UFR 3-35 Evaluation

Cylinder-wall junction flow

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Evaluation

The evaluation of the numerical and experimental data sets in the symmetry plane upstream a wall-mounted cylinder refers to the time-averaged flow fields indicated by:

• the streamlines
• the location of the characteristic flow structures
• selected vertical and horizontal profiles of the velocity components $\langle u(z)\rangle$ and $\langle w(x)\rangle$ as well as the Reynolds sresses $\langle u'_{i}u'_{j}\rangle$ and the trubulent kinetic energy $\langle k(z)\rangle$
• the distribution of the turbulent kinetic energy and its buget terms such as production, transport, and dissipation
• horizontal profiles of the pressure coefficient $c_{\mathrm {p} }(x)$, and the friction coefficient $c_{\mathrm {f} }(x)$

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Streamlines

The streamlines of the PIV and the LES data show high similarity and agree well with each other. The plots are flooded with the normalized magnitude of the velocity field in the symmetry plane, thus $||{\vec {U}}||={\sqrt {\langle u^{2}\rangle +\langle w^{2}\rangle }}/u_{\mathrm {b} }$. The approaching turbulent boundary layer is redirected downwards at the flow facing edge of the cylinder caused by a vertical pressure gradient. This downflow reaches the bottom plate of the flume at the stagnation point S3. Here, it becomes redirected (i) in the out-of-plane direction bending around the cylinder; (ii) towards the cylinder rolling up and forming the corner vortex V3; and (iii) in the upstream direction accelerating and fomring a wall-parallel jet. Due to the strong acceleration of the jet, a high vertical velocity gradient is exerted onto the bottom plate, which induces high wall shear stress. Parts of the approaching boundary layer is dragged downwards forming the horseshoe vortex V1. Upstream of thsi vortex system, the approaching flow is blocked and recirculates, and as a consequence a saddle point S1 with zero velocity magnitude appears.

Streamlines of time-averaged flow field flooded with the in-plane velocity magnitude $||{\vec {U}}_{\mathrm {PIV} }||={\sqrt {\langle u^{2}\rangle +\langle w^{2}\rangle }}/u_{\mathrm {b} }$

Streamlines of time-averaged flow field flooded with the in-plane velocity magnitude $||{\vec {U}}_{\mathrm {LES} }||={\sqrt {\langle u^{2}\rangle +\langle w^{2}\rangle }}/u_{\mathrm {b} }$

Location of the characteristic flow structures

The position of the characteristic flow structures highlited in the streamline plots is listed in the following table

Position of flow structures

	PIV		LES
	$x/D$	$z/D$	$x/D$	$z/D$
S1	$-0.788$	$0.03$	$-0.843$	$0.037$
S2	$-0.918$	$0$	$-1.1$	$0$
S3	$-0.533$	$0$	$-0.534$	$0$
S4	$-0.507$	$0.036$	$-0.50$	$0.04$
V1	$-0.697$	$0.051$	$-0.735$	$0.06$
V3	$-0.513$	$0.017$	$-0.513$	$0.02$

Horizontal and vertical profiles of the velocity components and Reynolds stresses

The vertical profiles are extracted at the following positions with respect to the time-averaged position of the horseshoe vortex, and can be found in the following plot.

Since the flow structure of the LES and the PIV is slightly different, we use an adjusted $x-$ coordinate, in order to compare the data at the same position in the flow. The coordinate is defined as follows:

$x_{\mathrm {adj} }={\frac {x-x_{\mathrm {Cyl} }}{x_{\mathrm {Cyl} }-x_{\mathrm {V1} }}}$,

with $x_{\mathrm {Cyl} }=-0.5D$, such that $x_{\mathrm {adj} }=-1.0$ represents the time-averaged location of the horseshoe vortex centre $x_{\mathrm {V1} }$.

