Polar lights (Aurora Borealis)

12.November 2025,Mammendorf in Obb, South Germany

Photographies by Thorsten Boeckel

A battle with fog banks around the polar light show

Aurora Borealis, Polar lights, November 2025, by Th. Boeckel   Aurora Borealis, Polar lights, November 2025, by Th. Boeckel

2:20 CET: The view from Lugberg/Germerswang looking north... Nothing happens. O.k, the solar storm takes its time. Fog!, change of location to the other side.

2:50: Still no aurora. Fog is coming up here too. It's pointless, so off home. But suddenly, a brief intense red shining, a polar light appeared through the mist. Arrival time exactly predicted by SWPC, Wow!

Aurora Borealis, Polar lights, November 2025, by Th. Boeckel    Aurora Borealis, Polar lights, November 2025, by Th. Boeckel

3:00h: The fast change of location towards Galgen/Mammendorf, no fog! And now the aurora borealis actually appeared along with the power line intended for connecting the aurora ;-)

Aurora Borealis, Polar lights, November 2025, by Th. Boeckel

3:10h: On the left in the background is the village of Mammendorf. Fog is rolling in again, frustrating!

Aurora Borealis, Polar lights, November 2025, by Th. Boeckel

3:30h: Again change of location to the wind turbine Mammendorf. An annoying bank of fog builds up again in front of me.

Aurora Borealis, Polar lights, November 2025, by Th. Boeckel

4:30: Change of location near Landsberiet. Now finally a clear view!

Aurora Borealis, Polar lights, November 2025, by Th. Boeckel  Aurora Borealis, Polar lights, November 2025, by Th. Boeckel  Aurora Borealis, Polar lights, November 2025, by Th. Boeckel

4:40: Shortly before dawn, the strongest aurora borealis rays appeared.

Aurora Borealis, Polar lights, November 2025, by Th. Boeckel

4:50h CET: The appearance was clearly visual. KP index of approx. 8+

 What a foggy thriller at 1°C.


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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          ©2025 photos by Thorsten Boeckel


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