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Proceedings of the International Conference on Mechanical Engineering 2011 (ICME2011) 18-20 December 2011, Dhaka, Bangladesh ICME11-FL-039 © ICME2011 1 FL-039 1. INTRODUCTION Many mathematicians, versed engineers and researchers studied the problems of MHD mixed convection for different types of cavity. Amongst them, Oreper and Szekely [2] studied the effect of an externally imposed magnetic field on buoyancy driven flow in a rectangular cavity. They found that the presence of a magnetic field can suppress natural convection currents and that the strength of the magnetic field is one of the important factors in determining the quality of the crystal. Ozoe and Maruo [3] investigated magnetic and gravitational natural convection of melted silicon two-dimensional numerical computations for the rate of heat transfer. Rudraiah et al. [4] investigated the effect of surface tension on buoyancy driven flow of an electrically conducting fluid in a rectangular cavity in the presence of a vertical transverse magnetic field to see how this force damps hydrodynamic movements. At the same time, Rudraiah et al.[5] also studied the effect of a magnetic field on free convection in a rectangular enclosure. The problem of unsteady laminar combined forced and free convection flow and heat transfer of an electrically conducting and heat generating or absorbing fluid in a vertical liddriven cavity in the presence of a magnetic field was formulated by Chamkha [1].Recently, Rahman et al.[6] studied the effect of a heat conducting horizontal circular cylinder on MHD mixed convection in a lid-driven cavity along with Joule Heating. The author considered the cavity consists of adiabatic horizontal walls and differentially heated vertical walls, but it also contains a heat conducting horizontal circular cylinder located somewhere inside the cavity. The results indicated that both the flow and thermal fields strongly depend on the size and locations of the inner cylinder, but the thermal conductivity of the cylinder has significant effect only on the thermal field. Rahman et al.[7] investigated the effect on magnetohydrodynamic (MHD) mixed convection around a heat conducting Horizontal circular cylinder placed at the center of a rectangular cavity along with joule heating. They observed that the streamlines, isotherms, average Nusselt number, average fluid temperature and dimensionless temperature at the cylinder center strongly depend on the Richardson number, Hartmann number and the cavity aspect ratio. Very recently, Rahman et al. [8] made numerical investigation on the effect of magneto hydrodynamic (MHD) mixed convection flow in a vertical lid driven square enclosure including a heat conducting horizontal circular cylinder with Joule heating. The author found that the Hartmann number, Reynolds number and Richardson number have strong influence on the streamlines and isotherms. To the best of our knowledge in the light of the above literatures, it has been pointed out that no work has been paid on MHD mixed convection inside a triangular cavity yet. FINITE ELEMENT ANALYSIS OF MAGNETO-HYDRODYNAMIC (MHD) MIXED CONVECTION FLOW ON A TRIANGULAR CAVITY. Aki Farhana 1 , Mohammed Nasir Uddin 2 , Mohammad Abdul Alim 3 1 Lecturer, Department of Mathematics, Mileston College, Dhaka, 2 Department of Mathematics, Bangladesh University of Business & Technology (BUBT), Dhaka, Bangladesh 3 Department of Mathematics, Bangladesh University of Engineering & Technology (BUET), Dhaka, Bangladesh. ABSTRACT In this paper, the effect of magneto-hydrodynamic (MHD) on mixed convection flow within triangular cavity has been numerically investigate. The bottom wall of the cavity considered as heated. Besides, the left and the inclined wall of the triangular cavity are assumed to be cool and adiabatic. The consequent mathematical model is governed by the coupled equations of mass, momentum and energy and solved by employing Galerkin weighted residual method of finite element formulation. The present numerical procedure adopted in this investigation yields consistent performance over a wide range of parameters Rayleigh number Ra (10 3 -10 4 ), Prandtl number Pr (0.7 - 3) and Hartmann number Ha (5 - 50). The numerical results are presented in terms of stream functions, temperature profile and nussult numbers. It is observed that the Hartmann and Rayleigh number has significant effect on the both flow and thermal fields. Keywords: MHD, Mixed Convection, Triangular Cavity, Finite Element Method And Galerkin Weighted Residual Method.

