Articles | Volume 11, issue 3
https://doi.org/10.5194/se-11-959-2020
© Author(s) 2020. This work is distributed under
the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
https://doi.org/10.5194/se-11-959-2020
© Author(s) 2020. This work is distributed under
the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
On the self-regulating effect of grain size evolution in mantle convection models: application to thermochemical piles
Jana Schierjott
CORRESPONDING AUTHOR
Institute for Geophysics, Department of Earth Sciences, Sonneggstrasse 5, 8092 Zurich, Switzerland
Antoine Rozel
Institute for Geophysics, Department of Earth Sciences, Sonneggstrasse 5, 8092 Zurich, Switzerland
Paul Tackley
Institute for Geophysics, Department of Earth Sciences, Sonneggstrasse 5, 8092 Zurich, Switzerland
Related authors
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Paul J. Tackley
EGUsphere, https://doi.org/10.5194/egusphere-2025-1543, https://doi.org/10.5194/egusphere-2025-1543, 2025
This preprint is open for discussion and under review for Geoscientific Model Development (GMD).
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Large density jumps in numerical simulations of solid Earth dynamics can cause numerical oscillations. An effective method to prevent these at a free surface already exists. Here this is tested for compositional layers deeper in the mantle. The stabilisation method works effectively if density gradients due purely to compositional gradients are used, but produces severe artefacts if total density is used.
Paul James Tackley
EGUsphere, https://doi.org/10.5194/egusphere-2025-1354, https://doi.org/10.5194/egusphere-2025-1354, 2025
This preprint is open for discussion and under review for Geoscientific Model Development (GMD).
Short summary
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Tracers are commonly used in geodynamical models to track composition, but a common problem is that over time, gaps in the tracer distribution can develop, as well as bunches. Here a method to correct such problems is presented and tested. The method perturbs or “nudges” the positions of tracers in such a way as to close gaps and eliminate bunching. Test results show that this tracer nudging method is highly effective. The computational cost is small.
Joshua Martin Guerrero, Frédéric Deschamps, Yang Li, Wen-Pin Hsieh, and Paul James Tackley
Solid Earth, 14, 119–135, https://doi.org/10.5194/se-14-119-2023, https://doi.org/10.5194/se-14-119-2023, 2023
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The mantle thermal conductivity's dependencies on temperature, pressure, and composition are often suppressed in numerical models. We examine the effect of these dependencies on the long-term evolution of lower-mantle thermochemical structure. We propose that depth-dependent conductivities derived from mantle minerals, along with moderate temperature and compositional correction, emulate the Earth's mean lowermost-mantle conductivity values and produce a stable two-pile configuration.
Anna Johanna Pia Gülcher, Maxim Dionys Ballmer, and Paul James Tackley
Solid Earth, 12, 2087–2107, https://doi.org/10.5194/se-12-2087-2021, https://doi.org/10.5194/se-12-2087-2021, 2021
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The lower mantle extends from 660–2890 km depth, making up > 50 % of the Earth’s volume. Its composition and structure, however, remain poorly understood. In this study, we investigate several hypotheses with computer simulations of mantle convection that include different materials: recycled, dense rocks and ancient, strong rocks. We propose a new integrated style of mantle convection including
piles,
blobs, and
streaksthat agrees with various observations of the deep Earth.
Daniela Paz Bolrão, Maxim D. Ballmer, Adrien Morison, Antoine B. Rozel, Patrick Sanan, Stéphane Labrosse, and Paul J. Tackley
Solid Earth, 12, 421–437, https://doi.org/10.5194/se-12-421-2021, https://doi.org/10.5194/se-12-421-2021, 2021
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We use numerical models to investigate the thermo-chemical evolution of a solid mantle during a magma ocean stage. When applied to the Earth, our study shows that the solid mantle and a magma ocean tend toward chemical equilibration before crystallisation of this magma ocean. Our findings suggest that a very strong chemical stratification of the solid mantle is unlikely to occur (as predicted by previous studies), which may explain why the Earth’s mantle is rather homogeneous in composition.
Robert I. Petersen, Dave R. Stegman, and Paul J. Tackley
Solid Earth, 8, 339–350, https://doi.org/10.5194/se-8-339-2017, https://doi.org/10.5194/se-8-339-2017, 2017
Short summary
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In this study we propose a dichotomy in the strength profile of tectonic plates. This apparent dichotomy suggests that plates at the Earth's surface are significantly stronger, by orders of magnitude, than the subducted slabs in the Earth's interior. Strong plates promote single-sided, Earth-like subduction. Once subducted, strong slabs transmit dynamic stresses and disrupt subduction. Slabs which are weakened do not disrupt subduction and furthermore exhibit a variety of observed morphologies.
Related subject area
Subject area: Mantle and core structure and dynamics | Editorial team: Structural geology and tectonics, paleoseismology, rock physics, experimental deformation | Discipline: Geodynamics
The impact of rheological uncertainty on dynamic topography predictions
Ömer F. Bodur and Patrice F. Rey
Solid Earth, 10, 2167–2178, https://doi.org/10.5194/se-10-2167-2019, https://doi.org/10.5194/se-10-2167-2019, 2019
Short summary
Short summary
Convection in the deep Earth dynamically changes the elevation of plates. Amplitudes of those vertical motions predicted from numerical models are significantly higher than observations. We find that at small wavelengths (< 1000 km) this misfit can be due to the oversimplification in viscosity of rocks. By a suite of numerical experiments, we show that considering the non–Newtonian rheology of the mantle results in predictions in amplitude of dynamic topography consistent with observations.
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Short summary
We investigate the size of mineral grains of Earth's rocks in computer models of the whole Earth. This is relevant because grain size affects the stiffness (large grains are stiffer) and deformation of the Earth's mantle. We see that mineral grains grow inside stable non-deforming regions of the Earth. However, these regions are less stiff than expected. On the other hand, we find that grain size diminishes during deformation events such as when surface material comes down into the Earth.
We investigate the size of mineral grains of Earth's rocks in computer models of the whole...