19
Nonlinear and Nonparallel Receptivity of
Zero-pressure Gradient Boundary Layer
Tapan K. Sengupta, Swagata Bhaumik, Vikram Singh, Sarvagy Shukl
Department of Aerospace Engineering, I.I.T. Kanpur, U.P. 208016, India;
e-mail: tksen@iitk.ac.in,
ABSTRACT
Nonlinear and nonparallel receptivity of zero pressure gradient boundary layer have been
investigated by solving the full two-dimensional Navier-Stokes equation with respect to wall
excitation at fixed frequency. The excitation is triggered through a blowing-suction strip at
a location near the leading edge of the plate. Results are reported for cases which are linearly
stable in a spatial formulation, for different amplitudes of the excitation of the strip.
Presented results for a lower amplitude of excitation for the chosen frequency of
excitation help explain the displayed nonlinearity of the streamwise component of the
disturbance velocity at intermediate heights inside the shear layer. The disturbance field
is noted to be neutrally stable at heights close to the plate and in the outer part of the
boundary layer. Overall, such behaviour of the disturbance field is explained in terms of
the presence of multiple modes and their spatiotemporal interactions and the importance
of nonlinearity at specific heights inside the shear layer. We report another case where
stationary bubbles are formed at the wall near the exciter, when the amplitude of
excitation is doubled over previous lower amplitude case. Presence of such bubbles alter
the disturbance growth significantly and is an early marker of bypass transition.
Key Words: Nonlinear Receptivity; Nonparallel effects; Navier-Stokes equation;
Orr-Sommerfeld Equation; Bypass Transition; Tollmien-Schlighting Waves
1. INTRODUCTION
Significant progress in the understanding of flow instability has been made over the last few decades
starting with the original works reported in Heisenberg [1], Tollmien [2] and Schlichting [3] that
theoretically established the process of flow transition from laminar to turbulent state to follow with the
creation and growth of waves (now known as Tollmien-Schlichting (TS) waves). The latter
nomenclature is a misnomer as under the guidance of Sommerfield, Heisenberg studied this flow for
his doctoral dissertation. His committee could find nothing wrong in the analysis, but found it difficult
to accept that viscous action can add to instability. Of course, it makes perfect sense when one realizes
that viscous action sets a phase delay that can lead to positive feedback and instability. Thus, the credit
for the original observation of the existence of viscous tuned instability waves should be conferred
equally to Heisenberg, Tollmien and Schlichting.
These theoretical results were obtained with restrictive assumptions on the growth of the equilibrium
flow whose stability was studied in a linear framework. These two restrictions cause error due to what
is known as non-inclusion of nonlinearity and non-parallelism. While these two neglected effects are
still the subject of many investigations- including the present one- the major issue of concern in
accepting the results of Tollmien [2] and Schlichting [3] were due to the challenge that these studies
posed to contemporary paradigmatic acceptance of the fact that viscous effects can only be stabilizing.
The latter point of view was based on the pioneering work done in this field earlier by Kelvin [4] and
Rayleigh [5,6] that was premised on the assumption that viscous action being dissipative in fluid flow,
its inclusion was not essential for the study of flow instability. Specifically, Rayleigh [5,6] propounded
a criterion that determined the inviscid instability of shear layers. In contrast to this, the work reported
in Tollmien [2] and Schlichting [3] stated that the complex interactions of viscous action along with
inertial terms of the governing equation can actually destabilize a flow that was otherwise pronounced
as stable. A typical example of such a flow is the zero pressure gradient boundary layer developing over
a flat plate. Apart from the problem of countering the prevalent idea of flow instability, the predicted
TS waves were not seen experimentally till the results of Schubauer & Skramstad [7] were published.
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Nonlinear and Nonparallel Receptivity of Zero-pressure Gradient Boundary Layer
Earlier experimental results were bedevilled due to the experimental device noise and in the design
of appropriate experiment that follows the conceptual construct of the theoretical formulation. This last
aspect relates to the eigenvalue problem in Tollmien [2] and Schlichting [3] that discussed genesis and
evolution of disturbance in the form of a wave, when the flow is excited by a time-harmonic localized
source. Also, in this eigenvalue formulation, there is an implicit view that the monochromatic
disturbance source is placed at the wall and the created disturbances decay with height. In a noisy
experimental device, there are distributed disturbance sources that are not monochromatic and the
desired decay of disturbance field with height is not possible. Even when these were accounted for by
placing a vibrating diaphragm at the wall as in Taylor [8], it was not successful because the frequency
of vibration was too low as compared to that predicted in the theory.
In the context of the discussion above, experimental results reported in Schubauer & Skramstad [7]
are extraordinary. They were the first to realise that the experimental facilities have to be made as quiet
as possible and then a deterministic wall excitation would provide response in the fluid dynamical
system as predicted by theoretical analysis. During the course of the research they found that the
vibrating ribbon excited near the wall was the most satisfactory means of exciting TS waves. The
results clearly demonstrated not only the existence of TS waves, but also helped chart out the neutral
curve that matched very well for higher Reynolds number (based on displacement thickness as the
length scale) with the analytical results. This was to be expected as with increasing Reynolds number
the boundary layer growth becomes progressively negligible making the parallel flow approximation
used in the theory more and more valid. This experiment also emphasized the link between stability
analysis and receptivity of shear layer to different types of disturbance sources.
