Ionospheric Scintillation and Geomagnetic Disturbance Caused by Space Hurricanes

Abstract A space hurricane is a large‐scale, cyclone‐shaped aurora characterized by a rotating magnetic structure and shears in plasma convection, driven by high‐latitude magnetic reconnection. It typically forms near the magnetic poles in summertime, providing an efficient energy transport channel...

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Bibliographic Details
Main Authors: Sheng Lu, Zan‐Yang Xing, Qing‐He Zhang, Yong‐Liang Zhang, Hui‐Gen Yang, Kjellmar Oksavik, L. R. Lyons, Kazuo Shiokawa, Yong Wang, Yu‐Zhang Ma, Xiang‐Yu Wang, Tong Xu, Shu‐Ji Sun, Duan Zhang
Format: Article
Language:English
Published: Wiley 2025-07-01
Series:Space Weather
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Online Access:https://doi.org/10.1029/2025SW004435
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