Paper
13 September 1994 Interferometric fiber arms for stellar interferometry
Francois Reynaud, J. J. Alleman, H. Lagorceix
Author Affiliations +
Abstract
In a synthesized aperture implemented for stellar interferometry application, the star light usually travels by mirrors train to reach the interferometric mixing station. Using fibers the number of freedom degrees to be controlled is reduced. Parameters to be servo are the fiber length, the dispersion compensation and the polarization control. We report experimental results demonstrating the fiber length stabilization with a 5 nm accuracy, the dispersion compensation over a 300 nm spectral bandwidth (600-900 nm) and the control of polarization effects.
© (1994) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Francois Reynaud, J. J. Alleman, and H. Lagorceix "Interferometric fiber arms for stellar interferometry", Proc. SPIE 2209, Space Optics 1994: Earth Observation and Astronomy, (13 September 1994); https://doi.org/10.1117/12.185277
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CITATIONS
Cited by 10 scholarly publications and 1 patent.
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KEYWORDS
Servomechanisms

Interferometry

Polarization

Stars

Stellar interferometry

Structured optical fibers

Astronomy

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