MHD Flow Heat and Mass Transfer of Micropolar Fluid
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Turbulent-Prandtl-Number.Pdf
Atmospheric Research 216 (2019) 86–105 Contents lists available at ScienceDirect Atmospheric Research journal homepage: www.elsevier.com/locate/atmosres Invited review article Turbulent Prandtl number in the atmospheric boundary layer - where are we T now? ⁎ Dan Li Department of Earth and Environment, Boston University, Boston, MA 02215, USA ARTICLE INFO ABSTRACT Keywords: First-order turbulence closure schemes continue to be work-horse models for weather and climate simulations. Atmospheric boundary layer The turbulent Prandtl number, which represents the dissimilarity between turbulent transport of momentum and Cospectral budget model heat, is a key parameter in such schemes. This paper reviews recent advances in our understanding and modeling Thermal stratification of the turbulent Prandtl number in high-Reynolds number and thermally stratified atmospheric boundary layer Turbulent Prandtl number (ABL) flows. Multiple lines of evidence suggest that there are strong linkages between the mean flowproperties such as the turbulent Prandtl number in the atmospheric surface layer (ASL) and the energy spectra in the inertial subrange governed by the Kolmogorov theory. Such linkages are formalized by a recently developed cospectral budget model, which provides a unifying framework for the turbulent Prandtl number in the ASL. The model demonstrates that the stability-dependence of the turbulent Prandtl number can be essentially captured with only two phenomenological constants. The model further explains the stability- and scale-dependences -
Analysis of Mass Transfer by Jet Impingement and Heat Transfer by Convection
Analysis of Mass Transfer by Jet Impingement and Study of Heat Transfer in a Trapezoidal Microchannel by Ejiro Stephen Ojada A thesis submitted in partial fulfillment of the requirements for the degree of Master of Science in Mechanical Engineering Department of Mechanical Engineering University of South Florida Major Professor: Muhammad M. Rahman, Ph.D. Frank Pyrtle, III, Ph.D. Rasim Guldiken, Ph.D. Date of Approval: November 5, 2009 Keywords: Fully-Confined Fluid, Sherwood number, Rotating Disk, Gadolinium, Heat Sink ©Copyright 2009, Ejiro Stephen Ojada i TABLE OF CONTENTS LIST OF FIGURES ii LIST OF SYMBOLS v ABSTRACT viii CHAPTER 1: INTRODUCTION AND LITERATURE REVIEW 1 1.1 Introduction (Mass Transfer by Jet Impingement ) 1 1.2 Literature Review (Mass Transfer by Jet Impingement) 2 1.3 Introduction (Heat Transfer in a Microchannel) 7 1.4 Literature Review (Heat Transfer in a Microchannel) 8 CHAPTER 2: ANALYSIS OF MASS TRANSFER BY JET IMPINGEMENT 15 2.1 Mathematical Model 15 2.2 Numerical Simulation 19 2.3 Results and Discussion 21 CHAPTER 3: ANALYSIS OF HEAT TRANSFER IN A TRAPEZOIDAL MICROCHANNEL 42 3.1 Modeling and Simulation 42 3.2 Results and Discussion 48 CHAPTER 4: CONCLUSION 65 REFERENCES 67 APPENDICES 79 Appendix A: FIDAP Code for Analysis of Mass Transfer by Jet Impingement 80 Appendix B: FIDAP Code for Fluid Flow and Heat Transfer in a Composite Trapezoidal Microchannel 86 i LIST OF FIGURES Figure 2.1a Confined liquid jet impingement between a rotating disk and an impingement plate, two-dimensional schematic. 18 Figure 2.1b Confined liquid jet impingement between a rotating disk and an impingement plate, three-dimensional schematic. -
Turbulence, Entropy and Dynamics
TURBULENCE, ENTROPY AND DYNAMICS Lecture Notes, UPC 2014 Jose M. Redondo Contents 1 Turbulence 1 1.1 Features ................................................ 2 1.2 Examples of turbulence ........................................ 3 1.3 Heat and momentum transfer ..................................... 4 1.4 Kolmogorov’s theory of 1941 ..................................... 4 1.5 See also ................................................ 6 1.6 References and notes ......................................... 6 1.7 Further reading ............................................ 7 1.7.1 General ............................................ 7 1.7.2 Original scientific research papers and classic monographs .................. 7 1.8 External links ............................................. 