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 next main enhancement to the auroral oval is expected during the early hours UTC of Friday 09 October, with the onset of a Coronal Mass Ejection (CME) that left the Sun at 06/0610UTC. Aurora may be visible across northern UK at peak and similar geomagnetic latitudes. On Friday and Saturday nights there is a small chance of visible aurora in northern Scotland and similar magnetic latitudes due to the fading influence of the CME and the possible arrival of a glancing blow from another CME PM of 10 Oct.
Southern Hemisphere
The next main enhancement to the auroral oval is expected during the early hours UTC of Friday 09 October, with the onset of a Coronal Mass Ejection (CME) that left the Sun at 06/0610UTC. Aurora may be visible across the south of the South Island of New Zealand at peak, perhaps also Tasmania and similar geomagnetic latitudes. On Friday and Saturday nights there is a reduced small chance of visible aurora due to the fading influence of the CME and the possible arrival of a glancing blow from another CME PM of 10 Oct.
Issued at: 03:36 (GMT) on Thu 8 Oct 2026
Forecast overview
Space Weather Forecast Headline: Chance of G2/Moderate storms Day 2 (09 Oct). Daily Chance of R1 Minor radio blackouts.
Analysis of Space Weather Activity over past 24 hours
Solar Activity: Solar activity is now at Low levels, with only Common-class flares observed in the past 24 hours. The peak being a C7.9 flare at 07/1317 UTC. There are currently four sunspot regions on the visible disc. The largest and most complex is near centre disc, which continues to show magnetic complexity, though appears to be generally stable in size. Another sunspot region, lying just to its northwest, is a smaller region, although this has recently increased in complexity too. The other regions are relatively simple sunspot regions.
A Coronal Mass Ejection (CME) associated with the peak flare was observed in imagery, which looks to give a glancing blow on Day 3 or 4 (10-11 Oct). No other earth directed CMEs have been observed.
Solar Wind / Geomagnetic Activity: Solar winds, as measured by SOLAR-1 at L1, suggest that Earth is now outside of the influence of the coronal hole fast winds. The solar wind speed has reduced from Slightly Elevated at 420km/s down to Background at 360-370km/s. The Interplanetary Magnetic Field, Bt, was Weak. The north-south component, Bz, was generally southward (negative). Geomagnetic activity was Quiet to Unsettled (Kp 1-3).
Energetic Particles / Solar Radiation: GOES18 10MeV proton flux has been predominantly at resting Background values.
Four-Day Space Weather Forecast Summary
Solar Activity: This is expected to be Low to Moderate, with a chance of Moderate-class activity from the more complex sunspot regions. These regions should remain on the Earth-facing disc throughout the next few days, with no significant returning regions otherwise due. This means there is an overall flat trend for a daily Chance of Moderate-class and very slight Chance of Strong flares.
Solar Wind / Geomagnetic Activity: The 06 Oct CME has been analysed with an arrival time most likely in the early UTC hours of Day 2 (09 Oct). There was a CME associated with the C7.9 flare at 07/1317 UTC, which has been analysed to give a glancing blow late on Day 3 (10 Oct) or early Day 4 (11 Oct).
Solar wind speeds have now declined to background levels, following the waning connection to the fast winds from a coronal hole. Other coronal hole influence is now unlikely to be a significant factor in the forecast, with two Earth-directed CMEs.
Geomagnetic activity is expected to be mostly Quiet on Days 1 (08 Oct), with a Slight Chance of G1/Minor Storm perhaps late Day 1 (08 Oct) if the CME arrives early. During Day 2 (09 Oct), with the expected CME arrival, conditions are likely to be Active to G1/Minor storm, with a chance of G2/Moderate storm intervals and a slight chance of G3/Strong storm intervals. These effects should span the remainder of Day 2 (09 Oct), before easing on Day 3 (10 Oct). However, if the 07 Oct CME arrives late on Day 3, this will keep conditions Unsettled to Active (Kp 3-4) with a chance of G1/Minor storms (Kp 5) and a slight chance of G2/Moderate storms (Kp 6). This CME is only a glancing blow and so the effects should be less than the early CME. While there is uncertainty with regards timing, by the end of Day 4 (11 Oct) it should ease back towards Quiet to Unsettled (Kp 1-3) with some Active (Kp 4) intervals and a reducing chance of G1/Minor storms (Kp 5).
Energetic Particles / Solar Radiation: There is a daily Slight Chance of S1 Minor Solar Radiation Storms, with this gradually increasing due to the westward progression of the two most complex sunspot regions.
Issued at: 00:29 (GMT) on Thu 8 Oct 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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