The diffusion of relativistic particles in a weakly-turbulent cosmic plasma.

Details The diffusion of relativistic particles in a weakly-turbulent cosmic plasma. The diffusion of relativistic particles in a weakly-turbulent cosmic plasma.

Jun 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ge%26ae..29..405d&link_type=abstract

Geomagn. Aeron., Vol. 29, No. 4, p. 405 - 409

Physics

1

Cosmic Rays: Magnetohydrodynamics

Scientific paper

A transfer equation is derived for cosmic rays in a moving medium with random, weak magnetohydrodynamic waves. The particle-wave interaction is described by a "quasi-linear collision integral" of general form. Wave polarization is given by the polarization matrix. The transfer equation describes the spatial diffusion, convective transfer, and the regular and statistical change in energy of the relativistic particles.

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