Why Do Small‐Scale Irregularities Migrate Beyond the Equatorial Plasma Bubble?

Abstract F‐region Field‐Aligned Irregularities (FAIs) observed by the Hainan Coherent Scatter Phased Array Radar (HCOPAR) and the Equatorial Plasma Bubbles (EPBs) observed by four All‐Sky Airglow Imagers (ASAIs) in the night of 4 November 2023 were compared. The spatiotemporal distribution of the FAIs was nearly consistent with that of the EPBs. However, certain FAIs were located outside the EPBs. Oblique band‐like echoes extended beyond the EPBs between 12:30 and 13:30 UT, with the opposite line‐of‐sight velocities of the echo components above and below. Electrostatic reconnection between adjacent bubbles was considered a driving mechanism for the irregularities extending outward. Between 14:30 and 15:30 UT, certain FAIs were located outside the eastern wall of the bubble. The upward electric field component in the westward tilted bubble will transport the plasma from eastern wall and make the high density gradient region extend outside the bubble, and the irregularities appeared due to the polarization electric field extending outside the bubble.

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Publication Details

Journal
Geophysical Research Letters
Published
2025-07-05
DOI
https://doi.org/10.1029/2024gl114399
Citations
1
Primary Topic
Ionosphere and magnetosphere dynamics
Type
article
Field-Weighted Citation Impact
1.15
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article

Why Do Small‐Scale Irregularities Migrate Beyond the Equatorial Plasma Bubble?

Wanlin Gong, Yuanlin Jia, Gang Chen, Chunxiao Yan et al.
1 citations
Geophysical Research Letters
Ionosphere and magnetosphere dynamics
1.15
article

Why Do Small‐Scale Irregularities Migrate Beyond the Equatorial Plasma Bubble?

Wanlin Gong, Yuanlin Jia, Gang Chen, Chunxiao Yan, Lianhuan Hu, Yimeng Xu, Jiyao Xu, Min Zhang, Pengfei Hu, Shaodong Zhang, Muchen Yang, Wei Jia
article en
1 citations

Abstract

Abstract F‐region Field‐Aligned Irregularities (FAIs) observed by the Hainan Coherent Scatter Phased Array Radar (HCOPAR) and the Equatorial Plasma Bubbles (EPBs) observed by four All‐Sky Airglow Imagers (ASAIs) in the night of 4 November 2023 were compared. The spatiotemporal distribution of the FAIs was nearly consistent with that of the EPBs. However, certain FAIs were located outside the EPBs. Oblique band‐like echoes extended beyond the EPBs between 12:30 and 13:30 UT, with the opposite line‐of‐sight velocities of the echo components above and below. Electrostatic reconnection between adjacent bubbles was considered a driving mechanism for the irregularities extending outward. Between 14:30 and 15:30 UT, certain FAIs were located outside the eastern wall of the bubble. The upward electric field component in the westward tilted bubble will transport the plasma from eastern wall and make the high density gradient region extend outside the bubble, and the irregularities appeared due to the polarization electric field extending outside the bubble.

Geophysical Research LettersVol. 52(13)
Chinese Academy of Sciences (CN), Wuhan University (CN), National Space Science Center (CN), Institute of Geology and Geophysics (CN)
Openalex Percentile: Top 18%
Ionosphere and magnetosphere dynamics
1.15
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Why Do Small‐Scale Irregularities Migrate Beyond the Equatorial Plasma Bubble? — Wanlin Gong, Yuanlin Jia, et al. · Geophysical Research Letters (2025) | TGRS Research Map | TGRS