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Turbulent magnetic reconnection is believed to occur in astrophysical plasmas, and it has been suggested to be a trigger of solar flares. It often occurs in long stretched and fragmented current sheets. Recent observations by the Parker Solar Probe, the Solar Dynamics Observatory and in situ satellite missions agree with signatures expected from turbulent reconnection. However, the underlying mechanisms, including how magnetic energy stored in the Sun s magnetic field is dissipated, remain unclear. Here we demonstrate turbul ...
Ping, Yongli; Zhong, Jiayong; Wang, Xiaogang; Han, Bo; Sun, Wei; Zhang, Yapeng; Yuan, Dawei; Xing, Chunqing; Wang, Jianzhao; Liu, Zhengdong; Zhang, Zhe; Qiao, Bin; Zhang, Hua; Li, Yutong; Zhu, Jianqiang; Zhao, Gang; Zhang, Jie;
Published by: Nature Physics Published on: feb
YEAR: 2023   DOI: 10.1038/s41567-022-01855-x