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.
Space weather notifications
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Aurora forecasts
Northern Hemisphere
No significant enhancements to the auroral oval are expected during the forecast period.
Southern Hemisphere
No significant enhancements to the auroral oval are expected during the forecast period.
Issued at: 00:41 (GMT) on Wed 2 Sep 2026
Forecast overview
Space Weather Forecast Headline: Slight-chance of Moderate-class flares.
Analysis of Space Weather Activity over past 24 hours
Solar Activity: Solar activity is Low. There are four numbered sunspot regions on the visible disc. The largest sunspot, in the northeast, is a relatively simple and stable uni-polar region. The most complex area remains in the southwest of the disc, with a bi-polar structure and continues to reduce in size. The remaining two regions are simple and relatively stable.
No Earth-directed CMEs were observed in available imagery.
Solar Wind / Geomagnetic Activity: Solar winds as measured at L1 by SOLAR-1, were at Slow or Slightly Elevated levels. Interplanetary Magnetic Field, Bt, was weak. The important north-south component was also Weak. This resulted in Quiet geomagnetic activity.
Energetic Particles / Solar Radiation: GOES18 >10MeV proton flux was at background levels.
Four-Day Space Weather Forecast Summary
Solar Activity: Activity is expected to remain Low or Very Low, with a slight-chance of Moderate levels from any isolated Moderate-class flares.
Solar Wind / Geomagnetic Activity: No Earth-directed Coronal Mass Ejections are currently forecast. Solar winds are expected to remain Slow or slightly elevated throughout the period, with no significant enhancements likely.
Geomagnetic activity is forecast to be mostly Quiet with a Chance of some Unsettled intervals.
Energetic Particles / Solar Radiation: GOES-18 >10MeV proton flux is expected to continue at background levels.
Issued at: 00:22 (GMT) on Wed 2 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.
Issued at: