Circalunar variations of the night sky brightness -- an FFT perspective on the impact of light pollution
Johannes Puschnig, Stefan Wallner, Thomas Posch

TL;DR
This study uses FFT analysis of two-year sky brightness data from 23 photometers in Austria to quantify how artificial light pollution diminishes the natural circalunar cycle's detectability in night sky brightness.
Contribution
It provides a quantitative assessment of light pollution's impact on circalunar periodicity detection using frequency analysis across multiple sites.
Findings
Light pollution reduces the circalunar signal amplitude significantly.
Natural lunar rhythms are detectable only in protected national parks.
Urban sites show seasonal variations linked to increased winter skyglow.
Abstract
Circa-monthly activity conducted by moonlight is observed in many species on Earth. Given the vast amount of artificial light at night (ALAN) that pollutes large areas around the globe, the synchronization to the circalunar cycle is often strongly perturbed. Using two-year data from a network of 23 photometers (Sky Quality Meters; SQM) in Austria (latitude ~48{\deg}), we quantify how light pollution impacts the recognition of the circalunar periodicity. We do so via frequency analysis of nightly mean sky brightnesses using Fast Fourier Transforms. A very tight linear relation between the mean zenithal night sky brightness (NSB) given in mag and the amplitude of the circalunar signal is found, indicating that for sites with a mean zenithal NSB brighter than 16.5 mag the lunar rhythm practically vanishes. This finding implies that the circalunar rhythm is still detectable…
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