||||
1029 | ||||||||||
1030 | Period: Orbit 17 [GRAV] (2017 May 16 – 2017 May 29) | |||||||||
1031 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | ||||
1032 | FUV | Grodent | HST/FUV-MAMA | high spatial and temporal resolution FUV observations of magnetosphere and ultraviolet auroras | May 16 (northern aurora) May 17 (northern and southern aurora) | Times may change by re-scheduling on the part of HST | ||||
1033 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | Continuous | |||||
1034 | visible/NUV | Wong | HST/WFC3 UVIS | hi-resolution map of perijove track | one orbit (50 min obs.) ~1-3 hours before perijove pass if possible, otherwise within one rotation of pass. | raw data available immediately from STScI archive; reduced maps and zonal wind profiles available within one month or potentially sooner; co-Is from MWR and JIRAM teams | ||||
1035 | near IR | Orton | IRTF/SpeX guide camera | filtered imaging at 5 strategic wavelengths, including 5.1µm and 3.4µm (H3+ auroral emission). | to be requested during 30-min interval whenever SpeX is being used | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired | ||||
1036 | mid IR | Orton | Subaru / COMICS via Keck exchange time | filtered radiometric imaging and spectroscopy to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology and auroral heating and chemistry. | mid-infrared imaging of Jupiter requested using a full set of filters close to the perijove time with observations on an adjacent night to map the comlementary hemisphere. Proposed for May 16-17 as *alternative* to May 2-3. | available for collaboration, subject to consent from collaborators | ||||
1037 | Thermal-IR | Fletcher | VLT/VISIR | High-resolution imaging 5, 8.6, 10.8, 12.3, 13.0, 17.6, 18.7, 19.5 µm. | Imaging of perijove longitude within ±36 hours of flyby. | Raw data available immediately, reduced and spatially mapped images within a few weeks. | ||||
1038 | ||||||||||
1039 | Scheduled observations by Juno. | |||||||||
1040 | ||||||||||
1041 | Perijove is 2017 May 17, 5:14:57 UTC. System-III longitude = 171.2°W | |||||||||
1042 | ||||||||||
1043 | Period: Orbit 17 [GRAV] (2017 May 16 – 2017 May 29) | |||||||||
1044 | Instrument | Description | ||||||||
1045 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||
1046 | MWR | N/S scans near perijove longitude, not centered on nadir. | ||||||||
1047 | UVS | TBD | ||||||||
1048 | JunoCam | TBD | ||||||||
1049 | JIRAM | TBD | ||||||||
1050 | ||||||||||
1051 | ||||||||||
1052 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed directly at the Earth. | |||||||||
1053 | ||||||||||
1054 | Period: Orbit 18 [GRAV] (2017 May 30 – 2017 June 12) | |||||||||
1055 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | ||||
1056 | FUV | Grodent | HST/FUV-MAMA | high spatial and temporal resolution FUV observations of magnetosphere and ultraviolet auroras | May 30-31 (Io aurora) May 30 (northern aurora) May 31 (southern aurora) | Times may change by re-scheduling on the part of HST | ||||
1057 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | Continuous | |||||
1058 | visible/NUV | Wong | HST/WFC3 UVIS | hi-resolution map of perijove track | one orbit (50 min obs.) ~1-3 hours before perijove pass if possible, otherwise within one rotation of pass. | raw data available immediately from STScI archive; reduced maps and zonal wind profiles available within one month or potentially sooner; co-Is from MWR and JIRAM teams | ||||
1059 | near IR | Orton | IRTF/SpeX guide camera | filtered imaging at 5 strategic wavelengths, including 5.1µm and 3.4µm (H3+ auroral emission). | to be requested during 30-min interval whenever SpeX is being used | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired | ||||
1060 | near IR | Bjoraker | IRTF/iSHELL | Spectra at 5 microns covering longitude of PJ 18 to support MWR | Requested HST 2017 May 29 and May 31 (first half) | Raw data available on IRTF website, reduced data available after a few months. | ||||
1061 | mid IR | Orton | Subaru / COMICS via Keck exchange time | filtered radiometric imaging and spectroscopy to map the distribution of temperatures, minor & trace constituents and aerosols defining climatology and auroral heating and chemistry. | mid-infrared imaging of Jupiter requested using a full set of filters close to the perijove time with observations on an adjacent night to map the comlementary hemisphere. Proposed for June 13-14. | available for collaboration, subject to consent from collaborators | ||||
1062 | Mid-IR | Livengood | IRTF/HIPWAC | high-resolution spectroscopy of C2H6 emission in auroral region stratosphere, 11.7 µm | Request 6 days straddling perijove to get 3 North aurora peaks, 3 south aurora peaks, midlatitudes in between peaks. | |||||
1063 | ||||||||||
1064 | Scheduled observations by Juno. | |||||||||
