SearcharxivSearch

arXiv subjects

Andrew D Gilbert

Publications and source records attributed to Andrew D Gilbert.

2 recordsLinked to original sources

Vortex filament dynamics and vortex ring motion revisited

The motion of a slender vortex in ideal incompressible fluid is a classic problem in hydrodynamics. Formulae for the velocity of a vortex ring go back to work of Kelvin, Helmholtz, Hicks and Dyson in the nineteenth century, while more recently a number of models have been created for simulating the motion of slender tubes of vorticity of general shape. For a vortex tube or filament localised near to a curve C(t), the relevant small parameter to measure slenderness is the tube radius divided by the radius of curvature of C. The present paper revisits this range of classic problems by introducing a coordinate system closely linked to the geometry of vortex surfaces in a slender vortex. The motion of fluid elements in this coordinate system has an action--angle form, and with this the vorticity equation simplifies radically. At the same time, however, most aspects of the shape or evolution of a vortex are thrown into the description of the coordinates, and in particular the corresponding metric and volume form. As the coordinate system is non-orthogonal and time-dependent, tools of differential geometry are most easily used to describe the structure of both vorticity and coordinate system, and a general mathematical framework is set out. This resulting system of equations is taken as far as possible with only the assumption of vortex slenderness in place, but allowing arbitrary motions and distortions of the vortex core and of the curve C(t). The modelling is applied to calculate the motion of a slender vortex ring with arbitrary axial flow, solving directly for the shape of perturbed vorticity surfaces and giving results in agreement with earlier studies. The general framework set up in this paper is suitable for the development of simplified equations for vortex motion and interaction in future studies.

physics.flu-dyn

Zonostrophic instabilities in magnetohydrodynamic Kolmogorov flow

This paper concerns the stability of Kolmogorov flow u = (0, sin x) in the infinite (x,y)-plane. A mean magnetic field of strength B0 is introduced and the MHD linear stability problem studied for modes with wave-number k in the y-direction, and Bloch wavenumber l in the x-direction. The parameters governing the problem are Reynolds number 1/nu, magnetic Prandtl number P, and dimensionless magnetic field strength B0. The mean magnetic field can be taken to have an arbitrary direction in the (x,y)-plane and a mean x-directed flow U0 can be incorporated. First the paper considers Kolmogorov flow with y-directed mean magnetic field, referred to as vertical. Taking l=0, the suppression of the pure hydrodynamic instability is observed with increasing field strength B0. A branch of strong-field instabilities occurs for magnetic Prandtl number P less than unity, as found by A.E. Fraser, I.G. Cresser and P. Garaud (J. Fluid Mech. 949, A43, 2022). Analytical results using eigenvalue perturbation theory in the limit k->0 support the numerics for both weak- and strong-field instabilities, and originate in the coupling of large-scale modes with x-wavenumber n=0, to smaller-scale modes. The paper considers the case of horizontal or x-directed mean magnetic field. The unperturbed state consists of steady, wavey magnetic field lines. As the magnetic field is increased, the purely hydrodynamic instability is suppressed again, but for stronger fields a new branch of instabilities appears. Allowing a non-zero Bloch wavenumber l allows further instability, and in some circumstances when the system is hydrodynamically stable, arbitrarily weak magnetic fields can give growing modes. Numerical results are presented together with eigenvalue perturbation theory in the limits k,l->0. The theory gives analytical approximations for growth rates and thresholds in good agreement with those computed.

physics.flu-dyn