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ANSYS Fluent Modelling of an Underexpanded Supersonic Sootblower Jet Impinging into Recovery
Boiler Tube Geometries
by
Shahed Doroudi
A thesis submitted in conformity with the requirements for the degree of Master of Applied Science
Graduate Department of Mechanical and Industrial Engineering University of Toronto
© Copyright by Shahed Doroudi 2015
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ANSYS Fluent Modelling of an Underexpanded Supersonic
Sootblower Jet Impinging into Recovery Boiler Tube Geometries
Shahed Doroudi
Master of Applied Science
Graduate Department of Mechanical and Industrial Engineering
University of Toronto
2015
Abstract
Sootblowers generate high pressure supersonic steam jets to control fireside deposition on heat
transfer tubes of a kraft recovery boiler. Sootblowing is energy expensive, using 3-12% of the
mill’s total steam production. This motivates research on the dynamics of sootblower jet
interaction with tubes and deposits, to optimize their use. A CFD investigation was performed
using ANSYS Fluent 15.0 to model three-dimensional steady-state impingement of a Mach 2.5
mildly underexpanded (PR 1.2) air jet onto arrays of cylindrical tubes with and without fins, at
various nozzle-to-tube centerline offsets.
A free jet and four impingement cases for each of the economizer and generating bank
geometries are compared to experimental visualizations. Pressure distributions on impinging
surfaces suggest that the fins in the economizer produce a reduced but uniform sootblowing
force. Pressure contours along the tubes (in the vertical direction) show a sharp decline one tube
diameter away from the jet mid-plane.
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Acknowledgments
I would like to express my heartfelt gratitude to my supervisor, Professor Markus Bussmann,
for his compassion, patience and constant guidance throughout the course of my research. You
have been the most inspirational figure in my academic career.
I would also like to thank my co-supervisor, Professor Honghi Tran, for providing me with this
research opportunity as well as the continuous support and encouragement to complete this
work. Your wisdom and experience helped me gain perspective to set my research on the right
track. Thank you for having confidence in me even when I was doubtful of myself.
I also wish to thank my co-supervisor Danny Tandra, as well as my committee members,
Professors Nasser Ashgriz and Javad Mostaghimi for their insightful comments and valuable
advice. To Professor Nasser Ashgriz, you have been a great mentor throughout my academic
career and I am indebted to you for many academic opportunities.
I would like to acknowledge members from the research program on “Increasing Energy and
Chemical Recovery Efficiency in the Kraft Pulping Process” for their financial support. This
research is jointly supported by the Natural Sciences and Engineering Research Council of
Canada (NSERC) and the following pulp and paper related companies: Abitibi-Bowater Inc.,
Andritz Inc., Babcock & Wilcox Company, Boise Inc., Carter Holt Harvey, Celulose Nipo-
Brasileira S.A., Clyde-Bergemann Inc., Daishowa-Marubeni International Ltd., Fibria,
FPInnovations, International Paper Company, Irving Pulp & Paper Limited, Klabin Company,
MeadWestvaco Corporation, Metso Power Oy, Stora Enso Research, Suzano Pulp and Paper,
Tolko Industries Ltd. and Tembec Inc. I would also like to thank the Ontario Graduate
Scholarship (OGS) for helping fund this research project.
I am grateful to Araz Sarchami and Esmaeil Safaei for their useful suggestions on modelling
using the ANSYS Workbench. Many thanks to my dear friends: Amirali, Sasan, Eric, Adam,
Shenglong, Hugo, Michael and Amirhossein for a fun and memorable graduate experience.
Last, but not least, I want to thank my family for their unconditional love throughout my life.
To my inspirational sister, Hamaseh Doroudi, thank you for babysitting me since the day I was
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born. To my selfless mother, Sogand Ijadi, you are the reason I never feel alone. To my father
and guide, Abolghasem Doroudi, I can only hope to someday be half the man you are.
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Table of Contents
ABSTRACT ................................................................................................................................................. II
ACKNOWLEDGMENTS ........................................................................................................................... IIII
TABLE OF CONTENTS ............................................................................................................................. III
LIST OF TABLES .................................................................................................................................... VII
LIST OF FIGURES .................................................................................................................................. VIII
LIST OF APPENDICES ............................................................................................................................ XI
CHAPTER 1 INTRODUCTION ................................................................................................................... 1
PROBLEM OVERVIEW ........................................................................................................................ 2 1.1
1.1.1 Kraft Recovery Process ......................................................................................................... 4
1.1.2 Fouling ................................................................................................................................... 6
1.1.3 Sootblowing ........................................................................................................................... 7
THESIS OBJECTIVES ......................................................................................................................... 9 1.2
CHAPTER SUMMARIES .................................................................................................................... 10 1.3
CHAPTER 2 BACKGROUND ................................................................................................................... 11
POPHALI’S EXPERIMENTAL SOOTBLOWING MODEL ........................................................................... 11 2.1
2.1.1 Air versus steam .................................................................................................................. 12
2.1.2 Schlieren technique ............................................................................................................. 13
2.1.3 Tube geometries .................................................................................................................. 14
KEY CONCEPTS .............................................................................................................................. 15 2.2
2.2.1 Shock waves ........................................................................................................................ 16
2.2.2 Peak impact pressure .......................................................................................................... 17
2.2.3 Off-design jets ...................................................................................................................... 19
2.2.4 Supersonic impingement ..................................................................................................... 20
RELEVANT CFD INVESTIGATIONS .................................................................................................... 21 2.3
CHAPTER 3 THEORETICAL CONSIDERATIONS.................................................................................. 23
GOVERNING EQUATIONS ................................................................................................................. 23 3.1
K-Ε TURBULENCE MODEL ................................................................................................................ 24 3.2
ENHANCEMENTS TO THE RKE MODEL .............................................................................................. 25 3.3
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CHAPTER 4 METHODOLOGY ................................................................................................................ 27
ANSYS MODELLING CHALLENGES .................................................................................................. 27 4.1
4.1.1 Initial mesh generation ........................................................................................................ 28
4.1.2 Divergence with the Density-based Solver .......................................................................... 30
4.1.3 Pressure-based Solver shortcomings.................................................................................. 31
4.1.4 The addition of a nozzle ...................................................................................................... 34
GEOMETRY AND MESH GENERATION ............................................................................................... 35 4.2
4.2.1 Free Jet ................................................................................................................................ 35
4.2.2 Economizer .......................................................................................................................... 37
4.2.3 Generating Bank .................................................................................................................. 40
4.2.4 Offset Models ....................................................................................................................... 42
PREPROCESSING AND SOLVING ....................................................................................................... 43 4.3
4.3.1 Setup ................................................................................................................................... 43
4.3.2 Boundary Conditions ........................................................................................................... 44
4.3.3 Solving ................................................................................................................................. 45
4.3.4 Solution Initialization ............................................................................................................ 46
4.3.5 Gradient-based Mesh Adaption ........................................................................................... 47
CHAPTER 5 RESULTS AND DISCUSSION ............................................................................................ 48
FREE JET VALIDATION ..................................................................................................................... 49 5.1
FREE JET, ECONOMIZER AND GENERATING BANK: COMPARISON WITH SCHLIEREN VISUALIZATION .... 53 5.2
ECONOMIZER AND GENERATING BANK: PRESSURE DISTRIBUTION ON IMPINGING SURFACES ............. 57 5.3
EFFECT OF ECONOMIZER FINS ........................................................................................................ 58 5.4
5.4.1 PIP Distribution: Leading Tube ............................................................................................ 59
5.4.2 PIP Distribution: Leading Fin ............................................................................................... 63
5.4.3 Maximum PIP ...................................................................................................................... 64
5.4.4 Free jet vs Midway offset ..................................................................................................... 65
SECONDARY JET CHARACTERIZATION .............................................................................................. 67 5.5
MODEL LIMITATIONS ....................................................................................................................... 69 5.6
CHAPTER 6 CLOSURE ........................................................................................................................... 71
SUMMARY ...................................................................................................................................... 71 6.1
CONCLUSIONS ................................................................................................................................ 72 6.2
IMPLICATIONS ON SOOTBLOWING ..................................................................................................... 73 6.3
RECOMMENDATIONS FOR FUTURE WORK ......................................................................................... 73 6.4
References……………………………………………..………………………………………………………74
Appendix A………………………………………………………………………………...……………….….78
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List of Tables
Table 1. A summary of observations from the PIP distributions on the leading tubes. ............................ 60
Table 2. Maximum PIP values associated with each simulation. ............................................................. 65
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List of Figures
Figure 1. The Kraft process is the conventional chemical process of turning wood into pulp for
papermaking. ...................................................................................................................................... 4
Figure 2. The layout of a typical kraft recovery boiler [3]. ......................................................................... 5
Figure 3. A boiler tube coated by a deposition of carryover and fume particles[8]. ................................... 6
Figure 4. The distal end of a sootblower lance tube showing the supersonic nozzle outlet. ....................... 7
Figure 5. A view of a sootblower in operation as it traverses into the boiler. ............................................. 7
Figure 6. Sootblowers operating near a superheater platen [3]. .................................................................. 8
Figure 7. A schematic of Pophali’s experimental apparatus [3]. .............................................................. 11
Figure 8. Schematic of a schlieren visualization apparatus in operation [3]. ............................................ 13
Figure 9. Pophali's experimental generating bank model [3]. ................................................................... 14
Figure 10. Experimental economizer model: (a) schematic of one row of tubes; (b) experimental setup
[3]. .................................................................................................................................................... 14
Figure 11. In the presence of a supersonic flow, an oblique shock is formed at the tip of an object [14].
.......................................................................................................................................................... 16
Figure 12. A jet flow diverges as it interacts with tube curvature, forming an expansion shock wave [3].
.......................................................................................................................................................... 16
Figure 13. As a blunt body moves right to left in a supersonic wind tunnel, a nomal shock propogates
perpendicular to the impinging surface [15]. .................................................................................... 17
Figure 14. Multi-cell shock structure of a supersonic underexpanded jet (nozzle exit on the left) [16]. .. 19
Figure 15. Three key parameters of incompressible jet impingement onto a cylinder [3]. ....................... 20
Figure 16. A comparison of the computed axial velocity distribution along the centerline of a free
supersonic jet [4] and corresponding experimental data [22]. ue and D represent the nozzle exit
velocity and diameter, respectively. ................................................................................................. 21
Figure 17. Mach contours of fully-expanded (top) and underexpanded (bottom) sootblower jets [2]. .... 27
Figure 18. 3D perspective view of economizer tubes. .............................................................................. 28
Figure 19. A top view of the hybrid mesh. ................................................................................................ 29
Figure 20. Cross sectional view of the hybrid mesh showing large size variation between elements which
leads to an overall low quality mesh. ............................................................................................... 29
Figure 21. Dimensions and boundary conditions for the Economizer model from the jet exit onwards. . 30
Figure 22. Velocity (m/s) contour of a DBS simulation for the economizer model from the jet exit
onwards. ........................................................................................................................................... 31
Figure 23. Mach contours of PBS economizer simulations in order of increasing inlet Mach number .... 32
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Figure 24. Mach contours of the Mach 2.5 underexpanded jet into an economizer, as solved by the PBS
.......................................................................................................................................................... 32
Figure 25. Visual comparison of experimental schlieren image (left) to the CFD Mach field (right) ...... 33
Figure 26. Centerline total pressure distribution from the coupled PBS economizer simulation. p0 = 2.14
MPa and de = 7.4 mm ....................................................................................................................... 33
Figure 27. Side-view of the converging-diverging nozzle used by Pophali.............................................. 34
Figure 28. Mach contour of flow within the experimental nozzle with a supply pressure of 2.14 MPa ... 34
Figure 29. Computational domain for the free jet simulation. Dt = 11 mm is the economizer tube
diameter. ........................................................................................................................................... 35
Figure 30. Side view of the cylindrical quarter model free jet mesh. ....................................................... 36
Figure 31. Front view of the free jet mesh showing the radial refinement near the jet core. .................... 36
Figure 32. Computational domain of a sootblower jet impinging head-on onto an economizer fin Dt = 11
mm. ................................................................................................................................................... 37
Figure 33. Top view of the economizer geometry blocks. ........................................................................ 38
Figure 34. Symmetry plane view of the economizer mesh for the head-on case. ..................................... 38
Figure 35. Front view of the economizer mesh displays the mesh sweeping in the vertical direction, with
an inflation bias towards the symmetry plane. ................................................................................. 39
Figure 36. a) Top view of the mapped nozzle mesh; b) O-grid mesh refinement around finned tubes .... 39
Figure 37. Computation domain of a sootblower jet impinging head-on onto a generating bank cylinder.
