The Synthetic X-ray Flare Spectra for the Electron Beam and the Return Current

Details The Synthetic X-ray Flare Spectra for the Electron Beam and the Return Current The Synthetic X-ray Flare Spectra for the Electron Beam and the Return Current

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008espm...12.3.48d&link_type=abstract

"12th European Solar Physics Meeting, Freiburg, Germany, held September, 8-12, 2008. Online at http://espm.kis.uni-freiburg.de/,

Physics

Scientific paper

The electron beams accelerated during flare in low corona create return currents of electrons in solar plasma. The accelerated electrons of the electron beam and return current influence the electron distribution function. The shape of the electron distribution which includes the interaction of the electron beam with plasma and formation of the return current has been modeled by PIC code. The synthetic X-ray spectra for a such kind of the electron distributions have been computed by using a modification of CHIANTI. The possibility to diagnose of the return current from X-ray spectra is discussed.

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