Earth's Free Oscillations Excited by the 26 December 2004 Sumatra-Andaman Earthquake

American Association for the Advancement of Science (AAAS) - Tập 308 Số 5725 - Trang 1139-1144 - 2005
Jeffrey Park1,2,3,4,5, Teh‐Ru Alex Song1,2,3,4,5, Jeroen Tromp1,2,3,4,5, Emile A. Okal1,2,3,4,5, Seth Stein1,2,3,4,5, G. Roult1,2,3,4,5, E. Clévédé1,2,3,4,5, G. Laske1,2,3,4,5, Hiroo Kanamori1,2,3,4,5, P. Davis1,2,3,4,5, J. Berger1,2,3,4,5, Carla Braitenberg1,2,3,4,5, Michel Van Camp1,2,3,4,5, Xiang’e Lei1,2,3,4,5, Heping Sun1,2,3,4,5, Houze Xu1,2,3,4,5, S. Rosat1,2,3,4,5
1Departement de Sismologie, Institut de Physique du Globe de Paris (IPGP), 4 Place Jussieu, 75252 Paris Cedex 05, France.
2Department of Geological Sciences, 1850 Campus Drive, Evanston, IL 60208–2150, USA.
3Department of Geology and Geophysics, Yale University, Post Office Box 208109, New Haven, CT 06520–8109, USA.
4Scripps Institution of Oceanography, University of California, San Diego, La Jolla, CA 92093–0225, USA.
5Seismological Laboratory, California Institute of Technology, MS 252–21, Pasadena, CA 91125, USA.

Tóm tắt

At periods greater than 1000 seconds, Earth's seismic free oscillations have anomalously large amplitude when referenced to the Harvard Centroid Moment Tensor fault mechanism, which is estimated from 300- to 500-second surface waves. By using more realistic rupture models on a steeper fault derived from seismic body and surface waves, we approximated free oscillation amplitudes with a seismic moment (6.5 × 10 22 Newton·meters) that corresponds to a moment magnitude of 9.15. With a rupture duration of 600 seconds, the fault-rupture models represent seismic observations adequately but underpredict geodetic displacements that argue for slow fault motion beneath the Nicobar and Andaman islands.

Từ khóa


Tài liệu tham khảo

10.1016/j.pepi.2004.09.006

Harvard CMT solutions can be accessed at www.seismology.harvard.edu/CMTsearch.html.

10.1038/434581a

10.1126/science.1112260

10.1126/science.1112250

10.1098/rsta.1975.0025

10.1038/277358a0

10.1785/BSSA0690061671

10.1029/GL012i003p00141

10.1038/325405a0

10.1029/JB093iB06p06369

10.1111/j.1365-246X.1991.tb05700.x

10.1038/47011

10.1126/science.285.5431.1231

10.1016/S0031-9201(00)00155-2

F. A. Dahlen J. Tromp Theoretical Global Seismology (Princeton Univ. Press Princeton NJ 1998). A spherical reference model describes a nonrotating planet whose stress-strain relation is elastic and either is isotropic or else exhibits anisotropy with a radial axis of symmetry.

10.1111/j.1365-246X.1980.tb04317.x

10.1111/j.1365-246X.1981.tb05944.x

10.1029/JB091iB07p07241

10.1111/j.1365-246X.1990.tb04472.x

10.1073/pnas.47.3.362

10.1111/j.1365-246X.1979.tb04797.x

10.1029/JZ066i002p00605

10.1029/JZ066i002p00621

10.1029/JZ066i002p00631

10.1029/JZ071i004p01183

10.1029/JB088iB12p10285

10.1046/j.1365-246x.2000.00220.x

10.1126/science.1061771

More information is available online at www.fdsn.org.

10.1029/2005EO060001

10.1029/2004EO230001

More information is available online at www.iris.edu.

J. Park et al., Seism. Res. Lett.76, 329 (2005).

10.1016/S0031-9201(99)00024-2

More information is available online at http://geoscope.ipgp.jussieu.fr.

10.1038/246470a0

10.1111/j.1365-246X.1975.tb01609.x

10.1016/S0012-8252(99)00028-8

The Grotta Gigante pendulum tiltmeter recorded both the 1960 Chile and the 2004 Sumatra-Andaman earthquakes.

10.1016/S0031-9201(99)00120-X

10.1016/S0031-9201(00)00158-8

10.1360/02tb9346

10.1126/science.1084531

Free oscillations may be resolvable if GPS data from a global network are stacked and corrections for second-order ionospheric effects remove biases that are spatially broad; see ( 58 ).

To calibrate gravimeter and seismometer spectra the free-oscillation spectral peaks must be corrected for the motion-induced gravitational forces on the seismic sensor ( 16 ). The breathing mode 0 S 0 involves only motion parallel to Earth's radius and the free-air correction to local gravity magnifies its apparent motion by 12%. For data from the Sumatra-Andaman earthquake an apparent initial amplitude of 55 μm for 0 S 0 shrinks to 49 μm after this correction. Similar corrections must be made for all modal amplitudes at frequencies f = 1000 s) including corrections for motion-induced accelerations associated with tilt and redistribution of Earth's mass. For instance the true vertical motion of the football mode 0 S 2 is 81.2% that computed from the seismometer response alone.

The instrumental self-noise of the broadband seismometers used in global seismic networks increases at low frequencies. Earth's gravest free oscillations have therefore been studied primarily with superconducting gravimeter data not seismometer records after correction for fluctuations in atmospheric pressure ( 28 59 – 61 ). The signal-to-noise ratio for seismometer records of the 23 June 2001 Peru event ( M w = 8.4) was not high enough to allow the observation of hybridized toroidal modes on the vertical seismic components but they are evident for the 2004 Sumatra-Andaman earthquake.

10.1029/JB084iB05p02348

S. Stein M. Wysession An Introduction to Seismology Earthquakes and Earth Structure (Blackwell Scientific Malden MA 2003).

M. Ishii P. Shearer H. Houston J. Vidale Nature in press.

R. Bilham E. R. Engdahl N. Feldl S. P. Satyabala Seism. Res. Lett. in press.

Synthetics are computed according to normal-mode perturbation theory ( 16 ). Perturbations from a spherical nonrotating Earth model such as rotation ellipticity and lateral heterogeneity are included. We adopt mantle model S20RTS ( 53 ) and crustal model crust2.0 ( 54 ) to account for lateral heterogeneity. The latest estimates of spheroidal and toroidal eigenfrequencies and quality factors are used in the calculation ( 55 ). Modal splitting and coupling due to rotation ellipticity and lateral heterogeneity are accounted for on the basis of a group coupling scheme using 36 subgroups of 117 modes below 3 mHz ( 56 ).

J. Ritsema, H. J. van Heijst, Sci. Prog. (New Haven)83, 243 (2000).

C. Bassin, G. Laske, G. Masters, Eos81 (Fall Meeting Suppl.), F897 (abstr. S21A-03) (2000).

The Reference Earth Model Web site is at http://mahi.ucsd.edu/Gabi/rem.html.

10.1046/j.1365-246X.2001.00502.x

10.1016/0031-9201(94)90039-6

10.1029/2003GL017639

10.1029/95GL03369

M. Van Camp, Phys. Earth Planet. Inter.116, 81 (2000).

10.1029/2003GL018304

This work was supported in part by NSF. Seismic waveform data from the Global Seismographic Network (funded by NSF and U.S. Geological Survey) were obtained from the Incorporated Research Institutions for Seismology (IRIS) Data Management System. Seismic waveform data was also obtained from the Geoscope Program (IPGP France) and the Southern California Earthquake Center.