論文

査読有り
2010年9月

Cooling system for the soft X-ray spectrometer onboard Astro-H

CRYOGENICS
  • Ryuichi Fujimoto
  • Kazuhisa Mitsuda
  • Noriko Yamasaki
  • Yoh Takei
  • Masahiro Tsujimoto
  • Hiroyuki Sugita
  • Yoichi Sato
  • Keisuke Shinozaki
  • Takaya Ohashi
  • Yoshitaka Ishisaki
  • Yuichiro Ezoe
  • Masahide Murakami
  • Shunji Kitamoto
  • Hiroshi Murakami
  • Toru Tamagawa
  • Madoka Kawaharada
  • Hiroya Yamaguchi
  • Kosuke Sato
  • Kenichi Kanao
  • Seiji Yoshida
  • Mike DiPirro
  • Peter Shirron
  • Gary Sneiderman
  • Richard L. Kelley
  • F. Scott Porter
  • Caroline A. Kilbourne
  • John Crow
  • Andrea Mattern
  • Ali Kashani
  • Dan McCammon
  • Jan-Willem den Herder
  • 全て表示

50
9
開始ページ
488
終了ページ
493
記述言語
英語
掲載種別
研究論文(学術雑誌)
DOI
10.1016/j.cryogenics.2010.02.004
出版者・発行元
ELSEVIER SCI LTD

The Soft X-ray Spectrometer (SXS) is a cryogenic high resolution X-ray spectrometer onboard the X-ray astronomy satellite Astro-H which will be launched in 2014. The detector array is cooled down to 50 mK using an adiabatic demagnetization refrigerator (ADR). The cooling chain from the room temperature to the ADR heat-sink is composed of superfluid liquid He, a Joule-Thomson cryocooler, and double-stage Stirling cryocoolers. It is designed to keep 301 of liquid He for more than 5 years in the normal case, and longer than 3 years even if one of the cryocoolers fails. Cryogen-free operation is also possible in the normal case. It is fully redundant from the room temperature to the ADR heat-sink. (c) 2010 Elsevier Ltd. All rights reserved.

リンク情報
DOI
https://doi.org/10.1016/j.cryogenics.2010.02.004
Web of Science
https://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=JSTA_CEL&SrcApp=J_Gate_JST&DestLinkType=FullRecord&KeyUT=WOS:000281944400002&DestApp=WOS_CPL
ID情報
  • DOI : 10.1016/j.cryogenics.2010.02.004
  • ISSN : 0011-2275
  • eISSN : 1879-2235
  • Web of Science ID : WOS:000281944400002

エクスポート
BibTeX RIS