Publié: 2019 Sep 20 1245 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 20 Sep 2019 | 067 | 006 |
| 21 Sep 2019 | 067 | 007 |
| 22 Sep 2019 | 067 | 007 |
Solar X ray flux remained below B level throughout the period. The Solar disk is spotless and X-ray flux is expected to remain at or below background levels.
A filament in the Southern hemisphere stretching from the central meridian towards the Eastern limb is seen to erupt in SDO/AIA 304 imagery from around 21:00UT. Corresponding STEREO/COR2 coronagraph data indicate a corresponding narrow CME may be Earth directed. SoHO/LASCO data do not show any clear signs of any (partial) halo CME but they are being analysed further in order to assess the possibility of an Earth directed component. There were otherwise no Earth-directed CMEs observed in coronagraph data.
An equatorial negative polarity coronal hole is about to cross the central meridian.
Proton levels were at background values and are expected to remain so.
Solar wind was nominal. Solar wind speed decreased from 380 km/s to 320 km/s. Total magnetic field was around 4nT. The magnetic field phi angle was mostly in the positive sector. Solar wind conditions are expected to remain nominal over the next 48 hours. Afterwards the influence of the negative polarity equatorial coronal hole is expected to increase solar wind conditions.
Geomagnetic conditions were quiet to unsettled (NOAA Kp 1-2 and local K Dourbes 0-3). Quiet geomagnetic conditions are expected the next 48 hours.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 000, sur la base de 21 stations.
| Nombre de Wolf, observé par Catania | 000 |
| Flux solaire à 10 cm | 067 |
| AK Chambon La Forêt | 008 |
| AK Wingst | 004 |
| Ap estimé | 005 |
| Nombre international de taches solaires estimé | 000 - 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
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