Understanding the global structure of the September 5, 2022, coronal mass ejection using sunRunner3D

Fast coronal mass ejections (CMEs) drive the most severe geomagnetic storms. In the past, forecasting their properties upstream of the Earth required developing and running complex numerical models. In this study, we present a new global MHD model for initiating and following the evolution of CMEs f...

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Autors principals:	Riley Pete, Ben-Nun Michal, González-Avilés J.J., Palmerio Erika, Török Tibor, Linker Jon A., Kouloumvakos Athanasios, Romeo Orlando M., Ervin Tamar, Sánchez-Cano Beatriz, Varsani Ali, Laky Gunter, Jeszenszky Harald, Orsini Stefano, Milillo Anna, Heyner Daniel, Auster Hans-Ulrich, Richter Ingo, Schmid Daniel, Fischer David
Format:	Artigo
Idioma:	Inglês
Publicat:	EDP Sciences 2025-01-01
Col·lecció:	Journal of Space Weather and Space Climate
Matèries:	coronal mass ejections magnetohydrodynamics heliosphere space weather
Accés en línia:	https://www.swsc-journal.org/articles/swsc/full_html/2025/01/swsc240071/swsc240071.html
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