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LICENTIATE THESIS Luleå University of Technology Department of Applied Physics and Mechanical Engineering Division of Fluid Mechanics 2007:06|:02-757|: -c -- 07⁄06 -- 2007:06 Parallel Computing of Fluid Flow Through Porous Media J. Gunnar I. Hellström

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LICENTIATE T H E S I S

Luleå University of TechnologyDepartment of Applied Physics and Mechanical Engineering

Division of Fluid Mechanics

2007:06|: 02-757|: -c -- 07⁄06 --

2007:06

Parallel Computing of Fluid Flow Through Porous Media

J. Gunnar I. Hellström

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Parallel Computing of Fluid Flow

Through Porous Media

by

J. Gunnar I. Hellström

Division of Fluid Mechanics Department of Applied Physics and Mechanical Engineering

Luleå University of Technology SE-971 87 Luleå

Sweden

Luleå, February 2007

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Preface

This work has been carried out at the Division of Fluid Mechanics, Department of Applied Physics and Mechanical Engineering, Luleå University of Technology, Sweden during the years 2005-2007.

The research presented here was carried out as a part of "Swedish Hydropower Centre - SVC". SVC has been established by the Swedish Energy Agency, Elforsk and Svenska Kraftnät together with Luleå University of Technology, The Royal Institute of Technology, Chalmers University of Technology and Uppsala University.

Alstom Hydro Sweden, CarlBro, E.ON Vattenkraft Sverige, Fortum Generation, GE Energy (Sweden), Jämtkraft, Jönköping Energi, Mälarenergi, Skellefteå Kraft, Sollefteåforsens, Statoil Lubricants, Sweco VBB, Sweco Energuide, SweMin, Tekniska Verken i Linköping, Vattenfall Research and Development and Vattenfall Vattenkraft, Waplans, VG Power and Öresundskraft are also participating in SVC.

Regarding paper A the authors gratefully acknowledge the support provided by Vattenfall Utveckling AB, the Swedish Agency for Innovation Systems (VINNOVA) and the participating industries in the Polhem Laboratory.

First of all I would like to thank my supervisor Prof. Staffan Lundström for his guidance and support in this work and also my assistant supervisor Dr. Hans Mattsson for his valuable comments.

Secondly, I would like to express my deepest appreciation to the colleagues at the Division, both former and present, for the many fruitful discussions and the pleasant and creative working environment. Especially thanks to Elianne Wassvik, my office companion, for the many giving discussions and help in keeping the office organized.

Finally I would like to thank all my friends and my family for always supporting me during this work.

Gunnar Hellström, Luleå, February 2007.

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Summary of contents

Fluid flow through porous media takes place in a variety of technical areas including ground water flow, flow through embankment dams, paper making, composites manufacturing, filtering, drying and sintering of iron ore pellets. When modelling these kinds of flows it is common practice to use averaging techniques rather than computing the detailed flow field in every single pore. This approach is very efficient when averaged quantities are sough for but it is not very convenient for local problems such as forces on particles within an embankment dam and drying of individual iron ore pellets. In this thesis the focus is set on the former and how such forces alter as a function of Reynolds number. Of particular interest are the effects of inertia and turbulence and when they need to be considered. For problem like this a Computational Fluid Dynamics (CFD) approach is well suited since rather complex geometries and flow conditions can be studied by using parallel computing techniques. By using this technique it is also possible to determine at which flow regimes Darcy law is applicable and thus when more elaborate descriptions of the flow like the Forchheimer equation and the Navier-Stokes equations need to be applied. In order to isolate the question above and be able to use advanced models for turbulence a neat geometry is applied being an array of quadratic packed cylinders. To start with the parallel computing capacity of the in-house cluster is scrutinized showing very promising results with up to almost full scalability. Following this study focus is set on the porous media and when inertia-effects need to be taken into account. The significance of this phenomenon turns out to be when Reynolds number is above 10. Then a study in when the flow has to be solved with a full turbulent description has been carried out with the results that as the Reynolds number increases above 100 the significance is clear. In addition a manuscript for a state of the art literature survey is appended.

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Appended papers

Paper A: Hellström, J. G. I., Marjavaara, B. D., Lundström, T. S., (2006), ”Parallel CFD simulations of an original and redesigned hydraulic draft tube”, Advances in Engineering Software, doi: 10.1016/j.advengsoft.2006.08.013.

Paper B: Hellström, J. G. I., Lundström, T. S., (2006), ”Flow through Porous Media at Moderate Reynolds Number”, Proceedings of the 4th

International Scientific Colloquium Modelling for Material Processing, Riga, June 8-9, pp. 129-134.

Paper C: Hellström, J. G. I., Jonsson, P. J. P., Lundström, T. S., (2007), ”Numerical Study of Turbulent Flow Through Porous Media”, to be submitted.

Additional appended paper of relevance

Report A: Hellström, J. G. I., Lundström, T. S., Mattsson, H., (2007), ”Fluid Mechanics of Internal Erosion of Embankment Dams”, manuscript.

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Paper abstracts

Paper A: The design of hydraulic turbine draft tubes has traditionally been based on simplified analytic methods, model and full-scale experiments. In the latest decades, however, the usage of numerical methods such as CFD has increased in the design process due to the rapid escalation in computer performance. Today with parallel computer architectures new aspects of the flow can be considered, but still several problems have to be solved before CFD can routinely be applied in product development. The present paper aims to investigate the parallel performance of a commercial CFD software on a homogeneous networks of computers, being very common solution strategies encountered in the industry today. In addition, the efficiency improvements obtained in earlier experiments by modifying the shape of the draft tube will be considered to deduce if the improvements can be captured with aid of CFD. Result from both the steady and unsteady CFD simulations shows that almost full scalability is obtained with the commercial CFD software CFX-5.7.1. Furthermore, no remarkable improvement in the pressure recovery factor or the flow field is noticed in the CFD simulations as compared to experiments. The discrepancy may be to the applied inlet boundary conditions and/or turbulence model.

Paper B: In modelling of flow through porous media inertia-effects must sometimes be considered. This is often done by usage of the empirically derived Ergun equation that can describe the response of several porous media but does not reveal the real mechanisms for the flow. In order to increase the understanding of such flows we have therefore performed a micromechanically based study of moderate Re’ flow between parallel cylinders using a Computational Fluid Dynamics approach. The simulations are carried out with quality and trust by using grid refinement techniques and securing that the iteration error is sufficiently small. Main results are that the Ergun equation fits well to simulated data up to Re’ 20, that inertia-effects must be taken into account when Re’ exceeds 10 and that results from stationary simulations replicate time resolved ones at least up to Re’ 880.

Paper C: When modelling flow through porous media it is necessary to know when to take inertia-effects into account as well as when to switch to

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a turbulent description of the flow. This is important in a large number of industrial processes such as flow through embankment dams, filtering, composites manufacturing, paper-making and in the refinement of iron ore. From an engineering point of view the problem is often solved with the empirically derived Ergun equation. The drawback with this approach is, however, that the mechanisms for the transitions between the three states of flow are not revealed and time-consuming experiments have to be performed. In order to increase the knowledge of the detailed flow a micromechanical analysis is here carried out by means of numerical studies of flow through arrays of quadratically packed cylinders at a variety of Reynolds number. Main results are that turbulent effects must be taken into account when Reynolds number is larger than 100 while inertia-effects must be considered when the Reynolds number is above 10.

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Division of work

The division of the work between the authors for the three papers is presented below.

Paper A

“Parallel CFD simulations of an original and redesigned hydraulic draft tube”J. G. I. Hellström, B. D. Marjavaara and T. S. Lundström

All the simulations and analysis was performed by Hellström under the supervision by Marjavaara. The paper was written by Hellström, Marjavaara and Lundström.

Paper B

“Flow through Porous Media at Moderate Reynolds Number” J. G. I. Hellström and T. S. Lundström

The simulations and analysis was performed by Hellström. The paper was written by Hellström and Lundström.

Paper C

“Numerical Study of Turbulent Flow Through Porous Media” J. G. I. Hellström, P. J. P. Jonsson and T. S. Lundström

The simulations and analysis was performed by Hellström and Jonsson. The paper was written by Hellström, Jonsson and Lundström.

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Paper A

PARALLEL CFD SIMULATIONS OF AN ORIGINALAND REDESIGNED HYDRAULIC DRAFT TUBE

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Parallel CFD simulations of an original and redesignedhydraulic turbine draft tube

J.G.I. Hellstrom 1, B.D. Marjavaara *, T.S. Lundstrom 2

Division of Fluid Mechanics, Lulea University of Technology, SE-97187 Lulea, Sweden

Received 12 September 2005; accepted 3 August 2006

Abstract

The design of hydraulic turbine draft tubes has traditionally been based on simplified analytic methods, model and full-scale exper-iments. In the recent years the use of numerical methods such as computational fluid dynamics (CFD) has increased in the design process,due to the rapid escalation in computer performance. Today with parallel computer architectures, new aspects of flow can be considered.However, several problems have still to be solved before CFD can routinely be applied in product development. This paper aims to inves-tigate the parallel performance of commercial CFD software on homogeneous computer networks, as common solutions encountered inthe industry today. In addition, the efficiency improvements obtained in earlier experiments by modifying the shape of the draft tube willbe considered, to deduce if the improvements can be captured with aid of CFD. Results from both the steady and the unsteady CFDsimulations show that almost full scalability is obtained with the commercial CFD software CFX-5.7.1. Furthermore, no noticeableimprovement in the pressure recovery factor or the flow field is noticed in the CFD simulations as compared to experiments. The dis-crepancy may be to the applied inlet boundary conditions and/or the turbulence model.� 2006 Elsevier Ltd. All rights reserved.

