The Unsteady Flow Magnetohydrodynamic in Micropolar Fluid through Porous Sphere

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Proceeding of The 6 th Annual Basic Science International Conference Published online, on June 7, 2016. The Unsteady Flow Magnetohydrodynamic in Micropolar Fluid through Porous Sphere Indira Anggriani 1*, Basuki Widodo 2,Chairul Imron 3 1,2,3 Department of Mathematics, Faculty of Mathematics and Natural Science, Institut Teknologi Sepuluh Nopember, Surabaya, Indonesia * Corresponding authors: [anggriani.indira@gmail.com] Abstract Micropolar fluid is non-newtonian fluid type with microstructure. Micropolar fluid support body couples and exhibit microrotational effects. The MHD is study about the motion of electrically conducting fluids under magnetic fields. This research is about unsteady MHD problem in micropolar fluid through porous sphere at stagnation point. The MHD effect in micropolar fluid is influence of magnetic field on the microrotation that also affect the motion of the fluid. The microrotation characteristic that has been taken into account is the attribute that distinguish micropolar fluid model from others. This research was developed from a mathematical model of MHD boundary layer flow in micropolar fluid. Micropolar fluid flow that influenced magnetic field evokes boundary layer. From the boundary layer formed a dimensional governing equation, it was continuity equation, momentum equation and angular of momentum equation. Then the equation is transformed into non-dimensional form and similiarity equation. The similiarity equations are solved numerically solution by Keller-Box method. Numerical results obtained, used to observe the influence of some parameters: magnetic parameter, micropolar parameter, and porous parameter of the velocity profile and the profile of the microrotation. The result of numerical solution that the velocity profile be increased along with magnetic parameter increased. Moreover the velocity decreased when micropolar parameter increased. When porous parameter increased, the velocity profile decreased but the difference not significant. Profile microrotation increased and changed with increased micropolar parameters. 1. INTRODUCTION Fluid is a subtance that has the ability to change shape when exposed to a continuously shear stress [1,2]. Two types of fluids are Newtonian fluid and Non Newtonian fluid. In most real cases, fluids cannot be easily modeled as viscous fluid under the Newton s law of motion or by the Navier-Stokes equations. Generally, any fluids that do not obey the Newton s law of motion are classed as non-newtonian fluids and micropolar fluid is one of them(hayat et al., 2009). Example of non-newtonian fluids is micropolar fluids.the theory of micropolar fluids developed by Eringen [4,5] has been of much interest because it can be used to explain the characteristics in certain fluids. Micropolar fluids is fluids with microstructure. The micropolar fluids are theoretically represent fluids that contain rigid randomly oriented particles with their own and microrotations, suspended in a viscous medium. In the micropolar fluid, rigid particels contained in a small volume element can rotate about the center of the volume element described by the microrotation vector [6]. Due to its importance, we conduct a research about micropolar fluid. In this paper will be discussed about the unsteady magnetohydrodynamics boundary layer flow in micropolar fluid past a porous sphere. Boundary layer is a thin layer which is near the solid surface caused by the viscosity of fluid flow on the porous medium. The equation is built by boundary layer theory which can be called boundary layer equation. By considering the MHD effect on micropolar fluid, this paper also discuss the influence of magnetic field on the microrotation and magnetohydrodynamics effect on velocity profiles. 2. METHODS 2.1 Procedures The governing equations are developed by continuity, conservation equations of linier momentum and angular momentum based from physical model of porous sphere. The boundary layer governing equations get under the Boussinesq approximation. Furthermore, we reduce the boundary layer equations to a dimensionless form by 363

