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Comment on “Linear instability of magnetic Taylor-Couette flow with Hall effect”

M. Rheinhardt and U. Geppert
Phys. Rev. E 71, 038301 – Published 11 March 2005

Abstract

In the paper we comment on [Rüdiger and Shalybkov (RS), Phys. Rev. E 69, 016303 (2004) ], the instability of the Taylor-Couette flow interacting with a homogeneous background field subject to the Hall effect is studied. We correct a falsely generalizing interpretation of results presented there which could be taken to disprove the existence of the Hall-drift-induced magnetic instability described in Rheinhardt and Geppert, Phys. Rev. Lett. 88, 101103 (2002). It is shown that, in contrast to what is suggested by RS, no additional shear flow is necessary to enable such an instability with a nonpotential magnetic background field, whereas for a curl-free one it is. In the latter case, the instabilities found in RS in situations where neither a hydrodynamic nor a magnetorotational instability exists are demonstrated to be most likely magnetic instead of magnetohydrodynamic. Further, some minor inaccuracies are clarified.

  • Figure
  • Received 5 February 2004

DOI:https://doi.org/10.1103/PhysRevE.71.038301

©2005 American Physical Society

Authors & Affiliations

M. Rheinhardt* and U. Geppert

  • Astrophysikalisches Institut Potsdam, An der Sternwarte 16, D-14482, Potsdam, Germany

  • *Electronic address: mreinhardt@aip.de
  • Present address: Max-Planck-Institut für Extraterrestriche Physik, Giessenbachstrasse, D-85748 Garching, Germany.Electronic address: urme@xray.mpe.mpg.de

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Original Article

Linear instability of magnetic Taylor-Couette flow with Hall effect

Günther Rüdiger and Dima Shalybkov
Phys. Rev. E 69, 016303 (2004)

References (Subscription Required)

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Issue

Vol. 71, Iss. 3 — March 2005

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Images

  • Figure 1
    Figure 1
    Growth rates (thick) and wave numbers (thin) of the most unstable axisymmetric magnetic-field modes (kinematic case, u=0) as a function of the background field strength. Length, time, and magnetic field are normalized by Rout, Rout2η, and ηβ, respectively. Bmax represents the maximum of the background field profile. RinRout=η̂=0.5. Boundary conditions as defined in RS. Vacuum-vacuum: solid; inner perfect conductor–outer vacuum: dashed; perfect conductor–perfect conductor: dot-dashed. The eigenmodes are nonoscillatory in the first two cases, but oscillatory in the third. Interestingly, for the vacuum-vacuum boundary condition, the instability emerges roughly at Bmax3 as in the plane model.Reuse & Permissions
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