There were some work reported in the literature (as in Ashpis & Reshotko [9] and other references
contained therein) that talked about the mathematical framework of receptivity analysis. It was only in
Sengupta [10] and in Gaster & Sengupta [11], first set of actual results for linear receptivity of zero
pressure gradient boundary layer to wall excitation were reported for the signal problem. A signal
problem corresponds to the assumption that the time behaviour of the response field is as described by
the time-harmonic excitation of the shear layer. Results were obtained based on parallel flow
approximation that identified the TS wave as the asymptotic part of the response field i.e. the computed
solution matched with TS wave away from the exciter. Apart from this asymptotic solution, the
receptivity analysis also revealed a solution in the immediate neighbourhood of the exciter - called the
local solution [10–12]. In Sengupta [10], solution was obtained using the Bromwich contour integral
method described in Sengupta and Rao [12] and Van Der Pol and Bremmer [13]. In Gaster and
Sengupta [11], solution obtained was based on the premise that the response of the boundary layer is
dominated by the least stable mode - an idea in the normal mode stability analysis. Apart from being
unable to explain the effects of local solution and presence of multiple modes (including the continuous
spectra), the normal mode stability analysis results do not agree with experiments at lower Reynolds
numbers and higher circular frequencies.
There have been some efforts made to improve agreement of theoretical results with experiments at
lower Reynolds number by including the effect of weak boundary-layer growth in the stability analysis
using the ansatz that the difference between the two can be bridged by introducing a simple scaling
function A(X), where X is a slowly varying scale that depends upon streamwise location only. This is
the basis of investigations in Gaster [14] and in Saric & Nayefeh [15]. These references employed
different definitions to define the non-parallel effects in terms of (a) kinetic energy integral of the
disturbance flow, (b) the integrated streamwise disturbance velocity squared over the shear layer width
and (c) the imaginary part of wave growth rate etc. While there were some improvements seen for the
lower Reynolds number ranges, mismatches still remained to be reconciled. An attempt was made to
explain these shortcomings and some interesting observations were made that is described below and
is taken from Sengupta [16].
Following the ideas in Gaster [14] and Saric and Nayefeh [15], the perturbation stream function can
be defined as
ψ(x, y, t ) = ∫ [A(X )Φ0 (X, y) + εΦ1 (X, y)]ei (α x − ω0 t ) dα
(1)
Here, the leading term without A(X) is the same that one obtains from the parallel flow
approximation and the second term is the leading correction term needed to represent the non-parallel
International Journal of Emerging Multidisciplinary Fluid Sciences
Tapan K. Sengupta, Swagata Bhaumik, Vikram Singh, Sarvagy Shukl
21
effects, along with that represented by A(X). A formal perturbation analysis reveals the governing
equations for Φ0 and Φ1 are given by,
L2(Φ0) = (U – ω0/α)(Φ″0 – α2Φ0) – U″– (Φiv0 – 2α2Φ″0 + α4Φ0)/(iαRe) = 0
(2)
and
L2 (Φ1 ) = F0 A + F1
dA
dX
(3)
where F0 and F1 are expressions similar to that given in Gaster [14] and Saric and Nayefeh [15] and
are functions of the mean flow quantities; various terms proportional to Φ0 and its derivatives. It was
therefore pointed out in Sengupta [16] that in trying to obtain Φ1 from Eq. (3) one would experience
secular growth, as both Φ0 and Φ1 are governed by the same Orr-Sommerfeld operator, an essential fact
overlooked in the formulations of [14,15]. In Gaster [14] and Saric and Nayefeh [15], an equation for
A(X) was obtained from Eq (3) by using a solvability condition and the non-parallel effects were
embedded from the first term of Eq (1) only. Furthermore, unlike in the stability analysis of [14,15],
when the problem is posed as a receptivity problem given in Eq. (1), satisfaction of wall boundary
condition would reveal that A(X) cancels out from the numerator and denominator when it is assumed
that the nonparallel effects introduce mere scaling without adding or altering eigenvalues of the
corresponding linear parallel flow formulation [14, 15].
Further developments on linear receptivity analysis were reported in Sengupta et al. [17–19]. In [17],
the linearized receptivity problem to localized harmonic wall excitation was studied by removing the
restriction of the signal problem and it revealed that any problem found spatially unstable remains so
even when it is viewed in a complete spatio-temporal framework. This was further studied for spatially
stable systems to explain spatio-temporal growth of wave-fronts in [18, 19], including validating a new
energy based receptivity analysis. In a variation of receptivity analysis, Seifert & Tumin [20] reported
experimental and theoretical results on receptivity of adverse pressure gradient shear layer to wall
excitation. The experimental results were novel and theoretical results were obtained by linear stability
analysis by matching the response at a fixed location. One of the major findings of this study was that
the mismatch between experiment and theory widened with increase in circular frequency. This also
prompts one to include both nonlinearity and non-parallelism of the equilibrium flow and one such
study was reported in Fasel & Konzelmann [21] that involved studying disturbance generation and its
evolution over a flat plate boundary layer via the solution of two-dimensional Navier-Stokes equation.
In this numerical study, the exciter employed was a simultaneous blowing-suction strip - as shown in
the schematic of Fig. 1. In the limit of vanishing width of the strip, this is equivalent to a doublet, that
helped satisfy mass conservation exactly at each time step for the stream function - vorticity
formulation of the problem. The authors categorically stated that the good agreement of some of the
theories with experiments is fortuitous and that the difference between experiments and theories
concerning the branch I neutral location cannot be explained by non-parallel effects. This work
restricted itself in studying the nonparallel effects of a zero pressure gradient boundary layer and not
much attention was paid on nonlinear effects. A similar but complimentary study was undertaken by
Venkatasubbaiah and Sengupta [22] that mainly focused on receptivity and stability of mixed
convection flow past a vertical plate. The stream function-vorticity formulation included the mixed
convection via Boussinesq assumption and the flow was excited by a blowing-suction strip, as in [21].
In the same paper, nonlinear aspect of receptivity for zero pressure gradient shear layer without heat
transfer and the associated leading spatio - temporal wave fronts are also reported.
