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Paper: A Fictitious Cartesian Grid Technique for the Simulation of 3D Meridional Circulation in Stars
Volume: 293, 3D Stellar Evolution
Page: 25
Authors: Talon, S.; Michaud, G.; Vincent, A.
Abstract: To simulate meridional circulation in the radiative zone of rotating stars, we developed a 3D finite volume, Cartesian code. We discuss the validation of an approach using fictitious points to apply boundary conditions at the star's surface. Preliminary results showing geostrophic balance are presented.
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