The unsteady, viscous, supersonic flow over a spike-nosed body of revolution is numerically investigated by solving the Navier-Stokes equations. The time-accurate computations are performed employing an implicit algorithm based on the second-order time-accurate LU-SGS scheme with the incorporation of a subiteration procedure to maintain time accuracy. The characteristics of the flow field for a Mach number of 3.0, Reynolds number of 7.87 x 10(6)/m, and angles of attack of 5 and 10 degrees are described. Self-sustained asymmetric shock wave oscillations were observed in the numerical computations for these angles of attack. The main characteristic of the flow field, as well as its influence on drag coefficient is discussed.
Unsteady flow; supersonic flow; spike-nosed body; time-accurate computations; Newton-like subiterations
Three-dimensional supersonic flow over a spike-nosed body of revolution
A. Morgenstern Jr.I
CTA-IAE/ASE Praça Marechal Eduardo Gomes 50 Jardim das Acácias 12228-904 São José dos Campos, SP. Brazil firstname.lastname@example.org
The unsteady, viscous, supersonic flow over a spike-nosed body of revolution is numerically investigated by solving the Navier-Stokes equations. The time-accurate computations are performed employing an implicit algorithm based on the second-order time-accurate LU-SGS scheme with the incorporation of a subiteration procedure to maintain time accuracy. The characteristics of the flow field for a Mach number of 3.0, Reynolds number of 7.87 x 106/m, and angles of attack of 5 and 10 degrees are described. Self-sustained asymmetric shock wave oscillations were observed in the numerical computations for these angles of attack. The main characteristic of the flow field, as well as its influence on drag coefficient is discussed.
Keywords: Unsteady flow, supersonic flow, spike-nosed body, time-accurate computations, Newton-like subiterations
Spikes ahead of the blunt nose of bodies of revolution have been investigated as a means of drag reduction and heat flux attenuation by a number of investigators. Crawford (1959) experimentally investigated the effects of spike-nosed blunt bodies on heat flux and pressure drag for a Mach number of 6.8 and a wide range of Reynolds numbers. In this work it was assessed the effects of varying spike length on pressure drag and heat transfer, which indicated the strong influence of Reynolds number on heat transfer and spike length on drag reduction. The experimental investigations of Bogdonoff and Irwin (1959) indicated that the shock-wave configuration in front of spike-tipped axisymmetric bodies in high-speed flows could be unstable. This instability arises primarily in cases where the forebody geometry has a forward-facing step. Later on, Demetriades and Hopkins (1977) conducted experiments at supersonic speeds for an axisymmetric spike geometry. In this work it was reported observations which implied a more complex shock motion than that previously imagined; the shock motion was thought limited to one degree of freedom in the radial direction; shock expanding-collapsing symmetrically about the body axis. It was suggested that one more degree of freedom exist. The shock oscillations would rotate about the spike. A more recent experimental investigation performed by Calarese and Hankey (1985) revealed the unstable shock structure as consisting of a strong detached bow shock at the spike's tip which then collapses into a conical shock that intersects a quasi normal shock near the body's shoulder. It was also given evidence that the shock oscillates axially in a symmetric fashion with respect to the spike as well as in an asymmetric fashion for certain configurations and flow conditions. This phenomenon is highly unstable, and the necessary conditions for it to occur are the presence of a shear layer with an inflection point in the velocity profile, a reflecting surface, and the appropriate spike length to permit in phase reflections of pressure waves. If these conditions are met, highly organized oscillations of the impinging flow are sustained by feedback of upstream pressure propagation through the subsonic separated region to the shear layer origin, and by amplification of the disturbances until a limit cycle is reached.
Numerical solutions for flows over spike-nosed bodies can be found as late as the beginning of last decade. Shang, et. al. (1980), investigated the longitudinal mode of oscillations, the pressure amplitude of the disturbance as well as the shear layer and shock wave systems. Shoemaker (1990) performed a numerical investigation of an optimal spike-nosed configuration to minimize drag at a design Mach number of 2.5. Mikhail (1991 and 1996) investigated the flow over projectiles with a spike-nosed configuration and tripping rings.
In all of these investigations, however, the flow around spike-nosed bodies was studied only for zero angle of attack. More recently, Yamauchi, et. al., (1995) computed numerically the flow around a spiked blunt body for angles of attack larger than zero. The geometry considered in these studies resulted in steady flows. Although these efforts succeeded in simulate this complex flow, the characteristics of the unsteady flow for angles of attack larger than zero has not been discussed.
In the present paper, supersonic flows over a spike-nosed body are numerically simulated to study the effects of varying angle of attack for an originally unsteady flow field at zero angle of attack. It is not assumed any symmetry of the flow field in order to capture any disturbance in the radial as well as axial directions.
