Literature DB >> 27232026

Observation of an Alfvén Wave Parametric Instability in a Laboratory Plasma.

S Dorfman1, T A Carter1.   

Abstract

A shear Alfvén wave parametric instability is observed for the first time in the laboratory. When a single finite ω/Ω_{i} kinetic Alfvén wave (KAW) is launched in the Large Plasma Device above a threshold amplitude, three daughter modes are produced. These daughter modes have frequencies and parallel wave numbers that are consistent with copropagating KAW sidebands and a low frequency nonresonant mode. The observed process is parametric in nature, with the frequency of the daughter modes varying as a function of pump wave amplitude. The daughter modes are spatially localized on a gradient of the pump wave magnetic field amplitude in the plane perpendicular to the background field, suggesting that perpendicular nonlinear forces (and therefore k_{⊥} of the pump wave) play an important role in the instability process. Despite this, modulational instability theory with k_{⊥}=0 has several features in common with the observed nonresonant mode and Alfvén wave sidebands.

Year:  2016        PMID: 27232026     DOI: 10.1103/PhysRevLett.116.195002

Source DB:  PubMed          Journal:  Phys Rev Lett        ISSN: 0031-9007            Impact factor:   9.161


  2 in total

1.  Parametric Instability, Inverse Cascade, and the 1/f Range of Solar-Wind Turbulence.

Authors:  Benjamin D G Chandran
Journal:  J Plasma Phys       Date:  2018-01-25       Impact factor: 2.014

2.  How Alfvén waves energize the solar wind: heat vs work.

Authors:  Jean C Perez; Benjamin D G Chandran; Kristopher G Klein; Mihailo M Martinović
Journal:  J Plasma Phys       Date:  2021-04-14       Impact factor: 2.014

  2 in total

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