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15th Australasian Fluid Mechanics Conference The University of Sydney, Sydney, Australia 13-17 December 2004 Scaling analysis and direct simulation of unsteady natural convection cooling of fluid with Pr < 1 in a vertical cylinder Wenxian Lin 1,2 and S. W. Armfield 1 1 School of Aerospace, Mechanical & Mechatronic Engineering, The University of Sydney, NSW 2006, AUSTRALIA 2 Solar Energy Research Institute, Yunnan Normal University, Kunming, Yunnan 650092, P. R. China Abstract The unsteady natural convection cooling of fluid with Pr < 1 in a vertical cylinder with an imposed lower temperature on verti- cal sidewalls is dominated by three distinct stages of develop- ment, i.e. the boundary-layer development stage adjacent to the sidewall, the stratification stage, and the cooling-down stage, respectively. Various scaling laws to describe the unsteady flow behavior at these respective stages are developed with scaling analysis and are verified and quantified by direct numerical sim- ulation with selected values of the aspect ratio of the cylinder A, the Rayleigh number Ra, and the Prandtl number Pr in the ranges of 1/3 A 3, 10 6 Ra 10 10 , and 0.01 Pr 0.5. Introduction Cooling/heating a body of fluid in an enclosure via natural con- vection with an imposed temperature difference or heat flux on the enclosure boundary is widely encountered in nature and in engineering settings, and the understanding of its transient flow behavior is of fundamental interest and practical importance. In the past decades, extensive experimental, numerical, and analyt- ical studies have been conducted on this issue, although mainly on the more specific case of a rectangular cavity with differen- tially heated sidewalls (see, e.g. [1, 2]). Patterson and Imberger [3] used a scaling analysis in their pio- neering investigation of the transient behavior that occurs when the opposing two vertical sidewalls of a two-dimensional rect- angular cavity are impulsively heated and cooled by an equal amount. They devised a classification of the flow development through several transient flow regimes to one of three steady- state types of flow based on the relative values of Ra, Pr, and A. This Patterson-Imberger flow model has since occupied the cen- ter stage of research into understanding natural convection flow in cavities, and numerous investigations subsequently focused on diverse aspects of the model (see, e.g. [4, 5, 6, 7]). The majority of the past studies have focused on fluids with Pr 1 owing to their relevance in theoretical and practical applications. Natural convection flows with Pr < 1 are very important as well, in such applications as the Earth’s liquid core convection, crystal growth in semiconductors, melting pro- cesses, etc., not to mention those using air and other gases as the working medium. However, studies on unsteady natural convection flows of fluids with Pr 1 resulting from heat- ing/cooling vertical boundaries, together with studies on the ef- fect of Pr variation, are scarce. This scarcity, together with the apparently incomplete understanding of Pr 1 flows, motivates the current study. Scaling Analysis Under consideration is the flow behavior of cooling a quiescent isothermal Newtonian fluid with Pr < 1 in a vertical cylinder by unsteady natural convection due to an imposed fixed lower 0 1 z r H R (a) Physical system T w T 0 (at t=0) Adiabatic A -1 0 (b) Computational domain Figure 1: A sketch of the physical system considered and the computational domain used for numerical simulations. temperature on the vertical sidewalls. The cylinder has a height of H and a radius of R 0 , as sketched in Fig. 1. It is assumed that the fluid cooling is the result of the imposed fixed temperature T w on the vertical sidewalls while all the remaining boundaries are adiabatic and all boundaries are non-slip, and the fluid in the cylinder is initially at rest and at a uniform temperature T 0 (T 0 > T w ). It is also assumed that the flows are laminar. The governing equations of motion are the Navier-Stokes equa- tions with the Boussinesq approximation for buoyancy, which together with the temperature transport equation can be written in the following two-dimensional form, 1 R (RU ) R + V Z = 0, (1) U t + 1 R (RUU ) R + ( VU ) Z = - 1 ρ P R + ν R 1 R (RU ) R + 2 U Z 2 , (2) V t + 1 R (RUV ) R + ( VV ) Z = - 1 ρ P Z + ν 1 R R R V R + 2 V Z 2 + gβ(T - T 0 ), (3) T t + 1 R (RU T ) R + ( VT ) Z = κ 1 R R R T R + 2 T Z 2 . (4) where U and V are the radial (R-direction) and vertical (Z- direction) velocity components, t is the time, P is the pressure, T is the temperature, g is the acceleration due to gravity, β, ν and κ are the thermal expansion coefficient, kinematic viscosity and thermal diffusivity of the fluid, respectively. The gravity acts in the negative Z-direction. The flow considered here is dominated by three distinct stages of development, i.e. the boundary-layer development stage, the
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Page 1: Scaling analysis and direct simulation of unsteady natural …web.aeromech.usyd.edu.au/15afmc/proceedings/papers/AFMC... · 2013-10-01 · 15th Australasian Fluid Mechanics Conference

