Välja antud: 2017 Oct 08 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
| 10 cm vool | Ap | |
|---|---|---|
| 08 Oct 2017 | 077 | 003 |
| 09 Oct 2017 | 075 | 003 |
| 10 Oct 2017 | 074 | 006 |
Solar activity was at very low levels. NOAA 2683 (Catania 57) had rotated over the west limb by the end of the period. It was the source of a B5 flare peaking on 08 October at 06:47UT. A small bipolar sunspot region emerged near N15W35. No earth-directed coronal mass ejections (CMEs) were observed in available coronagraphic imagery. The greater than 10 MeV proton flux was at nominal levels.
Quiet flaring conditions are expected, with still a slight chance on an isolated C-class flare.
Solar wind speed varied between 400 and 460 km/s (DSCOVR). Bz fluctuated between -5 and +6 nT, being mostly positive after 04UT. 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, with unsettled levels reached in Dourbes at the end of the period. Mostly quiet geomagnetic conditions are expected, with a chance on an isolated unsettled interval.
Tänane hinnanguline rahvusvaheline päikeselaikude arv (ISN): 000, põhineb 14 jaamadel.
| Catania Wolfi number | /// |
| 10cm päikesevoog | 080 |
| AK Chambon La Forêt | 009 |
| AK Wingst | 004 |
| Hinnanguline Ap | 003 |
| Hinnanguline rahvusvaheline päikeselaikude arv | 013 - Põhineb 18 jaamal |
| Päev | Algus | Maks | Lõpp | Lokatsioon | Tugevus | OP | 10cm | Catania/NOAA | Raadiosignaalipursete tüübid | |
|---|---|---|---|---|---|---|---|---|---|---|
| Puuduvad | ||||||||||
Andmed on esitanud Päikeseinfektide Andmeanalüüsi Keskus (Solar Influences Data Analysis Center)© - SIDC - Töötleb SpaceWeatherLive
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