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
Slight enhancement to the aurora is expected later on 27 Aug and 28 Aug, due to a mixture of fast solar winds and a weak Coronal Mass Ejection arrival. This could bring some viewings to northern geomagnetic latitudes, including northern Scotland.
Southern Hemisphere
Slight enhancement to the aurora is expected later on 27 Aug and 28 Aug, due to a mixture of fast solar winds and a weak Coronal Mass Ejection arrival. This could bring some viewings to southern geomagnetic latitudes, perhaps including the south of New Zealand.
Issued at: 18:16 (GMT) on Wed 26 Aug 2026
Forecast overview
Space Weather Forecast Headline: Moderate-class flares likely. Chance of isolated G1-G2 Minor to Moderate Geomagnetic Storms Days 2-4 (27-29 Aug).
Analysis of Space Weather Activity over past 24 hours
Solar Activity: Moderate, with a a single low Moderate class flare observed 26/0634 UTC from the complex sunspot region, now just west of the centre disc. Despite its relatively modest size, this is a relatively complicated region comprised of a number of small spots with multiple mixed magnetic polarities, and continues to show dynamical evolution. The other regions are all smaller and simpler, including a region now approaching the northwest limb, and relatively simple bipolar group in the northwest, and a simple mature unipolar spot
At least two Coronal Mass Ejections (CMEs) have been assessed as being potentially on the Earth-Sun line, including one from a Moderate flare which was just before this period. This was followed by a weak eruption around 25/1300UTC in a similar vicinity to the same spot. While these were deflected east, glancing impacts are likely on days 3 (28 Aug), perhaps continuing into early day 4 (29 Aug). A third slower CME potentially followed from around 25/2100UTC, however this has an uncertain source, is faint in imagery and slow, leading to very low confidence. The Moderate-class flare flare on 26 Aug also likely produced a weak CME, however this has yet to be identified on available imagery.
Solar Wind / Geomagnetic Activity: Solar winds, as measured at L1 by SOLAR-1, were indicative of the slow wind. Background solar wind speeds slowly declined from 340 km/s to just below 300km/s. Interplanetary Magnetic Field was weak with the north-south component also varying weakly. Geomagnetic activity was Quiet to Unsettled (Kp0-1).
Energetic Particles / Solar Radiation: The count rate of energetic particles (high energy protons) remained a little above normal background, but below the S1/Minor Radiation Storm threshold and easing.
Four-Day Space Weather Forecast Summary
Solar Activity: Moderate activity is forecast, with further Moderate-class flares most likely from the complex region near centre disc. There a slight chance of Strong-flares (X-class) from this region.
Solar Wind / Geomagnetic Activity: At least one CME arrival is likely to be observed on day 3 (28 Aug) from the eruptions on 25 Aug. Fast solar winds from a coronal hole are expected to be observed from early day 2 (27 Aug), with solar winds peaking around 500km/s. Geomagnetic activity will be mainly Quiet, but with spells of Unsettled to Active, with a likelihood of isolated G1 Minor Storms, with both the coronal hole and CME arrivals. There is a chance for isolated G2 intervals on day 3-4 (28-29). from any persistent CME influence.
Energetic Particles / Solar Radiation: The count rate of energetic particles (high energy protons) is most likely to continue at Background, but given the history of enhancements from the complex centre-disc region, even when it was in an unfavourable location, then any similar events bring a chance for these rates to rise. This give a chance for an S1-S2 Minor to Moderate radiation storm, most likley on day 3-4 (28-29 Aug).
Issued at: 12:20 (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: