Coupling equations for a flow-wave field used to faculae heating

Details Coupling equations for a flow-wave field used to faculae heating Coupling equations for a flow-wave field used to faculae heating

Jan 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982soph...75...83l&link_type=abstract

Solar Physics, vol. 75, Jan. 1982, p. 83-98.

Physics

4

Faculae, Magnetohydrodynamic Flow, Plasma Heating, Solar Physics, Photosphere, Propagation Modes, Stress Tensors

Scientific paper

The coupling equations for the mean flow-wave field are derived, for the case of the binary system of a background fluid-wave field, from the general thermodynamic properties of the medium. The corresponding representation of the wave stress tensor is found for the following wave modes: (1) Langmuir wave, (2) ion-acoustic oscillations, (3) whistlers, (4) Alfven waves, (5) magnetoacoustic oscillations, and (6) transverse plasma wave. A result consistent with observations is obtained through the application of the representation of the Alfven waves to faculae heating, which leads to the suggestion that wave action is likely to decrease the height of the corresponding layer of the undisturbed photosphere and thereby increase pressure, temperature and density.

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