SCR steady state distribution function and scattering properties of the interplanetary medium

被引：3
|
作者：
Fedorov, Yu.
Stehlik, M.
机构：
[1] Natl Acad Sci Ukraine, Main Astron Observ, UA-03680 Kiev, Ukraine
[2] Slovak Acad Sci, Inst Expt Phys, Kosice 04353, Slovakia
来源：
ASTROPHYSICS AND SPACE SCIENCE | 2006年 / 302卷 / 1-4期
关键词：
kinetic equation; solar cosmic rays; ground level event;
D O I：
10.1007/s10509-005-9010-y
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The propagation of energetic particles in the interplanetary space is considered on the basis of kinetic equation describing the scattering of charged particles by magnetic irregularities and the particle focusing by regular magnetic field. Our analysis confirms that angular distribution of solar cosmic rays contains a valuable information about properties of the particle scattering in the interplanetary magnetic field. Steady state solutions of the kinetic equation are applied to the analysis of solar proton events.
引用
收藏
页码：99 / 107
页数：9
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