斯皮卡
红外线的
空格(标点符号)
航空航天工程
物理
航空学
计算机科学
工程类
天文
操作系统
作者
Keisuke Shinozaki,Yoichi Sato,Chihiro Tokoku,Masaru Saijo,Hiroyuki Ogawa,Takao Nakagawa,Kenichiro Sawada,Hiroyuki Sugita,Tadahito Mizutani,Hideo Matsuhara,Shoji Tsunematsu,Seiji Yoshida,Kenichi Kanao,Akinobu Okabayashi,Katsuhiro Narasaki,Hiroshi Shibai
出处
期刊:Space Telescopes and Instrumentation 2020: Optical, Infrared, and Millimeter Wave
日期:2020-12-11
被引量:6
摘要
The Space Infrared Telescope for Cosmology and Astrophysics (SPICA) mission is to be launched into orbit around the second Lagrangian point (L2) in the Sun-Earth system. Taking advantage of the thermal environment in L2, a 2.5m-class large IR telescope is cooled below 8K in combination with effective radiant cooling and a mechanical cooling system. SPICA adopts a cryogen-free system to prevent the mission operation lifetime being limited by the amount of cryogen as a refrigerant. Currently, the mechanical cooler system with the feasible solution giving a proper margin is proposed. As a baseline design, 4K / 1K-class Joule-Thomson coolers are used to cool the telescope and thermal interface for Focal Plane Instruments (FPIs). Additionally, two sets of double stage stirling coolers (2STs) are used to cool the telescope shield. In this design, nominal operation of FPIs can be kept when one mechanical cooler is in failure. In this paper, current baseline configuration of the mechanical cooler system and current status of mechanical coolers developments which need to satisfy the specific requirements of SPICA cryogenic system are presented.
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