Space Weather

Space weather describes changing environmental conditions in near-Earth space. Magnetic fields, radiation, particles and matter, which have been ejected from the Sun, can interact with the Earth’s upper atmosphere and surrounding magnetic field to produce a  variety of effects.

Image courtesy of NASA/SDO and the AIA, EVE, and HMI science teams

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Aurora forecasts

Northern Hemisphere

Coronal hole fast winds are expected throughout the four day period, from two separate events. This will bring a chance of aurora sightings each night, though with the greatest chance on Thursday 24th September, across parts of northern Scotland, and similar latitudes, where skies are clear.

Southern Hemisphere

Coronal hole fast winds are expected throughout the four day period, from two separate events. This will bring a chance of aurora sightings each night, though with the greatest chance on Thursday 24th September UTC, across parts of southern New Zealand, and similar latitudes, where skies are clear.

Issued at: 12:42 (GMT) on Thu 24 Sep 2026

Forecast overview

Space Weather Forecast Headline: Chance of G1/Minor Geomagnetic Storming and R1/Radio Blackouts throughout.

Analysis of Space Weather Activity over past 24 hours

Solar Activity: Solar activity has been Low, peaking at 24/0903 UTC. There are currently eight sunspot regions on the visible disc. The largest sunspot is in the west, though appears relatively stable. There is a cluster of three modestly sized spots in the northwest, with limited magnetic complexity but each with intermediate spots. The remaining spots reside in the east, all of which are small and simple and mostly showing signs of decay.

There were no Earth-directed coronal mass ejections observed during the period.

Solar Wind / Geomagnetic Activity: Solar wind observations suggested possible early influence from fast winds. Solar wind speeds were slow-ambient, but rising, peaking at Slightly Elevated at 24/1033 UTC. The Interplanetary Magnetic Field started Weak, but rose to Moderate levels, peaking at 24/0600 UTC. The north-south component followed a similar trend, though initially positive, then becoming largely negative after 24/0345 UTC. Geomagnetic activity was largely Quiet to Unsettled (Kp 0-3) with a single Active interval (Kp 4) to end the period. 

Energetic Particles / Solar Radiation: No Solar Radiation Storms were observed.

Four-Day Space Weather Forecast Summary

Solar Activity: Solar activity is expected to be Low or Very Low, with a Chance of becoming Moderate should any isolated Moderate-class flares occur.

Solar Wind / Geomagnetic Activity: No Earth-directed coronal mass ejections currently feature in the forecast period. Earth has now connected to coronal hole fast winds, with solar wind speeds peaking briefly at Slightly Elevated, but will likely peak Elevated later Day 1 or Day 2 (24-25 Sep). The next coronal hole fast winds, with wind speeds peaking Elevated once again, is most likely on Day 3 (26 Sep). Either a relatively smooth transition between high speed streams is possible, or a brief dip in wind speeds between the peak of each fast wind.

Quiet to Unsettled (Kp 1-3) Geomagnetic activity is expected at first, rising to likely Active (Kp 4) intervals, with a chance of G1/Minor Storms (Kp 5) and a slight chance of G2/Moderate storm (Kp 6) intervals on Day 1 (24 Sep). A chance of isolated G1/Minor Storms (Kp 5) then continues from Day 2 to Day 4 (25-27 Sep) due to residual fast winds from the first coronal hole, followed by the next fast wind enhancement.

Energetic Particles / Solar Radiation: No Solar Radiation Storms are expected.

Issued at: 12:19 (GMT) on Thu 24 Sep 2026

Solar imagery

SDO AIA-193

This channel highlights the outer atmosphere of the Sun - called the corona - as well as hot flare plasma. Hot active regions, solar flares, and coronal mass ejections will appear bright here. The dark areas - called coronal holes - are places where very little radiation is emitted, yet are the main source of solar wind particles.

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SDO AIA-304

This channel is especially good at showing areas where cooler dense plumes of plasma (filaments and prominences) are located above the visible surface of the Sun. Many of these features either can't be seen or appear as dark lines in the other channels. The bright areas show places where the plasma has a high density.

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