Issued: 2013 Feb 10 1203 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
10cm flux | Ap | |
---|---|---|
10 Feb 2013 | 108 | 003 |
11 Feb 2013 | 108 | 012 |
12 Feb 2013 | 109 | 011 |
The background X-ray flax has a low B-level. There were no C-class flares during last 24 hours. C-class flares are still possible, in particular from the Catania sunspot group 80 (NOAA AR 1670) which has the beta-gama configuration of its photospehric magnetic field. Earth is currently inside a slow solar wind with a speed of about 350 km/s. The interplanetary magnetic field magnitude is stable with value of about 5 nT. The partial halo CME from February 9 might arrive at the Earth on February 12 producing unsettled geomagnetic conditions. We expect geomagnetic conditions in the next 48 hours.
Today's estimated international sunspot number (ISN): 029, based on 12 stations.
Wolf number Catania | /// |
10cm solar flux | 108 |
AK Chambon La Forêt | 008 |
AK Wingst | 003 |
Estimated Ap | 003 |
Estimated international sunspot number | 039 - Based on 11 stations |
Day | Begin | Max | End | Loc | Strength | OP | 10cm | Radio burst types | Catania/NOAA | |
---|---|---|---|---|---|---|---|---|---|---|
None |
Provided by the Solar Influences Data analysis Center© - SIDC - Processed by SpaceWeatherLive
All times in UTC
Current data suggests there is a slight possibility for aurora to appear at the following high latitude regions in the near future
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