This chapter is a review of the receptivity and resulting global instability of boundary layers due to free-stream vortical and acoustic disturbances at subsonic and moderately supersonic Mach numbers. The vortical disturbances produce an unsteady boundary layer flow that develops into oblique instability waves with a viscous triple-deck structure in the downstream region. The acoustic disturbances (which have phase speeds that are small compared to the free stream velocity) produce boundary layer fluctuations that evolve into oblique normal modes downstream of the viscous triple-deck region. Asymptotic methods are used to show that both the vortically and acoustically-generated disturbances ultimately develop into modified Rayleigh modes that can exhibit spatial growth or decay depending on the nature of the receptivity process.
- boundary layer
- boundary layer receptivity
- compressible boundary layers
- global instability
This chapter is concerned with the effect of unsteady free-stream disturbances on laminar to turbulent transition in boundary layer flows. The exact mechanism depends on the nature and intensity of the disturbances. Transition at high disturbance levels (say >1%) usually begins with the excitation of low frequency streaks in the boundary layer flow that eventually break down into turbulent spots. This phenomena was initially studied by Dryden  and much later for compressible flows by Marensi et al. . But the focus of this chapter is on low free steam disturbances levels (say less than 1%) where the transition usually results from a series of events beginning with the generation of spatially growing instability waves by acoustic and/or vortical disturbances in the free-stream. This so-called receptivity phenomenon results in a boundary value problem and therefore differs from classical instability theory which results in an eigenvalue problem for the Rayleigh or Orr-Sommerfeld equations that only apply when the mean flow can be treated as being nearly parallel (see, for example, Reshotko, ). The relevant boundary conditions cannot be imposed on the Orr-Sommerfeld or Rayleigh equations in the infinite Reynolds number limit being considered here but the free-stream disturbances can produce unsteady boundary layer perturbations in regions of rapidly changing mean flow that eventually produce unstable Rayleigh or Orr-Sommerfeld equation eigensolutions further downstream. These regions of nonparallel flow can result from surface roughness elements [4, 5], blowing or suction effects  or from the nonparallel mean flow that occurs near the boundary layer leading edge [7, 8].
The mechanism is similar in all cases but the simplest and arguably the most fundamental of these is the one resulting from the nonparallel leading edge flow and the focus here is, therefore, on that case. The initial studies were carried out for two dimensional incompressible flows. Ref.  used a low frequency parameter matched asymptotic expansion to show that there is an overlap domain where appropriate asymptotic solutions to the forced boundary layer equations (which apply near the edge) match onto the so-called Tollmien-Schlichting waves that satisfy the Orr-Sommerfeld equation in a region that lies somewhat further downstream. The coupling to the free-stream disturbances turns out to be fairly weak for the two dimensional incompressible flow considered in  due to the relatively large decay of boundary layer disturbances upstream of the Tollmien-Schlichting wave region where the Orr-Sommerfeld equation applies.
But there can be a much stronger coupling in supersonic flows which can support a number of different instabilities . The coupling mechanism can be either viscous or inviscid and the instability can either be of the viscous Tollmien-Schlichting type or can be purely inviscid when the mean boundary layer flow has a generalized inflection point. The inviscid coupling, which was first analyzed in , tends to be dominant when the obliqueness angle of the disturbance differs from the critical angle, , where the is the free-stream Mach number, by an amount. Figure 1 shows that the theoretical results of Ref.  are in good agreement with experimental data when but the agreement breaks down when  and a new rescaled analysis was carried out in Ref.  to deal with this case.
Fedorov and Khokhlov  analyzed the generation of inviscid instabilities in a supersonic flat plate boundary layer by fast and slow acoustic disturbances in the free stream. They showed that the slow acoustic mode propagates downstream/upstream when the obliqueness angle of the acoustic disturbances is smaller/larger than the critical angle and that downstream propagating slow acoustic modes with generate unsteady boundary layer disturbances that match onto the inviscid 1st Mack mode instability without undergoing any significant decay. The focus of that reference was on hypersonic flows while the interest here is in the moderately supersonic regime (Mach number less than 4), where the so called 1st Mack mode is the dominant instability, but (as shown in Section 6) emerges much too far downstream to be of practical interest when generated by the inviscid mechanism analyzed in . The instability produced by the small analysis of Ref.  can, however, occur much further upstream when is sufficiently small. But there is a smallest value of for which the instability wave coupling can occur.
