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arxiv: 1204.6339 · v1 · pith:4FUXQ7QLnew · submitted 2012-04-27 · ⚛️ physics.flu-dyn · astro-ph.IM

Observation of a Free-Shercliff-Layer Instability in Cylindrical Geometry

classification ⚛️ physics.flu-dyn astro-ph.IM
keywords instabilitynumberaxialelsasserfree-shercliff-layergloballayermode
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We report on observations of a free-Shercliff-layer instability in a Taylor-Couette experiment using a liquid metal over a wide range of Reynolds numbers, $Re\sim 10^3-10^6$. The free Shercliff layer is formed by imposing a sufficiently strong axial magnetic field across a pair of differentially rotating axial endcap rings. This layer is destabilized by a hydrodynamic Kelvin-Helmholtz-type instability, characterized by velocity fluctuations in the $r-\theta$ plane. The instability appears with an Elsasser number above unity, and saturates with an azimuthal mode number $m$ which increases with the Elsasser number. Measurements of the structure agree well with 2D global linear mode analyses and 3D global nonlinear simulations. These observations have implications for a range of rotating MHD systems in which similar shear layers may be produced.

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