Internal Activities in a Solar Filament and Heating in Its Threads

Internal Activities in a Solar Filament and Heating in Its Threads

Filaments are one of the most common features in the solar atmosphere and are of significance in solar, stellar, and laboratory plasma physics. Using data from the Chinese H α Solar Explorer, the Solar Upper Transition Region Imager, and the Solar Dynamics Observatory, we report on multiwavelength i...

Full description

Bibliographic Details
Main Authors: Hengyuan Wei, Zhenghua Huang, Chuan Li, Zhenyong Hou, Ye Qiu, Hui Fu, Xianyong Bai, Lidong Xia
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astrophysical Journal
Subjects:
Solar physics
Solar atmosphere
Solar corona
Solar magnetic reconnection
Solar filaments
Astronomy data analysis
Online Access:https://doi.org/10.3847/1538-4357/acf569

Internet

https://doi.org/10.3847/1538-4357/acf569

Similar Items