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 auroral oval is expected to remain mostly quiet through the period, with auroral sightings unlikely.
Southern Hemisphere
The auroral oval is expected to remain mostly quiet through the period, with auroral sightings unlikely.
Issued at: 03:05 (GMT) on Thu 10 Sep 2026
Forecast overview
Space Weather Forecast Headline: Chance of G1/Minor storm, Day 2 (11 Sep).
Analysis of Space Weather Activity over past 24 hours
Solar Activity: Solar activity was at Low levels, with occasional Common-class flares observed.
There are currently up to eight sunspot regions visible on the solar disc. Most regions remain relatively simple, unipolar groups. The exception is a small bipolar region in the north centre disc. No Earth-directed Coronal Mass Ejections (CMEs) have been seen in available imagery in the last 24 hours.
A CME was observed departing the Sun at approximately 09/0900 UTC and, while the results of its analysis are still pending, it is not expected to be Earth-directed.
Solar Wind / Geomagnetic Activity: Solar winds reflected the ongoing influence of the magnetic cloud associated with one or possibly two CME arrivals. Wind speeds were slightly elevated at around 400 km/s; however, from approximately 09/0410 UTC, they increased modestly, peaking near 460 km/s. This enhancement is most likely associated with the arrival of a weak CME. The Interplanetary Magnetic Field was generally weak, but strengthen following the arrival of the weak CME, briefly reaching moderate levels. The important north-south component varied weakly but was often southward directed. Geomagnetic activity remained Quiet to Unsettled (Kp 2-3).
Energetic Particles / Solar Radiation: Solar radiation was at normal background levels.
Four-Day Space Weather Forecast Summary
Solar Activity: Solar activity is expected to remain Low to Very Low, although there is a slight chance of isolated M-class flaring.
Solar Wind / Geomagnetic Activity: Earth continues to experience the influence of a magnetic cloud associated with one or possibly two weak CMEs, with solar wind speeds currently around 460 km/s.
A coronal hole, CH92/+, may bring a high-speed stream, potentially driving solar wind speeds back above 500 km/s late on Day 2 and into Day 3 (11-12 Sep). However, this feature is not recurrent, resulting in low confidence in both the timing of arrival and the magnitude of any associated solar wind enhancement.
As a result, geomagnetic activity is expected to remain predominantly Quiet to Unsettled, with a slight chance of isolated Active intervals through Day 1 (10 Sep). Activity is then expected to increase late on Day 2 (11 Sep) as the CH92/+ high-speed stream begins to influence Earth, bringing a chance of Active to G1 (Minor Storm) conditions from late 11 Sep into 12 Sep. Thereafter, activity is expected to gradually subside, with predominantly Quiet to Unsettled conditions likely on Day 4 (13 Sep).
Energetic Particles / Solar Radiation: Solar radiation is now at background, with a very slight chance of further enhancements above the S1/Minor Radiation Storm threshold.
Issued at: 00:12 (GMT) on Thu 10 Sep 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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