Estimation of Velocities of Ukrainian GNSS Stations in the IGb08 Reference Frame

IF 0.5 4区 物理与天体物理 Q4 ASTRONOMY & ASTROPHYSICS Kinematics and Physics of Celestial Bodies Pub Date : 2024-09-27 DOI:10.3103/S0884591324050039
O. O. Khoda
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Abstract

The cumulative solution for GPS weeks 935–1933 (December 7, 1997–January 28, 2017) was obtained in the GNSS Data Analysis Centre of the Main Astronomical Observatory of the National Academy of Sciences of Ukraine after adjustment of 6993 daily normal equation files received as a result of the regular processing and the second reprocessing campaign of archival observations. The ADDNEQ2 program of the Bernese GNSS Software ver. 5.2 was used. Before the adjustment, the times series of station coordinates received from the mentioned processing were analyzed to find outliers and determine sets of coordinates and velocities. For foreign EPN stations, the files prepared by the EUREF Permanent GNSS Network were used (EPN_outliers.lst and EPN_discontinuities.snx respectively). For 233 permanent GNSS stations, the 356 sets of coordinates and 256 sets of velocities that correspond them were established. According to the duration of observations, the coordinate sets were divided into three groups: (1) less than 1 year (94 sets), (2) 1–3 years (92 sets), (3) more than 3 years (166 sets). Four coordinate sets were excluded from further analysis. The IGb08 reference frame was realized by applying No-Net-Translation conditions on the coordinates of the IGS Reference Frame stations. The velocities of these stations were heavily constrained (10–9 m/year for each components) that, in term of adjustment means, a fixing of velocities values. As result, the coordinates and velocities of the Ukrainian and the Eastern European stations in the IGb08 reference frame at epoch 2005.0 were estimated with high precision. The mean repeatabilities for components of station coordinates are 1.69, 1.40, and 3.63 mm for the north, east, and height components respectively.

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在 IGb08 参照系中估算乌克兰全球导航卫星系统台站的速度
乌克兰国家科学院主要天文观测台全球导航卫星系统数据分析中心在对常规处理和第二次档案观测再处理活动中收到的6993个每日正常方程文件进行调整后,获得了全球定位系统第935-1933周(1997年12月7日至2017年1月28日)的累积解。使用了伯尔尼全球导航卫星系统软件 5.2 版的 ADDNEQ2 程序。5.2 版的 ADDNEQ2 程序。在调整之前,对上述处理过程中收到的台站坐标时间序列进行了分析,以查找异常值并确定坐标和速度集。对于外国 EPN 台站,使用了 EUREF 永久 GNSS 网络编制的文件(分别为 EPN_outliers.lst 和 EPN_discontinuities.snx)。对于 233 个永久性全球导航卫星系统台站,建立了与之对应的 356 组坐标和 256 组速度。根据观测时间的长短,坐标集被分为三组:(1) 小于 1 年(94 组),(2) 1-3 年(92 组),(3) 3 年以上(166 组)。有四组坐标被排除在进一步分析之外。IGb08 参考框架是通过对 IGS 参考框架站点的坐标应用无净平移条件实现的。这些站点的速度受到严格限制(每个分量为 10-9 米/年),调整意味着速度值的固定。因此,IGb08 参照系中的乌克兰和东欧站点在 2005.0 历元的坐标和速度估算精度很高。台站坐标各分量的平均重复性分别为 1.69、1.40 和 3.63 毫米(北、东和高度分量)。
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来源期刊
Kinematics and Physics of Celestial Bodies
Kinematics and Physics of Celestial Bodies ASTRONOMY & ASTROPHYSICS-
CiteScore
0.90
自引率
40.00%
发文量
24
审稿时长
>12 weeks
期刊介绍: Kinematics and Physics of Celestial Bodies is an international peer reviewed journal that publishes original regular and review papers on positional and theoretical astronomy, Earth’s rotation and geodynamics, dynamics and physics of bodies of the Solar System, solar physics, physics of stars and interstellar medium, structure and dynamics of the Galaxy, extragalactic astronomy, atmospheric optics and astronomical climate, instruments and devices, and mathematical processing of astronomical information. The journal welcomes manuscripts from all countries in the English or Russian language.
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