Emesso: 2015 Oct 23 1230 UTC
C-class flares expected, (probability >=50%)
Minor storm expected (A>=30 or K=5)
Quiet
10cm flux | Ap | |
---|---|---|
23 Oct 2015 | 115 | 006 |
24 Oct 2015 | 110 | 012 |
25 Oct 2015 | 105 | 016 |
Solar activity was low without any significant flare. NOAA active region 2436 remains the most complex region, but was inactive. The > 10 MeV proton flux was enhanced from 23:00 UT on, but remained well below the event threshold. This disturbance probably was due to the long duration flare of October 22. Flaring at the C-level is expected. No Earth-directed CMEs were observed in current available coronagraphic images.
The solar wind speed was at 400 km/s till 22UT, when the speed became variable between 400 and 500 km/s. The interplanetary magnetic field was at a constant magnitude around 5 nT. Quiet (K<3) to unsettled (K=3) geomagnetic conditions were observed, which are expected to continue for the next 24 hours. From the second half of October 24 the solar wind might be disturbed due to a glancing blow from the October 22 CME. This can result in (at maximum) minor storm (K=5) conditions.
Today's estimated international sunspot number (ISN): 090, based on 08 stations.
Wolf number Catania | /// |
10cm solar flux | 121 |
AK Chambon La Forêt | 012 |
AK Wingst | 006 |
Estimated Ap | 005 |
Estimated international sunspot number | 095 - Based on 19 stations |
Day | Begin | Max | Fine | Loc | Strength | OP | 10cm | Catania/NOAA | Radio burst types | |
---|---|---|---|---|---|---|---|---|---|---|
Nessuna |
Provided by the Solar Influences Data analysis Center© - SIDC - Processed by SpaceWeatherLive
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