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Next: Self-Similar Boundary Layers Up: Incompressible Boundary Layers Previous: No Slip Condition


Boundary Layer Equations

Consider a rigid stationary obstacle whose surface is (locally) flat, and corresponds to the $ x$ -$ z$ plane. Let this surface be in contact with a high Reynolds number fluid that occupies the region $ y>0$ . (See Figure 8.1.) Let $ \delta$ be the typical normal thickness of the boundary layer. The layer thus extends over the region $ 0< y\stackrel {_{\normalsize <}}{_{\normalsize\sim}}\delta$ . The fluid that occupies the region $ \delta\stackrel {_{\normalsize <}}{_{\normalsize\sim}}y<\infty$ , and thus lies outside the layer, is assumed to be both irrotational and (effectively) inviscid. On the other hand, viscosity must be included in the equation of motion of the fluid within the layer. The fluid both inside and outside the layer is assumed to be incompressible.

Figure 8.1: A boundary layer.
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Suppose that the equations of irrotational flow have already been solved to determine the fluid velocity outside the boundary layer. This velocity must be such that its normal component is zero at the outer edge of the layer (i.e., at $ y\simeq \delta$ ). On the other hand, the tangential component of the fluid velocity at the outer edge of the layer, $ U(x)$ (say), is generally non-zero. Here, we are assuming, for the sake of simplicity, that there is no spatial variation in the $ z$ -direction, so that both the irrotational flow and the boundary layer are effectively two-dimensional. Likewise, we are also assuming that all flows are steady, so that any time variation can be neglected. The motion of the fluid within the boundary layer is governed by the equations of steady-state, incompressible, two-dimensional, viscous flow, which take the form (see Section 1.14)

$\displaystyle \frac{\partial v_x}{\partial x} +\frac{\partial v_y}{\partial y}$ $\displaystyle = 0,$ (8.1)
$\displaystyle v_x\,\frac{\partial v_x}{\partial x} + v_y\,\frac{\partial v_x}{\partial y}$ $\displaystyle =-\frac{1}{\rho}\,\frac{\partial p}{\partial x} + \nu\left(\frac{...
...\,2} v_x}{\partial x^{\,2}}+\frac{\partial^{\,2} v_x}{\partial y^{\,2}}\right),$ (8.2)
$\displaystyle v_x\,\frac{\partial v_y}{\partial x} + v_y\,\frac{\partial v_y}{\partial y}$ $\displaystyle =-\frac{1}{\rho}\,\frac{\partial p}{\partial y} + \nu\left(\frac{...
...\,2} v_y}{\partial x^{\,2}}+\frac{\partial^{\,2} v_y}{\partial y^{\,2}}\right),$ (8.3)

where $ \rho$ is the (constant) density, and $ \nu$ the kinematic viscosity. Here, Equation (8.1) is the equation of continuity, whereas Equations (8.2) and (8.3) are the $ x$ - and $ y$ -components of the fluid equation of motion, respectively. The boundary conditions at the outer edge of the layer, where it interfaces with the irrotational fluid, are

$\displaystyle v_x(x,y)$ $\displaystyle \rightarrow U(x),$ (8.4)
$\displaystyle p(x,y)$ $\displaystyle \rightarrow P(x)$ (8.5)

as $ y/\delta\rightarrow \infty$ . Here, $ P(x)$ is the fluid pressure at the outer edge of the layer, and

$\displaystyle U\,\frac{dU}{dx} = - \frac{1}{\rho}\,\frac{dP}{dx}$ (8.6)

(because $ v_y=0$ , and viscosity is negligible, just outside the layer). The boundary conditions at the inner edge of the layer, where it interfaces with the impenetrable surface, are

$\displaystyle v_x(x,0)$ $\displaystyle = 0,$ (8.7)
$\displaystyle v_y(x,0)$ $\displaystyle =0.$ (8.8)

Of course, the first of these constraints corresponds to the no slip condition.

Let $ U_0$ be a typical value of the external tangential velocity, $ U(x)$ , and let $ L$ be the typical variation length-scale of this quantity. It is reasonable to suppose that $ U_0$ and $ L$ are also the characteristic tangential flow velocity and variation length-scale in the $ x$ -direction, respectively, of the boundary layer. Of course, $ \delta$ is the typical variation length-scale of the layer in the $ y$ -direction. Moreover, $ \delta/L\ll 1$ , because the layer is assumed to be thin. It is helpful to define the normalized variables

$\displaystyle X$ $\displaystyle = \frac{x}{L},$ (8.9)
$\displaystyle Y$ $\displaystyle = \frac{y}{\delta},$ (8.10)
$\displaystyle V_x(X,Y)$ $\displaystyle = \frac{v_x}{U_0},$ (8.11)
$\displaystyle V_y(X,Y)$ $\displaystyle = \frac{v_y}{U_1},$ (8.12)
$\displaystyle \widehat{P}(X,Y)$ $\displaystyle = \frac{p}{p_0},$ (8.13)

where $ U_1$ and $ p_0$ are constants. All of these variables are designed to be $ {\cal O}(1)$ inside the layer. Equation (8.1) yields

$\displaystyle \frac{U_0}{L}\,\frac{\partial V_x}{\partial X} + \frac{U_1}{\delta}\,\frac{\partial V_y}{\partial Y} = 0.$ (8.14)

In order for the terms in this equation to balance one another, we need

$\displaystyle U _1= \frac{\delta}{L}\,U_0.$ (8.15)

In other words, within the layer, continuity requires the typical flow velocity in the $ y$ -direction, $ U_1$ , to be much smaller than that in the $ x$ -direction, $ U_0$ .

