Abstract

Results are presented from modeling two different conditions for parameterizing the geometry of Earth’s atmosphere and the spectrum of primary cosmic rays. In the first, the input data correspond to solar cosmic rays and calculations are made for all geographic latitudes and longitudes. The second is devoted to estimating the contribution from the nuclei of galactic cosmic rays while considering only a local region of the atmosphere.

中文翻译：

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使用地球大气的整体模型计算GLE事件期间的电离速率，并从Z> 2的银河宇宙射线粒子估计该过程的贡献

摘要

通过对两个不同的条件进行建模得出了结果，这些条件用于参数化地球大气的几何形状和主要宇宙射线的光谱。首先，输入数据对应于太阳宇宙射线，并针对所有地理纬度和经度进行计算。第二个致力于估算银河系宇宙射线核的贡献，同时仅考虑大气的局部区域。