Ausgestellt: 2023 Jul 31 1314 UTC
M-class flares expected (probability >=50%)
Active conditions expected (A>=20 or K=4)
Quiet
| 10cm Fluss | Ap | |
|---|---|---|
| 31 Jul 2023 | 170 | 007 |
| 01 Aug 2023 | 168 | 028 |
| 02 Aug 2023 | 166 | 023 |
The solar flaring activity was moderate during the last 24 hours, with one M1 flare produced by NOAA Active Region (AR) 3390 (magnetic type Beta) which peaked at 08:42 UTC today. Several C-class flares ranging from C1 to C6 were also produced in the last 24 hours: the brightest C6 by NOAA AR 3390 (magnetic type Beta). For the next 24 hours we are expecting few C-class flares and M-class flare from NOAA AR 3390. There are very likely a small chance of an X-flare.
No Earth-directed Coronal Mass Ejections (CME) were observed in the last 24 hours.
A small positive polarity coronal hole has crossed central meridian, and it is expected to have an impact on Earth environment on 3 Aug.
Earth is presently inside the slow solar wind with velocity ranging from about 400 to 500 km/s and the interplanetary magnetic field ranging from 2 nT to 6 nT. The North-South component (Bz) ranged between -5 and 4 nT. We expect to see increase in the solar wind velocity once the expected CMEs arrive at Earth.
During the last 24 hours, the geomagnetic conditions were quiet to unsettled (NOAA Kp and K BEL 1 to 3) and we expect to see active condition or minor storm conditions when the expected CMEs arrive at Earth.
The greater than 10 MeV proton flux dropped below the 10 pfu threshold level yesterday at 16:30 UTC. It is expected to stay below the threshold level for the next 24 hours.
The 2 MeV electron flux, as measured by the GOES-16 satellite, was below the threshold level in the last 24 hours, and it is expected to remain below the threshold level in the coming 24 hours.
Die heute international geschätzte Sonnenfleckenanzahl (ISN): 180, basierend auf 14 Stationen.
| Wolf-Zahl Catania | /// |
| 10cm Solarflux | 174 |
| AK Chambon La Forêt | 012 |
| AK Wingst | 012 |
| Geschätzer Ap-Wert | 011 |
| Geschätzte internationale Sonnenfleckenzahl | 182 - Basierend auf 33 Stationen |
| Tag | Start | Max | Ende | Loc | Stärke | OP | 10cm | Catania/NOAA | Radioburst-Typen |
|---|---|---|---|---|---|---|---|---|---|
| 31 | 0842 | 0900 | 0913 | S20E44 | M1.6 | 2F | 08/3390 |
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 | |
|---|---|
| Februar 2026 | 78.2 -34.3 |
| März 2026 | 75 -3.2 |
| Letzte 30 Tage | 55.6 -70.1 |