Keywords: CFD; Parallel computing; Draft tube; Hydropower

1. Introduction

A hydropower plant converts the potential energy ofwater stored in a dam into electricity by the hydraulic tur-bine and the generator. In general, one of three types ofturbines is chosen depending on the head and dischargeof the hydropower plant: either a Pelton, a Francis or aKaplan turbine. A Pelton impulse turbine is suited for highheads and low discharges, while Francis and Kaplan reac-tion turbines are more appropriate for medium and lowheads, respectively, and high discharges. Turbines are gen-erally highly effective, transforming up to about 95% of the

available head into electric energy [1]. Even small efficiencyimprovements in the turbine are of interest for the industrydue to huge production volumes, especially in the runnerand draft tube since they are responsible for a large amountof the losses in medium and low headed turbines [2]. Thedesign of these two components has traditionally beenbased on simplified analytical methods, model tests andfull-scale tests. The use of numerical methods such as com-putational fluid dynamics (CFD) in the design process has,however, increased considerably due to the rapid develop-ment in computer technology, and it is an area that willdefinitely continue to evolve. So far, most of the workhas been focused on the runner, but with enhanced com-puter performance more attention is shifted towards thedraft tube and, in particular, to the reliability of CFD sim-ulations in this context [3–8]. This is due to the fact thatCFD predictions of the flow field in draft tubes are verychallenging and time consuming, caused by complex flowfeatures such as turbulence, unsteadiness, swirl, separation

0965-9978/$ - see front matter � 2006 Elsevier Ltd. All rights reserved.doi:10.1016/j.advengsoft.2006.08.013

* Corresponding author. Tel.: +46 920 492424; fax: +46 920 491047.E-mail addresses: [email protected] (J.G.I. Hellstrom), daniel.

[email protected] (B.D. Marjavaara), [email protected] (T.S.Lundstrom).1 Tel.: +46 920 491045; fax: +46 920 491047.2 Tel.: +46 920 492392; fax: +46 920 491047.

www.elsevier.com/locate/advengsoft

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and secondary flow. Nowadays, with parallel computerarchitectures, computer power is approaching sufficientand, consequently, CFD predictions of the main flow fea-tures are becoming quite accurate. However, models forturbulence still need to be tested and sensitivity to theapplied boundary conditions needs to be investigated fur-ther. Automatic shape optimisation of draft tubes withthe aid of CFD as well as computer optimisation have alsobeen performed recently, where the CPU requirements areeven more demanding due to the fact that several CFDsimulations have to be evaluated for different draft tubegeometries before an optimal design can be found [9,10].Results from these studies show, however, the potentialof using CFD and computer optimisations in the design/rehabilitation process of hydraulic turbine draft tubes.However, several problems also have to be solved here,before the technique can be routinely applied in productdevelopment. For example, the stability of the estimatedoptimum design is often unknown and it is not obvioushow to choose the best optimisation technique.

To solve these problems in an efficient and accurate waythere exists today an array of CFD software and a varietyof parallel computer architectures, using either shared ordistributed memory configuration with a homogeneous orheterogeneous network of computers. This paper aims toinvestigate the parallel performance of a common solutionstrategy (commercial CFD software + parallel computerarchitecture) often applied in the industry in order to solve3D complex flow in a hydraulic turbine draft tube. Thechosen CFD software, which is representative of modernnumerics, is CFX-5.7.1 from ANSYS [11], and the parallelcomputer architecture is a homogeneous Windows clusterwith dual Intel Xeon 2.4 GHz 32-bit processors, with2GB ram available on each node and with a 1 Gb/s com-munication bandwidth network. For decomposition ofthe grid the MeTiS partitioning method is selected, andfor communication between the nodes the MPICH mes-sage-passing libraries (MPI) are used [11].

From a turbine designer point of view, the surpris-ingly small efficiency improvements obtained in earlierCFD simulations by Marjavaara [10], compared toexperiments by Dahlback [12], will be investigated indetail here. In the latter case a total efficiency improve-ment of about 0.5% was obtained in the turbine, whilein the former case an improvement in the pressure recov-ery of about 0.02% was obtained in the draft tube. Theinconsistency can be traced to the assumptions madeabout the applied inlet boundary conditions, the turbu-lence model and/or the steady/unsteady flow behaviour[10]. In this paper the steady/unsteady hypothesis willbe evaluated by carrying out both steady and unsteadyCFD simulations.

The paper is organised as follows: Section 2 describesthe two draft tube geometries investigated. Section 3 pre-sents details of the CFD simulations, and in Sections 4and 5 the results and conclusions of the parallel perfor-mance and the CFD analysis are presented.

2. Geometrical description

The main purpose with a draft tube is to convertdynamic pressure into static pressure and thereby increasethe efficiency of the turbine. This is done by graduallyincreasing the cross-section area and consequently deceler-ating the fluid flow motion, see Fig. 1. A common measureof its performance is the pressure recovery factor Cp, beingdefined as:

Cp ¼1

Aout

RAout

pdA� 1Ain

RAin

pdA

12q Qin

Ain

� �2; ð1Þ

where A is the area, p is the static pressure, Q is the flowrate, q is the density and the subscripts ‘in’ and ‘out’ arecorrespond to the inlet and outlet, respectively. This mea-sure will be used here in order to compare the draft tubeperformance with the original and the redesigned drafttube geometry of Holleforsen Kaplan turbine, located inIndalsalven, Sweden. The original draft tube geometry iswell mapped out in two ERCOFTAC Turbine-99 Work-shops [4] by using a 1:11 scale model of the real turbineincluding the spiral case and the draft tube. The designof this draft tube is representative of designs in the1940s and is characterised by a sharp heel, see Fig. 1.In the redesigned draft tube geometry, suggested by Dahl-back [12], a removable curved insert has been placed inthe sharp heel corner in order to make it smoother, seeFig. 2.

3. CFD simulations

The 3D flow field in the two draft tube geometries aresolved with the commercial CFD code CFX-5.7.1, withrespectively incompressible, turbulent, steady and unsteadyflow assumption. The CFX-5.7.1 solver is based on thefinite volume method applied on an unstructured grid.The solver is coupled, meaning that the hydrodynamicequations are solved in a single step [11]. In this case theflow field is calculated based on the Reynolds-AveragedNavier Stokes (RANS) equations which are derived fromthe governing Navier–Stokes equations by decomposingthe total velocity ~u into a mean U and fluctuation compo-

Fig. 1. A CAD model of Holleforsen draft tube.

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nent u (i.e. ~u ¼ U þ u, where U � �~uÞ, resulting in the fol-lowing equations:

otU i þ UjojU i ¼ � 1

qoiP þ mr2Ui � ojujui; ð2Þ

oiU i ¼ 0: ð3Þ

where q is the fluid (water) density, P is the pressure, m isthe viscosity and uiuj are the Reynolds stresses. These equa-tions represent the mean flow characteristics where the tur-bulent effects are modelled via the Reynolds stresses. Toobtain closure, the Reynolds stresses are modelled withthe standard k–e turbulence model and with scalable wallfunctions [11]. Theoretically, a more ‘‘advanced’’ turbu-lence model would predict the flow field more accurately,but the standard k–e turbulence model is used here sinceit has been shown that this model is able to predict themain flow features quite accurately with reasonable usageof CPU, as compared to Reynolds stress models and LESmodels [4]. In the standard k–e turbulence model the Rey-nolds stresses are modelled with the constitutive equation,and thus the Reynolds stresses are linearly related to thestrain:

�ujui ¼ 2mT Sij � 2

3kdij; ð4Þ

where mT is the eddy viscosity and Sij is the mean straintensor:

Sij ¼ 1

2ðoiU j � ojU iÞ: ð5Þ

The eddy viscosity is modelled by predicting the velocityand length scales (u and l) of the eddy viscosity (mT � l * u)with the turbulent kinetic energy k and the turbulent dissi-pation rate e (u � k1/2 and l � k3/2/e), i.e.:

mT ¼ Clk2

e; ð6Þ

where Cl is a model constant. The turbulent kinetic energyand the dissipation rate in Eq. (6) are described by:

okot

þ Ujokoxj

¼ �ujuioUi

oxj� eþ o

oxjmþ mT

rk

� �okoxj

� �; ð7Þ

oeot

þ Ujoeoxj

¼ �Ce1ekujui

oUi

oxj� Ce2

e2

kþ ooxj

mþ mTre

� �oeoxj

� �

ð8Þwith the following standard values on the model constants:Cl = 0.09, Ce1 = 1.44, Ce2 = 1.92, rk = 1 and re = 1.3. Fora more elaborate derivation of these equations please read[13].

3.1. Numerical discretisation

The numerical discretisation in CFX-5.7.1 is node basedand it uses shape functions to evaluate the derivatives forthe pressure gradient term and the diffusion terms in themomentum, continuity and turbulent equations (Eqs. (2),(3), (7) and (8)). A second order accurate scheme was cho-sen for the discretisation of the advection term in themomentum and continuity equations (Specific Blend, witha blend factor of 1.0) while only a first order accuratescheme was used for the turbulent equations (First Orderupwind) due to boundness problem, which may reducethe accuracy. For the unsteady CFD simulations the sec-ond order Euler backward scheme was applied for theunsteady term. The total time for the unsteady CFD simu-lation was set to 40 s, to ensure that the CFD simulationswere well converged. The time-step was set to 0.1 s whichcorresponds to approximately one runner rotation. Moredetails about the numerical discretisation in the CFX-5.7.1 software can be found in [11].

3.2. Parallelisation

The parallelisation strategy in CFX-5.7.1 is based on theSingle Program Multiple Data (SPMD) model, which basi-cally runs identical versions of the software on several pro-cessors. It is designed so that all numerical intensive tasksare run in parallel while the administrative tasks (like

Fig. 2. Two draft tube geometries, the original geometry (left) and a sharp heel modification of it (right).

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input/output) are performed in a sequential manner by themaster process. The communication between the proces-sors is done with either Parallel Virtual Machine (PVM)or the MPICH message-passing libraries (MPI – messagepassing interface). In this case only the MPICH implemen-tation is tested since it was considerably faster than thePVM implementation. For example, it reduced the execu-tion time per outer solver iteration with about 1.4%, andthe preparation and finalisation of the solver solution bymore than 100%. A disadvantage of the MPICH as com-pared to the PVM implementation is, however, that it isnot completely interoperable between all supportedplatforms.

