Numerical Simulation of Solar Magnetic Flux Emergence Using the AMR–CESE–MHD Code

Numerical Simulation of Solar Magnetic Flux Emergence Using the AMR–CESE–MHD Code

Magnetic flux emergence from the solar interior to the atmosphere is believed to be a key process in the formation of solar active regions and driving solar eruptions. Due to the limited capabilities of observations, the flux emergence process is commonly studied using numerical simulations. In this...

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Bibliographic Details
Main Authors: Zhipeng Liu, Chaowei Jiang, Xueshang Feng, Pingbing Zuo, Yi Wang
Format: Article
Language:English
Published: IOP Publishing 2022-01-01
Series:The Astrophysical Journal Supplement Series
Subjects:
Solar corona
Solar magnetic fields
Magnetohydrodynamics
Solar active regions
Magnetohydrodynamical simulations
Online Access:https://doi.org/10.3847/1538-4365/ac9d2b

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