Vydáno: 2014 Feb 06 1237 UTC
Active (M-class flares expected, probability >=50%)
Active conditions expected (A>=20 or K=4)
Warning condition (activity levels expected to increase, but no numeric forecast given)
10cm flux | Ap | |
---|---|---|
06 Feb 2014 | 197 | 005 |
07 Feb 2014 | 200 | 013 |
08 Feb 2014 | 196 | 009 |
Catania sunspot group 28 (NOAA AR 1967) is showing signs of decay, although it still maintains the beta-gamma-delta configuration of its photospheric magnetic field. It produced the strongest flare of the past 24 hours, the M1.3 flare peaking yesterday at 16:20 UT. No CME was associated with this flare. The area of Catania sunspot group 27 (NOAA AR 1968) is growing, but this group maintains the beta-gamma configuration of its photospheric magnetic field and produces only C-class flares. We expect further flaring activity on the C- and M-level in these two groups, with an X-class flare being possible but unlikely. A CME associated with a flare in these active regions may still arrive at the Earth. Due to position of these groups in the western hemisphere, a major CME in one of them may lead to a proton event, so we maintain the warning condition. The Earth is currently inside a slow (around 400 km/s) solar wind flow with elevated (7-8 nT) interplanetary magnetic field magnitude. Due to low solar wind speed, we expect quiet geomagnetic conditions in the coming hours. Late on February 7 we expect the arrival of the fast flow from an extended solar coronal hole (currently stretched across the solar central meridian), resulting in a geomagnetic disturbance up to active (K = 4) level.
Today's estimated international sunspot number (ISN): 112, based on 12 stations.
Wolf number Catania | /// |
10cm solar flux | 194 |
AK Chambon La Forêt | 010 |
AK Wingst | 004 |
Estimated Ap | 004 |
Estimated international sunspot number | 124 - Based on 22 stations |
Day | Begin | Max | Konec | Loc | Strength | OP | 10cm | Catania/NOAA | Radio burst types |
---|---|---|---|---|---|---|---|---|---|
05 | 1611 | 1620 | 1642 | ---- | M1.3 | 28/1967 |
Provided by the Solar Influences Data analysis Center© - SIDC - Processed by SpaceWeatherLive
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