Publié: 2018 Oct 02 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 02 Oct 2018 | 070 | 007 |
| 03 Oct 2018 | 069 | 010 |
| 04 Oct 2018 | 068 | 010 |
One active region visible on the solar disc, NOAA 2723 with beta magnetic field configuration. No C-class flares in past 24 h. Solar activity is expected to remain at low levels.
No Earth directed Coronal Mass Ejections (CMEs) have been detected. Solar protons have remained at background levels over the past 24 hours.
The solar wind speed is at 480 km/s with interplanetary magnetic fields of 5 nT. Geomagnetic conditions reached active levels between 15:00 UT and 17:00 UT on October 1 at Dourbes (K=4), at planetary levels Kp reached 4 between 12:00 UT and 15:00 UT on October 1 and between 00:00 UT and 03:00 UT on October 2. This was due to solar wind of relatively high speed (reaching 530 km/s) with interplanetary magnetic fields up to 10 nT with oscillating periods including negative Bz. Quiet to unsettled conditions for the coming hours are foreseen. The fast solar wind associated with a small negative polarity equatorial coronal hole is expected to arrive on October 4 (or late on October 3), causing up to active geomagnetic conditions.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 014, sur la base de 14 stations.
| Nombre de Wolf, observé par Catania | 017 |
| Flux solaire à 10 cm | 070 |
| AK Chambon La Forêt | 021 |
| AK Wingst | 012 |
| Ap estimé | 011 |
| Nombre international de taches solaires estimé | 017 - Basé sur 25 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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