The decomposition of the grid into a number of parti-tions, which then are distributed and solved on separateprocessor in CFX-5.7.1, can be of either equal or unequalsize depending on whether the computer network is homo-geneous or heterogeneous. This decomposition is nodebased since it is consistent with the node base coupled sol-ver. Three main base partitioners are available in the codeand the MeTiS partitioning method is the recommendedone due to its fast and efficient algorithm. The other twobase partitioners are the Recursive Co-ordinate Bisectionand the Optimised Co-ordinate Bisection, which may bepreferable in some cases where the memory requirementis restricted. In addition, four additional partitioners exists(User Defined Direction, Radial, Circumferential andJunction Box) where the user can specify the direction ofthe decomposition. In this work, however, only the MeTiSalgorithm was tested since all of the other partitioners con-tained, in general, larger overlap regions. The MeTiS algo-rithm uses the advanced Multilevel Graph PartitioningMethod, as follows. A graph is first build up containingthe topology information of the mesh to be partitioned.Then the graph is coarsened down and a bisection of eachcoarsened graph is calculated. Finally the resulting parti-tions are projected back to the original graph, by conse-quently refining the partitions. For more details of theparallelisation in the CFX-5.7.1 software please see [11].

3.3. Numerical setup

At the inlet of the two draft tube geometries exactly thesame steady boundary conditions (velocity components,radial velocity assumption, dissipation length scale, etc.)used in the second ERCOFTAC Turbine-99 Workshopwere applied [4]. At the outlet of the fluid domain a zeroaverage static pressure condition was employed and thewalls were considered rough, with a roughness of

1e�5 m. The roughness effects are accounted in CFX-5.7.1 by modifying the logarithmic profile of the wall func-tions, such that it moves closer to the wall [11].

The unstructured computational grids (containing bothtetrahedral and prism elements) were generated by thecommercial grid generator ICEM CFD 5.0 [14]. To mini-mise the variation in numerical errors as a function of gridtopology, the same mesh parameters were applied to bothdraft tube geometries. To ensure that the grid topology alsohad as good quality as possible (near wall resolution,angles, aspect ratios, etc.) the grid resolution is non-uni-form, with higher density of grid points near the wallsand near the inlet boundary. Grids of different sizes weretested in order to determine the grid that provided the bestbalance in terms of solution convergence and solution runtime. The selected grids consisted of 1470k and 1445knodes (respectively, original and redesigned geometry)and had a minimum angle of about 11�, a max. edge lengthratio of about 280 and a max. element volume ratio ofabout 30.

Note that in order to improve the convergence rate andminimise the risk of solver failing, an initial guess was usedfor both the steady and unsteady CFD simulations. An ini-tial guess for the steady calculations was generated by usinga first order accurate scheme (First Order upwind) for allequations, and an outlet that allows both in and out flowfrom the fluid domain. The initial guess for the unsteadycalculations was simply the steadiest, one. In addition theoutlet of the draft tube geometry was extended down-stream, to prevent it crossing a possible recirculation atthe actual outlet.

4. Result

4.1. Parallel performance

The evaluation of parallel performance in the CFX-5.7.1software was performed on a homogeneous Windows clus-ter with dual Intel Xeon 2.4 GHz 32-bit processors, with2 GB ram available on each node and with the 1 Gb/s com-munication bandwidth network mentioned earlier. Onlythe original draft tube geometry was considered in the eval-uation since it is expected that both geometries will giveabout the same speedup. The parallel efficiency obtainedin this case was almost ideal, as shown in Table 1 wherethe efficiency (for the initial, steady and unsteady CFD sim-ulations) is presented for 6–12 processors. It is, however,noticed (in Table 1) that the execution time for the steadycalculations with six processors differs from the rest of the

Table 1The efficiency (and total execution time) related to the six processor configuration

# Proc./6 Initial Steady Unsteady

1 100 (5.18 · 104 s) 100 (6.55 · 104 s) 100 (3.80 · 105 s)1.33 94.75 (4.10 · 104 s) 161.07 (3.05 · 104 s) 96.61 (2.95 · 105 s)1.67 98.04 (3.17 · 104 s) 173.85 (2.26 · 104 s) 101.33 (2.25 · 105 s)2 95.57 (2.71 · 104 s) 167.09 (1.96 · 104 s) 97.93 (1.94 · 105 s)

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CFD simulations, indicating that there was a problem withthe processor availability, memory availability or commu-nication bandwidth during this simulation [15]. Note thatsix processors was the minimum number of CPUs neces-sary to avoid memory swapping in the CFD simulations,and that the same mesh partition was used for the initial,steady and unsteady calculations. The total execution timefor the unsteady CFD simulation with 12 processors wasabout 2 days and 6 h, where the communication time wasabout 4% of the total time and increased slightly with thenumber of processors.

4.2. Flow analysis

Results from both the steady and unsteady CFD simu-lations show on small efficiency improvements (pressurerecovery) compared to the experiments performed byDahlback [12], but they are in accordance with the CFDsimulations performed by Marjavaara [10]. For example,an enhancement in the pressure recovery factor for the

redesigned draft tube geometry, compared to the originaldraft tube geometry, of about 0.006% for both the steadyand unsteady CFD simulations, see Table 2. This shouldbe weighed against a total efficiency improvement in theexperiments of about 0.5%. It is also noticed that thereare small differences between the steady and unsteadyCFD simulations, about 0.001%, see Table 2.

Likewise, the velocity and pressure fields are nearly iden-tical in the CFD simulations but in conflict with the exper-imental result by Dahlback [12], see Figs. 3 and 4. Theonly difference in the flow field is obtained in the sharp heelcorner where the separated region disappears in the rede-signed geometry, as expected. However, there were no effi-ciency improvements, see Fig. 5. The CFD simulationsperformed here also show positive agreement with the sim-ulations carried out in the two ERCOFTAC workshops onthe original geometry. Regions with separated flow, sec-ondary flow after the sharp heel corner with two main vor-tices, and a vortex rope moving from one side of the drafttube to the other is captured, compare [4].

The average y+ values at near wall nodes for the twoCFD simulations were about 250, which may reduce theaccuracy of the calculations since they are higher thanthe recommended value of 100 [11]. However most of thesevalues can be traced to the extension of the draft tube,where their effects should not be critical. Removing theextension the average y+ is also getting closer to 100, which

Table 2The pressure recovery factor for the original and redesigned geometry

Geometry Steady Unsteady

Original 0.95878 0.95880Redesigned 0.95314 0.95319

Fig. 3. Streamlines from the runner and velocity contour plots for the original geometry (left) and redesigned geometry (right).

Fig. 4. Pressure distribution at a mid plane for the original geometry (left) and redesigned geometry (right).

J.G.I. Hellstrom et al. / Advances in Engineering Software xxx (2006) xxx–xxx 5

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are more satisfactory but not optimal. Each CFD simula-tion was assumed converged when all root mean square(RMS) residuals had drop to about 10�8, which is sufficientfor most industrial engineering applications [11].

5. Conclusion

The present paper illustrates the need of parallel com-puting architectures when performing draft tube CFD sim-ulations due to lack of RAM memory and to reduce theoverall computational time. This High Performance Com-puting requirement is even more essential when the gridbecomes finer, when more advanced turbulence modelsare used and when performing shape optimisations. Usingthe commercial CFD software CFX-5.7.1, almost idealspeedup can be obtained for draft tube flow simulations,which reduces the execution time satisfactorily. If MPICHcommunication is also available on the specific platformsused, the execution time can be reduced even further.

The result of the calculated flow field in both draft tubegeometries (original and redesigned) agrees well with CFDsimulations previously performed by Marjavaara (originaland redesigned) [10] and by participants in the twoERCOFTAC Workshops (only original) [4]. Conversely,there were no improvements in the pressure recoverybetween the original and redesigned draft tube geometryfor both the steady and unsteady CFD simulations com-pared, to the experiment by Dahlback [12]. An exampleof this would be the inlet velocity profile used for the drafttube geometry modifications, which remains fixed duringthe CFD simulations. This implies that including the run-ner in the calculations may give better agreement. A finergrid (especially the near wall resolution) and a moreadvanced turbulence model would certainly also predictthe flow field more accurately. Note that the unsteadinessof the unsteady CFD simulation can be discussed in thiscase, since it is based on the RANS equation, a standardk–e turbulence model and fixed steady inlet boundary con-ditions. All of these suggestions imply more expensive cal-

culations, some of them which can only be realised byintensifying the parallel computation with the methodstudied here.

Acknowledgments

The authors gratefully acknowledge the support pro-vided by Vattenfall Utveckling AB, the Swedish Agencyfor Innovation Systems (VINNOVA) and the participatingindustries in the Polhem Laboratory that made this workpossible.

References

[1] ASME. The guide to hydropower mechanical design. Kansas City:HCI Publications; 1996.

[2] Eberle P, Couston M, Sabourin M. Refurbishment of low headFrancis turbines. In: Avellan F, Ciocan G, Kvicinsky S, editors.Proceedings of the XXIst IAHR symposium on hydraulic machineryand systems. Lausanne: IAHR; 2002.

[3] Avellan F. Flow investigation in a Francis draft tube: the FLINDTProject. In: Proceedings of 20th IAHR symposium on hydraulicmachinery and system, Charlotte, NC, US; 2000.

[4] Turbine-99. The IAHR workshops on draft tube flow. URL: http://www.turbine-99.org/, cited May 2005.

[5] Mauri S. Numerical simulation and flow analysis of an elbow diffuser.Doctoral thesis, Ecole Politechnique Federale de Lausanne, Lau-sanne, Switzerland; 2002.

[6] Nilsson H. Numerical investigation of turbulent flow in waterturbines. Doctoral thesis, Chalmers University of Technology,Gothenbourg, Sweden; 2002.

[7] Engstrom TF. Simulations and experiments of turbulent diffuser flowwith hydropower applications. Doctoral thesis, Lulea University ofTechnology, Lulea, Sweden, vol. 10; 2003.

