Submit manuscript...
eISSN: 2577-8242

Fluid Mechanics Research International Journal

Short Communication Volume 1 Issue 1

Peculiarity of Taylor’s and wavy vortices beginning, generated by a rotating magnetic field

AF Zibold

Donbas State Technical University, Ukraine

Correspondence: AF Zibold, Researcher, Donetsk, Ukraine

Received: May 22, 2017 | Published: June 12, 2017

Citation: Zibold AF. Peculiarity of Taylor’s and wavy vortices beginning, generated by a rotating magnetic field. Fluid Mech Res Int J. 2017;1(1):1-2. DOI: 10.15406/fmrij.2017.01.00001

Download PDF

Abstract

Results of research of stationary instability of axisymmetric laminar flow of a conducting liquid, arising under the influence of the rotating magnetic field of any rotary symmetry, are briefly presented. It is shown, that the secondary flow arises in the form of Taylor's vortices or wavy vortices of this or that order. The correctness of linear statement of a problem of stability is established.

Introduction

Stationary instability of axisymmetric laminar flow of a viscous conducting liquid in the infinitely long circular cylinder, arising under the influence of coaxially rotating magnetic field (RMF) of any rotary symmetry, has been investigated. The nearest analogue of the conducting liquid flow raised by the rotating magnetic field is Couette flow between two concentric cylinders from which internal one rotates and external remains motionless. While analyzing stability of such flow, Lin 1 has noticed, that the first approximation equations for small perturbations of velocity and pressure allow for periodic solution with respect to φ MathType@MTEF@5@5@+= feaagKart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaeqOXdOgaaa@37B3@  and z : MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbdfwBIj xAHbstHrhAaeXatLxBI9gBaerbd9wDYLwzYbItLDharuavP1wzZbIt LDhis9wBH5garqqtubsr4rNCHbGeaGak0Jf9crFfpeea0xh9v8qiW7 rqqrFfpeea0xe9Lq=Jc9vqaqpepm0xbbG8FasPYRqj0=yi0dXdbba9 pGe9xq=JbbG8A8frFve9Fve9Ff0dmeaabaqaciGacaGaaeqabaWaaq aafaaakeaacaWG6bGaaiOoaaaa@3EA1@

f = f ( r ) exp ( σ t + i n φ + i a z ) , MathType@MTEF@5@5@+= feaagKart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamOzaiabg2 da9iaadAgadaqadaqaaiaadkhaaiaawIcacaGLPaaacqGHflY1ciGG LbGaaiiEaiaacchadaqadaqaaiabeo8aZjaadshacqGHRaWkcaWGPb GaamOBaiabeA8aQjabgUcaRiaadMgacaWGHbGaamOEaaGaayjkaiaa wMcaaiaacYcaaaa@4DA1@ (1)

where σ MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbdfwBIj xAHbstHrhAaeXatLxBI9gBaerbd9wDYLwzYbItLDharuavP1wzZbIt LDhis9wBH5garqqtubsr4rNCHbGeaGak0Jf9crFfpeea0xh9v8qiW7 rqqrFfpeea0xe9Lq=Jc9vqaqpepm0xbbG8FasPYRqj0=yi0dXdbba9 pGe9xq=JbbG8A8frFve9Fve9Ff0dmeaabaqaciGacaGaaeqabaWaaq aafaaakeaacqaHdpWCaaa@3EA7@  is the complex constant, n MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbdfwBIj xAHbstHrhAaeXatLxBI9gBaerbd9wDYLwzYbItLDharuavP1wzZbIt LDhis9wBH5garqqtubsr4rNCHbGeaGak0Jf9crFfpeea0xh9v8qiW7 rqqrFfpeea0xe9Lq=Jc9vqaqpepm0xbbG8FasPYRqj0=yi0dXdbba9 pGe9xq=JbbG8A8frFve9Fve9Ff0dmeaabaqaciGacaGaaeqabaWaaq aafaaakeaacaWGUbaaaa@3DD7@  is the integer number (order of sinuosity), and a MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbdfwBIj xAHbstHrhAaeXatLxBI9gBaerbd9wDYLwzYbItLDharuavP1wzZbIt LDhis9wBH5garqqtubsr4rNCHbGeaGak0Jf9crFfpeea0xh9v8qiW7 rqqrFfpeea0xe9Lq=Jc9vqaqpepm0xbbG8FasPYRqj0=yi0dXdbba9 pGe9xq=JbbG8A8frFve9Fve9Ff0dmeaabaqaciGacaGaaeqabaWaaq aafaaakeaacaWGHbaaaa@3DCA@  is the real (dimensionless wave number).

