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

Earth is under the influence of fast solar winds. This combined with possible Coronal Mass Ejection influence may bring enhanced auroral activity over the next day or so,. Aurora may occasionally be visible during the limited hours of darkness across northern areas of Scotland where skies remain clear.

Southern Hemisphere

Earth is under the influence of fast solar winds. This combined with possible Coronal Mass Ejection influence may bring enhanced auroral activity over the next day or so.. Aurora may be visible where skies are clear, from the South Island of New Zealand and Tasmania and perhaps visible to the far south of Australia.

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Forecast overview

Space Weather Forecast Headline: Occasional Moderate flares expected with chance of isolated Strong flares. Chance of Minor geomagnetic storm intervals due to Coronal Mass Ejections (CMEs).

Analysis of Space Weather Activity over past 24 hours

Solar Activity: Solar activity is High. A large and complex sunspot region in the northwest has continued to produce numerous moderate flares in the last 24 hours. A second, now larger region in the south-centre disc is less active, but has rapidly developed with a complex magnetic configuration. These two groups are part of nine sunspot regions on the visible disc. The remaining sunspots on the disc are smaller, stable and magnetically simple. 

A Coronal Mass Ejection (CME) appears to have occurred, starting around 07/0000 UTC from a region close to the sunspot group in the south-centre disc. Analysis is ongoing to determine if there is an Earth-directed component to it. 

Solar Wind / Geomagnetic Activity: Solar winds were predominantly at slightly elevated to elevated levels resulting from the connection one or more coronal holes. Speeds peaked briefly at strong levels (602km/s at 07/0150 UTC). The Interplanetary Magnetic Field remained mainly at moderate levels initially before declining to weak levels around 06/1730 UTC. The important north-south component was very variable but declined from moderate levels to become weak. Geomagnetic activity was Quiet to Active (Kp 1-4).

Energetic Particles / Solar Radiation: Solar radiation was at normal background levels.

Four-Day Space Weather Forecast Summary

Solar Activity: Moderate to High solar activity is forecast to continue with occasional Moderate flares expected and a chance of isolated Strong flares, principally from the large sunspot regions located in the northwest and south-centre parts of the visible disc.

Solar Wind / Geomagnetic Activity: There are multiple potential Earth-directed CMEs in the forecast period, although confidence is low due to a lack of solar imagery in recent days. Of these, the majority, if not all are expected to pass above or below Earth orbit, most likely limiting any impacts to glancing blows. Earth is under the influence of a HSS (High speed stream) from a couple of coronal holes and expected to peak at elevated levels on Day 1 (07 May) before slowly declining between Days 2-4 (08-10 May) towards slightly elevated or background levels.

Geomagnetic activity should generally fall between Quiet to Active levels through the period, but with a chance of Minor Storm (Kp5) intervals on all days, given the potential for peripheral CME enhancements.

Energetic Particles / Solar Radiation: Solar radiation levels is most likely to remain at background levels through the period. There is a slight chance for an S1/Minor Storm or greater event occurring throughout however, primarily from the large, complex sunspot region in the northwest disc.

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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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