Andre Weiner, Institute of Fluid Mechanics
workload and requirements
resources and communication
exercise time slot options
lecture and exercise on April 25 (next week)
recipe for issue reporting
an issue with issues
how to report properly
additional (optional) tips
see also: 45 Github Issues Dos and Don't
refer to the GitHub repository
source: F. X. Trias et al. (link)
Properties of turbulent flows:
source: J. H. Lee et al. (link)
source: Michal Choma (link)
Turbulence is not a well-defined problem awaiting solution but is a state of motion with innumerable different facets which depend on the context in which it occurs. We do not regard the state of laminar flow as a single problem; much less should turbulence be thought of as a single problem. The properties of turbulence are flow dependent, and therein lies the difficulty. Each turbulent flow field which is studied reveals new aspects of turbulence, and we are a very long way from being able to assemble a comprehensive physical description of this many-sided state of motion.
G. K. Batchelor in J. Fröhlich:
LES turbulenter Strömungen (p. 1)
What do we expect from a turbulence model?
... an ideal model should introduce the minimum amount of complexity while capturing the essence of the relevant physics.
D. C. Wilcox:
Turbulence modeling for CFD (p. 2)
What do we expect from a turbulence model?
most common modeling approaches
source: Martin Petry (link)
modeling complexity vs. efficiency
conservation of mass
$\mathbf{x} = (x, y, z)^T$, $\mathbf{u} = (u, v, w)^T$
compressibility condition
$$\frac{\mathrm{D}\rho}{\mathrm{D}t} = \frac{\partial \rho}{\partial t} + \mathbf{u}\cdot \nabla\rho = 0$$
$\begin{aligned} \frac{\partial \rho}{\partial t} + \nabla\cdot \left(\rho\mathbf{u}\right) &= \frac{\partial \rho}{\partial t} + \mathbf{u}\cdot\nabla\rho + \rho\nabla\cdot\mathbf{u}\\ &= \frac{\mathrm{D}\rho}{\mathrm{D}} + \rho\nabla\cdot\mathbf{u} \end{aligned}$
$$\rho\nabla\cdot\mathbf{u} = 0 \rightarrow \nabla\cdot\mathbf{u} = 0$$
conservation of momentum $$\frac{\partial \rho\mathbf{u}}{\partial t} + \nabla\cdot\left(\rho\mathbf{uu}\right) = \mathbf{f}$$
$$\mathbf{f} = \mathbf{f}_s + \mathbf{f}_b$$ external forces = surface forces + body forces
surface forces $$\mathbf{f}_s = \nabla\cdot \mathbf{S}$$
(total) stress tensor $$\mathbf{S} = \underbrace{-p\mathbf{I}}_{\text{pressure}} + \underbrace{\mathbf{\tau}}_{\text{viscous}}$$
$$p=-\mathrm{tr}(\mathbf{S})$$
gravitational body forces $$\mathbf{f}_b = \rho\mathbf{g}$$
$\mathbf{g}$ - gravitational acceleration vector
momentum equation with forces $$\frac{\partial \rho\mathbf{u}}{\partial t} + \nabla\cdot\left(\rho\mathbf{uu}\right) = -\nabla p + \nabla\cdot\mathbf{\tau} + \rho\mathbf{g}$$
Newtonian fluids $$\mathbf{\tau} = \mu \underbrace{\left(\nabla\mathbf{u} + (\nabla\mathbf{u})^T\right)}_{\text{strain rate}} + \lambda (\nabla\cdot \mathbf{u})\mathbf{I}$$
$\mu$ - dynamic viscosity, $\lambda = -2/3\mu$ - bulk viscosity
final (incompressible) form
$$\frac{\partial \rho\mathbf{u}}{\partial t} + \nabla\cdot\left(\rho\mathbf{uu}\right) = -\nabla
p + \nabla\cdot \left[\mu \left(\nabla\mathbf{u} + (\nabla\mathbf{u})^T\right)\right] +
\rho\mathbf{g}$$
constant density
$$\frac{\partial \mathbf{u}}{\partial t} + \nabla\cdot\left(\mathbf{uu}\right) = -\nabla
\tilde{p} + \nabla\cdot \left[\nu \left(\nabla\mathbf{u} + (\nabla\mathbf{u})^T\right)\right] +
\mathbf{g}$$
$\tilde{p} = p/\rho$ - kinematic pressure, $\nu = \mu/\rho$ - kinematic viscosity