Publié: 2017 Oct 07 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 07 Oct 2017 | 081 | 005 |
| 08 Oct 2017 | 078 | 003 |
| 09 Oct 2017 | 075 | 003 |
Solar activity was at very low levels. NOAA 2683 (Catania 57) produced all of the low-level B-class flaring during the period, a B9.8 flare peaking on 06 October at 16:34UT being the strongest. It was also the source of a Long Duration B4.6 flare peaking at 00:28UT. Eruptive activity to the north and northwest of NOAA 2682 (Catania 56; now beyond the Sun's west limb) resulted in 2 coronal mass ejections (CMEs) observed by SOHO/LASCO C2 at resp. 09:12UT and 12:36UT on 06 October. None of the observed CMEs had an earth-directed component. The greater than 10 MeV proton flux was at nominal levels.
Quiet flaring conditions are expected, with a small chance on an isolated C-class flare.
Solar wind was enhanced, probably influenced by the weak particle stream from the small negative equatorial coronal hole (CH). Solar wind speed reached a maximum speed around 470 km/s (DSCOVR) at the beginning of the period, gradually declining to its current values near 410 km/s. Bz oscillated between -5 and +6 nT. The interplanetary magnetic field was mostly directed towards the Sun. The extension of a positive polar CH started its transit of the Central Meridian early on 07 October and may influence the earth environment around 10-11 October.
The geomagnetic field was at quiet levels. Quiet to unsettled conditions are expected, with a small chance on an isolated active interval.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 012, sur la base de 12 stations.
| Nombre de Wolf, observé par Catania | 026 |
| Flux solaire à 10 cm | 084 |
| AK Chambon La Forêt | 012 |
| AK Wingst | 010 |
| Ap estimé | 009 |
| Nombre international de taches solaires estimé | 025 - Basé sur 33 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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