Marko Rummelsburg
@doktornihil • 1,447 subscribers
Space Weather Enthusiast #AuDHD https://t.co/oLIp56qfhZ
Shorts
24-hour development and flaring of sunspot region 4366 – more and more coronal loops and dense core filaments are appearing.
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Complex eruption associated with an X1.9 flare - the dimming almost reaches the center
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5½ days of sunspot group 4366 We've seen 63 M-class flares, 6 X-class flares, 0 radiation storms, 5 coronal mass ejections (CMEs) - 3 of them slow. It has passed its zenith, but it is not yet at an end. The big question is: will it produce another CME?
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Development of sunspot group 4366. A complex 'bad actor' that produces many strong to very strong flares, but so far only one very slow coronal mass ejection. It mainly fires blanks. The animation shows the sun's photospheric magnetic field (the 'surface' field), sunspots and flares.
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7 days of sunspot group 4366 – after a certain decay, it is now showing new flux emergence and growth. The leading spot has changed its direction of rotation. It is now rotating counterclockwise.
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