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Rotational Transport Processes

Published online by Cambridge University Press:  26 May 2016

Suzanne Talon
Suzanne Talon*
Affiliation:
CERCA, 5160 boul. Décarie suite 400, Montréal, Québec H3X 2H9 and Département de physique, Université de Montréal, Québec H3C 3J7

Abstract

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In this review, I discuss physical mechanisms leading to momentum and chemical transport in stars. Various instabilities leading to turbulence are discussed. I then present a self-consistent description of rotational mixing under the action of turbulence and meridional circulation in 1D models. Limitations of the model are discussed, both in terms of an extra mechanism for momentum transport in the Sun and solar-type stars (magnetic field and/or gravity waves) and in terms of our understanding of turbulent properties.

Information

Type
Session 3 Rotation, Solar and Stellar Physics
Information
Symposium - International Astronomical Union , Volume 215: Stellar Rotation , 2004, pp. 336 - 345
Copyright
Copyright © Astronomical Society of the Pacific 2004 

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