Influence of turbulent pressure on solar convective modes
- 1 October 1983
- journal article
- research article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 204 (3) , 865-881
- https://doi.org/10.1093/mnras/204.3.865
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 wave-number plot which correspond to the observed features associated with granulation and super granulation.Keywords
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