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  • Cited by 5
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    This article has been cited by the following publications. This list is generated based on data provided by CrossRef.

    Rempel, Erico L Chian, Abraham C-L and Brandenburg, Axel 2012. Lagrangian chaos in an ABC-forced nonlinear dynamo. Physica Scripta, Vol. 86, Issue. 1, p. 018405.


    Smith, Frank T. 2012. On internal fluid dynamics. Bulletin of Mathematical Sciences, Vol. 2, Issue. 1, p. 125.


    Koshel, K V Sokolovskiy, M A and Davies, P A 2008. Chaotic advection and nonlinear resonances in an oceanic flow above submerged obstacle. Fluid Dynamics Research, Vol. 40, Issue. 10, p. 695.


    Tobias, Steven M. and Cattaneo, Fausto 2008. Limited Role of Spectra in Dynamo Theory: Coherent versus Random Dynamos. Physical Review Letters, Vol. 101, Issue. 12,


    Kivotides, D Mee, A J and Barenghi, C F 2007. Magnetic field generation by coherent turbulence structures. New Journal of Physics, Vol. 9, Issue. 8, p. 291.


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  • Journal of Fluid Mechanics, Volume 498
  • January 2004, pp. 1-21

Vortex dynamos

  • STEFAN G. LLEWELLYN SMITH (a1) and S. M. TOBIAS (a2)
  • DOI: http://dx.doi.org/10.1017/S0022112003007006
  • Published online: 01 January 2004
Abstract

We investigate the kinematic dynamo properties of interacting vortex tubes. These flows are of great importance in geophysical and astrophysical fluid dynamics: for a large range of systems, turbulence is dominated by such coherent structures. We obtain a dynamically consistent $2 \frac{1}{2}$-dimensional velocity field of the form $\left(u(x,y,t),v(x,y,t),w(x,y,t)\right)$ by solving the $z$-independent Navier–Stokes equations in the presence of helical forcing. This system naturally forms vortex tubes via an inverse cascade. It has chaotic Lagrangian properties and is therefore a candidate for fast dynamo action. The kinematic dynamo properties of the flow are calculated by determining the growth rate of a small-scale seed field. The growth rate is found to have a complicated dependence on Reynolds number $\Rey$ and magnetic Reynolds number $\Rem$, but the flow continues to act as a dynamo for large $\Rey$ and $\Rem$. Moreover the dynamo is still efficient even in the limit $\Rey \,{\gg}\, \Rem$, providing $\Rem$ is large enough, because of the formation of coherent structures.

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Journal of Fluid Mechanics
  • ISSN: 0022-1120
  • EISSN: 1469-7645
  • URL: /core/journals/journal-of-fluid-mechanics
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