Publié: 2019 Jan 12 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 12 Jan 2019 | 068 | 005 |
| 13 Jan 2019 | 068 | 019 |
| 14 Jan 2019 | 068 | 007 |
The solar activity has been quiet over the past 24 hours. The X-ray flux remains below B-level, and the visible solar disc is spotless. Solar activity is expected to remain at low levels.
No Earth directed Coronal Mass Ejection has been observed. The greater than 10 MeV solar protons flux remained at nominal levels over the past 24 hours and is expected to remain so.
The influence of the coronal hole that transited the central meridian on Jan 8 is weakening. The solar wind speed decreased from around 470 km/s to the current values around 380 km/s. Total interplanetary magnetic field strength was below 6.8 nT. The southward magnetic component remained between -4.1 and 4.1 nT. The influence of the equatorial coronal hole that has reached the central meridian on Jan 9 is expected to re-enhance the solar wind parameters on Jan 13.
The geomagnetic conditions were quiet and are expected to remain quiet until the arrival of the coronal hole influences on the solar wind measurements near Earth on Jan 13. Possible isolated minor storm conditions may be observed, in particular, if the Bz component stays negative for longer periods.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 000, sur la base de 03 stations.
| Nombre de Wolf, observé par Catania | /// |
| Flux solaire à 10 cm | 068 |
| AK Chambon La Forêt | 006 |
| AK Wingst | 007 |
| Ap estimé | 005 |
| Nombre international de taches solaires estimé | 000 - Basé sur 15 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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