Applied Computational Fluid Dynamics by Hyoung Woo Oh - HTML preview

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particularly aggressive (Oshima e al., 2001).

Therefore, the possibility of predicting cavitation is fundamental in hydraulic components

design and both experiments and numerical simulation have to be employed and integrated

in order to help the understanding of the basics of cavitation occurrence. Particularly,

numerical analysis can provide a great amount of data that can extend the experimental area

and deepen the insight of the physical phenomenon (Yang, 2002, 2005). Nevertheless, the

accuracy and reliability of the numerical models have to be addressed when approaching a

new problem or when they are modified to account for a more detailed description of the

physical process. The model sensitivity with respect to the fluid-dynamics characteristics of the case studied (such as the Reynolds number in the critical sections, the geometry

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complexity and the boundary conditions) must be properly addressed before adopting the

numerical tool as a predictive design tool.

When addressing numerically the flow through the metering section of hydraulic

components, particular care should also be devoted to the operating conditions accounted

for in the simulations. In fact, the behaviour of the flow is usually highly time dependent, as well as the geometry of the component varies according to the working conditions. Thus,

the choice of carrying out a steady state or a fully transient CFD simulation of the

component is a critical issue in the design methodology. On one hand, the former approach

is characterized by a significantly lower computational effort as well as a shorter case setup time, but it evaluates the fluid-dynamics performance of the hydraulic component only

under the assumption of steady state operation, which is often a very limiting restriction

compared to the real operations. Conversely, the fully transient CFD calculation predicts

more accurately the real behaviour of the flow within the hydraulic component, but the

required computational effort is remarkably large and both the setup time and the

simulation execution duration can be considerably long. Therefore, it is important to

highlight the quality of the results that can be obtained by performing these two types of

CDF simulations, in order to select the correct approach for each analysis that has to be

carried out.

In this chapter, the above mentioned critical aspects in the application of multidimensional numerical analysis for the design of mechanical devices and components for hydraulic

systems are addressed. The objective of the chapter is to provide a roadmap for the

multidimensional numerical analysis of the hydraulic components to be used effectively in

the design process. In particular, two examples of hydraulic systems are accounted for in the application of the CFD analysis: a proportional control valve and a fuel accumulator for

multi-fuel injection systems. These test cases have been selected due to their

representativeness in the field of hydraulic applications and to the complexity and variety of the physical phenomena involved.

2. Prediction capabilities of the numerical models

The Navier–Stokes equations for isothermal, incompressible flows are solved by means both

of the open source multidimensional CFD code OpenFOAM (OpenCFD, 2010,

OpenFOAM®-Extend Project, 2010), and the commercial CFD code ANSYS CFX. Bounded

central differencing is used for the discretization of the momentum, second-order upwind

for subgrid kinetic energy. Pressure–velocity coupling was achieved via a SIMPLE similar

procedure. The second-order implicit method is used for time integration scheme. No time

integration scheme is involved, and all the calculations are performed under steady state

conditions.

In the modeling of the turbulent cases the performance of three turbulence models are

investigated:

1. The standard k-ε model (KE), including wall functions for the near-wall treatment;

2. the a low-Reynolds number model developed by Launder and Sharma (LS), (Launder &

Sharma, 1974) in which the transport equations for the turbulent quantities are

integrated to the walls;

3. the two zonal version of the k-ω model, known as the shear stress transport model (SST)

(Menter, 1993).

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251

Since the objective of this investigation is the analysis of confined flows, the attention is paid to near-wall behaviour, to the damping functions and to the boundary conditions. Hence the

choice of addressing the predictive capabilities of turbulence models with a different near

wall treatment is made. In the k- model, the transport equations are not integrated to the

walls. Instead the production and dissipation of kinetic energy are specified in the near-wall cell, using the logarithmic law-of-the-wall. The validity of the near wall treatment requires that the values of the y must be in the range between 30 and 100. In the k- ε model formulation proposed by Launder and Sharma the definition of the turbulent kinetic energy

dissipation is modified to account for the low Reynolds regions close to the wall. In fact, this equation is solved for  instead of ε, and a new term E is added to compensate for additional production and to further balance diffusion and dissipation in the vicinity of the walls. In this way, the Launder and Sharma approach has the advantage of the natural

boundary condition   0 at the walls. The model’s constants are the same as the standard formulation, but the damping factor functions are evaluated as a function of the turbulent

