Data-constrained Magnetohydrodynamic Simulation for Magnetic Flux Rope Eruptions Driven by Magnetic Reconnection

We conducted data-constrained magnetohydrodynamic (MHD) simulations for solar active region (AR) NOAA AR 11429, which produced two X-class flares within a span of 63 minutes. The simulations were performed using the zero- β MHD approximation, with the initial condition derived from the nonlinear for...

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Detalhes bibliográficos

Principais autores:	Nian Liu, Satoshi Inoue, Ying Wang, Haimin Wang
Formato:	Artigo
Idioma:	Inglês
Publicado em:	IOP Publishing 2025-01-01
coleção:	The Astrophysical Journal
Assuntos:	Solar flares Magnetohydrodynamics Solar active region magnetic fields Magnetohydrodynamical simulations
Acesso em linha:	https://doi.org/10.3847/1538-4357/adba56
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