Usually one deals with a special case of rotary symmetry n = 0. MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbdfwBIj xAHbstHrhAaeXatLxBI9gBaerbd9wDYLwzYbItLDharuavP1wzZbIt LDhis9wBH5garqqtubsr4rNCHbGeaGak0Jf9crFfpeea0xh9v8qiW7 rqqrFfpeea0xe9Lq=Jc9vqaqpepm0xbbG8FasPYRqj0=yi0dXdbba9 pGe9xq=JbbG8A8frFve9Fve9Ff0dmeaabaqaciGacaGaaeqabaWaaq aafaaakeaacaWGUbGaeyypa0JaaGimaiaac6caaaa@4049@  In this case a primary flow is independent of ϕ , MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbdfwBIj xAHbstHrhAaeXatLxBI9gBaerbd9wDYLwzYbItLDharuavP1wzZbIt LDhis9wBH5garqqtubsr4rNCHbGeaGak0Jf9crFfpeea0xh9v8qiW7 rqqrFfpeea0xe9Lq=Jc9vqaqpepm0xbbG8FasPYRqj0=yi0dXdbba9 pGe9xq=JbbG8A8frFve9Fve9Ff0dmeaabaqaciGacaGaaeqabaWaaq aafaaakeaacqaHvpGzcaGGSaaaaa@3F5C@  but disturbances of velocity u r , MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbdfwBIj xAHbstHrhAaeXatLxBI9gBaerbd9wDYLwzYbItLDharuavP1wzZbIt LDhis9wBH5garqqtubsr4rNCHbGeaGak0Jf9crFfpeea0xh9v8qiW7 rqqrFfpeea0xe9Lq=Jc9vqaqpepm0xbbG8FasPYRqj0=yi0dXdbba9 pGe9xq=JbbG8A8frFve9Fve9Ff0dmeaabaqaciGacaGaaeqabaWaaq aafaaakeaacaWG1bWaaSbaaSqaaiaadkhaaeqaaOGaaiilaaaa@3FBB@ u φ , MathType@MTEF@5@5@+= feaagKart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamyDamaaBa aaleaacqaHgpGAaeqaaOGaaiilaaaa@3993@ u z MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbdfwBIj xAHbstHrhAaeXatLxBI9gBaerbd9wDYLwzYbItLDharuavP1wzZbIt LDhis9wBH5garqqtubsr4rNCHbGeaGak0Jf9crFfpeea0xh9v8qiW7 rqqrFfpeea0xe9Lq=Jc9vqaqpepm0xbbG8FasPYRqj0=yi0dXdbba9 pGe9xq=JbbG8A8frFve9Fve9Ff0dmeaabaqaciGacaGaaeqabaWaaq aafaaakeaacaWG1bWaaSbaaSqaaiaadQhaaeqaaaaa@3F09@  and pressure q MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbdfwBIj xAHbstHrhAaeXatLxBI9gBaerbd9wDYLwzYbItLDharuavP1wzZbIt LDhis9wBH5garqqtubsr4rNCHbGeaGak0Jf9crFfpeea0xh9v8qiW7 rqqrFfpeea0xe9Lq=Jc9vqaqpepm0xbbG8FasPYRqj0=yi0dXdbba9 pGe9xq=JbbG8A8frFve9Fve9Ff0dmeaabaqaciGacaGaaeqabaWaaq aafaaakeaacaWGXbaaaa@3DDA@  are not zero. The series of papers in which stability was investigated in the approximation of small values of relative frequency ω ¯ MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbdfwBIj xAHbstHrhAaeXatLxBI9gBaerbd9wDYLwzYbItLDharuavP1wzZbIt LDhis9wBH5garqqtubsr4rNCHbGeaGak0Jf9crFfpeea0xh9v8qiW7 rqqrFfpeea0xe9Lq=Jc9vqaqpepm0xbbG8FasPYRqj0=yi0dXdbba9 pGe9xq=JbbG8A8frFve9Fve9Ff0dmeaabaqaciGacaGaaeqabaWaaq aafaaakeaadaqdaaqaaiabeM8a3baaaaa@3EC2@  4,5 in the approximation of big ω ¯ MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbdfwBIj xAHbstHrhAaeXatLxBI9gBaerbd9wDYLwzYbItLDharuavP1wzZbIt LDhis9wBH5garqqtubsr4rNCHbGeaGak0Jf9crFfpeea0xh9v8qiW7 rqqrFfpeea0xe9Lq=Jc9vqaqpepm0xbbG8FasPYRqj0=yi0dXdbba9 pGe9xq=JbbG8A8frFve9Fve9Ff0dmeaabaqaciGacaGaaeqabaWaaq aafaaakeaadaqdaaqaaiabeM8a3baaaaa@3EC2@  6 and for intermediate values ω ¯ MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbdfwBIj xAHbstHrhAaeXatLxBI9gBaerbd9wDYLwzYbItLDharuavP1wzZbIt LDhis9wBH5garqqtubsr4rNCHbGeaGak0Jf9crFfpeea0xh9v8qiW7 rqqrFfpeea0xe9Lq=Jc9vqaqpepm0xbbG8FasPYRqj0=yi0dXdbba9 pGe9xq=JbbG8A8frFve9Fve9Ff0dmeaabaqaciGacaGaaeqabaWaaq aafaaakeaadaqdaaqaaiabeM8a3baaaaa@3EC2@  9,10 has been issued by the Donetsk group of fluid dynamicists, lead by A. B. Kapusta. Within all investigated ranges of flow parameters only one-vortical (in the radial direction) structures of Taylor's vortices have been found in the calculations.

The case n 0 MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbdfwBIj xAHbstHrhAaeXatLxBI9gBaerbd9wDYLwzYbItLDharuavP1wzZbIt LDhis9wBH5garqqtubsr4rNCHbGeaGak0Jf9crFfpeea0xh9v8qiW7 rqqrFfpeea0xe9Lq=Jc9vqaqpepm0xbbG8FasPYRqj0=yi0dXdbba9 pGe9xq=JbbG8A8frFve9Fve9Ff0dmeaabaqaciGacaGaaeqabaWaaq aafaaakeaacaWGUbGaeyiyIKRaaGimaaaa@4058@  corresponds to the occurrence of the so-called wavy vortices. For the first time, such problem for Couette flow between coaxial cylinders have been considered by Daveyet al 2 The work investigated bifurcation of Taylor vortices into wavy vortices, i.e. in such flow when waves extend along the axis of Taylor's vortices. As the number of waves which are passing on these vortices, can be only integer it is clear why in (1) n MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbdfwBIj xAHbstHrhAaeXatLxBI9gBaerbd9wDYLwzYbItLDharuavP1wzZbIt LDhis9wBH5garqqtubsr4rNCHbGeaGak0Jf9crFfpeea0xh9v8qiW7 rqqrFfpeea0xe9Lq=Jc9vqaqpepm0xbbG8FasPYRqj0=yi0dXdbba9 pGe9xq=JbbG8A8frFve9Fve9Ff0dmeaabaqaciGacaGaaeqabaWaaq aafaaakeaacaWGUbaaaa@3DD7@  is the integer ( n MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbdfwBIj xAHbstHrhAaeXatLxBI9gBaerbd9wDYLwzYbItLDharuavP1wzZbIt LDhis9wBH5garqqtubsr4rNCHbGeaGak0Jf9crFfpeea0xh9v8qiW7 rqqrFfpeea0xe9Lq=Jc9vqaqpepm0xbbG8FasPYRqj0=yi0dXdbba9 pGe9xq=JbbG8A8frFve9Fve9Ff0dmeaabaqaciGacaGaaeqabaWaaq aafaaakeaacaWGUbaaaa@3DD7@  is the order of sinuosity). The results obtained in this work, will well be in agreement with results of experiments by Coles 1 and Gollub & Swinney.3

