TY - JOUR
T1 - Free-space optical-frequency comparison over rapidly moving links
AU - McSorley, Shawn M.P.
AU - Dix-Matthews, Benjamin P.
AU - Frost, Alex M.
AU - McCann, Ayden S.
AU - Karpathakis, Skevos F.E.
AU - Gozzard, David R.
AU - Walsh, Shane M.
AU - Schediwy, Sascha W.
N1 - Publisher Copyright:
© 2025 American Physical Society.
PY - 2025/2
Y1 - 2025/2
N2 - 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.
AB - 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.
UR - http://www.scopus.com/inward/record.url?scp=85218455359&partnerID=8YFLogxK
U2 - 10.1103/PhysRevApplied.23.L021003
DO - 10.1103/PhysRevApplied.23.L021003
M3 - Letter
AN - SCOPUS:85218455359
SN - 2331-7019
VL - 23
SP - 1
EP - 6
JO - Physical Review Applied
JF - Physical Review Applied
IS - 2
M1 - L021003
ER -