Abstract

Abstract. High-velocity lower crust (HVLC) and seaward-dipping reflector (SDR) sequences are typical features of volcanic rifted margins. However, the nature and origin of HVLC is under discussion. Here we provide a comprehensive analysis of deep crustal structures in the southern segment of the South Atlantic and an assessment of HVLC along the margins. Two new seismic refraction lines off South America fill a gap in the data coverage and together with five existing velocity models allow for a detailed investigation of the lower crustal properties on both margins. An important finding is the major asymmetry in volumes of HVLC on the conjugate margins. The seismic refraction lines across the South African margin reveal cross-sectional areas of HVLC 4 times larger than at the South American margin, a finding that is opposite to the asymmetric distribution of the flood basalts in the Paraná–Etendeka Large Igneous Province. Also, the position of the HVLC with respect to the SDR sequences varies consistently along both margins. Close to the Falkland–Agulhas Fracture Zone in the south, a small body of HVLC is not accompanied by SDRs. In the central portion of both margins, the HVLC is below the inner SDR wedges while in the northern area, closer to the Rio Grande Rise-Walvis Ridge, large volumes of HVLC extend far seaward of the inner SDRs. This challenges the concept of a simple extrusive/intrusive relationship between SDR sequences and HVLC, and it provides evidence for formation of the HVLC at different times during the rifting and breakup process. We suggest that the drastically different HVLC volumes are caused by asymmetric rifting in a simple-shear-dominated extension.

Highlights

  • A lower crustal zone with high density and high seismic P -wave velocity is part of the magmatic “trinity” that characterizes volcanic rifted margins: continental flood basalts, seaward-dipping reflector (SDR) sequences and high-velocity lower crust (HVLC) (e.g., Menzies et al, 2002; White et al, 1987; Talwani and Abreu, 2000)

  • This brings up two important questions: how did the strong asymmetry of magmatism develop during rifting and breakup in the South Atlantic, and why is there such a difference in the sense of asymmetry from the offshore and onshore evidence? One point to consider is that the Paraná–Etendeka Large Igneous Province is a feature of the northern end of the margins only and not necessarily related to the Atlantic rifting which started in a magma-poor setting in the south

  • Two new refraction seismic models complemented by gravity models fill a gap in the data coverage on the Argentine margin and prove the existence of high-velocity lower crust (HVLC; Vp > 7.0)

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Summary

Introduction

A lower crustal zone with high density and high seismic P -wave velocity is part of the magmatic “trinity” that characterizes volcanic rifted margins: continental flood basalts, seaward-dipping reflector (SDR) sequences and high-velocity lower crust (HVLC) (e.g., Menzies et al, 2002; White et al, 1987; Talwani and Abreu, 2000). HVLC at volcanic rifted margins is thought to represent magmatic (gabbroic) intrusions and related cumulate layers (Farnetani et al, 1996; Furlong and Fountain, 1986; Kelemen and Holbrook, 1995; White and McKenzie, 1989; Thybo and Artemieva, 2013). HVLC can make up a large part of the total magmatic output along volcanic rifted margins, and as studies in the North Atlantic have shown, variations in size and physical properties of the HVLC in these settings hold important clues to mantle melting scenarios (Fernàndez et al, 2010; Kelemen and Holbrook, 1995; Korenaga et al, 2002; Ridley and Richards, 2010; Voss et al, 2009; White et al, 2008). The development of SDR sequences is roughly symmetrical, and there are variations in the relative position of HVLC bodies with respect to the SDRs which question a simple intrusive vs. extrusive relationship and have implications for the timing of HVLC formation relative to rifting and breakup

Geologic framework
Existing profiles and interpretation
Seismic velocity
Checkerboard tests and resolution
Gravity models
Distribution and geometric analysis of the HVLC
Origin of the HVLC bodies
Relationship of HVLC and SDR sequences
Asymmetry of magmatism and implications for the breakup process
Conclusions
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