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

Two CMEs (coronal mass ejections) may give glancing effects later on 14 Jul, or during 15 Jul. These may enhance aurora over northern Scotland and similar magnetic latitudes on Tuesday night and Wednesday night UTC. However, any aurora sightings are likely to be limited by short hours of darkness.

Southern Hemisphere

Two CMEs (coronal mass ejections) may give glancing effects later on 14 Jul, or during 15 Jul. These may enhance aurora over southern New Zealand and similar magnetic latitudes on Tuesday night and Wednesday night UTC.

Issued at: 21:58 (GMT) on Mon 13 Jul 2026

Forecast overview

Space Weather Forecast Headline: Chance of Moderate solar activity. Chance of G1/Minor Geomagnetic Storms Day 1 and 2 (13 and 14 July).

Analysis of Space Weather Activity over past 24 hours

Solar Activity: Solar activity is Low, with only occasional, low-level Common-class flares observed. There are four sunspot regions visible on the solar disc. One on the southwest limb, which is the most active region on the disc but is becoming difficult to analyse, as it transitions around the limb. Another sunspot group resides in the southwest, which is the largest region, but appears stable and simple. A new, moderately sized spot rotated into view on the southeast limb. This spot appears to be magnetically simple. A previous sunspot region re-emerged in the northwestern disc as a small and simple group. 

Despite occasional near-limb activity, no new Earth-directed Coronal Mass Ejections (CMEs) have been observed. 

Solar Wind / Geomagnetic Activity: Solar winds were indicative of a waning high speed stream accompanied by glancing CME. Winds speeds were initially Elevated before falling to Slightly Elevated after 12/1800 UTC, lowering further tp 430km/s by the end of the period. Total Interplanetary Magnetic Field was Moderate initially, lowering to Weak from 12/1530 UTC. The north-south component varied Weakly. Geomagnetic activity was Quiet to Unsettled (Kp1-3) with an Active (Kp4) interval 12/1200-1500UTC. 

Energetic Particles / Solar Radiation: The count rate of energetic particles (high energy protons) was at Background levels. 

Four-Day Space Weather Forecast Summary

Solar Activity: Mostly Low or Very Low, but with a Chance of further isolated Moderate-class flares (Moderate activity).

Solar Wind / Geomagnetic Activity: Up to four Coronal Mass Ejections (CMEs) may arrive at Earth during the period, two either late Day 1 or Day 2 (13-14 July), with the other two possibly giving glancing effects from Day 3 (15 July).

Solar wind speeds are Slightly Elevated, due to waning coronal hole fast winds and post glancing 09 July CME impact. Solar wind speeds are likely to erratically decline close to Background for the remainder of the period. The exceptions to this are the possible arrivals of CMEs when speeds may become briefly Elevated.

Geomagnetic activity is expected to be Quiet to Unsettled through much of the period. Active intervals, with a Chance of G1/Minor Geomagnetic storms are possible each day, though with an overall reducing likelihood, due to possible CME arrivals.

Energetic Particles / Solar Radiation: The count rate of energetic particles (high energy protons) is expected to remain at Background levels.

Issued at: 12:29 (GMT) on Mon 13 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.

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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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