Ausgestellt: 2025 Oct 09 1231 UTC
C-class flares expected, (probability >=50%)
Quiet (A<20 and K<4)
Quiet
| 10cm Fluss | Ap | |
|---|---|---|
| 09 Oct 2025 | 117 | 010 |
| 10 Oct 2025 | 110 | 007 |
| 11 Oct 2025 | 105 | 004 |
Solar flaring activity was low over the past 24 hours, with only two C1 flares identified. They were emitted by SIDC Sunspot Group 661 (NOAA Active Region [AR] 4241, Beta magnetic configuration) and SIDC Sunspot Group 663 (NOAA AR 4242, Beta magnetic configuration). A limited number of low-intensity C-class flares is expected in the next 24 hours.
No Earth-directed Coronal Mass Ejections (CME) were observed in the last 24 hours.
The Solar Wind (SW) conditions appear to be affected by a glancing blow that arrived in the first half of 9 Oct. It is probably associated with the SIDC CME 577 that was launched on 5 Oct at 03:25 UTC. The SW speed ranged from 320 to 430 km/s, while the interplanetary magnetic field (B) varied between 4 and 15 nT, and its North-South component (Bz) fluctuated between -6 and 13 nT. The SW speed is expected to remain at the same level and the magnetic field is expected to slowly drop in the next 24 hours.
During the last 24 hours geomagnetic conditions were both globally and locally quiet to unsettled (NOAA Kp 1- to 3- and K BEL 1 to 3). They are expected to remain at the same level, both globally and locally, for the next 24 hours.
The greater than 10 MeV proton flux, as measured by the GOES-19 satellite, was at background levels over the past 24 hours and is likely to remain so in the next 24 hours.
Over the last 24 hours the greater than 2 MeV electron flux, as measured by GOES 19, was above the 1000 pfu alert threshold until 8 Oct 22:00 UTC, with a peak value at 5000 pfu. In the next 24 hours it is expected to remain below the 1000 pfu alert threshold. The 24-hour electron fluence was at moderate levels during the past 24 hours. It is expected to drop further and reach normal levels in the next 24 hours.
Die heute international geschätzte Sonnenfleckenanzahl (ISN): 060, basierend auf 13 Stationen.
| Wolf-Zahl Catania | 060 |
| 10cm Solarflux | 120 |
| AK Chambon La Forêt | 009 |
| AK Wingst | 010 |
| Geschätzer Ap-Wert | 011 |
| Geschätzte internationale Sonnenfleckenzahl | 073 - Basierend auf 19 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 | X4.3 |
| Letzte Klasse M-Eruption | 08/02/2026 | M2.8 |
| Letzter geomagnetischer Sturm | 05/02/2026 | Kp5+ (G1) |
| Tage ohne Flecken | |
|---|---|
| Letzter fleckenlose Tag | 08/06/2022 |
| Monatliche mittlere Sonnenfleckenzahl | |
|---|---|
| Januar 2026 | 112.6 -11.4 |
| Februar 2026 | 137.7 +25.1 |
| Letzte 30 Tage | 126 +20.7 |