UNIVERSITI PUTRA MALAYSIA STABILITY OF MARANGONI CONVECTION IN A FLUID LAYER WITH TEMPERATURE-DEPENDENT VISCOSITY NURUL HAFIZAH BINTI ZAINAL ABIDIN

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UNIVERSITI PUTRA MALAYSIA STABILITY OF MARANGONI CONVECTION IN A FLUID LAYER WITH TEMPERATURE-DEPENDENT VISCOSITY NURUL HAFIZAH BINTI ZAINAL ABIDIN IPM 2007 3

STABILITY OF MARANGONI CONVECTION IN A FLUID LAYER WITH TEMPERATURE-DEPENDENT VISCOSITY By NURUL HAFIZAH BINTI ZAINAL ABIDIN Thesis Submitted to the School of Graduate Studies, Universiti Putra Malaysia, in Fulfilment of the Requirements for the Degree of Master of Science OCTOBER 2007

To My Family and Friends. ii

Abstract of thesis presented to the Senate of Universiti Putra Malaysia in fulfilment of the requirement for the degree of Master of Science STABILITY OF MARANGONI CONVECTION IN A FLUID LAYER WITH TEMPERATURE-DEPENDENT VISCOSITY By NURUL HAFIZAH BINTI ZAINAL ABIDIN October 2007 Chair Institute : Norihan Md Arifin, PhD : Institute for Mathematical Research The onset of steady Marangoni convection induced by surface tension gradients along the upper surface of a horizontal layer of fluid have been the subject of a great deal of theoretical work since the pioneering theoretical investigations of Pearson (1958). The system is heated from below and cooled from above. The purpose of the thesis is to study in detail the onset of Marangoni convection with temperaturedependent viscosity. Few cases of boundary conditions at the bottom surface are studied which are conducting with no-slip, conducting with free-slip and insulating with no-slip. We perform a detailed numerical calculation of the marginal stability curves. We showed that the effect of a temperature-dependent viscosity may be either stabilizing or destabilizing depending on the measurement of the relative variation of viscosity in the fluid volume (viscosity group, R v ). We also present the problem to a case where the fluid layer is overlying a solid layer and here, we undertake a detailed investigation to look at the effect of the thickness or the iii

conductivity of the solid layer to the onset of Marangoni convection with temperature-dependent viscosity. Again we perform a detailed numerical calculation of marginal stability curves. We showed that the coupled effect of the solid layer depth (or its conductivity) and a temperature-dependent viscosity (with negative sign of variation of viscosity with temperature) is to stabilize the fluid layer. iv

Abstrak tesis yang dikemukakan kepada Senat Universiti Putra Malaysia sebagai memenuhi keperluan untuk ijazah Master Sains KESTABILAN OLAKAN MARANGONI DALAM LAPISAN BENDALIR DENGAN KELIKATAN BERSANDAR PADA SUHU Oleh NURUL HAFIZAH BINTI ZAINAL ABIDIN Oktober 2007 Pengerusi Institut : Norihan Md Arifin, PhD : Institut Penyelidikan Matematik Permulaan olakan Marangoni mantap yang wujud disebabkan kecerunan tegangan permukaan diatas permukaan bebas menjadi penting sejak Pearson (1958) mengkajinya secara teori. Sistem pemodelan ini dipanaskan dari bawah dan disejukkan daripada atas. Tujuan tesis ini adalah untuk mengkaji secara terperinci kesan kelikatan bersandar pada suhu ke atas permulaan olakan Marangoni. Beberapa syarat sempadan pada permukaan bawah telah dikaji iaitu berkonduksi dengan tak gelincir, berkonduksi dengan bebas gelincir, dan berpenebat dengan tak gelincir. Kami menunjukkan secara berangka lengkung kestabilan sut dan mengkaji samada kelikatan bersandar kepada suhu akan menstabilkan atau menyahstabilkan sistem yang mana ia bergantung pada pekali variasi relatif kelikatan di dalam ruang bendalir (kumpulan kelikatan, R v ). Seterusnya, kami mengkaji kesan ketebalan atau kekonduksian satu lapisan pejal terhadap permulaan olakan Marangoni mantap dengan kelikatan bersandar kepada suhu sekiranya ia berada di bawah satu lapisan v

bendalir. Sekali lagi, kami tunjukkan secara terperinci pengiraan berangka lengkung kestabilan sut. Kami tunjukkan bahawa kedua-dua faktor ketebalan (atau kekonduksian) lapisan pejal dan kelikatan bersandar kepada suhu (dimana pekali variasi kumpulan kelikatan bernilai negatif) akan menstabilkan lapisan bendalir. vi

