Випущено: 2014 Jan 15 1241 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Warning condition (activity levels expected to increase, but no numeric forecast given)
10cm flux | Ap | |
---|---|---|
15 Jan 2014 | 137 | 004 |
16 Jan 2014 | 131 | 007 |
17 Jan 2014 | 125 | 006 |
The flaring activity is at the low C-class level. The last C-class flare reported was C3.2 flare which peaked at 16:04 UT, on January 14. The flare originated from the Catania sunspot group 98 (NOAA AR 1944). The background X-ray flux has high B-level, so we expect C-class flares, while M-class flares are not probable. The Catania sunspot group 98 (NOAA AR 1944) just rotated behind the West solar limb and we maintain the warning condition for a proton event for the following 24 hours. The eruption, originating from the Catania sunspot group 9 (NOAA AR 1950) at about 08:30 UT on January 14, was accompanied by coronal dimming, EIT wave and a post- eruption arcade observed by SDO/AIA. Due to data gap the associated partial halo CME was first seen in the SOHO/LASCO C2 field of view only at the height of about 4.5 solar radii, at 11:36 UT on January 14. The CME had a width of about 180 degrees and approximate speed of 400 km/s. The bulk of the CME mass was directed somewhat northward of the Sun-Earth line and we expect at least the glancing blow from the associated CME-driven shock wave, on January 18. The solar wind speed is still slowly decreasing and its current value is about 500 km/s. The interplanetary magnetic field is stable with the magnitude between 2 and 3 nT. The geomagnetic conditions are currently quiet and expected to remain so in the following 24 hours.
Today's estimated international sunspot number (ISN): 066, based on 08 stations.
Wolf number Catania | /// |
10cm solar flux | 137 |
AK Chambon La Forêt | 012 |
AK Wingst | 012 |
Estimated Ap | 012 |
Estimated international sunspot number | 070 - Based on 11 stations |
Day | Begin | Max | Кінець | Loc | Strength | OP | 10cm | Catania/NOAA | Radio burst types | |
---|---|---|---|---|---|---|---|---|---|---|
Немає |
Provided by the Solar Influences Data analysis Center© - SIDC - Processed by SpaceWeatherLive
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