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The May 2024 solar storm: what happened, step by step?

On 10 May 2024, a sequence of solar eruptions drove an extreme G5 geomagnetic storm at Earth. The event produced unusually widespread auroras. Solar flares, arriving coronal mass ejections and the resulting geomagnetic disturbance were different stages, with different timestamps.

Pink and green coronal aurora radiating across the sky above tree silhouettes in southwestern British Columbia on 10 May 2024.Open figure at full size ↗
NASA / Mara Johnson-Groh · southwestern British Columbia, 10 May 2024. An archival photograph of this event, not today’s conditions. Source record (opens in a new tab) · NASA media-use guidelines (opens in a new tab). Resized to WebP; no further crop or retouching.

First, distinguish the three events

A solar flare is a burst of electromagnetic radiation. A coronal mass ejection, or CME, is an outward eruption of plasma and magnetic field. A geomagnetic storm describes the disturbance of Earth’s magnetic environment. One spectacular solar image does not timestamp all three. NOAA: coronal mass ejections [6].

During 7–11 May, NASA reported multiple strong flares and at least seven Earth-directed CMEs. The series, rather than a single photograph of a flare, is the useful starting point for this storm’s story. NASA’s event account [1].

10 May: from reported arrival to extreme conditions

Schumann Pulse · field notes

10 May 2024: the escalation.

Three distinct milestones reported by NOAA.

  1. 16:37 UTC

    First CME arrival reported

    NOAA event update

  2. 17:39 UTC

    Severe · G4 observed

    NOAA event update

  3. 22:54 UTC

    Extreme · G5 observed

    NOAA G5 bulletin

Historical record, not current conditions. Arrival and storm classifications are separate events. Times are converted from EDT to UTC.

Open original wide figure ↗
Schumann Pulse · original chronology of NOAA’s event updates. EDT times converted to UTC (+4 hours). The 16:37 time is the agency’s reported arrival, not an assertion that every instrument measured the same onset.
  1. NOAA reports the first CME arrival.

    The agency’s event update gives 12:37 p.m. EDT. This is the reported arrival marker, not the time the G5 classification began.

  2. Severe G4 conditions are observed.

    The same update gives 1:39 p.m. EDT, after G3 at 1:08 p.m. EDT.

  3. Extreme G5 conditions are first observed.

    NOAA’s G5 bulletin states 6:54 p.m. EDT. The bulletin itself was published at 23:58 UTC; publication time and observation time differ.

Sources: NOAA’s 10 May event update [2] and the G5 observation bulletin [3]. EDT was UTC−4 on this date; we add four hours for this timeline. “Arrival” can depend on the instrument or boundary being discussed, so these times are explicitly attributed rather than presented as identical in every dataset.

What does G5 mean here?

G5 is NOAA’s extreme geomagnetic storm category. It describes a space-weather condition, not the brightness of every aurora and not a medical risk score. NOAA’s scale connects geomagnetic levels with possible effects on systems such as power networks, satellites and navigation. NOAA space-weather scales [4].

The label also does not mean every minute of the multi-day event was equally intense. Our G1–G5 guide explains the categories and why a peak and a current reading answer different questions.

What the photograph shows—and does not show

The image above records a coronal aurora over southwestern British Columbia on 10 May 2024, credited to NASA / Mara Johnson-Groh. Its date and location make it evidence of this event, unlike a generic stock aurora. NASA image record [5].

It does not establish the view from another country, the brightness to an unaided eye or the precise moment of G5 onset. Those questions need separate observations. Our aurora visibility guide explains why even a very strong event can be missed locally.

Why the May 14 flare is not the beginning of this storm

Images of a later X8.7 flare on 14 May also appear in NASA’s account of the active region. That flare came after the 10 May onset. Reusing it without its date can reverse the sequence and make a dramatic image explain the wrong event. NASA’s dated chronology [1].

What to take into the next storm

When you encounter a viral screenshot, ask: which phenomenon, which source, and which time? Keep a forecast separate from an observation and a historical peak separate from conditions now. Those three checks are useful even when the headline is accurate.

This article is a historical explainer. For current, timestamped readings, open space weather today.

Sources

References in the text lead here. Original publications open in a new tab; this guide stays open.

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