A G3 – Strong Geomagnetic Storm Watch is in effect for June 4 and 5, 2026, following three significant solar flares from Active Region 4455. NOAA’s Space Weather Prediction Center (SWPC) issued the watch at 14:52 UTC on June 3 after Earth-directed CME components were identified from two eruptions earlier in the day.
A G2 – Moderate geomagnetic storm watch is in effect for May 15, 2026, due to the anticipated impact of a corotating interaction region (CIR) associated with a negative polarity coronal hole high speed stream (CH HSS). G1 conditions are forecast for May 16 and 17.
A strong solar flare measuring M7.5 erupted from Active Region 4409 at 01:17 UTC on April 4, 2026. The event started at 01:07 and ended at 01:23 UTC. No radio signatures indicating a coronal mass ejection (CME) were detected, despite the region’s position near the center of the solar disk, where any CME produced would likely be Earth-directed. Forecast conditions indicate solar activity will likely remain at moderate levels through April 6, with a slight chance of X-class flares, while geomagnetic conditions are expected to reach G1 – Minor to G2 – Moderate storm levels on April 4 under the combined influence of the April 1 CME and a negative polarity coronal hole high-speed stream.
A G3 – Strong geomagnetic storm developed late on March 20 into early March 21, 2026, after a coronal mass ejection that left the Sun on March 18 impacted Earth. The storm intensified after at least two CME arrivals, with solar wind speeds reaching 567 km/s and the interplanetary magnetic field turning strongly southward to −28 nT.
A G1 – Minor geomagnetic storm is in progress on February 22, 2026, with Kp index values reaching 5 since 03:00 UTC, according to the NOAA Space Weather Prediction Center (SWPC). At 08:00 UTC, the agency issued a G2 – Moderate warning valid through 15:00 UTC, forecasting a possible rise to Kp 6 later in the day as solar-wind conditions remain elevated.
A positive polarity coronal hole high speed stream currently interacting with Earth’s magnetic field produced a G2 – Moderate geomagnetic storm, with the K-index peaking at 6 at 20:00 UTC on February 16, 2026. The storm may generate visible aurora across northern U.S. latitudes and cause minor operational effects in satellite and power systems.
A coronal mass ejection (CME) associated with an X8.1 solar flare from Region 4366 at 23:57 UTC on February 1 is forecast to glance Earth late on February 5, 2026. The impact is expected to produce G1 – Minor geomagnetic storm conditions and possible auroral activity poleward of 60 degrees Geomagnetic Latitude. This was the third-strongest solar flare of Solar Cycle 25.
Severe geomagnetic storm on January 19, 2026, generated a rare auroral glow inside the South Atlantic Anomaly, a region where Earth’s magnetic field is significantly weaker. Photographers in Brazil captured a diffuse purple band over Cambará do Sul during peak geomagnetic activity, documenting the latest in rare instances of possible auroral or SAR arc activity within the anomaly.
The impact of a full halo coronal mass ejection (CME) at Earth on January 19, 2026, drove geomagnetic activity to G4 – Severe levels, producing widespread aurora across Europe, Asia, and the United States.
A G4 – Severe solar radiation storm is in progress after ≥10 MeV proton flux exceeded 10 000 pfu at 18:10 UTC on January 19, 2026, following the X1.9 solar flare on January 18. As the associated full-halo coronal mass ejection approaches Earth, forecasters warn that a G4 – Severe geomagnetic storm is likely early on January 20.