ACKNOWLEDGEMENTS Bismillahirrahmanirrahim. Alhamdulillah. In the Name of Allah, the Beneficient, the Merciful, I would like to express my appreciation for the guidance and assistance received throughout the journey of this thesis writing. Research will be a very lonesome activity if not for the wonderful researchers of the domain and the environment. Now it has come to the crossing point, I realize, I may not arrive to this stage without the experience I gained from people around me. I would like to thank my respected supervisor and co-supervisor; Dr. Norihan Md. Arifin and Prof. Dr. Mohd. Salmi Md. Noorani, for the endless motivation, support, trust and for teaching me to be more patient and wiser. I am very grateful for the opportunity to do my research in Institute for Mathematical Research UPM which provides a very good research environment. Thank you to the institute for providing all equipments that I need. Special thanks to the staff from the institute who have been very supportive and very helpful throughout my studies here. I want to thank all my dear friends and research colleagues for being my shoulder to cry on, for the generous information sharing, constructive arguments and accompany. Last, but never the least, to the most important person of my life, my parent and to the members of the family who always giving their unconditional love and support throughout my ups and downs, not only for me as a student but also as their still growing child. Thank you very much. vii

I certify that an Examination Committee has met on 5 th October 2007 to conduct the final examination of Nurul Hafizah binti Zainal Abidin on her Master of Science thesis entitled Stability of Marangoni Convection in a Fluid Layer with Temperature-dependant Viscosity in accordance with Universiti Pertanian Malaysia (Higher Degree) Act 1980 and Universiti Pertanian Malaysia (Higher Degree) Regulations 1981. The Committee recommends that the student be awarded the degree of Master of Science. Members of the Examination Committee were as follows: Nik Mohd Asri Nik Long, PhD Lecturer Institute for Mathematical Research Universiti Putra Malaysia (Chairman) Fudziah Ismail, PhD Associate Professor Institute for Mathematical Research Universiti Putra Malaysia (Internal Examiner) Mohd Noor Saad, PhD Lecturer Faculty of Science Universiti Putra Malaysia (Internal Examiner) Bachok M. Taib, PhD Professor Faculty of Science & Technology Universiti Sains Islam Malaysia (External Examiner) HASANAH MOHD. GHAZALI, PhD Professor and Deputy Dean School of Graduate Studies Universiti Putra Malaysia Date: 17 December 2007 viii

This thesis was submitted to the Senate of Universiti Putra Malaysia and has been accepted as fulfilment of the requirement for the degree of Master of Science. The members of the Supervisory Committee were as follows: NORIHAN MD ARIFIN, PhD Lecturer Institute for Mathematical Research Universiti Putra Malaysia (Chairman) MOHD SALMI MD NOORANI, PhD Professor Institute for Mathematical Research Universiti Putra Malaysia (Member) AINI IDERIS, PhD Professor and Dean School of Graduate Studies Universiti Putra Malaysia Date: 22 January 2008 ix

DECLARATION I hereby declare that the thesis is based on my original work except for quotations and citations, which have been duly acknowledged. I also declare that it has not been previously or concurrently submitted for any other degree at UPM or other institutions. NURUL HAFIZAH BINTI ZAINAL ABIDIN Date: x

TABLE OF CONTENTS Page DEDICATION ABSTRACT ABSTRAK ACKNOWLEDGEMENTS APPROVAL DECLARATION LIST OF TABLES LIST OF FIGURES LIST OF ABBREVIATIONS ii iii v vii viii x xiii xiv xviii CHAPTER 1 INTRODUCTION 1-1 1.1 Convection in a Fluid Layer 1-2 1.1.1 Physical Mechanism for Marangoni Convection 1-3 1.1.2 Convection with Variable Viscosity Effect 1-4 1.2 Mathematical Formulation of a Model Problem 1-7 1.3 Linear Theory of Marangoni Convection 1-15 1.4 Objectives 1-18 1.5 The Scope of The Thesis 1-18 2 LITERATURE REVIEW 2-1 3 METHODOLOGY 3-1 3.1 Problem Formulation 3-1 3.2 Linear Stability Analysis 3-2 3.3 Numerical Solution 3-7 4 MARANGONI CONVECTION WITH TEMPERATURE-DEPENDENT VISCOSITY 4-1 4.1 Background 4-1 4.2 Conducting Case with No-slip Condition 4-11 4.3 Conducting Case with Free-slip Condition 4-13 4.4 Insulating Case with No-slip Condition 4-16 4.5 Conclusion 4-18 xi

