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 that left the Sun at 06/0610UTC. Aurora may be visible across northern UK at peak and similar geomagnetic latitudes. There remains a chance of visible aurora in northern Scotland and similar latitudes due to the fading influence of the 06 Oct coronal mass ejection on Friday 09 Oct night. On Saturday 10 Oct night, a possible glancing arrival of the 07 Oct coronal mass ejection will bring a Chance of visible aurora across Scotland and similar latitudes where skies are clear.
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 that left the Sun at 06/0610UTC. Aurora may be visible across Southern New Zealand and Tasmania at peak and similar geomagnetic latitudes. On Saturday 10 Oct UTC, a possible glancing arrival of the 07 Oct coronal mass ejection will bring a Chance of visible aurora across the far south of New Zealand and similar latitudes where skies are clear.
Issued at: 12:57 (GMT) on Thu 8 Oct 2026
Forecast overview
Space Weather Forecast Headline: G1/Minor Expected, Chance of G2/Moderate Geomangnetic Storms Day 2. G1/Minor Geomagnetic Storms Likely Days 3 and 4. 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. Peaking at 07/1317 UTC from near centre disc.
There are currently three sunspot regions on the visible disc. The largest and most complex is in the northwest. This area continues to exhibit areal growth and elongation, with significant magnetic complexity. A smaller and less complex region lies just to the northwest. The remaining region, in the southeast, is a small, mature and simple spot.
A coronal mass ejection 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 coronal mass ejections have been observed.
Solar Wind / Geomagnetic Activity: Solar winds have exhibited background conditions. The solar wind speed was Slow-Ambient. The Interplanetary Magnetic Field was Weak. The north-south component was generally southward (negative) but Weak. Geomagnetic activity was Quiet to Unsettled (Kp 1-3).
Energetic Particles / Solar Radiation: GOES18 10MeV proton flux has been predominantly at 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 complex sunspot in the northwest.
Solar Wind / Geomagnetic Activity: Two coronal mass ejections feature in the forecast. A likely direct hit from the 06 Oct coronal mass ejection is due early Day 2 (09 Oct), followed by a glancing blow of 07 Oct coronal mass ejection later Day 3 (10 Oct) or early on Day 4 (11 Oct).
Slow winds should continue through Day 1 (08 Oct). The next significant coronal hole fast wind, is likely to arrive beyond the current forecast period.
Geomagnetic activity is expected to be mostly Quiet Day 1 (08 Oct), with a Slight Chance of G1-G3/Minor-Strong (Kp5-7) storms late Day 1 (08 Oct) if the 06 Oct coronal mass ejection arrives early. G1/Minor (Kp5) storms are Expected, with a Chance of G2/Moderate (Kp6) and a Slight Chance of G3/Strong storm (Kp7) intervals on Day 2 (09 Oct), before easing back to Quiet to Active (Kp2-4) into early Day 3 (10 Oct). Later on Day 3 or early Day 4 (10-11 Oct), the glancing blow of 07 Oct coronal mass ejection will bring Likely G1/Minor storms (Kp5) and a Slight Chance of G2/Moderate storms (Kp6). Later Day 4 (11 Oct), geomagnetic activity should ease to Quiet to Unsettled (Kp1-3).
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 complex sunspot region.
Issued at: 12:11 (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.
Issued at: