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Characterizing the Diurnal Signature in Two Way Satellite Time Transfer (TWSTT) Data with a Kalman Filter

机译:用卡尔曼滤波器在两种方式中表征两种方式卫星时间转移(TWSTT)数据的昼夜签名

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This purpose of this paper is to call further attention to the technique of using a Kalman filter [1] to estimate the diurnal signature in TWSTT data. Accordingly, we have reduced all publicly available data since 2004 on inter-Europe and Europe-North American baselines [2], for site pairs as well as triplets. Variations in the diurnal amplitude and phase are easily identified, including some that are too weak to be identified by simple inspection. Changes in the variations of the amplitude and phase of the diurnals in the TAI-generating observations are evident when the chip rate and bandwidth were reduced in 2009 (MJD 55042) and the bandwidth was further reduced in 2011 (MJD 55769), as indicated in Table 1. This technique would be a useful tool when used in conjunction with less readily-available information, both meteorological and instrumental.
机译:本文的这种目的是进一步关注使用卡尔曼滤波器[1]来估计TWSTT数据中的昼夜签名的技术。因此,自2004年以来,我们在欧洲欧洲和欧洲 - 北美基线[2]以来减少了所有公开的数据,适用于地点对以及三胞胎。容易识别日幅度和相位的变化,包括通过简单检查来识别的一些太弱。当芯片速率和带宽在2009年(MJD 55042)减少时,在太极观察中的幅度和阶段的变化的变化是明显的(MJD 55042),并且在2011年进一步减少了带宽(MJD 55769),如图2所示表1.当与较易于可用的信息一起使用时,这种技术将是一种有用的工具,包括气象和乐器。

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