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首页> 外文期刊>Journal of Geodesy >Influence of subdaily model for polar motion on the estimated GPS satellite orbits
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Influence of subdaily model for polar motion on the estimated GPS satellite orbits

机译:次极子运动的次日模型对估计GPS卫星轨道的影响

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摘要

In this contribution, it is shown that GPS orbits are able to absorb some diurnal signals in polar motion. The arising implications for the influence of the subdaily pole model on GPS solutions are discussed. Two signals in polar motion can be absorbed by GPS orbits: a retrograde signal with a period of a sidereal day (23h 56min 4s) and a prograde signal with a period matching the revolution period of the GPS satellites in the terrestrial reference frame (23h 55min 56s). We show that the retrograde signal contributes to the absolute orientation of the orbital planes in space and the prograde signal, due to coincidence of its period with the period of revolution of the GPS satellites, contributes to the position of the geocenter for each individual satellite. It is known from previous studies that there are systematic differences between orbital parameters from GPS solutions computed with different subdaily pole models. We show in this paper that this behavior can be explained by the absorption effects in 1-day GPS orbits. Diurnal signals cannot be spectrally separated over a time interval of 1 day. Adjustment of any diurnal prograde or retrograde signal to a subdaily pole time series given by a subdaily model over 24 h will lead to an estimated signal with a nonzero amplitude. Thus, any subdaily pole model used in the processing of space geodetic observations contains a part which corresponds numerically to the discussed prograde signal and a part which corresponds to the retrograde diurnal signal. Different pole models show different amplitudes of the diurnal signals which will be absorbed by the orbits. As a result, GPS orbits computed with different subdaily pole models have systematically different orientation and position in space. Using 1-day GPS solutions over a time span of 13 years (1994-2007), we show that the systematic variations in orbit position and orientation caused by individual tidal terms in polar motion can be well predicted and explained by the suggested mechanism.
机译:在这一贡献中,表明了GPS轨道能够吸收极运动中的一些昼夜信号。讨论了次极点模型对GPS解决方案影响的潜在含义。 GPS轨道可以吸收两个极移信号:一个为恒星周期的逆行信号(23h 56min 4s)和一个与地面参考帧中GPS卫星的旋转周期相匹配的周期的逆行信号(23h 55min) 56s)。我们表明,逆行信号有助于空间中轨道平面的绝对定向,而正行信号由于其周期与GPS卫星的旋转周期一致而有助于每个卫星的地球中心位置。从以前的研究中可以知道,用不同的次日极模型计算的GPS解的轨道参数之间存在系统差异。我们在本文中表明,这一行为可以通过1天GPS轨道的吸收效应来解释。每日信号在1天的时间间隔内无法进行光谱分离。在24小时内将任何昼夜前进或后退信号调整到由子日模型给出的子日极时间序列,将导致估计信号的振幅为非零。因此,在空间大地观测的处理中使用的任何次日极模型都包含一个数字上对应于所讨论的前进信号的部分和一个对应于逆行昼间信号的部分。不同的极点模型显示了将被轨道吸收的昼夜信号的不同幅度。结果,用不同的次日极模型计算出的GPS轨道在空间上的系统方向和位置都不同。使用为期13年(1994-2007年)的1天GPS解决方案,我们表明,由极潮中各个潮汐项引起的轨道位置和方向的系统变化可以通过建议的机制很好地预测和解释。

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