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...
Saved in:
| 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 |
| Subjects: | |
| Online Access: | https://doi.org/10.1029/2025SW004435 |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
How Do Space Hurricanes Disturb the Polar Thermosphere: A Statistical Survey
by: Zhi‐Feng Xiu, et al.
Published: (2025-04-01) -
Statistical Analysis of the Occurrence of Ionospheric Scintillations at the Low-Latitude Sanya Station During 2004–2021
by: Bo Xiong, et al.
Published: (2024-12-01) -
Observations of three-dimensional ionospheric plasma properties in a space hurricane
by: Sheng Lu, et al.
Published: (2024-12-01) -
A comparison between large‐scale irregularities and scintillations in the polar ionosphere
by: Y. Wang, et al.
Published: (2016-05-01) -
Occurrence of ionospheric scintillation during geomagnetic storms in Indonesia (2003–2024) using superposed epoch analysis
by: Angga Yolanda Putra, et al.
Published: (2025-07-01)