Publication Abstracts
Stothers 2000
, 2000: Turbulent eddy viscosity and large-scale convection in the Sun. Mon. Not. Roy. Astron. Soc., 314, L7-L9, doi:10.1046/j.1365-8711.2000.03499.x.
It is suggested that the laminar character of the large-scale ddeep convective flows appearing in numerical simulaations 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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BibTeX Citation
@article{st04200b,
author={Stothers, R. B.},
title={Turbulent eddy viscosity and large-scale convection in the Sun},
year={2000},
journal={Monthly Notices of the Royal Astronomical Society},
volume={314},
pages={L7--L9},
doi={10.1046/j.1365-8711.2000.03499.x},
}
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RIS Citation
TY - JOUR ID - st04200b AU - Stothers, R. B. PY - 2000 TI - Turbulent eddy viscosity and large-scale convection in the Sun JA - Mon. Not. Roy. Astron. Soc. JO - Monthly Notices of the Royal Astronomical Society VL - 314 SP - L7 EP - L9 DO - 10.1046/j.1365-8711.2000.03499.x ER -
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