Title
Internal deformation of the subducted Nazca slab inferred from seismic anisotropy
Date Issued
01 January 2016
Access level
open access
Resource Type
journal article
Author(s)
Eakin C.M.
Long M.D.
Scire A.
Beck S.L.
Wagner L.S.
Zandt G.
Publisher(s)
Nature Publishing Group
Abstract
Within oceanic lithosphere a fossilized fabric is often preserved originating from the time of plate formation. Such fabric is thought to form at the mid-ocean ridge when olivine crystals align with the direction of plate spreading. It is unclear, however, whether this fossil fabric is preserved within slabs during subduction or overprinted by subduction-induced deformation. The alignment of olivine crystals, such as within fossil fabrics, can generate anisotropy that is sensed by passing seismic waves. Seismic anisotropy is therefore a useful tool for investigating the dynamics of subduction zones, but it has so far proved difficult to observe the anisotropic properties of the subducted slab itself. Here we analyse seismic anisotropy in the subducted Nazca slab beneath Peru and find that the fast direction of seismic wave propagation aligns with the contours of the slab. We use numerical modelling to simulate the olivine fabric created at the mid-ocean ridge, but find it is inconsistent with our observations of seismic anisotropy in the subducted Nazca slab. Instead we find that an orientation of the olivine crystal fast axes aligned parallel to the strike of the slab provides the best fit, consistent with along-strike extension induced by flattening of the slab during subduction (A. Kumar et al., manuscript in preparation). We conclude that the fossil fabric has been overprinted during subduction and that the Nazca slab must therefore be sufficiently weak to undergo internal deformation.
Start page
56
End page
59
Volume
9
Issue
1
Language
English
OCDE Knowledge area
Ingeniería ambiental y geológica Geología Ingeniería oceanográfica
Scopus EID
2-s2.0-84951762604
Source
Nature Geoscience
ISSN of the container
17520894
Sponsor(s)
The PULSE deployment was facilitated by the PASSCAL program of IRIS (Incorporated Research Institutions for Seismology) and the data was accessed through the IRIS Data Management Center (DMC). We thank all those from Yale University, University of North Carolina—Chapel Hill, University of Arizona and the Instituto Geofísico del Perú (IGP) who participated in the fieldwork. We thank R. Clayton and P. Davis for providing access to data from PeruSE stations. We acknowledge helpful discussions and suggestions by S. Karato on modelling anisotropy within the slab. The PULSE experiment was supported by National Science Foundation grants EAR-0943962 (M.D.L.), EAR-0944184 (L.S.W.), and EAR-0943991 (S.L.B.).
Sources of information: Directorio de Producción Científica Scopus