Spatial distribution of the solar particles during the 7 May 1978 flare

Details Spatial distribution of the solar particles during the 7 May 1978 flare Spatial distribution of the solar particles during the 7 May 1978 flare

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icrc....4..185l&link_type=abstract

IN: International Cosmic Ray Conference, 18th, Bangalore, India, August 22-September 3, 1983, Conference Papers. Volume 4 (A85-2

Physics

Cosmic Rays, Interplanetary Magnetic Fields, Solar Corpuscular Radiation, Solar Flares, Particle Diffusion, Solar Corona, Solar Protons, Spatial Distribution

Scientific paper

An extended study has been made of the satellite and ground-based cosmic-ray data for the nearly scatter-free solar particle event on May 7, 1978. From the Helios A and IMP 7 cosmic-ray telescope data, the coronal propagation is characterized by a diffusion coefficient of 2-3 x 10 to the 16th sq cm/s from 38 MeV (270 MV) to 400 MeV (954 MV). The loss rate of particles in the solar corona decreased from 2.4 per hr at 4.15 GeV (5 GV) to 0.1 per hr at 100 MeV (445 MV).

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