Issued: 2014 Oct 01 1234 UTC
Eruptive (C-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 | |
---|---|---|
01 Oct 2014 | 155 | 015 |
02 Oct 2014 | 150 | 017 |
03 Oct 2014 | 147 | 017 |
Only one C-class flare was observed during the period. This C6.7 flare was located in NOAA 2172 and peaked at 03:06UT. The other 8 sunspot groups have been quiet. NOAA 2178 seems to be the most complex, with opposite magnetic polarities close to each other but no apparent delta structure. A CME first observed by LASCO at 08:48UT on 01 October was associated to a prominence eruption near the east limb. It is not Earth directed. The x-ray background flux is still above the C1-level. Two 20-degrees long filaments visible in the western solar hemisphere have remained quiet. C-class flaring is expected, with still a chance on an isolated M-class flare. Solar wind speed varied between 350 and 400 km/s, with peaks near 450 km/s. Bz fluctuated between -7 and +5 nT. A few isolated active periods were recorded. Geomagnetic conditions are expected to be quiet to unsettled, with isolated active periods possible.
Today's estimated international sunspot number (ISN): 103, based on 12 stations.
Wolf number Catania | 185 |
10cm solar flux | 162 |
AK Chambon La Forêt | 023 |
AK Wingst | 014 |
Estimated Ap | 014 |
Estimated international sunspot number | /// - Based on /// 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
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