Open Access Paper
5 January 2018 Low frequency noise fiber delay stabilized laser with reduced sensitivity to acceleration
B. Argence, C. Clivati, J.-L. Dournaux, D. Holleville, B. Faure, P. Lemonde, G. Santarelli
Author Affiliations +
Proceedings Volume 10564, International Conference on Space Optics — ICSO 2012; 105643N (2018) https://doi.org/10.1117/12.2309248
Event: International Conference on Space Optics 2012, 2012, Ajaccio, Corsica, France
Abstract
Lasers with sub-hertz line-width and fractional frequency instability around 1×10-15 for 0.1 s to 10 s averaging time are currently realized by locking onto an ultra-stable Fabry-Perot cavity using the Pound-Drever-Hall method. This powerful method requires tight alignment of free space optical components, precise polarization adjustment and spatial mode matching. To circumvent these issues, we use an all-fiber Michelson interferometer with a long fiber spool as a frequency reference and a heterodyne detection technique with a fibered acousto optical modulator (AOM)1. At low Fourier frequencies, the frequency noise of our system is mainly limited by mechanical vibrations, an issue that has already been explored in the field of optoelectronic oscillators.2,3,4
© (2018) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
B. Argence, C. Clivati, J.-L. Dournaux, D. Holleville, B. Faure, P. Lemonde, and G. Santarelli "Low frequency noise fiber delay stabilized laser with reduced sensitivity to acceleration", Proc. SPIE 10564, International Conference on Space Optics — ICSO 2012, 105643N (5 January 2018); https://doi.org/10.1117/12.2309248
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