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Page 1: FINITE ELEMENT ANALYSIS OF MAGNETO ...me.buet.ac.bd/icme/icme2011/Proceedings/PDF/ICME 11-FL...FINITE ELEMENT ANALYSIS OF MAGNETO-HYDRODYNAMIC (MHD) MIXED CONVECTION FLOW ON A TRIANGULAR

Proceedings of the International Conference on Mechanical Engineering 2011

(ICME2011) 18-20 December 2011, Dhaka, Bangladesh

ICME11-FL-039

© ICME2011 1 FL-039

1. INTRODUCTION Many mathematicians, versed engineers and

researchers studied the problems of MHD mixed

convection for different types of cavity. Amongst them, Oreper and Szekely [2] studied the effect of an

externally imposed magnetic field on buoyancy driven

flow in a rectangular cavity. They found that the

presence of a magnetic field can suppress natural

convection currents and that the strength of the

magnetic field is one of the important factors in

determining the quality of the crystal. Ozoe and Maruo

[3] investigated magnetic and gravitational natural

convection of melted silicon two-dimensional

numerical computations for the rate of heat transfer.

Rudraiah et al. [4] investigated the effect of surface tension on buoyancy driven flow of an electrically

conducting fluid in a rectangular cavity in the presence

of a vertical transverse magnetic field to see how this

force damps hydrodynamic movements. At the same

time, Rudraiah et al.[5] also studied the effect of a

magnetic field on free convection in a rectangular

enclosure. The problem of unsteady laminar combined

forced and free convection flow and heat transfer of an

electrically conducting and heat generating or

absorbing fluid in a vertical liddriven cavity in the

presence of a magnetic field was formulated by Chamkha [1].Recently, Rahman et al.[6] studied the

effect of a heat conducting horizontal circular cylinder

on MHD mixed convection in a lid-driven cavity along

with Joule Heating. The author considered the cavity

consists of adiabatic horizontal walls and differentially

heated vertical walls, but it also contains a heat

conducting horizontal circular cylinder located

somewhere inside the cavity. The results indicated that both the flow and thermal fields strongly depend on the

size and locations of the inner cylinder, but the thermal

conductivity of the cylinder has significant effect only

on the thermal field. Rahman et al.[7] investigated the

effect on magnetohydrodynamic (MHD) mixed

convection around a heat conducting Horizontal

circular cylinder placed at the center of a rectangular

cavity along with joule heating. They observed that the

streamlines, isotherms, average Nusselt number,

average fluid temperature and dimensionless

temperature at the cylinder center strongly depend on the Richardson number, Hartmann number and the

cavity aspect ratio. Very recently, Rahman et al. [8]

made numerical investigation on the effect of magneto

hydrodynamic (MHD) mixed convection flow in a

vertical lid driven square enclosure including a heat

conducting horizontal circular cylinder with Joule

heating. The author found that the Hartmann number,

Reynolds number and Richardson number have strong

influence on the streamlines and isotherms.

To the best of our knowledge in the light of the above

literatures, it has been pointed out that no work has been paid on MHD mixed convection inside a

triangular cavity yet.

FINITE ELEMENT ANALYSIS OF MAGNETO-HYDRODYNAMIC

(MHD) MIXED CONVECTION FLOW ON A TRIANGULAR CAVITY.

Aki Farhana1, Mohammed Nasir Uddin

2, Mohammad Abdul Alim

3

1Lecturer, Department of Mathematics, Mileston College, Dhaka,

2Department of Mathematics, Bangladesh University of Business & Technology (BUBT), Dhaka,

Bangladesh 3Department of Mathematics, Bangladesh University of Engineering & Technology (BUET), Dhaka, Bangladesh.

