A Finite Element Method for MHD that Preserves Energy, Cross-Helicity, Magnetic Helicity, Incompressibility, and $\operatorname{div} B = 0$
Evan S. Gawlik, Fran\c{c}ois Gay-Balmaz

TL;DR
This paper introduces a finite element method for incompressible MHD that maintains key physical invariants like energy, helicities, and divergence constraints at discrete levels, ensuring accurate and stable simulations.
Contribution
The authors develop a structure-preserving finite element and time-stepping scheme that exactly conserves multiple physical invariants in incompressible MHD simulations.
Findings
Preserves energy, cross-helicity, and magnetic helicity exactly.
Maintains divergence-free magnetic field to machine precision.
Ensures mass and density conservation in discretized form.
Abstract
We construct a structure-preserving finite element method and time-stepping scheme for inhomogeneous, incompressible magnetohydrodynamics (MHD). The method preserves energy, cross-helicity (when the fluid density is constant), magnetic helicity, mass, total squared density, pointwise incompressibility, and the constraint to machine precision, both at the spatially and temporally discrete levels.
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Taxonomy
TopicsComputational Fluid Dynamics and Aerodynamics · Solar and Space Plasma Dynamics · Magnetic confinement fusion research
