http://dx.doi.org/10.4236/ajcm.2016.62009
Group Method Analysis of MHD Mixed
Convective Flow Past on a Moving Curved
Surface with Suction
Dipika Rani Dhar
1, Mohammad Abdul Alim
2, Laek Sazzad Andallah
31Department of Mathematics, Gouripur M.F.R. Government College, Comilla, Bangladesh
2Department of Mathematics, Bangladesh University of Engineering and Technology, Dhaka, Bangladesh 3Department of Mathematics, Jahangirnagar University, Dhaka, Bangladesh
Received 23 February 2016; accepted 6 June 2016; published 9 June 2016
Copyright © 2016 by authors and Scientific Research Publishing Inc.
This work is licensed under the Creative Commons Attribution International License (CC BY).
http://creativecommons.org/licenses/by/4.0/
Abstract
The group-theorytic approach is applied for solving the problem of the unsteady MHD mixed con-vective flow past on a moving curved surface. The application of two-parameter groups reduces the number of independent variables by two, and consequently the system of governing partial differential equations with boundary conditions reduces to a system of ordinary differential equa-tions with appropriate boundary condiequa-tions. The obtained ordinary differential equaequa-tions are solved numerically using the shooting method. The effects of varying parameters governing the problem are studied. A comparison with previous work is presented.
Keywords
Moving Curved Surface, MHD Flow, Two-Parameter Group-Theory Method, Buoyancy Parameter, Suction
1. Introduction
fluid past a stationary body. This flow regime is concerned with circumstances where in both the natural and forced mechanisms of the flow must be considered simultaneously. The laminar boundary layer flow due to such combined forced and natural convection i.e. mixed convection has received considerable attention for steady and unsteady situations in evaluating flow parameters for technical purposes. The problem of mixed convective boundary layer flow gained different dimensions in the manufacturing processes in industry. There has been great interest in the study of Magnetic Hydro-Dynamic (MHD) flow due to the effect of magnetic fields on the boundary layer flow control and on the performance of many systems using electrically conducting fields. This type of flow has attracted the interest of many researchers due to its applications in many engineering problems such as MHD generators, plasma studies, nuclear reactors, geothermal energy extraction etc.
Sparrow, Eichorn and Gregg [1], were the first investigators, who dealt with the combined forced and free convective boundary layer flow about a vertical flat plate. The laws governing the motion of mixed convective boundary layer incompressible viscous fluid expressed in general orthogonal curvilinear co-ordinates are re-cently studied by Maleque [2]. Quiser Azam [3] studied mixed convection about the vertical developable flow surfaces with transpiration and heat flux effects. “Mixed convection boundary layer flow over a permeable ver-tical cylinder with prescribed surface heat flux” studied by Anuar Is hak et al.[4]. M.Y. Ali et al.[5] investi-gated similarity solutions for unsteady laminar boundary layer flow around a vertical heated curvilinear surface. Zakerullah [6] derived similarity solutions of some of possible cases of unsteady mixed convection by group theory without suction. Alam et al. [7] investigated “Magnetohydrodynamic free convection along a vertical wavy surface. S.M.M. EL-Kabeir et al. [8] studied Unsteady MHD combined convection over a moving vertical sheet in a fluid saturated porous medium with uniform surface heat flux. Dipika Rani Dhar [9] studied group- theory method on similarity solution of unsteady free convection flow from a moving vertical surface with suc-tion and injecsuc-tion.
The mathematical technique used in the present analysis is two-parameter group transformation that leads to a similarity representation of the problem. Morgan [10] presented a theory that led to improvements over earlier similarity methods. Michal [11] extended Morgan’s theory. Group methods, as a class of methods which lead to a reduction of the number of independent variables, were first introduced by Birkoff [12]. He made use of one parameter group transformations to reduce a system of partial differential equations in two independent va-riables to a system of ordinary differential equations in one independent variable, the similarity variable. Morgan and Gaggioli [13] presented general systematic group formalism for similarity analysis, where a given system of partial differential equations was reduced to a system of ordinary differential equations.
In this work, the effect of MHD mixed convective flow past on a moving curved surface has been investigated. Problems are solved analytically using group methods and then numerically by Runge-Kutta shooting method. Under the application of two-parameter group, the governing partial differential equations are reduced to system of ordinary differential equations with the appropriate boundary conditions and then numerically using the sixth order Runge-Kutta shooting method known as Runge-Kutta-Butcher initial value solver of Butcher [14] together with the Nachtsheim-Swigert iteration scheme described by Nachtsheim and Swigert [15]. Programming codes have been written in FORTRAN 90 to implement shooting method for the present problem.
Attention has been taken on the evaluation of the velocity profiles as well as temperature profiles for selected values of parameters consisting ,magnetic parameter M, Prandtl number Pr, buoyancy parameter λ1 and suction parameter Ew. The numerical results of the velocity profiles as well as temperature profiles are displayed
graph-ically for different values of magnetic parameter M, Prandtl number Pr, buoyancy parameter λ1 and suction pa-rameter Ew. The post processing software TECPLOT has been used to display the numerical results. A
compari-son with previous work is presented.
