Thermal analyses for initial operations of the soft x-ray spectrometer onboard the Hitomi satellite

被引:5
作者
Noda, Hirofumi [1 ,2 ]
Mitsuda, Kazuhisa [3 ]
Okamoto, Atsushi [4 ]
Ezoe, Yuichiro [5 ]
Ishikawa, Kumi [3 ]
Fujimoto, Ryuichi [6 ]
Yamasaki, Noriko [3 ]
Takei, Yoh [3 ]
Ohashi, Takaya [5 ]
Ishisaki, Yoshitaka [5 ]
Mitsuishi, Ikuyuki [7 ]
Yoshida, Seiji [8 ]
DiPirro, Michel [9 ]
Shirron, Peter [9 ]
机构
[1] Tohoku Univ, Frontier Res Inst Interdisciplinary Sci, Sendai, Miyagi, Japan
[2] Tohoku Univ, Astron Inst, Sendai, Miyagi, Japan
[3] Japan Aerosp Explorat Agcy, Inst Space & Astronaut Sci, Sagamihara, Kanagawa, Japan
[4] Japan Aerosp Explorat Agcy, Res & Dev Directorate, Tsukuba, Ibaraki, Japan
[5] Tokyo Metropolitan Univ, Dept Phys, Hachioji, Tokyo, Japan
[6] Kanazawa Univ, Fac Math & Phys, Kanazawa, Ishikawa, Japan
[7] Nagoya Univ, Dept Phys, Nagoya, Aichi, Japan
[8] Sumitomo Heavy Ind Ltd, Niihama, Ehime, Japan
[9] NASA, Goddard Space Flight Ctr, Greenbelt, MD USA
基金
日本学术振兴会;
关键词
Hitomi (ASTRO-H); soft x-ray spectrometer; x-ray microcalorimeter; cryogenics; thermal mathematical model; thermal simulation; FLOW SUPPRESSION SYSTEM; PLUG PHASE SEPARATOR; POROUS PLUG; ORBIT OPERATION; HELIUM DEWAR; PERFORMANCE;
D O I
10.1117/1.JATIS.4.1.011202
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
The soft x-ray spectrometer (SXS) onboard the Hitomi satellite achieved a high-energy resolution of similar to 4.9 eV at 6 keV with an x- ray microcalorimeter array cooled to 50 mK. The cooling system utilizes liquid helium, confined in zero gravity by means of a porous plug (PP) phase separator. For the PP to function, the helium temperature must be kept lower than the. point of 2.17 K in orbit. To determine the maximum allowable helium temperature at launch, taking into account the uncertainties in both the final ground operations and initial operation in orbit, we constructed a thermal mathematical model of the SXS dewar and PP vent and carried out time-series thermal simulations. Based on the results, the maximum allowable helium temperature at launch was set at 1.7 K. We also conducted a transient thermal calculation using the actual temperatures at launch as initial conditions to determine flow and cooling rates in orbit. From this, the equilibrium helium mass flow rate was estimated to be similar to 34 to 42 mu g/s, and the lifetime of the helium mode was predicted to be similar to 3.9 to 4.7 years. This paper describes the thermal model and presents simulation results and comparisons with temperatures measured in the orbit. (C) The Authors. Published by SPIE under a Creative Commons Attribution 3.0 Unported License. Distribution or reproduction of this work in whole or in part requires full attribution of the original publication, including its DOI.
引用
收藏
页数:7
相关论文
共 50 条
  • [21] Porous plug and superfluid helium film flow suppressor for the soft X-ray spectrometer onboard Astro-H
    Ishikawa, Kumi
    Ezoe, Yuichiro
    Yamaguchi, Hiroya
    Mitsuishi, Ikuyuki
    Yoshitake, Hiroshi
    Mitsuda, Kazuhisa
    Fujimoto, Ryuichi
    Ohashi, Takaya
    Murakami, Masahide
    Kanao, Ken-ichi
    Yoshida, Seiji
    Tsunematsu, Shoji
    DiPirro, Michael
    Shirron, Peter
    CRYOGENICS, 2010, 50 (09) : 507 - 511
  • [22] Soft X-ray Imager (SXI) Onboard ASTRO-H
    Tsunemi, Hiroshi
    Hayashida, Kiyoshi
    Tsuru, Takeshi Go
    Dotani, Tadayasu
    Hiraga, Junko S.
    Anabuki, Naohisa
    Bamba, Aya
    Hatsukade, Isamu
    Kohmura, Takayoshi
    Mori, Koji
    Murakami, Hiroshi
    Nakajima, Hiroshi
    Ozaki, Masanobu
    Uchida, Hiroyuki
    Yamauchi, Makoto
    SPACE TELESCOPES AND INSTRUMENTATION 2010: ULTRAVIOLET TO GAMMA RAY, 2010, 7732
  • [23] Development of basic theory and application of cryogenic X-ray spectrometer in light sources and X-ray satellite
    Zhang Shuo
    Cui Wei
    Jin Hai
    Chen Liu-Biao
    Wang Jun-Jie
    Wu Wen-Tao
    Wu Bing-Jun
    Xia Jing-Kai
    Song Yan-Ru
    Yang Jin-Ping
    Weng Tsu-Chien
    Liu Zhi
    ACTA PHYSICA SINICA, 2021, 70 (18)
  • [24] Development of the Onboard Digital Processing System for the Soft X-ray Spectrometer of ASTRO-H - Performance in the Engineering Model Tests
    Seta, H.
