Researchers Identified Solar Superflare Potential

A study linked the 1947 Great Spot to energy levels capable of exceeding past solar flare records.

Updated on Sept. 21, 2026 in Energy

A high-contrast, detailed image of a massive sunspot on the solar surface, showing swirling magnetic structures.
Researchers identified that historical sunspots, like the 1947 Great Spot, possessed sufficient energy to trigger solar superflares capable of disrupting modern infrastructure. AI Illustration. Upload story photo >

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Between 2010 and 2016, researcher Natalie Krivova analyzed solar active regions to determine the Sun's capacity for superflares. The study found that sunspots like the 1947 Great Spot possessed the potential to release energy exceeding 10³⁴ ergs.

Why it matters

Understanding the physical limits of solar activity helps scientists evaluate the risks that severe space weather poses to modern power grids. Estimates suggest that superflare events occur roughly once per century.

Researchers utilized data from the Solar Dynamics Observatory to establish that flare ribbon width correlates with active region area. The model indicates energy levels scale exponentially based on this surface area.

The players

Natalie Krivova

A researcher who identified the correlation between solar active regions and flare intensity.

Solar Dynamics Observatory

A NASA space observatory that provided the data used to re-examine historical solar anomalies.

The details

Solar flares originate when twisted magnetic fields snap and reconnect, releasing energy in proportion to the flare ribbon area. By applying this model to historical anomalies, scientists confirmed the 1947 Great Spot was more than twice the size of the 1859 solar region.

Timeline

  1. The Carrington Event took place in 1859.

  2. The Great Spot was recorded in 1947.

  3. Researchers analyzed Solar Dynamics Observatory data between 2010 and 2016.

The Big Picture

This research challenges previous assumptions about solar limits by proving that the Sun has historically generated regions larger than the Carrington Event of 1859. These findings shift the theoretical ceiling for solar flare energy and redefine long-term risk assessment for space weather.

A direct hit from a solar superflare is expected to disable regional power grids on a global scale. Confirming this potential helps engineers develop more resilient infrastructure against extreme electromagnetic disruptions.

The takeaway

Superflare events remain a rare but significant risk that necessitates ongoing monitoring of solar activity. Society should prioritize grid hardening and emergency preparedness to mitigate the impact of future extreme space weather.

Further reading

Learn more about the potential impacts of space weather on power systems in our Energy section.

Source note: This article includes information reported by PravdaReport.

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Should the nation increase funding to harden power grids against the risk of solar superflares?