Publié: 2015 Dec 27 1230 UTC
C-class flares expected, (probability >=50%)
Quiet (A<20 and K<4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 27 Dec 2015 | 113 | 015 |
| 28 Dec 2015 | 110 | 017 |
| 29 Dec 2015 | 115 | 013 |
Solar flaring activity was low with the strongest flare a C4.1 flare peaking at 15:26 UT from NOAA AR 2473 (beta-gamma-delta, Catania nr 5). NOAA AR 2473 remains the most complex of the two regions on disk. It showed some further consolidation in the leading an intermediate spots. Flaring is expected at C level with also M level flaring quite possible. No Earth directed CME's have been detected. Solar wind speed continued to climb over the first half of the period reaching a short lived peak of around 640 km/s at 20:24 UT. The increase was associated with a rise in total interplanetary magnetic field to around 7-8 nT and a sustained period of negative Bz around -6nT before midnight. Solar wind speed meanwhile recovered to an intermediate value of around 530 km/s and also magnetic field recovered to 5-6 nT. A corresponding isolated period of minor geomagnetic storm levels was reported around midnight (both NOAA Kp and local K Dourbes 5 for the 21-24 UT period) with otherwise quiet to active conditions (local K Dourbes 2-4, NOAA Kp 2-3). Slightly enhanced solar wind conditions are expected to persist with essentially quiet to unsettled geomagnetic conditions although some periods of active geomagnetic conditions can not be excluded. The influence of a positive polarity coronal hole high speed stream may further enhance solar wind and geomagnetic conditions from late December 28 onwards.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 063, sur la base de 15 stations.
| Nombre de Wolf, observé par Catania | /// |
| Flux solaire à 10 cm | 117 |
| AK Chambon La Forêt | /// |
| AK Wingst | 019 |
| Ap estimé | 015 |
| Nombre international de taches solaires estimé | 056 - Basé sur 23 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 | 30/03/2026 | X1.4 |
| 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 | 88.4 +10.2 |
| 30 derniers jours | 88.4 +14.9 |