Super Equatorial Plasma Bubbles Observed Over South America During the October 10 and 11, 2024 Strong Geomagnetic Storm

On October 10th, 2024, the second most intense geomagnetic storm of solar cycle 25 to date took place. This storm was triggered by multiple coronal mass ejections (CMEs) that arrived at Earth from October 7th to 9th, causing significant geomagnetic disturbances. The geomagnetic Kp index peaked at its highest level (Kp=9), indicating a red alert status. This study investigated equatorial plasma bubbles (EPBs) over South America during this geomagnetic storm using ground-based Global Navigation Satellite System (GNSS) rate of total electron content index (ROTI) and Global-scale Observations of the Limb and Disk (GOLD)satellite oxygen atom (OI) 135.6 nm radiance wavelength data. The analysis revealed that the EPBs observed in South America lasted for an unusually long duration of approximately 14 hours, from around 23:00 UT (18:00 LT) on October 10th to about 14:00 UT (9:00 LT) on October 11th. Additionally, these super EPBs extended over a wide latitude range, reaching approximately 35 ° N in the north and down to 50 ° S in the south, gradually forming an inverted C-shaped pattern. The observed characteristics of the EPBs are likely associated with changes in solar wind parameters and the effects of the prompt penetration electric field (PPEF).

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Publication Details

Journal
IEEE Geoscience and Remote Sensing Letters
Published
2025-01-01
DOI
https://doi.org/10.1109/lgrs.2025.3603418
Primary Topic
Ionosphere and magnetosphere dynamics
Type
article
Field-Weighted Citation Impact
0.00

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article

Super Equatorial Plasma Bubbles Observed Over South America During the October 10 and 11, 2024 Strong Geomagnetic Storm

Fan Xu, Qiong Ding, Hong Zhang, Yumei Li et al.
IEEE Geoscience and Remote Sensing Letters
Ionosphere and magnetosphere dynamics
article

Super Equatorial Plasma Bubbles Observed Over South America During the October 10 and 11, 2024 Strong Geomagnetic Storm

Fan Xu, Qiong Ding, Hong Zhang, Yumei Li, Long Tang
article en

Abstract

On October 10th, 2024, the second most intense geomagnetic storm of solar cycle 25 to date took place. This storm was triggered by multiple coronal mass ejections (CMEs) that arrived at Earth from October 7th to 9th, causing significant geomagnetic disturbances. The geomagnetic Kp index peaked at its highest level (Kp=9), indicating a red alert status. This study investigated equatorial plasma bubbles (EPBs) over South America during this geomagnetic storm using ground-based Global Navigation Satellite System (GNSS) rate of total electron content index (ROTI) and Global-scale Observations of the Limb and Disk (GOLD)satellite oxygen atom (OI) 135.6 nm radiance wavelength data. The analysis revealed that the EPBs observed in South America lasted for an unusually long duration of approximately 14 hours, from around 23:00 UT (18:00 LT) on October 10th to about 14:00 UT (9:00 LT) on October 11th. Additionally, these super EPBs extended over a wide latitude range, reaching approximately 35 ° N in the north and down to 50 ° S in the south, gradually forming an inverted C-shaped pattern. The observed characteristics of the EPBs are likely associated with changes in solar wind parameters and the effects of the prompt penetration electric field (PPEF).

IEEE Geoscience and Remote Sensing LettersVol. 22
Guangdong University of Technology (CN)
National Natural Science Foundation of China, Guangzhou Municipal Science and Technology Project, Basic and Applied Basic Research Foundation of Guangdong Province
Life below water
Openalex Percentile: Top 84%
Ionosphere and magnetosphere dynamics
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Super Equatorial Plasma Bubbles Observed Over South America During the October 10 and 11, 2024 Strong Geomagnetic Storm — Fan Xu, Qiong Ding, et al. · IEEE Geoscience and Remote Sensing Letters (2025) | TGRS Research Map | TGRS