MECHANICS RESEARCH COMMUNICATIONS
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Voi.13(3),155-163, 1986. Printed in the USA. Copyright (c) 1986 Pergamon Journals Ltd.
FINITE-DIFFERENCE ANALYSIS OF MHD STOKES PROBLEM FOR A VERTICAL INFINITE PLATE IN A DISSIPATIVE FLUID WITH CONSTANT HEAT FLUX V.M.Soundalgekar and S.B.Hiremath 7/lO,Vivekanand Housing Society, Saraswat Colony Dombivali (E) 421201, India
(Received 10 January 1986; accepted for print 5 May 1986)
Introduction Stokes ~ ] first studied the unsteady flow of a viscous incompressible fluid past an infinite horizontal plate moving impulsively in its own plane.Stewartson[2,3]presented the analytical solution of unsteady flow past an impulsively moving semi-infinite plate.The numerical solution of Stewartson's problem was presented by Hall[4].The flow of a compressible _gas past an infinite vertical plate was studied by Illingworth[51who presented approximate solution.Elliott 6 studied the flo~ ~ast an infinite vertical plate with time-dependent motion. In Ref.[6]only mathematical solution was presented and the corresponding physical situation was not discussed.In case of motion past a vertical plate,the presence of free-convection currents due to temperature difference between the plate temperature T~ and T~ must be considered.IIence such a study,on taking into account the free-convection currents, of flow past an impulsively started infinite vertical plate was recently presented by Soundalgekar[7~who gave an exact solution by using Laplace-transform technique.Another situation which is also of interest in technology is the study of flow past an impulsively started vertical plate receiving heat at constant rate. Exact solution to the ~roblem considered in ~ef.~7]with constant heat flux was presented by Soundalgekar and l~atil[8].In both these papers,the effects of viscous dissipative heat were neglected.On tsd~ing into account the viscous dissipative heat,the oroblem is governed by coupled nonlinear equations and hence exact or approximate solutions could not be obtained.So in case of both isothermal and constant heat flux,these nonlinear coupled equations were solved by explicit finite-difference method by Soundalgekar, Bhat and Mohiuddin [9,10]. Rossow[ll]first presented the exact solution of MHD Stokes problem on negleting the induced magnetic field. The corresoonding I~ID flow past a vertical plate was presented by Soundalgekar, Gupta and A r a n ~ e [ 1 2 ] . I n thes~, last two pap~:r,~,-~l,~cous dissipative heat ~Jas assumed to be neglected.On taking into account 155
156
V.M. SOUNDALGEKAR and S.B. HIREMATH
viscous dissipative heat but neglecting Joule dissipative heat, the coupled nonlinear equations governing the MHD flow past an impulsively started infinite plate were studied by finite-difference method by Soundalgekar and Hiremath[13].The plate was assumed to be isothermal.The MHD flow past an impulsively started infinite plate in the presence of constant heat flux and viscous dissipative heat has not been studied as yet.Hence the motivation to study this problem. In Sec.2,the mathematical analysis has been presented and in Sec.3,the conclusions are set out. Analysis Here
the MHD flow of an electrically
viscous
fluid past an impulsively
te under transverse magnetic
conducting incompressible
started infinite
vertical pla-
field is considered. The x-axis is
taken along the plate and the y-axis is taken normal to the plate, Initially,the
temperature of the fluid and the plate is assumed
to be the same for all y.At time t'>O,the plate is being heated by supplying heat at constant rate and simultaneously,the
plate
is assumed to get an impulsive motion in the upward direction. Applying the usual Boussinesq's an infinite
approximation,the
vertical plate is now governed by the following
tem of coupled nonlinear
equations in non-dimensional
~u ~2u ~Y - ~y2 + GO - Mu p ~0 t-
The initial
~.G~D flow past
u(y,t)
:
(i)
~2e ~u 2 a y2 + PE ( ~ )
and boundary
form
sys-
(2)
conditions are
u(o,t)
= O, @(y,t) = 0 30 = o, y ~ = - i
u(~,t)
= O, O(~,t)
= 0
t~O
(3) t~O
The nondimensional quantities are defined as follows : ' °2 ' u = u/U o, t = tU /~ , y = YUo/~ , O = ( T ' - T ~ ) / ( q ' ~ / k U o)
G =~g~(q'~/kUo)/Uo 2 , P =.~Cp/k
, ~ = Uo2/Cp(q'~/kU o)
!
