Solar activity during the reporting period reached moderate levels, driven primarily by multiple flares from Active Region 14566. This region rotated onto the solar disk at the eastern limb near the end of the previous week. Overall, X-ray background flux remained at mid-B levels through November 4 before gradually increasing to high-B levels as flare activity intensified.
The most significant event of the week was an impulsive M3.5 flare on November 5, produced by Active Region 14566. During the final two days of the reporting period, the same region generated six additional low-level M-class flares along with frequent C-class activity. In total, seven M-class flares were observed during the week. In addition, approximately 80 C-class flares were recorded, of which about 75 originated from Active Region 14566, making it the most prolific flare-producing region on the visible solar disk during the reporting period. No Earth-directed coronal mass ejections (CMEs) were detected during the week.
Recent helioseismic maps of the Sun's far side suggest the emergence of a new moderate-sized active region that could rotate into the Earth-facing hemisphere around November 14. However, its appearance on the eastern limb will depend on its continued evolution and survival during the transiting period, as the region may either develop further or decay before becoming visible from Earth.
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