Ausgestellt: 2021 Oct 23 1236 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
| 10cm Fluss | Ap | |
|---|---|---|
| 23 Oct 2021 | 092 | 005 |
| 24 Oct 2021 | 095 | 006 |
| 25 Oct 2021 | 100 | 006 |
Solar activity was at very low levels. The newly numbered NOAA Active Region (AR) 2887, which has rotated onto the south-east of the disk, is a large complex region with beta configuration and has been producing B-level flaring activity. NOAA AR 2886 (Catania sunspot region 64) remained stable. Catania sunspot group 65 also did not develop further. The largest flare of the period was a B9.6 flare that originated from beyond the limb at 18:38 UT. Solar activity is expected to be low over the next 24 hours with C-class flares possible, particularly from NOAA AR2887 and from further ARs expected to rotate onto the solar disk over the coming 24 hours.
A number of Coronal Mass Ejections (CME) were observed originating beyond the eastern limb but are not expected to be Earth-directed. No Earth directed CMEs have been detected in the available coronagraph imagery.
The greater than 10 MeV proton flux was at nominal levels over the past 24 hours and is expected to remain so for the next 24 hours. The greater than 2 MeV electron flux remained below the 1000 pfu alert threshold and is expected to remain below this threshold during the next 24 hours. The 24h electron fluence was at nominal levels and is expected to remain so.
The solar wind speed (DSCOVR) decreased from 500 to 390 km/s. The total magnetic field decreased from 5 nT to around 2 nT. The Bz varied between -3 and +4 nT. The interplanetary magnetic field phi angle was predominantly in the negative sector (directed towards from the Sun). The solar wind speed is expected to reflect a slow solar wind regime from Oct 24 as the influence of the high speed stream continues to wane.
Geomagnetic conditions were mostly at quiet levels (NOAA Kp and local K Dourbes recorded values of 1-2 and 0-3, respectively). Geomagnetic conditions are expected to be quiet to unsettled on Oct 23 and Oct 24.
Die heute international geschätzte Sonnenfleckenanzahl (ISN): 046, basierend auf 22 Stationen.
| Wolf-Zahl Catania | /// |
| 10cm Solarflux | 087 |
| AK Chambon La Forêt | 008 |
| AK Wingst | 004 |
| Geschätzer Ap-Wert | 002 |
| Geschätzte internationale Sonnenfleckenzahl | 037 - Basierend auf 27 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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