Publié: 2020 Feb 12 1231 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 12 Feb 2020 | 070 | 008 |
| 13 Feb 2020 | 071 | 010 |
| 14 Feb 2020 | 070 | 008 |
The solar activity has been quiet over the past 24 hours. The visible solar disc is spotless and the X-ray flux is below B-level. The solar activity is expected to remain at low levels over the next 24 hours.
No earth-directed coronal mass ejections (CMEs) have been observed in the available coronagraphic imagery. The greater than 10 MeV proton flux was at nominal values.
The influence of the high-speed stream coming from the positive polarity coronal hole has dropped on February 11 around 19:30 UTC when the phi angle switched to the negative sector. The solar wind parameters remained, however, slightly enhanced. The wind speed first decreased up to 350 km/s to then re-increase up to 420 km/s, the total interplanetary magnetic fields was below 6 nT, and the southward magnetic component fluctuated between -4.5 nT and 5.0 nT. The solar wind conditions are expected to remain slightly enhanced for the next 24-hour period. Solar wind coming from the equatorial coronal hole (negative polarity) that reached the central meridian on February 9, may then contribute to the solar wind enhancement in about 1-2 days.
The geomagnetic conditions were quiet with few short periods of unsettle condition observed in Dourbes station (K-Dourbes = 3). We expect the geomagnetic conditions to remain mostly quiet with some short sporadic periods of unsettled condition for the next days.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 000, sur la base de 22 stations.
| Nombre de Wolf, observé par Catania | 000 |
| Flux solaire à 10 cm | 071 |
| AK Chambon La Forêt | 008 |
| AK Wingst | 007 |
| Ap estimé | 006 |
| Nombre international de taches solaires estimé | 000 - Basé sur 24 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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