空间环境中使用的锗伽马射线光谱仪中中子和质子感应本底的测量

A. Entwistle, C. Dyer, J. Quenby, A. Evans, M. Joshi
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引用次数: 4

摘要

空间环境下用于天体物理和遥感测量的锗光谱仪的粒子感应本底对仪器的最终灵敏度有重要的限制。为了帮助未来的实验设计和解释,将典型的传感器暴露在已知的慢中子和快中子以及高能质子的影响下,以预测线和连续介质背景成分。快中子弹性散射是重型航天器内无屏蔽探测器100kev以下背景辐射的主要来源。在更高的能量下,从中子非弹性散射和中子和质子诱导的放射性中可以确定类似的贡献。在600 MeV的1.2*1010个质子辐照后,n型高纯锗探测器的分辨率展宽了1.8倍。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Measurement of neutron and proton-induced background in germanium gamma-ray spectrometers for use in a space environment
Particle-induced background in germanium spectrometers used for astrophysical and remote sensing measurement in a space environment provides an important limitation to the ultimate instrument sensitivity. To aid future experimental design and interpretation, laboratory exposure of typical sensors to known fluences of slow and fast neutrons and energetic protons is carried out to predict the line and continuum background components. Fast neutron elastic scatter is found to be the chief source of background below 100 keV for an unshielded detector inside a heavy spacecraft. At higher energies, comparable contributions are identified from neutron inelastic scattering and neutron- and proton-induced radioactivity. Radiation damage to an n-type high purity Ge detector caused broadening in resolution by a factor of 1.8 after subjection to 1.2*1010 protons of 600 MeV.
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