Warning · Geomagnetic Storm · 07:34
Issue Time: 2026 Sep 08 0734 UTC
Peaks at Kp 5.0 around 05:00
Dark from 22:40 to 03:10.
A southward field opens Earth's magnetic field. Everything below the dashed line helps. Lowest −5.3 nT at 17:19.

C2 shows the inner corona, C3 the outer. The white streaks are particles hitting the camera.
Warning · Geomagnetic Storm · 07:34
Issue Time: 2026 Sep 08 0734 UTC
Warning · Geomagnetic Storm · 05:46
Issue Time: 2026 Sep 08 0546 UTC
Warning · Geomagnetic Storm · 05:45
Issue Time: 2026 Sep 08 0545 UTC
Warning · Geomagnetic Storm · 20:01
Issue Time: 2026 Sep 07 2001 UTC
Charged particles from the sun follow Earth's magnetic field down towards the poles and collide with oxygen and nitrogen high in the atmosphere. Those collisions emit light: green from oxygen around 100 km, red higher up, violet from nitrogen.
Bz is the direction of the magnetic field carried by the solar wind. When it points south, meaning negative, it links up with Earth's own field and lets energy in. A strongly southward Bz and a high speed produce aurora even at moderate Kp.
Kp measures global geomagnetic disturbance on a scale from 0 to 9. At Sortland, Kp 2–3 is enough for aurora to the north, while Kp 5 and above drags the oval so far south that the light stands directly overhead.
From late August to the middle of April. For the rest of the year the sun sits too high at night. The activity can be just as good, but the sky is too bright for anything to show.