5 BOUNDARY EFFECT ON MARANGONI CONVECTION IN A VARIABLE VISCOSITY FLUID LAYER 5-1 5.1 Background 5-1 5.2 Problem Formulation 5-5 5.3 Numerical Results 5-7 5.3 Conclusion 5-14 5 CONCLUSION AND FURTHER WORK 6-1 5.1 Conclusion 6-1 5.3 Further Work 6-3 REFERENCES R-1 APPENDICES A-1 BIODATA OF THE AUTHOR B-1 xii

LIST OF TABLES Table Page 1.1 Viscosities of some common fluids. 1-5 4.1 Critical values of the steady Marangoni numbers M sc, oscillatory Marangoni number M oc and corresponding wave numbers at R = B i = 0, B o = 0.1 and P r =1. 4-7 5.1 Critical values of the critical Marangoni numbers M c and corresponding wave numbers α c for k r = 1 and C r = 0. 5-8 xiii

LIST OF FIGURES Figure Page 1.1 (a) Honeycomb like pattern observed in Bénard convection and (b) Hexagon geometry showing the wavelength λ (Maroto et al. 2007). 1-2 1.2 Convection mechanism caused by surface tension gradient. 1-4 1.3 Laminar shear. 1-6 1.4 Pearson s model. 1-7 1.5 Marginal stability curve. 1-15 1.6 Marginal Stability Curve for (a) Conducting case and (b) Insulating case calculated from equation (1.43) and (1.44) where C r = 0 and B o = 0. 1-16 1.7 Marginal stability curve for a conducting case with a free-slip condition at the bottom where C r = 0 and B o = 0. 1-17 3.1 Physical model. 3-2 4.1 Marginal stability curves in the conducting case for Cr = 0, B i = 0 and various values of the viscosity number: (1) N = 0, (2) N = 0.7, (3) N = 1.5, (4) N = 3. 4-3 4.2 Marginal stability curves in the conducting case for N = 0.7, B i = 0, B o = 0.1 and various values of the crspation number: (1) C r = 10-6, (2) C r = 0.7 x 10 3, (3) C r = 0.85 x 10-3, (4) C r = 10-2. 4-3 c 4.3 Critical Marangoni number M c (marked as Ma ) vs. the viscosity parameter N in the conducting case for C r = 0 and B i = 0. The crosses are values for a linear viscosity law. 4-4 4.4 Marginal stability curves in the conducting case for Cr = 0, B i = 0 and various values of the viscosity number: (1) N = 0.18, (2) N = 1, (3) N = 2, (4) N = 3. 4-5 4.5 Critical Marangoni number M (marked as c c Ma ) vs. the modified Crispation number Cr in the conducting case for B i = 0, B o = 0.1 and xiv

various values of the viscosity number: (1) N = 0.18, (2) N = 1, (3) N = 2, (4) N = 3. 4-5 4.6 Marginal stability curves in the conducting case for Cr = 0, B i = 1 and various values of the viscosity number: (1) N = 0.18, (2) N = 1, (3) N = 2, (4) N = 3. 4-6 4.7 Marginal stability curves M vs. α, for B o = 0.1, B i = 0, Γ = 0.8 and different values of the Crispation number : C r = 0 (label 1); 3 C (label 2); C r = 10 2 r = 10 (label 3). Solid curves refer to R v = 0 and dashed curves to R v = 0.3. 4-8 4.8 Critical Marangoni number M c (marked as Ma sc ) vs. the Crispation number C r (marked as for Cr ) for B o = 0.1, B i = 0, Γ = 0.8 and various values of the viscosity group: R v = 0.5 (label 1); R v = 0.3 (label 2); R v = 0 (label 3); R v = 0.3 (label 4); R v = 0.5 (label 5). 4-9 4.9 Critical Marangoni number M c (marked as Ma sc ) vs. the Rayleigh number Ra c for B o = 0.1, P r = 1, Bi = 0 and various values of the Crispation number: C r = 0.0015 (label 1); C r = 0.001 (label 2); C r = 0.0005. (label 3). Solid curves refer to steady critical Marangoni Number, M sc and dashed ones to oscillatory Marangoni number, M oc. The viscosity group is equal to 0 and 0.3 on a, and b, respectively. 4-10 4.10 Critical Marangoni number M c (marked as Ma c ) vs. the Rayleigh number Ra c for C = 0.0005 r, R v = 20.3, P r = 1, B i = 0 and various values of the Bond number: B o = 0.1 (label 1); B o = 0.5 (label 2); B o = 1 (label 3). Solid curves refer to steady critical Marangoni number, M sc and dashed ones to oscillatory Marangoni number, M oc. 4-10 4.11 Marginal stability curves M vs. α, for B i = 0, C r = 0 and different values of the viscosity, R v. 4-12 4.12 Marginal stability curves M vs. α, for B o = 0.1, B i = 0, R v = 0.3 and different values of Crispation number, C r. 4-12 4.13 Marginal stability curves M vs. α, for B o = 0.1, B i = 0, R v = 0 and different values of Crispation number, C r. 4-13 4.14 Marginal stability curves M vs. α, for B i = 0, C r = 0 and different values of the viscosity group, R v. 4-14 4.15 Marginal stability curves M vs. α, for B o = 0.1, B i = 0, C r = 0.001 and different values of viscosity group, R v. 4-15 4.16 Marginal stability curves M vs. α, for B o = 0.1, B i = 0, R v = -0.3 and xv

