On Numerical Simulation of Cavitating Flows Under Thermal Regime

Total Page:16

File Type:pdf, Size:1020Kb

On Numerical Simulation of Cavitating Flows Under Thermal Regime International Journal of Heat and Mass Transfer 105 (2017) 411–428 Contents lists available at ScienceDirect International Journal of Heat and Mass Transfer journal homepage: www.elsevier.com/locate/ijhmt On numerical simulation of cavitating flows under thermal regime ⇑ D. Colombet a,b,c, , E. Goncalvès Da Silva b,c,1, R. Fortes-Patella b,c a CNES, DLA, 52 rue Jacques Hillairet, 75612 Paris Cedex, France b Univ. Grenoble Alpes, LEGI, F-38000 Grenoble, France c CNRS, LEGI, F-38000 Grenoble, France article info abstract Article history: In this work, we investigate closure laws for the description of interfacial mass transfer in cavitating flows Received 3 April 2016 under thermal regime. In a first part, we show that, if bubble resident time in the low pressure area of the Received in revised form 15 September flow is larger than the inertial/thermal regime transition time, bubble expansion are no longer monitored 2016 by Rayleigh equation, but by heat transfer in the liquid phase at bubbles surfaces. The modelling of inter- Accepted 23 September 2016 facial heat transfer depends thus on a Nusselt number that is a function of the Jakob number and of the bubble thermal Péclet number. This original approach has the advantage to include the kinetic of phase change in the description of cavitating flow and thus to link interfacial heat flux to interfacial mass flux Keywords: during vapour production. The behaviour of such a model is evaluated for the case of inviscid cavitating Bubble Mixture model flow in expansion tubes for water and refrigerant R114 using a four equations mixture model. Compared Cavitation with inertial regime (Rayleigh equation), results obtained considering thermal regime seem to predict Heat/mass transfer lower local gas volume fraction maxima as well as lower gradients of velocity and gas volume fraction. Numerical simulation It is observed that global vapour production is closely monitored by volumetric interfacial area (bubble size and gas volume fraction) and mainly by the Jakob number variations. It is found that, in contrast with phase change occurring in common boiling flow, Jakob number variation is influenced by phasic temper- /ðq =q ÞD ature difference but also by density ratio variation with pressure and temperature (Ja L G T). Ó 2016 Elsevier Ltd. All rights reserved. 1. Introduction and model based on inertial [4] or thermal bubble growth [5].To estimate locally vapour volume fraction, one first approach is to Cavitation is involved in various flow applications such as assimilate the gas–liquid mixture to a barotropic fluid. In other hydraulic turbines, pumps, rocket turbopump inducers, fuel injec- words, the density of the gas–liquid mixture is considered to be tors, marine propellers, underwater bodies, etc. In most of cases, a function of the local static pressure in the flow. For the simulation cavitation is an undesirable phenomenon, significantly degrading of a cavitating flow through a venturi, [1] proposed a sinus barotro- performance, resulting in lower pressure head of pumps, asymmet- pic law considering a direct link between the gas volume fraction, ric load on turbomachinery blades, vibrations, noise and erosion. In phasic densities, local pressure and vapour saturation pressure. For industrial applications, cavitating flows usually take form as a tur- the simulation of cavitating flows in tubopump inducers of spatial bulent vapour polydispersed bubbly flow with phase change, bub- rockets, [6] proposed a sinus barotropic law with a vapour satura- ble break-up and coalescence. In the literature, various gas–liquid tion pressure calculated from local temperature in the flow. Those mixture or two-fluid models have been developed to investigate robust approaches have provided interesting results for the simu- isothermal and non-isothermal cavitating flows. According to the lation of hydrofoils [7], venturies [8], turbopump inducers [9–11], assumptions made, those models differ on two main points: equa- pump-turbines [12] or fuel injectors [13]. Although the simplicity tions solved and description of phase change. of this modelling approach, this model enable to study complex Among cavitation models, different approaches can be found to industrial applications. However, the adaptability of such model describe phase change due to cavitation: barotropic model [1], for thermosensitive liquids, where temperature gradients are sig- short relaxation time model [2], velocity divergence model [3] nificant, seem to suffer from a lake of physical descriptions of mass and heat transfers induced by phase change at bubbles surfaces. ⇑ Corresponding author at: Univ. Grenoble Alpes, LEGI, F-38000 Grenoble, France. One second approach is to express explicitly mass and heat E-mail addresses: [email protected] (D. Colombet), eric. transfer terms and to consider that interfacial transfers are [email protected] (E. Goncalvès Da Silva), [email protected] instantaneous. In that case, as proposed by [2] or [14], by introduc- (R. Fortes-Patella). ing infinite relaxation parameters (or infinite global transfer 1 Present address: ENSMA, Poitiers, France. http://dx.doi.org/10.1016/j.ijheatmasstransfer.2016.09.070 0017-9310/Ó 2016 Elsevier Ltd. All rights reserved. 