| タイトル | Viscous, resistive magnetohydrodynamic stability computed by spectral techniques |
| 著者（英） | Hussaini, M. Y.; Zang, T. A.; Dahlburg, R. B.; Montgomery, D. |
| 著者所属（英） | College of William and Mary|NASA Langley Research Center |
| 発行日 | 1983-09-01 |
| 言語 | eng |
| 内容記述 | Expansions in Chebyshev polynomials are used to study the linear stability of one-dimensional magnetohydrodynamic quasi-equilibria, 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 Alfven speeds, length scales, kinematic viscosity, and magnetic diffusivity govern the stability boundaries, which are determined by the geometric 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. |
| NASA分類 | PLASMA PHYSICS |
| レポートNO | 84A12275 |
| 権利 | Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/400838 |
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