Begin Max End Rgn Loc Xray Op 245MHz 10cm Sweep 0000 0000 0000 100 0532 0532 0532 220 0538 0538 0538 160 0540 0540 0540 120 0624 0637 0719 370 0730 0731 0732 180 0744 0757 0821 470 0828 0828 0828 110 0910 0917 0921 B9.7 150 0923 0924 0924 170 0929 0930 0932 210 0933 0934 0934 120 0938 0938 0938 150 0941 0944 0944 260 0948 0949 0950 1000 0953 0953 0953 140 0958 1003 1005 470 1009 1010 1012 220 1014 1014 1014 150 1017 1022 1024 320 1028 1028 1029 120 1046 1055 1105 2940 C1.1 130 1841 1841 1841 340
10 cm 130 SSN 100 Afr/Ap 008/010 X-ray Background B6.1 Daily Proton Fluence (flux accumulation over 24 hrs) GT 1 MeV 7.7e+05 GT 10 MeV 4.7e+04 p/(cm2-ster-day) (GOES-16 satellite synchronous orbit W75 degrees) Daily Electron Fluence GT 2 MeV 7.90e+07 e/(cm2-ster-day) (GOES-16 satellite synchronous orbit W75 degrees) 3 Hour K-indices Boulder 2 3 2 4 2 2 2 2 Planetary 2 3 2 3 2 2 3 2
None
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
Edmonton, AB, Gillam, MB, Whitehorse, YT, Yellowknife, NTA lot of people come to SpaceWeatherLive to follow the Sun's activity or if there is aurora to be seen, but with more traffic comes higher server costs. Consider a donation if you enjoy SpaceWeatherLive so we can keep the website online!
The anticipated strong G3 geomagnetic storm watch never materialized as the coronal mass ejection that was supposed to arrive early yesterday didn't arrive until today just past midnight UTC. The impact was very lackluster with the Bt (total strength of the IMF) increasing to a moderate 15nT at best and the solar wind speed reaching just 420km/s. A far cry from the anticipated 700 to 800km/s. That once again goes to show how hard it is to forecast space weather events and any resulting geomagnetic conditions. We remain under the influence of the CME and high latitude sky watchers should remain alert for some nice aurora displays but middle latitude sky watchers will probably have to wait for the next opportunity.
Read moreA transequatorial coronal hole is facing Earth. Enhanced solar wind could arrive in ~3 days
Active geomagnetic conditions (Kp4) Threshold Reached: 02:33 UTC
Last X-flare | 2025/02/23 | X2.0 |
Last M-flare | 2025/03/21 | M1.2 |
Last geomagnetic storm | 2025/03/22 | Kp6- (G2) |
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 |
March 2025 | 138.3 -16.4 |
Last 30 days | 136.1 -18.1 |