Ausgestellt: 2016 Jan 27 1238 UTC
C-class flares expected, (probability >=50%)
Active conditions expected (A>=20 or K=4)
Quiet
| 10cm Fluss | Ap | |
|---|---|---|
| 27 Jan 2016 | 115 | 008 |
| 28 Jan 2016 | 116 | 018 |
| 29 Jan 2016 | 117 | 016 |
Over the past 24 hours solar activity has been low. The largest flare was a C1.3 class flare. NOAA Active Region (AR) 2489 (Beta Dao) has been most active. Both ARs 2488 and 2489 appear stable but have exhibited some flux emergence. There is currently a large Northern polar coronal hole which has moved into the Western hemisphere and may increase solar wind speeds over the coming days. A filament channel adjacent to Active Region (AR) 2487 (Alpha Axx) erupted at approximately 16:40 UT yesterday (2016-Jan-26). The filament was located in the Western hemisphere around S20W50. The CME was first observed at 18:24 UT in LASCO observations. The Computer Aided CME Tracking (CACTUS) tool measured the velocity to be 437 km/s. The CME may arrive at the Earth on 30-Jan-2016 at 06:00 UT +/- 12 hours. Solar activity is expected to remain low over the next 24 hours with a high probability of C-class flares and a low probability of M-class flares. The solar wind speed has fluctuated between 340 and 380 km/s over the past 24 hours. The total magnetic field strength has slowly increased from around 5 to 10 nT. The Bz component was largely positive, fluctuating between 0 and 8 nT. Geomagnetic conditions ranged between Kp index 1-3 (NOAA) and local K index 1-3 (Dourbes) over the past 24 hours. A positive polar coronal hole has rotated into the Western hemisphere and the resulting high-speed stream (HSS) is expected to enhance solar wind speeds later today / early tomorrow and persist for a couple of days, this may increase geo-activity in the coming days.
Die heute international geschätzte Sonnenfleckenanzahl (ISN): 086, basierend auf 08 Stationen.
| Wolf-Zahl Catania | 080 |
| 10cm Solarflux | 115 |
| AK Chambon La Forêt | 009 |
| AK Wingst | 003 |
| Geschätzer Ap-Wert | 003 |
| Geschätzte internationale Sonnenfleckenzahl | 065 - Basierend auf 18 Stationen |
| Tag | Start | Max | Ende | Loc | Stärke | OP | 10cm | Catania/NOAA | Radioburst-Typen | |
|---|---|---|---|---|---|---|---|---|---|---|
| Keine | ||||||||||
Zur Verfügung gestellt vom Solar Influences Data Analysis Center© - SIDC - Verarbeitet von SpaceWeatherLive
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