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
A high speed stream from a coronal hole has arrived at earth, giving a low chance of visible aurora to the north of Scotland and similar latitudes on Saturday night UTC where skies are clear. After this the chances decrease, becoming background levels by Sunday.
Southern Hemisphere
A high speed stream from a coronal hole has arrived at earth, giving a low chance of visible aurora to the south of New Zealand and similar latitudes on Saturday night UTC where skies are clear. After this the chances decrease, becoming background levels by Sunday.
Issued at: 11:34 (GMT) on Sat 16 May 2026
Forecast overview
Space Weather Forecast Headline: Slight chance of isolated Moderate-class solar flares. G1/Minor storm intervals Likely Day 1 (16 May).
Analysis of Space Weather Activity over past 24 hours
Solar Activity: Solar Activity was Low over the past 24hrs, with occasional Common-class flares observed, peaking at C9.5 at 15/1614 UTC from a sunspot region in the northwest.
There are up to five sunspot regions on the visible disc. The largest region on the disc is now transiting the northwest quadrant. This has slowly decreased in overall size, losing some of the peripheral spots and simplifying to a unipolar configuration. A bipolar region has rotated to the northwest limb. Another bipolar region, also in the northwest, has shown some weakening of the lead/trailer spots, with some minor spot emergence in its intermediate portion. Two additional relatively small regions have now rotated from the eastern limb, although these are difficult to fully assess due to the viewing angle.
No Earth-directed Coronal Mass Ejections (CMEs) were observed in the past 24hrs.
Solar Wind / Geomagnetic Activity: Solar wind speeds, as observed by ACE and DSCOVR at L1, increased as coronal hole fast winds strengthened into the overnight UTC period, before easing slightly. Speeds were initially Elevated, 550km/s, rising to Strong and peaking 700-800km/s, before easing slightly to 650km/s. The Interplanetary Magnetic Field was Moderate, trending to Weak after midnight UTC. The north-south component followed a similar trend and was variable, often favouring negative (southward). Geomagnetic activity was at Active to G2/Moderate storm levels (Kp 4-6).
Energetic Particles / Solar Radiation: GOES18 high energy (>10 MeV) proton flux was at Background.
Four-Day Space Weather Forecast Summary
Solar Activity: Solar activity is forecast to continue generally Low, but with a slight chance of Moderate-class flares.
Solar Wind / Geomagnetic Activity: There no Earth-directed CMEs in the forecast.
Ongoing fast solar winds are expected for Day 1 (16 May), then slowly declining Days 2 and 3 (17 and 18 May). Winds may reach Background to Slightly Elevated levels by Day 4 (19 May). Geomagnetic activity is expected to be Unsettled to Active (Kp 3-4), with a chance of further isolated G1/Minor storm intervals (Kp 5) on Day 1 (16 May). During Day 2 (17 May) activity will likely slowly decrease to mainly Quiet to Unsettled levels (Kp 2–3), with a chance of Active to G1/Minor storm intervals. (Kp 4-5). Through Days 3 and 4 (18 and 19 May), activity is expected to gradually reduce further.
Energetic Particles / Solar Radiation: GOES18 high energy (>10 MeV) proton flux is expected to remain at Background levels, with no solar radiation storms expected.
Issued at: 12:02 (GMT) on Sat 16 May 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: