Solutions of the two-dimensional steady-state cosmic-ray transport equation in interplanetary space

Details Solutions of the two-dimensional steady-state cosmic-ray transport equation in interplanetary space Solutions of the two-dimensional steady-state cosmic-ray transport equation in interplanetary space

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icrc...10....5p&link_type=abstract

IN: International Cosmic Ray Conference, 18th, Bangalore, India, August 22-September 3, 1983, Late Papers. Volume 10 (A85-22801

Computer Science

Cosmic Rays, Interplanetary Space, Transport Theory, Diffusion Coefficient, Diurnal Variations, Heliosphere, Steady State

Scientific paper

The authors present further numerical solutions of the two-dimensional
steady-state cosmic ray transport equation in a three-dimensional
axisymmetric heliosphere. They illustrate the effect of the inclusion of
particle drift and compare the results with some experimental data.

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