East–West Difference in the Ionospheric Response During the Recovery Phase of May 2024 Super Geomagnetic Storm Over the East Asian

IF 2.6 2区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS Journal of Geophysical Research: Space Physics Pub Date : 2024-09-17 DOI:10.1029/2024JA033170
Xu Guo, Biqiang Zhao, Tingting Yu, Honglian Hao, Wenjie Sun, Guojun Wang, Maosheng He, Tian Mao, Guozhu Li, Zhipeng Ren
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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]/[N2] 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]/[N2].

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2024 年 5 月东亚上空超级地磁暴恢复阶段电离层响应的东西差异
在本研究中,我们对2024年5月超级风暴期间的F区电离层扰动进行了广泛研究,主要侧重于东亚的中低纬度地区。我们的分析以大量数据源为基础,包括电子总含量(TEC)、电离层参数 NmF2 和 hmF2、无线电掩星数据获取的电子密度剖面(EDP)以及全球紫外线成像仪(GUVI)获取的∑[O]/[N2]等,并辅以模型模拟。观测到的负电离层风暴效应的特点是整个中国的电子密度显著而持久地降低,在 5 月 10 日风暴突然开始后立即开始,并持续到 5 月 11 日风暴的主要阶段和早期恢复阶段。5 月 11 日至 12 日,从后半夜到日出,最初在有限的地理区域观测到正电离层暴风影 响,首先表现在中国东部地区,然后转移到中部地区。随后,在整个恢复阶段的后期,持续出现了明显的负风暴效应。与此相反,中国西部地区在 5 月 12 日出现了正暴雨效应,随后出现了相对温和的负暴雨阶段。整个东亚地区电子密度的这种持续广泛的地带性梯度类似于以前热层环流模式引起的超级风暴所描述的情况。该地区电离层从东到西的反应差异可能是超级风暴期间的一个共同特征,可能是∑[O]/[N2]升高的拱形结构造成的。
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来源期刊
Journal of Geophysical Research: Space Physics
Journal of Geophysical Research: Space Physics Earth and Planetary Sciences-Geophysics
CiteScore
5.30
自引率
35.70%
发文量
570
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