Publié: 2017 Feb 27 1250 UTC
Quiet conditions (<50% probability of C-class flares)
Active conditions expected (A>=20 or K=4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 27 Feb 2017 | 078 | 007 |
| 28 Feb 2017 | 077 | 010 |
| 01 Mar 2017 | 076 | 016 |
Solar activity was very low with no C class flares. NOAA active regions (ARs) 2638, 2639 and 2640 were stable. X-ray flux is expected to remain at background level. No Earth directed CMEs have been recorded in coronagraph data. The transequatorial extension of the negative polarity southern polar coronal hole is expected to become geoeffective around midnight 28-Feb-2017/01-March-2017. Proton flux values are expected to remain at background levels. Solar wind speed declined from around 450 km/s to around 350 km/s. Total magnetic field was in the 3:6nT range. Bz was in the -3:4nT range. Solar wind is expected to be at nominal levels over the next 24 hours before an anticipated increase late 28-Feb-2017 due to high speed stream from the negative polarity coronal hole. Geomagnetic conditions have been quiet (local K Dourbes 0-2, NOAA Kp 1-2). Over the next days, geomagnetic conditions are expected to be quiet to unsettled and increasing to quiet to active by late 28-Feb 2017 with the anticipated high speed stream.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 041, sur la base de 18 stations.
| Nombre de Wolf, observé par Catania | /// |
| Flux solaire à 10 cm | 079 |
| AK Chambon La Forêt | 006 |
| AK Wingst | 002 |
| Ap estimé | 001 |
| Nombre international de taches solaires estimé | 032 - Basé sur 19 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
Toutes les heures sont indiquées en UTC
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