East–West Difference in the Ionospheric Response During the Recovery Phase of May 2024 Super Geomagnetic Storm Over the East Asian
Abstract In this study, we offer an extensive examination of the F‐region ionospheric disturbances during the May 2024 superstorm, focusing primarily on the middle‐low latitude regions of East Asia. Our analysis is grounded in a wealth of data sources including Total Electron Content (TEC), ionospheric parameters NmF2 and hmF2, Electron Density Profile (EDP) retrieved from Radio Occultation (RO) data, and ∑[O]/[N 2 ] from the Global Ultraviolet Imager (GUVI), among others, complemented by model simulations. The observed negative ionospheric storm effect, characterized by a significant and long‐lasting reduction in electron density across the entire China, commenced immediately following the sudden storm commencement (SSC) on 10 May and continued through the main and early recovery phase of the storm on 11 May. On 11–12 May, positive ionospheric storm impacts were initially observed in a restricted geographical area from the post‐midnight to sunrise, first manifesting over the eastern regions of China and then shifting to the central regions. Subsequently, a pronounced negative storm effect persisted throughout the later stages of recovery phase. In contrast, the western regions of China experienced a positive storm effect on 12 May followed by a comparatively mild negative storm phase. This persistent extensive zonal gradient in electron density across the East Asian region resembles the scenarios depicted in prior superstorms attributed to the thermospheric circulation patterns. The disparity in the ionospheric response from east to west in this area is probably a common feature during superstorms, potentially resulting from an arch‐shaped structure of elevated ∑[O]/[N 2 ].
Authors
- Tingting Yu (ORCID: https://orcid.org/0000-0003-3926-6829)
- Wenjie Sun (ORCID: https://orcid.org/0000-0003-3129-5350)
- Xu Guo (ORCID: https://orcid.org/0000-0001-8711-5449)
- Guozhu Li (ORCID: https://orcid.org/0000-0002-7669-3590)
- Honglian Hao (ORCID: https://orcid.org/0000-0002-1092-4165)
- Maosheng He (ORCID: https://orcid.org/0000-0001-6112-2499)
- Tian Mao (ORCID: https://orcid.org/0000-0001-7340-811X)
- Guojun Wang (ORCID: https://orcid.org/0000-0003-2401-5816)
- Biqiang Zhao (ORCID: https://orcid.org/0000-0002-0553-9473)
- Zhipeng Ren (ORCID: https://orcid.org/0000-0002-9935-7071)
Institutions
- China Meteorological Administration (CN)
- Chinese Academy of Sciences (CN)
- National Space Science Center (CN)
- Institute of Geology and Geophysics (CN)
- University of Chinese Academy of Sciences (CN)
Publication Details
- Journal
- Journal of Geophysical Research Space Physics
- Published
- 2024-09-01
- DOI
- https://doi.org/10.1029/2024ja033170
- Citations
- 39
- Primary Topic
- Ionosphere and magnetosphere dynamics
- Type
- article
- Field-Weighted Citation Impact
- 12.93
Funders
- National Natural Science Foundation of China
- Chinese Academy of Sciences
- Youth Innovation Promotion Association of the Chinese Academy of Sciences