中国科学院乌鲁木齐天文站
纸质出版:1995
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[1]桑思武,刘志华,陈金莲,李留才,孙晓雷,张谦.乌鲁木齐VLBI站25m天线定向方法及测站座标[J].新疆大学学报(自然科学版),1995(01).
桑思武, 刘志华, 陈金莲, et al. 乌鲁木齐VLBI站25m天线定向方法及测站座标[J]. Journal of Xinjiang University (Natural Science Edition in Chinese and English), 1995, (1).
我们根据乌鲁木齐VLBI站的1954北京座标系的座标(x,y),利用Gauss的反算公式,计算出乌鲁木齐VLBI站的大地座标(L,B),并通过有关公式得到了天文座标(λ,),然后根据测站的天文座标计算北极星大距时的位置,再由北极星大距时的位且找到天极的方向,最后解决了大型天文测量设备的定向问题(仪器方位零点).我们给出的测站座标在25m大型射电望远镜的安装、调试和国际联测中一直在使用之中.最近又与全球定位系统(GPS)测量结果进行了比较,比较结果令人满意.
The geodetic coordinates(L
B ) of Urumchi VLBI station was calculated with the method of Gauss coordinate translated according to the coordinates (x
y) of Urumchi VLBI station of Beijing coordinate system
1954 ; then
the values of astronomical coordinates (λ ) was obtained by related formulae ; the position of the Polaris at elongation was calculated by the coordinates ;the direction of the north Pole was found out according to the position ;finaly the orientational problem of according to the position if maly the orientational problem of the large astronomical observing equipment (the null point position of the azimuth about the radio telescope) was solved.The coordinates which we calculated was used in the installation and modulation of the 25m radio telescope
and the international joint observations. Recently
the coordinates was compared with which obtained by GPS
The results are satisfactory.
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