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Article

Feedback Control for Transition Suppression in Direct Numerical Simulations of Channel Flow

Department of Aerospace Engineering & Mechanics, University of Minnesota, Minneapolis, MN 55455, USA
*
Author to whom correspondence should be addressed.
Energies 2019, 12(21), 4127; https://doi.org/10.3390/en12214127
Submission received: 12 September 2019 / Revised: 24 October 2019 / Accepted: 26 October 2019 / Published: 29 October 2019
(This article belongs to the Special Issue Control of Dynamic Flow Fields)

Abstract

:
For channel flow at subcritical Reynolds numbers ( R e < 5772 ), a laminar-to-turbulent transition can emerge due to a large transient amplification in the kinetic energy of small perturbations, resulting in an increase in drag at the walls. The objectives of the present study are three-fold: (1) to study the nonlinear effects on transient energy growth, (2) to design a feedback control strategy to prevent this subcritical transition, and (3) to examine the control mechanisms that enable transition suppression. We investigate transient energy growth of linear optimal disturbance in plane Poiseuille flow at a subcritical Reynolds number of R e = 3000 using linear analysis and nonlinear simulation. Consistent with previous studies, we observe that the amplification of the given initial perturbation is reduced when the nonlinear effect is substantial, with larger perturbations being less amplified in general. Moreover, we design linear quadratic optimal controllers to delay transition via wall-normal blowing and suction actuation at the channel walls. We demonstrate that these feedback controllers are capable of reducing transient energy growth in the linear setting. The performance of the same controllers is evaluated for nonlinear flows where a laminar-to-turbulent transition emerges without control. Nonlinear simulations reveal that the controllers can reduce transient energy growth and suppress transition. Further, we identify and characterize the underlying physical mechanisms that enable feedback control to suppress and delay laminar-to-turbulent transition.

1. Introduction

Channel flow is ubiquitous in engineering applications, and the laminar-turbulent state of the flow is of great practical consequence. In general, since laminar flows experience smaller wall friction than turbulent flows, laminar-to-turbulent transition suppression has been a primary objective in many flow control studies of channel flow. Extensive studies have been performed to understand the characteristics of channel flows [1,2,3,4,5], among which hydrodynamic stability analysis is widely used to examine behaviors of small perturbations around a laminar equilibrium state of the flow. The linear stability result is often used to determine the critical condition for a laminar-to-turbulent transition to arise [6,7,8,9]. For plane Poiseuille flows, linear stability analysis identifies a critical Reynolds number of R e = 5772 , below which the flow state will remain laminar and infinitesimal perturbations will decay to zero asymptotically [7]. However, a laminar-to-turbulent transition in plane Poiseuille flow has been observed in experiments and simulations at Reynolds numbers far smaller than the critical one [10,11,12]. This phenomenon is caused by a short-time transient amplification of small perturbations before their eventual decay. This so-called transient energy growth results from the non-normality of the linearized perturbation dynamics [13,14], which can contribute to the laminar-to-turbulent transition observed in plane Poiseuille flow at subcritical Reynolds numbers. To delay or suppress a transition in plane Poiseuille flow, modern feedback control theory has been investigated [15,16,17,18,19]. One approach is to reduce transient energy growth by designing feedback control laws based on the linearized perturbation dynamics, as the large energy amplification plays an important role in the transition process. Kim and Bewley have summarized the essential ingredients of linear control theory for fluid mechanics in a review paper [20]. Bewley and Liu applied linear optimal ( H 2 ) and robust ( H ) control methods on both subcritical and supercritical channel flows aiming at reducing disturbance response [16]. Moreover, Jovanović and Bamieh have investigated componentwise energy amplification in channel flows via input–output analysis, finding that wall-normal and spanwise forces can affect the flow more significantly than streamwise force [21], which inspires a use of wall-normal or spanwise velocity actuation in flow control studies. Martinelli et al. designed a linear optimal control strategy to suppress the maximum transient energy growth experienced in subcritical channel flow [19]. Although the nonlinearity can be taken into consideration within the control synthesis [22,23], linear control synthesis is more accessible and has been more commonly employed for flow control.
Among all the possible disturbances, the optimal disturbance leads to the maximum transient energy growth [9], which has the highest chance to induce a laminar-to-turbulent transition of the flow. The optimal disturbance is usually computed based on the linearized operator [24], though nonlinear notions can also be determined [25]. In the present work, we focus on the initial optimal disturbance computed based on the linear model. The optimal disturbance is calculated for the uncontrolled and controlled systems. Control will alter the perturbation dynamics, and so, the optimal disturbance for the controlled flow will differ from that of the uncontrolled flow, in general [26]. This point has been emphasized in recent studies [27,28,29] aiming to evaluate the overall performance of feedback controllers.
In this paper, we first perform linear and nonlinear simulations to study transient energy growth and transition in plane Poiseuille flows. We investigate nonlinear effects using direct numerical simulations. In contrast to previous studies, we adopt a relatively large domain to faithfully capture the full transition process. It is found that the nonlinearity serves to suppress the amplification of kinetic energy and that this effect becomes more pronounced for larger perturbations. For the oblique and streamwise wave disturbances, streamwise vortices grow based on the development of coherent vortical structures initiated from the optimal disturbances. The breakdown of these streamwise vortices leads to a laminar-to-turbulent transition. For the spanwise wave disturbance, high shear is induced between merged and large-scale streamwise vortices, where secondary instabilities grow and break the coherent structure to trigger a laminar-to-turbulent transition. Although these transition mechanisms are not entirely new, we will focus on how feedback control favorably alters these mechanisms to impede the transition process.
Linear quadratic controllers are designed to reduce the large transient energy growth experienced in the uncontrolled flows. Actuation is implemented in the form of wall blowing/suction within the nonlinear simulation, which has been shown to be capable of suppressing or delaying transition [19]. Here, we investigate the control mechanism by which actuation favorably conditions the flow to prevent transition. For the oblique and streamwise wave disturbances, wall actuation modifies the distribution of high shear present in the flow, which prevents the large transient energy growth associated with the development of coherent structures. For the spanwise wave disturbance, we will show that wall actuation induces small streamwise vortices near the channel wall, which hinders the growth of merged vortices and further reduces the high shear formed between adjacent streamwise vortical structures.
Finally, we note that, although numerous studies have considered linear feedback control for transition suppression in channel flow, a detailed investigation into the role of nonlinearities on control performance has not been presented elsewhere. Here, we investigate the role of nonlinearities on controller performance—both in terms of reducing transient energy growth and of suppressing transition—within direct numerical simulations. In an effort to keep our analysis relevant within the context of the established literature, we implement a simple actuator model based on wall-normal blowing and suction along the walls of the channel. Further, by adopting a larger computational domain than previous investigations, our analysis captures a richer set of the relevant nonlinear flow physics underlying the laminar-to-turbulent transition process.
The paper is organized as follows. Numerical approaches are provided in Section 2, including details on the computational setup for direct numerical simulations and methods for feedback control synthesis. In Section 3, we discuss uncontrolled flows that exhibit transition for various optimal disturbances. The results for controlled flows are also provided in this section with detailed discussions of the control mechanisms. Finally, conclusions are summarized in Section 4.

