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作 者:YongQiang Shi LianSheng Li JianWu Chen FuChang Zuo XiaoPing Zhang ZhiWu Mei Li Wang Keke Zhang
机构地区:[1]Beijing Institute of Control Engineering,Beijing 100190,China [2]State Key Laboratory of Lunar and Planetary Sciences,Macao University of Science and Technology,Macao 999078,China
出 处:《Earth and Planetary Physics》2023年第1期125-130,共6页地球与行星物理(英文版)
基 金:the China National Space Administration(CNSA);the Macao University of Science and Technology Foundation for their support of this paper。
摘 要:The solar X-ray detector(SXD)onboard the Macao Science Satellite-1B was designed to monitor solar flare bursts and to study the solar activity in the 25th solar cycle.The SXD includes two parts:a soft X-ray detection unit and a hard X-ray detection unit.Both the soft X-ray detection unit and the hard X-ray detection unit include two collimators,two X-ray detectors(a silicon drift detector and a cadmium-zinc-telluride detector),and a processing circuit.Compared with similar instruments,the energy range of the SXD is wider(1–600 ke V)and the energy resolution is better(150 e V at 5.9 ke V,12%at 59.5 ke V,and 3%at 662 keV).
关 键 词:Macao Science Satellite-1B(MSS-1B) solar X-ray detector solar X-ray SPECTROMETER
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