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

The auroral oval may be visible tonight (20-21 May), with reasonable confidence of sightings (where skies are clear) across parts of Scotland and Northern Ireland, but perhaps as far south as northern England and North Wales.

Southern Hemisphere

The auroral oval may be visible tonight (20-21 May), with reasonable confidence of sightings (where skies are clear) across parts of Tasmania and South Island of New Zealand, but perhaps as far north as the southern parts of mainland Australia and North Island of New Zealand.

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Forecast overview

Space Weather Forecast Headline: Chance of isolated Moderate-class flares throughout. Chance of G1-G2 (Minor/Moderate) Storm conditions Days 1-3 (from 20th to 22nd May). 

Analysis of Space Weather Activity over past 24 hours

Solar Activity: Solar activity has been Moderate, the strongest flare being a Moderate-class event that occurred at 19/1756 UTC from the moderately large region in the southeast. A Low-class flare occurred at 20/0554 UTC from a relatively small region in the southwest. 

There are currently seven sunspot regions on the visible disc. The largest region remains in the southeast. It comprises of a number of large, mature spots, with recent consolidation of some of the smaller spots. This region did consist of a small delta spot, which has now faded. The next largest region is in the southwest and has been the source of some low-level C-class activity. Although the main lead and trailer regions are well-separated there are a number of small pores or spots of mixed polarity occupying the intermediate portion of the group. The region responsible for the latest Low-class flare indicates modest magnetic complexity, with numerous small trailing spots and some consolidation. The other sunspot regions are generally smaller, simpler and generally stable.

A large filament (arc of plasma) lift-off from the southern hemisphere that began around 18/2200UTC has been modelled as missing below Earth orbit. Another large filament eruption observed after the Low-class flare that occurred at 20/0554 UTC from the region in the southwest. We are currently awaiting the results of the analysis but given its location and early imagery, it is likely to have an Earth-directed component. Otherwise, no Earth-directed CMEs were observed in the past 24 hours.  

Solar Wind / Geomagnetic Activity: 

Solar winds were indicative of a near background regime, though perhaps with minor positive coronal hole influence. Solar wind speeds have ranged between 340-410km/s. The Interplanetary Magnetic Field (IMF) was in between weak and moderate, around 8nT. The all-important north-south component was stable and fluctuating slowly between positive and negative values. Geomagnetic activity was at Quiet to Unsettled levels (Kp1-3).

Energetic Particles / Solar Radiation: The count rate of energetic particles (high energy protons) remained below the S1/Minor Radiation Storm levels and are now at normal background levels.

Four-Day Space Weather Forecast Summary

Solar Activity: Low to Moderate activity is expected with a chance of isolated Moderate-class flares and a very slight chance of isolated Strong flares. The moderately sized sunspot region in the southeast disc is most likely to be the source of significant flare activity. 

Solar Wind / Geomagnetic Activity: There is the chance of a glancing blow from a CME at Earth late day 1 (20 May) or perhaps early day 2 (21 May), resulting from the M7.2 flare that occurred late on 17 May from the large sunspot region in the southeast. We are also awaiting the results of the analysis from the halo CME that occurred earlier today (20/05:54 UTC) but there is potential for Earth to take another glancing blow on Day 3 (22nd). In the meantime, solar winds are forecast to remain at or near background speeds, with no significant coronal hole enhancements expected.

Quiet to Unsettled conditions initially, before a possible glancing blow from a CME (which left the Sun on 17 May) arrives at Earth late day 1 (20th) or early day 2 (21st) with a chance of Active to G1-G2/Minor-Moderate (Kp5-6) intervals. Another chance of G1-G2/Minor-Moderate Storm is possible at the end of Day 2 (21st) and on Day 3 (22nd), under the influence of the halo CME. Activity should then subside towards Quiet to Unsettled levels by Day 4 (23rd).  

Aurora Forecast: Two significant enhancements to the auroral oval are expected tonight (20-21 May) and tomorrow (21-22 May), following the forecast potential arrival of two different CMEs. Should the CME be detected at Earth, aurora may become visible (where skies are clear) across parts of Scotland and Northern Ireland, with a slight chance that views of the aurora may also be possible from northern England and North Wales. The chance of enhanced aurora activity is expected to decline again on subsequent nights. 

Energetic Particles / Solar Radiation: Solar radiation is below the S1/Minor Storm threshold, on a slightly declining trend, but remains just above normal background levels following flare activity from the past week. There is a persistent slight chance of further enhancements should any large flares occur.

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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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