Issued: 2017 Feb 09 1230 UTC
C-class flares expected, (probability >=50%)
Quiet (A<20 and K<4)
Quiet
10cm flux | Ap | |
---|---|---|
09 Feb 2017 | 073 | 007 |
10 Feb 2017 | 074 | 007 |
11 Feb 2017 | 075 | 007 |
Minor C-class flaring occurred from a new region (NOAA AR 2635) that emerged to the north of NOAA AR 2634. The strongest was a C1.3 flare peaking at 03:26 UT. More C-class flares can be expected.
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 = 2-3 levels. Solar wind speed is now at 415 km/s with interplanetary magnetic fields of 5 nT. The expected high speed stream (HSS) from the equatorial coronal hole has missed the Earth. Quiet geomagnetic conditions expected.
Today's estimated international sunspot number (ISN): 017, based on 01 stations.
Wolf number Catania | 025 |
10cm solar flux | 073 |
AK Chambon La Forêt | 011 |
AK Wingst | 004 |
Estimated Ap | 004 |
Estimated international sunspot number | 000 - Based on 08 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 |
April 2025 | 136.4 +2.2 |
Last 30 days | 134.2 -8.9 |