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The irregular polarity reversals of the Earth's magnetic field have attracted much interest during the last decades. Despite the fact that recent numerical simulations of the geodynamo have shown nice polarity transitions, the very reason…

地球物理 · 物理学 2007-05-23 F. Stefani , G. Gerbeth , U. Guenther

We study a simple magnetohydrodynamical approach in which hydrodynamics and MHD turbulence are coupled in a shell model, with given dynamo constrains in the large scales. We consider the case of a low Prandtl number fluid for which the…

地球与行星天体物理 · 物理学 2015-05-13 Roberto Benzi , Jean-Francois Pinton

One of the most intriguing features of Earth's axial magnetic dipole field, well-known from the geological record, is its occasional and unpredictable reversal of polarity. Understanding the phenomenon is rendered very difficult by the…

地球物理 · 物理学 2019-01-02 Christian R. Scullard , Bruce A. Buffett

The geodynamo usually appears as a somewhat intimidating subject. Its understanding seems to require the intricate theory of magnetohydrodynamics. The solution of the corresponding equations can only be achieved numerically. It seems to be…

科普物理 · 物理学 2020-09-30 Friedrich Herrmann , Tobias Vorbach

In a recent paper (Phys. Rev. Lett. 94 (2005), 184506; physics/0411050) it was shown that a simple mean-field dynamo model with a spherically symmetric helical turbulence parameter alpha can exhibit a number of features which are typical…

地球物理 · 物理学 2007-05-23 Frank Stefani , Gunter Gerbeth , Uwe Guenther , Mingtian Xu

Differential rotation is widely supposed to be essential for the dynamo effects that sustain solar and planetary magnetic fields, but dynamo effects tend to oppose the flows that drive them, and it is uncertain what drives differential…

天体物理学 · 物理学 2009-07-10 Bertrand C. Barrois

We argue that global magnetic field reversals similar to those observed in the Milky Way occur quite frequently in mean-field galactic dynamo models that have relatively strong, random, seed magnetic fields that are localized in discrete…

星系天体物理 · 物理学 2015-06-11 David Moss , Dmitri Sokoloff

Geomagnetic field reversals remain as one of the most intriguing problems in geophysics and are regarded as chaotic processes resulting from a dynamo mechanism. In this article, we use the polarity scale data set for the last 170 Myr from…

The existence of magnetohydrodynamic mean-field alpha^2-dynamos with spherically symmetric, isotropic helical turbulence function alpha is related to a non-self-adjoint spectral problem for a coupled system of two singular second order…

数学物理 · 物理学 2014-11-20 Uwe Guenther , Heinz Langer , Christiane Tretter

The variable magnetic field of the solar photosphere exhibits periodic reversals as a result of dynamo activity occurring within the solar interior. We decompose the surface field as observed by both the Wilcox Solar Observatory and the…

太阳与恒星天体物理 · 物理学 2015-06-11 M. L. DeRosa , A. S. Brun , J. T. Hoeksema

The asymmetric time dependence and various statistical properties of polarity reversals of the Earth's magnetic field are utilized to infer some of the most essential parameters of the geodynamo, among them the effective (turbulent)…

地球物理 · 物理学 2009-05-15 Michael Fischer , Gunter Gerbeth , Andre Giesecke , Frank Stefani

We report the first experimental observation of reversals of a dynamo field generated in a laboratory experiment based on a turbulent flow of liquid sodium. The magnetic field randomly switches between two symmetric solutions B and -B. We…

We study the process of magnetic reversals in the presence of a stably-stratified layer below the core-mantle boundary using direct numerical simulations of the incompressible magnetohydrodynamics equations under the Boussinesq…

流体动力学 · 物理学 2026-01-22 Nicolás Pablo Müller , Christophe Gissinger , François Pétrélis

Numerical simulations of the geodynamo in presence of an heterogeneous heating are presented. We study the dynamics and the structure of the magnetic field when the equatorial symmetry of the flow is broken. If the symmetry breaking is…

流体动力学 · 物理学 2012-03-20 Christophe Gissinger , Ludovic Petitdemange , Martin Schrinner , Emmanuel Dormy

Two non-local asymptotic invariants of magnetic fields for the ideal magnetohydrodynamics are introduced. The velocity of variation of the invariants for a non-ideal magnetohydrodynamics with a small magnetic dissipation is estimated. By…

数学物理 · 物理学 2011-10-06 Petr M. Akhmet'ev

The inverse problem for electromagnetic field produced by arbitrary altered charge distribution in dipole approximation is solved. The charge distribution is represented by its dipole moment. It is assumed that the spectral properties of…

经典物理 · 物理学 2015-05-06 V. Epp , J. G. Janz

The rapid rotation of planets causes cyclonic thermal turbulence in their cores which may generate the large-scale magnetic fields observed outside the planets. We consider the model which enables us reproduce the typical features of…

流体动力学 · 物理学 2020-01-29 M. Reshetnyak , P. Hejda

The asymmetric shape of reversals of the Earth's magnetic field indicates a possible connection with relaxation oscillations as they were early discussed by van der Pol. A simple mean-field dynamo model with a spherically symmetric $\alpha$…

地球物理 · 物理学 2009-05-20 Frank Stefani , Mingtian Xu , Luca Sorriso-Valvo , Gunter Gerbeth , Uwe Günther

We present a new mechanism for oscillatory or random reversals of the magnetic field that occur from a stationary dynamo state. The basic ingredient is the existence of two nearly critical dynamo eigenmodes, a stable and an unstable one,…

地球物理 · 物理学 2008-10-29 F. Petrelis , S. Fauve

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…

流体动力学 · 物理学 2012-09-25 P. Hejda , M. Reshetnyak
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