Impact of the May 2024 Extreme Geomagnetic Storm on the Ionosphere and GNSS Positioning

Global navigation satellite systems provide important data sets that can be used to study the influence of various space weather factors. We analyzed the effects of the main phase of the May 2024 extreme geomagnetic storm on the ionosphere and GPS kinematic precise point positioning (PPP). ROTI and global ionospheric maps showed the ionospheric dynamics. The auroral oval expanded up to low latitudes: up to 30°N in the American sector and up to 45°N in the European–Asian sector during the main phase of the geomagnetic storm. The ROTI peaked at 2 TECU/min, which is four times as much against the background. The equatorial anomaly crest intensified considerably (up to 200 TECU) and shifted poleward in the American sector. The counter-propagation finally caused the equatorial anomaly to cross the auroral oval boundary. The ROTI correlated with errors in the kinematic PPP. Positioning errors increased 1.5–5 times at the boundary of the auroral oval. Increased positioning errors propagated according to the shift of the auroral oval boundary. The geomagnetic storm significantly affected the positioning and the ionosphere, threatening various applications based on navigation and communication.

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Publication Details

Journal
Remote Sensing
Published
2025-04-23
DOI
https://doi.org/10.3390/rs17091492
Citations
17
Primary Topic
Ionosphere and magnetosphere dynamics
Type
article
Field-Weighted Citation Impact
19.63

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Impact of the May 2024 Extreme Geomagnetic Storm on the Ionosphere and GNSS Positioning

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article

Impact of the May 2024 Extreme Geomagnetic Storm on the Ionosphere and GNSS Positioning

Yury Yasyukevich, Ekaterina Danilchuk, Артем Веснин, Baocheng Zhang, Aleksandr Klyusilov
article en
17 citations

Abstract

Global navigation satellite systems provide important data sets that can be used to study the influence of various space weather factors. We analyzed the effects of the main phase of the May 2024 extreme geomagnetic storm on the ionosphere and GPS kinematic precise point positioning (PPP). ROTI and global ionospheric maps showed the ionospheric dynamics. The auroral oval expanded up to low latitudes: up to 30°N in the American sector and up to 45°N in the European–Asian sector during the main phase of the geomagnetic storm. The ROTI peaked at 2 TECU/min, which is four times as much against the background. The equatorial anomaly crest intensified considerably (up to 200 TECU) and shifted poleward in the American sector. The counter-propagation finally caused the equatorial anomaly to cross the auroral oval boundary. The ROTI correlated with errors in the kinematic PPP. Positioning errors increased 1.5–5 times at the boundary of the auroral oval. Increased positioning errors propagated according to the shift of the auroral oval boundary. The geomagnetic storm significantly affected the positioning and the ionosphere, threatening various applications based on navigation and communication.

Remote SensingVol. 17(9)
Chinese Academy of Sciences (CN), Institute of Solar-Terrestrial Physics (RU), Institute of Geodesy and Geophysics (CN), Irkutsk State University (RU)
Russian Science Foundation, Istituto Nazionale di Geofisica e Vulcanologia, University of California, San Diego
Openalex Percentile: Top 1%
Ionosphere and magnetosphere dynamics
19.63
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