Publié: 2015 Aug 18 1241 UTC
Quiet conditions (<50% probability of C-class flares)
Active conditions expected (A>=20 or K=4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 18 Aug 2015 | 085 | 021 |
| 19 Aug 2015 | 086 | 021 |
| 20 Aug 2015 | 086 | 017 |
Solar activity has been quiet over the past 24 hours. There have been a few low magnitude B-class flares and no C, or above, class flares. However, a large Active Region (AR) has just rotated into view on the east limb and produced several B-class flares, this region may lead to increased activity. A second region on the south-east limb showed evidence of a failed eruption at 00:30 UT this morning. AR 2401 (Macintosh:Cro/Type:Beta) has remained stable. No evident Earth directed Coronal Mass Ejections (CMEs) were produced in the past 24 hours. The solar wind speed has been slowly decreasing over the past 24 hours, from 600 to 500 km/s. The total magnetic field has been stable around 5 nT, and the Bz component has fluctuated between +5 nT and -5nT over the past 24 hours. Geomagnetic conditions were quiet to active over the past 24 hours, with the Local K index (Dourbes) reaching 4 and the Kp index (NOAA) reaching 5 around 15:00 UT on 2015-Aug-17, these conditions are probably caused by a high speed stream created by a geoeffective coronal hole. The continued presence of the coronal hole is likely to cause continued unsettled conditions.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 042, sur la base de 12 stations.
| Nombre de Wolf, observé par Catania | /// |
| Flux solaire à 10 cm | 087 |
| AK Chambon La Forêt | 031 |
| AK Wingst | 024 |
| Ap estimé | 027 |
| Nombre international de taches solaires estimé | 028 - Basé sur 18 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 | 18/03/2026 | M2.7 |
| Dernier orage géomagnétique | 14/03/2026 | Kp6 (G2) |
| Jours sans taches solaires | |
|---|---|
| 365 derniers jours | 3 jours |
| 2026 | 3 jours (4%) |
| Dernier jour sans taches solaires | 24/02/2026 |
| Nombre mensuel moyen de taches solaires | |
|---|---|
| février 2026 | 78.2 -34.3 |
| mars 2026 | 80.1 +1.9 |
| 30 derniers jours | 64.9 -40.9 |