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

No significant enhancement to the auroral oval is currently expected in the 72-hour period.

Southern Hemisphere

No significant enhancement to the auroral oval is currently expected in the 72-hour period.

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Forecast overview

Space Weather Forecast Headline: Moderate-class X-ray flares likely (R1-R2 radio blackouts).

Analysis of Space Weather Activity over past 24 hours

Solar Activity: Solar activity has been Moderate, with a triple-peak moderate flare at 15/0937 UTC originating from the large region in the southwest, this sunspot accompanies 15 other spots on the disk, but is by far the largest and most complex region. The next largest region is in the southeast, this spot continues to develop in size and complexity. There are two small and unstable spots near centre disk which also pose a threat of flaring. All other regions are considered to be relatively small and simple at present.

Despite the number and scale of solar flares, no Earth-directed coronal mass ejections have been observed.

Solar Wind / Geomagnetic Activity: The solar wind signal comprised variations on a slow regime, with a late enhancement noted. The solar wind speed was at background levels but rose a little to end the period. The interplanetary magnetic field was weak, becoming moderate from 15/2150UTC. The north-south variation was also weak initially, becoming consistently negative and moderate after 15/2200 UTC. The net result of the above solar wind measures was Quiet (Kp 1), until the final period where the provisional result was Unsettled (Kp 3).

Solar Radiation: No solar radiation storms were observed. 

Four-Day Space Weather Forecast Summary

Solar Activity: Further Moderate-class flares are likely, with a slight chance of further Strong-class flares, most likely from the most complex region. This risk abates slightly after midweek with the main sunspot group leaving the facing side of the Sun.

Solar Wind /Geomagnetic Activity: No Earth-directed coronal mass ejections feature in the forecast. A recent minor enhancement has been noted. The only other potential enhancement currently possible is that of a very uncertain coronal hole high speed stream later in the period, otherwise, solar winds should remain background. Geomagnetic activity is expected to be mostly Quiet, with a slight chance of G1/Minor storms early day 1 (16 Jul) due to the ongoing weak enhancement. Quiet conditions should then prevail, with a chance of Unsettled or Active spells and a slight chance of G1/Minor storms days 3 and 4 (18-19 Jul).

Energetic Particles / Solar Radiation: No solar radiation storms are expected, with a slight chance of rising in response to any notable flares, mainly from the large off-going sunspot.

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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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