Add to ORKGA 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
Large solar eruptive events, including solar flares and coronal mass ejections (CMEs), can lead to s...
In some large solar energetic particle (SEP) events, the intensities of higher energy SEPs decay mor...
We present Linear Energy Transfer (LET) spectra calculated for the 1990-1991 CRRES mission using the...
Helium data measured by the University of Chicago instrument, ONR-604, are employed to determine the...
Solar Energetic Particles (SEP) events are interesting from a scientific perspective as they are the...
Recent progress in measuring the composition and energy spectra of solar energetic particles (SEPs) ...
The Sun emits energetic particles following eruptive events such as solar flares and Coronal Mass Ej...
Solar Energetic Particle (SEP) events are interesting from a scientific perspective as they are the ...
We present a model for composition of heavy ions in the solar energetic particles (SEP). The SEP com...
We develop a database of 110 gradual solar energetic particle (SEP) events, over the period 1967–200...
The Synchronous Orbit Particle Analyzer (SOPA), on board the satellite 1989-046 and others, has dete...
Solar energetic particles (SEPs) constitute an important component of the radiation environment in i...
A new catalogue of 314 solar energetic particle (SEP) events extending over a large time span from 1...
©2015. American Geophysical Union. All Rights Reserved. Solar energetic particle (SEP) events are a ...
A statistical analysis of the relationship between solar energetic particles (SEPs) and properties o...
Large solar eruptive events, including solar flares and coronal mass ejections (CMEs), can lead to s...
In some large solar energetic particle (SEP) events, the intensities of higher energy SEPs decay mor...
We present Linear Energy Transfer (LET) spectra calculated for the 1990-1991 CRRES mission using the...
Helium data measured by the University of Chicago instrument, ONR-604, are employed to determine the...
Solar Energetic Particles (SEP) events are interesting from a scientific perspective as they are the...
Recent progress in measuring the composition and energy spectra of solar energetic particles (SEPs) ...
The Sun emits energetic particles following eruptive events such as solar flares and Coronal Mass Ej...
Solar Energetic Particle (SEP) events are interesting from a scientific perspective as they are the ...
We present a model for composition of heavy ions in the solar energetic particles (SEP). The SEP com...
We develop a database of 110 gradual solar energetic particle (SEP) events, over the period 1967–200...
The Synchronous Orbit Particle Analyzer (SOPA), on board the satellite 1989-046 and others, has dete...
Solar energetic particles (SEPs) constitute an important component of the radiation environment in i...
A new catalogue of 314 solar energetic particle (SEP) events extending over a large time span from 1...
©2015. American Geophysical Union. All Rights Reserved. Solar energetic particle (SEP) events are a ...
A statistical analysis of the relationship between solar energetic particles (SEPs) and properties o...
Large solar eruptive events, including solar flares and coronal mass ejections (CMEs), can lead to s...
In some large solar energetic particle (SEP) events, the intensities of higher energy SEPs decay mor...
We present Linear Energy Transfer (LET) spectra calculated for the 1990-1991 CRRES mission using the...