different values of Crispation number, C r. 4-15 4.17 Marginal stability curves M vs. α, for B o = 0.1, B i = 0, R v = 0.3 and different values of Crispation number, C r. 4-16 4.18 Marginal stability curves M vs.α, for B i = 0, C r = 0 and different values of the viscosity, R v. 4-17 4.19 Marginal stability curves M vs.α, for B o = 0.1, B i = 0, R v = 0.3 and different values of Crispation number, C r. 4-17 5.1 Variation of R c with B for different values of d r and k r = 1. The solid lines correspond to B i -1 = 0 and the dashed lines to B i = 0. 5-2 5.2 Variation of R c with B for different values of k r and d r = 1. The solid lines correspond to B i -1 = 0 and the dashed lines to B i = 0. 5-2 5.3 Variation of R c with B for different values of Γ when B i = 0 and d r = 10. The solid lines correspond to k r = 10 and the dashed lines to k r = 0.1. 5-3 5.4 Variation of R c with B for different values of k r and Γ when d r = 10. The solid lines correspond to B i = 1.0 and the dashed lines to B i = 10. 5-4 5.5 Comparison of the critical Rayleigh number R c between asymptotic solution (dashed curves) and numerical solution (solid curves) for Γ = -0.1 and Γ = 1 when k r d r = 0.5 and B i = 0. 5-5 5.6 Physical model with a boundary slab. 5-6 5.7 Variation of marginal stability curves M with α, for different values of the depth ratio, d r. 5-9 5.8 Marginal stability curves M vs. α, for different values of the viscosity, R v where C r = 0, k r = 1, d r = 0.01. The solid lines correspond to B i = 2 and the dashed line to B i = 0. 5-10 5.9 Marginal stability curves M vs. α, for different values of the viscosity, R v where C r = 0, k r = 1, d r = 10. The solid lines correspond to B i = 2 and the dashed line to B i = 0. 5-11 5.10 Marginal stability curves M c vs. d r, for B i = 0, C r = 0, k r = 1 and different values of the viscosity, R v. 5-11 5.11 Variation of marginal stability curves M with α, for different values of the thermal conductivity ratio, k r. 5-12 5.12 Marginal stability curves M vs. α, for different values of the xvi

viscosity, R v where C r = 0, d r = 1, k r = 0.1. The solid lines correspond to B i = 2 and the dashed line to B i = 0. 5-13 5.13 Marginal stability curves M vs. α, for different values of the viscosity, R v where C r = 0, d r = 1 k r = 10. The solid lines correspond to B i = 2 and the dashed line to B i = 0. 5-13 5.14 Marginal stability curves M c vs. k r, for B i = 0, C r = 0, d r = 1 and different values of the viscosity, R v. 5-14 xvii

LIST OF ABBREVIATIONS a B i B o c C r d thermal expansion coefficient of density Biot number Bond number specific heat Crispation number depth of fluid layer d r depth ratio, d s /d d s f g h H k depth of solid layer shear stress gravity heat transfer coefficient mean curvature of the surface thermal conductivity of fluid k r thermal conductivity ratio, k s /k k s M p p g P r R R v s thermal conductivity of solid layer Marangoni number pressure gas pressure Prandtl number Rayleigh number Viscosity group growth rate xviii

t T T g time temperature of fluid temperature of the ambient gas T s temperature of solid layer u velocity x, y, z Cartesian coordinates Greek Abbreviations α γ δ d wavenumber thermal expansion coefficient of dynamic viscosity surface deflection ε ζ θ κ thermal expansion coefficient of surface tension thermal expansion coefficient of kinematic viscosity temperature disturbance thermal diffusivity of fluid κ s thermal diffusivity of solid layer μ ν ρ σ dynamic viscosity of fluid kinematic viscosity of fluid density of fluid surface tension xix

