Vydáno: 2014 Mar 22 1206 UTC
Eruptive (C-class flares expected, probability >=50%)
Quiet (A<20 and K<4)
Quiet
10cm flux | Ap | |
---|---|---|
22 Mar 2014 | 145 | 007 |
23 Mar 2014 | 145 | 006 |
24 Mar 2014 | 145 | 006 |
NOAA AR 2011 released an M1.1 flare today, March 22, peak 07:02UT. This flare was followed by another peak in the x-ray flux not entirely visible due to data dropouts from the GOES satellite occurring during a satellite eclipse. The Solar Demon software detected an eruption in SDO/AIA 94 images in the neighbourhood of NOAA AR 2005, peak 9:30UT. We expect more flaring activity in the C-level. Isolated M-flares are possible. CACTus software sent out a halo CME alert about a plasma eruption on March 20. It concerns the plasma eruption mentioned in the ursigram of March 20 associated with the M1.7 flare. Newly arrived data shows a faint appearance of a CME front in LASCO/SOHO C2 images that comes into the FOV at 04:36UT. The CME has an angular width of around 180 degrees. The solar wind picked up speed (around 450 km/s). The Bz component is positive resulting in a Kp of 2. We expect quiet geomagnetic conditions.
Today's estimated international sunspot number (ISN): 118, based on 08 stations.
Wolf number Catania | 152 |
10cm solar flux | 153 |
AK Chambon La Forêt | 014 |
AK Wingst | 009 |
Estimated Ap | 010 |
Estimated international sunspot number | 087 - Based on 23 stations |
Day | Begin | Max | Konec | Loc | Strength | OP | 10cm | Catania/NOAA | Radio burst types |
---|---|---|---|---|---|---|---|---|---|
22 | 0658 | 0702 | 0705 | S10W71 | M1.1 | 1F | 87/2011 |
Provided by the Solar Influences Data analysis Center© - SIDC - Processed by SpaceWeatherLive
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