applying several dimensionless variable and using boundary layer approximation. Then the equation is transformed into dimensionless form and similiarity equation. The similiarity equations are solved numerically solution by using Keller-Box method. 2.2 Problem Formulation We consider the unsteady state two-dimensional near a porous sphere in micropolar fluid, as shown in Fig. 1, where Q is the radius of the sphere. In this figure, the coordinate R and V are chosen such that R measures the distance along the surface of the sphere from the lower stagnation point and V measures the distance normal to the surface of the sphere, respectively[7]. For an incompressible micropolar fluid, in the presence of MHD, by neglecting the body force and body couple, the equation of continuity, the conservation equations of linier momentum and angular momentum are as follow. Continuity Equation : Momentum Equation : Figure 1. Physical model and coordinates for a porous sphere \([ ³X) \ \([ W) + =0 (1) \µw Momentum Angular Equation `( \³X MTW \³X \³X MÒ *= \0 M*aM )( \ê ³X + \ê ³X \ \ \µw \ \ ê \µw ê*+ \ X @Õ TW @ G \µw 3 TW (2) `( \W MTW \W \W MÒ *= \0 M*aM W \ \ \µw \µw )(\ê + \ê W \ ê \µw ê*+ \ X @Õ Ò @ G Ò \ 3 In this problem the dimensionless variables are given as ` ( \ X MTW \ X \ X X MÒ \ \ \µw *=Ó(\ê + \ê X \ ê \µw ê* (2 X+ \³X @ \ \µw \ ) (3) R=,V=Y\/µW ³X,T=,,= ¾ p, '*R)=[ ( ) ¾ p,ò=y\œ ê W,U= 0 ¾ p Y¾ê (4) p where Reynold Number Y\= ¾ p. Substitution (4) into (1-3) leads to the following non-dimensional equations q \³ \ +T\³ \ +Ò\³ \µ =@\0 \ +( 3) \ ê ³ 6r \([³) + \([) =0 (5) \ \µ \ ê+(1+s)\ê ³ \µ ê+s\ \µ 6r (\ \ +T\ \ +Ò\ \µ *=@\0 \µ +( 3) \ ê \ ê 6r ê \ ê+( 3) 6r \µ ê 3 \ 6r \ \ \ +T\ \ +Ò\ \µ =(1+3 *( 6r \ ê \ ê+ \ê \µ ê* s(2 +\³ @(K+ i)t (6) \µ 6r where micropolar s, magnetic K and microrotation field are dimensionless parameter. t) (è Ò 6r \ \ ) (7) 364

In order to solve (5-7) using the same procedure of boundary layer approximation and the stream function, the following variables are assumed where stream function @ defined as By substituting (8-9) into (5-7), we obtain : @=Rñ(R,V), Ñ =Ñ(R,V) (8) T= \^ \µ, Ò= \^ \. (9) (1+s) \ì u \v ì+ v \ ê u \v ê+n w,#1@(\u* +ñ \ê u \v \v ê$+s\x \v +(K+ i),(1@\u \v *=, \ê u \w\ (10) (1+ 3 x *\ê \v ê+ v \x with respect to the following Boundary Conditions \v + h+n w,(ñ\x \v @h\u \v *=,\x,<0 :ñ= \u \v =h=0atr,v +,s(2h+ \ê x \ \vê) (11),±0:ñ= \u =0. u \y _= -\ê \yê,ate=0 (12) \u \y =1, _=0ate At the lower stagnation point of the solid sphere, R g0, Equation (12-14) are reduced to the following ordinary differential equation : and, (1+s)ñ ùùù + v ñùù + N w, 1@(ñù ) +ñ ñ ùù ÀMs _ ù M*KM i),(1@ñ ù )=, \uù \ (13) 3. RESULTS AND DISCUSSION (1M 3 *_ùù M y _ù M x MN, ñ_ù @_ ñ ù À=, \x M, s \ *2_Mñùù ) (14) The system of equation (13) and (14) are solved numerically for some values of the micropolar parameter (K) and magnetic parameter (M) using Keller-box method [8,9]. The variation on velocity and microrotation profile at front stagnation point (R= 0 ) with various value of magnetic parameter are illustrated in Fig. 2(a) and Fig. 2(b) respectively. These numerical results have been made at fixed values of micropolar K = 1. The results show that velocity profiles in Fig. 2(a) increase when the magnetic parameters increase, there is no values of velocity in negative. The microrotation profile of boundary layer flow in the MHD micropolar fluid of -=0 at R= 0 and when s=1. Increasing M leads to higher microrotation @h under the influence of MHD at the region near the surface of a porous sphere but as e>0.5,@_is decreased under the effect of MHD. Figure 2.(a) Velocity profile for various z at lower stagnation point *{= ),}=k,~=k, and = (b) Microrotation profile for various z at lower stagnation point ({= ),}=k,~=k, and = 365

