Open Access Paper
21 November 2017 High accuracy absolute distance metrology
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Proceedings Volume 10567, International Conference on Space Optics — ICSO 2006; 105670Z (2017) https://doi.org/10.1117/12.2308057
Event: International Conference on Space Optics 2006, 2006, Noordwijk, Netherlands
Abstract
One of ESA’s future missions is the Darwin Space Interferometer, which aims to detect planets around nearby stars using optical aperture synthesis with free-flying telescopes. Since this involves interfering white (infra-red) light over large distances, the mission is not possible without a complex metrology system that monitors various speeds, distances and angles between the satellites. One of its sub-systems should measure absolute distances with an accuracy of around 70 micrometer over distances up to 250 meter. To enable such measurements, we are investigating a technique called frequency sweeping interferometry, in which a single laser is swept over a large known frequency range. Central to our approach is the use of a very stable, high finesse Fabry-P´erot cavity, to which the laser is stabilized at the endpoints of the frequency sweep. We will discuss the optical set-up, the control system that controls the fast sweeping, the calibration and the data analysis. We tested the system using long fibers and achieved a repeatability of 50 micrometers at a distance of 55 meters. We conclude with some recommendations for further improvements and the adaption for use in space.
© (2017) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Bas L. Swinkels, Nandini Bhattacharya, Ad L. Verlaan, and Joseph J. M. Braat "High accuracy absolute distance metrology", Proc. SPIE 10567, International Conference on Space Optics — ICSO 2006, 105670Z (21 November 2017); https://doi.org/10.1117/12.2308057
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KEYWORDS
Distance measurement

Phase measurement

Interferometers

Interferometry

Calibration

Digital signal processing

Control systems

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