Current study briefly presents results of researching the case of n 0 MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbdfwBIj xAHbstHrhAaeXatLxBI9gBaerbd9wDYLwzYbItLDharuavP1wzZbIt LDhis9wBH5garqqtubsr4rNCHbGeaGak0Jf9crFfpeea0xh9v8qiW7 rqqrFfpeea0xe9Lq=Jc9vqaqpepm0xbbG8FasPYRqj0=yi0dXdbba9 pGe9xq=JbbG8A8frFve9Fve9Ff0dmeaabaqaciGacaGaaeqabaWaaq aafaaakeaacaWGUbGaeyiyIKRaaGimaaaa@4058@  as applied to the flow of a conducting liquid arising in a cylindrical vessel under the influence of rotating magnetic field. The problem of stability for arbitrary symmetry of RMF has been considered in linear formulation. 11 Certainly, the use of linear statement in the research of loss of stability of Taylor's vortices and transition to wavy vortices, can raise some doubts. After the loss of stability resulting flow will represent superposition of a primary azimuthal flow and system of Taylor's vortices. Furthermore it is necessary to investigate stability of already complex flow involving occurrence of wavy vortices. The strategy of such a research is illustrated by the citation from the monograph of Richtmyer.8

In recent years, the nonlinear theory developed by Daveyet al. 2 has led to an understanding of the structure and stability of the finite-amplitude Taylor vortices, the second bifurcation to the wavy vortices, and the structure and stability of the wavy vortices, as discussed below.

In a problem like this, involving a sequence of bifurcations, the theory consists ideally of a sequence of alternately linear and nonlinear investigations. After each bifurcations the structure and amplitude of the new flow is found by a nonlinear calculations. Its stability is then investigated by linear zing the equations about the new flow and studying the growth of infinitesimal disturbances, in order to find the next bifurcation, and so on.

Apparently, the MHD flow raised by weak rotating magnetic field is most closely analogous to Couette flow between two concentric cylinders. Daveyet al. 2 have theoretically established, that Taylor's critical number at which Taylor's vortices become unstable and wavy vortices appear exceeds by 8% the Taylor's number at which the primary one-dimensional flow loses the stability and for the first time Taylor's vortices appear. In the assumption, that in weak RMF and the primary flow will be weak, and nonlinear additions will be even weaker, the similar estimation for linear statement of a problem of stability has been made. As Daveyet al. 2 used Taylor's number as criterion of an estimation of the stability for the correct comparison of the results in our case, we will take advantage of analogue of Taylor's number for magnetic hydrodynamics ‒ Taylor's magnetic number. Corresponding excess of Taylor's magnetic number for the case of one pair of poles of the RMF makes up 6.78% that close to the result obtained by Daveyet al.2