So far our discussion on calculating receptivity of boundary layers is restricted to specific wall
excitation type. Efforts have been made earlier by different investigators to study the receptivity of
boundary layers to convected disturbances in the free stream. The effects of free stream turbulence on
the stability of laminar boundary layers also comes under this category. Some of the most relevant
experimental and theoretical studies are listed here in [23–30]. The types of disturbances studied in the
experiments correspond to passing wakes and vortices [23,25,26,28,30] and free stream turbulence
[24,26,27,30]. In the numerical simulations [27–30], the major issue is to decide upon the convecting
speed of the disturbances in the free stream. There appears to be some misunderstanding on this issue
(discussed in [27,30]) as many researchers have erroneously assumed that vortices will travel with the
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Nonlinear and Nonparallel Receptivity of Zero-pressure Gradient Boundary Layer
free stream speed and that invariably shows the response field to be damped. However, a detailed
analysis by Sengupta et al. [30] has clarified this issue via simulations and analytical results that there
exists a narrow band of convection speed of disturbances (between 0.26 to 0.33 times the free stream
speed) at which the receptivity is maximum for periodically passing wakes. Created response field by
such excitations continues to be wave packets consists of TS waves - however, they amplify much
faster than that is experienced by disturbances created by constant frequency wall exciter.
In [28,31], the authors discuss about transition that takes place in fluid flow without the appearance
of TS waves and is caused by free stream turbulence. The work in [28] identifies the bypass events with
the appearance of upstream propagating modes and turbulent spots created in the outer part of the shear
layer. The analytical explanation for the existence of upstream propagating modes were provided earlier
in [27] and other references contained therein. These type of disturbances are still within the purview
of linear stability theory caused by periodic disturbance sources in the free stream. Another bypass
mode was shown theoretically and experimentally in [32,33] that is created by convecting a periodic
disturbances in the free stream. In many practical situations, actual transition will be a consequence of
the presence of some or all the prototypical mechanisms discussed so far.
In the present work, we focus upon the nonlinear receptivity of a zero pressure gradient boundary
layer excited by a blowing-suction type of wall-exciter [21,22]. The main intention is to show the role
of multi-modal nature of the instability of the flow field, that cannot be explained by normal mode
analysis practised in the linear stability theory. The multi-modal interactions cause disturbance growth
in regions of flow, which otherwise have been pronounced as stable by linear spatial stability analysis.
Such multi-modal interactions have also been attempted to be explained as weakly nonparallel effects
[14,15]. In the next section the governing equations and the used numerical methods have been
described. In section 3, numerical results have been presented along with their detailed discussion.
Section 4 contains the summary and closing remarks on the present work.
3. GOVERNING EQUATIONS AND NUMERICAL METHOD
The two-dimensional Navier-stokes equations in stream function-vorticity formulation are solved here
and are given below in non-dimensional form with respect to reference length, velocity, time, vorticity
U∞ , LU ,
and stream-function respectively as L, U∞ , –––
L , –––
∞
U∞ L
∂ω KH
1 2
+ V C ∇ω =
∇ ω
∂t
Re
(4)
∇2 ψ = –ω
(5)
LU∞ , where v is the kinematic viscosity. The out of
Here the Reynolds number Re is defined as Re = ––––
v
KH
plane vorticity is given by ω and the velocity is related to the stream function by V C = ∇ × Ψ, where
Ψ = (0, 0, ψ). The (ψ – ω) formulation is preferred here due to its accuracy and efficiency in satisfying
mass conservation exactly everywhere. The flow is computed in the transformed orthogonal (ξ – η)
plane that is utilized for grid refinement whenever necessary. In a transformed orthogonal (ξ – η) plane,
the vorticity-transport equation and the stream-function equation transforms to,
∂ω ∂ψ ∂ω ∂ψ ∂ω
1 1 ∂ h2 ∂ω
∂ h1 ∂ω
)]
+
−
=
[ (
)+
(
∂ t ∂η ∂ξ ∂ξ ∂η Re h1h2 ∂ ξ h1 ∂ ξ ∂η h2 ∂η
∂ h2 ∂ψ
∂ h1 ∂ψ
(
)+
(
) = −h1h2 ω
∂ ξ h1 ∂ ξ ∂ η h2 ∂ η
(6)
(7)
where the contra-variant components of the velocity vector are given by
u=
1 ∂ψ
h2 ∂η
(8)
International Journal of Emerging Multidisciplinary Fluid Sciences
Tapan K. Sengupta, Swagata Bhaumik, Vikram Singh, Sarvagy Shukl
v=−
1 ∂ψ
h1 ∂ξ
23
(9)
Where h1 and h2 are the scale factors of the transformation given by, h1 = (xξ2 + y2ξ )1/2 and
h2 = (x2η + yη2)1/2. In the used transformed grid, ξ is in the direction parallel to the wall and η is in the
wall-normal direction. Hence the transformation is given by x = x(ξ ) and y = y(η), so that h1 = xξ and
h2 = yη. The equations (6) and (7) are known as the vorticity transport equation (VTE) and stream
function equation (SFE), respectively.
3.1. Boundary and initial condition
Specification of proper boundary conditions and their implementation in the numerical method is an
issue of great importance in DNS. To obtain higher resolution and easily implement boundary
conditions, we compute the equations in the orthogonally transformed (ξ – η) plane, obtained from the
Cartesian frame via the transformation given by,
x(ξ ) = xin + LD [1 −
y(η ) = Lh [1 −
tanh(β (1 −ξ ))
]
tanhβ
tanh(β (1 −η ))
]
tanhβ
(10)
(11)
with 0 ≤ ξ, η ≤ 1. In the above, xin is the streamwise coordinate of the inflow of the computational
domain whose streamwise extent is given by LD = xout– xin, where xout is the location of the outflow of
the computational domain taken as 10L. Similarly, the second transformation relates the wall-normal
physical distance of Lh (equal to L), to the transformed co-ordinate η. Here, we have taken β = 2.0 to
obtain grid clustering near the inflow and the wall. A very localised wall-excitation is applied at a
location near the inflow and for this reason the grid clustering in the vicinity is required. This type of
tangent-hyperbolic transformation apart from producing desired grid clustering, also helps in reducing
aliasing error and is widely used in simulations [34].
