QR Code

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...

Description complète

Enregistré dans:
Détails bibliographiques
Auteurs principaux: Nian Liu, Satoshi Inoue, Ying Wang, Haimin Wang
Format: Artigo
Langue:Inglês
Publié: IOP Publishing 2025-01-01
Collection:The Astrophysical Journal
Sujets:
Accès en ligne:https://doi.org/10.3847/1538-4357/adba56
Tags: Ajouter un tag
Pas de tags, Soyez le premier à ajouter un tag!