太阳极小期强地磁风暴恢复阶段在小于30°经度的海面上发生的显著的东西电子密度差异

IF 2.9 2区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS Journal of Geophysical Research: Space Physics Pub Date : 2025-01-23 DOI:10.1029/2024JA033549
Jiawei Kuai, Qiaoqiao Ma, Tingting Yu, Kun Wu, Hao Sun, Yedan Zhang
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引用次数: 0

摘要

我们于2021年5月12日对地磁风暴的电离层响应进行了观测研究。选取了3个气象、电离层和气候-2星座观测系统(COSMIC-2)观测到的电子密度高度剖面图在小于30°经度范围内存在显著纵向差异的案例。这些病例发生在大西洋上空和风暴恢复阶段。三种情况下,在干扰和安静时间之间,西侧的变化相对较弱(<10%),而东侧的正/负电子密度变化明显(高达100%)。GOLD和ICON观测表明,热层成分在纵向差异中起次要作用,而中性风和扰动电场起主要作用。此外,还观察到E×B漂移和中性风的显著纵向差异,这将是未来工作的一部分。这项研究提供了对海洋上空30度经度范围内电离层响应的独特见解。
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Significant East-West Electron Density Differences Occurring in Less Than 30° Longitude Over the Ocean During the Recovery Phase of a Strong Geomagnetic Storm in Solar Minimum

We conducted observational studies of ionospheric responses to the geomagnetic storm on 12 May 2021. We selected three cases that the electron density altitude profiles observed by Constellation Observing System for Meteorology, Ionosphere, and Climate-2 (COSMIC-2) exhibited significant longitudinal differences in less than 30° longitudes. These cases occurred over the Atlantic Ocean and during the storm's recovery phase. All three cases show relatively weaker variations on the west side between disturbed and quiet time (<10%), while displaying pronounced positive/negative electron density variations on the east side (as large as 100%). GOLD and ICON observations illustrate that the thermospheric composition plays a minor role in the longitudinal differences, while neutral winds and disturbed electric fields make major contributions. Furthermore, significant longitudinal differences in E×B drift and neutral winds have also been observed, which will be part of the future work. This study provides unique insights into ionospheric responses within 30-degree longitude range over the ocean.

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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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