In this computation, the steady-state solution is obtained first and thereafter we perturb the flow by
providing excitation at the wall. In the following, we discuss the boundary conditions separately - so
that the process of obtaining the mean and disturbed flows are clearly revealed. For the disturbance
flow, these boundary-conditions reveal the nature of applied excitation at the wall. However, the
boundary condition for equations (6) and (7) will be used for the total quantities (without splitting them
into mean and disturbance components) for the receptivity calculations.
In computing the steady-flow, following wall-boundary conditions have been used,
ψ wall = const.
ω wall = –
1 ∂2 ψ
h22 ∂η 2
| wall
(12)
For the computation of the perturbed flow with excitation at the wall, the boundary conditions used are
υ wall = ( −
1 ∂ψ
)|
h1 ∂ξ wall
1 ∂2 ψ
1 ∂ h2 ∂ψ
(
)− 2
|wall
ω wall = −
h 1 h2 ∂ξ h1 ∂ξ
h2 ∂η 2
(13)
The boundary condition for the stream function at the wall has been deduced from the zero normal
velocity for the equilibrium flow and from the prescribed time-dependent normal velocity at the wall,
for the perturbed flow. The wall vorticity has been calculated imposing no-slip condition at the wall in
the expression for SFE. For the receptivity calculation, the prescribed time-dependent normal velocity
at the wall corresponds to a simultaneous blowing and suction on a localised strip (as in [21,22]). The
prescribed time-dependent normal velocity at the wall is given by:
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Nonlinear and Nonparallel Receptivity of Zero-pressure Gradient Boundary Layer
Am ( x )sin(β d t )
υ wall ( x ) =
0
for x1 ≤ x ≤ x2
(14)
for x ≤ x1 or x ≥ x2
where βd is the non-dimensional disturbance angular velocity and Am(x) is the amplitude of the imposed
disturbance. Here x1 and x2 represent the beginning and the end of the streamwise extent of the strip
along the wall. The amplitude function is defined along the blowing-suction strip (as given in Fasel and
Konzelmann [21]) by:
5
4
x − x1
x − x1
x − x1
AFK ( x ) = 15.1875
− 35.4375
+ 20.25
xst − x1
xst − x1
xst − x1
3
(15)
for x1 ≤ x ≤ xst and
5
4
x −x
x −x
x −x
AFK ( x ) = − 15.1875 2
− 20.25 2
+ 35.4375 2
x2 − xst
x2 − xst
x2 − xst
3
(16)
1 + x2 , where we have taken A = αA .
for xst ≤ x ≤ x2where xst = –x–––––
m
FK
2
At the inflow and at the far-field boundary (at the top of the domain), to calculate steady as well as
the perturbed flow the following boundary conditions have been used,
U∞ = 1
ω=0
(17)
At the outflow, following convective boundary condition on vorticity has been used,
∂ω
∂ω
+ Uc
=0
∂t
∂t
(18)
The value of the convective speed Uc has been chosen as 0.5U∞. The stream-function ψ, at the outflow
–– = 0 which using (9) translates in terms of ψ as
boundary has been calculated from the condition ∂v
∂x
∂ 1 ∂ψ
(
)=0
(19)
∂ ξ h1 ∂ξ
3.2. Numerical discretization
∂ω
∂ω and –––
In the computations, the terms –––
representing convection in the VTE are discretised using high
∂ξ
∂η
∂ψ
∂ψ
resolution OUCS3 compact schemes developed in Sengupta et al. [34,35]. The terms ––– and –––
∂ξ
∂η
appearing in the VTE are discretized using second order central difference scheme. This is done to
minimize errors caused by aliasing. Since the VTE specifically tells us about the transport of vorticity,
and since the vortices are like wave-packets we need to resolve the vortices as accurately as possible
maintaining their correct group velocities as they convect. However, the convection terms are nonlinear and hence if we use high resolution schemes to discretize them then that would lead to aliasing
error. The diffusion term that appears in the VTE as well as the terms involving Laplacian operator that
appears in the SFE are all discretised using second order central difference scheme. The compact
OUCS3 scheme [34,35] used here to calculate first derivative terms are represented by primes on the
left hand side of the following equations. To begin with, explicit equations are used for the nearboundary points given by,
1
( −3u1 + 4u2 − u3 )
h
1 2β 1
8β 1
8β 1
2β
u2′ = ( 1 − )u1 − ( 1 − )u2 + (4β1+ 1)u3 − ( 1+ )u5 + 1u5
h 3 3
3 2
3 6
3
u1′ =
International Journal of Emerging Multidisciplinary Fluid Sciences
Tapan K. Sengupta, Swagata Bhaumik, Vikram Singh, Sarvagy Shukl
25
with β1, a floating constant used to stabilize computations and improving dispersion relation
preservation of the overall numerical scheme. If there are N points in that direction, for the interior
points (3 ≤ j ≤ N – 2), following implicit equations are used in the scheme [34,35],
1 k =2
∑ k = −2 qk u j + k
h
η
F
η
= D± ; q±2 = ± +
;
60
4 300
p j −1u′j −1 + u′j + p j +1u′j +1 =
where
p j ±1
q ±1 = ±
E η
+ ;
2 30
q0 = −
11η
150
with D = 0.3793894912; E = 1.57557379; F = 0.183205192 and η = –2.0. The stencil for j = N – 1 and
j = N are similar to the stencil written for j = 2 and j = 1, respectively. For better numerical properties,
one requires to use β = –0.025 for j = 2 and β = 0.09 for j = N – 1. The VTE is time advanced using
the 4th order Runge-kutta scheme with time-step of ∆t = 5.0 × 10–5. The discretized SFE is solved using
unpreconditioned Bi-CGSTAB algorithm [36].
