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 coronal mass ejection (CME) arrival is likely to arrive early on the 03 Jul, leading to an increase in potential visible aurora. However, any aurora is likely to be restricted to the northern parts of the UK and similar latitudes. Viewing opportunities will also be limited by any cloud cover and the short hours of darkness at this time of year.
Southern Hemisphere
A coronal mass ejection (CME) arrival is likely to arrive early on the 03 Jul, leading to an increase in potential visible aurora during the southern hemisphere Thursday night. However, any aurora is likely to be restricted to southern New Zealand and similar latitudes. Viewing opportunities will also be limited by any cloud cover and the short hours of darkness at this time of year.
Issued at: 01:43 (GMT) on Thu 2 Jul 2026
Forecast overview
Space Weather Forecast Headline: High solar activity likely. Slight Chance of Minor storms from CME influence Day 1 (02 Jul). Another CME arrival is expected Day 2 (03 Jul), with Minor to Moderate storms expected.
Analysis of Space Weather Activity over past 24 hours
Solar Activity: Activity has been High over the last 24 hours, with the largest flare a high level Moderate class observed at 01/2309 UTC from the largest region on the disc in the southwest, which is also magnetically complex. There are currently three other sunspot regions on the Earth-facing disc, one of which is reasonably large and is also magnetically complex and active. A region in the southwest has also been active, and has developed into a small but moderately complex region. The remaining region is small, magnetically simple and weakening.
Several Moderate class flares occurred through the period, and at least two at 01/1454 UTC and 01/1943 UTC have produced Coronal Mass Ejections (CME's) which are likely to have an Earth directed component. These will be analysed once sufficient imagery is available.
Solar Wind / Geomagnetic Activity: Solar wind speeds, have mostly been at Background to Slightly Elevated levels, ranging between 365-420km/s, following the arrival of a weak CME on 30 Jun. The strength of the solar wind's magnetic field was Moderate to Strong. The north-south component was Weak to Moderate following the CME arrival, but remained largely positive, with brief re-orientations to negative. . Geomagnetic activity was Unsettled to Active at first, then declined to current Quiet conditions.
Energetic Particles / Solar Radiation: The count rate of energetic particles (high energy protons) has persisted at Background with no Solar Radiation Storms occurring.
Four-Day Space Weather Forecast Summary
Solar Activity: High activity is likely, with occasional Moderate class flares expected and a chance of an isolated Strong flare.
Solar Wind / Geomagnetic Activity: A slow-moving CME from 27 Jun may arrive early Day 1 (02 Jul). A further CME is expected Day 2 (03 Jul) following the Strong flare on 30 Jun. Further CME's are likely to feature in the forecast once analysis has been undertaken of at least two CME's associated with Moderate Class flares on 01 Jul.
Solar winds are currently Slightly Elevated and are likely to remain Slightly Elevated, despite the potential arrival of a weak CME (which left the Sun on 27 Jun) early Day 1 (02 Jul). The CME following the Strong flares is expected to arrive on Day 2 (03 Jul) with solar winds perhaps rising to reach Elevated, perhaps Strong levels, before gradually declining on Day 3 (04 Jul). Further CME's are likely to feature in the forecast, with solar winds potentially increasing to Strong levels at times.
Geomagnetic activity is expected to be mainly Quiet with a chance of increasing Unsettled to Active if a weak CME arrives early Day 1 (02 Jul). A CME associated with the Strong flare on 30 Jun is likely to arrive Day 2 (03 Jul), with geomagnetic activity likely to reach Active to minor geomagnetic storm with a chance of isolated Moderate storm (Kp 6) intervals, and a slight chance of Strong storm, if the CME is more impactful than anticipated. Activity is likely to decrease thereafter, unless further CME's arrive.
Energetic Particles / Solar Radiation: The count rate of energetic particles (high energy protons) is expected to be at Background levels, but with a chance of reaching Minor-Moderate Radiation storming with any significant flares.
Issued at: 00:29 (GMT) on Thu 2 Jul 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.
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