.......................................................................................................................................................... 40
Figure 38. Top view of the generating bank geometry blocks. ................................................................. 41
Figure 39. Symmetry plane view of the generating bank mesh for the head-on case. .............................. 41
Figure 40. O-grid mesh and radial refinement around generating bank cylinders. ................................... 41
Figure 41. The following offset cases were selected for CFD modelling. ................................................ 42
Figure 42. The final mesh of the generating bank mid-platen offset case ................................................ 43
Figure 43. Boundary conditions imposed on the economizer domain. ..................................................... 44
Figure 44. A wall was created around the nozzle exit to avoid backflow into the surrounding outlet
surfaces. ............................................................................................................................................ 44
Figure 45. The Fluent mass balance report for the generating bank simulation. ...................................... 45
Figure 46. Mach contour of an initial economizer solution, as determined by FMG initialization. ......... 46
Figure 47. The effects of shock resolution on the Mach contour of the head-on economizer simulation. 47
Figure 48. Jet centerline PIP distribution: CFD vs. experimental measurement [3]. ............................... 49
Figure 49. Radial PIP distribution of the Pophali [3] experimental jet 10.8 diameters from the nozzle
exit. ................................................................................................................................................... 51
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Figure 50. A comparison of the jet radial expansion: CFD vs. experimental results [3]. ......................... 52
Figure 51. Flow visualization of a free jet (Top to bottom: experimental, density gradient magnitude,
Mach number) .................................................................................................................................. 53
Figure 52. Visualization of flow into an economizer at various offsets (left to right: Mach number,
density gradient magnitude, experimental) ...................................................................................... 54
Figure 53. Visualization of flow into a generating bank at various offsets (left to right: Mach number,
density gradient magnitude, experimental) ...................................................................................... 55
Figure 54. The pressure distribution on the tubes and fins of the economizer. ......................................... 57
Figure 55. The pressure distribution on the tubes of the generating bank. ............................................... 57
Figure 56. PIP distribution on the top quadrant of the leading tube EC tube............................................ 59
Figure 57. PIP distributions on the top quadrant of the leading GB tube. ................................................ 60
Figure 58. PIP distribution on the top surface of the EC leading fin. ....................................................... 63
Figure 59. Position of maximum PIP for the GB and EC “slight offset” cases. ....................................... 64
Figure 60 Experimental centerline PIP distribution for a free jet, and jets midway between tubes of EC
& GB [3]. .......................................................................................................................................... 66
Figure 61. CFD centerline PIP distribution for a free jet, and jets midway between EC and GB tubes [3].
.......................................................................................................................................................... 66
Figure 62. A Mach contour plot showing the secondary jets for the "top half of first tube" case. ........... 67
Figure 63. The angular PIP distributions on the leading and secondary tubes of EC. .............................. 68
Figure 64. The angular PIP distributions on the leading and secondary tubes of GB. .............................. 69
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List of Appendices
Appendix A. Turbulence Correction UDF Codes ……………………………………………………….78
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Chapter 1 Introduction
A persistent problem in kraft recovery boilers is “fouling”, the accumulation of fireside deposits
onto heat transfer surfaces. Fouling is controlled by the use of “sootblowers”, long lance tubes
with radially opposed nozzles that are periodically used to blow steam at supersonic velocities
(typically around Mach 2.5.) to erode and remove deposits. The effectiveness of a sootblower jet
is a strong function of the force it exerts on deposits, which is largely dependent on the local
geometry it impinges upon. In the superheater section of a recovery boiler, sootblower jets have
easier access to deposits due to the generous spacing between platens. Tubes in the generating
bank and economizer sections are more closely spaced, limiting jet access to interior deposits
beyond the leading tube. In either case, the interaction of a supersonic steam jet with tubes and
deposits is a complex phenomenon that requires further investigation.
For most of a decade, research at the University of Toronto has examined the dynamics of
sootblower jet interaction with tube geometries characteristic of a recovery boiler, in order to
quantify sootblower effectiveness. This research has involved both experimental and CFD
analyses. Pophali [3] performed experiments with a quarter scale sootblower model, using the
schlieren technique to visualize the flow of a supersonic air jet impinging onto recovery boiler
tube geometries. Pophali also used a pitot tube to measure static pressures within the jet core at
various nozzle-to-tube offsets. Tandra [1] investigated fully expanded jets with CFD, including
a study of the effectiveness of low pressure sootblowing. Emami [2] extended the CFD work to
off-design (over and underexpanded) jets impinging on geometries characteristic of superheater
platens in kraft recovery boilers. Tandra [1] and Emami [2] employed the CFDLib research code
(developed at the Los Alamos National Laboratory), and developed various modifications to the
k-ε turbulence model in order to accurately capture sootblower jet flow features. This modified
code was dubbed “Sootblower Jet Turbulence” (SJT) model [4].
The aforementioned CFD studies accurately predicted sootblower jet characteristics as well as
jet impingement onto solid surfaces. However, it was difficult to apply the CFDLib code to
flows in more complex geometries, such as those in the generating bank and economizer
sections of a recovery boiler. The present work creates such a model using ANSYS Fluent 15.0,
commercial CFD software capable of modelling and solving the 3D flow of a supersonic jet
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impinging onto complex geometries. This work builds on the work of Tandra and Emami [4] by
implementing the modifications of the SJT model into the Fluent realizable k-ε turbulence
model. The two geometries considered in this work are the economizer and generating bank
within a kraft recovery boiler, also studied experimentally by Pophali [3]. The spreading rate
and centerline Peak Impact Pressure (PIP) distributions of a free jet simulation are compared to
experimental data for validation of the CFD model. Sootblower flow into the economizer and
generating bank geometries is studied by plotting and analyzing pressure distributions on tube
surfaces. The key difference between the two geometries is the presence of fins connecting the
economizer tubes. The ANSYS Fluent model is used to assess the influence of these fins on
sootblower jet/tube interaction. Furthermore, the secondary jets that form as the primary jet
deflects off the leading tube are studied by examining the pressure distributions they exerts on
an interior tube.
In what follows, section 1.1 is a review of background information on the kraft pulping process,
fouling and sootblowing. There will be a focus on the implications of sootblowing in capital and
energy expenditures. Section 1.2 presents the thesis objectives as well as a summary of the rest
of the thesis.
Problem Overview 1.1
The pulp and paper industry refers to manufacturing enterprises that use wood as raw material to
produce pulp, paper, paperboard, and other paper-related products. In 2011, the pulp and paper
industry was responsible for 25% percent of the total energy consumption in the Canadian
manufacturing sector, making it the most energy-intensive manufacturing subsector [5]. As
result, improving energy efficiency is of utmost importance to the industry.
Paper is made of pulp, a fibrous material extracted from wood. A pulp mill is the facility in
which pulp is produced, usually by means of a chemical process. The kraft process is the most
common such process, due to its versatility and the high quality of the pulp it produces. The first
step of this process is a chemical reaction between wood chips and the pulping chemicals. A
byproduct of this process is “black liquor”, a solution of the pulping chemicals as well as the
dissolved organic matter from wood. This solution is concentrated, and then burned in a kraft
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recovery boiler to recover the inorganic chemicals, and to produce steam and power from the
combustion of the organic matter.
Fouling occurs in kraft recovery boilers because large quantities of inorganic, low-melting
temperature “fly ash” particles accumulate on heat transfer surfaces. These ash deposits have a
low thermal conductivity and restrict heat transfer between the hot flue gas and tube surfaces.
The deposits reduce overall boiler thermal efficiency and can corrode boiler tubes. In severe
cases, fouling may completely block flue gas passages requiring a costly shutdown of the boiler
to water wash the deposits.
Fouling in recovery boilers is controlled by the regular operation of sootblowers. These long
tubes traverse in between heat transfer surfaces, and produce two radially opposed supersonic
steam jets that attempt to remove deposits upon impact, to control deposit accumulation.
Anywhere from 3% to 12% of the total steam produced by a kraft recovery boiler is used for
sootblowing.
Brewster [6] describes the pulp business as “one of the most capital intensive businesses in the
world with total capital investment for a new mill being roughly four times the annual sales
revenue generated”. The recovery boiler alone represents 20% of the total investment and its
efficient operation is crucial to achieving maximum economic return from the capital
investment. A characteristic of capital intensive businesses is that the difference between net
losses and gains lies in the small final fraction of production. Brewster shows that a 5% increase
in production volume of a mill can represent a 35% increase in profits. With an annual profit as
high as $20 million dollars, an incremental change in the production of a boiler may have
substantial financial consequences. Fouling poses the greatest threat to steam generation,
especially because sootblower effectiveness is difficult to measure. This motivates research on
understanding and improving two aspects of sootblower operation. First, understanding the
pressure exerted on tube banks can help devise a strategy to maximize deposit removal. Second,
research on minimizing steam consumption while maintaining the effectiveness of sootblowers
could result in substantial financial gain for pulp mill owners.
The remainder of this section provides a more detailed overview of the kraft process, recovery
boiler fouling, and sootblowing.
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1.1.1 Kraft Recovery Process
Figure 1. The Kraft process is the conventional chemical process of turning wood into pulp for papermaking.
The kraft process is the most widely used chemical pulping process within the pulp and paper
industry. Wood chips are treated with a solution containing a mixture of sodium hydroxide
(NaOH) and sodium sulfide (Na2S) at temperatures as high as 170 °C to create pulp for
papermaking (see figure 1). The pulp is then water washed creating a liquid solution called
“weak black liquor” consisting of the inorganic cooking chemicals of the pulping process as
well as the leftover organic material from the wood. The inorganic cooking chemicals of the
pulping process are too costly for one time use [7]. Consequently, a subsequent step in the kraft
process is to recover and reconstitute the pulping chemicals to be used again.
To start the chemical recovery process, the dilute “weak black liquor” is sent to an evaporator
where its concentration is increased to the 65-85% range to form “black liquor”. The black
liquor is then fed into a kraft recovery boiler and burnt by a furnace at the bottom (see figure 2).
Upon combustion, the inorganic portion of the black liquor forms “smelt” on the bed at the
bottom of the recovery boiler. Smelt is dissolved in water to form “green liquor”, a solution
from which sulphur and sodium are extracted to recycle the chemical agents.
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Figure 2. The layout of a typical kraft recovery boiler [3].
In addition to the chemical recovery process, the recovery boiler generates steam and power
using the heat from the organic portion of black liquor. Unlike the inorganic compounds which
fall onto the bed to form smelt, the organic material burns and forms a hot flue gas which rises
and passes through several arrays of boiler tubes. Feedwater circulating inside the boiler tubes
extracts the thermal energy from the hot flue gas to produce high pressure steam. As shown in
figure 2, there are three types of tube banks within the top portion of a recovery boiler that form
a heat transfer circuit. Feedwater entering the economizer is heated to a temperature slightly
below the boiling temperature. In the subsequent generating bank and superheater sections, the
water becomes steam and superheated steam respectively. Note that in figure 2 the flue gases
flow from left to right, while the water flows from the rightmost tubes of the economizer into
the superheater.
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1.1.2 Fouling
Figure 3. A boiler tube coated by a deposition of carryover and fume particles[8].
Fouling is a persistent problem in recovery boiler operation, caused by fly ash particles
entrained in the hot flue gas, that accumulate on the surface of heat transfer tubes. Fly ash
particles consist of carryover, larger particles formed during black liquor combustion, and fume
particles that condensate from inorganic volatile compounds. Figure 3 shows the accumulation
of these two deposit types on a boiler tube. Carryover particles range from 20 μm to 3 mm in
size and tend to accumulate by impaction, and form hard deposits that adhere to tube surfaces.
Fume particles are much finer at an average diameter of 0.5 μm, and form softer deposits that
can sinter into more dense deposits. Carryover deposition is dominant in the superheater section
that particles first encounter. Fume, on the other hand, only forms at the lower flue gas
temperatures downstream of the superheater, and so tends to deposit in the generating bank and
economizer sections.
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1.1.3 Sootblowing
Figure 4. The distal end of a sootblower lance tube showing the supersonic nozzle outlet.
Sootblowing is the industry standard means of mitigating fouling within kraft recovery boilers.
