Publié: 2018 Jan 24 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 24 Jan 2018 | 070 | 003 |
| 25 Jan 2018 | 069 | 003 |
| 26 Jan 2018 | 069 | 005 |
Solar activity was at very low levels. The Sun is spotless. No earth-directed coronal mass ejections (CMEs) were observed in available coronagraphic imagery. The greater than 10 MeV proton flux was at nominal levels.
Solar activity is expected to remain at very low levels.
Solar wind speed decreased from an initial 470 km/s to current values near 350 km/s (DSCOVR). Bz varied between -3 and +3 nT. The interplanetary magnetic field was directed towards the Sun until about 02UT, after which is was mainly directed away from the Sun. A diffuse extension of the northern polar coronal hole (CH) is transiting the central meridian.
The geomagnetic field was mostly at quiet levels and is expected to remain so, with a chance on an unsettled episode.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 000, sur la base de 07 stations.
| Nombre de Wolf, observé par Catania | 000 |
| Flux solaire à 10 cm | 071 |
| AK Chambon La Forêt | 005 |
| AK Wingst | 004 |
| Ap estimé | 004 |
| Nombre international de taches solaires estimé | 000 - Basé sur 22 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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