1065 | ||||||||||
1066 | Perijove is 2017 May 31, 4:12:29 UTC. System-III longitude = 81.0°W | |||||||||
1067 | ||||||||||
1068 | Period: Orbit 18 [GRAV] (2017 May 30 – 2017 June 12) | |||||||||
1069 | Instrument | Description | ||||||||
1070 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||
1071 | MWR | N/S scans near perijove longitude, not centered on nadir. | ||||||||
1072 | UVS | TBD | ||||||||
1073 | JunoCam | TBD | ||||||||
1074 | JIRAM | TBD | ||||||||
1075 | ||||||||||
1076 | ||||||||||
1077 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed directly at the Earth. | |||||||||
1078 | ||||||||||
1079 | Period: Orbit 19 [GRAV] (2017 June 13 – 2017 June 26) | |||||||||
1080 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | ||||
1081 | FUV | Grodent | HST/FUV-MAMA | high spatial and temporal resolution FUV observations of magnetosphere and ultraviolet auroras | Jun 13 (northern aurora) Jun 14 (northern and southern aurora) Jun 21 (northern aurora) | Times may change by re-scheduling on the part of HST | ||||
1082 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | Continuous | |||||
1083 | visible/NUV | Wong | HST/WFC3 UVIS | hi-resolution map of perijove track | one orbit (50 min obs.) ~1-3 hours before perijove pass if possible, otherwise within one rotation of pass. | raw data available immediately from STScI archive; reduced maps and zonal wind profiles available within one month or potentially sooner; co-Is from MWR and JIRAM teams | ||||
1084 | near IR | Orton | IRTF/SpeX guide camera | filtered imaging at 5 strategic wavelengths, including 5.1µm and 3.4µm (H3+ auroral emission). | to be requested during 30-min interval whenever SpeX is being used | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired | ||||
1085 | mid IR | Johnson | IRTF/iSHELL | Scans of the southern auroral H3+ emission at ~3.4µm. Simultaneous to JIRAM, MAG, JADE and JEDI measurements. | Proposed 14th June 2017 | Raw data available on IRTF website, reduced data available after a few months. | ||||
1086 | Thermal-IR | Fletcher | VLT/VISIR | High-resolution imaging 5, 8.6, 10.8, 12.3, 13.0, 17.6, 18.7, 19.5 µm. | Imaging of perijove longitude within ±36 hours of flyby. | Raw data available immediately, reduced and spatially mapped images within a few weeks. | ||||
1087 | ||||||||||
1088 | Scheduled observations by Juno. | |||||||||
1089 | ||||||||||
1090 | Perijove is 2017 June 14, 3:10:03 UTC. System-III longitude = 350.7°W | |||||||||
1091 | ||||||||||
1092 | Period: Orbit 19 [GRAV] (2017 June 13 – 2017 June 26) | |||||||||
1093 | Instrument | Description | ||||||||
1094 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||
1095 | MWR | N/S scans near perijove longitude, not centered on nadir. | ||||||||
1096 | UVS | TBD | ||||||||
1097 | JunoCam | TBD | ||||||||
1098 | JIRAM | TBD | ||||||||
1099 | ||||||||||
1100 | ||||||||||
1101 | ||||||||||
1102 | ||||||||||
1103 | ||||||||||
1104 | ||||||||||
1105 | ||||||||||
1106 | ||||||||||
1107 | ||||||||||
1108 | ||||||||||
1109 | ||||||||||
1110 | ||||||||||
1111 | ||||||||||
1112 | ||||||||||
1113 | ||||||||||
1114 | ||||||||||
1115 | ||||||||||
1116 | ||||||||||
1117 | ||||||||||
1118 | ||||||||||
1119 | ||||||||||
1120 | ||||||||||
1121 | ||||||||||
1122 | ||||||||||
1123 | ||||||||||
1124 | ||||||||||
1125 | ||||||||||
1126 | ||||||||||
1127 | ||||||||||
1128 | ||||||||||
1129 | ||||||||||
1130 | ||||||||||
1131 | ||||||||||
1132 | ||||||||||
1133 | ||||||||||
1134 | ||||||||||
1135 | ||||||||||
1136 | ||||||||||
1137 | ||||||||||
1138 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed directly at the Earth. | |||||||||
1139 | ||||||||||
1140 | Period: Orbit 20 [GRAV] (2017 June 27 – 2017 July 10) | |||||||||
1141 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | ||||
1142 | X-ray | Gladstone | Chandra | 5-hour observation for day of perijove only targeting the northern aurora | 28 June 2017 | |||||
1143 | FUV | Grodent | HST/FUV-MAMA | high spatial and temporal resolution FUV observations of magnetosphere and ultraviolet auroras | Jun 27 (northern aurora) Jun 28 (northern and southern aurora) Jul 05 (southern aurora) | Times may change by re-scheduling on the part of HST | ||||
1144 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | Continuous | |||||
1145 | visible/NUV | Wong | HST/WFC3 UVIS | hi-resolution map of perijove track | one orbit (50 min obs.) ~1-3 hours before perijove pass if possible, otherwise within one rotation of pass. | raw data available immediately from STScI archive; reduced maps and zonal wind profiles available within one month or potentially sooner; co-Is from MWR and JIRAM teams | ||||
1146 | near IR | Orton | IRTF/SpeX guide camera | filtered imaging at 5 strategic wavelengths, including 5.1µm and 3.4µm (H3+ auroral emission). | to be requested during 30-min interval whenever SpeX is being used | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired | ||||