ABSTRACT In this paper, the effect of magneto-hydrodynamic (MHD) on mixed convection flow within triangular

cavity has been numerically investigate. The bottom wall of the cavity considered as heated. Besides, the

left and the inclined wall of the triangular cavity are assumed to be cool and adiabatic. The consequent

mathematical model is governed by the coupled equations of mass, momentum and energy and solved by

employing Galerkin weighted residual method of finite element formulation. The present numerical

procedure adopted in this investigation yields consistent performance over a wide range of parameters

Rayleigh number Ra (103-104), Prandtl number Pr (0.7 - 3) and Hartmann number Ha (5 - 50). The

numerical results are presented in terms of stream functions, temperature profile and nussult numbers. It

is observed that the Hartmann and Rayleigh number has significant effect on the both flow and thermal

fields.

Keywords: MHD, Mixed Convection, Triangular Cavity, Finite Element Method And Galerkin

Weighted Residual Method.

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© ICME2011 FL-039

2

2. PHYSICAL MODEL AND ASSUMPTIONS

The physical model considered here is shown in

Fig.-1, along with the important geometric parameters. The heat transfer and the fluid flow in a two-

dimensional triangular cavity with MHD flow whose

left wall and bottom wall are subjected to cold Tc and

hot Th temperatures respectively while the inclined

walls are kept adiabatic. The fluid was assumed with

Prandtl number (Pr = 0.71, 1.0, 7.0) and Newtonian,

and the fluid flow is considered to be laminar. The

properties of the fluid were assumed to be constant.

Fig1. Schematic diagram of the square open cavity

3. MATHEMATICAL MODEL

The fundamental laws used to solve the fluid flow

and heat transfer problems are the conservation of mass

(continuity equations), conservation of momentums (momentum equations), and conservation of energy

(energy equations), which constitute a set of coupled,

nonlinear, partial differential equations. For laminar

incompressible thermal flow, the buoyancy force is

included here as a body force in the v-momentum

equation. The governing equations for the two-

dimensional steady flow after invoking the Boussinesq

approximation and neglecting radiation and viscous

dissipation then the governing equations in non-

dimensional form are written as follow:

0

Y

V

X

U…… …(1)

2 2

2 2

1U U P U UU V

X Y X Re X Y

…(2)

VHa

RaY

V

X

V

Y

P

Y

UV

X

UU

RePr)(

Re

1 2

2

2

2

2

…(3)

2 2

2 2

1U V

X Y Re Pr X Y

…(4)

With the boundary conditions

The dimensionless boundary conditions under

consideration can be written as:

At the left vertical wall: 0

At the bottom wall: 1

At the inclined wall: 0

N

Where N is the non-dimensional distances either along

X or Y direction acting normal to the surface and K is

the dimensionless thermal conductivity. According to

Singh and Sharif (2003), the average Nusselt number at

the heated wall of the cavity based on the non-

dimensional variables may be expressed as

0

L Lh

Nu dYX

and the bulk average

temperature defined as /av dV V , where V is

the cavity volume.

The above equations were normalized using the

following dimensionless scales:

L

xX

L

yY

00 U

vV

U

uU

Pr

Pr,,,Pr,Re22

02

2

3

GrRaLB

HaTLg

GrLui

p

chC

andTTT

4. NUMERICAL ANALYSIS

The governing equations along with the boundary

conditions are solved numerically by employing

Galergkin weighted residual finite techniques. The

finite element formulation and computational procedure are omitted herein for brevity.

5. RESULTSAND DISCUSSION

The MHD mixed convection flow and temperature

fields as well as heat transfer rates and bulk

temperature inside the triangular cavity has been numerically investigated. The MHD mixed convection

phenomenon inside the enclosure is strongly influenced

by governing as well as physical parameters, namely

and Hartman number Ha,Reynolds number Re, Prandtl

number Pr, Rayleigh number Ra. As the nature of flow

and thermo physical properties of fluid strongly

influenced on the heat transfer rate, and the numerical

computation were performed for a range of Ha, Re and

Pr (Ha=0.0-50, Re= 40-100, Pr=0.71-6). In addition,

for each value of mentioned parameters, computations

are performed at Ra =5103 that focuses on pure

mixed convection. Moreover, the results of this study are presented in terms of streamlines and isotherms.

