Hostname: page-component-cd9895bd7-mkpzs Total loading time: 0 Render date: 2024-12-27T02:37:22.877Z Has data issue: false hasContentIssue false

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
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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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
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