[8] Cervantes MJ. Effects of boundary conditions and unsteadiness ondraft tube flow. Doctoral thesis, Lulea University of Technology,Lulea, Sweden, vol. 11; 2003.

[9] Eisinger R, Ruprecht A. Automatic shape optimization of hydroturbine components based on CFD. TASK Quart 2001;6(1):101–11.

[10] Marjavaara BD. Parameterisation and flow design optimisation ofhydraulic turbine draft tubes. Licentiate thesis, Lulea University ofTechnology, Lulea, Sweden, vol. 32; 2004.

[11] CFX�, Version 5.7.1, Copyright � 1996–2004, ANSYS Europe Ltd.

Fig. 5. Velocity vectors and contour plot at the sharp heel corner for the original geometry (left) and redesigned geometry (right).

6 J.G.I. Hellstrom et al. / Advances in Engineering Software xxx (2006) xxx–xxx

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[12] Dahlback N. Redesign of sharp heel draft tube – Results from tests inmodel and prototype. In: Cabrera E, Espert V, Martınes F, editors,Proceedings of XVIII IAHR symposium on hydraulic machinery andcavitation, vol. 2; 1996. p. 985–93.

[13] Durbin PA, Reif BA. Statistical theory and modelling for turbulentflows. (NY) USA: Wiley; 2000.

[14] ICEM CFD�, Version 5.1, Copyright � 2004. ANSYS, Inc.[15] Naik VK. Scalability issues for a class of CFD applications. In:

Proceedings of the scalable high performance computing conference-SHPCC-92, Williamsburg, VA, USA; 1992. p. 268–75.

J.G.I. Hellstrom et al. / Advances in Engineering Software xxx (2006) xxx–xxx 7

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Paper B

FLOW THROUGH POROUS MEDIA AT MODERATEREYNOLDS NUMBER

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129

International Scientific Colloquium Modelling for Material Processing

Riga, June 8-9, 2006

Flow through Porous Media at Moderate Reynolds Number

J. G. I. Hellström, T. S. Lundström

Abstract

In modelling of flow through porous media inertia-effects must sometimes be considered. This is often done by usage of the empirically derived Ergun equation that can describe the response of several porous media but does not reveal the real mechanisms for the flow. In order to increase the understanding of such flows we have therefore performed a micromechanically based study of moderate Re’ flow between parallel cylinders using a Computational Fluid Dynamics approach. The simulations are carried out with quality and trust by using grid refinement techniques and securing that the iteration error is sufficiently small. Main results are that the Ergun equation fits well to simulated data up to Re’ 20, that inertia-effects must be taken into account when Re’ exceeds 10 and that results from stationary simulations replicate time resolved ones at least up to Re’ 880.

Introduction

Fluid flow through porous media takes place in a number of technical areas including ground water flows, flow through embankment dams, paper making, composites manufacturing, filtering, drying and sintering of iron ore pellets. In several of these areas the flow can simply be described by Darcy’s law, which in its general and one-dimensional form may be written as

jij

i pK

u ,μ= and ,

A

Q

L

pK=

Δμ

(1a-b)

respectively. In these equations u is the superficial velocity, K the permeability, μ the viscosity of the fluid, p the pressure, Q the flow rate through an area A and Δp the pressure drop over an length L in the stream-wise direction. Darcy’s law is valid as long as Re is sufficiently low, the fluid can be treated as incompressible and Newtonian and the porous medium is fixed. When Re increases over a certain level, which may be the case for erosion in embankment dams and drying of iron ore pellets, the pressure drop becomes higher than what is predicted by (1a-b) and additional non-linear terms are introduced in the so called Forchheimer equation

m

A

Qb

A

Q

L

pK⎟⎠⎞

⎜⎝⎛+=

Δμ

(2)

where b is a property of the porous media and m is a measure of the influence of fluid inertia. The equation was later modified by Ergun by fittings to experimental data according to

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130

( ) ( )pp

D

A

Q

DA

Q

gL

p

2

323

2 175.1

1150

⎟⎠⎞

⎜⎝⎛

−+

−=

Δρ

εεμ

εε

(3)

where ε is the fractional void volume in the bed and Dp is the effective diameter of particles [1]. From (3) a modified Reynolds (Re’) number can be defined

εμ

ρ

−=

1

1Re' A

QDp

. (4)

The Ergun equation does not have a micromechanical basis and the geometrical parameters shaping the form of the equation are therefore unknown. Previous works also indicate that the parameters of the Ergun equation may be improved [2, 3]. To increase the knowledge about higher Re flow through porous media we will here study the detailed flow through an array of quadratic packed parallel cylinders with Computational Fluid Dynamics (CFD). The CFD simulations are performed with the commercial software ANSYS CFX 10.0 with quality and trust regarding grid refinement and iterative errors. To achieve this within reasonable computational time the CFD simulations are run with a parallel computing procedure and by this retaining the iterative error low within reasonable computing time. Another effect that is studied is whether unsteady effects take place at higher Re and if this effect is of importance for the apparent permeability.

1. Numerical setup

In order to simplify the simulations unit-cells are defined for steady and unsteady flow, see Fig. 1. For both unit-cells, the discretization is performed with ANSYS ICEM CFD 10.0 Hexa where the block-structure is defined and projected onto the geometry to achieve as correct and smooth description of the unit-cell as possible. For the grid refinement study the grid is refined uniformly in the in-plane directions while the number of nodes in the out-of-plane direction is two for all cases. For the unsteady simulations the geometry is mirrored so the whole cylinder is encapsulated in the unit-cell. Consequently the domain is doubled and so is the number of nodes required for a certain mesh density. In order to drive the flow perpendicular to the cylinders a pressure gradient is introduced into the momentum equations by in a sub-domain specifying a general momentum source [4].

Regarding the boundary conditions for the simulations the top and the bottom of the unit-cells are defined as symmetry-planes, the cylinder wall is assumed to be smooth with a no-slip condition and the left- and right-hand sides of the

R

ΔL

L/2

R

L

Fig. 1. The 2 unit-cells used in the simulations, the left for the steady calculations and the right one for the unsteady.

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131

unit-cells are periodic domain interfaces representing the structure of the array. The advection scheme used to solve the continuity and momentum equations are strictly 2nd order accurate, which is realised by setting the specified blend factor equal to 1 in CFX-Pre. The simulations are considered well converged when the Root Mean Square (RMS) -residuals has dropped 5-6 decades and the max-residuals is no more than 1.5 decade above the RMS-residuals.

For the simulations with Re less than 150 the flow-field is solved by assuming the flow to be steady. At higher Re both steady and unsteady simulations are carried out following the results in the literature [5, 6]. The convergence criteria are the same as for the steady simulations and the mass-flow quantity is stabilized to a constant value.

2. Results

This part is divided into 3 sections dealing with grid refinement, effect on apparent permeability from solid fraction and Re’ and the unsteady calculations evaluated in order to check whether or not it is required to use an unsteady approach in order to get the correct apparent permeability.

2.1. Grid refinement study The grid refinement study is performed with a solid fraction of 60% and a Re’ of approximately 12 for 10 mesh densities, see Tab 1. The parameter of interest is the apparent permeability which is derived by usage of (1) where Q is calculated as the mass-flow obtained from CFX-Post divided with the density of the fluid. A polynomial fit to the results indicates that the simulations are in the asymptotic range since the curve approaches a specific value as the grid is refined, see Fig. 2. The simulated values are in all cases close to the asymptotic one with a difference of only 0.3 per mil for the mesh with 370 000 nodes. This accuracy is by all means god enough and since the computational time is short enough for this case all simulations, from now on, are performed with a mesh density in this range.

Tab.1. Meshes with the corresponding permeability.

2.2. Different solid fractions The simulations are performed with solid fractions of 40, 60 and 70% at a number of Re’ ranging from about 0.001 to around 1000. At the creeping flow regime (Re’ < 1) true permeability data are obtained see Fig. 3. As the flow-rate is increased the apparent permeability decreases for all solid fractions but predominantly for the highest one. To shed

Normalized number of nodes Number of nodes K

8.72 125 000 7.3839E-08

5.74 190 000 7.3825E-08

3.89 280 000 7.3815E-08

2.95 370 000 7.3810E-08

2.22 490 000 7.3807E-08

2.02 540 000 7.3805E-08

1.73 630 000 7.3803E-08

1.43 760 000 7.3801E-08

1.18 920 000 7.3800E-08

1 1 090 000 7.3798E-08 Fig. 2. Plot of the different meshes and the corresponding permeability

y = -1,504E-13x2 + 6,648E-12x + 7,379E-08

7,375E-08

7,378E-08

7,380E-08

7,383E-08

7,385E-08

0 2 4 6 8 10

Normalized number of nodes

K

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132

some light on this phenomenon the flow field is plotted for two solid fractions and three Re’Fig. 4 and 5. As seen the circulation zone and the corresponding stagnation points formed move towards the nip as Re’ is increased. The circulation zone then becomes small and the velocity near the wall high indicating large losses.

Fig. 4. Flow fields for a solid fraction of 70% at different Re’, 0.001, 80 and 700.

Fig. 3. The result from the simulations with different solid fractions, the apparent permeability is normalized with the true permeability and then plotted against Re’.

0

0,2

0,4

0,6

0,8

1

1,2

0,001 0,01 0,1 1 10 100 1000 10000

Re'

app

aren

t /

tru

e p

erm

eab

ilit

y

f=0.4

f=0.6

f=0.7

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133

When comparing the simulations at f = 60% with the Ergun equation it is obvious that the simulation exhibit fair agreement up to Re’ of about 20 Fig. 6. where the parameter evaluated are the Blake-type friction factors

εε

ρ −Δ

=1

'3

2 L

D

u

pf p and

Re'

15075.1' +=f . (5)

Above this value the slope of the Ergun curve decreases while the gradient of the simulated data stays more or less fixed. This phenomenon indicates that the empirical constants should be upgraded to suit the problem studied better.

