MHD Modeling of Solar Coronal Magnetic Evolution Driven by Photospheric Flow

It is well-known that magnetic fields dominate the dynamics in the solar corona, and new generation of numerical modeling of the evolution of coronal magnetic fields, as featured with boundary conditions driven directly by observation data, are being developed. This paper describes a new approach of...

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Bibliographic Details
Main Authors: Chaowei Jiang, Xinkai Bian, Tingting Sun, Xueshang Feng
Format: Article
Language:English
Published: Frontiers Media S.A. 2021-05-01
Series:Frontiers in Physics
Subjects:
Online Access:https://www.frontiersin.org/articles/10.3389/fphy.2021.646750/full