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 aurora oval is expected to be at or near background levels at first. The onset of the fast wind from a large coronal hole, either on Wednesday 3rd or Thursday 4th December is expected to enhance the auroral oval to lower latitudes. Following its arrival, aurora may be visible, where skies are sufficiently clear, mainly from northern Scotland, with a lower chance further south. A possible coronal mass ejection (CME) glance around a similar time may also cause increased enhancement, with aurora potentially visible further south still.

Southern Hemisphere

The aurora oval is expected to be at or near background levels at first. The onset of faster solar winds, either on Wednesday 3rd or Thursday 4th December UTC is expected to enhance the auroral oval to lower latitudes. Following its arrival, aurora may be visible, where skies are sufficiently clear, from the far south of New Zealand and perhaps also Tasmania at peak. A possible coronal mass ejection (CME) glance around a similar time may also cause increased enhancement, with aurora potentially visible further north.

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Forecast overview

Space Weather Forecast Headline: Moderate to High Solar Activity expected. G1 Minor Storms Likely, Chance of G2 Moderate Storms day 1-2 (03-04 Dec).

Analysis of Space Weather Activity over past 24 hours

Solar Activity: Solar activity has been Low over the past 24 hours with a peak flare from the small but complex region in the northeast. There are nine other regions on the visible disc. Of these, there is a collection of large spots across the southeast disc, these are split into three regions. The most notable is the central-most spot, this is the largest and most magnetically complex spot with multiple parts which may by cause instability and possible flaring. The other two regions in the southeast are large yet less magnetically complex. The remaining regions, mostly located in the western hemisphere, appear smaller and simple.

The main coronal mass ejection of note was from the Strong flare early on 01 Dec, and a subsequent sympathetic filament eruption. This resulted in a complex eruption, with the majority of the material passing north and behind Earth, however there are some signs that the filament eruption potential included a component deflected more towards the Earth-Sun line. Any subsequent coronal mass ejection is likely to glance at most, perhaps late on day 1 (03 Dec), however this is very low confidence. No further Earth-Directed coronal mass ejections were observed.

Solar Wind / Geomagnetic Activity: Solar wind parameters showed declining fast winds before a perturbation was observed starting around 02/2300UTC either associated with a weak coronal mass ejection effects or perhaps the prerequisite to the solar sector boundary crossing ahead of the next coronal hole high speed stream. Solar wind speeds gradually fell from Slightly Elevated to Slow-Ambient. Total Interplanetary Magnetic Field started Weak, then became Moderate after 03/0500UTC, on a continual rise since. The north-south component started Weak, but followed a similar increase after 03/0730UTC, and was notable negatively (southward) orientated peaking at Moderately negative at 03/1143UTC. Geomagnetic activity was Quiet to Unsettled (Kp 1-3).

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

Four-Day Space Weather Forecast Summary

Solar Activity: Moderate or High solar activity is expected, with isolated Moderate class flares and a chance of isolated Strong solar flares.

Solar Wind / Geomagnetic Activity: There are no clear Earth-directed CMEs, however the filament eruption after the Strong flare on 01 Dec may have an Earth-directed component that could arrive late day 1 (03 Dec). The next fast wind enhancement, from the next coronal hole, is expected late on day 1 to day 2 (03-04 Dec), and this may combine with any CME arrival.

Geomagnetic activity is forecast to be Quiet with isolated Unsettled intervals initially on day 1 (02 Dec), increasing to Active to G1 Minor Storm with any coronal hole fast wind, and a chance of stronger activity, especially if any glancing CME arrival is also observed alongside this, however this is very low confidence.

Energetic Particles / Solar Radiation: The count rate of energetic particles (high energy protons) is expected to persist at Background, with no Solar Radiation Storms occurring. However, there is an increasing chance of his rising as a response to any significant flares from the sunspot regions currently on the eastern disc, especially as these move towards the centre 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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