Abstract

Abstract. We evaluate the spatial and temporal evolution of Earth's long-wavelength surface dynamic topography since the Jurassic using a series of high-resolution global mantle convection models. These models are Earth-like in terms of convective vigour, thermal structure, surface heat-flux and the geographic distribution of heterogeneity. The models generate a degree-2-dominated spectrum of dynamic topography with negative amplitudes above subducted slabs (i.e. circum-Pacific regions and southern Eurasia) and positive amplitudes elsewhere (i.e. Africa, north-western Eurasia and the central Pacific). Model predictions are compared with published observations and subsidence patterns from well data, both globally and for the Australian and southern African regions. We find that our models reproduce the long-wavelength component of these observations, although observed smaller-scale variations are not reproduced. We subsequently define geodynamic rules for how different surface tectonic settings are affected by mantle processes: (i) locations in the vicinity of a subduction zone show large negative dynamic topography amplitudes; (ii) regions far away from convergent margins feature long-term positive dynamic topography; and (iii) rapid variations in dynamic support occur along the margins of overriding plates (e.g. the western US) and at points located on a plate that rapidly approaches a subduction zone (e.g. India and the Arabia Peninsula). Our models provide a predictive quantitative framework linking mantle convection with plate tectonics and sedimentary basin evolution, thus improving our understanding of how subduction and mantle convection affect the spatio-temporal evolution of basin architecture.

Highlights

  • At short spatial scales, Earth’s topography depends on interactions between crustal structures, tectonic deformation and surface processes

  • Note that to calculate dynamic topography, we focus on long-wavelength subduction-driven global flow below the lithosphere, as this is the contribution to dynamic topography that does not depend on the specific structure of the lithosphere and the depth of the lithosphere– asthenosphere boundary

  • We varied the blanking temperature of 2150 K, but since the chosen temperature is applied to the entire spherical shell, it is always neutral with respect to the mantle buoyancy structure and the amplitude of dynamic topography does not depend on the specific temperature choice

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Summary

Introduction

Earth’s topography depends on interactions between crustal structures, tectonic deformation and surface processes. Colli et al (2016) demonstrate that mantle convection with a depthdependent viscosity generates small perturbations (geoid 37 m; gravity 8 mGal), considerable dynamic topography (1.1 km) and a gravitational admittance of mostly less than 10 mGal km−1 This supports the idea that relatively small long-wavelength free-air gravity anomalies do not preclude dynamic topography at amplitudes substantially larger than 300 m. Present-day dynamic topography is discussed on a global scale by Ricard et al (1993), Steinberger (2007), Zhang et al (2012) and Flament et al (2013), but relatively few studies We propose a categorisation of regions on Earth’s surface in terms of their exposure to the effects of dynamic support over the past 200 Myr, which is corroborated by an automated classification technique

Model set-up
Model robustness
Predicted mantle structure
Global and regional dynamic topography
Global models of dynamic topography
Australia
Southern Africa
Modes of long-term dynamic surface topography evolution
Category I – Topographic stable areas
Category II – Dynamically subsiding areas
Category III – Fluctuating areas
Cluster analysis
Conclusions
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