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Thermal Issues in Emerging Technologies, ThETA 3, Cairo, Egypt, Dec 19-22 2010

ON THE SYNERGY FIELD BETWEEN VELOCITY VECTOR AND TEMPERATURE GRADIENT IN TURBULENT VORTICAL FLOWS

Charbel, Habchi

1,2

; Thierry, Lemenand

1

; Dominique, Della Valle

1,3

& Hassan, Peerhossaini

1,

*

1

Thermofluids, Complex Flows and Energy Research Group, LTN, CNRS UMR 6607, École Polytechnique - University of Nantes, rue Christian Pauc, B.P. 50609, 44306 Nantes, France

2

Agence de l’Environnement et de la Maîtrise de l’Énergie, ADEME, 20 avenue du Grésillé, B.P. 90406, 49004 Angers, France

3

ONIRIS, rue de la Géraudière, B.P. 82225, 44322 Nantes, France

Abstract

The intensity of the secondary flow induced, especially, by streamwise vorticity, which are generated in their turn by vortex generators or in flows with curved streamlines[Ajakh et al,1] has a direct impact on the heat transfer process. Thus the understanding and quantification of the physical mechanisms underlying the heat transfer by streamwise vorticity are fundamental for practical applications such as multifunctional heat exchangers/reactors (MHER) used in chemical processing industry, cooling of electronic systems and data centers, as well as biomedical engineering. In the present study, CFD simulations are performed to investigate the synergy field in two different flows. The synergy field principle is based on the assertion that the included angles θ between the streamlines and the isotherms is related to the heat flux that arises. From the local distribution of the intersection angle in the flow cross section, it is found that in the thinning region of the thermal boundary layer where the Nusselt number is the highest, θ is minimum. By introducing a characteristic parameter defined as the volume-averaged θ, it is found that the lowest θ value corresponds to the flow configuration presenting the highest Nusselt number. This confirms that the transport phenomena are intensified in the flow where the geometry minimizes this parameter. Finally, the study discusses the use of the synergy field principle in three dimensional turbulent vortical flows, and presents a new intensified MHER which can be used in several industrial processes.

1. Introduction

Large-scale eddies appear essentially in form of transverse and longitudinal vorticity [2]. These embedded flow structures can be generated due to shear instabilities or pressure gradients, and they play a crucial role in the heat and mass transfer mechanisms. The rearrangement of these vortices in the flow has a significant impact on the hydrodynamic and thermal performances for several practical interests [4-6]. The understanding of this impact is fundamental for the optimization of the energetic

efficiency of multifunctional heat exchangers-reactors (MHER). Recently, Guo et al. [7,8] proposed a new concept for the physical analysis and understading of the convective heat transfer mechanism. This concept is based on the combined actions or the synergy of temperature gradients and velocity vector, and it is therefore called

“synergy field principle”. It was shown by Guo et al. [7,8]

and Tao et al. [9,10] that the heat transfer enhancement is not only caused by the increase of the velocity vectors, but it is also related to the included angles between the streamlines and the isotherms, and to the fullness of dimensionless velocity and temperature profiles.

The synergy field principle can be applied to threedimensional flows especially for the design and optimization of MHER [9-12]. In fact, the convective heat transfer enhancement can be realized by reducing the intersection angle between the velocity and temperature gradient, and by producing the most possible uniform velocity and temperature profiles in the flow cross sections. In channel and straight pipe flows this angle is maximal (≈ 90°) since the flow streamlines are perpendicular to the temperature gradient.

In the present work, the heat transfer mechanism in turbulent vortical flows is investigated, and the effects of the flow structure on the convective heat transfer process are characterized by using the synergy field principle. To this end, physical vortices are produced by using different positionings of vortex generators in a turbulent pipe flow.

Numerical simulations of the flow and heat transfer, whose procedure is detailed in section 2, are performed by using the CFD code Fluent® 6.3 [13]. The numerical results are validated by the experimental results and discussed in section3. Finally, concluding remarks are given in section 4.

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2. Numerical procedure 1.1 Physical domains

Two flow configurations are considered in the present work, as shown in Figure 1, to study different vorticity arrangements on the fluid flow and heat transfer.

