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GPS-based Sub-Hourly Polar Motion Estimates: Strategies and Applications.

机译:基于GPS的每小时小时极地运动估计:策略和应用。

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摘要

Since their advent in the late 1970's, satellite geodetic techniques have revolutionized the monitoring of the Earth's orientation in inertial space and significantly contributed to advances in geodynamics. Long- and mid-term features manifesting in the Earth Rotation Parameters power spectra are, in general, accurately determined and explained. In contrast, sub-daily fluctuations affecting polar motion and length-of-day are not known as precisely. The lack of highly-resolved time series is currently a strong limiting factor for gaining more insight into rapid polar motion - the parameter of interest here - and its geophysical implications. This thesis was aimed at customizing an estimation strategy targeting the recovery of polar motion at very high temporal resolution based on GPS ground observations only. To this end, the trade-space existing between the precise determination of the GPS satellite orbits and clocks themselves and the retrieval of the Earth's pole coordinates at sufficient accuracy for geodetic purposes was extensively investigated. The strategy design and underlying rationale are described. Candidate strategies are presented and results obtained from the reanalysis of one year of data are shown and analyzed. The challenges associated with the determination of ultra-rapid polar motion are discussed. In particular, mathematical singularities stemming from various sources are emphasized and handling techniques proposed. Difficulties inherent to the quality assessment of the estimates are stressed and the methodology employed for conducting relevant performance analyses is detailed. The validity of the solutions generated is demonstrated through the recovery of geophysical signals such as the major semidiurnal and diurnal ocean tides and large-scale oceanic and atmospheric circulations. Among other geophysical applications, preliminary results for the detection of so-called megaquakes are shown based on the 2011 M9.0 Honshu earthquake event. Recommendations and guidelines for the determination of polar motion at high frequencies are formulated based on the numerous test cases studied.
机译:自1970年代后期问世以来,卫星大地测量技术已经彻底改变了对惯性空间中地球方向的监视,并极大地推动了地球动力学的发展。通常,可以准确地确定和解释“地球自转参数”功率谱中表现出的长期和中期特征。相比之下,影响极地运动和一天中时间长度的次日波动是未知的。当前缺乏高度解析的时间序列是一个强大的限制因素,它不能使您对快速极地运动(这里感兴趣的参数)及其地球物理意义有更多的了解。本文旨在基于仅基于GPS地面观测的自定义估计策略,以极高的时间分辨率恢复极地运动。为此,广泛地研究了精确确定GPS卫星轨道和时钟本身与以大地测量目的以足够的精度获取地球极坐标之间的贸易空间。描述了策略设计和基本原理。提出了候选策略,并显示和分析了从对一年数据的重新分析中获得的结果。讨论了与确定超快速极性运动有关的挑战。特别是,强调了来自各种来源的数学奇异点并提出了处理技术。强调了评估质量评估所固有的困难,并详细介绍了进行相关绩效分析所采用的方法。所产生的解决方案的有效性通过地球物理信号(例如主要的半日和昼间海潮以及大规模的海洋和大气环流)的恢复来证明。在其他地球物理应用程序中,基于2011年本州M9.0级地震事件,给出了检测所谓的特大地震的初步结果。根据研究的大量测试案例,制定了确定高频极运动的建议和指南。

著录项

  • 作者

    Sibois, Aurore E.;

  • 作者单位

    University of Colorado at Boulder.;

  • 授予单位 University of Colorado at Boulder.;
  • 学科 Engineering Aerospace.
  • 学位 Ph.D.
  • 年度 2011
  • 页码 293 p.
  • 总页数 293
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

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