Issued: 2020 Aug 26 1231 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
10cm flux | Ap | |
---|---|---|
26 Aug 2020 | 071 | 013 |
27 Aug 2020 | 071 | 012 |
28 Aug 2020 | 071 | 013 |
Solar X-ray flux has been below background (B) level throughout the period. There are no spotted regions on disc and X-ray flux is expected to remain at or below background (B) values.
There were no Earth directed coronal mass ejections observed in coronagraph data.
The greater than 10 MeV proton flux was at background levels over the past 24 hours. It is expected to stay at background levels for the next 24 hours. The greater than 2 MeV electron flux was at nominal levels over the past 24 hours and is expected to remain so over the next 24 hours.
Another coronal hole of positive polarity seems to be forming around disc centre and adds to the likelihood of Solar wind perturbations later in the week.
Solar wind conditions showed the expected enhancements. Solar wind speed rose from under 350 km/s to currently just under 450 km/s. The magnetic field phi angle switched into the away sector early in the period. The total magnetic field reached a peak of 8.5 nT this morning and remains at levels around 6nT, while Bz was overall variable. As other coronal holes are lining up, these moderate Solar wind enhancements are expected to last on and off over the next days.
Quiet to unsettled geomagnetic conditions have been recorded (NOAA Kp 1-2 while local K Dourbes reaching 3 just recently). Geomagnetic conditions are expected to be mostly quiet to unsettled, with some isolated active periods not excluded depending on the evolution of the Solar wind enhancements.
Today's estimated international sunspot number (ISN): 000, based on 14 stations.
Wolf number Catania | /// |
10cm solar flux | 071 |
AK Chambon La Forêt | 009 |
AK Wingst | 004 |
Estimated Ap | 003 |
Estimated international sunspot number | 000 - Based on 23 stations |
Day | Begin | Max | End | Loc | Strength | OP | 10cm | Catania/NOAA | Radio burst types | |
---|---|---|---|---|---|---|---|---|---|---|
None |
Provided by the Solar Influences Data analysis Center© - SIDC - Processed by SpaceWeatherLive
All times in UTC
Current data suggests there is a slight possibility for aurora to appear at the following high latitude regions in the near future
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The OVATION model predicts the Hemispheric Power Index to reach 50GW at 04:56 UTC
Active geomagnetic conditions (Kp4) Threshold Reached: 01:32 UTC
Moderate M2.5 flare
Minor R1 radio blackout in progress (≥M1 - current: M1.45)
Last X-flare | 2025/03/28 | X1.1 |
Last M-flare | 2025/04/01 | M2.5 |
Last geomagnetic storm | 2025/03/27 | Kp5 (G1) |
Spotless days | |
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Last spotless day | 2022/06/08 |
Monthly mean Sunspot Number | |
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February 2025 | 154.6 +17.6 |
April 2025 | 152.5 -2.1 |
Last 30 days | 130.7 -17.9 |