On quasilinear perpendicular diffusion of cosmic rays in weak turbulence

Details On quasilinear perpendicular diffusion of cosmic rays in weak turbulence On quasilinear perpendicular diffusion of cosmic rays in weak turbulence

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aipc..719..317s&link_type=abstract

PHYSICS OF THE OUTER HELIOSPHERE. AIP Conference Proceedings, Volume 719, pp. 317-322 (2004).

Physics

Solar Wind Plasma, Sources Of Solar Wind, Particle Emission, Solar Wind

Scientific paper

The quasilinear calculation of perpendicular diffusion of cosmic ray particles for weak dynamical magnetic turbulence of arbitrary geometry is presented. Starting from the equations of motion a detailed point-by-point derivation of quasilinear Fokker-Planck coefficients is given. It is shown that, in order to have diffusive behaviour of the Fokker-Planck coefficients, the existence of a finite correlation time of the magnetic fluctuations is essential.

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