A,^=inviscid Jacobian matrix in x direction
B,^= inviscid Jacobian matrix in h direction
C,^= inviscid Jacobian matrix in z direction
CD = drag coefficient
cfx = axial force coefficient
cfy = lateral force coefficient
cfz = normal force coefficient
D = central second order accurate finite difference operator
F,^= inviscid flux vector in x direction
F,^V= viscous flux vector in x direction
G,^= inviscid flux vector in h direction
G,^V= viscous flux vector in h direction
H,^= inviscid flux vector in z direction
H,^V= viscous flux vector in z direction
PSD = power spectral density
p = pressure
Q,^= vector of conservative variables
R = radius
t = time
n = time index
a = angle of attack
q = circular angle
x, h, z = contravariant generalized coordinates.
¥ = free stream condition
Problem Definition and Solution Approach
The geometry of the configuration used in the present study is shown in Fig. 1. It was used the same spike-nosed body configuration that Calarese and Hankey (1985) employed in their experiments. The model is an axisymmetric cone frustum with a 9º cone angle.
Freestream Mach number is 3.0, Reynolds is 7.87 x 106/m, and the flow is assumed to be laminar. This assumption was made since the characteristic length scales are limited to 38.1 mm. The Reynolds number based on the running length is 2.998 x 105 which ensures that the flow is initially laminar. The flow conditions were selected to enable the comparison of the numerical results with experimental data in axisymmetric flows. Although, for this geometry and flow conditions Calarese and Hankey (1985) did not report asymmetries for zero angles of attack, in this numerical investigation a full three-dimensional flow was considered to allow any asymmetry to develop in the cases of angles of attack larger than zero.
The three-dimensional computational grid employed in this study is presented in Fig. 2. The number of grid points in the axial, circumferencial, and radial, directions are 121x37x81 respectively. The grid was constructed by rotating a 121x81 two-dimensional grid in 10 degrees intervals.
The compressible laminar flow over a spike-nosed body is governed by the Navier-Stokes equations, which are written in strong conservation law form in a generalized coordinate system of the form x =x (x,y,z,t), h =h (x,y,z,t), z =z (x,y,z,t).
The equations are solved using a time-accurate numerical method, which is based on the observation (Matsuno, 1989), that a d -form of the governing unsteady equations may be constructed with various combinations of the flux formulae and their Jacobians through the use of Newton-like sub-iterations. Furthermore a suitable choice of the factorization procedure yields a scheme with fast convergence and low computational time per iteration.
Equation (1) can be written in difference form as
where a second order accurate Euler three-point backward time discretization is used. The inviscid and viscous fluxes are linearized by
F,^n+1 = F,^n + A,^DQ,^n, F,^n+1,v = F,^n,v,
and the inviscid flux Jacobian matrix is defined as
similarly for G,^, G,^v, H,^, H,^v, B,^, and C,^.
A finite volume approach is used in the treatment of the spatial discretization of the fluxes. Second order central differences are used in the left hand side. A fourth order artificial dissipation model is added to the right hand side to control the undesired effects of odd and even point decoupling characteristic of central differences.
In the present algorithm, the lower-upper symmetric-Gauss-Seidel factorization scheme proposed by Yoon and Kwak (1992) is used. The advantage of this factorization is that the construction of the diagonal of the L and U matrices permits a scalar inversion, leading to a very efficient and vectorizable algorithm.
A detailed description of the algorithm implementation can be found in Morgenstern (1997).
Initial and Boundary Conditions
The initial flow field is set to be freestream everywhere. All variables are extrapolated at the outflow boundary and nonslip wall condition is applied on the surface of the body. Isothermal wall condition is imposed with wall temperature of 311 K.
Results and Discussion
The fully three-dimensional axisymmetric flow at zero angle of attack was computed to compare the results with data obtained by the experimental investigation of Calarese and Hankey (1985), and numerically computed results of Morgenstern (1997). The latter were obtained employing an axisymmetric formulation. Fig. 3 shows the comparison of the spectral estimate of a pressure time history data sample collected at a radius of 24.13 mm on the frustum face as indicated in Fig. 1. The primary mode associated with axial shock oscillations has a fundamental frequency of about 2800 Hz. The computed results captured all nine frequencies with very good accuracy when compared with the experiments. The experimental observation of an oscillation wave being modulated with another wave of about half the frequency was also present in the computed results. The comparison between the numerical results also showed good agreement, confirming the experimental evidence that for this geometry and flow condition the flow is axisymmetric.
