On the Linear Stability of Weakly-Ionized, Magnetized Planar Shear Flows

Details On the Linear Stability of Weakly-Ionized, Magnetized Planar Shear Flows On the Linear Stability of Weakly-Ionized, Magnetized Planar Shear Flows

2008-01-07

arxiv.org/abs/0801.0974v1

Astronomy and Astrophysics

Astrophysics

18 pages, 8 figures; accepted by MNRAS

Scientific paper

10.1111/j.1365-2966.2008.12928.x

We investigate the effects of ambipolar diffusion and the Hall effect on the stability of weakly-ionized, magnetized planar shear flows. Employing a local approach similar to the shearing-sheet approximation, we solve for the evolution of linear perturbations in both streamwise-symmetric and non-streamwise-symmetric geometries using WKB techniques and/or numerical methods. We find that instability arises from the combination of shear and non-ideal magnetohydrodynamic processes, and is a result of the ability of these processes to influence the free energy path between the perturbations and the shear. They turn what would be simple linear-in-time growth due to current and vortex stretching from shear into exponentially-growing instabilities. Our results aid in understanding previous work on the behaviour of weakly-ionized accretion discs. In particular, the recent finding that the Hall effect and ambipolar diffusion destabilize both positive and negative angular velocity gradients acquires a natural explanation in the more general context of this paper. We construct a simple toy model for these instabilities based upon transformation operators (shears, rotations, and projections) that captures both their qualitative and, in certain cases, exact quantitative behaviour.

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