Issued: 2013 Jul 28 1309 UTC
Eruptive (C-class flares expected, probability >=50%)
Quiet (A<20 and K<4)
Quiet
10cm flux | Ap | |
---|---|---|
28 Jul 2013 | 106 | 010 |
29 Jul 2013 | 104 | 004 |
30 Jul 2013 | 105 | 004 |
Several weak C-class flares were detected during the last 24 hours in Catania sunspot groups 33 (NOAA AR 1793, currently behind the north-west limb) and 35 (NOAA AR 1800). We expect flaring activity to continue at the C-level (with an M-class flare unlikely), especially in the Catania sunspot group 35 (NOAA AR 1800) that keeps the beta-gamma configuration of its photospheric magnetic field. The Earth is currently inside a slow (around 440 km/s) solar wind flow with slightly elevated (around 6 nT) interplanetary magnetic field magnitude. We expect quiet to unsettled geomagnetic conditions.
Today's estimated international sunspot number (ISN): 048, based on 09 stations.
Wolf number Catania | /// |
10cm solar flux | 108 |
AK Chambon La Forêt | 020 |
AK Wingst | 014 |
Estimated Ap | 014 |
Estimated international sunspot number | 047 - Based on 17 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
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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