21 research outputs found
Taylor's (1935) dissipation surrogate reinterpreted
New results from direct numerical simulation of decaying isotropic turbulence show that Taylorâs expression for the viscous dissipation rate Δ = CΔU3/L is more appropriately interpreted as a surrogate for the inertial energy flux. As a consequence, the well known dependence of the Taylor prefactor CΔ on Reynolds number CΔ(RL)âCΔ,â can be understood as corresponding to the onset of an inertial range
Flux and dissipation of energy in the LET theory of turbulence
The first part of this thesis examines and compares the separate closure formalisms
of Wyld and Martin, Siggia, and Rose (MSR). The simplicity of Wyldâs perturbation
scheme is offset by an incorrect renormalisation, this contrasts with the formally exact
analysis of MSR. The work here shows that a slight change in Wyldâs renormalisation
keeps the main results intact and, in doing so, demonstrates that this formalism is
equivalent to MSR.
The remainder of the thesis is concerned with turbulent dissipation. A numerical
solution of the Local Energy Transfer theory, or LET, is reworked and extended
to compute decaying and forced turbulence at large Reynolds numbers. Using this
numerical simulation, the phenomenon of turbulent dissipation is investigated.
In order to use decaying turbulence to study the turbulent dissipation rate as a
function of Reynolds number, it is necessary to choose an appropriate time with which
a measurement can be taken. Using phenomenological arguments of the evolution of a
turbulent fluid, criteria for establishing such a time are developed.
An important study in turbulence is the dissipation rate in the limit of vanishing
viscosity, also known as the dissipation anomaly. This thesis derives an equation for the
dissipation rate from the spectral energy balance equation. Using the LET computation
for both decaying and forced turbulence, results are obtained that can be used along
with the equation to study the mechanisms behind the dissipation anomaly. It is found
that there is a difference in the behaviour of the normalised dissipation rate between
decaying and forced turbulence and, for both cases, it is largely controlled by the energy
flux
Turbulent states in plane Couette flow with rotation
Shearing and rotational forces in fluids can significantly alter the
transport of momentum.A numerical investigation was undertaken to study the
role of these forces using plane Couette flow subject to rotation about an axis
perpendicular to both wall-normal and streamwise directions. Using a set of
progressively higher Reynolds numbers up to Re = 5200, we find that the torque
for a given Re is a non-monotonic function of rotation number, Ro. For
low-to-moderate turbulent Reynolds numbers we find a maximum that is associated
with flow fields that are dominated by downstream vortices and calculations of
2-d vortices capture the maximum also quantitatively. For higher shear Reynolds
numbers a second stronger maximum emerges at smaller rotation numbers, closer
to non-rotating plane Couette flow. It is carried by flows with a markedly 3-d
structure and cannot be captured by 2-d vortex studies. As the Reynolds number
increases, this maximum becomes stronger and eventually overtakes the one
associated with the 2-d flow state.Comment: 15 pages, 10 figure
Publisher Correction: Demonstration of reduced neoclassical energy transport in Wendelstein 7-X
Flux and dissipation of energy in the LET theory of turbulence
The first part of this thesis examines and compares the separate closure formalisms of Wyld and Martin, Siggia, and Rose (MSR). The simplicity of Wyldâs perturbation scheme is offset by an incorrect renormalisation, this contrasts with the formally exact analysis of MSR. The work here shows that a slight change in Wyldâs renormalisation keeps the main results intact and, in doing so, demonstrates that this formalism is equivalent to MSR. The remainder of the thesis is concerned with turbulent dissipation. A numerical solution of the Local Energy Transfer theory, or LET, is reworked and extended to compute decaying and forced turbulence at large Reynolds numbers. Using this numerical simulation, the phenomenon of turbulent dissipation is investigated. In order to use decaying turbulence to study the turbulent dissipation rate as a function of Reynolds number, it is necessary to choose an appropriate time with which a measurement can be taken. Using phenomenological arguments of the evolution of a turbulent fluid, criteria for establishing such a time are developed. An important study in turbulence is the dissipation rate in the limit of vanishing viscosity, also known as the dissipation anomaly. This thesis derives an equation for the dissipation rate from the spectral energy balance equation. Using the LET computation for both decaying and forced turbulence, results are obtained that can be used along with the equation to study the mechanisms behind the dissipation anomaly. It is found that there is a difference in the behaviour of the normalised dissipation rate between decaying and forced turbulence and, for both cases, it is largely controlled by the energy flux.EThOS - Electronic Theses Online ServiceGBUnited Kingdo