Solar Region 4366 Unleashes Massive X4.2 Flare: Current Analysis and Earthward Impact Forecast

Author: Uliana S.

Flare X4.2 @ N15°E5° (NOAA 4366) 2026-02-04 12:02 / 12:13 \ 12:18 UT

Active Region 4366, which has been under intense scrutiny by the global scientific community for several days, has finally demonstrated its volatile nature. On February 4, 2026, at precisely 12:13 UTC, this massive solar complex produced a powerful geo-effective eruption directed squarely at Earth. This event, officially classified as an X4.21 (or X4.2) flare, represents the third most intense solar explosion recorded during the 2025-2026 period. Crucially, it marks the first extreme, top-tier flare to occur since the region moved into a position of direct influence over our planet. The immediate consequences were felt across Africa and Europe, where significant disruptions to shortwave radio communications were reported.

A CME has been detected, but judging by its low speed (~450 km/s), it is more likely to be a stealth CME from the X8.1 flare.

While initial observations did not immediately reveal a massive coronal mass ejection (CME) associated with the X4.2 event, subsequent data analysis has confirmed an impending impact. A plasma cloud is currently traversing the space toward Earth at a relatively modest speed of approximately 450 km/s. Experts suggest this is likely not the direct result of the recent X4.2 flare, but rather a "stealth CME"—potentially originating from the gargantuan X8.1 flare that occurred on February 2. Real-time solar wind monitoring already indicates significant disturbances; the interplanetary magnetic field (Bt) has reached 20 nT, while its vertical component (Bz) shows a negative polarity. This specific magnetic orientation is highly conducive to transferring solar energy into Earth's magnetosphere.

At 04.12.13 UTC in region 4366 an impulsive X4.2 flare occurred. At present, no signs of a coronal mass ejection have been detected in the images. Stay tuned for updates.

Given the current physical parameters of the approaching solar wind, space weather forecasters are anticipating the onset of a geomagnetic storm. If the current magnetic conditions persist, the storm is expected to reach G2 (moderate) or even G3 (strong) levels. Such disturbances can lead to vivid auroral displays at lower latitudes than usual and may necessitate precautions for satellite operations and high-frequency radio users. Scientists are closely monitoring the situation as the plasma cloud interacts with the Earth's magnetic shield, preparing for the peak of the geomagnetic activity within the next 24 hours.

The recent X-class flare serves as the climax of an extraordinary period of activity for Region 4366, a solar behemoth that has grown to exceed 15 times the diameter of Earth. The sheer scale of this active region is reflected in the staggering frequency of its eruptions. On February 4 alone, the Sun registered a total of 20 flares: one X-class, 12 M-class, and 7 C-class events. This transition from a state of anticipation to one of active impact underscores the dynamic nature of the current solar cycle. The environment has shifted from theoretical threat to a phase of direct physical interaction with the terrestrial environment.

As researchers continue to refine the estimated arrival time of the primary plasma cloud, it is increasingly evident that Earth is facing a multi-faceted solar assault rather than a single isolated event. The combined impact of these successive eruptions is expected to manifest over the coming day, potentially causing fluctuations in power grids and creating spectacular light shows in the upper atmosphere. Because Active Region 4366 remains in a geo-effective position, it continues to pose a significant threat for further high-energy events. The scientific community remains on high alert, as the potential for additional powerful flares remains elevated while this massive sunspot group traverses the solar disk.

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