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Published February 2020 | Supplemental Material + Published
Journal Article Open

Numerical Modeling of Mantle Flow Beneath Madagascar to Constrain Upper Mantle Rheology Beneath Continental Regions

Abstract

Over the past few decades, azimuthal seismic anisotropy measurements have been widely used proxy to study past and present‐day deformation of the lithosphere and to characterize convection in the mantle. Beneath continental regions, distinguishing between shallow and deep sources of anisotropy remains difficult due to poor depth constraints of measurements and a lack of regional‐scale geodynamic modeling. Here, we constrain the sources of seismic anisotropy beneath Madagascar where a complex pattern cannot be explained by a single process such as absolute plate motion, global mantle flow, or geology. We test the hypotheses that either Edge‐Driven Convection (EDC) or mantle flow derived from mantle wind interactions with lithospheric topography is the dominant source of anisotropy beneath Madagascar. We, therefore, simulate two sets of mantle convection models using regional‐scale 3‐D computational modeling. We then calculate Lattice Preferred Orientation that develops along pathlines of the mantle flow models and use them to calculate synthetic splitting parameters. Comparison of predicted with observed seismic anisotropy shows a good fit in northern and southern Madagascar for the EDC model, but the mantle wind case only fits well in northern Madagascar. This result suggests the dominant control of the measured anisotropy may be from EDC, but the role of localized fossil anisotropy in narrow shear zones cannot be ruled out in southern Madagascar. Our results suggest that the asthenosphere beneath northern and southern Madagascar is dominated by dislocation creep. Dislocation creep rheology may be dominant in the upper asthenosphere beneath other regions of continental lithosphere.

Additional Information

© 2019 The Authors. This is an open access article under the terms of the Creative Commons Attribution‐NonCommercial‐NoDerivs License, which permits use and distribution in any medium, provided the original work is properly cited, the use is non‐commercial and no modifications or adaptations are made. Received 16 AUG 2019; Accepted 22 DEC 2019; Accepted article online 27 DEC 2019. This work has been supported by the National Science Foundation (NSF) grant EAR‐1551864. Most figures in this paper have been generated with Generic Mapping Tools V5.4.2 (Wessel et al., 2013). We also created one figure with VISIT v2.9 developed by the Lawrence Livermore National Laboratory. The predicted anisotropy model output files are available at the PANGAEA repository with doi:10.1594/PANGAEA.909406. The mantle flow model are available at the Open Science Framework repository with doi:10.17605/OSF.IO/TEJM4. We thank the Computational Infrastructure for Geodynamics for supporting the development of ASPECT, which is funded by National Science Foundation Awards EAR‐0949446 and EAR‐1550901.

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Published - 2019JB018560.pdf

Supplemental Material - jgrb53943-sup-0002-text_si-s01.pdf

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August 22, 2023
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