412 D. Colombet et al. / International Journal of Heat and Mass Transfer 105 (2017) 411–428 Nomenclature Tk tempreature of phase k,K À1 List of symbols u stretching velocity, m s À1 3 aI volumetric interfacial area, m V b bubble volume, m v ; À1 B B factor k velocity of phase k ms v gas liquid mixture velocity, m sÀ1 Cpk specific heat capacity of phase k at constant pressure, m À1 À1 v Jkg K r mean relative velocity between phases, v ¼ v À v ; msÀ1 Cvk specific heat capacity of phase k at constant volume, r G L À À Jkg 1 K 1 À1 cw Wood’s speed of sound, m s Greek symbols À1 cEOS speed of sound based on sinus equation of state, m s ak volume fraction of phase k ; À1 c ; c ¼ = ck speed of sound of phase k ms k heat capacity ratio for phase k k Cpk Cvk À3 À1 db mean Sauter diameter of the bubble size distribution, m Ck mass transfer term of phase k; kg m s th ; th ¼ k =ðq Þ; 2 À1 k ; À1 À1 Dk thermal diffusivity of phase k Dk k kCpk m s k conductivity of phase k Wm K À1 l ek specific internal energie of phase k; Jkg k dynamic viscosity of phase k,Pas À À1 2 1 mk kinematic viscosity of phase k; m s Ek total energy of phase k; Jkg À1 pk internal energy reference in stiffened gas equation of Em gas liquid mixture total energy, J kg À1 ; À2 À1 state, J kg HL heat transfer coefficient in phase k Wm K À À q ; 3 1 k density of phase k kg m hk specific enthalpie of phase k; Jkg À À s time for inception of thermal regime, s J local mass flux, kg m 2 s 1 loc s0 time for inception of thermal regime with effect of the Ja Jakob number, Ja ¼ q C DT=ðq LÞ L pL G relative velocity, s l mean length of bubble path in the low pressure area s resident time of bubbles in the low pressure area, s where p < psat; m res À1 L latent heat of vaporisation L ¼ hG À hL; Jkg Supercripts NuL Nusselt number I at the bubble surface NuL0 Nusselt number wihout wlip p pressure, Pa sat at saturation 1 T at triple point pk pressure reference in stiffened gas equation of state, Pa ¼ = th Pe thermal Péclet number, Pe Udb DL Pec critical thermal Péclet number, Subscripts ¼ m = G gas phase Pr Prandtl number, Pr L DLth 00 ; À3 À1 k phase k qk interfacial heat flux from phase k Jm s R bubble radius, m L liquid phase ¼ q v =l m gas liquid mixture Re bubble Reynolds number, Re L rdb L À s surface tension of the fluid, Nm 1 0 initial value 2 Sb bubble surface, m t time, s coefficients), momentum, mass and heat transfers can be evaluated injectors [31]. For the simulation of cavitating flow in cryogenic considering very short equilibrium relaxation times between pha- fluids, [32,33] use the formulation proposed by [21]. sic pressures, velocities, temperatures, Gibbs free energy. This Various authors have attempted to take into account the effect approach, initially devoted for the simulation of diphasic detona- of liquid phase thermal gradients in the flow on cavitation. For bar- tion waves [15], is considered to be valid for cavitating flow at very otropic approach [34,6] as well as for inertial controlled growth high velocity. As shown recently by [3], very similar results can be model [33,35,36], it has been done meanly by calculating the satu- achieved considering simply that the mass transfer term is propor- rated vapour pressure as a function of the local temperature tional to the mixture velocity divergence. This approach has been (psatðTÞ) and by estimating the bubble temperature variation using recently used for non isothermal cavitation by [16] for the 2D sim- energy balance at the bubble scale. In the same time, a few numer- ulations of cavitating flow through a venturi. ical works evoked that vapour production can be driven by thermal To describe cavitation, one last approach is to consider finite controlled growth of vapour bubbles [37–39,5].In[37], authors rate mass transfer and to express explicitly mass transfer exchange recall that bubble growth follow two steps. The increase of bubble term due to phase change. In the literature, a large number of such volume is initially controlled by the liquid inertial (inertial growth) cavitation models consider that vapour production in a cavitating and then is controlled by heat transfer at bubble surface (thermal flow is only driven by inertial controlled growth of vapour bubbles.
