Publié: 2016 Oct 15 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Active conditions expected (A>=20 or K=4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 15 Oct 2016 | 094 | 015 |
| 16 Oct 2016 | 094 | 017 |
| 17 Oct 2016 | 094 | 012 |
Only a single C flare was observed from the new unnumbered region rotating on the disk in the South East. This C1 flare peaked at 14:49UT. The other regions on disk were mostly inactive and background X-ray flux declined to the B2 level over the period. Apart from an isolated C flare, which remains possible especially from the new region, solar activity is expected to be quiet. Solar proton flux levels were at background values and expected to remain so. Associated to the C1 flare, an Eastbound CME was observed in coronagraph images. It is not expected to influence Earth. No other Earth directed CMEs were observed in coronagraph images.
Solar wind conditions showed a further trend towards nominal conditions, but remain enhanced with solar wind speed actually increasing again to around 500 km/s. The magnetic field magnitude declined from around 16nT at the start of the period to around 8nT presently. The North South component was variable but mostly positive, while the magnetic field phi angle switched into the negative sector around 15:45UT and mostly remained there. Solar wind conditions are expected to remain enhanced and increase further in the next 24-48 hours under the influence of a negative polarity coronal hole high speed stream. Geomagnetic conditions were quiet to unsettled (both NOAA Kp and local K Dourbes 1-3). Geomagnetic conditions are expected to first remain quiet to unsettled and later increase to possibly active to minor storm conditions under the influence of the expected recurrent high speed stream.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 036, sur la base de 07 stations.
| Nombre de Wolf, observé par Catania | /// |
| Flux solaire à 10 cm | 093 |
| AK Chambon La Forêt | 019 |
| AK Wingst | 025 |
| Ap estimé | 027 |
| Nombre international de taches solaires estimé | 045 - 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 | X4.3 |
| Dernière classe M | 12/02/2026 | M1.4 |
| Dernier orage géomagnétique | 05/02/2026 | Kp5+ (G1) |
| 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 | 125.3 +12.7 |
| 30 derniers jours | 130.4 +32.7 |