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Issue A&A
Volume 416, Number 3, March IV 2004
Page(s) L13 - L16
Section Letters
DOI http://dx.doi.org/10.1051/0004-6361:20040034



A&A 416, L13-L16 (2004)
DOI: 10.1051/0004-6361:20040034

Letter

Collisional excitation and ionization of hydrogen by return current in solar flares

M. Karlický, J. Kasparová and P. Heinzel

Astronomical Institute of the Academy of Sciences of the Czech Republic, 25165 Ondrejov, Czech Republic
(Received 5 December 2003 / Accepted 30 January 2004)

Abstract
First a problem of the transport of electron beams with high energy fluxes into the cold chromosphere during the flare is presented. Then it is shown that the problem might be solved by the return current formed by superthermal (runaway) electrons. In such a case the return current electrons could influence hydrogen excitations and ionizations. Therefore, we computed collisional rates of such a return current and compared them with those of the thermal plasma and of a monoenergetic (10 keV) electron beam with the energy flux $F_{\rm E} = 10^{12}~\mbox{erg\,cm}^{-2}\,\mbox{ s}^{-1}$ penetrating into the flare atmosphere described by the F1 model (Machado et al. 1980). We show that in this situation the return current collisional rates can be dominant for some transitions.


Key words: Sun: flares -- plasmas -- atomic processes

Offprint request: M. Karlický, karlicky@asu.cas.cz




© ESO 2004


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