Temperature minimum heating in solar flares by resistive dissipation of Alfven waves

Details Temperature minimum heating in solar flares by resistive dissipation of Alfven waves Temperature minimum heating in solar flares by resistive dissipation of Alfven waves

Aug 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981stin...8210975e&link_type=abstract

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Physics

Energy Dissipation, Magnetohydrodynamic Waves, Solar Corona, Solar Flares, Solar Temperature, Solar Energy, Solar Magnetic Field, Wave Propagation

Scientific paper

The possibility that the strong heating produced at temperature-minimum levels during solar flares is due to resistive dissipation of Alfven waves generated by the primary energy release process in the corona is studied. It is shown how, for suitable parameters, these waves can carry their energy essentially undamped into the temperature-minimum layers and can then produce a degree of heating consistent with observations.

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