Subscript 0 reference quantity c s r critical state property of the solid plate ratio of the solid plate property to the fluid property xx

CHAPTER 1 INTRODUCTION Convection is the transfer of heat by the motion of or within a fluid. It may arise from the temperature differences either within the fluid or between the fluid and its boundary, other sources of density variations (such as variable salinity) or from the application of an external motive force. It is one of the three primary mechanisms of heat transfer, the others being conduction and radiation. Convection has a wide range of applications, including calculating forces and moments on aircraft, determining the mass flow rate of petroleum through pipelines and to predict weather patterns. Some of its principles are even used in traffic engineering, where the traffic is treated as a continuous fluid. Generally, convection means fluid motion caused by temperature difference with the temperature gradient pointing in any direction (Chapmen 1984). In this thesis, the stability on convection in a plane horizontal fluid layer heated from below is considered as it is one of the most common types of convection. It was studied for the first time by Pellew and Southwell (1940) and then was summarized by Chandrasekhar s (1961) book, where a nearly complete picture of the linear analysis called Rayleigh-Bénard convection was presented. Usually, the term Rayleigh-Bénard convection is attributed to convection due to buoyancy mechanism, while the term Marangoni convection refers to surface tension gradient mechanism. 1-1

(a) (b) Figure 1.1: (a) Honeycomb like pattern observed in Bénard convection and (b) Hexagon geometry showing the wavelength λ (Maroto et al. 2007) 1.1 Convection in a Fluid Layer When a fluid layer in a horizontal plane is heated from below, instabilities arise when the temperature gradient across the layer exceeds a certain critical value which is caused by buoyancy or by the surface tension gradient. Bénard (1900) and Block (1959) were the pioneers of the comprehensive investigation of convection for both mechanism. Bénard (1900), carrying his experiment on a thin horizontal layer of molten spermaceti with a free surface observed the establishment of a regular, steady pattern of flow cells when the layer is heated from below. These cells, which are known as Bénard cells, were mainly hexagonal, and the pattern resembled a honeycomb as shown in Figure 1.1. The distance between the central points of neighbouring hexagonal cells defines the wavelength of the system. Bénard (1900) believed that the phenomenon was caused by buoyancy and therefore, this experiment was regarded as the starting point of convection instabilities. But later, Block (1956) and 1-2

Pearson (1958) suggested that the convection was caused by surface tension gradient as the case studied used a thin fluid layer with a free surface where buoyancy may not exist. Block (1956) is the pioneer of convection that is caused by a surface tension gradient and the study is known as Marangoni convection. The experimental investigation of the convection led to the conclusion that the hexagonal pattern observed by Bénard (1900) was due to the surface tension gradient and not the buoyancy. In the experiment, a thin hydrocarbon film less than one millimeter with a free surface was used and Block (1956) observed that convection would stop when the fluid layer was covered on the top by a thin silicone layer. Hence, Block (1956) concluded that the convection in a fluid layer with a free surface was caused by surface tension gradient. Later, Pearson (1958) furthers the study of Marangoni convection theoretically. 1.1.1 Physical Mechanism for Marangoni Convection Consider a horizontal fluid layer bounded from below by a rigid boundary and from above by a free surface. An infinitesimal disturbance of the temperature on the surface, say a warm spot, creates surface tension traction on the surface if the surface tension coefficient of the fluid is a function of temperature. Since surface tension usually decreases with temperature, a warm spot will be a soft spot at the surface from which the fluid will be pulled away laterally as shown in figure 1.2. The fluid underneath the warm spot must consequently rise. The fluid motion at the surface 1-3

cold Warm spot hot Figure 1.2: Convection mechanism caused by surface tension gradient will be transmitted by viscosity to the interior of the fluid layer, but viscosity will also dampen the motion. The motion in the fluid can be sustained only if energy is provided to overcome the frictional losses. The required energy can be provided by a vertical temperature differences across the fluid layer, which can be heated from below. If sufficient energy is supplied, and if a critical vertical temperature difference is reached, convection caused by surface tension gradients will commence and will be sustained. 1.1.2 Convection with Variable Viscosity Effect Viscosity is a measure of the resistance of a fluid to deform under shear stress. Realistically, viscosity in a fluid depends on density. The higher the density of the fluid, the higher the viscosity will be. Fluid also possess a temperature-dependent viscosity which influences heat transport and the spatial structure of the fluid. When the temperature increases, the viscosity decreases, but for gases, the viscosity will increase. Viscosity varies widely with temperature, but temperature variation has the opposite effect on the viscosities of fluids because of their fundamentally different 1-4