{"title":"2024 年 5 月超级风暴期间场对齐电流和极地电射流的本地时间和半球不对称现象","authors":"Hui Wang, Qihang Cheng, Hermann Lühr, Yunfang Zhong, Kedeng Zhang, Hao Xia","doi":"10.1029/2024JA033020","DOIUrl":null,"url":null,"abstract":"<p>This study examines field-aligned currents (FACs) and polar electrojet (PEJ) characteristics during the extreme May 2024 geomagnetic storms across dawn, dusk, daytime, and nighttime in both hemispheres. FACs and PEJ intensities were up to 9 times greater than usual, with equatorward FACs reaching −44° Magnetic Latitude. Maximum FACs and PEJ are larger at dawn than dusk in the Northern Hemisphere but larger at dusk than at dawn in the Southern Hemisphere. Dawn and duskside FACs correlate best with Dst or solar wind dynamic pressure (Pd) in both hemispheres. On the dayside (nightside), most FACs in both hemispheres are primarily correlated with Pd (merging electric field, Em or Pd). The PEJs correlate largely with Dst and partly with Em and Pd. Duskside (nighttime) currents are located at lower latitudes than dawnside (daytime), and northern currents are positioned more poleward than southern currents. The latitudes of peak FACs are most strongly correlated with Dst or Pd in both hemispheres. However, in the northern daytime sector, they are primarily influenced by Em. The latitudes of peak PEJ show the strongest correlation with Dst or Pd in both hemispheres, except on the northern dawnside, where they are primarily influenced by Em. The qualitative relationships between peak current density, corresponding latitude, solar wind parameters, and the Dst index are derived.</p>","PeriodicalId":15894,"journal":{"name":"Journal of Geophysical Research: Space Physics","volume":"129 11","pages":""},"PeriodicalIF":2.6000,"publicationDate":"2024-11-07","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Local Time and Hemispheric Asymmetries of Field-Aligned Currents and Polar Electrojet During May 2024 Superstorm Periods\",\"authors\":\"Hui Wang, Qihang Cheng, Hermann Lühr, Yunfang Zhong, Kedeng Zhang, Hao Xia\",\"doi\":\"10.1029/2024JA033020\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<p>This study examines field-aligned currents (FACs) and polar electrojet (PEJ) characteristics during the extreme May 2024 geomagnetic storms across dawn, dusk, daytime, and nighttime in both hemispheres. FACs and PEJ intensities were up to 9 times greater than usual, with equatorward FACs reaching −44° Magnetic Latitude. Maximum FACs and PEJ are larger at dawn than dusk in the Northern Hemisphere but larger at dusk than at dawn in the Southern Hemisphere. Dawn and duskside FACs correlate best with Dst or solar wind dynamic pressure (Pd) in both hemispheres. On the dayside (nightside), most FACs in both hemispheres are primarily correlated with Pd (merging electric field, Em or Pd). The PEJs correlate largely with Dst and partly with Em and Pd. Duskside (nighttime) currents are located at lower latitudes than dawnside (daytime), and northern currents are positioned more poleward than southern currents. The latitudes of peak FACs are most strongly correlated with Dst or Pd in both hemispheres. However, in the northern daytime sector, they are primarily influenced by Em. The latitudes of peak PEJ show the strongest correlation with Dst or Pd in both hemispheres, except on the northern dawnside, where they are primarily influenced by Em. The qualitative relationships between peak current density, corresponding latitude, solar wind parameters, and the Dst index are derived.</p>\",\"PeriodicalId\":15894,\"journal\":{\"name\":\"Journal of Geophysical Research: Space Physics\",\"volume\":\"129 11\",\"pages\":\"\"},\"PeriodicalIF\":2.6000,\"publicationDate\":\"2024-11-07\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Journal of Geophysical Research: Space Physics\",\"FirstCategoryId\":\"89\",\"ListUrlMain\":\"https://onlinelibrary.wiley.com/doi/10.1029/2024JA033020\",\"RegionNum\":2,\"RegionCategory\":\"地球科学\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q2\",\"JCRName\":\"ASTRONOMY & ASTROPHYSICS\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Journal of Geophysical Research: Space Physics","FirstCategoryId":"89","ListUrlMain":"https://onlinelibrary.wiley.com/doi/10.1029/2024JA033020","RegionNum":2,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0
摘要
本研究考察了 2024 年 5 月极端地磁暴期间两个半球黎明、黄昏、白天和夜间的场对准电流(FACs)和极地电射流(PEJ)特征。FACs和PEJ强度比平时高出9倍,赤道方向的FACs达到-44°磁纬度。在北半球,黎明时的FAC和PEJ最大值大于黄昏时,但在南半球,黄昏时的FAC和PEJ最大值大于黎明时。在两个半球,黎明和黄昏的 FAC 与 Dst 或太阳风动压(Pd)的相关性最好。在日侧(夜侧),两个半球的大多数 FAC 主要与 Pd(合并电场,Em 或 Pd)相关。PEJ 主要与 Dst 相关,部分与 Em 和 Pd 相关。黄昏(夜间)洋流的纬度比黎明(白天)洋流的纬度低,北方洋流的位置比南方洋流的位置更靠极。在两个半球,FACs 峰值的纬度与 Dst 或 Pd 的相关性最强。然而,在北部的白天区,它们主要受 Em 的影响。PEJ 峰值的纬度在两个半球都与 Dst 或 Pd 的相关性最强,但在北部黎明区,它们主要受 Em 的影响。得出了峰值电流密度、相应纬度、太阳风参数和 Dst 指数之间的定性关系。
Local Time and Hemispheric Asymmetries of Field-Aligned Currents and Polar Electrojet During May 2024 Superstorm Periods
This study examines field-aligned currents (FACs) and polar electrojet (PEJ) characteristics during the extreme May 2024 geomagnetic storms across dawn, dusk, daytime, and nighttime in both hemispheres. FACs and PEJ intensities were up to 9 times greater than usual, with equatorward FACs reaching −44° Magnetic Latitude. Maximum FACs and PEJ are larger at dawn than dusk in the Northern Hemisphere but larger at dusk than at dawn in the Southern Hemisphere. Dawn and duskside FACs correlate best with Dst or solar wind dynamic pressure (Pd) in both hemispheres. On the dayside (nightside), most FACs in both hemispheres are primarily correlated with Pd (merging electric field, Em or Pd). The PEJs correlate largely with Dst and partly with Em and Pd. Duskside (nighttime) currents are located at lower latitudes than dawnside (daytime), and northern currents are positioned more poleward than southern currents. The latitudes of peak FACs are most strongly correlated with Dst or Pd in both hemispheres. However, in the northern daytime sector, they are primarily influenced by Em. The latitudes of peak PEJ show the strongest correlation with Dst or Pd in both hemispheres, except on the northern dawnside, where they are primarily influenced by Em. The qualitative relationships between peak current density, corresponding latitude, solar wind parameters, and the Dst index are derived.