Three-dimensional stabilization mechanism for the auroral Farley-Buneman instability

Details Three-dimensional stabilization mechanism for the auroral Farley-Buneman instability Three-dimensional stabilization mechanism for the auroral Farley-Buneman instability

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992jatp...54.1633j&link_type=abstract

Journal of Atmospheric and Terrestrial Physics (ISSN 0021-9169), vol. 54, no. 11-12, p. 1633-1641, 1643.

Physics

6

Atmospheric Models, Auroral Electrojets, E Region, Magnetohydrodynamic Stability, Three Dimensional Models, Magnetic Field Configurations, Plasma Drift, Two Fluid Models

Scientific paper

The effect of the three-dimensional auroral geometry on the saturation of the gradient drift instability and the Farley-Buneman instability of the auroral ionospheric E-region, using three-dimensional two-fluid simulations of the E-region irregularities. The simulations show 3D altitude coupling in the auroral ionosphere that significantly damps the otherwise extremely unstable Farley-Buneman waves.

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