2. Numerical Approaches

2.1. Direct Numerical Simulation

Two- and three-dimensional direct numerical simulations of plane Poiseuille flow are performed using the spectral code Channelflow [30,31] to solve the incompressible Navier–Stokes equations. A second-order Runge–Kutta temporal scheme is used. Streamwise, wall-normal, and spanwise directions are indicated by x, y, and z, respectively, and the corresponding velocity components are u , v , and w , respectively. Time is denoted by t. As shown in Figure 1, the flow between two infinite planes has a base velocity profile of [ u ¯ , v ¯ , w ¯ ] = [ 1 ( y / h ) 2 , 0 , 0 ] at Reynolds number of R e = u ¯ c h / ν = 3000 , where h is the channel half-height, u ¯ c denotes the center velocity of the base flow, and ν is the kinematic viscosity of the fluid. The velocity is non-dimensionalized by u ¯ c . In the simulations, periodic boundary conditions are assumed in the x- and z-directions in which the flow variables (velocity and pressure) are represented by Fourier expansion. In the y-direction, flow variables are represented by Chebyshev polynomials, and no-slip boundary condition is specified at upper and lower walls for the uncontrolled flow. Moreover, a constraint of constant bulk velocity is specified. For the controlled flow, actuation in the form of blowing and suction in the y-direction is introduced on the entire upper and lower walls, which follows the Fourier expansion in the x- and z-directions as well. The actuation is illustrated in Figure 1 using an example of a case having streamwise wave-like actuation. The amplitude of wall actuation is determined by the feedback law described later in Section 2.2.
We use a rectangular computational domain of size 8 π h × 2 h × 2 π h in the x-, y-, and z-directions, respectively. Chebyshev points of N = 101 in the y-direction are prescribed to discretize the flow field for all the cases. Uniform grids of 128 × 64 are used for the x- and z-directions, respectively. Although the cases with either streamwise-constant or spanwise-constant disturbances are two-dimensional flows, the laminar-to-turbulent transition is a three-dimensional flow phenomenon [32] such that a three-dimensional mesh is necessary to resolve the transition process in the simulations. For both uncontrolled and controlled flows, grid resolution studies with doubled grids in each direction have been performed to ensure accuracy of the results. Moreover, we have also studied the influences of computational domain size on the simulations results. In past studies, the domain size is usually set to fit one wavelength of the wavenumber of interest for each direction. However, as the transition includes large-scale deformation of the original perturbation structures, the underlying physics during the transition processes cannot be fully captured with a limited domain size. Hence, we select a relatively large domain to capture a broader extent of flow physics involved in the transition process. This provides a more realistic setting to assess transition control performance. The evolution of the perturbation prior to transition is not affected by the domain size, but the post-transition process is dependent on the domain size. Once a sufficiently large domain size is determined, the simulations are converged and the observations among cases are consistent regardless of increasing domain size.
For the simulations of both uncontrolled and controlled flows, the initial condition of the flow field consists of the base flow [ u ¯ , v ¯ , w ¯ ] and a small initial perturbation [ u 0 , v 0 , w 0 ] , where subscript ( · ) 0 denotes initial value. The perturbation is the optimal disturbance associated with a wavenumber pair of ( α , β ) , and its kinetic energy density is denoted by E 0 . The optimal disturbance can lead to a maximum transient energy growth, and it is pre-calculated using the algorithm proposed by Whidborne and Amar [24]. Since the dynamical systems of the uncontrolled and controlled flows are different, the optimal disturbance is calculated for each system independently to guarantee that we examine the largest transient energy growth in each case. Moreover, a random perturbation with kinetic energy density of 1 % of E 0 is added to expedite the emergence of a laminar-to-turbulent transition in the flows. The addition of a random perturbation has a negligible influence on the shape of the optimal disturbance and is a common practice in transition studies [32].

