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Vienna Mapping Functions in VLBI Analyses

机译:Vienna映射在VLBI分析中的函数

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摘要

In recent years numerical weather models (NWM) have been applied to improve mapping functions which are used for tropospheric delay modeling in VLBI and GPS data analyses. The Vienna Mapping Functions VMF (Boehm and Schuh, 2004, [1]) are based on direct raytracing through NWM, and allow exploitation of the full information provided in the NWM. On the other hand, the Isobaric Mapping Functions IMF (Niell, 2001, [4]) use intermediate parameters calculated from the NWM. In this study, pressure level data from the ECMWF (European Centre for Medium-Range Weather Forecasts) are applied to determine the coefficients of the VMF and the IMF. Used for the analyses of IVS-R1 and IVS-R4 VLBI sessions, both mapping functions improve the repeatability of baseline lengths (by ~10% for IVS-R1 and ~5% for IVS-R4) compared to the Niell Mapping Functions NMF (Niell, 1996, [3]).
机译:近年来,已经应用了数控天气模型(NWM)以改善用于在VLBI和GPS数据分析中用于对流层延迟建模的映射功能。维也纳映射函数VMF(Boehm和Schuh,2004,[1])基于直接的光线路径通过NWM,并允许利用NWM中提供的完整信息。另一方面,等因素映射函数IFF(Niell,2001,[4])使用从NWM计算的中间参数。在本研究中,应用来自ECMWF的压力水平数据(欧洲的中距离天气预报中心)来确定VMF和IMF的系数。用于IVS-R1和IVS-R4 VLBI会话的分析,映射函数的映射函数都提高了基线长度的可重复性(对于IVS-R1和IVS-R4的〜5%的〜10%)与Niell映射函数NMF( Niell,1996,[3])。

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