Vertical profiles of the streamwise velocity component $\langle u(z)\rangle /u_{\mathrm {b} }$

The vertical velcoity profiles $u(z)$ are presented at the seleted locations. When the downflow is deflected at the bottom plate at $S3$, the wall-parallel jet starts to develop, and consequently, the flow accelerates. At $x_{\mathrm {adj} }=-0.25$, a near-wall velocity peak appears, which becomes more pronounced in the upstream direction (see $x_{\mathrm {adj} }=-0.5$). In this region, the wall shear stress reaches on one hand its maximum value and on the other hand reveals a plateau-like shape. This means that the largest values of the gradient ${\frac {\partial \langle u\rangle }{\partial z}}$ appear. Underneath the horseshoe vortex, the flow decelerates and the wall-peak of the velocity lifts from the bottom plate and becomes less distinct. Further upstream, the near-wall peak of the streamwise velocity disappears and therefore, the wall-parallel jet fades out. Due to the evaluation of the PIV images by an interrogation window based cross correlation, the strong gradient ${\frac {\partial \langle u\rangle }{\partial z}}$ at the wall cannot be fully resolved, and therefore, the near-wall peak of the streamwise velocity is damped in the experimental data.

Vertical profiles of the Reynolds stresses $\langle u_{i}'u_{j}'(z)\rangle /u_{\mathrm {b} }^{2}$ and the turbulent kinetic energy $\langle k(z)\rangle =0.5(\langle u'^{2}\rangle +\langle w'^{2}\rangle )/u_{\mathrm {b} }^{2}$

The vertical profiles of the Reynolds stresses and the resulting turbulent kinetic eneryg is presented only at $x_{\mathrm {adj} }=-1.5$, $x_{\mathrm {adj} }=-1.0$, and $x_{\mathrm {adj} }=-0.5$. The accelerating jet is again indicated by a near wall peak of the $\langle u'u'\rangle$ stress, while the horseshoe vortex leaves its footprint in the stresses $\langle u'u'\rangle$ and $\langle w'w'\rangle$ as (local) peak at $z_{\mathrm {V1} }/D$. The shear stress distribution $\langle u'w'\rangle$ inside the wall-paralle jet is negative (in average) according to the flow direction (in average). The experimental and numerical data agree with each other both in amplitude as well as in shape. Again, the quality of the PIV data near the wall is underminded by the strong gradients being evaluated using interrogation windows.

[[File:UFR3-35_W_x_V1.png|centre|frame|Horizontal profiles of the vertical velocity component $\langle w(x)\rangle /u_{\mathrm {b} }$ at the height $]]Analysingtheprofileoftheverticalvelocitycomponent<math>\langle w(x)\rangle$ along the $x-$ axis at the height of the horseshoe vortex, reveals on the one hand the clockwise rotation of the vortex, and on the other hand two minima between the horseshoe vortex and the cylinder. At $x_{\mathrm {adj} }\approx -0.1$, the peak in the downwards directed flow stems from the downflow, while the second local minimum at approximately $x_{\mathrm {adj} }=-0.65$ represents the downwards rotation of the horseshoe vortex. Both data agree well in shape. However, the LES data indicate higher amplitudes in general.

[[File:UFR3-35_uiuj_x_V1.png|centre|frame|Horizontal profiles of the Reynolds stresses $\langle u_{i}'u_{j}'(x)\rangle /u_{\mathrm {b} }^{2}$ and the turbulent kinetic energy $\langle k(x)\rangle =0.5(\langle u'^{2}\rangle +\langle w'^{2}\rangle )/u_{\mathrm {b} }^{2}$ at the height $]]TheReynoldsstresses<math>\langle u_{i}'u_{j}'\rangle$ and the turbulent kinetic energy $\langle k\rangle$ at the height of the horseshoe vortex show similar distributions. At the centre of the vortex, the normal stresses, and consequently the turbulent kinetic energy as well, reveal a peak, which wears off in the up- and downstream direction. In addition, the downflow close to the cylinder surface generates stresses as well. The shear sresses play a minor role in the region between the cylinder and the horseshoe vortex, while they become negative upstream of the horseshoe vortex indicating the interference of the approaching flow wiht the horseshoe vortex.

