Välja antud: 2015 Feb 06 1231 UTC
Eruptive (C-class flares expected, probability >=50%)
Quiet (A<20 and K<4)
Quiet
| 10 cm vool | Ap | |
|---|---|---|
| 06 Feb 2015 | 142 | 006 |
| 07 Feb 2015 | 142 | 007 |
| 08 Feb 2015 | 146 | 007 |
Solar activity was low, with only a couple of isolated low level C flares. The strongest one originated from NOAA region 2280 (Catania 82) peaking at 10:17 UT at C1.4 level only. A new spotted region started to appear near S10W45. We expect some further C flaring, mainly from NOAA regions 2277 and 2280. Incomplete SOHO LASCO coronagraph data so far seem to indicate that the filament eruptions of February 4 did not result in Earth directed CMEs. Solar wind conditions showed a sector boundary crossing with the magnetic field phi angle completing the shift which was started in the previous reporting period and settling on a firmly positive value during the present reporting period. Associated with this shift the total magnetic field increased from levels around 3.5 nT to values in the 6-8 nT range. Bz was variable with negative peaks down to -6.4 nT. Solar wind speed remained in the 400 to 450 km/s range. Geomagnetic conditions were quiet to active (both NOAA Kp and local K Dourbes 1-4), with the active period associated to the sector boundary crossing. Similar solar wind conditions are expected to persist, with associated quiet to unsettled geomagnetic conditions.
Tänane hinnanguline rahvusvaheline päikeselaikude arv (ISN): 065, põhineb 12 jaamadel.
| Catania Wolfi number | /// |
| 10cm päikesevoog | 142 |
| AK Chambon La Forêt | 014 |
| AK Wingst | 014 |
| Hinnanguline Ap | 013 |
| Hinnanguline rahvusvaheline päikeselaikude arv | 066 - Põhineb 16 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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