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Seismic structure of the crust and uppermost mantle of the Capricorn and Paterson Orogens and adjacent cratons, Western Australia, from passive seismic transects
Citation
Reading, AM and Tkalcic, H and Kennett, BLN and Johnson, SP and Sheppard, S, Seismic structure of the crust and uppermost mantle of the Capricorn and Paterson Orogens and adjacent cratons, Western Australia, from passive seismic transects, Precambrian Research, 196-197 pp. 295-308. ISSN 0301-9268 (2012) [Refereed Article]
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Copyright Statement
Copyright 2011 Elsevier B.V.
DOI: doi:10.1016/j.precamres.2011.07.001
Abstract
The seismic structure of the Proterozoic Capricorn and Paterson Orogens and adjacent Archaean Yilgarn
and Pilbara Cratons, Western Australia, is determined using a passive seismic approach. We use
recordings of distant earthquakes made along two transects of 3-component broadband stations. The
stations were deployed for approximately 1 year (mid 20062007) during which time 70 earthquakes
were recorded at each station with a suitable signal to noise ratio for receiver function analysis and hence
the S wavespeed profiles of the crust and uppermost mantle beneath each recording station are determined.
We investigate the deep crustal constraints on terrane boundary locations, the patterns of seismic
discontinuities in the crust, and the variations in the depth and character of the Moho. This broad-scale
information regarding the present day crustal architecture, and hence the crustal evolution, of Western
Australia, complements previous surface geological and other geophysical studies. Western Australia is
an exceptionally large, well preserved region of ancient crust and hence this work also adds to the body
of knowledge regarding Proterozoic orogenic processes in general. The new passive seismic work shows
a region of double crust or upper mantle discontinuities beneath the Glenburgh Terrane, adjacent to the
northwest Yilgarn Craton. The upper crust of the orogens is always layered whereas the cratons have a
simple upper crust. Both the Capricorn and Paterson Orogens are characterised by deeper Moho discontinuities
with a lesser wavespeed contrast than the very sharp discontinuity observed beneath the adjacent
Pilbara and Yilgarn Cratons. This is consistent with the weaker orogenic crust of the Capricorn and Paterson
Orogens accommodating most of the horizontal deformation during assembly and reworking of the
West Australian Craton while the Pilbara and Yilgarn Cratons acted as rigid crustal blocks.
Item Details
Item Type: | Refereed Article |
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Keywords: | Capricorn Orogen, Paterson Orogen, Proterozoic, crustal structure, passive seismic, receiver function |
Research Division: | Earth Sciences |
Research Group: | Geophysics |
Research Field: | Seismology and seismic exploration |
Objective Division: | Expanding Knowledge |
Objective Group: | Expanding knowledge |
Objective Field: | Expanding knowledge in the earth sciences |
UTAS Author: | Reading, AM (Professor Anya Reading) |
ID Code: | 78259 |
Year Published: | 2012 |
Web of Science® Times Cited: | 21 |
Deposited By: | Centre for Ore Deposit Research - CODES CoE |
Deposited On: | 2012-06-19 |
Last Modified: | 2017-10-25 |
Downloads: | 7 View Download Statistics |
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