Cosmic ray transport in a vortex flow

Details Cosmic ray transport in a vortex flow Cosmic ray transport in a vortex flow

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aipc..719..243v&link_type=abstract

PHYSICS OF THE OUTER HELIOSPHERE. AIP Conference Proceedings, Volume 719, pp. 243-248 (2004).

Physics

Particle Emission, Solar Wind, Solar Wind Plasma, Sources Of Solar Wind, Discontinuities

Scientific paper

There is experimental evidence that the solar wind is populated with nonlinear waves and coherent structures. There is also experimental as well as theoretical evidence that solar wind MHD turbulence can be approximated in terms of dynamic composite two-dimensional plus slab turbulence. Within this framework turbulence in the heliospheric plasma sheet, for example, is expected to consist of two-dimensional non-linear MHD vortex structures plus slab turbulence associated with quasi-linear Alfven waves. We reexamine energetic particle transport in the heliosphere by taking into account scattering on vortices.

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