A model of solar energetic particles for use in calculating let spectra developed from ONR-604 data

Document Type

Article

Publication Date

1-1-1994

Abstract

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. © 1994.

Publication Source (Journal or Book title)

Advances in Space Research

First Page

675

Last Page

680

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