2 papers
astro-ph.SR2025
Efficient magnetohydrodynamic modelling of the time-evolving corona by COCONUT
Haopeng Wang, Stefaan Poedts, Andrea Lani +6
Compared to quasi-steady-state corona models that are constrained by a time-invariant magnetogram over a CR period, time-evolving corona models driven by time-varying photospheric…
astro-ph.SR2025
SIP-IFVM: Efficient time-accurate magnetohydrodynamic model of the corona and coronal mass ejections
H. P. Wang, J. H. Guo, L. P. Yang +7
In this paper, we present an efficient and time-accurate three-dimensional (3D) single-fluid MHD solar coronal model and employ it to simulate CME evolution and propagation. Based…