On the numerical convergence of MRI simulations
Thomas Jannaud, Henrik N. Latter

TL;DR
This paper critically examines the common use of the MRI quality factor as a convergence indicator in simulations, demonstrating its limitations and proposing a modified metric for better assessment.
Contribution
The authors identify shortcomings of the MRI quality factor in convergence tests and introduce a revised metric to improve the reliability of MRI simulation analysis.
Findings
The MRI quality factor often fails to indicate convergence in zero-net-flux simulations.
Linear MRI theory assumptions do not hold in nonlinear, variable magnetic field conditions.
A modified quality factor is proposed to better assess numerical convergence in MRI simulations.
Abstract
The magnetorotational instability (MRI) plays a crucial role in the evolution of many types of accretion disks. It is often studied using ideal-MHD numerical simulations. In principle, such simulations should be numerically converged, i.e. their properties should not change with resolution. Convergence is often assessed via the MRI quality factor, , the ratio of the Alfv\'en length to the grid-cell size. If it is above a certain threshold, the simulation is deemed numerically converged. In this paper we argue that the quality factor is not a good indicator of numerical convergence. First, we test the performance of the quality factor on simulations known to be unconverged, i.e. local ideal-MHD simulations with zero net-flux, and show that their s are well over the typical convergence threshold. The quality-factor test thus fails in these cases. Second, we take issue with the…
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Taxonomy
TopicsAstrophysics and Star Formation Studies · Astrophysical Phenomena and Observations · Astronomy and Astrophysical Research
