Aurora Borealis

German: Nordlicht / Polarlicht

Northern lights dancing across the sky when solar particles interact with Earth's magnetic field.

Aurora Borealis - photography example

The northern lights are among the most spectacular natural phenomena a photographer can capture. They occur when charged particles from the sun interact with Earth's magnetic field and atmosphere, creating curtains and waves of green, purple, and pink light dancing across the sky.

Inverza uses the Kp geomagnetic index (adjusted for your latitude - higher latitudes need lower Kp values), cloud cover (must be below 30%), and darkness level (sun must be at least 12 degrees below the horizon). At mid-latitudes, you need a strong geomagnetic storm (Kp 5+) to see aurora; near the Arctic Circle, Kp 2 can be enough.

Tip: Use a fast wide-angle lens (f/2 or faster), ISO 1600-3200, and 8-25 second exposures. A sturdy tripod is essential. Face north (or follow the predicted direction) and find a composition with a foreground element - water reflections work beautifully.

Frequently asked

What Kp value do I need to see aurora?

It depends on latitude. Near the Arctic Circle, Kp 2-3 is enough. In Germany or the northern US, you usually need Kp 5 or higher. Inverza adjusts the threshold automatically for your location.

What camera settings work for aurora?

A fast wide-angle lens (f/2 or faster), ISO 1600-3200, and 8-25 second exposures on a tripod. Shorter exposures freeze motion in fast displays; longer ones capture more light in weak ones.

Inverza detects every condition above automatically. Set your location and get notified when something special is coming.

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