We perform high-resolution numerical simulations of homogenous and isotropic compressible turbulence, with an average 3D Mach number close to 0.3. We study the statistical properties of intermittency for velocity, density, and entropy. For the velocity field, which is the only quantity that can be compared to the isotropic incompressible case, we find no statistical differences in its behavior in the inertial range due either to the slight compressibility or to the different dissipative mechanism. For the density field, we find evidence of “frontlike” structures, although no shocks are produced by the simulation
With the aim of determining the statistical properties of relativistic turbulence and unveiling nove...
PACS. 47.27Qb { Turbulent diusion. PACS. 47.27Gs { Isotropic turbulence; homogeneous turbulence. PAC...
Context. Supersonic turbulence is ubiquitous in the interstellar medium and plays an important role ...
We perform high-resolution numerical simulations of homogenous and isotropic compressible turbulence...
We perform high-resolution numerical simulations of homogenous and isotropic compressible turbulence...
We investigate how compressibility affects the turbulent statistics from a Lagrangian point of view,...
We study statistics and structures of pressure and density in the presence of large-scale shock wave...
Fully developed homogeneous isotropic turbulent fields, computed by direct numerical simulation, are...
Theory of turbulence at small scales plays a fundamental role in modeling turbulence and in retrievi...
With the aim of determining the statistical properties of relativistic turbulence and unveiling nove...
We report a detailed study of Eulerian and Lagrangian statistics from high resolution Direct Numeric...
general statistical theory of the intermittency in turbulence based on short-lived coherent structur...
The scaling and statistical properties of three-dimensional compressible turbulence are studied usin...
This paper considers compressible turbulent flows at low turbulent Mach numbers. Con-trary to the ge...
Compressible turbulence shapes the structure of the interstellar medium of our Galaxy and likely pla...
With the aim of determining the statistical properties of relativistic turbulence and unveiling nove...
PACS. 47.27Qb { Turbulent diusion. PACS. 47.27Gs { Isotropic turbulence; homogeneous turbulence. PAC...
Context. Supersonic turbulence is ubiquitous in the interstellar medium and plays an important role ...
We perform high-resolution numerical simulations of homogenous and isotropic compressible turbulence...
We perform high-resolution numerical simulations of homogenous and isotropic compressible turbulence...
We investigate how compressibility affects the turbulent statistics from a Lagrangian point of view,...
We study statistics and structures of pressure and density in the presence of large-scale shock wave...
Fully developed homogeneous isotropic turbulent fields, computed by direct numerical simulation, are...
Theory of turbulence at small scales plays a fundamental role in modeling turbulence and in retrievi...
With the aim of determining the statistical properties of relativistic turbulence and unveiling nove...
We report a detailed study of Eulerian and Lagrangian statistics from high resolution Direct Numeric...
general statistical theory of the intermittency in turbulence based on short-lived coherent structur...
The scaling and statistical properties of three-dimensional compressible turbulence are studied usin...
This paper considers compressible turbulent flows at low turbulent Mach numbers. Con-trary to the ge...
Compressible turbulence shapes the structure of the interstellar medium of our Galaxy and likely pla...
With the aim of determining the statistical properties of relativistic turbulence and unveiling nove...
PACS. 47.27Qb { Turbulent diusion. PACS. 47.27Gs { Isotropic turbulence; homogeneous turbulence. PAC...
Context. Supersonic turbulence is ubiquitous in the interstellar medium and plays an important role ...