0,1

1

10

100

1000

10000

100000

0,01 0,1 1 10 100 1000

Re'

f'

s imulated values

ergun equation

Fig. 6. Comparison between the simulated data for a solid fraction of 60% and the Ergun equation.

Fig. 5. Flow fields for a solid fraction of 40% at different Re’, 0.3, 150 and 1280.

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134

2.3. Unsteady simulations When comparing the steady and the unsteady simulations at Re’ equal to 880 it appears

that the final flow fields differs marginally but that the apparent permeabilities are in-principal the same. In addition the residuals for the steady calculations performed do not oscillate, indicating a steady behaviour of the flow. Unsteady calculations when Re’ is less than 880 are therefore not required, which considerably reduces the computational time needed to achieve reliable values of the simulated apparent permeability.

Conclusions

The results from the simulations are verified with a grid refinement study and are also in the same range as results from previous work indicating that the simulations are reliable and can be trusted. This is very important since there are by definition uncertainties with numerical simulations.

The simulations show that the limit of Re’ when inertia-effects must be taken into account when simulating flow through porous media is 10. The Ergun equation fit well to the simulations up to Re’ about 20, however the discrepancy thereafter shows that the need to update the constants in the Ergun equation is rather obvious. The simulations show that steady calculations can be used at least up to Re’ equal to 880.

References [1] Ergun, S.: Fluid flow through packed columns. Chemical Engineering Progress, Vol. 48, 1952, No. 2, pp.

89-94. [2] Nemec, D., Levec, J.: Flow through packed bed reactors: 1. Single-phase flow, Chemical Engineering

Science, Vol. 60, 2005, pp. 6947-6957. [3] Papathanasiou, T. D., Markicevic, B., Dendy, E. D.: A computational evaluation of the Ergun and

Forchheimer equations for fibrous media. Physics of Fluids, Vol. 13, 2001, No. 10, pp. 2795-2804. [4] Gebart, B. R.: Permeability of unidirectional reinforcements for RTM, Journal of Composite Materials, Vol.

26, 1992, No. 8, pp. 1100-1133. [5] Ghaddar, C. K.: On the permeability of unidirectional fibrous media: A parallel computational approach.

Phys. Fluids, Vol. 7 1995, No. 11, pp. 2563-2586. [6] Koch, D. L., Ladd, A. J. C.: Moderate Reynolds number flows through periodic and random arrays of

aligned cylinders. J. Fluid Mech., Vol. 349, 1997, pp. 31-66.

Authors Ph. D. student Hellström, J. Gunnar I. Prof. Lundström, T. Staffan Division of Fluid Mechanics Luleå University of Technology S - 971 87 Luleå, Sweden E-mail: [email protected]

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Paper C

NUMERICAL STUDY OF TURBULENT FLOWTHROUGH POROUS MEDIA

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Numerical Study of Turbulent Flow Through Porous Media

J. G. I. Hellström, P. J. P. Jonsson‡ & T. S. Lundström Division of Fluid Mechanics, Luleå University of Technology, SE-971 87 Luleå, Sweden. Corresponding author: [email protected]

Abstract

When modelling flow through porous media it is necessary to know when to take inertia-effects into account as well as when to switch to a turbulent description of the flow. This is important in a large number of industrial processes such as flow through embankment dams, filtering, composites manufacturing, paper-making and in the refinement of iron ore. From an engineering point of view the problem is often solved with the empirically derived Ergun equation. The drawback with this approach is, however, that the mechanisms for the transitions between the three states of flow are not revealed and time-consuming experiments have to be performed. In order to increase the knowledge of the detailed flow a micromechanical analysis is here carried out by means of numerical studies of flow through arrays of quadratically packed cylinders at a variety of Reynolds number. Main results are that turbulent effects must be taken into account when Reynolds number is larger than 100 while inertia-effects must be considered when the Reynolds number is above 10.Keywords:

Introduction

Flow through porous media takes place in a number of technical areas of application including ground water flow, flow through embankment dams, paper-making, composites manufacturing, filtering, drying and sintering of iron ore pellets. The flow characteristics will however vary as a function of pore geometry and ambient conditions. At one end the fluid is creeping between the pores and Darcy law is fully valid according to:

‡ Currently at Epsilon High Tech AB, Sweden.

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jij

i pK

u , and .AQ

LpK (1 & 2)

where (1) represent the general form of Darcy’s law and (2) the one-dimensional one. In these equations u is the superficial velocity, K the permeability, the dynamic viscosity of the fluid, p the pressure, Q the flow rate through an area Aand p the pressure drop over an length L in the stream-wise direction. At the other end the flow in the pores is fully or partly turbulent and additional non-linear terms are introduced in the so called Forchheimer equation

m

AQb

AQ

LpK (3)

where b is the property of the porous media and m, in this case, is a measure of the influence of fluid turbulence, Forchheimer (1901). In between the creeping region and the turbulent, laminar inertia gives a substantial contribution to the resistance to flow and experiments have indicated that it is possible to use (3) for this case as well. Since (3) can be applied in a variety of flow situations it is in-place to scrutinize it further.

A modified version of (3) was presented by Ergun by fittings to experimental data according to the following expression

pp DAQ

DAQ

gLp

2

323

2 175.11150 (4)

where g is the gravitational constant, the fractional void volume in the bed, Dpthe effective diameter of particles and the density of the fluid, Ergun (1952). The Ergun equation has shown best agreement with a bed of randomly distributed spheres and is therefore not optimal in for all geometries. The equation has therefore recently been generalised by Nemec & Levec (2005) to yield the following expression

*

*

*

*2

ReRe1Ga

BGa

AgL

p (5)

where A and B are tabulated material dependent constants derived from experiments, revealing that the knowledge of the material in itself must be

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improved. The Reynolds number and the Galileo number are modified according to Niven (2002),

1*Re

UDp and 32

3332

1* pDg

Ga (6 & 7)

where Re* represent the true averaged velocity in the pores taking the pore volume fraction into account and including the tortuousity . The Galileo number in its turn gives us the ratio between gravitational and viscous forces but please also notice the strong dependency on particle diameter and pore volume fraction. Other important contributions for the experimental approach of flow through porous media, Rose (1945), Lesage et al (2004), Wakeland & Keolian, (2003) and Gebart, (1992). From an numerical approach the significant contributions earlier can be considered as the following references, Koch & Ladd (1997), Ghaddar (1995), Edwards et al (1990), Beetstra et al (2007), Papathanasiou et al (2001) and Andrade Jr. et al (1999).

When increasing Reynolds number over the on-set of turbulence the equations to solve become the Reynolds-Averaged Navier-Stokes (RANS) equations. These are derived from the governing Navier-Stokes equations by decomposing the total velocity u~ into a mean U and fluctuation component u(i.e. uUu~ , where uU ~ ), resulting in the following equations

ijjiiijjit uuUPUUU 21 and 0iiU . (8 & 9)

Here is the kinematic viscosity and jiuu are the Reynolds stresses. These equations represent the mean flow characteristics where turbulent effects are modelled via the Reynolds stresses, in order to obtain closure. When considering flow around a number of periodically arranged cylinders having curved surfaces, as will be done here, the Shear-Stress-Transport (SST), Menter (1993) can be an appropriate choice. In the SST-model the best elements from the k- and the k-model are combined via a blending factor. This factor activates the k- model in the near-wall region and the k- model in the bulk, yielding that the transition from the k- to the k- formulation takes place in the logarithmic part of the boundary layer. The model is based on the assumption that the principal shear-stress is proportional to the turbulent kinetic energy, which is introduced into the definition of the eddy-viscosity, the so-called Bradshaw’s assumption. The mathematical formulations thus develop into

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jTk

jj

iij x

kx

kxu

SDt

kD * (10)

jjjT

jj

iij

T xxkF

xxxuS

DtD 112 21

2

(11)

where k is the turbulent kinetic energy, Sij the mean strain tensor, the turbulent frequency, T the turbulent dynamic viscosity, T the turbulent kinematic viscosity and *

k F1 and 2 are constants. For a more elaborate description of the SST-model see Menter (1993).

It is now of interest to study the validity of the SST-model for a variety of Reynolds number for a typical porous medium. It is also relevant to compare the results of laminar set-ups with turbulent ditto. For the purpose of having trustful and high quality results the geometry should remain as simple as possible but still capture pertinent phenomena.

Geometry and numerical verification

The geometry chosen for this study is an array of quadratically packed infinite long cylinders and in order to reduce the number of volumes to solve the problem a unit-cell is defined, see figure 1. For the calculations the geometry of interest is divided into finite volumes with aid of ANSYS ICEM CFD 10.0 Hexa. The block structure generated is projected onto the geometry in order to get as correct and smooth description of the unit-cell as possible. The number of blocks used in this procedure are eight and for laminar flow it has previously been shown that the quality of the grid it is by all means good enough yielding an error less than 0.3‰ when using 370 000 nodes, see Hellström & Lundström (2006) for a detailed description. To solve the flow the commercial software ANSYS CFX 10.0 is used. The computational domain is parallelized with the MeTis partitioning method and simulated on homogenous Windows and LINUX clusters. For the Windows part of the simulations the MPICH-1.2.5 message-passing libraries (MPI) are used and for the LINUX part a HP-MPI-2.1 routine is chosen, see Hellström et al (2006). For the turbulent simulations measures are taken to keep the y-plus value low enough. To exemplify when Re’ is equal to 2 000 the maximum y-plus is 1.3 being lower than the value recommended in the CFX-manual, the y-plus value should be lower than 2, and also fulfils the y-plus

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requirements from ERCOFTAC Best practice Guidelines (2000), which is below 4 and close to unity.

R

LL/2

Figure 1: Schematic sketch of the computational domain.

