The required lifetime for the Astro-E X-Ray Spectrometer (XRS) is 2 years, with a goal of 2.5 years. To meet this requirement, significant advances in state-of-the-art longlife cryogenic systems are required. The XRS system is a hybrid neon/helium system with a final stage of cooling provided by an
Design of the second generation XRS detector
โ Scribed by Galeazzi, M; Boyce, K.R; Brown, G.V; Chen, C; Cottam, J; Figueroa-Feliciano, E; Jacobson, M.B; Kelley, R.L; Liu, D; McCammon, D; Porter, F.S; Rocks, L.E; Stahle, C.K; Szymkowiak, A.E; Vaillancourt, J.E
- Book ID
- 103852945
- Publisher
- Elsevier Science
- Year
- 2004
- Tongue
- English
- Weight
- 194 KB
- Volume
- 520
- Category
- Article
- ISSN
- 0168-9002
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โฆ Synopsis
Microcalorimeter performance is limited by non-ideal effects that were not included in the standard theory of bolometers and microcalorimeters developed 20 years ago by Mather (Appl. Opt. 21 (1982) 1125). These include the hot-electron effect, absorber decoupling, thermometer non-ohmic behavior, and all related extra noise sources. Models that include these effects have been developed and can be used to optimize the design of microcalorimeters for best performance. The design of the array for the XRS detector on the Astro-E2 satellite was completely optimized based on the required performance and on the characteristics of the materials used. The characteristic heat capacity and thermal conductivity of all the detector components have been measured and the values have been used as input to the models to design the detector geometry for best performance. Mechanical modeling has also been carried out in parallel to ensure the mechanical integrity of the microcalorimeter. We report here the analysis involved in the optimization of the detectors, and the comparison between modeled and measured performance.
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