Figure 3(a) Velocity profile for various at lower stagnation point ({= ),z=k,~=k, and = (b) Microrotation profile for various at lower stagnation point ({= ),z=k,~=k, and = Figure 3(a) shows the velocity profile of the boundary layer flow in the magnetohydrodynamic micropolar fluid at various s when -=0 and K =1. It is noticed that T a micropolar fluid is decreasing with increasing s. The microrotation profile of boundary layer flow in the maghnetohydrodynamic micropolar fluid of -=0 at R= 0 and when K=1. Increasing s leads to higher microrotation @h under the influence of micropolar parameter at the region near the surface of a porous sphere but as e>0.5,@_is increased under the effect of micropolar parameter. 366

Figure 4(a) Velocity profile for various ~ at lower stagnation point ({= ),z=k,}=k, and = (b) Microrotation profile for various ~ at lower stagnation point ({= ),z=k,}=k, and = The variation on velocity and microrotation profile at front stagnation point (R= 0 ) with various value of porosity parameter are illustrated in Fig. 4(a) and Fig. 4(b) respectively. These numerical result have been made at fixed values of micropolar s=1. The results show that velocity profiles in Fig. 4(a) increase when the porosity parameters increase, there is no values of velocity in negative. The microrotation profile of boundary layer flow in the MHD micropolar fluid of -=0 at R= 0 and when s=1. Increasingϕ leads to higher microrotation @h under the influence of porous at the region near the surface of a porous sphere but as e> 0.5,@_is decreased under the effect of porous. 4. CONCLUSION This paper considers the boundary layer flow in the MHD microfluid past a solid sphere. From the analysis and discussion of the result, the following conclusions are: 1. The governing equations are developed from continuity, momentum, and momentum anguler. Furthermore, those equations are transformed into boundary layer equations and transformed into a non-dimensional form. The resulting nonlinear system of partial differential equations are solved numerically using the Keller-Box method. 2. This research has revealed how the microrotation,magnetic and porosity parameter affect the velocity flow and microrotation characteristics. The velocity distributions increase and the microrotation decreases when the value of magnetic parameter and porous parameter increase.the velocity decreases and the microrotation increase when micropolar parameter increase. 5. REFERENCES 1. Widodo, B., Fatahillah, A., Rahayuningsih, T., MathematicalModelling and Numerical Solution of Iron Corrosion Problem Based on Condensation Chemical Properties, Australian Journal of Basic and Applied Sciences, 2011,5(1), pp. 79-86. 2. Widodo, B., Wen, X., Ingham, D. B, The Free Surface Fluid Flow in an Arbitary Shaped in a Channel, J of Enginering Analysis with Boundary Element, 1997, pp. 299-308. 3. Mohammad, N. F., Unsteady Magnetohydrodynamic Convective Boundary Layer Flow Past A Sphere in Viscous and Micropolar Fluids, 2014, Universiti Technology Malaysia, Malaysia. 367

4. Eringen, A. C., Theory of micropolar fluids,1965, Technical Report. DTIC Document. 5. Lukaszewicz, G., Micropolar fluids: theory and applications, 1999, Springer. 6. Widodo, B. Anggriani, I. Imron, C., The Characterization of Boundary Layer in The Magnetohydrodynamic Micropolar Fluid Past a Solid Sphere, 2015, Proceedings of ISERD International Conference. 105-108. 7. Cheng, C-Y., Natural Convection Heat and Mass Transfer from a sphere in micropolar fluids with constant wall temperature and concentrartion. International Communications in Heat and Mass Transfer, 2008, 35(6):750-755. 8. Ali, F.M., Nazar, R., Arifin, N. M, Numerical Solutions of Unsteady Boundary Layer Flow due to an Impulsively Stretching Surface,2010, Journal of Applied Computer Science and Mathematics, no. 8(4)/2010, Suceava. 9. Imron, C., Suhariningsih. Widodo, B., Yuwono, T., Numerical Simulation of Fluid Flow Around Circular and I-Shape Cylinder in a Tandem Configuration, 2013, Applied Mathematical Sciences, Vol. 7, 2013, no. 114, 5657-5666 HIKARI Ltd. 368