MHD Simulation of a Solar Eruption from Active Region 11429 Driven by a Photospheric Velocity Field

Data-driven simulation is becoming an important approach for realistically characterizing the configuration and evolution of solar active regions, revealing the onset mechanism of solar eruption events, and hopefully achieving the goal of accurate space weather forecasting, which is beyond the scope...

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Библиографические подробности

Главные авторы:	Xinyi Wang, Chaowei Jiang, Xueshang Feng
Формат:	Artigo
Язык:	Inglês
Опубликовано:	IOP Publishing 2023-01-01
Серии:	The Astrophysical Journal Letters
Предметы:	Solar coronal mass ejections Solar flares Solar active region magnetic fields Magnetohydrodynamics Magnetohydrodynamical simulations
Online-ссылка:	https://doi.org/10.3847/2041-8213/acaec3
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