Dueling lasers! A comparative analysis of two different sodium laser technologies on sky

Sodium guide star technologies for Adaptive Optics (AO) have been around for over 20 years. During this time, the technologies for the lasers used to excite the mesospheric sodium have been in constant development, with the goals being not only to excite as much sodium as possible, but to do so efficiently, while producing a round guide star, and while offering a reliable facility. The first lasers in use were dye lasers with a liquid gain medium, while these lasers were able to produce sodium guide stars, the liquid dye used was toxic and flammable. The second generation of guide star lasers used sum-frequency-mixed solid-state lasers. These lasers provided excellent return but were notoriously difficult to calibrate and maintain, requiring a full-time laser engineer on staff. The current third generation of sodium guide star lasers use Raman fiber amplification to generate a laser that is very efficient at exciting sodium with a good spot profile and offer a high degree of reliability. The Gemini South observatory for the last few years has been in the process of obtaining one of these third-generation lasers, a Toptica Sodium Star 20/2 while maintaining its second-generation Lockheed Martin Coherent Technologies (LMCT) 50W CW Mode-locked laser. In October of 2017 successful on-sky commissioning of the Toptica laser was executed while the LMCT laser was still active and in operations. During the course of the commissioning run both lasers were used on sky in close in time in possible. We present a comparative study of the performance of each laser.

[1]  Céline d'Orgeville,et al.  Four generations of sodium guide star lasers for adaptive optics in astronomy and space situational awareness , 2016, Astronomical Telescopes + Instrumentation.

[2]  Herbert W. Friedman,et al.  Sodium beacon laser system for the Lick Observatory , 1995, Optics & Photonics.

[3]  F. Rigaut,et al.  Characterization of the sodium layer at Cerro Pachon, and impact on laser guide star performance , 2013, 1301.3690.

[4]  I. Hook,et al.  The Gemini–North Multi‐Object Spectrograph: Performance in Imaging, Long‐Slit, and Multi‐Object Spectroscopic Modes , 2004 .

[5]  Antoine Labeyrie,et al.  Feasibility of adaptive telescope with laser probe , 1985 .

[6]  Olivier Guyon,et al.  Commissioning status of Subaru laser guide star adaptive optics system , 2010, Astronomical Telescopes + Instrumentation.

[7]  D. Bonaccini Calia,et al.  First light of the ESO laser guide star facility , 2006, SPIE Astronomical Telescopes + Instrumentation.

[8]  Charles P. Cavedoni,et al.  Gemini multiconjugate adaptive optics system review - I. Design, trade-offs and integration , 2013, 1310.6199.

[9]  Chester S. Gardner,et al.  Experiments on laser guide stars at Mauna Kea Observatory for adaptive imaging in astronomy , 1987, Nature.

[10]  Vincent Fesquet,et al.  Polarization control optimization of the Gemini South beam transfer optics , 2014, Astronomical Telescopes and Instrumentation.

[11]  Andrew Serio,et al.  Gemini South multi-conjugate adaptive optics (GeMS) laser guide star facility on-sky performance results , 2012, Other Conferences.

[12]  R. Holzlohner,et al.  Optimization of cw sodium laser guide star efficiency , 2009, 0908.1527.

[13]  Gabriel Pérez,et al.  Switching between two laser guide star facilities: an overview of the optomechanical design for the new laser beam injector at the Gemini South Observatory , 2018, Astronomical Telescopes + Instrumentation.

[14]  Robert Q. Fugate,et al.  The Sodium LGS Brightness Model over the SOR , 2007 .

[15]  Patrick Leisching,et al.  Series production of next-generation guide-star lasers at TOPTICA and MPBC , 2014, Astronomical Telescopes and Instrumentation.

[16]  Sarah J. Diggs,et al.  Gemini multiconjugate adaptive optics system review – II. Commissioning, operation and overall performance , 2014, 1402.6906.

[17]  R. Rampy Advancing adaptive optics technology: Laboratory turbulence simulation and optimization of laser guide stars , 2013 .

[18]  Robert Q. Fugate,et al.  Realization of a 50-watt facility-class sodium guidestar pump laser , 2005, SPIE LASE.

[19]  T. Jeys,et al.  Development Of Mesospheric Sodium Laser Beacon For Atmospheric Adaptive Optics , 1990, LEOS '90. Conference Proceedings IEEE Lasers and Electro-Optics Society 1990 Annual Meeting.

[20]  Sebastian Rabien,et al.  Design of PARSEC the VLT laser , 2003, SPIE Astronomical Telescopes + Instrumentation.

[21]  Claire E. Max,et al.  Sodium-layer laser-guide-star experimental results , 1994 .