Experimental Verification of the Stationary Inertial Alfven Wave and its Relevance to Auroral Plasma Physics

COFFEE_KLATCH  · Invited

Abstract

A small, off-axis mesh anode electrode at one plasma-column end is used to create a paraxial channel of both electron current and depleted density in the Large Plasma Device Upgrade (LAPD-U) at UCLA. It is shown that the on-axis, larger, surrounding-plasma column rotates about its cylindrical axis because a radial electric field is imposed by a multiple-segmented-disk termination electrode on the same end as the mesh-anode electrode. The radial profile of azimuthal velocity is shown to be consistent with rigid-body rotation. Launched inertial Alfven waves are shown to concentrate in the off-axis channel of electron current and depleted plasma density. In the absence of launched waves, time varying boundary conditions, or spatially structured boundary conditions, we demonstrate that a non-fluctuating, non-traveling pattern in the plasma density arises spontaneously in the channel, but only in the combined presence of electron current, density depletion, and cross-field convection (i.e., rotation). The experimental verification of stationary inertial Alfven waves is based on these results and the predictions from a model of finite-collisionality, finite-pressure stationary Alfven waves that links laboratory and auroral plasma regimes. Ground-based optical observations will be shown that indicate the need for a quasi- static theory of structured electron acceleration within auroral arcs. The properties of the stationary inertial Alfven wave suggest it as promising candidate.

*This work is supported by the BAPSF (at UCLA), NSF (US), DoE (US), and the National Sciences and Engineering Research Council (Canada). This work is performed in collaboration with S. M. Finnegan, D. J. Knudsen, S. Vincena, M. Tornquist, and E. Donovan.

Authors

  • Mark Koepke

    • Department of Physics, West Virginia University, Morgantown, WV 26506