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Improved MLT and Its Applications to Solar Models

Published online by Cambridge University Press:  13 May 2016

Y. Li  and
J. Y. Yang
Y. Li
Affiliation:
Yunnan Observatory, NAOCAS, P.O. Box 110, Kunming, 650011 China
J. Y. Yang
Affiliation:
Yunnan Observatory, NAOCAS, P.O. Box 110, Kunming, 650011 China

Abstract

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Based on an improved MLT that takes the anisotropy and dissipation of the turbulence into account, we found that the dissipation of the turbulence in the solar convection zone should be fairly strong, while the turbulence anisotropy plays a less significant role.

Type
Session II: Convection Zone and Local Area Helioseismology
Information
Symposium - International Astronomical Union , Volume 203: Recent Insights into the Physics of the Sun and Heliosphere: Highlights from Soho and Other Space Missions , 2001 , pp. 198 - 201
Copyright
Copyright © Astronomical Society of the Pacific 2001 

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