Viscous flow down an incline

Goals

  • Present the equations of linear viscous flow down an inclined plane

Linear viscous flow

Viscous flow down an incline

Figure 1. Viscous flow down an incline

Shear stress in the fluid

For a fluid flowing down an inclined slope, the change in potential energy per unit area of the contact surface along some length of the slope \(\delta x\) is

\[\begin{split}\begin{align} \Delta E_{\mathrm{P}} &= \rho g h \delta z\\ &= \rho g h (\bar{u} S) \end{align}\end{split}\]

where \(\Delta E_{\mathrm{P}}\) is the change in potential energy, \(\rho\) is the fluid density, \(g\) is the acceleration due to gravity, \(h\) is the thickness of the flow, \(\delta z\) is the elevation change over the distance \(x\), \(\bar{u}\) is the average flow velocity, and \(S\) is the slope of the incline.

Viscous flow down an incline

Figure 2. Viscous flow down an incline

The downslope component of the gravity force on the flow is thus \(\rho g h S\), which must be opposed by the drag force at the base of the flow \(\tau_{0}\). Thus, we can say

\[\tau_{0} = \rho g h S\]

We can also calculate the shear stress for any position \(z\) above the base of the flow, which is a function of the thickness of the overlying fluid \((h - z)\)

\[\begin{split}\begin{align} \tau_{z} &= \rho g S (h - z) && \text{Since we know that }\tau_{0} = \rho g h S\\ \tau_{z} &= \tau_{0} \left( 1 - \frac{z}{h} \right) \end{align}\end{split}\]

Attention

What does this suggest about the shear strength as a function of depth in the fluid?

Linking to viscous flow

For a laminar flow, we know \(\tau = \eta du/dz\), so we can rewrite the resistance equation as

\[\begin{split}\begin{align} \tau_{z} &= \eta \frac{du}{dz}\\ \tau_{z} &= \rho g S (h - z)\\ \eta \frac{du}{dz} &= \rho g S (h - z)\\ \frac{du}{dz} &= \frac{\rho g S (h - z)}{\eta}\\ \frac{du}{dz} &= \frac{\rho g S}{\eta} (h - z) \end{align}\end{split}\]

If we integrate this equation with respect to \(z\), we find

\[\begin{split}\begin{align} \int \frac{du}{dz} &= \frac{\rho g S}{\eta} \int (h - z)\\ u &= \frac{\rho g S}{\eta} \left(zh - \frac{z^{2}}{2} \right) + c_{1} \end{align}\end{split}\]

If we assume the flow velocity \(u = 0\) at \(z = 0\) (the base of the flow), the constant \(c_{1} = 0\), so we are left with

\[u = \frac{\rho g S}{\eta} \left(zh - \frac{z^{2}}{2} \right)\]

Attention

  • What would the velocity profile look like in this flow?
  • Where is the maximum velocity?
  • What happens if the viscosity decreases? Slope increases? Thickness increases?

Viscous flow take-home messages

  • The flow is a balance between the gravitational force on the fluid and resistance (drag) at the base
  • The flow velocity increases following a parabolic geometry from \(u = 0\) at the base to \(\frac{\rho g S}{\eta} \frac{z^{2}}{2}\)

Caveats

  • Steady-state
  • 1-D
  • Laminar flow!
  • Constants are constant
  • No temperature dependence