The problem is solved for two cases: in low-frequency approach and for any value of relative frequency. With the use of Galerkin's method the curves of neutral stability corresponding to occurrence of Taylor's and wavy vortices are calculated. Already for p = 1 MathType@MTEF@5@5@+= feaagKart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGaamiCaiabg2 da9iaaigdaaaa@38AC@  interesting enough results have been obtained. It was found, that the curves of neutral stability obtained for n = 1 MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbdfwBIj xAHbstHrhAaeXatLxBI9gBaerbd9wDYLwzYbItLDharuavP1wzZbIt LDhis9wBH5garqqtubsr4rNCHbGeaGak0Jf9crFfpeea0xh9v8qiW7 rqqrFfpeea0xe9Lq=Jc9vqaqpepm0xbbG8FasPYRqj0=yi0dXdbba9 pGe9xq=JbbG8A8frFve9Fve9Ff0dmeaabaqaciGacaGaaeqabaWaaq aafaaakeaacaWGUbGaeyypa0JaaGymaaaa@3F98@  cross the curves of neutral stability for n = 0 ; MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbdfwBIj xAHbstHrhAaeXatLxBI9gBaerbd9wDYLwzYbItLDharuavP1wzZbIt LDhis9wBH5garqqtubsr4rNCHbGeaGak0Jf9crFfpeea0xh9v8qiW7 rqqrFfpeea0xe9Lq=Jc9vqaqpepm0xbbG8FasPYRqj0=yi0dXdbba9 pGe9xq=JbbG8A8frFve9Fve9Ff0dmeaabaqaciGacaGaaeqabaWaaq aafaaakeaacaWGUbGaeyypa0JaaGimaiaacUdaaaa@4056@  curves for n = 2 MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbdfwBIj xAHbstHrhAaeXatLxBI9gBaerbd9wDYLwzYbItLDharuavP1wzZbIt LDhis9wBH5garqqtubsr4rNCHbGeaGak0Jf9crFfpeea0xh9v8qiW7 rqqrFfpeea0xe9Lq=Jc9vqaqpepm0xbbG8FasPYRqj0=yi0dXdbba9 pGe9xq=JbbG8A8frFve9Fve9Ff0dmeaabaqaciGacaGaaeqabaWaaq aafaaakeaacaWGUbGaeyypa0JaaGOmaaaa@3F99@  cross curves for n = 1 MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbdfwBIj xAHbstHrhAaeXatLxBI9gBaerbd9wDYLwzYbItLDharuavP1wzZbIt LDhis9wBH5garqqtubsr4rNCHbGeaGak0Jf9crFfpeea0xh9v8qiW7 rqqrFfpeea0xe9Lq=Jc9vqaqpepm0xbbG8FasPYRqj0=yi0dXdbba9 pGe9xq=JbbG8A8frFve9Fve9Ff0dmeaabaqaciGacaGaaeqabaWaaq aafaaakeaacaWGUbGaeyypa0JaaGymaaaa@3F98@  etc. Taylor's vortices ( n = 0 ) MathType@MTEF@5@5@+= feaagKart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaWaaeWaaeaaca WGUbGaeyypa0JaaGimaaGaayjkaiaawMcaaaaa@3A32@  arise in wide enough, but limited range of flow parameters, but upon the increase in parameters, they lose stability and convert to wavy vortices ( n > 0 ) MathType@MTEF@5@5@+= feaagKart1ev2aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq=Jc9 vqaqpepm0xbba9pwe9Q8fs0=yqaqpepae9pg0FirpepeKkFr0xfr=x fr=xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaWaaeWaaeaaca WGUbGaeyOpa4JaaGimaaGaayjkaiaawMcaaaaa@3A34@ . It is established, that under certain conditions the loss of stability of a primary flow leads to the direct appearance of wavy vortices of some order, by-passing the stage of Taylor's vortices. All this means that the use of linear statement in the study of stability of the flow raised by the RMF, is quite correct. On the curve of neutral stability separating area of one-dimensional azimuthal flow from the region of a three-dimensional vortical flow, points of bifurcation are defined corresponding to the transition from secondary flow in the form of Taylor's vortices to the secondary flow in the form of wavy vortices with n = 1 MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbdfwBIj xAHbstHrhAaeXatLxBI9gBaerbd9wDYLwzYbItLDharuavP1wzZbIt LDhis9wBH5garqqtubsr4rNCHbGeaGak0Jf9crFfpeea0xh9v8qiW7 rqqrFfpeea0xe9Lq=Jc9vqaqpepm0xbbG8FasPYRqj0=yi0dXdbba9 pGe9xq=JbbG8A8frFve9Fve9Ff0dmeaabaqaciGacaGaaeqabaWaaq aafaaakeaacaWGUbGaeyypa0JaaGymaaaa@3F98@  and further with consecutively higher orders of a sinuosity. It is typical that such transitions are accompanied by step-wise increase in wave number, i.e. transition to smaller and smaller scale vortices. Such a cascade of bifurcations is observed both on the branch of the neutral stability corresponding to low-frequency approach, and on the branch corresponding to the case of arbitrary values of relative frequency.

