Turbulent eddy viscosity and large-scale convection in the Sun

Details Turbulent eddy viscosity and large-scale convection in the Sun Turbulent eddy viscosity and large-scale convection in the Sun

May 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000mnras.314l...7s&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 314, Issue 1, pp. L7-L9.

Astronomy and Astrophysics

Astronomy

4

Convection, Turbulence, Sun: Granulation, Sun: Interior

Scientific paper

It is suggested here that the laminar character of the large-scale deep
convective flows appearing in numerical simulations of the convective
envelope of the Sun arises from the effect of turbulent eddy viscosity.
Previously, M. Schwarzschild suggested the same idea to explain the
observed surface granulation in the Sun.

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