Influence of the Return Current on the EUV and X-Ray Flare Line Emissions

Details Influence of the Return Current on the EUV and X-Ray Flare Line Emissions Influence of the Return Current on the EUV and X-Ray Flare Line Emissions

Aug 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008soph..250..329d&link_type=abstract

Solar Physics, Volume 250, Issue 2, pp.329-338

Physics

8

Electron Beam, Return Current, Non-Thermal Distributions, Euv And X-Ray Emission

Scientific paper

Electron beams accelerated during solar flares carry electric currents which should be neutralized by so-called return currents. Both the electron beam and return current modify the electron distribution function in the solar transition region and low corona. Thus, they influence the intensities of the spectral lines formed in these layers. Synthetic spectra for the solar flare atmosphere are computed from model conditions and the possibilities of diagnostics of the return current from the EUV and X-ray line spectra are discussed.

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