Issued: 2021 Feb 22 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Minor storm expected (A>=30 or K=5)
Quiet
10cm flux | Ap | |
---|---|---|
22 Feb 2021 | 075 | 018 |
23 Feb 2021 | 075 | 031 |
24 Feb 2021 | 075 | 008 |
The solar activity has been mostly quiet over the past 24 hours. The sunspot (Catania 73, NOAA-AR 2803) remained quiet on the visible solar disc without any significant flaring activity. A new northern central small region, of beta-gamma configuration, appeared. The solar flaring activity is expected to remain at low levels for the next 24 hours.
No Earth directed Coronal Mass Ejections (CME) were observed in the available coronagraphic imagery.
The greater than 10 MeV proton flux was at nominal levels in the past 24 hours and is expected to remain so in the next 24 hours. The greater than 2 MeV electron flux remained mainly over the 1000 pfu threshold. The electron flux is expected to remain on this level from the combined effects of the negative polarity Coronal Holes (CH) due to the enhancement of the solar wind conditions and the arrival of the expected CME from Feb 20. The greater than 2 MeV electron fluence remained on moderate levels in the past 24 hours. It is expected to remain so in the next 24 hours.
Over the past 24 hours, the Earth has remained under the influence of the fast solar wind regime. The solar wind speed ranged between 540 km/s and 625 km/s. The total magnetic field ranged between 3 nT and 6 nT. The Bz component fluctuated between -6 nT and 5 nT. The fast solar wind streams associated with southern coronal holes (negative magnetic polarity) are expected to have a decreasing influence on the solar wind environment near Earth for the 24 hours, possibly followed by a solar wind shock due to the arrival of the CME on Feb 20.
The geomagnetic conditions over the past 24 hours were unsettled, to active. The geomagnetic conditions are expected to remain in the same levels with a slight chance of minor storm conditions (Kp and K-Dourbes equal to 5) in response to the enhancement of the solar wind parameters and possible prolonged periods of southward directed Bz component and the CME on Feb 20.
Today's estimated international sunspot number (ISN): 017, based on 19 stations.
Wolf number Catania | /// |
10cm solar flux | 075 |
AK Chambon La Forêt | 032 |
AK Wingst | /// |
Estimated Ap | 026 |
Estimated international sunspot number | 011 - Based on 22 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 |