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2. Manifestations of the Interaction between Convection and Rotation in Stellar Atmospheres (Lee Hartmann)

Published online by Cambridge University Press:  25 April 2016

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According to dynamo theories, the interaction between convection and rotation is responsible for the generation of magnetic fields in solar-type stars. Stellar observations can explore the ways the global parameters, like the surface rotation and internal structure, affect the production of magnetic fields. In this very brief review I wish to concentrate on recent progress in understanding the evolution of stellar rotation, and the dependence of stellar cycles and magnetic activity on rotation, internal structure, and age.

Type
Research Article
Information
Transactions of the International Astronomical Union , Volume 19 , Issue 1 , 1985 , pp. 507 - 510
Copyright
Copyright © Reidel 1985

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