Data-driven Modeling of a Coronal Magnetic Flux Rope: From Birth to Death

Magnetic flux ropes are a bundle of twisted magnetic field lines produced by internal electric currents, which are responsible for solar eruptions and are the major drivers of geomagnetic storms. As such, it is crucial to develop a numerical model that can capture the entire evolution of a flux rope...

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מידע ביבליוגרפי

Principais autores:	J. H. Guo, Y. W. Ni, Y. Guo, C. Xia, B. Schmieder, S. Poedts, Z. Zhong, Y. H. Zhou, F. Yu, P. F. Chen
פורמט:	Artigo
שפה:	Inglês
יצא לאור:	IOP Publishing 2024-01-01
סדרה:	The Astrophysical Journal
נושאים:	Magnetohydrodynamical simulations Solar coronal mass ejections Solar magnetic fields Solar flares
גישה מקוונת:	https://doi.org/10.3847/1538-4357/ad088d
תגים:	הוספת תג אין תגיות, היה/י הראשונ/ה לתייג את הרשומה!