Publié: 2014 Dec 24 1236 UTC
Eruptive (C-class flares expected, probability >=50%)
Active conditions expected (A>=20 or K=4)
Warning condition (activity levels expected to increase, but no numeric forecast given)
| Flux de 10 cm | Ap | |
|---|---|---|
| 24 Dec 2014 | 150 | 013 |
| 25 Dec 2014 | 140 | 006 |
| 26 Dec 2014 | 140 | 006 |
Six C-class flares were observed since our last bulletin. Catania sunspot regions 39 and 38 (NOAA active regions 2241 and 2242 respectively) once more were the main players. The strongest flare was a C4.9 flare peaking at 22:49 UT on December 23, erupted from Catania 38. A C3.7 flare occurred in Catania 39, peaking at on December 24. During the event plasma material was ejected as seen on SDO/AIA imagery, indicating the possibility for an accompanying CME. Due to a data gap in SOHO/LASCO coronagraphic imagery, this can not be confirmed yet. Catania region 42 (NOAA 2244) was not very productive and only produced small C-flares, though it still has a beta-gamma magnetic structure. More C-flares are expected, with a chance for an isolated M-flare. The > 10 MeV proton flux has decreased again to 1 to 4 pfu, but still remains at this enhanced level. The proton warning is retained. Flaring activity from Catania regions 38 and 39, currently positioned near the west limb, might introduce an increase of the proton flux. No Earth-effective CMEs were observed yet. The solar wind speed first obtained values between 400 and 500 km/s and increased around 23 UT to about 600 km/s. The magnitude of the interplanetary magnetic field decreased from about 30 to 7 nT, with a fluctuating Bz component. The shock arrival at 10:30 UT on December 23, is believed to be associated to a CME on December 21 (first measurement in LASCO at 12:12 UT, related to the M1.0 flare at 12:17 UT). The phi component indicated a few sector boundary crossings, starting at a positive sector and then from 17:30 UT on going back and forth between positive and negative sectors. Geomagnetic conditions were active (NOAA Kp till K=4), with a single time slot of minor storm conditions at the local level (Dourbes reached K=5 around 21 UT). Geomagnetic conditions might further be influenced by CME effects, probably resulting in unsettled to active levels for the next day.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 063, sur la base de 10 stations.
| Nombre de Wolf, observé par Catania | 151 |
| Flux solaire à 10 cm | 166 |
| AK Chambon La Forêt | 025 |
| AK Wingst | 013 |
| Ap estimé | 013 |
| Nombre international de taches solaires estimé | 086 - 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 | 18/01/2026 | X1.9 |
| Dernière classe M | 21/01/2026 | M3.4 |
| Dernier orage géomagnétique | 22/01/2026 | Kp5+ (G1) |
| Jours sans taches solaires | |
|---|---|
| Dernier jour sans taches solaires | 08/06/2022 |
| Nombre mensuel moyen de taches solaires | |
|---|---|
| décembre 2025 | 124 +32.2 |
| janvier 2026 | 118.7 -5.3 |
| 30 derniers jours | 120.4 +5.6 |