Propagation of solar cosmic rays in the interplanetary medium, taking adiabatic focusing into account

Details Propagation of solar cosmic rays in the interplanetary medium, taking adiabatic focusing into account Propagation of solar cosmic rays in the interplanetary medium, taking adiabatic focusing into account

Apr 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ge%26ae..29..204b&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 29, Mar.-Apr. 1989, p. 204-209. In Russian.

Physics

7

Energetic Particles, Interplanetary Medium, Particle Motion, Solar Cosmic Rays, Adiabatic Conditions, Interplanetary Magnetic Fields, Particle Diffusion, Pitch (Inclination)

Scientific paper

The numerical solution of the equations of the propagation of energetic solar particles in the interplanetary magnetic field in the case of an instantaneous source is presented. The earth-orbit time variations of the density, anisotropy, and pitch-angle distribution of the particles are determined. When the transport path Lambda exceeds 0.2 AU, the results differ substantially from those obtained with the elementary diffusion model.

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