Stability of internal gravity wave beams to three-dimensional modulations

• Published in: Journal of fluid mechanics Vol. 736; pp. 67 - 90
• Main Authors: Kataoka, T., Akylas, T. R.
• Format: Journal Article
• Language: English
• Published: Cambridge, UK Cambridge University Press 10.12.2013
• Subjects: Beams (radiation); Brunt-vaisala frequency; Dimensional stability; Earth, ocean, space; Exact sciences and technology; External geophysics; Geophysics. Techniques, methods, instrumentation and models; Gravitation; Gravitational waves; Gravity; Gravity waves; Instability; Internal waves; Perturbations; Slopes; Stability; Wavelength; geophysical and geological flows; internal waves; instability; Linear stability; Eigenvalue problem; Internal gravity wave; Geophysical fluid dynamics
• ISSN: 0022-1120; 1469-7645
• DOI: 10.1017/jfm.2013.527

The linear stability of uniform, plane internal wave beams with locally confined spatial profile, in a stratified fluid of constant buoyancy frequency, is discussed. The associated eigenvalue problem is solved asymptotically, assuming perturbations of long wavelength relative to the beam width. In this limit, instability is found only for oblique disturbances which vary in the along-beam and the horizontal transverse directions. The mechanism of instability is a first-harmonic–mean resonant interaction between the underlying wave beam and three-dimensional perturbations that comprise a time-harmonic component, with the beam frequency, and a mean flow. Progressive beams which transport energy in one direction, in particular, are unstable if the beam steepness exceeds a certain threshold value, whereas purely standing beams are unstable even at infinitesimal steepness. A distinguishing feature of this three-dimensional modulational instability is the generation of circulating horizontal mean flows at large distances from the vicinity of the beam.