Publié: 2017 Feb 17 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Active conditions expected (A>=20 or K=4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 17 Feb 2017 | 074 | 017 |
| 18 Feb 2017 | 074 | 021 |
| 19 Feb 2017 | 074 | 022 |
In the past 24 hours, no C flares were observed. Very low solar activity (no C flares) is expected in the next 24 hours. The solar wind near Earth is under the influence of a high speed stream by a positive coronal hole. In the past 24 hours, solar wind speed measured by DSCOVR rose from about 375 km/s to about 500 km/s, as the solar wind from the broader part of the coronal hole arrived at Earth. The magnitude of the Interplanetary Magnetic Field (IMF) varied between about 2 and 13 nT, with current values around 6 nT. There were a few short intervals with negative Bz, down to -9 nT. Quiet to active geomagnetic conditions (K Dourbes between 2 and 4; NOAA Kp between 2 and 4) were registered in the past 24 hours. Due to the influence of the high speed stream, quiet to active geomagnetic levels (K Dourbes < 5) are expected on February 17, 18 and 19, with possible minor storm episodes (K Dourbes = 5).
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 012, sur la base de 15 stations.
| Nombre de Wolf, observé par Catania | 025 |
| Flux solaire à 10 cm | 074 |
| AK Chambon La Forêt | 019 |
| AK Wingst | 008 |
| Ap estimé | 008 |
| Nombre international de taches solaires estimé | 012 - Basé sur 35 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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