Paper
28 June 2006 DARWIN fringe sensor: experimental results on the BRISE bench
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Abstract
Interferometer performances are linked to the measurement and the correction of telescope aberrations. For cophasing the large number of beams required by the DARWIN mission with the specified requirements (realtime piston/tip/tilt correction and measurement of higher orders up to spherical aberration), focal-plane approach has been selected due to its simple opto-mechanical device. Several focal-plane algorithms, developed at ONERA and gathered in the stand-alone MASTIC tool, were validated by experiment with a dedicated breadboard on the laboratory test bench BRISE. Our study shows the correct behaviour of the algorithms for linearity and repeatability; specific requirements are reached for piston/tip/tilt and higher order aberrations. These results confirm the validity of focal-plane sensors for the cophasing of multiple-aperture telescopes.
© (2006) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Isabelle Mocœur, Frédéric Cassaing, Fabien Baron, Laurent Mugnier, Stephan Hofer, and Hans Thiele "DARWIN fringe sensor: experimental results on the BRISE bench", Proc. SPIE 6268, Advances in Stellar Interferometry, 62682B (28 June 2006); https://doi.org/10.1117/12.671705
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Cited by 3 scholarly publications.
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KEYWORDS
Phase retrieval

Sensors

Image retrieval

Telescopes

Interferometers

Monochromatic aberrations

Point spread functions

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