Issued: 2016 Sep 03 1231 UTC
C-class flares expected, (probability >=50%)
Active conditions expected (A>=20 or K=4)
Quiet
10cm flux | Ap | |
---|---|---|
03 Sep 2016 | 095 | 022 |
04 Sep 2016 | 097 | 017 |
05 Sep 2016 | 098 | 017 |
Solar activity has been very low, no C-class flares. Active region NOAA AR has developed its magnetic field configuration into beta-gamma, C-class (and low chances of M-class) flares can be expected. No Earth directed CMEs were detected. The Earth is under the influence of a high speed stream from a coronal hole. As a consequence, in the past 24 h minor storm conditions were reached at Dourbes (K = 5, at 23:00 UT on September 2) and major storm conditions at planetary levels (Kp = 6 at 06:00 UT today). Currently, solar wind speed is at 680 km/s with magnetic field intensity of 6 nT with negative (oscillating) Bz. Increased geomagnetic activity is expected to persist for the next 24 h.
Today's estimated international sunspot number (ISN): 066, based on 20 stations.
Wolf number Catania | /// |
10cm solar flux | 095 |
AK Chambon La Forêt | 050 |
AK Wingst | 037 |
Estimated Ap | 042 |
Estimated international sunspot number | 067 - Based on 31 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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Last 30 days | 134.2 -8.9 |