Flow direction in aligned arrays

Flow direction in reversed arrays

Figure 1. 3D views of the aligned and reversed arrays

These geometries are based on a classical straight pipe with trapezoidal vortex generators named HEV (High Efficiency Vortex) mixer [14]. The HEV has been studied as mixer and heat exchanger [15-19] and has shown good efficiency compared to other geometries, especially due to its low energy consumption. In the present study, the dimensions of the two geometries are the same, having 20 mm inner diameter, 140 mm total length and seven arrays each composed of four vortex generators diametrically opposed and inclined to the wall with 30° angle. More details on the vortex generator dimensions are given in Mohand Kaci et al. [19].

Downstream from each vortex generator, a pair of counter-rotating vortex (CVP) is generated due to the pressure gradients between the two sides of the tab surfaces [20,21]. The CVP generated in the aligned arrays provide a common out-flow in the tab symmetry plane, i.e.

from the wall towards the centerline; the reversed arrays are used to generate a common in-flow, i.e. from the centerline towards the wall [6,22].

1.2 Solution method and turbulence model

The numerical simulations are carried out by using the CFD code Fluent® 6.3 [13]. The conservation equations for mass, momentum and energy are solved sequentially with double precision, segregated and second-order accuracy. Pressure-velocity coupling is performed by finite volumes with the SIMPLE algorithm.

Mohand Kaci et al. [19] tested five different turbulence models to predict the flow dynamics in the HEV mixer, i.e.

aligned arrays in the present case, and showed that the

standard k and the RSM models, both associated with a two-layer model to compute the wall region, provide a satisfactory description of the flow pattern in this geometry. Therefore, these two turbulence models, that is the standard k and RSM, are used in the present study.

In this work, the RSM model is used, in addition to previous LDV measurements [22], to simulate the higher Reynolds numbers in both geometries for validating the results obtained by the k model. Once validated, the

k model is used to simulate the other Reynolds numbers since it requires far less computational time than RSM model.

The flow in the near-wall region is computed by using a two-layer model. In the viscous sub-layer, the one- equation model of Wolfstein [23] is used, where only the equation for turbulent kinetic energy transport is solved and the turbulent viscosity and energy dissipation are computed from empirical correlations based on length scales [24]. The two-layer model avoids the use of empirical wall standard functions, which are not valid for three-dimensional complex flows.

1.3 Boundary conditions

The heat conduction in the vortex generators surfaces and thickness is taken in to account in the present study by using coupled option of two-sided walls model. This model is useful when the solid region, i.e. the tab, has a fluid region on each side. The thermal conductivity in the tab is taken constant (100 W m-1K-1).

The physical properties of the working fluid (water) change significantly with the temperature. Therefore, the viscosity and thermal conductivity of water are assumed piecewise linear functions of temperature, as proposed by Rahmani et al. [25]. The specific heat and density are assumed to be constant for the temperature range used and are respectively set at 4182 J kg-1K-1 and 998 kg m3. No-slip boundary conditions are applied at the solid surface of the tabs and at the pipe wall. A fully developed turbulent flow velocity profile is used at the computational domain inlet; the TKE and the turbulence energy dissipation rate at the inlet are fixed by the turbulence intensity I derived from the equilibrium turbulent tube flow [26]. The fluid temperature at the inlet is set at 298.15 K.

Flow and heat-transfer simulations are carried out in a steady turbulent flow for Reynolds numbers 7500, 10000, 12500 and 15000 and for constant wall temperature

K

360

Tw .

1.4 Meshing and solution accuracy

Both geometries are reduced to a 1/8 sector by axial symmetry. A non-uniform unstructured three-dimensional mesh with hexahedral volumes is constructed and refined at all solid boundaries (by using the software Gambit®).

Mesh size is controlled by adjusting the number of the

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nodes in the radial direction, on the periphery of the element, and on the axial element length.

In each of the two geometries, the mesh density is increased until no effect on result quality is detected. The relative difference between the numerical results for two consecutive mesh densities does not exceed 1%. The criterion for grid sensitivity is based on velocity profiles, turbulence dissipation rate, and temperature profile at a radial direction in the tab symmetry plane at the outlet.

The mesh with lowest node density yielding high-quality results is used to generate and simulate the entire geometry. More details on mesh density validation can be found in Mohand Kaci et al. [19]. The final mesh size after refinement is 695,178 for the aligned arrays and 723,778 for reversed arrays.

The maximum final value of the wall dimensionless distance y in the first grid point after refinement does not exceed 3.4 in both geometries. The maximum value of y is less than 2.2 in both geometries. Hence, as y4, it is guaranteed that the viscous sub-layer is properly modeled.

