地-火-地航线中太阳高能粒子通量对太阳活动周期的依赖性。

The dependence of solar energetic particle fluxes in the Earth-Mars-Earth route on solar activity period.

作者信息

Kuznetsov N V, Nymmik R A

机构信息

Institute of Nuclear Physics, Moscow State University, Moscow, Russia.

出版信息

Adv Space Res. 2002;30(4):981-4. doi: 10.1016/s0273-1177(02)00165-5.

DOI:10.1016/s0273-1177(02)00165-5

PMID:12539773

Abstract

This report presents the results of analyzing the relative importance of particle fluxes of different origin in the Earth-Mars-Earth route during different solar activity periods. The analysis has been made in terms of the galactic cosmic ray and solar energetic particle flux models developed at Moscow State University. The results demonstrate the extreme importance of the high-energy solar particle fluxes in interplanetary space even during the years of "quiet" Sun.

摘要

本报告展示了在不同太阳活动时期，分析地球 - 火星 - 地球路线上不同来源粒子通量相对重要性的结果。该分析是依据莫斯科国立大学开发的银河宇宙射线和太阳高能粒子通量模型进行的。结果表明，即使在太阳“平静”的年份，高能太阳粒子通量在行星际空间中也极为重要。