The crustal structure of the Madagascar Ridge

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Abstract

Summary. The Madagascar Ridge is an elongated aseismic plateau in the southwest Indian Ocean, which separates two ocean basins of mid‐to late Cretaceous age. From interpretations of a reversed refraction line on the ridge and a continuous gravity profile across it we conclude that it formed during the Cretaceous as thickened oceanic crust, at a mid‐ocean ridge which possibly overlay a mantle hot‐spot. The seismic data consist of record sections from five recording sonobuoys. Forty‐one shots were fired along a 210 km long NNE—SSW line across the central part of the ridge. Simple horizontal‐layer analysis of first arrivals reveals a lower crustal refractor with Vp= 7 kms−1 at a depth of 8–8.5 km and the Moho at an apparent depth of 18 km, but fails to characterize the crustal structure as either oceanic or continental. We obtain a definitively oceanic structure by using synthetic seismogram techniques together with Tau(p) analysis and second arrival correlations. The model which best fits the data consists of 2.2 km of water and 1 km of sediments overlying a velocity gradient from 4 to 7 kms−1. Beneath this, at a depth of 7.5 km, is a 9.5 km thick layer with Vp= 6.9–7.1 kms−1. A 7.5 kms−1 layer, not observed in the first arrival analysis, is found at the base of the crust. The Moho is a transition zone 1 km thick and occurs at ∼ 25 km depth. The gravity data consist of a continuous NE—SW profile across the ridge and on to the flanking basins. Two‐dimensional gravity modelling allows a structure consistent with the synthetic seismogram results, and supports the existence of a high‐density basal layer in the crust. We use in addition a time‐series analysis approach to estimate the depth of compensation assuming an Airy model, and lithospheric thickness assuming an elastic plate model. Convolution of bathymetry along the profile with a range of model filters gives minimum rms gravity residuals for a crustal compensation depth of 23 ± 5 km, and a plate thickness of less than 2–5 km. Copyright © 1981, Wiley Blackwell. All rights reserved

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Sinha, M. C., Louden, K. E., & Parsons, B. (1981). The crustal structure of the Madagascar Ridge. Geophysical Journal of the Royal Astronomical Society, 66(2), 351–377. https://doi.org/10.1111/j.1365-246X.1981.tb05960.x

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