1147 | mid IR | Johnson | IRTF/iSHELL | Scans of the southern auroral H3+ emission at ~3.4µm. Simultaneous to JIRAM, MAG, JADE and JEDI measurements. | Proposed 28th June 2017 | Raw data available on IRTF website, reduced data available after a few months. | ||||
1148 | ||||||||||
1149 | Scheduled observations by Juno. | |||||||||
1150 | ||||||||||
1151 | Perijove is 2017 June 28, 3:40:40 UTC. System-III longitude = 316.7°W | |||||||||
1152 | ||||||||||
1153 | Period: Orbit 20 [GRAV] (2017 June 27 – 2017 July 10) | |||||||||
1154 | Instrument | Description | ||||||||
1155 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||
1156 | MWR | N/S scans near perijove longitude, not centered on nadir. | ||||||||
1157 | UVS | TBD | ||||||||
1158 | JunoCam | TBD | ||||||||
1159 | JIRAM | TBD | ||||||||
1160 | ||||||||||
1161 | ||||||||||
1162 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed directly at the Earth. | |||||||||
1163 | ||||||||||
1164 | Period: Orbit 21 [GRAV] (2017 July 11 – 2017 July 24) | |||||||||
1165 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | ||||
1166 | FUV | Grodent | HST/FUV-MAMA | high spatial and temporal resolution FUV observations of magnetosphere and ultraviolet auroras | Jul 11 (northern aurora) Jul 12 (southern aurora) Jul 18-19 (northern aurora) | Times may change by re-scheduling on the part of HST | ||||
1167 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | Continuous | |||||
1168 | visible/NUV | Wong | HST/WFC3 UVIS | hi-resolution map of perijove track | one orbit (50 min obs.) ~1-3 hours before perijove pass if possible, otherwise within one rotation of pass. | raw data available immediately from STScI archive; reduced maps and zonal wind profiles available within one month or potentially sooner; co-Is from MWR and JIRAM teams | ||||
1169 | near IR | Orton | IRTF/SpeX guide camera | filtered imaging at 5 strategic wavelengths, including 5.1µm and 3.4µm (H3+ auroral emission). | to be requested during 30-min interval whenever SpeX is being used | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired | ||||
1170 | mid IR | Johnson | IRTF/iSHELL | Scans of the southern auroral H3+ emission at ~3.4µm. Simultaneous to JIRAM, MAG, JADE and JEDI measurements. | Proposed 12th July 2017 | Raw data available on IRTF website, reduced data available after a few months. | ||||
1171 | Thermal-IR | Fletcher | VLT/VISIR | High-resolution imaging 5, 8.6, 10.8, 12.3, 13.0, 17.6, 18.7, 19.5 µm. | Imaging of perijove longitude within ±36 hours of flyby. | Raw data available immediately, reduced and spatially mapped images within a few weeks. | ||||
1172 | ||||||||||
1173 | Scheduled observations by Juno. | |||||||||
1174 | ||||||||||
1175 | Perijove is 2017 July 12, 2:38:12 UTC. System-III longitude = 226.4°W | |||||||||
1176 | ||||||||||
1177 | Period: Orbit 21 [GRAV] (2017 July 11 – 2017 July 24) | |||||||||
1178 | Instrument | Description | ||||||||
1179 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||
1180 | MWR | N/S scans near perijove longitude, not centered on nadir. | ||||||||
1181 | UVS | TBD | ||||||||
1182 | JunoCam | TBD | ||||||||
1183 | JIRAM | TBD | ||||||||
1184 | ||||||||||
1185 | ||||||||||
1186 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed directly at the Earth. | |||||||||
1187 | ||||||||||
1188 | Period: Orbit 22 [GRAV] (2017 July 25 – 2017 August 7) | |||||||||
1189 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | ||||
1190 | X-ray | Gladstone | Chandra | 5-hour observation for day of perijove only targeting the northern aurora | 26 July 2017 | |||||
1191 | FUV | Grodent | HST/FUV-MAMA | high spatial and temporal resolution FUV observations of magnetosphere and ultraviolet auroras | Jul 25 (northern aurora) Jul 26 (northern and southern aurora) Aug 02 (northern aurora) | Times may change by re-scheduling on the part of HST | ||||
1192 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | Continuous | |||||
1193 | visible/NUV | Wong | HST/WFC3 UVIS | hi-resolution map of perijove track | one orbit (50 min obs.) ~1-3 hours before perijove pass if possible, otherwise within one rotation of pass. | raw data available immediately from STScI archive; reduced maps and zonal wind profiles available within one month or potentially sooner; co-Is from MWR and JIRAM teams | ||||
1194 | near IR | Orton | IRTF/SpeX guide camera | filtered imaging at 5 strategic wavelengths, including 5.1µm and 3.4µm (H3+ auroral emission). | to be requested during 30-min interval whenever SpeX is being used | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired | ||||
1195 | ||||||||||
1196 | Scheduled observations by Juno. | |||||||||
1197 | ||||||||||