As depicted in figure 4, sootblowers are steel lance tubes, typically a few meters in length and 9
cm in diameter, with two radially opposing nozzles that produce supersonic steam jets to erode
and remove deposits [2]. The two mechanisms by which sootblowers remove deposits are
“brittle breakup” and “debonding”. Brittle breakup occurs by imposing internal stresses on
deposits above their ultimate tensile strength, to induce fracture. Debonding refers to the
weakening of the adhesive force between a deposit and a tube.
Figure 5. A view of a sootblower in operation as it traverses into the boiler.
A large kraft recovery boiler has about 100 sootblowers. Sootblowers rotate into and out of the
space between tube platens (see figure 6), and are operated a few at a time in a strategic
sequence intended to maximize deposit degradation. The insertion and retraction of a typical
8
sootblower into a boiler takes about 4 minutes, while the preset sequence for all sootblowers
may take as long as several hours to complete. The sootblowing requirements of a boiler are
based on feedback parameters, such as pressure and temperature, which are monitored
continuously. Pressure probes are located in between platens to monitor pressure gradients
within the flue gas. An unusually high pressure gradient across a tube bank may be indicative of
plugging. Recovery boiler operators also monitor power to the ID fan, and flue gas exit
temperature as additional indications of plugging
Figure 6. Sootblowers operating near a superheater platen [3].
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Thesis Objectives 1.2
The objectives of this thesis are:
1. To provide an accessible CFD model that predicts the flow behaviour of sootblower jets
using the commercial software ANSYS Fluent solver in combination with the SJT
turbulence model previously developed by Tandra [1] and Emami [2]. The model is used
to produce 3D steady-state simulations of an underexpanded supersonic sootblower jet
impinging onto complex boiler tube geometries. A comparison of the CFD jet centerline
pressure distribution with experimental data will be used to assess and validate the
Fluent model.
2. To utilize the Fluent model to simulate the sootblower flows studied experimentally by
Pophali [3], within the economizer and generating bank sections of a kraft recovery
boiler, and to compare sootblower performance within those geometries. In particular,
the effect of economizer fins on sootblower flow behavior will be assessed.
Note that sootblowing involves the concurrent operation of many sootblowers in between a
large number of heat transfer tubes. The simulations at hand model instances of sootblowing at
specific orientations to the tubes. An understanding of the complex flows that result from a
supersonic underexpanded jet impinging onto the fins and cylinders of the boiler is a first step in
investigating sootblower efficiency. Furthermore, sootblower flow into the superheater
convective section of the recovery boiler will not be investigated in the present work as it has
been previously studied by Emami [2]. The economizer and generating bank geometries are
more complex and better suited for assessing ANSYS Fluent’s capabilities.
10
Chapter Summaries 1.3
Chapter 2 is a review of the literature and scientific concepts relevant to sootblower operation.
Chapter 3 reviews the governing equations of supersonic turbulent flow that are solved by
ANSYS Fluent. This chapter also presents the implementation of enhancements to the ANSYS
Fluent realizable k-ε turbulence model, appropriate for sootblower modelling.
Chapter 4 presents a comprehensive review of the ANSYS Fluent modelling process. The
governing equations of the solver will be reviewed. The choices of domain and mesh generation,
solver controls and boundary conditions will be presented and justified. There will also be a
section on the various challenges faced during the modelling process.
Chapter 5 presents the results of a free jet simulation, as well as simulations of a sootblower jet
impinging onto the economizer and generating bank geometries at four nozzle-to-tube offsets. A
comparison of the jet centerline pressure values to experimental data will be used to validate the
ANSYS Fluent model. A qualitative comparison of the results to experimental visualization will
be presented and discussed.
Chapter 6 summarizes and concludes the thesis. The implications of the CFD investigation on
sootblower performance are discussed, and recommendations are offered for future work.
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Chapter 2 Background
An overview of the literature and scientific concepts pertaining to sootblower operation is
presented. Section 2.1 is a detailed review of the work by Pophali [3], particularly the free jet,
economizer and generating bank experiments which were modelled in the present work. There
will be an emphasis on the experimental setup and boiler tube geometries which were modelled
with ANSYS Fluent. The reader may choose Section 2.2 introduces the scientific background
and key physical parameters characteristic of sootblower jets. Finally, section 2.3 presents CFD
investigations, and particularly previous research at the University of Toronto, relevant to
sootblower operation.
Pophali’s Experimental Sootblowing Model 2.1
Figure 7. A schematic of Pophali’s experimental apparatus [3].
Pophali [3] created a ¼ scale experimental model of a sootblower nozzle, and tube arrangements
characteristic of the superheater, generating bank and economizer convective sections of a kraft
recovery boiler. The objective of the experiments was to characterize the interaction of a
supersonic air jet impinging on these tube arrangements. A schlieren flow visualization
technique coupled with a high speed camera was used to image all interactions. Pitot pressure
measurements were also made within the jet core to quantify the jet structure. As shown in
figure 7, a solenoid valve connected to an air tank supplied a supersonic convergent-divergent
12
sootblowing nozzle with compressed air at a supply pressure (Po) of 2.14 MPa, similar to actual
sootblowers. The supersonic nozzle consists of a bell shaped converging portion leading to a
final throat diameter (dt) of 4.5 mm which then diverges to a nozzle exit diameter (de) of 7.4 mm
[3]. A small pitot probe was designed to move freely in the axial direction to measure static
pressure. The supersonic nozzle was adjustable in two directions: into and out of the page, as
well as axially towards the tubes. The offset between the jet and tube centerlines, the diameters
of the tubes, and the distance between the nozzle and tube were varied to examine their effects
on jet/tube interaction. The subsequent discussion in this section pertains to aspects of the
aforementioned experiment relevant to the present CFD study: the choice of air as a model fluid
for the experimental sootblower jet, an overview of the schlieren visualization technique, and
the geometries of the model economizer and generating bank tubes.
2.1.1 Air versus steam
Actual sootblowers operate with high pressure steam, but air was chosen as the model fluid for
the experiments for reasons of safety and simplicity. Pophali designed the experimental nozzle
to create a supersonic air jet geometrically and dynamically similar to actual steam sootblower
jets. The justification for using air as the model fluid is as follows:
Pophali [3] shows that both air and superheated steam are both homogenous fluids.
The heat capacity ratio,
, for air is 1.4 and similar to for steam.
The jet exit Mach number has been shown to be the most important parameter for
creating a dynamically similar jet [9]. Consequently, with a supply pressure (Po) of 2.14
MPa, the experimental nozzle produced a nozzle exit Mach number of 2.5,
corresponding to that of an actual sootblower jet.
The ¼ scale geometry using air resulted in a lab jet Reynolds number of 1.6 x 106, a
value close to the actual jet Reynolds number of 1.9 x 106.
Another characteristic to consider is the spreading rate of the supersonic jet, which is
mainly affected by the jet exit Mach number and the ratio of the ambient fluid density to
13
the density of the fluid within the jet core. Pophali imposed flow conditions similar to an
actual sootblower to ensure that the experimental jet expanded at a similar rate.
Field trials in Sweden [10] measured sootblower jet forces that were consistent with lab
scale experiments using air as a model fluid.
As a consequence of the above design choices, Pophali claimed that the results of the
experimental work were applicable to actual sootblowing inside a kraft recovery boiler.
2.1.2 Schlieren technique
Figure 8. Schematic of a schlieren visualization apparatus in operation [3].
The schlieren technique, invented by August Toepler, has long been used to visualize invisible
fluid mechanics phenomena such as shock waves [11]. The basic principle of the schlieren
visualization technique is to shine a collimated source of light, where the light rays are strictly
parallel, onto an area of interest. A transparent target medium, such as air, will bend each light
ray differently due to variations in the local refractive index. It has been shown [12] that the
local reflective index of air is directly proportional to its local density. Consequently, a density
gradient, such as the one occuring across shock wave, will result in a variation of light intensity
as light bends dissimilarly. Figure 8 shows an apparatus that facilitates the imaging of such flow
visualization. Note that the variation in how light rays are deflected as they pass through the
medium, in this case the supersonic air jet, makes it difficult to focus the resultant image. As a
result, a critical component of schlieren visualization is the placement of a knife edge at the
14
focal point of the second mirror (M2) to block half the light. Light rays that have been deflected
sufficiently to pass by the knife edge illuminate the focusing lens, brightening certain regions of
the focused image. This creates a contrast across the final schlieren image corresponding to a
change in the density gradient (first derivative of the density) in the direction normal to the knife
edge. In the absence of a knife edge, the resultant image would be a shadowgraph.
Shadowgraphs simply reflect the shadows of a transparent material exhibiting a fluid density
variation and are often observed in nature (hot air casting shadow on a nearby surface). The
variation of light intensity in a simple shadowgraph represents the second derivative of the
density gradient [13].
2.1.3 Tube geometries
Figure 9. Pophali's experimental generating bank model [3].
Figure 10. Experimental economizer model: (a) schematic of one row of tubes; (b) experimental setup [3].
15
The two tube geometries studied by Pophali that are of interest here are the economizer and
generating bank sections. Both tube configurations comprise an array of cylindrical tubes, with
the key difference being that fins interconnect the tubes of the economizer. In a kraft recovery
boiler, the fins are intended to extend the heating surfaces to maximize heat transfer.
As shown in figure 9, the generating bank model consists of a 40 tube array with a surface-to-
surface spacing of 12.7 mm. The tubes are arranged in four parallel rows of 10 tubes, with each
tube having an outer diameter of 14.3 mm. The distance between the nozzle exit and the leading
tube of the model bank is 48.35 mm. The economizer model is shown in figure 10, and consists
of two platens, 12.7 mm apart. Each platen consists of six 11 mm (outer diameter) tubes
connected by 1.2 mm thick welded fins. The tubes in each platen are a surface-to-surface
distance of 22 mm apart, and two additional fins, 11 mm in length, are welded on the windward
(facing the nozzle) and leeward (away from the nozzle) ends of each platen. The distance
between the nozzle exit and the leading fin (on the windward side) is 39 mm.
Despite the different tube diameters in the economizer and generating bank models, the fins are
of central importance in dictating the difference in flow behaviour as the sootblower jet
impinges onto the tube banks. In addition to comparing sootblower flow into the generating
bank and economizer, this difference offers an opportunity to characterize the effects of the
leading fin, essentially a flat plate, in its interaction with a turbulent supersonic jet.
Finally, experiments involving a free jet in the absence of any obstacles were also performed by
Pophali. The free jet results will be used to validate the CFD model, and to compare with jet
propagation results midway between two rows of economizer and generating bank tubes.
Key Concepts 2.2
The following section is a review of the underlying physics and key parameters of the
experimental sootblower model of Pophali, which will be examined with the CFD results of the
present work.
16
2.2.1 Shock waves
In compressible flows, substantial pressure and temperature gradients lead to variations in the
density of the flow field. The Mach number (M), the local ratio of flow velocity to the speed of
sound (a), is an indicator of compressibility within a flow field at values higher than about 0.3.
A Mach number value higher than 1 is supersonic, meaning that the local flow velocity exceeds
the speed of sound. The local speed of sound for an ideal gas such as air is directly proportional
to the square root of the absolute temperature.
Figure 11. In the presence of a supersonic flow, an oblique shock is formed at the tip of an object [14].
Figure 12. A jet flow diverges as it interacts with tube curvature, forming an expansion shock wave [3].
17
Figure 13. As a blunt body moves right to left in a supersonic wind tunnel, a nomal shock propogates
perpendicular to the impinging surface [15].
The Mach number of the Pophali jet at the nozzle exit was 2.5. A characteristic of such a flow is
the formation of oblique shock and expansion waves as the flow attempts to adjust to sudden
disturbances caused by sharp pressure gradients. An oblique shock occurs when a flow is turned
into itself and is compressed. The static pressure, which is equivalent to the pressure measured
by a pitot tube stagnating the flow, increases across an oblique shock. Figure 11 shows the
propagation of an oblique shock in a supersonic flow. Conversely, expansion shock waves are
formed when the flow adjusts to a sudden divergence or turning away of the flow, such as the
Coanda effect-induced divergence of a supersonic jet interacting with tube curvature (see figure
12). The Coanda effect refers to the tendency of a flow to be attracted to a nearby solid surface
and can lead to deviations in the flow direction. An expansion shock wave is associated with a
decrease in the static or pitot tube pressure across its shear layer.
