Publié: 2014 Dec 22 1228 UTC
Active (M-class flares expected, probability >=50%)
Minor storm expected (A>=30 or K=5)
Warning condition (activity levels expected to increase, but no numeric forecast given)
| Flux de 10 cm | Ap | |
|---|---|---|
| 22 Dec 2014 | 200 | 026 |
| 23 Dec 2014 | 200 | 020 |
| 24 Dec 2014 | 200 | 010 |
Solar activity remains dominated by NOAA active region 2242. This beta-gamma-delta region has produced four C-class and one M-class flares in the past period. An impulsive M1.0 flare, peaking at 1:49 UT on December 22 was the strongest one. More strong flares, at the C- and M-level are expected from NOAA 2241 and especially 2242. Also X-flares are possible (chance at 25%). The > 10 MeV proton flux as observed by GOES started rising gradually after the C5.6 flare of 20:35 UT on December 20. A faster ascent is noted after the M1.0 flare of 12:17 UT on December 21. The proton flux is decreasing again, but is still at an elevated level (near 1 pfu). As the NOAA regions 2241 and 2242 are approaching the west limb, we retain the warning for a proton event, which might occur in case of more strong flares. No additional Earth-bound CMEs were observed. A shock in the solar wind was observed by both ACE and SOHO/CELIAS near 18:25 UT on December 21. The solar wind velocity went from 360 to 440 km/s instantaneously, accompanied by a sudden increase of the solar wind density and temperature. The magnitude of the Interplanetary Magnetic Field (IMF) jumped from 9 to 17 nT and remained at these high levels till about 3:40 UT when it dropped to about 13 nT. These are strong indications for the arrival of the December 19 CME. The vertical component of the magnetic field was mainly negative and varied between -17 and 8 nT. Active geomagnetic conditions were observed at Dourbes (local K= 4), with even minor storm conditions at the global level (NOAA estimated Kp up to 5). A continuation of the active to minor storm conditions (K=4 to 5) are expected, certainly in case of the estimated arrival of the December 20 CME in the course of today.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 089, sur la base de 06 stations.
| Nombre de Wolf, observé par Catania | /// |
| Flux solaire à 10 cm | 206 |
| AK Chambon La Forêt | 033 |
| AK Wingst | 014 |
| Ap estimé | 014 |
| Nombre international de taches solaires estimé | 106 - Basé sur 16 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 | 16/02/2026 | Kp6 (G2) |
| 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 | 100.6 -12 |
| 30 derniers jours | 117.7 +9.9 |