56th Annual Meeting of the APS Division of Plasma Physics
Volume 59, Number 15
Monday–Friday, October 27–31, 2014;
New Orleans, Louisiana
Session DI2: Waves in Plasmas
3:00 PM–5:00 PM,
Monday, October 27, 2014
Room: Bissonet
Chair: Joel Fajans, University of California, Berkeley
Abstract ID: BAPS.2014.DPP.DI2.2
Abstract: DI2.00002 : Laboratory Studies of Nonlinear Interactions Relevant to Alfv\'{e}n Wave Decay Instabilities*
3:30 PM–4:00 PM
Preview Abstract
Abstract
Author:
Seth Dorfman
(University of California, Los Angeles)
Alfv\'{e}n waves, a fundamental mode of magnetized plasmas, are ubiquitous in both laboratory and space plasmas. Many theoretical predictions show that these waves may be unstable to various decay instabilities (e.g. [1,2]). Despite the possible importance of these processes in problems such as the heating of the solar corona and the transfer of energy to small spacial scales in the solar wind, observational evidence is limited. The present work at UCLA's Large Plasma Device (LAPD) represents the first fundamental laboratory study of the non-linear Alfv\'{e}n wave interactions responsible for this class of instabilities; in particular, we present 1) laboratory observation of the Alfv\'{e}n-acoustic mode coupling at the heart of the Parametric Decay Instability [3] and 2) laboratory observations consistent with a decay instability in which a Kinetic Alfv\'{e}n Wave (KAW) decays into two co-propagating KAWs. The first study is conducted by launching counterpropagating Alfv\'{e}n waves from antennas placed at either end of the LAPD. A resonance in the beat wave response produced by the two launched Alfv\'{e}n waves is observed and is identified as a damped ion acoustic mode based on the measured dispersion relation. Results are consistent with theoretical predictions for a three-wave interaction driven by a nonlinear ponderomotive force. In the second experiment, a single high-frequency $\omega/\omega_{ci}\sim0.7$ Alfv\'{e}n wave is launched, resulting in two daughter modes with frequencies and wave numbers that suggest co-propagating KAWs produced by decay of the pump wave. The observed process is parametric in nature, with the frequency of the daughter modes varying as a function of pump amplitude. Efforts are underway to fully characterize the second set of experiments and compare with decay instabilities predicted by theory and simulations.
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[1] JV Hollweg, J. Geophys. Res. 99, 23 431 (1994).\\[0pt]
[2] YM Voitenko, Journal of plasma physics 60.03 (1998).\\[0pt]
[3] S Dorfman and T Carter, Phys. Rev. Lett. 110, 195001 (2013).
*Supported by DOE, NSF, and DOE FES and NASA Eddy Postdoctoral Fellowships
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2014.DPP.DI2.2