Publié: 2017 Aug 07 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Active conditions expected (A>=20 or K=4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 07 Aug 2017 | 074 | 007 |
| 08 Aug 2017 | 075 | 013 |
| 09 Aug 2017 | 076 | 006 |
Over the past 24 hours solar activity has been very low. No significant flares have been recorded. Active Region (AR) 12670 (Mcintosh class:Hsx; Mag. type:Alpha) has been most active, producing a few B-class flares. However, AR 12670 has shown some evidence of flux emergence and cancellation in HMI magnetogram observations, which may result in flaring activity. No Earth directed Coronal Mass Ejections (CMEs) have been detected. 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 has decreased from around 650 to 500 km/s over the past 24 hours. The total magnetic field strength has remained around 5 nT. The Bz component fluctuated around 0 nT, ranging between -4 and +3 nT. Geomagnetic conditions ranged between Kp index 1-4 (NOAA) and local K index 0-4 (Dourbes) over the past 24 hours. There is currently a small positive polarity Northern polar coronal hole extending to lower latitudes located in the Western hemisphere and the resulting high-speed stream (HSS) may enhance solar wind speeds for a short period over the coming days. Geomagnetic conditions are expected to be quiet, with the possibility of a small enhancement later today or early tomorrow.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 011, sur la base de 17 stations.
| Nombre de Wolf, observé par Catania | /// |
| Flux solaire à 10 cm | 074 |
| AK Chambon La Forêt | 022 |
| AK Wingst | 015 |
| Ap estimé | 016 |
| Nombre international de taches solaires estimé | 012 - Basé sur 30 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 | 62.9 -47.9 |