摘要
为了使LAMOST(大天区多目标光纤光谱天文望远镜)能够准确运转,需要对焦面板上光纤的位置进行检测和标定。在这一过程中,还需要对由前照法拍摄后所提取的光斑位置与单元实际位置进行匹配。在研究位置匹配的过程中,提出了一种经改进的以背照法[1]中的匹配方法为基础的新型匹配方法——最小值匹配法,有效地解决了原匹配方法在前照法检测过程中光斑数量众多、位置随机、计算量大等问题。实验证明,最小值匹配法的匹配正确率可满足LAMOST的使用需要。
In order to ensure that the Large Sky Area Multi-Object Fiber Spectroscopy Telescope(LAMOST)system can run accurately,it is necessary to measure the position of optical fibers on the focal plate of LAMOST.It is needed to match on the position of light spot extracted by front illuminate with the actual positions of units.During the study of position matching,a new pattern(the minimum matching method)based on the old one and more appropriate to front illuminate method is presented.With the new method,problems found in matching of front illuminate method,such as excessive amounts of light spots,random location,complicated calculations,are solved effectively.
出处
《光学技术》
CAS
CSCD
北大核心
2014年第6期520-523,共4页
Optical Technique
关键词
光学测量
LAMOST
最小值匹配法
前照法
位置匹配
定位参数
optical measurement
LAMOST
minimum matching method
front illuminate method
position matching
positioning parameters