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Proceedings Paper

The Rayleigh technical demonstrator: a novel concepts platform
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Paper Abstract

As part of a collaboration between Durham University and ESO, an experimental platform is presented whose purpose is for testing generic laser-based wavefront sensors (WFS) for adaptive optics. The Rayleigh Technical Demonstrator (RTD) has been designed to allow a laser launch and Rayleigh back-scatter collection by installing components solely on a Nasmyth platform of the William Herschel Telescope, La Palma. The aim is to provide a WFS testing port within the RTD, permitting new WFS concepts to be tested rapidly in conjunction. This means that the RTD only requires small modifications for each concept to be tested. The second goal is to permit near-contemporaneous comparison of WFS data with that from a tomographic WFS. Currently, the RTD is planned to trial with three "cone effect-free" WFS concepts as part of the CALDO project. Presented here is an overview of the RTD design with detailed information on novel components and design choices.

Paper Details

Date Published: 27 June 2006
PDF: 10 pages
Proc. SPIE 6272, Advances in Adaptive Optics II, 627248 (27 June 2006); doi: 10.1117/12.672966
Show Author Affiliations
Nazim A. Bharmal, Univ. of Durham (United Kingdom)
Domenico Bonaccini Calia, European Southern Observatory (Germany)
Stephen J. Goodsell, Univ. of Durham (United Kingdom)
Gordon D. Love, Univ. of Durham (United Kingdom)
Timothy J. Morris, Univ. of Durham (United Kingdom)
Richard M. Myers, Univ. of Durham (United Kingdom)


Published in SPIE Proceedings Vol. 6272:
Advances in Adaptive Optics II
Brent L. Ellerbroek; Domenico Bonaccini Calia, Editor(s)

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