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Heating of the solar corona by Alfvén wave envelopes
Authors:Dirk K Callebaut  Nodar L Tsintsadze
Institution:(1) Phys. Dept., UIA, Univ. of Antwerp, B-2610, Antwerp, Belgium;(2) Inst. of Physics, Academy of Sciences, 380077, Rep. of Georgia
Abstract:Alfvén waves are investigated including dissipation and dispersion (Hall effect). The latter leads to a modulational instability and to a soliton envelope so that the temperature may increase by an order of magnitude. Applications are the heating of the solar corona, a possible triggering of flares and maybe tokamak heating.
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