Viscous, resistive magnetohydrodynamic stability computed by spectral techniques
Author(s) -
R. B. Dahlburg,
T. A. Zang,
David Montgomery,
M. Yousuff Hussaini
Publication year - 1983
Publication title -
proceedings of the national academy of sciences
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 5.011
H-Index - 771
eISSN - 1091-6490
pISSN - 0027-8424
DOI - 10.1073/pnas.80.18.5798
Subject(s) - magnetic diffusivity , reynolds number , hagen–poiseuille equation , wavenumber , couette flow , marginal stability , hydrodynamic stability , physics , magnetohydrodynamic drive , magnetic reynolds number , mechanics , instability , mathematics , mathematical analysis , linear stability , chebyshev polynomials , laminar flow , classical mechanics , magnetohydrodynamics , viscosity , flow (mathematics) , magnetic field , thermodynamics , turbulence , optics , quantum mechanics
Expansions in Chebyshev polynomials are used to study the linear stability of one-dimensional magnetohydrodynamic quasiequilibria, in the presence of finite resistivity and viscosity. The method is modeled on the one used by Orszag in accurate computation of solutions of the Orr-Sommerfeld equation. Two Reynolds-like numbers involving Alfvén speeds, length scales, kinematic viscosity, and magnetic diffusivity govern the stability boundaries, which are determined by thegeometric mean of the two Reynolds-like numbers. Marginal stability curves, growth rates versus Reynolds-like numbers, and growth rates versus parallel wave numbers are exhibited. A numerical result that appears general is that instability has been found to be associated with inflection points in the current profile, though no general analytical proof has emerged. It is possible that nonlinear subcritical three-dimensional instabilities may exist, similar to those in Poiseuille and Couette flow.
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