activity
20222026
most citedEffects of Mesh Topology on MHD Solution Features in Coronal Simulations

24 citations · 29 across the 5 of their papers we have counts for

collaborators

5 papers

math.NA2026

An improved estimate of the intermediate internal energy in the energy-consistent HLLD scheme

Fan Zhang

The robustness of approximate Riemann solutions has been a crucial topic in computational magnetohydrodynamics, from both theoretical and practical perspectives. Recently, the wide…

astro-ph.SR2026

COCONUT: Toward practical time-evolving Sun-to-Earth magnetohydrodynamic modeling

Haopeng Wang, Stefaan Poedts, Andrea Lani +16

Due to computational efficiency and numerical stability limitations, coronal simulations constrained by static magnetograms are typically performed first and then used to drive inn…

physics.flu-dyn2025

On energy consistency of intermediate states in HLL-type MHD Riemann solvers

Fan Zhang, Andrea Lani, Stefaan Poedts

Approximate Riemann solvers are widely used for solving hyperbolic conservation laws, including those of magnetohydrodynamics (MHD). However, due to the nonlinearity and complexity…

astro-ph.SR2025★ 5 cited

Time-evolving coronal modelling of the solar maximum around the solar storms in May 2024 by COCONUT

Haopeng Wang, Stefaan Poedts, Andrea Lani +8

Time-evolving MHD coronal models deliver more realistic results than traditional quasi-steady-state models. The fully implicit time-evolving coronal model COCONUT performs efficien…

astro-ph.SR2022★ 24 cited

Effects of Mesh Topology on MHD Solution Features in Coronal Simulations

Michaela Brchnelova, Fan Zhang, Peter Leitner +3

Magnetohydrodynamic (MHD) simulations of the solar corona have become more popular with the increased availability of computational power. Modern computational plasma codes, relyin…