Responses of the Daytime Low and Equatorial Ionosphere and Thermosphere Over the Indian Region During the Geomagnetic Storm of April 2023

IF 2.6 2区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS Journal of Geophysical Research: Space Physics Pub Date : 2025-03-17 DOI:10.1029/2024JA033141
Lalitha G. Krishnan, Kazuo Shiokawa, Tarun Kumar Pant, Gang Lu, P. R. Shreedevi, Yuichi Otsuka, Surendra Sunda
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Abstract

Study of the response of Thermosphere–Ionosphere (TI) system over the Indian longitude sector during the geomagnetic storm of April 23–24, 2023, is presented. The ionosonde observations at the dip equatorial station, Trivandrum (8.52°N, 77°E, dip lat. = 1.96°N), are found to have unusually high F2 peak plasma density (foF2), with three maxima during the daytime on April 24. The Total Electron Content (TEC) observations from different latitudes showed enhancements temporally progressing from north to south. These features are identified as Traveling Ionospheric Disturbances (TIDs) with speeds ∼400 to 750 m/s. Two major enhancements in TEC observed over Trivandrum were concurrent to the first and third maxima in foF2. Simulations of meridional wind and temperature for this storm were carried out using the Thermosphere–Ionosphere–Electrodynamics General Circulation Model (TIEGCM) that was driven with high-latitude inputs derived from the Assimilative Mapping of Ionospheric Electrodynamics (AMIE) technique. Simulations show the signatures of Traveling Atmospheric Disturbances (TADs) in ionospheric F-region, which conform with the TID observations. The second foF2 peak is found to be simultaneous to the modulation in Prompt Penetration Electric Field (PPEF), which is also observed in the drift of the E-region ionospheric plasma irregularities using an HF radar and the Equatorial Electrojet (EEJ) strength measured by ground-based magnetometer. Simultaneously increasing electric field and foF2 implies the presence of storm-time equatorward wind, inhibiting the plasma fountain. This is the first report comparing comprehensive observations and AMIE-TIEGCM modeling studies of daytime responses of low and equatorial TI during a geomagnetic storm.

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2023 年 4 月地磁暴期间印度地区白天低层和赤道电离层及热层的响应
本文介绍了对 2023 年 4 月 23-24 日地磁风暴期间印度经度扇区上空热层-电离层(TI)系统响应的研究。在特里凡得琅(北纬 8.52°,东经 77°,倾角纬度 = 北纬 1.96°)倾角赤道站的电离层探测仪观测发现,F2 峰等离子体密度(foF2)异常高,4 月 24 日白天有三个最大值。从不同纬度观测到的总电子含量(TEC)显示出从北向南的时间性增强。这些特征被确定为电离层移动扰动(TID),速度为每秒 400 至 750 米。在特里凡得琅上空观测到的两次 TEC 增强与 foF2 的第一和第三次最大值同时出现。使用热层-电离层-电动力学大气环流模式(TIEGCM)对这次风暴的经向风和 温度进行了模拟,该模式由电离层电动力学同化绘图技术得出的高纬度输入驱动。模拟显示了电离层 F 区的移动大气扰动(TAD)特征,与 TID 观测结果一致。发现第二个 foF2 峰值与快速穿透电场(PPEF)的调制同时出现,利用高频雷达和地基磁强计测量的赤道电射流(EEJ)强度也观测到了 E 区电离层等离子体不规则漂移。同时增加的电场和 foF2 意味着风暴时赤道风的存在,从而抑制了等离子体喷泉。这是第一份对地磁暴期间低纬度和赤道 TI 的昼间响应进行综合观测和 AMIE-TIEGCM 建模研究的比较报告。
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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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