Furthermore, the heat transfer effectiveness of the

enclosure is displayed in terms of average Nusselt

number Nu and the dimensionless average bulk

temperature. Obviously for high values of Ra number the errors

encountered are appreciable and hence it is necessary

to perform some grid size testing in order to establish a

suitable grid size. Grid independent solution is ensured

by comparing the results of different grid meshes for

B0

Adiabatic

Th

Tc

X

Y

g

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© ICME2011 FL-039

3

Ra = 105, which was the highest Grashof number. The

total domain is discretized into 41520 elements that

results in 62280 nodes. In order to validate the

numerical code, pure natural convection with Pr = 0.71

in a square open cavity was solved and the average

Nusselt numbers is presented by graphically. The

results were compared with those reported by Basak et

al., obtained with an extended computational domain.

In Table1, a comparison between the average Nusselt numbers is presented. The results from the present

experiment are almost same as Basak et.al.

Table 1: Comparison of the results for the constant

surface temperature with Pr = 0.71.

Ra

Nuav

Present

work

Basak et al.

(2007)

103 5.49 5.40

104 5.77 5.56

105 7.08 7.54

5.1 Effects of Reynolds Number (Re) The effects of Reynolds number on the flow structure

and temperature distribution are depicted in Fig. 2.7. The streamlines are presented for different values of

Rayleigh numbers (Ra), Reynolds numbers (Re)

ranging from 103 to 104 and 40 to 100 respectively

while Pr = 0.71, and Ha=20. Now at Re = 40, the fluid

near to the hot (bottom) wall has lower density, so it

moves upward while the relatively heavy fluid near to

cold (left) wall and this fluid is heated up. Thus the

fluid motion completes the circulation. Using the

definition of stream function, the streamlines with +

correspond to anti-clockwise circulation, and those

with − correspond to clockwise circulation. A very

small magnitude value of contour rotating cell is

observed in the middle part of the cavity as primary

vortex. The secondary vortex cell are shown around the

primary vortex in the cavity. The secondary vortex are

more packed to the respective wall dramatically for the

increasing value of Re that’s imply the flow moves

faster and the velocity boundary layer become thinner.

Moreover, it is clearly seen that the center vortex become bigger with increasing Re due to conduction

intensified gradually. The value of the magnitudes of

the stream function greater due to mechanically driven

circulations.

The corresponding isotherm pattern for different

value of Reynolds number while Pr = 0.71 and Ha=20

is shown in the Fig. 2. From this figure, it is found that

the isotherms are more congested at the heated wall of

the cavity testifying of the noticeable increase in

convective heat exchange. The temperature gradients

are very small due to mechanically driven circulations at the left wall of the cavity. It is also noticed that the

thermal boundary layer near the heated wall becomes

thinner with increasing Re. Due to high circulations,

the temperature contours condensed in a very small

regime at the upper portion of the left wall and this

may cause greater heat transfer rates at the heated wall.

The effects of Reynolds number on average Nusselt

number Nu at the heated wall and the average bulk

temperature av of the fluid in the cavity are illustrated

in Fig 4 &5, while Pr = 0.71, Ha=20. From Fig.4(i), it

is seen that the average Nusselt number Nu increases

steadily with increasing Rayleigh number. This arises

from the fact that physical properties of fluid changes

to better heat transfer. For Re = 100, it is noticed that

the average Nusselt number Nu increases sharply but

for lower values of Re (= 40) then the increase of Nu befall slower.

Fig. 5 displays the variation of the average bulk

temperature against the Rayleigh number for various

Reynolds numbers. The average temperature decreases

smoothly with increase of Ra. It is an interesting

observation that at lower Re, the average bulk

temperature is affected by Rayleigh number.

