Please use this identifier to cite or link to this item: https://hdl.handle.net/2440/65435
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Type: Conference paper
Title: A bright, pulsed, guide star laser for very large telescopes
Author: Munch, J.
Hamilton, M.
Hosken, D.
Simakov, N.
Veitch, P.
Citation: Proceedings of Adaptive Optics Systems II, Proc. SPIE 7736, 77361X (2010): 2010
Publisher: SPIE
Publisher Place: USA
Issue Date: 2010
Series/Report no.: Proceedings of SPIE ; 7736
ISBN: 9780819482266
ISSN: 0277-786X
Conference Name: Adaptive Optics Systems II (2010 : San Diego, USA)
Editor: Ellerbroek, B.L.
Hart, M.
Hubin, N.
Wizinowich, P.L.
Statement of
Responsibility: 
Jesper Munch, Murray Hamilton, David Hosken, Nikita Simakov and Peter Veitch
Abstract: We demonstrate for the first time the practical feasibility of a new sodium guide star laser with a pulsed burst output of sufficient energy at 589nm to be useful for current applications and readily scalable to meet future requirements. We describe complete experimental design verification results of the pulse burst laser concept, optimized to eliminate guide-star elongation issues and to meet all requirements for Multi Conjugate Adaptive Optics (MCAO) for future extremely large ground-based telescopes (ELTs). It makes use of sum frequency generation (SFG) of two, Q-switched, injection mode-locked, wavelength stabilized Nd:YAG lasers, producing a macro-micro, pulse-burst output which is optimized in power and bandwidth to maximize the fluorescence from the high altitude sodium layer. © 2010 SPIE.
Rights: © 2010 COPYRIGHT SPIE--The International Society for Optical Engineering. Downloading of the abstract is permitted for personal use only.
DOI: 10.1117/12.856821
Published version: http://dx.doi.org/10.1117/12.856821
Appears in Collections:Aurora harvest
Environment Institute publications
IPAS publications
Physics publications

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