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Solar flare blasts out strongest radiation storm since 2017


It’s the sunspot region that just does not want to quit! 

Beastly sunspot AR3697 has made headlines again just before it makes another exit. The sunspot region, formerly known as AR3664, produced the historic geomagnetic storm that led to May’s global auroras.

On Saturday (June 8), the sunspot fired off a M9.7-class solar flare, the second strongest type on the classification scale. The flare was powerful enough that it produced the strongest radiation storm since 2017, according to NOAA’s Space Weather Prediction Center (SWPC). These types of events can pose a risk of impact to space launch operations and satellites, and can also disrupt shortwave radio signals.

A view of a solar flare blasting from the sun in the lower left of the image. (Image credit: NASA/SDO)

Solar flares are intense bursts of electromagnetic radiation that originate from sunspots on our sun’s surface. They are classified into lettered groups (X, M, C, B and A) according to their size, with X-class flares being the most powerful. Within each of these classes, numbers from 1 to 10 (and beyond for X-class flares) denote a flare’s relative strength. That means M-class flares like this one are 10 times weaker than X-class flares but are 10 times stronger than C-class flares.

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