2.2. Linearized Navier–Stokes Equations and Feedback Control Design

To use modern control theory to design feedback controllers, a state-space representation of the fluid flow problem is required. For plane Poiseuille flow, we decompose the flow state q ˜ into a base state q ¯ and a small perturbation q , where q = [ u , v , w , p ] T ( p is pressure) and the base state velocity profile is [ u ¯ , v ¯ , w ¯ ] = [ 1 ( y / h ) 2 , 0 , 0 ] . The kinetic energy density of a perturbation is defined as follows:
E = 1 2 V v o l = V ( u 2 + v 2 + w 2 ) d v o l ,
where V is the volume of the computational domain.
By substituting the expression of q ˜ = q ¯ + q into the Navier–Stokes equations and by assuming that the perturbation is much smaller than the base state in magnitude ( | q | | q ¯ | ), we linearize the equations by retaining linear terms and by neglecting higher-order nonlinear terms. Next, the real-valued perturbation is expressed using a Fourier expansion:
q ( x , y , z , t ) = q ^ ( y , t ) e i ( α x + β z ) + complex conjugate ,
where q ^ ( y , t ) is the amplitude function of the perturbation associated with streamwise wavenumber α and spanwise wavenumber β such that each disturbance analyzed in the present work is with a prescribed wavenumber pair of ( α , β ) . By substituting Equation (2) into the linearized Navier–Stokes equations, we can reformulate the governing equations into a state-space form:
X t = A ( q ¯ ; α , β ) X ,
where X = [ v ^ , η ^ ] T ; v ^ and η ^ denote wall-normal velocity perturbation and wall-normal vorticity perturbation, respectively; and superscript ( · ) T represents transpose. The dynamics matrix A is derived from linearized Navier–Stokes equations, which follow the form proposed by Schmid and Henningson [9]. By choosing a real-valued wavenumber pair ( α , β ), we can analyze perturbations associated with various structures. In the present work, we examine optimal disturbances for three different wavenumber pairs— ( α , β ) = ( 1 , 0 ) , (0,2), and (1,1). Disturbances associated with these three types of wavenumber pairs—streamwise wave (Tollmien–Schlichting wave), spanwise wave, and oblique wave disturbances—cover the most representative laminar-to-turbulent transitions following different routes [32]. The features of each optimal disturbance will be discussed in Section 3.
In the control design, we introduce actuation in the form of blowing and suction on the upper and lower channel walls. We admit the difficulty in implementing such actuation in practice; however, this control configuration has been conventionally adopted in other channel flow studies. In the present study, this choice enables a focused study of nonlinear effects and control mechanisms for successful transition suppression without introducing complexities of more practical actuator models. To synthesize this actuation into the dynamical system, we add a control input term B U to the uncontrolled system (Equation (3)) to form the following system:
X c t = A c X c + B U ,
where the control inputs in U = t [ v ^ + h , v ^ h ] T are the rate of change of wall-normal velocity on the upper and lower walls and B is the input matrix that maps the influence of control inputs on the system. Due to the no-slip boundary condition ( v ^ ± h = 0 ) applied on the walls of the uncontrolled flow, v ^ ± h is excluded while forming the flow state X in Equation (3). As v ^ ± h is nonzero in the controlled flow, we will append these two variables to the flow state X to form a new state X c = [ X , v ^ + h , v ^ h ] T . Analogously, the dynamics matrix A is modified and denoted by A c to account for the new state. More information about the system modeling can be found in the work by McKernan et al. [33].
Based on the state-space model in Equation (4), linear-quadratic regulator (LQR) is designed for use in feedback control. The control objective is to minimize the cost function:
J = 0 ( X c T Q X c + U T R U ) d t
which is subject to the linear dynamics (Equation (4)), where Q and R are weight matrices. The term X c T Q X c represents kinetic energy density E. The input weighting matrix R serves to penalize the control effort and is chosen here to be a diagonal matrix with each element equal to 10 6 . The weight matrix R is chosen to be small to impose a minimal penalty on the control input. This serves to prioritize the regulation of perturbation energy in the objective function. The feedback control law is given by U = K X c , where matrix K is the state feedback control gain. This feedback control law requires full knowledge of flow state. Given the dynamics matrix A c , input matrix B, and weight matrices Q and R, the control gain matrix K can be calculated by solving an algebraic Riccati equation [34]. The LQR controller is implemented in the direct numerical simulations, as described earlier. Results are presented in the next section.

3. Results and Discussions

In this section, transient energy growth of optimal disturbances associated with three wavenumber pairs of ( α , β ) = ( 1 , 0 ) , ( 0 , 2 ) , and ( 1 , 1 ) are investigated using direct numerical simulations for the subcritical plane Poiseuille flow at R e = 3000 . The required conditions for a laminar-to-turbulent transition to appear in a fully nonlinear flow are examined for each case, and the flow features that are responsible for the transition are examined as well. Moreover, we present LQR feedback controllers that can successfully suppress or delay the transition and then examine the underlying physics related to the control mechanisms.

3.1. Transient Energy Growth of Optimal Disturbance

We start the discussion from the nonlinear analysis of transient energy growth resulting from a pure optimal disturbance, i.e., without a random perturbation added. Using the optimal disturbance as the initial condition, the Navier–Stokes equations were integrated to obtain the response of kinetic energy density, as shown in Figure 2. All of the optimal disturbances considered in the present work experience large transient energy amplifications with orders of magnitude from O ( 10 1 ) to O ( 10 3 ) ; the disturbance of streamwise vortices ( ( α , β ) = ( 0 , 2 ) in Figure 2b) reaches the largest maximum transient energy growth. In the linear simulation—denoted by red dots in each subplot—the normalized energy response E / E 0 does not depend on the magnitude of the initial perturbation.
In the nonlinear simulations, we integrate the Navier–Stokes equations of full state velocity q ˜ and report the kinetic energy density of perturbations after subtracting the base flow q ¯ . As shown in Figure 2, when the perturbation is small enough such as E 0 10 6 for cases with ( α , β ) = ( 1 , 0 ) and ( 1 , 1 ) and E 0 10 8 for case with ( α , β ) = ( 0 , 2 ) , nonlinear effects are negligible and the energy response is identical to that of the linear result. However, when the amplitude of initial disturbance increases, the amplification of kinetic energy density E / E 0 decreases, which indicates that the nonlinearity suppresses energy amplification. In other words, the nonlinearity competes with the linear non-modal growth and inhibits the transient energy amplification for sufficiently large E 0 .
Although we have seen transient energy growth in both linear and nonlinear simulations, there is no laminar-to-turbulent transition observed, suggesting that the growth of optimal disturbance alone cannot trigger the transition. As discussed in the study by Reddy et al. [32], the addition of a random perturbation is required to observe transition in simulations. Hence, we added a random perturbation with a contribution of 1 % of E 0 to the optimal disturbance to initiate laminar-to-turbulent transitions. Before the laminar-to-turbulent transition, the energy response due to this modified disturbance is nearly identical to the energy response due to a purely optimal disturbance. Since the transition process of each wavenumber pair follows different routes, we will discuss all the three paths to transition below.