15th Australasian Fluid Mechanics ConferenceThe University of Sydney, Sydney, Australia13-17 December 2004

Scaling analysis and direct simulation of unsteady natural convection cooling of fluid withPr < 1 in a vertical cylinder

Wenxian Lin1,2 and S. W. Armfield1

1School of Aerospace, Mechanical & Mechatronic Engineering,The University of Sydney, NSW 2006, AUSTRALIA

2Solar Energy Research Institute, Yunnan Normal University,Kunming, Yunnan 650092, P. R. China

Abstract

The unsteady natural convection cooling of fluid with Pr < 1 ina vertical cylinder with an imposed lower temperature on verti-cal sidewalls is dominated by three distinct stages of develop-ment, i.e. the boundary-layer development stage adjacent to thesidewall, the stratification stage, and the cooling-down stage,respectively. Various scaling laws to describe the unsteady flowbehavior at these respective stages are developed with scalinganalysis and are verified and quantified by direct numerical sim-ulation with selected values of the aspect ratio of the cylinderA, the Rayleigh number Ra, and the Prandtl number Pr in theranges of 1/3 ≤ A ≤ 3, 106 ≤ Ra ≤ 1010, and 0.01 ≤ Pr ≤ 0.5.

Introduction

Cooling/heating a body of fluid in an enclosure via natural con-vection with an imposed temperature difference or heat flux onthe enclosure boundary is widely encountered in nature and inengineering settings, and the understanding of its transient flowbehavior is of fundamental interest and practical importance. Inthe past decades, extensive experimental, numerical, and analyt-ical studies have been conducted on this issue, although mainlyon the more specific case of a rectangular cavity with differen-tially heated sidewalls (see, e.g. [1, 2]).

Patterson and Imberger [3] used a scaling analysis in their pio-neering investigation of the transient behavior that occurs whenthe opposing two vertical sidewalls of a two-dimensional rect-angular cavity are impulsively heated and cooled by an equalamount. They devised a classification of the flow developmentthrough several transient flow regimes to one of three steady-state types of flow based on the relative values of Ra, Pr, and A.This Patterson-Imberger flow model has since occupied the cen-ter stage of research into understanding natural convection flowin cavities, and numerous investigations subsequently focusedon diverse aspects of the model (see, e.g. [4, 5, 6, 7]).

The majority of the past studies have focused on fluids withPr ≥ 1 owing to their relevance in theoretical and practicalapplications. Natural convection flows with Pr < 1 are veryimportant as well, in such applications as the Earth’s liquidcore convection, crystal growth in semiconductors, melting pro-cesses, etc., not to mention those using air and other gases asthe working medium. However, studies on unsteady naturalconvection flows of fluids with Pr � 1 resulting from heat-ing/cooling vertical boundaries, together with studies on the ef-fect of Pr variation, are scarce. This scarcity, together with theapparently incomplete understanding of Pr ≤ 1 flows, motivatesthe current study.

