Publié: 2016 Sep 06 1230 UTC
C-class flares expected, (probability >=50%)
Active conditions expected (A>=20 or K=4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 06 Sep 2016 | 094 | 013 |
| 07 Sep 2016 | 093 | 008 |
| 08 Sep 2016 | 092 | 004 |
NOAA 2585 is decaying and produced the only flare of the period (B3.0 peaking at 21:46UT). The other two sunspot regions (Catania 23 and 24) are small and inactive. The 40-degrees long filament in the northwest quadrant remained quiet. The coronal mass ejection (CME) associated with the prominence eruption early on 06 September (07:30-09:00UT; southwest limb) was not directed to Earth.
C-class flares are possible, with a small chance on an isolated M-class event.
Solar wind speed continued its gradual decline from about 580 km/s to its current value around 520 km/s. Bz fluctuated between -6 and +4 nT, with a sustained negative period near -5 nT from 15-19UT. The interplanetary magnetic field (IMF) was directed away from the Sun (positive). Mostly quiet to unsettled geomagnetic conditions were reported, with an isolated minor storming episode during the 18-21UT interval.
Quiet to active geomagnetic conditions are expected, with still a small chance on a minor storming episode. Geomagnetic conditions are expected to return to mostly quiet levels over the next few days in view of the gradually waning effects of the coronal hole high speed stream.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 043, sur la base de 12 stations.
| Nombre de Wolf, observé par Catania | /// |
| Flux solaire à 10 cm | 094 |
| AK Chambon La Forêt | 031 |
| AK Wingst | 019 |
| Ap estimé | 021 |
| Nombre international de taches solaires estimé | 031 - Basé sur 26 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
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