Non-diffusive transport of cosmic rays in homogeneous. regular magnetic fields

Details Non-diffusive transport of cosmic rays in homogeneous. regular magnetic fields Non-diffusive transport of cosmic rays in homogeneous. regular magnetic fields

Oct 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995a%26a...302..623f&link_type=abstract

Astronomy and Astrophysics, v.302, p.623

Astronomy and Astrophysics

Astrophysics

8

Cosmic Rays, Sun: Particle Emission, Magnetic Fields

Scientific paper

The cosmic ray charged particle scattering in the presence of a regular magnetic field is considered starting from the Boltzmann kinetic equation. It is shown that Green's function for the kinetic equation can be represented as the sum of the distribution function of non-scattered particles, which propagate in the injection direction, and the scattered ones. Both the weak scattering and diffusive approximations of the obtained general solution are performed. The obtained Green function of the Boltzmann equation and also the particle density describe the space-time-pitch angle distribution that corresponds to an instantaneous particle injection at a particular pitch angle.

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