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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Updates from the ESWW
The European Space Weather Week ( ESWW ) is taking place this week (2-6 Nov. 2026) in Florence, Italy. The overall theme of this meeting is...
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The peakfind results for GONG Month 302 show that the frequency shifts have started to decrease indicating that the solar maximum has alrea...
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Solar activity remained at low levels during the reporting period, with X‑ray flux generally at mid‑B levels except for a few impulsive, lo...
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The report from India received on 24 Sep. 2026, indicated that "the sky continues to be clear and favorable for observations since last...

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