| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 4637861 | Journal of Computational and Applied Mathematics | 2016 | 13 Pages |
Abstract
Fast advection in rotating gaseous objects (FARGO, Masset (2000)) algorithm has been widely used in simulating disk-type object in computational astrophysics. In this paper, we revisit this algorithm and propose some improvement. We also propose a semi-Lagrangian adaptive mesh refinement for this algorithm to enhance resolution locally near the embedded proto-planet. Numerical tests are provided to demonstrate the effectiveness of our method.
Related Topics
Physical Sciences and Engineering
Mathematics
Applied Mathematics
Authors
Shengtai Li, Hui Li,