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
Geomagnetic activity is expected to be limited in the period. This will be further constrained by the short hours of darkness at this time of year at suitable viewing latitudes.
Southern Hemisphere
Geomagnetic activity is expected to be limited in the period, perhaps improving slightly around midweek UTC when a fast wind may develop, although this may only be visible in far southern New Zealand and similar geomagnetic latitudes.
Issued at: 14:10 (GMT) on Mon 22 Jun 2026
Forecast overview
Space Weather Forecast Headline: Rising chance of Moderate-class X-ray flares.
Analysis of Space Weather Activity over past 24 hours
Solar Activity: Activity has been Moderate over the past 24 hours, peaking at 21/1929UTC, with an earlier smaller flare at 21/0246UTC from the same region in the southeast of the Sun. Both events were associated with Coronal Mass Ejections (CMEs).
There are currently up to five regions visible on the solar disc, including a small unnumbered region on the western limb. The main focus remains on the eastern limb, where an impulsive Moderate flare was observed overnight. The responsible region remains magnetically complex, although the recent growth in sunspots has stopped and some smaller spots are fading. It appears separate from a more stable nearby region to the east, although the boundary between them is still unclear.
Several filaments are currently present on the Sun's central disc and will require close monitoring for any signs of lift-off, particularly as they rotate across the western hemisphere.
A complex, multi-directional CME was observed leaving the Sun in the early UTC hours of Monday. However, based on STIX quick-look data from the ESA/NASA Solar Orbiter spacecraft, it is very likely to be far-sided. No Earth-directed CMEs have been observed in available imagery.
Solar Wind / Geomagnetic Activity: The solar wind suggested an ongoing slow regime. Solar wind speeds remained steady at around 350–380 km/s. The number of particles in the solar wind and their associated magnetic field were both within their typical range. The net result of the above solar wind measures was for provisionally quiet geomagnetic activity throughout.
Energetic Particles / Solar Radiation: No solar radiation storms were observed, with no obvious enhancement related to the Moderate-class x-ray activity in the east of the Sun.
Four-Day Space Weather Forecast Summary
Solar Activity: There is a slightly increasing chance of moderate activity, mainly from the recent most active grouo in the southeast and an oncoming larger region from midweek UTC. There is a rising slight chance of Strong-class x-ray flares for the same reason.
Solar Wind / Geomagnetic Activity: The sole CME in the forecast at present is a possible glancing blow from the 19 June southeastern CME, due to cross Earth's orbit later on 22 June, with effects perhaps extending into early 23 June (UTC).
The next fast wind may occur later on 24 June, although this is low confidence.
Despite the above, geomagnetic activity is expected to remain mainly quiet, probably peaking below Minor Geomagnetic Storm G1, should glancing CME influence and/or a fast solar wind enhancement occur.
Energetic Particles / Solar Radiation: No solar radiation storms are expected given the absence of suitably large and active regions in the better-connecting (with Earth) western solar hemisphere.
Issued at: 11:21 (GMT) on Mon 22 Jun 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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