2. Governing Equations
We consider the flow direction along the ξ-axis and η-axis and be defined in the surface over which the boun-dary layer is flowing. For simplicity h3
(
ξ η,)
=1 has been set such that ζ represents actual distance measured normal to the surface. The body force is taken as the gravitational force g g(
ξ(
ξ η, ,)
gη(
ξ η, ,0)
)
. The physical configuration is considered as shown in Figure 1.Figure 1. Physical model and co-ordinate system.
( )
h u2( )
h v1(
h h w1 2)
0ξ η ζ
∂ + ∂ + ∂ =
∂ ∂ ∂ (1)
Momentum equations
(
)
2
1 2
2
1 2 1 2 1 2 1
2 2
1 2
2
1 2 1 2 1 2 1 2
0
T e
e e e e e e e
e
g TL U
h h
u u u v u w u uv v
t h h h h h h hU t
U U V U U V h V h u M u U
h h h h h h h h
ξβ θ
ξ η ζ η ξ
ξ η η ξ ζ
∆ ∂ ∂ ∂ ∂ + ∂ + ∂ + ∂ + − + − ∂ ∂ ∂ ∂ ∂ ∂ ∂ ∂ ∂ ∂ ∂ ∂ − − − + − + − = ∂ ∂ ∂ ∂ ∂ (2)
(
)
2 2 1 21 2 1 2 1 2 2
2 2
2 1
2
1 2 1 2 1 2 1 2
0
T e
e e e e e e e
e
g TL V
h h
v u v v v w v uv u
t h h h h h h h U t
U V V V U V h U h v M v V
h h h h h h h h
ηβ θ
ξ η ζ ξ η
ξ η ξ η ζ
∆ ∂ ∂ ∂ ∂ ∂ ∂ ∂ + + + + − + − ∂ ∂ ∂ ∂ ∂ ∂ ∂ ∂ ∂ ∂ ∂ ∂ − − − + − + − = ∂ ∂ ∂ ∂ ∂ (3) Energy equation
(
)
(
)
(
)
221 2 1 2
ln ln ln 0
u v w T u T v T
t h h t h h Pr
θ θ θ θ θ ν θ
ξ η ζ ξ η ζ
∂ ∂ ∂ ∂ ∂ ∂ ∂ ∂
+ + + + ∆ + ∆ + ∆ − =
∂ ∂ ∂ ∂ ∂ ∂ ∂ ∂ (4)
With initial and boundary conditions
(
)
(
) (
)
(
)
(
)
00(
) (
)
00(
)
0, , , , , , 0, , , , , ,
0, , , , , , 0, , , , ,
u u v v
w w
ξ η ζ ξ η ζ ξ η ζ ξ η ζ
ξ η ζ ξ η ζ θ ξ η ζ θ ξ η ζ
= =
= = (5)
(
)
(
)
(
)
(
)
(
)
(
)
(
)
0
, , ,0 1, , , ,0 0, , , ,0 , , , ,0 1 at 0
and , , ,0 e, , , ,0 e, , , ,0 0 at
w
u t v t w t t
U
u t U v t V t
ξ η ξ η ξ η θ ξ η ζ
ξ η ξ η θ ξ η ζ
= = = − = =
= = = → ∞
where
1 1
2 2
, , , , , , , e, e, ,
e e
w
U V T T
t u v w
t U Re u v w Re U V
L L L L U U U U U T T
ξ η ζ
ξ η ζ θ ∞
∞ ′ ′ ′ ′ ′ ′ ′ ′ ′ − = = = = = = = = = = − 2 2 0 0B L M
Re
σ µ
= is
the magnetic parameter; B0 is the magnetic induction; p
c Pr
k
µ
= is the Prandtl number of the fluid; α is the thermal diffusivity.
