A sodium laser guide star coupling efficiency measurement method
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作者:
Lu Feng
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机构:
Key Laboratory of Optical Astronomy,National Astronomical Observatories,Chinese Academy of SciencesKey Laboratory of Optical Astronomy,National Astronomical Observatories,Chinese Academy of Sciences
Lu Feng
[1
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Zhi-Xia Shen
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机构:
Key Laboratory of Optical Astronomy,National Astronomical Observatories,Chinese Academy of SciencesKey Laboratory of Optical Astronomy,National Astronomical Observatories,Chinese Academy of Sciences
Zhi-Xia Shen
[1
]
Suijian Xue
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机构:
Key Laboratory of Optical Astronomy,National Astronomical Observatories,Chinese Academy of SciencesKey Laboratory of Optical Astronomy,National Astronomical Observatories,Chinese Academy of Sciences
Suijian Xue
[1
]
Yang-Peng Li
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Key Laboratory of Optical Astronomy,National Astronomical Observatories,Chinese Academy of SciencesKey Laboratory of Optical Astronomy,National Astronomical Observatories,Chinese Academy of Sciences
Yang-Peng Li
[1
]
Kai Jin
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机构:
The Institute of Optics and Electronics,Chinese Academy of SciencesKey Laboratory of Optical Astronomy,National Astronomical Observatories,Chinese Academy of Sciences
Kai Jin
[2
]
Angel Otarola
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机构:
Thirty Meter Telescope Corporation
4. Technical Institute of Physics and Chemistry,Chinese Academy of SciencesKey Laboratory of Optical Astronomy,National Astronomical Observatories,Chinese Academy of Sciences
Angel Otarola
[3
]
Yong Bo
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机构:Key Laboratory of Optical Astronomy,National Astronomical Observatories,Chinese Academy of Sciences
Yong Bo
[4
]
Jun-Wei Zuo
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机构:Key Laboratory of Optical Astronomy,National Astronomical Observatories,Chinese Academy of Sciences
Jun-Wei Zuo
[4
]
Qi Bian
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机构:Key Laboratory of Optical Astronomy,National Astronomical Observatories,Chinese Academy of Sciences
Qi Bian
[4
]
Kai Wei
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机构:
The Institute of Optics and Electronics,Chinese Academy of SciencesKey Laboratory of Optical Astronomy,National Astronomical Observatories,Chinese Academy of Sciences
Kai Wei
[2
]
Jing-Yao Hu
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机构:
Key Laboratory of Optical Astronomy,National Astronomical Observatories,Chinese Academy of SciencesKey Laboratory of Optical Astronomy,National Astronomical Observatories,Chinese Academy of Sciences
Jing-Yao Hu
[1
]
机构:
[1] Key Laboratory of Optical Astronomy,National Astronomical Observatories,Chinese Academy of Sciences
[2] The Institute of Optics and Electronics,Chinese Academy of Sciences
[3] Thirty Meter Telescope Corporation
4. Technical Institute of Physics and Chemistry,Chinese Academy of Sciences
A large telescope’s adaptive optics(AO) system requires one or more bright artificial laser guide stars to improve its sky coverage. The recent advent of a high power sodium laser is perfect for such application. However, besides the output power, other parameters of the laser also have a significant impact on the brightness of the generated sodium laser guide star, mostly in non-linear relationships. When tuning and optimizing these parameters it is necessary to tune based on a laser guide star generation performance metric. Although return photon fluxis widely used, variability of the atmosphere and sodium layer makes it difficult to compare results from different sites or even within a short time period for the same site. A new metric, coupling efficiency, is adopted in our field tests. In this paper, we will introduce our method for measuring the coupling efficiency of a 20 W class pulse sodium laser for AO application during field tests that were conducted during 2013–2015.
机构:
Gran Telescopio CANARIAS SA, C Cuesta San Jose S-N, E-38712 Brena Baja, La Palma, Spain
Inst Astrofis Canarias, Via Lactea S-N, E-38205 Tenerife, SpainGran Telescopio CANARIAS SA, C Cuesta San Jose S-N, E-38712 Brena Baja, La Palma, Spain
Lombardi, G.
Calia, D. Bonaccini
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机构:
European Southern Observ, Karl Schwarzschild Str 2, D-85748 Garching, GermanyGran Telescopio CANARIAS SA, C Cuesta San Jose S-N, E-38712 Brena Baja, La Palma, Spain
Calia, D. Bonaccini
Centrone, M.
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机构:
INAF OAR Natl Inst Astrophys, Via Frascati 33, I-00078 Rome, ItalyGran Telescopio CANARIAS SA, C Cuesta San Jose S-N, E-38712 Brena Baja, La Palma, Spain
Centrone, M.
Postigo, A. de Ugarte
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机构:
Univ Cote dAzur, Artemis, Observ Cote dAzur, Blvd Observ, F-06304 Nice, FranceGran Telescopio CANARIAS SA, C Cuesta San Jose S-N, E-38712 Brena Baja, La Palma, Spain
Postigo, A. de Ugarte
Geier, S.
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机构:
Gran Telescopio CANARIAS SA, C Cuesta San Jose S-N, E-38712 Brena Baja, La Palma, Spain
Inst Astrofis Canarias, Via Lactea S-N, E-38205 Tenerife, SpainGran Telescopio CANARIAS SA, C Cuesta San Jose S-N, E-38712 Brena Baja, La Palma, Spain