Here u is the velocity, U o the velocity of the plate,t' the time~ Cp the specific heat at constant pre~sure, k the thermal conductivity,
the kinematic
viscosity,
T' the temperature
MHD STOKES PROBLEM
157
of the fluid,T'cothe temperature of the fluid far away from the plate,g the acceleration due to g r a v i t y , ~ t h e
coefficient of vo-
lume expansion,q' the heat flux per unit a r e a , ~ t h e
coefficient
of viscosity, o-the scalar electrical conductivity,B o the constant magnetic field, e the non-dimensional temperature,P the Prand t l number,E the Eckert number and M is the magnetic parameter. Equations (1) and (2) are coupled and nonlinear equations and their analytical solutions are not possible to obtain.Hence, we solve them by finite-difference method.The mesh-system is shown on Fig. 1.
X
-1
0
1 2
40 41
FIG.I. M E S H
SYSTEM
We can write the explicit finite-difference equations (1) and (2) as follows :
u(i+i,j)
u(i,j+l) - u(i,j)
: G~(i,j)
+
-2u(i,j)+u(i-l,j) (Ay) z
- Mu(i,j)
~(i,j+l) - @(i,j) P
~t
(5)
~(i+l,j) - 2~(i,j) + @(i-l,j) :
(AY) 2
+ 2
PEI u(i+l'J) u ( i '-J ) - ~ Z 1 y
(6)
The index i refers to y and j to t.AY is taken as O.1.We can write the initial conditions from (3) as u(o,o)
= l, e ( o , o )
= o
(7)
This means that due to sudden velocity given to the plate, the
158
V.M.
velocity
at y = 0 c h a n g e s
at t < 0 . T h e adual
initial
c h a n g e in the
of c o n s t a n t h e a t conditions
from
discontinuously
(]),the
that
temperature
due
of the p l a t e
: 0
boundary
for all i
the b o u n d a r y
@(i,j)
: i
for all
form
(6
lated j=O.
grid-point
(i0)
(-l,j)
from the s e c o n d The b o u n d a r y
the v e l o c i t y
0.?i,
compared our
ence
rw>d.Hencc
of thes~ ~ re±" c~aiua-
(6).~ut e(-l,O)
is
calcu-
time-ster;
t ~ k e n as y : 4 and h e n c e j.From
(9),we
calculate :i,~O,
compute ~(i,j+l),
j = lO00,i.e,
in
earlier
i : O,L~O.This
t = i.
on a c o m p u t e r
for P = 0.~,
i[ = ~ , 4 . T h e
order
the a c c u r a c y
of the r e s u l t s , w e
have
the a n a l y t i c a l
solution obtained
for
cent. To
0.0006,O.000~
at the h y p o t h -
at p o i n t s on the
computations
(l<~)
±~ = 0 . 0 1 , O . 0 2 , to check
solutions
scheme,we
follov/i-
:-i
for the i n i t i a l
at y = o ~ i s
(6),we
with
time-step ~t
and 1 for the entire
and the a g r e e m e n t
than i per
the
- 8(-1,j)
the v a l u e s
: 0 for all
tiil
these
L = 0 at t = 0 . 2 , 0 . 9 i = 1,~O
takes
to take
time-axis.
Z3 Y
(i0)
and t e m p e r a t u r e s
c a r r i e d out
en as O . O 0 1 . 1 n
have
end of a t i m e - s t e p , v i z . , u ( i , j + l ) , i
is r e p e a t e d
C = 2,6,
or
side of
e q u a t i o n of
: O, @ ( 4 l , j )
at the
-i
and we ta/~e a v e r a g e
time-steps. Similarly,from
',Te have
(9)
side of the p l a t e on
for {J give
condition
terms of velocities
procedure
j
8(©,j) =
on the r i g h t h a n d
we set u(41,j)
tsdtcs the
,on the p l a t e , w e
- 8(-l,j)
equations in
tini[ @ ( O , j + ! )
(8)
:
2~),
etical
initial
(>0)
c o n d i t i o n on ~ at the p l a t e
finite-difference
two
zero.The
:
a p o i n t i = -i on the left h a n d
These
is a gr-
to the p r e s e n c <
c o n d i t i o n on u at y = 0
N o w to c o m p u t e ~ at i : O , f r o m
ng
is t a k e n
there
o
are
u(O,j)
Then
at i from its v a l u e
c o n d i t i o n on ~ i n d i c a t e s
: O, @ ( i , O )
follov~ing form
and S.B. HIREMATH
flux and h e n c e ~ ( © , 0 )
for y>O
u(i,O) Also
SOUNDALGEKAR
the c o n v e r g e n c e the
solutions
and an i n s i g n i f i c a n t
~w c o n c l u d e
and c o n v e r g e n t .