From the continuity Equation (1), there exists two stream functions ψ
(
t, , ,ξ η ζ)
and φ ξ η ζ(
t, , ,)
such that(
)
2 , 1 , 1 2
h u h v h h w
ζ ζ ξ η
ψ = Φ = − ψ + Φ =
η
Applying h1 = 1 and h2 = ξ in Equations (2)-(4) we have
2 2
2 2 2 2 2
2 2
2 2
3 3
3 3 2 2 2 2 2
2 3 0
T e e e
e e e e
e
t
g L T U U U V U V M MU
t U
ξ
ψ ψ ψ ψ φ ψ ψ ψ φ ψ φ
ξ ξ ξ ξ ξ ξ
ζ ζ ξ ζ ζ ζ η ζ ξ ζ η ζ ζ
ξ β θ ξ ξ ξ ξ ξ ψ ξ ψ ξ
ξ η ζ ζ
∂ + ∂ ∂ − ∂ + ∂ ∂ − ∂ ∂ − ∂ ∂ − ∂
∂ ∂ ∂ ∂ ∂ ∂ ∂ ∂ ∂ ∂ ∂ ∂ ∂ ∂
∆ ∂ ∂ ∂ ∂ ∂
+ − − − + − + − =
∂ ∂ ∂ ∂ ∂
(6)
2 2 2 2 2
3 2 2 2 2 2
2 2 2
2 3
3 3 2 2 3 2 2
2 3 0
T e e e
e e e e e
t
g L T V U V V V U V M M V
t U
η
φ ψ φ φ φ φ φ ψ φ φ φ φ ψ
ξ ξ ξ ξ ξ ξ ξ
ζ ζ ξ ζ η ζ ζ η ξ ζ η ζ ζ ζ
ξ β θ ξ ξ ξ ξ ξ φ ξ φ ξ
ξ η ζ ζ
∂ ∂ ∂ ∂ ∂ ∂ ∂ ∂ ∂ ∂ ∂ ∂ ∂
+ − + − − +
∂ ∂ ∂ ∂ ∂ ∂ ∂ ∂ ∂ ∂ ∂ ∂ ∂ ∂ ∂
∆ ∂ ∂ ∂ ∂ ∂
+ − − − − − + − =
∂ ∂ ∂ ∂ ∂
(7)
( )
( )
( )
2
2
2
T T T
t T t
Pr
θ ψ θ φ θ ψ φ θ θ ψ φ
ξ ξ
ζ ξ ζ η ξ η ζ ζ ξ ζ η
ξ θ
ζ
∂ +∂ ∂ +∂ ∂ − ∂ +∂ ∂ + ∂ ∆ +∂ ∂ ∆ +∂ ∂ ∆
∂ ∂ ∂ ∂ ∂ ∂ ∂ ∂ ∆ ∂ ∂ ∂ ∂ ∂
∂ =
∂
(8)
With initial and boundary conditions
0
1 1, 0, 1 , 1 at 0
1
and , , 0 at 0.
ψ φ ψ φ θ ζ
ξ ζ ζ ξ ξ η
ψ φ θ ζ
ξ ζ ζ
∂ = ∂ = − ∂ +∂ = − = =
∂ ∂ ∂ ∂
∂ ∂
= = = =
∂ e ∂ e
w U
U V
(9)
3. Solution of the Problem
The problem is solved by applying a two parameter group transformation to the partial differential Equations (6)-(8). This transformation reduces the four independent variables
(
t, , ,ξ η ζ)
to one similarity variable(
t, , ,)
γ ξ η ζ and the governing Equations (6)-(8) are transformed to a system of ordinary differential equations in terms of the similarity variable γ.
3.1. The Group Systematic Formulation
Define the procedure is initiated with the group G, a class of transformation of two parameters
(
a a1, 2)
of the form(
1 2)
(
1 2)
: S , S ,
G S c a a S K a a= + (10)
S stands for t, ξ, η, ζ, Ψ, ϕ, Ue, Ve, ∆T and θ, CS and KS are real-valued and at least differentiable in their real
arguments
(
a a1, 2)
.3.2. The Invariance Analysis
The transformation of the dependent variables and their partial derivatives are obtained from G via chain-rule operations
(
)
(
)
, , , ,S i
i i
S i j ij ij
S c c S
i j t
S c c c S ξ η ζ
=
=
= (11)
where S stands for ψ, φ, θ. i.e.
(
t)
, 2(
t)
2t t c c t t t c c c t
ψ ψ ξ
ξ
ψ ψ ψ ψ
ψ ψ
ξ ξ
∂ ∂ ∂ ∂
= = = =
∂ ∂ ∂ ∂ ∂ ∂ etc.
(
)
2 2
2 2 2 2 2
2 2
2 2
3 3
3 3 2 2 2 2 2
2 3
2
2 2
2 1 1, 2
T e e e
e e e e
t
g L T U U U V U V M MU
t U
H a a
t ξ
ψ ψ ψ ψ φ ψ ψ ψ φ ψ φ
ξ ξ ξ ξ ξ ξ
ζ ζ ξ ζ ζ ζ η ζ ξ ζ η ζ ζ
ξ β ψ ψ
θ ξ ξ ξ ξ ξ ξ ξ
ξ η ζ ζ
ψ ξ ψ ψ ψ ξ φ
ζ ζ ξ ζ ζ
∂ + ∂ ∂ − ∂ + ∂ ∂ − ∂ ∂ − ∂ ∂ − ∂ ∂ ∂ ∂ ∂ ∂ ∂ ∂ ∂ ∂ ∂ ∂ ∂ ∂ ∂ ∆ ∂ ∂ ∂ ∂ ∂ + − − − + − + − ∂ ∂ ∂ ∂ ∂ ∂ ∂ ∂ ∂ ∂ = + − + ∂ ∂ ∂ ∂ ∂ ∂ ∂ 2
2 2 2
2
2 2
3 3
3 3 2 2 2 2 2
2 3
T e e e
e e e e
e
g L T U U U V U V M MU
t U
ξ
ψ ξ ψ ψ ξ φ ψ ξ φ
ζ η ζ ξ ζ η ζ ζ
ξ β ψ ψ
θ ξ ξ ξ ξ ξ ξ ξ
ξ η ζ ζ
∂ ∂ ∂ ∂ ∂ ∂ − − − ∂ ∂ ∂ ∂ ∂ ∂ ∂ ∆ ∂ ∂ ∂ ∂ ∂ + − − − + − + − ∂ ∂ ∂ ∂ ∂ (12)
