Toward Astrophysical Turbulence in the Laboratory
G. G. Howes, D. J. Drake, K. D. Nielson, T. A. Carter, C. A. Kletzing,, and F. Skiff

TL;DR
This paper reports the first laboratory experiment confirming the nonlinear interaction between counterpropagating Alfven waves, a key process in astrophysical plasma turbulence, thus bridging theory and real plasma observations.
Contribution
It provides the first experimental verification of Alfven wave interactions, supporting theoretical models of plasma turbulence in space environments.
Findings
First laboratory measurement of Alfven wave interaction
Supports theoretical models of astrophysical turbulence
Establishes experimental basis for plasma turbulence studies
Abstract
Turbulence is a ubiquitous phenomenon in space and astrophysical plasmas, driving a cascade of energy from large to small scales and strongly influencing the plasma heating resulting from the dissipation of the turbulence. Modern theories of plasma turbulence are based on the fundamental concept that the turbulent cascade of energy is caused by the nonlinear interaction between counterpropagating Alfven waves, yet this interaction has never been observationally or experimentally verified. We present here the first experimental measurement in a laboratory plasma of the nonlinear interaction between counterpropagating Alfven waves, the fundamental building block of astrophysical plasma turbulence. This measurement establishes a firm basis for the application of theoretical ideas developed in idealized models to turbulence in realistic space and astrophysical plasma systems.
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