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
Weak enhancements to the aurora are possible overnight Wednesday into Thursday (22-23rd). This will bring a chance for brief glimpses of visible aurora from northern Scotland and other locations at similar geomagnetic latitudes. However, the shortened hours of darkness at this time of year will significantly limit viewing opportunities.
Southern Hemisphere
Weak enhancements to the aurora are possible during the southern hemisphere Wednesday into Thursday (22-23rd). This will bring a chance for brief glimpses of visible aurora from the southernmost parts of New Zealand and other locations at similar geomagnetic latitudes.
Issued at: 06:05 (GMT) on Wed 22 Jul 2026
Forecast overview
Space Weather Forecast Headline: Moderate-class flares likely. Chance of Minor Storms days 1-2 (22-23 Jul).
Analysis of Space Weather Activity over past 24 hours
Solar Activity: Moderate with two Moderate-class flares from the most notable of the four regions on the Earth-facing disc, located in the centre disc. This has at least one mixed polarity spot, but is showing a simplifying trend as it moves into the western hemisphere. The remaining spots are mature unipolar spots and generally showing a decaying trend.
A CME (Coronal Mass Ejection) from the northwest on 21 Jul is under analysis for any glancing impacts, but is most likely to pass to the north of Earth. No other CMEs were observed in available imagery that could have a potential Earth-directed component
Solar Wind / Geomagnetic Activity: Solar winds showed a slight enhancement, likely due to the fast winds from the southern coronal hole in the southwest. Solar wind speeds have been Background to Slightly Elevated at 370-460 km/s. Total Interplanetary Magnetic Field eased from Strong, to be Background to Moderate from 21/1700 UTC. The north-south component remained Moderate and variable in direction. Geomagnetic activity was Quiet to Unsettled (Kp 2-3).
Energetic Particles / Solar Radiation: The count rate of energetic particles (high energy protons) was at Background with no Solar Radiation storms observed.
Four-Day Space Weather Forecast Summary
Solar Activity: Low to Moderate activity is likely to continue, with further M-class flares likely and a slight chance of X-class flares, mainly from the region moving into the western disc.
Solar Wind / Geomagnetic Activity: There are no Earth-directed CMEs however an eruption to the northwest is under analysis for any Earth-directed component. Ongoing Slightly Elevated winds are expected, before likely becoming Elevated to Strong, perhaps peaking 600km/s, due to a further enhancement from the next coronal hole sourced fast winds. This is most likely later day 1 or day 2 (22-23 Jul) , before easing later in the period. Geomagnetic activity is expected to be Quiet to Unsettled, but with Active spells and a chance of G1 Minor Storm intervals if any fast wind enhancement is observed. Any CME glance also brings a slight chance of G1-G2 Minor Storms, however this is low confidence for timing or if any impact will occur at this stage.
Energetic Particles / Solar Radiation: The count rate of energetic particles (high energy protons) is expected to be Background with no Solar Radiation storms occurring. However, any significant eruptions from the central disc sunspot could increase the observed count rates.
Issued at: 12:20 (GMT) on Wed 22 Jul 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.
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