Substitution from Equations (10) & (11) into Equation (12) yields 0
e e
U V T
kξ =kθ =k∆ =k =k =
( )
( )
( )
( )
( ) ( )
( )
( )
( )
( )
( )
( )
( )
( )
( )
( )
( )
2 2 2 2
3
2 2 2
3 2 2 2 2 2 2 2 3
e e e
e e
T t
U U V
U V
t
U
c c c c c c c c
c c c
c c c c c c
c c c c c
c c c c
c c
c c c c
c c c
c
ξ ψ ψ ξ φ ψ ξ φ
ξ θ
ζ ζ η ζ ζ
ξ ξ
ξ ξ
η
ξ ψ ξ ψ
ξ ζ ζ ∆ = = = = = = = = = = =
(
)
1 1, 2 e H a a
=
where H a a1
(
1, 2)
=constant.In a similar manner, the invariant transform of (7) gives
( )
( )
( ) ( )
( ) ( )
( )
( )
( )
( ) ( )
( )
( )
( )
( )
( )
( )
( )
3 2 2 2 2 2 2 2
2 2 2 2
2 2
3 3
2 e e e e 2
e e
t
V V U V
U V T
t
c c c c c c c c c c c c c c
c c c c c c c c c c c
c c
c c c c c
c c c c c c
c c c
ξ φ ξ φ ψ ξ φ ξ φ ξ ψ φ ξ φ
ζ ζ ζ η ζ η ξ ζ η ζ
ξ
ξ ξ
ξ θ ξ
ξ η ∆ = = = = = = = = = =
( )
( )
( )
( )
(
)
3 2 22 1 2
3 Ve ,
c c c c
c c H a a
c c
ξ φ ξ φ
ξ ζ ζ = = = =
where H a a2
(
1, 2)
=constant.Similarly equation (8) is invariantly transformed giving
( )
( )
(
)
2
3 1 2
2 ,
t t
c c c c c c c c c c
H a a
c c c c c c c
ξ θ θ ψ θ φ θ ξ ξ θ
ξ ζ η ζ ζ
= = = = =
where H a a3
(
1, 2)
=constantThe initial and boundary conditions being also invariant implies that kt = 0, kζ = 0.
( )
( )
( )
( )
2 2 3 2 1 s e e e et c t
c G k c c k G c k U U V V T T c ζ ζ η ζ ζ ψ ζ φ ζ ξ ξ η η ζ ζ ψ ψ φ φ θ θ = = = = + = = + = = + = = = ∆ = ∆ (13)
3.3. The Complete Set of Absolute Invariants
Our aim is to make use of group methods to represent the problem in the form of an ordinary differential equa-tion (Similarity representaequa-tion) in a single independent variable (Similarity variable). Then we have to proceed in our analysis to obtain a complete set of absolute invariants.
The complete set of absolute invariants is:
a) γ γ=
(
t, , ,ξ η ζ)
is the absolute invariant of the independent variables t, ξ, η, ζ.b) g tj
(
, , , ; , , , , ,ξ η ζ ΨϕU Ve e θ ∆T)
=Fj(
γ(
t, , ,ξ η ζ)
)
,j=1, 2,3, 4,5 are the five absolute invariants corres-ponding to the five dependent variables Ψ, ϕ, Ue, Ve,θ, ∆T.A function g t
(
, , , ; , , , , ,ξ η ζ ΨϕU Ve e θ ∆T)
is an absolute invariant of a two-parameter group if it satisfiesthe following two first- order linear differential equations:
(
)
(
)
(
)
(
)
(
)
(
)
(
)
(
)
(
)
(
)
1 2 3 4 5 6 7 8 9 10 11 12
13 e 14 15 e 16 17 18 19 20 0
e e
g g g g g g
t
t
g g g g
U V T
U V T
α α α ξ α α η α α ζ α α ψ α α φ α
ξ η ζ ψ ϕ
α α α α α α α θ α
θ ∂ ∂ ∂ ∂ ∂ ∂ + + + + + + + + + + + ∂ ∂ ∂ ∂ ∂ ∂ ∂ ∂ ∂ ∂ + + + + + ∆ + + + = ∂ ∂ ∂∆ ∂ (14a)
(
)
(
)
(
)
(
)
(
)
(
)
(
)
(
)
(
)
(
)
1 2 3 4 5 6 7 8 9 10 11 12
13 e 14 15 e 16 17 18 19 20 0
e e
g g g g g g
t
t
g g g g
U V T
U V T
β β β ξ β β η β β ζ β β ψ β β φ β
ξ η ζ ψ ϕ
β β β β β β β θ β
θ ∂ ∂ ∂ ∂ ∂ ∂ + + + + + + + + + + + ∂ ∂ ∂ ∂ ∂ ∂ ∂ ∂ ∂ ∂ + + + + + ∆ + + + = ∂ ∂ ∂∆ ∂ (14b)
(
0 0)
(
0 0)
(
0 0)
(
0 0)
1 1 2 1 1 2 1 1 2 2 1 2
1 1 2 2
, , , , , , ,
t t t t
c a a k a a c a a k a a
a a a a
α
= ∂α
= ∂β
= ∂β
= ∂∂ ∂ ∂ ∂ etc.
