Publié: 2014 Dec 07 1241 UTC
Eruptive (C-class flares expected, probability >=50%)
Warning condition (activity levels expected to increase, but no numeric forecast given)
Warning condition (activity levels expected to increase, but no numeric forecast given)
| Flux de 10 cm | Ap | |
|---|---|---|
| 07 Dec 2014 | 127 | 015 |
| 08 Dec 2014 | 122 | 009 |
| 09 Dec 2014 | 120 | 006 |
The solar activity is rather low, and the strongest flare during last 24 hours was a C3.7 flare (peaked at 13:52 UT on December 6) which originated from the Catania sunspot group 24 (NOAA AR 2222). We expect C-class flares in the coming hours. An issolated M-class flare is possible from the Catania sunspot group 24 (NOAA AR 2222) which is currently situated close to the west solar limb (S20W70). The strong flaring activity originating from this active region might be accompanied with the proton event. Therefore, we maintain the warning conditions for a proton event. No Earth directed CMEs were observed during last 24 hours. The Earth is currently inside of a fast solar wind with the speed of about 690 km/s, and the interplanetary magnetic field magnitude is about 7nT. The fast solar wind originating from the large polar coronal hole with the extent to the low latitudes (up to about S40) arrived at the Earth yesterday, as expected. The concurrent slow increase of the solar wind speed, density and the interplanetary magnetic field which started early on December 6, indicate strong compression region in front of the fast flow. Decrease of density and strong increase of the solar wind speed and temperature (observed at about 16:00 UT on December 6), indicate arrival of the fast flow itself. The maximum solar wind speed of about 800 km/s was observed this morning. The highest value of the interplanetary magnetic field magnitude of about 25nT, was recorded at about 15:00 UT on December 6. Due to arrival of the fast flow we observed few intervals of negative value of the Bz component of the interplanetary magnetic field (down to -14 nT at about 18:30 UT on December 6), which induced active to minor storm geomagnetic conditions from about 18:00 UT on December 6 until early this morning (the local station at Dourbes and Izmiran reported values of K=4, and NOAA reported one interval of Kp=5). We expect unsettled to active geomagnetic conditions in the coming hours.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 043, sur la base de 06 stations.
| Nombre de Wolf, observé par Catania | /// |
| Flux solaire à 10 cm | 129 |
| AK Chambon La Forêt | 032 |
| AK Wingst | 012 |
| Ap estimé | 013 |
| Nombre international de taches solaires estimé | 044 - Basé sur 21 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
De nombreuses personnes consultent SpaceWeatherLive pour suivre l'activité solaire ou observer les aurores boréales, mais l'augmentation du trafic engendre des coûts plus élevés pour maintenir les serveurs en ligne. Si vous appréciez SpaceWeatherLive et souhaitez soutenir le projet, vous pouvez vous abonner pour un site sans publicité ou faire un don. Grâce à votre aide, SpaceWeatherLive restera accessible !
| Dernière classe X | 04/02/2026 | X4.21 |
| Dernière classe M | 16/02/2026 | M2.4 |
| Dernier orage géomagnétique | 22/02/2026 | Kp5+ (G1) |
| Jours sans taches solaires | |
|---|---|
| 365 derniers jours | 1 jour |
| 2026 | 1 jour (2%) |
| Étirement actuel | 3 jours |
| Nombre mensuel moyen de taches solaires | |
|---|---|
| janvier 2026 | 112.6 -11.4 |
| février 2026 | 86.1 -26.5 |
| 30 derniers jours | 94.1 -27.9 |