High-average-power narrow-line-width sum frequency generation 589 nm laser
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Wei Zhang | Lei Zhang | Min Wan | Huaijin Ren | Guo-bin Fan | Yanhua Lu | Xiafei Xu | Wei Zhang | Huaijin Ren | Lei Zhang | Xiafei Xu | Yanhua Lu | Min Wan | Guo-bin Fan
[1] Fang Shi,et al. Design and field tests of an 8-W sum-frequency laser for adaptive optics , 1998, Astronomical Telescopes and Instrumentation.
[2] Paul D. Hillman,et al. Comparison of pump-laser characteristics for producing a mesospheric sodium guidestar for adaptive optical systems on large-aperture telescopes , 1998, Photonics West.
[3] Yan Feng,et al. 50W CW visible laser source at 589nm obtained via frequency doubling of three coherently combined narrow-band Raman fibre amplifiers. , 2010, Optics express.
[4] Robert Q. Fugate,et al. Realization of a 50-watt facility-class sodium guidestar pump laser , 2005, SPIE LASE.
[5] Xu Zuyan,et al. Investigation of 30 W-Class Second-Generation Sodium Beacon Laser , 2011 .
[6] Vincent Fesquet,et al. System overview of 30 W and 55 W sodium guide star laser systems , 2010, Astronomical Telescopes + Instrumentation.
[7] Erez N. Ribak. Laser guide star projection for large telescopes , 2006, SPIE Astronomical Telescopes + Instrumentation.
[8] Ming Liang,et al. The Laser Guide Star Facility for the Thirty Meter Telescope , 2006, SPIE Astronomical Telescopes + Instrumentation.
[9] Lee C. Bradley,et al. Pulse-train excitation of sodium for use as a synthetic beacon , 1992 .
[10] Wei Zhang,et al. High-energy all-solid-state sodium beacon laser with line width of 0.6 GHz , 2015 .