5 citations
- Centre National de la Recherche ScientifiqueFR1 paper
- KU LeuvenBE1 paper
- Kyung Hee UniversityKR1 paper
- LIRA - Laboratoire d'instrumentation et de recherche en astrophysiqueFR1 paper
- Maria Curie-Skłodowska UniversityPL1 paper
- National Space Science CenterCN1 paper
- Observatoire de ParisFR1 paper
- University of GlasgowGB1 paper
- University of OsloNO1 paper
- Von Karman Institute for Fluid DynamicsBE1 paper
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astro-ph.SR2026★ 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.SR2025★ 2 cited
Investigating the impact of the dynamic solar wind on the propagation of a coronal mass ejection with two models and multi-spacecraft measurements
Tinatin Baratashvili, Emma Davies, Eva Weiler +3
Coronal mass ejections (CMEs) are the main drivers of disturbances in the solar heliosphere because they propagate and interact with the magnetic field of the solar wind. It is cru…