
Get Ready For 50 Years Of Intense Northern Lights, Scientists Say
The sun has a solar cycle lasting roughly 11 years, during which its magnetic intensity waxes and wanes. It's presently close to solar maximum, the peak of that cycle.
There have been frequent sightings of the aurora far from the poles in the last year or two, the most severe of which was an extreme G5 geomagnetic storm on May 10-11, 2024, the most severe since 2003. Some researchers think it may have been the most powerful for hundreds of years.
A paper published in Space Weather found that the sun may be on the cusp of entering a multi-decade period of intensity called the Centennial Gleissberg Cycle. A repeating longer-term pattern in solar activity, the CGC is a theoretical variation in the intensity of solar cycles over a century or so.
It's possible that the last three solar cycles occurred during the CGC's minimum period, with the following three set to occur during its maximum. That could mean solar cycles over the next 50 years or so becoming more intense.
The evidence for the CGC's current period is based on a correlation between the 11-year solar cycle and high-energy protons in Earth's inner radiation belt. Proton flux increases when solar activity decreases. Using two NOAA satellites, the scientists have seen a decline in proton flux during the recent uptick in solar activity, which correlates with the midpoint of the CGC. Until 2022, the proton flux had been increasing.
Not all solar scientists agree with this theory. Scott McIntosh at space weather company Lynker Space and formerly of the National Center for Atmospheric Research at CU Boulder, told Live Science that it's 'too early' to make conclusions about the CGC and that the new paper may overestimate its effects.
The scientists looked at the proton flux above the South Atlantic Anomaly in the South Atlantic Ocean, where Earth's magnetic shield is weakest. 'The protons are clearly decreasing in measurements we obtained from NOAA's Polar Operational Environmental Satellites,' lead author Kalvyn Adams, an astrophysics student at the University of Colorado, told SpaceWeather.com. Other evidence includes sunspot numbers — direct indicators of solar activity — now at their highest levels in over 20 years, signaling a more turbulent and energetic sun. The CGC could also explain why solar cycle 24 — which occurred between 2008 and 2019 — was the weakest for 100 years.
While the paper focuses on proton flux, higher solar activity generally means more. and more intense, geomagnetic storms — an essential cause of spectacular displays of auroras. This new insight into the CGC could mean more opportunities for aurora sightings in mid-latitude regions, including in the U.S. and Europe.
Even if the CGS theory is wrong, expect more aurora. As the sun's magnetic activity begins to wane from solar maximum, another landmark display of aurora could likely result. 'This period of solar decline is marked by a decreasing number of sunspots, but not necessarily by fewer impacts, even after the solar maximum,' said Lisa Upton, co-chair of NASA and NOAA's Solar Cycle 25 Prediction Panel, announcing the arrival of solar maximum in October 2024. The declining phase is notable for having extreme solar events.
The Northern and South Lights (aurora borealis and australis) result from an interplay between the solar wind — a stream of charged particles constantly flowing from the sun — and Earth's magnetic field. When energetic particles reach Earth, they enter the polar regions, colliding with atoms and molecules in the upper atmosphere, exciting them and releasing energy as green and red lights.
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