Dynamics of spectrally truncated inviscid turbulence
arXiv:0712.2801 · doi:10.1063/1.2219766
Abstract
The evolution of the turbulent energy spectrum for the inviscid spectrally truncated Euler equations is studied by closure calculations. The observed behavior is similar to the one found in direct numerical simulations [Cichowlas, Bonaïtiti, Debbasch, and Brachet, Phys. Rev. Lett. 95, 264502 (2005)]. A Kolmogorov spectral range and an equipartition range are observed simultaneously. Between these two ranges a "quasi-dissipative" zone is present in the kinetic energy spectrum. The time evolution of the wave number that marks the beginning of the equipartition range is analyzed and it is shown that spectral nonlocal interactions are governing this evolution.
References in corpus (1)
Cited by in corpus (17)
- Cascades and transitions in turbulent flows
- Hyperviscosity, Galerkin truncation and bottlenecks in turbulence
- A neural network approach for the blind deconvolution of turbulent flows
- Bottleneck crossover between classical and quantum superfluid turbulence
- Cascades, thermalization and eddy viscosity in helical Galerkin truncated Euler flows
- Energy cascade with small-scales thermalization, counterflow metastability and anomalous velocity of vortex rings in Fourier-truncated Gross-Pitaevskii equation
- Energy cascade and the four-fifths law in superfluid turbulence
- Mesoscale Equipartition of kinetic energy in Quantum Turbulence
- Two-fluid model of the truncated Euler Equations
- Numerical Solutions of the Isotropic 3-Wave Kinetic Equation
- On the thermalization of the three-dimensional, incompressible, Galerkin-truncated Euler equation
- Large-scale bottleneck effect in two-dimensional turbulence
- Self-truncation and scaling in Euler-Voigt- and related fluid models
- Note on specific chiral ensembles of statistical hydrodynamics: "order function" for transition of turbulence transfer scenarios
- Chaotic motion in classical fluids with scale relativistic methods
- Relating statistics to dynamics in axisymmetric homogeneous turbulence
- Poles, Shocks and Tygers: The Time-reversible Burgers equation