Absolute versus convective helical magnetorotational instabilities in Taylor-Couette flows

Rainer Hollerbach, Nigel Sibanda, Eun Jin Kim

Research output: Contribution to journalArticle

2 Citations (Scopus)
3 Downloads (Pure)

Abstract

We study magnetic Taylor-Couette flow in a system having nondimensional radii r i = 1 and r o = 2, and periodic in the axial direction with wavelengths . The rotation ratio of the inner and outer cylinders is adjusted to be slightly in the Rayleigh-stable regime, where magnetic fields are required to destabilize the flow, in this case triggering the axisymmetric helical magnetorotational instability (HMRI). Two choices of imposed magnetic field are considered, both having the same azimuthal component , but differing axial components. The first choice has B z = 0.1, and yields the familiar HMRI, consisting of unidirectionally traveling waves. The second choice has , and yields HMRI waves that travel in opposite directions depending on the sign of B z. The first configuration corresponds to a convective instability, the second to an absolute instability. The two variants behave very similarly regarding both linear onset as well as nonlinear equilibration.

Original languageEnglish
Article number045501
JournalFluid Dynamics Research
Volume49
Issue number4
Early online date21 Apr 2017
DOIs
Publication statusPublished - 22 May 2017
Externally publishedYes

    Fingerprint

Keywords

  • instabilities
  • magnetohydrodynamics
  • pattern formation
  • Taylor-Couette flows

ASJC Scopus subject areas

  • Mechanical Engineering
  • Physics and Astronomy(all)
  • Fluid Flow and Transfer Processes

Cite this