SCR Steady State Distribution Function and Scattering Properties of the Interplanetary Medium

Details SCR Steady State Distribution Function and Scattering Properties of the Interplanetary Medium SCR Steady State Distribution Function and Scattering Properties of the Interplanetary Medium

Apr 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006ap%26ss.302...99f&link_type=abstract

Astrophysics and Space Science, Volume 302, Issue 1-4, pp. 99-107

Astronomy and Astrophysics

Astrophysics

Kinetic Equation, Solar Cosmic Rays, Ground Level Event

Scientific paper

The propagation of energetic particles in the interplanetary space is considered on the basis of kinetic equation describing the scattering of charged particles by magnetic irregularities and the particle focusing by regular magnetic field. Our analysis confirms that angular distribution of solar cosmic rays contains a valuable information about properties of the particle scattering in the interplanetary magnetic field. Steady state solutions of the kinetic equation are applied to the analysis of solar proton events.

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