3.1.1. Oblique Disturbance ( α , β ) = ( 1 , 1 )

Flow fields of a laminar-to-turbulent transition case with ( α , β ) = ( 1 , 1 ) and E 0 = 0.5 × 10 4 are shown in Figure 3, and the iso-surface of Q -criterion [35] is calculated using full flow state q ˜ . The initial optimal disturbance is in an oblique wave with large amplitude near the channel walls, as shown in the subplot in Figure 3. As the disturbance evolves over time, large-scale oblique structures form with sizes comparable to the channel half-height. After the transient energy reaches the maximum value around t u ¯ c / h = 20 (see Figure 4), large amplitudes of streamwise vorticity appear in the vicinity of the coherent structures at the channel walls at t u ¯ c / h = 36 . Meanwhile, slight spatial variations of the coherent structures appear along the oblique direction. Later, at time t u ¯ c / h = 72 , streamwise vortices are induced from the oblique coherent structures and grow into streamwise streaks, although the overall transient energy density has started to decay, as shown in Figure 4. After t u ¯ c / h = 84 , these streamwise streaks break into small-scale structures and a laminar-to-turbulent transition emerges.
The time evolution of kinetic energy density E for a range of optimal disturbances is presented in Figure 4. For optimal disturbance with E 0 < 0.5 × 10 4 (denoted by grey lines), the initial disturbance is the most amplified yet the induced streamwise vortices do not grow significantly. The disturbance eventually decays to zero without triggering a laminar-to-turbulent transition. We also note that the nonlinear flow with small disturbance ( E 0 = 1.0 × 10 6 ) is well predicted by the linear analysis as seen by the overlap between nonlinear simulation and linear results in Figure 4a. By examining the absolute value of the perturbation kinetic energy (Figure 4b), the transition cases have relatively high values in E, which suggests that a combined effect of initial optimal disturbance and its corresponding amplification determines whether or not a transition occurs. The larger amplitude disturbance gives a higher chance of triggering transition to turbulent state, which also indicates that a reduction in transient energy growth has potential to suppress or delay the transition observed in the uncontrolled flow. This motivates using control to reduce transient energy growth.
Friction velocity u * is defined using wall shear stress τ w and density of the flow:
u * = τ w ρ ,
where τ w = μ ( u / y ) , μ is dynamic viscosity, and density ρ is set to one for incompressible flow. As a sharp increase in friction velocity u * indicates an emergence of laminar-to-turbulent transition, a summary of transition cases are shown in Figure 5 illustrating the features of friction velocity u * , in which the flow in turbulent state has been denoted by dashed lines. Based on the feature of friction velocity, the larger the initial disturbance, the earlier laminar-to-turbulent transition appears. Moreover, a large initial disturbance leads to large shear stress in the wall-normal direction near the channel walls.

3.1.2. Streamwise Wave Disturbance ( α , β ) = ( 1 , 0 )

The optimal disturbance with wavenumber pair of ( α , β ) = ( 1 , 0 ) is the well-known Tollmien–Schlichting wave of which the structures are uniform in the spanwise direction. The evolution of the optimal disturbance is shown in Figure 6 with E 0 = 1.0 × 10 4 . The feature of the optimal disturbance is similar to the case with oblique disturbance: a large disturbance is observed in streamwise velocity and resides near the channel walls. As the optimal disturbance grows into large-scale spanwise coherent structures, streamwise vorticity increases near channel walls, especially where the coherent structures reside, as seen in Figure 6 at t u ¯ c / h = 60 . When the streamwise vorticity is large enough, a Λ -shaped structure emerges, splits the spanwise coherent structure, and connects to the adjacent spanwise coherent structure in front, as seen at t u ¯ c / h = 108 ; then, the break of these vortices leads to a laminar-to-turbulent transition of the flow.
The transition process in this case is very similar to the oblique disturbance discussed above in Section 3.1.1. The transition is directly caused by a break of streamwise streaks that grow from the amplified optimal disturbance. It suggests that the transient energy growth of the optimal disturbance alone does not trigger the transition; rather, it is the combined effect of the growing optimal disturbance and induced secondary instabilities that leads to a laminar-to-turbulent transition. The friction velocity and evolution of transient energy density of disturbance with ( α , β ) = ( 1 , 0 ) are shown in Figure 7 and Figure 8, respectively. The features observed from the case ( α , β ) = ( 1 , 1 ) also apply on this streamwise wave disturbance. The flow tends to transition into a turbulent state when the kinetic energy density E of a disturbance becomes large; this is influenced by both the initial amplitude of the disturbance and the corresponding amplification rate.

3.1.3. Spanwise Wave Disturbance ( α , β ) = ( 0 , 2 )

The optimal disturbance associated with wavenumber pair of ( α , β ) = ( 0 , 2 ) is in the form of streamwise vortices. Shown in Figure 9 are the flow fields with initial kinetic energy density of E 0 = 1.0 × 10 4 . Relating the flow feature to normalized kinetic energy density of perturbation E / E 0 shown in Figure 10a, when the optimal disturbance grows initially, two corotating vertically aligned vortices merge into a large streamwise vortical structure. The structure remains uniform in the streamwise direction, and the corresponding transient energy reaches the maximum value around t u ¯ c / h = 60 . After the kinetic energy starts to decrease, the flow gradually experiences spatial variation as seen at t u ¯ c / h = 150 . This is associated with axial rotational motion around the streamwise vortical structures with comparable scale to the length of the streamwise domain. Next, the kinetic energy density of the flow increases again after t u ¯ c / h = 150 , and smaller structures appear in the flow (as seen at t u ¯ c / h = 240 ). After a short duration of rotational motion in the flow, a laminar-to-turbulent transition occurs around t u ¯ c / h = 300 . Based on the features of transient energy growth and corresponding flow fields, we note that the transition is a slow process covering several stages which cannot be determined simply based on the features of energy growth time histories. The features of transition cases revealed by friction velocity are similar to the cases of oblique disturbances and streamwise wave disturbances discussed above, and the friction velocity of case ( α , β ) = ( 0 , 2 ) is shown in Figure 11.

3.2. Suppression of Laminar-to-Turbulent Transition

We synthesize a full-state feedback LQR controller. The transient energy growth is significantly reduced with the corresponding wall actuation, as shown in Figure 12. In the nonlinear simulations, we update the control input U at each time step using the flow state X c and the gain matrix K calculated from the linear analysis. Accordingly, the boundary condition of wall-normal velocity v ± h is modified based on the control input U. To evaluate the overall performance of the controlled flow in terms of reducing large transient energy growth, the optimal disturbance was recalculated for the closed-loop controlled system to evaluate the maximum transient energy growth.

