Publié: 2017 Oct 29 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 29 Oct 2017 | 075 | 005 |
| 30 Oct 2017 | 074 | 007 |
| 31 Oct 2017 | 073 | 007 |
Quiet solar conditions were reported with the X-ray flux touching only briefly into the B level. Both active regions on disk are relatively simple (Mag.Type: Alpha) and quiet. The X-ray flux is expected to remain below C level. Proton flux levels were at background values and are expected to remain so. No Earth directed CME's were recorded in coronagraph data. A negative polarity low latitude coronal hole is starting its transit of the central meridian on the Southern hemisphere. It may influence Solar wind conditions starting 3 days from now.
Solar wind conditions were nominal with Solar wind speed decreasing to below 350 km/s while total magnetic field was mostly in a nominal 2-4nT range with the Bz component variable. The phi angle indicated connection to a positive sector. Nominal Solar wind conditions are expected over the next days. By noon November 1 the high speed stream from the southern, low latitude coronal hole and the sector boundary change preceding it could potentially enhance Solar wind conditions. Geomagnetic conditions were quiet (local K Dourbes 1, NOAA Kp 1-2) and are expected to remain so over the next days.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 024, sur la base de 15 stations.
| Nombre de Wolf, observé par Catania | /// |
| Flux solaire à 10 cm | 075 |
| AK Chambon La Forêt | 010 |
| AK Wingst | 006 |
| Ap estimé | 005 |
| Nombre international de taches solaires estimé | 025 - Basé sur 20 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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