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Magnetism and Activity of the Sun and Stars
J. Arnaud and N. Meunier (eds)
EAS Publications Series, Vol. 9, 2003

DOI: 10.1051/eas:2003080

Stellar dynamos - perspectives and challenges

M. Korpi1, 2 and I. Tuominen2

1  Laboratoire d'Astrophysique, Observatoire Midi-Pyrénées, 14 Av. Edouard Belin, 31400 Toulouse, France
2  Astronomy Division, University of Oulu, PO Box 3000, 90014 University of Oulu, Finland


Abstract
In this paper the present status of theoretical understanding - mostly relying on mean-field dynamo models - of global magnetic activity of late-type stars with convective envelopes is reviewed. The principles of the mean-field dynamo theory are introduced, and a discussion on some of the present-day problems and challenges is presented. The remaining sections are devoted to discuss the current status of solar and stellar dynamo models.



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