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Download Volume II Accomplisments (28 Mb pdf). - IRIS

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Upper Mantle Structure of Southern Africa from Rayleigh Wave<br />

Tomography with 2-D Sensitivity Kernels<br />

Aibing Li (University of Houston)<br />

A 3-D shear wave model in southern Africa has been developed from fundamental mode Rayleigh wave phase velocities,<br />

which are computed at the period range of 20 to 167 s using a two-plane-wave tomography method. 2-D sensitivity kernels are<br />

applied in the phase velocity inversion to account for finite-frequency effects, which are significant at periods greater than 100<br />

s. The new model (Figure 1 and 2) confirms the first-order observations found by Li and Burke [2006], a fast mantle lid extending<br />

to ~180 km depth and being underlain by a low velocity zone. One new feature in the model is the vertical alignment of a<br />

shallow low velocity anomaly with a deep high velocity anomaly at the western Bushveld province. The alignment makes more<br />

sense for interpreting the slow as the result of high iron content from the Bushveld intrusion and the fast as a more depleted<br />

residual mantle. A low velocity channel at the depths of 220-310 km from the southern end of the Kheiss belt to the northwest<br />

of the Kaapvaal craton is also imaged for the first time. It suggests that the hot asthenosphere outside the craton could migrate<br />

into the craton area through a weak channel and thermally erode the cratonic lithosphere from below. In addition, low velocity<br />

anomalies from 100 to 180 km agree well with the localities of kimberlites erupted at 65-104 Ma in the Kaapvaal craton, providing<br />

additional evidence for the depth extent of mantle xenoliths.<br />

References<br />

Li, A., and K. Burke (2006), Upper mantle structure of southern Africa from Rayleigh wave tomography, J. Geophys. Res., 111, B10303,<br />

doi:10.1029/2006JB004321.<br />

Jelsma, H. A., M. J. De Wit, C. Thiart, P. H. Dirks, G. Viola, I. J. Basson, and E. Anckar (2004), Preferential distribution along transcontinental<br />

corridors of kimberlites and related rocks of Southern Africa, S. Afr. J. Geol., 107, 301-324.<br />

Yang, Y., and D.W. Forsyth (2006), Regional tomographic inversion of amplitude and phase of Rayleigh waves with 2-D sensitivity kernels,<br />

Geophys. J. Int., 166, 1148-1160.<br />

Acknowledgements: Data used in this study are from the <strong>IRIS</strong> DMC. Yingjie Yang kindly provided the inversion codes with 2-D sensitivity kernels.<br />

This research is supported by NSF grant EAR-0645503.<br />

Figure 1. Shear-wave velocity variations at 4 depth ranges. Black squares delineate<br />

the sites of kimberlites at 104 to 65 Ma based on Fig. 7c in Jelsma et al.<br />

(2004), which show a better correlation with slow regions in shallow upper mantle<br />

(a and b). Red lines show the locations of profiles in Figure. 2. Dashed lines<br />

are tectonic boundaries.<br />

Figure 2. Shear-wave velocity profiles at the depths of 50-300 km. A relative low<br />

velocity zone appears on all profiles at roughly 160-260 km depths. (a-c) Velocity<br />

profiles of AA', BB' and CC' from this study. (d) Shear-wave velocity profile along<br />

CC' from the study of Li & Burke (2006). Note the good alignment of the shallow,<br />

slow anomaly and the deep, fast anomaly at the distance of 8 degree in (c),<br />

which is not well imaged in (d).<br />

2010 <strong>IRIS</strong> Core Programs Proposal | <strong>Volume</strong> <strong>II</strong> | Upper Mantle Structure and Dynamics | <strong>II</strong>-201

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