Publié: 2016 Jan 18 1231 UTC
Quiet conditions (<50% probability of C-class flares)
Active conditions expected (A>=20 or K=4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 18 Jan 2016 | 098 | 002 |
| 19 Jan 2016 | 096 | 013 |
| 20 Jan 2016 | 094 | 003 |
Solar x-ray flux flatlined near the B2-level, with no flares observed during the last 24 hours. The currently visible sunspot groups are small with little signs of growth. A small filament eruption took place near the Central Meridian (CM) on 17 January, starting around 20:30UT. Some coronal dimming was observed, but currently available coronagraphic imagery from SOHO and STEREO-A do not show an associated earth-directed coronal mass ejection (CME).
Mostly quiet flaring conditions are expected, with only a small chance on an isolated C-class flare. Solar wind speed showed an overall declining trend and varied between 350 and 300 km/s. Bz varied slowly between -5 and +4 nT, and the Interplanetary Magnetic Field was directed mostly away from the Sun. Quiet geomagnetic conditions were observed. A southern polar coronal hole (CH) extension is transiting the CM.
Quiet geomagnetic conditions are expected, with active episodes possible as a result of the faint and slow 14 January CME which is expected to arrive on 19 January.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 045, sur la base de 12 stations.
| Nombre de Wolf, observé par Catania | /// |
| Flux solaire à 10 cm | 101 |
| AK Chambon La Forêt | 007 |
| AK Wingst | 003 |
| Ap estimé | 002 |
| Nombre international de taches solaires estimé | 058 - 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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