On two different models of solar cosmic ray propagation

Details On two different models of solar cosmic ray propagation On two different models of solar cosmic ray propagation

Oct 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002kfnt...18..450s&link_type=abstract

Kinematika i Fizika Nebesnykh Tel, vol. 18, no. 5, p. 450-453.

Physics

Scientific paper

We investigated the characteristic features of temporal evolution of the distribution function for particles of solar cosmic rays on an example of exact analytical solutions of the Boltzmann and Fokker-Planck kinetic equations for isotropic scattering in a spatially homogeneous case. It turned out that the Fokker-Planck scattering reduces the initial anisotropic distribution to an isotropic one much faster than the Boltzmann scattering. This enables us to judge the character of the magnetohydrodynamic turbulence in the interplanetary space from the data on solar proton events.

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