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The Magneto-Rotational Instability Near Threshold: Spatio-Temporal Amplitude Equation and Saturation

Published online by Cambridge University Press:  15 August 2009

O. Regev*
Affiliation:
Department of Physics, Technion – Israel Institute of Technology, Israël Department of Astronomy, Columbia University, USA
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Abstract

We show, by means of a perturbative weakly nonlinear analysis, that the axisymmetric magneto-rotational instability (MRI) in a magnetic Taylor-Couette (mTC) flow in a thin-gap gives rise, for very small magnetic Prandtl numbers $({\cal P}_{\rm m})$, to a real Ginzburg-Landau equation for the disturbance amplitude. The saturation amplitude As is found to scale in this regime as ${\cal P}_{\rm m}^\delta$, with 1/2 < δ < 2/3 (depending on the boundary conditions adopted). The asymptotic results are shown to comply with numerical calculations performed by using a spectral code. They suggest that the transport due to the nonlinearly developed MRI may be vanishingly small for ${\cal P}_{\rm m} \ll$ 1.

Type
Research Article
Copyright
© EAS, EDP Sciences, 2009

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