Omnidirectional and vertical fluxes of charged particles in the Earth's atmosphere during solar proton events

被引：3

作者：

Bazilevskaya, GA ^{[1
]}

Flueckiger, E ^{[1
]}

Makhmutov, VS ^{[1
]}

Mizin, SV ^{[1
]}

机构：

[1] UNIV BERN,INST PHYS,CH-3012 BERN,SWITZERLAND

来源：

RADIATION MEASUREMENTS | 1996年 / 26卷 / 03期

关键词：

D O I：

10.1016/1350-4487(96)00037-6

中图分类号：

TL [原子能技术]; O571 [原子核物理学];

学科分类号：

0827 ; 082701 ;

摘要：

The monitoring of ionizing radiation in the Earth's atmosphere provides a way to detect solar protons with E = 100-500 MeV at polar latitudes. At certain periods during solar proton events the experimental results may be understood in terms of the energy-dependent anisotropic angular distribution of solar protons at the top of the atmosphere. The calculation of proton trajectories shows that such a distribution could only be formed inside the magnetosphere. Copyright (C) 1996 Elsevier Science Ltd

引用

页码：443 / 446

页数：4