The v e l o c i t y
profiles
are
s h o w n on
of the
i.u.
e r r o r of l e s s finite-differ-
for small v a l u e s of At =
c h a n g e in the v a l u e s
that o u r e x p l i c i t
me is stable
chos-
of y - v a l u e s ,
was g o o d v&ith a m a x i m u m
test
repeated
range
was
was obse-
finite-difference
Figs.2
sche-
and ~ for P : ;9.5 an<~
MHD STOKES PROBLEM
159
0.71 respectively.We observe from these two figures that the velocity decreases due to the application of the magnetic field.An increase in G or E leads to an increase in the velocity.On Figs. 4 and 5,the temperature profiles are shown. We observe from these figures that due to the application of the magnetic field,the temperature increases.An increase in G or E also leads to an increase in the temperature.From the velocity field,we now calculate the skin-friction. It is given by ~g = -
~u i ~Y IY = 0
(il)
l
whereT=~/~U~.The
numerical values o f ~ a r e
calculated by numeric~
al differentiation using Newton's 5-point interpolation formula by taking 5 points.These values are entered in Table I and Fig.6. We observe from this table and Fig. 6 that due to the application of the magnetic field,there is a rise in the value of the skin-friction.An increase in G or E leads to a fall in the value of the skin-friction under the action of the magnetic
field.~g increases
with increasing the Prandtl number. We now calculate the rate of heat transfer at the plate.lt is given in terms of the Nusselt number as Nu
=-
1 ~--~
d8 I dy y=0
=
1 ~
d9 (Vdy
-
(12)
r
The numerical values of Nu are calculated and are entered in Table I and also shown in Fig. 7.We observe from this table and Fig.7 that due to the application of the magnetic field,there is a fall in the value of the Nusselt number as compared to non-magnetic case.Greater viscous dissipative heat or an increase in G leads to an increase in the value of Nu but the Nusselt number decreases due to increasing the strength of the magnetic field. Conclusions 1.Due to the application of the magnetic field,there is a decrease in the velocity and an increase in temperature,skin-friction and the Nusselt number.2.Greater viscous dissipative heat or an increase in G leads to a fall in the skin-friction but a rise in the Nusselt number.3.An increase in P leads to a rise in the value of the skin-friction and the Nusselt number.4.Greater viscous dissipative heat or an increase in G leads to a rise in
160
V.M.
SOUNDALGEKAR
and S.B. HIREMATH
