Diffusion of relativistic particles in a weakly turbulent cosmic plasma

Details Diffusion of relativistic particles in a weakly turbulent cosmic plasma Diffusion of relativistic particles in a weakly turbulent cosmic plasma

Aug 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ge%26ae..29..529d&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 29, July-Aug. 1989, p. 529-536. In Russian.

Statistics

Computation

1

Cosmic Plasma, Magnetohydrodynamic Waves, Particle Interactions, Relativistic Particles, Wave Interaction, Computational Astrophysics, Transport Properties, Weak Energy Interactions

Scientific paper

An equation for the transport of cosmic rays in a moving medium with
random weak MHD waves is derived. The particle-wave interaction is
described by a general quasi-linear collision integral. The transport
equation describes the spatial diffusion, convective transport, and
regular and statistical energy variations of relativistic particles.

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