Sato Tatsuhiko, Nagamatsu Aiko, Ueno Haruka, Kataoka Ryuho, Miyake Shoko, Takeda Kazuo, Niita Koji
Japan Atomic Energy Agency, Shirakata 2-4, Tokai, Ibaraki, Japan.
Japan Aerospace Exploration Agency, Sengen 2-1-1, Tsukuba, Ibaraki, Japan.
Radiat Prot Dosimetry. 2018 Aug 1;180(1-4):146-149. doi: 10.1093/rpd/ncx192.
Estimation of cosmic-ray doses is of great importance not only in aircrew and astronaut dosimetry but also in evaluation of background radiation exposure to public. We therefore calculated the cosmic-ray doses on Earth, Moon and Mars as well as inside spacecraft, using Particle and Heavy Ion Transport code System PHITS. The same cosmic-ray models and dose conversion coefficients were employed in the calculation to properly compare between the simulation results for different environments. It is quantitatively confirmed that the thickness of physical shielding including the atmosphere and soil of the planets is the most important parameter to determine the cosmic-ray doses and their dominant contributors. The comparison also suggests that higher solar activity significantly reduces the astronaut doses particularly for the interplanetary missions. The information obtained from this study is useful in the designs of the future space missions as well as accelerator-based experiments dedicated to cosmic-ray research.
估算宇宙射线剂量不仅在机组人员和宇航员剂量测定中非常重要,而且在评估公众的背景辐射暴露方面也很重要。因此,我们使用粒子与重离子传输代码系统PHITS计算了地球、月球和火星以及航天器内部的宇宙射线剂量。在计算中采用了相同的宇宙射线模型和剂量转换系数,以便对不同环境的模拟结果进行恰当比较。定量结果证实,包括行星大气和土壤在内的物理屏蔽厚度是决定宇宙射线剂量及其主要贡献因素的最重要参数。比较结果还表明,太阳活动增强会显著降低宇航员所受剂量,特别是对于行星际任务而言。从本研究中获得的信息对未来太空任务的设计以及致力于宇宙射线研究的基于加速器的实验很有用。