Issued: 2013 Sep 20 1202 UTC
Eruptive (C-class flares expected, probability >=50%)
Active conditions expected (A>=20 or K=4)
Quiet
10cm flux | Ap | |
---|---|---|
20 Sep 2013 | 109 | 010 |
21 Sep 2013 | 113 | 007 |
22 Sep 2013 | 115 | 014 |
There are currently nine numbered sunspot groups on the solar disc, and three of them have beta configuration of the photospheric magnetic field. Three low C-class level flares were reported during last 24 hours and all originated from the same NOAA AR 1850, which just turned from behind the east solar limb. We expect more flaring activity at the C-class level. The M-class flares are possible but not very probable. The solar wind speed is about 480 km/s and slowly decreasing, and the interplanetary magnetic field magnitude is stable amounting about 3 nT. The geomagnetic conditions are at the moment quiet. We expect quiet to active geomagnetic conditions in the following 48 hours due to the arrival of a fast flow (in the morning of September 22), associated with the low-latitude coronal hole in the northern hemisphere.
Today's estimated international sunspot number (ISN): 062, based on 12 stations.
Wolf number Catania | 094 |
10cm solar flux | 108 |
AK Chambon La Forêt | 019 |
AK Wingst | 012 |
Estimated Ap | 013 |
Estimated international sunspot number | 044 - Based on 19 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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