    Tashiro, M. S.
    Ishisaki, Y.
    Tsujimoto, M.
    Shimoda, Y.
    Takeda, S.
    Yamaguchi, S.
    Mitsuda, K.
    Fujimoto, R.
    Takei, Y.
    Kelley, R. L.
    Boyce, K. R.
    Kilborne, C. A.
    Porter, F. S.
    Miko, J. J.
    Masukawa, K.
    Matsuda, K.
    SPACE TELESCOPES AND INSTRUMENTATION 2012: ULTRAVIOLET TO GAMMA RAY, 2012, 8443
  • [25] Performance verification and system integration tests of the pulse shape processor for the soft X-ray spectrometer onboard ASTRO-H
    Takeda, Sawako
    Tashiro, Makoto S.
    Ishisaki, Yoshitaka
    Tsujimoto, Masahiro
    Seta, Hiromi
    Shimoda, Yuya
    Yamaguchi, Sunao
    Uehara, Sho
    Terada, Yukikatsu
    Fujimoto, Ryuichi
    Mitsuda, Kazuhisa
    SPACE TELESCOPES AND INSTRUMENTATION 2014: ULTRAVIOLET TO GAMMA RAY, 2014, 9144
  • [26] Cryogen-free operation of the Soft X-ray Spectrometer instrument
    Sneiderman, Gary A.
    Shirron, Peter J.
    Fujimoto, Ryuichi
    Bialas, Thomas G.
    Boyce, Kevin R.
    Chiao, Meng P.
    DiPirro, Michael J.
    Eckart, Megan E.
    Hartz, Leslie
    Ishisaki, Yoshitaka
    Kelley, Richard L.
    Kilbourne, Caroline A.
    Masters, Candace
    McCammon, Dan
    Mitsuda, Kazuhisa
    Noda, Hirofumi
    Porter, Frederick S.
    Szymkowiak, Andrew E.
    Takei, Yoh
    Tsujimoto, Mashiro
    Yoshida, Seiji
    SPACE TELESCOPES AND INSTRUMENTATION 2016: ULTRAVIOLET TO GAMMA RAY, 2016, 9905
  • [27] A versatile wide energy range spectrometer for soft X-ray FELs
    Principi, Emiliano
    Svetina, Cristian
    De Angelis, Dario
    Fava, Claudio
    Mincigrucci, Riccardo
    Foglia, Laura
    Simoncig, Alberto
    Manfredda, Michele
    Mahne, Nicola
    Gobessi, Riccardo
    Scarcia, Martin
    Gessini, Alessandro
    Bencivenga, Filippo
    Capotondi, Flavio
    Zangrando, Marco
    Masciovecchio, Claudio
    NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT, 2024, 1058
  • [28] System design and implementation of the detector assembly of the Astro-H soft x-ray spectrometer
    Chiao, Meng P.
    Adams, Joseph
    Goodwin, Phillip
    Hobson, Clair W.
    Kilbourne, Caroline Anne
    McCammon, Daniel
    McGuinness, Daniel S.
    Moseley, Samuel J.
    Porter, Frederick S.
    Shuman, Sandy
    Watanabe, Tomomi
    JOURNAL OF ASTRONOMICAL TELESCOPES INSTRUMENTS AND SYSTEMS, 2018, 4 (02)
  • [29] A flat-field soft X-ray spectrometer for X-ray absorption spectroscopy measurement of warm dense matter
    Kang, Gyeongbo
    Kim, Minju
    Bae, Leejin
    Yang, Seong Hyeok
    Cho, Min Sang
    Yap, Chum Hong
    Jung, Jae Hyung
    Kang, Seung Woo
    Choi, Il Woo
    Nam, Chang Hee
    Cho, Byoung Ick
    NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT, 2019, 922 : 114 - 118
  • [30] Ground test results of the microvibration interference for the x-ray microcalorimeter onboard x-ray imaging and spectroscopy mission
    Hasebe, Takashi
    Imamura, Ryuta
    Tsujimoto, Masahiro
    Awaki, Hisamitsu
    Chiao, Meng
    Fujimoto, Ryuichi
    Hartz, Leslie S.
    Kilbourne, Caroline A.
    Sneiderman, Gary A.
    Takei, Yoh
    Yasuda, Susumu
    JOURNAL OF ASTRONOMICAL TELESCOPES INSTRUMENTS AND SYSTEMS, 2023, 9 (01) : 14003