Publié: 2014 Feb 07 1303 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 | |
|---|---|---|
| 07 Feb 2014 | 188 | 012 |
| 08 Feb 2014 | 185 | 012 |
| 09 Feb 2014 | 182 | 005 |
Catania sunspot group 28 (NOAA AR 1967) is slowly decaying, although still maintaining the beta-gamma-delta configuration of its photospheric magnetic field. It produced the strongest flare of the past 24 hours, the M2.0 flare peaking at 04:56 UT today. Catania sunspot group 27 (NOAA AR 1968, beta-gamma configuration of the photospheric field) produced an M1.9 flare peaking today at 10:29 UT. Neither of the flares was associated with a CME. We expect further flaring activity on the C- and M-level in these two groups, with an X-class flare being possible but unlikely. 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 350 km/s) solar wind flow with a slightly elevated (around 6 nT) interplanetary magnetic field magnitude. Due to low solar wind speed, we expect quiet geomagnetic conditions in the coming hours. Later today 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 : 108, sur la base de 09 stations.
| Nombre de Wolf, observé par Catania | 157 |
| Flux solaire à 10 cm | 191 |
| AK Chambon La Forêt | 008 |
| AK Wingst | 008 |
| Ap estimé | 007 |
| Nombre international de taches solaires estimé | 112 - Basé sur 15 stations |
| Jour | Commencer | Max | Fin | Loc | Force | OP | 10cm | Catania/NOAA | Types de sursaut radio |
|---|---|---|---|---|---|---|---|---|---|
| 06 | 2256 | 2305 | 2310 | ---- | M1.5 | 180 | 28/1967 | ||
| 07 | 0447 | 0456 | 0504 | S15W50 | M2.0 | 2N | 28/1967 | ||
| 07 | 1025 | 1029 | 1031 | N09W53 | M1.9 | 1N | 27/1968 |
Données fournies par le Solar Influences Data analysis Center© - SIDC - Traité par SpaceWeatherLive
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