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Technical Report 2015-05
DNS Study on Motion around a Vortex Ring in Transitional
Boundary Layers
Yiqian Wang Shuhyi Chern Chaoqun Liu
American Institute of Aeronautics and Astronautics
1
DNS Study on Motion around a Vortex Ring
in Transitional Boundary Layers
Yiqian Wang1, Shuhyi Chern
2, Chaoqun Liu
3
University of Texas at Arlington, Arlington, Texas 76019
Vortex rings are common in turbulent flows of liquids and gases. Therefore, considerable
attention has been paid to investigate their movement and deformation. However, researches
on the motion around vortex rings, especially in turbulent boundary layer, are relatively
rare. In this paper, the motion around a vortex ring in turbulent boundary layers is carefully
examined using the DNS results of a flat-plate boundary layer. Velocities, vorticities, vortex
filaments and pressure distribution are illustrated with iso-surfaces of λ2 representing the
vortices and vortex filaments. The toroidal motion of the vortices is also studied to show how
quick the vortex rotation is. It is found that there is substantial discrepancy between the
DNS results and time-averaged mathematical modeling like RANS or regular experiments
for the transitional boundary layer flow. The emphasis is put on these differences and some
distinguished characteristics of vortex rings in turbulent boundary layers.
Key words: Vortex ring, rotation, Boundary Layer, Transition
Nomenclature
∞M = Mach number Re = Reynolds number
inδ = inflow displacement thickness wT = wall temperature
∞T = free stream temperature inLz = height at inflow boundary
outLz = height at outflow boundary
Lx = length of computational domain along x direction
Ly = length of computational domain along y direction
inx = distance between leading edge of flat plate and upstream boundary of computational domain
dA2 = amplitude of 2D inlet disturbance
dA3 = amplitude of 3D inlet disturbance
ω = frequency of inlet disturbance
2 3d d,α α = two and three dimensional streamwise wave number of inlet disturbance
β = spanwise wave number of inlet disturbance R = ideal gas constant
γ = ratio of specific heats ∞µ = viscosity
x, y, z – stremwise, spanwise, normal directions
I. Introduction
y definition, a vortex ring refers to a region in which fluid spins around a closed axis loop. Vortex rings are
frequently seen as smoke rings (Figure 1), fiery vortex rings and in firing of certain artillery, in mushroom
clouds and in microbursts. Because of the plentiful appearance, vortex rings are studied both experimentally and
mathematically. One of the earliest mathematical models for vortex rings is Hill’s spherical vortex (1894), in which
an axisymmetric and uniform vorticity vortex region was achieved. On the other hand, generating and visualizing
vortex rings using dye and hydrogen bubbles experimentally are not a very sophisticated task. Therefore, ring
1 Visiting PhD student from Nanjing University of Aeronautics and Astronautics.
2 Adjunct Professor, Department of Math, P.O. Box 19408, AIAA Associate Fellow.
3 Professor, Department of Math, P.O. Box 19408, AIAA Associate Fellow.
B
American Institute of Aeronautics and Astronautics
2
velocity, growth rate and vorticity distribution were extensively investigated (Maxworthy 1972). More models
(Lamb 1945; Saffman 1970) were developed thereafter based on these characteristics.
Figure 1: Smoke ring from a smoke chamber (Traitor 2006)
It is not until the arrival of high computational capacity and advanced experimental methods, such as 3-D PIV,
that make researchers able to study the instantaneous vortical structures in boundary layer flows. It is found that
many ring-like vortices exist in boundary layer and believed to play a significant role in turbulence generation and
sustenance. These vortex rings differ from the axisymmetric rings in many ways. For example, the axis loop is not
closed and generally the velocity is slower near the wall and higher away from the wall. However, a surprising fact
is that the highest velocity locates near the “neck” rather than the top around some vortex rings (Figure 2).
Figure 2: A typical ring-like vortex in boundary layer flows
These vortex rings, as part of the so called “hairpin vortices”, play significant role in turbulence generation and
sustenance in turbulent boundary layers. Therefore, in pursue of knowledge about the more physically meaningful
ring-like vortices, a high order direct numerical simulation (DNS) was performed including 1920×241×128 grid
points along streamwise spanwise and normal wise direction respectively over 600, 000 time steps at a free Mach
number of 0.5 (Chen et al., 2010a, 2010b; Liu et al., 2012, 2014; Lu et al., 2011a, 2011b; Yan et al., 2014; Wang et
al, 2015) which is a continuation of our early work (Liu et al, 1995, 1998.) The purpose of this study is to study the
unique characteristics of vortex rings in turbulent boundary layers and reveal why the maximum velocity is located
around the neck region. Moreover, how does the maximum velocity reach 1.06 faster than 1 (in non-dimensional
sense) when the incoming velocity is 1?
