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甚长基线干涉测量数据分析中与基线相关的时钟偏移。

Baseline-dependent clock offsets in VLBI data analysis.

作者信息

Krásná Hana, Jaron Frédéric, Gruber Jakob, Böhm Johannes, Nothnagel Axel

机构信息

Department of Geodesy and Geoinformation, Technische Universität Wien (TU Wien), Wiedner Hauptstraße 8-10, 1040 Vienna, Austria.

Astronomical Institute, Czech Academy of Sciences, Boční II 1401, 141 00 Prague, Czech Republic.

出版信息

J Geod. 2021;95(12):126. doi: 10.1007/s00190-021-01579-5. Epub 2021 Nov 1.

DOI:10.1007/s00190-021-01579-5
PMID:34789964
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC8558298/
Abstract

The primary goal of the geodetic Very Long Baseline Interferometry (VLBI) technique is to provide highly accurate terrestrial and celestial reference frames as well as Earth orientation parameters. In compliance with the concept of VLBI, additional parameters reflecting relative offsets and variations of the atomic clocks of the radio telescopes have to be estimated. In addition, reality shows that in many cases significant offsets appear in the observed group delays for individual baselines which have to be compensated for by estimating so-called baseline-dependent clock offsets (BCOs). For the first time, we systematically investigate the impact of BCOs to stress their importance for all kinds of VLBI data analyses. For our investigations, we concentrate on analyzing data from both legacy networks of the CONT17 campaign. Various aspects of BCOs including their impact on the estimates of geodetically important parameters, such as station coordinates and Earth orientation parameters, are investigated. In addition, some of the theory behind the BCO determination, e.g., the impact of changing the reference clock in the observing network on the BCO estimate is introduced together with the relationship between BCOs and triangle delay closures. In conclusion, missing channels, and here in particular at S band, affecting the ionospheric delay calibration, are identified to be the dominant cause for the occurrence of significant BCOs in VLBI data analysis.

摘要

大地测量甚长基线干涉测量(VLBI)技术的主要目标是提供高精度的地球和天体参考框架以及地球定向参数。根据VLBI的概念,必须估计反映射电望远镜原子钟相对偏移和变化的附加参数。此外,实际情况表明,在许多情况下,各个基线的观测群时延中会出现显著偏移,必须通过估计所谓的基线相关时钟偏移(BCO)来进行补偿。我们首次系统地研究了BCO的影响,以强调其在各类VLBI数据分析中的重要性。在我们的研究中,我们专注于分析CONT17活动遗留网络的数据。研究了BCO的各个方面,包括它们对大地测量重要参数(如台站坐标和地球定向参数)估计的影响。此外,还介绍了BCO确定背后的一些理论,例如观测网络中参考时钟变化对BCO估计的影响,以及BCO与三角形时延闭合之间的关系。总之,影响电离层时延校准的缺失通道,特别是在S波段的缺失通道,被确定为VLBI数据分析中出现显著BCO的主要原因。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/ef63/8558298/cc0156db34f0/190_2021_1579_Fig17_HTML.jpg
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https://cdn.ncbi.nlm.nih.gov/pmc/blobs/ef63/8558298/bd51205e9b3b/190_2021_1579_Fig1_HTML.jpg
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https://cdn.ncbi.nlm.nih.gov/pmc/blobs/ef63/8558298/a7258e25b981/190_2021_1579_Fig6_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/ef63/8558298/20ed9ad012f5/190_2021_1579_Fig7_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/ef63/8558298/b20b14ad1446/190_2021_1579_Fig8_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/ef63/8558298/6ceeb62f4bc5/190_2021_1579_Fig9_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/ef63/8558298/cf8583634b0e/190_2021_1579_Fig10_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/ef63/8558298/b0b324805b44/190_2021_1579_Fig11_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/ef63/8558298/9b50edd2c774/190_2021_1579_Fig12_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/ef63/8558298/b95ee66539b8/190_2021_1579_Fig13_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/ef63/8558298/1dbac2dba51a/190_2021_1579_Fig14_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/ef63/8558298/d10bb7696b79/190_2021_1579_Fig15_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/ef63/8558298/60db98432c88/190_2021_1579_Fig16_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/ef63/8558298/cc0156db34f0/190_2021_1579_Fig17_HTML.jpg

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