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一种高精度的固体地球潮汐旋转椭球体模型。

A rotational ellipsoid model for solid Earth tide with high precision.

作者信息

Yang Yongfeng, Zhang Yunfei, Liu Qiang, Lv Xianqing, Huang Pu

机构信息

Water Resources Comprehensive Development Center, Bureau of Water Resources of Shandong Province, Jinan, 250013, China.

Frontier Science Center for Deep Ocean Multispheres and Earth System (FDOMES), Physical Oceanography Laboratory, Ocean University of China, Qingdao, 266100, China.

出版信息

Sci Rep. 2024 Nov 18;14(1):28527. doi: 10.1038/s41598-024-79898-8.

DOI:10.1038/s41598-024-79898-8
PMID:39558007
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC11574028/
Abstract

Solid Earth tide represents the response of solid Earth to the lunar (solar) gravitational force. The yielding solid Earth due to the force has been thought to be a prolate ellipsoid since the time of Lord Kelvin, yet the ellipsoid's geometry such as major semi-axis's length, minor semi-axis's length, and flattening remains unresolved. Additionally, the tidal displacement of reference point is conventionally resolved through a combination of expanded potential equations and given Earth model. Here we present a geometric model in which both the ellipsoid's geometry and the tidal displacement of reference point can be resolved through a rotating ellipse with respect to the Moon (Sun). We test the geometric model using 23-year gravity data from 22 superconducting gravimeter (SG) stations and compare it with the current model recommended by the IERS (International Earth Rotation System) conventions (2010), the average Root Mean Square (RMS) deviation of the gravity change yielded by the geometric model against observation is 6.47 µGal (equivalent to 2.07 cm), while that yielded by the current model is 30.77 µGal (equivalent to 9.85 cm). The geometric model will greatly contribute to many application fields such as geodesy, geophysics, astronomy, and oceanography.

摘要

固体地球潮汐代表了固体地球对月球(太阳)引力的响应。自开尔文勋爵时代以来,由于该力作用而产生的可变形固体地球一直被认为是一个长椭球体,然而,该椭球体的几何形状,如长半轴长度、短半轴长度和扁率,仍然没有得到解决。此外,参考点的潮汐位移通常通过扩展势方程和给定的地球模型相结合来求解。在此,我们提出一种几何模型,其中椭球体的几何形状和参考点的潮汐位移都可以通过一个相对于月球(太阳)旋转的椭圆来求解。我们使用来自22个超导重力仪(SG)台站的23年重力数据对该几何模型进行了测试,并将其与国际地球自转服务组织(IERS)(2010年)推荐的当前模型进行了比较,几何模型产生的重力变化与观测值的平均均方根(RMS)偏差为6.47微伽(相当于2.07厘米),而当前模型产生的偏差为30.77微伽(相当于9.85厘米)。该几何模型将对大地测量学、地球物理学、天文学和海洋学等许多应用领域做出巨大贡献。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b7ce/11574028/9579eb33b027/41598_2024_79898_Fig5_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b7ce/11574028/6754053a37e1/41598_2024_79898_Fig1_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b7ce/11574028/6545040bbe6a/41598_2024_79898_Fig2_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b7ce/11574028/7a386d84a339/41598_2024_79898_Fig3_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b7ce/11574028/c1459026b2b4/41598_2024_79898_Fig4_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b7ce/11574028/9579eb33b027/41598_2024_79898_Fig5_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b7ce/11574028/6754053a37e1/41598_2024_79898_Fig1_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b7ce/11574028/6545040bbe6a/41598_2024_79898_Fig2_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b7ce/11574028/7a386d84a339/41598_2024_79898_Fig3_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b7ce/11574028/c1459026b2b4/41598_2024_79898_Fig4_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b7ce/11574028/9579eb33b027/41598_2024_79898_Fig5_HTML.jpg

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本文引用的文献

1
Measurement of the Earth Tides with a Diamagnetic-Levitated Micro-Oscillator at Room Temperature.室温下利用抗磁悬浮微振荡器测量地球潮汐。
Phys Rev Lett. 2024 Mar 22;132(12):123601. doi: 10.1103/PhysRevLett.132.123601.
2
Probing asthenospheric density, temperature, and elastic moduli below the western United States.探测美国西部下地幔的密度、温度和弹性模量。
Science. 2011 May 20;332(6032):947-51. doi: 10.1126/science.1202584. Epub 2011 Apr 14.