4. RESULTS AND DISCUSSION
To calculate the receptivity of a zero pressure gradient boundary layer, Navier-Stokes equation given
in the previous section has been solved with the following numerical parameters. We have chosen the
length scale such that Re based on the reference length scale L is 105. The computational domain along
the streamwise direction domain is taken as –0.05 ≤ x ≤ 10; while in the wall-normal direction, the
computational domain is taken as 0 ≤ y ≤ 1. A total of 1600 points in the streamwise and 600 points in
the wall-normal directions are taken. For this shear layer, the reference length is taken as L ≅ 60 × δD∗ ,
where δD∗ is the displacement thickness at the outflow of the computational domain shown in Fig. 1(a).
We have taken the grid mapping in such a way that the wall-resolution is given by: ∆y 0 = 2.455 × 10–4
and the smallest grid size in the streamwise direction is given by: ∆x0 = 9.218 × 10–4. Simulation results
are presented here for the case when the suction-blowing strip exciter is located between x1 = 0.22 and
x2 = 0.264 that is excited harmonically at a circular frequency of βd. Different values of the amplitude
of the excitation is calculated with Am = αAFK, where AFK is the amplitude function taken in Fasel and
Konzelmann [21], as given here in Eqs. (15) and (16). Here, the results are shown for only α = 0.01
y
Far-field boundary
Inflow
y=1.0
Edge of shear
layer
Exciter
U∞
x1
Outflow
x
x2
xout=10
xin=–0.05
Fig. 1(a) Schematic of the flow and the computational domain including the simultaneous
blowing and suction (SBS) strip.
Amplitude
0.8000
Amplitude=0.05
Amplitude=0.1
0.6000
0.4000
0.2000
0.0000
0
100
200
300
400
500
600
k
Fig. 1(b) Fourier transform of the input disturbance through the SBS strip for the amplitudes
of excitation 0.05AFK and 0.1AFK with AFK as defined in equations (15) and (16). The exciter
is located from x1 = 0.22 to x2 = 0.264.
Volume 1 · Number 1 · 2009
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Nonlinear and Nonparallel Receptivity of Zero-pressure Gradient Boundary Layer
A
0.2
ω
0.15
0.1
0.05
O
0
1000
2000
3000
Reδ*
Fig. 1(c) The neutral curve based on linear stability theory. The straight line OA corrosponds
to the constant non-dimensional frequency parameter 3.0×10–4 considered here for
simulations.
and 0.05, while the input spectrum shown in Fig. 1(b) compares the cases of α = 0.05 and 0.10. This
comparison shows that various wave numbers in the input do not necessarily scale by the maximum
amplitude of the various cases studied. This type of nonlinear attribute of input was also studied and
reported in [22] for the zero pressure gradient boundary layer and will not be repeated here.
The non-dimensional frequency parameter that is often used to present stability analysis results relates
the circular frequency with the Reynolds numbers by Ff = βd/Re- as in [22]. In the present investigation,
we have chosen specifically the value of Ff equal to 3.0 × 10–4. The reason for this choice of frequency
will be apparent by looking at the neutral curve shown in Fig. 1(c) that is obtained using a parallel flow
stability analysis. Any disturbance that is created by a constant frequency wall exciter follows a ray
starting from the origin - as shown in this figure for the chosen frequency indicated by OA. As the flow
is linearly stable for all rays that remain outside the neutral loop, the chosen frequency represents a
linearly stable case. Upon performing receptivity calculations by solving the full Navier-Stokes equation,
if we perceive any qualitative differences from linear stability results, then that could be due to either
nonparallel or nonlinear or due to both the effects. This is the central theme of the present work.
To study the receptivity of a boundary layer, it is necessary to first obtain an equilibrium state whose
response to well-defined disturbances have to be investigated. For this purpose, the VTE and SFE given
by Eqs. (6) and (7) are solved in succession till such a time when the flow evolves to the equilibrium
state. For the present investigation, this is continued till t = 30 to obtain the equilibrium flow. In
reporting the receptivity of this steady state, we apply the simultaneous blowing-suction excitation at
the wall given by Eqs. (14)-(16) and such results are shown in Fig. 2 for the case of Ff = 3 × 10–04 and
Am = 0.05 AFK. In showing the signal in Fig. 2(a), the origin refers to the leading edge of the flat plate.
From the solution of Eqs. (6) and (7), one obtains instantaneous values of vorticity and velocity
components. The disturbance quantities are obtained (as displayed in Fig. 2) by subtracting the mean
from the total quantity. As noted earlier, this corresponds to a spatially stable case in linear theory. For
the displayed data at all heights, the disturbance velocity has a local component in the immediate
neighbourhood of the exciter (will be referred henceforth as the local solution) and this is followed by
the asymptotic wavy solution - earlier identified as the TS wave. However, one must distinguish
between the TS wave obtained by the normal mode analysis and the asymptotic solution reported here.
In normal mode analysis, only the least stable eigenmode is tracked and reported, ignoring the existence
and the contribution of other modes. In contrast, the present approach produces solution that is
contributed by all the discrete and continuous modes.
The displayed variation of streamwise disturbance velocity with streamwise coordinate at different
heights over the plate indicate an interesting phenomenon. This solution corresponds to the time t = 20.
While the linear normal mode analysis, predicts this flow field to be stable, we notice that barring the
top and bottommost frames in Fig. 2(a), the disturbances actually grow spatially at intermediate heights.
