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Magnetic Cycles and Rotation in Active Late–Type Stars
Published online by Cambridge University Press: 26 May 2016
Abstract
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Observational evidence, based both on spectroscopic Doppler imaging and long-term photometry, of strongly nonaxisymmetric spot distributions in magnetically very active late-type stars, with a special cyclic behaviour (the “flip-flop” effect), is presented. Theoretical implications of these results are discussed from the point of view of nonlinear mean-field dynamo theory.
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- Session 2 Rotation in Relation with Abundances and Magnetic Fields
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- Copyright © Astronomical Society of the Pacific 2004
References
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