Non-magnetic motions in the photosphere and chromosphere.
Abstract
The author discusses four major problems in the area of solar atmospheric dynamics: the coupling of convective to atmospheric motions, the transport of energy from the convection zone to the chromosphere and corona, the nature of the motions that produce the non-thermal line broadening, and the nature and location of the dissipation mechanisms that heat the chromosphere and corona.
- Publication:
-
Max Planck Institut fur Astrophysik Report
- Pub Date:
- 1985
- Bibcode:
- 1985MPARp.212...48S
- Keywords:
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- Solar Atmosphere:Dynamics;
- Solar Chromosphere:Heating;
- Solar Chromosphere:Motions;
- Solar Photosphere:Motions