Smith  showed that viscous instabilities, which exhibit the same triple-deck structure as the subsonic Tollmien-Schlichting waves, can also occur at supersonic speeds when the obliqueness angles is greater than the critical angle . Their phase speeds are very small and they must therefore be produced by a viscous wall layer mechanism similar to the one identified in .
The analysis of Ref.  was extended to compressible subsonic and supersonic flat plate boundary layer flows by Ricco and Wu  who showed that highly oblique vortical disturbances can generate a limiting form of the Smith instability . They found that the instability wave lower branch lies further upstream at supersonic speeds than the subsonic lower branch and much further upstream than the incompressible lower branch considered in , which means that the instability wave/free-stream disturbance coupling is much greater at supersonic speeds than it is in the incompressible flow considered in . Goldstein and Ricco  show that the instability does not possess an upper branch in this case and matches onto a low frequency (short streamwise wavenumber) Rayleigh instability (that can be identified with the 1st Mack mode) when the downstream distance is slightly smaller than the downstream distance where acoustically generated instability corresponding to the smallest possible emerges. It therefore makes sense to consider both of these receptivity mechanisms simultaneously.
As noted above, the present chapter is concerned with the unsteady flow in a flat plate boundary layer generated by mildly oblique vortical disturbance and small acoustic disturbances in a moderately supersonic Mach number free stream. The results are expected to be relevant to transition in the straight wing boundary layers on supersonic aircraft such as the low-sweep Aerion AS2 Bizjet, shown in Figure 2.
2. Imposed free-stream disturbances
Since the boundary layer is believed to be convectively unstable, the receptivity phenomena are best illustrated by considering a small amplitude harmonic distortion with angular frequency superimposed on a subsonic or moderately low Mach number supersonic flow of an ideal gas past an infinitely thin flat plate with uniform free-stream velocity , temperature , dynamic viscosity and density . The velocities, pressure fluctuations, temperature and dynamic viscosity are normalized by , , and , respectively. The time is normalized by and the Cartesian coordinates, say , are normalized by with the coordinate being normal to the plate.
As noted above the phenomenon is analyzed by requiring the Reynolds number to be large, or equivalently requiring the frequency parameter to be small, and using asymptotic theory to explain how the imposed harmonic distortion generates oblique instabilities at large downstream distances in the viscous boundary layer that forms on the surface of the plate. The natural expansion parameter turns out to be
The free-steam disturbances will be inviscid at the lowest order of approximation and, as is well known , can be decomposed into an acoustic component that carries no vorticity, and vortical and entropic components that produce no pressure fluctuations. But only the first two will be considered here.
The vortical disturbance is given
where is a common scale factor and satisfy the continuity condition
but are otherwise arbitrary constants while the acoustic component is governed by the linear wave equation which has a fundamental plane wave solution
for the velocity and pressure perturbation where
and, as noted in Section 1, denotes the free-stream Mach number.
The leading edge interaction will produce large scattered fields for values of the incidence angles and of the acoustic and vortical disturbances, respectively. And, in order to focus on the fundamental mechanisms, we assume that the incidence angles of the vortical disturbances are small and that the incidence angles of the acoustic disturbances are zero, which requires that
for the former disturbances and that
for the latter, where the subscripts −/+ refer to the slow/fast acoustic modes. Eq. (7) shows that the slow mode wavenumber becomes infinite when the obliqueness angle is equal to the critical angle referred to in the introduction.
3. Boundary layer disturbances
As indicated above our interest here is in explaining how the incident harmonic distortions generate oblique instabilities at large downstream distances in the viscous boundary layer that forms on the surface of the plate. We begin by considering the fluctuations imposed on this flow by the free-stream vortical disturbance (2).
3.1 Boundary layer disturbances generated by the free-stream vorticity
As noted in the introduction, these disturbances will generate oblique Tollmien-Schlichting instability waves which are known to exhibit a triple-deck structure in the vicinity of their lower branch which lies at an distance downstream  of the leading edge in the high Reynolds number flow being considered here. The Tollmien-Schlichting waves will have spanwise wavenumbers and we therefore require that
since the spanwise wavenumber must remain constant as the disturbances propagate downstream.
