空间参照基准 SGUGiT 的线长比较结果

N.S. Kosarev, A.A. Sholomitskii, M.A. Khanzadyan, L. Serdakov, V.S. Krapivin, I.O. Suchkov
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引用次数: 0

摘要

本文给出了 2021 年和 2023 年春夏季使用 Leica TM30 全站仪以及 2023 年同季使用 Leica AT403 激光跟踪仪对 SGUGiT 空间基准(SRB)进行的线长比较结果。根据对每段基础的多次测量(至少 30 次)分析,计算了标准偏差和不确定性。与此同时,在基准段的极值点,由两台独立仪器记录气象参数(温度、压力和相对湿度),然后在使用 Leica TM 30 电子全站仪计量时立即输入。在使用徕卡 AT403 激光跟踪仪的情况下,空间分析仪测量数据的专门管理和处理软件会自动将这些参数考虑在内。研究结果表明,使用徕卡 AT403 激光跟踪仪和徕卡 TM30 电子全站仪在 WPT 上测量 12 米至 192 米范围内的基本线长度时,考虑到影响最终结果的公认误差,扩大的不确定度不超过 1.4 毫米,而 B 类估计的标准不确定度对确定线长度的误差影响最大。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Line lengths comparison results on the spatial reference basis SGUGiT
The results of line lengths comparison on the spatial reference basis (SRB) of SGUGiT, carried out according to the program in all combinations measurements in the forward direction from point BI01 to point BI10 in spring and summer of 2021 and 2023 using total station Leica TM30, as well as, in the same seasons of 2023 done by laser tracker Leica AT403 are given. Based on the analysis of multiple measurements of each section of the basis (at least 30 ones), the standard deviation and uncertainty were calculated. Meanwhile, at the extreme points of the base section, meteorological parameters (temperature, pressure and relative humidity) were recorded by two independent instruments, which were then entered immediately when metering with a Leica TM 30 electronic total station. In the case of the Leica AT403 laser tracker, they were automatically taken into account in specialized software management and processing of Spatial Analyzer measurement data. Due to the research results, it was found out that the expanded uncertainty in measuring the lengths of the basic lines in the range from 12 to 192 m on the WPT using a Leica AT403 laser tracker and a Leica TM30 electronic total station, taking into account the accepted errors that affect the final result, is no more than 1,4 mm, and the maximum contribution to the mistake in determining line lengths is made by the standard uncertainty estimated by type B. In addition, seasonal fluctuations in the position of individual basis points are observed
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