Formation of an Intermediate Filament Driven by Small-scale Magnetic Reconnection

Formation of an Intermediate Filament Driven by Small-scale Magnetic Reconnection

We present the formation process of a filament in NOAA active region 12765 from 2020 June 5 to 8, using observations from the New Vacuum Solar Telescope, the Solar Dynamics Observatory, and the Global Oscillation Network Group. We found that intermittent small-scale magnetic reconnection occurs at t...

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Bibliographic Details
Main Authors: Xia Sun, Xiaoli Yan, Hongfei Liang, Zhike Xue, Jincheng Wang, Liheng Yang, Zhe Xu, Liping Yang, Yang Peng, Qiaoling Li, Zihan li, Xinsheng Zhang
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astrophysical Journal
Subjects:
Solar filaments
Solar activity
Solar magnetic reconnection
Solar magnetic fields
Online Access:https://doi.org/10.3847/1538-4357/acaa3e

Internet

https://doi.org/10.3847/1538-4357/acaa3e

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