Recommended publications
  • Convection Heat Transfer
    Convection Heat Transfer Heat transfer from a solid to the surrounding fluid Consider fluid motion Recall flow of water in a pipe Thermal Boundary Layer • A temperature profile similar to velocity profile. Temperature of pipe surface is kept constant. At the end of the thermal entry region, the boundary layer extends to the center of the pipe. Therefore, two boundary layers: hydrodynamic boundary layer and a thermal boundary layer. Analytical treatment is beyond the scope of this course. Instead we will use an empirical approach. Drawback of empirical approach: need to collect large amount of data. Reynolds Number: Nusselt Number: it is the dimensionless form of convective heat transfer coefficient. Consider a layer of fluid as shown If the fluid is stationary, then And Dividing Replacing l with a more general term for dimension, called the characteristic dimension, dc, we get hd N ≡ c Nu k Nusselt number is the enhancement in the rate of heat transfer caused by convection over the conduction mode. If NNu =1, then there is no improvement of heat transfer by convection over conduction. On the other hand, if NNu =10, then rate of convective heat transfer is 10 times the rate of heat transfer if the fluid was stagnant. Prandtl Number: It describes the thickness of the hydrodynamic boundary layer compared with the thermal boundary layer. It is the ratio between the molecular diffusivity of momentum to the molecular diffusivity of heat. kinematic viscosity υ N == Pr thermal diffusivity α μcp N = Pr k If NPr =1 then the thickness of the hydrodynamic and thermal boundary layers will be the same.
    [Show full text]
  • 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
    [Show full text]
  • Chapter 5 Dimensional Analysis and Similarity
    Chapter 5 Dimensional Analysis and Similarity Motivation. In this chapter we discuss the planning, presentation, and interpretation of experimental data. We shall try to convince you that such data are best presented in dimensionless form. Experiments which might result in tables of output, or even mul- tiple volumes of tables, might be reduced to a single set of curves—or even a single curve—when suitably nondimensionalized. The technique for doing this is dimensional analysis. Chapter 3 presented gross control-volume balances of mass, momentum, and en- ergy which led to estimates of global parameters: mass flow, force, torque, total heat transfer. Chapter 4 presented infinitesimal balances which led to the basic partial dif- ferential equations of fluid flow and some particular solutions. These two chapters cov- ered analytical techniques, which are limited to fairly simple geometries and well- defined boundary conditions. Probably one-third of fluid-flow problems can be attacked in this analytical or theoretical manner. The other two-thirds of all fluid problems are too complex, both geometrically and physically, to be solved analytically. They must be tested by experiment. Their behav- ior is reported as experimental data. Such data are much more useful if they are ex- pressed in compact, economic form. Graphs are especially useful, since tabulated data cannot be absorbed, nor can the trends and rates of change be observed, by most en- gineering eyes. These are the motivations for dimensional analysis. The technique is traditional in fluid mechanics and is useful in all engineering and physical sciences, with notable uses also seen in the biological and social sciences.
