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M2 constituent of ocean tide loading displacements from VLBI CONT14 hourly sessions

机译:M2潮汐潮加载VLBI Cont14小时会议的位移

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Several studies prove that ocean tide loading (OTL) displacements can be observed with space geodetic techniques. In this study, the amplitudes and Greenwich phase lags for each coordinate component, i.e., radial, west, and south of the principal lunar semidiurnal tide, M 2 of OTL displacements were estimated at the very long baseline interferometry (VLBI) sites of the 15 days long continuous VLBI campaign, CONT14, carried out by the International VLBI Service for Geodesy and Astrometry (IVS). In the estimation of the amplitudes and Greenwich phase lags of the M 2 tidal constituent, hourly VLBI station coordinate time series were used as observations derived through analyzing 1 hour VLBI sessions of the CONT14 campaign. In the analysis of hourly sessions of the CONT14 campaign, to derive accurate hourly station coordinates, troposphere delays estimated from daily sessions were reduced from the observations a priori to the analysis. The estimated amplitudes and Greenwich phase lags of the M 2 constituent of OTL displacements were compared with the predictions the state-of-the-art ocean tide models, among others, FES2012 [Lyard et al., 2006; Carreì?re et al., 2012], FES2014 [Carreì?re et al., 2016], and TPXO8 [Egbert and Erofeeva, 2002; Egbert et al., 2010]. Both the amplitudes and the phases between CONT14 estimates and ocean tide models agree well for the M 2 tide at all the sites and in most of the coordinate components. The RMS misfits of the M 2 tide of OTL displacements in all coordinate components between CONT14 and ocean tide models over coastal sites are found about two times larger than those of inland sites. This result confirms the modeling insufficiencies in shallow waters of ocean tide models which cause an accuracy restriction of OTL displacement predictions around coastal regions.
机译:有几项研究证明,可以使用太空大地测量技术观察到海潮装载(OTL)位移。在这项研究中,每个坐标部件的幅度和格林威治阶段滞后,即主要的月球半潮汐潮的径向,西和南部,在15的长基线干涉测量(VLBI)位点估计了OTL位移的M 2天长连续VLBI活动,CONT14,由国际VLBI服务进行大地测量和ASTROMY(IVS)进行。在M 2潮汐组分的幅度和格兰维奇期滞后的估计中,使用每小时VLBI站坐标时间序列作为通过分析CONT14运动的1小时VLBI会话来源的观察结果。在分析CONT14运动的每小时会议时,为了获得准确的小时驻地坐标,从观察到分析的观察结果降低了日常会话的对流层延迟。将估计的OTL位移组成的巨大幅度和Greenwich阶段滞后与预测最先进的海浪模型,等等,FES2012 [Lyard等,2006; carreȱ吗?re等人,2012],fes2014 [carreì吗?re等,2016]和tpxo8 [Egbert和Erofeeva,2002; Egbert等人。,2010]。 CONT14估计和海潮模型之间的幅度和阶段都非常适合所有网站的M 2潮汐和大多数坐标组件。在CONT14和海浪模型之间的所有坐标组件中的M 2潮汐位移的RMS不合适率大约比内陆地点大约两倍。该结果证实了海浪模型浅水区中的模型不足,这导致沿海地区周围的OTL位移预测的精度限制。

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