Solar p-modes oscillations and heating of the corona

Details Solar p-modes oscillations and heating of the corona Solar p-modes oscillations and heating of the corona

May 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992soph..139..201z&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 139, no. 1, May 1992, p. 201-203.

Physics

6

Heating, Magnetoacoustic Waves, Solar Corona, Solar Oscillations, Magnetohydrodynamic Waves, Plasma Resonance, Solar Magnetic Field

Scientific paper

Resonator properties are investigated analytically for fast magnetoacoustic waves in a finite conductivity medium permeated by a nearly horizontal magnetic field. Excitation of the Alfven waves at the Alfven resonance or heating of the medium in the vicinity of the Alfven resonance result from the tunnel penetration of the resonator waves. It is concluded that solar p-mode oscillations can contribute significantly or account for nonradiative heating of the corona.

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