Results 101 to 110 of about 270,968 (216)
Earth and Mars Interior Structures Set by Remelting of the First Solid Mantle
Magma-ocean crystallization sets up the early structure and long-term evolution of terrestrial planets. Recent seismic evidence signals the presence of a silicate layer at the base of Mars’s mantle. Magma-ocean crystallization and subsequent overturn has
Antonio Manjón-Cabeza Córdoba +2 more
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Evolution of the continental upper mantle : numerical modelling of thermo-chemical convection including partial melting [PDF]
This thesis elaborates on the evolution of the continental upper mantle based on numerical modelling results. The descriptive and explanatory basis is formed by a numerical thermo-chemical convection model.
Mantle dynamics & theoretical geophysics +3 more
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Convection in fluid and porous media [PDF]
The subject of convection in fluid and porous media is investigated. Particular attention is paid to penetrative convection. The first two chapters are devoted to penetrative convection when fluid overlies and saturates a porous medium.
Carr, Magda
core
Thermal, Elastic and Seismic Signature of High-Resolution Mantle Circulation Models [PDF]
A long-standing question in the study of Earth’s deep interior is the origin of seismic mantle heterogeneity. The challenge is to efficiently mine the wealth of information available in complex seismic waveforms and to separate the potential ...
Schuberth, Bernhard
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Long-range slab interaction controls trench advance in double-subduction systems
Subduction is a fundamental process that drives plate tectonics. The dynamics of subducting slabs strongly influence trench migration, mantle flow, and the thermal and compositional structure of the mantle.
Haoyuan Li, Magali I. Billen
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Energy balance of mantle convection
A calculation of the thermodynamic efficiency of a convecting upper mantle with finite strength is extended to the lower mantle by appealing to the non-equilibrium ellipticity for a value of strength.
Stacey, F. D.
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Accelerating the Discovery of Steady‐States of Planetary Interior Dynamics With Machine Learning
Simulating mantle convection often requires reaching a computationally expensive steady‐state, crucial for deriving scaling laws for thermal and dynamical flow properties and benchmarking numerical solutions.
Siddhant Agarwal +4 more
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Constraints on thermo-chemical convection from numerical modelling and geophysical data. Geologica Ultraectina (298) [PDF]
In modern geoscience, mounting evidence in support of large-scale lateral variations in the composition of Earth's deep mantle has fueled the debate on the structure and evolution of mantle convection.
Kwantitatieve seismologie: naar een nieuw begrip van het diepe binnenste van de aarde +4 more
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Polar Motion Dynamics on Slow‐Rotating Venus: Signatures of Mantle Flow
With its 1 day lasting 243 days on Earth, Venus is the slowest‐spinning planet in the Solar System and its rotational bulge is anomalously small. A rotational bulge stabilizes the orientation of planets. Having only a tiny stabilizer, the rotational pole
Vojtěch Patočka +2 more
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