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.

Sciortino, L., Lo Cicero, U., Ferruggia Bonura, S., D'Anca, F., Buttacavoli, A., Puccio, E., et al. (2018). Thermal modelling of the ATHENA X-IFU filters. In Proceedings of SPIE - The International Society for Optical Engineering (pp. 177). SPIE [10.1117/12.2314453].

Thermal modelling of the ATHENA X-IFU filters

Sciortino, Luisa
;
Lo Cicero, Ugo;Ferruggia Bonura, Salvatore;Buttacavoli, Antonino;Puccio, Elena;Barbera, Marco
2018-07-06

Abstract

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.
6-lug-2018
Settore FIS/05 - Astronomia E Astrofisica
978-1-5106-1952-4
Sciortino, L., Lo Cicero, U., Ferruggia Bonura, S., D'Anca, F., Buttacavoli, A., Puccio, E., et al. (2018). Thermal modelling of the ATHENA X-IFU filters. In Proceedings of SPIE - The International Society for Optical Engineering (pp. 177). SPIE [10.1117/12.2314453].
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/10447/302540
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