Size distributions of solar energetic particle events

Details Size distributions of solar energetic particle events Size distributions of solar energetic particle events

Aug 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991icrc....3...25c&link_type=abstract

IN: International Cosmic Ray Conference, 22nd, Dublin, Republic of Ireland, Aug. 11-23, 1991, Laboratory for High Energy Astroph

Physics

2

Energetic Particles, Particle Flux Density, Solar Electrons, Solar Protons, Satellite Observation, Solar Physics

Scientific paper

NASA particle detectors on the IMP-8 are employed to determine the size distributions of the peak fluxes of events related to solar-energetic particles including protons and electrons. The energetic proton events show a flatter size distribution which suggests that not all flares are proton flares. Both the electron and proton events are classified as either 'impulsive' or 'gradual', and the impulsive events tend to have a steeper power-law distribution.

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