首页 | 本学科首页   官方微博 | 高级检索  
     检索      

基于大视场光学测量设备的多星观测和解算天文经纬度研究
引用本文:王康相,何昕,魏仲慧,余辉龙,王东鹤,汶迎辉.基于大视场光学测量设备的多星观测和解算天文经纬度研究[J].测绘科学,2010,35(3):24-25,33.
作者姓名:王康相  何昕  魏仲慧  余辉龙  王东鹤  汶迎辉
作者单位:长春光学精密机械与物理研究所,长春,130033;中国科学院研究生院,北京,100039;华阴兵器试验中心,陕西华阴,714200;长春光学精密机械与物理研究所,长春,130033;长春光学精密机械与物理研究所,长春,130033;中国科学院研究生院,北京,100039
摘    要:本文提出了一种新的基于大视场光学测量设备和GPS测量点位天文坐标的方法,即测量多个星体方位角相对于主光轴方位角的增量,然后通过非线性最小二乘法解算出点位的天文坐标。采用该方法不仅可以避免讨论大气蒙气差的修正问题,而且能够满足高精度天文坐标的测量要求。

关 键 词:大视场光学测量设备  GPS  天文坐标  非线性最小二乘法

Research on multi-star observation and astronomical longitude and latitude calculation based on optical wide field measurement equipment
WANG Kang-xiang,HE Xin,WEI Zhong-hui,YU Hui-long,WANG Dong-he,WEN Ying-hui.Research on multi-star observation and astronomical longitude and latitude calculation based on optical wide field measurement equipment[J].Science of Surveying and Mapping,2010,35(3):24-25,33.
Authors:WANG Kang-xiang  HE Xin  WEI Zhong-hui  YU Hui-long  WANG Dong-he  WEN Ying-hui
Abstract:A new method for measuring the astronomical coordinate of a location based on optical wide field measurement equipment is discussed in this paper. Firstly we measure the increment of multi-star's azimuth angle from mean optical axis' s azimuth angle. Then we can calculate the astronomical coordinate of a location by the method of nonlinear least square. Using this method we can avoid the discussion of the atmospheric refraction, and achieve a higher measuring precision.
Keywords:GPS  optical wide field measurement equipment  GPS  astronomical coordinate  nonlinear least square
本文献已被 万方数据 等数据库收录!
设为首页 | 免责声明 | 关于勤云 | 加入收藏

Copyright©北京勤云科技发展有限公司  京ICP备09084417号