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Theory of Transport Processes

Published online by Cambridge University Press:  12 April 2016

J.-P. Zahn
J.-P. Zahn*
Affiliation:
Observatoire Midi-Pyrénées, 14, avenue E. Belin, S1400 Toulouse, FranceandColumbia University,New York, N.Y. 10027, U.S.A.

Abstract

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This review focuses on the transport of matter and angular momentum in the radiative zones of stellar interiors. The two main causes of such transport are the convective overshooting in the vicinity of convection zones, and the slow motions (meridional circulation and turbulence) due to the rotation of the star. In addition, momentum can be transfered through waves (generated by the motions above) and through magnetic stresses. The characteristics of those processes are examined, with special emphasis on turbulent diffusion.

Type
Part 4: Solar Cycle, Dynamo and Transport Processes
Information
International Astronomical Union Colloquium , Volume 121: Inside the Sun , 1990 , pp. 425 - 436
Copyright
Copyright © Kluwer 1990

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