All the frames clearly indicate the presence of multiple modes and that is also directly evident from the
multiple peaks of the Fourier transform of these signals shown in Fig. 2(b). The Fourier amplitudes
show the dominant normal mode near the wall, while multiple dominant modes are seen in the third
and fourth frames showing the transform. Also, one notices the contribution responsible for the local
solution as the distant low peak at high wave numbers in Fig. 2(b). It is easy to identify the peaks in
International Journal of Emerging Multidisciplinary Fluid Sciences
Tapan K. Sengupta, Swagata Bhaumik, Vikram Singh, Sarvagy Shukl
27
(b)
(a)
10.000
Fourier amplitude
0.04
ud
0.02
0
–0.02
–0.04
0
1
2
8.000
6.000
4.000
2.000
0.000
3
50
0.03
Fourier amplitude
ud
0
–0.015
0
1
2
100
150
100
150
100
150
100
150
5.000
4.000
3.000
2.000
1.000
0.000
3
50
x
k
0.02
Fourier amplitude
5.000
0.01
ud
150
6.000
0.015
0
–0.01
–0.02
0
1
2
4.000
3.000
2.000
1.000
0.000
3
50
x
k
Fourier amplitude
0.02
ud
100
k
x
0
4.000
3.000
2.000
1.000
–0.02
0
1
2
0.000
3
50
x
k
Fourier amplitude
0.02
ud
0.01
0
–0.01
–0.02
3.000
2.500
2.000
1.500
1.000
0.500
0.000
0
1
2
x
3
50
k
Fig. 2(a) ud plotted as a function of x for t=20 at the heights 0.00385; 0.00521; 0.00662;
0.00808; 0.00958 and 0.0144 respectively from top to bottom. The signals are for the SBS
strip excitation amplitude of Am=0.05AFK; Ff=3.0×10–4 and exciter location between
x1 = 0.22 and x2 =0.264. (b) Fourier transforms of the signals shown in (a).
the spectral plane with the solution in the physical plane through Abel’s and Tauber’s theorem [13]. The
second to fourth frames in Fig. 2(a) clearly show different streamwise stretches at different heights over
which the disturbance actually grows with x corresponding to a particular mode that moves downstream
at a faster speed. The presence of this mode becomes weaker as the height increases. However, there is
another damped mode that dominates with increasing height over the plate. It is noted that in earlier
nonparallel studies (as referred to in [21]), various investigators have tried to explain experimental data
that indicated instability at particular heights for the streamwise disturbance velocity components.
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Nonlinear and Nonparallel Receptivity of Zero-pressure Gradient Boundary Layer
1
0.75
0.5
0.25
0
−0.25
−0.5
−0.75
−1
20
Fourier amplitude
(b)
20.5
t
20.75
20.25
20.5
t
20.75
800
600
400
200
21
Fourier amplitude
20.25
5
10
Frequency
15
20
5
10
Frequency
15
20
5
10
Frequency
15
20
5
10
Frequency
15
20
5
10
Frequency
15
20
800
600
400
200
21
Fourier amplitude
800
20.25
20.5
t
20.75
20.25
20.5
t
20.75
20.25
20.5
t
20.75
600
400
200
21
Fourier amplitude
normalised streamwise disturbance
1
0.75
0.5
0.25
0
−0.25
−0.5
−0.75
−1
20
normalised streamwise disturbance
1
0.75
0.5
0.25
0
−0.25
−0.5
−0.75
−1
20
(a)
800
600
400
200
21
Fourier amplitude
normalised streamwise disturbance
1
0.75
0.5
0.25
0
−0.25
−0.5
−0.75
−1
20
normalised streamwise disturbance
1
0.75
0.5
0.25
0
–0.25
–0.5
–0.75
−1
20
normalised streamwise disturbance
It has been variously noted in [12, 17–19] that there are no particular physical reasons as to why one
has to adopt either spatial or temporal framework in studying boundary layer stability. This is also readily
apparent from the information in Figs. 2 and 3. An interesting aspect of the computed results is noted with
respect to time variation - as shown in Fig. 3(a) for signals collected at a distance of x = 0.3L from the
leading edge at the indicated heights. Despite the fact that the fluid dynamic system is excited at a single
constant frequency (βd), the Fourier transform in Fig. 3(b) indicates presence of superharmonics at all
heights and of different proportions. From Fig. 1(c) one clearly notes the corresponding normal modes to
21
800
600
400
200
Fig. 3 (a) Normalised streamwise disturbance velocity time series plotted for a distance of
0.3 from the exciter at the heights 0.00385; 0.00662; 0.00808; 0.00958 and 0.0144,
respectively from top to bottom. The figure is shown for the SBS strip excitation amplitude of
0.05AFK, Ff=3.0×10–4 and the exciter location between x1 = 0.22 and x2 = 0.264.
(b) Fourier transforms of the signal shown in (a) clearly show the presence of
superharmonics.
International Journal of Emerging Multidisciplinary Fluid Sciences
Tapan K. Sengupta, Swagata Bhaumik, Vikram Singh, Sarvagy Shukl
29
be more stable from linear stability point of view for these additional superharmonics. Of specific interest
is the data for y = 0.00662 and 0.00808 that shows the presence of strong second and third harmonics. In
Fig. 2(a) also, we noted most pronounced instability at these heights. Thus, the disturbance growth at these
heights must be related to nonlinear effect and is experienced at intermediate heights only.
