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Cooldown strategies and transient thermal simulations for the Simons Observatory

Authors :
Michael D. Niemack
Grant Teply
Lucio Piccirillo
Maria Salatino
Mark J. Devlin
Patricio A. Gallardo
Marius Lungu
Michele Limon
Andrew May
Gabriele Coppi
Jack L. Orlowski-Scherer
Brian Keating
Simon Dicker
Sara M. Simon
Zhilei Xu
Aamir Ali
Robert Thornton
Ningfeng Zhu
Eve M. Vavagiakis
Nicholas Galitzki
Giuseppe Puglisi
Jeff McMahon
AstroParticule et Cosmologie (APC (UMR_7164))
Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris
Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP)
Observatoire de Paris
PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
Coppi, G
Xu, Z
Ali, A
Galitzki, N
Gallardo, P
May, A
Orlowski-Scherer, J
Zhu, N
Devlin, M
Dicker, S
Keating, B
Limon, M
Lungu, M
Mcmahon, J
Niemack, M
Piccirillo, L
Puglisi, G
Salatino, M
Simon, S
Teply, G
Thornton, R
Vavagiakis, E
Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)
Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris
PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)
Source :
Proc.SPIE Int.Soc.Opt.Eng., SPIE Astronomical Telescopes + Instrumentation 2018, SPIE Astronomical Telescopes + Instrumentation 2018, Jun 2018, Austin, United States. pp.1070827, ⟨10.1117/12.2312679⟩
Publication Year :
2018
Publisher :
HAL CCSD, 2018.

Abstract

International audience; The Simons Observatory (SO) will provide precision polarimetry of the cosmic microwave background (CMB) using a series of telescopes which will cover angular scales from arc-minutes to tens of degrees, contain over 60,000 detectors, and observe in frequency bands between 27 GHz and 270 GHz. SO will consist of a six-meter-aperture telescope initially coupled to roughly 35,000 detectors along with an array of half-meter aperture refractive cameras, coupled to an additional 30,000+ detectors. The large aperture telescope receiver (LATR) is coupled to the SO six-meter crossed Dragone telescope and will be 2.4 m in diameter, weigh over 3 metric tons, and have five cryogenic stages (80 K, 40 K, 4 K, 1 K and 100 mK). The LATR is coupled to the telescope via 13 independent optics tubes containing cryogenic optical elements and detectors. The cryostat will be cooled by two Cryomech PT90 (80 K) and three Cryomech PT420 (40 K and 4 K) pulse tube cryocoolers, with cooling of the 1 K and 100 mK stages by a commercial dilution refrigerator system. The secondo component, the small aperture telescope (SAT), is a single optics tube refractive cameras of 42 cm diameter. Cooling of the SAT stages will be provided by two Cryomech PT420, one of which is dedicated to the dilution refrigeration system which will cool the focal plane to 100 mK. SO will deploy a total of three SATs. In order to estimate the cool down time of the camera systems given their size and complexity, a finite difference code based on an implicit solver has been written to simulate the transient thermal behavior of both cryostats. The result from the simulations presented here predict a 35 day cool down for the LATR. The simulations suggest additional heat switches between stages would be effective in distribution cool down power and reducing the time it takes for the LATR to reach its base temperatures. The SAT is predicted to cool down in one week, which meets the SO design goals.

Details

Language :
English
Database :
OpenAIRE
Journal :
Proc.SPIE Int.Soc.Opt.Eng., SPIE Astronomical Telescopes + Instrumentation 2018, SPIE Astronomical Telescopes + Instrumentation 2018, Jun 2018, Austin, United States. pp.1070827, ⟨10.1117/12.2312679⟩
Accession number :
edsair.doi.dedup.....b42be114af4737e40ca4b19e2d0343cc