低温恒温器
滤波器(信号处理)
发射率
探测器
材料科学
噪音(视频)
热的
光学滤波器
光学
光电子学
物理
计算机科学
工程类
电气工程
图像(数学)
人工智能
气象学
量子力学
超导电性
作者
Elena Puccio,Luisa Sciortino,Ugo Lo Cicero,Salvatore Ferruggia Bonura,Fabio D’Anca,Antonino Buttacavoli,Marco Barbera
出处
期刊:Space Telescopes and Instrumentation 2018: Ultraviolet to Gamma Ray
日期:2018-07-06
卷期号:: 177-177
被引量:3
摘要
The X-IFU instrument of the ATHENA mission requires a set of thermal filters to reduce the photon shot noise onto its cryogenic detector and to protect it from molecular contamination. A set of five filters, operating at different nominal temperatures corresponding to the cryostat shield temperatures, is currently baselined. The knowledge of the actual filter temperature profiles is crucial to have a good estimation of the radiative load on the detector. Furthermore, a few filters may need to be warmed-up to remove contaminants and it is necessary to ensure that a threshold temperature is reached throughout the filters surface. For these reasons, it is fundamental to develop a thermal modeling of the full set of filters in a representative configuration. The baseline filter is a polyimide membrane 45 nm thick coated with 30 nm of highpurity aluminum, mechanically supported by a metallic honeycomb mesh. In this paper, we describe the implemented thermal modeling and report the results obtained in different studies: (i) a trade-off analysis on how to reach a minimum target temperature throughout the outer filter, (ii) a thermal analysis when varying the emissivity of the filter surfaces, and (iii) the effect of removing one of the filters.
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