Ausgestellt: 2021 Mar 17 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Active conditions expected (A>=20 or K=4)
Quiet
| 10cm Fluss | Ap | |
|---|---|---|
| 17 Mar 2021 | 079 | 003 |
| 18 Mar 2021 | 077 | 004 |
| 19 Mar 2021 | 077 | 023 |
Solar activity was very low in the past 24 hours, no C-class flares were recorded. NOAA Active Region (AR) 2808 has decayed into a plage region. The new active region, is now numbered as Catania group 81 (NOAA AR 2810) and has been quiet. Overall, solar activity is expected to remain at very low levels, with a small chance of a C-class flare.
A back-sided partial halo Coronal Mass Ejections (CME) was first seen at 10:24 UT on the 16th March in LASCO-C2 images. It is not expected to arrive at Earth. No Earth-directed CMEs have been observed in the available coronagraph data.
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 exceeded the 1000 pfu threshold during the last 24 hours and is expected to remain above the threshold for the next 24 hours. The 24h electron fluence was at moderate levels and it is expected to remain at this level in the next 24 hours.
Solar wind speed continued to decrease in the last 24 hours with values between 400 km/s and 340 km/s. The total interplanetary magnetic field was between 0 and 6 nT during the last 24 hours. The magnetic field phi angle switched from negative to mostly positive after approximately 18:00 UT March 16th. Solar wind conditions are expected to generally reflect a slow solar wind regime during March 17th and 18th. On March 19th the solar wind high speed stream associated with the corona hole, which crossed that solar central meridian on 17th March, is expected to arrive.
Geomagnetic conditions were at quiet levels (NOAA Kp 0-2 and local K Dourbes 1-2). Geomagnetic conditions are expected to be at quiet levels over the next 24 hours. However, the geomagnetic conditions are expected to reach active levels on the 19th March, due to the expected high speed stream.
Die heute international geschätzte Sonnenfleckenanzahl (ISN): 011, basierend auf 11 Stationen.
| Wolf-Zahl Catania | /// |
| 10cm Solarflux | 079 |
| AK Chambon La Forêt | 007 |
| AK Wingst | 003 |
| Geschätzer Ap-Wert | 002 |
| Geschätzte internationale Sonnenfleckenzahl | 020 - Basierend auf 20 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 | 144.3 +52.5 |
| Letzte 30 Tage | 107.5 +8.8 |