Journal
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 314, Issue 1, Pages L7-L9Publisher
BLACKWELL SCIENCE LTD
DOI: 10.1046/j.1365-8711.2000.03499.x
Keywords
convection; turbulence; Sun : granulation; Sun : interior
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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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