Quasilinear Theory of Cosmic Ray Transport in Weak Magnetohydrodynamic Plasma Turbulence

Details Quasilinear Theory of Cosmic Ray Transport in Weak Magnetohydrodynamic Plasma Turbulence Quasilinear Theory of Cosmic Ray Transport in Weak Magnetohydrodynamic Plasma Turbulence

Dec 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999ptep.proc..225s&link_type=abstract

Plasma Turbulence and Energetic Particles in Astrophysics, Proceedings of the International Conference, Cracow (Poland), 5-10 Se

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

Several recent results of quasilinear cosmic ray transport theory are reviewed. It is shown that modelling the plasma turbulence beyond the magnetostatic approximation is most important for a correct description of cosmic ray dynamics. In particular, the effects of finite plasma wave speeds play a crucial role both for the behaviour of the particles' spatial diffusion coefficient and the diffusive acceleration by super-Alfvenic shock waves.

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