Welcome to the new version of CaltechAUTHORS. Login is currently restricted to library staff. If you notice any issues, please email coda@library.caltech.edu
Published October 2011 | Published
Journal Article Open

Lithospheric structure beneath the Zagros collision zone resolved by non-linear teleseismic tomography

Abstract

The upper-mantle structure across the Zagros collision zone, in southwest Iran, is investigated using a non-linear weighted damped least-squares teleseismic tomography approach. The resolution of the structures/transitions in the upper mantle is enhanced significantly by correcting the teleseismic relative arrival time residuals for an a priori crustal velocity model and then performing the inversion with fixed crustal blocks. To investigate whether or not the lithospheric blocks and major transitions in the resulting model are required by the data or are artefacts of the inversion, the data were inverted using two different inverse methods (singular value decomposition and a quadratic programming method). New high-quality seismic velocity models show apparent correlation between surface geological features and seismic velocity structures at lithospheric depth across the Zagros collision zone. The image shows a sharp lithospheric boundary at the Main Zagros Thrust between 100 km and 250 km depth with P-wave velocity about 3 per cent faster within the Arabian Shield to the south. A step-like increase in lithospheric thickness across the Zagros collision zone is assumed to separate two different mantle structures namely the Arabian (to the south) and the Eurasian (to the north) domains. The most striking feature resolved is a north-dipping slab-like positive velocity anomaly.

Additional Information

© 2011 The Authors. Geophysical Journal International © 2011 RAS. Accepted 2011 July 11. Received 2011 July 11; in original form 2010 April 6. Article first published online: 8 Aug. 2011. Seismological data used in this paper were retrieved from the data management centre of the French portable seismic instrument pool hosted by LGIT (Grenoble University-CNRS), http://bdsis.obs.ujfgrenoble.fr/. We thank C. Péquegnat and H. Pedersen (LGIT Grenoble) for their valuable help. Some figures were made using the Generic Mapping Tools (GMT) version 4.2.1 (Wessel & Smith 1998; www.soest.hawaii.edu/gmt, last accessed 2010 August). We would also like to thank the Associate Editor, Gabi Laske, and four anonymous reviewers for their constructive comments and useful suggestions. We also thank Roland Roberts (Department of Earth Sciences, Uppsala University, Sweden) and Faramarz Tutti (Department of Geology, University of Tehran, Iran) for their valuable comments on the manuscript.

Attached Files

Published - Shomali2011p16031Geophys_J_Int.pdf

Files

Shomali2011p16031Geophys_J_Int.pdf
Files (1.3 MB)
Name Size Download all
md5:5985aec83ded04ec88b5b5491b6101d2
1.3 MB Preview Download

Additional details

Created:
August 22, 2023
Modified:
October 24, 2023