The boundary conditions of the unit-cell are defined as follows, the top and the bottom part are symmetry-planes, the cylinder wall is assumed to be smooth with a no-slip condition and the left and right hand sides are periodic domain interfaces representing the repeatable structure of the array. In order to drive the flow a momentum source is defined in a subdomain. The advection scheme used to solve the continuity and momentum equations are strictly second order accurate which is realised by setting the specified blend factor equal to one in CFX. The simulations are furthermore assumed to be well converged when the Root Mean Square (RMS) residuals have dropped 5-6 orders of magnitude and when the maximum residuals are less than 1.5 orders of magnitude above the RMS-residuals.

For the unsteady calculations a second order backward Euler scheme is applied and the time step is selected so that the Courant number is between 0 and 5. To discern the unsteady behaviour of the simulations a number of monitor-points were introduced recording pressure at nine locations and also logging the massflow at the domain interfaces. The turbulent simulations were performed with the following turbulence models k- , Reynolds stress (SSG), SST and a transition model available in CFX. It turned out that the SST-model is the most suitable since it catches the free stream behaviour and since it has a potential to accurately model the flow close to the cylinder wall. In order to shorten the simulation time most simulations were initially based on former runs, in particular each turbulent simulation was based on its laminar counterpart. The turbulent intensity is set as medium (5%) being the default value in CFX, for the eddy frequency the value is set to 300 Hz, based on post-processing of earlier results although the recommendation through the Strouhal number based on the Karman vortex frequency is 15 Hz. The turbulent kinetic energy were chosen to 0.03 J/kg based on post-processing of earlier results, the length scale is a tenth of the diameter of the cylinder and the viscosity ratio is set to 10. To ensure that the

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values of the turbulent parameters are in the right region a perturbation analysis were carried out. These variations only weekly influence the results indicating that the solutions obtained are stable in this context.

At higher Reynolds number the simulations were performed with an unsteady approach since the steady simulations indicated that this was necessarily. Investigations for the turbulent case point out that there is not the same need when doing turbulent simulations. This is based on the monitor points for the solver part of the simulation and that the parameters studied show a stable nature for steady simulations.

Results and discussions

For the simulation carried out with the full Navier-Stokes Equations but without adding turbulent equations there is a drop in permeability at Re’ 10, see figure 2 where Reynolds number prime is defined with the following formula

11Re' A

QDp. (12)

As apparent for simulations with solid volume fraction 60 %, the permeability curve then makes a smooth bend and seems to level out. At the high end of this curve it is likely that turbulent effects need to be modelled. Before doing this let us study the flow field calculated for various set-ups.

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0,0

0,2

0,4

0,6

0,8

1,0

1,2

0,001 0,01 0,1 1 10 100 1000 10000

Re'

appa

rent

/ "t

rue"

per

mea

bilit

y

solid fraction 40%solid fraction 60%solid fraction 70%

Figure 2: The apparent permeability divided by the true permeability for the three solid fractions studied here, 40, 60 and 70%.

As Re’ is increased the stagnation point on the left hand side of the cylinder climbs “uphill” towards the top of the cylinder and the corresponding recirculation zone becomes smaller and seemingly more chaotic, see figure 3. Hence at very low Re’ the circulation generated can be neglected but as Re’ increases it becomes important and as shown in the former figure it gives a noticeable contribution to the resistance to flow. The fact that the circulation zone becomes smaller at even higher Re’ may explain the result that the apparent permeability levels out, cf. figure 2 and 3.

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Figure 3: Vectors representing the velocity for the laminar configuration with different Re’ for the solid fraction of 60%; top left Re’ = 0.02, top right Re’ = 200, bottom left Re’ = 1 000 and bottom right Re’ = 4 000.

Before deepening this discussion let us compare the simulated results with experiments. It is then convenient to form the Blake-type friction factor according to:

1'

3

2

AQ

DLpf p and

Re'15075.1'f (13 & 14)

where (13) is used for the values from the simulations and (14) is a neat form of the Ergun Equation. The correspondence between the simulated value and the Ergun-equation is good until Re’ 10 but as Re’ increases further the simulated results start to deviate from this equation, see figure 4.

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0,01

0,1

1

10

100

1000

10000

100000

1000000

0,001 0,01 0,1 1 10 100 1000 10000

Re'

Bla

ke-ty

pe fr

ictio

n fa

ctor

f = 40%, simulated valuesf = 60%, simulated valuesf = 70%, simulated valuesErgun equationModified Ergun equation

Figure 4: The Blake-type friction factor calculated for the simulations as well as the Ergun equation and the modification by Nemec & Levec for the different solid fractions.

In addition the agreement between the simulations and the modified Ergun-equation is very good up to Re’ 10, but when Re’ increases the curves diverge in the same way as before. Whether this is an effect of turbulence or not will now be discussed.

When comparing the turbulent simulations with the laminar equivalents it is shown that the apparent permeability is similar until a certain Re’. Increasing Re’ further implies that the turbulent simulations give lower apparent permeability values. This is expected and there is no sign of a harsh transition, as the one in pipe flow, in conformity with experimental work presented in Bear, (1972), see figure 5. The deviation is dependent on the solid fraction and for f = 60% it starts when Re’ > 300.

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0

0,2

0,4

0,6

0,8

1

1,2

0,001 0,01 0,1 1 10 100 1000 10000

Re'

appa

rent

/ "t

rue"

per

mea

bilit

y

f = 40%, laminarf = 40%, turbulentf = 60%, laminarf = 60%, turbulentf = 70%, laminarf = 70%, turbulent

Figure 5: The apparent permeability divided by the true permeability for the three solid fractions 40, 60 and 70%, both the values for the laminar and also the turbulent case.

By studying the averaged velocity field for the turbulent case it can be seen that the circulation zone has more or less the same position for all Re’ but increases in strength with Re’, see figure 6.

Figure 6: Vectors representing the velocity field for the turbulent configuration with different Re’ for the solid fraction of 60%; top left Re’ = 1.5, top right Re’ = 200, bottom left Re’ = 1 000 and bottom right Re’ 2 000.

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The most significant difference regarding the flow field occurs on the right hand side of the cylinder where now a clear separation takes place as the circulation zone increases in size. The point of separation climbs closer to the top of the cylinder and causes a more disordered flow scenario as Re’ increases, see figure 7.

igure 7: The length of the vectors represent the velocity and the velocity gradient,

top righ

hen comparing the simulated values with the Ergun and the modified Ergun equation the discrepancy for Re’ > 10 is now reduced although there still is some translation for the simulated values in both the horizontal and vertical direction.

Fdydu / , is displayed on the cylinder wall for different Re’-numbers: top left: Re’ = 1.5,

t: Re’ = 65, middle left: Re’ = 120, middle right: Re’ = 210, bottom left: Re’ = 1 000 and bottom right: Re’ = 2 000, when the velocity gradient turn black the gradient switches sign and separation occurs.

W

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0,01

0,1

1

10

100

1000

10000

100000

0,01 0,1 1 10 100 1000 10000

Re'

Bla

ke-ty

pe fr

ictio

n fa

ctor

f = 60%, laminar, simulated valuesf = 60%, turbulent, simulated valuesErgunmodified Ergun

Figure 8: The Blake-type friction factor for the Ergun and the modified Ergun equation as well as the simulated values, only for the solid fraction of 60%.

rence between the mulated values and the Ergun equations are larger, but the characteristic bend

To ensure that the trend presented in figure 8 is general, simulations were performed for the solid fraction 70% as well. The diffesifor the Blake-type friction factor is evident, see figure 9.

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1

10

100

1000

10000

100000

1000000

0,001 0,01 0,1 1 10 100 1000

Re'

Bla

ke-ty

pe fr

ictio

n fa

ctor

f = 70%, laminar, simulated valuesf = 70%, turbulent, simulated valuesf = 70%, Ergunf = 70%, modified Ergun

Figure 9: The Blake-type friction factor for the Ergun and the modified Ergun equation as well as the simulated values, for the solid fraction of 70%.

When instead plotting the force per unit area acting on the cylinder it is seen that it increases dramatically with Reynolds number but the onset is very much dependent on the solid fraction. It is also evident that a turbulent flow will generate larger forces on the cylinder than a laminar one, see figures 10 and 11. When comparing figures 10 and 11 it is also clear that the normal force stand for the larger part of the force acting on the cylinder.

0

0,2

0,4

0,6

0,8

1

1,2

1,4

1,6

1,8

0,001 0,01 0,1 1 10 100 1000 10000

Re'

forc

e / a

rea

f = 40%, laminarf = 40%, turbulentf = 60%, laminarf = 60%, turbulentf = 70%, laminarf = 70%, turbulent

Figure 10: The shear force acting on the cylinder for different solid fractions.

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0

10

20

30

40

50

60

70

80

0,001 0,01 0,1 1 10 100 1000 10000

Re'

forc

e / a

rea

f = 40%, laminarf = 40%, turbulentf = 60%, laminarf = 60%, turbulentf = 70%, laminarf = 70%, turbulent

Figure 11: The normal forces acting on the cylinder for different solid fractions.

Conclusions

The main result of this investigation is that the Shear Stress Turbulence model can predict the main flow features in a good way. Furthermore inertia-effects must be taken into account when Reynolds number is above 10 and the turbulent effects ought to be considered when Reynolds number is increased above 100. The normal force on a cylinder dominates over the shear forces and it is clear that it is dependent on the solid fraction as well as if the turbulence is modelled or not.

Acknowledgement

The research presented was carried out as a part of "Swedish Hydropower Centre - SVC". SVC has been established by the Swedish Energy Agency, Elforsk and Svenska Kraftnät together with Luleå University of Technology, The Royal Institute of Technology, Chalmers University of Technology and Uppsala University. www.svc.nu

References

Andrade Jr., J. S., Costa, U. M. S., Almeida, M. P., Stanley, H. E., “Inertial Effects on Fluid Flow through Disordered Porous Media”, Physical review letters, Vol. 82, 1999, No. 26, pp. 5249-5252.

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Bear, J., “Dynamics of Fluids in Porous Media”, Dover publications, 1972, ISBN 0-486-65675-6.

