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
Low activity is expected overnight on 22 Oct (UTC) with visible aurora unlikely. However, with possible connection to a coronal hole on 23/24 Oct, it is possible there could be a chance of visible aurora in northern Scotland and similar latitudes on Saturday (UTC) night. On 25 Oct there may be a glancing blow from a Coronal Mass Ejection, giving a chance of aurora in northern Scotland where skies are clear on Sunday (UTC) night.
Southern Hemisphere
Low activity is expected overnight on 22 Oct (UTC) with visible aurora unlikely. However, with possible connection to a coronal hole on 23/24 Oct, it is possible there could be a chance of visible aurora in the far south of New Zealand and similar latitudes on Saturday (UTC) night. On 25 Oct there may be a glancing blow from a Coronal Mass Ejection, giving a chance of aurora in southern New Zealand where skies are clear on Sunday (UTC) night.
Issued at: 15:37 (GMT) on Thu 22 Oct 2026
Forecast overview
Space Weather Forecast Headline: Slight chance of isolated Moderate-class flares. Chance of G1/Minor Storm Day 4 (25 Oct).
Analysis of Space Weather Activity over past 24 hours
Solar Activity: Solar activity has been Low with occasional Common-class flares, peaking at C3.5 at 22/0309 UTC. There are two sunspot regions on the disc. One area, in the far west is a relatively straightforward bipolar region. The region in the northwest quadrant, is the biggest region and has increased in magnetic complexity in its intermediate region.
During 21 Oct, a coronal re-alignment was seen in the Sun's northern hemisphere. This appears to have been responsible for at least one Coronal Mass Ejection (CME). 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, as measured by SOLAR-1 at L1, showed weak connection the fast winds of a coronal hole Wind speeds have generally been Slightly Elevated, though did become Elevated for a time between 21/1354 UTC and 21/1533 UTC. Interplanetary Magnetic Field, Bt, started moderate and since 21/1755 UTC has been slowly decreasing, becoming generally Weak from 22/0057 UTC. The north-south component, Bz, has been generally weak and southward (negative), but did become weak and northward (positive) for a time between 21/2329 UTC and 22/0347 UTC. Geomagnetic activity was Quiet to Active (Kp 2-4) with a G1/Minor Storm (Kp 5) 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 October, a coronal re-alignment was seen in the Sun's northern hemisphere. This appears to have been responsible for at least one CME, alongside the creation of a new coronal hole near centre disc. 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 coronal hole fast winds is expected to ease during Day 1 (22 Oct), with the slightly elevated wind speeds erratically declining towards background on Day 1 into Day 2 (22-23 Oct). However, a newly developed coronal hole near centre disc could give fast winds Day 3 into Day 4 (24-25 Oct), although confidence in this is low. MOSWOC Enlil is not providing useful guidance at this point, as it has been over-estimating the current fast winds, and has not yet captured any fast winds from the new coronal hole.
Geomagnetic activity is expected to be Quiet to Unsettled (Kp 0-3), with Active (Kp 4) intervals possible at first. The potential onset of fast winds during Days 3-4 then perhaps bringing Unsettled to Active (Kp 3-4) conditions with a slight chance of G1/Minor storm (Kp 5) intervals, increasing to a chance of G1/Minor storm (Kp 5) intervals during Day 4 (24 Oct).
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: 12:00 (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.
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: