27–31 Oct 2025
Europe/Stockholm timezone

Subauroral and Auroral Conditions in the Mid- and Low-Midlatitude Ionosphere over Europe During the May 2024 Mother’s Day Superstorm

Not scheduled
15m
Mon 27/10: Idun - Tue 28/10, Wed 29/10: Studion

Mon 27/10: Idun - Tue 28/10, Wed 29/10: Studion

Poster SWR4 - Interactions in the Earth’s Magnetosphere-Ionosphere-Thermosphere System and their Space Weather Impact SWR4 –Interactions in the Earth’s Magnetosphere-Ionosphere-Thermosphere System and their Space Weather Impact

Speaker

Veronika Barta (HUN-REN Institute of Earth Physics and Space Science)

Description

This study focuses on the mid- and low-midlatitude ionospheric response to the 2024 Mother’s Day superstorm, utilizing ground-based and Swarm satellite observations. The ground-based ionosonde measured F1, F2-layer, B0 and B1 parameters, as well as isodensity data, were used. The ionospheric absorption was investigated with the so-called amplitude method, which is based on ionosonde data. Auroral sporadic E-layer was the first time ever recorded at Sopron. Moreover, the auroral F-layer appeared at exceptionally low latitude (35◦ mlat, over San Vito) during the storm main phase. These unprecedented detections were confirmed by optical all-sky cameras. The observations revealed that these events were linked to the extreme equatorward shift of the auroral oval along with the midlatitude trough. As a result, the midlatitude ionosphere became confined to the trough itself. Three stages of F2-layer uplift were identified during the night of 10/11 May, each caused by different mechanisms: most probably by the effect of prompt penetration electric fields (PPEFs) (1), the travelling ionospheric disturbances (TIDs) (2) and the combination of electrodynamic processes and decreased O/N2 ratio (3). After a short interval of G condition, an unprecedented extended disappearance of the layers was observed during daytime hours on 11 May, which was further confirmed by Swarm data. This phenomenon appeared to be associated with a reduced O/N2 along with the influence of disturbance dynamo electric fields (DDEFs) and it cannot be explained only by the increased ionospheric absorption according to the results of the amplitude method.

Reference:
Berényi, K.A.; Barta, V.; Szárnya, C.; Buzás, A.; Heilig, B. Subauroral and Auroral Conditions in the Mid- and Low-Midlatitude Ionosphere over Europe During the May 2024 Mother’s Day Superstorm. Remote Sens. 2025, 17, 2492. https:// doi.org/10.3390/rs17142492

Primary author

Dr Kitti Berényi (HUN-REN-ELTE Space Research Group)

Co-authors

Attila Buzás (HUN-REN Institute of Earth Physics and Space Science) Balazs Heilig (SSE) Csilla Szárnya (HUN-REN Institute of Earth Physics and Space Science) Veronika Barta (HUN-REN Institute of Earth Physics and Space Science)

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