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Opportunities and value that small satellites offer for space weather research

Paul O’Brien

Space Sciences Department

The Aerospace Corporation

Second International Workshop on Small Satellites for Space Weather Research & Forecasting

Acknowledgements: C. Gabrielse, L. Blum, J. Lee, X. Li, and J. Carroll provided information on GTOsat/REMS, uCPT, REPtile, and LEMUR

© The Aerospace Corporation, 2022

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Outline

  • Test new sensors
  • Targeted re-flight of flagship science sensors
  • In situ validation of simple sensors
  • Rapid turnaround on critical needs
  • Proliferation of sensors

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Test new sensors

  • AC-6 Dos1 was a test flight for REACH Z dosimeter
    • AC-6 two 0.5U cubesats
    • REACH is a constellation of 32 dosimeter pairs on IridiumNEXT
    • At the time REACH was conceived, a new class of dosimeter, for low energies, was only on the drawing board
    • The AeroCube-6 mission flew and proved out these new dosimeters
    • They were incorporated as the “Z” flavor of dosimeter on the REACH constellation (https://doi.org/10.5281/zenodo.5988170)
  • Flight of uCPT on AC-10
    • 7.6x4.8x4.1 cm
    • 268 g
    • Electrons 0.1-2.5 MeV
    • Protons and ions 80 keV-1 MeV
    • Raised TRL of compact environmental sensor

AC-6

REACH 0 POD

Z Dosimeter

uCPT

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Targeted re-flight

  • SmallSats offer an opportunity to re-fly simplified/miniaturized proven sensors from flagship missions
    • Increase chance to witness extreme events
    • Get more science out of flagship mission investment
    • Transition to space weather monitoring mission
  • REPTile on CSSWE
    • Based on REPT from Van Allen Probes
    • Mission PI Xinlin Li
    • LEO (~600 km, 65o)
    • 0.6-4 MeV electrons
    • 1.25 kg sensor
    • Launched 2012, operated until 2014, CIRBE follow-up in mid-2023
  • REMS on GTOsat:
    • Based on MagEIS from Van Allen Probes
    • Mission PI Lauren Blum, REMS PI Christine Gabrielse, DPI Drew Turner
    • GTO (~6 RE, < 50o)
    • 0.1-1 MeV electrons
    • ~0.6-7 MeV protons
    • 1 kg sensor
    • Launch TBD, 1 year main mission

CC A-S 3.0 : https://commons.wikimedia.org/wiki/ File:CSSWE_CubeSat_and_PPOD_prior_to_integration.png

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In situ validation

  • SmallSats can be used to calibrate simple sensors hosted on multiple vehicles: allow the smallsat orbit to drift among the vehicles hosting the sensors
  • For example, AMPERE uses engineering magnetometers from Iridium satellites to estimate field-aligned currents
  • One could fly a science magnetometer on a smallsat in a perturbed Iridium-like orbit to
    • Visit each Iridium satellite and validate the interpretation of its engineering magnetometer
    • Validate interpolated fields between satellites
  • One could use the same approach to calibrate the REACH dosimeters or any other hosted sensor payloads

  • Key technology need: propulsion to get into wandering orbit

Calibration

Wanderer

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Rapid turnaround

  • SmallSats typically have faster development cycles to launch, allowing them to more rapidly prove out new sensor technologies or approaches
  • AeroCube-6 is a perfect example of this, as the REACH program was already underway when AC-6 launched
  • The AC-6 low energy dosimeters had never been flown before, and the REACH program wanted flight data before committing to them
  • The successful demonstration of low energy dosimeters on AC-6 allowed the REACH program to embrace the technology
  • AC-6 launch was June 2014
  • First REACH low energy dosimeter (flavor Z) was launched February 2017

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Proliferation of sensors

  • For small-scale phenomena or phenomena requiring continuous monitoring, large constellations are required
  • SmallSats enable proliferation of sensors throughout orbits of interest
  • E.g., Spire Global LEMUR: 6kg, ~500 km orbit, >2 year lifetime, carries a GNSS-RO sensor

Image Credit: NASA, �https://www.nasa.gov/feature/esnt/2022/

nasa-to-launch-6-small-satellites-to-monitor-study-tropical-cyclones

Image courtesy of Spire Global,

used with permission

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Conclusions

  • SmallSats have lower cost, shorter lifecycles, and higher risk profiles than their conventional counterparts
  • This opens up a variety of opportunities to provide value to space weather research and operations
    • Test new sensors: raise TRL on an operational sensor
    • Targeted re-flight of flagship science sensors: fly just-what-you-need for space weather monitoring
    • In situ validation of simple sensors: validate hosted sensors with a wandering calibration satellite
    • Rapid turnaround on critical needs: demonstrate sensor technology or CONOPS while developing the main mission
    • Proliferation of sensors: enables continuous monitoring and monitoring of small-scale phenomena
  • A key enabling technology for SmallSat missions in space weather is on-board propulsion to achieve and maintain the desired orbit, and then to dispose at end of mission

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Acronyms

  • AC – AeroCube
  • AMPERE – active magnetosphere and planetary electrodynamics response experiment
  • CIBRE – Colorado inner radiation belt experiment
  • CONOPS – concept of operations
  • CSSWE- Colorado student space weather experiment
  • DPI – deputy principal investigator
  • GTOsat – geosynchronous transfer orbit satellite
  • LEMUR - low Earth multi-use receiver
  • LEO – low Earth orbit
  • MagEIS – magnetic electron-ion spectrometer
  • uCPT – micro charged particle telescope
  • PI – principal investigator
  • REACH – responsive environmental assessment commercially hosted
  • REMS – relativistic electron magnetic spectrometer
  • REPTile – relativistic electron and proton telescope integrated little experiment
  • TBD – to be determined
  • TRL – technical readiness level

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