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Displacement Sensors Applied on Active Optics in Astronomical Telescope
Qi Yongjun; Zhang Zhenchao
2006-06-27
会议录名称Millimeter and Submillimeter Detectors and Instrumentation for Astronomy III
卷号6275
期号6275
页码Vol.6275 1X-1-5
会议日期2006-5-24
会议地点Orlando, FL
会议主办者The International Society for Optical Engineering
出版者SPIE
摘要
;
Many types displacement sensors used in active optics in many astronomical telescopes over the world ware describedand the measurement theory of different sensors were explained in this paper. Based on the displacement sensor’s specification of LAMOST, a test bed to check it which used dual-frequency laser interferometer was established. Some main parameters affect on the measurement accuracy of the test bed such as temperature, vibration as well as some mechanism characteristics of fixing devices were analyzed in detail, and correspond solutions were adopted. According to theoretic analysis, rectification method was brought forward to compensate the errors of sensor cause by tip-tilt, thermal shift, non-linearity, and combined with the test results of some types sensors, their advantages and disadvantages was concluded. At last it forecasted the most appropriate displacement will be used in future active optics based on the discussion above and the developing trend of large telescope.
关键词Displacement Sensor Active Optics Lamost Laser Interferometer Rectification
学科领域郭守敬望远镜(lamost) ; 天文技术与方法
文献类型会议论文
条目标识符http://ir.niaot.ac.cn/handle/114a32/439
专题会议论文
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GB/T 7714
Qi Yongjun,Zhang Zhenchao. Displacement Sensors Applied on Active Optics in Astronomical Telescope[C]:SPIE,2006:Vol.6275 1X-1-5.
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