Magneto-acoustic-gravity waves on the sun. III - The theory of running penumbral waves

Details Magneto-acoustic-gravity waves on the sun. III - The theory of running penumbral waves Magneto-acoustic-gravity waves on the sun. III - The theory of running penumbral waves

Apr 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984a%26a...133..333z&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 133, no. 2, April 1984, p. 333-340.

Astronomy and Astrophysics

Astrophysics

17

Gravity Waves, Magnetoacoustic Waves, Penumbras, Solar Atmosphere, Wave Propagation, Astronomical Models, Chromosphere, Doppler Effect, Photosphere, Shear Flow, Surface Waves

Scientific paper

A model of running penumbral waves based on the theory of linear transformation of magneto-acoustic-gravity waves has been constructed. Penumbral waves arise as a result of transformation in the almost horizontal magnetic field of five-minute waves trapped in the solar convection zone. The main properties of penumbral waves are explained within the framework of the model suggested.

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