Lithospheric Boundaries and Upper Mantle Structure Beneath Southern Africa Imaged by P and S Wave Velocity Models

Abstract We report new P and S wave velocity models of the upper mantle beneath southern Africa using data recorded on seismic stations spanning the entire subcontinent. Beneath most of the Damara Belt, including the Okavango Rift, our models show lower than average velocities (−0.8% Vp; −1.2% Vs) w...

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Main Authors: A. L. White‐Gaynor, A. A. Nyblade, R. Durrheim, R. Raveloson, M. van derMeijde, I. Fadel, H. Paulssen, M. Kwadiba, O. Ntibinyane, N. Titus, M. Sitali
Format: Article
Language:English
Published: Wiley 2020-10-01
Series:Geochemistry, Geophysics, Geosystems
Subjects:
Online Access:https://doi.org/10.1029/2020GC008925
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author A. L. White‐Gaynor
A. A. Nyblade
R. Durrheim
R. Raveloson
M. van derMeijde
I. Fadel
H. Paulssen
M. Kwadiba
O. Ntibinyane
N. Titus
M. Sitali
author_facet A. L. White‐Gaynor
A. A. Nyblade
R. Durrheim
R. Raveloson
M. van derMeijde
I. Fadel
H. Paulssen
M. Kwadiba
O. Ntibinyane
N. Titus
M. Sitali
author_sort A. L. White‐Gaynor
collection DOAJ
description Abstract We report new P and S wave velocity models of the upper mantle beneath southern Africa using data recorded on seismic stations spanning the entire subcontinent. Beneath most of the Damara Belt, including the Okavango Rift, our models show lower than average velocities (−0.8% Vp; −1.2% Vs) with an abrupt increase in velocities along the terrane's southern margin. We attribute the lower than average velocities to thinner lithosphere (~130 km thick) compared to thicker lithosphere (~200 km thick) immediately to the south under the Kalahari Craton. Beneath the Etendeka Flood Basalt Province, higher than average velocities (0.25% Vp; 0.75% Vs) indicate thicker and/or compositionally distinct lithosphere compared to other parts of the Damara Belt. In the Rehoboth Province, higher than average velocities (0.3% Vp; 0.5% Vs) suggest the presence of a microcraton, as do higher than average velocities (1.0% Vp; 1.5% Vs) under the Southern Irumide Belt. Lower than average velocities (−0.4% Vp; −0.7% Vs) beneath the Bushveld Complex and parts of the Mgondi and Okwa terranes are consistent with previous studies, which attributed them to compositionally modified lithosphere resulting from Precambrian magmatic events. There is little evidence for thermally modified upper mantle beneath any of these terranes which could provide a source of uplift for the Southern African Plateau. In contrast, beneath parts of the Irumide Belt in southern and central Zambia and the Mozambique Belt in central Mozambique, deep‐seated low velocity anomalies (−0.7% Vp; −0.8% Vs) can be attributed to upper mantle extensions of the African superplume structure.
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spelling doaj.art-e6ab10f2f0594e02b8c94e96ad26fb7d2023-11-03T16:55:21ZengWileyGeochemistry, Geophysics, Geosystems1525-20272020-10-012110n/an/a10.1029/2020GC008925Lithospheric Boundaries and Upper Mantle Structure Beneath Southern Africa Imaged by P and S Wave Velocity ModelsA. L. White‐Gaynor0A. A. Nyblade1R. Durrheim2R. Raveloson3M. van derMeijde4I. Fadel5H. Paulssen6M. Kwadiba7O. Ntibinyane8N. Titus9M. Sitali10Department of Geosciences The Pennsylvania State University University Park PA USADepartment of Geosciences The Pennsylvania State University University Park PA USASchool of Geosciences The University of Witwatersrand Johannesburg South AfricaSchool of Geosciences The University of Witwatersrand Johannesburg South AfricaFaculty of Geo‐Information Science and Earth Observation (ITC) University of Twente Enschede NetherlandsFaculty of Geo‐Information Science and Earth Observation (ITC) University of Twente Enschede NetherlandsDepartment of Earth Sciences Utrecht University Utrecht NetherlandsBotswana Geosciences Institute Lobatse BotswanaBotswana Geosciences Institute Lobatse BotswanaGeological Survey of Namibia Windhoek NamibiaGeological Survey of Namibia Windhoek NamibiaAbstract We report new P and S wave velocity models of the upper mantle beneath southern Africa using data recorded on seismic stations spanning the entire subcontinent. Beneath most of the Damara Belt, including the Okavango Rift, our models show lower than average velocities (−0.8% Vp; −1.2% Vs) with an abrupt increase in velocities along the terrane's southern margin. We attribute the lower than average velocities to thinner lithosphere (~130 km thick) compared to thicker lithosphere (~200 km thick) immediately to the south under the Kalahari Craton. Beneath the Etendeka Flood Basalt Province, higher than average velocities (0.25% Vp; 0.75% Vs) indicate thicker and/or compositionally distinct lithosphere compared to other parts of the Damara Belt. In the Rehoboth Province, higher than average velocities (0.3% Vp; 0.5% Vs) suggest the presence of a microcraton, as do higher than average velocities (1.0% Vp; 1.5% Vs) under the Southern Irumide Belt. Lower than average velocities (−0.4% Vp; −0.7% Vs) beneath the Bushveld Complex and parts of the Mgondi and Okwa terranes are consistent with previous studies, which attributed them to compositionally modified lithosphere resulting from Precambrian magmatic events. There is little evidence for thermally modified upper mantle beneath any of these terranes which could provide a source of uplift for the Southern African Plateau. In contrast, beneath parts of the Irumide Belt in southern and central Zambia and the Mozambique Belt in central Mozambique, deep‐seated low velocity anomalies (−0.7% Vp; −0.8% Vs) can be attributed to upper mantle extensions of the African superplume structure.https://doi.org/10.1029/2020GC008925seismic tomographysouthern Africa plateauupper mantlelithospheric structure
spellingShingle A. L. White‐Gaynor
A. A. Nyblade
R. Durrheim
R. Raveloson
M. van derMeijde
I. Fadel
H. Paulssen
M. Kwadiba
O. Ntibinyane
N. Titus
M. Sitali
Lithospheric Boundaries and Upper Mantle Structure Beneath Southern Africa Imaged by P and S Wave Velocity Models
Geochemistry, Geophysics, Geosystems
seismic tomography
southern Africa plateau
upper mantle
lithospheric structure
title Lithospheric Boundaries and Upper Mantle Structure Beneath Southern Africa Imaged by P and S Wave Velocity Models
title_full Lithospheric Boundaries and Upper Mantle Structure Beneath Southern Africa Imaged by P and S Wave Velocity Models
title_fullStr Lithospheric Boundaries and Upper Mantle Structure Beneath Southern Africa Imaged by P and S Wave Velocity Models
title_full_unstemmed Lithospheric Boundaries and Upper Mantle Structure Beneath Southern Africa Imaged by P and S Wave Velocity Models
title_short Lithospheric Boundaries and Upper Mantle Structure Beneath Southern Africa Imaged by P and S Wave Velocity Models
title_sort lithospheric boundaries and upper mantle structure beneath southern africa imaged by p and s wave velocity models
topic seismic tomography
southern Africa plateau
upper mantle
lithospheric structure
url https://doi.org/10.1029/2020GC008925
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