the velocity,temperature. References l.G.G.Stokes,Camb.Phil.Trans.iX,8(1851) 2.K.Stewartson,Quart.Mech. Appi.Math.4,182(1951) 3.K.Stewartson,quart.Mech. Appl.Math.26,i43(1973) 4.M.G.Hail,Proc.Roy. Soc.(London),310A,401(1969) 5.C.R.lllingworth,Proc. Camb.Phil.Soc.,46,60j(1950) 6.L.Elliott,Zeit.Angew.Math. Mech.,49,647(1969) 7.V.M.Soundalgekar,J.Heat Transfer(Tr.ASME)99C,499(1977) 8.V.M.Soundalgekar and M.R.Patil,Astrophysics and Space gci.,70, 179(1980) 9.V.M.Soundalgekar,J.P.Shat and M.Mohiuddin,lntl.j.~ingng. Sci.,17, i283(1979) i0.V.M.Soundalgekar,J.P.Bhat and M.Mohiuddin,Latin American J. Heat Mass Tr.,9,(1985) II.V.J.Rossow,NASA Report No 1358(1958) 12.V.M.Soundalgekar,S.K.Gupta and R.N.Aranke,J.Nuciear Engng Des. 51,405(1978) lj.V.M.Soundalgekar and S.}~.Hiremath,Magnetohydrodynamics(USSR) (To be published) Table I
Values of "g and
q~ ~
MQ
~
/t
o.~ 2"> d.bl 2 2 2 4 4 0 0
2 0.02 40.01 4 0.02 2 0.0! 2 0.02 20.O1 2 0.02
0.712 2 2 2 4
2 0.01 2 0.02 4 0.0i 4 0.02 20.O1
4 2 0.02
0 20.01 0 2 0.02
Nu
Nu
1.0
o.2
t".4290 1.4270 1.1259 1.1220
o.1378 0.1341 -1.1487 -1.1556 0.9091 0.9053 -i.0726 -1.0774
i~300 1.4232 1.4303 1.4238 1.4294 1.4220 1.4306 1.4243
1.O O. 897'2 O. 6322 0.8944 O. 6309 0.8976 o. 6922 0.8952 o. 63lo 0.8967 o. 6317 0.8933 0.6300 0.8977 o. 6323 0.8954 0.6311
1.4967 1.4944 1.2612 1.2568 1.9254 1.9232 1.O120 1.0097
0.9255 0.4088 0.9219 0.4041 0.3677 -0.6066 0.3611 -0.6145 1.5083 1.1288 1.5048 1.1243 0.1669 -0.7062 0.1632 0.7114
1.7096 1.6983 1.71oo 1.6991 1.7086 1.6963 1.7106 1.7003
i.O710 1.O662 1.o715 1.0673 1.0700 1.0642 1.0719 1.0680
O.2
O.5
0.7708 0.7677 0.0584 0.0527 1.8620 1.3734 1.8600 1.3703 0.9394-0.0157 0.9373-0.0191
b.~
O. 7541 0. 7517 0. 7545 0.7525 0.7532 0.7501 O. 7546 0.7527
0
0.2
0.z,
U
0.6
0.8
1'°II
Y
2
0.2 0,2 0.2 0.2 0.5 0.2
t 0.2
FIG. 2. VELOCITY PROFILES
1
II HI IV V Vl VI'[
I
3
P: 0.5
2 2 2 4 2 0
M 2 2 2 4 2 2 2
G 2 0.01 0.02 0,01 0.01 0.01 0.01
E 0
0.2
0.4
U
0.6
0.8
1.o
2
y
3
P= 0.71
M 2 2 2 2 4 2 0
FIG. 3. VELOCITY PROFILES
1
1; I 0.2 fT 0.2 ]]'I 0,2 IV 0.2 V 0.2 VI 0.5 V~ 0.2
G 2 2 2 4 2 2 2
E 0 0.01 0.02 0.01 0.01 0.01 0.01
! 4.
~ o
r.~
O
0
0,2
0.4
1
Y
2
3
G 2 4 2 2 2 2 2
FIG. 4. TEMPERATURE PROFILES
1
P:0.5
M 2 2 2 2 2 0 2
~J---
E 0 0.01 0.01 0.01 0.02 0.01 0.01
0
0.2
0.4
O
0.6
t I 0.2 IV 0.2 II 0.2 V 0.2 flT 0.2 VII 0.2 V[ 0.5
0,6
8
0.8
0.~
2
y
G 2 4 2 2 2 2 2
3
P : 0.71
M 2 2 2 4 2 0 2
FIG 5 TEMPERATURE PROFILES
1
t I 0.2 IV 0.2 II 0.2 V 0.2 ffT 0.2 VE 0,2 VI 0.5
E 0 0.01 0.01 0.01 0'02 0.01 0.01
~-]
t~
i-I
Z t~
r.~ 0
~o
0
.
FIG. 6
0"5
t
0.71
=0-5
I "0
THE SKIN- FRICTION
E 0"01 I \ 0-02 II 0.01111 0.01 IV
0.2
IMG 0./-, 2 2 2 2 2 Z, 2
0"8
"12
1"2
1.(
2-1
I
III
I!
0"4
Nu
0
1-0
1"I
Ill
I
1,0
II
II
I
III
III
THE NUSSELT NUMBER
I
0"5 t
0.01
I
FIG. 7
I
0.02 II
0-01
0-2
~
2 2
2
2
2
M
= 0.71-
P=0"5
O
l,.o
O
"O
i'x/