Scaling Analysis

Under consideration is the flow behavior of cooling a quiescentisothermal Newtonian fluid with Pr < 1 in a vertical cylinderby unsteady natural convection due to an imposed fixed lower

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0

1z

r

H

R

(a) Physical system

Tw

T0 (at t=0)

Adiabatic

A−1

0

(b) Computational domain

Figure 1: A sketch of the physical system considered and thecomputational domain used for numerical simulations.

temperature on the vertical sidewalls. The cylinder has a heightof H and a radius of R0, as sketched in Fig. 1. It is assumed thatthe fluid cooling is the result of the imposed fixed temperatureTw on the vertical sidewalls while all the remaining boundariesare adiabatic and all boundaries are non-slip, and the fluid inthe cylinder is initially at rest and at a uniform temperature T0(T0 > Tw). It is also assumed that the flows are laminar.

The governing equations of motion are the Navier-Stokes equa-tions with the Boussinesq approximation for buoyancy, whichtogether with the temperature transport equation can be writtenin the following two-dimensional form,

1R

∂(RU)

∂R+

∂V∂Z

= 0, (1)

∂U∂t

+1R

∂(RUU)

∂R+

∂(VU)

∂Z= −

∂P∂R

+ ν{

∂∂R

[

1R

∂(RU)

∂R

]

+∂2U

∂Z2

}

, (2)

∂V∂t

+1R

∂(RUV )

∂R+

∂(VV )

∂Z= −

∂P∂Z

+ ν[

1R

∂∂R

(

R∂V∂R

)

+∂2V

∂Z2

]

+gβ(T −T0), (3)

∂T∂t

+1R

∂(RUT )

∂R+

∂(V T )

∂Z= κ

[

1R

∂∂R

(

R∂T∂R

)

+∂2T

∂Z2

]

. (4)

where U and V are the radial (R-direction) and vertical (Z-direction) velocity components, t is the time, P is the pressure,T is the temperature, g is the acceleration due to gravity, β, νand κ are the thermal expansion coefficient, kinematic viscosityand thermal diffusivity of the fluid, respectively. The gravityacts in the negative Z-direction.

The flow considered here is dominated by three distinct stagesof development, i.e. the boundary-layer development stage, the

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τ=1 τ=10τ=4

τ=20 τ=45 τ=80

τ=170 τ=350 τ=650

Figure 2: Numerically simulated temperature contours at thestages of the boundary-layer development (top row), the strati-fication (middle row), and the cooling-down (bottom row), re-spectively, for Ra = 108, A = 1, and Pr = 0.1.

stratification stage, and the cooling-down stage, respectively, asillustrated in Fig. 2, where numerically simulated temperaturecontours are shown for the three stages for the specific case ofRa = 108, Pr = 0.1 and A = 1, where Ra, Pr and A are definedas

Ra =gβ(T0 −Tw)H3

νκ, Pr =

νκ

, A =HR0

.

In this case the boundary-layer development is seen in the tem-perature contours adjacent to the righthand, cooled, wall, withthe boundary-layer development completed by around τ = 10,where τ is the dimensionless time, made dimensionless byH2/(κRa1/2). The cooled fluid ejected by the boundary layeracts to fill and stratify the domain, seen in the stratificationstage, from τ = 20 to 80. Finally the stratification is graduallyreduced in the cooling-down stage of the flow, for τ > 170. Inthis section, scaling relations will be developed for the relevantparameters characterizing the flow behavior at these respectivestages of flow development.

The vertical boundary layer adjacent to the cooled sidewall ex-periences a start-up stage, followed by a short transitional stagebefore reaching a steady-state stage. The parameters character-izing the flow behavior at this development stage are the ther-mal boundary-layer thickness ∆T , the maximum vertical veloc-ity Vm, the time ts for the boundary-layer development to reachthe steady state, and the Nusselt number Nu across the sidewall.

