Statistical acceleration and stationary transport of solar cosmic rays in interplanetary space

Details Statistical acceleration and stationary transport of solar cosmic rays in interplanetary space Statistical acceleration and stationary transport of solar cosmic rays in interplanetary space

Apr 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ge%26ae..25..177s&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 25, Mar.-Apr. 1985, p. 177-183. In Russian.

Physics

Condensed Matter

Statistical Mechanics

Interplanetary Space, Particle Acceleration, Solar Cosmic Rays, Statistical Mechanics, Transport Properties, Adiabatic Conditions, Convection, Deceleration, Nonrelativistic Mechanics, Particle Diffusion, Solar Wind Velocity

Scientific paper

The transport equation for nonrelativistic solar cosmic rays is solved in the spherically symmetric case and for a constant solar wind. Convection processes, adiabatic deceleration, spatial diffusion, and diffusion in momentum space are taken into account. The energy spectrum of protons and helium nuclei at distances from the sun not exceeding 1 AU is examined, and the radial gradient of protons with an energy of 10-50 MeV is determined. Attention is given to Helios-1, 2 and IMP-7, 8 measurements.

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