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LOCAL GEODETIC TIE BETWEEN THE VLBI ANTENNA REFERENCE POINT AND THE SCAR GPS SITE AT SYOWA STATION, ANTARCTICA

机译:南极洲sYOWa站的VLBI天线参考点和sCaR Gps站点之间的本地大地测量

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摘要

A local geodetic tie between the VLBI (Very Long Baseling Interferometry) antenna reference point in the air and the nearby SCAR GPS site on the ground was made at Syowa Station during the wintering period (April-December 1992) of the 33rd Japanese Antarctic Research Expedition (JARE-33). By attaching a one-frequency and 4 channel GPS receiver at the periphery of the 11m S/X-band antenna dish, which was pointing to the zenith, GPS relative positioning was done between the SCAR GPS site (No. 23-16 geodetic marker) as a fixed point to obtain the location of the GPS receiver electrical phase center. Such GPS relative positionings were made for 12 baseline solutions of 8 azimuths, and Cartesian coordinates of the center of a presumed circle on which these 8 electrical phase centers must overlie were obtained. There is a constraint that the antenna heights of the above electrical phase centers must coincide with each other, constituting a plane which is parallel to the ground surface. Iterative trial and error adjustment was made for the presumed center of the antenna dish to find the least square error for the residual radius (=calculated radius minus actual radius based on the mechanical design value). Since the mechanical design value between the antenna reference point and the antenna dish center along a plumbline is known, Cartesian coordinates of the VLBI antenna reference point can be estimated with the resultant offset vector (dx, dy, dz) from the VLBI antenna to the SCAR GPS site. The finally estimated offset vector was (dx, dy, dz)=(-11.68m, -74.06m, -12.02m). Because of limited functioning and short duration tracking (30min) by the one-frequency GPS receiver, the convergent error was±10cm for each direction. Thus precise connection to obtain 1-2cm accuracy is desired on the future expeditions.
机译:在第33届日本南极研究考察队的越冬期(1992年4月至12月),在Syowa站建立了VLBI(甚长基线干涉)天线参考点与附近地面SCAR GPS站点之间的局部大地测量关系。 (JARE-33)。通过在指向天顶的11m S / X波段天线天线的外围安装一个单频和4通道GPS接收器,在SCAR GPS站点(第23-16号大地标记)之间进行了GPS相对定位。 )作为固定点,以获取GPS接收器电相位中心的位置。针对8个方位角的12个基线解进行了这样的GPS相对定位,并获得了这8个电相位中心必须位于其上的假定圆的中心的笛卡尔坐标。存在这样的约束,即,上述电相位中心的天线高度必须彼此重合,构成与地面平行的平面。对天线碟的假定中心进行迭代试验和误差调整,以找到剩余半径的最小平方误差(=根据机械设计值计算出的半径减去实际半径)。由于沿铅垂线的天线参考点和天线碟形中心之间的机械设计值是已知的,因此可以使用从VLBI天线到天线的合成偏移矢量(dx,dy,dz)估算VLBI天线参考点的笛卡尔坐标。 SCAR GPS网站。最终估计的偏移矢量为(dx,dy,dz)=(-11.68m,-74.06m,-12.02m)。由于单频GPS接收机功能有限且跟踪持续时间短(30分钟),因此每个方向的收敛误差均为±10cm。因此,在未来的探险中需要精确的连接以获得1-2cm的精度。

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