(
0 0)
1, 2a a indicates the value of
(
a a1, 2)
which yields the identity element of the group. Independent Variables as Absolute InvariantsThe absolute invariant γ
(
t, , ,ξ η ζ)
of the independent variables(
t, , ,ξ η ζ)
is determined using Equation (14)(
)
(
)
(
)
(
)
(
)
(
)
(
)
(
)
1 2 3 4 5 6 7 8
1 2 3 4 5 6 7 8
0 0 t t t t
γ γ γ γ
α α α ξ α α η α α ζ α
ξ η ζ
γ γ γ γ
β β β ξ β β η β β ζ β
ξ η ζ
∂ ∂ ∂ ∂ + + + + + + + = ∂ ∂ ∂ ∂ ∂ ∂ ∂ ∂ + + + + + + + = ∂ ∂ ∂ ∂ (15)
A successive elimination of ζ γ and ξ γ
ζ ξ
∂ ∂
(
)
17t t 37 57 67 0
γ γ γ
λ λ ξ λ η λ
ξ η
∂ ∂ ∂
+ + + =
∂ ∂ ∂ (16a)
(
)
13t t 53 63 73 0
γ γ γ
λ λ η λ λ ζ
η ζ
∂ ∂ ∂
+ + + =
∂ ∂ ∂ (16b)
where λij =α βi j−α βj i, ,i j=1, 2,3, 4,5,6,7,8
Invoking the group given in Equation (13) and the definition of the α’s and β’s we get α1=α3=2α7,
1 3 7 0
β =β =β = thus
13 73 0
λ =λ =
From Equation (16b) we obtain γ 0
η
∂ =
∂ , which means that γ is independent of η and γ is a function of t, ξ and
ζ; Solving Equations (16a) and (16b) implies γ ζπ=
( )
t,ξDependent Variables as Absolute Invariants
Similarly the absolute invariants of the dependent variables; Ψ, ϕ, Ue, Ve, θ are obtained from the group trans-
formation (13),
(
)
( )
(
)
( )
(
)
( )
1
2
3
, , , ; , , , ; , , , ;
e e e e
g t
g t U U
g t V V
ξ η ζ θ θ γ
ξ η ζ γ
ξ η ζ γ
= = =
A function g t4
(
, , , ;ξ η ζ ψ)
is absolute invariant of a two-parameter group if it satisfies the first-order linear differential equations(
)
(
)
(
)
(
)
(
)
(
)
(
)
(
)
4 4 4 4
1 2 3 4 5 6 9 10
4 4 4 4
1 2 3 4 5 6 9 10
0
0
g g g g
t
t
g g g g
t
t
α α α ξ α α η α α ψ α
ξ η ψ
β β β ξ β β η β β ψ β
ξ η ψ
∂ ∂ ∂ ∂
+ + + + + + + =
∂ ∂ ∂ ∂
∂ ∂ ∂ ∂
+ + + + + + + =
∂ ∂ ∂ ∂
(17)
The solution of Equation (17) gives
(
)
(
(
)
)
( )
4 , , , ; 1 1 , ,
g t ξ η ζ ψ =χ ψ Γ t ξ η =E γ (18)
In similar manner, we get
(
)
(
(
)
)
( )
5 , , , ; 2 2 , ,
g tξ η ζ ϕ =χ ϕ Γ t ξ η =F γ (19)
(
)
(
)
( )
6( , , ; ) 3 3 , ,
g t ξ η ∆T =χ ∆ ΓT tξ η =G γ (20) Since Ue(γ) and Ve(γ) are independent of ζ, whereas γ depends on ζ, it follows that Ue(γ) and Ve(γ) must be
equal to constant, say one. Without loss of generality, the χ’s in Equations (18)-(19) are selected to the identity functions. So we can write
(
t, , ,)
1(
t, ,) ( )
Eψ ξ η ζ = Γ ξ η γ (21)
(
t, , ,)
2(
t, ,) ( )
Fϕ ξ η ζ = Γ ξ η γ (22)
(
, ,)
3(
, ,) ( )
T tξ η t ξ η G γ
∆ = Γ (23)
Again ∆T is independent of ζ, whereas γ depends on ζ, it follows that G(γ) is equal to a constant, say G0. Without loss of generality G0 is equated to one. So
(
, ,)
3(
, ,)
T t ξ η t ξ η
∆ = Γ (24)
(
1 2)
1 22(
3 4 5)
2 6 4 22 22 3
7 2 8 1 1 9 3 10 0
E E E E F E
c c c c c c c c E
E F E E
c F c c c M M
γ
γ γ γ γ γ γ
λ θ γ γ γ γ ∂ ∂ ∂ ∂ ∂ ∂ + + + + − + − ∂ ∂ ∂ ∂ ∂ ∂ ∂ ∂ ∂ ∂ − − + + − + − = ∂ ∂ ∂ ∂ (25)
(
11 12)
(
13 14 18)
12 2 2(
15 16)
2 3
17 2 2 1 19 3 20 0
F E F F F
c c c c c c c c F
F F F
c F c c M M
γ
γ γ γ γ γ
λ θ γ γ γ ∂ ∂ ∂ ∂ ∂ + + + + + − − ∂ ∂ ∂ ∂ ∂ ∂ ∂ ∂ − + − − + − = ∂ ∂ ∂ (26) 2
22 23 24 25 26 27 2
1 0
E F
c E c F c c c c
Pr
θ θ θ θ θ θ
γ γ γ γ γ
∂ ∂ ∂ ∂ ∂
− − + + + − =
∂ ∂ ∂ ∂ ∂ (27)
where
2 2 2 2 2
2
1 1 1 1 1 2 1 1 2
