Publié: 2017 Sep 06 1254 UTC
M-class flares expected (probability >=50%)
Major (ISES: Severe) magstorm expected (A>=100 or K>=7)
Proton event in progress (>10 MeV)
| Flux de 10 cm | Ap | |
|---|---|---|
| 06 Sep 2017 | 150 | 073 |
| 07 Sep 2017 | 150 | 093 |
| 08 Sep 2017 | 150 | 017 |
After yesterdays multiple M flares from Catania group 46 (NOAA active region 2673) this region first seemed to become less activite but this was just the prelude to the X2.2 flare that it generated this morning peaking at 9:10UT. While writing this report another X9.3 flare from this region appeared to be ongoing (peak time 12:02UT) with associated radio bursts of large magnitude recorded in multiple wavelengths. Given the persistent complexity of the region and the magnitude of the ongoing flaring observed, we expect further flaring at M level from this region with a very significant chance for further X flares. Several radio bursts were observed in relation to the X2.2 flare. Currently available coronagraph data show some ejecta towards the South West following the X2.2 flare, but the angular extent appears to be limited. No other Earth directed CMEs are visible in coronagraph data. The >10 MeV proton flux values reached a peak of near 200pfu around 19:30UT before declining again to currently around 25pfu. No increase was recorded following the X2.2 flare. But renewed increases should be anticipated in relation with the ongoing activity.
Solar wind was recovering over the past 24 hours towards nominal conditions with no sign yet of the arrival of the September 4 CME. Solar wind speed decreased to under 475 km/s and total magnetic field was nominally below 5nT. This afternoon we should see increased solar wind conditions with the arrival of the September 4 CME which may increase solar wind speed to over 800 km/s. Geomagnetic conditions were quiet to unsettled (local K Dourbes 1-3, NOAA Kp 2-3). Associated with the arrival of the September 4 CME, geomagnetic storms are expected to set in over the next 24 hours and persist into the next 48 hours. Storm levels may reach major or possibly severe levels.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 113, sur la base de 17 stations.
| Nombre de Wolf, observé par Catania | 148 |
| Flux solaire à 10 cm | 121 |
| AK Chambon La Forêt | 014 |
| AK Wingst | 015 |
| Ap estimé | 015 |
| Nombre international de taches solaires estimé | 133 - Basé sur 20 stations |
| Jour | Commencer | Max | Fin | Loc | Force | OP | 10cm | Catania/NOAA | Types de sursaut radio |
|---|---|---|---|---|---|---|---|---|---|
| 05 | 1737 | 1743 | 1751 | S09W24 | M2.3 | 1N | 46/2673 | ||
| 06 | 0857 | 0910 | 0917 | S07W33 | X2.2 | SF | 410 | 46/2673 | VI/1 |
| 06 | 1153 | 1202 | 1210 | ---- | X9.3 | 12000 | --/---- | III/2II/2 |
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 | 16/02/2026 | M2.4 |
| Dernier orage géomagnétique | 16/02/2026 | Kp6 (G2) |
| 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 | 103.9 -8.7 |
| 30 derniers jours | 120.3 +12.4 |