We find an asymptotic expression for the characteristic timescales of decorrelation processes in weakly compressible and isothermal turbulence. This result is used in the Eddy-Damped Quasi-Normal Markovian equation to derive the scalings of compressible energy spectra: (1) if the acoustic waves are dominant, the compressible energy spectra exhibit scaling; (2) if local eddy straining is dominant, the compressible energy spectra are scaled as . Meanwhile, the energy spectra of incompressible components display the same scaling of as those in incompressible turbulence. The direct numerical simulations of weakly compressible turbulence are used to examine the scaling.</p
The physical nature of compressible turbulence is of fundamental importance in a variety of astrophy...
This letter investigates the compressible energy transfer process. We extend a methodology developed...
The energy spectrum in the inertial and dissipation ranges in two-dimensional steady turbulence is e...
We find an asymptotic expression for the characteristic timescales of decorrelation processes in wea...
This paper proposes temporal scaling laws of the density-weighted energy spectrum for compressible t...
An extensive investigation of velocity fluctuation spectra has been performed in the weakly compress...
Scaling arguments are applied directly to the Navier-Stokes equations with the isentropic-flow stipu...
In this paper we develop spectral laws for the small- and large-wavenumber regimes of the energy and...
In this work, direct numerical simulations of the compressible fluid equations in turbulent regimes ...
In statistically stationary conditions, the turbulent energy spectrum in a high Reynolds number flow...
An exact relation has been derived for homogeneous polytropic turbulence in terms of the two-point f...
In the study of weakly turbulent wave systems possessing incomplete self-similarity, it is possible ...
We study precessing turbulence, which appears in several geophysical and astrophysical systems, by d...
In the study of weakly turbulent wave systems possessing incomplete self-similarity it is possible t...
Decaying turbulence is studied numerically using as initial condition a random flow whose shell-inte...
The physical nature of compressible turbulence is of fundamental importance in a variety of astrophy...
This letter investigates the compressible energy transfer process. We extend a methodology developed...
The energy spectrum in the inertial and dissipation ranges in two-dimensional steady turbulence is e...
We find an asymptotic expression for the characteristic timescales of decorrelation processes in wea...
This paper proposes temporal scaling laws of the density-weighted energy spectrum for compressible t...
An extensive investigation of velocity fluctuation spectra has been performed in the weakly compress...
Scaling arguments are applied directly to the Navier-Stokes equations with the isentropic-flow stipu...
In this paper we develop spectral laws for the small- and large-wavenumber regimes of the energy and...
In this work, direct numerical simulations of the compressible fluid equations in turbulent regimes ...
In statistically stationary conditions, the turbulent energy spectrum in a high Reynolds number flow...
An exact relation has been derived for homogeneous polytropic turbulence in terms of the two-point f...
In the study of weakly turbulent wave systems possessing incomplete self-similarity, it is possible ...
We study precessing turbulence, which appears in several geophysical and astrophysical systems, by d...
In the study of weakly turbulent wave systems possessing incomplete self-similarity it is possible t...
Decaying turbulence is studied numerically using as initial condition a random flow whose shell-inte...
The physical nature of compressible turbulence is of fundamental importance in a variety of astrophy...
This letter investigates the compressible energy transfer process. We extend a methodology developed...
The energy spectrum in the inertial and dissipation ranges in two-dimensional steady turbulence is e...