Series of simulations are carried out for testing several stop-criteria values ranging from 10-3 to 10-9. It is found that beyond the value 10-6, no significant changes are observed in the temperature field and turbulence quantities, and the value 10-6 is retained as the convergence criterion for the simulations.

2 Results and discussions 2.1 Experimental validation

To evaluate the effects of the wall heating on the numerical results of the hydrodynamic and turbulence parameters, two cases are compared in both geometries.

The first case is for unheated (adiabatic) wall, and the second one is for heated wall of constant temperature at

K

360

Tw . After comparing different radial profiles of the mean axial velocity W , TKE k and its dissipation rate , it is found that the relative difference between the two cases, heated and unheated wall, do not exceed 1% in both geometries. Therefore, no significant effects of the wall heating are found on the hydrodynamic and turbulence parameters. This test is done by using both

k and RSM models.

Hence, the numerical results obtained from both models with heated wall are compared to those obtained experimentally in previous work of Habchi et al. [6] by using laser Doppler velocimetry (LDV). Figure 2 shows radial profiles at the outlet in the tab symmetry plane for both geometries. The mean axial velocity obtained numerically reproduces fairly well the experimental data as shown in Figure 2 (a). Moreover, the mean axial velocities obtained numerically from both turbulence models are very close to each other. On the same radial

profiles, Figure 2 (b) represents the turbulence kinetic dissipation rate in both geometries. It is observed that both turbulence models reproduce well the experimental results especially in the flow core

0r/R0.4

and in the shear region

0.4r/R0.7

, but in the wake region near the wall, the numerical results do not correlate very well with experimental ones. This fact can be attributed to the LDV measurements noise in the near wall region as was reported previously [6,19]. Moreover, the turbulence energy dissipation obtained from LDV measurements is obtained by using Taylor hypothesis of “frozen turbulence” which requires the definition of a convective velocity. This hypothesis is adequate in the flow core and shear region since the convective velocity is very close to advective one, i.e. mean velocity. However, in the wake region, the advective velocity is negative due to recirculation flow, and hence Taylor hypothesis is not completely adequate to be used in this region.

0.0 0.2 0.4 0.6 0.8 1.0

-0.5 0.0 0.5 1.0 1.5 -0.5 0.0 0.5 1.0 1.5

W (m/s)

Reversed arrays:

k- RSM LDV

r/R Aligned arrays:

k- RSM LDV

(a)

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0.0 0.2 0.4 0.6 0.8 1.0 0

10 20 30 400 10 20 30 40

(m2 /s3 )

Reversed arrays:

k- RSM LDV

r/R Aligned arrays:

k- RSM LDV

(b)

Figure 2. Numerical and experimental radial profiles at the outlet of each geometry in the tab symmetry

plane of the (a) mean streamwise velocity and (b) turbulence energy dissipation rate for Re= 15000 in

both geometries (experiments are adapted from Habchi et al. (2010))

2.2 Flow structure and temperature distribution In this section, the flow structures induced by the vortex generators and their effects on the temperature distribution are discussed.

It is observed from post-processing studies that the increase in the Reynolds number leads to increase quantitatively the turbulence and thermal parameters, without a significant change in the qualitative behavior of the flow structure. Therefore, and for simplicity, only results for Reynolds number of 15000 are discussed.

Moreover, the flow is observed to be periodic after the 4th row of vortex generators in both geometries. Hence, further investigations are focused on the 1st and 7th arrays in both geometries.

In Figure 3, the temperature distribution superposed on the secondary velocity vector field and the flow streamlines are present on a flow cross section at the outlet of both geometries. A CVP is observed in Figure 3 (a) which is caused by the pressure gradient between the

high momentum fluid in the flow core and the low momentum fluid in the wake of the tab. The common out- flow, in the tab symmetry plane in both geometries, ejects hot fluid from the near wall region towards the flow core forming high temperature strikes and thus thickening the thermal boundary layer.

In the reversed arrays, the pressure gradient generating the primary CVP is reversed relative to the aligned configurations. Hence, the rotation of the CVP is also reversed as is seen from the velocity vector field presented in Figure 3(b). Therefore, the CVP generated by a reversed vortex generator induces a common in-flow in the tab plane of symmetry, i.e. from the flow core towards the wall. The common out-flow, induced by two neighbor vortices of the same array, pumps hot fluid from the near- wall region towards the flow core. Moreover, it can be observed that the CVP centers in the reversed arrays are closer to the wall than in aligned arrays enhancing in suite the heat transfer as was demonstrated by Habchi et al.

