Solar activity remained at low levels during the reporting period. X‑ray flux was predominantly within the B‑class range, with only occasional short‑lived increases into the C‑class. Active region 14419 was the dominant contributor, responsible for five of the seven C‑class flares recorded, including the strongest event of the week, a C4.1 flare on April 17. Additional low‑level C‑class flares were observed on April 13, 16, 17, and 18, while the remainder of the week stayed within the B‑class range. A few CMEs were detected, none with Earth‑directed components.
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Solar Activity Report: April 13 - 19, 2026
Solar activity remained at low levels during the reporting period. X‑ray flux was predominantly within the B‑class range, with only occasion...
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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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A notification was posted on the BVES website regarding the outage: Southern California Edison (SCE)- Restoration and Continued Public S...
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GONG/Learmonth (Australia) took observations of a large two-ribbon flare, which was the source of Earth-directed halo Coronal Mass Ejectio...
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