上海新建的2台VGOS(VLBI global observing system)天线被其附近原有的大天线遮挡,为了开展VGOS站网的联合观测,提出了一种基于天线几何位置关系的地平遮挡角计算方法。根据台站相对位置、天线口径及天线参考点到边缘点的距离等参数,即...上海新建的2台VGOS(VLBI global observing system)天线被其附近原有的大天线遮挡,为了开展VGOS站网的联合观测,提出了一种基于天线几何位置关系的地平遮挡角计算方法。根据台站相对位置、天线口径及天线参考点到边缘点的距离等参数,即可得到VGOS天线的地平遮挡角。天马VGOS天线的最大遮挡角为22.3°,遮挡天区面积占5°以上天区面积的比值为2.19%;佘山VGOS天线的最大遮挡角为23.4°,遮挡天区面积占5°以上天区面积的比值为3.14%。通过在观测纲要中添加天线的地平遮挡角信息,成功实施了VGOS站网的联测。利用VieVS软件仿真分析了天马-维泽尔基线上VGOS天线的UT1测量精度,结果表明,天马VGOS天线的地平遮挡对UT1的测量精度没有显著的影响。展开更多
The fast slewing rate and wide band of the VLBI2010 Global Observing System(VGOS) telescopes are beneficial to procure more observations and to obtain VLBI reference points(RPs) of high precisions.Meanwhile, with the ...The fast slewing rate and wide band of the VLBI2010 Global Observing System(VGOS) telescopes are beneficial to procure more observations and to obtain VLBI reference points(RPs) of high precisions.Meanwhile, with the development of synchronous tracking of fixed targets on telescopes during the observing, the RPs also can be determined in near real time based on a frame defined by other techniques. These opportunities provide us a possibility to explore the high geodetic resolution of VGOS telescopes. We design a thermal variation in RP as true values, and schedule a synchronous session of VGOS and target point(TP) series observing. Then VGOS delays and TP series are simulated and solved via piecewise functions. The results show that the accuracy of vertical component of the RP could be determined at an accuracy of 0.5 ± 0.3 mm in an hour using TP series, whereas the vertical components of RP solved by using VGOS delay measurements have a greater uncertainty due to the random error in the simulated atmosphere and bad radio source sky coverage in a shorter time interval. Some details in the data processing and accuracy evaluation are also introduced.展开更多
文摘上海新建的2台VGOS(VLBI global observing system)天线被其附近原有的大天线遮挡,为了开展VGOS站网的联合观测,提出了一种基于天线几何位置关系的地平遮挡角计算方法。根据台站相对位置、天线口径及天线参考点到边缘点的距离等参数,即可得到VGOS天线的地平遮挡角。天马VGOS天线的最大遮挡角为22.3°,遮挡天区面积占5°以上天区面积的比值为2.19%;佘山VGOS天线的最大遮挡角为23.4°,遮挡天区面积占5°以上天区面积的比值为3.14%。通过在观测纲要中添加天线的地平遮挡角信息,成功实施了VGOS站网的联测。利用VieVS软件仿真分析了天马-维泽尔基线上VGOS天线的UT1测量精度,结果表明,天马VGOS天线的地平遮挡对UT1的测量精度没有显著的影响。
基金supported by National Natural Science Foundation of China (1703067)
文摘The fast slewing rate and wide band of the VLBI2010 Global Observing System(VGOS) telescopes are beneficial to procure more observations and to obtain VLBI reference points(RPs) of high precisions.Meanwhile, with the development of synchronous tracking of fixed targets on telescopes during the observing, the RPs also can be determined in near real time based on a frame defined by other techniques. These opportunities provide us a possibility to explore the high geodetic resolution of VGOS telescopes. We design a thermal variation in RP as true values, and schedule a synchronous session of VGOS and target point(TP) series observing. Then VGOS delays and TP series are simulated and solved via piecewise functions. The results show that the accuracy of vertical component of the RP could be determined at an accuracy of 0.5 ± 0.3 mm in an hour using TP series, whereas the vertical components of RP solved by using VGOS delay measurements have a greater uncertainty due to the random error in the simulated atmosphere and bad radio source sky coverage in a shorter time interval. Some details in the data processing and accuracy evaluation are also introduced.
