Three-dimensional linear stability of a weak, compressible shock layer is analyzed using exact Reynolds-number-independent forms of the governing base flow and linear stability equations, obtained by rescaling the problem onto the shock's own natural viscous length and time scales. For any base flow with zero transverse velocity components, depending on the shock-normal coordinate alone, the resulting eigenvalue problem is proved covariant under rotation of the transverse wavenumber vector: the eigenvalue depends on the transverse wavenumbers only through their magnitude, and every three-dimensional eigenmode, throughout the continuous spectrum, decouples exactly into two independent constituents. A two-dimensional, in-plane acoustic--entropy branch carries the disturbance's entire dilatation, pressure and thermodynamic coupling, and a one-dimensional, out-of-plane purely solenoidal vortical branch is governed by a single scalar shear-diffusion equation. Three-dimensional shock-layer stability is thus resolved exactly into its compressible and vortical constituents, confirmed to machine precision by the Grosch--Salwen far-field companion spectra. Both decoupled operators carry an explicit damping term growing with the total transverse wavenumber, so a three-dimensional, oblique disturbance is never less stable than the two-dimensional disturbance sharing its in-plane wavenumber alone; the vortical branch, whose spectrum is controlled directly by this term, is shown to retreat from the imaginary axis in close proportion to the wavenumber squared. This finding is an exact, Reynolds-free analogue of Squire's classical theorem, with the stabilizing role of Reynolds number played here by the transverse wavenumber magnitude.
While accurate description of the internal structure of strong shock layers is beyond the scope of the Navier–Stokes equations [2, 4, 18, 30], continuum equations may still be used to describe weak shock layers at low Mach numbers. The present work extends the steady laminar base flow model of [11] and the two-dime...
We establish the asymptotic stability of planar viscous shock waves for the outflow problem of the three-dimensional barotropic compressible Navier--Stokes equations in a half-space, with periodic boundary conditions imposed in the transverse directions. For a weak shock located sufficiently far from the boundary, we p...
Moon-Jin Kang, Hyeonseop Kim, Ho-Bin Lee· 0 citations
How the local energy transfer across scales in turbulence is encoded in the instantaneous deformation of fluid elements remains a fundamental question. We exploit the spherical geometry of the real-space energy cascade at length scale $\ell$. An exact derivation shows that it can be decomposed locally by strain self-am...
Abstract Content of image described in text. We study temporal instabilities of an inviscid, compressible, hyperbolic tangent shear layer. For this, we use a newly developed algorithm to avoid spurious modes based on remapping of the physical transverse coordinate using the analytic flow profile and connecting Frobeniu...
S. Görtz, L. DeBroeck, Paul Hollmann et al.· Journal of Fluid Mechanics· 0 citations
This paper studies the existence and asymptotic stability of traveling shock waves for the one-dimensional full compressible Navier--Stokes--Poisson equations, which model viscous heat-conducting ions in a self-consistent electrostatic field. We first prove the existence and uniqueness of a smooth shock profile of smal...
Using a comprehensive set of three-dimensional, high-resolution direct numerical simulations, we investigate the existence of a dissipative anomaly in isothermal, homogeneous, isotropic compressible turbulence driven by solenoidal forcing. We find that the total kinetic-energy dissipation rate, as well as its solenoida...
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