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Lg-wave attenuation in the Australian crust
We estimate the Lg-wave quality factor (Q) across the Australian continent from vertical-component Lg waveforms. A tomographic inversion is performed to construct an Lg attenuation model for 58 frequencies between 0.05 and 10.0Hz. The available spatial resolution is approximately 1.5°×1.5° for the 0...
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Published in: | Tectonophysics 2017-10, Vol.717, p.413-424 |
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Main Authors: | , , |
Format: | Article |
Language: | English |
Subjects: | |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
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Summary: | We estimate the Lg-wave quality factor (Q) across the Australian continent from vertical-component Lg waveforms. A tomographic inversion is performed to construct an Lg attenuation model for 58 frequencies between 0.05 and 10.0Hz. The available spatial resolution is approximately 1.5°×1.5° for the 0.5–2.0Hz band. At 1.0Hz, the Lg-wave Q over the whole island continent varies from 50 to 1250 with an average value of 850. Significant regional variations in the Lg-wave Q images tie well with many geological features and boundaries in Australia. The cratons in western, northern and southern parts of Australia usually have higher Q values (700–1250), while the volcanic regions, sedimentary basins and orogenic areas in eastern Australia are characterized by increased attenuation (lower Q values, 50–650). We determine the frequency-dependent Q of Lg waves for different blocks across Australia, and find the frequency dependence of Q is much more complex than the traditional single power law representation. When combined with the assumed geometrical spreading relation, the Lg Q maps provide a new way of assessing potential ground motion across the continent for any event location.
•An Lg attenuation model is constructed for the Australian crust.•Variations of Lg-wave Q tie well with the Australian geological features.•Frequency dependence of Lg Q varies in different geological areas.•Lg Q maps provide a new way of assessing potential ground motion in Australia. |
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ISSN: | 0040-1951 1879-3266 |
DOI: | 10.1016/j.tecto.2017.08.022 |