Study of Ionospheric Equatorial Plasma Bubbles Based on GOLD Observations

Abstract Using peak electron density data from the Global‐scale Observations of the Limb and Disk (GOLD) imager, equatorial plasma bubbles (EPBs) from October 2018 to December 2022 are identified in this paper. The occurrence characteristics of EPBs is statistically analyzed. The results show that EPBs have strong seasonal and longitudinal variations in the range of longitude −60°–0° and magnetic latitude 25° to −20°: (a) The occurrence of EPBs is highest during the spring and autumn equinoxes and lowest during the summer. (b) Equinox asymmetry is found, that the occurrence of EPBs is much higher in autumn than in spring. (c) A peak in the longitudinal distribution of EPBs is observed, with the highest occurrence occurring between −10° and 0° longitude. Additionally, a second peak is evident at −50° longitude in autumn. The GOLD imager is capable of conducting prolonged observations of EPBs in the same region from space, thereby offering a novel perspective on EPBs.

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Publication Details

Journal
Journal of Geophysical Research Space Physics
Published
2024-09-01
DOI
https://doi.org/10.1029/2024ja032844
Citations
3
Primary Topic
Ionosphere and magnetosphere dynamics
Type
article
Field-Weighted Citation Impact
0.99

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article

Study of Ionospheric Equatorial Plasma Bubbles Based on GOLD Observations

J. H. Zou, Jinbin Cao, Xing Li, Zhipeng Ren
3 citations
Journal of Geophysical Research Space Physics
Ionosphere and magnetosphere dynamics
0.99
article

Study of Ionospheric Equatorial Plasma Bubbles Based on GOLD Observations

J. H. Zou, Jinbin Cao, Xing Li, Zhipeng Ren
article en
3 citations

Abstract

Abstract Using peak electron density data from the Global‐scale Observations of the Limb and Disk (GOLD) imager, equatorial plasma bubbles (EPBs) from October 2018 to December 2022 are identified in this paper. The occurrence characteristics of EPBs is statistically analyzed. The results show that EPBs have strong seasonal and longitudinal variations in the range of longitude −60°–0° and magnetic latitude 25° to −20°: (a) The occurrence of EPBs is highest during the spring and autumn equinoxes and lowest during the summer. (b) Equinox asymmetry is found, that the occurrence of EPBs is much higher in autumn than in spring. (c) A peak in the longitudinal distribution of EPBs is observed, with the highest occurrence occurring between −10° and 0° longitude. Additionally, a second peak is evident at −50° longitude in autumn. The GOLD imager is capable of conducting prolonged observations of EPBs in the same region from space, thereby offering a novel perspective on EPBs.

Journal of Geophysical Research Space PhysicsVol. 129(9)
Chinese Academy of Sciences (CN), Institute of Geology and Geophysics (CN), University of Chinese Academy of Sciences (CN), Beihang University (CN), Ministry of Industry and Information Technology (CN)
National Natural Science Foundation of China, Chinese Academy of Sciences
Openalex Percentile: Top 23%
Ionosphere and magnetosphere dynamics
0.99
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Study of Ionospheric Equatorial Plasma Bubbles Based on GOLD Observations — J. H. Zou, Jinbin Cao, et al. · Journal of Geophysical Research Space Physics (2024) | TGRS Research Map | TGRS