Abstract:Context. We use a two-fluid model to study the heating of the solar chromosphere by magnetoacoustic and magnetoacoustic-gravity waves. In the model, we include energy dissipation as a result of ion-neutral collisions. Aims. The aim of this paper is to study impulsively generated two-fluid magnetoacoustic and magnetoacoustic-gravity waves and to quantify their contribution to chromosphere heating and the generation of plasma outflows. Methods. We consider a 2D model of the gravitationally stratified and partial… Show more
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