The numerical treatment of solar particle diffusion in the magnetic fields of interplanetary space

Details The numerical treatment of solar particle diffusion in the magnetic fields of interplanetary space The numerical treatment of solar particle diffusion in the magnetic fields of interplanetary space

Dec 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985phdt........23s&link_type=abstract

Ph.D. Thesis Kiel Univ. (Germany, F.R.). Inst. für Reine und Angewandte Kernphysik.

Physics

15

Interplanetary Magnetic Fields, Interplanetary Space, Particle Diffusion, Boltzmann Transport Equation, Diffusion Coefficient, Solar Corona, Solar Wind

Scientific paper

The injection and diffusion of charged particles in interplanetary magnetic fields are discussed. The advantages of a numerical treatment of diffusion and transport models, where influences on particle diffusion and velocity are not taken into account, are assessed. Numerical treatment offers a solution for the transport equation and shows influences of the interplanetary magnetic field, pitch angle scattering, and the duration of solar injection on the equation.

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