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机构地区:[1]School of Astronomy & Space Science, Nanjing University, Nanjing 210093, China [2]National Astronomical Observatories / Nanjing Institute of Astronomical Optics & Technology, Chinese Academy of Sciences, Nanjing 210042, China [3]Key Laboratory of Astronomical Optics & Technology, Nanjing Institute of Astronomical Optics & Technology, Chinese Academy of Sciences, Nanjing 210042, China [4]Key Laboratory of Modem Astronomy and Astrophysics (Nanjing University), Ministry of Education, Nanjing 210093, China
出 处:《Research in Astronomy and Astrophysics》2012年第5期584-590,共7页天文和天体物理学研究(英文版)
基 金:supported by the dedicated operation funding forastronomical observation stations and facilities from the Chinese Academy of Sciences
摘 要:An atmospheric turbulence phase screen generated using a fractal method is introduced. It is etched onto fused silica and tested in the laboratory. The etched screen has relatively low cost, high resolution, and can be used in the broad waveband under severe temperature conditions. Our results are shown to agree well with the theory.An atmospheric turbulence phase screen generated using a fractal method is introduced. It is etched onto fused silica and tested in the laboratory. The etched screen has relatively low cost, high resolution, and can be used in the broad waveband under severe temperature conditions. Our results are shown to agree well with the theory.
关 键 词:instrumentation adaptive optics -- turbulence atmospheric effects
分 类 号:TN241[电子电信—物理电子学] TP391.41[自动化与计算机技术—计算机应用技术]
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