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The boronated scintillator detector of the ISS-CREAM experiment

机译:ISS-CREAM实验的硼化闪烁探测器

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The Cosmic Ray Energetics And Mass for the International Space Station (ISS-CREAM) instrument is a next-generation experiment for the direct detection and study of cosmic-ray nuclei and electrons. With a long exposure in low Earth orbit, the experiment will determine the particle fluxes and spectral details of cosmic-ray nuclei from hydrogen to iron, over an energy range of about 10(12) eV to >10(15) eV, and of cosmic-ray electrons over an energy range of about 5 x10(10) eV to > 10(13) eV. The instrument was deployed to the ISS in August 2017 on the SpaceX CRS-12 mission. We review the design, implementation and performance of one of the ISS-CREAM detector systems: a boron loaded scintillation detector used in discriminating electron-induced events from the much more abundant cosmic-ray nuclei.
机译:国际空间站的宇宙射线能量和质量(ISS-CREAM)仪器是用于直接检测和研究宇宙射线核和电子的下一代实验。在低地球轨道上长时间暴露的情况下,该实验将确定在大约10(12)eV至> 10(15)eV的能量范围内,从氢到铁的宇宙射线核的粒子通量和光谱细节。宇宙射线电子在大约5 x10(10)eV到> 10(13)eV的能量范围内。该仪器于2017年8月在SpaceX CRS-12任务中部署到ISS。我们回顾了ISS-CREAM检测器系统之一的设计,实现和性能:硼加载闪烁检测器,用于将电子诱发的事件与更丰富的宇宙射线核区分开。

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