In addition to oblique and expansion shock waves, a normal shock wave forms upstream of a
supersonic flow impinging directly onto an obstacle, such as a tube or deposit. A normal shock
wave occurs when a flow is turned to such a degree that it cannot remain attached to the
impinging body, and propagates perpendicular to its surface. Normal shocks always result in a
deceleration of the flow velocity to subsonic conditions (Mach number becomes lower than 1).
Figure 13 shows the formation of a normal shock as a supersonic flow impinges onto a blunt
object.
2.2.2 Peak impact pressure
The parameter that is considered representative of sootblower jet effectiveness is the “Peak
Impact Pressure” (PIP). PIP is the pressure a jet would exert, upon impingement, on a deposit
18
positioned somewhere along its centerline, and varies with distance from the nozzle exit. Emami
[2] defines PIP as “as the stagnation pressure on the downstream side of a normal shock wave
(when the local Mach number is greater than one), or the stagnation pressure itself (in subsonic
regions of the flow)”. To justify the applicability of PIP, Emami also shows that the force
exerted by a supersonic sootblower jet on a perpendicular flat plate [2] agrees well with the
value calculated by multiplying the plate surface area by the PIP of a free jet. Experimentally,
PIP is simply measured by probing a point along the jet centerline with a pitot tube pressure
transducer. Pophali was able to measure PIP with great repeatability [3]. To exactly replicate
this measurement in a CFD simulation, one would have to model a small cylinder, having the
diameter of the experimental probe, at various locations of interest in the computational domain.
This is not feasible considering the number of simulations one would have to run to obtain a
reasonable number of data points along the jet centerline. An alternate approach is to assume an
infinitely small tube diameter, and evaluate the effect of a normal shock wave normal to the
flow direction. This is a reasonable assumption for the Pophali experiments considering that the
nozzle exit diameter is 2.5 times that of the 3 mm probe tip. On the basis of the above
assumption, we can approximate PIP using the Rayleigh pitot tube equation which calculates the
total pressure downstream of a normal shock as a function of the upstream total pressure, the
ratio of specific heats ( ), and the upstream Mach number, as follows:
represents the local total pressure, M represents the local Mach number, and is
the heat capacity ratio of air. Using post processing tools, we can extract the local total pressure
and Mach number from a CFD result to “virtually” probe along a jet centerline. Note that the
PIP distribution on walls within the computational domain, where flow velocity is zero due to
the no-slip condition, is equivalent to the total pressure.
19
2.2.3 Off-design jets
Figure 14. Multi-cell shock structure of a supersonic underexpanded jet (nozzle exit on the left) [16].
The supersonic nozzles at the end of a sootblower lance tube are intended to operate at a certain
design pressure, to create a fully expanded jet. A study by Jameel et al. [17] showed that fully
expanded nozzles increase the jet energy exerted on deposits for removal and are therefore
desirable. However, fluctuations in the supply pressure (Po), and perhaps nozzle manufacturing
defects will produce “off-design” jets. If the static pressure of the jet at the nozzle exit plane is
higher than the ambient pressure, the jet is underexpanded. Conversely, if the static pressure at
the nozzle exit is lower than the ambient pressure, an overexpanded jet is produced. An
important characteristic of these “off-design” jets is the formation of multi-cell shock structures.
As displayed in figure 14, sudden pressure fluctuations in the form of conical expansion and
compression waves occur as an underexpanded jet acclimatizes to the ambient pressure. Upon
leaving the nozzle exit, an underexpanded jet expands rapidly to match the ambient conditions,
creating the initial bulging of the jet in figure 14. These expansion waves propagate to the
constant pressure boundaries of the jet and reflect back as compression waves to form an
adjacent oblique shock. These compression waves then reflect off the jet boundary as expansion
waves. This process repeats itself to form the diamond shock structure seen in figure 14. As the
jet radially expands, these shock cells interact with the turbulent shear layer and decay
downstream of the nozzle exit. The experiments performed by Pophali were conducted at an exit
pressure ratio of 1.2, which is a mildly underexpanded jet. The resultant shock structures have
significant implications on the CFD modelling that is presented in Chapter 3 and 4.
20
2.2.4 Supersonic impingement
Figure 15. Three key parameters of incompressible jet impingement onto a cylinder [3].
The Pophali experiments of jet/tube interaction exmained supersonic jet impingement onto
cylindrical surfaces. In the economizer model, there is the additional complication of flow
impingement onto the tip of the fin. The impingment of an incompressible jet onto cylindrical
surfaces has been studied extensively. However, the underexpanded supersonic equivalent of
this flow has not been widely studied. The shock structures characteristic of underexpanded
supersonic flows complicate flow behaviour. Nonetheless, a review of jet impingement onto
cylindrical surfaces provides insight into the interactions which we model in this thesis. Figure
15 is a schematic showing the three key governing parameters of incompressible jet
impingement onto a cylinder: the nozzle-cylinder distance, the jet diameter relative to the tube
diameter, and the offset of the nozzle centerline with respect to the tube centerline [18][19][20].
Based on these studies, the most important parameter in the Pophali generating bank
configuration is the small distance between the nozzle and the leading tube. The leading tube of
the experimental model is situated in the jet core (the region downstream of the nozzle exit
where the jet retains its properties).
Aside from the findings of Pophali, which have been discussed in detail, we are unaware of
other studies of the impingment of supersonic underexpanded jets onto finned tubes.
Furthermore, there is no research on the impingement of a supersonic jet onto the edge of a flat
plate. Much of the research on flat plate impingement involves a supersonic jet impinging onto a
normal flate plate. However, this flow behaviour is not representative of the one encountered in
an economizer. The results of this interaction will be presented in Chapter 5.
21
Relevant CFD Investigations 2.3
The University of Toronto has been involved with CFD modelling of sootblowers for the last
decade or so. Tandra [1] initiated the development of a numerical model to describe the
interaction of a fully-expanded turbulent supersonic sootblower jet with tube banks and
deposits. Tandra used this model to study a sootblower jet propagating between superheater
platens. In conjunction with laboratory experiments, he also studied the feasibility of using less
expensive low pressure steam for sootblowing operation. In the initial stages of his work,
Tandra recognized the lack of numerical models able to adequately describe the turbulence
within a supersonic sootblower jet, and so developed modified k-ε turbulence model that he
incorporated into the open source CFDLib code (developed at the Los Alamos National
Laboratory). This modification incorporated the effect of compressibility on reducing the
turbulent kinetic energy redistribution [21], into the standard k-ε model. The resulting
simulations of a fully expanded supersonic sootblower jet were in good agreement with
laboratory measurements of a free jet, and jet flows between superheater platens. An important
finding of this work is that by increasing the nozzle dimensions and steam flow rate, low
pressure sootblowing can exert forces on deposits comparable to those of high pressure
sootblowing.
Figure 16. A comparison of the computed axial velocity distribution along the centerline of a free supersonic
jet [4] and corresponding experimental data [22]. ue and D represent the nozzle exit velocity and diameter,
respectively.
0 5 10 15 200.4
0.5
0.6
0.7
0.8
0.9
1
1.1
x / D
u /
ue
Simulation
Experimental Data
22
Emami [2] built on the work of Tandra [1] by accounting for the effects of turbulence
realizability and shock unsteadiness. The improved model predicted jet characteristics more
accurately, producing results of a supersonic jet impinging onto solid surfaces that agreed well
with experimental results. Figure 16 shows an axial velocity distribution of a fully expanded jet,
modelled by Emami, compared to the experimental data of Panda and Seasholtz [22]. The
Emami model was also used to study the impingement of underexpanded sootblower jets onto
cylindrical deposit geometries. An essential finding of this work was the central importance of
the position along the multi-cell shock jet structure at which the interaction occurs, due to the
large variations in the centerline PIP within an underexpanded jet. This was confirmed by the
pitot tube PIP measurements of Pophali [3] along the jet centerline. The work of Tandra and
Emami set the groundwork for the CFD investigation in this thesis, and will be referred to again
in Chapter 3.
In addition to the above literature, a large number of CFD investigations were surveyed to
inform the setup of ANSYS Fluent boundary conditions and solver settings (e.g.
[23][24][16][34]). In particular, Garcia [25] used ANSYS Fluent to model high speed
underexpanded jet impingement onto a stationary deflector (flat disk). This work proved a
valuable resource for developing the model presented here. Garcia had success producing
accurate results using the ANSYS Fluent standard k-ε turbulence model. Furthermore, Garcia
included the nozzle as part of the computational domain; that proved to be a solution to
difficulties encountered in the present work.
23
Chapter 3 Theoretical Considerations
This chapter provides an overview of the governing equations for a supersonic compressible
turbulent flow, which are solved by ANSYS Fluent. In section 3.2, the formulations of the
standard and realizable k-e turbulence models are introduced. Section 3.3 presents two
enhancements: the removal of the dilatation dissipation term, and a structural compressibility
correction, to the Fluent realizable k-ε turbulence model, and the implementation of these
enhancements into ANSYS Fluent using User-Defined Functions (UDFs).
Governing Equations 3.1
The flow of a sootblower jet as it exits a lance tube is supersonic, highly compressible and
turbulent. The smallest turbulence scales of a supersonic flow are greater than the molecular
scales [26], rendering the flow a continuum phenomenon. Consequently, the Navier-Stokes (N-
S) equations which govern the conservation of mass and momentum of a continuum fluid can be
used to represent the flow. The N-S equations are solved by ANSYS Fluent to obtain the
velocity and pressure fields within a domain, and for compressible flows, Fluent also solves the
conservation of energy equation to couple the velocity and static temperature field. Finally, the
pressure and static temperature fields are used to determine the density field using the ideal gas
equation. The aforementioned equations are as follows:
Conservation of Mass:
Conservation of Momentum:
Conservation of Energy:
24
Equation of State (Ideal Gas Law):
is the fluid density, is time, ⃗ is the velocity vector, is the static pressure, ̿ is the stress
tensor, is the total fluid energy, is the thermal conductivity of air, is the ambient
pressure of the flow, set to atmospheric pressure of 101.3 kPa, = 286.9 J/(kgK) is the
specific gas constant for air, and is the static temperature.
k-ε Turbulence Model 3.2
The N-S equations describe any turbulent flow and can be solved numerically using the Direct
Numerical Simulation (DNS) technique. However, DNS modelling of a sootblower jet is not
feasible because to the random fluctuations and eddy motions take place over a wide range of
length scales. The grid size of such a simulation, dictated by the smallest Kolmogorov
turbulence scales, would require immense computational resources [1].
An alternative approach is the two-equation k-ε model which requires far less computation, yet
provides the means of capturing the mean-flow features of turbulence relevant to the present
research objectives. The standard k-ε model describes flow turbulence using two transport
equations for the turbulent kinetic energy (k) and rate of dissipation (ε), as follows:
is the velocity component, is the production of k due to the mean velocity gradients, is
the production of k due to buoyancy, is the contribution of the fluctuating dilatation in
compressible turbulence to the overall dissipation rate, is the viscosity, and is the turbulent
viscosity which is assumed to be constant. is a user-defined source term for modifying the
turbulent kinetic energy equation. The rest of the parameters are constant values fitted to
various turbulent flows: σk = 1, σϵ = 1.3, C1ϵ= 1.44, C2ϵ = 1.92 and C3ϵ = 0.09 as per the ANSYS
Fluent User Guide [27].
25
The standard k-ε model cannot accurately capture flow fields with adverse pressure gradients,
separation and complex secondary flow features, all of which are present in a sootblower jet
flow. The realizable k-ε (RKE) model, a variation of the standard k- ε model addresses these
limitations [28]. The term ‘realizable’ refers to satisfying mathematical constraints on the
Reynold stresses which are consistent with the physics of a turbulent flow. To achieve this, RKE
replaces the standard k-ε dissipation rate transport equation with an improved one “derived from
an exact equation for the transport of the mean-square vorticity fluctuation” [28]. Furthermore,
RKE introduces a variable formulation for the turbulent viscosity term that is a constant in the k
and ε equations. This new turbulent viscosity formulation is a function of the mean strain and
rotation rates as well as the turbulence field (k and ε).
Enhancements to the RKE model 3.3
The robustness of the RKE model comes at the price of accuracy when capturing certain aspects
of sootblower jet flow. There are two aspects of supersonic flow in particular with which the
RKE model struggles: the compressibility of high Mach number flows, and the shock structure
of an underexpanded jet.
