Hostname: page-component-586b7cd67f-rcrh6 Total loading time: 0 Render date: 2024-11-30T16:16:33.597Z Has data issue: false hasContentIssue false
  • English
  • Français

Non-linear Convection with Free Boundaries at High Rayleigh Number

Published online by Cambridge University Press:  25 April 2016

J. O. Murphy
J. O. Murphy*
Affiliation:
Department of Mathematics, Monash University, Melbourne
Get access Rights & Permissions [Opens in a new window]

Extract

It has been suggested, for example by Wilson and Spiegel, that the results from the study of convection in incompressible fluids may provide a basis for the study of the solar convection zone. In fact Wilson’s models contain temperature fluctuation maxima, a feature exhibited by the results obtained from the convection problem for large values of the Rayleigh number.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 2 , Issue 1 , July 1971 , pp. 51 - 52
Copyright
Copyright © Astronomical Society of Australia 1971

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

1 Wilson, P. R., Solar Physics, 9, 303 (1969).CrossRefGoogle Scholar
2 Spiegel, E. A. and Bohm, K., ‘Aerodynamic Phenomena in Stellar Atmospheres’ IAU Symposium No. 28, 1967 p. 347.Google Scholar
3 van der Borght, R., Proc. ASA, 2, 45 (1971).Google Scholar
4 Roberts, P. H., ‘Non-Equilibrium Thermodynamics, Variational Techniques and Stability’, University of Chicago Press, Chicago 1966 p. 125. Murphy, J. O., Aust. J. Phys. (to be published) (1971).Google Scholar