Damping of Fast Modes of MHD Turbulence and Electron Acceleration in Solar Flares

Details Damping of Fast Modes of MHD Turbulence and Electron Acceleration in Solar Flares Damping of Fast Modes of MHD Turbulence and Electron Acceleration in Solar Flares

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007ebhe.conf..339y&link_type=abstract

ENERGY BUDGET IN THE HIGH ENERGY UNIVERSE . Proceedings of the International Workshop. Held 22-24 February 2006 in Kashiwa, Japa

Physics

Scientific paper

We address the problem of turbulence damping and particle acceleration in Solar flares. We consider turbulent energy cascade of fast modes and their collisional and collisionless damping processes, which also include damping through the transfer of turbulent energy to non-thermal particles. We identify collisionless damping by thermal particles as the dominant process for damping of fast modes in Solar corona conditions. This makes it possible to decouple particle acceleration and turbulence damping, which simplifies the problem substantially. We estimate the effect of particle acceleration on the cascade of fast modes, and show that our approach provides sufficiently accurate results.

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