The k-ε model was initially developed assuming that compressibility effects are negligible [1],
and as reported by Thies & Tam [29], results depart significantly from experimental data at
supersonic Mach numbers. Furthermore, as reported by Sinha et al [30] and Liou et al [31], the
k-ε model fails to accurately describe flows within shock waves as it overpredicts the k
production across each shock. Consequently, to model sootblower jet flow one must suppress
the amplification of k across shocks [1].
To address the aforementioned shortcomings of the k-ε model, Emami [32] incorporated the
corrections into two User Defined Functions (UDFs), which are presented next. The UDF codes
are in Appendix A.
Removing the Dilatation Dissipation term
Sarkar [33] proposed an additional “Dilatation dissipation” term to the turbulent kinetic energy
equation to account for the failure of the k-ε model to “predict the observed decrease in
spreading rate with increasing Mach number for compressible mixing and other free shear
layers”. This correction term, previously presented on the right hand side of equation (3.5), is:
26
As reported by Gross [35], the addition of this term yields a solution that “does not exhibit
sufficient mixing at the higher Mach numbers seen for the 3-D jet because it suppresses
turbulence growth excessively.” It has been shown that this term is not necessary for
sootblowing simulations [32].
The first UDF code in Appendix A implements the Sarkar correction term (3.7) into the right
hand side of equation (3.5) as the user defined source (Sk) term. The addition of this term
effectively eliminates the Fluent implementation of the Sarkar term (in the form of the term
YM). In other words, adding the correction term through the source term Sk removes it from the
k transport equation.
Structural Compressibility Correction
Compressibility strongly reduces the growth of turbulent kinetic energy in supersonic flows. As
one of the first to address this problem, Heinze [21] used the results of the DNS compressible
flow simulations performed by Pantano and Sarkar [36] to obtain an empirical expression
relating the k production to Mach gradients. As the structural compressibility (Mach gradients)
increases, the turbulent viscosity reduces significantly. This results in a reduction of the
turbulent stresses and suppresses the turbulent kinetic energy production, a phenomenon
neglected by ANSYS Fluent.
Tandra [1] implemented the empirical expression into the k-ε model to obtain an expression for
the turbulent viscosity μt as a function of and the Mach gradient Mg, as follows:
The second UDF code in Appendix A implements the turbulent viscosity formulation of
equation (3.8) into the ANYS Fluent solver.
27
Chapter 4 Methodology
The approach to modelling sootblower jet flows, defined as the steady-state impingement of a
3D turbulent, highly compressible, supersonic (Mach 2.5) underexpanded jet onto complex
geometries, with ANSYS Fluent is presented. First, various challenges of using the ANSYS
Fluent software for modelling supersonic flow over complex geometries are discussed. Then the
modeling process is presented, starting from choices of geometry and mesh generation, to
boundary condition selection, solution initialization and finally solution convergence.
With ANSYS Fluent, one is constrained by the parameters the software provides, and often it is
through trial and error that the best setup for a particular problem is found. Consequently, this
chapter serves as an overview of ANSYS Fluent capabilities and limitations in predicting under-
expanded supersonic flow over complex geometries.
ANSYS Modelling Challenges 4.1
Prior CFD sootblowing models developed at the University of Toronto were generated using the
CFDLib code from the the Los Alamos National Laboratory. Tandra implemented the k-ε
modifications of Chapter 3 into CFDLib and Emami further incorporated a realizability and
shock unsteadiness condition into the standard k-ε model. In what turned out to be important to
the present work, Emami modelled fully-expanded and underexpanded sootblower jets from the
nozzle exit onwards (result shown on figure 17).
Figure 17. Mach contours of fully-expanded (top) and underexpanded (bottom) sootblower jets [2].
28
This earlier CFD work served as the starting point for the ANSYS Fluent modelling. In section
3.4, the final preprocessing for the simulations in this thesis will be presented to the reader.
However, to provide the reader with a clearer picture of the modelling process, we first present
various difficulties and obstacles encountered while working with ANSYS Fluent, which
informed the development of the final model.
4.1.1 Initial mesh generation
Figure 18. 3D perspective view of economizer tubes.
The economizer geometry consists of rows of cylindrical tubes connected by fins that resemble
flat plates. Although this geometry is comprised of simple shapes, it is a complex geometry to
mesh. Initially, the geometry was blocked into ten rectangular subcomponents and meshed with
1.8 million elements. The outer blocks, where there would little to no flow, were meshed with
hexahedral elements. The core blocks aligned with the economizer fins were meshed with
tetrahedral elements and refined near high curvatures. Furthermore, the mesh was refined within
the jet core, in the space between the nozzle exit and the leading fin. Despite several versions of
the tetrahedral mesh with inflations around the cylinders and fins, a quality mesh was not
obtained. All simulations with this hybrid tetrahedral mesh diverged due to the low mesh
quality. Figure 19 and 20 illustrate a cross sectional view of the hybrid mesh and shows that
large size variations exist between adjacent elements, which lead to numerical errors and thus a
low quality mesh. Nonetheless, through appropriate blocking of the geometry, a higher quality
29
hexahedral mesh was developed. The details of this mesh will be presented in section 3.3 when
discussing the final modelling process.
Figure 19. A top view of the hybrid mesh.
Figure 20. Cross sectional view of the hybrid mesh showing large size variation between elements which
leads to an overall low quality mesh.
30
4.1.2 Divergence with the Density-based Solver
ANSYS Fluent offers two solvers, the density-based solver (DBS) and the pressure-based solver
(PBS). In both approaches, the governing momentum equation (3.2) is solved to obtain a
velocity field. However, the DBS then uses the continuity (3.1) equation to determine the
density field, while the pressure field is determined via the equation of state (3.3). Consequently,
the DBS solves the energy equation to determine the temperature field used in equation (3.3).
On the other hand, the PBS manipulates the N-S equations to determine a pressure correction
equation which it uses to obtain the pressure field. Traditionally, the PBS is favored for
incompressible or slightly compressible flows (around Mach 0.3 or less), while the DBS
approach was designed for highly compressible and supersonic flows. Over the years,
improvements to both approaches have made them capable of solving a broad range of flows.
For instance, similar to the DBS, the coupled PBS [37] couples velocity and pressure, solving all
equations simultaneously. This makes the coupled PBS an alternative to the DBS that is
applicable to compressible flows. However, for a supersonic underexpanded sootblower jet, the
DBS offers the advantage of better shock resolution and therefore greater accuracy of results
[38].
Figure 21. Dimensions and boundary conditions for the Economizer model from the jet exit onwards.
31
For this reason, the DBS was the first choice for modelling sootblower jet flow into an
economizer. The boundary conditions displayed in figure 21 were implemented into ANSYS
Fluent and solved with DBS starting from an initial zero-velocity solution. The resulting
simulations diverged or plateaued at high residuals. Figure 6 shows that the flow field stagnated
shortly after entering the domain.
Figure 22. Velocity (m/s) contour of a DBS simulation for the economizer model from the jet exit onwards.
4.1.3 Pressure-based Solver shortcomings
As mention, the coupled PBS offers an alternative DBS solver for modelling supersonic
compressible flows. The problem setup presented in figure 21 solved by the coupled PBS
resulted in similar divergence issues previously discussed in section 3.2.2.
Convergence stability is hard to achieve in compressible flows due to the high degree of
coupling between velocity, density, pressure and energy. The ANSYS User Guide [39] offers
multiple strategies to address this solution instability. One suggestion offered by the Guide is to
start by solving with a reduced inlet to outlet pressure ratio, for example one that corresponds to
Mach 0.3. That solution can then be used to initialize a higher inlet Mach number simulation
until the desired value of 2.5 is reached. Using this approach with the coupled PBS, a converged
second order solution was finally obtained for the underexpanded Mach 2.5 sootblower jet into
an economizer (see figures 23 and 24).
32
Figure 23. Mach contours of PBS economizer simulations in order of increasing inlet Mach number
Figure 24. Mach contours of the Mach 2.5 underexpanded jet into an economizer, as solved by the PBS
33
Figure 25. Visual comparison of experimental schlieren image (left) to the CFD Mach field (right)
As displayed in figure 25 the PBS simulation of a Mach 2.5 underexpanded jet into an
economizer is in good qualitative agreement with the schlieren visualization in terms of the flow
separation points on the impinging leading fin. However, as expected, the PBS struggles with
resolving the shock structure, resulting in smeared shocks. The major shortcoming of the PBS
simulation, however, is that it fails to predict a reasonable pressure field within the core of the
underexpanded jet. A centerline profile (figure 26) shows that the jet total pressure remains at a
constant value of 2.14 MPa, the pressure specified at the simulation inlet.
Figure 26. Centerline total pressure distribution from the coupled PBS economizer simulation.
p0 = 2.14 MPa and de = 7.4 mm
34
4.1.4 The addition of a nozzle
A look at similar simulations of underexpanded jet modelling using ANSYS Fluent, by Garcia
[25], Brown [40] and Munday [41], prompted the idea of including the converging-diverging
nozzle in the computational domain. Subsequently, a personal communication with an ANSYS
developer [42] confirmed that including the nozzle is crucial for capturing the flow features of a
supersonic underexpanded jet.
Figure 27. Side-view of the converging-diverging nozzle used by Pophali.
Figure 28. Mach contour of flow within the experimental nozzle with a supply pressure of 2.14 MPa
The bell shaped converging-diverging nozzle used by Pophali [3] was measured and modelled
with ANSYS Workbench. Note that adding the nozzle changes the mass flowrate inlet
boundary condition, previously presented in Figure 21, to a nozzle inlet pressure boundary
condition of 2.14 MPa. This value is reported by Pophali [3] as the average supply pressure of
the compressed air tank, used to produce the experimental model sootblower jet. To confirm the
35
accuracy of the nozzle geometry for generating the desired conditions at the nozzle exit, an
independent 3D steady state simulation of the flow inside the nozzle was performed. A highly
refined mesh of 1 million tetrahedral elements was generated and a boundary condition of 2.14
MPa was imposed on the nozzle inlet. The Mach contour plot in figure 28 shows that the Mach
number at the nozzle exit plane is 2.5, as is expected. Furthermore, the static pressure
approximately 0.5 mm downstream of the nozzle exit plane reached an approximate value of 19
kPa gauge. This result is in agreement with the outlet to ambient pressure ratio of 1.2 measured
by Pophali [3].
Geometry and Mesh Generation 4.2
This section describes the geometrical modelling and meshing that was done for the simulations
presented in this thesis. All geometries were modelled using SolidWorks 2012 and imported into
ANSYS Workbench using the .sat file format. All meshes were generated using ANSYS
Workbench.
4.2.1 Free Jet
Figure 29. Computational domain for the free jet simulation. Dt = 11 mm is the economizer tube diameter.
36
Pophali [3] measured the centerline PIP values of a free jet up to 46 nozzle exit diameters from
the nozzle exit. The free jet simulation serves as a source of validation for the subsequent
economizer and generating bank simulations. A free jet was modelled in 2D using the ANSYS
Fluent axisymmetric solver, but a converged solution could not be obtained. Consequently, a 3D
cylindrical quarter geometry, with two planes of symmetry, was generated for the free jet
simulation. As shown in figure 29, the cylindrical domain is scaled in the radial direction by 8
nozzle diameters and 42 nozzle diameters in the axial direction.
Figure 30. Side view of the cylindrical quarter model free jet mesh.
Figure 31. Front view of the free jet mesh showing the radial refinement near the jet core.
37
The domain was meshed with 0.1 mm tetrahedral elements in the nozzle region and hexahedral
elements in the remainder. From the nozzle exit onwards, the mesh spacing was controlled in
the radial direction by 80 divisions with an inflation growth rate of 5%, in the angular direction
by 70 equal divisions, and in the axial direction by 360 divisions with an inflation growth rate of
1%. The resultant quarter model mesh consists of 3.6 million elements with an orthogonal
quality of 0.91 (shown in figures 30 and 31).
4.2.2 Economizer
Figure 32. Computational domain of a sootblower jet impinging head-on onto an economizer fin Dt = 11 mm.
Pophali’s ¼ scale economizer model consists of two finned tube platens separated by a tube-to-
tube spacing of 23.7 mm. All other dimensions of the experimental economizer platens are
presented in figure 10a of Chapter 2. A 3D rectangular geometry, scaled with respect to the 11
mm tube diameter, as shown in figure 32, was generated as the computational domain for the
economizer simulations. In order to minimize the computational costs, only the first three finned
tubes of each platen were included in the domain. The centerline of the nozzle was aligned with
the centerline of the leftmost platen in order to simulate the head-on economizer experiment.
