Javascript must be enabled to continue!
Energy and enstrophy transfer in numerical simulations of two-dimensional turbulence
View through CrossRef
Numerical simulations of statistically steady two-dimensional (2-D) turbulence are analyzed to determine the relative importance of the types of wave-vector triad interactions that transfer energy and enstrophy in the both the energy and enstrophy inertial ranges. In the enstrophy inertial range, it is found (in agreement with previous studies [J. Fluid Mech. 72, 305 (1975); Phys. Fluids A 2, 1529 (1990)]) that the important triads (i.e., those associated with the highest transfer rates) are typically very elongated. On the average, nearly all of the enstrophy transfer within these triads is directed from the intermediate to the largest wave-number mode (i.e., downscale transfer). Energy, too, is transferred downscale in this manner, but is also transferred upscale due to the interaction of the intermediate with the smallest wave-number mode of the triad, resulting in no net flux of energy in the enstrophy inertial range. Analysis of the geometry of the important triads indicates they are not of similar shapes at all scales, and that the enstrophy transferring triads generally consist of one wave vector near the scale of the energetic peak, no matter how large the other wave vectors are. In the energy inertial range, elongated triads are also important. As in the enstrophy inertial range, there is downscale transfer of energy and enstrophy due to the interaction of the intermediate with the largest wave-number mode. There is also upscale transfer of both energy and enstrophy due to a very nonlocal interaction involving the smallest wave-number modes. The result is a net upscale flux of energy and no net flux of enstrophy in the energy inertial range. Comparison of the transfer functions from the simulations with those calculated by an eddy-damped quasinormal closure show agreement in the gross functional forms, but display certain quantitative differences in integrated quantities such as total transfer into and flux past a given wave number.
Title: Energy and enstrophy transfer in numerical simulations of two-dimensional turbulence
Description:
Numerical simulations of statistically steady two-dimensional (2-D) turbulence are analyzed to determine the relative importance of the types of wave-vector triad interactions that transfer energy and enstrophy in the both the energy and enstrophy inertial ranges.
In the enstrophy inertial range, it is found (in agreement with previous studies [J.
Fluid Mech.
72, 305 (1975); Phys.
Fluids A 2, 1529 (1990)]) that the important triads (i.
e.
, those associated with the highest transfer rates) are typically very elongated.
On the average, nearly all of the enstrophy transfer within these triads is directed from the intermediate to the largest wave-number mode (i.
e.
, downscale transfer).
Energy, too, is transferred downscale in this manner, but is also transferred upscale due to the interaction of the intermediate with the smallest wave-number mode of the triad, resulting in no net flux of energy in the enstrophy inertial range.
Analysis of the geometry of the important triads indicates they are not of similar shapes at all scales, and that the enstrophy transferring triads generally consist of one wave vector near the scale of the energetic peak, no matter how large the other wave vectors are.
In the energy inertial range, elongated triads are also important.
As in the enstrophy inertial range, there is downscale transfer of energy and enstrophy due to the interaction of the intermediate with the largest wave-number mode.
There is also upscale transfer of both energy and enstrophy due to a very nonlocal interaction involving the smallest wave-number modes.
The result is a net upscale flux of energy and no net flux of enstrophy in the energy inertial range.
Comparison of the transfer functions from the simulations with those calculated by an eddy-damped quasinormal closure show agreement in the gross functional forms, but display certain quantitative differences in integrated quantities such as total transfer into and flux past a given wave number.
.
Related Results
Impact of magneto-rotational instability on grain growth in protoplanetary disks
Impact of magneto-rotational instability on grain growth in protoplanetary disks
Grain growth in protoplanetary disks is the first step towards planet formation. One of the most important pieces in the grain growth model is calculating the collisional velocity ...
Quantum turbulence
Quantum turbulence
Abstract
Chapter 5 delves into quantum turbulence in superfluid helium and atomic Bose-Einstein condensates (BECs). The foundation of quantum turbulence research ...
Stagnation Region Heat Transfer Augmentation at Very High Turbulence Levels
Stagnation Region Heat Transfer Augmentation at Very High Turbulence Levels
A database for stagnation region heat transfer has been extended to include heat transfer measurements acquired downstream from a new high intensity turbulence generator. This work...
Effects of Turbulence Intensity and Scale on Turbine Blade Heat Transfer
Effects of Turbulence Intensity and Scale on Turbine Blade Heat Transfer
The effects of turbulence intensity and length scale on turbine blade heat transfer and aerodynamic losses are investigated. The importance of freestream turbulence on heat transfe...
Characteristic parameters of adaptive optical imaging system in oceanic turbulence
Characteristic parameters of adaptive optical imaging system in oceanic turbulence
Since recently one is interested in underwater communications, imaging, sensing and lidar appeared, it is important to study characteristic parameters of the adaptive optical imagi...
Passive scalar mixing: Analytic study of time scale ratio, variance, and mix rate
Passive scalar mixing: Analytic study of time scale ratio, variance, and mix rate
Some very reasonable approximations, consistent with numerical and experimental evidence, were applied to the skewness and palinstrophy coefficients in the dissipation equations to...
Variation of enstrophy production and strain rotation relation in a turbulent boundary layer
Variation of enstrophy production and strain rotation relation in a turbulent boundary layer
The production of enstrophy is strongly coupled to the vortex stretching process that is of inherent importance to the cascading process, one of the driving processes of turbulence...
Unraveling the lidar-turbulence paradox
Unraveling the lidar-turbulence paradox
The meteorological community, and in particular the wind energy community, have been trying to establish a methodology to correct/convert turbulence measures derived from measureme...

