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

Some enhancements to the auroral oval are possible at times over the coming days, due to potential minor fast wind and possible glancing CME (coronal mass ejection) influences. 24 Dec is currently assessed as the most likely day for any enhanced activity.

Southern Hemisphere

Some enhancements to the auroral oval are possible at times over the coming days, due to potential minor fast wind and possible glancing CME (coronal mass ejection) influences. 24 Dec is currently assessed as the most likely day for any enhanced activity, however short hours of darkness would severely limit the visibility of any minor activity.

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Forecast overview

Space Weather Forecast Headline: Minor/Moderate radio blackouts likely. Possible glancing CME early on 24 Dec. 

Analysis of Space Weather Activity over past 24 hours

Solar Activity: Solar activity has been Moderate with three Moderate-class flares observed from the cluster of sunspot regions located in the southeast quadrant. 

There are currently nine sunspot regions on the visible, one of which is unnumbered near the southeast limb. The southeast quadrant remains the focus of main solar activity, containing a cluster of the four largest regions, three of which are moderately wide bi-polar spot groups, showing some degree of magnetic complexity. A region in the southwest has recently seen a small opposite polarity spot develop, and is now a simple bi-polar group. Another region in the northeast is also appearing to be a fairly large group as it comes more into view. Other remaining regions are relatively small, stable and magnetically simple.

A filament (arc of plasma) lift-off from the northeast and associated Coronal Mass Ejection (CME) from late in the UTC day on 20 Dec was modelled and gives a potential peripheral glance around 24/0000 UTC.

A number of other CMEs have been observed in available imagery during the period. Analysis of these suggests none have an Earth directed component, however confidence in the complex number of CMEs is currently low.  

Solar Wind / Geomagnetic Activity: Solar winds have shown elevated to strong conditions with uncertain cause - perhaps connection to a central 'coronal hole' in the southwestern quadrant. The solar wind speeds have averaged around 600km/s, staying Elevated throughout the period. The associated magnetic field was moderate at times, with an erratic but weak north-south component. Geomagnetic activity was Quiet to Unsettled (Kp2-3).

Energetic Particles / Solar Radiation: High energy proton flux gradually increased early in the period before levelling off, remaining sub-Minor Solar radiation storm level.

Four-Day Space Weather Forecast Summary

Solar Activity: Isolated Moderate-class flares are likely, mainly from the regions in the southeast quadrant, and perhaps bolstered slightly beyond the current UTC weekend by returning regions. A slight chance of isolated Strong-class flares is maintained throughout.

Solar Wind / Geomagnetic Activity: A filament lift-off from the northeast from late in the UTC day on 20 Dec was modelled and gives a potential peripheral glance around 24/0000 UTC. No other Earth-directed CMEs appear in the forecast, however the number of CMEs over the past few days means confidence is low. 

Overall, conditions are likely to remain Quiet to Unsettled. Given current Elevated solar wind speeds, there is a chance of Active conditions through the period, tentatively peaking around days 1 and 2 (23-24 Dec) due to coronal hole influence and possible glancing influence from 20 Dec CME, with a slight chance of G1 Minor Geomagnetic Storms.

Energetic Particles / Solar Radiation: There is a slight chance of Solar Radiation storms through current UTC weekend due to current slightly enhanced near-Earth proton counts. This risk should relax back in the absence of any significant flares, with most of the risk from the front-side then tied to the westward advance of the cluster of sunspot regions currently located in the southeast.

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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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