• ISSN 2097-1893
    • CN 10-1855/P

    太阳风动压突减期间赤道电离层驼峰的演化分析

    The responses of equatorial ionization anomaly to the sudden decrease in solar wind dynamic pressure

    • 摘要: 2023年9月12日14:24 UT时刻出现了典型的动压突减现象,其幅度从接近23 nPa短时间内迅速削弱至10 nPa以内,降幅超过50%. 本文使用天地基协同观测体系,联合热层电离层电动力学耦合模型(thermosphere ionosphere electrodynamic general circulation model, TIEGCM)调研了太阳风动压突减造成的赤道电离异常结构(equatorial ionization anomaly, EIA)响应. 动压突减期间,高纬瞬时穿透电场(prompt penetration electric field, PPEF)驱动大尺度低纬西向电场,故MBO台站随后观测到极强的西向赤道电集流. 由于低纬度地磁场磁力线接近水平方向,因此,大尺度西向电场将抑制赤道喷泉效应和EIA驼峰的幅度. 电离层电子密度的响应需要时间来累积,TIEGCM模拟结果显示当动压突减现象形成半小时后,EIA响应具有显著的东西半球差异. 南美洲EIA纬度削弱幅度较强,接近−1×1011 m−3. 同时,大西洋和非洲扇区的EIA响应形成类似上下收紧、中间饱满的波浪状结构:南北半球EIA主体区域削弱但靠赤道侧弱增强,其削弱和增强的平均幅度分别为−5×1010 m−3和2.5×1010 m−3,磁赤道地区电离层电子密度微弱增强了0.5×1010 m−3. EIA响应主要来自垂直E×B漂移的影响,水平E×B漂移、风场、双极扩散以及化学作用的贡献可忽略不计. 动压突减源自太阳风密度和速度的共同作用,本文进一步调研了太阳风密度和速度的定量贡献. 基于全局敏感性分析,该事件中太阳风速度贡献了41.08%,太阳风密度贡献了114.14%,非线性耦合作用占比为−55.22%.

       

      Abstract: A typical event of the sudden decrease in solar wind dynamic pressure (PDyn) is observed at 14:24 universal time (UT) on 12 September 2023. The magnitude drops from ~23 nPa to less than 10 nPa within minutes, with a relative decrease larger than 50%. To ensure the reliability of TIEGCM, a data-model comparison is performed. The responses of EIA to the sudden decrease in PDyn are estimated in this work, which show an obvious east-west hemispheric asymmetry. EIA is significantly reduced in both the American and African regions. However, in the equatorward of EIA latitudes over Africa, it is weakly enhanced. The primary driver of the EIA responses is the westward prompt penetration electric field (PPEF) during the sudden decrease in PDyn. The westward PPEF is simultaneously superposed into the equatorial ionosphere. It drives a downward E×B drift, and suppresses the equatorial fountain effects, hence the generated reduction of EIA. Based on the term analysis in the model, it is found that only vertical E×B drift is responsible for the reduction of EIA during the sudden decrease in PDyn. The roles of neutral winds, horizontal E×B drift, and ambipolar diffusion are ignorable. The sudden decrease in PDyn is controlled by both the density and velocity of the solar wind. The former and the latter account 114.14% and 41.08% in percentage for the EIA responses, respectively. The non-linear coupling processes account −55.22%.

       

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