A Comparative Analysis of High-resolution Shock-capturing Schemes for Two-dimensional Magnetohydrodynamic Simulation of Flux Emergence in the Solar Atmosphere (Son et al., 2025)
Overview
This paper tests how modern high-resolution shock-capturing schemes behave in a classic two-dimensional solar flux-emergence problem. The central issue is not just which method looks sharpest, but which one balances sharp feature capture against physical fidelity in shocks, compression, and magnetic divergence control. Across the full comparison, IMWENO-P emerges as the most convincing choice at fine resolution.
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