A sodium laser guide star coupling efficiency measurement method

被引:0
|
作者
Lu Feng [1 ]
Zhi-Xia Shen [1 ]
Suijian Xue [1 ]
Yang-Peng Li [1 ]
Kai Jin [2 ]
Angel Otarola [3 ]
Yong Bo [4 ]
Jun-Wei Zuo [4 ]
Qi Bian [4 ]
Kai Wei [2 ]
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
基金
中国国家自然科学基金;
关键词
instrumentation:adaptive optics; methods:observational; atmospheric effects;
D O I
暂无
中图分类号
P111 [天文仪器];
学科分类号
摘要
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.
引用
收藏
页码:99 / 104
页数:6
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