Ra= 103 Ra= 5×10

3 Ra= 10

4

296.91

300.00

302.57

305.00

310.0

0

315.00

318.52

295.00290.00

28

5.0

02

80

.00

28

0. 0

0

295.00

296.20298.13

300.00

302.00

303.94

305.00

310.0

0

315.00290.00

28

5.0

02

85

.00

295.00

297.20

299.19

300.00

302.00303.45

305.00

310.0

0

315.00290.00

28

5.0

02

85

.00

28

0. 0

0

295.00

296.20298.13

300.00

302.00

303.94

305.00

310.0

0

315.00290.00

28

5.0

02

85

.00

295.00

296.90

297.85

299.38

300.00

302.38

305.00

310.0

0

315.00290.00

29

0.0

02

85

. 00

28

0.0

0

295.00

296.98

298.65

299.54

300.00

302.39

305.00

310.0

0

310.00290.00

29

0.0

02

80

. 00

295.00

297.20

299.19

300.00

302.00303.45

305.00

310.0

0

315.00290.00

28

5.0

02

85

.00

28

0. 0

0

295.00

296.36

297.52

298.45

299.33

300.00

302.19

305.00

310.0

0

315.00290.00

29

0.0

02

85

.00

295.00

296.44

298.04

299.09

299.56

300.00

302.10

305.00

310.00315.00

290.00

28

0.0

0

Fig 2:Isotherms patterns for different Re

(40,70,100)when Pr = 0.71 and Ha=20

0.50

1.00

2.00

2.50

3.50 5.00

6.50

6.00

2.504.50

5.506.00

2.00

1.0

0

0.503.00

6.5

04

.00

3.5

0

2.50

2.00

1.50

3.0

0

1.00

2.00

4.00

8.00

10.00

14.00

16.0016.00

1.003.00

10.0013.009.00

5.0

0

6.0

0

7.00

7.0

017.0

013.0

0

12.00

3.0

0

2.00

4.00

8.00

10.00

16.00

20.00

22.0

0

24.00

10.0014.00 18.00

24.00

22

.00

16

.00

10

. 00

20

.00

2.0

0

4.00 2.00

2.0

0

0.50

1.00

2.00

2.504.00

5.00

6.50

7.00

3.005.00

6.50

4.0

02

.50

6.0

02.0

0

1.00

2.00 0.50

5.00

1.00

2.00

3.00

6.00

11.00

11.00

13.00

5.00

2.0011.0011.00

17.00

8.0

0

6.0

0

8.0

01

3.0

03

.00

7.00

18

.00

2.00

2.006.00

10.0016.00

20.00

22.00

24.00

10.006.00

10.0020.00 8.00 2.00

4.00

2.0

01

0.0

0

16

.00

14

.00

8.0

01

8.0

0

4.00

0.50

1.00

3.003.00

5.507.00

7.5

0

4.5

04

.50

3.50

3.5

0

1.5

0

2.00

4.00

6.00

7.00

4.502.50

1.00

1.50 2.00

4.00

10.00

14.00

14.00

16.00

4.0

0

2.008.0010.00

18.00 10.00

18

.00

10

.00

10

.00

6.0

0

2.00

2.00

2.0

0

2.00

10.0014.00

14.00

22.00

14.00

2.0010.00

16.0022.00

14.0

0

6.0

0

16

.00

10

.00

8.0

0

2.00

Fig 3:Streamlines patterns for different Re(20,70,100)

when P = 0.71and Ha=20

Re=

40

Re=

10

0

Re=

70

Re=

70

Re=

100

Re=

40

Page 4: FINITE ELEMENT ANALYSIS OF MAGNETO ...me.buet.ac.bd/icme/icme2011/Proceedings/PDF/ICME 11-FL...FINITE ELEMENT ANALYSIS OF MAGNETO-HYDRODYNAMIC (MHD) MIXED CONVECTION FLOW ON A TRIANGULAR

© ICME2011 FL-039

4

Ra

Nu

2000 4000 6000 8000 10000

3

4

5

6

7

8

9

10

11

12

13

Re= 40

Re= 50

Re= 70

Re= 100

Fig-4: Effect of average Nusselt number and Rayleigh

number while Pr = 0.71, Ha = 20.

