Effects of rheological parameters on the stability of thermochemical piles: A comparison of different origins

Large low shear velocity provinces have been observed beneath Africa and the Pacific. These large-scale structures are considered to have been stable the last hundred million years with their origin and nature still being an open question. In our 2D Cartesian study, we numerically investigate the temporal and spatial stability of thermochemical piles. We consider two different scenarios, in which the piles either arise from a primordial layer above the core-mantle boundary (CMB) or from an influx of iron-rich material through the CMB. The investigated mantle flow depends on viscosity varying with composition, depth, and stress. The rheological parameters affect the strength of convection and consequently the stability of piles. An increased top or bottom viscosity reduces the convective vigor yielding longer-lived and more stable piles. Likewise, a thermal expansivity decreasing with depth exhibits longer pile lifetimes and less pile movement. Furthermore, piles and plumes are two closely linked structures. While thermochemical plumes are anchored by piles, thermal plumes attract piles and deform them. Long-lived plumes tend to be located in the center of piles, but during dynamical processes, such as merging of piles, plumes also occur at the edges remaining there for several million years. In summary, we suggest that the LLSVPs might have formed early after the magma ocean, probably as several initially thin structures due to strong convection in the hot Archean mantle. With the cooling of the mantle, the structures would have broadened and stabilized in space and time, yielding the present-day state. • Stability of piles forming from a primordial layer or by core-mantle interaction. • Similar behavior for both scenarios but influx structures tend to be smaller. • Long-lived and stable piles are achieved with an increased top or bottom viscosity. • Large plumes sit in the center of piles but temporally also occur at their edges. • Plumes outside of thermochemical piles can attract and deform these.

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Publication Details

Journal
Physics of The Earth and Planetary Interiors
Published
2025-12-03
DOI
https://doi.org/10.1016/j.pepi.2025.107476
Primary Topic
High-pressure geophysics and materials
Type
article
Field-Weighted Citation Impact
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article

Effects of rheological parameters on the stability of thermochemical piles: A comparison of different origins

Claudia Stein, Christoph Weber, Ulrich Hansen, Henry W. Sitte
Physics of The Earth and Planetary Interiors
High-pressure geophysics and materials
article

Effects of rheological parameters on the stability of thermochemical piles: A comparison of different origins

Claudia Stein, Christoph Weber, Ulrich Hansen, Henry W. Sitte
article en

Abstract

Large low shear velocity provinces have been observed beneath Africa and the Pacific. These large-scale structures are considered to have been stable the last hundred million years with their origin and nature still being an open question. In our 2D Cartesian study, we numerically investigate the temporal and spatial stability of thermochemical piles. We consider two different scenarios, in which the piles either arise from a primordial layer above the core-mantle boundary (CMB) or from an influx of iron-rich material through the CMB. The investigated mantle flow depends on viscosity varying with composition, depth, and stress. The rheological parameters affect the strength of convection and consequently the stability of piles. An increased top or bottom viscosity reduces the convective vigor yielding longer-lived and more stable piles. Likewise, a thermal expansivity decreasing with depth exhibits longer pile lifetimes and less pile movement. Furthermore, piles and plumes are two closely linked structures. While thermochemical plumes are anchored by piles, thermal plumes attract piles and deform them. Long-lived plumes tend to be located in the center of piles, but during dynamical processes, such as merging of piles, plumes also occur at the edges remaining there for several million years. In summary, we suggest that the LLSVPs might have formed early after the magma ocean, probably as several initially thin structures due to strong convection in the hot Archean mantle. With the cooling of the mantle, the structures would have broadened and stabilized in space and time, yielding the present-day state. • Stability of piles forming from a primordial layer or by core-mantle interaction. • Similar behavior for both scenarios but influx structures tend to be smaller. • Long-lived and stable piles are achieved with an increased top or bottom viscosity. • Large plumes sit in the center of piles but temporally also occur at their edges. • Plumes outside of thermochemical piles can attract and deform these.

Physics of The Earth and Planetary InteriorsVol. 370
University of Münster (DE)
Openalex Percentile: Top 61%
High-pressure geophysics and materials
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