| No. | Type | Alerts | Warnings | Watches |
|---|---|---|---|---|
| 1 | Proton Flux 10MeV Alert |
S1:
03:15 (GMT) on Fri 31 Jul 2026 |
||
| 1 | Proton Flux 10MeV Warning |
S1:
18:59 (GMT) on Thu 30 Jul 2026 to 09:00 (GMT) on Fri 31 Jul 2026 |
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
Aurora forecasts
Northern Hemisphere
Only minor enhancements to the auroral oval are expected over the coming days. Any visible aurora is likely to remain confined to high geomagnetic latitudes, where observations will also be limited by the short hours of darkness at this time of year.
Southern Hemisphere
Only minor enhancements to the auroral oval are expected over the coming days. Any visible aurora is likely to remain confined to high geomagnetic latitudes.
Issued at: 01:47 (GMT) on Fri 31 Jul 2026
Forecast overview
Space Weather Forecast Headline: Chance of isolated Moderate-class flares.
Analysis of Space Weather Activity over past 24 hours
Solar Activity: Solar activity has reached Moderate following a low level Moderate class flare peaking at 30/1700UTC.
There are currently eight regions on the Earth-facing disc, none of which displayed any significant development. The largest is a region in the northeast, which is moderately magnetically complex. The most complex region is also in the northeast, with a small delta spot in it's main intermediate spot group. However, the most active region has been a moderately sized and apparently simple and stable group approaching the northwest limb. The remaining regions are smaller and mostly magnetically simple.
A filament eruption in the northwest triggered a Moderate class flare from a region in the northwest. An associated Coronal Mass Ejection (CME) is visible in (currently limited) coronagraph imagery. This CME will be analysed but it is expected to have an Earth directed component.
Solar Wind / Geomagnetic Activity: Solar wind observations showed weak slow wind conditions with Background speeds, below 400km/s. Interplanetary Magnetic Field was Weak, with the north-south component also weak and occasionally southward. Geomagnetic activity was Quiet.
Energetic Particles / Solar Radiation: The count rate of energetic particles (high energy protons) started the period at Background levels, but rapidly increased following the Moderate class flare. Minor radiation storm levels were reached at 30/1903 UTC and are currently ongoing.
Four-Day Space Weather Forecast Summary
Solar Activity: Low activity is likely, but with a chance of rising to Moderate due to isolated Moderate-class flares. No significant regions are expected to rotate onto the disc during the forecast period.
Solar Wind / Geomagnetic Activity: A weak, slow, and faint CME may deliver glancing impacts late day 1 (31 July), with a potential weak CME that was possibly arriving early on the 30th now considered to have missed Earth. The CME arrival on day 1 is considered more likely to mostly miss Earth. Modelling is awaited for the CME that was associated with the filament eruption and M1.9 flare on the 30th, with the expectations there will be an Earth directed component. Outside of any CME arrivals Background slow winds conditions are expected to largely prevail, with only a slight enhancement possible from any fast wind from a coronal hole feature in the southern hemisphere, which is expected to pass mostly south of Earth. Quiet activity is generally expected, with isolated Unsettled spells, but also a chance of Active intervals from any CME glance or fast wind enhancement until late Day 2 or Day 3 (1st or 2nd Aug) when there is a potential for Minor geomagnetic storms should the CME from the 30th arrive.
Energetic Particles / Solar Radiation: The count rate of energetic particles (high energy protons) is currently at Minor storms levels and is expected to gradually decline through Days 1 and 2 (31st and 1st), returning to Background levels by the end of the period, provided no further proton events occur.
Issued at: 00:28 (GMT) on Fri 31 Jul 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: