A finite volume code for meridional circulation in stars.

DOI10.1016/S0021-9991(02)00029-3zbMath1040.85002OpenAlexW1981480161MaRDI QIDQ1869851

Suzanne Talon, Georges Michaud, Jacques Richer, A. P. Vincent

Publication date: 28 April 2003

Published in: Journal of Computational Physics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1016/s0021-9991(02)00029-3

Mathematics Subject Classification ID

Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30)

Uses Software

• Djehuty

Cites Work

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• Development of the mask method for incompressible unsteady flows
• Boundary conditions for direct simulations of compressible viscous flows
• An accurate Cartesian grid method for viscous incompressible flows with complex immersed boundaries
• A Cartesian grid finite-volume method for the advection-diffusion equation in irregular geometries
• DIFFUSE-INTERFACE METHODS IN FLUID MECHANICS
• A Generalization of the Mixing-Length Theory of Turbulent Convection.
• The Importance of Rotation in Stellar Evolution
• Rotation and Stellar Evolution
• A sharp interface Cartesian grid method for simulating flows with complex moving boundaries

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