Direct numerical simulation (DNS) of decaying compressible isotropic turbulence at turbulence Mach numbers of M-r = 0.2-0.7 and Taylor Reynolds numbers of 72 and 153 is performed by using the 7th order upwind-biased difference and 8th order center difference schemes. Results show that proper upwind-biased difference schemes can release the limit of "start-up" problem to Mach numbers. Compressibility effects on the statistics of turbulent flow as well as the mechanics of shocklets in compressible turbulence are also studied, and the conclusion is drawn that high Mach number leads to more dissipation. Scaling laws in compressible turbulence are also analyzed. Evidence is obtained that scaling laws and extended self similarity (ESS) hold in th...
The results of an asymptotic theory for statistical closures for compressible turbulence are explore...
Direct numerical simulation (DNS) of turbulent flows began in the early 1970s with the study of inco...
For weakly compressible turbulent fluctuations there exists a small parameter, the square of the flu...
Direct numerical simulation (DNS) of decaying compressible isotropic turbulence at turbulence Mach n...
To overcome the difficulty in the DNS of compressible turbulence at high turbulent Mach number, a ne...
Reynolds averaged Navier Stokes (RANS) solvers have become the workhorse for simulating turbulent fl...
© 2014 Elsevier Ltd. The influence of numerical dissipation on direct numerical simulation (DNS) of ...
This paper reviews the authors' recent studies on compressible turbulence by using direct numerical ...
This paper reviews the authors' recent studies on compressible turbulence by using direct numerical ...
We apply the gas-kinetic scheme (GKS) for the direct numerical simulations (DNSs) of compressible de...
Relationships between diverse thermodynamic quantities appropriate to weakly compressible turbulence...
In this study, we investigate the behaviour of decaying compressible anisotropic turbulence using Di...
A stable high-order numerical scheme for direct numerical simulation (DNS) of shock-free compressibl...
A stable high-order numerical scheme for direct numerical simulation (DNS) of shock-free compressibl...
Abstract This paper reviews the authors ’ recent studies on compressible turbulence by using direct ...
The results of an asymptotic theory for statistical closures for compressible turbulence are explore...
Direct numerical simulation (DNS) of turbulent flows began in the early 1970s with the study of inco...
For weakly compressible turbulent fluctuations there exists a small parameter, the square of the flu...
Direct numerical simulation (DNS) of decaying compressible isotropic turbulence at turbulence Mach n...
To overcome the difficulty in the DNS of compressible turbulence at high turbulent Mach number, a ne...
Reynolds averaged Navier Stokes (RANS) solvers have become the workhorse for simulating turbulent fl...
© 2014 Elsevier Ltd. The influence of numerical dissipation on direct numerical simulation (DNS) of ...
This paper reviews the authors' recent studies on compressible turbulence by using direct numerical ...
This paper reviews the authors' recent studies on compressible turbulence by using direct numerical ...
We apply the gas-kinetic scheme (GKS) for the direct numerical simulations (DNSs) of compressible de...
Relationships between diverse thermodynamic quantities appropriate to weakly compressible turbulence...
In this study, we investigate the behaviour of decaying compressible anisotropic turbulence using Di...
A stable high-order numerical scheme for direct numerical simulation (DNS) of shock-free compressibl...
A stable high-order numerical scheme for direct numerical simulation (DNS) of shock-free compressibl...
Abstract This paper reviews the authors ’ recent studies on compressible turbulence by using direct ...
The results of an asymptotic theory for statistical closures for compressible turbulence are explore...
Direct numerical simulation (DNS) of turbulent flows began in the early 1970s with the study of inco...
For weakly compressible turbulent fluctuations there exists a small parameter, the square of the flu...