Sound generation by random phase Alfven waves in the solar atmosphere

Details Sound generation by random phase Alfven waves in the solar atmosphere Sound generation by random phase Alfven waves in the solar atmosphere

Dec 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976azh....53.1260p&link_type=abstract

Astronomicheskii Zhurnal, vol. 53, Nov.-Dec. 1976, p. 1260-1263. In Russian.

Astronomy and Astrophysics

Astronomy

Acoustic Excitation, Magnetoacoustic Waves, Magnetohydrodynamic Waves, Solar Atmosphere, Solar Corona, Wave Interaction, Kinetic Equations, Low Frequencies, Solar Magnetic Field, Waveguides

Scientific paper

The problem of acoustic excitation by opposed Alfven waves in the solar plasma is considered. Kinetic equations for interacting waves are developed and analyzed on the assumption that the Alfven waves have random phases. Estimates of the waveguide parameters for these waves show that they could produce low-frequency pulsations in the solar atmosphere.

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