Issued: 2020 Feb 12 1231 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
10cm flux | Ap | |
---|---|---|
12 Feb 2020 | 070 | 008 |
13 Feb 2020 | 071 | 010 |
14 Feb 2020 | 070 | 008 |
The solar activity has been quiet over the past 24 hours. The visible solar disc is spotless and the X-ray flux is below B-level. The solar activity is expected to remain at low levels over the next 24 hours.
No earth-directed coronal mass ejections (CMEs) have been observed in the available coronagraphic imagery. The greater than 10 MeV proton flux was at nominal values.
The influence of the high-speed stream coming from the positive polarity coronal hole has dropped on February 11 around 19:30 UTC when the phi angle switched to the negative sector. The solar wind parameters remained, however, slightly enhanced. The wind speed first decreased up to 350 km/s to then re-increase up to 420 km/s, the total interplanetary magnetic fields was below 6 nT, and the southward magnetic component fluctuated between -4.5 nT and 5.0 nT. The solar wind conditions are expected to remain slightly enhanced for the next 24-hour period. Solar wind coming from the equatorial coronal hole (negative polarity) that reached the central meridian on February 9, may then contribute to the solar wind enhancement in about 1-2 days.
The geomagnetic conditions were quiet with few short periods of unsettle condition observed in Dourbes station (K-Dourbes = 3). We expect the geomagnetic conditions to remain mostly quiet with some short sporadic periods of unsettled condition for the next days.
Today's estimated international sunspot number (ISN): 000, based on 22 stations.
Wolf number Catania | 000 |
10cm solar flux | 071 |
AK Chambon La Forêt | 008 |
AK Wingst | 007 |
Estimated Ap | 006 |
Estimated international sunspot number | 000 - Based on 24 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 high possibility for aurora to appear at the following high latitude regions in the near future
ReykjavikCurrent data suggests there is a moderate possibility for aurora to appear at the following high latitude regions in the near future
TórshavnCurrent data suggests there is a slight possibility for aurora to appear at the following high latitude regions in the near future
KuopioCurrent data suggests there is a slight possibility for aurora to appear at the following middle latitude regions in the near future
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The OVATION model predicts the Hemispheric Power Index to reach 75GW at 21:49 UTC
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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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March 2025 | 134.2 -20.4 |
April 2025 | 143 +8.8 |
Last 30 days | 129.8 -16.3 |