American Institute of Aeronautics and Astronautics
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II. Case Setup and Code Validation
2.1 Case setup The computational domain is shown in Figure 3(a). The grid includes 1920×128×241 points in streamwise (x),
spanwise (y), and wall normal (z) directions respectively. A uniform grid is employed in both streamwise and
spanwise directions, while a stretching grid is used in normal direction. The first grid interval is carefully chosen to
make sure the grid is fine enough to capture all the small scales. The Message Passing Interface (MPI) plus the
streamwise direction domain decomposition which is shown in Figure 3(b) is utilized for parallel computation. The
flow conditions, including Reynolds number, Mach number, etc. are listed in Table 1. Lx and Ly are the lengths of
the computational domain in streamwise and spanwise directions, while Lzin is the height of the computational
domain at the inlet. xin is the distance between inlet and the leading edge of the flat plate and Tw represents the wall
temperature.
Table 1: Flow parameters
∞M 1000Re = 300 79in inx .= δ 798 03Lx .= δ 22in
Ly = δ 40in in
Lz = δ 273 15w
T . K= 273 15T .∞ =
0.5 1000 300.79 inδ 798.03 inδ 22 inδ 40 inδ 273.15K 273.15K
(a)
(b)
Figure 3. (a) Computational domain (b) Domain decomposition along the streamwise direction
2.2 Code Validation The code “DNSUTA” was developed at the University of Texas at Arlington and carefully validated by NASA
Langley and UTA researchers (Jiang et al., 2003; Liu et al., 2010b, Lu et al., 2011). The results have been compared
to experiments (Lee C B & Li R Q, 2007) and other’s DNS results (Rist et al., 2002), and the consistence shows our
results are correct and accurate. Since the detailed validation has been reported, only a brief describtion will be
given here.
2.2.1 Comparison with Log Law and grid convergence Time and spanwise-averaged streamwise velocity profiles for various streamwise locations in two different grid
levels are shown in Fig. 4. The inflow velocity profiles at x=300.79δin is a typical laminar flow velocity profile. At
x=632.33δin, the mean velocity profile approaches a turbulent flow velocity profile (Log law). This comparison
shows that the velocity profile from the DNS results is turbulent flow velocity profile and the grid convergence has
been realized.
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(a) Coarse Grids (960x64x121) (b) Fine Grids (1920x128x241)
Figure 4. Log-linear plots of the time-and spanwise-averaged velocity profile in wall unit
2.2.2 Comparison with Experiment
By using λ2-eigenvalue visualization method, the vortex structures shaped by the nonlinear evolution of T-S
waves in the transition process are shown in Fig. 5. The evolution details are studied in our previous paper (Liu et al)
and the formation of ring-like vortices chains is consistent with the experimental work (Lee C B & Li R Q, 2007,
Fig. 6) .
Figure 5. Evolution of vortex structure at the late-stage of transition (Where T is the period of T-S wave)
z+
U+
100
101
102
103
0
10
20
30
40
50
x=300.79
x=632.33
Linear Law
Log Law
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5
Figure 6. Evolution of the ring-like vortex chain
by experiment (Lee et al, 2007)
2.2.3 Comparison with Rist’s DNS data Fig. 7 shows a comparison of our DNS results with the data set provided by Rist as his personal kindness. The
comparison shows both DNS have same vortex structure. All these verifications and validations above show that our
code is correct and our DNS results are reliable.
(a) Our DNS (b) Rist’s DNS data
Figure 7. Comparison of our DNS results with Rist’s DNS data including vortex filaments and 2λ
All these verifications and validations above show that our code is correct and our DNS results are reliable.
III. DNS observation on vortex rings in boundary layer 1. The shape of vortex rings in boundary layer differs from axisymmetric vortex rings
The vortex rings in boundary layer has an open axis loop. Accordingly, the vortex filaments passing
through the vortex ring is not closed and originate from side boundaries as shown in Fig. 8. This unique
shape might be a decisive factor in the role vortex rings play in a boundary layer flow.
