Transport of charged particle pulses in interplanetary magnetic fields

Details Transport of charged particle pulses in interplanetary magnetic fields Transport of charged particle pulses in interplanetary magnetic fields

Sep 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995czjph..45..767f&link_type=abstract

Czechoslovak Journal of Physics, vol. 45, Issue 9, p.767-775

Physics

Scientific paper

The charged particle scattering in the presence of a regular magnetic field is considered starting from the Boltzmann kinetic equation in the case of an arbitrary relation between the mean free path and the distance from a particle source. It is shown that the Green function for the kinetic equation can be represented as the sum of the distribution functions of non-scattered particles which propagate with the injection pitch angle and of the scattered ones. The obtained Green function of the Boltzmann equation and also the particle density describe the space-time-pitch angle cosmic ray distribution that corresponds to an instantaneous particle injection at a particular pitch angle.

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