Abstract We study the properties of flare accelerated particles using gamma ray observations. We derive ion and electron energy spectra, electron to proton ratios, and numbers of interacting particles. We investigate the effects of the abundance variations implied by the gamma ray data on these parameters. We compare the results with interplanetary observations of solar flare particles.
Acceleration in solar flares: Interacting particles versus interplanetary particles
Advances in Space Research ; 13 , 9 ; 275-284
1993-01-01
10 pages
Article (Journal)
Electronic Resource
English
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