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.

Image courtesy of NASA/SDO and the AIA, EVE, and HMI science teams

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Aurora forecasts

Northern Hemisphere

There is a chance of visible aurora from northern Scotland where skies are clear, overnight Friday 14 August UTC into Saturday 15 August. Activity will otherwise be subdued.

Southern Hemisphere

There is a chance of visible aurora from high latitudes where skies are clear, during the southern hemisphere morning on Saturday 15 August. Auroral activity will otherwise be subdued.

Issued at: 02:14 (GMT) on Fri 14 Aug 2026

Forecast overview

Space Weather Forecast Headline: Chance of Minor Geomagnetic Storm Friday 14 August.

Analysis of Space Weather Activity over past 24 hours

Solar Activity: Activity remained very low, with no significant x-ray flares recorded (below common-class throughout).

There are currently six numbered sunspot regions on the visible disc, and one small and weak yet to be numbered region in the southeast. The most significant region is a moderately sized region approaching centre disc, as this region has grown through the period to become magnetically complex as a small delta spot has recently developed within the penumbra of the lead spot. The remaining regions on the disc are magnetically simple unipolar or bipolar regions, most are small and have only shown slight changes through the period.

No Earth directed Coronal Mass Ejections (CME's) were observed in available imagery.

Solar Wind / Geomagnetic Activity: Solar winds were predominantly at background levels of 400 km/s or below, but did occasionally reach Slightly Elevated levels, peaking at 412 km/s at 13/0154 UTC. The strength  of the solar winds magnetic strength was at weak levels, as was the important north-south component which weakly fluctuated.

The net result of the above solar wind measures was for Quiet geomagnetic activity increasing to Unsettled at the end of the period.

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 moderately sized region should depart the disc to end the UTC weekend. Two returning regions may rotate onto the disc through the next two days, but they are unlikely to be significant. Therefore, there is only a slight chance of isolated Moderate class flares.

Solar Wind / Geomagnetic Activity: No CMEs feature in the forecast. The current solar wind regime may give way to a solar wind enhancement from a coronal hole later Day 1 or early Day 2 (14 and 15 Aug). Should the enhancement arrive the initial Quiet to Unsettled activity is expected to increase to become Unsettled to Active, with a Chance of Minor geomagnetic storms intervals, later Day 1 (14 Aug) into Day 2 (15 Aug). Activity then declines to become increasingly Quiet through Days 3 and 4 (16 and 17 Aug).   

Energetic Particles / Solar Radiation: No solar radiation storms are expected - given the lack of suitably complex, well-connected sunspot regions (i.e. larger regions in the west).

Issued at: 00:17 (GMT) on Fri 14 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.

Issued at:

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