Sequential Ejections of Plasma Blobs Due to Unbraiding of Tangled Loops in the Solar Atmosphere

Sequential Ejections of Plasma Blobs Due to Unbraiding of Tangled Loops in the Solar Atmosphere

Nanoflares, which are consequences of braids in tangled magnetic fields, are an important candidate to heat the solar corona to a million degrees. However, their observational evidence is sparse, and many of their observational characteristics are yet to be discovered. With the high-resolution obser...

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Bibliographic Details
Main Authors: Xiuhui Zuo, Zhenghua Huang, Hengyuan Wei, Chao Zhang, Boyu Sun, Youqian Qi, Hui Fu, Weixin Liu, Mingzhe Sun, Ming Xiong, Lidong Xia
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
Subjects:
Solar atmosphere
Solar coronal heating
Solar transition region
Solar coronal loops
Solar corona
Solar magnetic reconnection
Online Access:https://doi.org/10.3847/1538-4357/adcf1c
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