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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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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The adjoint equations for thermochemical compressible mantle convection: derivation and verification by twin experiments. [PDF]
Ghelichkhan S, Bunge HP.
europepmc +1 more source
Continuous reorientation of synchronous terrestrial planets due to mantle convection. [PDF]
Leconte J.
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We developed a numerical model of thermal convection of highly viscous incompressible fluids, aiming at reproducing plate tectonics in the framework of mantle convection.
Hiroki Taito +3 more
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A rapid tectonic plate reorganization event driven by changes at subduction locations in a mantle convection model. [PDF]
Guerrero JM +4 more
europepmc +1 more source
Effect of bridgmanite-ferropericlase grain size evolution on Earth's average mantle viscosity: implications for mantle convection in early and present-day Earth. [PDF]
Paul J +5 more
europepmc +1 more source
Deep mantle anomalies block early Earth melting, challenging a primordial origin. [PDF]
Roy A, Mittelstaedt E, Cooper CM.
europepmc +1 more source