1 1 2 3 4 5 2 6 7
2 2 3 1 2 2 2
8 2 9 1 10 11 12 2 13 1 14 1 2
2
2
2 2
15 2 16 2 2 17 2
, , , , , , ,
, , , , , , ,
, ,
c c c c c c c
t t
c c c c c c c
t t
c c c
π π π π
π π π π
ξ ξ ξ ξ ξ ξ η ξ η
π π π
π π ξπ ξ π π
ξ ξ ξ
π π π
η η
∂Γ Γ ∂Γ Γ Γ Γ ∂Γ Γ ∂Γ
∂ ∂
= Γ = = = = = =
∂ ∂ ∂ ∂ ∂ ∂
Γ ∂Γ ∂ ∂Γ ∂
= Γ = Γ = = = Γ = Γ = Γ Γ
∂ ∂ ∂ ∂
∂Γ ∂ Γ
= Γ = Γ = Γ
∂ ∂
2
3
2 1 2
18 19 2 20 2 21 1
2
3 3 3
1 2 1 2
22 23 24 25 26 27
3 3 3
, , , , ,
, , , , ,
c c c c
c c c c c c
t
π ξ π π π
η ξ ξ
π π
ξ
π π ξπ
ξ η ξ η
∂Γ =Γ Γ = Γ = Γ = Γ ∂
∂ ∂
∂Γ ∂Γ ∂Γ
∂Γ ∂Γ Γ Γ
= = = = = =
∂ ∂ Γ ∂ Γ ∂ Γ ∂
(28)
and c’s are constant
(
( )
3 2)
(
( )
)
2 2 21 gξ T L T U L Gr Re
λ = β ξ ∆ ν ξ ν = and
(
3 2)
(
)
22 gη TL T UL
λ = β ∆ ν ν
are buoyancy parameter or mixed convection parameter. Let in (28) c9/c10 = 1; then it follows that 1 2
1 12
,c 0,c 0
π ξ= − = =
By considering c5 may be taken to be unity, we get from (28) the following 3 2
1 ξ ,c2 0,c3 3 2,c4 1 2,c6 0,c9 1,c10 1,c21 1 2,c22 3 2,c27 1
Γ = = = = − = = = = − = =
Now if we consider c8 = 1, (28) implies 1 2
2 ξ ,c11 0,c13 1 2,c14 1 2,c15 0,c16 0,c17 0,c18 1,c19 1,c20 1,c23 0
Γ = = = = − = = = = = = = , c25= −1
implies 1
3 ξ−,c24 0,c26 0
Γ = = =
Evaluation of c’s implies γ ζξ= −1 2.
Equations (25)-(27) gives u-momentum equation 2
3 2
1
3 2
3 1 1 0
2
E E E F λ θ M E
γ γ γ γ ∂ ∂ ∂ ∂ + + − − − − = ∂ ∂
∂ ∂ (29)
v-momentum equation
3 2
2
3 2
3 1 1 0
2
F E F E F
λ θ
M Fγ γ
γ
γ
γ
∂ + ∂ −∂ ∂ − − ∂ − + =
∂ ∂ ∂
∂ ∂ (30)
Energy equation
2
3 32 0
E
Pr E
θ
θ
θ
γ
γ
γ
∂ + ∂ +∂ =
∂ ∂
∂ (31)
( )
( )
1, 0, , 1 at 0
and 1, 1, 0 at
w
E F E E
E F
θ γ γ
γ γ
θ γ γ
γ γ
∂ = ∂ = = = →
∂ ∂
∂ = ∂ = = → ∞
∂ ∂
(32)
Equations (29)-(31) together with the boundary condition (32) are solved numerically using the sixth order Runge-Kutta shooting method known as Runge-Kutta-Butcher initial value solver of Butcher (1974) together with the Nachtsheim-Swigert iteration scheme described by Nachtsheim and Swigert (1965).
The numerical results of the velocity profiles as well as temperature profiles for different values of magnetic parameter M, Prandtl number Pr, buoyancy parameter λ1 and suction parameter Ew will be discussed and display
graphically.
5. Results and Discussion
The main objective of the present study is to analyze the effect of MHD mixed-convection flow on a moving curved surface. Figure 2 and Figure 3 illustrate the dimensionless velocity profiles along ξ and η directions, re-spectively for fixed values of Pr = 0.73, λ1 = −13.29, λ2 = −0.76 and Ew = 1.53 with several values of M. Since
magnetic parameter is inversely proportional with Reynold number, Re so increasing values of the magnetic pa-rameter M decreases the flow rate in the velocity boundary layer thickness. It has been seen from Figure 2, due to moving surface the u-velocity profiles at the boundary surface fall down slowly then u-velocity profiles de-creases rapidly corresponds to opposing flow up to the peak points γ = 3.25, 2.85, 2.55 and then velocity inte-
Figure 2. Dimensionless u-velocity profiles against similarity variable γ for different values of M (Pr,λ1,λ2 and Eware fixed).
