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
Auroral activity is expected to remain at background levels initially. However, the arrival of the CH73 high-speed stream during 09 July may lead to an enhancement of the auroral oval. As a result, aurora may become visible from northern Scotland and similar geomagnetic latitudes, although observations are likely to be limited by short hours of darkness and cloud cover.
Southern Hemisphere
Auroral activity is expected to remain at background levels initially. However, the arrival of the CH73 high-speed stream during 09 July (UTC) may enhance the auroral oval. As a result, aurora may become visible across southern New Zealand and similar geomagnetic latitudes.
Issued at: 02:19 (GMT) on Thu 9 Jul 2026
Forecast overview
Space Weather Forecast Headline: Chance of Moderate solar activity. Chance of G1 Day 1 (09 Jul), decreasing chance into Day 2 (10 Jul).
Analysis of Space Weather Activity over past 24 hours
Solar Activity: Solar activity has been Moderate over the past 24 hours, with two impulsive M-class flares from the large spot in the southeast.
There are five sunspot regions visible on the solar disc. The largest and most magnetically complex region is located in the southeast. It is dominated by a large leading spot, followed by two smaller trailing spots. A region in the southwest has undergone some raid development in the past 24hrs, and is one to watch. The remaining three regions are relatively small and magnetically simple.
A CME may have occurred in association with a Common class flare from a region in the southwest, but relevant imagery is still awaited to determine whether it contains an Earth-directed component.
Solar Wind / Geomagnetic Activity: Solar wind speeds likely showed the onset of coronal hole fast winds from a coronal hole just west of centre disc. Solar winds were background to slightly elevated for much of the period (350–430 km/s), but rose to around 470 km/s from 09/1130UTC. Total Interplanetary Magnetic Field, Bt, was weak to moderate. The north south component was predominantly weakly negative through the period. Geomagnetic activity was Quiet to Active (Kp1-4).
Energetic Particles / Solar Radiation: The count rate of energetic particles (high energy protons) was near background levels.
Four-Day Space Weather Forecast Summary
Solar Activity: Low to Moderate activity is expected to continue with a chance of further Moderate class flares.
Solar Wind / Geomagnetic Activity: No Earth-directed CMEs currently feature in the forecast period, but a CME may have occurred near centre disc on the morning of the 09th July, but relevant imagery is being awaited to conduct an analysis. The only significant feature during the forecast period is the largest coronal hole in the west of the solar disc This recurrent coronal hole is expected to connect with Earth through Day 1 (09 Jul), with speeds up to 600 km/s possible. A slow decline is then expected from Day 2 (10 Jul).
Geomagnetic activity is expected to remain mostly Quiet to Unsettled (Kp0–3) ahead of the expected fast winds during Day 1 (09 Jul). Activity is then expected to increase, becoming Unsettled to Active (Kp3-4), with a chance of G1 (Minor) geomagnetic storm intervals (Kp5), before activity begins to decline again from Days 2 and 3 (10-11 Jul) onward.
Energetic Particles / Solar Radiation: The count rate of energetic particles (high energy protons) have been at background levels in the past 24 hours, with no significant enhancements expected through this period.
Issued at: 12:26 (GMT) on Thu 9 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.
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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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