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The High-energy Burst Spectrometer for SMESE Mission
Authors:Qiang Gu  Jin Chang
Institution:1. Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008;2. Graduate School of Chinese Academy of Sciences, Beijing 100039;3. National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012
Abstract:The SMall Explorer for Solar Eruptions (SMESE) is a small satellite being developed jointly by China and France. It is planed to launch around the next solar maximum year (∼ 2011) for observing simultaneously the two most violent types of eruptive events on the sun (the coronal mass ejection (CME) and the solar flare) and investigating their relationship. As one of the 3 main payloads of the small satellite, the high energy burst spectrometer (HEBS) adopts the upto- date high-resolution LaBr3 scintillation detector to observe the high-energy solar radiation in the range 10 keV—600 MeV. Its energy resolution is better than 3.0% at 662 keV, 2-fold higher than that of current scintillation detectors, promising a breakthrough in the studies of energy release in solar flares and CMEs, particle acceleration and the relationship between solar flares and CMEs.
Keywords:Instrumentation: spectrographs  Space vehicles: instruments
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