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SAT Thermal Analysis

and Verification

John Groh (he/him)�May 2, 2024

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Quick design recap

  • 3 optics tubes per mount with shared vacuum space and sub-Kelvin refrigeration
    • 1 x Bluefors SD400 (or similar)
    • 2+1 x Cryomech PT410s
  • Cryogenic design largely driven by power footprint, which is dominated by the PTCs

75.5 kW + 12 kW + 6 kW = 93.5 kW93.5 kW

  • Aggressive cryogenic design w/ notable risk
    • Mitigating w/ R&D into alternative configurations and prototyping

2

Project workshop | May 2024

(SSAs likely to mount at 4k instead)

(slight PTC geometry change since this rendering)

100mK

1K

4K

50K

300K

Cryostat

Mount

Readout

Steady state total

SAT site budget

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Steady state

  • Current status:
    • Nodal estimate structure for estimating heat loads
      • IR: adapted/updated from BICEP model
      • Supports: spreadsheet macro integrals w/ hand-curated material properties
      • Radiation: idealized MLI w/ no conduction terms
      • Readout: from Readout L3 via readout_load_calculator
      • Large uncertainties & tight budget!
    • Initial estimates have been made of gradients across metal bodies w/ FEA and basic formulae
  • Possible directions for future development:
    • Update as design evolves (e.g. strut geometries, wire count)
    • Iterate on model assumptions and methods based on prototype tests (esp. IR, MLI, (+readout))
    • Enable generating full set of thermal loads w/ new assumptions from single program
    • Document methods and assumptions
    • Account for fridge capacity curves
    • Progress beyond nodal description

3

Project workshop | May 2024

50K

4K

1K

100mK

Optical

32.1 W

0.5 W

15 mW

1 uW

Radiation

15.0 W

~0 W

~0 mW

~0 uW

Supports

9.1 W

0.4 W

~0 mW

small (TBC)

Readout

13.7 W

0.7 W

0.5 mW

49 uW

Total

~70 W

~1.7 W

~16 mW

~50 uW

Budget

80 W

2 W

20 mW

400 uW

(Some inconsistencies and omissions found while filling this table - revisit needed…)

50K and 1K budgets currently tightest w/ largest estimated contribution from optical loading

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Steady state: optical loading

  • Methodology from Jamie Bock, Denis Barkat, Lingzhen Zeng, David Goldfinger
  • “Conventional” model integrating over photon distributions, featuring:
    • Radial temperature gradients
    • Non-constant thicknesses
    • Temperature dependent thermal conductivities (hand curated)
    • Constant optical properties w/ temperature (hand curated)
  • Link to reports and model code
  • Would be interesting to compare to other calculators (incl. the ACT/SO-style ray tracing method)

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Project workshop | May 2024

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Cooldown time

  • Naive scaling from Simons Observatory SAT suggests unaided cooldown (~8 days) will be too long
    • We have ~3x the payload and ~3/4ths the cooling power
    • Initial requirement from I&C scheduling concerns (CMBS4-L3-467): <11.25 days
  • Ongoing study of speedup options
    • Survey of turnkey and custom heat switch and precooling options
    • Network model-based simulation tool

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Project workshop | May 2024

gas-gap

mechanical

LN2 precool

Toy model

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R&D and Prototyping

  • R&D efforts targeting PTC risks:
    • Alternative low-power model
    • Optimization w/ inverter compressor
    • Water cooling of PTC exterior
    • Study of tilt, helium charge, motor frequency dependence of candidate models w/ realistic hoses & joints
  • Optics testbed cryostat:
    • Iterate on optical load model based on measurements
  • Prototype SAT cryostat:
    • Iterate on radiative, conductive, cabling model inputs based on measurements
    • Retire thermal risk of 3-tube design w/ constrained cooling
  • High-level plan captured in SAT logic flow chart

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Project workshop | May 2024

Tiltable PTC test cryostat

Presentation reference

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Mutual benefit opportunities w/ LATR, HTCs

  • Overall strategy as we progress beyond a basic nodal model
  • Refrigerator optimization & alternative studies
  • IR loading knowledge
  • Material property assumptions (utilize S4 conductivity database?)
  • Cooldown speedup solutions

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Project workshop | May 2024

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Backup

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Project workshop | May 2024

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References

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Project workshop | May 2024

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IR thermal model

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Project workshop | May 2024

(modulo some refinements since the PBDR)

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Cryostat cross section

Project workshop | May 2024

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Feed horns

(1.05 - Modules)

Metal Mesh LP Edge Filter

Field Lens

Absorptive Baffling

Nylon Filter

Objective Lens and Aperture Stop

RT-MLI foam stack

Vacuum Window

Absorptive Baffling inside magnetic shielding

Alumina Filter

Front of cryostat replaceable to allow space for half-wave plate

1 K

100 mK

50 K

250-140 K

Ambient

(modulo some refinements since the PBDR)