Publié: 2021 Jun 17 1231 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 17 Jun 2021 | 076 | 007 |
| 18 Jun 2021 | 075 | 005 |
| 19 Jun 2021 | 075 | 004 |
Solar activity remained at very low levels in the last 24 hours. NOAA AR2833 (Catania sunspot group 7) remained with simple unipolar magnetic filed configuration and is the only active region one the visible solar disc. The X-ray flare activity is expected to remain at very low levels for the next 24 hours.
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 2MeV electron flux crossed the 1000 pfu threshold at 08:20 UTC this morning and is expected to remain above the threshold for an extended period of time. The 24h electron fluence increased from nominal to moderate level and is expected to remain at moderate levels for the next 24 hours.
Over the past 24h the solar wind (ACE and DSCOVR) remained under the influence of a high speed stream (HSS). The solar wind speed varied between 535 km/s and 633 km/s. The total magnetic field was at low values, in the range of 1.5 nT to 5.6 nT. The Bz component mildly fluctuated between -4.4 nT and 3.3 nT. The solar temperature remained elevated and the orientation of the interplanetary magnetic field remained predominantly in the negative sector.
The geomagnetic conditions over the past 24 hours were quiet to unsettled. Quiet to unsettled geomagnetic conditions are expected for the next 24 hours. Isolated active periods remain possible until the effects of the HSS fade away.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 012, sur la base de 25 stations.
| Nombre de Wolf, observé par Catania | 011 |
| Flux solaire à 10 cm | 076 |
| AK Chambon La Forêt | 019 |
| AK Wingst | 017 |
| Ap estimé | 018 |
| Nombre international de taches solaires estimé | 011 - Basé sur 29 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 | 30/03/2026 | X1.5 |
| Dernière classe M | 09/04/2026 | M1.0 |
| Dernier orage géomagnétique | 03/04/2026 | Kp7- (G3) |
| Jours sans taches solaires | |
|---|---|
| 365 derniers jours | 3 jours |
| 2026 | 3 jours (3%) |
| Dernier jour sans taches solaires | 24/02/2026 |
| Nombre mensuel moyen de taches solaires | |
|---|---|
| mars 2026 | 85.9 +7.7 |
| avril 2026 | 101.7 +15.8 |
| 30 derniers jours | 97.2 +38.9 |