Beetstra, R., van der Hoef, M. A., Kuipers, J. A. M., “Drag Force of Intermediate Reynolds Number Flow Past Mono- and Bidisperse Arrays of Spheres”, AIChE Journal, Vol. 53, 2007, No. 2, pp. 489-501.

CFX® (Copyright© 1996-2005), Version 10.0, ANSYS Europe Ltd.

Edwards, D. A., Shapiro, M., Bar-Yoseph, P., Shapira, M., “The influence of Reynolds number upon the apparent permeability of spatially periodic arrays of cylinders”, Phys. Fluids A, Vol. 2, 1990, No. 1, pp. 45-55.

ERCOFTAC (European Research Community On Flow, Turbulence And Combustion), “Special Interest Group on Quality and Trust in Industrial CFD: Best Practice Guidelines”, Version 1.0, 2000, edited by Casey, M., Wintergerste, T.

Ergun, S., “Fluid flow through packed columns”, Chemical Engineering Progress, Vol. 48, 1952, No. 2, pp. 89-94.

Forchheimer, P., “Wasserbevegung durch Boden“, Z. Ver. Deutsch, Ing., 45, 1782-1788, 1901.

Gebart, B. R., “Permeability of unidirectional reinforcements for RTM”, Journal of Composite Materials, Vol. 26, 1992, No. 8, pp. 1100-1133.

Ghaddar, C. K., “On the permeability of unidirectional fibrous media: A parallel computational approach”, Phys. Fluids, Vol. 7, 1995, No. 11, pp. 2563-2586.

Hellström, J. G. I., Marjavaara, B. D., Lundström, T. S., “Parallel CFD simulations of an original and redesigned hydraulic drat tube”, Advances in Engineering Software, 2006, doi: 10.1016/j.advengsoft.2006.08.013.

Hellström, J. G. I., Lundström, T. S., “Flow through Porous Media at Moderate Reynolds Number”, Proceedings of the 4th International Scientific Colloquium Modelling for Material Processing, Riga 2006, pp. 129-134.

Koch, D. L., Ladd, A. J. C., “Moderate Reynolds number flows through periodic and random arrays of aligned cylinders”, J. Fluid Mech., Vol. 349, 1997, pp. 31-66.

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Lesage, F., Midoux, N., Latifi, M. A., “New local measurements of hydrodynamics in porous media”, Experiments in Fluids, Vol. 37, 2004, pp. 257-262.

Menter, F. R., “Zonal two equation k- turbulence models for aerodynamic flows”, AIAA Paper 93-2906, July 1993.

Nemec, D., Levec, J., “Flow through packed bed reactors: 1. Single-phase flow”, Chemical Engineering Science, Vol. 60, 2005, pp. 6947-6957.

Niven, R. K., “Physical insight into the Ergun and Wen & Yu equations for fluid flow in packed and fluidised beds”, Chemical Engineering Science, Vol. 57, 2002, pp. 527-534.

Papathanasiou, T. D., Markicevic, B., Dendy, D., “A computational evaluation of the Ergun and Forchheimer equations for fibrous media”, Physics of Fluids, Vol. 13, 2001, No. 10, pp. 2795-2804.

Rose, H. E., “An Investigation into the Laws of Flow of Fluids through Beds of Granular Materials”, Proceedings Institution of Mechanical Engineering, Vol. 153, 1945, pp. 141-148.

Wakeland, R. S., Keolian, R. M., “Measurements of Resistance of Individual Square-Mesh Screens to Oscillating Flow at Low and Intermediate Reynolds Numbers”, Journal of Fluids Engineering, Vol. 125, 2003, pp. 851-862.

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Report A

FLUID MECHANICS OF INTERNAL EROSION OF EMBANKMENT DAMS

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Fluid Mechanics of Internal Erosion in Embankment Dams

J. G. I. Hellström†, T. S. Lundström† & H. Mattsson‡

† Division of Fluid Mechanics, Luleå University of Technology, SE-971 87 Luleå, Sweden.‡ Division of Mining and Geotechnical Engineering, Luleå University of Technology, SE-971 87 Luleå, Sweden.

Introduction

We will here briefly outline the status of fluid mechanics of internal erosion in embankment dams. Of particular interest is models for fluid flow generated forces on particles located in porous beds. This condensed review will be divided into two parts where part one deals with homogenous materials for which averaged expressions such as Darcy’s law and Ergun Equation can be applied. This includes a general background to porous media flow, continuum models for flow through embankment dams and routes to numerically model the flow. In part two, models to derive forces on individual particles are discussed starting from dilute (single particle) systems and ending with very dense and periodic systems of particles. The review is then finalised with a discussion. Let us however start with a presentation of some scenarios for internal erosion in embankment dams and please notice that the review has no intention of being complete. It rather aims at given a flavour of the area hopefully inspiring the reader to search for more information from other sources some of which are presented in the list of references.

Internal erosion processes

Internal erosion in embankment dams is not a completely understood phenomenon. Dam failures, accidents and deterioration of dams caused by ageing do take place as a result of internal erosion. Even if dams generally should be considered as safe constructions, a large part of the present knowledge about problems associated with internal erosion is a result of studies of former dam

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incidents. This circumstance is almost inevitable since internal erosion processes are very complex and have effect inside the embankment or foundation making the erosion transparency limited until it has progressed enough to be visible or detected by measurements.

The soil fractions that are considered as most susceptible to erosion are relatively uniform coarse silt and fine sand. Cohesive soils as clays are more resistant to erosion as long as the chemical bonds are not destroyed, Srbulov (1988). It seems like some core materials of glacial origin can be particularly susceptible to internal erosion. Glacial till is of special interest since it is a common core material in Swedish dams. Erosion susceptibility of glacial till is described in e.g. Foster et al. (2000), Ravaska (1997) as well as Norstedt & Nilsson (1997).

According to Fell et al. (2005), four conditions must exist for internal erosion and piping to occur. These are:”1) there must be a seepage flow path and a source of water; 2) there must be erodible material within the flow path and this material must be carried by the seepage flow; 3) there must be an unprotected exit, from which the eroded material may escape and 4) for a pipe to form, the material being piped, or the material directly above, must be able to form and support “roof” for the pipe”. Hence for internal erosion to occur particles within the dam must be subjected to forces high enough to make them move. It is therefore in-place to determine the magnitude and direction of the hydrodynamic forces generated by the flow on different types of particles at a variety of conditions.

In a central core earth and rockfill dam there are mainly three processes, Fell et al. (2005), which can initiate piping: backward erosion, concentrated leak and suffusion. Backward erosion is initiated at the exit point of seepage and the erosion is gradually progressing backward forming a pipe. Concentrated leak initiates a crack or a soft zone emanating from the source of water to an exit point. Erosion gradually continues along the walls of the erosion hole causing the concentrated leak. Suffusion is the process where the fine particles of the soil wash out or erode through the voids formed by the coarser particles. This can be prevented if the soil has a well graded particle size distribution with sufficiently small voids.

Internal erosion and piping might occur in the embankment, in the foundation and from embankment into the foundation, see Fell et al. (2005). Failure statistics presented by Foster et al. (2000) show that piping through the embankment is the most common piping mode of failure of those mentioned above, while piping from embankment into the foundation is the least common. In Figure 1, backward erosion piping through the embankment is sketched.

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Figure 1. Backward erosion piping.

It is reasonable to assume, that under normal conditions processes of internal erosion and piping may be in progress in dams to a smaller extent without any accidents or failures as result. However, potential breach mechanisms (Fell et al., 2005) for extensive internal erosion and piping might be: ”gross enlargement of the pipe hole, unravelling of the toe, crest settlement or sinkhole on the crest leading to overtopping and instability of the downstream slope”.

A concentrated leak in the embankment (Fell et al., 2005) may be initiated by e.g. cracking due to differential settlements, hydraulic fracturing, and soft zones with high permeability as well as piping modes associated to the presence of conduits or walls. There are a lot of different scenarios in connection to the development of cracks because of differential settlements, see e.g. Fell et al. (2005) and Kim et al. (2004). Hydraulic fracturing, see e.g. Ng & Small (1999) and Sherard (1986), can occur in a core if the vertical effective stress is reduced enough to allow the water pressure to create a crack or a soft zone. This can for example happen if the core settles more than the material in adjacent zones and thereby “hangs up” on it, with a decrease in the vertical stress locally in the core as a result. Soft zones with high permeability in a dam can have several reasons, e.g. segregation of materials. Segregation is the process that causes separation of a graded soil material into finer and coarser zones. It might occur at placement of material by downslope discharge during dumping and spreading operations. The larger particles have a tendency to accumulate at the bottom of the slope. Milligan (2003) warns that the issue of segregation is a critical uncertainty that is generally poorly recognized and dealt with in dam engineering. Foster et al. (2000) points out that many piping failures and accidents through the embankment are associated with the presence of conduits. In Fell et al. (2005) three different modes of such piping are described: piping into the conduit, piping along and above the conduit as well as flow out of the conduit.

Some common observations during piping incidents in embankment dams are listed in Fell et al. (2005) as: excess pore pressures, whirlpool in reservoir, sand boils, cracking, settlements, sinkholes, muddy leakage and increase in leakage. Further, Fell et al. (2005) states that ”it is apparent that many accidents would have become failures if they had not been detected by monitoring and surveillance and some action taken”. According to Fell et al. (2005), the most

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important detection methods and items to monitor in dam surveillance are: ”inspection by trained observers, seepage flow, vertical and horizontal displacement by direct survey of surface points, pore pressures as well as reservoir water level and rainfall (as these link to the other factors)”.

In recent years, numerical methods have been used to an increasing degree for solving more complicated problems in geotechnical engineering. A wide range of problems have been analysed with e.g. the finite element method. By utilizing the finite element method, based on a continuum approach, stresses, strains, deformations and pore pressures in an embankment dam can be theoretically analysed and it might be possible to draw conclusions from that information about the initiation of internal erosion processes. An approach worth considering, when initiation is established, is to interpret internal erosion numerically as a type of localisation and describe the constitutive behaviour with micromechanical models in localised zones. The mathematical description of the strain localisation phenomenon is nowadays an intensive research area (see e.g. Adachi et al., 1997) and, hopefully, models for strain localisation could give valuable input to the formulation of internal erosion localisation. Such a numerical software could be useful for: increasing the knowledge about internal erosion processes, evaluating the risk for dam incidents caused by internal erosion, estimating the time for progression of internal erosion and piping, studying self-healing of leaks and ageing effects in dams, analysing the amount of instrumentation needed and the proper location for monitoring and surveillance, designing dams etc.

