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Perturbation in the Earth's Pole due to the Recent 31 Large Earthquakes of Magnitude over 8.0

  • Na, Sung-Ho (Space Geodetic Observation Center) ;
  • Kyung, Jai-Bok (Department of Earth Science Education, Korea National University of Education)
  • 투고 : 2016.07.18
  • 심사 : 2016.09.22
  • 발행 : 2016.09.30

초록

We present our estimate of pole shift caused by the recent 31 largest earthquakes of magnitude over 8.0. After reviewing theory of perturbation in the Earth's rotation, each co-seismic as well as post-seismic pole shifts by the earthquakes are acquired and illustrated. A total co-seismic excitation due to these earthquakes is ($x_1$, $x_2$)=(-3.35, 5.89) milliarcsec, which increased about twice the initial estimation when the post-seismic deformation is considered. The single largest co-seismic excitation by 2011 Japan earthquake was ($x_1$, $x_2$)=(-2.06, 2.36) milliarcsec, which corresponds to 9.7 cm pole shift on the surface of the Earth.

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참고문헌

  1. Baek, J., Shin, Y.H., Na, S.H., Shestakov, N.V., Park, P.H., and Cho, S., 2012, Coseismic and postseismic crustal deformations of the Korean peninsula caused by the 2011 M 9.0 Tohoku earthquake, Japan from GPS data, Terra Nova, 24, 295-300, doi:10.1111/j.1365-3121.2012.01062.x.
  2. Bizouard, C. and Gambis, D, 2009, The combined solution C04 for Earth Orientation Parameters consistent with International Terrestrial Reference Frame 2005. IAG Symposium 134, 265-270, doi:10.1007/978-3-642-00860-3_41.
  3. Chao, B.F., 2016, Rotational normal modes in classical mechanics: resonance, excitation, convolution/deconvolution etc. Lecture of GAGER 2016, July 18-24, Wuhan, China.
  4. Chung, T.W. and Na, S.H., 2016, A least square fit analysis on the Earth's polar motion time series:implication against Smylie's conjecture. Jigu-Mulli-wa-Mulli-Tamsa, 19, 91-96, doi:10.7582/GGE.2016.19.2.091.
  5. Dahlen, F.A., 1971, The excitation of the Chandler wobble by earthquakes, Geophysical Journal Royal Astronomical Society, 25, 157-206. https://doi.org/10.1111/j.1365-246X.1971.tb02336.x
  6. Dahlen, F.A., 1973, A correction to the excitation of the Chandler wobble by earthquakes. Geophysical Journal Royal Astronomical Society, 32, 203-217. https://doi.org/10.1111/j.1365-246X.1973.tb06527.x
  7. Gross, R.S., 1986, The influence of earthquakes on the Chandler wobble during 1977-1983. Geophysical Journal Royal Astronomical Society, 85, 161-177. https://doi.org/10.1111/j.1365-246X.1986.tb05176.x
  8. Gross, R.S., 2000, The excitation of the Chandler wobble. Geophysical Research Letters, 27, 15, 2329-2332, doi:10.1029/2000GL011450.
  9. Gross, R.S., 2009, Earth rotation variation - long period. In Schubert, G. (ed.), Trietise of Geophysics vol. 3 Geodesy, Elsevier, Amsterdam, 239-294.
  10. Gross, R.S. and Chao, B.F., 2006, The rotational and gravitational signature of the December 26, 2004 Sumatran earthquake. Surveys in Geophysics, 27, 615-632. https://doi.org/10.1007/s10712-006-9008-1
  11. Hearn, E.H., 2003, What can GPS data tell us about the dynamics of post-seismic deformation? Geophysical Journal International, 155, 753-777. https://doi.org/10.1111/j.1365-246X.2003.02030.x
  12. Lambeck, K., 1980, The Earth's variable rotation: geophysical causes and consequences. Cambridge University Press, Cambridge, 449 p.
  13. Plag, H.P., Chao, B., Gross, R, and van Dam T. (eds.), 2005, Proceedings of the workshop: forcing of polar motion in the Chandler frequency band: a contribution to understanding interannual climate variation. April 21-23, 2004, Luxemburg, European Centre for Geodynamics and Seismilogy, 165 p.
  14. Smylie, D.E. and Manshina, L., 1968, Earthquakes and observed motion of the rotation pole. Journal of Geophysical Research, 73, 7661-7673. https://doi.org/10.1029/JB073i024p07661
  15. Smylie, D.E. and Zuberi, M., 2009, Free and forced polar motion and modern observation of the Chandler wobble. Journal of Geodynamics, 48, 226-229, doi:10.1016/j.jog.2009.09.028.