Vorhersage Details

Ausgestellt: 2026 May 16 1230 UTC
Erstellt von NOAA, Space Weather Prediction Center und verarbeitet SpaceWeatherLive.com

Sonnenaktivität

24h Zusammenfassung
Solar activity was at low levels. Region 4435 (N22W89, Dao/beta) produced the strongest flare of the period, a C9.5/Sf at 15/1614 UTC. Associated with the flare was a Type II radio sweep (est. 529 km/s). Only minor changes were observed in the three numbered active regions on the visible disk. No Earth-directed CMEs were observed in available coronagraph imagery.
Vorhersage
Solar activity is expected to remain predominately at low levels, with a chance for M-class (R1-R2/Minor-Moderate) flares through 18 May.

Energiereiche Teilchen

24h Zusammenfassung
The greater than 2 MeV electron flux was at normal to moderate levels. The greater than 10 MeV proton flux was at background levels.
Vorhersage
The greater than 2 MeV electron flux is expected to remain at moderate levels through 16 May, likely increasing to high levels on 17-18 May as -CH HSS influences persist. The greater than 10 MeV proton flux is expected to stay at background levels through 18 May.

Sonnenwind

24h Zusammenfassung
The solar wind parameters reflected increased influence from a negative polarity CH HSS. Total interplanetary magnetic field strength unsteadily increased from around 3 nT to reach as high as 17 nT. The Bz component briefly reached as far south as -14 nT. Phi was in a predominantly negative orientation. Wind speeds steadily increased to a peak of ~800 km/s between 15/2300-16/0330 UTC. A gradual decline to a speed near 650 km/s was observed by the end of the reporting period.
Vorhersage
Solar wind parameters are expected to continued to be enhanced through 18 May due to the persistent influence of the negative polarity CH HSS.

Geospace

24h Zusammenfassung
The geomagnetic field reached G1-G2 (Minor-Moderate) geomagnetic storm levels due to the influence of a CIR ahead of negative polarity CH HSS.
Vorhersage
G1 (Minor) conditions are expected to continue through 16 May due to the ongoing effects of a negative polarity CH HSS. Active to G1 (Minor) storm levels are likely to continue on 17 May, decreasing to unsettled to active conditions by 18 May as lingering CH HSS influences diminish.

Neueste Nachrichten

Unterstützen Sie SpaceWeatherLive!

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!

Keine Werbung auf SWL Pro!
Keine Werbung auf SWL Pro! Abonnements
Spenden
Unterstützen Sie SpaceWeatherLive! Spenden
Unterstütze SpaceWeatherLive mit unseren Merchandise-Artikeln
Schaue nach unseren Merchandise-Artikeln

Weltraumwetter-Fakten

Letzte Klasse X-Eruption24/04/2026X2.5
Letzte Klasse M-Eruption10/05/2026M5.7
Letzter geomagnetischer Sturm15/05/2026Kp6+ (G2)
Tage ohne Flecken
Letzte 365 Tage3 Tage
20263 Tage (2%)
Letzter fleckenlose Tag24/02/2026
Monatliche mittlere Sonnenfleckenzahl
April 202679.3 -6.6
Mai 202693.3 +14
Letzte 30 Tage94.4 +1.9

An diesem Tag in der Vergangenheit*

Sonneneruptionen
12023M9.62
22000M4.69
32022M2.4
42005M2.31
52005M2.1
DstG
11981-119G2
22005-101G2
31969-94G2
41995-93G2
52024-90G2
*seit 1994

Aurora on this day in history

No observations submitted for this day in history. If you've observed the aurora and you have some amazing photos to show off, submit your observations now!
Submit your aurora observation

Soziale Netzwerke