Publié: 2013 Nov 09 1411 UTC
Active (M-class flares expected, probability >=50%)
Active conditions expected (A>=20 or K=4)
Warning condition (activity levels expected to increase, but no numeric forecast given)
| Flux de 10 cm | Ap | |
|---|---|---|
| 09 Nov 2013 | 144 | 022 |
| 10 Nov 2013 | 144 | 005 |
| 11 Nov 2013 | 146 | 004 |
Only three weak C-class flares were reported since the previous bulletin. However, Catania sunspot group 35 (NOAA AR 1890) keeps the beta-gamma-delta configuration of its photospheric magnetic field. We therefore expect the flaring activity to continue on the M-level, with an X-class flare being possible but unlikely. Due to the position of the Catania sunspot group 35 (NOAA AR 1890) right to the west of the solar central meridian, a warning condition for a proton event is maintained. Currently the proton flux at energies above 10 MeV is slowly growing, but this growth is most probably due to earlier eastern hemisphere events and is not expected to lead to a proton event. Since late November 8, the Earth is inside a region of elevated interplanetary magnetic field (IMF) magnitude (up to 17 nT), probably representing an ICME. The corresponding solar CME is not clear at the moment. The solar wind speed remained low (around 400-450 km/s), so only active (K = 4, Dourbes, IZMIRAN, NOAA) to minor storm (K = 5, IZMIRAN) geomagnetic conditions were reported. Currently the solar wind speed reaches 530 km/s, and the IMF magnitude is still increased (around 10 nT), so active geomagnetic conditions are still possible.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 077, sur la base de 15 stations.
| Nombre de Wolf, observé par Catania | 172 |
| Flux solaire à 10 cm | 146 |
| AK Chambon La Forêt | 015 |
| AK Wingst | 005 |
| Ap estimé | 005 |
| Nombre international de taches solaires estimé | 100 - Basé sur 20 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 | 01/02/2026 | X1.0 |
| Dernière classe M | 01/02/2026 | M5.2 |
| Dernier orage géomagnétique | 28/01/2026 | Kp5+ (G1) |
| Jours sans taches solaires | |
|---|---|
| Dernier jour sans taches solaires | 08/06/2022 |
| Nombre mensuel moyen de taches solaires | |
|---|---|
| décembre 2025 | 124 +32.2 |
| 30 derniers jours | 119.2 +2.7 |