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相关论文: Growth rate degeneracies in kinematic dynamos

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We study the geometry of the first two eigenvalues of a magnetic Steklov problem on an annulus $\Sigma$ (a compact Riemannian surface with genus zero and two boundary components), the magnetic potential being the harmonic one-form having…

谱理论 · 数学 2023-10-13 Luigi Provenzano , Alessandro Savo

We have introduced a new transfer operator for chaotic flows whose leading eigenvalue yields the dynamo rate of the fast kinematic dynamo and applied cycle expansion of the Fredholm determinant of the new operator to evaluation of its…

chao-dyn · 物理学 2009-10-22 N. J. BALMFORTH , P. CVITANOVIC , G. R. IERLEY , E. A. SPIEGEL , G. VATTAY

We study the kinematic dynamo equation on the three-torus and provide a rigorous proof of fast dynamo action for a time-periodic, divergence-free, Lipschitz velocity field. Our construction is based on a stretch-fold-shear mechanism…

偏微分方程分析 · 数学 2026-05-20 Michele Coti Zelati , Massimo Sorella , David Villringer

We study a single, motionless three-dimensional droplet growing by adsorption of diffusing monomers on a 2D substrate. The diffusing monomers are adsorbed at the aggregate perimeter of the droplet with different boundary conditions. Models…

统计力学 · 物理学 2009-10-31 Z. Tavassoli , G. J. Rodgers

We study domain growth kinetics in a random-field system in the presence of a spatially correlated disorder $h_{i}(\vec r)$ after an instantaneous quench at a finite temperature $T$ from a random initial state corresponding to $T=\infty$.…

统计力学 · 物理学 2025-05-13 Subhanker Howlader , Prasenjit Das , Manoj Kumar

In the VKS2 (von K\'arm\'an Sodium 2) successful dynamo experiment of September 2006, the magnetic field that was observed showed a strong axisymmetric component, implying that non axisymmetric components of the flow field were acting. By…

流体动力学 · 物理学 2009-11-13 R. Laguerre , C. Nore , A. Ribeiro , J. Léorat , J. -L. Guermond , F. Plunian

We are concerned with large scale magnetic field dynamo generation and propagation of magnetic fronts in turbulent electrically conducting fluids. An effective equation for the large scale magnetic field is developed here that takes into…

天体物理学 · 物理学 2009-11-06 Sergei Fedotov , Alexey Ivanov , Andrey Zubarev

Analytic solutions of the mean-field induction equation predict a nonoscillatory dynamo for homogeneous helical turbulence or constant alpha effect in unbounded or periodic domains. Oscillatory dynamos are generally thought impossible for…

太阳与恒星天体物理 · 物理学 2017-02-15 Axel Brandenburg

We perform numerical optimization of the axisymmetric flows in a sphere to minimize the critical magnetic Reynolds number Rm_cr required for dynamo onset. The optimization is done for the class of laminar incompressible flows of von Karman…

等离子体物理 · 物理学 2012-11-09 I. V. Khalzov , B. P. Brown , C. M. Cooper , D. B. Weisberg , C. B. Forest

We present a high-order numerical study of the dependence of the dynamo onset on different electromagnetic boundary conditions, in convecting Boussinesq flows forced by a temperature gradient. Perfectly conducting boundaries, vacuum, and…

流体动力学 · 物理学 2023-03-21 Mauro Fontana , Pablo D. Mininni , Pablo Dmitruk

At second order in perturbation theory, the unstable r-mode of a rotating star includes growing differential rotation whose form and growth rate are determined by gravitational-radiation reaction. With no magnetic field, the angular…

高能天体物理现象 · 物理学 2018-03-05 John L. Friedman , Lee Lindblom , Luciano Rezzolla , Andrey I. Chugunov

(Abridged) The small-scale dynamo may play a substantial role in magnetizing the Universe under a large range of conditions, including subsonic turbulence at low Mach numbers, highly supersonic turbulence at high Mach numbers and a large…

宇宙学与河外天体物理 · 物理学 2015-06-12 Dominik R. G. Schleicher , Jennifer Schober , Christoph Federrath , Stefano Bovino , Wolfram Schmidt

Galaxies are observed to host magnetic fields with a typical total strength of around 15microgauss. A coherent large-scale field constitutes up to a few microgauss of the total, while the rest is built from strong magnetic fluctuations over…

星系天体物理 · 物理学 2024-01-09 Maarit J. Korpi-Lagg , Mordecai-Mark Mac Low , Frederick A. Gent

This paper concerns kinematic helical dynamos in a spherical fluid body surrounded by an insulator. In particular, we examine their behaviour in the regime of large magnetic Reynolds number $\Rm$, for which dynamo action is usually…

地球与行星天体物理 · 物理学 2015-05-19 Henrik Latter , David Ivers

Using direct numerical simulations, we verify that "flow IV" of Roberts (1972) exhibits dynamo action dominated by horizontally averaged large-scale magnetic field. With the test-field method we compute the turbulent magnetic diffusivity…

太阳与恒星天体物理 · 物理学 2013-08-09 Ebru Devlen , Axel Brandenburg , Dhrubaditya Mitra

Several one and two dimensional mean field models are analyzed where the effects of current helicity fluxes and boundaries are included within the framework of the dynamical quenching model. In contrast to the case with periodic boundary…

天体物理学 · 物理学 2007-05-23 Axel Brandenburg , Kandaswamy Subramanian

We find that in the kinematic limit the ensemble averaged square of the curvature of magnetic field lines is exponentially amplified in time by the turbulent motions in a highly conductive plasma. At the same time, the ensemble averaged…

天体物理学 · 物理学 2009-11-06 Leonid Malyshkin

A topological constraint on the dynamics of a magnetic field in a flux tube arises from the fixed point indices of its field line mapping. This can explain unexpected behaviour in recent resistive-magnetohydrodynamic simulations of magnetic…

等离子体物理 · 物理学 2015-03-19 A. R. Yeates , G. Hornig

Recently Shukurov et al [Phys Rev E 72, 025302 (2008)], made use of non-orthogonal curvilinear coordinate system on a dynamo Moebius strip flow, to investigate the effect of stretching by a turbulent liquid sodium flow. In plasma physics,…

数学物理 · 物理学 2009-06-22 Garcia de Andrade

Small-scale dynamos (SSDs) amplify magnetic fields in turbulent plasmas. Theory predicts nonlinear magnetic energy growth $E_\mathrm{mag} \propto t^{p_\mathrm{nl}}$, but this scaling has not been tested across flow regimes. Using a large…

等离子体物理 · 物理学 2026-05-01 Neco Kriel , James R. Beattie , Mark R. Krumholz , Jennifer Schober , Patrick J. Armstrong