    [Show full text]
  • Turbulent Prandtl Number and Its Use in Prediction of Heat Transfer Coefficient for Liquids
    Nahrain University, College of Engineering Journal (NUCEJ) Vol.10, No.1, 2007 pp.53-64 Basim O. Hasan Chemistry. Engineering Dept.- Nahrain University Turbulent Prandtl Number and its Use in Prediction of Heat Transfer Coefficient for Liquids Basim O. Hasan, Ph.D Abstract: eddy conductivity is unspecified in the case of heat transfer. The classical approach for obtaining the A theoretical study is performed to determine the transport mechanism for the heat transfer problem turbulent Prandtl number (Prt ) for liquids of wide follows the laminar approach, namely, the momentum range of molecular Prandtl number (Pr=1 to 600) and thermal transport mechanisms are related by a under turbulent flow conditions of Reynolds number factor, the Prandtl number, hence combining the range 10000- 100000 by analysis of experimental molecular and eddy viscosities one obtain the momentum and heat transfer data of other authors. A Boussinesq relation for shear stress: semi empirical correlation for Prt is obtained and employed to predict the heat transfer coefficient for du the investigated range of Re and molecular Prandtl ( ) 1 number (Pr). Also an expression for momentum eddy m dy diffusivity is developed. The results revealed that the Prt is less than 0.7 and is function of both Re and Pr according to the following relation: and the analogous relation for heat flux: Prt=6.374Re-0.238 Pr-0.161 q dT The capability of many previously proposed models of ( h ) 2 Prt in predicting the heat transfer coefficient is c p dy examined. Cebeci [1973] model is found to give good The turbulent Prandtl number is the ratio between the accuracy when used with the momentum eddy momentum and thermal eddy diffusivities, i.e., Prt= m/ diffusivity developed in the present analysis.
    [Show full text]
  • Anomalous Viscosity, Resistivity, and Thermal Diffusivity of the Solar
    Anomalous Viscosity, Resistivity, and Thermal Diffusivity of the Solar Wind Plasma Mahendra K. Verma Department of Physics, Indian Institute of Technology, Kanpur 208016, India November 12, 2018 Abstract In this paper we have estimated typical anomalous viscosity, re- sistivity, and thermal difffusivity of the solar wind plasma. Since the solar wind is collsionless plasma, we have assumed that the dissipation in the solar wind occurs at proton gyro radius through wave-particle interactions. Using this dissipation length-scale and the dissipation rates calculated using MHD turbulence phenomenology [Verma et al., 1995a], we estimate the viscosity and proton thermal diffusivity. The resistivity and electron’s thermal diffusivity have also been estimated. We find that all our transport quantities are several orders of mag- nitude higher than those calculated earlier using classical transport theories of Braginskii. In this paper we have also estimated the eddy turbulent viscosity. arXiv:chao-dyn/9509002v1 5 Sep 1995 1 1 Introduction The solar wind is a collisionless plasma; the distance travelled by protons between two consecutive Coulomb collisions is approximately 3 AU [Barnes, 1979]. Therefore, the dissipation in the solar wind involves wave-particle interactions rather than particle-particle collisions. For the observational evidence of the wave-particle interactions in the solar wind refer to the review articles by Gurnett [1991], Marsch [1991] and references therein. Due to these reasons for the calculations of transport coefficients in the solar wind, the scales of wave-particle interactions appear more appropriate than those of particle-particle interactions [Braginskii, 1965]. Note that the viscosity in a turbulent fluid is scale dependent.