Reynolds number. The boundary conditions at the wall are k  0 and   0 . For the low Reynolds number turbulence models the requirement on the y values is more stringent, in fact y should never be larger than one. The. shear stress transport model is derived from the original two zonal version of the k-ω model proposed by Wilcox (Wilcox, 1988), and

based on the transport equation proposed by Kolmogorov. In this model the damping

functions in near-wall regions are not necessary. The eddy viscosity is calculated as the ratio between the turbulent kinetic energy and the the specific dissipation, . The original version of the model demonstrated to be very sensitive to  specified in the free-stream (Menter,

1994). Therefore a new formulation was proposed by Menter combining the the k- model

by Wilcox in the inner region of the boundary layer, and the standard k - ε in the outer

region and the free-stream. The equation differs from the one of the original k- model

because of an additional cross-diffusion term. In the inner part of the boundary region the

model’s constants are the same as the k-ω model, while in the outer region they become

similar the k–ε ones. The boundary conditions do not change from the original k- model

formulation, and similarly require y smaller than 3. In this analysis careful attention was paid in order to comply with the requirements on the y values for the different turbulence models adopted.

2.1 Flow through a circular pipe

First phase of the analysis is the simulation of the fundamental test case represented by the flow through a circular pipe. The geometrical domain is assumed to be a straight circular

pipe, characterized by an axial length equal to 1.0 m and a diameter of 10 mm, pure water is considered as the operating fluid and both laminar and turbulent conditions are accounted

for. Due to the axial symmetry of both the geometry and the boundary conditions, the

simulations assume a two dimensional domain. Therefore, the meshes are defined as

circular sectors with an angular amplitude equal to 5° (see Fig.1).

A preliminary sensitivity analysis with respect to the grid resolution is carried out, in order to assess the best compromise between the accuracy of the results and the computational

cost. Different grids are constructed varying the cell spacing both in the axial and radial

direction. For the laminar case, the cell axial dimensions equal to 1.0, 2.5, and 10 mm are

compared keeping constant the resolution along the cylinder radius (i.e. 0.3 mm); whereas

the grids used in the turbulent case are characterized by a radial cell size equal to 0.3, 0.1

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Fig. 1. 2D mesh for the straight circular pipe

Grid

Turbulence

Case #

CFD code

(ax. & rad.)

Model

A_1; A_2; A_3; A_4

FOAM

1.0x0.3; 2.5x0.3; 5.0x0.3; 10.0x0.3

Laminar

A_5; A_6; A_7; A_8

CFX

1.0x0.3; 2.5x0.3; 5.0x0.3; 10.0x0.3

Laminar

A_9; A_10; A_11

FOAM

5.0x0.05; 5.0x0.1; 5.0x0.3

LS

A_12; A_14; A_16

CFX

5.0x0.05; 5.0x0.1; 5.0x0.3

KE

A_13; A_15; A_17

CFX

5.0x0.05; 5.0x0.1; 5.0x0.3

SST

Table 1. List of simulations for the laminar and turbulent flow through the circular pipe

and 0.05 mm and a constant axial dimension (i.e. 5 mm). The meshes consist only in

hexahedrons and prisms along the cylinder axis; the height of the cells near the walls is

carefully chosen in order to comply with the requirements of the turbulence models used in

the simulations on the distance to the wall of the first node. Table 1 shows the

comprehensive list of the simulations performed. For the laminar cases a fluid axial velocity of 0.1 m/s is set at the inlet boundary, while a static pressure boundary condition was

considered at the pipe outlet. The numerical results for the laminar regime were compared

with the Hagen-Poiseuille theory (Pao, 1995), that is applicable when no relative motion

between the fluid and the wall appears, and an incompressible Newtonian fluid undergoes

to a isothermal laminar flow. Under these assumptions, the axial velocity profile versus the distance from the axis can be determined from the expression:

1 

p

 

v

 

  2 2

 0

r

r

4

(1)

z

 

As well known, the laminar velocity assumes the fully developed profile at a distance from

the pipe inlet on the basis of the Langhaar length, defined as:

'

L  0.058  Re D

(2)

In Figs. 2 a) and c) the theoretical axial velocity profile as a function of the distance from the cylinder axis is compared with the calculated profiles for the different grid resolutions. Both codes used in the simulations demonstrated a good agreement with the axial velocity profile

derived from the Hagen-Poiseuille, and also demonstrated a negligible influence on the cell

dimension. Similar behaviour could be noticed in the velocity profile prediction, see Figs. 2

b) and d), and practically no differences could be seen among the simulated cases.

