Publié: 2013 Aug 21 1240 UTC
Eruptive (C-class flares expected, probability >=50%)
Active conditions expected (A>=20 or K=4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 21 Aug 2013 | 135 | 018 |
| 22 Aug 2013 | 138 | 008 |
| 23 Aug 2013 | 138 | 003 |
Solar activity was eruptive with a C2.2 flare as strongest flare originating from NOAA AR 1828. A faint partial halo CME was observed in LASCO/C2 around 5h00 UT which was confirmed by STEREO A and B data. It seems to be associated to a small filament eruption located near S15E15, observed in PROBA2/SWAP and GONG H-alpha data. The CME seems to be travelling mainly to the east with a projected speed of 360 km/s. First analysis suggests a possible arrival at 25 August at 9h UT, but this will be further evaluated. We expect C-class flaring activity to continue. There is a slight chance for M-class flares, especially from NOAA active regions 1820 and 1827 that currently have a beta-gamma configuration of their photospheric magnetic field. ACE has observed a jump yesterday at 22h UT in all the plasma parameters jump, but not the magnetic field. This seems to be the arrival of the equatorial CH fast speed stream. Local K-index at Dourbes currently is at K=3 and Kp went up to Kp=4, due to combined effects of the fast speed stream and some influence of a flank of the CME of August 17, that possibly arrived at 2h this morning. Unsettled geomagnetic conditions are expected to continue and return to quiet after 24 hours.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 095, sur la base de 13 stations.
| Nombre de Wolf, observé par Catania | /// |
| Flux solaire à 10 cm | 132 |
| AK Chambon La Forêt | 012 |
| AK Wingst | 004 |
| Ap estimé | 004 |
| Nombre international de taches solaires estimé | 086 - Basé sur 21 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 | 21/03/2026 | Kp7 (G3) |
| 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 | 76.1 -2.1 |
| 30 derniers jours | 65.3 -33.8 |