Figure 3. Dimensionless v-velocity profiles against similarity variable γ for different values of M (Pr,λ1,λ2 and Ew are fixed).
γ
u-ve
lo
ci
ty
0 1 2 3 4 5
0 0.2 0.4 0.6 0.8 1
M=0.9 M=0.09 M=0.01
γ
v-ve
lo
ci
ty
0 1 2 3 4 5
0 0.5 1 1.5
[image:9.595.206.421.347.502.2] [image:9.595.207.423.538.694.2]grate slowly for magnetic parameter M = 0.9, 0.09, 0.01. It is observed from Figure 3 that v-velocity profiles decreases with the increasing values of magnetic parameter M that is velocity profiles meet together at the posi-tion of γ = 3.4 and cross the sides. It has been seen from Figure 4 when the Prandtl number Pr = 0.80, 0.74, 0.73, 0.70 u-velocity profiles fall down up to the position of γ = 2.05, 2.15, 2.50 and from that positions of γ, u-velocity profiles rising up and finally approach to one. In Figure 5 shown that the maximum values of v-velocities are recorded as 1.9452, 1.9515, 1.9580 and 1.9768 for Prandtl number Pr = 0.75, 0.74, 0.73, 0.70 at the position of γ= 1.30, 1.35, 1.35, 1.40 respectively. It is observed from Figure 6 that u-velocity profiles de-
Figure 4. Dimensionless u-velocity profiles against similarity variable γ for different values of Pr (M, λ1, λ2 and Ew are fixed).
Figure 5. Dimensionless v-velocity profiles against similarity variable γ for different values of Pr (M, λ1, λ2 and Ew are fixed).
Figure 6. Dimensionless u-velocity profiles against similarity variable γ for different values of Ew (M, λ1, λ2 and Pr are fixed).
γ
u-ve
lo
ci
ty
0 1 2 3 4 5
0 0.2 0.4 0.6 0.8 1 1.2
Pr=0.80 Pr=0.74 Pr=0.73 Pr=0.70
1.2
γ
v-ve
lo
ci
ty
0 1 2 3 4 5
0 0.5 1 1.5
Pr=0.75 Pr=0.74 Pr=0.73 Pr=0.70
γ
u-ve
lo
ci
ty
0 1 2 3 4 5
0 0.2 0.4 0.6 0.8 1
[image:10.595.215.420.184.332.2] [image:10.595.210.418.369.513.2] [image:10.595.213.416.551.697.2]creases with the increasing values of suction parameter Ew. It has been seen from Figure 7 that as the suction
parameter Ew increases, the v-velocity profiles increases up to the position of γ = 1.50, 1.50, 1.35, 1.30 and from
that positions of γ velocity profiles decreases with the increasing values of suction parameter Ew. From Figure 8,
it is observed that owing to the effect of the buoyancy parameter λ1 = −13.29, −12.80, −12, −11, u-velocity pro-files decreases up to the position of γ = 2.10, 1.85, 1.65, 1.45 and from those positions of γ, u-velocities integrate rapidly and increases for increasing values of γ. In Figure 9 it is shown that the v-velocities of the fluid against γ
decreases for increasing values of buoyancy parameter λ1. The maximum values of the v-velocity are found to be
Figure 7. Dimensionless v-velocity profiles against similarity variable γ for different values of Ew (M, λ1, λ2 and Pr are fixed).
Figure 8. Dimensionless u-velocity profiles against similarity variable γ for different values of λ1 (M, Ew, λ2 and Pr are fixed).
Figure 9. Dimensionless v-velocity profiles against similarity variable γ for different values of λ1 (M, Ew, λ2 and Pr are fixed).
γ
v-ve
lo
ci
ty
0 1 2 3 4 5 6
0 0.5 1 1.5
EW=1.59 EW=1.53 EW=1.42 EW=1.40
γ
u-ve
lo
ci
ty
0 1 2 3 4
0 0.2 0.4 0.6 0.8 1
λ1= −11.0 λ1= −12.0 λ1= −12.80 λ1= −13.29
γ
v-ve
lo
ci
ty
0 1 2 3 4 5
0 0.5 1 1.5
[image:11.595.211.421.180.327.2] [image:11.595.211.418.363.513.2] [image:11.595.209.419.549.697.2]1.9628, 1.9548, 1.9453 and 1.9334 for λ1 = −13.29, −12.80, −12, −11 respectively. It is noted that the v-velocity decreases by approximately1.5% as λ1 increases from −13.29 to −11. Figure 10 illustrates for fixed values of Pr
= 00.73, λ1 = −13.29, λ2 = −0.76 and Ew = 1.53 the temperature profiles decreases with the increasing values of
magnetic parameter M. Figure 11 and Figure 12 display the results for the temperature profiles. It is observed from the Figure 11 and Figure 12 that the thermal boundary layer thickness decrease for the increasing values of Prandtl number Pr and suction parameter respectively. Figure 13 shows the small increment on the tempera-ture for increasing values of the buoyancy parameter λ1.
