Issued: 2013 Nov 12 1322 UTC
Active (M-class flares expected, probability >=50%)
Active conditions expected (A>=20 or K=4)
Warning condition (activity levels expected to increase, but no numeric forecast given)
10cm flux | Ap | |
---|---|---|
12 Nov 2013 | 164 | 009 |
13 Nov 2013 | 168 | 017 |
14 Nov 2013 | 172 | 010 |
Since the CME-less M2.4 flare which peaked at 11:18 UT on November 11, only six C-class flares were reported. We expect M-class flares and possibly but not very probably X-class flares, in particular from the Catania sunspot group 35 (NOAA AR 1890) and NOAA AR 1897. The Catania sunspot group 35 (NOAA AR 1890) is situated in the western solar hemisphere and still has the beta-gamma-delta configuration of its photospheric magnetic field, therefore we maintain the warning condition for a proton event. From the currently available data it seems that the CME first observed in SOHO/LASCO C2 field of view at about 08:48 UT on November 12, is possibly Earth- oriented. This will be confirmed when more data will be available. The solar wind speed is around 420 km/s and the interplanetary magnetic field (IMF) magnitude is about 4 nT. We expect quiet geomagnetic conditions in the coming hours and active geomagnetic conditions late on November 13 due to arrival of the halo CME which erupted on November 10.
Today's estimated international sunspot number (ISN): 093, based on 07 stations.
Wolf number Catania | /// |
10cm solar flux | 164 |
AK Chambon La Forêt | 018 |
AK Wingst | 021 |
Estimated Ap | 021 |
Estimated international sunspot number | 078 - Based on 18 stations |
Day | Begin | Max | End | Loc | Strength | OP | 10cm | Catania/NOAA | Radio burst types |
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Provided by the Solar Influences Data analysis Center© - SIDC - Processed by SpaceWeatherLive
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