38
Figure 33. Top view of the economizer geometry blocks.
To create a high quality mesh, the domain was blocked to establish greater control over mesh
sizing. As shown in figure 33, blocks were sliced to segregate regions of prominent flow
features from outer blocks where the velocities are near zero and pressure gradients are small.
The rectangular volume around each finned tube was sliced into eight smaller quadrilateral
sections. Once sliced, the element growth rate along the slice lines was used to control the radial
growth of the mesh around each tube.
Figure 34. Symmetry plane view of the economizer mesh for the head-on case.
39
Figure 35. Front view of the economizer mesh displays the mesh sweeping in the vertical direction, with an
inflation bias towards the symmetry plane.
Figure 36. a) Top view of the mapped nozzle mesh; b) O-grid mesh refinement around finned tubes
Once the geometry was blocked, the meshing process involved imposing the number of element
divisions on the resultant edges. The choices of element sizing were made to ensure a smooth
transition from refined areas of interest to the coarse inconsequential blocks. The symmetry
plane mesh was replicated (defined as “sweeping” by ANSYS) in the vertical direction with a
growth rate of 4% (see figure 35). As shown on figure 36a, the nozzle surfaces were mapped
(following the nozzle topology) and a sizing of 0.2 mm was imposed on all elements throughout
the body. Figure 36b shows a close-up of the O-grid mesh (element size refining as they
approach the tube circumference) with the leading cylinder having greater radial refinement.
The final mesh (top view shown in figure 34) comprised of 4.8 million elements, with an
40
average orthogonal quality of 0.96, and a minimum of 0.22. The orthogonal quality represents
the deviation of the element edges from the perfect orthogonal orientation of a cuboid element,
having an orthogonal quality of 1 [43]. Using this blocking approach, we were able to create a
high quality mesh consisting entirely of hexahedral elements from the nozzle exit onwards.
4.2.3 Generating Bank
Figure 37. Computation domain of a sootblower jet impinging head-on onto a generating bank cylinder.
The generating bank model created by Pophali was a 4 x 10 array of 14.3 mm wide cylindrical
tubes separated by 12.7 mm (surface to surface) in all directions. A 2 x 3 representation of the
array was chosen for the CFD model since the prime area of interest is the flow interaction with
the leading and secondary cylinders. The reader may refer to the economizer computational
domain of figure 32 for the dimensions not shown in the generating bank domain of figure 37.
41
Figure 38. Top view of the generating bank geometry blocks.
Figure 39. Symmetry plane view of the generating bank mesh for the head-on case.
Figure 40. O-grid mesh and radial refinement around generating bank cylinders.
42
The generating bank geometry and mesh were generated in a similar way to that of the
economizer. The lack of fins allowed for easier blocking (shown in figure 38) around the
cylinders. This resulted in a smooth meshing surrounding the leading and secondary cylinders,
as shown in figure 40. The edge size divisions throughout the meshing process were chosen to
create a mesh consistent with that of the economizer. The final mesh (shown in figure 39)
comprised of 4.6 million elements with an average quality of 0.97 and a minimum of 0.22.
4.2.4 Offset Models
Figure 41. The following offset cases were selected for CFD modelling.
Pophali performed schlieren visualizations of offset cases for both the generating bank and
economizer models. Starting from the initial head on case, the nozzle was offset in increments
of 2 mm towards the final mid-platen position. Pophali performed visualizations of eight offset
cases for each of the generating bank and economizer models, of which we chose four for CFD
modelling.
43
Figure 42. The final mesh of the generating bank mid-platen offset case
Using ANSYS Workbench, the nozzle body was selected and translated by the necessary
increment in the Y-direction (as defined in figures 34 and 39). Adjustments were made to the
blocking of each offset case to accommodate the shifting of prominent flow features. Figure 42
shows an example of this accommodation in a mesh for the mid-platen offset case of the
generating bank, where the elements around leading cylinder of both platens are equally refined.
The number of elements, and the quality of all offset meshes were close to the values previously
presented for the head on cases.
Preprocessing and Solving 4.3
This section outlines the boundary conditions and setup parameters for implementing an
accurate and convergent sootblower jet model into Fluent. How the solving process is initiated
and monitored to achieve convergence, and how shock resolution is enhanced through grid
adaption, are also discussed.
4.3.1 Setup
All results presented in Chapter 5 are second-order accurate steady-state simulations using the
Density-Based Solver (DBS) along with the energy equation. The density of air was modelled
using the ideal gas law. Explicit and implicit formulations were both used throughout the
simulations, depending on convergence behavior. A total temperature value of 293 K, as per the
Pophali experiments, was imposed on all boundary conditions. ROE-FDS was used as the
convective flux type for all simulations. Both the Green-Gauss and node-based gradient
44
evaluation approaches were used, depending on convergence behavior. A very low Courant
number (0.1 < CFL < 0.01), and under-relaxation, were used throughout the simulations to
maintain convergence of flow residuals. Finally, the two UDFs previously discussed in Chapter
3 were implemented into ANSYS Fluent:
The Heinze structural compressibility model was set to define the turbulent viscosity.
The Sarkar dilatation dissipation term was eliminated from the turbulent kinetic energy
equation by subtracting it via a source term.
4.3.2 Boundary Conditions
Figure 43. Boundary conditions imposed on the economizer domain.
Figure 44. A wall was created around the nozzle exit to avoid backflow into the surrounding outlet surfaces.
45
The boundary conditions shown in figure 43 were imposed in order to produce an undexpanded
sootblower jet into the economizer geometry. A pressure inlet boundary condition at a uniform
value of 2.14 MPa gauge was imposed on the distal surface of the nozzle. Using the nozzle exit
diameter of 7.4 mm as the flow hydraulic diameter and a turbulent intensity of 1%, the turbulent
kinetic energy at the inlet was initialized to a calculated value of 49 m2/s
2 with a dissipation rate
of 2.2 x 105 m
2/s
3. The nozzle and tube surfaces were defined as no slip walls. The top surface
of the domain was defined as a symmetry boundary condition as only half of the nozzle was
included in the domain. Finally, all other surfaces were defined as pressure outlets at 0 kPa
gauge. The turbulent kinetic energy at the outlet was initialized to a value of 1.0 m2/s
2 with a
dissipation rate of 1.0 m2/s
3 as these values were determined to be inconsequential to the
simulation results. An additional wall surface, shown in figure 44, was defined surrounding the
nozzle exit in order to prevent backflow into the immediately adjacent pressure outlet. The same
The boundary conditions of the economizer model in figure 43 were also applied to the
generating bank and free jet models, with only a change in geometry.
4.3.3 Solving
In order to determine convergence of CFD simulations, the residual behavior of the energy,
velocity, turbulence and continuity terms are usually monitored with respect to the number of
solver iterations. The residuals for all simulations were monitored to reach an order of 10-2
. The
residual behavior was constantly monitored and under-relaxation factors adjusted to achieve an
optimal balance between solution stability and convergence acceleration. However, the ANSYS
User Guide [44] points out that “there are no universal metrics for judging convergence” and
that “residual definitions that are useful for one class of problem are sometimes misleading for
other classes of problems”. Consequently, in addition to monitoring residuals, the overall mass
balance of each simulation was monitored (an example of this is shown in figure 45).
Monitoring the mass ensures that the difference between the outlet and inlet mass fluxes
represents at most a 5% mass imbalance.
Figure 45. The Fluent mass balance report for the generating bank simulation.
46
4.3.4 Solution Initialization
In the case of complex flows, such as that of a sootblower jet impinging onto the finned tubes of
an economizer, an appropriate initial solution is critical for establishing and accelerating
convergence. One approach is to initialize all variables in interior domain cells to those of the
inlet, except for the velocity which is set to zero. The logic behind this technique is that the
velocity field will develop from the inlet onwards, making it an appropriate initial guess. In the
preliminary stages of running simulations, we struggled to achieve solution convergence with
the Density-Based Solver using this initialization technique.
An alternative initialization technique, as suggested by the ANSYS Tutorial Guide on modelling
external compressible flow [38], is to utilize the Full Multigrid (FMG) feature that involves
constructing a number of grid levels of varying coarseness. The flow is solved quickly on the
coarsest grid level; this provides a rough solution of the major flow features, which is
interpolated onto a finer mesh in a subsequent iteration. This process is repeated until a solution
is obtained on the finest level available, which the original grid. The default settings of the FMG
feature were used to initiate all simulations.
Figure 46. Mach contour of an initial economizer solution, as determined by FMG initialization.
As seen in figure 46, the FMG initialization creates a rough, qualitative solution for the solver to
iterate on. This can help to accelerate convergence, but may also lead to difficulty achieving
very low residuals, as certain values are quite close to those of the converged solution.
47
4.3.5 Gradient-based Mesh Adaption
Achieving a mesh independent solution, one for which a parameter of interest does not differ
appreciably as the mesh is refined, is desired for all CFD simulations. For simple geometries,
such as external flow over a single cylinder, this can be easily done by refining a mesh until
further computational costs are not justified by the change in solution accuracy. Furthermore,
the parameter of interest is usually a single value such as the drag coefficient on the cylinder. In
the case of sootblower jet flow onto economizer and generating bank geometries, there are many
meshing parameters to alter and many field variables to monitor. To add to this complexity,
offset simulations can have refinements that differ from one another. Consequently, it is very
difficult to investigate mesh independence by generating multiple meshes of varying refinement
for each case.
One solution to this problem is to use solution-adaptive mesh refinement determined by the
numerical solution. Fluent offers a Gradient Adaption feature that refines a mesh using gradients
of any particular field variable. Refining with respect to gradients of total pressure is a suitable
choice for resolving the shocks of an underexpanded jet and progressing to a mesh-independent
solution. The maximum pressure gradient was calculated and all cells within 10% of this value
were selected for refinement. Figure 47 shows the improvement in shock resolution after using
Gradient Adaption. A total pressure-based Gradient-based mesh Adaption was performed on all
simulations in this thesis.
Figure 47. The effects of shock resolution on the Mach contour of the head-on economizer simulation.
48
Chapter 5 Results and Discussion
ANSYS Fluent results of sootblower jet flow into economizer and generating bank geometries
are presented. With the convergence criteria described in section 3.4.3, each simulation took 4-5
days to complete on an Intel i7-3770 3.4 GHz machine with 24 GB of RAM.
To validate the ANSYS Fluent model, the results of a free jet simulation are compared with
experimental data. Then density gradient and Mach contours of the simulation results are
qualitatively compared to schlieren visualizations of Pophali [3]. Finally, PIP distributions of the
following flow scenarios are examined:
a primary jet impinging on a leading tube, for all simulations,
a primary jet impinging on the leading fin of the economizer geometry,
the impingement of a secondary jet onto interior tubes, and
the propagation of a free jet midway between tubes.
Additionally, we also present the values and location of the maximum PIP exerted on the
impinging surfaces.
49
Free Jet Validation 5.1
Figure 48. Jet centerline PIP distribution: CFD vs. experimental measurement [3].
Figure 38 illustrates a comparison of jet centerline pitot tube measurements with PIP values
calculated from the Fluent free jet model results using the Rayleigh pitot tube formula (eq 2.1).
The PIP to supply pressure (Po) ratio at the nozzle exit is 0.46 for both results. As the
underexpanded jet leaves the nozzle, it completes its first expansion outside the nozzle and thus
the PIP decreases. The ensuing oscillations represent compression / expansion waves of the
shock structure. Note that each peak-to-peak variation of the PIP represents one shock cell. A
comparison of the plot in figure 48 to that of the fully-expanded jet in figure 16 shows the
importance of the location of jet impingement on the flow behaviour. Depending on the position
50
of the shock cells, at impingement positions only one nozzle diameter apart a deposit may
experience a 50% difference in PIP.
The experimental results exhibit 8 shock cells. The first four dissipate very little as they reach a
similar peak PIP value; the last four shock cells gradually dissipate as the jet weakens. Fluent
predicts 5 shock cells within the jet core which dissipate gradually, similar to to the last four of
the experimental results. Overall, the CFD predicted shock cells diffuse in strength and size at a
faster rate than the experimental data.
