Ausgestellt: 2025 Aug 20 1231 UTC
C-class flares expected, (probability >=50%)
Active conditions expected (A>=20 or K=4)
Quiet
| 10cm Fluss | Ap | |
|---|---|---|
| 20 Aug 2025 | 116 | 022 |
| 21 Aug 2025 | 118 | 017 |
| 22 Aug 2025 | 118 | 007 |
Solar flaring activity was low over the past 24 hours, with only C-class flares identified. A total of 4 numbered sunspot groups were identified on the disk over the past 24 hours, having all Alpha or Beta magnetic configuration. The largest flare was a C2.9 flare (SIDC Flare 5179) peaking on August 20 at 09:30UTC, from SIDC Sunspot Group 607 currently located at N10E90 (Alpha magnetic configuration). Solar flaring activity is expected to be low over the next 24 hours, with C-class flares likely and a small chance for M-class flares.
No new Earth-directed Coronal Mass Ejections (CMEs) have been detected in the available coronagraph images.
Fast solar wind conditions were recorded over the past 24 hours, following the arrival of the High Speed Stream associated with SIDC Coronal Hole 116. The speed increase to mainly 620 km/s with a peak at 688 km/s. The interplanetary magnetic field gradually decreased from 20 nT to 4nT, with the Bz reaching a minimum value of -11 nT. The solar wind speed is expected to remain fast in the next 24 hours.
Over the past 24 hours, the geomagnetic activity was mainly active, with a isolated period of minor storm, both globally and locally, due to the arrival of the high speed stream. Active geomagnetic conditions are expected in the next 24 hours.
The greater than 10 MeV proton flux remained below the 10 pfu threshold and is expected to remain so over the next days.
The greater than 2 MeV electron flux remained below the 1000 pfu alert threshold, and is expected to remain below the threshold during the next 24 hours. The 24h electron fluence was at normal levels and is expected to remain so.
Die heute international geschätzte Sonnenfleckenanzahl (ISN): 056, basierend auf 15 Stationen.
| Wolf-Zahl Catania | /// |
| 10cm Solarflux | 116 |
| AK Chambon La Forêt | 032 |
| AK Wingst | 019 |
| Geschätzer Ap-Wert | 024 |
| Geschätzte internationale Sonnenfleckenzahl | 037 - Basierend auf 22 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 | 04/02/2026 | X4.21 |
| Letzte Klasse M-Eruption | 25/02/2026 | M2.4 |
| Letzter geomagnetischer Sturm | 03/03/2026 | Kp5 (G1) |
| Tage ohne Flecken | |
|---|---|
| Letzte 365 Tage | 3 Tage |
| 2026 | 3 Tage (5%) |
| Letzter fleckenlose Tag | 24/02/2026 |
| Monatliche mittlere Sonnenfleckenzahl | |
|---|---|
| Januar 2026 | 112.6 -11.4 |
| März 2026 | 75.5 -37.1 |
| Letzte 30 Tage | 61.4 -62.2 |