Geospace response to May 2024 X-class flare and coronal mass ejection

The space weather events from May 8–12, 2024, including solar flares and a coronal mass ejection, significantly impacted the Earth’s magnetosphere, ionosphere and thermosphere system. These events also affected space technologies such as Global Navigation Satellite Systems (GNSS). On the May 10 post-noon period, a large amount of solar wind energy was transferred to the dayside Earth magnetosphere through the southward Bz-directed interplanetary magnetic field (IMF), initiating a sudden storm commencement (SSC) which reached a minimum DST of −412 nT on May 11. A recovery phase was extended to 12 May. The storm was the strongest since 2002. During the storm’s early recovery phase on May 11, there was a negative ionospheric response of the Total Electron Content (TEC) in all six stations, although more pronounced in the mid-latitude stations than the equatorial stations, leading to an improved GNSS positioning accuracy. This negative TEC response could be explained by changes in the composition of ∑ O / N 2 in the thermosphere. In the Southern Hemisphere, the equatorward flow of the predominant N 2 in the thermospheric circulation occurs before it arrives in the Northern Hemisphere.

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Publication Details

Journal
Advances in Space Research
Published
2025-04-17
DOI
https://doi.org/10.1016/j.asr.2025.04.036
Primary Topic
Ionosphere and magnetosphere dynamics
Type
article
Field-Weighted Citation Impact
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article

Geospace response to May 2024 X-class flare and coronal mass ejection

D.M. Moeketsi, Joseph Omojola, K. Greer
1 links
Advances in Space Research
Ionosphere and magnetosphere dynamics
article

Geospace response to May 2024 X-class flare and coronal mass ejection

D.M. Moeketsi, Joseph Omojola, K. Greer
article en

Abstract

The space weather events from May 8–12, 2024, including solar flares and a coronal mass ejection, significantly impacted the Earth’s magnetosphere, ionosphere and thermosphere system. These events also affected space technologies such as Global Navigation Satellite Systems (GNSS). On the May 10 post-noon period, a large amount of solar wind energy was transferred to the dayside Earth magnetosphere through the southward Bz-directed interplanetary magnetic field (IMF), initiating a sudden storm commencement (SSC) which reached a minimum DST of −412 nT on May 11. A recovery phase was extended to 12 May. The storm was the strongest since 2002. During the storm’s early recovery phase on May 11, there was a negative ionospheric response of the Total Electron Content (TEC) in all six stations, although more pronounced in the mid-latitude stations than the equatorial stations, leading to an improved GNSS positioning accuracy. This negative TEC response could be explained by changes in the composition of ∑ O / N 2 in the thermosphere. In the Southern Hemisphere, the equatorward flow of the predominant N 2 in the thermospheric circulation occurs before it arrives in the Northern Hemisphere.

Advances in Space ResearchVol. 76(12)
North-West University (ZA), Federal University Lafia (NG), Laboratory for Atmospheric and Space Physics (US)
Climate action
Openalex Percentile: Top 94%
Ionosphere and magnetosphere dynamics
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