Heat is initially transferred out through the vertical wall fromthe fluid by conduction after the initiation of the flow, resultingin a vertical thermal boundary layer of thickness O(∆T ) adja-cent to the wall, where at height Z, from Eq. (4), the balance be-tween the inertial term O([T0 −Tw]/t) and the conductive termO(κ[T0 −Tw]/∆2

T ) dominates the flow, which gives,

∆T ∼ κ1/2t1/2, (5)

or, in dimensionless form,

δT =∆T

H∼ Ra−1/4τ1/2, (6)

in which “∼” means “scales with” and τ = t/(H/V0) is the di-mensionless time, where V0 = κRa1/2/H is the characteristicvelocity scale. During this start-up stage, the dominant balancein Eq. (3) for Pr < 1 is that between the inertia force O(Vm/t)and the buoyant force O(gβ[T0 −Tw]), which gives

Vm ∼ gβ(T0 −Tw)t ∼RaνκH3 t, (7)

or, in dimensionless form,

vm =Vm

V0∼ Pr τ, (8)

After the start-up stage, the dominant balance at height Z inEq. (4) gradually shifts from that between the inertial termO([T0 − Tw]/t) and the conductive term O(κ[T0 − Tw]/∆2

T )to that between the inertial term and the convective termO(Vm[T0 −Tw]/[H −Z]), until the latter balance becomes fullydominant and the thermal boundary-layer development thenreaches its steady-state stage. The inertia-convective balancein Eq. (4) gives

T0 −Tw

t∼

Vm[T0 −Tw]

H −Z. (9)

Using Eqs. (5) and (7), this leads to

tb ∼

[

H −Zgβ(T0 −Tw)

]1/2

∼H2

κRa1/2Pr1/2

(

1−ZH

)1/2

, (10)

or, in dimensionless form,

τb =tb

(H/V0)∼

(

1− zPr

)1/2

, (11)

which represents the local time scale for the thermal boundarylayer at height Z to reach the steady state, where z = Z/H is thedimensionless vertical coordinate.

At time tb, the thermal boundary layer at height Z reaches itssteady-state thickness scale ∆T,b, which, from Eq. (5), is as fol-lows,

∆T,b ∼ κ1/2[

H −Zgβ(T0 −Tw)

]1/4

∼H3/4(H −Z)1/4

Ra1/4Pr1/4, (12)

or, in dimensionless form,

δT,b =∆T,b

H∼

(

1− zPrRa

)1/4

, (13)

and the steady-state vertical velocity scale Vm,b at height Zwithin this thermal boundary layer is, from Eq. (7), as follows,

Vm,b ∼κRa1/2Pr1/2

H

(

1−ZH

)1/2

, (14)

or, in dimensionless form,

vm,b =Vm,b

V0∼ [(1− z)Pr]1/2. (15)

The heat transfer across the vertical sidewall is represented bythe following local Nusselt number Nu at height Z,

Nu ∼

[

R0

(T0 −Tw)

∂T∂R

]

R=R0

. (16)

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Therefore, during the start-up stage,

Nu ∼R0

∆T∼

R0

κ1/2t1/2∼

1A

Ra1/4τ−1/2, (17)

and at the steady-state stage,

Nub ∼R0

∆T,b∼

(PrRa)1/4

A(1−Z/H)1/4∼

1A

(

PrRa1− z

)1/4

, (18)

Equations (6), (8), and (17) clearly show that during the start-upstage, the boundary-layer development on the vertical sidewallsis independent of z, however, as shown by (13), (15), and (18),the boundary-layer development and the heat transfer across thevertical sidewall become z dependent at the steady-state stage ofthe boundary-layer development.

Once the boundary layer is fully developed, the fluid in thecylinder is gradually stratified by the cooled fluid ejected fromthe boundary layer, starting from the bottom of the cylinder.The time ts for the full stratification of the whole fluid in thecylinder will be at the moment when the volume of the cooledfluid ejected from the boundary layer is equal to the volume ofthe cylinder. The rate of flow of fluid through the boundarylayer is characterized by ∆T,bVm,b, and therefore the time to fullstratification is characterized by

ts ∼HR0

κRa1/2

(

RaPr

)1/4

, (19)

which is in dimensionless form as follows,

τs =ts

(H/V0)∼

1A

(

RaPr

)1/4

. (20)

After the full stratification, the fluid in the cylinder is contin-ually cooled down until the whole body of fluid has the sametemperature as that imposed on the sidewalls. The appropri-ate parameters to characterize this cooling-down process are thetime t f for the fluid to be fully cooled down, the average fluidtemperature Ta(t) over the whole volume of the cylinder at timet, and the average Nusselt number on the cooling wall.

