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 predominantly at background, resulting in only limited opportunities for visible aurora. Any viewing prospects 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 remain largely at background levels, with auroral visibility likely to be limited and largely confined to the Antarctic continent.
Issued at: 12:26 (GMT) on Fri 19 Jun 2026
Forecast overview
Space Weather Forecast Headline: No significant activity.
Analysis of Space Weather Activity over past 24 hours
Solar Activity: Activity has been Low, with only two small Common-class flares observed.
There are four sunspot regions on the Earth-facing side of the Sun, with one of these now becoming visible in the southeast. This group is apparently magnetically unipolar, however the gradually improving viewing angle may yet reveal further detail. All of the current regions on the Earth-facing side were in slight decay.
A small 'disappearing filament' was observed in ground-based near-infrared imagery at 19/0230UTC. This was potentially then visible ion satellite imagery during the ensuing early hours UTC, although very faint. This Coronal Mass Ejection (CME) is tentatively due to cross the radius of the Earth's orbit later in the UTC day of 22 June, mainly missing south and east of the Sun-Earth line. An earlier disturbance in a filament further south in the southeast of the Sun does not appear to have resulted in any CME.
Solar Wind / Geomagnetic Activity: Solar wind speeds were within background for much of the period, however after 19/0900UTC, a rise was observed that may be related to the onset of CH68's fast wind, with speeds becoming slightly elevated along with an associated increase in solar wind temperature. The number of particles in the solar wind was within typical background values throughout. The associated magnetic field rose to become moderate and more erratic in character in the period, with the north-south component variable within this range.
The net result of the above solar wind measures was for mainly quiet geomagnetic activity.
Energetic Particles / Solar Radiation: No solar radiation storms were observed.
Four-Day Space Weather Forecast Summary
Solar Activity: Low activity is expected at first, with an increasing chance of rising to Moderate due to regions rotating on from the Sun's far side through the period.
Solar Wind / Geomagnetic Activity: A minor glance from a 19 June southeastern CME later in the UTC day of Monday 22 June is not expected to result in significant impacts as it passes Earth as a possible glancing blow later day 4. The sole fast wind due in the period may now be arriving to bring slightly elevated winds into the UTC weekend, but soon easing. Day 3, Sunday 21 June is therefore perhaps the most reliably favourable day geomagnetic activity-wise, although the bookending activity is not likely to be significantly impactful - below Minor Storm G1.
Energetic Particles / Solar Radiation: The current dearth of activity and suitably complex regions in prone locations mean that solar radiation storms are not expected in the forecast period.
Issued at: 12:14 (GMT) on Fri 19 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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