期刊
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
卷 314, 期 1, 页码 L7-L9出版社
BLACKWELL SCIENCE LTD
DOI: 10.1046/j.1365-8711.2000.03499.x
关键词
convection; turbulence; Sun : granulation; Sun : interior
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.
作者
我是这篇论文的作者
点击您的名字以认领此论文并将其添加到您的个人资料中。
推荐
暂无数据