Distribution of turbulent kinetic energy and its budgets terms: Production, Transport, Dissipation and Convection

Turbulent kinetic energy

Turbulent kinetic energy $\langle k_{\mathrm {PIV} }\rangle =0.5(\langle u'^{2}\rangle +\langle w'^{2}\rangle )/u_{\mathrm {b} }^{2}$

Turbulent kinetic energy $\langle k_{\mathrm {LES} }\rangle =0.5(\langle u'^{2}\rangle +\langle w'^{2}\rangle )/u_{\mathrm {b} }^{2}$

The spatial distribution of the time-averaged in-plane turbulent kinetic energy $\langle k_{\mathrm {PIV} }\rangle =0.5(\langle u'^{2}\rangle +\langle w'^{2}\rangle )/u_{\mathrm {b} }^{2}$ reveals on the one hand the well-known c-shaped structure (e.g. Paik 2007) with the largest amplitude at the centre of the horseshoe vortex stemming from vertical fluctuations induced by the horizontal oscillations of the horseshoe vortex. The lower branch of the c-shape contains mainly streamwise (horizontal) fluctuations linked to the dynamics of the wall-parallel jet. On the other hand, the experimental and numerical data sets show high similarity and agree well with each other, as the peak amplitude is approximately the same: $\langle k_{\mathrm {PIV} }\rangle =0.074u_{\mathrm {b} }^{2}$; $\langle k_{\mathrm {LES} }\rangle =0.079u_{\mathrm {b} }^{2}$. The black circle marks the centre of the horseshoe vortex.

The budget equation of the turbulent kinetic energy is the balancing sum of the convection $C$, the transport term $\nabla T$ (diffusion), the production $P$, and the dissipation $\epsilon$:

$0=P+\nabla T-\epsilon$ + C,

while $P=-\langle u_{i}'u_{j}'\rangle {\frac {\partial \langle u_{i}\rangle }{\partial x_{j}}}$,

$T=\underbrace {-{\frac {1}{2}}\langle u_{i}'u_{j}'u_{j}'\rangle } _{\text{turbulent fluctuations}}\underbrace {-{\frac {1}{\rho }}\langle u_{i}'p'\rangle } _{\text{pressure transport}}\underbrace {+2\nu \langle u_{j}'s_{ij}\rangle } _{\text{viscous diffusion}}$,

$\epsilon =2\nu \langle s_{ij}s_{ij}\rangle$, and $s_{ij}={\frac {1}{2}}\left({\frac {\partial u_{i}'}{\partial x_{j}}}+{\frac {\partial u_{j}'}{\partial x_{i}}}\right)$ as the fluctuating rate-of-strain tensor,

and $C=-{\frac {\partial k}{\partial t}}-\langle u_{i}\rangle {\frac {\partial k}{\partial x_{i}}}$.

The individual terms of the budget equation of the TKE are normalized by $D/u_{\mathrm {b} }^{3}$ and presented in the following part:

Production of turbulent kinetic energy

Production of turbulent kinetic energy $P_{\mathrm {PIV} }=-\langle u_{i}'u_{j}'\rangle {\frac {\partial \langle u_{i}\rangle }{\partial x_{j}}}\cdot D/u_{\mathrm {b} }^{3}$

Production of turbulent kinetic energy $P_{\mathrm {LES} }=-\langle u_{i}'u_{j}'\rangle {\frac {\partial \langle u_{i}\rangle }{\partial x_{j}}}\cdot D/u_{\mathrm {b} }^{3}$

The main region of positive production of turbulent kinetic energy can be found upstream of the centre of the hoseshoe vortex (black circle) and underneath inside the wall-parallel jet. The amplitude of both data sets is about $0.3u_{\mathrm {b} }^{3}/D$ in the region of the horseshoe vortex, while the LES data resolve the TKE production in the jet in more detail than the PIV data. The amplitudes here are $P_{\mathrm {LES} }\approx 0.4u_{\mathrm {b} }^{3}/D$ and $P_{\mathrm {PIV} }\approx 0.2u_{\mathrm {b} }^{3}/D$. The oscillations of the horsesoe vortex are responsible for causing fluctuations, which in turn produce turbulent kinetic energy.

