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
There are currently no active notifications.
Aurora forecasts
Northern Hemisphere
A slight enhancement to the aurora oval is expected to develop later Friday, continuing through to Saturday due to a mixture of enhanced solar winds and CME arrivals. This may bring viewings to higher latitudes, with a chance of sightings from southern Scotland and similar magnetic latitudes, where skies are clear during the limited hours of darkness.
Southern Hemisphere
Slight enhancement to the auroral oval is expected to develop later 28 Aug (UTC), continuing through 29 Aug and easing into 30 Aug (UTC), due to a mixture of coronal hole fast winds and CME arrivals. This is likely to bring viewings to higher latitudes, with a chance of sightings from southern New Zealand and similar magnetic latitudes.
Issued at: 13:11 (GMT) on Fri 28 Aug 2026
Forecast overview
Space Weather Forecast Headline: Chance of Moderate class flares. Minor Geomagnetic Storm likely Day 1 (28 Aug), chance of Moderate Storm.
Analysis of Space Weather Activity over past 24 hours
Solar Activity: Solar activity has been Low over the past 24 hours, with only Common class flares. There are six regions on the visible disc. A moderately sized group in the northwest has been the most complex, but continues tor educe in size and complexity. The largest region on the disc is also in the northwest and has become longer in recent hours. The remaining spots are smaller and magnetically simple, including a NEW region in the southeast.
No significant Earth directed Coronal Mass Ejections (CME) were seen in available imagery over the last 24 hours.
Solar Wind / Geomagnetic Activity: Solar winds, as measured at L1 by SOLAR-1, were indicative of a slow wind. Solar wind speeds were at background levels, below 300km/s. Interplanetary Magnetic Field was mainly weak but did become Moderate at the end of the period. The north-south component mainly varied weakly, but did become moderately southwards to end the period. Geomagnetic activity was Quiet.
Energetic Particles / Solar Radiation: The count rate of energetic particles (high energy protons) was near background, with no Solar Radiation Storms observed.
Four-Day Space Weather Forecast Summary
Solar Activity: Activity is expected to remain Low, with a slight but increasing chance of isolated M-class flares over the coming days.
Solar Wind / Geomagnetic Activity: At least two Coronal Mass Ejections (CMEs) from 25 Aug may reach Earth, along with a third, much lower confidence CME. The first two are likely to give a glancing, but potentially combined, impact on Day 1 (28 Aug), with any enhancement from the third perhaps prolonging CME influence into Day 2 (29 Aug). A solar wind enhancement is still expected, arriving early Day 1, potentially peaking with speeds 450-500km/s. There are significant uncertainties regarding the onset of coronal hole fast winds and this may influence the timings of the aforementioned CMEs, potentially resulting in later-than-expected arrivals and reducing confidence in the short-term geomagnetic forecast.
Geomagnetic activity is expected to be Quiet (Kp0-2) initially, before becoming Unsettled to Active (Kp3-4), with G1/Minor Storm (Kp5) intervals likely. There is a Slight Chance of G2/Moderate storm (Kp6) intervals upon any CME impact. Activity then likely to continue into Day 2 before gradually waning into Days 3 and 4.
Energetic Particles / Solar Radiation: The count rate of energetic particles (high energy protons) is most likely to continue at background levels, but with a slight chance of solar radiation reaching S1/Minor Radiation Storm.
Issued at: 12:19 (GMT) on Fri 28 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: