Publié: 2016 Nov 20 1232 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 20 Nov 2016 | 077 | 011 |
| 21 Nov 2016 | 077 | 013 |
| 22 Nov 2016 | 077 | 007 |
Solar activity was very low with X-ray flux remaining below C level and just a single B1.1 flare observed from NOAA region 2611. NOAA region 2610 has decayed and also region 2611 is continuing to decay. There is only a very minor chance for C-flares. Proton flux values are at background levels and expected to remain so. No Earth directed CMEs have been observed in coronagraph data. A positive polarity equatorial coronal hole is starting to cross the central meridian and can be expected to become geoeffective starting late November 23, early November 24.
Solar wind speed has remained low around 320 km/s for most of the period and only started its expected increase around the end of the period to around 350-370 km/s. Total magnetic field fluctuated between 1 and 5.5nT and increased to around 7 nT at the end of the period. Bz was variable. The magnetic field phi angle shifted into the positive sector during the second half of the period. Solar wind speed is expected to further increase under influence of a positive polarity coronal hole.
Geomagnetic conditions were quiet (both local K Dourbes and NOAA Kp 0-1) and are expected to become quiet to unsettled as solar wind speed increases.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 007, sur la base de 11 stations.
| Nombre de Wolf, observé par Catania | /// |
| Flux solaire à 10 cm | 077 |
| AK Chambon La Forêt | 005 |
| AK Wingst | 002 |
| Ap estimé | 002 |
| Nombre international de taches solaires estimé | 015 - Basé sur 22 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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