Structure of the Mt Isa region from seismic ambient noise tomography

被引:4
作者
Saygin, E. [1 ]
McQueen, H. [1 ]
Hutton, L. J. [2 ]
Kennett, B. L. N. [1 ]
Lister, G. [1 ]
机构
[1] Australian Natl Univ, Res Sch Earth Sci, Canberra, ACT 0200, Australia
[2] Geol Survey Queensland, Dept Nat Resources & Mines, Brisbane, Qld 4000, Australia
基金
澳大利亚研究理事会;
关键词
Mt Isa; Australia; lithosphere; Proterozoic; seismology; ambient seismic noise tomography; LITHOSPHERIC STRUCTURE; WAVE TOMOGRAPHY; UPPER-MANTLE; EVOLUTION; INSIGHTS; QUEENSLAND; ANISOTROPY; AUSTRALIA; BENEATH; FORM;
D O I
10.1080/08120099.2013.837098
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
We use seismic tomography, exploiting group velocities derived from ambient noise, to delineate the crustal structure beneath Mt Isa and the surrounding blocks and basins. The depth extent of the blocks can be traced into the mid-crust and the spatial extent of the associated velocity anomalies mapped over an area of approximately 500km by 500km. The Proterozoic Mt Isa block is imaged as a region of elevated seismic velocities comparable to the Yilgarn craton in Western Australia, while the surrounding basins have relatively low velocities. Seismic velocity anomalies display correlations with the regional Bouguer gravity data and with high crustal temperatures in the region. There are a number of isolated low-velocity anomalies under the Millungera basin that suggest either previously unknown thermal anomalies or zones with high permeability, which can also produce lowered velocities.
引用
收藏
页码:707 / 718
页数:11
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