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Published September 1, 2018 | Supplemental Material
Journal Article Open

A long-lived Indian Ocean slab: Deep dip reversal induced by the African LLSVP

Abstract

A slab-like high seismic velocity anomaly (referred as SEIS) has been inferred beneath the central-southern Indian Ocean in a recent tomographic inversion. Although subduction has previously been suggested regionally by surface observations, the new inversion is consistent with a north-dipping slab extending from the upper mantle to the core mantle boundary (CMB). We propose that SEIS anomaly originated from an oceanic plate in the Paleo-Tethys that was consumed by a south-dipping intra-oceanic subduction zone during the Triassic and Jurassic periods. SEIS challenges traditional concepts of the dynamics of slab descent by its relatively shallow depths and a present-day polarity opposite to the geometry of subduction. Geodynamic models show the upwelling mantle flow exerted by a thermochemical pile can hold and stagnate the descending SEIS slab at shallow depths for more than 100 Myr. The spatial distribution of resistance from the upwelling mantle flow can reverse the slab dip, producing a structure consistent with seismic inversions as well as with our proposed tectonic scenario and geology constraining the Tethyan tectonic domain. The results suggest that slabs can descend through the lower mantle at rates substantially lower than 1 cm/yr, and even reverse their polarity through interactions with background mantle flow.

Additional Information

© 2018 Elsevier B.V. Received 31 October 2017, Revised 28 May 2018, Accepted 30 May 2018, Available online 15 June 2018. We thank two anonymous reviewers for their invaluable comments and suggestions. We also thank Nathan Simmons for earlier discussions on the origin of the SEIS and Kara Matthews for discussions of Tethyan reconstructions. HW and MG were supported by the National Science Foundation through EAR-1600956 and EAR-1645775 and by Statoil ASA. YW participated through the Visiting Undergraduate Research Program (VURP) at Caltech. SZ was supported by the Australian Research Council through IH130200012. The original CitcomS code is obtained from Computational Infrastructure for Geodynamics (http://geodynamics.org).

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