TY - JOUR
T1 - Quantifying the Relationship Between Short-Wavelength Dynamic Topography and Thermomechanical Structure of the Upper Mantle Using Calibrated Parameterization of Anelasticity
AU - Richards, Fred D.
AU - Hoggard, Mark J.
AU - White, Nicky
AU - Ghelichkhan, Siavash
N1 - Publisher Copyright:
©2020. The Authors.
PY - 2020/9/1
Y1 - 2020/9/1
N2 - Oceanic residual depth varies on (Formula presented.) 5,000 km wavelengths with amplitudes of ±1 km. A component of this short-wavelength signal is dynamic topography caused by convective flow in the upper ∼300 km of the mantle. It exerts a significant influence on landscape evolution and sea level change, but its contribution is often excluded in geodynamic models of whole-mantle flow. Using seismic tomography to resolve buoyancy anomalies in the oceanic upper mantle is complicated by the dominant influence of lithospheric cooling on velocity structure. Here, we remove this cooling signal from global surface wave tomographic models, revealing a correlation between positive residual depth and slow residual velocity anomalies at depths <300 km. To investigate whether these anomalies are of sufficient amplitude to account for short-wavelength residual depth variations, we calibrate an experimentally derived parameterization of anelastic deformation at seismic frequencies to convert shear wave velocity into temperature, density, and diffusion creep viscosity. Asthenospheric temperature anomalies reach +150°C in the vicinity of major magmatic hot spots and correlate with geochemical and geophysical proxies for potential temperature along mid-ocean ridges. Locally, we find evidence for a ∼150 km-thick, low-viscosity asthenospheric channel. Incorporating our revised density structure into models of whole-mantle flow yields reasonable agreement with residual depth observations and suggests that ±30 km deviations in local lithospheric thickness account for a quarter of total amplitudes. These predictions remain compatible with geoid constraints and substantially improve the fit between power spectra of observed and predicted dynamic topography. This improvement should enable more accurate reconstruction of the spatiotemporal evolution of Cenozoic dynamic topography.
AB - Oceanic residual depth varies on (Formula presented.) 5,000 km wavelengths with amplitudes of ±1 km. A component of this short-wavelength signal is dynamic topography caused by convective flow in the upper ∼300 km of the mantle. It exerts a significant influence on landscape evolution and sea level change, but its contribution is often excluded in geodynamic models of whole-mantle flow. Using seismic tomography to resolve buoyancy anomalies in the oceanic upper mantle is complicated by the dominant influence of lithospheric cooling on velocity structure. Here, we remove this cooling signal from global surface wave tomographic models, revealing a correlation between positive residual depth and slow residual velocity anomalies at depths <300 km. To investigate whether these anomalies are of sufficient amplitude to account for short-wavelength residual depth variations, we calibrate an experimentally derived parameterization of anelastic deformation at seismic frequencies to convert shear wave velocity into temperature, density, and diffusion creep viscosity. Asthenospheric temperature anomalies reach +150°C in the vicinity of major magmatic hot spots and correlate with geochemical and geophysical proxies for potential temperature along mid-ocean ridges. Locally, we find evidence for a ∼150 km-thick, low-viscosity asthenospheric channel. Incorporating our revised density structure into models of whole-mantle flow yields reasonable agreement with residual depth observations and suggests that ±30 km deviations in local lithospheric thickness account for a quarter of total amplitudes. These predictions remain compatible with geoid constraints and substantially improve the fit between power spectra of observed and predicted dynamic topography. This improvement should enable more accurate reconstruction of the spatiotemporal evolution of Cenozoic dynamic topography.
KW - Earth rheology
KW - anelasticity
KW - dynamic topography
KW - lithosphere-asthenosphere system
KW - mantle dynamics
KW - mantle thermomechanical structure
UR - http://www.scopus.com/inward/record.url?scp=85091485604&partnerID=8YFLogxK
U2 - 10.1029/2019JB019062
DO - 10.1029/2019JB019062
M3 - Article
SN - 2169-9313
VL - 125
JO - Journal of Geophysical Research: Solid Earth
JF - Journal of Geophysical Research: Solid Earth
IS - 9
M1 - e2019JB019062
ER -