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Attività solare
Attività aurorale
Coronal hole stream onset, G1 geomagnetic storm

Auroral activity has reached the minor G1 geomagnetic storm threshold during the past 24 hours thanks to a coronal hole high speed solar wind stream. The direction of the IMF (Bz) is pointing southward most of the time and this is causing enhanced auroral displays at high latitude locations. Auroral displays have been visible from many locations all over the world and in the northern hemisphere it was even seen as far south as Norfolk, England (!) where James Rowley-Hill took this amazing image that serves as our header. Fantastic!

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Notizie sul meteo spaziale

Ultimo brillamento X2026/02/04X4.3
Ultimo brillamento M2026/02/13M1.0
Ultima tempesta geomagnetica2026/02/15Kp5+ (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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