Propagation of solar cosmic rays in the high-velocity solar-wind flow

Details Propagation of solar cosmic rays in the high-velocity solar-wind flow Propagation of solar cosmic rays in the high-velocity solar-wind flow

Feb 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ge%26ae..27...12k&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 27, Jan.-Feb. 1987, p. 12-17. In Russian.

Astronomy and Astrophysics

Astronomy

2

Cosmic Rays, Solar Flares, Solar Protons, Solar Radiation, Solar Wind Velocity, Astronomical Models, Particle Diffusion, Plasma-Particle Interactions

Scientific paper

Numerical solutions are obtained for the equation of the anisotropic diffusion of solar cosmic rays (with allowance for convection processes and particle-energy variations in interplanetary space) and for the kinetic equation of solar-cosmic-ray propagation. The solutions obtained and an analysis of experimental data are used to study the effect of long-lived high-velocity solar-wind flows on the propagation of fast protons generated in solar flares. It is shown that the motion of fast charged particles with a low degree of scattering can occur in high-velocity solar-wind flows.

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