Ra

?a

v

2000 4000 6000 8000 10000

0.1495

0.15

0.1505

0.151

Re= 40

Re= 50

Re=70

Re= 100

Fig.-5: Effect of average bulk temperature and Rayleigh number while Pr = 0.71, Ha = 20.

5.2 Effect of Prandtl Number (Pr) The effects of Prandtl number on flow fields for the

considered Ra is depicted in Fig.6&7, while Re = 50

and Ha=20 are kept fixed. Now, from the figure, it seen

that a small vortex is formed at the center of the cavity.

It is evident that the size of the vortex is increased with

the increasing value of Pr. The influence of Prandtl

number Pr on thermal fields for the selected value of

Ra is displayed in Fig.6 for Re = 50 and Ha=20. As

expected, the thermal boundary layer decreases in

thickness as Pr increases. This is reflected by the denser deserting of isotherms close to the heated wall

and cooled wall as Pr increases. The spread of

isotherms at low values of Pr is due to a strong stream

wise conduction that decreases the stream wise

temperature gradient in the field. At the increase of Pr

the isotherms become linear in the cavity and

impenetrable to respective wall. From the Fig. 6, it can

easily be seen that the isotherms for different values of

Pr at Ra = 104 are clustered near the heated horizontal

wall and cooled vertical heated surface of the

enclosure, indicating steep temperature gradient along the vertical direction in this region. Besides, the

thermal layer near the heated wall becomes thinner

moderately with increasing Pr.

The effects of Prandtl number on average Nusselt

number Nu at the heated surface and average bulk

temperature av in the cavity is illustrated in Fig. 8 & 9

with Re =50 and Ha=20. From this figure, it is found

that the average Nusselt number Nu goes up

penetratingly with increasing Pr. It is to be highlighted

that the highest heat transfer rate occurs for the highest

values of Pr (= 6). The average bulk temperature of the fluid in the cavity declines very mildly for higher

values of Pr (0.71- 6.0). But for the lower values of Pr,

the average bulk temperature is linear. It is to be

mentioned here that the highest average temperature is

documented for the lower value of Pr (=0.71) in the

free convection dominated region.

Ra= 103 Ra= 5×103 Ra= 104

295.00

297.58

300.00

301.70

303.35

305.00

310.0

0

315.00

290.00

28

5.0

02

80

.00

295.00

297.66

299.21300.00

300.78

302.42 303.22

305.00

310.00

315.00290.00

29

0.0

02

80

. 00

295.00

297.05

298.18

299.39

300.00

300.99

302.91

305.00

310.0

0

315.00290.00

28

5.0

0

28

0.0

0

290.00

292.12

294.06

295.00

296.36

297.19

297.98300.00

305.00

315.00310.00

290.0

02

85

.00

290.00

291.90

293.62

295.00

296.01

296

.37

298.33

296.37

305.00315.00

29

0.0

0

27

5.0

0

290.00

292.10

293.41

294.26

295.00

295.94

297.45

300.00

305.00315.00

28

5.0

02

80

. 00

290.00

292.29

293.16

294.18

295.00

295.79

296.41

298.42

295.79

310.00310.00

28

5.0

02

85

. 00

290.00

291.31

292.60

293.48

294.44

295.00

296.62

296.62310.00

29

1.3

1

290.00

290.87

291.98

292.69

293.51

294.27

295.00

300.00285.00

29

1.9

8

Fig-6:Isotherms patterns for different Pr (0.71,3.0,6.0)

when Re = 50 and Ha=20

0.50

1.00

2.00

2.00

3.50

5.00 6.50

1.50

0.5

0

3.505.00

6.50

4.00

1.50

3.0

0

3.00

3.0

06

.50

6.50

2.00 0.50

2.00

4.00

6.00

10.00

12.00

14.00

16.00

6.0010.0012.00

16.00

16

.00

14

.00

12.0

04

.00

2.0

0

4.0

0

2.008.00

2.00

4.00

6.00

10.00 16.0020.00

24.00

24.00

22.00

20.00

16.0012.00

2.00

2.006.006.002

6.0

01

8.0

01

2.0

08

.00

22

.00

0.50

1.00

2.00

3.50

4.00

6.50

8.50

1.502.00 3.00

3.50 1.5

0

4.504.00

2.0

02

.00

6.0

03.0

03.0

08.5

0

3.50

2.002.00

4.006.0010.00

16.

