Publié: 2018 Dec 03 1231 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 03 Dec 2018 | 069 | 006 |
| 04 Dec 2018 | 069 | 005 |
| 05 Dec 2018 | 070 | 006 |
The solar activity has been quiet over the past 24 hours. The visible solar disc is spotless, and no significant flare has been recorded. Quiet flaring conditions are expected for the next 24-hour period.
No Earth directed Coronal Mass Ejection has been observed over the past 24 hours. The greater than 10 MeV solar protons flux remained at nominal levels over the past 24 hours and is expected to remain so.
The solar wind measurements remained under the influence of the enhanced solar wind associated with the Coronal Hole (which reached the central meridian on November 27). The wind speed ranged between 411 and 472 km/s; The interplanetary magnetic field strength fluctuated between 1.4 and 7.5 nT and the southward magnetic component between -5.8 and 6.2 nT. The solar wind conditions are expected to remain the same for the next 24 hours and start to slowly decrease afterwards.
The geomagnetic conditions were quiet to unsettled and are expected to remain the same as Earth remains under the influence of the enhanced solar wind conditions associated to the Coronal Hole.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 000, sur la base de 14 stations.
| Nombre de Wolf, observé par Catania | /// |
| Flux solaire à 10 cm | 069 |
| AK Chambon La Forêt | 024 |
| AK Wingst | /// |
| Ap estimé | 016 |
| Nombre international de taches solaires estimé | 000 - Basé sur 16 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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