Transport in random magnetic fields: diffusion, subdiffusion and nonlinear second diffusion

Details Transport in random magnetic fields: diffusion, subdiffusion and nonlinear second diffusion Transport in random magnetic fields: diffusion, subdiffusion and nonlinear second diffusion

Sep 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aipc..679..664q&link_type=abstract

SOLAR WIND TEN: Proceedings of the Tenth International Solar Wind Conference. AIP Conference Proceedings, Volume 679, pp. 664-6

Computer Science

1

Particle Emission, Solar Wind, Interplanetary Magnetic Fields, Solar Wind Plasma, Sources Of Solar Wind

Scientific paper

We present numerical results that show, first, conditions under which parallel scattering reduces the effectiveness of perpendicular scattering, leading to the phenomenon of subdiffusion (``compound diffusion''), and second, that when sufficiently strong three dimensional effects are present, true diffusion is restored, with a suppressed perpendicular diffusion coefficient that depends upon the parallel mean free path.

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