Computer Science
Scientific paper
Oct 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ge%26ae..29..181b&link_type=abstract
Geomagn. Aeron., Vol. 29, No. 2, p. 181 - 185
Computer Science
Solar Cosmic Rays: Propagation, Solar Cosmic Rays: Interplanetary Matter
Scientific paper
The results of the numerical solution of the equation of propagation of energetic solar particles in the interplanetary magnetic field for a momentary source are presented. The temporal trend at the Earth's orbit of the density, anisotropy, and particle pitch-angle distribution function are determined. With values of the transport mean-free path Λ > 0.2 a.u., the results differ significantly from the results of the elementary diffusion model. The parameters of the temporal profiles permitting comparison with experiment are given.
Bazilevskaya Galina A.
Golynskaya R. M.
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