Stochastic Acceleration in the Diffusion Region and the Structure of Slow Shocks in Solar Flares

Details Stochastic Acceleration in the Diffusion Region and the Structure of Slow Shocks in Solar Flares Stochastic Acceleration in the Diffusion Region and the Structure of Slow Shocks in Solar Flares

Jul 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994kofu.symp..231h&link_type=abstract

In: Proceedings of Kofu Symposium, Kofu, Japan, Sept. 6-10, 1993, p.231-234.

Computer Science

2

Scientific paper

Stochastic particle accelerations in the diffusion region of magnetic neutral sheet expected in solar flares are studied. The bulk energy and short time scale of flares are found to be accounted for by electron accelerations due to the turbulent Lower Hybrid Drift waves. Independent from above, the Petschek-type slow shock, if it exists, is found to be collisionless, and the relevant energy conversion is discussed. Finally a comparison between the stagnant diffusion model and slow shock model is made.

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