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.
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Auroral activity may me initially enhanced due to connection to a fast winds from a large coronal hole, and any minor influence from a coronal mass ejection (CME) glancing blow. Chance of peak G1/Minor Geomagnetic Storm conditions in the early hours of 05 Dec with views of the aurora potentially across Scotland and parts of Northern Ireland. Activity should subside by 06 Dec with views likely restricted to the far north of Scotland.
Auroral activity may be initially enhanced due to connection to a large coronal hole high-speed stream, and any minor influence from a coronal mass ejection (CME) glancing blow. Chance of peak G1/Minor Geomagnetic Storm conditions in the early UTC hours of 05 Dec with views of the aurora mostly restricted to the Antarctic continent. Views in some places may be limited by available hours of darkness at this time of year in the southern hemisphere. Activity should subside by Wednesday 06 Dec with the auroral oval likely returning to near background levels again..
Space Weather Forecast Headline: Slight chance of a G1/Minor Geomagnetic Storm early Day 1 but risk reducing as solar winds ease into the next few days. Chance of isolated M-Class flares (R1-R2 Blackouts) throughout.
Analysis of Space Weather Activity over past 24 hours
Solar Activity: Solar activity is currently Moderate with the largest flare of the past 24 hours a Moderate flare at 05/0639 UTC from what looks to be the small recently numbered region rounding the northeast limb. There are currently 9 sunspot regions on the disc, 7 of which are numbered with two in the far southwest no longer visible having rotated beyond the western limb. The two main complex regions on the disc are close to centre disc in the south. Both regions have seen continued slow intermediate growth but with some consolidation around the main spots. The remaining regions on the visible disc appear small and stable or in slow decay.
Despite a number of coronal mass ejection signatures evidenced in coronagraph imagery during the past 24 hours, none are considered Earth-directed. However, a filament eruption from near one of the south-eastern spots around 04/07000 UTC produced a CME that may give a glancing blow on Day 3 (07 Dec).
Solar Wind / Geomagnetic Activity: Solar wind speeds have been at elevated levels throughout, varying between 520-560 km/s. The Interplanetary Magnetic Field (IMF), Bt, was initially weak before rising to moderate levels. Since around 04/1540 UTC IMF increased more steeply and peaked at 15nT at around 05/0200 UTC before reducing back down to weak to moderate levels by the end of the period. The north-south component of the IMF (Bz), was largely positive initially, more variable through the second half of the period but only weakly fluctuating. Resultant Geomagnetic activity was Quiet to Active (Kp 1-4).
Energetic Particles / Solar Radiation: The count rate of energetic particles (high energy protons) persisted at Background levels with no solar radiation storms occurring.
Four-Day Space Weather Forecast Summary
Solar Activity: Solar activity is expected to be Low to Moderate with a chance for isolated Moderate flares (R1-R2 Blackouts) throughout.
Solar Winds / Geomagnetic Activity: A CME that left the Sun around 04/0700 UTC is expected to miss, but there is a slight chance of a glancing blow on Day 3 (07 Dec). No further CMEs are currently thought to be Earth-directed.
Enhancement of solar winds from a coronal hole fast stream is expected to persist through Days 1-2 (05-06 Dec) with winds at Elevated levels, possibly peaking around 600-620km/s Day 1. Winds are expected to slowly return to Slightly Elevated levels on Days 3-4 (07-08 Dec).
Geomagnetic activity is expected to be largely Quiet to Unsettled through the forecast period (Kp 1-3). There is a chance during Day 1 (05 Dec) that influences from the HSS may see activity increase to Active (Kp 4) and a slight chance of G1/Minor Geomagnetic Storm (Kp 5) levels. This risk reducing into the period as solar winds ease. There is a slight chance on Day 3 (07 Dec) that a glancing blow from a CME produce an Active or G1/Minor Geomagnetic Storm interval, but this is considered a low probability.
Auroral activity may become slightly enhanced overnight Day 1 into Day 2 (05-06 Dec) due to the faster solar winds currently being seen. From the UK views of aurora may be possible across parts of northern Scotland and perhaps Northern Ireland Tuesday night, with activity waning into the forecast period.
Energetic Particles / Solar Radiation: The count rate of energetic particles (high energy protons) is expected to remain at background levels with no Solar Radiation Storms expected.
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.
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.