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Towards a Generalization of a Mixing-length Model for Nonradially Pulsating Stars: Convection in a Shear

Published online by Cambridge University Press:  13 May 2016

G. Houdek  and
D. O. Gough
G. Houdek
Affiliation:
Institute of Astronomy, University of Cambridge, CB3 0HA, England
D. O. Gough
Affiliation:
Institute of Astronomy and Department of Applied Mathematics and Theoretical Physics, University of Cambridge, CB3 9EW, England

Abstract

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We discuss a generalization of a mixing-length formalism for convection in the presence of a mean flow, and present the convective fluxes for convective cells with the geometry of rolls and of hexagons.

Type
Session I: Global Structure and Evolution of the Solar Interior
Information
Symposium - International Astronomical Union , Volume 203: Recent Insights into the Physics of the Sun and Heliosphere: Highlights from Soho and Other Space Missions , 2001 , pp. 115 - 117
Copyright
Copyright © Astronomical Society of the Pacific 2001 

References

Christopherson, D.G., 1940, Quart. J. Math. 11, 63.CrossRefGoogle Scholar
Gough, D.O., 1978, in: Proc. Workshop on Solar Rotation, Belvedere, G., Paternó, L. (eds.), p. 337.Google Scholar
Gough, D.O., Houdek, G., 2000, in: SOHO 10/GONG 2000: Helio- and Asteroseismology at the Dawn of the Millennium, ESA-SP-464, ESTEC, Noordwijk, in press.Google Scholar
Spiegel, E.A., Veronis, G., 1960, ApJ 131, 442.Google Scholar
Unno, W., 1967, PASJ 19, 140.Google Scholar