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.
Authors
- D.M. Moeketsi (ORCID: https://orcid.org/0000-0002-1619-3594)
- Joseph Omojola
- K. Greer (ORCID: https://orcid.org/0000-0003-4435-4778)
Institutions
- North-West University (ZA)
- Federal University Lafia (NG)
- Laboratory for Atmospheric and Space Physics (US)
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
- 0.00