The vortical velocity (2) will then interact with the plate to produce an inviscid velocity field  that generates a slip velocity at the surface of the plate which must be brought to zero in a thin viscous boundary layer whose temperature, density and streamwise velocity, say , respectively, are assumed to be functions of the Dorodnitsyn-Howarth variable
We begin by considering the flow in the vicinity of the leading edge where the streamwise length scale is . Since the inviscid velocity field can only depend on the streamwise coordinate through this relatively long streamwise length scale the solution for the velocity and temperature perturbation in this region is given by , 
where satisfies the three dimensional compressible linearized boundary layer equations (with unit spanwise wavenumber) subject to the boundary conditions 
while is a quasi-two dimensional solution that satisfies the two dimensional linearized boundary layer equations subject to the boundary conditions
The lowest order triple-deck solution will match onto the quasi-two dimensional solution of the two dimensional boundary layer equations, where the spanwise dependence only enters parametrically through the exponential factor in(11) .
is an exact eigensolution of the two-dimensional linearized unsteady boundary layer equations that satisfies the homogeneous boundary conditions for all , but does not necessarily satisfy the no-slip condition at the wall.
Lam and Rott ,  analyzed the two dimensional flat plate boundary layer and showed that the linearized equations possess asymptotic eigensolutions that satisfy a no-slip condition at the wall when becomes large. These solutions exhibit a two-layer structure consisting of an outer region that encompasses the main part of the boundary layer and a thin viscous region near the wall. The outer solution is given by (14) and (15) with the arbitrary function determined by matching with the viscous wall layer flow.
Ref.  showed that the Lam and Rott [20, 21] analysis also applies to compressible flows when the full compressible solution (14) and (15) is used in the outer region and the viscous wall layer solution is slightly modified to account for the temperature and viscosity variations. The function is then given by
where , , and is a root of
The only difference from the Lam-Rott result is the factor in the exponent. The asymptotic solution to the full inhomogeneous boundary value problem can now be expressed as the sum of a Stokes layer solution plus a number of these asymptotic eigensolutions. The first few were determined from numerical solutions to the boundary layer problem in Ref. . But we are primarily concerned with the lowest order mode because that is the only one that matches onto a spatially growing oblique Tollmien-Schlicting wave further downstream . The receptivity problem can then be solved by combining the numerical computations with appropriate matched asymptotic expansions to relate the instability wave amplitude to that of the free-stream disturbance. But we will analyze the boundary layer disturbances generated by the free-stream acoustic disturbances before considering these expansions.
3.2 Boundary layer disturbances generated by the Fedorov/Khokhlov mechanism for obliqueness angles close to critical angle
Fedorov and Khokhlov  used matched asymptotic expansions to analyze the generation of Mack mode instabilities by oblique acoustic waves of the form (4) where the wavenumbers and satisfy the dispersion relation (7) when the incidence angle is equal to zero, which, as noted, above is the case being considered here. Their focus was on hypersonic flows where the most rapidly growing disturbances are usually two dimensional 2nd Mack modes, while, as noted in the introduction, the focus of the present chapter is on the relatively low supersonic Mach number regime (say, less than about 4) where the most rapidly growing instability waves are highly oblique 1st Mack modes. Numerical results  show that the obliqueness angle of the most rapidly growing 1st mode lies between 50 and 70 degrees at Mach numbers between 2 and 6.
Ref.  shows that the boundary layer disturbance produced by diffraction of the slow acoustic wave by the nonparallel mean flow in the region where can be matched onto a 1st Mack mode instability in the downstream region where when the deviation
of the obliqueness angle from the critical angle
takes on positive values. The diffraction region has a double layer structure which consists of a region that fills the mean boundary layer and an outer diffraction region of thickness . (The purely passive Stokes layer near the wall does not play a role in the diffraction process and can be ignored).
The instability emerges from the downstream limit of the solution in this region. But as noted in the introduction this occurs too far downstream to be of practical interest when scaled up to actual flight conditions if  at the moderately supersonic Mach numbers being considered here. It will however emerge much further upstream when is close to the critical angle , i.e., when . But the solution in Ref.  does not apply when and a new analysis was developed in Ref.  to extend their result into the small -regime.
It follows from (7) that
when since in that case.
This shows that also becomes large when and that will expand in powers of as indicated in (21) if is fixed at the indicated value to all orders in (which we now assume to be the case).
The spanwise wavenumber will equal the vortical spanwise wavenumber (8) when and as in that case the diffraction wave solution will eventually develop a triple-deck structure but the resulting solution will (as shown in ) not decay at large wall normal distances and is therefore invalid. This means that the diffraction region solution cannot be continued downstream for .