1198 | Perijove is 2017 July 26, 1:35:46 UTC. System-III longitude = 136.2°W | |||||||||
1199 | ||||||||||
1200 | Period: Orbit 22 [GRAV] (2017 July 25 – 2017 August 7) | |||||||||
1201 | Instrument | Description | ||||||||
1202 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||
1203 | MWR | N/S scans near perijove longitude, not centered on nadir. | ||||||||
1204 | UVS | TBD | ||||||||
1205 | JunoCam | TBD | ||||||||
1206 | JIRAM | TBD | ||||||||
1207 | ||||||||||
1208 | ||||||||||
1209 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed directly at the Earth. | |||||||||
1210 | ||||||||||
1211 | Period: Orbit 23 [GRAV] (2017 August 8 – 2017 August 21) | |||||||||
1212 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | ||||
1213 | FUV | Grodent | HST/FUV-MAMA | high spatial and temporal resolution FUV observations of magnetosphere and ultraviolet auroras | Aug 8 (northern and southern aurora) Aug 9 (southern aurora) | Times may change by re-scheduling on the part of HST | ||||
1214 | visible/NUV | Wong | HST/WFC3 UVIS | hi-resolution map of perijove track | one orbit (50 min obs.) ~1-3 hours before perijove pass if possible, otherwise within one rotation of pass. | raw data available immediately from STScI archive; reduced maps and zonal wind profiles available within one month or potentially sooner; co-Is from MWR and JIRAM teams | ||||
1215 | near IR | Orton | IRTF/SpeX guide camera | filtered imaging at 5 strategic wavelengths, including 5.1µm and 3.4µm (H3+ auroral emission). | to be requested during 30-min interval whenever SpeX is being used | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired | ||||
1216 | Thermal-IR | Fletcher | VLT/VISIR | High-resolution imaging 5, 8.6, 10.8, 12.3, 13.0, 17.6, 18.7, 19.5 µm. | Imaging of perijove longitude within ±36 hours of flyby. | Raw data available immediately, reduced and spatially mapped images within a few weeks. | ||||
1217 | ||||||||||
1218 | Scheduled observations by Juno. | |||||||||
1219 | ||||||||||
1220 | Perijove is 2017 August 9, 0:33:19 UTC. System-III longitude = 45.9°W | |||||||||
1221 | ||||||||||
1222 | Period: Orbit 23 [GRAV] (2017 August 8 – 2017 August 21) | |||||||||
1223 | Instrument | Description | ||||||||
1224 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||
1225 | MWR | N/S scans near perijove longitude, possibly centered on Great Red Spot close to nadir viewing. | ||||||||
1226 | UVS | TBD | ||||||||
1227 | JunoCam | TBD | ||||||||
1228 | JIRAM | TBD | ||||||||
1229 | ||||||||||
1230 | ||||||||||
1231 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed directly at the Earth. It is during this orbit that the MWR and other remote-sensing instrument, if they still function, have the best opportunity to measure the Great Red Spot. | |||||||||
1232 | ||||||||||
1233 | Period: Orbit 24 [GRAV] (2017 August 22 – 2017 September 3) | |||||||||
1234 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | ||||
1235 | visible/NUV | Wong | HST/WFC3 UVIS | hi-resolution map of perijove track | one orbit (50 min obs.) ~1-3 hours before perijove pass if possible, otherwise within one rotation of pass. | raw data available immediately from STScI archive; reduced maps and zonal wind profiles available within one month or potentially sooner; co-Is from MWR and JIRAM teams | ||||
1236 | near IR | Orton | IRTF/SpeX guide camera | filtered imaging at 5 strategic wavelengths, including 5.1µm and 3.4µm (H3+ auroral emission). | to be requested during 30-min interval whenever SpeX is being used | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired | ||||
1237 | ||||||||||
1238 | Scheduled observations by Juno. | |||||||||
1239 | ||||||||||
1240 | Perijove is 2017 August 23, 0:08:07 UTC. System-III longitude = 338.1°W | |||||||||
1241 | ||||||||||
1242 | Period: Orbit 24 [GRAV] (2017 August 22 – 2017 September 3) | |||||||||
1243 | Instrument | Description | ||||||||
1244 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||
1245 | MWR | N/S scans near perijove longitude, not centered on nadir. | ||||||||
1246 | UVS | TBD | ||||||||
1247 | JunoCam | TBD | ||||||||
1248 | JIRAM | TBD | ||||||||
1249 | ||||||||||
1250 | ||||||||||
1251 | ||||||||||
1252 | ||||||||||
1253 | ||||||||||
1254 | ||||||||||
1255 | ||||||||||
1256 | ||||||||||
1257 | ||||||||||
1258 | ||||||||||
1259 | ||||||||||
1260 | ||||||||||
1261 | ||||||||||
1262 | ||||||||||
1263 | ||||||||||
1264 | ||||||||||
1265 | ||||||||||
1266 | ||||||||||
1267 | ||||||||||
1268 | ||||||||||
1269 | ||||||||||
1270 | ||||||||||
1271 | ||||||||||
1272 | ||||||||||
1273 | ||||||||||
1274 | ||||||||||
1275 | ||||||||||
1276 | ||||||||||
1277 | ||||||||||
1278 | ||||||||||
1279 | ||||||||||
1280 | ||||||||||
1281 | ||||||||||
1282 | ||||||||||
1283 | ||||||||||
1284 | ||||||||||
1285 | ||||||||||
