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Surprise Solar Storm Creates Auroras Across United States

A surprise G3 geomagnetic storm, caused by a hidden magnetic feature on the sun, triggered stunning aurora displays visible across much of the United States.

Dr. Evelyn Reed
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Dr. Evelyn Reed

Dr. Evelyn Reed is Archeonis' science editor, specializing in astronomy, astrophysics, and space weather. With a Ph.D. in Astrophysics, she translates complex celestial phenomena for a general audience.

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Surprise Solar Storm Creates Auroras Across United States

A powerful and unexpected geomagnetic storm reached Earth over the weekend of September 14-15, producing vibrant aurora displays visible across large parts of the United States. The event, classified as a G3 or "strong" storm, was triggered by a previously undetected magnetic feature on the sun, surprising scientists and delighting skywatchers.

Key Takeaways

  • An unforeseen G3-level geomagnetic storm occurred on September 14-15.
  • The cause was a hidden "magnetic island" of positive polarity within a larger negative-polarity coronal hole on the sun.
  • Auroras were sighted much farther south than usual, with reports from New York, Wyoming, Wisconsin, and even Texas.
  • Initial forecasts predicted only a minor to moderate G1 or G2 storm, highlighting the event's surprising intensity.

An Unforeseen Solar Event

Space weather forecasters had anticipated a minor solar event over the weekend. They were monitoring a large, butterfly-shaped coronal hole on the sun's surface. Predictions suggested a G1 (minor) or G2 (moderate) geomagnetic storm at most. However, the solar wind that reached Earth was far more potent than expected.

The resulting G3 storm caught many by surprise. These strong geomagnetic events have the potential to disrupt satellite operations and power grids, but in this case, the most notable effect was a spectacular and widespread display of the northern lights.

The Hidden Cause of the Storm

The source of the storm's unexpected strength was a subtle feature that was difficult to detect. Space weather physicist Tamitha Skov explained that the coronal hole itself had a negative polarity, which typically does not lead to intense geomagnetic activity.

However, as the feature rotated across the sun's disk, a small "island" of positive polarity emerged within it. This created a powerful magnetic connection that channeled a high-speed stream of solar wind directly toward Earth.

What is a Coronal Hole?

A coronal hole is an area in the sun's upper atmosphere, or corona, that is cooler and less dense than its surroundings. These regions are sources of fast-moving solar wind, which is a stream of charged particles that flows outward from the sun. When a coronal hole faces Earth, this solar wind can trigger geomagnetic storms.

"That positive polarity is what ended up giving us about 6 hours worth of really intense storming," Skov stated in a recent forecast. "Little things like this can really make a big difference and change a nothingburger into a G3-level solar storm."

Understanding Geomagnetic Storms

Geomagnetic storms are major disturbances of Earth's magnetosphere, the region of space controlled by our planet's magnetic field. They are caused by the exchange of energy from the solar wind into the space environment surrounding Earth.

Scientists use a five-level G-scale to measure the intensity of these storms:

  • G1: Minor
  • G2: Moderate
  • G3: Strong
  • G4: Severe
  • G5: Extreme

The primary visual effect of these storms is the aurora, also known as the northern lights (aurora borealis) or southern lights (aurora australis). The phenomenon occurs when charged particles from the sun collide with gases in Earth's upper atmosphere. These collisions excite the gas molecules, causing them to release energy in the form of light. The colors depend on the type of gas involved, with oxygen typically producing green and red light, and nitrogen producing blue and purple hues.

Did You Know?

A G3 storm is considered strong and can cause intermittent satellite navigation and low-frequency radio navigation problems. The auroras from such a storm can often be seen as far south as Illinois and Oregon in the United States.

Widespread Sightings Across the U.S.

The surprise G3 storm produced auroras far beyond their typical arctic range. Social media platforms were flooded with images and videos from skywatchers across the northern and central United States who were treated to the unexpected light show.

Midwest and Mountain West

In Monroe, Wisconsin, photographer Ross Harried captured stunning images of green and purple pillars of light filling the night sky. In Casper, Wyoming, Andrew Towne photographed a vibrant aurora display that shared the sky with a clear view of the Milky Way galaxy.

Northeast and Beyond

The lights were also visible in the Northeast. Tony Rodriguez reported seeing spectacular red and green structures with the naked eye from the shore of Seneca Lake in New York. Joshua Grisewood, also in New York, noted he was "caught off guard" by the surprise show. Colton Flint shared a timelapse video from Massachusetts that showed the dynamic and rapidly changing nature of the display.

Southern Sightings

Perhaps most remarkably, the aurora was photographed as far south as Texas. Photographer Blake Brown captured the faint glow on the northern horizon, which appeared in the same frame as a distant lightning storm. The event provided a rare opportunity for people in lower latitudes to witness a phenomenon usually reserved for those living closer to the poles.

The widespread nature of the event highlights the intensity of the G3 storm and the unique solar conditions that produced it. It serves as a reminder of the sun's dynamic and sometimes unpredictable behavior.