From the stagnation point S3 onwards in the upstream direction, the TKE production is negative, meaning that inside the accelerating jet TKE is transferred into mean kinetic energy. When the jet decelerates at about $x=-0.7D$, the jet becomes more unstable, fluctuations occur, and therefore, $P$ becomes positive.

Transport of turbulent kinetic energy

The transport of TKE can be split up into three individual terms: the transport due to turbulent fluctuations, due to pressure fluctuations, and due to viscous diffusion. Since the pressure in general is not contained in the PIV data, the velocity-pressure correlations, which are required to obtain the transport due to pressure, cannot be calculated, as well. Therefore, we present the three terms individually and the latter for the LES alone.

Transport of turbulent kinetic energy due to turbulent fluctuations $\nabla T_{\mathrm {turb,PIV} }=-{\frac {1}{2}}{\frac {\partial \langle u_{i}'u_{j}'u_{j}'\rangle }{\partial x_{i}}}\cdot D/u_{\mathrm {b} }^{3}$

Transport of turbulent kinetic energy due to turbulent fluctuations $\nabla T_{\mathrm {turb,LES} }=-{\frac {1}{2}}{\frac {\partial \langle u_{i}'u_{j}'u_{j}'\rangle }{\partial x_{i}}}\cdot D/u_{\mathrm {b} }^{3}$

The distribution of the tubrulent transport shows a similar structure as the one of the production. The region of large positive TKE production, we observe a large negative transport. In particular close to the wall at $x=-0.75D$, the large production of $0.4u_{\mathrm {b} }^{3}/D$ is nealy balanced by the turbulent transport $T_{\mathrm {turb,LES} }\approx 0.35u_{\mathrm {b} }^{3}/D$. The positive transport indicates that TKE is transported towards these regions. Since they can be found above the centre of the horseshoe vortex, vertical eruptions from the wall , which coincide with the observations of Apsilidis et al. (2015).

Transport of turbulent kinetic energy due to pressure fluctuations $\nabla T_{\mathrm {press,LES} }=-{\frac {1}{\rho }}{\frac {\partial \langle u_{i}'p'\rangle }{\partial x_{i}}}\cdot D/u_{\mathrm {b} }^{3}$

Transport of turbulent kinetic energy due to viscous diffusion $\nabla T_{\mathrm {visc,LES} }=2\nu {\frac {\partial \langle u_{j}'s_{ij}\rangle }{\partial x_{i}}}\cdot D/u_{\mathrm {b} }^{3}$

The pressure fluctuations play an important role in the TKE transport. In some regions, the transport terms $\nabla T_{\mathrm {turb} }$ and $\nabla T_{\mathrm {press} }$ cancel each other while the horseshoe vortex oscillates in the horizontal direction. When the horseshoe vortex is shifted towards the cylinder, the instantaneous wall-normal component becomes zero and the corresponding fluctuation $w'>0$ as the mean value is negative in this region. Therefore, the turbulent transport becomes negative in total, and the transport due to pressure fluctuations become positve as $p'<0$ in the vortex centre (low pressure), resulting in a mutaul balance.

The transport of TKE due to viscous diffusion shows an increased negative transport only close to the wall, which is intuitive as viscous effects increase towards the wall. In the remaining part, however, the amplitude of $\nabla T_{\mathrm {visc} }$ is below $|0.05|u_{\mathrm {b} }^{3}/D$, and therefore, the contribution of this term to the TKE transport around the horseshoe vortex is of minor importance.

