Physics
Scientific paper
Feb 1976
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976soph...46..347n&link_type=abstract
Solar Physics, vol. 46, Feb. 1976, p. 347-375.
Physics
13
Astronomical Models, Interplanetary Space, Particle Motion, Solar Cosmic Rays, Solar Flares, Anisotropy, Kinetic Energy, Particle Diffusion, Stellar Models, Time Dependence
Scientific paper
A simplified complete model of solar flare cosmic ray events is proposed, consisting of two stages: a near-sun diffusion model, and a model of propagation in interplanetary space. The basic assumption is impulsive release at a point on the sun and subsequent propagation in a thin layer over the solar surface with continuous leakage into the interplanetary region. This leakage forms the source for the interplanetary propagation, and attention is focused on showing that some form of time-dependent injection is necessary to account for the observational data. Concentration is on the kinetic energy range from a few MeV to about 50 MeV, and the study concerns the temporal variations of the cosmic ray differential number density and anisotropy at a fixed point, and also the longitudinal distribution of the cosmic rays in space.
Gleeson Leo John
Ng Chee K.
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