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An Evolution and Eruption of the Coronal Magnetic Field through a Data-driven MHD Simulation

We present a newly developed data-driven magnetohydrodynamics (MHD) simulation code under a zero- β approximation based on a method proposed by Hayashi et al. 2018 and 2019. Although many data-driven MHD simulations have been developed and conducted, there are not many studies on how accurately thos...

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Autors principals: Satoshi Inoue, Keiji Hayashi, Takahiro Miyoshi
Format: Artigo
Idioma:Inglês
Publicat: IOP Publishing 2023-01-01
Col·lecció:The Astrophysical Journal
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Accés en línia:https://doi.org/10.3847/1538-4357/ac9eaa
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