Quasi-linear theory of energetic particle diffusion in stationary 3-dimensional turbulence

Details Quasi-linear theory of energetic particle diffusion in stationary 3-dimensional turbulence Quasi-linear theory of energetic particle diffusion in stationary 3-dimensional turbulence

Aug 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999icrc....4..229f&link_type=abstract

Proceedings of the 26th International Cosmic Ray Conference. August 17-25, 1999. Salt Lake City, Utah, USA. Under the auspices o

Physics

Scientific paper

A quasi-linear theory of cosmic ray diffusion in fully three-dimensional magnetic turbulence is developed, to lead to better understanding of perpendicular diffusion and the effects of imperfect symmetry in the magnetic turbulence. Calculation of the pitch angle scattering coefficient, in terms of the elements of the power spectrum tensor, in the case of turbulence symmetric about the direction of the mean field, is given as a demonstration of the method.

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