Implication of the lopsided growth for the viscosity of Earth's inner core
Hugau Mizzon, Marc Monnereau

TL;DR
This study investigates how the interplay between translation and convection in Earth's inner core affects seismic anisotropy and viscosity, revealing that high viscosity favors translation-driven asymmetry, while lower viscosity promotes convection.
Contribution
It introduces a 3D spherical model analyzing the combined effects of translation and convection on inner core anisotropy and viscosity, highlighting the conditions under which each mode dominates.
Findings
Pure translation dominates at viscosities >10^{20} Pas.
Convection dominates at viscosities <10^{18} Pas.
Mixed behavior occurs at intermediate viscosities.
Abstract
Two main seismic features characterize the Earth's inner core: a North-South polar anisotropy and an East-West asymmetry of P-wave velocity and attenuation. Anisotropy is expected if shear deformation is induced by convective motions. Translation has recently been put forward as an important mode of convection of the inner core. Combined with a simple diffusive grain growth model, this mechanism is able to explain the observed seismic asymmetry, but not the bulk anisotropy. The source of anisotropy has therefore to be sought in the shear motions caused by higher modes of convection. Using a hybrid finite-difference spherical harmonics Navier-Stokes solver, we investigate the interplay between translation and convection in a 3D spherical model with permeable boundary conditions at the inner core boundary. Three parameters act independently: viscosity, internal heating and convection…
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