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

Waning fast winds may still give some high latitude aurora early on 22 Oct UTC, with a chance of this reaching northern Scotland and similar magnetic latitudes. This activity is expected to ease later on 22 Oct UTC, but another high latitude increase is possible on 24 Oct UTC due to potential further fast winds, followed by a possible glancing Coronal Mass Ejection on 25 Oct UTC, which could bring aurora back to northern Scotland and similar latitudes.

Southern Hemisphere

Waning fast winds may still give some high latitude aurora early on 22 Oct UTC, with a chance of this reaching the far south of New Zealand and similar magnetic latitudes. This activity is expected to ease later on 22 Oct UTC, but another high latitude increase is possible on 24 Oct UTC due to potential further fast winds, followed by a possible glancing Coronal Mass Ejection on 25 Oct UTC, which could bring aurora back to far southern New Zealand and similar latitudes.

Issued at: 02:31 (GMT) on Thu 22 Oct 2026

Forecast overview

Space Weather Forecast Headline: Slight chance of isolated Moderate-class flares. Chance of G1/Minor Storm Days 1 and 4 (22/25 Oct).

Analysis of Space Weather Activity over past 24 hours

Solar Activity: Solar activity has been Low with occasional Common class flares. There are three sunspot regions on the disc. The region on the west limb was previously the most active, however this is no longer fully visible as it is rotating off the disc. A region in the northwest has declined slightly in area, and remains a fairly straightforward region. Another region in the northwest quadrant has seen slight growth of penumbra, and appears to have developed a little magnetic complexity.

During 21 Oct, a re-alignment of the Sun's outer layer appears to have been responsible for at least one CME. Initial analysis suggests the CME will mostly pass behind Earth's orbit, but given the central location of the likely lift off point, a glancing blow is possible, likely during Day 4 (25 Oct). 

Solar Wind / Geomagnetic Activity: Solar winds showed a weak connection to coronal hole fast winds. Wind speeds were initially mostly background, between 370-410 km/s, but increased to vary between 450-520 km/s. Interplanetary Magnetic Field was mostly moderate, with the north-south component also varying moderately, favouring a southward (negative) orientation. Geomagnetic activity was Quiet to Active (Kp2-4), with a G1/Minor Storm (Kp5) interval 21/2100-2359 UTC.

Energetic Particles / Solar Radiation: No solar radiation storms were observed with the count rate of energetic particles persisting at background levels.

Four-Day Space Weather Forecast Summary

Solar Activity: Mainly Low activity is expected to continue, but with a slight chance of increasing to Moderate.

Solar Wind / Geomagnetic Activity: During 21 Oct, a re-alignment of the Sun's outer layer generated at least one CME, and a new coronal hole near centre disc. Initial analysis of the CME suggests it will mostly pass behind Earth's orbit, but a glancing blow is possible, likely during Day 4 (25 Oct). Weak influence from the current fast wind is likely to erratically decline towards background on Day 1 into Day 2 (22-23 Oct). The newly developed coronal hole near centre disc could give fast winds Day 3 into Day 4 (24-25 Oct), although with low confidence.

Geomagnetic activity is expected to be Unsettled to Active at first, with a chance of G1/Minor storm intervals, easing to mostly Quiet during Day 1. The potential onset of fast winds during Days 3-4 then perhaps bringing Unsettled to Active conditions with a slight chance of G1/Minor storm intervals, this becoming a chance of G1 during Day 4 if the CME arrives.

Energetic Particles / Solar Radiation: No solar radiation storms are forecast with the count rate of energetic particles expected to persist at background levels.

Issued at: 00:12 (GMT) on Thu 22 Oct 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.

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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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