Turbulence transport and shock acceleration in solar corona

Details Turbulence transport and shock acceleration in solar corona Turbulence transport and shock acceleration in solar corona

Aug 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aipc..932..350v&link_type=abstract

TURBULENCE AND NONLINEAR PROCESSES IN ASTROPHYSICAL PLASMAS; 6th Annual International Astrophysics Conference. AIP Conference P

Astronomy and Astrophysics

Astrophysics

Mhd Waves, Plasma Waves, Turbulence, Energetic Particles, Coronal Mass Ejection

Scientific paper

Recent efforts on modeling coronal turbulence transport and shock acceleration self-consistently are reviewed. The considered models are based on the assumption that the turbulence responsible for the scattering of energetic ions consists of slab-mode Alfvén waves. A short discussion of the applied wave transport equation and particle transport coefficients is followed by a more extensive review of analytical and numerical modeling results of coupled evolution of energetic particle fluxes and wave intensities.

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