Issued: 2014 Oct 05 1240 UTC
Eruptive (C-class flares expected, probability >=50%)
Quiet (A<20 and K<4)
Quiet
| 10cm flux | Ap | |
|---|---|---|
| 05 Oct 2014 | 121 | 011 |
| 06 Oct 2014 | 117 | 011 |
| 07 Oct 2014 | 114 | 009 |
The only C-class event of the period was a C1 flare peaking at 09:54UT and produced by NOAA 2178. The 7 groups currently visible on the solar disk have a relatively simple magnetic configuration and have been quiet. Numerous filaments are present on the solar disk, but they are mostly small and quiet. There remains a chance on an C-class flare. No obvious CMEs were observed during the period. A corotating interaction region has influenced the solar wind since late on 3 October. Around 17:00UT on 4 October, the direction of the IMF turned towards the Sun, and solar wind speed peaked near values of 480 km/s early on 5 October. Bz was mostly positive, fluctuating between -5 and +10 nT during the latter half of the observation period. Geomagnetic conditions were quiet to unsettled and are expected to remain so.
Today's estimated international sunspot number (ISN): 068, based on 11 stations.
| Wolf number Catania | /// |
| 10cm solar flux | 128 |
| AK Chambon La Forêt | 008 |
| AK Wingst | 004 |
| Estimated Ap | 004 |
| Estimated international sunspot number | 079 - Based on 21 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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