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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. HeinzelAstronomical 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
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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