Northern Crest Weakening Induces Large-Scale Hemispheric EIA Disappearance in GOLD Observations During a Storm

IF 2.9 2区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS
Kun Wu, Liying Qian, Fuliang Xiao, Si Liu, Ji Luo, Xuguang Cai, Guochun Shi
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Abstract

The equatorial ionization anomaly (EIA) is a crucial phenomenon for understanding the ionospheric dynamics. However, the discrepancies in observations from different instruments resulting from the north-south EIA differences remain unreported and understudied. Here, we present the first comprehensive observation of a large-scale single-peak EIA event, detected by the Global-scale Observations of the Limb and Disk (GOLD) mission from longitude ∼−80° to ∼−20° during a storm. However, total electron content (TEC) observations and Whole Atmosphere Community Climate Model-eXtended (WACCM-X) simulations show that the single-peak EIA observed by GOLD is not a real single-peak structure. WACCM-X simulations reveal that the rapid weakening of the northern crest west of 20°W makes the OI 135.6 nm emission undetectable by GOLD, resulting in an unrealistic single-peak EIA in GOLD observations. This weakening is attributed to downward plasma transport by neutral winds dominating over upward plasma transport by E × ${\times} $ B, which lowers the F-region peak electron density height (hmF2) altitude and accelerates recombination. In addition, disturbance dynamo electric field caused by geomagnetic storms should have played an important role in the processes mentioned above. This study reveals unique EIA evolution dynamics and exposes limitations in single-data set observations, establishing multi-instrument validation as essential for EIA characteristic investigations.

Abstract Image

风暴期间北波峰减弱导致大尺度半球EIA消失
赤道电离异常(EIA)是理解电离层动力学的一个重要现象。然而,南北环境影响评估差异造成的不同仪器观测结果的差异仍未得到报告和充分研究。在这里,我们首次对大规模单峰EIA事件进行了全面观测,该事件是由全球尺度的翼盘观测(GOLD)任务在风暴期间从经度~−80°到~−20°探测到的。然而,总电子含量(TEC)观测和全大气群落气候模式扩展(WACCM-X)模拟表明,GOLD观测到的单峰EIA并非真正的单峰结构。WACCM-X模拟表明,20°W以西的北波峰的快速减弱使得OI 135.6 nm发射无法被GOLD探测到,从而导致GOLD观测中的单峰EIA不切实际。这种减弱是由于中性风的下行等离子体输运主导了E × ${\times} $ B的上行等离子体输运,从而降低了f区峰值电子密度高度(hmF2)并加速了复合。此外,地磁风暴引起的扰动发电机电场在上述过程中也起了重要作用。该研究揭示了独特的EIA演化动态,揭示了单数据集观测的局限性,建立了多仪器验证对EIA特征研究至关重要。
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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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