Ref.  shows that the smallest value of is and the diffraction region will then occur at an distance downstream. The relevant solution will have the triple-deck structure shown in Figure 3: a main boundary layer region that fills the mean boundary layer (region 1), an outer diffraction region of thickness (region 2) and an thick viscous wall layer in which the unsteady, convective and viscous terms all balance.
The pressure in region 2 is of the form
and the surface pressure is related to the up-wash velocity at the outer edge of the boundary layer by
where denotes the pressure in the boundary layer region 1 (which is independent of the wall normal direction) and the wall normal velocity is given in terms of
and the integral and the derivative of the Airy function by
which behaves like
as since (, pp. 446–447)
which is formally the same as the equation considered in  who showed that the solution behaves like
The acoustically and vortically generated boundary layer disturbances considered in this section will eventually evolve into propagating eigensolutions in regions that lie further downstream. The resulting flow will have a triple-deck structure of the type considered in ,  and  in the former (i.e., vortically generated) case. But the acoustically generated disturbance will only develop an eigensolution structure much further downstream. The minimum distance occurs when . We begin by considering the triple-deck region.
4. The viscous triple-deck region
in the triple-deck region where is the common scale factor introduced at the beginning of Section 2,
in the main boundary layer where ,
is a scaled transverse coordinate. The complex wavenumber has the expansion .
whose solution must satisfy the inequality
in order to insure that the eigensolution does not exhibit unphysical wall normal growth.
This requirement will be satisfied for all but will only be satisfied at supersonic Mach numbers when the obliqueness angle is greater than the critical angle [11, 13]. The dispersion relation (38) and (39) reduces to the dispersion relation given by Eqs. (4.52), (5.2) and (5.3) of  when and are set to zero.
4.1 Matching with the Lam-Rott solution
4.2 Numerical results
The dispersion relation (38) is expected to have at least one root corresponding to each of the infinitely many roots of (18). But only the lowest order root can produce the spatially growing modes of (38). The wall temperature and viscosity can be scaled out of this equation by introducing the rescaled variables.
The real and negative imaginary parts of calculated from (38) together with the Lam-Rott initial condition (41) are plotted as a function of the scaled streamwise coordinate in Figures 4 and 5 for three values of the frequency scaled transverse wavenumber . The insets are included to more clearly show the changes at small . The dashed curves in the insets denote the real and imaginary parts of the small-asymptotic formula (41).
The triple-deck eigensolution (33) (which contains the Lam-Rott solution as an upstream limit) can undergo a significant amount of damping before it turns into a spatially growing instability wave at the lower branch of the neutral stability curve.
The exponential damping in Eq. (33) is proportional to , where and denote the scaled and unscaled streamwise location of the lower branch of the neutral stability, which implies that the total damping is proportional to the area under the growth rate curve between zero and the lower branch in Figure 5. The inset shows that the length of this upstream region is very short and therefore that the total amount of damping is relatively small.
5. The inviscid triple-deck region
As noted above the acoustically driven solution will only match onto an eigensolution in the downstream region when . This region will lie downstream of the viscous triple-deck region considered above and will be closest to that region when . It will have an inviscid triple- deck structure and the relevant dispersion relation can be obtained by putting in (21), inserting the rescaled variables
when the square root is required to remain finite as .
5.1 Matching with the small Fedorov/Khokhlov solution
It can then be shown by direct substitution that the solution behaves like
The pressure component of the resulting solution will then match onto the downstream limit (32) and (30) of the acoustically generated diffraction region solution when and is given by (24) since it follows from (8),(35),(43) and (45) that
5.2 Numerical results
Figure 6 is a plot of the scaled lowest order wavenumber as a function of the scaled streamwise coordinate for various values of the free-stream Mach number calculated from the inviscid triple-deck dispersion relation(44) together with the asymptotic initial condition (45) which is shown by the dashed curves in the figure. The lowest order wave number is purely real which means that exponential growth (if it occurs) can only occur at higher order. This suggests that the acoustically generated instabilities will be less significant than the vortically-generated instabilities which appear upstream.
6. The next stage of evolution
6.1 Downstream behavior of the triple-deck solution
when and, therefore, that
when is allowed to approach zero as .
The dashed curves in the main plot of Figure 4 represent the re-scaled large-asymptote (48). It confirms that the numerical results are well approximated by the (appropriately rescaled) large-asymptote (48).
of (48), which can be considered to be a special case of this result if we put
and is defined in (43).
