Stationary solar cosmic-ray modulation in interplanetary space

Details Stationary solar cosmic-ray modulation in interplanetary space Stationary solar cosmic-ray modulation in interplanetary space

Oct 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976ge%26ae..16..215v&link_type=abstract

(Geomagnetizm i Aeronomiia, vol. 16, Mar.-Apr. 1976, p. 215-220.) Geomagnetism and Aeronomy, vol. 16, Oct. 1976, p. 129-131. Tra

Physics

Interplanetary Space, Solar Cosmic Rays, Solar Protons, Boltzmann Transport Equation, Distribution Functions, Laplace Transformation, Power Spectra, Steady State, Taylor Series

Scientific paper

An analytical solution is obtained for the transport equation describing the propagation of solar cosmic ray particles in interplanetary space. The equation takes account of particle convection, diffusion and adiabatic deceleration and the emission of the particles is assumed to be steady state, spherically symmetric with a power spectrum. The modulation of nonrelativistic solar protons is studied as a particular case.

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