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ORIGINAL RESEARCH article

Front. Astron. Space Sci.

Sec. Space Physics

Volume 12 - 2025 | doi: 10.3389/fspas.2025.1550923

This article is part of the Research Topic Impacts of the Extreme Gannon Geomagnetic Storm of May 2024 throughout the Magnetosphere-Ionosphere-Thermosphere System View all 3 articles

The geomagnetic and geoelectric response to the May 2024 geomagnetic storm in the United Kingdom

Provisionally accepted
  • 1 British Geological Survey, The Lyell Centre, Edinburgh, United Kingdom
  • 2 The University of Manchester, Manchester, England, United Kingdom

The final, formatted version of the article will be published soon.

    The 'Gannon' geomagnetic storm of 10-12 May 2024 was the first extreme storm of the solar cycle 25 and the largest storm in more than 20 years. The auroral electrojet, driven by a strong negative interplanetary magnetic field exceeding -50 nT, moved towards the equator in the evening of the 10th May reaching the latitudes of central and southern England (below 54 • N) for several hours. Widespread sightings of the aurora were observed across the country, and rapid variations of the magnetic field were recorded in the UK.Here we present the geomagnetic and geoelectric data recorded during the storm in the UK together with models of ground effects and images of auroral displays around the country. We use the geomagnetic observations and a ground electric field model based on magnetotelluric data combined with the high-voltage power grid network information to estimate geomagnetically induced currents (GICs) at substation level during the storm. The highest modelled GICs exceeded 60 A in substations in southwest and east-central England as well as northern Wales. Substation GICs modelled in higher latitude stations in Scotland exhibited lower values because the leading edge of the auroral oval rapidly moved to lower latitudes.

    Keywords: Space weather, Geomagnetic Storm, geomagnetic field, Geoelectric field, Geomagnetically induced currents

    Received: 24 Dec 2024; Accepted: 19 Feb 2025.

    Copyright: © 2025 Lawrence, Richardson, Reay, Thompson, Clarke, Orr, Beggan, HÜbert and Smedley. This is an open-access article distributed under the terms of the Creative Commons Attribution License (CC BY). The use, distribution or reproduction in other forums is permitted, provided the original author(s) or licensor are credited and that the original publication in this journal is cited, in accordance with accepted academic practice. No use, distribution or reproduction is permitted which does not comply with these terms.

    * Correspondence: Ewelina Lawrence, British Geological Survey, The Lyell Centre, Edinburgh, United Kingdom

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