Dissipation of turbulent kinetic energy

The dissipation is the sink term in the budget of the TKE transport equation, as the TKE was produced and transported by $P$ and $\nabla T$, respectively, and is dissipated into heat by $\epsilon$. The dissipation is positive by definition, and therefore, it appears with a negive sign in the budget equation. In the LES data, the modelled dissipation due to subgird stresses is included and was quantified to be approximately one third of the total dissipation rate.

Dissipation of turbulent kinetic energy $\epsilon _{\mathrm {PIV} }=2\nu \langle s_{ij}s_{ij}\rangle \cdot D/u_{\mathrm {b} }^{3}$

Dissipation of turbulent kinetic energy $\epsilon _{\mathrm {LES} }=2\nu \langle s_{ij}s_{ij}\rangle \cdot D/u_{\mathrm {b} }^{3}$

The distribution of the dissipation shows a similar c-shaped structure as the TKE and the production term $P$ due to the horizontal oscillations of the vortex. Three regions with a high dissipation rate can be located: (i) around the centre of the horseshoe vortex; (ii) underneath the horseshoe vortex inside the wall-parallel jet; and (iii) at the corner vortex V3. The amplitude of the measured dissipation rate exceeds the one stemming from the LES data due to measurement noise undermining the quality of the instantaneous fluctuating velocity gradients. The spatial resolution of the PIV was anyway too coarse to estimate the dissipation correctly such that we did not apply any correction to the experimental data, and used the data as a qualitative comparison rather than a quantitative one. However, the dissipation rate and the production of the TKE do not cancel each other out as the maximum amplitude in the centre of the horseshoe vortex is $\epsilon _{\mathrm {LES} }=0.066u_{\mathrm {b} }^{3}/D$, which is approximately one third of the production here. Furthermore, the maximum value of the production is located upstream of the horseshoe vortex indicating the role of the transport of small-sclae structures between the location of $P_{\mathrm {max} }$ towards $\epsilon _{\mathrm {max} }$.

Convection of turbulent kinetic energy

Since we analyes a steady state flow, the spatial derivative becomes irrelevant and the mean convection reduces to $C_{\mathrm {PIV} }=-\langle u_{i}\rangle {\frac {\partial k}{\partial x_{i}}}$.

Mean convection of turbulent kinetic energy $C_{\mathrm {PIV} }=-\langle u_{i}\rangle {\frac {\partial k}{\partial x_{i}}}\cdot D/u_{\mathrm {b} }^{3}$

Mean convection of turbulent kinetic energy $C_{\mathrm {LES} }=-\langle u_{i}\rangle {\frac {\partial k}{\partial x_{i}}}\cdot D/u_{\mathrm {b} }^{3}$

The approaching flow separates from the bottom wall of the flume and, consequently, becomes unstable increasing TKE. Therefore, the mean convection is negative upstream of the horseshoe vortex as the TKE increases along the streamlines. The same applies for the wall-parallel jet. After the deflection at S3, the jet accelerates, which decreases TKE in the first place. When the jet starts to decelerate ($x\approx -0.63D$) the flow becomes more unstable and TKE increases. Underneath the horsehsoe vortex, $C$ changes sign again and the TKE decreases further upstream.

Budget of turbulent kinetic energy

Finally, the sum of the above mentioned terms is presented as the total budget of the TKE. Since, the PIV data cannot provide information concerning the pressure, the budget will not cancel out.

Residual of turbulent kinetic energy budget $R_{\mathrm {PIV} }=P+\nabla T-\epsilon$ + C \cdot D/u_{\mathrm{b}}^3 </math>

However, when analysing the distribution and amplitude of the residual of the TKE budget obtained from PIV, it appears that the structure is similar to the one of $-\nabla T_{\mathrm {press,LES} }$. Therefore, the missing piece in the experimental data of this flow configuration is the contribution of the pressure fluctuations to the transport mechanisms of the TKE.

