Issued: 2013 Apr 22 1049 UTC
Active (M-class flares expected, probability >= 50%)
Active conditions expected (A>=20 or K=4)
Warning condition
10cm flux | Ap | |
---|---|---|
22 Apr 2013 | 109 | 005 |
23 Apr 2013 | 109 | 004 |
24 Apr 2013 | 109 | 020 |
A recurrent coronal hole will influence geomagnetic conditions from April 24 onwards. In the last rotation, this coronal hole increased the solar wind speed up to 550 km/s and resulted in minor storm conditions (Kp=5). The CACTus CME detection software issued yesterday two automated halo CME alerts but these are not Earth-directed. Flaring conditions. NOAA AR 1726 keeps the potential for major flares although its magnetic complexity has decreased in the past 24 hours: a parasitic patch of opposite polarity has disappeared from the leading sunspot. Still M-class flares are likely. Proton >10 MeV fluxes are enhanced since yesterday 09:54 but not cross event thresholds. A warning conditions for more proton flux enhancements has been issued.
Today's estimated international sunspot number (ISN): 065, based on 06 stations.
Wolf number Catania | /// |
10cm solar flux | 109 |
AK Chambon La Forêt | 007 |
AK Wingst | 004 |
Estimated Ap | 003 |
Estimated international sunspot number | 064 - Based on 17 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
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