00

8.00

10.00

12.00

14.00

12.00

14

.00

14

.00

14

.00

2.0

0

2.002.00 4.00

8.0018.00

10.0010.00

14.00

16.00

20.00

16.00

14

.00

26

.00

2.0

0

16

.00

4.0

0

0.501.50

2.5

0

4.50

5.50

6.50

7.00

2.002.503.504.00

3.5

0

1.5

06

.50

3.0

0

4.502.00

4.006.00

12

.00

6.0

01

6.0

0

2.006.00

12.00

14.00

10

.00

16.002.00 4.00

6.00 8.00

8.00

6.00

14.00

20.00

20.00

8.0

01

2.0

0

4.0

06

.00

Fig-7:Streamline patterns for different Pr (0.71,3,6)

when Re = 50 and Ha=20

Pr=

0.7

1

Pr=

6.0

P

r=3

.0

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Fig 8: Effect of average Nusselt number and Rayleigh

number while Re = 50 and Ha=20

Fig 9: Effect of average bulk temperature and Rayleigh

number while Re = 50 and Ha=20.

5.3 Effects of Hartmann Number The influences of Hartmann number Ha on the flow

and thermal fields at Ra= 1e3 to 1e4 is

illustrated in Figure 10& 11, while Pr = 0.71 and Re =

50 are kept fixed. In absence of the magnetic field Ha

(= 0.0), a remarkable strong vortex is found near the

center of the cavity. In this folder, the size of the

counter clockwise vortex also decreases sharply with

increasing Ha. This is because application of a

transverse magnetic field has the tendency to slow

down the movement of the buoyancy induced flow in the cavity. The effects of Hartmann number Ha on

isotherms are shown in the Figure 10 while Re = 50

and Pr = 0.71 are kept fixed. In absences of magnetic

field Ha = 0.0), it is observed that the higher values

isotherms are more tightened at the vicinity of the

heated wall of the cavity for the considered value of

Ra. A similar trend is found for the higher values of

Ha. From this figure it can easily be seen that

isotherms are almost parallel at the vicinity of the

bottom horizontal hot wall but it changes to parabolic

shape with the increasing distance from inclined wall

for the highest value of Ha (=20.0) at Pr=0.71, indicating that most of the heat transfer process is

carried out by conduction. In addition, it is noticed that

the isothermal layer near the heated surface becomes

slightly thin with the decreasing Ha. However in the

remaining area near the left wall of the cavity, the

temperature gradients are small in order to

mechanically driven circulations. The effects of Ha on

average Nusselt number Nu at the heated surface and

average bulk temperature av in the cavity is illustrated

in Fig. 12 &13 with Re =50 and Pr =0.71. From this

figure, it is found that the average Nusselt number Nu

decreases with increasing Pr. It is to be highlighted that

the highest heat transfer rate occurs for the lowest values of Ha (= 5). The average bulk temperature of

the fluid in the cavity is high for higher values of Ha (0

- 6.0). It is to be mentioned here that the highest

average temperature is documented for the higher value

of Ha in the free convection dominated region.

Ha= 0.0 Ha= 20.0 Ha= 50.0

Fig10:Isotherm patterns for different Ha

(00,20.0,50.0) when Re = 50 and Ra=103

Fig11:Stream line patterns for different Ha

(00,20.0,50.0) when Re = 50 and Ra=103

Ra

Nu

2000 4000 6000 8000 10000

4

5

6

7 Ha= 5

Ha= 10

Ha= 20

Ha= 50

Fig.12: Effect of average Nusselt number and Rayleigh

number while Pr = 0.71 and Re = 50.

