Publié: 2018 Feb 10 1251 UTC
C-class flares expected, (probability >=50%)
Quiet (A<20 and K<4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 10 Feb 2018 | 078 | 005 |
| 11 Feb 2018 | 077 | 003 |
| 12 Feb 2018 | 076 | 008 |
Solar activity was low, no C-class flares in past 24 h. NOAA 2699 has decayed from beta-gamma to beta magnetic field configuration, however it can still produce C-class flares in the coming hours. Proton flux levels are at background values and are expected to remain so. No Earth-directed CMEs were observed. Solar wind speed is at 340 km/s with interplanetary magnetic field magnitude of 6 nT. Geomagnetic conditions reached unsettled levels (K = 3) this morning due to interplanetary magnetic field elevated values of 10.7 nT. Bz component remained strictly positive around 9 nT, and speeds elevated simultaniously only till 380 km/s. Quiet to unsettled conditions can be expected in the next 48 h.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 027, sur la base de 10 stations.
| Nombre de Wolf, observé par Catania | /// |
| Flux solaire à 10 cm | 078 |
| AK Chambon La Forêt | 008 |
| AK Wingst | 006 |
| Ap estimé | 005 |
| Nombre international de taches solaires estimé | 026 - Basé sur 19 stations |
| Jour | Commencer | Max | Fin | Loc | Force | OP | 10cm | Catania/NOAA | Types de sursaut radio | |
|---|---|---|---|---|---|---|---|---|---|---|
| Aucun | ||||||||||
Données fournies par le Solar Influences Data analysis Center© - SIDC - Traité par SpaceWeatherLive
Toutes les heures sont indiquées en UTC
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