TOPEX/Poseidon任务台站相关LRA校正参数估计

J. Zeitlhöfler, M. Bloßfeld, S. Rudenko, F. Seitz
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摘要

TOPEX/Poseidon (T/P)任务于1992年发射,是首批主要的测高任务之一。它是Jason卫星的前身,Jason卫星在一个非常相似的轨道上绕地球运行。大地测量空间技术SLR(卫星激光测距)通过瞄准安装在航天器上的激光后向反射器阵列(LRA)提供这次任务的观测。T/P LRA非常大,而且没有经过优化设计。这就导致了LRA相位中心的巨大变化。这些变化是轨道精度的一个重要限制因素,因此必须应用测量校正来精确确定轨道。到目前为止,只有需要插值的表化LRA校正可用。在这篇文章中,我们提出了一种新的方法来确定与台站相关的LRA校正,以改善相位中心的变化。该方法基于连续解析校正函数,该函数只使用观测方位角和天顶角结合四个参数。这些参数是在每个观测单反站的估计过程中计算的。因此,使用基于原始单反正态点观测的未校正单反残差。校正值被添加到单反测量中,抵消了LRA相位中心的变化。该方法的优点是连续函数,易于在现有软件包中实现,并且避免了表值之间的插值。此外,还将介绍经过和没有经过LRA校正的轨道之间的差异。为了证明获得的LRA改正的高质量,研究了站坐标时间序列和轨道与外部T/P轨道的比较。
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Estimation of station-dependent LRA correction parameters for the TOPEX/Poseidon mission

Launched in 1992, the TOPEX/Poseidon (T/P) mission is one of the first major altimetry missions. It is the predecessor of the Jason satellites which orbit the Earth on a very similar orbit. The geodetic space technique SLR (Satellite Laser Ranging) provides observations of this mission by targeting the Laser Retroreflector Array (LRA) mounted on the spacecraft. The T/P LRA is extremely large and not optimally designed. It thus causes big variations in the LRA phase center. These variations are a significant limiting factor of the orbit accuracy which makes it essential to apply a measurement correction for precise orbit determination. Up to now, only tabulated LRA corrections are available which require an interpolation.

In this contribution, we present a new approach to determine station-dependent LRA corrections to improve the phase center variations. The approach is based on a continuous analytical correction function which only uses the observation azimuth and zenith angle in combination with four parameters. These parameters are computed within an estimation process for each observing SLR station. Therefore, uncorrected SLR residuals based on raw SLR normal point observations are used. The correction value is added to the SLR measurement and counteracts the LRA phase center variations.

The advantages of this method are the continuous functional, which is easy to implement in existing software packages, as well as the avoidance of an interpolation between tabulated values. Furthermore, the differences between orbits determined with and without the LRA correction will be presented. Station coordinate time series and orbit comparisons with external T/P orbits are investigated in order to prove the high quality of the obtained LRA corrections.

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