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Free-space optical-frequency comparison over rapidly moving links

Shawn M.P. McSorley*,†, Benjamin P. Dix-Matthews†, Alex M. Frost, Ayden S. McCann, Skevos F.E. Karpathakis, David R. Gozzard, Shane M. Walsh, and Sascha W. Schediwy

  • *Contact author: shawn.mcsorley@research.uwa.edu.au, 22706094@student.uwa.edu.au
  • †These two authors contributed equally.

Phys. Rev. Applied 23, L021003 – Published 18 February, 2025

DOI: https://doi.org/10.1103/PhysRevApplied.23.L021003

Abstract

The comparison of optical reference frequency signals over free-space optical links is limited by the relative motion between local and remote sites. For ground to low-Earth-orbit comparison, the expected Doppler shift and Doppler rate typically reach ±4 GHz at 100 MHz s−1, which prevents the narrow-band detection required to compare optical frequencies at the highest levels of stability. As an important step to achieve these goals, we demonstrate a system capable of optical-frequency comparison in the presence of significant Doppler shifts. This system is demonstrated over a retroreflected drone link, with a maximum line-of-sight velocity of 15 m s−1 and Doppler shift of 19 MHz at a Doppler rate of 1 MHz s−1. The best fractional frequency stability obtained is 7×10−18 at an integration time of 5 s. These results are an important step toward ground to low-Earth-orbit optical frequency comparison, providing a scalable terrestrial testbed.

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