Previsioni Meteorologiche Spaziali - Discussione

Emesso: 2026 Feb 16 0030 UTC
Preparati dal Dipartimento di Commercio degli Stati Uniti, NOAA, Centro di Previsione Meteorologica Spaziale e elaborati da SpaceWeatherLive.com

Attività solare

Sommario di 24 ore
Solar activity remained at low levels. The largest flare of the period was a C1.8 at 15/2106 UTC from AR 4374 (N10W11, Hsx/alpha). All regions were either stable or in decay, with Region 4377 (N08E55, Cro/beta) exhibiting the most decay. No Earth-directed CMEs were detected in available imagery.
Previsione
Solar activity is expected to be at low levels through 18 Feb.

Particelle energetiche

Sommario di 24 ore
The greater than 2 MeV electron flux reached moderate levels. The greater than 10 MeV proton flux remained at background levels.
Previsione
The greater than 2 MeV electron flux is expected to reach moderate levels on 16 Feb, before increasing to high levels on 17-18 Feb. The greater than 10 MeV proton flux is expected to continue at background levels through 18 Feb.

Vento Solare

Sommario di 24 ore
Solar wind parameters were consistent with the onset of CIR effects preceding positive polarity CH HSS influences. Total magnetic field strength (Bt) reached a peak of 13 nT. The Bz (north-south) component was predominantly northward, with regular southward deviations by as much as -11 nT. Solar wind speeds steadily increased from a low of around 520 km/s to a peak just over 750 km/s at 15/1157 UTC; afterward it averaged around 650 km/s. The phi angle was predominantly positive (away from the Sun).
Previsione
The solar wind environment is expected to remain enhanced through 18 Feb due to positive polarity CH HSS influences, likely transitioning to negative polarity CH HSS influence on 18 Feb.

Geospaziale

Sommario di 24 ore
The geomagnetic field reached G1 (Minor) storm levels in response to CIR effects preceding positive polarity CH HSS influences.
Previsione
Isolated periods of G1 (Minor-Moderate) geomagnetic storming are likely on 16 Feb due to positive polarity CH HSS influences with potential weak CME enhancements as a CME from 13 Feb might pass in close proximity. Active conditions are likely on 17 Feb as CH HSS influences begin to wane, with quiet to unsettled expected on 18 Feb.

Ultime notizie

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Notizie sul meteo spaziale

Ultimo brillamento X2026/02/04X4.3
Ultimo brillamento M2026/02/13M1.0
Ultima tempesta geomagnetica2026/02/05Kp5+ (G1)
Giorni senza macchie
Ultimo giorno senza macchie2022/06/08
Media mensile Numero di Macchie Solari
gennaio 2026112.6 -11.4
febbraio 2026112.1 -0.5
Ultimi 30 giorni128.2 +28

Questo giorno nella storia*

Brillamenti solari
12024X2.56
21999M4.64
32024M3.0
42011M2.36
51999M2.14
DstG
11980-132G2
21967-130G4
31959-104G2
41990-99G3
51962-78G2
*dal 1994

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