模拟地球上空间辐射环境的要素

J. Miller, S. Guetersloh, L. Heilbronn, C. Zeitlin
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引用次数: 0

摘要

空间辐射研究正在为解决长期太空任务中人类受到的辐射问题奠定基础。这项研究在很大程度上依赖于对地基质子和重离子加速器的研究。对这些实验数据的解释敏感地依赖于这些重电离粒子如何将能量沉积在束线材料和用于测量辐射的仪器中的细节。我们报告了几个加速器上离子束测量的结果,包括Bevalac(劳伦斯伯克利国家实验室),AGS(布鲁克海文国家实验室),HIMAC(日本千叶国家放射科学研究所)和布鲁克海文的新NASA空间辐射实验室(NSRL)。这些测量说明了重带电粒子相互作用的一些关键特征。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Simulating elements of the space radiation environment on Earth
Space radiation research is laying the groundwork for addressing the problem of radiation exposure to humans on extended space missions. This research relies heavily on investigations at ground-based proton and heavy ion accelerators. The interpretation of the data from these experiments depends sensitively on the details of how these heavily ionizing particles deposit their energy in beamline materials and in the instruments used to measure the radiation. We report on the results of measurements with ion beams at several accelerators, including the Bevalac (Lawrence Berkeley National Laboratory), AGS (Brookhaven National Laboratory), HIMAC (National Institute of Radiological Sciences, Chiba, Japan), and the new NASA Space Radiation Laboratory (NSRL) at Brookhaven. These measurements illustrate some of the critical features of heavy charged particle interactions.
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