Emesso: 2014 Aug 09 1204 UTC
Eruptive (C-class flares expected, probability >=50%)
Quiet (A<20 and K<4)
Quiet
10cm flux | Ap | |
---|---|---|
09 Aug 2014 | 115 | 008 |
10 Aug 2014 | 110 | 007 |
11 Aug 2014 | 110 | 007 |
Four C-class flares were observed since our last bulletin. The largest one was a C4.5 flare at 16:57 UT on August 8 in NOAA AR 2135, that has developed into a beta-gamma region. This region, as well as NOAA AR 2132, is expected to produce more C-class flares in the coming days. There is also a small chance for an M-flare. CACTus reported on a halo CME observed in LASCO images on August 8 around 16:36 UT. This full halo CME was associated to a strong eruption observed in the center of the solar disk in STEREO-a/EUVI 195 images starting at 15:55 UT. This is thus a back- sided event and therefore the CME will not be geo-effective. We expect quiet geomagnetic conditions to persist, with a chance for unsettled conditions (K maximum 3) under the possible influence of a coronal hole wind stream.
Today's estimated international sunspot number (ISN): 062, based on 15 stations.
Wolf number Catania | /// |
10cm solar flux | 123 |
AK Chambon La Forêt | 010 |
AK Wingst | 014 |
Estimated Ap | 013 |
Estimated international sunspot number | 061 - Based on 20 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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