Solar Flare 8.26.22 (Eddie Bagwell)

Contains: Solar system body or event

Solar Flare 8.26.22

Acquisition type: Lucky imaging

Here is another spectacular flare from the Sun. The height and plasma mass on this one is extraordinaire.

It’s widely known that the Sun fluctuates between maximum and minimum activity over an 11-year cycle. Recent solar flares suggest a rise in internal solar activity, an observation that would be consistent with the predicted maximum occurring during the spring of 2025.

Solar flares like this one occur when the sun’s magnetic lines of force breach the photosphere, exposing the deeper, hotter solar interior, allowing the super-heated plasma to escape, providing a brilliant display across the electromagnetic spectrum. If the flare is strong enough, an accompanying CME (Coronal Mass Ejection) can occur, ejecting prodigious amounts of charged, super-heated plasma.

Inside a flare, the temperature typically reaches 10 to 20 million degrees Kelvin.

Thanks, Eddie

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