2018
DOI: 10.1029/2018gc007516
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On the Scales of Dynamic Topography in Whole‐Mantle Convection Models

Abstract: Mantle convection shapes Earth's surface by generating dynamic topography. Observational constraints and regional convection models suggest that surface topography could be sensitive to mantle flow for wavelengths as short as 1,000 and 250 km, respectively. At these spatial scales, surface processes including sedimentation and relative sea‐level change occur on million‐year timescales. However, time‐dependent global mantle flow models do not predict small‐scale dynamic topography yet. Here we present 2‐D spher… Show more

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Cited by 29 publications
(29 citation statements)
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“…While it is still a question whether plate-like velocities can be modelled with this approach, recent advances using continental rafts suggest Earth-like convective vigor may be in reach (e.g., Coltice et al 2013;Arnould et al 2018;Rolf et al 2018).…”
Section: Discussionmentioning
confidence: 99%
“…While it is still a question whether plate-like velocities can be modelled with this approach, recent advances using continental rafts suggest Earth-like convective vigor may be in reach (e.g., Coltice et al 2013;Arnould et al 2018;Rolf et al 2018).…”
Section: Discussionmentioning
confidence: 99%
“…An interesting alternative is the use of the "yield-stress" rheology (e.g., Tackley 2000) which has been demonstrated to lead to plate-like behavior without the requirement of prescribing the geometry of the plates. While it is still a question whether plate-like velocities can be modeled with this approach, recent advances using continental rafts suggest Earth-like convective vigor may be in reach (e.g., Arnould et al 2018;Coltice et al 2013;and Rolf et al 2018).…”
Section: Discussionmentioning
confidence: 99%
“…We solve the equations of mass, momentum and energy conservation under the Boussinesq approximation:where v is velocity, p is pressure, η is viscosity, T is temperature and C is composition. H is the mantle internal heat production rate, α is a depth-dependent thermal expansivity coefficient set as in Arnould et al 2018 56 , B is the chemical buoyancy ratio and e r is the radial unit vector. The Rayleigh number of the system is:where α 0 is the surface thermal expansivity, D the mantle’s thickness, g the gravitational acceleration, Δ T the temperature gradient across the mantle, ρ 0 the reference density, η 0 the reference viscosity and κ the reference thermal diffusivity.…”
Section: Methodsmentioning
confidence: 99%