Publié: 2021 Nov 05 1231 UTC
C-class flares expected, (probability >=50%)
Active conditions expected (A>=20 or K=4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 05 Nov 2021 | 093 | 026 |
| 06 Nov 2021 | 091 | 026 |
| 07 Nov 2021 | 091 | 007 |
Only two C flares occurred during the period, the largest of which peaked at a C2.9 magnitude at 14:53UT, from the new region in the South East that is now numbered NOAA 2894. That new region awaits to be analysed in more detail. Meanwhile the unipolar region 2893 remained overall stable with some additional smaller spots emerging, while region 2891 remains the most complex on disc though showing signs of decay. C flares are quite likely, with a very small chance for an M flare.
No new Earth directed CMEs have been recorded in coronagraph data.
The more than 10MeV proton flux has returned almost to background conditions as is expected to remain at background conditions. The greater than 2 MeV electron flux was below the 1000 pfu threshold. The 24h electron fluence is at normal levels and is expected to increase from normal to moderate or even high levels over the next days in the wake of the enhanced Solar wind conditions.
Solar wind conditions were enhanced due to the CME passage that started late November 3. Solar wind speed followed a decaying trend to now under 600 km/s. The magnitude of the interplanetary magnetic field also followed a decaying trend to now under 10nT while the Bz component was positive throughout the period. Solar wind conditions are expected to remain enhanced over the next days as CME effects wane.
Geomagnetic conditions were initially at minor to moderate storm levels (NOAA Kp 6 and local K Dourbes 5) but as Bz remained positive during the period, only quiet to active conditions were recorded during the remainder of the period. Quiet to active conditions are expected in the next 24-48 hours with an overall decreasing trend, and initially still minor storm levels are possible depending on the Solar wind magnetic field orientation.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 035, sur la base de 21 stations.
| Nombre de Wolf, observé par Catania | /// |
| Flux solaire à 10 cm | 094 |
| AK Chambon La Forêt | 045 |
| AK Wingst | 043 |
| Ap estimé | 051 |
| Nombre international de taches solaires estimé | 026 - Basé sur 25 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 |