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 23 Oct (UTC) with visible aurora unlikely. However, a possible weak solar wind enhancement on Oct 24 could lead to a chance of visible aurora across the far north of Scotland and similar latitudes on Saturday (UTC) night. On 25 Oct there may be a glancing blow from a weak CME, giving a chance of aurora across northern Scotland where skies are clear on Sunday (UTC) night.
Southern Hemisphere
Low activity is expected at first with visible aurora unlikely. However, a possible weak solar wind enhancement could lead to a chance of visible aurora across the far south of New Zealand, and similar latitudes, through the southern hemisphere Saturday night. On 25 Oct there may be a glancing blow from a weak CME, giving a chance of aurora across southern New Zealand and similar latitudes during the southern hemisphere night, where skies are clear.
Issued at: 01:21 (GMT) on Fri 23 Oct 2026
Forecast overview
Space Weather Forecast Headline: Slight chance of isolated Moderate-class flares. Chance of Minor Storm Day 3 (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, both in the northwest quadrant and showing recent slight growth. One is a relatively straightforward bipolar region. The remaining region is the largest region and currently has moderate magnetic complexity, after a previous small delta spot faded.
No Earth directed Coronal Mass Ejections (CME's) were observed in available imagery.
Solar Wind / Geomagnetic Activity: Solar winds showed a continued weak connection to the fast winds from a small coronal hole in the northwest, with Slightly Elevated winds throughout, peaking at 493 km/s at 22/0119 UTC. The strength of the solar winds magnetic field remained Weak. The north-south component was Weak throughout and predominantly southward but did become northward at times from 22/2155 UTC. Geomagnetic activity was Quiet to Active.
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 coronal re-alignment occurred in the Sun's northern hemisphere. This appears to have been responsible for at least one CME. Analysis suggests the CME will mostly pass behind Earth's orbit, but given the central location of the lift off point, a glancing blow is possible, likely during Day 3 (25 Oct).
Residual weak coronal hole influence is expected to gradually ease, with the current slightly elevated wind speeds erratically declining towards background through Day 1 into Day 2 (23-24 Oct). A recently developed small coronal hole, now in the western hemisphere, could bring fast winds to Earth Days 2 into Day 3 (24-25 Oct), although confidence in this is low. Therefore potentially, through Day 3 (25 Oct) a glancing CME arrival and a new weak high speed stream influence could combine.
Geomagnetic activity is expected to be Unsettled to Active initially, then declining through Day 1 (23 Oct) to become Quiet to Unsettled, and mainly Quiet early Day 3 (25 Oct). Later Day 2 into Day 3 conditions may increase to become mostly Unsettled to Active with a chance of Minor storm intervals during Day 3. Through Day 4 (26th Oct) geomagnetic conditions are expected to decrease to become Quiet to Unsettled again, as any coronal hole influence declines.
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: 00:17 (GMT) on Fri 23 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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