    [Show full text]
  • Prandtl Number and Thermoacoustic Refrigerators M
    Prandtl number and thermoacoustic refrigerators M. E. H. Tijani, J. C. H. Zeegers, and A. T. A. M. de Waele Department of Applied Physics, Eindhoven University of Technology, P.O. Box 513, 5600 MB Eindhoven, The Netherlands ͑Received 28 November 2001; revised 25 April 2002; accepted 4 May 2002͒ From kinetic gas theory, it is known that the Prandtl number for hard-sphere monatomic gases is 2/3. Lower values can be realized using gas mixtures of heavy and light monatomic gases. Prandtl numbers varying between 0.2 and 0.67 are obtained by using gas mixtures of helium–argon, helium–krypton, and helium–xenon. This paper presents the results of an experimental investigation into the effect of Prandtl number on the performance of a thermoacoustic refrigerator using gas mixtures. The measurements show that the performance of the refrigerator improves as the Prandtl number decreases. The lowest Prandtl number of 0.2, obtained with a mixture containing 30% xenon, leads to a coefficient of performance relative to Carnot which is 70% higher than with pure helium. © 2002 Acoustical Society of America. ͓DOI: 10.1121/1.1489451͔ PACS numbers: 43.35.Ud, 43.35.Ty ͓RR͔ I. INTRODUCTION while compressing and expanding. The interaction of the moving gas in the stack with the stack surface generates heat The basic understanding of the physical principles un- transport.2 A detailed description of the refrigerator can be derlying the thermoacoustic effect is well established and has found in the literature.3,6 been discussed in many papers.1,2 However, a quantitative experimental investigation of the effect of some important parameters on the behavior of the thermoacoustic devices is II.
    [Show full text]
  • Numerical Calculations of Two-Dimensional Large Prandtl Number Convection in a Box
    J. Fluid Mech. (2013), vol. 729, pp. 584–602. c Cambridge University Press 2013 584 doi:10.1017/jfm.2013.330 Numerical calculations of two-dimensional large Prandtl number convection in a box J. A. Whitehead1,†, A. Cotel2, S. Hart3, C. Lithgow-Bertelloni4 and W. Newsome5 1Physical Oceanography Department, Woods Hole Oceanographic Institution, Woods Hole, MA 02543, USA 2Civil and Environmental Engineering Department, University of Michigan, 1351 Beal Avenue, Ann Arbor, MI 48109, USA 3Geology and Geophysics Department, Woods Hole Oceanographic Institution, Woods Hole, MA 02543, USA 4Department of Earth Sciences, University College London, Gower Street, London WC1E 6BT, UK 5Geological Sciences Department, University of Michigan, 1100 North University Avenue, Ann Arbor, MI 48109, USA (Received 30 August 2012; revised 17 June 2013; accepted 22 June 2013; first published online 24 July 2013) Convection from an isolated heat source in a chamber has been previously studied numerically, experimentally and analytically. These have not covered long time spans for wide ranges of Rayleigh number Ra and Prandtl number Pr. Numerical calculations of constant viscosity convection partially fill the gap in the ranges Ra 103–106 and Pr 1; 10; 100; 1000 and . Calculations begin with cold fluid everywhereD and localizedD hot temperature at1 the centre of the bottom of a square two-dimensional chamber. For Ra > 20 000, temperature increases above the hot bottom and forms a rising plume head. The head has small internal recirculation and minor outward conduction of heat during ascent. The head approaches the top, flattens, splits and the two remnants are swept to the sidewalls and diffused away.
    [Show full text]
  • The Influence of Prandtl Number on Free Convection in a Rectangular Cavity
    hr. J. Heor Mm\ Transfer. Vol. 24, pp. 125-131 0017-93lO/8ljOlOl-0125SOsoZ.OO/O 0 Pergamon Press Ltd. 1981. Printed in GreatBritain THE INFLUENCE OF PRANDTL NUMBER ON FREE CONVECTION IN A RECTANGULAR CAVITY W. P. GRAEBEL Department of Mechanical Engineering and Applied Mechanics, The University of Michigan, Ann Arbor, MI. 48109, U.S.A. (Receioed 19 May 1980) Abstract-Natural convection in a rectangular cavity is considered for the problem where one vertical wall is heated and the other is cooled. The boundary layer flow is solved using a modified Oseen technique in a manner similar to Gill’s solution. Temperature and velocity profiles in the core, and the Nusselt number, are found as functions of the Rayleigh and Prandtl numbers and the length ratio. The solution indicates that for a Prandtl number less than l/7, a midsection shear layer develops. NOMENCLATURE more reasonable matching condition and obtained overall Nusselt numbers which are in good agreement C, constant of integration; with available experimental and numerical heat- 9, gravitational constant ; transfer data. H, cavity height; The present note generalizes Gill’s results for arbit- K = (Pr - l)/(Pr + 1); rary values of the Prandtl number, so that the small L, cavity length; Prandtl number limit, suitable for liquid metals, can Nu, Nusselt number ; pressure; also be obtained. The method of Bejan is used in P? evaluating the constant of integration which appears Pr, Prandtl number ; in the solution. 49 =2u,/v2 (K + 1)3; Q, total heat flux; BASIC ASSUMPTIONS Ra, = jlgL3(TL - T&q Rayleigh number; The height of the cavity is taken as H and the T, temperature; horizontal spacing of the walls as The vertical walls 11,w, velocity components, u = a*/az, w = L.
