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Australian Journal of Earth Sciences
An International Geoscience Journal of the Geological Society of Australia
Volume 53, 2006 - Issue 4
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Original Articles

Insights into the structure of the upper mantle beneath the Murray basin from 3D teleseismic tomography

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Pages 595-604 | Received 28 Jul 2005, Accepted 30 Jan 2006, Published online: 19 Feb 2007
 

Abstract

Distant earthquake records from a passive array of 20 short-period seismometers are used to image the 3D P-wave velocity structure of the upper mantle beneath the Murray Basin in southern New South Wales and northern Victoria. During the five-month deployment period of the array, 158 teleseisms with good signal-to-noise ratios were recorded, allowing 3085 relative arrival time residuals to be picked with high accuracy. These arrival time residuals are mapped as 3D perturbations in P-wave velocity with respect to the ak135 global reference model using teleseismic tomography. The resulting images exhibit lateral variations in wave speed in the upper mantle to depths of nearly 300 km, and help to reveal the deep structure beneath a region almost devoid of Palaeozoic outcrop. Of particular significance is an east – west high – low – high relative wave speed variation that is present throughout the upper mantle between 70 and 250 km depth. The transition from faster to slower wave speeds in the west is indicative of a change from Proterozoic to Phanerozoic lithosphere that has also been observed further south in a previous teleseismic study. The transition from slower to faster wave speeds in the east has a less obvious association, but may well signal an underlying change in lithospheric structure related to the convergence of the western and central Lachlan subprovinces. At shallower depths (<70 km), the structural pattern is dominated by a fast perturbation (>3.5%) which overlies the slower region across the northern margin of the Bendigo Zone, and may be a consequence of localised thrusting and emplacement of denser lithosphere during the Early – Middle Devonian Tabberabberan Orogeny.

Acknowledgements

We would like to thank Tony Percival, Armando Arcidiaco and Erdinc Saygin for assistance with the deployment of short-period seismometers in the field. We also thank the many private landowners for their generous permission in allowing us to install instruments on their property. The use of short-period seismic equipment from the ANSIR Major National Research Facility is gratefully acknowledged. D. Gray and S. Hearn are thanked for providing constructive reviews of the submitted manuscript. The SEAL experiment was supported by ARC grant DP0342618. NR and MH are supported by ARC grants DP0556282 and DP0342618, respectively.

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