Polar lights (Aurora Borealis)

19/20.January 2026,Germerswang, South Germany

Photographies by Thorsten Boeckel

At first the end of the main attraction.

 19th of January

Aurora Borealis, Polar Lights, January 2026, by Th. Boeckel

23:17 CET: Nice to see the 140° red arc, may it is a deformed SAR bow. (Composite of 3 images)

KP index ca. 8+ / 9-

Aurora Borealis, Polar Lights, January 2026, by Th. Boeckel   Aurora Borealis, Polar Lights, January 2026, by Th. Boeckel

Intensive colours   /  Weaker colours

Aurora Borealis, Polar Lights, January 2026, by Th. Boeckel   Aurora Borealis, Polar Lights, January 2026, by Th. Boeckel

Still missing the hour before ...

... but on the 20th of January fine auroras appeared again

Aurora Borealis, Polar Lights, January 2026, by Th. Boeckel    Aurora Borealis, Polar Lights, January 2026, by Th. Boeckell

18:30; CET: The view from Lugberg/Germerswang looking north shows a pink polarlight

Aurora Borealis, Polar Lights, January 2026, by Th. Boeckell     Aurora Borealis, Polar Lights, January 2026, by Th. Boeckel

19:40h: And now a aurora borealis actually appeared more red with strong beamer

Aurora Borealis, Polar Lights, January 2026, by Th. Boeckel

Aurora Borealis, Polar Lights, January 2026, by Th. Boeckel    Aurora Borealis, Polar Lights, January 2026, by Th. Boeckel

Change of place

23:30, Again a deep red aurora appeared :-)

  Aurora Borealis, Polar Lights, January 2026, by Th. Boeckel    Aurora Borealis, Polar Lights, January 2026, by Th. Boeckel

Aurora Borealis, Polar Lights, January 2026, by Th. Boeckel

Aurora Borealis, Polar Lights, January 2026, by Th. Boeckel

The final red, KP index ca. 7+


Look at the aurora in Mai 2024


Basics about sightings of Aurora Borealis also known as Northern- or polar lights, in middle latitudes

 KP index*: Roughly speaking, auroras can already be observed visually from KP 5-6 (G1/2 storm) in northern Germany. At KP 7/8 (G3/4 storm) or above also in southern Germany (Alps to southern Europe). Among other things, the density and speed of the flares or CME's (earth directed solar mass ejection forms) or corona holes are relevant parameters for the strength of the solar storms and visual sightings. But the Bz value which definite the north- south  alignment of the earth magnetic field ( May 2024, Bz -50nT ) is the most important factor. If this Bz value is to weak, the protons can't invade in the earth magnetic field. By the way, the glowing phenomenon is triggered by 'animated' oxygen and nitrogen atoms. Oxygen up to ~100 km shows greenish colors and from ~100-200 km red to orange.  Nitrogen atoms up  to ~300 km shows more seldom purple or blue colors.


NOAA Space Weather Prediction Center


Aurora Borealis & Atmospheric phenomena


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          ©2026 photos by Thorsten Boeckel


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