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ASTROPHYSICS AND COSMOLOGY RELATED TO PARTICLES AND NUCLEI

Thermal analysis and expected performance of the low energy instrument on board the HXMT satellite

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2010 Chinese Physical Society and the Institute of High Energy Physics of the Chinese Academy of Sciences and the Institute of Modern Physics of the Chinese Academy of Sciences and IOP Publishing Ltd
, , Citation Wang Yu-Sa et al 2010 Chinese Phys. C 34 1812 DOI 10.1088/1674-1137/34/12/005

1674-1137/34/12/1812

Abstract

The Low Energy X-ray Instrument (LE) of the Hard X-ray Modulation Telescope (HXMT) uses the Swept Charge Device (SCD) to detect the X-rays in 1−15 keV. The performance of SCD is vulnerable to temperature. We analyzed the thermal condition of LE at different satellite working attitudes with the Finite Element Method (FEM). It is shown that the angle between the sunlight and the normal line of the barrier should be less than 26°, to keep the SCD detectors working in the required temperature range, i.e. −40 °C to −80 °C. We find that the performance of LE is very stable in this temperature range, with a typical energy resolution of 160 eV at 5.9 keV.

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10.1088/1674-1137/34/12/005