3.2.1. Reduction in Transient Energy Growth

Transient energy growth in each controlled case is observed to exhibit similar features as in the uncontrolled cases, namely that an increase in initial kinetic energy makes the amplification of perturbation energy decrease as shown in Figure 12. Using case ( α , β ) = ( 1 , 0 ) as an example, since the amplification of the optimal disturbance is effectively reduced with the feedback controller, the energy responses with E 0 1.1 × 10 3 almost overlap the linear result, which are denoted by red dots. This suggests that, as the growth of the disturbance is suppressed to a small magnitude by introducing control, the importance of the nonlinearity is weakened. Therefore, the results from nonlinear simulations match the result from the linear analysis as the small disturbance assumption is satisfied. The kinetic energy density of the controlled flow, initialized from the optimal disturbance calculated for the uncontrolled system, is also shown in Figure 12. The energy amplification of this disturbance is less than that of the optimal disturbance for the controlled system with the same initial amplitude. Indeed, this trend holds true regardless of the initial perturbation amplitude, though only a single perturbation amplitude is reported in the figure for clarity. This confirms that the optimal disturbance for the closed-loop dynamics should be considered when assessing control performance for transient energy growth reduction.
For each wavenumber pair, a comparison of the maximum of E / E 0 initiated from a range of optimal disturbance amplitudes is shown in Figure 13. For small disturbance amplitudes, the percent reduction of maximum transient energy remains nearly identical, indicating that the nonlinearity of small disturbances is negligible as assumed in the linear analysis. Moreover, each wavenumber scenario reaches the largest reduction of 80 % in ( E / E 0 ) max for small initial amplitudes of disturbance. For the case with ( α , β ) = ( 0 , 2 ) , this large amount of reduction in E / E 0 only applies to the cases with E 0 O ( 10 5 ) . As the initial disturbance grows in amplitude, the control performance in terms of suppressing the energy amplification degrades, such that ( E / E 0 ) max is nearly unchanged for cases with E 0 > O ( 10 3 ) . Similar findings are also observed in the other two disturbance scenarios, but the reduction in ( E / E 0 ) max is maintained for E 0 O ( 10 4 ) and E 0 O ( 10 3 ) for cases ( α , β ) = ( 1 , 1 ) and ( α , β ) = ( 1 , 0 ) , respectively.

3.2.2. Controlled Flow with Oblique or Streamwise Wave Disturbances

By reducing the transient energy growth using feedback control, the laminar-to-turbulent transition experienced in the flow with oblique or streamwise wave disturbances has been successfully suppressed. The threshold becomes higher in terms of triggering the transition process. Here, we examine how the wall actuation modifies the flow characteristics to prevent the transition in the uncontrolled flow. Because the control mechanism is similar in the cases with oblique and streamwise wave disturbances, i.e., ( α , β ) = ( 1 , 1 ) and ( 1 , 0 ) , respectively, we will use the flow with oblique disturbance as an example to illustrate the control mechanism.
As the wall actuation is in the form of Fourier waves in space, here, we show the amplitude of the wall-normal velocity at [ x , y , z ] / h = [ 0 , 1 , 0 ] to illustrate the actuation time history in Figure 14. The wall-normal velocity is normalized by the corresponding E 0 . For the case with E 0 = 1.0 × 10 4 , the transition is successfully suppressed by introducing the wall actuation. The wall-normal velocity is similar to the actuation history of smaller disturbance cases ( E 0 = 1.0 × 10 5 ). Large blowing and suction are applied initially during time 0 < t u ¯ c / h < 30 when large transient energy growth is present in the flow. Once the growth has been suppressed, the wall actuation gradually decays to zero. For the cases with larger perturbations ( E 0 = 1.0 × 10 3 and 1.0 × 10 2 ), the linear feedback control strategy fails to suppress the transition and the flow transitions to a turbulent state. The normalized wall-normal velocity deviates from the successfully controlled cases and oscillates longer in time. In the study of Lee et al. [36], a constant wall blowing and suction in the form of a traveling wave was investigated, in which phase speed and wavenumber of the actuation may not be the same as the disturbance examined. Their work uncovered the phase speed relation between the wall actuation and the flow disturbance needed to stabilize or destabilize the flows via open-loop control. In contrast, here, we investigate a closed-loop control strategy, in which the phase speed and wavenumber of the wall actuation and the disturbance are consistent.
The transient energy growth present in the uncontrolled flow is caused by a development of large-scale coherent structures, which induced streamwise vortices that further cause a transition to turbulence, as discussed above. A comparison of flow features between uncontrolled and controlled flows during the transition process is shown in Figure 15. For a fair comparison, both simulations start from the same optimal disturbance calculated from the uncontrolled flow. In the uncontrolled flow, large magnitude of the initial optimal disturbance is concentrated near the upper and lower walls, where coherent structures denoted by Q -criterion gradually grow into large-scale coherent structures. When the vertical size of the structures increases to approximately the half height of the channel ( t u ¯ c / h 21 ), the kinetic energy of perturbation reaches its maximum value. During this process, streamwise vortices creep in near the walls following the advection of the coherent structures. After t u ¯ c / h 21 , the coherent structures start to decay, leaving the induced streamwise vortices in the flow; this is especially evident in the vicinity of the channel walls. As these vortices evolve, break, and interact with each other, the flow becomes chaotic and a laminar-to-turbulent transition occurs. Therefore, the key factor leading to the final transition to turbulence is the breakdown of the streamwise vortices. These streamwise vortices are generated by the rapid growth of the large-scale coherent structures.
Compared to the mechanism observed from the uncontrolled flow, the most apparent change in the flow by introducing wall-normal actuation is the growth of the coherent structures. As shown in Figure 16, the actuation on the wall modifies the distribution of high shear in the flow, in which local areas of high shear stress are created and constrained in the vicinity of the channel walls. As a consequence, the growth of the coherent structure is confined near the walls. Because the strength of these relatively small coherent structures is not enough to induce high levels of streamwise vorticity, the transition observed from the uncontrolled flow is avoided ultimately. (Figure 15 (right)).

