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SLR precision analysis for LAGEOS I and II

机译:LAGEOS I和II的SLR精度分析

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This paper deals with the problem of properly weighting satellite observations which are non-uniform in quality. The technique, the variance component estimation method developed by Helmert, was first applied to the 1987 LAGEOS I SLR data by Sahin et al. (1992). This paper investigates the performance of the globally distributed SLR stations using the Helmert type variance component estimation. As well as LAGEOS I data, LAGEOS II data were analysed, in order to compare with the previously analysed 1987 LAGEOS I data. The LAGEOS I and II data used in this research were obtained from the NASA Crustal Dynamics Data Information System (CDDIS), which archives data acquired from stations operated by NASA and by other U.S. and international organizations. The data covers the years 1994, 1995 and 1996. The analysis is based on "full-rate" laser observations, which consist of hundreds to thousands of ranges per satellite pass. The software used is based on the SATAN package (SATellite ANalysis) developed at the Royal Greenwich Observatory in the UK.
机译:本文讨论了对质量不均匀的卫星观测值进行适当加权的问题。该技术,由Helmert开发的方差分量估计方法,最早由Sahin等人于1987年对LAGEOS I SLR数据应用。 (1992)。本文使用Helmert类型方差分量估计来研究全球分布的SLR电台的性能。与LAGEOS I数据一样,对LAGEOS II数据也进行了分析,以便与先前分析的1987 LAGEOS I数据进行比较。这项研究中使用的LAGEOS I和II数据是从NASA地壳动力学数据信息系统(CDDIS)获得的,该系统对从NASA和其他美国及国际组织运营的站点获取的数据进行存档。数据涵盖了1994年,1995年和1996年。该分析基于“全速率”激光观测,其中每卫星通过数百到数千个范围。使用的软件基于英国皇家格林威治天文台开发的SATAN软件包(SATellite ANalysis)。

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