A massive and rapidly growing sunspot region on the Sun, designated Active Region 4366, has become one of the most energetic solar flare producers in recent years, unleashing a torrent of powerful bursts that have grabbed the attention of space weather scientists around the world. Over the past several days, the Sun has emitted dozens […]

A massive and rapidly growing sunspot region on the Sun, designated Active Region 4366, has become one of the most energetic solar flare producers in recent years, unleashing a torrent of powerful bursts that have grabbed the attention of space weather scientists around the world.

Over the past several days, the Sun has emitted dozens of solar flares from AR 4366, including numerous M-class flares and several X-class eruptions, the strongest category of solar flare. Among these was an X8-class flare detected on February 1–2, one of the most powerful recorded so far in 2026 and the most intense event this year to date.
Solar flares occur when magnetic energy built up in the Sun’s atmosphere is suddenly released. X-class flares produce intense radiation and can interfere with Earth’s ionosphere, leading to temporary radio blackouts, degraded high-frequency communications, and navigation signal disruptions. The X8 event and subsequent strong blasts have already caused R3-level radio blackouts in parts of the South Atlantic region.

In addition to the X8-class flare, researchers have recorded other powerful eruptions, including a recent X4.2 flare from the same active region. In the past 24 hours alone, NOAA scientists observed dozens of flares from AR 4366, including at least 26 events ranging from moderate M-class to X-class strengths.

The sheer number and intensity of flares from this sunspot has led forecasters to describe AR 4366 as a “solar flare factory.” As it rotates further into a position more directly facing Earth, space weather agencies warn that any future coronal mass ejections (CMEs)which are huge clouds of charged particles launched from the Sun, would be more likely to intersect Earth’s magnetic field. Even glancing blows from CMEs can spark enhanced auroras, possibly visible at lower latitudes than usual later this week.
Scientists continue to monitor AR 4366 closely. Its increasing size and magnetic complexity make it capable of further strong eruptions, and forecasters expect more activity as the Sun remains near the peak of its current 11-year cycle. Solar flares and related space weather effects, from radio transmission disruptions to vivid auroral displays, may persist as long as the region remains active.
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