Publié: 2020 Nov 21 1234 UTC
C-class flares expected, (probability >=50%)
Active conditions expected (A>=20 or K=4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 21 Nov 2020 | 083 | 006 |
| 22 Nov 2020 | 087 | 022 |
| 23 Nov 2020 | 089 | 019 |
Solar activity was at low levels with two C-class flares registered in the past 24 hours. A C1 flare (peak at 18:44 UTC) was produced from an active region behind the east limb and a C1.9 flare with peak time at 17:03UTC on Nov 20th was produced by active region NOAA 2783 (Hsx/alpha). A new unnamed and unclassified active region has formed in the north-east quadrant, approximately at N32E35. The solar activity is expected to remain at low levels with a 50% chance for C-class flares and a slight chance for an M class flare. No Earth-directed coronal mass ejections (CMEs) were detected in the available coronagraph imagery.
The greater than 10 MeV proton flux was at nominal levels in the past 24 hours and is expected to remain so in the next 24 hours. The greater than 2 MeV electron flux remained under the 1000 pfu threshold. The 24h electron fluence was at nominal levels. Enhancements of the > 2MeV electron flux and fluence are foreseen within the next 24 hours related to the expected arrival of a high speed stream originating from coronal hole CH 96.
Over the past 24 hours the solar wind speed was relatively stable with maximal velocity remaining below 390 km/s (ACE and DSCOVR). The total magnetic field reached a maximal strength of 7 nT with Bz component varying between -6 nT and 6 nT. The phi angle showed long periods in the positive sectors and is currently fluctuating between the positive and negative sectors.
Geomagnetic activity was globally quiet with a single locally unsettled period when K Dourbes registered 3. Quiet to active geomagnetic conditions are expected for the next 24 hours due to the foreseen arrival of a high speed stream (HSS) originating from coronal hole CH 96 by the morning of Nov. 22nd. With the arrival of the HSS there are slight chances for a minor geomagnetic storm.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 021, sur la base de 14 stations.
| Nombre de Wolf, observé par Catania | 011 |
| Flux solaire à 10 cm | 082 |
| AK Chambon La Forêt | 009 |
| AK Wingst | 008 |
| Ap estimé | 007 |
| Nombre international de taches solaires estimé | 010 - 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 | 25/02/2026 | M2.4 |
| Dernier orage géomagnétique | 03/03/2026 | Kp5 (G1) |
| 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 | 75.1 -3.1 |
| 30 derniers jours | 54.5 -72.1 |