Issued: 2016 Nov 03 1253 UTC
Quiet conditions (<50% probability of C-class flares)
Active conditions expected (A>=20 or K=4)
Quiet
10cm flux | Ap | |
---|---|---|
03 Nov 2016 | 076 | 024 |
04 Nov 2016 | 075 | 013 |
05 Nov 2016 | 074 | 009 |
Solar activity was very low in the past 24 hours. No C-class flares, no Earth-directed CMEs were observed. NOAA AR 2605 (Catania 52) is decaying, while old active region NOAA 2602 is rounding the northeast limb. There are 2 stable filaments on the visible side of the solar disk. Solar proton flux intensity is expected to lie within the background levels. Quiet flaring conditions are expected to continue, with a small chance of an isolated B-class flare. Solar wind speed decreased from about 440 km/s to its current values near 390 km/s. Total Interplanetary Magnetic Field (IMF) strength fluctuated between 6 nT and 8 nT, while Bz fluctuated between +1 nT and -6.5 nT, and was mostly negative. As the result the geomagnetic conditions have been slightly disturbed in the past 24 hours, (K Dourbes between 2 and 4; NOAA Kp between 2 and 4). The geomagnetic environment is expected to continue at the slightly disturbed levels, minor geomagnetic storm (Kp=4, Dst = 60) can be expected today.
Today's estimated international sunspot number (ISN): 031, based on 21 stations.
Wolf number Catania | 000 |
10cm solar flux | 076 |
AK Chambon La Forêt | 024 |
AK Wingst | 021 |
Estimated Ap | 019 |
Estimated international sunspot number | 000 - Based on 28 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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