7 2 Turbulence modeling 8 2.1 Closure problem ............................................ 8 2.2 Eddy viscosity ............................................. 8 2.3 Prandtl’s mixing-length concept .................................... 8 2.4 Smagorinsky model for the sub-grid scale eddy viscosity ....................... 8 2.5 Spalart–Allmaras, k–ε and k–ω models ................................ 9 2.6 Common models ........................................... 9 2.7 References ............................................... 9 2.7.1 Notes ............................................. 9 2.7.2 Other ............................................. 9 3 Reynolds stress equation model 10 3.1 Production term ............................................ 10 3.2 Pressure-strain interactions -
Influence of Heat Source/Sink on Free Convection in Annular Porous Region
International Journal of Heat and Technology Vol. 39, No. 3, June, 2021, pp. 841-850 Journal homepage: http://iieta.org/journals/ijht Influence of Heat Source/Sink on Free Convection in Annular Porous Region Anurag1, Shyam Lal Yadav2*, Ashok Kumar Singh1 1 Department of Mathematics, Institute of Science, Banaras Hindu University, Varanasi 221005, Uttar Pradesh, India 2 Department of Mathematics, Lok Nayak Jai Prakash Institute of Technology, Chhapra 841302, Bihar, India Corresponding Author Email: [email protected] https://doi.org/10.18280/ijht.390318 ABSTRACT Received: 4 January 2020 The significant interpretation of this model is to explore the influence of temperature- Accepted: 26 December 2020 dependent heat source/sink on laminar free-convective flow in an annular porous region such as petroleum engineering, thermal technique and groundwater hydrology. For a Keywords: unified solution of the Brinkman-Darcy model, the regulatory equations solved analytically fully developed flow, natural convection, by applying the variation of parameter technique in terms of Bessel's functions for the heat source and sink, isothermal and constant heat source and sink. Moreover, we have investigated the Variations of Darcy number, Heat flux, modified Bessel function source/sink and viscosity ratio in the presence of isothermal and constant heat flux sequentially. As a result, we received the critical value of the velocity for the radii ratio (R = 2.05 and 2.92) in both the cases of source and sink (S = 1.0 and Si = 0.1) respectively which is exhibited through the graphs. Further, the numerical outcomes present of the skin friction including volume flow with annular gap by the graphs as well as tables. -
Huq, P. and E.J. Stewart, 2008. Measurements and Analysis of the Turbulent Schmidt Number in Density
GEOPHYSICAL RESEARCH LETTERS, VOL. 35, L23604, doi:10.1029/2008GL036056, 2008 Measurements and analysis of the turbulent Schmidt number in density stratified turbulence Pablo Huq1 and Edward J. Stewart2 Received 18 September 2008; revised 27 October 2008; accepted 3 November 2008; published 3 December 2008. [1] Results are reported of measurements of the turbulent where rw is the buoyancy flux, uw is the Reynolds shear Schmidt number Sct in a stably stratified water tunnel stress. The ratio Km/Kr is termed the turbulent Schmidt experiment. Sct values varied with two parameters: number Sct (rather than turbulent Prandtl number) as Richardson number, Ri, and ratio of time scales, T*, of salinity gradients in water are used for stratification in the eddy turnover and eddy advection from the source of experiments. Prescription of a functional dependence of Sct turbulence generation. For large values (T* 10) values on Ri = N2/S2 is a turbulence closure scheme [Kantha and of Sct approach those of neutral stratification (Sct 1). In Clayson, 2000]. Here the buoyancy frequency N is defined 2 contrast for small values (T* 1) values of Sct increase by the gradient of density r as N =(Àg/ro)(dr/dz), and g is with Ri. The variation of Sct with T* explains the large the gravitational acceleration. S =dU/dz is the velocity scatter of Sct values observed in atmospheric and oceanic shear. Analyses of field, lab and numerical (RANS, DNS data sets as a range of values of T* occur at any given Ri. and LES) data sets have led to the consensus that Sct The dependence of Sct values on advective processes increases with Ri [see Esau and Grachev, 2007, and upstream of the measurement location complicates the references therein]. -