As well the interesting phenomena are observed at an increase in the order of rotary symmetry of the RMF. At p = 2 MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbdfwBIj xAHbstHrhAaeXatLxBI9gBaerbd9wDYLwzYbItLDharuavP1wzZbIt LDhis9wBH5garqqtubsr4rNCHbGeaGak0Jf9crFfpeea0xh9v8qiW7 rqqrFfpeea0xe9Lq=Jc9vqaqpepm0xbbG8FasPYRqj0=yi0dXdbba9 pGe9xq=JbbG8A8frFve9Fve9Ff0dmeaabaqaciGacaGaaeqabaWaaq aafaaakeaacaWGWbGaeyypa0JaaGOmaaaa@3F9B@  the range of parameters at which the loss of stability of a primary flow leads to occurrence of Taylor's vortices, is reduced. At p = 3 MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbdfwBIj xAHbstHrhAaeXatLxBI9gBaerbd9wDYLwzYbItLDharuavP1wzZbIt LDhis9wBH5garqqtubsr4rNCHbGeaGak0Jf9crFfpeea0xh9v8qiW7 rqqrFfpeea0xe9Lq=Jc9vqaqpepm0xbbG8FasPYRqj0=yi0dXdbba9 pGe9xq=JbbG8A8frFve9Fve9Ff0dmeaabaqaciGacaGaaeqabaWaaq aafaaakeaacaWGWbGaeyypa0JaaG4maaaa@3F9C@  Taylor's vortices do not arise at all, instead thee wavy vortices appear with n 1. MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbdfwBIj xAHbstHrhAaeXatLxBI9gBaerbd9wDYLwzYbItLDharuavP1wzZbIt LDhis9wBH5garqqtubsr4rNCHbGeaGak0Jf9crFfpeea0xh9v8qiW7 rqqrFfpeea0xe9Lq=Jc9vqaqpepm0xbbG8FasPYRqj0=yi0dXdbba9 pGe9xq=JbbG8A8frFve9Fve9Ff0dmeaabaqaciGacaGaaeqabaWaaq aafaaakeaacaWGUbGaeyyzImRaaGymaiaac6caaaa@410A@  At p = 4 MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbdfwBIj xAHbstHrhAaeXatLxBI9gBaerbd9wDYLwzYbItLDharuavP1wzZbIt LDhis9wBH5garqqtubsr4rNCHbGeaGak0Jf9crFfpeea0xh9v8qiW7 rqqrFfpeea0xe9Lq=Jc9vqaqpepm0xbbG8FasPYRqj0=yi0dXdbba9 pGe9xq=JbbG8A8frFve9Fve9Ff0dmeaabaqaciGacaGaaeqabaWaaq aafaaakeaacaWGWbGaeyypa0JaaGinaaaa@3F9D@  a zone of occurrence of wavy vortices with n = 1 MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbdfwBIj xAHbstHrhAaeXatLxBI9gBaerbd9wDYLwzYbItLDharuavP1wzZbIt LDhis9wBH5garqqtubsr4rNCHbGeaGak0Jf9crFfpeea0xh9v8qiW7 rqqrFfpeea0xe9Lq=Jc9vqaqpepm0xbbG8FasPYRqj0=yi0dXdbba9 pGe9xq=JbbG8A8frFve9Fve9Ff0dmeaabaqaciGacaGaaeqabaWaaq aafaaakeaacaWGUbGaeyypa0JaaGymaaaa@3F98@  is reduced, and at p = 5 MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbdfwBIj xAHbstHrhAaeXatLxBI9gBaerbd9wDYLwzYbItLDharuavP1wzZbIt LDhis9wBH5garqqtubsr4rNCHbGeaGak0Jf9crFfpeea0xh9v8qiW7 rqqrFfpeea0xe9Lq=Jc9vqaqpepm0xbbG8FasPYRqj0=yi0dXdbba9 pGe9xq=JbbG8A8frFve9Fve9Ff0dmeaabaqaciGacaGaaeqabaWaaq aafaaakeaacaWGWbGaeyypa0JaaGynaaaa@3F9E@  wavy vortices appear already only at n 2. MathType@MTEF@5@5@+= feaagKart1ev2aqatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbdfwBIj xAHbstHrhAaeXatLxBI9gBaerbd9wDYLwzYbItLDharuavP1wzZbIt LDhis9wBH5garqqtubsr4rNCHbGeaGak0Jf9crFfpeea0xh9v8qiW7 rqqrFfpeea0xe9Lq=Jc9vqaqpepm0xbbG8FasPYRqj0=yi0dXdbba9 pGe9xq=JbbG8A8frFve9Fve9Ff0dmeaabaqaciGacaGaaeqabaWaaq aafaaakeaacaWGUbGaeyyzImRaaGOmaiaac6caaaa@410B@  The increase in the values of Hartmann number, the relative frequency and in the order of rotary symmetry of the RMF, reduces the characteristic size both Taylor's and wavy vortices. The vortices centre is thus displaced towards the cylinder wall.