3.2.3. Controlled Flow of Spanwise Wave Disturbances

Wall-normal velocity histories at [ x , y , z ] / h = [ 0 , 1 , 0 ] in the controlled flows for spanwise wave disturbance are shown in Figure 17. A sharp increase in wall-normal velocity is induced when the control is turned on; then, the velocity quickly decays to a relatively small value and gradually decreases later in time. The oscillations in the wall-normal velocity at later times correspond to the fact that the flow has reached a turbulent state.
In the transition process associated with a spanwise wave disturbance ( α , β ) = ( 0 , 2 ) , the merging two corotating vortices highly distorts the base velocity profile, as seen in Figure 18. The generation of high-shear areas introduces secondary instabilities into the flow for the uncontrolled flow. To examine the control mechanism, we compare the shear flow fields at t u ¯ c / h = 50 in Figure 18. In the uncontrolled flow, high magnitude of shear stress u / z is formed between the merged vortices, where we previously observe instabilities in Figure 9. In the controlled flow, a strong actuation forms small-scale streamwise vortices near walls, as seen in Figure 18b. The introduction of these new vortices by control hinders the growth of the merged vortices. Instead, the large streamwise vortical structures are compressed and centralized in the channel. The high shear stress between the vortices is also weakened, as revealed by u ˜ / z , providing less chances for secondary instabilities to arise.
Although the controller has suppressed the growth in large streamwise vortical structures, the actuation actually introduces extra high-shear regions. As shown in Figure 19a,b, the areas denoted by (i) and (ii) indicate induced high shear stress. Accordingly, as seen in Figure 19c, new secondary instabilities creep in based on the new high-shear regions of (i) and (ii), which ultimately leads to a transition to turbulence. Hence, the secondary instabilities are introduced by the actuation in the nonlinear simulations, which are not accounted for in the controller design from the linear model.

3.2.4. Increase in Perturbation Threshold for Laminar-to-Turbulent Transition

A summary of the cases considered in the present work is provided in Figure 20 based on the nonlinear simulation results. For all three wavenumber pairs, the LQR controller successfully suppresses the transient energy growth within linear analysis. In nonlinear simulations, LQR control increases the perturbation threshold E 0 for a laminar-to-turbulent transition by roughly an order of O ( 10 ) in amplitude in the cases of streamwise wave ( α , β ) = ( 1 , 0 ) and oblique ( α , β ) = ( 1 , 1 ) disturbances. For the spanwise wave disturbance ( α , β ) = ( 0 , 2 ) , LQR controller successfully suppresses the transient energy growth of the streamwise coherent structures. However, new instabilities are induced by the strong actuation applied on the walls, which leads to laminar-to-turbulent transition by another route; hence, the perturbation threshold does not change based on the cases considered.

4. Conclusions

In this paper, we examined the laminar-to-turbulent transition in plane Poiseuille flow due to transient energy growth of optimal disturbances at a subcritical Reynolds number of R e = 3000 . A large domain is used in the present work in order to capture the large-scale dynamics that are critical to the laminar-to-turbulent transition process. Nonlinear effects on transient energy growth were investigated by performing direct numerical simulations. We found that, with the presence of nonlinearity in the flow, an increase in initial energy density of an optimal disturbance leads to a reduction in amplification rate. Moreover, we uncovered the underlying physics of the transition process for all the disturbances considered. For disturbances associated with ( α , β ) = ( 1 , 1 ) and (1,0), the transient energy growth corresponds to the development of large coherent structures. The evolution of these large-scale coherent structures induces a growth of streamwise vortices near the channel walls, and the breakdown of these vortices leads to a laminar-to-turbulent transition. For a disturbance associated with ( α , β ) = ( 0 , 2 ) , the base flow is highly distorted due to the growth of streamwise vortices, which results in high-shear-stress regions formed between the streamwise vortical structures. These high-shear areas introduce secondary instabilities that lead to a laminar-to-turbulent transition.
LQR feedback controllers were designed and shown to be capable of reducing transient energy growth via wall-normal blowing and suction actuation at the upper and lower walls. In the controlled flow, the wall actuation modified the shear distribution in the flow, such that coherent structures only formed in the vicinity of the channel walls. For streamwise wave ( α , β ) = ( 1 , 0 ) and oblique ( 1 , 1 ) disturbances, this resulted in a more rapid decay of disturbance energy than for the uncontrolled flow. Laminar-to-turbulent transition was prevented because the hindered growth of coherent structures significantly inhibits the strength of induced streamwise vortices. The control strategy was found to increase the threshold for transition by approximately O ( 10 ) in magnitude. For the case with spanwise wave disturbance of ( α , β ) = ( 0 , 2 ) , the controller did not effectively increase the threshold for the transition; the actuation was found to induce extra instabilities that led the flow to transition from a laminar to turbulent state.
The present work has shown the capability of feedback control for suppressing transient energy growth and for preventing laminar-to-turbulent transition. The nonlinear effects and underlying physics related to transition process have been investigated by performing direct number simulations. Although LQR control has been shown to suppress transition in past studies, we note that the resulting reduction of transient energy growth is not sufficient to fully suppress transition due to large amplitude perturbations. The nonlinear effects should be considered in control designs in order to improve the control performance for large disturbance. Moreover, we have identified physical mechanisms that enable actuation to delay transition, providing valuable insights that can guide the design of future actuation strategies.

Author Contributions

Conceptualization, M.S.H. and Y.S.; methodology, M.S.H. and Y.S.; software, Y.S.; validation, M.S.H. and Y.S.; formal analysis, Y.S.; investigation, Y.S.; resources, M.S.H.; data curation, Y.S.; writing–original draft preparation, Y.S.; writing–review and editing, M.S.H. and Y.S.; visualization, Y.S.; supervision, M.S.H.; project administration, M.S.H.; funding acquisition, M.S.H.

Funding

This material is based upon work supported by the Air Force Office of Scientific Research under award numbers FA9550-17-1-0252 and FA9550-19-1-0034.

Acknowledgments

We thank Minnesota Supercomputing Institute for providing computational resources.

Conflicts of Interest

The authors declare no conflict of interest.

