Publié: 2017 Nov 26 1233 UTC
Quiet conditions (<50% probability of C-class flares)
Active conditions expected (A>=20 or K=4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 26 Nov 2017 | 075 | 006 |
| 27 Nov 2017 | 075 | 008 |
| 28 Nov 2017 | 075 | 016 |
Over the past 24 hours solar activity has been quiet. No significant flares have been recorded. All Active Regions (AR) have shown low levels of activity. A small filament eruption occurred near disk centre at around 04:00 UT on 2017-Nov-25, Coronagraph imagery suggests the bulk of the ejection headed to the East of the Sun-Earth line and only a glancing blow, if any, can be expected. If so, this is anticipated to arrive at Earth late on 2017-Nov-28. However, projection effects make it difficult to ascertain an accurate speed. The greater than 10MeV proton flux remained at background levels over the past 24 hours. Solar activity is expected to remain low over the next 24 hours with a low probability of C-class flares. The solar wind speed been been decreasing from 400 to 320 km/s over the past 24 hours. The total magnetic field strength has fluctuated between 0 and 5 nT, peaking around 00:00 UT this morning. The Bz component has fluctuated between positive and negative, between -4 and +5 nT. Geomagnetic conditions ranged between Kp index 0-2 (NOAA) and local K index 0-2 (Dourbes) over the past 24 hours. A small transient coronal hole has just passed the central meridian and may enhance solar wind speeds in a couple of days. Geomagnetic conditions are expected to be quiet.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 018, sur la base de 17 stations.
| Nombre de Wolf, observé par Catania | /// |
| Flux solaire à 10 cm | 074 |
| AK Chambon La Forêt | 005 |
| AK Wingst | 006 |
| Ap estimé | 005 |
| Nombre international de taches solaires estimé | 016 - 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 | 30/03/2026 | X1.4 |
| Dernière classe M | 28/03/2026 | M1.3 |
| Dernier orage géomagnétique | 25/03/2026 | Kp5+ (G1) |
| Jours sans taches solaires | |
|---|---|
| 365 derniers jours | 3 jours |
| 2026 | 3 jours (3%) |
| Dernier jour sans taches solaires | 24/02/2026 |
| Nombre mensuel moyen de taches solaires | |
|---|---|
| février 2026 | 78.2 -34.3 |
| mars 2026 | 86.6 +8.4 |
| 30 derniers jours | 86.6 +11.2 |