A G4 – Severe or greater geomagnetic storm is forecast for early January 20, 2026, as a full-halo coronal mass ejection from the January 18 X1.9 solar flare approaches Earth. If G4 conditions materialize, auroral activity is expected to expand significantly equatorward, with visibility possible as far south as Alabama and northern California.
Modeling and analysis indicate that the CME produced by the long-duration X1.9/3b flare from Active Region 4341 on January 18 is likely to reach Earth early on January 20. The eruption generated a full-halo CME observed in coronagraph imagery shortly after the flare peak, indicating an Earth-directed trajectory.
Space weather forecasts now indicate a high likelihood of severe geomagnetic storming after CME arrival. NOAA’s Space Weather Prediction Center has issued a geomagnetic storm watch predicting G4 – Severe conditions, superseding all prior watches. Weaker storming at G1 – Minor levels is expected to persist into January 21 as CME effects gradually wane and coronal-hole influences resume.
At G4 intensity, geomagnetically induced currents may cause widespread voltage control problems in power transmission systems, with some protective systems potentially tripping out key assets. Satellite systems may experience surface charging, increased drag on low Earth orbit spacecraft, and tracking or orientation difficulties. Satellite navigation systems, including GPS, may be degraded or unavailable for several hours.
High-frequency radio propagation is expected to become sporadic or completely blacked out at polar latitudes. Aviation operations on polar routes may be affected due to communication disruptions and increased radiation exposure linked to the ongoing S3 – Strong solar radiation storm.
Auroral activity is expected to expand significantly equatorward during peak storming. If G4 conditions materialize, aurora may be visible well beyond typical high-latitude regions, potentially reaching as far south as Alabama and northern California under favorable viewing conditions.
The geomagnetic response will depend strongly on the magnetic structure of the CME upon arrival, particularly the orientation and duration of southward interplanetary magnetic field components. Space weather conditions remain dynamic, and forecasts may be adjusted as upstream solar wind observations become available closer to impact.