    [Show full text]
  • Summary of Dimensionless Numbers of Fluid Mechanics and Heat Transfer 1. Nusselt Number Average Nusselt Number: Nul = Convective
    Jingwei Zhu http://jingweizhu.weebly.com/course-note.html Summary of Dimensionless Numbers of Fluid Mechanics and Heat Transfer 1. Nusselt number Average Nusselt number: convective heat transfer ℎ퐿 Nu = = L conductive heat transfer 푘 where L is the characteristic length, k is the thermal conductivity of the fluid, h is the convective heat transfer coefficient of the fluid. Selection of the characteristic length should be in the direction of growth (or thickness) of the boundary layer; some examples of characteristic length are: the outer diameter of a cylinder in (external) cross flow (perpendicular to the cylinder axis), the length of a vertical plate undergoing natural convection, or the diameter of a sphere. For complex shapes, the length may be defined as the volume of the fluid body divided by the surface area. The thermal conductivity of the fluid is typically (but not always) evaluated at the film temperature, which for engineering purposes may be calculated as the mean-average of the bulk fluid temperature T∞ and wall surface temperature Tw. Local Nusselt number: hxx Nu = x k The length x is defined to be the distance from the surface boundary to the local point of interest. 2. Prandtl number The Prandtl number Pr is a dimensionless number, named after the German physicist Ludwig Prandtl, defined as the ratio of momentum diffusivity (kinematic viscosity) to thermal diffusivity. That is, the Prandtl number is given as: viscous diffusion rate ν Cpμ Pr = = = thermal diffusion rate α k where: ν: kinematic viscosity, ν = μ/ρ, (SI units : m²/s) k α: thermal diffusivity, α = , (SI units : m²/s) ρCp μ: dynamic viscosity, (SI units : Pa ∗ s = N ∗ s/m²) W k: thermal conductivity, (SI units : ) m∗K J C : specific heat, (SI units : ) p kg∗K ρ: density, (SI units : kg/m³).
    [Show full text]
  • SUPERCOMPUTATIONS of LOW-PRANDTL-NUMBER CONVECTION FLOWS Jorg¨ Schumacher1 and Janet D
    XXIV ICTAM, 21-26 August 2016, Montreal, Canada SUPERCOMPUTATIONS OF LOW-PRANDTL-NUMBER CONVECTION FLOWS Jorg¨ Schumacher1 and Janet D. Scheel2 1Department of Mechanical Engineering, Technische Universitat¨ Ilmenau, Ilmenau, Germany 2Department of Physics, Occidental College, Los Angeles, USA Summary Massively parallel supercomputations are an important analysis tool to study the fundamental local and global mechanisms of heat and momentum transfer in turbulent convection. We discuss the perspectives and challenges in this vital field of fundamental turbulence research for the case of convection at very low Prandtl numbers. MOTIVATION AND SIMULATION MODEL Turbulent convection is an important area of present research in fluid dynamics with applications to diverse phenomena in nature and technology. The turbulent Rayleigh-Benard´ convection (RBC) model is at the core of all these turbulent flows. It can be studied in a controlled manner, but has enough complexity to contain the key features of turbulence in heated fluids. This flow in cylindrical cells has been investigated intensively over the last few years in several laboratory experiments all over the world [1]. In RBC, a fluid cell or layer is kept at a constant temperature difference ∆T = Tbottom − Ttop between top and bottom plates which are separated by a vertical distance H. The Rayleigh and Prandtl numbers are given by gαH3∆T ν Ra = and P r = : (1) νκ κ The parameter Ra characterizes the thermal driving in convective turbulence with the acceleration due to gravity, g, the thermal expansion coefficient, α, the kinematic viscosity, ν, and the thermal diffusivity, κ. The hard turbulence regime in RBC is established for Ra ≥ 106.