As the fluid cooling-down is achieved by maintaining a fixedtemperature Tw on the vertical sidewalls while keeping the topand bottom boundaries adiabatic, all the heat used to fully cooldown the fluid in the cylinder must pass through the sidewalls,and then energy conservation in the cylinder requires that,

ρcpVc(T0 −Tw) ∼ t f Ask(T0 −Tw)

∆T,b, (21)

where Vc = πR20H is the volume of the fluid in the cylinder,

As = 2πR0H is the surface area of the sidewall, k is the thermalconductivity of fluid, and ∆T,b is the average thermal boundary-layer thickness which is calculated as follows,

∆T,b =1H

Z H

0∆T,bdZ. (22)

Therefore, t f has the following scaling relation,

t f ∼R0∆T,b

κ∼

R0H

κ(PrRa)1/4, (23)

where κ = k/(ρcp), which is in dimensionless form as follows,

τ f =t f

(H/V0)∼

1A

(

RaPr

)1/4

. (24)

0 0.5 1 1.5 20

0.5

1

1.5

0 0.5 1 1.5 20

0.5

1

1.5

0 5 10 150

5

10

δδ

T

T,b

ττb

ττb

ττb

( )1/2

( )-1/2

vvm,b

m

NuNub

(a)

(b)

(c)

Figure 3: Numerical results for (a) δT /δT,b plotted against(τ/τb)

1/2; (b) vm/vm,b plotted against τ/τb; and (c) Nu/Nub

plotted against (τ/τb)−1/2. solid line, linear fit for the start-up

stage; dashed line, linear fit for the steady-state stage.

The decay of the average fluid temperature Ta(t) is expected toobey an exponential relation[8], that is,

Ta(t)−T0

T0 −Tw= e− f (Ra,Pr,A)t

−1, (25)

where f (Ra,Pr,A) is some function of Ra, Pr, and A, which isin dimensionless form as follows

θa(τ) = e−C f A( PrRa )

1/4τ−1, (26)

where C f is a constant of proportionality which will be deter-mined below by numerical results.

Numerical results

In this section, the scaling relations obtained above will be val-idated and quantified by a series of direct numerical simula-tions with selected values of A, Ra, and Pr in the ranges of1/3 ≤ A ≤ 3, 106 ≤ Ra ≤ 1010, and 0.01 ≤ Pr ≤ 0.5. A to-tal of 12 simulation runs have been carried out for this pur-pose. Specifically, results have been obtained with Ra = 106,107, 108, 109, and 1010, while keeping A = 1 and Pr = 0.1 un-changed, to show the dependence of the scaling relations on Ra(Runs 1-5); the runs with A = 1/3, 1/2, 1, 2, and 3, while keep-ing Ra = 108 and Pr = 0.1 unchanged, have been carried out toshow the dependence on A (Runs 6-7, 3, and 8-9); and the runswith Pr = 0.01, 0.05, 0.1, and 0.5, while keeping Ra = 108 andA = 1 unchanged, have been carried out to show the dependenceon Pr (Runs 10-11, 3, and 12), respectively.

Detailed information about the numerical algorithm, mesh con-struction, initial and boundary conditions, and numerical accu-racy tests can be found in [5, 6].

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0 1 2 3 4 5-1

-0.5

0

Run 1Run 2Run 3Run 4

Run 5Run 6Run 7Run 8Run 9

Run 10Run 11Run 12

0 0.5 1-1

-0.5

0

θ (τ)

θ (τ)a

A(Pr/Ra)1/4τ

a

Exp{-1.142 }A(Pr/Ra)1/4τ

(a)

(b)

Figure 4: Numerical results for θa(τ) plotted against (a)

A(Pr/Ra)1/4τ and (b) e−1.142A(Pr/Ra)1/4τ for all simulation runs.

