Formation of Fan-spine Magnetic Topology through Flux Emergence and Subsequent Jet Production

Formation of Fan-spine Magnetic Topology through Flux Emergence and Subsequent Jet Production

Fan-spine magnetic structure, as a fundamental three-dimensional topology in magnetic reconnection theory, plays a crucial role in producing solar jets. However, how fan-spine configurations form in the solar atmosphere remains elusive. Using the Chinese H α Solar Explorer (CHASE) and the Solar Dyna...

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Bibliographic Details
Main Authors: Yadan Duan, Hui Tian, Hechao Chen, Yuandeng Shen, Zheng Sun, Zhenyong Hou, Chuan Li
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal Letters
Subjects:
Solar activity
Solar magnetic flux emergence
Solar magnetic reconnection
Solar magnetic fields
Solar filaments
Online Access:https://doi.org/10.3847/2041-8213/ad24f3

Internet

https://doi.org/10.3847/2041-8213/ad24f3

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