DETERMINATION OF CRUSTAL STRUCTURE IN CENTRAL AUSTRALIA BY INVERSION OF TRAVEL-TIME RESIDUALS

Citation
Hws. Mcqueen et K. Lambeck, DETERMINATION OF CRUSTAL STRUCTURE IN CENTRAL AUSTRALIA BY INVERSION OF TRAVEL-TIME RESIDUALS, Geophysical journal international, 126(3), 1996, pp. 645-662
Citations number
31
Categorie Soggetti
Geochemitry & Geophysics
ISSN journal
0956540X
Volume
126
Issue
3
Year of publication
1996
Pages
645 - 662
Database
ISI
SICI code
0956-540X(1996)126:3<645:DOCSIC>2.0.ZU;2-9
Abstract
Teleseismic traveltime anomalies for events recorded on portable seism ograph arrays across the northern and southern margins of the Amadeus Basin in central Australia are inverted to obtain a picture of the vel ocity structure at a scale on the order of 5-10 km. A modified SIRT al gorithm is used to iteratively redistribute traveltime anomalies along incoming ray paths, subject to regularization constraints, to obtain a direct estimate of the lithospheric velocity field beneath the array s. Model structure is assumed to be 2-D, based on the strong east-west strike of surface geology and gravity structure in the area. Spurious structures commonly generated in SIRT inversions are suppressed using a filter based on the density of rays. A weighting towards near-surfa ce structure is also applied to test the robustness of the inference o f deep structures.The most prominent feature of the solutions for all three lines is a sharp interface between slow and fast regions, dippin g away from the basin and beneath the adjacent basement blocks. The fa stest region, on the upper side of the interface, corresponds to a bel t of high-grade metamorphic rocks where they crop out at the surface. The interface between slow and fast regions extends to at least 50 km depth in all cases, dipping at about 50-60 degrees on the northern lin es and 60-80 degrees on the southern line. On the northern lines the i nterface can be correlated with the Redbank Thrust identified in deep seismic reflection data, but the velocity interface seems to dip more steeply. Secondary features on the profiles include a possible change in dip of the interface on the southern line and a more complex struct ure on one of the northern lines, suggesting that one or more steeper faults cut through the hanging wall of the thrust there. Predicted gra vity profiles derived from the velocity sections using empirical veloc ity-density relations resemble observed gravity surprisingly well in t heir style and approximate magnitude, providing support for the genera l features of the models. The results are consistent with a thick-skin ned thrusting model for the deformation of the central segment of the basin margins and indicate that the style of deformation in the Late P roterozoic-Cambrian compressional event at the southern edge of the Am adeus Basin was similar to that in the later Alice Springs Orogeny in the north.