When investigating the flow field under fully turbulent conditions a fluid axial velocity of 5.0 m/s was set at the inlet boundary. Calculations were performed for three grids having

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Multidimensional Design of Hydraulic Components and Systems

253

different cell dimensions, and the performance of the turbulence models described in the

previous sections (i.e. the standard k -  model, the k – ω shear stress transport model and the low Reynolds Launder-Sharma models) is investigated. The results were compared

with the experimental measurements performed by Nikuradse available in literature (Pao,

1995). In Figs. from 3 to 5 the axial velocity versus the distance from the cylinder axis and the cylinder outlet are depicted. The KE model demonstrated a good agreement with the

measurements and a scarce sensitivity to the grid size; in particular the logarithmic law-

of-the-wall was able to capture the curvature of the axial velocity in proximity to the wall.

Whereas, the SST model resulted to be remarkably more influenced by the mesh

resolution. In fact Fig. 4 b) shows that the predicted axial velocity differs significantly for the three simulated grids. In particular the coarser grid calculation underestimates the

velocity magnitude, while the discrepancy between the curves relating the fine and

intermediate meshes are less evident and closer to the results found for the KE model. The

more evident sensitivity of the SST model to the grid size is due to the stricter

requirement on the distance of the first grid node to the wall. The sensitivity to the mesh

resolution was found to be even more marked for the LS model (see Fig. 5). In this model,

in fact, the transport equations are integrated up to the wall and the effect of the near wall cell is more directly transferred to the inner domain. This model demonstrated to

overestimate the axial velocity in the core region as a consequence of the velocity

magnitude tendency when approaching the wall boundary. The dissipation of the

turbulent kinetic energy is therefore overestimated and the model constant should be

tuned accordingly. For the present study the constants of the considered models were

kept the same as the suggested values.

a)

b)

c)

d)

Fig. 2. a) and c) Axial velocity profile vs. the distance from the axis and b) and d) axial

velocity profile along the cylinder axis vs. the distance from the pipe inlet: comparison

among different grid resolutions (laminar regime)

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a)

b)

Fig. 3. a) Axial velocity profile vs. the distance from the axis and b) Axial velocity profile along the cylinder axis vs. the distance from the pipe inlet: comparison among different grid resolutions (KE model)

a)

b)

Fig. 4. a) Axial velocity profile vs. the distance from the axis and b) Axial velocity profile along the cylinder axis vs. the distance from the pipe inlet: comparison among different grid resolutions (SST model)

a)

b)

Fig. 5. a) Axial velocity profile vs. the distance from the axis and b) Axial velocity profile along the cylinder axis vs. the distance from the pipe inlet: comparison among different grid resolutions (LS model)

2.2 Flow through a small sharp-edged cylindrical orifice

Further step of the analysis is the investigation of the flow pattern through a sharp-edged

cylindrical orifice. Although the geometry of this test case is very simple, it well represents the fluid-dynamics conditions which can be found in the critical sections of many hydraulic

components. In addition, experimental measurements of the flow through abrupt section

change in circular pipes are available in literature. Therefore, it is possible to address the predictive capabilities of the numerical calculations by comparing the main flow

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255

characteristics with experiments. In the present work the measurements carried out by

Ramamurthi and Nandakumar in 1999 were taken as a reference. In the experiments, with

reference to pure water, the effects of varying the diameters of the sharp-edge orifice and the ratio of the inlet diameter ( d) and the orifice length ( l) are investigated for different Reynolds numbers of operation. The experimental set-up consisted of a tank for the water, a nitrogen

gas source for pressurizing the tank and a feed-line fitted with flow control valves for

supplying water to the orifice. The modelling of the experimental device focuses only on the orifice geometry, and particular care is paid to assure that the flow at the orifice extremes is not influenced by the inlet and outlet of the CFD domain. To do this, two plenums are

considered at the orifice inlet and outlet, each one having a diameter and an axial length ten times larger than the orifice diameter. Thanks to the axial symmetry of the geometry and of

the boundary conditions, it is possible to account only for a 5° sector of the whole domain, and to simulate the experiments as two dimensional cases. Fig. 6 shows an example of the

CFD domain used. The simulations accounted for three orifice diameters (i.e. 0.5, 1 and 2

mm), three aspect ratios (i.e. 1, 5 and 20) and different Reynolds numbers. The complete list of the simulations, together with their main features, is detailed in Table 2.