Effects of Angle of Attack
The main characteristics of the flow over a spike-nosed body at an angle of attack larger than zero is described in Figures 4a-c . Velocity vectors and density contour plots are shown for a given instant in time at a = 10º in three streamwise planes corresponding to q = 0, 90, and 180 degrees, respectively. In Fig. 4a, corresponding to the leeward side, q = 0º , the oblique bow shock wave from the nose of the spike interacts with the reattachment shock wave from the frustum corner above the body. At this instant in time the shear layer passes over the frustum face providing relieve in pressure within the separated region over the spike. A large separated region is observed in front of the frustum. Fig. 4b shows the lateral position, corresponding to q = 90º . At this position the conical bow shock wave interacts with a quasi-normal reflected shock wave from the frustum face. This quasi-normal shock wave is originated due to the collapse of the separated shear layer into the frustum face at the reattachment point, which then pumps high pressure flow upstream. The reattachment point of the separated shear layer occurs close to the frustum corner. The separated region over the spike displays a more complex flow structure with secondary separations, vortical structures, and shock waves. Fig. 4c shows the windward position, corresponding to q = 180º . The same flow structure foundfor the q = 90º plane can be observed. The shear layer impinges on the frustum face at a steeper angle resulting in stronger reflected shock waves. The cross flow over the spike can be seen in Fig. 5. Velocity vectors around the spike present an asymmetric vortex shedding pattern. This vortex shedding, originated at the secondary separation on the spike, causes a sudden burst of pressure on one side of the spike, being responsible for asymmetric disturbances on the shock structure. Fig. 6 shows the instantaneous pressure distribution on the 90 and 270 degrees planes, illustrating this asymmetry.
Unsteadiness of the Flow
The flow over the spike-nosed body at 5 degrees angle of attack is described by a sequence of instantaneous plots shown in Fig. 7 over one cycle of shock oscillation. Figure 7a show the flow field velocity vectors and density contours on the spike surface, and 7b show flow field and spike surface density contours. At time t1 the shock structure starts to move upstream driven by a reflected shock wave from the frustum face. It continues its movement upstream at time t2 until the shear layer escapes from the frustum face edge. This causes a pressure relieving effect that triggers the downstream motion of the shock structure, time t3, that continues until time t4, when the shock structure interacts again with the frustum face, closing the cycle. This cycle is repeated in a periodic way. For zero angle of attack this oscillation cycle occurs in an axisymmetric fashion. For angles of attack different than zero the flow in the leeward and windward positions display a non-symmetric character as can be seen in figures 7a and 7b. Moreover, as observed in the previous section, Fig. 6, an oscillation wave in the lateral direction is generated by the asymmetric pressure distribution on the sides of the spike. The integrated forces in the axial, x, lateral, y, and normal, z, directions over one cycle of oscillation are shown in Figure 8. The oscillatory behavior of the flow field can be clearly observed. It is also shown that although the magnitude of the force increases with increasing angle of attack, the amplitude of the oscillations decreases with increasing angle of attack. The lateral force coefficient, cfy, also shows oscillations, however at a much smaller amplitude.
Power spectral estimate of the pressure time history at the leeward and windward positions on the frustum face for the a = 5º flow is shown in figure 9. In the windward plane all nine modes of oscillations found in the axisymmetric case are present. However, in the leeward plane only the first mode, the primary mode associated with the axial shock oscillations, is in agreement. The other modes of oscillation are shifted or not present. This is attributed to the vortex shedding from the sides of the spike that interfere with the shock oscillations on the leeward side of the spike.
Drag coefficients for the angles of attack considered were computed from the averaged flow fields. These computations include both pressure and viscous contributions. However, the contribution from the base region is not included, i.e., the pressure in the base region is assumed to have the freestream value when computing the drag coefficient. As seen in Table 1 the drag coefficient increases with increasing angle of attack. However it is worth noting that from zero to 5 degrees angle of attack the drag coefficient is increased by 8% and from 5 to 10 degrees angle of attack it is increased by 3.7%. This reduction in the increase of the drag coefficient with increasing angle of attack is attributed to the lesser interaction of the shock wave oscillations with the leeward face of the frustum. With a larger angle of attack the conical bow shock wave reattaches very close to the frustum corner, allowing the separated shear layer to escape sooner, and as a consequence, providing a less severe pressure environment in the leeward side.
Supersonic flows at an angle of attack larger than zero over a spike-nosed body was numerically simulated. The flowfields for angles of attack of 5 and 10 degrees are characterized by a conical shock wave, a separated region in front of the body, and the interaction of the bow shock wave with reflected and reattachment shock waves. The separated region in front of the body is larger in the leeward side and the pressure environment is more severe in the windward side. The asymmetric shock wave structure is evident. Nevertheless, the principal mode of oscillation remains unaltered in both sides. The higher mode of oscillations in the leeward side is shifted or not present when compared with the mode of oscillations in windward side or the axisymmetric flow.
Integrated forces showed large amplitudes of oscillation in the axial and normal directions. In the lateral direction small amplitude oscillations were observed due to the break down of vortices induced by the cross flow on the sides of the spike surface. The drag coefficient increased with increasing angle of attack. However, the rate of increase reduced as the angle of attack increased.
A good agreement is obtained between the present computation and the available experimental data for the axisymmetric flow.
The Centro Nacional de Supercomputação - UFRGS provided time on the Cray Y-MP computer. The author gratefully acknowledges this support.
Article received August, 2001
Technical Editor: Atila P. Silva Freire
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