6.2 Derivation of the governing equations
Eq. (49) shows, among other things, that the lowest order wave number and streamwise growth rate approach zero but do not become negative as the disturbance propagates downstream. The boundary layer thickness which is continues to increase and the triple-deck scaling breaks down at the streamwise location
where it becomes of the order of the spanwise length scale, which remains constant at . This region is located well upstream of the region where the unsteady flow is governed by the full Rayleigh equation considered in .
as where is an function of (given by (53)) and
which means that the solution should be proportional to , where is an function of that behaves like
in this stage of evolution. The solution should remain inviscid in the main boundary layer and the viscous wall layer (i.e., a Stokes layer) is expected to be completely passive.
The scaled variable
will be in the main boundary layer since its thickness is now of the order of the spanwise length scale, . It therefore follows from (53) and (57) that the transverse pressure gradients will come into play and the solution in this region should expand like
where is a function of the slow variable . Substituting (58) into the linearized Navier-Stokes equations shows that the wall normal velocity perturbation is determined by the incompressible reduced Rayleigh equation
whose solution must satisfy the following boundary conditions
which means that
6.3 Matching with the triple-deck solution
Eq. (64) clearly approaches zero when which means that will be consistent with the matching condition (54) if we require that it behave like
where are (in general complex) constants such that
Ref.  proved that (60)–(64) possess an asymptotic solution of the form as when satisfies (65) which implies that their solutions are able to match onto the lowest order triple-deck solution upstream and are consistent with the higher order solutions in this region.
6.4 Numerical results
The Rayleigh eigenvalues are determined by the boundary value problem (60), (61) and (62). We assume in the following that the Prandtl number is equal to unity and that the viscosity satisfies the simple linear relation .
Parts (a) and (b) of Figure 7 are plots of the real and imaginary parts respectively of these eigenvalues as a function of . They show that the numerical solution for will be consistent with the matching conditions (65)and(66) if the higher order terms in the triple-deck expansion(51) satisfy and =, where the values of
This chapter uses high Reynolds number asymptotics to study the nonlocal behavior of boundary layer instabilities generated by small amplitude free-stream disturbances at subsonic and moderate supersonic Mach numbers. The appropriate small expansion parameter turns out to be where denotes the frequency parameter. The oblique 1st Mack mode instabilities generated by free-stream acoustic disturbances are compared with those generated by elongated vortical disturbances. The focus is on explaining the relevant physics and not on obtaining accurate numerical predictions.
The free-stream vortical disturbances generate unsteady flows in the leading edge region that produce short spanwise wavelength instabilities in a viscous triple-deck region which lies at an distance downstream from the leading edge. The mechanism was first considered for two dimensional incompressible flows in Ref. , but the instability onset occurs much further upstream in the supersonic case and is, therefore, much more likely to be important at the higher Mach numbers considered in this chapter. The lowest order triple-deck solution does not possess an upper branch and evolves into an inviscid 1st Mack mode instability with short spanwise wavelength at an distance downstream.
Fedorov and Khokhlov  used asymptotic methods to study the generation of inviscid instabilities in supersonic boundary layers by fast and slow acoustic disturbances in the free stream whose obliqueness angle deviated from its critical value by an amount and showed that slow acoustic disturbances generate unsteady boundary layer disturbances that produce spanwise wavelength inviscid 1st Mack mode instabilities a much larger distance downstream. But the calculations in Ref.  show that the physical streamwise distance corresponding to this scaled downstream location is at least equal to about 7 m for the typical supersonic flight conditions at end an altitude of 20 km with an upper bound of 100 kHz for the characteristic frequency. This means that this instability occurs too far downstream to be of any practical interest at the moderately low supersonic Mach numbers considered in this chapter.
But, the inviscid instability, which first appears at an distance downstream when is reduced to can be significant when scaled to flight conditions. It is therefore appropriate to compare the vortically-generated instabilities with the instabilities generated by oblique acoustic disturbances with obliqueness angles in this range as done in this chapter.
This research was sponsored by NASA’s by the Transformative Aeronautics Concepts Program of the Aeronautics Research Mission Directorate under the Transformational Tools and Technologies (TTT) Project. PR was supported by the Air Force Office of Scientific Research award number AFOSR Grant FA9550-15-1-0248. We would also like to thank Dr. Meelan Choudhari for bringing the photograph in Figure 2 to our attention.