[27].

T (K)

(a)

(b)

Figure 3. Temperature distribution superpose on the secondary velocity vector field at the outlet cross section of the (a) aligned and (b) reversed arrays, Re=

15000

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2.3 Hydrothermal performances

In order to evaluate the thermal performance of both geometries, first the global Nusselt number Nu is calculated from the following equation:

mean w

inlet , b outlet , p b

T T

T T

L c Nu m

 

 (1)

where Tmean

Tb,inletTb,outlet

/2 and  the thermal conductivity of the water. Tb is the bulk temperature computed from a UDF (user defined function) and,m is the mass flow rate.

The global friction factor is then obtained from the flowing expression:

2

2 Wm

P D / f L

  (2)

where P is the pressure difference between the flow inlet and outlet.

To compare the hydrothermal efficiency of these configurations for a constant pumping power, the thermal enhancement factor  is used: it is the ratio of the convective heat transfer coefficient h to that in an empty (no tabs) pipe flow h0 for a constant pumping power and defined as [28,29]:

3 1 0 0

/

f f Nu

Nu



 



 



 (3)

The Nusselt number is normalized by the empty pipe Nusselt number in a turbulent flow Nu0 given in Eq. (4).

In fact, Kakac et al. [30] examined a large number of correlations for fully developed turbulent flow in a circular tube and concluded that the Gnielinski [31]

equation (Eq. (4)) describes the available data better than any other over a range of Prandtl number from 0.5 to 200 and Reynolds number from 2300 to 5x106.

  

8

 

1

7 12 1

1000 8

3 2 2 1 0 0 0

 / /

Pr /

f .

Pr Re

/

Nu f (4)

where f0 is the friction factor in the empty pipe flow (Kakac et al., 1987):

25 0 0 0.079Re .

f (5)

Figure 4 shows the variation of the thermal enhancement factor  with the Reynolds number for both flow configurations. It is observed from this figure that  is always greater than unity. The enhancement factor tends to decrease with the Reynolds number, implying that the role of the vortex generators in the thermal enhancement is better for small Reynolds numbers. The enhancement

factors  of the reversed arrays is higher than that of the aligned arrays configuration; revalg0.6 . The present values of  are much higher than the data found for other mixing devices in the literature [28, 29].

6000 8000 10000 12000 14000 16000

1.6 1.8 2 2.2 2.4 2.6 2.8 3

Aligned arrays Reversed arrays

-0.34

Re -0.34

Figure 4. Variation of thermal enhancement factor as a function of Reynolds number

2.4 Synergy field principle

This section is devoted to the analysis of the synergy field, i.e. the intersection angle, between velocity and temperature gradients [7-10]. The energy equation for steady state fluid flow can be written as:

T T

U

cp  2

(6)

Using the Gauss theorem to integrate Eq. (6) over the computational domain and by neglecting the axial heat conduction in the fluid (as the Péclet number is larger than 100 [31]) the energy equation can be written as (see He et al. [32] for more details) :

 

   

pVolU T dxdydz Nu

c

(7)

where U

and T

are respectively the mean velocity and the temperature gradient in the cartesian coordinate,  is the total wall heat flux which is proportional to the Nusselt number.

Thus from Eq. (7) it can be concluded that the heat transfer expressed in terms of Nu depends on the dot product UTU T cos

 

, where  is the intersection angle between the velocity vector and the temperature gradient, and the operator represents the magnitude of the considered vector. Hence, for fixed magnitudes of velocity and temperature gradient, the smaller the intersection angle , the larger the convective heat transfer rate, i.e. the dot product UT

.

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From the present numerical simulations the local  distribution can be obtained from the following expression:

2 2 2

2 2 2

arccos

z T z T z W T V U

z W T y V T x U T

(8)

Variations of the global intersection angle Vol are obtained from the volume-weighted average in the computational domain:



 

 

 





 



Vol

Vol Voldxdydz dxdydz

 (9)

It should be noticed that the intersection angle varies between 0° and 180°, and hence two ideal synergy cases exists for  0cos

 

 1 and

 

1 cos 180 

 

 ; the non-synergy case is when

 

0 cos

90 

 

 . Moreover, regarding Eq. (9), the global heat transfer is equal to the integration of local scalar between the velocity and the temperature gradient and thus the integration depends on the sign of the local synergy values. In the case of (fluid) heating, the flow configuration must be designed in a way to reduce  aiming to attain the highest values of positive cos

 

 . In the case of (fluid) cooling, the flow configuration must be designed in such a way to have  as much as possible close to 180°. Hence, in the present study, as the fluid is heated by constant wall temperature, it is desirable to have intersection angles as close as possible to 0°.

