Space Weather

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

A glancing Coronal Mass Ejection (CME) arrival is likely early on Thursday 18 April but effects should largely subside by the later part of the UTC day, limiting views of the aurora into the overnight period. Aurora may briefly be visible in the far north of Scotland.

Southern Hemisphere

A glancing Coronal Mass Ejection (CME) arrival is likely early on Thursday 18 April but effects should largely subside by the later part of the UTC day, limiting views of the aurora into the overnight period.

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Forecast overview

Space Weather Forecast Headline: Further Moderate-flares likely and a slight chance of Strong-flares. Chance of G1/Minor Storm conditions day 1 and 3 (18 and 20 Apr). 

Solar Activity: Activity is currently Moderate. The largest flare was a Moderate flare at 16/1802 UTC from a small region amongst a cluster of sunspot groups in the southeast disc.

There are fourteen sunspot regions currently visible on the disc. The largest and most magnetically complex region lies in the northeast and provides the bulk of the significant flare risk. The next largest region, located in the northwest, although sizeable, maintains a more magnetically simple appearance. The complex multi spot region in the southeast contains several groups with enhanced magnetic complexity. Remaining regions appear generally more stable with only slow evolution. The remaining regions appear generally stable with little overall change in appearance.

A filament eruption (arc of the Sun's plasma) was observed around 17/0200 UTC lifting off in the northern hemisphere, although unlikely to have any Earth-directed component as the bulk of material appears to be heading north away from the Earth-Sun line. Three separate, but slow CMEs were observed from an area near a sunspot in the southeast late on 17 Apr. These may have a minor Earth-directed component, but have been analysed to be slow and would only expected to be observed as weak transients on 22 or 23 Apr. 

Solar Wind / Geomagnetic Activity: Solar wind parameters were indicative of minor CME influence during the period. Solar winds were largely background, but with a peak of 481km/s (slightly elevated) observed at 17/0938 UTC. The Interplanetary magnetic field (IMF) strength was weak initially, but became predominantly moderate following the arrival of the CME around 17/0900 UTC. The important north-south component was weakly northwards directed at first, becoming generally weakly to moderately southwards directed between 17/0900-1800 UTC, then largely weakly northward directed thereafter. Resultant geomagnetic activity ranged from Kp1 (Quiet) to Kp3 (Unsettled).

Energetic Particles / Solar Radiation: The count rate of energetic particles (high energy protons) was at background with no Solar Radiation Storms occurring.

Four-Day Space Weather Forecast Summary

Solar Activity: Moderate activity is forecast with isolated Moderate-class flares likely and a slight chance of isolated Strong flares.

Solar Wind / Geomagnetic Activity: A CME that left the Sun on 15 Apr is expected to give a glancing impact at Earth early on day 1 (18 Apr). A second CME that occurred late on 16 Apr has been analysed as a likely miss below Earth orbit on day 3 (21 Apr).

Solar winds are currently at normal background speeds. A minor enhancement is expected with the anticipated arrival of the CME from 15 Apr, early on day 1 (18 Apr). A recurrent coronal hole high-speed stream is expected to become geoeffective on day 3 (20 Apr) likely increasing speeds to slightly elevated or elevated levels, continuing into day 4 (21 Apr). 

Geomagnetic activity is expected to be at Quiet to G1/Minor Storm levels on day 1 (18 Apr), then Quiet to Unsettled on days 2 and 3 (19 and 20 Apr), likely increasing Unsettled to G1/Minor Storm levels during day 3 (19 Apr). On day 4 (21 Apr) activity is forecast at Quiet to Unsettled levels. 

Energetic Particles / Solar Radiation: The count rate of energetic particles (high energy protons) is forecast to remain at background with no Solar Radiation storms occurring. 

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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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