Viscous boundary layer

A viscous boundary layer is a boundary layer next to a surface in which viscosity remains important even when the outer flow has a large Reynolds number. It reconciles the outer inviscid velocity with the no-slip boundary condition.

The Prandtl limit observes a high-Reynolds number flow within a shrinking wall-normal layer. For streamwise distance $x$ and outer speed $U$, rescale the normal distance by $\delta =\sqrt{\nu x/U}$ and the normal velocity by $U\delta /x$. Convection and normal viscous diffusion then remain comparable, while streamwise viscous diffusion is smaller. The leading normal momentum equation makes pressure independent of the rescaled normal coordinate, and the tangential equation is the Prandtl boundary-layer equation. This laminar asymptotic balance is local and need not remain valid through separation or instability.

For a steady two-dimensional incompressible boundary layer with tangential velocity $u(x,y)$, normal velocity $v(x,y)$, outer tangential velocity $U(x)$, and kinematic viscosity $\nu$,The pressure is uniform across the layer, and the outer Euler equation supplies $-p_x/\rho =UdU/dx$.

For a steady incompressible viscous boundary layer over a flat plate with constant outer speed $U$, the stream function $\psi =\sqrt{\nu Ux}f(y\sqrt{U/(\nu x)})$ reduces the Prandtl boundary-layer equation to the displayed ordinary differential equation. The wall and outer conditions are $f(0)=f^{\prime }(0)=0$ and $f^{\prime }(\infty )=1$. The wall shear is $\rho U\sqrt{\nu U/x}{f}^{\prime \prime }(0)$, so its integral on one plate face of length $L$ is $2\rho U^{2}L{f}^{\prime \prime }(0)/\sqrt{UL/\nu }$. Both equally exposed faces contribute twice this value.

The unsteady form of the Prandtl boundary-layer equation evolves the tangential boundary-layer velocity under advection, outer pressure forcing and normal viscous diffusion. Incompressibility supplies the normal velocity. A stationary wall imposes the no-slip boundary condition, and tangential velocity matches the prescribed outer slip velocity far from the wall. The normal far-field disturbance need not vanish.

For a fixed outer pressure and slip velocity, retain terms linear in a disturbance of a base flow $(U,V)$. The tangential equation has the displayed form and continuity is ${\tilde{u}}_x+{\tilde{v}}_y=0$. Disturbances vanish at the wall and the tangential disturbance vanishes in the far field. A local parallel-profile approximation may freeze the coefficients even when the profile is not an exact global steady solution.

For a frozen real parallel profile and modes proportional to $e^{i\alpha (x-ct)}$, continuity eliminates tangential velocity and gives this third-order equation. Wall conditions are $v=v^{\prime }=0$; outer tangential matching gives $v^{\prime }\to 0$, with bounded $v$. Real coefficients give the spectral symmetry $(\alpha ,c)\mapsto (-\alpha ,c^{\ast })$. For positive real wavenumber, growth means $\mathrm{Im}c>0$.

For streamwise length $L$, outer speed $U$, and layer thickness $\delta$, balancing $u{u}_x\sim U^2/L$ with $\nu u_{yy}\sim \nu U/{\delta }^2$ gives