176 citations
- KU LeuvenBE14 papers
- Université Libre de BruxellesBE10 papers
- Politecnico di MilanoIT6 papers
- Centre National de la Recherche ScientifiqueFR5 papers
- École PolytechniqueFR5 papers
- Laboratoire de Physique des PlasmasFR5 papers
- Maria Curie-Skłodowska UniversityPL5 papers
- Universidad Carlos III de MadridES4 papers
- Universidade da CoruñaES4 papers
- University of OttawaCA4 papers
- Centre de Mathématiques Appliquées de l'École polytechniqueFR3 papers
- UCLouvainBE3 papers
6 papers · 1 filter
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…
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…
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…
Self-consistent propagation of flux ropes in realistic coronal simulations
L. Linan, F. Regnault, B. Perri +5
The aim of this paper is to demonstrate the possible use of the new coronal model COCONUT to compute a detailed representation of a numerical CME at 0.1~AU, after its injection at…
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…
Multifluid modeling of magnetosonic wave propagation in the solar chromosphere -- effects of impact ionization and radiative recombination
Yana G. Maneva, Alejandro A. Laguna, Andrea Lani +1
In order to study chromospheric magnetosonic wave propagation including, for the first time, the effects of ion-neutral interactions in the partially ionized solar chromosphere, we…