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Frequency-dependent effects on global S-wave traveltimes: wavefront-healing, scattering and attenuation

Authors :
Zaroli, Christophe
Debayle, Eric
Sambridge, Malcolm
Ecole et Observatoire des Sciences de la Terre (EOST)
Université de Strasbourg (UNISTRA)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)
Laboratoire de Sciences de la Terre (LST)
Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Claude Bernard Lyon 1 (UCBL)
Université de Lyon-Université de Lyon-École normale supérieure - Lyon (ENS Lyon)
Research School of Earth Sciences [Canberra] (RSES)
Australian National University (ANU)
École normale supérieure de Lyon (ENS de Lyon)-Université Claude Bernard Lyon 1 (UCBL)
Université de Lyon-Université de Lyon-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)
Source :
Geophysical Journal International, Geophysical Journal International, Oxford University Press (OUP), 2010, 182 (2), pp.1025-1042. ⟨10.1111/j.1365-246X.2010.04667.x⟩, Geophysical Journal International, 2010, 182 (2), pp.1025-1042. ⟨10.1111/j.1365-246X.2010.04667.x⟩
Publication Year :
2010
Publisher :
HAL CCSD, 2010.

Abstract

International audience; We present a globally distributed data set of similar to 400 000 frequency-dependent SH-wave trayeltimes. An automated technique is used to measure teleseismic S, ScS and SS traveltimes at several periods ranging from 10 to 51 s. The targeted seismic phases are first extracted from the observed and synthetic seismograms using an automated time window algorithm. Traveltimes are then measured at several periods, by cross-correlation between the selected observed and synthetic filtered waveforms. Frequency-dependent effects due to crustal reverberations beneath each receiver are handled by incorporating crustal phases into WKBJ synthetic waveforms. After correction for physical dispersion due to intrinsic anelastic processes, we observe a residual traveltime dispersion on the order of 1-2 s in the period range of analysis. This dispersion occurs differently for S, ScS and SS, which is presumably related to their differing paths through the Earth. We find that: (1) Wavefront-healing phenomenon is observed for S and to a lesser extent SS waves having passed through very low velocity anomalies. (2) A preferred sampling of high velocity scatterers located at the CMB may explain our observation that ScS waves travel faster at low-frequency than at high-frequency. (3) A frequency-dependent attenuation q(w) proportional to q(0) x w(-alpha), with alpha similar to 0.2, is compatible with the globally averaged dispersion observed for S waves.

Details

Language :
English
ISSN :
0956540X and 1365246X
Database :
OpenAIRE
Journal :
Geophysical Journal International, Geophysical Journal International, Oxford University Press (OUP), 2010, 182 (2), pp.1025-1042. ⟨10.1111/j.1365-246X.2010.04667.x⟩, Geophysical Journal International, 2010, 182 (2), pp.1025-1042. ⟨10.1111/j.1365-246X.2010.04667.x⟩
Accession number :
edsair.dedup.wf.001..5f0b1735b5b471f4a74e1d445becb3f2
Full Text :
https://doi.org/10.1111/j.1365-246X.2010.04667.x⟩