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Rotation of the Earth as a triaxial rigid body

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Geo-spatial Information Science

Abstract

The Earth is taken as a triaxial rigid body, which rotates freely in the Euclidian space. The starting equations are the Euler dynamic equations, with A smaller than B and B smaller than C. The Euler equations are solved, and the numerical results are provided. In the calculations, the following parameters are used: (C-B)/A=0.003 273 53; (B-A)/C=0.000 021 96; (C-A)/B=0.003 295 49, and the mean angular velocity of the Earth’s rotation, ω=0.000 072 921 15 rad/s. Calculations show that, besides the self-rotation of the Earth and the free Euler procession of its rotation, there exists the free nutation: the nutation angle, or the angle between the Earth’s momentary rotation axis and the mean axis that periodically change with time. The free nutation is investigated.

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References

  1. Groten E (2000) Parameters of common relevance of astronomy, geodesy, and geodynamics[J]. Journal of Geodesy, 74: 134–140

    Google Scholar 

  2. Goldstein H, Poole C, Safko J (2002) Classical mechanics (3rd ed.)[M]. Massachusetts: Addison-Wesley Press

    Google Scholar 

  3. Qiang Yuanqi (2003) Classical mechanics II[M]. Beijing: Science Press (in Chinese)

    Google Scholar 

  4. Lambeck K (1980) The Earth’s variable rotation: geophysical causes and consequences[M]. Cambridge: Cambridge University Press

    Google Scholar 

  5. Weinberg S (1972) Gravitation and cosmology[M]. New York: John Wiley and Sons

    Google Scholar 

  6. Burśa M, Śima Z (1984) Equatorial flattening and principal moments of inertia of the Earth[J]. Studia Geoph et Geod, 28: 9–10

    Article  Google Scholar 

  7. Liu H S, Chao B F (1991) The Earth’s equatorial principal axes and moments of inertia[J]. Journal of Geophysical Research, 106: 699–702

    Article  Google Scholar 

  8. Yoder C F (1995) Astrometric and geodetic properties of Earth and the solar system[M]//Ahrens T J. Global Earth physics: a handbook of physical constants. Washington D C: American Geophysical Union

    Google Scholar 

  9. NIMA (2000) World geodetic system 1984 [R]. NIMA TR 8350, National Imagery and Mapping Agency, Bethesda, Maryland

    Google Scholar 

  10. Wei Ziqing (2005) Earth’s principal moments of inertia[J]. Acta Geodaetica et Cartographica Sinica, 34(1): 7–13 (in Chinese)

    Google Scholar 

  11. Wang Wenjun (2004) Dynamical mechanism for secular trend [C]//Zhu Yaozhong, Sun Heping. Proceedings on Geodesy and Geodynamics. Wuhan.: Hubei Science and Technology Press: 706–715

    Google Scholar 

  12. Wang Wenjun, Shen Wenbin (2006) Chaotic reversals of geomagnetic poles[C]. COSPAR 36th Joint Assembly, Beijing

Download references

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Funded by the National Natural Science Foundation of China (No.40574004).

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Shen, W., Chen, W., Wang, W. et al. Rotation of the Earth as a triaxial rigid body. Geo-spat. Inf. Sc. 10, 85–90 (2007). https://doi.org/10.1007/s11806-007-0020-5

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  • DOI: https://doi.org/10.1007/s11806-007-0020-5

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