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The Gannon Storm: Citizen science observations during the geomagnetic superstorm of 10 May 2024

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.

By Grandin, Bruus, Ledvina +12

Score█████░░░░░5.4

VerdictWorth a reader's time today.

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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. (...)

Maxime Grandin, Emma Bruus, Vincent E. Ledvina, Noora Partamies, Mathieu Barthelemy, Carlos Martinis, Rowan Dayton-Oxland, Bea Gallardo-Lacourt, Yukitoshi Nishimura, Katie Herlingshaw, Neethal Thomas, Eero Karvinen, Donna Lach, Marjan Spijkers, Calle Bergstrand

The editor's rubric

Heuristic review

DimensionLevelWeightWhat that level means
Leverage███░░ 318%A method or resource many groups across the field will adopt within a year.
Magnitude██░░░ 220%Solid incremental gain on a meaningful problem.
Evidence████░ 422%Strong: large scale, preregistered, independently replicated, or a well-powered randomized trial.
Novelty██░░░ 222%A new combination of known ideas.
Trajectory██░░░ 210%Some room to improve with obvious engineering.
Stakes███░░ 38%Meaningful benefit to many people within a few years.

Editor’s rationale

Heuristic triage from title and abstract text only, not a reading of the paper. Cues found: novelty (open problem); design (multicenter); verification (code released); stakes (global scale, energy, climate).

How the score was computed

rank-2026-10-07

Score█████░░░░░5.4

Score = 10 × (75% × adjusted merit / 10 + 15% × attention + 10% × freshness)

Merit
5.4 / 10
Weighted rubric, evidence-gated.
Adjusted merit
4.6 / 10
Shrunk toward the desk prior by editor confidence (40%).
Attention
73%
Citations, upvotes, points, mentions.
Freshness
92%
Half-life decay since publication.
  • Citations48 (reference 20, via openalex, Oct 15, 2026, 07:29 UTC)

The record

  • Reviewed by heuristic-v6 on Oct 15, 2026, 07:29 UTC. Paper type: empirical.
  • Categories: physics.space-ph, physics.geo-ph
  • LEAD, No.1 in the Physics edition of October 15, 2026.
  • LEAD, No.1 in the Climate & Energy edition of October 15, 2026.