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
Aurora activity is expected to be near background levels until the arrival of a solar wind enhancement late 11 June (UTC). This is likely to slightly enhance aurora activity, with aurora potentially visible across northern parts of Scotland and similar magnetic latitudes during the UTC night of the 11 June, and less likely through the night of 12 June. However, short hours of darkness will limit any viewings where skies are clear.
Southern Hemisphere
Aurora activity is expected to be near background levels until the arrival of a solar wind enhancement late 11 June (UTC). This is likely to slightly enhance aurora activity, with aurora potentially visible where skies are clear, across the far south of New Zealand and similar magnetic latitudes during the UTC night of the 11 June, and less likely through the night of 12 June.
Issued at: 01:06 (GMT) on Wed 10 Jun 2026
Forecast overview
Space Weather Forecast Headline: Minor storms Likely Days 2-3 (11-12 June). Chance of isolated Moderate-class flares throughout.
Analysis of Space Weather Activity over past 24 hours
Solar Activity: Solar activity has been Low over the past 24 hours, with frequent Common-class flares.
There are currently ten regions on the Earth-facing disc, of which seven are numbered. A region in the northeast is the largest and most complex, with a small delta spot now apparent. A region in the southeast is the second largest region, although it is magnetically straightforward. The remaining regions are smaller and magnetically simple. Most regions are stable or have shown limited changes, but one new region in the northwest has emerged over the past 24 hours, and has developed into a small Csi/beta-gamma.
A CME was seen leaving the Sun in the northwest around 09/1557 UTC. Analysis is on-going, but the CME is not expected to be Earth-directed. Another CME was seen leaving the Sun, after a Common class flare from a plage region in the southwest. Once sufficient corongraph imagery is available analysis will be undertaken, as this later CME has a much greater potential of having an Earth directed component.
Solar Wind / Geomagnetic Activity: Solar winds were slightly elevated, with a weak CME arrival at 09/0955 UTC. Wind speeds were slightly elevated between 400-500km/s. Interplanetary magnetic field was weak until the CME arrival when it jumped to moderate. The north-south component varied weakly. Geomagnetic activity was Quiet to Unsettled.
Energetic Particles / Solar Radiation: No solar radiation storms were observed with energetic particles near background.
Four-Day Space Weather Forecast Summary
Solar Activity: Solar activity is forecast to be Low to Moderate, with a chance of isolated Moderate-class flares and a slight chance of a Strong flare.
Solar Wind / Geomagnetic Activity: The CME that emerged on 06 June arrived at 09/0955 UTC, but was slow and very weak. The current slightly elevated solar wind speeds are expected to decline towards background through Day 1 (10 Jun). The next enhancement is expected to come from a coronal hole feature currently near centre disc, potentially bringing wind speeds of 650-700 km/s, and arriving later Day 2 (11 Jun). Solar wind speeds are expected to decline to elevated levels either later Day 3 (12 Jun) or through Day 4 (13 Jun).
Geomagnetic activity is expected to start at Quiet to Unsettled levels then decline through Day 1 (10 Jun) to become mainly Quiet until the arrival of the fast winds. Then activity is expected to increase to become Active to Minor Storms, with Minor Storms Likely late Day 1 into early Day 2 (11 Jun). Through Day 4 (13 Jun) activity is expected to decline to become Quiet to Unsettled.
Energetic Particles / Solar Radiation: High energy proton flux is expected to remain close to background, although there is a slight chance of S1 (Minor) solar radiation storms if any notable flares occur.
Issued at: 00:29 (GMT) on Wed 10 Jun 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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