Computational modeling of magnetoconvection: effects of discretization method, grid refinement and grid stretching
A. Gelfgat, O. Zikanov

TL;DR
This study investigates the effects of discretization, grid refinement, and grid stretching on the numerical modeling of magnetoconvection in a cubic cavity, providing benchmark results and analyzing magnetic field orientation impacts.
Contribution
It offers a detailed comparison of numerical methods and grid strategies for magnetoconvection, highlighting the importance of grid stretching near boundaries for accurate results.
Findings
Magnetic field orientation significantly influences flow patterns.
Proper grid stretching is crucial for convergence in magnetoconvection simulations.
Magnetic suppression effects depend on the magnetic field direction.
Abstract
The problem of natural convection in a laterally heated three-dimensional cubic cavity under the action of an externally imposed magnetic field is revisited. Flows at the Rayleigh number Ra=10^6 and the Hartmann number Ha=100, and three different orientations of the magnetic field are considered. The problem is solved using two independent numerical methods based on the second order finite-volume discretization schemes on structured Cartesian grids. Convergence toward grid-independent results is examined versus the grid refinement and near-wall grid stretching. Converged benchmark-quality results are obtained. It is shown that for convection flows with a strong magnetic field a steep, sometimes extremely steep, stretching near some of the boundaries is needed. Three-dimensional patterns and integral properties of the converged flow fields are reported and discussed. It is shown that the…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsFluid Dynamics and Turbulent Flows · Solar and Space Plasma Dynamics · Advanced Numerical Methods in Computational Mathematics
