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The new approach to the mechanism of solar magnetic cycle

Published online by Cambridge University Press:  14 March 2005

A. A. Solov'ev  and
E. A. Kiritchek
A. A. Solov'ev
Affiliation:
Main Astronomical Observatory of Russian Academy of Sciences, Pulkovo, St. Petersburg, 196140 Russia, email: solov@kalmsu.ru Present address: Kalmyk State University, 11 Pushkin Street, Elista, 358000 Russia
E. A. Kiritchek
Affiliation:
Department of Theoretical Physics, Kalmyk State University, Elista, 358000 Russia
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Traditionally the $\alpha - \omega$-dynamo is regarded as a basic theory of solar activity (SA) cycle. Here the model of solar magnetic cycle based on the new MHD-solutions for the mean large-scale magnetic field is presented. The hypothesis of gyrotropic plasma turbulence and cyclic restoring of the poloidal magnetic field from the rising toroidal magnetic flux tubes due to the $\alpha$-effect is not used (see Solov'ev and Kiritchek (2004)).To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUS223 , June 2004 , pp. 143 - 144
Copyright
© 2004 International Astronomical Union