1286 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed directly at the Earth. | |||||||||
1287 | ||||||||||
1288 | Period: Orbit 25 [GRAV] (2017 September 4 – 2017 September 17) | |||||||||
1289 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | ||||
1290 | near IR | Orton | IRTF/SpeX guide camera | filtered imaging at 5 strategic wavelengths, including 5.1µm and 3.4µm (H3+ auroral emission). | to be requested during 30-min interval whenever SpeX is being used | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired | ||||
1291 | ||||||||||
1292 | Scheduled observations by Juno. | |||||||||
1293 | ||||||||||
1294 | Perijove is 2017 September 5, 23:05:44 UTC. System-III longitude = 247.9°W | |||||||||
1295 | ||||||||||
1296 | Period: Orbit 25 [GRAV] (2017 September 4– 2017 September 17) | |||||||||
1297 | Instrument | Description | ||||||||
1298 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||
1299 | MWR | N/S scans near perijove longitude, not centered on nadir. | ||||||||
1300 | UVS | TBD | ||||||||
1301 | JunoCam | TBD | ||||||||
1302 | JIRAM | TBD | ||||||||
1303 | ||||||||||
1304 | ||||||||||
1305 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed directly at the Earth. | |||||||||
1306 | ||||||||||
1307 | Period: Orbit 26 [GRAV] (2017 September 18 – 2017 October 1) | |||||||||
1308 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | ||||
1309 | near IR | Orton | IRTF/SpeX guide camera | filtered imaging at 5 strategic wavelengths, including 5.1µm and 3.4µm (H3+ auroral emission). | to be requested during 30-min interval whenever SpeX is being used | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired | ||||
1310 | ||||||||||
1311 | Scheduled observations by Juno. | |||||||||
1312 | ||||||||||
1313 | Perijove is 2017 September 19, 22:03:21 UTC. System-III longitude = 157.6°W | |||||||||
1314 | ||||||||||
1315 | Period: Orbit 26 [GRAV] (2017 September 18– 2017 October 1) | |||||||||
1316 | Instrument | Description | ||||||||
1317 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||
1318 | MWR | N/S scans near perijove longitude, not centered on nadir. | ||||||||
1319 | UVS | TBD | ||||||||
1320 | JunoCam | TBD | ||||||||
1321 | JIRAM | TBD | ||||||||
1322 | ||||||||||
1323 | ||||||||||
1324 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed directly at the Earth. It is during this orbit that the MWR and other remote-sensing instrument, if they still function, have the second-best opportunity to measure the Great Red Spot. | |||||||||
1325 | ||||||||||
1326 | Period: Orbit 27 [GRAV] (2017 October 2 – 2017 October 15) | |||||||||
1327 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | ||||
1328 | near IR | Orton | IRTF/SpeX guide camera | filtered imaging at 5 strategic wavelengths, including 5.1µm and 3.4µm (H3+ auroral emission). | to be requested during 30-min interval whenever SpeX is being used | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired | ||||
1329 | ||||||||||
1330 | Scheduled observations by Juno. | |||||||||
1331 | ||||||||||
1332 | Perijove is 2017 October 3, 21:00:55 UTC. System-III longitude = 67.4°W | |||||||||
1333 | ||||||||||
1334 | Period: Orbit 27 [GRAV] (2017 October 2– 2017 October 15) | |||||||||
1335 | Instrument | Description | ||||||||
1336 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||
1337 | MWR | N/S scans near perijove longitude, not centered on nadir. | ||||||||
1338 | UVS | TBD | ||||||||
1339 | JunoCam | TBD | ||||||||
1340 | JIRAM | TBD | ||||||||
1341 | ||||||||||
1342 | ||||||||||
1343 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed directly at the Earth. Jupiter reaches solar conjunction on October 26, so the prospect of obtaining any Earth-based observations during this period is low. | |||||||||
1344 | ||||||||||
1345 | Period: Orbit 28 [GRAV] (2017 October 16 – 2017 October 29) | |||||||||
1346 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | ||||
1347 | ||||||||||
1348 | ||||||||||
1349 | Scheduled observations by Juno. | |||||||||
1350 | ||||||||||
1351 | Perijove is 2017 October 17, 20:5:43 UTC. System-III longitude = 359.6°W | |||||||||
1352 | ||||||||||
1353 | Period: Orbit 28 [GRAV] (2017 October 16 – 2017 October 29) | |||||||||
1354 | Instrument | Description | ||||||||
1355 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||
1356 | MWR | N/S scans near perijove longitude, not centered on nadir. | ||||||||
1357 | UVS | TBD | ||||||||
1358 | JunoCam | TBD | ||||||||
1359 | JIRAM | TBD | ||||||||
1360 | ||||||||||
1361 | ||||||||||
1362 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed directly at the Earth. With solar conjunction on October 26, there may be few Earth-based observations of Jupiter during this time frame. | |||||||||
1363 | ||||||||||
1364 | ||||||||||
1365 | ||||||||||
1366 | ||||||||||