Capturing shock cells of a supersonic underexpanded jet is notoriously difficult and the above
represents our best effort using the modelling process presented in Chapter 4. A possible cause
of the accelerated shock cell diffusion in the Fluent result may be due to an overprediction of the
turbulence generated in the shear layer. This overprediction may be attributed to the choice of
inlet turbulence boundary conditions. The initial inlet turbulence parameters (k and ε) of all
simulations were calculated by Fluent based on our input of 1% turbulent intensity and a
hydraulic diameter of 7.4 mm (equal to nozzle exit diameter). These input values were based on
an investigation of turbulence in external flows over a bluff body, similar to the flow considered
here [23]. Furthermore, note that the Fluent results are subject to the limitations of the Rayleigh
equation (eq. 2.1) that assumes a perfect normal shock on an infinitely small pitot tube.
Nonetheless, the ANSYS Fluent free jet does a good job at capturing the general trend observed
in the centerline PIP distribution of the experimental free jet results. As a result, the Fluent
model is deemed appropriate for a study of the relative performance of a sootblower jet
impinging onto the economizer and generating bank geometries at various offsets. It should be
noted that the results far downstream of the nozzle exit, at about 35 nozzle diameters, are
distorted by the limited domain size. This is inconsequential to the investigations of the present
work, as impingement in the economizer and generating bank occur in at about 5 to 6 nozzle
diameters downstream of the nozzle.
51
Figure 49. Radial PIP distribution of the Pophali [3] experimental jet 10.8 diameters from the nozzle exit.
Another source of validation for the Fluent model is the jet spreading rate measured by Pophali
[3]. One way to characterize the spreading rate of a supersonic jet is to determine the effective
jet radius at various axial positions. Pophali [3] defines jet radius as the radial distance between
the centerline and the point where PIP decreases to 5% of its maximum value at that cross
section. Pophali measured PIP, in increments of 1 mm across the jet radius, at various axial
distances. For example, figure 49 shows the radial PIP distribution at an axial position of 10.8
nozzle diameters, along with an indication of the jet radius. Using radial PIP profiles at various
axial positions selected by Pophali , a set of corresponding jet radii were determined from the
Fluent results. A comparison of the results is presented in figure 50, and shows a strong
agreement between the Fluent model and two experimental data sets. The additional
experimental data comes from Kweon et al [45] who studied jet spreading of a slightly more
underexpanded jet under similar operating conditions. As seen in the plot of figure 50, the jet
radius initially increases due to expansion at the nozzle exit; further downstream the jet radius
increases due to the entrainment of the surrounding air and turbulent mixing. Overall, the jet
spread is small as is expected with a focused highly supersonic jet.
52
Figure 50. A comparison of the jet radial expansion: CFD vs. experimental results [3].
53
Free Jet, Economizer and Generating Bank: 5.2
Comparison with Schlieren Visualization
Figures 51-53 provide a visual comparison of Fluent results, in the form of density gradient
magnitude and Mach number contours, to schlieren images of a free jet, and jet flows into
economizer and generating bank tube geometries. The offsets that are specified in figures 52 and
53 are defined in figure 41 of section 3.3.4.
Figure 51. Flow visualization of a free jet (Top to bottom: experimental, density gradient magnitude, Mach
number).
54
Figure 52. Visualization of flow into an economizer at various offsets (left to right: Mach number, density gradient magnitude, experimental).
55
Figure 53. Visualization of flow into a generating bank at various offsets (left to right: Mach number, density gradient magnitude, experimental).
56
Comparing these figures, the Fluent simulations are in reasonable agreement with the schlieren
images, exhibiting similarly located shock cells, normal shock waves and points of separation
from the impinging surfaces.
The free jet simulation exhibits fewer and wider shock cells in comparison to the experimental
results. As previously observed on the centerline PIP distribution, Fluent predicts 5 observable
shock cells in the free jet core. The “midway between tubes” offset does not impinge on any
surface, and so is similar to that of the free jet. Expansion waves, that look like arrow heads,
form on the leeward (the side opposite the surface facing the jet) side of the first and second
tubes for the case of jet flow midway between tubes. This expansion wave, associated with a
sudden pressure drop, may be caused by the supersonic jet adjusting to the Coanda effect as the
flow diverges (following the tube curvature). This pressure drop was calculated (using Fluent
results) as the difference between PIP values upstream and downstream of the shock apparent
shear layer. A visual comparison of the “midway between tubes” results (bottom row of figures
52 and 53) shows that the CFD model has resolved the boundaries of these expansion waves
with reasonable accuracy.
One prominent visual discrepancy, present on the zero and slight offset generating bank and
economizer simulations, is the diffusion of the secondary jet following impingement. This
diffusion causes the secondary jet to form at a very different angle than in the schlieren images.
Conversely, the secondary jet of “top half of first tube” is in surprising agreement with the
schlieren image. Recall the free jet centerline PIP distribution comparison of figure 49: the jet
impinges in the region between 5 to 6 nozzle diameters. At 5 nozzle diameters downstream, the
Fluent sootblower jet is at the peak of its expansion (PIP is at a local minimum) while the
experimental model is at the peak of its compression (PIP is at a local maximum). However, the
PIP values of the Fluent and experimental model are in better agreement further downstream.
The third offset case is nearly one nozzle diameter above the leading tube centerline and
experiences impingement much closer to 6 nozzle diameters downstream of the jet core.
This explains the weak secondary jet behavior of the first two offset cases, while explaining the
agreement observed in the “top half of first tube” case. For the purposes of the study at hand,
this is the only offset for which the secondary jet behavior will be quantitatively characterized.
57
Economizer and Generating Bank: 5.3
Pressure Distribution on Impinging Surfaces
Figure 54. The pressure distribution on the tubes and fins of the economizer.
Figure 55. The pressure distribution on the tubes of the generating bank.
A 3D simulation of a sootblower jet allows for investigation of the pressure distributions on the
tubes and fins. As a sootblower impinges onto the geometry, a portion of its kinetic energy is
transferred to the impacted surface and the weakened jet is then deflected in three dimensions.
Although sootblowers are installed on most upper floors of a recovery boiler, a common issue is
the inability to effectively reach and clean deposits in transitional regions between two
58
sootblowers. This issue is exacerbated by the focused nature (low spread) of highly supersonic
jets. To visualize the effectiveness of a jet in cleaning a tube length, figures 54 and 55 present
pressure contours of the tubes in the vertical direction (away from the nozzle mid-plane), for
three offsets. The “midway between tubes” offset was omitted as there is very little interaction
between the jet and the tubes. Note that the black lines to the left of the tubes represent one tube
diameter. The flow velocity on all surfaces is zero due to the no-slip wall boundary condition.
Recall that at subsonic conditions the total pressure is equivalent to the PIP.
In the generating bank, the zero and slightly offset jets essentially imprint their radial pressure
profile on the windward face of the leading tube. However, as the jet is offset to the top half of
the leading tube, it can be felt further down the tube length. In the economizer cases, the
presence of the leading fin reduces the average pressure value on the impinging surface but
extends the jet reach in the vertical direction as well as along the tube curvature. The
economizer case, where the nozzle is offset to the top half of the leading tube, is the most
effective in the vertical direction, imposing a reasonable pressure distribution, as far as two
economizer tube diameters down. Another feature of this case (indicated by the red streak) is the
high pressure values along the junction of the fin and tube geometry. This may imply that
deposits are less likely to accumulate at the tube-fin junction.
Effect of Economizer Fins 5.4
The presence of interconnecting fins, as well as different tube diameters, mark the key
differences between the generating bank and economizer tube bank geometries. However, at a
ratio of 1.3 (generating bank to economizer tube diameter), the latter does not significantly alter
the flow field. On the other hand, the leading fin dramatically changes the flow field, as the
supersonic jet is split by the flat plate (the leading fin) and impinges onto an immediately
adjacent cylinder (leading tube). Moreover, the leading fin of the economizer is nearly one
nozzle diameter closer to the nozzle exit than the leading tube of the generating bank.
In this section, PIP distributions on the impinging surfaces are presented and discussed. The
focus is on characterizing the effect of the leading fin on sootblowing performance. For all
subsequent discussions, GB (generating bank) and EC (economizer) will be used to distinguish
between the two sets of data.
59
5.4.1 PIP Distribution: Leading Tube
Figure 56. PIP distribution on the top quadrant of the leading tube EC tube.
60
Figure 57. PIP distributions on the top quadrant of the leading GB tube.
The angular PIP distributions on the top windward quadrant of the leading tube for all GB and
EC offsets are presented in figures 56 and 57. Note that these measurements are from the mid-
plane of the jet core. The location of maximum PIP for each offset is marked by thin dashed
lines. Table 1 summarizes notable observations regarding the above plots.
Table 1. A summary of observations from the PIP distributions on the leading tubes.
Offset GB - Max PIP EC - Max PIP Shock
Zero 842 kPa @ 18 degrees 300 kPa @ 64 degrees GB - Oblique @ 31 degrees
Slight 870 @ 31 degrees 392 kPa @ 41 degrees
GB - Oblique @ 41 degrees
EC - Oblique @ 42 degrees
Top half of first tube 1000 kPa @ 20 degrees 648 kPa @ 18 degrees GB - Oblique @ 87 degrees
61
The following are additional observations pertaining to the plots in figures 56 and 57:
Figure 57, for the GB, indicate that the “zero offset” and “slight offset” cases reach zero
PIP at 65 and 70 degrees respectively. These are points of flow separation. In all other
simulations, separation takes place at angular positions greater than 90 degrees. This can
be confirmed by referring to the visualizations in section 4.3.
The shocks specified in Table 1 correspond to a sudden increase in PIP for an oblique
shock and a sudden drop in PIP for an expansion wave.
The following is a list of remarks regarding the above observations:
As the nozzle is offset away from the initial head on position, the average value of the
angular PIP distribution increases. This occurs because a larger portion of the resultant
jet, split upon impingement, comes in contact with the top quadrant of the leading tube
windward face.
When the offset is “midway between tubes” for both tube geometries, the PIP is two
orders of magnitude smaller than at other offsets, and so sootblowing is inconsequential.
Oblique shock waves exist on the surface of the leading tube for all GB offsets. As the
nozzle is offset away from the “head on” position, the oblique shock tends to shift
towards the leeward side. An oblique shock is the response of a supersonic jet to the
flow turning inwards and into itself. Therefore, these shocks occur where the curvature
of the tube surface is “felt” by the supersonic jet. Oblique shocks are associated with a
sudden increase in pressure and may be considered as provide a small boost to the PIP
distribution.
On the EC tubes, the angular position of the maximum PIP is shifted towards to the
windward face as the nozzle is offset away from the “head on” position. This reflects the
fact that as the nozzle is offset, the deviation of the primary jet by the leading fin
decreases. On the other hand, the angular position of the maximum PIP on the GB
leading tube increases (towards the leeward side) between the “zero” and “slight” offset
cases, but then shifts back towards the windward side with the final offset. Looking back
at figure 52, it may be that the primary jet does not split when it impacts the top half of
62
the first tube, and so the increased jet radius capable exerts its maximum PIP value at a
more windward angular position.
Conversely, an expansion wave occurs in the “slight offset” case on the EC leading tube.
As seen in figure 52, upon impingement the leading fin creates a substantially deviated
yet strong resultant jet on its top surface. This causes the flow to turn away from itself, to
which the supersonic jet responds with an expansion wave. As expansion waves are
associated with a sudden pressure drop, this behavior may be detrimental to sootblowing
performance. Note that this behavior is limited to the small offset range in between the
“head on” and “top half of first tube” cases.
Overall, the GB leading tube experiences higher PIP forces than the EC leading tube,
because the leading fin reduces the maximum PIP exerted on the top quadrant of the
leading tube. The leading fin of the EC tube reduces the maximum PIP by 64%, 55% and
35% for the “zero”, “slight” and “top half of first tube” offset cases respectively. This
difference is expected as the leading fin of the EC splits the primary jet, so that a
weakened and deflected jet impinges onto the leading tube surface. However, based on
the PIP distributions at various offsets, the aforementioned primary jet breakup also
leads to a more uniform PIP distribution on the top windward quadrant of the EC leading
tube. For all offsets onto of the GB leading tube, PIP drops by about 800 kPa (peak-to-
trough) in the angular direction. The corresponding PIP variation on the EC leading tube
is no more than 100 kPa.
On the basis of the above discussion, there exists substantial evidence that the maximum PIP
value exerted on the leading tube in the presence of a leading fin is reduced, but that the
resulting angular PIP distribution tends to be more uniform.