    [Show full text]
  • Constant-Wall-Temperature Nusselt Number in Micro and Nano-Channels1
    Constant-Wall-Temperature Nusselt Number in Micro and Nano-Channels1 We investigate the constant-wall-temperature convective heat-transfer characteristics of a model gaseous flow in two-dimensional micro and nano-channels under hydrodynamically Nicolas G. and thermally fully developed conditions. Our investigation covers both the slip-flow Hadjiconstantinou regime 0рKnр0.1, and most of the transition regime 0.1ϽKnр10, where Kn, the Knud- sen number, is defined as the ratio between the molecular mean free path and the channel Olga Simek height. We use slip-flow theory in the presence of axial heat conduction to calculate the Nusselt number in the range 0рKnр0.2, and a stochastic molecular simulation technique Mechanical Engineering Department, known as the direct simulation Monte Carlo (DSMC) to calculate the Nusselt number in Massachusetts Institute of Technology, the range 0.02ϽKnϽ2. Inclusion of the effects of axial heat conduction in the continuum Cambridge, MA 02139 model is necessary since small-scale internal flows are typically characterized by finite Peclet numbers. Our results show that the slip-flow prediction is in good agreement with the DSMC results for Knр0.1, but also remains a good approximation beyond its ex- pected range of applicability. We also show that the Nusselt number decreases monotoni- cally with increasing Knudsen number in the fully accommodating case, both in the slip-flow and transition regimes. In the slip-flow regime, axial heat conduction is found to increase the Nusselt number; this effect is largest at Knϭ0 and is of the order of 10 percent. Qualitatively similar results are obtained for slip-flow heat transfer in circular tubes.
    [Show full text]
  • Fluid Dynamics Analysis and Numerical Study of a Fluid Running Down a Flat Surface
    29TH DAAAM INTERNATIONAL SYMPOSIUM ON INTELLIGENT MANUFACTURING AND AUTOMATION DOI: 10.2507/29th.daaam.proceedings.116 FLUID DYNAMICS ANALYSIS AND NUMERICAL STUDY OF A FLUID RUNNING DOWN A FLAT SURFACE Juan Carlos Beltrán-Prieto & Karel Kolomazník This Publication has to be referred as: Beltran-Prieto, J[uan] C[arlos] & Kolomaznik, K[arel] (2018). Fluid Dynamics Analysis and Numerical Study of a Fluid Running Down a Flat Surface, Proceedings of the 29th DAAAM International Symposium, pp.0801-0810, B. Katalinic (Ed.), Published by DAAAM International, ISBN 978-3-902734- 20-4, ISSN 1726-9679, Vienna, Austria DOI: 10.2507/29th.daaam.proceedings.116 Abstract The case of fluid flowing down a plate is applied in several industrial, chemical and engineering systems and equipments. The mathematical modeling and simulation of this type of system is important from the process engineering point of view because an adequate understanding is required to control important parameters like falling film thickness, mass rate flow, velocity distribution and even suitable fluid selection. In this paper we address the numerical simulation and mathematical modeling of this process. We derived equations that allow us to understand the correlation between different physical chemical properties of the fluid and the system namely fluid mass flow, dynamic viscosity, thermal conductivity and specific heat and studied their influence on thermal diffusivity, kinematic viscosity, Prandtl number, flow velocity, fluid thickness, Reynolds number, Nusselt number, and heat transfer coefficient using numerical simulation. The results of this research can be applied in computational fluid dynamics to easily identify the expected behavior of a fluid that is flowing down a flat plate to determine the velocity distribution and values range of specific dimensionless parameters and to help in the decision-making process of pumping systems design, fluid selection, drainage of liquids, transport of fluids, condensation and in gas absorption experiments.
    [Show full text]