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.

Image courtesy of NASA/SDO and the AIA, EVE, and HMI science teams

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Aurora forecasts

Northern Hemisphere

The expected Coronal Mass Ejection arrived around midday (UTC) on Sunday 02 August. Any ongoing lingering influence could allow for some potential glimpses of the aurora across northernmost parts of Scotland and similar magnetic latitudes into early Monday morning (UTC), where cloud breaks allow, but viewings likely hampered by shorter hours of darkness. Thereafter, the auroral oval is expected to return to background conditions.

Southern Hemisphere

The expected Coronal Mass Ejection arrived around midday (UTC) on Sunday 02 August. Any ongoing lingering influence could allow for enhancement of the aurora across higher magnetic latitudes early Monday morning (UTC), where cloud breaks allow. Thereafter, the auroral oval is expected to return to background conditions.

Issued at: 01:59 (GMT) on Mon 3 Aug 2026

Forecast overview

Space Weather Forecast Headline:  Slight chance of isolated G1/Minor geomagnetic storms at first on day 1 (03 August). Chance of isolated Moderate-class flares.

Analysis of Space Weather Activity over past 24 hours

Solar Activity: 

Solar activity has been Low in the last 24 hours, with a C1.4 flare recorded at 03/1133 UTC.

There are currently six regions on the visible disc. Two areas are located in close proximity in the north centre disc. The largest sunspot region, located in the central western part of the disc comprising a moderately large central spot with a clustering of peripheral minor spots to the south. These are showing some waxing/waning development with a possible very weak delta configuration evident in one of the spots. The smaller region just to the northeast of this, has reduced in size and complexity, becoming unipolar in recent imagery. The region in the central southern part of the disc, has shown some development, with a spot in the east of the sunspot region increasing in size. The remaining regions are relatively simpler, smaller and largely stable.

No Earth-directed Coronal Mass Ejections were observed in the available imagery.

Solar Wind / Geomagnetic Activity: 

The 30 July CME arrived at L1 around 02/1130UTC. Solar windspeeds, as observed by SOLAR-1, increased through the afternoon of the 2 August to peak at 439km/s at 02/1717 UTC. winds persisted around 400km/s  until around 03/0200 UTC when they dropped below 400 km/s to become around 370-390km/s. Since then they have generally been similar, just going above 400km/s for a short period around 03/0600 UTC.

Interplanetary Magnetic Field, Bt, has generally been Moderate, although it did briefly peak at Strong at 02/1455 UTC. From around 03/0400 UTC there has been a slow decline, becoming Weak to Moderate. The north-south component, Bz, has generally been negative (southward), with a period of positive (northward) between around 02/1900 UTC to 02/2300UTC, and another positive (northward) period between 03/0500 UTC and 03/0700 UTC. Geomagnetic activity was in the range Unsettled to G1/Minor storm (Kp 3-5) until 02/2100 UTC, but has been Quiet since then.

Energetic Particles / Solar Radiation:

GOES18 high energy (>10MeV) proton flux returned to background, after recent enhancements. 

Four-Day Space Weather Forecast Summary

Solar Activity:

Low solar activity is expected to continue with a chance of isolated Moderate-class flares.

Solar Wind / Geomagnetic Activity: 

Due to the Coronal Mass Ejection arriving on 30 July there is a slight chance of isolated G1 Minor storms possible on Day 1 (03 August), before geomagnetic activity eases to mainly Quiet, with isolated Unsettled intervals. A further Coronal Mass Ejection from the southeast disc on 31 July is expected to miss Earth, but there is an outside chance of a weak glancing impact. No other Earth directed Coronal Mass Ejections are currently expected.

Energetic Particles / Solar Radiation:

GOES18 >10MeV proton flux is expected to continue at Background with no further enhancement currently forecast..

Issued at: 12:16 (GMT) on Mon 3 Aug 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:

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