Publié: 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)
| Flux de 10 cm | 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.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 112, sur la base de 12 stations.
| Nombre de Wolf, observé par Catania | /// |
| Flux solaire à 10 cm | 194 |
| AK Chambon La Forêt | 010 |
| AK Wingst | 004 |
| Ap estimé | 004 |
| Nombre international de taches solaires estimé | 124 - Basé sur 22 stations |
| Jour | Commencer | Max | Fin | Loc | Force | OP | 10cm | Catania/NOAA | Types de sursaut radio |
|---|---|---|---|---|---|---|---|---|---|
| 05 | 1611 | 1620 | 1642 | ---- | M1.3 | 28/1967 |
Données fournies par le Solar Influences Data analysis Center© - SIDC - Traité par SpaceWeatherLive
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