Caliste-SO X-ray micro-camera for the STIX instrument on-board Solar Orbiter space mission

被引:22
|
作者
Meuris, A. [1 ]
Hurford, G. [2 ]
Bednarzik, M. [3 ]
Limousin, O. [1 ]
Gevin, O. [1 ]
Le Mer, I. [1 ]
Martignac, J. [1 ]
Horeau, B. [1 ]
Grimm, O. [4 ]
Resanovic, R. [3 ]
Krucker, S. [4 ]
Orleanski, P. [5 ]
机构
[1] CEA DSM Irfu, F-91191 Gif Sur Yvette, France
[2] Univ Appl Sci NW Switzerland FHNW, Sch Engn, Inst Technol 4D, CH-5210 Windisch, Switzerland
[3] PSI, Lab Micro & Nanotechnol, CH-5232 Villigen, Switzerland
[4] ETH, Inst Particle Phys, CH-8093 Zurich, Switzerland
[5] Polish Acad Sci, Space Res Ctr, PL-00716 Warsaw, Poland
关键词
CdTe; X-ray spectroscopy; ASIC; Solar flare; Solar Orbiter;
D O I
10.1016/j.nima.2011.11.016
中图分类号
TH7 [仪器、仪表];
学科分类号
0804 ; 080401 ; 081102 ;
摘要
The Spectrometer Telescope for Imaging X-rays (STIX) is an instrument on the Solar-Orbiter space mission that performs hard X-ray imaging spectroscopy of solar flares. It consists of 32 collimators with grids and 32 spectrometer units called Caliste-SO for indirect Fourier-transform imaging. Each Caliste-SO device integrates a 1 cm(2) CdTe pixel sensor with a low-noise low-power analog front-end ASIC and circuits for supply regulation and filtering. The ASIC named IDeF-X HD is designed by CEA/Irfu (France) whereas CdTe-based semiconductor detectors are provided by the Laboratory for Micro- and Nanotechnology, Paul Scherrer Institute (Switzerland). The design of the hybrid, based on 3D Plus technology (France), is well suited for STIX spectroscopic requirements (1 keV FWHM at 6 key, 4 keV low-level threshold) and system constraints (4W power and 5 kg mass). The performance of the sub-assemblies and the design of the first Caliste-SO prototype are presented. (C) 2011 Elsevier B.V. All rights reserved.
引用
收藏
页码:288 / 292
页数:5
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