Antia, H. M. ; Chitre, S. M. ; Narasimha, D. (1983) Influence of turbulent pressure on solar convective modes Monthly Notices of the Royal Astronomical Society, 204 . pp. 865-881. ISSN 0035-8711
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Official URL: http://articles.adsabs.harvard.edu/cgi-bin/nph-iar...
Abstract
The stability of linear convective modes in the solar envelope model is investigated by incorporating in a very crude manner the effects of turbulent pressure and eddy transport coefficients calculated in the mixing length approximation. It is demonstrated that for a reasonable choice of the parameters there occur two peaks in the growth rate versus horizontal wavenumber plot which correspond to the observed features associated with granulation and supergranulation.
Item Type: | Article |
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Source: | Copyright of this article belongs to John Wiley and Sons. |
ID Code: | 75591 |
Deposited On: | 24 Dec 2011 13:59 |
Last Modified: | 24 Dec 2011 13:59 |
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