Publié: 2018 Jul 29 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 29 Jul 2018 | 068 | 006 |
| 30 Jul 2018 | 068 | 007 |
| 31 Jul 2018 | 068 | 007 |
The Sun is spotless and produced only a few A flares in the past 24 hours, from a new region near the East limb. The chance for a C flare in the next 24 hours is estimated at 5%.
No Earth-directed Coronal Mass Ejections (CMEs) were observed in available coronagraphic imagery.
The greater than 10 MeV proton flux was at nominal levels in the past 24 hours, and is expected to stay at nominal levels in the next 24 hours.
Solar wind speed as registered by DSCOVR further decreased from about 370 to 315 km/s. The Interplanetary Magnetic Field (IMF) was oriented towards the Sun and its magnitude varied between about 3 and 5 nT. Bz was never below -5 nT. The solar wind is expected to stay at nominal levels in the next days.
Quiet to unsettled geomagnetic conditions (K Dourbes between 1 and 3; NOAA Kp between 1 and 2) were registered in the past 24 hours. Quiet to unsettled conditions (K Dourbes < 4) are expected on July 29, 30 and 31.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 000, sur la base de 20 stations.
| Nombre de Wolf, observé par Catania | /// |
| Flux solaire à 10 cm | 068 |
| AK Chambon La Forêt | /// |
| AK Wingst | 006 |
| Ap estimé | 006 |
| Nombre international de taches solaires estimé | 000 - Basé sur 36 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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