Paper
13 September 1994 Positioning telescopes of a synthesized aperture in a star wave plane using an interferometric metrology
Author Affiliations +
Abstract
The precise location of telescopes in a stellar interferometer makes position servo necessary. We propose a metrology configuration for synthesized aperture using a fiber linkage with the mixing station. Interference layers parallel to star wave fronts are generated in order to materialize a reference plane. Fringe position sensors generate error signals and drive the telescope position assembly to place the fiber input in a reference star wave plane.
© (1994) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Francois Reynaud "Positioning telescopes of a synthesized aperture in a star wave plane using an interferometric metrology", Proc. SPIE 2209, Space Optics 1994: Earth Observation and Astronomy, (13 September 1994); https://doi.org/10.1117/12.185287
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CITATIONS
Cited by 1 scholarly publication.
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KEYWORDS
Telescopes

Stars

Servomechanisms

Metrology

Interferometry

Space telescopes

Signal generators

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