Solar atmosphere constantly changes. The changes could be large as during the last week M-class flare, or they could be relative small. Watch filament near the North polar region (upper part of image) slowly rising and then erupting. LASCO coronagraphs do not seem to show a clear signature of a CME eruption associated with this partial filament eruption.
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Solar Activity Report: April 27 - May 3, 2026
Solar activity during the reporting week remained generally low, with X‑ray flux staying within the low C‑class range aside from a few high‑...
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The 246th AAS meeting (joint with the Laboratory Astrophysics and Solar Physics Divisions) took place the of week 8-12 June 2025 in Anchorag...

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