The Gannon Storm: Citizen science observations during the geomagnetic superstorm of 10 May 2024
Abstract
The 10 May 2024 geomagnetic storm, referred to as the Gannon Storm in this paper, was one of the most extreme to have occurred in over 20 years. In the era of smartphones and social media, millions of people from all around the world were alerted to the possibility of exceptional auroral displays. Hence, many people not only witnessed but also photographed the aurora during this event. These citizen science observations, although not from scientific instruments operated by observatories or research groups, can prove invaluable in obtaining data to characterise this extraordinary event. In particular, many observers saw and photographed the aurora at mid-latitudes, where ground-based instruments targeting auroral studies are sparse or absent. We created an online survey and circulated it within networks of aurora photographers to collect observations of the aurora and disruptions in technological systems that were experienced during this superstorm. We obtained 696 citizen science reports from over 30 countries, containing information such as the time and location of aurora sightings, observed colours and auroral forms during the geomagnetic storm. We supplemented the obtained dataset with 186 auroral observations logged in the Skywarden catalogue by citizen scientists. The main findings enabled by the data collected through these reports are that the aurora was widely seen from locations at geomagnetic latitudes ranging between 30° and 60°, with a few reports from even lower latitudes. This was significantly further equatorward than predicted by auroral oval models. The reported auroral emission colours, predominantly red and pink and intense enough to reach naked-eye visibility, suggest that the auroral electron precipitation contained large fluxes of low-energy (< 1 keV) particles. (...)
Versions
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BibTeX
@misc{grandin2026gannon,
title = {{The Gannon Storm: Citizen science observations during the geomagnetic superstorm of 10 May 2024}},
author = {Maxime Grandin and Emma Bruus and Vincent E. Ledvina and Noora Partamies and Mathieu Barthelemy and Carlos Martinis and Rowan Dayton-Oxland and Bea Gallardo-Lacourt and Yukitoshi Nishimura and Katie Herlingshaw and Neethal Thomas and Eero Karvinen and Donna Lach and Marjan Spijkers and Calle Bergstrand},
howpublished = {arXiv},
year = {2026},
month = oct,
doi = {10.48550/arxiv.2610.19929},
eprint = {2610.19929},
archivePrefix = {arXiv},
url = {https://arxiv.org/abs/2610.19929},
note = {CC BY 4.0},
}
RIS
TY - UNPB
TI - The Gannon Storm: Citizen science observations during the geomagnetic superstorm of 10 May 2024
AU - Maxime Grandin
AU - Emma Bruus
AU - Vincent E. Ledvina
AU - Noora Partamies
AU - Mathieu Barthelemy
AU - Carlos Martinis
AU - Rowan Dayton-Oxland
AU - Bea Gallardo-Lacourt
AU - Yukitoshi Nishimura
AU - Katie Herlingshaw
AU - Neethal Thomas
AU - Eero Karvinen
AU - Donna Lach
AU - Marjan Spijkers
AU - Calle Bergstrand
PY - 2026
DA - 2026/10/14
PB - arXiv
DO - 10.48550/arxiv.2610.19929
UR - https://arxiv.org/abs/2610.19929
AB - The 10 May 2024 geomagnetic storm, referred to as the Gannon Storm in this paper, was one of the most extreme to have occurred in over 20 years. In the era of smartphones and social media, millions of people from all around the world were alerted to the possibility of exceptional auroral displays. Hence, many people not only witnessed but also photographed the aurora during this event. These citizen science observations, although not from scientific instruments operated by observatories or research groups, can prove invaluable in obtaining data to characterise this extraordinary event. In particular, many observers saw and photographed the aurora at mid-latitudes, where ground-based instruments targeting auroral studies are sparse or absent. We created an online survey and circulated it within networks of aurora photographers to collect observations of the aurora and disruptions in technological systems that were experienced during this superstorm. We obtained 696 citizen science reports from over 30 countries, containing information such as the time and location of aurora sightings, observed colours and auroral forms during the geomagnetic storm. We supplemented the obtained dataset with 186 auroral observations logged in the Skywarden catalogue by citizen scientists. The main findings enabled by the data collected through these reports are that the aurora was widely seen from locations at geomagnetic latitudes ranging between 30° and 60°, with a few reports from even lower latitudes. This was significantly further equatorward than predicted by auroral oval models. The reported auroral emission colours, predominantly red and pink and intense enough to reach naked-eye visibility, suggest that the auroral electron precipitation contained large fluxes of low-energy (< 1 keV) particles. (...)
ER -