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The principal moments of inertia calculated with the hydrostatic equilibrium figure of the Earth

机译:利用地球的静水平衡图计算出的主要惯性矩

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摘要

As an indication of the Earth's mass distribution,the principal moments of inertia (PMOI,i.e.,A,B,C) of the Earth are the basic parameters in studies of the global dynamics of the earth,like earth nutation,and the geophysics.From the aspect of observation,the PMOI can be calculated from the spherical coefficients of observed gravity field.In this paper,the PMOI are calculated directly according to its definition with the figures of the Earth's interior derived by a generalized theory of the hydrostatic equilibrium figure of the Earth.We obtain that the angle between the principal axis of the maximum moment of PMOI and the rotational axis is 0.184°,which means that the other two principal axes are very closely in the equatorial plane.Meanwhile,B-A is 1.60 × 10-s MR2,and the global dynamical flattening (H) is calculated to be 3.29587 × 10 3,which is 0.67% different from the latest observation derived value Hob s(3.273795 × 10-3) (Petit and Luzum,2010),and this is a significant improvement from the 1.1% difference between the value of H derived from traditional theories of the figure of the Earth and the value of Hobs.It shows that we can calculate the PMOI and H with an appropriate accuracy by a generalized theory of the hydrostatic equilibrium figure of the Earth.
机译:作为地球质量分布的指示,地球的主要惯性矩(PMOI,即A,B,C)是研究地球整体动力学(如地球章动和地球物理学)的基本参数。从观测的角度来看,可以从观测重力场的球面系数计算出PMOI。本文根据广义流体静力学平衡理论推导的地球内部图形,根据其定义直接计算出PMOI。我们得到PMOI最大矩的主轴与旋转轴之间的角度为0.184°,这意味着其他两个主轴在赤道平面内非常接近。同时,BA为1.60×10 -s MR2,计算得出的全局动力学平坦度(H)为3.29587×10 3,与最新观测值Hob s(3.273795×10-3)(Petit and Luzum,2010)的差异为0.67%,并且这是一个重大改进由传统的地球图理论得出的H值与霍布斯值之间的1.1%的差异得出t.t.它表明,我们可以根据流体静力学平衡图的广义理论以适当的精度计算PMOI和H地球的。

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  • 来源
    《大地测量与地球动力学(英文版)》 |2017年第3期|201-205|共5页
  • 作者单位

    CAS Key Laboratory of Planetary Sciences, Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai, 200030, China;

    University of Chinese Academy of Sciences, Beijing, 100049, China;

    CAS Key Laboratory of Planetary Sciences, Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai, 200030, China;

    University of Chinese Academy of Sciences, Beijing, 100049, China;

    CAS Key Laboratory of Planetary Sciences, Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai, 200030, China;

    University of Chinese Academy of Sciences, Beijing, 100049, China;

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