Publié: 2015 Dec 28 1230 UTC
M-class flares expected (probability >=50%)
Quiet (A<20 and K<4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 28 Dec 2015 | 107 | 007 |
| 29 Dec 2015 | 112 | 012 |
| 30 Dec 2015 | 115 | 007 |
Solar activity has been low with only a couple of C flares over the period. NOAA AR 2473 produced the strongest one, a C8.0 flare peaking at 00:28UT. During the writing of this report another flare from NOAA AR 2473 was ongoing, likely to peak near M1 level. NOAA AR 2473 remains capable of strong flaring. Flaring at M level is likely with also a slight chance for an X flare. No CMEs have been detected in coronagraph data. Total interplanetary magnetic field has decreased over the period from over 5nT to around the 2-4 nT range. After initially remaining elevated at levels around 520 km/s, solar wind speed started to decrease towards current levels of 440 km/s. Also temperature has decreased over the period. The magnetic field Bz component has been variable but with an extended period of positive values. The magnetic field phi angle switched back and forth between inward and outward direction and is expected to settle in the outward direction. Later today or tomorrow we may experience a renewed increase in solar wind conditions due to the possible influence of a high speed stream from a small equatorial coronal hole. Geomagnetic conditions have been quiet to unsettled (both NOAA Kp and local K Dourbes 1-3). Quiet to unsettled conditions are expected to continue with some active periods possible.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 065, sur la base de 18 stations.
| Nombre de Wolf, observé par Catania | /// |
| Flux solaire à 10 cm | 110 |
| AK Chambon La Forêt | 014 |
| AK Wingst | 012 |
| Ap estimé | 011 |
| Nombre international de taches solaires estimé | 062 - 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 | 28/03/2026 | M1.3 |
| Dernier orage géomagnétique | 25/03/2026 | Kp5+ (G1) |
| Jours sans taches solaires | |
|---|---|
| 365 derniers jours | 3 jours |
| 2026 | 3 jours (3%) |
| Dernier jour sans taches solaires | 24/02/2026 |
| Nombre mensuel moyen de taches solaires | |
|---|---|
| février 2026 | 78.2 -34.3 |
| mars 2026 | 85.2 +7 |
| 30 derniers jours | 85.2 +8.6 |