Diffusion of strongly magnetized relativistic particles in a random magnetic field

Details Diffusion of strongly magnetized relativistic particles in a random magnetic field Diffusion of strongly magnetized relativistic particles in a random magnetic field

Oct 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987izssr..51.1799p&link_type=abstract

Akademiia Nauk SSSR, Izvestiia, Seriia Fizicheskaia (ISSN 0367-6765), vol. 51, Oct. 1987, p. 1799-1801. In Russian.

Physics

Cosmic Rays, Diffusion Theory, Magnetic Fields, Relativistic Particles, Convective Flow, Fokker-Planck Equation, Magnetohydrodynamic Waves, Particle Energy, Random Processes

Scientific paper

A diffusion equation is derived for strongly magnetized cosmic-ray particles propagating in a medium with a regular magnetic field and an ensemble of random MHD waves. Formulas are obtained which show the physical meaning of the equation coefficients, determining the mean particle velocity and the mean rate of the change in the particle momentum modulus.

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