Numerical stability analysis and general flow characterization were performed for the flow induced by transverse rotating magnetic fields in cylindrical containers. Starting from Richardson’s theoretical critical value for the generation of Taylor vortices in infinite cylinders, overstability in finite cylinders with different aspect ratios was investigated. Decreasing aspect ratio leads to a more stable configuration. For small cylinders and reasonable frequencies of the magnetic field, instabilities arise at low magnetic inductions, e.g., [gallium as model liquid, with radius of the cylinder aspect ratio and frequency ]. As a source of instabilities Taylor vortices have been identified. They are transported by the secondary flow, emerging in finite cylinders due to the imbalance of pressure gradient and centrifugal force close to the top and bottom, thus generating time-dependent flow. Their generation is statistical and manifests itself in, e.g., nonperiodic temperature oscillations with small amplitudes in a classical Bénard configuration. Furthermore the intensity of the secondary flow was investigated for the isothermal case to give hints on its general influence on the overall mass transport.
Skip Nav Destination
Article navigation
Research Article|
May 01 1998
Taylor vortex instabilities induced by a rotating magnetic field: A numerical approach Available to Purchase
Th. Kaiser;
Th. Kaiser
Kristallographisches Institut der Universität Freiburg, Hebelstr. 25, D-79104 Freiburg, Germany
Search for other works by this author on:
K. W. Benz
K. W. Benz
Kristallographisches Institut der Universität Freiburg, Hebelstr. 25, D-79104 Freiburg, Germany
Search for other works by this author on:
Th. Kaiser
Kristallographisches Institut der Universität Freiburg, Hebelstr. 25, D-79104 Freiburg, Germany
K. W. Benz
Kristallographisches Institut der Universität Freiburg, Hebelstr. 25, D-79104 Freiburg, Germany
Physics of Fluids 10, 1104–1110 (1998)
Article history
Received:
June 27 1997
Accepted:
January 21 1998
Citation
Th. Kaiser, K. W. Benz; Taylor vortex instabilities induced by a rotating magnetic field: A numerical approach. Physics of Fluids 1 May 1998; 10 (5): 1104–1110. https://doi.org/10.1063/1.869635
Download citation file:
Pay-Per-View Access
$40.00
Sign In
You could not be signed in. Please check your credentials and make sure you have an active account and try again.
Citing articles via
Phase behavior of Cacio e Pepe sauce
G. Bartolucci, D. M. Busiello, et al.
Direct numerical simulations of immiscible two-phase flow in rough fractures: Impact of wetting film resolution
R. Krishna, Y. Méheust, et al.
Chinese Academy of Science Journal Ranking System (2015–2023)
Cruz Y. Li (李雨桐), 李雨桐, et al.
Related Content
Experimental and numerical study of Rayleigh-Bénard convection affected by a rotating magnetic field
Physics of Fluids (April 1999)
Instabilities and spin-up behaviour of a rotating magnetic field driven flow in a rectangular cavity
Physics of Fluids (November 2017)
Nonaxisymmetric flow in a finite-length cylinder with a rotating magnetic field
Physics of Fluids (July 1999)
Spin-up of a liquid metal flow driven by a rotating magnetic field in a finite cylinder: A numerical and an analytical study
Physics of Fluids (May 2005)
Effects of viscosity and mass diffusion in hydrodynamically unstable plasma flows
Phys. Plasmas (August 2004)