A model of solar energetic particles for use in calculating LET spectra developed from ONR-604 data.
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.
Chen
J
J
Department of Physics and Astronomy, Louisiana State University, Baton Rouge 70803, USA.
Chenette
D
D
Guzik
T G
TG
Garcia-Munoz
M
M
Pyle
K R
KR
Sang
Y
Y
Wefel
J P
JP
D006371:Helium; D018499:Linear Energy Transfer; D008962:Models, Theoretical; D011522:Protons; D019445:Solar Activity; D013026:Space Flight / Q000295:instrumentation*; D018531:Spacecraft / Q000295:instrumentation*
D011522:Protons; D006371:Helium