Apart from the fact that the instability is noted at intermediate heights, we also note the similarity of
flow field at heights very close to the wall and those in the outer edge of the boundary layer. This aspect
is depicted in Fig. 4(a), where spatial variation of the streamwise disturbance velocity is shown for
(b)
(a)
0.1
Fourier amplitude
ud
0.05
0
–0.05
–0.1
0
1
2
10.00
5.00
0.00
3
50
x
0.1
Fourier amplitude
ud
0
–0.05
–0.1
0
1
2
100
150
100
150
100
150
100
150
10.00
5.00
0.00
3
50
x
k
Fourier amplitude
0.05
ud
150
15.00
0.05
0
–0.05
0
1
2
10.00
5.00
0.00
3
50
x
k
0.01
1.600
Fourier amplitude
0.005
ud
100
k
0
–0.005
1.400
1.200
1.000
0.800
0.600
0.400
0.200
0
1
2
0.000
3
50
x
k
0.01
1.400
Fourier amplitude
ud
0.005
0
–0.005
1.200
1.000
0.800
0.600
0.400
0.200
–0.01
0
1
2
x
3
0.000
50
k
Fig. 4 (a) Streamwise disturbance velocity plotted against x for t=20 for the SBS strip
excitation with A =0.05AFK, Ff=3.0×10–4 and exciter located between x1 = 0.22 and
x2 = 0.264. The data are shown for the heights 0.00124; 0.00252; 0.00384; 0.03 and 0.032,
respectively from top to bottom. (b) Fourier transform of the signals shown in (a).
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Nonlinear and Nonparallel Receptivity of Zero-pressure Gradient Boundary Layer
1) Maximum growth height
0.015
2) Critical layer for the superharmonic of TS mode
3) Critical layer for superharmonic of 2nd mode
4) Critical layer for TS mode
0.0125
5) Critical layer for the 2nd mode
y
0.01
0.0075
1
2
3
0.005
ud
0
U
4
0.0025
5
0
0.25
0.5
0.75
1
U
Fig. 5 Mean and disturbance component of streamwise velocity shown along with various
estimates of critical layer for the TS and the second spatial mode. The line-1 indicates the
height where maximum local spatial growth is noted. Presented data are for the SBS
excitation with Am=0.05AFK; Ff=3.0×10–4 and the exciter located between x1 = 0.22 and
x2 = 0.264.
points those are either very near the wall or are in the outer part of the shear layer. Corresponding
Fourier transform of these signals are shown in Fig. 4(b). At these heights, signals display a range of x
for which they remain neutral, while in the other part, the signals decay with streamwise distance. Thus,
the Figs. 2 to 4 show that this particular case represents nonlinear receptivity at intermediate heights;
neutral stability near the wall and in the outer part of the boundary layer.
Presence of growing solution at intermediate heights is further investigated by plotting the mean and
disturbance component of streamwise velocity with height, in Fig. 5. In the same figure, we have
identified the height at which the direct simulation indicates maximum growth rate by drawing the
horizontal line-1. We have already noted that there are multiple spatial modes (including the normal
mode, identified as the TS mode in the figure) and superharmonics of the excitation frequency present
in the simulated cases. Their effects are different at different heights, as shown already in Figs. 2 to 4.
For example, in Fig. 3, one can clearly note the presence of dominant superharmonics at y = 0.00662
and 0.00808. While they are also noted at different heights, they play secondary roles there. In
discussing this aspect of Fig. 3, we have reasoned that these are essentially nonlinear effects which
come into play in the proximity of critical layers. These critical layers for the TS and the second modes
are identified in Fig. 5 - their location indicated by lines 2 to 5. It is seen that the maximum growth
height is located closer to the critical heights of the TS and second modes corresponding to the first
superharmonics-at which the linearized convection terms disappear in the governing Orr-Sommerfeld
equation for the TS mode-fundamental frequency combination.
4.1. Role of amplitude of excitation
To understand the role of the amplitude of excitation through the blowing-suction strip, another case is
computed with identical excitation parameters, except the amplitude of wall excitation is doubled to
Am = 0.10 AFK. We note that the used numerical methods used here do not attenuate the signal
International Journal of Emerging Multidisciplinary Fluid Sciences
Tapan K. Sengupta, Swagata Bhaumik, Vikram Singh, Sarvagy Shukl
31
0.003
y
0.002
0.001
Bubbles
0.000
0
1
2
3
x
Fig. 6 Streamline contours shown in the physical plane for t=20 for the case of Am=0.10AFK;
Ff=3.0×10–4 and exciter located between x1 = 0.22 and x2 = 0.264. Note the micro-bubbles
near the exciter on the plate.
(a)
(b)
Fourier amplitude
0.04
ud
0.02
0
–0.02
–0.04
0
1
x
2
3
8.000
7.000
6.000
5.000
4.000
3.000
2.000
1.000
0.000
50
100
k
150
200
50
100
k
150
200
50
100
k
150
200
0.06
Fourier amplitude
0.04
ud
0.02
0
–0.02
–0.04
15.000
10.000
5.000
–0.06
0
1
x
2
0.000
3
Fourier amplitude
0.01
ud
0.005
0
–0.005
–0.01
0
1
x
2
3
2.000
1.000
0.000
Fig. 7(a) Disturbance streamwise velocity component plotted for the heights 0.00245;
0.00521 and 0.035, respectively from top to bottom at t=20. Results presented are for
the SBS strip excitation with Am=0.10AFK; Ff=3.0×10–4 and the exciter located between
x1 = 0.22 and x2 = 0.264. (b) Fourier transform of the signals shown in (a).
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Nonlinear and Nonparallel Receptivity of Zero-pressure Gradient Boundary Layer
artificially and it is for this reason that the amplitudes considered here are a small fraction of the
excitation amplitude taken in [21]. Even the large amplitude case considered in this subsection
corresponds to the amplitude that is one-tenth the amplitude considered in [21]. Doubling of the
blowing-suction amplitude causes micro-separation near the exciter, on the plate. Resultant steady
separation bubbles are confined to small height at the wall - as shown in the stream function contours
shown in Fig. 6 at t = 20. Only a few representative contours have been shown plotted in this figure
that clearly show the micro-bubbles near the exciter seen up to x ≤ 1.6 only. However, effects of the
present bubbles are noted in the other contours shown at other heights.
