Thermal Modeling of the ATHENA X-IFU Filters

被引:0
|
作者
Sciortino, Luisa [1 ]
Lo Cicero, Ugo [1 ,2 ]
Bonura, Salvatore Ferruggia [1 ,2 ]
D'Anca, Fabio [3 ]
Buttacavoli, Antonino [2 ]
Puccio, Elena [2 ]
Barbera, Marco [1 ,2 ]
机构
[1] Univ Palermo UNIPA, Dipartimento Fis & Chim DiFC, Palermo, Italy
[2] Ist Nazl Astrofis, Osservatorio Astron Palermo GS Vaiana, Palermo, Italy
[3] CNR, Ist BioFis UOS Palermo, Palermo, Italy
来源
SPACE TELESCOPES AND INSTRUMENTATION 2018: ULTRAVIOLET TO GAMMA RAY | 2018年 / 10699卷
基金
欧盟地平线“2020”;
关键词
ATHENA; X-IFU; thermal simulation; thermal filters; EMISSIVITY;
D O I
10.1117/12.2314453
中图分类号
P1 [天文学];
学科分类号
0704 ;
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 high-purity 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.
引用
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页数:10
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