Fig. 6. CFD domain for the small sharp-edged cylindrical orifice test case

Turbulence

Case #

Section diameter

l/d

Reynolds number

Model

B_1; B_4; B_7

0.5; 1.0; 2.0 mm

1

5x103; 1x104; 2x104

KE

B_2; B_5; B_8

0.5; 1.0; 2.0 mm

5

1.1x104; 2x104; 4x104

KE

B_3; B_6; B_9

0.5; 1.0; 2.0 mm

20

2x104; 4x104; 6x104

KE

B_10; B_13; B_16

0.5; 1.0; 2.0 mm

1

5x103; 1x104; 2x104

SST

B_11; B_14; B_17

0.5; 1.0; 2.0 mm

5

1.1x104; 2x104; 4x104

SST

B_12; B_15; B_18

0.5; 1.0; 2.0 mm

20

2x104; 4x104; 6x104

SST

B_19; B_22; B_25

0.5; 1.0; 2.0 mm

1

5x103; 1x104; 2x104

LS

B_20; B_23; B_26

0.5; 1.0; 2.0 mm

5

1.1x104; 2x104; 4x104

LS

B_21; B_24; B_27

0.5; 1.0; 2.0 mm

20

2x104; 4x104; 6x104

LS

Table 2. List of simulations for the turbulent flow through a small sharp-edged cylindrical

orifice

In the modelling, the above mentioned standard k- model, the shear stress transport model

and the low Reynolds Launder-Sharma model are compared. Moreover, similarly to the

flow through a circular pipe case, different grid resolutions are tested to reduce the grid

sensitivity. Finally, a ratio between the radial cell dimension and the orifice radius of 0.02 is found to be a good compromise between computational cost and results accuracy. The

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numerical results are compared with measurements mainly in terms of the orifice discharge

coefficients. In the experiments the discharge coefficient is calculated using the relation: 2 p

Q Cd o

A

(3)

where p

 is the pressure drop across the orifice,  the fluid density, A0 the orifice

geometrical area and Q the volumetric flow rate.

Particular care was devoted in calculating the pressure drop and, in order to assess the

influence of the abrupt section change only, it was defined as the difference between the

inlet static pressure, pin , and the static pressure at the vena contracta position, pvc .

Fig. 7. Axial pressure for the small sharp-edged cylindrical orifice test case

With reference to Fig. 7, the fluid pressure in the vena contracta section, and the axial

position of both the vena contracta ( xvc ) and the reattachment section ( xr ) are accurately estimated using the pressure distribution along the orifice length. In particular, the latter parameter is assumed as the axial coordinate of the relative maximum of the pressure profile downstream the vena contracta position. Fig. 8 a) collects, for all the cases reported in Table 3, the comparison between the experimental and the predicted discharge coefficients. As shown,

for a given test case and for a wide variation of the Reynolds Number, each graph directly

compares the experimental discharge coefficient with the numerical predictions obtained by

using all the turbulence models previously depicted. The agreement of the calculated

discharge coefficients and the experiments varied significantly among the test cases. The

simulations demonstrate a better predictive capability for larger aspect ratios and lower

Reynolds number. Under these conditions, the values calculated by using the KE and SST

models are sufficiently close to the measured ones. On the other hand, a worse agreement is

found for lower aspect ratios. Both turbulence models are able to capture the overall trend of the experiments, even though the SST model demonstrated a better accuracy.

While the behaviour of the KE and SST resulted to be similar, the values calculated by the

LS model are found to be significantly different from measurements, and in particular for

cases characterized by a small diameter and a low aspect ratio. The tendency of the LS

turbulence model of underestimating the velocity close to the wall (highlighted in the flow

through a circular pipe analysis also) is therefore confirmed. Consequently, the high

turbulent kinetic energy dissipation rate causes a reduced velocity in proximity to the wall, thus forcing a smaller orifice effective area. This behaviour can be noticed also when

comparing the axial coordinate of the vena contracta and of the reattaching point calculated by using the three turbulence models (see Fig. 8 b) and c) ). A similarity can be noticed for the KE and SST models: while the reattaching points calculated by the LS model result to be

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257

Fig. 8. a) Experimental and calculated discharge coefficients and axial coordinate of b)the

vena contracta position and c) the reattaching point for different Reynolds number

Fig. 9. Turbulence models influence on the velocity magnitude and pressure distribution

more distant from the orifice inlet. In many cases the relative maximum in the pressure

profile along the geometry axis is found to be downstream the orifice outlet. This behaviour can be explained by investigating the velocity and pressure distribution along the channel

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(see Figs. 9). Finally, it is possible to conclude that the standard k- model and the k–ω shear stress transport models demonstrate a sufficient accuracy in calculating the discharge

coefficients for most of the analyzed cases. Contrarily, the low Reynolds Launder-Sharma

model is found to overestimate the turbulent kinetic energy dissipation, particularly in the wall proximity, thus causing an underestimation in the orifice effective area prediction. For the small diameter and low aspect ratio cases, the cavitating phenomena cannot be

neglected in order to predict with a reasonable accuracy the discharge coefficients.

3. Modelling of cavitation and aeration

Once the predictive capabilities of the numerical models for the simulation of the

incompressible flow are investigated, further step of the analysis is the modelling of the