Effects of the Kelvin-Helmholtz surface instability on supersonic jets
Author(s) -
P. E. Hardee
Publication year - 1983
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/161022
Subject(s) - physics , supersonic speed , instability , mechanics , jet (fluid) , turbulence , wavenumber , phase velocity , computational physics , classical mechanics , astrophysics , optics
We have performed an exact numerical calculation of the linear growth and phase velocity of Kelvin-Helmholtz unstable wave modes on a supersonic jet of cylindrical cross section. An expression for the maximally unstable wavenumber of each wave mode is found. Provided a sharp velocity discontinuity exists, all wave modes are unstable. A combination of rapid jet expansion and velocity shear across a jet can effectively stabilize all wave modes. The more likely case of slow jet expansion and of velocity shear at the jet surface allows wave modes with maximally unstable wavelength longer than or on the order of the jet radius to grow. The relative energy in different wave modes and effect on the jet is investigated. Energy input into a jet resulting from surface instability is discussed and the effect on source morphology is considered.
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