A model of Solar Energetic Particles (SEP) has been developed and is applied to solar flares during the 1990/1991 Combined Release and Radiation Effects Satellite (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 influence, 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.
A model of solar energtic particles for use in calculating LET spectra developed from ONR-604 data
1994-10-01
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Englisch
A Model of Solar Energetic Particles for use in Calculating LET Spectra developed from ONR-604 Data
Online Contents | 1994
|The energy spectra of solar energetic particles
NTRS | 1984
|The energy spectra of solar energetic particles
Elsevier | 1984
|Calculating Electronic Spectra Of Diatomic Molecules
NTRS | 1991
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