1367 | ||||||||||
1368 | ||||||||||
1369 | ||||||||||
1370 | ||||||||||
1371 | ||||||||||
1372 | ||||||||||
1373 | ||||||||||
1374 | ||||||||||
1375 | ||||||||||
1376 | ||||||||||
1377 | ||||||||||
1378 | ||||||||||
1379 | ||||||||||
1380 | ||||||||||
1381 | ||||||||||
1382 | ||||||||||
1383 | ||||||||||
1384 | ||||||||||
1385 | ||||||||||
1386 | ||||||||||
1387 | ||||||||||
1388 | ||||||||||
1389 | ||||||||||
1390 | ||||||||||
1391 | ||||||||||
1392 | ||||||||||
1393 | ||||||||||
1394 | ||||||||||
1395 | ||||||||||
1396 | Period: Orbit 29 [GRAV] (2017 October 30 – 2017 November 12) | |||||||||
1397 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | ||||
1398 | near IR | Orton | IRTF/SpeX guide camera | filtered imaging at 5 strategic wavelengths, including 5.1µm and 3.4µm (H3+ auroral emission). | to be requested during 30-min interval whenever SpeX is being used | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired | ||||
1399 | ||||||||||
1400 | Scheduled observations by Juno. | |||||||||
1401 | ||||||||||
1402 | Perijove is 2017 October 31, 19:33:14 UTC. System-III longitude = 269.3°W | |||||||||
1403 | ||||||||||
1404 | Period: Orbit 29 [GRAV] (2017 October 30 – 2017 November 12) | |||||||||
1405 | Instrument | Description | ||||||||
1406 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||
1407 | MWR | N/S scans near perijove longitude, not centered on nadir. | ||||||||
1408 | UVS | TBD | ||||||||
1409 | JunoCam | TBD | ||||||||
1410 | JIRAM | TBD | ||||||||
1411 | ||||||||||
1412 | ||||||||||
1413 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed directly at the Earth. | |||||||||
1414 | ||||||||||
1415 | Period: Orbit 30 [GRAV] (2017 November 13 – 2017 November 26) | |||||||||
1416 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | ||||
1417 | near IR | Orton | IRTF/SpeX guide camera | filtered imaging at 5 strategic wavelengths, including 5.1µm and 3.4µm (H3+ auroral emission). | to be requested during 30-min interval whenever SpeX is being used | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired | ||||
1418 | ||||||||||
1419 | Scheduled observations by Juno. | |||||||||
1420 | ||||||||||
1421 | Perijove is 2017 November 14, 18:30:45 UTC. System-III longitude = 179.0°W | |||||||||
1422 | ||||||||||
1423 | Period: Orbit 30 [GRAV] (2017 November 13 – 2017 November 26) | |||||||||
1424 | Instrument | Description | ||||||||
1425 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||
1426 | MWR | N/S scans near perijove longitude, not centered on nadir. | ||||||||
1427 | UVS | TBD | ||||||||
1428 | JunoCam | TBD | ||||||||
1429 | JIRAM | TBD | ||||||||
1430 | ||||||||||
1431 | ||||||||||
1432 | ||||||||||
1433 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed directly at the Earth. | |||||||||
1434 | ||||||||||
1435 | Period: Orbit 31 [GRAV] (2017 November 27 – 2017 December 10) | |||||||||
1436 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | ||||
1437 | near IR | Orton | IRTF/SpeX guide camera | filtered imaging at 5 strategic wavelengths, including 5.1µm and 3.4µm (H3+ auroral emission). | to be requested during 30-min interval whenever SpeX is being used | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired | ||||
1438 | ||||||||||
1439 | Scheduled observations by Juno. | |||||||||
1440 | ||||||||||
1441 | Perijove is 2017 November 28, 17:28:16 UTC. System-III longitude = 88.8°W | |||||||||
1442 | ||||||||||
1443 | Period: Orbit 31 [GRAV] (2017 November 27 – 2017 December 10) | |||||||||
1444 | Instrument | Description | ||||||||
1445 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||
1446 | MWR | N/S scans near perijove longitude, not centered on nadir. | ||||||||
1447 | UVS | TBD | ||||||||
1448 | JunoCam | TBD | ||||||||
1449 | JIRAM | TBD | ||||||||
1450 | ||||||||||
1451 | ||||||||||
1452 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed directly at the Earth. | |||||||||
1453 | ||||||||||
1454 | Period: Orbit 32 [GRAV] (2017 December 11 – 2017 December 24) | |||||||||
1455 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | ||||
1456 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | Continuous | |||||
1457 | near IR | Orton | IRTF/SpeX guide camera | filtered imaging at 5 strategic wavelengths, including 5.1µm and 3.4µm (H3+ auroral emission). | to be requested during 30-min interval whenever SpeX is being used | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired | ||||
1458 | ||||||||||
1459 | Scheduled observations by Juno. | |||||||||
1460 | ||||||||||
1461 | Perijove is 2017 December 12, 17:02:53 UTC. System-III longitude = 20.9°W | |||||||||
1462 | ||||||||||
1463 | Period: Orbit 32 [GRAV] (2017 December 11 – 2017 December 24) | |||||||||
1464 | Instrument | Description | ||||||||
1465 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||
