Marina M. Romanova, Alexander V. Koldoba, Galina V. Ustyugova, Akshay K. Kulkarni, Min Long, Richard V. E. Lovelace
Published 2009-01-27Version 1
We present results of global 3D MHD simulations of disk accretion to a rotating star with dipole and more complex magnetic fields using a Godunov-type code based on the "cubed sphere" grid developed earlier in our group. We describe the code and the grid and show examples of simulation results.
Comments: 7 pages, 3 figures. Proceedings of the 3RD International Conference on Numerical Modeling of Space Plasma Flows (ASTRONUM-2008), June 8-13, 2008, St. John, U.S.V.I
MRI-driven Accretion on to Magnetized stars: Global 3D MHD Simulations of Magnetospheric and Boundary Layer Regimes
Evolution of Massive Protostars via Disk Accretion
Accretion, Outflows, and Winds of Magnetized Stars
![QR code for arXiv:0901.4269 [astro-ph.SR]](http://oss.arxitics.com/images/favicon.svg)