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2024年5月超级磁暴期间中高纬地区特征性等离子体结构的动态相互作用和演变(“纪念肖佐教授诞辰90周年”专刊)

Shun-Rong Zhang Anthea Coster 阿尔察 Jayachandran P. T. Yongliang Zhang

Shun-Rong Zhang, Anthea Coster, 阿尔察, Jayachandran P. T., Yongliang Zhang. 2024年5月超级磁暴期间中高纬地区特征性等离子体结构的动态相互作用和演变(“纪念肖佐教授诞辰90周年”专刊)[J]. 空间科学学报. doi: 10.11728/cjss2026-0019
引用本文: Shun-Rong Zhang, Anthea Coster, 阿尔察, Jayachandran P. T., Yongliang Zhang. 2024年5月超级磁暴期间中高纬地区特征性等离子体结构的动态相互作用和演变(“纪念肖佐教授诞辰90周年”专刊)[J]. 空间科学学报. doi: 10.11728/cjss2026-0019
Coupled Evolution of Storm-Enhanced Density, Tongue of Ionization, and Polar Ionospheric Hole During the May 10, 2024 Superstorm[J]. Chinese Journal of Space Science. doi: 10.11728/cjss2026-0019
Citation: Coupled Evolution of Storm-Enhanced Density, Tongue of Ionization, and Polar Ionospheric Hole During the May 10, 2024 Superstorm[J]. Chinese Journal of Space Science. doi: 10.11728/cjss2026-0019

2024年5月超级磁暴期间中高纬地区特征性等离子体结构的动态相互作用和演变(“纪念肖佐教授诞辰90周年”专刊)

doi: 10.11728/cjss2026-0019

Coupled Evolution of Storm-Enhanced Density, Tongue of Ionization, and Polar Ionospheric Hole During the May 10, 2024 Superstorm

  • 摘要: This study investigates the concurrent evolution of subauroral storm-enhanced density (SED), the polar tongue of ionization (TOI), and the polar ionospheric hole (PIH) during the May 10, 2024 geomagnetic superstorm. Using global GNSS total electron content (TEC) and TIMED/GUVI thermospheric O/N2 ratio measurements, we focus on the interplay between ionized and neutral density structures at polar latitudes. Our observation exhibited the following scenario that highlights the new understanding of peculiar O/N2 influences on TOI and plasma patches during this storm. (1) With the arrival of the ICME shock and subsequent Interplanetary Magnetic Field (IMF) Bz southward turning,  Prompt Penetration Electric Field (PPEF) drove Equatorial Ionization Anomaly (EIA) crests moving poleward, causing a midlatitude density enhancement. At midlatitude, the poleward  Subauroral Polarization Stream (SAPS) provided significantly intensified sunward flow, while PPEF generated poleward flow, thus the two ion drift components led to the buildup of high electron density, forming the SED base and plume. (2) At noon, the SED plume was entrained into the anti-sunward flow channel toward the polar cap. (3) An unusual dayside PIH was formed as the neutral gas with a depleted O/N2 ratio began circulating in the morning sector toward afternoon. This presumed neutral circulation was primarily driven by the increased ion drag associated with significant storm-time auroral electric fields. (4) Fresh TOI plasma is moving into the polar cap and rotating eastward, with some portion continuing antisunward convecting. Successively following the TOI eastward convection, the PIH also rotates eastward. (5) PIH and TOI continued to be depleted, with TOI being segmented, as the entire polar cap was soaked by the substantially suppressed O/N2 air. The TOI and PIH remained eastward convicting for several hours, including a 2-hour interval of larger positive IMF By.

     

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出版历程
  • 收稿日期:  2026-01-22
  • 录用日期:  2026-04-22
  • 修回日期:  2026-04-01
  • 网络出版日期:  2026-06-16

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