Author/Authors :
Meuris، نويسنده , , A. and Hurford، نويسنده , , G. and Bednarzik، نويسنده , , M. and Limousin، نويسنده , , O. and Gevin، نويسنده , , O. and Le Mer، نويسنده , , I. and Martignac، نويسنده , , J. and Horeau، نويسنده , , B. and Grimm، نويسنده , , O. and Resanovic، نويسنده , , R. and Krucker، نويسنده , , S. and Orlea?ski، نويسنده , , P.، نويسنده ,
Abstract :
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 cm2 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 keV, 4 keV low-level threshold) and system constraints (4 W power and 5 kg mass). The performance of the sub-assemblies and the design of the first Caliste-SO prototype are presented.
Keywords :
CdTe , X-ray spectroscopy , ASIC , Solar flare , Solar Orbiter