The numerical results for δT , vm, and Nu at the boundary-layerdevelopment stage are plotted as a ratio with respect to theirsteady-state values against the scaled times τ/τb in Fig. 3. Theresults for τ/τb < 1 fall onto a straight line, confirming the scal-ing laws at the start-up stage, while the results for τ/τb ≥ 1fall onto a horizontal line, confirming the scaling laws at thesteady-state stage. The numerically quantified scaling laws aretherefore as follows,

τb = 2.395

(

1− zPr

)1/2

, (27)

δT,b = 4.845

(

1− zPrRa

)1/4

, (28)

vm,b = 0.872[(1− z)Pr]1/2, (29)

Nub =0.519

A

(

PrRa1− z

)1/4

, (30)

Nub =0.658

A(PrRa)1/4 . (31)

δT = 3.131Ra−1/4τ1/2, (32)

vm = 0.364Pr τ, (33)

Nu =0.803

ARa1/4τ−1/2, (34)

Nu =1.018

ARa1/4τ−1/2. (35)

The numerical results show that τs can be well approximated bythe following expression

τs =0.313

A

(

RaPr

)1/4

. (36)

which clearly demonstrate that the scaling law (20) is correctfor the stratification stage.

The numerical results also show that τ f can be well approxi-

mated by the following expression

τ f =4.031

A

(

RaPr

)1/4

, (37)

where τ f was determined as the time at which θa(τ f ) = −0.99,which clearly demonstrate that the scaling law (24) is correctfor the cooling-down stage. Therefore, the full expression forthe time decay of θa, Eq. (26), is obtained as

θa(τ) = e−1.142A( PrRa )

1/4τ−1. (38)

The numerical results presented in Fig. 4 show that all sets ofdata fall onto a single curve, indicating that the scaling relation(26) is correct.

Conclusions

The cooling down behavior of a fluid contained in a verticalcylinder subjected to isothermal boundary condition on the ver-tical walls is examined via scaling analysis and direct numericalsimulation. Scaling laws have been obtained for the develop-ment time and properties of the initial vertical thermal bound-ary layer, of the stratification time and of the full cooling downtime. The scalings have been obtained for Pr < 1, yielding dif-ferent relations from those obtained for Pr > 1. For instancethe scaling relations for the time development of the bound-ary layer, stratification and full cooling down stages are τb ∼

(1 − z)1/2Pr−1/2, τs ∼ Ra1/4Pr−1/4/A, τ f ∼ Ra1/4Pr−1/4/A

respectively for Pr < 1, and τb ∼ (1 − z)1/2, τs ∼ Ra1/4/A,τ f ∼ Ra1/4/A respectively for Pr > 1 [6]. It is seen that forPr > 1 the scaled quantities are independent of Pr, while forPr < 1 they show a Pr dependency.

Acknowledgements

The financial support of the Australian Research Council, via anAustralian Postdoctoral Fellowship (Grant No. DP0449876),the National Natural Science Foundation of China (Grant No.10262003), and the Natural Science Foundation of YunnanProvince of China (Key Project, Grant No. 2003E0004Z) aregratefully acknowledged.

References

[1] Gebhart, B., Jaluria, Y., Mahajan, R.L. and Sammakia,B., Buoyancy-Induced Flows and Transport, Hemisphere,1988.

[2] Hyun, J.M., Unsteady bouyant convection in an enclosure,Adv. Heat Transfer, 24, 1994, 277–320.

[3] Patterson, J.C. and Imberger, J., Unsteady natural convec-tion in a rectangular cavity, J. Fluid Mech., 100, 1980, 65–86.

[4] Bejan, A., Convection Heat Transfer (2nd Edn.), John Wi-ley & Sons, 1995.

[5] Lin, W. and Armfield, S.W., Direct simulation of naturalconvection cooling in a vertical circular cylinder, Int. J.Heat Mass Transfer, 1999, 42, 4117–4130.

[6] Lin, W. and Armfield, S.W., Natural convection cooling ofrectangular and cylindrical containers, Int. J. Heat FluidFlow, 22, 2001, 72–81.

[7] Lin, W. and Armfield, S.W., Long-term behavior of cool-ing fluid in a rectangular container, Phys. Rev. E, 69, 2004,056315.

[8] Mills, A.F., Heat Transfer (2nd Edn.), Prentice Hall, 1999.


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