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Figure 1. Schematic of plane Poiseuille flow with streamwise wave disturbance (not to scale), both with and without wall actuation.
Figure 1. Schematic of plane Poiseuille flow with streamwise wave disturbance (not to scale), both with and without wall actuation.
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Figure 2. Transient energy growth (TEG) of optimal disturbance with a range of initial kinetic energy density E 0 from linear (red dots) and nonlinear (solid lines) simulations for uncontrolled flows.
Figure 2. Transient energy growth (TEG) of optimal disturbance with a range of initial kinetic energy density E 0 from linear (red dots) and nonlinear (solid lines) simulations for uncontrolled flows.
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Figure 3. Time evolution of flow field to illustrate the laminar-to-turbulent transition process for the case ( α , β ) = ( 1 , 1 ) : The flow is initialized by optimal disturbance with kinetic energy density of E 0 = 0.5 × 10 4 . Iso-surfaces of Q -criterion [35] ( Q ( h / u ¯ c ) 2 = 0.001 ) colored by streamwise vorticity ω ˜ x h / u ¯ c are visualized. Only the upper half domain ( y 0 ) is displayed for clarity.
Figure 3. Time evolution of flow field to illustrate the laminar-to-turbulent transition process for the case ( α , β ) = ( 1 , 1 ) : The flow is initialized by optimal disturbance with kinetic energy density of E 0 = 0.5 × 10 4 . Iso-surfaces of Q -criterion [35] ( Q ( h / u ¯ c ) 2 = 0.001 ) colored by streamwise vorticity ω ˜ x h / u ¯ c are visualized. Only the upper half domain ( y 0 ) is displayed for clarity.
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Figure 4. Time evolution of kinetic energy density E of case ( α , β ) = ( 1 , 1 ) initialized by different amplitudes of optimal disturbance E 0 : Red lines represent transition cases, and grey lines denote that the flow remains laminar. Dashed line indicates that the flow is in turbulent state. (a) Kinetic energy density normalized by its initial value E / E 0 and (b) kinetic energy density E.
Figure 4. Time evolution of kinetic energy density E of case ( α , β ) = ( 1 , 1 ) initialized by different amplitudes of optimal disturbance E 0 : Red lines represent transition cases, and grey lines denote that the flow remains laminar. Dashed line indicates that the flow is in turbulent state. (a) Kinetic energy density normalized by its initial value E / E 0 and (b) kinetic energy density E.
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Figure 5. Time evolution of friction velocity u * of case ( α , β ) = ( 1 , 1 ) initialized by different amplitudes of optimal disturbance E 0 : Red lines represent transition cases, and grey lines denote that the flow remains laminar. Dashed line indicates that the flow is in turbulent state.
Figure 5. Time evolution of friction velocity u * of case ( α , β ) = ( 1 , 1 ) initialized by different amplitudes of optimal disturbance E 0 : Red lines represent transition cases, and grey lines denote that the flow remains laminar. Dashed line indicates that the flow is in turbulent state.
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Figure 6. Time evolution of flow field to illustrate the laminar-to-turbulent transition process for the case ( α , β ) = ( 1 , 0 ) : The flow is initialized by optimal disturbance with kinetic energy density of E 0 = 1.0 × 10 4 . Iso-surfaces of Q -criterion ( Q ( h / u ¯ c ) 2 = 0.005 ) colored by streamwise vorticity ω ˜ x h / u ¯ c are visualized. Only the upper half domain ( y 0 ) is displayed for clarity.
Figure 6. Time evolution of flow field to illustrate the laminar-to-turbulent transition process for the case ( α , β ) = ( 1 , 0 ) : The flow is initialized by optimal disturbance with kinetic energy density of E 0 = 1.0 × 10 4 . Iso-surfaces of Q -criterion ( Q ( h / u ¯ c ) 2 = 0.005 ) colored by streamwise vorticity ω ˜ x h / u ¯ c are visualized. Only the upper half domain ( y 0 ) is displayed for clarity.
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Figure 7. Time evolution of friction velocity u * of case ( α , β ) = ( 1 , 0 ) initialized by different amplitudes of optimal disturbance E 0 : Red lines represent transition cases, and grey lines denote that the flow remains laminar. Dashed line indicates that the flow is in turbulent state.
Figure 7. Time evolution of friction velocity u * of case ( α , β ) = ( 1 , 0 ) initialized by different amplitudes of optimal disturbance E 0 : Red lines represent transition cases, and grey lines denote that the flow remains laminar. Dashed line indicates that the flow is in turbulent state.
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Figure 8. Time evolution of kinetic energy density E of case ( α , β ) = ( 1 , 0 ) initialized by different amplitudes of optimal disturbance E 0 : Red lines represent transition cases, and grey lines denote that the flow remains laminar. Dashed line indicates that the flow is in turbulent state. (a) Kinetic energy density normalized by its initial value E / E 0 and (b) kinetic energy density E.
Figure 8. Time evolution of kinetic energy density E of case ( α , β ) = ( 1 , 0 ) initialized by different amplitudes of optimal disturbance E 0 : Red lines represent transition cases, and grey lines denote that the flow remains laminar. Dashed line indicates that the flow is in turbulent state. (a) Kinetic energy density normalized by its initial value E / E 0 and (b) kinetic energy density E.
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Figure 9. Time evolution of flow field to illustrate the laminar-to-turbulent transition process for the case ( α , β ) = ( 0 , 2 ) : The flow is initialized by optimal disturbance with kinetic energy density of E 0 = 1.0 × 10 4 . Iso-surfaces of Q -criterion ( Q ( h / u ¯ c ) 2 = 0.0004 ) colored by streamwise vorticity ω ˜ x h / u ¯ c are visualized.
Figure 9. Time evolution of flow field to illustrate the laminar-to-turbulent transition process for the case ( α , β ) = ( 0 , 2 ) : The flow is initialized by optimal disturbance with kinetic energy density of E 0 = 1.0 × 10 4 . Iso-surfaces of Q -criterion ( Q ( h / u ¯ c ) 2 = 0.0004 ) colored by streamwise vorticity ω ˜ x h / u ¯ c are visualized.
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Figure 10. Time evolution of kinetic energy density E of case ( α , β ) = ( 0 , 2 ) initialized by different amplitudes of optimal disturbance E 0 : Red lines represent transition cases, and grey lines denote that the flow remains laminar. Dashed line indicates that the flow is in turbulent state. (a) Kinetic energy density normalized by its initial value E / E 0 and (b) kinetic energy density E.
