Astronomy and Astrophysics – Astronomy
Scientific paper
Apr 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985pazh...11..278d&link_type=abstract
(Pis'ma v Astronomicheskii Zhurnal, vol. 11, Apr. 1985, p. 278-285) Soviet Astronomy Letters (ISSN 0360-0327), vol. 11, Mar.-Apr
Astronomy and Astrophysics
Astronomy
3
Solar Cycles, Solar Oscillations, Convection, Field Strength, Magnetohydrodynamics, Solar Magnetic Field, Torsional Vibration
Scientific paper
The possibility is considered that the observed 11-year torsional oscillations of the sun may be primary eigen-mode oscillations of the surface layers excited by convection. Estimates of both frequency and amplitude of the torsional wave are obtained. The magnetic manifestation of the solar cycle probably results from the modulation (by torsional oscillations) of the field generation process.
Dolginov Arkady Z.
Muslimov Alex G.
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