The Evolution of Photospheric Magnetic Fields at the Footpoints of Reconnected Structures in the Solar Atmosphere

The Evolution of Photospheric Magnetic Fields at the Footpoints of Reconnected Structures in the Solar Atmosphere

Magnetic reconnection is believed to play an important role in the release and conversion of energy among magnetized plasma systems. So far, we have been unable to understand under what conditions magnetic reconnection can take place. Based on observations from the New Vacuum Solar Telescope and the...

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Bibliographic Details
Main Authors: Tao Ding, Jun Zhang, Yue Fang, Junchao Hong, Yi Bi, Yongyuan Xiang
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
Solar activity
Solar magnetic fields
Solar magnetic reconnection
Online Access:https://doi.org/10.3847/1538-4357/ad245f

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