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Nonlinear Modeling of the Solar Tachocline

Published online by Cambridge University Press:  13 May 2016

M. S. Miesch
M. S. Miesch*
Affiliation:
DAMTP, University of Cambridge, Silver St, Cambridge CB3 9EW, UK

Abstract

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As a first step toward a more realistic model of the solar tachocline, we report simulations of rotating, stably-stratified turbulence in a thin spherical shell.

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. 202 - 204
Copyright
Copyright © Astronomical Society of the Pacific 2001 

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