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The giant 1947 sunspot could store superflare-scale energy

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One of the largest recorded sunspot groups had enough estimated magnetic capacity to enter the superflare range.

Capacity is not occurrence probability, timing or proof of a historical eruption.

Method

Modern relationships between spot area, complexity and flare upper limits were extended to historical observations.

Scale

The group covered about 0.6% of the visible disk and spanned roughly 40 Earth diameters.

The giant 1947 sunspot could store superflare-scale energy
This AI-generated image explains the topic; it is not a photograph of the actual site, experiment, animal or fossil.

Potential

Stored magnetic energy and the instability that releases it are separate requirements.

Earth impact

Radiation, coronal mass ejections and particles differ; direction and magnetic orientation control damage.

Next

Better historical magnetic reconstruction and stellar comparisons are needed; preparedness should use live official space-weather warnings.

Primary source and independent checks

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