Geometry of the diffusive propagation region in the August 14, 1982 solar electron event

Details Geometry of the diffusive propagation region in the August 14, 1982 solar electron event Geometry of the diffusive propagation region in the August 14, 1982 solar electron event

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....4..309e&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 4 p 309-312 (SEE N85-34729 23-92)

Physics

Electrons, Gamma Rays, Solar Cosmic Rays, Solar Flares, Diffusion, Interplanetary Space, Particle Flux Density, Solar Flux Density, Solar Maximum Mission

Scientific paper

On August 14, 1982, relativistic electrons arrived promptly after an impulsive gamma ray flare, indicating that very little scattering was taking place in interplanetary space. By ignoring anisotropy data the time profile of the event is well described by interplanetary diffusion except for the derived particle injection time. This discrepancy provides independent evidence that the particles are diffusing in a volume close to the Sun rather than in interplanetary space. The flux at maximum method of determining the number of particles produced is still a good approximation when appropriately applied.

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