Issued: 2013 Nov 27 1334 UTC
Eruptive (C-class flares expected, probability >=50%)
Quiet (A<20 and K<4)
Quiet
10cm flux | Ap | |
---|---|---|
27 Nov 2013 | 116 | 002 |
28 Nov 2013 | 118 | 007 |
29 Nov 2013 | 120 | 007 |
Solar activity has been low, no C-class flares in past 24 hours. The activity levels are expected to increase while a recurring active region rotates over the eastern limb. There was a partial halo CME seen at 02:15 UT by LASCO-C2 after a data gap, apparently originating in a filament eruption over the western limb. Part of the material is backsided and the bulk of the CME is directed towards the south, so most likely the Earth will not be affected. Solar wind speed is currently at 300 km/s with interplanetary magnetic field intensity at 6 nT. Geomagnetic conditions are quiet and expected to remain so.
Today's estimated international sunspot number (ISN): 054, based on 13 stations.
Wolf number Catania | /// |
10cm solar flux | 116 |
AK Chambon La Forêt | 003 |
AK Wingst | 002 |
Estimated Ap | 001 |
Estimated international sunspot number | 028 - Based on 15 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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