Issued: 2017 Jun 08 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
10cm flux | Ap | |
---|---|---|
08 Jun 2017 | 072 | 006 |
09 Jun 2017 | 072 | 007 |
10 Jun 2017 | 072 | 007 |
NOAA AR 2661 produced some C flares in the past 24 hours. The chance for a C flare to occur in the next 24 hours is estimated at 33%. No Earth directed CMEs have been observed in available coronagraph images. Proton flux levels are at background values and are expected to remain so. Solar wind speed measured by DSCOVR varied between about 290 and 350 km/s in the past 24 hours, while the magnitude of the Interplanetary Magnetic Field (IMF) ranged between about 0.5 and 5 nT. Quiet geomagnetic conditions (K Dourbes between 0 and 2; NOAA Kp between 0 and 2) were registered in the past 24 hours. Quiet to unsettled levels (K Dourbes < 4) are expected on June 8, 9 and 10.
Today's estimated international sunspot number (ISN): 016, based on 16 stations.
Wolf number Catania | 033 |
10cm solar flux | 076 |
AK Chambon La Forêt | 008 |
AK Wingst | 006 |
Estimated Ap | 004 |
Estimated international sunspot number | 016 - Based on 27 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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Last M-flare | 2025/04/13 | M1.6 |
Last geomagnetic storm | 2025/04/06 | 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 |
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Last 30 days | 134.2 -8.9 |