Solar CR kinetics in the radial regular IMF

Details Solar CR kinetics in the radial regular IMF Solar CR kinetics in the radial regular IMF

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001icrc....8.3334f&link_type=abstract

Proceedings of the 27th International Cosmic Ray Conference. 07-15 August, 2001. Hamburg, Germany. Under the auspices of the Int

Physics

Scientific paper

Theory of cosmic ray propagation in the radial regular magnetic field with superimposed magnetic irregularities is advanced. The particles can be divided into two parts which describe the unscattered and scattered populations. In result, the unscattered particles appear as a strongly anisotropic beam with a small angular width due to the magnetic focusing of charged particles in radial regular magnetic field. Evolution of the angular distribution of both populations and the temporal profiles of CR intensity are analyzed. The obtained results can be used for description of energetic particle streams in the turbulent interplanetary magnetic field.

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