Paper
28 June 2006 VLTI-PRIMA fringe tracking testbed
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Abstract
One of the key components of the planned VLTI dual feed facility PRIMA is the Fringe Sensor Unit (FSU). Its basic function is the instantaneous measurement of the Optical Path Difference (OPD) between two beams. The FSU acts as the sensor for a complex control system involving optical delay lines and laser metrology with the aim of removing any OPD introduced by the atmosphere and the beam relay. We have initiated a cooperation between ESO and MPE with the purpose of systematically testing this Fringe Tracking Control System in a laboratory environment. This testbed facility is being built at MPE laboratories with the aim to simulate the VLTI and includes FSUs, OPD controller, metrology and in-house built delay lines. In this article we describe this testbed in detail, including the environmental conditions in the laboratory, and present the results of the testbed subsystem characterisation.
© (2006) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Roberto Abuter, Sebastian Rabien, Frank Eisenhauer, Johannes Sahlmann, Nicola Di Lieto, Marcus Haug, Anders Wallander, Samuel Lévêque, Serge Ménardi, Françoise Delplancke, Nicolas Schuhler, Stefan Kellner, and Robert Frahm "VLTI-PRIMA fringe tracking testbed", Proc. SPIE 6268, Advances in Stellar Interferometry, 62682Y (28 June 2006); https://doi.org/10.1117/12.671318
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Cited by 4 scholarly publications.
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KEYWORDS
Mirrors

Sensors

Control systems

Relays

Observatories

Atmospheric optics

Device simulation

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