The Analogy Between Heat and Mass Transfer in Low Temperature Crossflow Evaporation
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by AUT Scholarly Commons The analogy between heat and mass transfer in low temperature crossflow evaporation Reza Enayatollahi*, Roy Jonathan Nates, Timothy Anderson Department of Mechanical Engineering, Auckland University of Technology, Auckland, New Zealand. Corresponding Author: Reza Enayatollahi Email Address: [email protected] Postal Address: WD308, 19 St Paul Street, Auckland CBD, Auckland, New Zealand Phone Number: +64 9 921 9999 x8109 Abstract This study experimentally determines the relationship between the heat and mass transfer, in a crossflow configuration in which a ducted airflow passes through a planar water jet. An initial exploration using the Chilton-Colburn analogy resulted in a coefficient of determination of 0.72. On this basis, a re-examination of the heat and mass transfer processes by Buckingham’s-π theorem and a least square analysis led to the proposal of a new dimensionless number referred to as the Lewis Number of Evaporation. A modified version of the Chilton-Colburn analogy incorporating the Lewis Number of Evaporation was developed leading to a coefficient of determination of 0.96. 1. Introduction Heat and mass transfer devices involving a liquid interacting with a gas flow have a wide range of applications including distillation plants, cooling towers and aeration processes and desiccant drying [1-5]. Many studies have gone through characterising the heat and mass transfer in such configurations [6-9]. The mechanisms of heat and mass transfer are similar and analogical. Therefore, in some special cases where, either the heat or mass transfer data are not reliable or may not be available, the heat and mass transfer analogy can be used to determine the missing or unreliable set of data. -
1 Pe = Re× Sc Peclet Number
Passive Scalar Diffusion in the Near Field Region of Turbulent Rectangular Submerged Free Jets Andrea Boghia, Ivan Di Venutab, Fabio Gorib,* a School of Water, Energy and Agrifood, Cranfield University, Cranfield, Bedfordshire MK43 0AL, United Kingdom, b Department of Industrial Engineering, University of Rome “Tor Vergata”, Via del Politecnico 1, 00133 Rome, Italy. * Corresponding Author, [email protected] Abstract Jets are a common way to transfer mass among fluids, or from a fluid to a surface. At moderate Reynolds numbers and low turbulent intensities the jet exhibits a Near Field Region (NFR) several diameters long. Numerical results and a theoretical model are presented for the passive scalar diffusion in the NFR of a submerged free jet. Large Eddy Simulations (LES), in the Reynolds number 5000-40,000 and the Schmidt number range 1-100, are performed obtaining the passive scalar fields. Three mathematical models for the passive scalar diffusion are presented; the first one is valid in the NFR, specifically in the Undisturbed Region of Flow (URF), and the other two, obtained under the hypotheses of Tollmien and Görtler momentum spreadings, are valid in the Potential Core Region (PCR). The last two models employ a turbulent Schmidt number inversely proportional to the mean velocity gradient, conclusion obtained by the LES numerical results. The self-similar solutions of the passive scalar show good agreement with the LES results. The wide range of Reynolds and Schmidt numbers investigated gives generality to the results. Keywords: Submerged Rectangular Free Jet; Turbulent Flow; Near Field Region; Undisturbed Region of Flow; Passive Scalar; Large Eddy Simulation; Self-Similarity. -
Stability of Thermosolutal Free Convection on Electrically Conducting Superposed Fluid and Porous Layer
