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上海天文台新SLR站精密定位和归心测量
引用本文:熊福文,朱文耀,章红平,张忠萍.上海天文台新SLR站精密定位和归心测量[J].天文学进展,2007,25(2):177-183.
作者姓名:熊福文  朱文耀  章红平  张忠萍
作者单位:1. 中国科学院,上海天文台,上海,200030;中国科学院,研究生院,北京,100039;上海市地质调查研究院,上海,200072
2. 中国科学院,上海天文台,上海,200030;同济大学,现代工程测量国家测绘局重点实验室,上海,200092
3. 中国科学院,上海天文台,上海,200030;中国科学院,研究生院,北京,100039
4. 中国科学院,上海天文台,上海,200030
摘    要:为使上海天文台新SLR站尽早投入全球SLR网的运行,根据中国SLR网的有关要求,对该站进行了精密定位和归心测量。测量中安置了特制的对中滑块设备,在小范围内采用三角测量的高差替代大地高差的近似,取得了较好的效果。测量结果表明:上海天文台新SLR站相对于上海IGS站归心测量精度可优于5 mm,由上海IGS站引得的点位精度可优于10 mm。

关 键 词:天体测量学  人卫激光测距  精密定位
文章编号:1000-8349(2007)02-0177-07
收稿时间:2006-03-15
修稿时间:2006-03-152006-04-27

Precise Determination of the new SLR Station of Shanghai Observatory
XIONG Fu-wen,ZHU Wen-yao,ZHANG Hong-ping,ZHANG Zhong-ping.Precise Determination of the new SLR Station of Shanghai Observatory[J].Progress In Astronomy,2007,25(2):177-183.
Authors:XIONG Fu-wen  ZHU Wen-yao  ZHANG Hong-ping  ZHANG Zhong-ping
Institution:1. Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai 200030, China; 2. Graduate School of Chinese Academy of Sciences, Beijing 100039, China; 3. Shanghai Institute of Geological Survey, Shanghai 200072, China;a 4. Key Laboratory of Advanced Engineering Survey of SBSM, Tongji university, Shanghai 200092, China
Abstract:To merge the new SLR observation-station in Shanghai Astronomical Observatory into the federal operation of global SLR network,here the high-precision GPS positioning and accurate reduction to the mark center of the new SLR station using traditional optical-electronic observation equipments are performed according to the precision requirements of the fidncial stations in Chinese SLR observation network.A little special sliding centering cquipment is set on the SLR telescope to help find the real center of the vertical wheeling axes.which is based on the un-movement characteristics of the vertical wheeling axes wherever the telescope wheeling toward.After the vertical axes is found,the plane center is then determined according to the vertical distance from the reference point at the sliding centering equipment to the reference wheeling plane of the telescope.The whole surveying process is accomplished with three steps. First,set three reference points around the telescope,obtain their three-dimension coordinates in the ITRF at the observing epoch using three GPS receivers' observations linking to the IGS permanent station-SHAO.Second,using two total stations to get the plane coordinates and geodetic height based on the three ITRF coordinates and the agreement between the geodetic height difference and the leveling height difference in a small area.Combining the GPS precise engineering surveying technology and the traditional optical spatial direction intersection,we get a good result of three-dimension coordinate.The result indicates that the baseline's accuracy between the IGS SHAO and the mark center of the new SLR observation station is about 5 mm. the absolute positioning error related to the geo-eenter is about 10 mm while taking account into the accuracy of IGS SHAO in the ITRF.
Keywords:GPS
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