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Earth Rotation Observed by Very Long Baseline Interferometry and Ring Laser

机译:极长基线干涉法和环形激光观测的地球自转

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摘要

We present a systematic and unified treatment of Earth rotation from the geodetic, astronomical, and geophysical point of view. A precise terminology of precession-nutation and polar motion is of great importance for understanding the interacting physical phenomena leading to rotational irregularities of the Earth. In total, four poles of the equatorial plane are defined for the description of Earth rotation. The various components of the Earth Orientation Parameters, i.e., precession-nutation, polar motion, and universal time (or length of day) are summarized. This paper shows how very long baseline interferometry and ring laser differ in terms of Earth rotation and presents the current state-of-the-art measurement accuracy that can be achieved.
机译:我们从大地,天文和地球物理的角度介绍了对地球自转的系统且统一的处理方法。旋进动动和极运动的精确术语对于理解导致地球自转不规则的相互作用的物理现象非常重要。为了描述地球自转,总共定义了赤道平面的四个极点。总结了地球方向参数的各个组成部分,即旋进运动,极动和通用时间(或一天中的时间)。本文说明了基线干涉法和环形激光在地球自转方面有多长时间的差异,并介绍了目前可以实现的最新测量精度。

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