4.6 Article

On the measurement of S-diff splitting caused by lowermost mantle anisotropy

期刊

GEOPHYSICAL JOURNAL INTERNATIONAL
卷 233, 期 2, 页码 900-921

出版社

OXFORD UNIV PRESS
DOI: 10.1093/gji/ggac490

关键词

Numerical modelling; Planetary interiors; Computational seismology; Seismic anisotropy; Wave propagation

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This article discusses the feasibility of using S-diff waves to infer lowermost mantle anisotropy. The authors use global wavefield simulations to analyze the influence of various factors on S-diff polarizations and evaluate the effects of seismic anisotropy in both the upper and the lowermost mantle on SHdiff waves. The research results demonstrate that the effects of anisotropy can be clearly distinguished through the splitting parameters of S-diff waves.
Seismic anisotropy has been detected at many depths of the Earth, including its upper layers, the lowermost mantle and the inner core. While upper mantle seismic anisotropy is relatively straightforward to resolve, lowermost mantle anisotropy has proven to be more complicated to measure. Due to their long, horizontal ray paths along the core-mantle boundary (CMB), S waves diffracted along the CMB(S-diff) are potentially strongly influenced by lowermostmantle anisotropy. S-diff waves can be recorded over a large epicentral distance range and thus sample the lowermost mantle everywhere around the globe. S-diff therefore represents a promising phase for studying lowermost mantle anisotropy; however, previous studies have pointed out some difficulties with the interpretation of differential SHdiff-SVdiff traveltimes in terms of seismic anisotropy. Here, we provide a new, comprehensive assessment of the usability of S-diff waves to infer lowermost mantle anisotropy. Using both axisymmetric and fully 3-D global wavefield simulations, we showthat there are cases inwhich S-diff can reliably detect and characterize deep mantle anisotropy when measuring traditional splitting parameters (as opposed to differential traveltimes). First, we analyze isotropic effects on S-diff polarizations, including the influence of realistic velocity structure (such as 3-D velocity heterogeneity and ultra-low velocity zones), the character of the lowermost mantle velocity gradient, mantle attenuation structure, and Earth's Coriolis force. Secondly, we evaluate effects of seismic anisotropy in both the upper and the lowermost mantle on SHdiff waves. In particular, we investigate how SHdiff waves are split by seismic anisotropy in the upper mantle near the source and how this anisotropic signature propagates to the receiver for a variety of lowermost mantle models. We demonstrate that, in particular and predictable cases, anisotropy leads to S-diff splitting that can be clearly distinguished from other waveform effects. These results enable us to lay out a strategy for the analysis of S-diff splitting due to anisotropy at the base of the mantle, which includes steps to help avoid potential pitfalls, with attention paid to the initial polarization of S-diff and the influence of source-side anisotropy. We demonstrate our S-diff splitting method using three earthquakes that occurred beneath the Celebes Sea, measured at many transportable array stations at a suitable epicentral distance. We resolve consistent and well-constrained S-diff splitting parameters due to lowermost mantle anisotropy beneath the northeastern Pacific Ocean.

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