Interplanetary propagation of flare-associated energetic particles

Details Interplanetary propagation of flare-associated energetic particles Interplanetary propagation of flare-associated energetic particles

Apr 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978stin...7824014m&link_type=abstract

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Astronomy and Astrophysics

Astronomy

Cosmic Rays, Interplanetary Medium, Particle Energy, Solar Flares, Astronomical Models, Electron Scattering, Magnetohydrodynamics, Normal Density Functions, Proton Scattering

Scientific paper

A propagation model which combines a Gaussian profile for particle release from the sun, with interplanetary particle densities predicted by focused diffusion, was proposed to explain the propagation history of flare associated energetic particles. This model, which depends on only two parameters, successfully describes the time-intensity profiles of 30 proton and electron events originating from the western hemisphere of the sun. Generally, particles are released from the sun over a finite interval. In almost all events, particle release begins at the time of flare acceleration.

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