SODIUM-LAYER LASER-GUIDE-STAR EXPERIMENTAL RESULTS

被引:30
作者
AVICOLA, K
BRASE, JM
MORRIS, JR
BISSINGER, HD
DUFF, JM
FRIEDMAN, HW
GAVEL, DT
MAX, CE
OLIVIER, SS
PRESTA, RW
RAPP, DA
SALMON, JT
WALTJEN, KE
机构
[1] Lawrence Livermore National Laboratory, Livermore, CA
来源
JOURNAL OF THE OPTICAL SOCIETY OF AMERICA A-OPTICS IMAGE SCIENCE AND VISION | 1994年 / 11卷 / 02期
关键词
D O I
10.1364/JOSAA.11.000825
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
We describe a series of experiments to characterize the sodium-layer guide star that was formed with the high-power laser developed for the Lawrence Livermore National Laboratory Atomic Vapor Laser Isotope Separation program. An emission spot size of 3.0 m was measured, with an implied laser irradiance spot diameter of 2.0 m. The rms spot motion at the higher laser powers, with active beam-pointing control, was less than 0.5 arcsec and had little effect on the observed spot size under these conditions. We measured the resonant backscatter from the sodium layer as a function of laser power to obtain a saturation curve. With a transmitted power of 1100 W and an atmospheric transmission of 0.6, the irradiance from the guide star at the ground was 10 (photons/cm(2))/ms, corresponding to a visual magnitude of 5.1. The implications for the performance of wave-front sensors with a laser guide star of this magnitude and resulting closed-loop adaptive-optics performance are discussed.
引用
收藏
页码:825 / 831
页数:7
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