Issued: 2014 Dec 11 1228 UTC
Eruptive (C-class flares expected, probability >=50%)
Quiet (A<20 and K<4)
Quiet
| 10cm flux | Ap | |
|---|---|---|
| 11 Dec 2014 | 155 | 008 |
| 12 Dec 2014 | 160 | 006 |
| 13 Dec 2014 | 165 | 005 |
Six C-class flares were measured during the past 24 hours. The strongest event was a C5.9 flare, peaking at 15:10 UT on December 10, originating from a filament region slightly west of NOAA 2230 (Catania 30). The associated CME is believed to be too narrow and directed to the South. Two other C-class flares erupted from new active region 2234 (no Catania number yet) which developed to a beta region. No geo-effective CME was observed in coronagraphic imagery. Flaring activity at the C-level is expected. A coronal hole with central location at N25E0 is passing the central meridian and is expected to cause the arrival of a high speed stream on December 14. Solar wind speed is gradually decreasing from 500 to about 400 km/s and the magnitude of the interplanetary magnetic field is relatively stable around 5 nT. The geomagnetic conditions were mostly quiet, with a time slot of active conditions (K=4 at Dourbes, 6-9 UT December 11). The NOAA estimated Kp remained below K=4 for the whole period. Quiet to unsettled conditions (K<4) are expected for the next 48 hours.
Today's estimated international sunspot number (ISN): 080, based on 07 stations.
| Wolf number Catania | /// |
| 10cm solar flux | 150 |
| AK Chambon La Forêt | 009 |
| AK Wingst | 010 |
| Estimated Ap | 008 |
| Estimated international sunspot number | 064 - Based on 18 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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