Issued: 2017 Feb 10 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
10cm flux | Ap | |
---|---|---|
10 Feb 2017 | 073 | 007 |
11 Feb 2017 | 075 | 007 |
12 Feb 2017 | 077 | 007 |
NOAA AR 2635 evolved into a beta magnetic field configuration but did not produce any more C-class flares, although they remain possible.
No Earth directed Coronal Mass Ejections (CMEs) have been detected. Solar protons have remained at background levels over the past 24 hours.
Geomagnetic conditions have been at k = 2 levels. Solar wind speed is now at 420 km/s with interplanetary magnetic fields of 4 nT. The low latitude extension of the northern polar coronal hole may affect the Earth within 48h, but it is possibly too high in latitude to do so. Quiet geomagnetic conditions expected.
Today's estimated international sunspot number (ISN): 017, based on 04 stations.
Wolf number Catania | /// |
10cm solar flux | 073 |
AK Chambon La Forêt | 013 |
AK Wingst | 008 |
Estimated Ap | 007 |
Estimated international sunspot number | 020 - Based on 09 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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Minor G1 geomagnetic storm (Kp5) Threshold Reached: 20:33 UTC
Moderate M1.99 flare
Minor R1 radio blackout in progress (≥M1 - current: M1.93)
Minor G1 geomagnetic storm (Kp5) Threshold Reached: 13:52 UTC
Minor G1 geomagnetic storm (Kp5) Threshold Reached: 11:42 UTC
Last X-flare | 2025/03/28 | X1.1 |
Last M-flare | 2025/04/21 | M1.9 |
Last geomagnetic storm | 2025/04/20 | Kp5 (G1) |
Spotless days | |
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Last spotless day | 2022/06/08 |
Monthly mean Sunspot Number | |
---|---|
March 2025 | 134.2 -20.4 |
April 2025 | 119.2 -15 |
Last 30 days | 111.1 -31.9 |