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“SODART” Telescope Silicon Detector Cooling System (Thermal Test Results of the Scale-Down Model)
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English
Abstract
The onboard “SODART” telescope silicon detector cooling system of the “Spectrum-X-Gamma” observatory, which is designed for the space objects X-ray radiation study, is described. The scale-down model of the passive cooling system description and thermal vacuum test results of this model are given. In the real cooling system the minimal detector temperature at 300 mW heat release is expected about 107 K.
Authors
- Aleksander Abrosimov - The Div. of the Scientific Research Institute of Electromechanics
- Oleg Baryshev - The Div. of the Scientific Research Institute of Electromechanics
- Vitalij Horonenko - The Div. of the Scientific Research Institute of Electromechanics
- Michail Kosorotov - The Div. of the Scientific Research Institute of Electromechanics
- Anatolij Lobanov - The Div. of the Scientific Research Institute of Electromechanics
- Aleksander Paramonov - The Div. of the Scientific Research Institute of Electromechanics
- Michail Parfentiev - The Div. of the Scientific Research Institute of Electromechanics
Citation
Abrosimov, A., Baryshev, O., Horonenko, V., Kosorotov, M. et al., "“SODART” Telescope Silicon Detector Cooling System (Thermal Test Results of the Scale-Down Model)," SAE Technical Paper 921365, 1992, https://doi.org/10.4271/921365.Also In
References
- Sipila H. Huttunen P. Kamarainen V.J. “Silicon X-Ray Array Detector on Spectrum-X-Gamma Satellite” EUV, X-Ray and Gamma-Ray Instrumentation for Astronomy II San Diego 21-26 July 1991