Figure 10. Time evolution of kinetic energy density E of case ( α , β ) = ( 0 , 2 ) initialized by different amplitudes of optimal disturbance E 0 : Red lines represent transition cases, and grey lines denote that the flow remains laminar. Dashed line indicates that the flow is in turbulent state. (a) Kinetic energy density normalized by its initial value E / E 0 and (b) kinetic energy density E.
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Figure 11. Time evolution of friction velocity u * of case ( α , β ) = ( 0 , 2 ) initialized by different amplitudes of optimal disturbance E 0 : Red lines represent transition cases, and grey lines denote that the flow remains laminar. Dashed line indicates that the flow is in turbulent state.
Figure 11. Time evolution of friction velocity u * of case ( α , β ) = ( 0 , 2 ) initialized by different amplitudes of optimal disturbance E 0 : Red lines represent transition cases, and grey lines denote that the flow remains laminar. Dashed line indicates that the flow is in turbulent state.
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Figure 12. Transient energy growth (TEG) of optimal disturbance with a range of initial kinetic energy densities E 0 from linear (red dots) and nonlinear (solid lines) simulations for controlled flows: Red dashed line is the kinetic energy density initialized from the optimal disturbance (OD) associated with the uncontrolled system.
Figure 12. Transient energy growth (TEG) of optimal disturbance with a range of initial kinetic energy densities E 0 from linear (red dots) and nonlinear (solid lines) simulations for controlled flows: Red dashed line is the kinetic energy density initialized from the optimal disturbance (OD) associated with the uncontrolled system.
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Figure 13. A comparison of maximum amplified transient energy density ( E / E 0 ) max of a range of amplitude of initial optimal disturbances between uncontrolled (solid lines) and controlled (dashed lines) cases.
Figure 13. A comparison of maximum amplified transient energy density ( E / E 0 ) max of a range of amplitude of initial optimal disturbances between uncontrolled (solid lines) and controlled (dashed lines) cases.
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Figure 14. Time history of normalized wall-normal velocity v bc / E 0 at the lower wall of the case ( α , β ) = ( 1 , 1 ) when actuation is turned on.
Figure 14. Time history of normalized wall-normal velocity v bc / E 0 at the lower wall of the case ( α , β ) = ( 1 , 1 ) when actuation is turned on.
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Figure 15. A comparison of instantaneous streamwise vorticity ω ˜ x h / u ¯ c flow fields at slice z / h = 0 between uncontrolled and controlled cases with ( α , β ) = ( 1 , 1 ) and E 0 = 0.5 × 10 4 : Black contour lines denote Q -criterion in a range of 0.01 Q ( h / u ¯ c ) 2 0.05 .
Figure 15. A comparison of instantaneous streamwise vorticity ω ˜ x h / u ¯ c flow fields at slice z / h = 0 between uncontrolled and controlled cases with ( α , β ) = ( 1 , 1 ) and E 0 = 0.5 × 10 4 : Black contour lines denote Q -criterion in a range of 0.01 Q ( h / u ¯ c ) 2 0.05 .
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Figure 16. A comparison of instantaneous flow field at slices z / h = 0 and t u c / h = 12 between uncontrolled and controlled flow with ( α , β ) = ( 1 , 1 ) and E 0 = 0.5 × 10 4 : Contours are wall-normal velocity v ˜ , and black contour lines denotes Q -criterion in a range from 0.01 to 0.05 with increment of 0.01.
Figure 16. A comparison of instantaneous flow field at slices z / h = 0 and t u c / h = 12 between uncontrolled and controlled flow with ( α , β ) = ( 1 , 1 ) and E 0 = 0.5 × 10 4 : Contours are wall-normal velocity v ˜ , and black contour lines denotes Q -criterion in a range from 0.01 to 0.05 with increment of 0.01.
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Figure 17. Time history of normalized wall-normal velocity v bc / E 0 at the lower wall of case ( α , β ) = ( 0 , 2 ) when actuation is turned on.
Figure 17. Time history of normalized wall-normal velocity v bc / E 0 at the lower wall of case ( α , β ) = ( 0 , 2 ) when actuation is turned on.
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Figure 18. Modification of instantaneous streamwise velocity gradient in spanwise direction u ˜ / z at slice x / h = 0 and t u ¯ c / h = 50 in (a) uncontrolled flow compared to (b) controlled flow: Actuation velocity is denoted by black arrows.
Figure 18. Modification of instantaneous streamwise velocity gradient in spanwise direction u ˜ / z at slice x / h = 0 and t u ¯ c / h = 50 in (a) uncontrolled flow compared to (b) controlled flow: Actuation velocity is denoted by black arrows.
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Figure 19. Secondary instabilities induced by the actuation in the flow field at t u ¯ c / h = 66 of the controlled case with ( α , β ) = ( 0 , 2 ) and E 0 = 1.0 × 10 4 : (a) Wall-normal vorticity at slice of x / h = 0 , (b) spanwise vorticity at slice of x / h = 0 , and (c) iso-surfaces of Q colored by streamwise vorticity.
Figure 19. Secondary instabilities induced by the actuation in the flow field at t u ¯ c / h = 66 of the controlled case with ( α , β ) = ( 0 , 2 ) and E 0 = 1.0 × 10 4 : (a) Wall-normal vorticity at slice of x / h = 0 , (b) spanwise vorticity at slice of x / h = 0 , and (c) iso-surfaces of Q colored by streamwise vorticity.
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Figure 20. Summary of cases considered in the present work: Solid circle represents that laminar-to- turbulent transition occurs; open circle denotes that the flow remains laminar. U and C denote uncontrolled and controlled cases, respectively.
Figure 20. Summary of cases considered in the present work: Solid circle represents that laminar-to- turbulent transition occurs; open circle denotes that the flow remains laminar. U and C denote uncontrolled and controlled cases, respectively.
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Sun, Y.; Hemati, M.S. Feedback Control for Transition Suppression in Direct Numerical Simulations of Channel Flow. Energies 2019, 12, 4127. https://doi.org/10.3390/en12214127

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Sun Y, Hemati MS. Feedback Control for Transition Suppression in Direct Numerical Simulations of Channel Flow. Energies. 2019; 12(21):4127. https://doi.org/10.3390/en12214127

Chicago/Turabian Style

Sun, Yiyang, and Maziar S. Hemati. 2019. "Feedback Control for Transition Suppression in Direct Numerical Simulations of Channel Flow" Energies 12, no. 21: 4127. https://doi.org/10.3390/en12214127

APA Style

Sun, Y., & Hemati, M. S. (2019). Feedback Control for Transition Suppression in Direct Numerical Simulations of Channel Flow. Energies, 12(21), 4127. https://doi.org/10.3390/en12214127

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