The three-dimensional diffusion of high-energy solar cosmic rays

Details The three-dimensional diffusion of high-energy solar cosmic rays The three-dimensional diffusion of high-energy solar cosmic rays

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icrc....4..135h&link_type=abstract

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

Statistics

Computation

Computational Astrophysics, Particle Diffusion, Solar Cosmic Rays, Solar Flares, Diffusion Coefficient, Interplanetary Magnetic Fields, Radiant Flux Density, Random Walk, Solar Activity Effects, Solar Magnetic Field, Temporal Distribution

Scientific paper

Basic features of solar cosmic-ray events are discussed using the solution of a three-dimensional diffusion equation of solar cosmic-ray propagation. The equation is derived on the basis of a new spiral coordinate system for the large-scale interplanetary spiral magnetic field. The solution depends on the solar magnetic longitude of the flare producing cosmic rays. The results agree well with observations.

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