Solution of the Boltzmann equation for nondiffusive solar cosmic ray propagation.

Details Solution of the Boltzmann equation for nondiffusive solar cosmic ray propagation. Solution of the Boltzmann equation for nondiffusive solar cosmic ray propagation.

Sep 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996angeo..14.1016f&link_type=abstract

Annales Geophysicae, Vol. 14, No. 9, p. 1016 - 1018

Physics

2

Solar Cosmic Rays: Interplanetary Space, Solar Cosmic Rays: Propagation

Scientific paper

Solar cosmic ray (SCR) propagation in interplanetary space is studied on
the basis of the Boltzmann kinetic equation. An analytic solution of the
kinetic equation has been derived for the three-dimensional spherical
geometry. The effect of the SCR injection duration on the time evolution
of the particle density is investigated.

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