The Kelvin-Helmholtz instability occurs at the interface between two fluids moving at different velocities. This instability is characterized by the formation of characteristic spiral vortices, which can be observed in nature, for example in clouds or on the surface of oceans.
The system is initialized with two fluid layers separated by a shear layer of thickness
- A central layer with negative velocity
$-U$ - An outer layer with positive velocity
$U$
To initiate the shear layers, we take an initial velocity written as:
where
With the definition of vorticity in 2D, we can find the initial vorticity:
Demonstration
We start from the definition of vorticity in 2D:
$$ \omega = \frac{\partial v}{\partial x} - \frac{\partial u}{\partial y} $$
Since
$$ \frac{d}{ds} erf(s) = \frac{2}{\sqrt{\pi}} e^{-s^2} $$
By making the following change of variable
$$ \begin{aligned} \omega &= - \frac{\partial u}{\partial y} = - U \frac{d}{dy}erf(\frac{y}{\delta}) - \frac{\partial u'}{\partial y}\ &= -\frac{U}{\delta} \frac{d}{ds}erf(s) + \omega' \end{aligned} $$
We thus obtain:
$$ \omega(x,y,0) = -\frac{U}{\delta} \frac{2}{\sqrt{\pi}} e^{-(\frac{y}{\delta})^2} + \omega'(x,y) $$
We need to non-dimensionalize the initial condition. For this, we introduce the same characteristic quantities as for the non-dimensionalization of the Navier-Stokes equations:
-
$L$ : characteristic length -
$U$ : characteristic velocity
The non-dimensional variables are defined by: $$ \begin{aligned} \tilde{x} &= \frac{1}{L}x \ \tilde{y} &= \frac{1}{L}y \ \tilde{\delta} &= \frac{1}{L}\delta \ \tilde{k} &= kL \ \tilde{\omega} &= \frac{L}{U}\omega \end{aligned} $$
Thus, the non-dimensional form of the initial condition is:
The first approach consists in introducing a random perturbation into the system. The equation for the initial vorticity becomes:
Simulation parameters:
- Perturbation intensity:
$\epsilon = 0.01$ - Shear layer thickness:
$\tilde{\delta} = 0.025$ - Reynolds number:
$Re = 2000$ - Simulation duration: 30 seconds
vorticity_mag.mp4
vorticity_z.mp4
Other physical quantities
streamfunction.mp4
velocity_mag.mp4
velocity_x.mp4
velocity_y.mp4
The second approach uses a controlled sinusoidal perturbation. This method allows a more systematic study of the instability.
Simulation parameters:
- Amplitude:
$A = 0.1$ - Wavenumber:
$\tilde{k} = 4$ - Other parameters identical to the previous simulation
