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首页> 外文期刊>Studia Geophysica et Geodaetica >Very short baseline interferometry: assessment of the relative stability of the GPS stations at the Yebes Observatory (Spain)
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Very short baseline interferometry: assessment of the relative stability of the GPS stations at the Yebes Observatory (Spain)

机译:基线干涉仪非常短:评估西班牙耶贝斯天文台GPS站的相对稳定性

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Using a very short baseline interferometer, the relative stability of the YEBE and YEB1 GPS stations at the Yebes Observatory (Spain) is assessed. A baseline length bias of 1 mm was found between estimates from different observed frequencies due most likely to phase center errors resulting from antenna calibration uncertainties and/or phase center migrations caused by the electromagnetic coupling of antenna and monument. Also a bias of 0.5 mm in the vertical component of the baseline length was found between estimates from different cut-off elevation angles due to elevation-dependent errors as phase center and multipath. In addition to these biases, significant variations in the horizontal component of the baseline length were found, mostly in the form of a trend of −0.45 ± 0.10 mm/yr and an annual oscillation of amplitude 1 ± 0.1 mm and phase 155 ± 5 (beginning of June). The annual oscillation showed a high correlation with ambient temperature variations. Bedrock thermal expansion seems not to be a significant contributor to the annual variation due to the excellent agreement between the phases of the baseline and temperature annual signals. Thermoelastic expansion of the station monuments, which are comprised of concrete pillars and buildings, driven by the sunshine heating, is likely the origin of this oscillation. Near-field multipath and phase center errors are also rejected as being the main contributor to the annual signal. Conversely, near-field multipath and phase center errors may significantly contribute together to the time-correlated noise content of the baseline time series at long periods (flicker noise amplitude of 1.2 ± 0.1 mm). This research provides thus an assessment of the GPS station stability at the Yebes Observatory, which may be extended to the level of station-dependent contamination of geophysical and geodetic studies (e.g., plate tectonics, surface loadings, local ties) when similar station installations on top of buildings are used.
机译:使用非常短的基线干涉仪,评估了耶贝斯天文台(西班牙)的YEBE和YEB1 GPS站的相对稳定性。在不同观测频率的估计值之间发现基线长度偏差为1 mm,这最有可能是由于天线校准不确定性和/或天线和纪念碑的电磁耦合引起的相位中心偏移而导致的相位中心误差。另外,由于与高度相关的误差(如相位中心和多径),在来自不同截止仰角的估计值之间,基线长度的垂直分量存在0.5 mm的偏差。除了这些偏差外,还发现基线长度的水平分量有显着变化,主要表现为-0.45±0.10 mm / yr的趋势以及振幅1±0.1 mm和155±5的年振荡(六月初)。年振荡显示与环境温度变化高度相关。由于基线和温度年度信号各阶段之间的极好的一致性,基岩的热膨胀似乎不是造成年度变化的重要因素。车站纪念碑的热弹性膨胀是由振荡引起的,这些纪念碑由混凝土柱和建筑物组成,由阳光加热驱动。近场多径和相位中心误差也被认为是造成年度信号的主要因素。相反,近场多径误差和相位中心误差可能会长时间共同导致基线时间序列的时间相关噪声含量(闪烁噪声幅度为1.2±0.1 mm)。因此,这项研究提供了对Yebes天文台GPS站稳定性的评估,当在类似站上安装类似装置时,可以将其扩展到与站有关的地球物理和大地测量污染水平(例如,板块构造,地表载荷,局部联系)。使用建筑物的顶部。

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