Models describing solar cosmic ray events

被引：11
|
作者：
Nymmik, RA
机构：
[1] Institute of Nuclear Physics, Moscow University
来源：
RADIATION MEASUREMENTS | 1996年 / 26卷 / 03期
关键词：
D O I：
10.1016/1350-4487(96)00052-2
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：
A set of experiment data on the energy spectra of peak (maximum) flux and fluence values in solar cosmic ray (SCR) events is analysed. It is shown that the proton energy spectra, averaged over events with identical fluences can be described by power law functions of the particle rigidity. The phenomenon of monotonic increase in the averaged spectral index with increase of SCR fluence is described. A classification of SCR events by fluence magnitude is suggested. Copyright (C) 1996 Elsevier Science Ltd.
引用
收藏
页码：417 / 420
页数：4
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