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Rapports
Activité solaire
Activité aurorale
Coronal hole faces Earth

The geomagnetic storm which was the result of a coronal mass ejection impact from the M9.8 solar flare has now subsided. The north-south (Bz) component of the interplanetary magnetic field is pointing northwards which is preventing any kind of geomagnetic unrest at the moment. We did peak at the strong G3 geomagnetic storm level which caused some very nice auroral displays at lower latitudes than usual. So does that mean we need to wait for weeks and weeks before the next geomagnetic storm? No! A very large coronal hole is currently facing our planet sending a high-speed solar wind stream towards us.

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La Météo Spatiale en faits

Dernière classe X08/12/2025X1.1
Dernière classe M12/12/2025M1.1
Dernier orage géomagnétique12/12/2025Kp5 (G1)
Jours sans taches solaires
Dernier jour sans taches solaires08/06/2022
Nombre mensuel moyen de taches solaires
novembre 202591.8 -22.8
décembre 2025135.1 +43.3
30 derniers jours107.1 +10.8

A ce jour dans l'histoire*

Éruptions solaires
12022M4.0
22002M3.66
32022M3.5
42002M2.84
52022M2.4
DstG
11960-132G2
22006-72
31987-70G2
41972-58G1
51988-58G1
*depuis 1994

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