NASA Langley Research Center, Hampton, Virginia 23681, USA.
NASA Johnson Space Center, Houston, Texas 77058, USA.
Life Sci Space Res (Amst). 2018 Aug;18:64-71. doi: 10.1016/j.lssr.2018.05.003. Epub 2018 Jun 28.
This paper is the third in a series of comparisons of American (NASA) and Russian (ROSCOSMOS) space radiation calculations. The present work focuses on calculation of fluxes of galactic cosmic rays (GCR), which are a constant source of radiation that constitutes one of the major hazards during deep space exploration missions for both astronauts/cosmonauts and hardware. In this work, commonly used GCR models are compared with recently published measurements of cosmic ray Hydrogen, Helium, and the Boron-to-Carbon ratio from the Alpha Magnetic Spectrometer (AMS). All of the models were developed and calibrated prior to the publication of the AMS data; therefore this an opportunity to validate the models against an independent data set.
本文是对美国（NASA）和俄罗斯（ROSCOSMOS）空间辐射计算的一系列比较的第三部分。本工作重点是计算银河宇宙射线（GCR）通量，这是辐射的恒定源，对于宇航员/航天员和硬件来说，这是深空探索任务中的主要危害之一。在这项工作中，常用的 GCR 模型与最近公布的阿尔法磁谱仪（AMS）测量的宇宙射线氢、氦和硼-碳比进行了比较。所有模型都是在 AMS 数据公布之前开发和校准的；因此，这是一个利用独立数据集验证模型的机会。