1466 | MWR | N/S scans near perijove longitude, not centered on nadir. | ||||||||
1467 | UVS | TBD | ||||||||
1468 | JunoCam | TBD | ||||||||
1469 | JIRAM | TBD | ||||||||
1470 | ||||||||||
1471 | ||||||||||
1472 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed directly at the Earth. | |||||||||
1473 | ||||||||||
1474 | Period: Orbit 33 [GRAV] (2017 December 25 – 2018 January 7) | |||||||||
1475 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | ||||
1476 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | Continuous | |||||
1477 | visible/NUV | Wong | HST/WFC3 UVIS | hi-resolution map of perijove track | one orbit (50 min obs.) ~1-3 hours before perijove pass if possible, otherwise within one rotation of pass. | raw data available immediately from STScI archive; reduced maps and zonal wind profiles available within one month or potentially sooner; co-Is from MWR and JIRAM teams | ||||
1478 | near IR | Orton | IRTF/SpeX guide camera | filtered imaging at 5 strategic wavelengths, including 5.1µm and 3.4µm (H3+ auroral emission). | to be requested during 30-min interval whenever SpeX is being used | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired | ||||
1479 | ||||||||||
1480 | Scheduled observations by Juno. | |||||||||
1481 | ||||||||||
1482 | Perijove is 2017 December 26, 16:00:20 UTC. System-III longitude = 290.6°W | |||||||||
1483 | ||||||||||
1484 | Period: Orbit 33 [GRAV] (2017 December 25 – 2018 January 7) | |||||||||
1485 | Instrument | Description | ||||||||
1486 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||
1487 | MWR | N/S scans near perijove longitude, not centered on nadir. | ||||||||
1488 | UVS | TBD | ||||||||
1489 | JunoCam | TBD | ||||||||
1490 | JIRAM | TBD | ||||||||
1491 | ||||||||||
1492 | ||||||||||
1493 | ||||||||||
1494 | ||||||||||
1495 | ||||||||||
1496 | ||||||||||
1497 | ||||||||||
1498 | ||||||||||
1499 | ||||||||||
1500 | ||||||||||
1501 | ||||||||||
1502 | ||||||||||
1503 | ||||||||||
1504 | ||||||||||
1505 | ||||||||||
1506 | ||||||||||
1507 | ||||||||||
1508 | ||||||||||
1509 | ||||||||||
1510 | ||||||||||
1511 | ||||||||||
1512 | ||||||||||
1513 | ||||||||||
1514 | ||||||||||
1515 | ||||||||||
1516 | ||||||||||
1517 | ||||||||||
1518 | ||||||||||
1519 | ||||||||||
1520 | ||||||||||
1521 | ||||||||||
1522 | ||||||||||
1523 | ||||||||||
1524 | ||||||||||
1525 | ||||||||||
1526 | ||||||||||
1527 | ||||||||||
1528 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed directly at the Earth. | |||||||||
1529 | ||||||||||
1530 | Period: Orbit 34 [GRAV] (2018 January 8 – 2018 January 21) | |||||||||
1531 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | ||||
1532 | X-ray | Gladstone | Chandra | 5-hour observation for day of perijove only targeting the northern aurora | 9 January 2018 | |||||
1533 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | Continuous | |||||
1534 | visible/NUV | Wong | HST/WFC3 UVIS | hi-resolution map of perijove track | one orbit (50 min obs.) ~1-3 hours before perijove pass if possible, otherwise within one rotation of pass. | raw data available immediately from STScI archive; reduced maps and zonal wind profiles available within one month or potentially sooner; co-Is from MWR and JIRAM teams | ||||
1535 | near IR | Orton | IRTF/SpeX guide camera | filtered imaging at 5 strategic wavelengths, including 5.1µm and 3.4µm (H3+ auroral emission). | to be requested during 30-min interval whenever SpeX is being used | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired | ||||
1536 | ||||||||||
1537 | Scheduled observations by Juno. | |||||||||
1538 | ||||||||||
1539 | Perijove is 2018 January 9, 14:57:50 UTC. System-III longitude = 200.3°W | |||||||||
1540 | ||||||||||
1541 | Period: Orbit 34 [GRAV] (2018 January 8 – 2018 January 21) | |||||||||
1542 | Instrument | Description | ||||||||
1543 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||
1544 | MWR | N/S scans near perijove longitude, not centered on nadir. | ||||||||
1545 | UVS | TBD | ||||||||
1546 | JunoCam | TBD | ||||||||
1547 | JIRAM | TBD | ||||||||
1548 | ||||||||||
1549 | ||||||||||
1550 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed directly at the Earth. | |||||||||
1551 | ||||||||||
1552 | Period: Orbit 35 [GRAV] (2018 January 22 – 2018 February 4) | |||||||||
1553 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | ||||
1554 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | Continuous | |||||
1555 | visible/NUV | Wong | HST/WFC3 UVIS | hi-resolution map of perijove track | one orbit (50 min obs.) ~1-3 hours before perijove pass if possible, otherwise within one rotation of pass. | raw data available immediately from STScI archive; reduced maps and zonal wind profiles available within one month or potentially sooner; co-Is from MWR and JIRAM teams | ||||
