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Nonlinear Modeling of the Solar Tachocline
Published online by Cambridge University Press: 13 May 2016
Abstract
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.
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- Session II: Convection Zone and Local Area Helioseismology
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- Copyright © Astronomical Society of the Pacific 2001