International Journal of Applied Engineering Research ISSN 0973-4562 Volume 13, Number 17 (2018) pp. 13022-13030 © Research India Publications. http://www.ripublication.com Stability of Thermosolutal Free Convection on Electrically Conducting Superposed Fluid and Porous Layer K.Sumathi1*, T.Arunachalam2 and S.Aiswarya3 Department of Mathematics, 1,3PSGR Krishnammal College for Women, Coimbatore – 641 004, TamilNadu, India. 2Kumaraguru College of Technology, Coimbatore – 641 049, TamilNadu, India. (*Corresponding Author) Abstract investigated the onset of convection in a horizontal sparsely packed porous medium with imposed thermal and The effect of thermosolutal convection on linear stability of an concentration gradient at both the boundaries and found that incompressible fluid in a horizontal fluid/porous interface in Darcy number destabilizes the system in case of stationary the presence of a vertical magnetic field has been analyzed. and oscillatory convection. Asymptotic solution is obtained for rigid boundaries using normal mode analysis and the analysis is restricted to long Jena et al. [6] by employing Darcy-Brinkman-Forchheimer wave approximations. The influence of various non- model studied about the linear stability of onset of dimensional parameters such as Chandrasekhar number, thermosolutal convection in a rectangular annulus which is magnetic Prandtl number, Schmidt number, Prandtl number, highly heated and soluted from within and exposed to low porosity, wave number and depth ratio on stability thermal and solutal gradients from outside in a non-Darcian characteristics of flow field are represented numerically. region. Abdullah et al. [2] studied the effect of thermosolutal convection of a viscous incompressible fluid in the presence Keywords: Thermosolutal convection, magnetic field, fluid- of rotation on the stability of the system and observed that porous interface, stability analysis. -
Compressible Effects Modelling in Turbulent Cavitating Flows Jean Decaix, Eric Goncalvès Da Silva
Compressible effects modelling in turbulent cavitating flows Jean Decaix, Eric Goncalvès da Silva To cite this version: Jean Decaix, Eric Goncalvès da Silva. Compressible effects modelling in turbulent cav- itating flows. European Journal of Mechanics - B/Fluids, Elsevier, 2013, 39, pp.11-31. 10.1016/j.euromechflu.2012.12.001. hal-00768757 HAL Id: hal-00768757 https://hal.archives-ouvertes.fr/hal-00768757 Submitted on 12 Feb 2013 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. Compressible Effects Modelling in Turbulent Cavitating Flows Jean Decaix∗, Eric Goncalv`es∗ LEGI-Grenoble INP, 1025 rue de la Piscine, 38400 St Martin d’Heres, France Abstract A compressible, multiphase, one-fluid RANS solver has been developed to study turbulent cavitating flows. The interplay between turbulence and cav- itation regarding the unsteadiness and structure of the flow is complex and not well understood. This constitutes a determinant point to accurately sim- ulate the dynamic behaviour of sheet cavities. In the present study, different formulations including compressibility effects on turbulence are investigated. Numerical results are given for two partial cavities on Venturi geometries and comparisons are made with experimental data. -
Stability and Instability of Hydromagnetic Taylor-Couette Flows
Physics reports Physics reports (2018) 1–110 DRAFT Stability and instability of hydromagnetic Taylor-Couette flows Gunther¨ Rudiger¨ a;∗, Marcus Gellerta, Rainer Hollerbachb, Manfred Schultza, Frank Stefanic aLeibniz-Institut f¨urAstrophysik Potsdam (AIP), An der Sternwarte 16, D-14482 Potsdam, Germany bDepartment of Applied Mathematics, University of Leeds, Leeds, LS2 9JT, United Kingdom cHelmholtz-Zentrum Dresden-Rossendorf, Bautzner Landstr. 400, D-01328 Dresden, Germany Abstract Decades ago S. Lundquist, S. Chandrasekhar, P. H. Roberts and R. J. Tayler first posed questions about the stability of Taylor- Couette flows of conducting material under the influence of large-scale magnetic fields. These and many new questions can now be answered numerically where the nonlinear simulations even provide the instability-induced values of several transport coefficients. The cylindrical containers are axially unbounded and penetrated by magnetic background fields with axial and/or azimuthal components. The influence of the magnetic Prandtl number Pm on the onset of the instabilities is shown to be substantial. The potential flow subject to axial fieldspbecomes unstable against axisymmetric perturbations for a certain supercritical value of the averaged Reynolds number Rm = Re · Rm (with Re the Reynolds number of rotation, Rm its magnetic Reynolds number). Rotation profiles as flat as the quasi-Keplerian rotation law scale similarly but only for Pm 1 while for Pm 1 the instability instead sets in for supercritical Rm at an optimal value of the magnetic field. Among the considered instabilities of azimuthal fields, those of the Chandrasekhar-type, where the background field and the background flow have identical radial profiles, are particularly interesting. -
