Publié: 2018 Dec 06 1233 UTC
Quiet conditions (<50% probability of C-class flares)
Active conditions expected (A>=20 or K=4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 06 Dec 2018 | 070 | 003 |
| 07 Dec 2018 | 070 | 020 |
| 08 Dec 2018 | 070 | 019 |
The solar activity has been quiet over the past 24 hours. One small bipolar sunspot group (Catania sunspot group 2, NOAA 2729) is visible on the disc, but no significant flare has been recorded. Flaring conditions is expected to remain quiet with a small change of C-class flare.
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 solar wind measurements remained under the influence of the enhanced solar wind associated with the Coronal Hole (which reached the central meridian on November 27). The wind speed decreased from 462 to about 390 km/s. The interplanetary magnetic field strength was below 5.5 nT and the southward magnetic component fluctuated between -4 and 4.5 nT. The solar wind parameters are expected to continue to decrease to the slow solar wind regime. Then the solar wind parameters are expected to be enhanced due to the fast solar wind associated with this coronal hole (which reached the central meridian on December 04) on December 7.
The geomagnetic conditions were quiet. The conditions are expected to be mainly quiet as the Earth is entering the slow solar wind speed regime. The geomagnetic conditions will then become more active due to the arrival of the fast solar wind on December 7.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 020, sur la base de 07 stations.
| Nombre de Wolf, observé par Catania | 017 |
| Flux solaire à 10 cm | /// |
| AK Chambon La Forêt | /// |
| AK Wingst | /// |
| Ap estimé | /// |
| Nombre international de taches solaires estimé | 017 - Basé sur 15 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 | X4.3 |
| Dernière classe M | 05/02/2026 | M1.1 |
| Dernier orage géomagnétique | 05/02/2026 | Kp5+ (G1) |
| Jours sans taches solaires | |
|---|---|
| Dernier jour sans taches solaires | 08/06/2022 |
| Nombre mensuel moyen de taches solaires | |
|---|---|
| janvier 2026 | 112.6 -11.4 |
| février 2026 | 140.8 +28.2 |
| 30 derniers jours | 124.4 +17 |