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.
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Aurora forecasts
Northern Hemisphere
The auroral oval is likely to become active following connection to a high speed stream on Thursday night, with aurora possibly visible across the north of Scotland and similar magnetic latitudes. This activity may persist on Friday evening, due to the potential arrival of a minor geomagnetic storm.
Southern Hemisphere
The auroral oval is likely to become active following connection to a high speed stream and the arrival of a geomagnetic storm on Thursday night, with aurora possibly visible across the southern portion of New Zealand and similar magnetic latitudes. This activity may persist on Friday evening, due to the potential arrival of a minor geomagnetic storm.
Issued at: 00:14 (GMT) on Wed 26 Aug 2026
Forecast overview
Space Weather Forecast Headline: R1/Minor Radio Blackouts likely. Chance of G1/Minor Geomagnetic Storm Days 2-3 (27-28 Aug).
Analysis of Space Weather Activity over past 24 hours
Solar Activity: Solar activity has been Moderate over the past 24 hours with several Moderate-class flares from the large and complex region near the centre disc, the largest peaking at 25/1002 UTC.
There are currently four sunspot regions on the visible disc. The aforementioned region near the centre disc remains the most notable due to its magnetic complexity, with two clear delta spots. The other regions are relatively simpler with little to no activity observed at this point.
The recent Moderate-class flare that was emitted from the large and complex region near the centre disc produced an Earth-directed CME (Coronal Mass Ejection). A filament eruption followed shortly afterwards in the vicinity of the active region; however, analysis is still ongoing to determine its characteristics and potential Earth-directed component. filament eruption followed shortly afterwards; however, analysis is still ongoing to determine its characteristics and potential Earth-directed component.
Solar Wind / Geomagnetic Activity: Solar winds were indicative of a slow regime. Speeds were stable and around 320-350 km/s. Interplanetary Magnetic Field was weak, with the north-south component also varying weakly. Geomagnetic activity was Quiet (Kp0-1).
Energetic Particles / Solar Radiation: GOES18 >10MeV proton flux was a little above normal background levels, but below the S1/Minor Radiation Storm threshold.
Four-Day Space Weather Forecast Summary
Solar Activity: Moderate activity is forecast, with further Moderate-class flares likely from the large region near centre disc. There remains a slight chance of Strong-flares from this region.
Solar Wind / Geomagnetic Activity: The recent Moderate-class flare produced an Earth-directed CME. Preliminary analysis suggests the CME could arrive at Earth on Day 3 (Friday).
Solar wind speeds are expected to remain slow on Day 1 (26 Aug) otherwise, before the arrival of the fast stream associated with CH90/+, likely on Day 2 (27 Aug). Wind speeds may increase to around 500 km/s, and potentially up to 550 km/s under the influence of the CME.
Geomagnetic activity is expected to remain Quiet (Kp 0–2) initially. However, conditions are likely to become Unsettled to Active (Kp 3–4) from Day 2 (27 August), with an increasing chance of G1/Minor Storm (Kp 5) intervals as the anticipated high-speed stream (HSS) from CH90/+ arrives.
The expected CME arrival on Day 3 (28 August) is then likely to maintain elevated geomagnetic activity, with a further chance of G1/Minor Storm intervals. Activity should begin to subside on Day 4, although Unsettled to Active (Kp 3–4) conditions may persist before gradually easing.
Energetic Particles / Solar Radiation: There is a generally increasing chance of solar radiation reaching above the S1/Minor radiation storm threshold through the period.
Issued at: 00:08 (GMT) on Wed 26 Aug 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.
Issued at:
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.
Issued at: