Falkner–Skan boundary layer


In fluid dynamics, the Falkner–Skan boundary layer describes the steady two-dimensional laminar boundary layer that forms on a wedge, i.e. flows in which the plate is not parallel to the flow. It is a generalization of the Blasius boundary layer.

Prandtl's boundary layer equations

's equations known as the boundary layer equations for steady incompressible flow with constant viscosity and density, are
Here the coordinate system is chosen with pointing parallel to the plate in the direction of the flow and the coordinate pointing towards the free stream, and are the and velocity components, is the pressure, is the density and is the kinematic viscosity.
The -momentum equation implies that the pressure in the boundary layer must be equal to that of the free stream for any given coordinate. Because the velocity profile is uniform in the free stream, there is no vorticity involved, therefore a simple Bernoulli's equation can be applied in this high Reynolds number limit
constant
or, after differentiation:
Here is the velocity of the fluid outside the boundary layer and is a solution of Euler equations.
A number of similarity solutions to this equation have been found for various types of flow, including flat plate boundary layers. The term similarity refers to the property that the velocity profiles at different positions in the flow are the same apart from a scaling factor. These solutions are often presented in the form of non-linear ordinary differential equations.

Falkner–Skan equation - First order boundary layerRosenhead, Louis, ed. Laminar boundary layers. Clarendon Press, 1963.

We can generalize the Blasius boundary layer by considering a wedge at an angle of attack from some uniform velocity field. We then estimate the outer flow to be of the form:
Where is a characteristic length and m is a dimensionless constant. In the Blasius solution, m = 0 corresponding to an angle of attack of zero radians. Thus we can write:
As in the Blasius solution, we use a similarity variable to solve the boundary layer equations.
It becomes easier to describe this in terms of its stream function which we write as
Thus the initial differential equation which was written as follows:
Can now be expressed in terms of the non-linear ODE known as the Falkner–Skan equation.
with boundary conditions
When, the problem reduces to the Hiemenz flow. Here, m < 0 corresponds to an adverse pressure gradient while m > 0 represents a favorable pressure gradient.. In 1937 Douglas Hartree showed that physical solutions to the Falkner–Skan equation exist only in the range. For more negative values of m, that is, for stronger adverse pressure gradients, all solutions satisfying the boundary conditions at η = 0 have the property that f > 1 for a range of values of η. This is physically unacceptable because it implies that the velocity in the boundary layer is greater than in the main flow.
Further details may be found in Wilcox.
The displacement thickness for the Falkner-Skan profile is given by
and the shear stress acting at the wedge is given by

Compressible Falkner–Skan boundary layerLagerstrom, Paco Axel. Laminar flow theory. Princeton University Press, 1996.

Here Falkner–Skan boundary layer with a specified specific enthalpy at the wall is studied. The density, viscosity and thermal conductivity are no longer constant here. In the low Mach number approximation, the equation for conservation of mass, momentum and energy become
where is the Prandtl number with suffix representing properties evaluated at infinity. The boundary conditions become
Unlike the incompressible boundary layer, similarity solution can exists for only if the transformation
holds and this is possible only if.

Howarth transformation

Introducing the self-similar variables using Howarth–Dorodnitsyn transformation
the equations reduce to
The equation can be solved once are specified. The boundary conditions are
The commonly used expressions for air are. If is constant, then.