Thermalization of Mesh Reinforced Ultra-Thin Al-Coated Plastic Films: A Parametric Study Applied to the Athena X-IFU Instrument
Author:
Montinaro Nicola12ORCID, Sciortino Luisa2ORCID, D’Anca Fabio2, Lo Cicero Ugo2ORCID, Bozzo Enrico3ORCID, Paltani Stéphane3ORCID, Todaro Michela2ORCID, Barbera Marco4ORCID
Affiliation:
1. Dipartimento di Ingegneria, Università Degli Studi di Palermo, Viale delle Scienze, Edificio 8, 90128 Palermo, Italy 2. Istituto Nazionale di Astrofisica (INAF), Osservatorio Astronomico di Palermo, Piazza del Parlamento 1, 90134 Palermo, Italy 3. Département D’astronomie, Faculté des Sciences, Université de Genève, Chemin d’Ecogia 16, 1290 Versoix, Switzerland 4. Dipartimento di Fisica e Chimica-Emilio Segrè, Università Degli Studi di Palermo, Via Archirafi 36, 90123 Palermo, Italy
Abstract
The X-ray Integral Field Unit (X-IFU) is one of the two focal plane detectors of Athena, a large-class high energy astrophysics space mission approved by ESA in the Cosmic Vision 2015–2025 Science Program. The X-IFU consists of a large array of transition edge sensor micro-calorimeters that operate at ~100 mK inside a sophisticated cryostat. To prevent molecular contamination and to minimize photon shot noise on the sensitive X-IFU cryogenic detector array, a set of thermal filters (THFs) operating at different temperatures are needed. Since contamination already occurs below 300 K, the outer and more exposed THF must be kept at a higher temperature. To meet the low energy effective area requirements, the THFs are to be made of a thin polyimide film (45 nm) coated in aluminum (30 nm) and supported by a metallic mesh. Due to the small thickness and the low thermal conductance of the material, the membranes are prone to developing a radial temperature gradient due to radiative coupling with the environment. Considering the fragility of the membrane and the high reflectivity in IR energy domain, temperature measurements are difficult. In this work, a parametric numerical study is performed to retrieve the radial temperature profile of the larger and outer THF of the Athena X-IFU using a Finite Element Model approach. The effects on the radial temperature profile of different design parameters and boundary conditions are considered: (i) the mesh design and material, (ii) the plating material, (iii) the addition of a thick Y-cross applied over the mesh, (iv) an active heating heat flux injected on the center and (v) a Joule heating of the mesh. The outcomes of this study have guided the choice of the baseline strategy for the heating of the Athena X-IFU THFs, fulfilling the stringent thermal specifications of the instrument.
Funder
Italian Space Agency European Union’s Horizon 2020 Program
Reference30 articles.
1. Athena: The X-ray observatory to study the hot and energetic Universe;Barcons;J. Phys. Conf. Ser.,2015 2. Nandra, K., Barret, D., Barcons, X., Fabian, A., Herder, J.W.D., Piro, L., Watson, M., Adami, C., Aird, J., and Afonso, J.M. (2013). The Hot and Energetic Universe: A White Paper presenting the science theme motivating the Athena+ mission. arXiv. 3. Bavdaz, M., Wille, E., Ayre, M., Ferreira, I., Shortt, B., Fransen, S., Millinger, M., Collon, M.J., Vacanti, G., and Barrière, N.M. (2022, January 17–23). ATHENA optics technology development. Proceedings of the SPIE Astronomical Telescopes + Instrumentation, Montréal, QC, Canada. 4. The Athena X-ray Integral Field Unit: A consolidated design for the system requirement review of the preliminary definition phase;Barret;Exp. Astron.,2023 5. Meidinger, N., Nandra, K., and Plattner, M. (2018, January 10–15). Development of the Wide Field Imager instrument for ATHENA. Proceedings of the SPIE Astronomical Telescopes + Instrumentation, Austin, TX, USA.
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