Continuum models

Flow through porous media is generally modelled by a continuum approach implying that the flow in the pores is averaged and that averaged quantities such as the permeability are introduced.

General background

The flow through porous materials is often described by Darcy’s law that gives a linear relationship between the flow rate and the pressure. The law was originally derived from experiment (Bear 1972; Scheidegger 1972; Dullien 1992) but Tucker and Dessenberger have shown that the law can be derived from the Navier-Stokes Equations (Tucker III 1994). The conditions are that inertia and long-range viscous effects are negligible of which the former is generally a too

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crude assumption for at least the final stages of internal erosion. Let us, however, for the moment stick to the stated assumptions and write Darcy’s law in its general form:

jij

i pK

v , , (1)

where v is the superficial velocity, K the permeability tensor the viscosity and pthe pressure. An obvious interpretation of (1) is that the permeability can vary as a function of direction. It is also important to notice that:

ii

vu , (2)

where ui is the average velocity in the pores and the porosity. In this rigorous form of Darcy’s law the permeability is solely dependent on the detail geometry of the porous material and has the unit m2.In the literature describing embankment dams it is also common to give the permeability the unit m/s, conductivity or velocity, Fell et al (2005). This implies that the viscosity and the gravitational constant are incorporated in the actual permeability value. The advantage of this approach is that a velocity-like

component is explicitly given. The draw-back is that the actual value is dependent on the conditions for the measurements.

Figure 2. Set-up by Darcy.

The permeability of a porous material is generally obtained from measurements although numerous models often based on the microgeometry of the porous media have been derived. The models are developed for special cases and measurements need to be carried out in order to calibrate the models (Gebart 1992). Many methods for the experimental assessment of the permeability tensor

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have been proposed since the experiments by Darcy, (Kershaw 1972; Adams 1988; Pikulik 1991; Parnas 1993; Parnas 1995; Young 1995; Gebart 1996; Lekakou 1996; Weitzenböck 1998; Lundström 1999; Lundström 2000). Most of these methods are based on either of two fundamentally different principles: (i) parallel flow, by which the liquid is made to flow in a controlled direction through the porous sample (the Darcy experiment, see Figure 2); and (ii) radial flow, by which the liquid is injected at a “point” and flows freely in all directions (usually in a plane). Either of these principles may be applied in a variety of ways, e.g. by driving the liquid by a constant flow rate or a constant pressure drop. The advantage of the radial flow techniques is that a full permeability tensor, including principal directions, can be obtained in a single experiment (Ahn 1995; Weitzenböck 1998). The disadvantage is that they are based on tracking a flow front, i.e., the flow must be unsaturated, with the risk of including various transient effects, such as capillary action and void formation at the wetting flow front. Parallel flow measurements, on the other hand, can be carried out under steady state conditions (Lundström 2000) and edge effects can be avoided (Lundström 2002). Hence there are by all means several ways to determine the overall permeability of a porous material.

As Re increases over 1-10 it is well-known that experimental data starts to deviate from Darcy’s law. The overall effect is that the pressure drop becomes higher than what is predicted by (1-2) due to inertia and turbulence and an additional term is introduced in the so called Forchheimer equation

m

AQb

AQ

LpK1 (3)

where b is a property of the porous media and m is a measure of the influence of fluid inertia. The equation was later modified by Ergun by fittings to experimental data according to

pp DAQ

DAQ

gLp

2

323

2 175.11150 (4)

where is the fractional void volume in the bed and Dp is the effective diameter of particles (Ergun 1952). The Ergun equation does not have any micromechanical basis and the geometrical parameters shaping the form of the equation are therefore unknown. Recent studies indicate that the parameters of the Ergun equation should be modified for certain geometries (Papathanasiou 2001;

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Nemec 2005) which was also confirmed by a study by Hellström and Lundström (2006).

Flow through embankment dams

The flow through embankment dams can be modelled in numerous ways as outlined in Bear (1972). It can, for instance, be convenient to apply Hodographic methods in which the boundaries of the fluid including the free surface within the dam are transformed to form simpler geometries. Although the flow in it-self can be treated with explicit expressions such as Darcy’s law non-homogeneous and anisotropic permeabilities and the naturally formed free surface often makes realistic modelling with analytical tools complex.

One possible way to model the flow through embankment dams is instead to solve for the momentum Equations for two phases and then add an advection Equation to deal with the motion of the surface formed between the phases, the air and the water, for instance. To deal with the sharp transition in viscosity and density a modified Heaviside-step function can be introduced, see (Sharif et al 2001). Adaptive FEM analysis of free surface flow is also applicable, (Chen Sheng-Hong, 1996). Another method is to combine spectral analysis with a Laplace transform in order to model the transport of material through for instance the riprap, (Wörman & Xu, 2001). A combination of the Finite Element Method with a stochastic approach and the FEM part is used to solve the mechanical behaviour of the earth structure while the stochastic method is used for the probabilistic part of the earth modelling. (Mellah et al, 2000). Numerical procedures based solely on the finite element method are also common. Such a technique can, for instance, be applied to for hydraulic fracturing in the core of earth and rock-fill dams. The finite element procedure makes then use of special joint elements that allow fluid flow and fracture to be modelled This technique allows the progress of pore pressure in the core of a dam to be simulated, (Ng & Small, 1999). The Finite Volume Method can be used to solve the flow through the porous material. With such approaches the main flow features are resolved in a better way (Yang & Hemström, 1999, Eriksson & Yang, 2005).

Micro mechanical models

Continuum formulations of flow through porous media often results in Equations consisting of a few unknown parameters such as the permeability. The physical

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background of such parameters can often be traced to the detailed flow in the pores and it is therefore in place to study the flow on this level, as well. To start with we can scrutinize models for single particles. The viscous drag force on a single sphere in an infinite fluid at Re < 1 is, for instance, described by Stokes law:

vRf 6 (5)

where R is the radius of the sphere and v the velocity of it. This expression was early extended by Oseen to be valid for Re up to about 10 according to Lamb (1932):

Re16316 vRf (6)

and later on by Happel and Brenner (1957) to be valid for the case of a sphere moving through a tube with diameter D to be:

DRvRf 1.216 (7)

It has also been derived for particles with other geometries than spherical. For slender rods the drag force per unit length along the rod is, Emersleben (1925):

f 4 v (8)

While the following expression has been derived for flow perpendicular to the rod, Lamb (1932):

f4

2v

ln(Re) (9)

The obvious conclusion is that the drag on a particle is linearly dependent on the averaged velocity as long as Re is less than unity. The importance of velocity then increases to 2nd order.

For very dense systems and at low Re the flow follows Darcy’s law and the porous media can be characterised by their permeability through measurements or by the usage of permeability models based on, for instance, the detailed rod geometry: cf. (Speilman 1968; Bear 1972; Scheidegger 1972; Sangani 1982; Jackson 1986; Dullien 1992; Wang 1994; Higdon 1996). Generally permeability

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models may be divided into the following models, Phenomenological, Conduit flow (Kozeny-Carman for instance), Empirical, Network, Deterministic (directly from Navier-Stokes) and models based on flow around submerged objects (models proposed by Brenner and Brinkman, for instance) (Dullien 1992).

The permeability is often represented by the Kozeny-Carman relation, according to:

22

3

11

SBK , (10)

where is the porosity, B a constant and S the specific particle surface. The Kozeny-Carman relation is based on a tube-like representation of a porous medium. The constant B has to be determined experimentally, but has never been determined explicitly Williams (1974). The Kozeny-Carman relation assumes an isotropic porous medium. For rods other Equations have been derived that distinguish between the permeability along and perpendicular to the direction of the rods, according to:

22

3

18 Rc

K , (11)

2

2/5

min 1 RCK (12)

where R is the radius of the rods and c and C are constants depending on the arrangement of the rods while min denote the minimum pore volume for this arrangement. Also in this case forces on individual particles can be calculated. Mei & Auriault (1991) derived, for instance, the average drag acting on a particle in a porous medium with fore-aft symmetry at small Reynolds number to be:

,Re220 kkvf (13)

for a two-dimensional array. Here k0 and k2 are non-dimensional constants to be determined which is, for instance, done for both ordered and random arrays of spheres by Hill, Koch & Ladd (2001). To summarize the forces on individual particles have been exploited for certain geometries and for a number of flow conditions. We however need to investigate further higher Reynolds number flows, more complex geometries and instationary conditions.

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Conclusions

To conclude fluid mechanics of internal erosion in embankment dams is rather complex independent on the scale studied. It is therefore of highest importance to do detailed studies of the flow to clarify the mechanisms behind the starting of the process, the development of it and then conditions for healing or complete progress to breakage. Such studies must then be coupled to formulations on the continuum scale giving macroscopic conditions.

Acknowledgement

The research presented in this thesis was carried out as a part of "Swedish Hydropower Centre - SVC". SVC has been established by the Swedish Energy Agency, Elforsk and Svenska Kraftnät together with Luleå University of Technology, The Royal Institute of Technology, Chalmers University of Technology and Uppsala University.

Alstom Hydro Sweden, CarlBro, E.ON Vattenkraft Sverige, Fortum Generation, GE Energy (Sweden), Jämtkraft, Jönköping Energi, Mälarenergi, Skellefteå Kraft, Sollefteåforsens, Statoil Lubricants, Sweco VBB, Sweco Energuide, SweMin, Tekniska Verken i Linköping, Vattenfall Research and Development and Vattenfall Vattenkraft, Waplans, VG Power and Öresundskraft are also participating in SVC.

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