COMPOSITION OF ENERGETIC PARTICLES FROM SOLAR-FLARES

被引:25
作者
GARRARD, TL
STONE, EC
机构
[1] 220-47 Downs Laboratory, California Institute of Technology, Pasadena
来源
LIFE SCIENCES AND SPACE RESEARCH XXV(2): RADIATION BIOLOGY | 1994年 / 14卷 / 10期
关键词
D O I
10.1016/0273-1177(94)90514-2
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
We present a model for composition of heavy ions in the solar energetic particles (SEP). The SEP composition in a typical large solar particle event reflects the composition of the Sun, with adjustments due to fractionation effects which depend on the first ionization potential (FIP) of the ion and on the ratio of ionic charge to mass (Q/M). Flare-to-flare variations in composition are represented by parameters describing these fractionation effects and the distributions of these parameters are presented.
引用
收藏
页码:589 / 598
页数:10
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