LgCoda Q in Australia and its Relation to Crustal Structure and Evolution
LgCoda Q in Australia and its Relation to Crustal Structure and Evolution
复制标题
DOI:
10.1007/s000240050211
复制
发表时间:
1998-12
影响因子:
2
通讯作者:
B. Mitchell;S. Baqer;A. Akinci;L. Cong
中科院分区:
文献类型:
--
作者:
B. Mitchell;S. Baqer;A. Akinci;L. Cong
We have determinedLgCodaQLgc) from ground motion recorded at seven broadband stations in Australia, using a stacked spectral ratio method. In spite of the relatively small number of events and less than optimum station coverage, we were able to use those data to obtain a tomographic mapQLgcand its frequency dependence, at 1 Hz for almost the entire island continent.QLgcat 1 Hz in Australia varies between about 330 and 600. The lowest values (330–400) characterize the Tasman Fold Belt in eastern Australia; these may be associated with fluids produced by orogenic activity that occurred during the Devonian and Carboniferous periods or by sedimentation that occurred in Jurassic and Triassic times. Smaller reductions ofQLgc, relative to maximum values, in central and western Australia, may be associated with sedimentation that occurred over a long-time interval between late Precambrian time and the Carboniferous period or with deformation that occurred in the Central Australian Mobile Belts during the Carboniferous.QLgcthroughout most of Australia is 30 to 60% lower than it is in most other stable continental regions. Assuming thatQLgcvaries in the same proportion asQLg, ground motion computations for one-dimensional models of the Australian crust and upper mantle indicate that up to 20% reductions inQLgccan be produced if a velocity gradient, rather than a sharp boundary, resides at the crust-mantle transition. The remaining portion of theQLgcreduction may be caused by lateral variability in the thickness, depth, and severity of the velocity gradient which causes additional Lg energy to leak into the mantle.