Towards Energy and Momentum Transfer by Electron Beams in a Flaring Atmosphere

Details Towards Energy and Momentum Transfer by Electron Beams in a Flaring Atmosphere Towards Energy and Momentum Transfer by Electron Beams in a Flaring Atmosphere

Oct 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999esasp.446..727z&link_type=abstract

8th SOHO Workshop: Plasma Dynamics and Diagnostics in the Solar Transition Region and Corona. Proceedings of the Conference hel

Astronomy and Astrophysics

Astrophysics

Scientific paper

Using solutions of the time-dependent kinetic equation for energy power law electron beam anisotropic precipitation into a flaring loop in a presence of the induced electric field of return current and converging magnetic field the energy deposition and momentum are calculated at different depths. Effect of different energy losses mechanisms on the energy deposition by electron beams is discussed. At the lower chromosphere for moderately intense and hard beams with higher upper energy the energy deposition was shown to be nearly a constant slowly decreasing with depth. The energy momentum was evaluated for different beam parameters at different depths and compared with those from the recent SOHO/MDI seismic observations. For preprints contact : valja@astro.gla.ac.uk

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