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
There is a chance of high geomagnetic latitude enhancement to the aurora, perhaps peaking later in the UTC day of Friday 14 August due to a possible fast solar wind developing, although this carries low confidence. Activity should otherwise be subdued.
Southern Hemisphere
There is a chance of high geomagnetic latitude enhancement to the aurora, perhaps peaking later in the UTC day of Friday 14 August due to a possible fast solar wind developing, although this carries low confidence. Activity should otherwise be subdued.
Issued at: 14:03 (GMT) on Thu 13 Aug 2026
Forecast overview
Space Weather Forecast Headline: Chance of Minor Geomagnetic Storm G1, peaking Friday 14 August.
Analysis of Space Weather Activity over past 24 hours
Solar Activity: Activity fell to very low, with no significant x-ray flares recorded (below common-class throughout).
There are currently up to six sunspot regions on the facing side of the Sun, with a new, small magnetically bipolar region developing. The complexity of the sunspot regions overall increased in the period, with three of the main bipolar regions showing growth, although this did not culminate in increased flaring in any case. Remaining regions were generally smaller, simpler and more stable.
Satellite imagery showed a faint, small Coronal Mass Ejection (CME) heading mainly south and west of the Sun-Earth line. This feature may be associated with a minor emission from the vicinity of a sunspot in the southwest. It has been analysed and is not expected to affect Earth.
Solar Wind / Geomagnetic Activity: Solar winds were slightly elevated in the period, perhaps due fading influence from a minor fast solar wind. The solar wind speed fell from early slightly elevated highs to become background by the end of the period. The number of particles in the solar wind and their associated magnetic field were both near average, which reduced any effect from the mainly anti-aligned north-south component of the field (with Earth's field).
The net result of the above solar wind measures was for provisionally quiet geomagnetic activity throughout.
Energetic Particles / Solar Radiation: No solar radiation storms were observed.
Four-Day Space Weather Forecast Summary
Solar Activity: Activity will most likely be low, with isolated Common-class flares. One of the larger and growing sunspot regions should depart the disc to end the UTC weekend, and with no returning regions due or evidence of them in far-side satellite imagery, there is therefore a falling slight chance of Moderate-class flares.
Solar Wind / Geomagnetic Activity: No CMEs feature in the forecast. The current solar wind regime may give way to a (stronger) fast wind before the end of the UTC working week. This is low confidence, with modelling suggesting the fast wind may alternatively pass slightly north of the plane of the Earth's orbit. There is felt to be a peak chance of G1/Minor geomagnetic storms Day 2, Friday 14 August, soon waning to increasingly Quiet activity over Day 4 (Sunday 16 August).
Energetic Particles / Solar Radiation: No solar radiation storms are expected - given the dearth of suitably complex, well-connected sunspot regions (i.e. larger regions in the west).
Issued at: 12:19 (GMT) on Thu 13 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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