Residual of turbulent kinetic energy budget $R_{\mathrm {PIV} }=P+\nabla T-\epsilon$ + C \cdot D/u_{\mathrm{b}}^3 </math>

The residual of the LES data is around zero in wide regions $<|0.01|u_{\mathrm {b} }^{3}/D$. Around the horseshoe vortex the residual is close to zero and no structure remains, which was not considered. Alone along the cylinder surface and the bottom wall the budget does not fully balance

Horizontal profiles of the pressure coefficient $c_{\mathrm {p} }(x)$, and of the friction coefficient $c_{\mathrm {f} }(x)$

The pressure coefficient $c_{\mathrm {p} }$ is computed as:

$c_{\mathrm {p} }={\frac {\langle p\rangle }{{\frac {\rho }{2}}u_{\mathrm {b} }^{2}}}$,

while the friction coefficient $c_{\mathrm {f} }$ is determined as:

$c_{\mathrm {f} }={\frac {\langle \tau _{\mathrm {w} }\rangle }{{\frac {\rho }{2}}u_{\mathrm {b} }^{2}}}$.

The following plots were taken from the LES data only since the pressure is not contained in the PIV data and the spatial resolution appeared to be too corase to calculate the wall shear stress, thus the friction coefficient, correctly. The first data point in the experimental data could be obtained at $z_{1}\approx 0.0036D\approx 10\mathrm {px}$. In the LES, the first grid point was at $z_{1}\approx 0.0005D$, which is about a factor of 7 finer than the experimental results. Additionally, a thinned streamline plot is given for the sake of better orientation in a qualitative sense showing the positions in the $z-$direction in which the profiles were extracted. The red symbols refer to the profiles near the wall indicated by the red solid line, whereas the blue symbols and the blue solid line refer to the profile at the height of the horseshoe vortex.

Pressure coefficient $c_{\mathrm {p} }$

Friction coefficient $c_{\mathrm {f} }$

At the stagnation point S3, the pressure coefficient reaches a maximum value of about $c_{\mathrm {p} }=1.08$ due to the downflow impinging at the bottom of the flume. The downflow is deflected in all directions forming an accelerating wall-parallel jet in particular in the uptream direction. The acceleration is indicated by the decrease of the pressure coefficient. At $x_{\mathrm {adj} }=-1.0$, underneath the horseshoe vortex, the pressure coefficient shows a kink and the rate of decreases is less significant than before.

The accelerating wall-parallel jet is also recognisable in the distribution of the friction ceofficient $c_{\mathrm {f} }$. From the stagnation point S3 on, with zero wall shear stress, the friction coefficient reveals a sharp peak underneath the foot vortex V3. In the upstream direcion, the wall shear stress increases due to the accelerating jet until a plateau is reached. Here, the friction coefficient is almoust constant at $|c_{\mathrm {f} }|=0.01$, which represents the maximum absolute value. It should be noted that the maximum is not located underneahth the horseshoe vortex. The distribution of $c_{\mathrm {f} }$ is dominated by the wall-parallel jet rather than by the horseshoe vortex. Further upstream, the value of $c_{\mathrm {f} }$ is small but negative, indicating the fading near-wall jet pointing still in the upstream direction. Unlike Apsilidis et al. (2015), we could not observe a second vortex here.

Following the downflow towards the bottom plate of the flume, the pressure increases with decreasing distance to the bottom. The pressure coefficient $c_{\mathrm {p} }$ increases likewise. Therefore, near the cylinder surface, the pressure coefficient shows a high amplitude at the height of the horseshoe vortex. Along a horizontal axis at $z_{\mathrm {V1} }=0.06D$, $c_{\mathrm {p} }$ decreases reaching its minimum value of about $0.3$ coinciding with the centre of the horseshoe vortex. Upstream of the horseshoe vortex, the horizontal profiles of the pressure coefficient coincide with each other irrespectively of the wall distance.

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Contributed by: Ulrich Jenssen, Wolfgang Schanderl, Michael Manhart — Technical University Munich

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Description

Test Case Studies

Evaluation

Best Practice Advice

References

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