American Institute of Aeronautics and Astronautics
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Figure 8. The shape of a vortex ring and its vortex filaments in boundary layers
2. Maximum velocity around some vortex rings in boundary layer flows locates near the “neck”.
The ring-like vortex rings are assumed to play a significant role in turbulence generation and sustenance
as to bring high speed flow from inviscid area to the bottom. However, this effect cannot create region near
the bottom of velocity higher than 1 (non-dimensional velocity) as shown in Fig. 2 by itself. It is a key
issue in this paper that how this extremely high speed region near the neck region is generated and what its
role in transition from laminar to turbulence is.
Figure 9 shows iso-surfaces of streamwise velocity u=1.005 with vortical structures. It is shown that the
T-S wave enforced at the inlet do induce velocity larger than 1. However, the maximum velocity at the inlet
around 1.005, the deviation is one order smaller than the maximum velocity increment we found around the
neck of a vortex ring. Therefore, the maximum velocity we are interested in cannot only due to the
disturbance at the inlet.
Figure 9. Vortical structures represented by iso-surfaces of λ2 and iso-surfaces of streamwise velocity
u=1.005
3. The larger than 1 high speed region comes into sight when the vortex ring becomes perpendicular.
American Institute of Aeronautics and Astronautics
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The maximum streamwise velocity around ring-like vortices is not always around the neck region unless
the vortex rings become perpendicular enough. Fig. 10 shows three consecutive vortex rings and their
streamwise velocity distribution. The second ring-like vortex is identified as the same one shown in Fig. 2
and Fig.8 at earlier time steps. Fig. 10(c) shows the maximum streamwise velocity of this vortex ring is at
top of it which differs from its later configuration in Fig. 2. However, the first vortex ring in Fig. 10(a) is
more perpendicular with maximum velocity around the neck region shown in Fig. 10(b). For the third
vortex ring, which is oblique more obviously, the maximum velocity also locates at the top as illustrated in
Fig. 10(d).
Fig. 11 shows the iso-surface of streamwise velocity u=1.045. It can be found that the maximum velocity
around some vortex rings locates around the neck region while the maxima around some rings are on the
top. Fig. 11 also verified the assumption that, when the ring is more perpendicular, the maxima tend to
locate at the neck region rather than on the top. Note that, for the rings in Fig. 11 with iso-surface of
streamwise velocity cover both the top and neck region, we cannot accurately determine where the
maximum velocity is just by this figure.
Figure 10. Three consecutive vortex rings and their streamwise velocity distribution
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Figure 11. Iso-surface of streamwise velocity u=1.045
4. The rotation speed of the ring vortex at different cross-section will be checked.
Form Fig. 9(c) and (d), we can see that even when the maximum velocity locates at the top of vortex ring,
the maximum streamwise velocity reaches 1.05, or even 1.06. This maximum speed is higher than the
incoming velocity, and cannot be caused by inflow disturbance since the disturbance is much smaller. The
vortex is defined as a region with rotating movement. So the rotation speed of the vortex rings is going to
be examined and their relationship with the high speed generation will be investigated.
5. The role of vortex rings in turbulent boundary layer.
The ring-like vortices are clear very important in turbulence generation and sustenance. However, the
movements around these rings are much more complicated than the axisymmetric ones. It is very important
to gain a better knowledge of these vortex rings in boundary layer.
III Conclusions and discussions
It has been noticed that the hairpin vortices, consisting of vortex rings and two quasi-streamwise vortices play
a significant role in turbulence generation and sustenance. Ejections and sweeps of hairpins are assumed to be very
important. Sweeps are believed to bring high speed flow from inviscid area (velocity around 1) to form high speed
region in the bottom of boundary layer. However, it is found the high speed region can has a velocity higher than 1
which cannot be just a result of high speed flow sweeps from the inviscid area. The flow around vortex rings in
boundary layer will be checked carefully to explore the reason why the high speed zone which is larger than 1
appears near the boundary layer bottom. The rotation of the vortex ring at multiple cross-sections will be examined
since it might contribute to high speed zone generation near the bottom of the boundary layer. The full analysis
will be given in the final paper.
Acknowledgments The work was supported by Department of Mathematics at University of Texas at Arlington. The authors are
grateful to Texas Advanced Computing Center (TACC) for the computation hours provided. This work is
accomplished by using Code DNSUTA released by Dr. Chaoqun Liu at University of Texas at Arlington in 2009.
Y. Wang also would like to acknowledge the Chinese Scholarship Council (CSC) for financial support.
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