Skip to main content
U.S. Department of Energy
Office of Scientific and Technical Information

Kelvin-Helmholtz instabilities of supersonic shear layers

Journal Article · · Astrophys. J.; (United States)
DOI:https://doi.org/10.1086/162311· OSTI ID:6045490
A study is made of the stability of finite-thickness compressible shear layers, v = zv/sub z/(x). Two different velocity profiles are investigated in detail using the analogy between the pressure perturbation, deltap = f(x) exp (i(k/sub y/y+k/sub z/z-..omega..t)), and the bound and scattering wave states of the one-dimensional Schroedinger equation. By analytical and numerical methods, fairly complete contour maps have been generated for the real and imaginary parts of the wave frequency (..omega../sub r/ and ..omega../sub i/) as a function of the two free dimensionless parameters, the ''reduced Mach number,'' Aequivalentk/sub z/v/sub z/m/(kc/sub s/), and the wavenumber, BequivalentkL. Here, v/sub z/(x = +- infinity) = +- v/sub z/m, (k/sub y//sup 2/ +k/sub z//sup 2/)/sup 1/2/, c/sub s/ is the adiabatic sound speed, and L is a length characterizing the thickness of the shear layer. Two distinct regimes of instability are delineated in the (A,B)-plane. In one regime there are unstable standing waves which are analogous to the well-known Kelvin- Helmholtz warping instability of a vortex sheet (where v/sub z/(x) is a step function). In the second regime, there are unstable traveling wave modes which are absent in the case of a vortex sheet.
Research Organization:
Department of Electrical Engineering, Cornell University
OSTI ID:
6045490
Journal Information:
Astrophys. J.; (United States), Journal Name: Astrophys. J.; (United States) Vol. 283:1; ISSN ASJOA
Country of Publication:
United States
Language:
English