M4.2 flare @ N7°W28° (NOAA 4317) 2025-12-28 22:01 / 22:39 \ 22:56 UT
M4.2 flare at 22:39 UTC on December 28, 2025.
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Author: Uliana Soloveva
M4.2 flare @ N7°W28° (NOAA 4317) 2025-12-28 22:01 / 22:39 \ 22:56 UT
M4.2 flare at 22:39 UTC on December 28, 2025.
As the year drew to a close, our Sun exhibited a burst of unexpected energy, setting the stage for a potential celestial light show visible from Earth. Following a period of relative quiet, a series of significant solar flares erupted, capable of impacting near-Earth space weather and offering the rare spectacle of the Northern and Southern Lights gracing the transition from December 31st into January 1st.
4.2 m-class solar flare from the Sun just now! Looks like some plasma was hurled towards Earth from this explosion, coronagraph imagery is needed to confirm the trajectory out into interplanetary space. Notice the activity on the left side of the Sun as well!
M4.2 flash at 22:39 UTC 28 декабря 2025 года.
This notable activity commenced between December 28th and December 29th, 2025. An active region, designated as AR 4317, situated in the Sun's northern hemisphere, was responsible for unleashing two powerful M-class flares. Specifically, an M4.2 flare occurred at 22:39 UTC, quickly followed by an M2.2 flare at 00:02 UTC. This sequence was particularly noteworthy because this specific region was the only one actively facing our planet in a geo-effective alignment.
Will we see a CME impact around the New Year? NASA is forecasting the M4.2 CME may graze Earth around 12-31 22 UT (Wednesday night). Kp 4-6 (G0-G2) conditions may occur, but I don't have too much hope. We'll see what shows up at L1!
Model of ejecta propagation from the M4.2 flash.
Subsequent space weather modeling indicated that a coronal mass ejection (CME) launched in the wake of these flares was projected to reach Earth around the New Year’s holiday. This massive cloud of solar plasma, spanning approximately 150 million kilometers, required roughly three days for its journey. Calculations suggest that the Earth’s magnetosphere will experience a glancing blow, but one that is certainly significant enough to be felt.
What are the implications of this solar event for observers across the globe?
The primary effects are expected to be concentrated in the higher latitudes, where the auroral oval typically resides. Residents in these regions have the best chance of witnessing the dazzling display:
Should the geomagnetic response prove stronger than initial forecasts suggest, the aurora could extend further south toward mid-latitudes—areas where these light shows are far less common occurrences. This scenario opens up the exciting possibility of seeing the aurora for residents in the northern United States (including states like Minnesota and Michigan), Central Europe, and the southern regions of Russia. This potential intensification means that even those accustomed to clear skies might get a front-row seat to this cosmic event, provided the solar impact is robust.
A G2 (Moderate) geomagnetic storm watch has been issued for 03-04 Apr, 2026, due to combined influence from on-going CH HSS and a CME that left the Sun on 02 Apr. Stay tuned to our website for updates.
G2 Watch for 31 Mar UTC-day still stands. We evaluated the 29 Mar (EDT) CME and feel fairly certain most ejecta will pass behind Earth's orbit; although we do anticipate enough flanking effects to warrant the G2 Watch, with a chance for G3. Stay aware at spaceweather.gov
REPOST: An X1.4 flare was produced by Region 4405, peaking at 0319 UTC on 30 March and resulted in an R3 (Strong) Radio Blackout. An associated coronal mass ejection is seen in coronagraph imagery and analysis is currently ongoing. Visit spaceweather.gov to stay informed.