Turbulent eddy viscosity and large-scale convection in the Sun

被引:5
作者
Stothers, RB [1 ]
机构
[1] NASA, Goddard Space Flight Ctr, Inst Space Studies, New York, NY 10025 USA
关键词
convection; turbulence; Sun : granulation; Sun : interior;
D O I
10.1046/j.1365-8711.2000.03499.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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.
引用
收藏
页码:L7 / L9
页数:3
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