Influence of turbulent pressure on solar convective modes

Astronomy and Astrophysics – Astronomy

Scientific paper

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Convective Flow, Plasma Turbulence, Pressure Effects, Solar Granulation, Mixing Length Flow Theory, Propagation Modes, Solar Atmosphere, Stellar Envelopes, Stellar Models

Scientific paper

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.

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