Astronomy and Astrophysics – Astrophysics
Scientific paper
Mar 2012
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012ap%26ss.tmp..111b&link_type=abstract
Astrophysics and Space Science, Online First
Astronomy and Astrophysics
Astrophysics
Diffusion, Magnetic Fields, Turbulence
Scientific paper
One can assume that energetic particles follow magnetic field lines while they propagate through a magnetized plasma. The latter scenario is usually described by the so-called field line random walk limit. This limit, however, is only valid if parallel diffusion is suppressed. As soon as the latter effect is taken into account, perpendicular transport becomes subdiffusive. This physical scenario is usually called compound diffusion or compound subdiffusion and can be described by a Chapman-Kolmogorov equation. In the latter equation the parallel distribution function is an essential ingredient. In the present paper we replace the standard Gaussian model by a Kappa distribution to compute distribution functions and mean square displacements across the field.
Buffie K.
Shalchi Andreas
No associations
LandOfFree
Compound diffusion of energetic particles: a Kappa model for the parallel distribution function does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Compound diffusion of energetic particles: a Kappa model for the parallel distribution function, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Compound diffusion of energetic particles: a Kappa model for the parallel distribution function will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1365071