Figure 10. Dimensionless temperature profiles against similarity variable γ for different values of Pr (M, λ1, λ2 and Ew are fixed).
Figure 11. Dimensionless temperature profiles against similarity variable γ for different values of Pr (M, λ1, λ2 and Ew are fixed).
Figure 12. Dimensionless temperature profiles against similarity variable γ for different values of Ew(M, λ1, λ2 and Pr are fixed).
γ
θ
0 1 2 3 4 5
-0.2 0 0.2 0.4 0.6 0.8 1
M=0.9 M=0.09 M=0.01
1
γ
θ
0 0.5 1 1.5 2
0 0.2 0.4 0.6 0.8 1
Pr=0.73 Pr=0.65 Pr=0.60
1
γ
θ
0 0.5 1 1.5 2
0 0.2 0.4 0.6 0.8 1
EW=1.59 EW=1.53 EW=1.42 EW=1.40
[image:12.595.215.417.180.328.2] [image:12.595.215.420.365.513.2] [image:12.595.218.418.551.696.2]Figure 13. Dimensionless temperature profiles against similarity variable γ for different values of λ1 (M, Ew, λ2 and Pr are fixed).
Table 1. Comparison of the values of E′′
( )
0 , F′′( )
0 and θ′( )
0 with Maleque Kh.A. [2] and Present work for the varia-tion of Prandtl number Pr while M = 0.0, Ew= 0 and λ λ1= 2=U UF2 e2=V VF2 e2=100.Pr E′′( )0 F′′( )0 θ ′( )0
Maleque kh.A. [2] Present results Maleque Kh.A. [2] Present results Maleque Kh.A. [2] Present results
0.7 1.33198 1.35000 1.20973 1.21000 −0.88811 −0.90000
1.0 1.32807 1.31200 1.20539 1.20500 −1.01137 −1.08000
5.0 1.31467 1.30500 1.19094 1.19050 −1.79200 −1.78000
7.0 1.31229 1.30100 1.18842 1.19000 −2.01368 −2.00000
10.0 1.30993 1.29500 1.18594 1.17250 −2.27706 −2.10000
6. Comparison with Previous Work and Code Validation
A comparison of the present numerical results of E′′
( )
0 , F′′( )
0 and θ′( )
0 with this, obtained by Maleque Kh.A. [2], is depicted in Table 1. Here, the parameters M and Ew are igno red with different values of Prandtlnumber Pr. It is evidently seen from Table 1 that the current results are concurrence with the solution of Male-que Kh.A. [2].
References
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in Curvilinear Coordinates. M. Phil. Thesis, Department of Mathematics, BUET, Dhaka.
[3] Azam, Q. (1998) Mixed Convection about the Vertical Developable Flow Surfaces with Transpiration and Heat Flux Effects. M. Phil. Thesis, Department of Mathematics, BUET, Dhaka.
[4] Ishak, A. and Bachok, N. (2009) Mixed Convection Boundary Layer Flow over a Permeable Vertical Cylinder with Prescribed Surface Heat Flux. European Journal of Scientific Research, 34, 46-54.
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[6] Zakerullah, Md. (2001) Similarity Analysis. Thesis, Bangladesh University of Engineering and Technology, Dhaka. [7] Alam, K.C.A., Hossain, M.A. and Rees, D.A.S. (1997) Magnetohydrodynamic Free Convection along a Vertical Wavy
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[8] EI-kabir, S.M.M., Rashad, A.M., Subba, R. and Gorla, R. (2007) Unsteady MHD Combined Convection over a Mov-ing Vertical Sheet in a Fluid Saturated Porous Medium with Uniform Surface Heat Flux. Science Direct Mathematical and Computer Modelling, 46, 384-397.
γ
θ
0 0.5 1 1.5
0 0.2 0.4 0.6 0.8 1
λ1= −13.29 λ1= −4.00 λ1= −2.00
[image:13.595.88.538.313.435.2][9] Dhar, D.R. (2007) Group-Theory Method on Similarity Solution of Unsteady Free Convection Flow from a Moving Vertical Surface with Suction and Injection. M. Phil. Thesis, Department of Mathematics, BUET, Dhaka.
[10] Moran, A.G.A. (1962) The Reduction by One of the Number of Independent Variables in Some Systems of Partial Differential Equations. Quarterly Journal of Mathematics, 3, 250-259. http://dx.doi.org/10.1093/qmath/3.1.250 [11] Michal, A.D. (1952) Differential Invariants and Invariant Partial Differential Equations under Continuous
Transforma-tion Groups in Normal Linear Spaces. Proceedings of the National Academy of Sciences of the United States of Amer-ica, 37, 623-627. http://dx.doi.org/10.1073/pnas.37.9.623
[12] Birkoff, G. (1948) Mathematics for Engineers. Electrical Engineering, 67, 1185.
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[14] Butcher, J.C. (1974) Implicit Runge-Kutta Process. Mathematics of Computation, 18, 50-55. http://dx.doi.org/10.1090/S0025-5718-1964-0159424-9