Paper
28 July 2010 System overview of 30 W and 55 W sodium guide star laser systems
Nicholas Sawruk, Ian Lee, Munib Jalali, Zachary Prezkuta, Ken Groff, Jared Roush, Nathan Rogers, Bruce Tiemann, Steve Hannon, Joe Alford, Céline d'Orgeville, Vincent Fesquet, Richard Oram, Sean M. Adkins, Kenny Grace
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Abstract
We report on the successful delivery of a 30 W solid-state sodium Guide Star Laser System (GLS) to the W. M. Keck Observatory in 2009, and the demonstration of a 55 W GLS delivered to the Gemini South Observatory in 2010. This paper describes the GLS performance results of both the Keck I and Gemini South GLSs with an emphasis on the system design and delivered performance. The 589 nm output was generated via Sum Frequency Mixing (SFM) of 1064 nm and 1319 nm Nd:YAG lasers in a LBO (Lithium Triborate) nonlinear crystal. The Keck GLS underwent extensive testing and has demonstrated consistent performance with a CW mode-locked output of > 30 W and measured beam quality of M2 < 1.2 while locked to the sodium D2a transition. The Keck GLS was installed on the telescope in late 2009 and first light on the sky was achieved in early 2010. Factory testing of the Gemini South GLS shows a CW modelocked output of > 55 W and measured M2 ~1.2 while locked to the sodium D2a line center. The Gemini South GLS has produced a maximum power of 76 W at 589 nm with 85 W of 1319 nm and 110 W of 1064 nm as inputs to the SFM, representing a single-pass conversion efficiency of 39%.
© (2010) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Nicholas Sawruk, Ian Lee, Munib Jalali, Zachary Prezkuta, Ken Groff, Jared Roush, Nathan Rogers, Bruce Tiemann, Steve Hannon, Joe Alford, Céline d'Orgeville, Vincent Fesquet, Richard Oram, Sean M. Adkins, and Kenny Grace "System overview of 30 W and 55 W sodium guide star laser systems", Proc. SPIE 7736, Adaptive Optics Systems II, 77361Y (28 July 2010); https://doi.org/10.1117/12.858218
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Cited by 13 scholarly publications.
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KEYWORDS
Optical amplifiers

Gemini Observatory

Laser systems engineering

Atomic force microscopy

Observatories

Sodium

Laser guide stars

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