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Fig.13: Effect of average bulk temperature and

Rayleigh number while Pr = 0.71and Re = 50

7. CONCLUSION A finite element method for steady-state

incompressible conjugate effect of mixed convection

and conduction has been presented. The finite element

equations were derived from the governing flow

equations that consist of the conservation of mass,

momentum, and energy equations. The derived finite

element equations are nonlinear requiring an iterative

technique solver. The Galerkin weighted residual

method is applied to solve these nonlinear equations

for solutions of the nodal velocity components, temperatures, and pressures. The above example

demonstrates the capability of the finite element

formulation that can provide insight to steady-state

incompressible conjugate effect of mixed convection

and conduction problem.

8. NOMENCLATURE

Symbol Meaning Unit

g gravitational

acceleration

(ms–2)

Gr Grashof

number

Ha Hartmann

Number

Re Reynolds

Number

Ra Rayleigh

Number

k thermal

conductivity of

the fluid

(Wm-1K1)

L hight and width

of the

enclosure

(m)

Nu Nusselt number

P pressure

(Nm–2)

Pr Prandtl

number, υ/α

q heat flux

(Wm–2)

T temperature

(K)

x, y Cartesian

coordinates

(m)

X, Y non-

dimensional

Cartesian

coordinates

θ dimensional

temperature

u, v velocity

components

(ms–1)

α thermal

diffusivity

(m2s–1)

β thermal

expansion

coefficient

(K–1)

ρ density of the fluid

(kgm–3)

υ kinematic visc

osity of the

fluid

(m2s–1)

9. REFERENCES

[1] Chamkha, A. J., “Hydromagnetic combined

convection flow in a vertical lid-driven cavity with

internal heat generation or absorption”, Numer.

Heat Transfer, Part A,Vol. 41, pp. 529-546, 2002.

[2] Oreper, G. M., Szekely, J., “The effect of an

externally imposed magnetic field on buoyancy

driven flow in a rectangular cavity”, J. of Crystal

Growth, Vol. 64, pp. 505-515, 1983.

[3] Ozoe, H., and Maruo, M., “Magnetic and

gravitational natural convection of melted silicon-

two dimensional numerical computations for the

rate of heat transfer”, JSME, Vol. 30, pp. 774-784,

1987.

[4] Rudraiah, N., Venkatachalappa, M., and Subbaraya,

C. K., “Combined surface tension and buoyancy-

driven convection in a rectangular open cavity in

the presence of magnetic field”, Int. J. Non-linear

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© ICME2011 FL-039

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Mech., Vol. 30(5), pp. 759-770, 1995a.

[5] Rudraiah, N., Barron, R. M., Venkatachalappa, M.,

and Subbaraya, C. K., “Effect of magnetic field on free convection in a rectangular enclosure”, Int. J.

Engng. Sci., Vol. 33, pp. 1075-1084, 1995b.

[6] Rahman, M.M., Mamun M.A.H., Saidur, R., and

Nagata Shuichi, “Effect Of a Heat Conducting

Horizontal Circular Cylinder on MHD Mixed

Convection In A Lid- Driven Cavity Along With Joule Heating”, Int. J. of Mechanical and Materials

Eng. (IJMME), Vol. 4, No. 3, pp.256-265, 2009a.

[7] Rahman, M. M., Alim, M. A., Chowdhury, M. K.,

“Megnetohydrodynamic mixed convection around

a heat conducting horizontal circular cylinder in a

rectangular liddriven cavity with Joule heating”, J. Sci Res. I (3), pp.461-472, 2009b

[8] Rahman, M. M., Alim, M. A., “MHD mixed

convection flow in a vertical lid-driven square

enclosure including a heat conducting horizontal

circular cylinder with Joule heating”, Nonlinear

Analysis: Modeling and Control, Vol 15, No. 2,

pp.199-211, 2010.

9.MAILING ADDRESS

Mohammad Abdul Alim

Department of Mathematics, Bangladesh University of Engineering & Technology (BUET), Dhaka, Bangladesh.

Email: [email protected]