Previsioni Meteorologiche Spaziali - Discussione
Emesso: 2026 Mar 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 reached moderate levels. Region 4396 (N20E55, Bxo/beta)
was numbered this period, but was otherwise unremarkable. Region 4392
(S16E28, Cso/beta) produced the strongest flare of the period, an
M1.0/Sf flare at 15/0939 UTC. Coronal dimming was observed with this
event in GOES Suvi 195 imagery and an associated narrow and faint CME
was then observed in LASCO C2 imagery at approximately 15/1036 UTC.
Modeling of this event determined a miss behind and south of Earth. No
Earth-directed CMEs were observed.
Previsione
Solar activity is expected to be at low levels, with a slight chance for
M-class (R1-R2/Minor-Moderate) flares through 18 Mar.
Particelle energetiche
Sommario di 24 ore
The greater than 2 MeV electron flux reached high levels with a peak
flux of 1,430 pfu at 15/1900 UTC. The greater than 10 MeV proton flux
was at background levels.
Previsione
The greater than 2 MeV electron flux is expected to continue to reach
high levels through 18 Mar. The greater than 10 MeV proton flux is
expected to continue at background levels through 18 Mar.
Vento Solare
Sommario di 24 ore
Solar wind parameters reflected the continued influence of a positive
polarity CH HSS. Total field was at 5-6 nT and the Bz component was +/-
5 nT. Solar wind speeds gradually decreased from peaks near 700 km/s to
end the period near 600 km/s. Phi was predominantly in a positive solar
sector.
Previsione
Solar wind parameters are expected to remain elevated, but gradually
decline over the next three days (16-18 Mar).
Geospaziale
Sommario di 24 ore
Geomagnetic field activity ranged from quiet to active levels.
Previsione
Geomagnetic field activity is expected to be primarily quiet to
unsettled through 18 Mar with isolated active periods persisting on day
one (16 Mar).