Publié: 2017 Dec 05 1242 UTC
Quiet conditions (<50% probability of C-class flares)
Minor storm expected (A>=30 or K=5)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 05 Dec 2017 | 066 | 022 |
| 06 Dec 2017 | 067 | 033 |
| 07 Dec 2017 | 068 | 024 |
The solar activity remained very quiet. The visible solar disc is spotless and no flare has been recorded in the past 24-hour. Quiet flaring conditions are expected.
No Earth directed Coronal Mass Ejection has been observed. The greater than 10 MeV solar protons flux remained at nominal levels over the past 24 hours and is expected to remain so.
The High Speed solar wind Stream (HSS) associated with the Coronal Hole (which has crossed the central meridian on Dec 01) has arrived, and the wind speed has shown a gradual increased from its nominal level to the current level of about 550 km/s. Since the arrival of the Corotating Interaction Region announcing the HSS on Dec 04 around 15:00 UT, the interplanetary magnetic field magnitude has increased to fluctuate between 9-12 nT, and the Bz component has fluctuated between -12 and 10 nT. The solar wind conditions are expected to persist until while under the influence of the HSS associated with the coronal hole.
Disturbed geomagnetic conditions were observed due to the fast solar wind and the Bz component of the interplanetary magnetic field reaching -12 nT. A minor storm was observed by the local stations at Dourbes (K=5 from 19:00 to 20:00 UT on Dec 04), while NOAA reported Kp=5 at 12:00 UT on Dec 05. The high speed stream is expected to persist and further minor to moderate geomagnetic storms cannot be excluded, especially if Bz component remains negative for long period of time.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 000, sur la base de 11 stations.
| Nombre de Wolf, observé par Catania | 000 |
| Flux solaire à 10 cm | 068 |
| AK Chambon La Forêt | 031 |
| AK Wingst | 013 |
| Ap estimé | 015 |
| Nombre international de taches solaires estimé | 000 - 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
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 | 2 jours |
| 2026 | 2 jours (4%) |
| Étirement actuel | 3 jours |
| Nombre mensuel moyen de taches solaires | |
|---|---|
| janvier 2026 | 112.6 -11.4 |
| février 2026 | 82.3 -30.3 |
| 30 derniers jours | 91 -31 |