1556 | near IR | Orton | IRTF/SpeX guide camera | filtered imaging at 5 strategic wavelengths, including 5.1µm and 3.4µm (H3+ auroral emission). | to be requested during 30-min interval whenever SpeX is being used | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired | ||||
1557 | ||||||||||
1558 | Scheduled observations by Juno. | |||||||||
1559 | ||||||||||
1560 | Perijove is 2018 January 23, 13:55:18 UTC. System-III longitude = 109.9°W | |||||||||
1561 | ||||||||||
1562 | Period: Orbit 35 [GRAV] (2018 January 22 – 2018 February 4) | |||||||||
1563 | Instrument | Description | ||||||||
1564 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||
1565 | MWR | N/S scans near perijove longitude, not centered on nadir. | ||||||||
1566 | UVS | TBD | ||||||||
1567 | JunoCam | TBD | ||||||||
1568 | JIRAM | TBD | ||||||||
1569 | ||||||||||
1570 | ||||||||||
1571 | Note: On this orbit the spacecraft orientation optimizes gravity sensing with the antenna pointed directly at the Earth. | |||||||||
1572 | ||||||||||
1573 | Period: Orbit 36 [EXTRA] (2018 February 5 – 2018 February 18) | |||||||||
1574 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | ||||
1575 | X-ray | Gladstone | Chandra | 5-hour observation for day of perijove only targeting the northern aurora | 6 February 2018 | |||||
1576 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | Continuous | |||||
1577 | visible/NUV | Wong | HST/WFC3 UVIS | hi-resolution map of perijove track | one orbit (50 min obs.) ~1-3 hours before perijove pass if possible, otherwise within one rotation of pass. | raw data available immediately from STScI archive; reduced maps and zonal wind profiles available within one month or potentially sooner; co-Is from MWR and JIRAM teams | ||||
1578 | near IR | Orton | IRTF/SpeX guide camera | filtered imaging at 5 strategic wavelengths, including 5.1µm and 3.4µm (H3+ auroral emission). | to be requested during 30-min interval whenever SpeX is being used | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired | ||||
1579 | ||||||||||
1580 | Scheduled observations by Juno. | |||||||||
1581 | ||||||||||
1582 | Perijove is 2018 February 6, 12:52:47 UTC. System-III longitude = 19.6°W | |||||||||
1583 | ||||||||||
1584 | Period: Orbit 36 [EXTRA] (2018 February 5 – 2018 February 18) | |||||||||
1585 | Instrument | Description | ||||||||
1586 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||
1587 | MWR | N/S scans near perijove longitude, not centered on nadir. | ||||||||
1588 | UVS | TBD | ||||||||
1589 | JunoCam | TBD | ||||||||
1590 | JIRAM | TBD | ||||||||
1591 | ||||||||||
1592 | ||||||||||
1593 | Note: On this orbit the spacecraft will be configured to enter the atmosphere of Jupiter and the nominal mission completed unless an extended mission is approved by NASA. | |||||||||
1594 | ||||||||||
1595 | Period: Orbit 37 [DEORBIT] (2018 February 19 – TBD) | |||||||||
1596 | Spectral Region | PI | Facility/ Instrument | Description | Date Scheduled/ Requested | Data Availability | ||||
1597 | Visible | Morgenthaler | Io Input/Output robotic telescope (IoIO) | 35-cm telescope and coronograph to study the Jovian sodium nebula and Io plasma torus in [SII] 6731A | Continuous | |||||
1598 | near IR | Orton | IRTF/SpeX guide camera | filtered imaging at 5 strategic wavelengths, including 5.1µm and 3.4µm (H3+ auroral emission). | to be requested during 30-min interval whenever SpeX is being used | raw images available immediately from IRTF web site; fully reduced images available within a month or sooner, as desired | ||||
1599 | ||||||||||
1600 | Scheduled observations by Juno. | |||||||||
1601 | ||||||||||
1602 | Perijove is 2018 February 20, 11:39:44 UTC. System-III longitude = 282.9°W | |||||||||
1603 | ||||||||||
1604 | Period: Orbit 37 [DEORBIT] (2018 February 19 – TBD) | |||||||||
1605 | Instrument | Description | ||||||||
1606 | MAG, JADE, JEDI, WAVES | Continuous measurements of magnetic field, plasma, energetic particles, and radio/plasma waves throughout this period. | ||||||||
1607 | MWR | TBD | ||||||||
1608 | UVS | TBD | ||||||||
1609 | JunoCam | TBD | ||||||||
1610 | JIRAM | TBD | ||||||||
1611 | ||||||||||
1612 | ||||||||||
1613 | ||||||||||
1614 | ||||||||||
1615 | ||||||||||
1616 | ||||||||||
1617 | ||||||||||
1618 | ||||||||||
1619 | ||||||||||
1620 | ||||||||||
1621 | ||||||||||
1622 | ||||||||||
1623 | ||||||||||
1624 | ||||||||||
1625 | ||||||||||
1626 | ||||||||||
1627 | ||||||||||
1628 | ||||||||||
1629 | ||||||||||
1630 | ||||||||||
1631 | ||||||||||
1632 | ||||||||||
1633 | ||||||||||
1634 | ||||||||||
1635 | ||||||||||
1636 | ||||||||||
1637 | ||||||||||
1638 | ||||||||||
1639 | ||||||||||
1640 | ||||||||||
1641 | ||||||||||
1642 | ||||||||||
1643 | ||||||||||
1644 | ||||||||||
1645 | ||||||||||
1646 |
1 | Timestamp | Untitled Question |
---|---|---|