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Carrington Event

The Carrington Event was a severe geomagnetic storm in September 1859, widely regarded as the most intense on record.

By Ethan Anderson| Reviewed by Olivia Bennett, Standards & Fact-Checking Lead| Updated July 26, 2026|2 min read| Fact-checked

The Carrington Event was a severe geomagnetic storm in September 1859, widely regarded as the most intense on record. It was associated with a solar flare observed by Richard Carrington and caused vivid auroras and widespread disruption to telegraph systems. The event is often used in Canada as a reference point for space-weather risk to power grids, communications, and satellites.

Background

The event began with a solar flare observed by Richard Carrington on 1 September 1859. The flare was later associated with a coronal mass ejection that reached Earth and disturbed the planet’s magnetosphere.

Effects on Earth

The storm produced intense auroral displays reported around the world, including at unusually low latitudes. Telegraph systems were disrupted, with sparks and fires reported at some stations.

Scientific importance

The Carrington Event helped establish the connection between solar activity and geomagnetic effects on Earth. It remains a major case study in space weather and its possible impacts on modern technology.

Historical naming

The broader 1859 storm is commonly called the Carrington Event in honor of Richard Carrington. Some sources also use terms such as the geomagnetic storm of 1859 or the solar storm of 1859.

Key facts

  • Occurred during solar cycle 10 in early September 1859.
  • Richard Carrington made the first recorded observation of a white-light solar flare on 1 September 1859.
  • A coronal mass ejection reached Earth quickly and triggered the storm.
  • Auroras were seen globally and at unusually low latitudes.
  • Telegraph networks experienced sparks, outages, and some fires.
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Canadian context

The Carrington Event is relevant to Canadian readers because auroras associated with the storm were reported across wide regions of North America, and the event is often used in Canada as a reference point for space-weather risk to power grids, communications, and satellites.

Frequently asked questions

What was the Carrington Event?
A major geomagnetic storm in 1859, considered the strongest recorded storm of its kind.
Why is it called the Carrington Event?
It is named after Richard Carrington, who observed the associated solar flare.
What caused it?
It was most likely caused by a coronal mass ejection from the Sun that struck Earth’s magnetosphere.
What were the main effects?
It produced widespread auroras and disrupted telegraph communications, including sparks and some fires.
Why is it important today?
It is used as a benchmark for extreme space weather and for assessing risks to modern power and communications systems.

References

  1. Wikipediahttps://en.wikipedia.org/wiki/Carrington_Event
    Supports: General description, date, auroral displays, telegraph disruptions, and association with a coronal mass ejection.
  2. Encyclopaedia Britannicahttps://www.britannica.com/event/geomagnetic-storm-of-1859
    Supports: Largest recorded geomagnetic storm, September 1859 timing, auroral displays, telegraph fires, and Richard Carrington’s observation.
  3. Space.comhttps://www.space.com/the-carrington-event
    Supports: Naming of the event, solar flare observation, and rapid arrival of the associated coronal mass ejection.
  4. Science Museumhttps://www.sciencemuseum.org.uk/objects-and-stories/how-does-space-weather-affect-earth
    Supports: 1859 storm as the largest geomagnetic solar storm on record and its disruption of telegraph communications.
  5. Astronomyhttps://www.astronomy.com/today-in-the-history-of-astronomy/sept-2-1859-the-carrington-event-peaks/
    Supports: First recorded solar flare observation, geomagnetic storm severity, and low-latitude auroras.
  6. Hong Kong Observatoryhttps://www.hko.gov.hk/en/education/space-weather/space-weather-events/00433-extreme-space-weather-events-in-history.html
    Supports: Telegraph current effects, arrival time of charged particles, and historical significance as an extreme space-weather event.