Publié: 2015 Sep 10 1231 UTC
Quiet conditions (<50% probability of C-class flares)
Active conditions expected (A>=20 or K=4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 10 Sep 2015 | 081 | 014 |
| 11 Sep 2015 | 080 | 020 |
| 12 Sep 2015 | 078 | 010 |
Only four small sunspot groups are presently visible on the solar disc. The flaring activity is on the B-class level and we expect it to remain so in the following 24 hours. No Earth directed CMEs were observed during last 24 hours.
The solar wind speed is currently 430 km/s, and the interplanetary magnetic field magnitude is about 9 nT. The long interval of the negative value of the Bz component (down to -8 nT) and at that moment still high solar wind speed (about 430 km/s) induced geomagnetic storm conditions lasting from about 18 UT yesterday until 03 UT today, NOAA reported Kp=6 and local station Dourbes reported K=5. The fast flow, associated with the elongated equatorial coronal hole (20S to 20N) which crossed central meridian in the morning of September 08, is expected late this evening or tomorrow morning. Additionally, the fast flow from the low latitude extension of the northern polar coronal hole which crossed the central meridian yesterday morning is expected late on September 11 or in the morning of September 12. Currently the geomagnetic conditions are quiet and we expected these conditions to persist in the coming hours. However, arrival of the fast flow can induced active to geomagnetic storm conditions later today and tomorrow morning.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 044, sur la base de 19 stations.
| Nombre de Wolf, observé par Catania | /// |
| Flux solaire à 10 cm | 082 |
| AK Chambon La Forêt | 064 |
| AK Wingst | 051 |
| Ap estimé | 053 |
| Nombre international de taches solaires estimé | 046 - Basé sur 25 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 | 18/03/2026 | M2.7 |
| Dernier orage géomagnétique | 22/03/2026 | Kp7- (G3) |
| Jours sans taches solaires | |
|---|---|
| 365 derniers jours | 3 jours |
| 2026 | 3 jours (4%) |
| Dernier jour sans taches solaires | 24/02/2026 |
| Nombre mensuel moyen de taches solaires | |
|---|---|
| février 2026 | 78.2 -34.3 |
| mars 2026 | 77 -1.2 |
| 30 derniers jours | 68.9 -24 |