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
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.