The completed research has allowed establishing in general terms that at the loss of stability of a primary flow, the occurrence of wavy vortices without an intermediate stage in the form of Taylor's vortices is possible. And, as it was already noted, at the increase in the order of rotary symmetry of the RMF Taylor's vortices may not appear at all. This is the basic difference between our results and the results of the classical research problem of stability of Couette flow between coaxial cylinders Daveyet al.,2 when transition to wavy vortices necessarily is preceded by a stage of Taylor's vortices. This is because Couette flow arises thanks to forces of viscosity (liquid sticking to the rotating cylinder) while in our case of using the RMF the flow is created due to field acting on the conducting liquid at a motionless wall of the cylinder. Profiles of a primary flow essentially differ: in our case there is always at least a thin boundary layer between a kernel of a flow and a cylinder wall.

 The completed research allows one to expand our views about the mechanisms of the rise of the instability of the conducting liquid flow generated by the RMF of any rotary symmetry in infinitely long cylindrical vessel. The results obtained thus far allow us to predict the loss of stability of a primary flow occurrence of a secondary flow in Taylor's vortices or wavy vortices of this or that order depending on the level of the power affecting the liquid and on the order of rotary symmetry of the RMF. Apparently, these conclusions would likely be fair and for sufficiently long cylinders of finite length when it is possible to neglect the influence of end faces on the flow in the central part of the vessel.

Acknowledgement

None.

Conflict of Interest

Author declares that there is no conflicts of interest.

References

  1. Lin CC. The Theory of Hydrodynamic Stability. 1955.
  2. Kapusta AB, Zibold AF. Stationary instability of axisymmetric flow of a liquid in a rotating magnetic field. Magnetohydro-dynamics. 1977;13(3):312?319.
  3. Kapusta AB, Zibold AF. The effect of rotating magnetic field symmetry on the stability of steady axially symmetric flow. Magnitnaya Gidrodinamika. 1981;17:134?136.
  4. Kapusta AB, Zibold AF. Stationary instability in an axisymmetric flow excited by a rotating high-frequency magnetic field. Magneto hydrodynamics. 1983;19(1):62?65.
  5. Zibold AF. The Stationary instability of axisymmetric flow of liquid in a weak rotating magnetic field. Plasma Physics. 1984:61?68.
  6. Zibold AF. On a simple formulation of stability problem in a weak rotating magnetic field. Magnitnaya Gidrodinamika. 1984;20:132?133.
  7. Davey A, Di Prima RC, Stuart JT. On the instability of Taylor vortices. Journal of Fluid Mechanics. 1968;31(1):17?52.
  8. Donald Coles. Transition in circular Couette flow. Journal of Fluid Mechanics. 1965;21(3):385–425.
  9. Gollub JP, Swinney HL. Onset of turbulence in a rotating fluid. Physical Review Letters. 1975;35(14):927?930.
  10. Zibold AF. Effect of the symmetry of a rotating magnetic field on the instability of a flow of the conducting liquid: Taylor's and wavy vortices. 10th PAMIR Intern Conf Fundamental and Applied MHD. 2016. p. 12?16.
  11. Richtmyer RD. Principles of Advanced Mathematical Physics. Springer. 1981. 323 p.
Creative Commons Attribution License

©2017 Zibold. This is an open access article distributed under the terms of the, which permits unrestricted use, distribution, and build upon your work non-commercially.