A MODEL OF SOLAR ENERGETIC PARTICLES FOR USE IN CALCULATING LET SPECTRA DEVELOPED FROM ONR-604 DATA

被引：4

作者：

CHEN, J

CHENETTE, D

GUZIK, TG

GARCIAMUNOZ, M

PYLE, KR

SANG, Y

WEFEL, JP

机构：

[1] LOCKHEED PALO ALTO RES LABS,PALO ALTO,CA 94304

[2] UNIV CHICAGO,ENRICO FERMI INST,CHICAGO,IL 60637

来源：

LIFE SCIENCES AND SPACE RESEARCH XXV(2): RADIATION BIOLOGY | 1994年 / 14卷 / 10期

基金：

美国国家航空航天局;

关键词：

D O I：

10.1016/0273-1177(94)90525-8

中图分类号：

V [航空、航天];

学科分类号：

08 ; 0825 ;

摘要：

A model of solar energetic particles (SEP) has been developed and is applied to solar flares during the 1990/1991 CRRES mission using data measured by the University of Chicago instrument, ONR-604. The model includes the time-dependent behavior, heavy-ion content, energy spectrum and fluence, and can accurately represent the observed SEP events in the energy range between 40 to 500 MeV/nucleon. Results are presented for the March and June, 1991 flare periods.

引用

页码：675 / 680

页数：6