Results 121 to 130 of about 4,233 (235)
On effect of precession-induced flows in the liquid core for early Earth's history [PDF]
Nonlinear Processes in Geophysics, 2006 Secondary and tertiary flow patterns seen in experiments simulating flow in the Earth's liquid core induced by luni-solar precession of the solid mantle (Vanyo et al., 1995) hint at the development of non-axisymmetric columnar periodic structures. A
S. L. Shalimov, S. L. Shalimov
doaj
The scientific case for magnetic field satellites [PDF]
To make full use of modern magnetic data and the paleomagnetic record, we must greatly improve our understanding of how the geodynamo system works. It is clearly nonlinear, probably chaotic, and its dimensionless parameters cannot yet be reproduced on a ...
Backus, George E. +3 more
core +1 more source
Turbulent geodynamo simulations: a leap towards Earth’s core [PDF]
, 2017 Nathanaël Schaeffer +3 more
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Low inertia reversing geodynamos
Physics of the Earth and Planetary InteriorsConvection driven geodynamo models in rotating spherical geometry have regimes in which reversals occur. However, reversing dynamo models are usually found in regimes where the kinetic and magnetic energy is comparable, so that inertia is playing a significant role in the dynamics.
Jones CA, Tsang Y-K
openaire +3 more sources
, 2012 Using Lagrangian formalism we consider evolution of the ensemble of interacting magnetohydrodynamic cyclones governed with Langevin type equations in the rotating medium. This problem is relevant to the planetary cores where the Rossby numbers are small and geostrophic balance takes place.
Hejda, P., Reshetnyak, M.
openaire +2 more sources
Testing the Magnetohydrodynamic Analysis Software with Natural Convection and Geodynamo Problems
, 2021 И. В. Бычин
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Detecting dipolarity of the geomagnetic field in the paleomagnetic record. [PDF]
Proc Natl Acad Sci U S A, 2023 Lhuillier F, Shcherbakov VP, Sycheva NK.
europepmc +1 more source
Core formation, evolution, and convection: A geophysical model [PDF]
A model is proposed for the formation and evolution of the Earth's core which provides an adequate energy source for maintaining the geodynamo. A modified inhomogeneous accretion model is proposed which leads to initial iron and refractory enrichment at ...
Anderson, D. L., Ruff, L.
core +1 more source
Preferential axisymmetric field growth in kinematic geodynamo models [PDF]
, 2004 Philip W. Livermore, Andrew Jackson
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