To understand the dynamics of this case better, instantaneous snapshot at t = 20 is shown for the
streamwise disturbance velocity variation with x at three heights in Fig. 7(a). In the figure on the right
hand side, corresponding Fourier transform is shown alongside in Fig. 7(b) that helps identify various
components of the solution in the physical space. There is an effect of increasing the amplitude of
excitation that is noted here for the increased amplitude. Presence of separation bubbles causes the fluid
particles outside the bubbles to traverse in the transverse direction more than in the streamwise
direction and this is reflected in the lower value of ud for the higher Am case, as can be ascertained by
comparing Figs. 7 with 2 and 4. Also, these micro-bubbles interfere with the local solution that is
clearly seen in the Fourier transform of Fig. 7(b) as compared to that shown in Fig. 2(b) for the peak
corresponding to the local solution near k = 145. In fact, for the data shown at the second height next
to the wall (y = 0.000245), the local solution peak is more pronounced as compared to the local solution
peaks for y = 0.00521 and y = 0.035. We conjecture that with increasing the width of the exciter and
increasing the amplitude of excitation further, separation bubbles will be more pronounced, that could
interfere destructively with the TS waves - as has happened in this case in a low intensity. However,
450
0.75
400
0.5
350
0.25
300
250
Amplitude
U
(b)
(a)
1
0
–0.25
200
150
–0.5
100
–0.75
50
–1
1.3
13.1
13.2
13.3
13.4
time
13.5
13.6
13.7
0
5
10
frequency
15
20
0
5
10
frequency
15
20
0
5
10
frequency
15
20
1
400
0.5
350
Amplitude
0.75
U
0.25
0
−0.25
300
250
200
150
−0.5
100
−0.75
50
−1
1.3
13.1
13.2
13.3
13.4
time
13.5
13.6
13.7
1
0.75
400
Amplitude
0.5
U
0.25
0
–0.25
–0.5
300
200
100
–0.75
–1
1.3
13.1
13.2
13.3
13.4
time
13.5
13.6
13.7
Fig. 8 (a) Normalised streamwise disturbance velocity time series plotted at a distance of
0.3 away from the exciter, at the heights: 0.00124; 0.00662 and 0.034 for the SBS stripexcitation with Am=0.10AFK, Ff=3.0×10–4 and the exciter located between x = 0.22 and
0.264. (b) Fourier transform of the signal shown in (a).
International Journal of Emerging Multidisciplinary Fluid Sciences
Tapan K. Sengupta, Swagata Bhaumik, Vikram Singh, Sarvagy Shukl
33
presence of TS waves is unmistakable for this case of Am = 0.1 AFK. There is another difference for the
results of the present case that is noted in the outer part of the boundary layer. For Am = 0.05AFK case,
solution shown at y = 0.032 in Fig. 4 did not show any instability. In contrast, for the case of
Am = 0.10 AFK the results shown for y = 0.035, one can distinctly see the presence of a streamwise
stretch over which the disturbance actually grows.
In Fig. 8(a), the time series for the streamwise disturbance velocity is shown at x = 0.3 for the three
indicated heights. These time series’ are multi-periodic, as it is evident from the Fourier transform
shown in Fig. 8(b). Once again, the dominant presence of second and third harmonics are noticeable in
the interior of the shear layer (at around y = 0.00662), similar to the case shown in Fig. 3. The
superharmonics are not seen for y = 0.034 and above in this case.
Thus, the results shown so far indicate why the experimental observation of nonparallel and
nonlinear effects were not predicted satisfactorily using weakly nonlinear and nonparallel theories.
While we have only presented results showing the effects of increasing the amplitude of excitation,
more simulations have been planned to further investigate the roles of frequency of excitation, width
and location of the SBS strip in near future.
5. SUMMARY
We have reported the receptivity of zero pressure gradient boundary layer to time-harmonic wall
excitations of different amplitudes here. While the effects of different frequencies and width of the
exciter strip is planned for future, we have reported here a single frequency case for two different
amplitudes to highlight the nonlinear and boundary layer growth effects.
Highly accurate numerical methods used here are not unduly dissipative and dispersive that allows
one to investigate systematically the above mentioned effects by solving the Navier-Stokes equation for
the receptivity study. In the present investigation, we have used amplitudes of excitations those are only
5% and 10% of the amplitudes considered in Fasel and Konzelmann [21]. We have investigated a
specific frequency that is known to produce stable normal mode obtained by linear spatial instability
analysis method. However, the corresponding earlier experiments in [7] and those referred in [14,15]
have reported them to be selectively unstable. Various authors have attributed this anomaly to the
growth of the boundary layer and the neglected nonlinearity in the normal mode analysis. Presented
results here tries to reconcile the same via direct simulation of Navier-Stokes equation. In this approach
most of the assumptions of linear theory can be removed (excepting the fact that the flow is twodimensional) and one can mainly account for all the present modes in a spatio-temporal framework. In
consonance with the results of Bromwich contour integral method as applied to this problem in
[12,17–19] for the linear receptivity approach, we have identified the numerical response as a
combination of local and asymptotic solution.
For the lower amplitude case, we have identified the local and asymptotic solution contributed by
different modes and their interactions. Resultant solution indicate instability at some intermediate
heights that seems compatible with the experimental observations. This is attributed to neglected
nonlinearity that appears to be important at the critical height corresponding to the spatial modes due
to the first superharmonics of the excitation frequency.
When the amplitude of excitation is doubled, while keeping other parameters of the simultaneous
blowing-suction strip the same, we notice clearly the amplitude effects in terms of some micro-bubbles
forming on the plate, near the exciter. These have the effects of reducing the streamwise distrubance
velocity magnitude, while creating high wave number disturbances affecting the local solution.
However, the wave number of the asymptotic solution do not change with the doubling of the excitation
amplitude.
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