Figure 5 shows the distribution of the synergy field T

Uxyxy

in the tube cross section of both geometries. It should be noticed that the index xy means that only the velocity and temperature gradient in the

 

x,y plane of the frame of reference are computed, i.e. in the flow cross section, in order to observe only the effect of the streamwise vortices on the synergy field. One should consider the temperature distribution represented in Figure 3 to better explain the synergy field distribution in the tube cross section. From Figure 5 (a) it can be seen that the synergy is almost negative in the region of the common out-flow. In fact, from Figure 3 (a) it can be seen that the velocity vectors of the common out-flow are in the opposite direction of the temperature gradient, leading to a negative intersection angle xy. The same result is observed in the common out-flow region of the reversed arrays. Moreover, in the center of the CVP in both geometries, the synergy UxyxyT 0

because the secondary velocity vector Uxy0

, and thus the heat is transported only by conduction. The case of

0

T Uxyxy

is also observed in other regions of the

cross sections where the velocity vector is perpendicular to the temperature gradient. The highest values of the positive UxyxyT

are observed in the regions where the velocity vector and the temperature gradient are aligned.

 

Ks1 T

Uxyxy

(a)

(b)

Figure 5. Distribution of the synergy field UxyxyT in the tube cross section for (a) aligned and (c) reversed

arrays, Re= 15000

Figure 6 (a) compares the global intersection angle Vol between the different geometries. From this figure it is observed that the highest Vol are obtained in the aligned arrays which have the lowest heat transfer efficiency, and the lowest Vol is obtained for the reversed arrays which is found to have the best heat transfer performances as discussed previously. However, the trends of Vol as a function of the Reynolds number seem to be almost constant: there is no significant effect of Reynolds number on the intersection angle. Meanwhile, from Figure 6 (b), it can be seen that the heat transfer strength  increases with the Reynolds number due to the increase in the velocity magnitude and temperature gradient in the flow with the largest magnitudes observed in the reversed arrays. Moreover,  in the reversed arrays is greater than

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that in the other two geometries and the levels of 

revalg

follow that of the Nusselt number for both geometries

NurevNualg

. Hence, it can be concluded from the variation trends of Vol and  that the increase in the Reynolds number increases only the magnitudes of the velocity and temperature gradient and do not affect the intersection angle. Therefore, to enhance the heat transfer mechanism, the geometry must be modified in such a way to increase  simultaneously with a decrease in Vol.

6000 8000 10000 12000 14000 16000

83 84 85 86 87 88 89 90

)

Re Aligned arrays Reversed arrays

(a)

6000 8000 10000 12000 14000 16000

0 100 200 300 400 500 600 700

Aligned arrays Reversed arrays

(W)

Re

(b)

Figure 6. (a) Intersection angle and (b) global heat transfer strength

3 Concluding remarks

In the present work, numerical simulations of the flow and heat transfer are performed to investigate the influence of the vorticity rearrangement on the heat transfer mechanisms by using different physical approaches. The numerical procedure and turbulence model are validated by previous experimental results using laser Doppler anemometry [6]. Transverse and streamwise vorticity are produced by using different rearrangements of vortex generators in a turbulent pipe flow: in the first, the vortex

generators are aligned and inclined in the direction of flow (the reference geometry for a high-efficiency vortex (HEV) static mixer), in the second, a periodic 45°

tangential rotation is applied to the tab arrays with respect to one another, and in the third the reference geometry is used in the direction opposite to the flow direction (reversed direction) aiming to reverse the sign of the streamwise vorticity.

The synergy field between the velocity and the temperature gradient [7-10] is also studied; it is found that the intersection angle between the velocity and temperature gradient is the smallest for the reversed arrays, which has the best performance. Moreover, it is concluded from the variation of the global intersection angle Vol and heat transfer strength  versus the Reynolds number, that the increase in the Reynolds number increases only the magnitudes of the velocity and temperature gradient and does not affect the intersection angle. Therefore, to enhance the heat transfer mechanism, the geometry must be modified in such a way to increase  simultaneously with a decrease in Vol.

4 Acknowledgement

This work was partially supported by ADEME (Agence de l’Environnement et de la Maîtrise de l’Énergie). Dr. C.

Garnier is kindly acknowledged for monitoring this grant.

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