Equation (8.2) gives

$\displaystyle \frac{U_0^{\,2}}{L}\left(V_x\,\frac{\partial V_x}{\partial X} + V...
...\,2} V_x}{\partial X^{\,2}}+\frac{\partial^{\,2} V_x}{\partial Y^{\,2}}\right].$ (8.16)

In order for the pressure term on the right-hand side of the previous equation to be of similar magnitude to the advective terms on the left-hand side, we require that

$\displaystyle p_0 = \rho\,U_0^{\,2}.$ (8.17)

Furthermore, in order for the viscous term on the right-hand side to balance the other terms, we need

$\displaystyle \frac{\delta}{L} =\frac{U_1}{U_0}= \frac{1}{{\rm Re}^{1/2}},$ (8.18)

where

$\displaystyle {\rm Re} = \frac{U_0\,L}{\nu}$ (8.19)

is the Reynolds number of the flow external to the layer. (See Section 1.16.) The assumption that $ \delta/L\ll 1$ can be seen to imply that $ {\rm Re}\gg 1$ . In other words, the normal thickness of the boundary layer separating an irrotational flow pattern from a rigid surface is only much less than the typical variation length-scale of the pattern when the Reynolds number of the flow is much greater than unity.

Equation (8.3) yields

$\displaystyle \frac{1}{{\rm Re}}\left(V_x\,\frac{\partial V_y}{\partial X} + V_...
...\,2} V_y}{\partial X^{\,2}}+\frac{\partial^{\,2} V_y}{\partial Y^{\,2}}\right].$ (8.20)

In the limit $ {\rm Re}\gg 1$ , this reduces to

$\displaystyle \frac{\partial \widehat{P}}{\partial Y} = 0.$ (8.21)

Hence, $ \widehat{P}=\widehat{P}(X)$ , where

$\displaystyle \frac{d\widehat{P}}{d X} = - \widehat{U}\,\frac{d\widehat{U}}{dX},$ (8.22)

$ \widehat{U}(X)=U/U_0$ , and use has been made of Equation (8.6). In other words, the pressure is uniform across the layer, in the direction normal to the surface of the obstacle, and is thus the same as that on the outer edge of the layer.

Retaining only $ {\cal O}(1)$ terms, our final set of normalized layer equations becomes

$\displaystyle \frac{\partial V_x}{\partial X} + \frac{\partial V_y}{\partial Y}$ $\displaystyle = 0,$ (8.23)
$\displaystyle V_x\,\frac{\partial V_x}{\partial X} + V_y\,\frac{\partial V_y}{\partial Y}$ $\displaystyle = \widehat{U}\,\frac{d\widehat{U}}{\partial X} + \frac{\partial^{\,2} V_y}{\partial Y^{\,2}},$ (8.24)

subject to the boundary conditions

$\displaystyle V_x(X,\infty)= \widehat{U}(X),$ (8.25)

and

$\displaystyle V_x(X,0)$ $\displaystyle = 0,$ (8.26)
$\displaystyle V_y(X,0)$ $\displaystyle =0.$ (8.27)

In unnormalized form, the previous set of layer equations are written

$\displaystyle \frac{\partial v_x}{\partial x} +\frac{\partial v_y}{\partial y}$ $\displaystyle = 0,$ (8.28)
$\displaystyle v_x\,\frac{\partial v_x}{\partial x} + v_y\,\frac{\partial v_x}{\partial y}$ $\displaystyle = U\,\frac{dU}{dx} + \nu\,\frac{\partial^{\,2} v_x}{\partial y^{\,2}},$ (8.29)

subject to the boundary conditions

$\displaystyle v_x(x,\infty)= U(x)$ (8.30)

(note that $ y=\infty$ really means $ y/\delta\rightarrow \infty$ ), and

$\displaystyle v_x(x,0)$ $\displaystyle = 0,$ (8.31)
$\displaystyle v_y(x,0)$ $\displaystyle =0.$ (8.32)

Equation (8.28) can be automatically satisfied by expressing the flow velocity in terms of a stream function: that is,

$\displaystyle v_x$ $\displaystyle =-\frac{\partial \psi}{\partial y},$ (8.33)
$\displaystyle v_y$ $\displaystyle =\frac{\partial\psi}{\partial x}.$ (8.34)

In this case, Equation (8.29) reduces to

$\displaystyle \nu\,\frac{\partial^{\,3}\psi}{\partial y^{\,3}}-\frac{\partial\p...
...rtial y}\,\frac{\partial^{\,2}\psi}{\partial x \,\partial y}= U\,\frac{dU}{dx},$ (8.35)

subject to the boundary conditions

$\displaystyle \frac{\partial\psi(x,\infty)}{\partial y}=-U(x),$ (8.36)

and

$\displaystyle \psi(x,0)$ $\displaystyle = 0,$ (8.37)
$\displaystyle \frac{\partial\psi(x,0)}{\partial y}$ $\displaystyle =0.$ (8.38)

To lowest order, the vorticity internal to the layer, $ \omega$ $ = \omega\,{\bf e}_z$ , is given by

$\displaystyle \omega = \frac{\partial^{\,2}\psi}{\partial y^{\,2}},$ (8.39)

whereas the $ x$ -component of the viscous force per unit area acting on the surface of the obstacle is written (see Section 1.18)

$\displaystyle \left.\sigma_{xy}\right\vert _{y=0} = \rho\,\nu\left.\frac{\parti...
... -\rho\,\nu\left.\frac{\partial^{\,2}\psi}{\partial y^{\,2}}\right\vert _{y=0}.$ (8.40)


next up previous
Next: Self-Similar Boundary Layers Up: Incompressible Boundary Layers Previous: No Slip Condition
Richard Fitzpatrick 2016-01-22