3D MHD Simulations of Disk Accretion onto Magnetized Stars: Numerical Approach and Sample Simulations
Marina M. Romanova, Alexander V. Koldoba, Galina V. Ustyugova, Akshay, K. Kulkarni, Min Long, Richard V.E. Lovelace

TL;DR
This paper introduces a numerical approach for 3D magnetohydrodynamic simulations of disk accretion onto magnetized stars, demonstrating the code's capabilities through sample simulation results.
Contribution
It presents a new Godunov-type numerical code on a cubed sphere grid for simulating 3D MHD disk accretion onto rotating stars with complex magnetic fields.
Findings
Successful implementation of the code for 3D MHD simulations.
Sample simulation results illustrating accretion processes.
Validation of the numerical approach against known scenarios.
Abstract
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.
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Taxonomy
TopicsAstrophysics and Star Formation Studies · Astro and Planetary Science · Solar and Space Plasma Dynamics
