Publié: 2015 Aug 27 1232 UTC
M-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 | |
|---|---|---|
| 27 Aug 2015 | 128 | 037 |
| 28 Aug 2015 | 130 | 028 |
| 29 Aug 2015 | 130 | 015 |
Solar flaring activity was moderate with an M2.9 flare peaking 5:44 UT from region 2403. The region produced also a C9.5 flare earlier in the period, peaking at 13:53UT which was related with a dimming and filament eruptions to the North of the region. Corresponding ejecta are seen in SoHO/LASCO C2 data on the West limb around 20:36, but seem insignificant. Region 2403 remains complex and may be the source of further M-flaring with a slight chance for an X flare. Meanwhile two new regions are also rotating onto the Eastern hemisphere but their flaring potential appears low. The warning condition for proton events in relation to AR 2403 is maintained. No Earth directed CME's were observed in coronagraph data. Solar wind saw a further decline of the solar wind speed from around 400 km/s to around 360 km/s. The already elevated total magnetic field (10 nT at the start of the period) reached peaks of around 14nT this morning. Along with sustained periods of pronounced negative Bz this caused associated minor to moderate geomagnetic storm conditions since afternoon/late August 26. While local K Dourbes reported only active conditions to minor storm conditions, the planetary NOAA Kp reached moderate storm conditions (Kp=6) for the 3-6 and 6-9UT intervals. The origin of the elevated magnetic field values is not very clear. While a corotating interaction region (CIR) was expected later today, the signatures of magnetic field rotation, low temperatures and declining speed profile are more indicative of an ICME preceding the expected CIR. After the passage of the expected CIR solar wind speeds are expected to rise due to coronal hole high speed stream influence. Thus, solar wind conditions are in any case expected to remain elevated and active to moderate storm conditions are expected to continue over the next day subject to solar wind magnetic field orientation.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 063, sur la base de 11 stations.
| Nombre de Wolf, observé par Catania | /// |
| Flux solaire à 10 cm | 126 |
| AK Chambon La Forêt | 053 |
| AK Wingst | 037 |
| Ap estimé | 036 |
| Nombre international de taches solaires estimé | 044 - Basé sur 32 stations |
| Jour | Commencer | Max | Fin | Loc | Force | OP | 10cm | Catania/NOAA | Types de sursaut radio |
|---|---|---|---|---|---|---|---|---|---|
| 27 | 0448 | 0544 | 0603 | S14W45 | M2.9 | 1N | --/2403 |
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 | 02/02/2026 | X1.6 |
| Dernière classe M | 02/02/2026 | M2.4 |
| Dernier orage géomagnétique | 28/01/2026 | 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 |
| février 2026 | 97 -27 |
| 30 derniers jours | 118.3 +3.5 |