63
5.4.2 PIP Distribution: Leading Fin
Figure 58. PIP distribution on the top surface of the EC leading fin.
Figure 58 presents the PIP distribution on the top surface of an EC leading fin, and shows that
the average PIP value on the leading fin for each offset case is lower than the corresponding
average PIP value on the leading tube surface. The PIP distribution is rather erratic and perhaps
indicative of shock wave formation near the fin surface. However, the PIP distribution for the
“top half of first tube” offset case displays an intriguing behaviour. There exists a sudden
fourfold increase in the PIP value at approximately the midway point of the fin length.
Referring back to the corresponding visualization for this offset, a possible explanation for this
behaviour is as follows. A unique characteristic of this offset case is that at some point in its
expansion, the jet shear layer boundary becomes coincident with the top surface of the leading
fin. As the jet expands radially in the downstream direction, the effective jet radius increases to
a value equivalent to the nozzle offset with respect to the fin top surface. Midway along the fin
64
length, the jet effectively shears the top surface, imprinting a strong PIP distribution. The sizable
and uniform nature of the PIP distribution on both the leading fin and the leading tube for the
“top half of first tube” offset case suggests that it is likely to maximize sootblowing efficiency.
5.4.3 Maximum PIP
Figure 59. Position of maximum PIP for the GB and EC “slight offset” cases.
Brittle breakup is one of two mechanisms by which sootblowers remove deposits. Brittle
breakup is a sudden fracture due to large local internal stresses within a deposit, stressed
induced by a sootblower jet. As a result, maximum PIP is a key parameter for gauging
sootblower effectiveness.
As an example, figure 59 shows the location of maximum PIP exerted on the impinging surface
of the “slight offset” case. For the EC, as the offset changes, the maximum PIP may occur at the
tip of the fin, or the top surface of the leading fin, or the leading tube surface. For the GB cases,
the maximum always occurs on the leading tube.
Table 2 shows the maximum PIP values in the GB and EC geometries, for all offset cases. The
location of maximum PIP is indicated in brackets below the values.
65
Table 2. Maximum PIP values associated with each simulation.
Boiler section Zero Offset Slight Offset Top Half of First Tube
Generating
Bank
842 kPa
(leading tube)
870 kPa
(leading tube)
1000 kPa
(leading tube)
Economizer
780 kPa
(fin tip)
787 kPa
(fin top surface)
648 kPa
(leading tube)
Notice that the maximum PIP values of the “zero” and “slight” EC offsets are comparable to
those of the corresponding GB simulations. The “top half of first tube” offset possesses the
lowest maximum PIP value (occurring on the leading tube).
5.4.4 Free jet vs Midway offset
Simulations of a sootblower jet propagating midway between the EC and GB tubes are
compared with free jet results. At this offset, there is no direct impingement onto a surface, and
so a free jet forms between the tubes. However, tubes adjacent to the supersonic jet alter its
behavior further downstream, leading to a more rapid decay of the centerline PIP. In the case of
the GB, the open gaps between arrays of tubes result in a fraction of the jet flow diverging and
forming a wall jet around the cylinders. This is due to entrainment of surrounding air into the jet
core, as well as to the Coanda effect, the natural tendency of a fluid to be attracted to a nearby
obstacle. Conversely, the fins of the EC form a planar confinement through which the free jet
flows. This confinement prevents the entrainment of surrounding air and reduces the decay of
PIP in the axial direction. Consequently, the jet centerline PIP distribution through the EC
decays at a slower rate than through the GB. This phenomena is documented by Pophali [3] in a
plot of PIP versus axial position in the EC and GB (figure 60). Figure 61 is a similar plot of the
present CFD results. Note that the dashed blue line indicates the position of the leading fin’s tip,
and the dotted red line indicates the front edge of the GB leading tube. Note that due to the
excessive computational cost of modelling the entire length of the experimental domain, the EC
and GB simulations were only 22 nozzle diameters long, which explains the strange jet behavior
near the domain boundary. Nonetheless, the general trend of the CFD results confirms that the
jet in the GB decays quicker.
66
Figure 60 Experimental centerline PIP distribution for a free jet, and jets midway between tubes of EC & GB [3].
Figure 61. CFD centerline PIP distribution for a free jet, and jets midway between EC and GB tubes [3].
67
Secondary Jet Characterization 5.5
Figure 62. A Mach contour plot showing the secondary jets for the "top half of first tube" case of EC (a) and GB (b).
Primary jet impingement onto an obstacle can create a weaker deflected “secondary jet”. At
certain nozzle offsets, the relatively close spacing of the GB and EC tube banks may lead to the
formation of a secondary jet that impinges onto an interior tube, which we refer to as the
“secondary tube”. Figure 62 visualizes impingement of the secondary jet onto a secondary tube
surface for the “top half of first tube” offset cases of the EC and GB.
Due to their reduced velocities and a smaller jet core radius, it is not clear whether secondary
jets actually contribute to effective sootblowing. Using the “top half of first tube” offset as a
case study, the plots in figures 63 and 64 compare the angular PIP distribution of a secondary jet
to that of the corresponding primary jet, for both the GB and EC. Note that the primary jet
results are on the top windward quadrant of the leading tube, whereas the secondary jet impacts
the bottom windward quadrant (theta defined in figure 62) of the secondary tube. The secondary
68
jet angular PIP distribution exhibits a relatively consistent profile, similar to that on the EC
leading tube. The maximum PIP values are 196 kPa (at 28 degrees) and 212 kPa (at 67 degrees)
for the EC and GB secondary tubes respectively. These values reflect a significant reduction in
the maximum PIP of the secondary jet when compared to the primary jet impinging onto the
leading tube. The reduction is 70% for the EC and 79% for the GB.
Figure 63. The angular PIP distributions on the leading and secondary tubes of EC.
69
Figure 64. The angular PIP distributions on the leading and secondary tubes of GB.
Model Limitations 5.6
In this chapter, possible reasons for specific discrepancies between the numerical and
experimental results were presented. The following list summarizes the limitations of the
ANSYS Fluent, which pertain to all simulations in this work:
The schlieren images were captured from a top view and are representative of a 3D flow
in all planes along the tube length. In the post processing of the CFD results, the
contours are from jet mid-plane. This may lead to qualitative discrepancies when
comparing the CFD contours to the schlieren images. Also, the PIP distributions
presented in this chapter are from the jet mid-plane, where we assume them to be at a
maximum.
70
As discussed in section 2.1.2, there is no CFD contour plot that corresponds directly to
the schlieren images. A density gradient contour would have to be resolved onto the
normal component of the knife edge, a direction vector that is unknown. This creates a
challenge in directly comparing Fluent CFD results with the corresponding schlieren
images. However, since visualizations are largely used for a qualitative assessment of
flow behaviour, a contour of the density gradient magnitude (first derivative) should
reproduce a flow field that corresponds to the schlieren visualization. This is why we
also presented Mach contours, that represent the change in density and velocity of the
jet.
To avoid excessive computational costs, the length of the computational domain for the
EC and GB simulations are of approximately half of the distance examined
experimentally. The experimental GB model consists of a 40 tube array of which only 6
are modelled. The geometry of the economizer experiment also consists of 6 tubes with
fins at both ends of each platen. In the CFD EC model, we included only the leading fin
and the first three interior tubes. This may explain discrepancies between the CFD and
experimental results near the distal boundary of the computational domain (around 15
nozzle diameters downstream). A similar limitation holds true for the free jet simulation,
although the effects of the boundary are observed much further from the nozzle exit
(around 35 nozzle diameters downstream).
The dimensions of the experimental geometry are based on measurements of limited
accuracy. This is not consequential for the larger dimensions, such as tube diameters and
the economizer fin length. However, the nozzle dimensions, such as the throat and
nozzle exit diameters, may be less accurate.
In the Pophali experiments, there are energy losses within the converging-diverging
nozzle, and the nozzle supply pressure fluctuates [3]. The CFD model cannot account for
changes in jet behaviour caused by the aforementioned phenomena.
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Chapter 6 Closure
Summary 6.1
An ANSYS Fluent model was created to predict the flow behaviour of a supersonic sootblower
jet and its interaction with complex tube geometries characteristic of a recovery boiler.
Turbulence model corrections, developed over a number of years at the University of Toronto,
were implemented into the Fluent realizable k-ε model as two UDFs. Using the Fluent model,
second-order accurate 3D steady-state simulations were run of a supersonic (Mach 2.5)
underexpanded sootblower jet propagating freely and impinging onto lab-scale economizer and
generating bank geometries. The generating bank and economizer simulations were run at four
nozzle-to-tube centerline offsets ranging from head on impact to jet propagation midway
between tubes.
The solution methodology involved obtaining a preliminary solution, followed by a grid
adaption of regions of high pressure gradients to improve the resolution of shock structures in
the flow. A summary of the modelling challenges, geometry definition and mesh generation
processes, and the Fluent solver controls was presented to help guide future sootblower jet flow
research using ANSYS Fluent. Comparisons of the CFD free jet centerline PIP distribution and
spreading rate to experimental data were used to validate the model. There is a need for further
validation of the current model using more accurate experimental measurements. Nonetheless,
the model was shown to produce an acceptable level of stability and accuracy in capturing
prominent flow features. The PIP distributions exerted by the sootblower jet on leading
impinging surfaces were presented and analyzed. The results and analysis clearly demonstrate
the efficacy of this accessible ANSYS Fluent model for further studies of sootblower jet
interactions with complex tube geometries.
72
Conclusions 6.2
Sootblower jet interaction with complex tube geometries is strongly affected by the large PIP
fluctuations that occur due to the shock structures that are present in an off-design jet. As a
result, it is difficult to draw conclusions on sootblower jet interaction produced by offsetting the
nozzle with respect to the tube centerline.
Mach and density gradient magnitude contours were used to compare the CFD results to the
experimental schlieren visualizations of Pophali [3], and were shown to be in good qualitative
agreement.
PIP distributions on tube surfaces were presented to assess the effectiveness of a sootblower jet
impinging onto tubes with (economizer) and without (generating bank) fins. The results suggest
that the presence of fins in the economizer reduces the maximum PIP generated by the
sootblower jet on the leading tube but creates a more uniform PIP distribution on its surface.
Pressure contours of tube surfaces in the vertical direction show a sharp decline (one order of
magnitude or more) of PIP within approximately one tube diameter from the nozzle mid-plane.
As previously shown in the experimental work of Pophali, a quantitative comparison of a free
jet propagating midway between the economizer and generating bank tubes suggests that the
fins preserve the jet strength downstream of the nozzle. Finally, PIP distributions exerted on an
interior tube by a secondary jet were presented. The results show that secondary jets are often
much weaker, by an order of magnitude or so, than the primary jet.
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Implications on Sootblowing 6.3
The results presented in this thesis clearly highlight the limitations of sootblowing into the
closely-spaced geometries of the economizer and generating bank. A sootblower jet is fairly
focused and so a majority of the substantial PIP force, that is capable of deposit removal, is
exerted on small areas of the leading tube surfaces. The secondary jet structures that reach the
interior tubes are often weaker and cannot be expected to effectively remove deposits. The
leading edges of the economizer fins tend to alleviate this problem by deflecting the primary jet
to create a slightly weaker yet more uniform interaction. Additionally, the fins enclose the space
in between economizer platens resulting in the preservation of secondary jet structures that
could contribute to deposit erosion.
Recommendations for Future Work 6.4
CFD is a powerful tool for predicting the flow behaviour of sootblowers, as well as many
similar complex supersonic impingement applications. With further research and development
on CFD algorithms, more accurate and stable means of conducting CFD studies will become
available to the wider engineering community. The ANSYS Fluent model presented here must
be improved to better capture the number of shock structures within the sootblower jet core.
More computationally expensive methods such as LES and DNS would provide more accurate
flow predictions.
In recent years, sootblower suppliers have begun to experiment with inclined sootblower
nozzles that direct steam jets at an angle to heat transfer surfaces. The computational model of
the present work provides a means to investigate the feasibility of installing inclined
sootblowers to improve the removal of fouling in the more complex generating bank and
economizer tube geometries.
Finally, a more comprehensive study would be to improve and couple the current CFD model
with a solid mechanics Finite Element Analysis (FEA) that models deposit breakup. This model
would provide a powerful means of investigating the underlying principles that determine
sootblower effectiveness in removing deposits.
74
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APPENDIX A: Turbulence Correction UDF Codes
79