Ausgestellt: 2021 Dec 18 1250 UTC
C-class flares expected, (probability >=50%)
Quiet (A<20 and K<4)
Quiet
| 10cm Fluss | Ap | |
|---|---|---|
| 18 Dec 2021 | 121 | 005 |
| 19 Dec 2021 | 125 | 006 |
| 20 Dec 2021 | 132 | 006 |
Six regions and one plage are present on the visible solar disk, of which Catania 84/NOAA 2907, Catania 86/NOAA2908 and Catania 88/NOAA 2911 (configuration beta-gamma) produced C class flares while the last flare in X-ray output originated from Catania 87/NOAA 2909 (configuration beta- gamma) produced a c2.3-class flare on Dec 17 13:25UT. A new region is about to rotate to the visible disk on the southern hemisphere. C-class flares can be expected and M-class flares possible over the next 24 hours.
No Earth directed CMEs were observed in the past 24 hours.
The greater than 10 MeV proton flux was at nominal levels in the past 24 hours and is expected to remain at nominal levels in the next 24 hours. The greater than 2 MeV electron flux remained below the 1000 pfu alert threshold and is expected to remain under the threshold during the next 24 hours. The greater than 2 MeV electron fluence was at nominal levels in the past 24 hours where it is expected to remain.
Over the past 24 hours, the total magnetic field had values between 1 and 5nT, and its southward component, Bz, fluctuated between -4 nT and +4 nT. The solar wind speed ranged from 325 to 390 km/s. The interplanetary magnetic field phi angle was predominantly on the negative sector (directed towards the Sun) until Dec 18 05:30UT, when it was varied. A negative polarity equatorial Coronal Hole(CH) is currently at central meridian. Any possible High Speed Stream (HSS) effects could be expected about Dec 22. A negative polarity CH appeared at the SW quadrant. Any effect of a HSS could be expected about Dec 19-20. Over the next 24 hours, the solar wind paramentes are expected to remain in these levels.
Geomagnetic conditions were quiet over the past 24 hours (NOAA Kp and K-BEL 0-2). Geomagnetic conditions are expected to be quiet to unsettled over the next 24 hours.
Die heute international geschätzte Sonnenfleckenanzahl (ISN): 099, basierend auf 08 Stationen.
| Wolf-Zahl Catania | 134 |
| 10cm Solarflux | 121 |
| AK Chambon La Forêt | 005 |
| AK Wingst | 003 |
| Geschätzer Ap-Wert | 002 |
| Geschätzte internationale Sonnenfleckenzahl | 105 - Basierend auf 14 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
Alle Zeiten in UTC
Viele Menschen nutzen SpaceWeatherLive, um die Sonnenaktivität zu verfolgen oder um zu schauen, ob es eine Chance gibt Polarlichter, zu sehen. Mit zunehmendem Datenverkehr steigen jedoch die Kosten für die Serververfügbarkeit. Wenn Ihnen SpaceWeatherLive gefällt und Sie das Projekt unterstützen möchten, können Sie ein Abonnement für eine werbefreie Website abschließen oder eine Spende tätigen. Mit Ihrer Hilfe können wir SpaceWeatherLive online halten!
| Letzte Klasse X-Eruption | 08/12/2025 | X1.1 |
| Letzte Klasse M-Eruption | 12/12/2025 | M1.1 |
| Letzter geomagnetischer Sturm | 12/12/2025 | Kp5 (G1) |
| Tage ohne Flecken | |
|---|---|
| Letzter fleckenlose Tag | 08/06/2022 |
| Monatliche mittlere Sonnenfleckenzahl | |
|---|---|
| November 2025 | 91.8 -22.8 |
| Dezember 2025 | 139.6 +47.8 |
| Letzte 30 Tage | 106.8 +8.5 |