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
No significant enhancements are expected to the auroral oval through the period, with aurora sightings limited to high geomagnetic latitudes.
Southern Hemisphere
No significant enhancements are expected to the auroral oval through the period, with aurora sightings limited to high geomagnetic latitudes.
Issued at: 08:10 (GMT) on Thu 6 Aug 2026
Forecast overview
Space Weather Forecast Headline: Slight chance of isolated Moderate-class flares.
Analysis of Space Weather Activity over past 24 hours
Solar Activity: Solar activity has been Very Low in the last 24 hours, with flare activity below Common-class levels.
There are currently five regions on the visible disc. In the northwest the largest sunspot region is located with its single moderate size alpha spot having separated in half and with some decrease in overall size. In the southwest is a modest size bipolar region, also showing some reduction in overall size. Remaining regions are small and simple.
Two slow Coronal Mass Ejections were detected on 03 Aug, associated with filament eruptions, though after analysis both are expected to miss Earth. A wide Coronal Mass Ejection from the northwest was detected on 04 Aug, with a possible glancing blow Day 3 (08 Aug).
Solar Wind / Geomagnetic Activity: Solar wind speeds were Background and on a slow downward trend from 370 km/s to 320 km/s. The Interplanetary Magnetic field was weak, with the north-south component also varying weakly, initially positive (northward) but trending mostly negative (southward) from 05/1500 UTC. Geomagnetic activity was Quiet.
Energetic Particles / Solar Radiation: GOES18 >10MeV proton flux is at background.
Four-Day Space Weather Forecast Summary
Solar Activity: Low to Very Low solar activity is expected to continue with just a slight chance of an isolated M-class flare.
Solar Wind / Geomagnetic Activity: Two slow Coronal Mass Ejections were detected on 03 Aug, though these are expected to miss Earth. A wide CME from the northwest was detected on 04 Aug, which may give a possible glancing blow Day 3 (08 Aug).
Solar winds are Slow-Ambient, and likely to remain at similar levels through much of the period. A narrow coronal hole evident in the southwest, is likely to be a little too far south to influence the current forecast, though should this connect with Earth it may give a slight enhancement to Slightly elevated levels on Day 3 (08 Aug).
Geomagnetic activity is expected to remain Quiet (Kp0-2), with a chance of Unsettled (Kp3) intervals for much of the period. On Day 3 (08 Aug), geomagnetic activity may rise to Unsettled (Kp3) with a chance of Active (Kp4) intervals, and a slight chance of an isolated G1/Minor Geomagnetic Storm (Kp5) interval due to possible glancing Coronal Mass Ejection and coronal hole high speed stream influences.
Energetic Particles / Solar Radiation: GOES18 >10MeV proton flux is expected to continue at Background.
Issued at: 12:07 (GMT) on Thu 6 Aug 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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