| |
 |
| 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. |
|
|
|
|
|