Numerical Simulation of Williamson Combined Natural and Forced
entropy Article Numerical Simulation of Williamson Combined Natural and Forced Convective Fluid Flow between Parallel Vertical Walls with Slip Effects and Radiative Heat Transfer in a Porous Medium Mohammad Yaghoub Abdollahzadeh Jamalabadi 1,*, Payam Hooshmand 2, Navid Bagheri 3, HamidReza KhakRah 4 and Majid Dousti 5 1 Department of Mechanical, Robotics and Energy Engineering, Dongguk Universit, Seoul 04620, Korea 2 Young Researchers and Elite Club, Mahabad Branch, Islamic Azad University, Mahabad 433-59135, Iran; [email protected] 3 Department of Energy Engineering, Graduate School of the Environment and Energy, Science and Research Branch, Islamic Azad University, Tehran 1477893855, Iran; [email protected] 4 Department of Mechanical Engineering, College of Engineering, Shiraz Branch, Islamic Azad University, Shiraz 71987-74731, Iran; [email protected] 5 Faculty of Engineering, Zanjan University, Zanjan 38791-45371, Iran; [email protected] * Correspondence: [email protected] or [email protected]; Tel.: +82-22-260-3073 Academic Editor: Milivoje M. Kostic Received: 29 February 2016; Accepted: 8 April 2016; Published: 18 April 2016 Abstract: Numerical study of the slip effects and radiative heat transfer on a steady state fully developed Williamson flow of an incompressible Newtonian fluid; between parallel vertical walls of a microchannel with isothermal walls in a porous medium is performed. The slip effects are considered at both boundary conditions. Radiative highly absorbing medium is modeled by the Rosseland approximation. The non-dimensional governing Navier–Stokes and energy coupled partial differential equations formed a boundary problem are solved numerically using the fourth order Runge–Kutta algorithm by means of a shooting method. Numerical outcomes for the skin friction coefficient, the rate of heat transfer represented by the local Nusselt number were presented even as the velocity and temperature profiles illustrated graphically and analyzed. -
Finite Element Solutions for Non-Newtonian Pulsatile Flow in a Non-Darcian Porous Medium Conduit ∗
Nonlinear Analysis: Modelling and Control, 2007, Vol. 12, No.3, 317–327 Finite Element Solutions for Non-Newtonian Pulsatile Flow in a Non-Darcian Porous Medium Conduit ∗ R. Bhargava1, H. S. Takhar2, S. Rawat1, Tasveer A. Bég3, O. Anwar Bég4 1Mathematics Department, Indian Institute of Technology Roorkee-247667, India [email protected] 2Engineering Department, Manchester Metropolitan University Oxford Rd., Manchester, M5 1GD, UK [email protected] 3Engineering Mechanics and Earthquake Dynamics Research 18 Milton Grove, Manchester, M16 OBP [email protected] 4Fire Engineering Sciences, Leeds College of Building / Leeds Metropolitan University North Street, Leeds, LS2 7QT, UK [email protected] Received: 17.05.2006 Revised: 08.11.2006 Published online: 31.08.2007 Abstract. The present analysis is motivated by the need to elucidate with more accuracy and sophistication the hydrodynamics of non-Newtonian flow via a channel containing a porous material under pulsating pressure gradient. A one-dimensional transient rheological model for pulsating flow through a Darcy-Forcheimmer porous channel is used. A modified Casson non-Newtonian constitutive model is employed for the transport fluid with a drag force formulation for the porous body force effects. The model is transformed and solved using a finite element numerical technique. Rheological effects are examined using a β parameter which vanishes in the limit (Newtonian flow). Velocity profiles are plotted for studying the influence of Reynolds number, Darcy number, Forchheimer number and the β (non-Newtonian) parameter. The channel considered is rigid with a pulsatile pressure applied via an appropriate pressure gradient term. The model finds applications in industrial filtration systems, pumping of polymeric fluids etc.