Dielectronic satellite lines and double layers in solar flares

Author: Dzifčáková E.   Karlický M.   Dudík J.  

Publisher: Edp Sciences

E-ISSN: 1432-0746|550|issue|A60-A60

ISSN: 0004-6361

Source: Astronomy & Astrophysics, Vol.550, Iss.issue, 2013-01, pp. : A60-A60

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Abstract

Context. Particle acceleration during solar flares results in departures of the distribution of particle energies from the Maxwellian distribution. Apart from the high-energy tail, the bulk of the distribution was recently also found to be significantly affected, due, e.g., to the presence of double layers.