AXAF detector backgrounds produced by cosmic ray protons

机译：由宇宙射线质子产生的Axaf探测器背景

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X-ray detector backgrounds expected for the planned AXAF mission due to the galactic cosmic ray (GCR) proton environment have been determined by detailed Monte Carlo simulations. The predicted GCR-induced prompt and activation backgrounds are about 0.03 and 0.02 counts/cm/sup 2/-s, respectively which are small compared to signal strengths expected for planned AXAF observation scenarios.

机译：由于Galactic Cosmic Ray（GCR）质子环境所预期的X射线探测器背景预期的Proton环境已经通过详细的蒙特卡罗模拟确定。预测的GCR诱导的提示和激活背景分别为0.03和0.02计数/ cm / sup 2 / -s，与计划的AXAF观察场景的预期信号强度相比，小。

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《Conference on the High Energy Radiation Background in Space》|1998年||共6页
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Armstrong T.W.; Colborn B.L.; Institute of Electric and Electronic Engineer;
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中图分类自动化技术、计算机技术;
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4. AXAF detector backgrounds produced by cosmic ray protons [C] . Armstrong, T.W., Colborn, . 1998

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AXAF detector backgrounds produced by cosmic ray protons

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