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30th April 2010
Friday, April 30, 2010
30th April 2010
Non-premixed 鍖ame extinction
phenomena: analytical and
numerical investigations
Friday, April 30, 2010
30th April 2010
Non-premixed 鍖ame extinction
phenomena: analytical and
numerical investigations
Praveen Narayanan
Department of Fire Protection Engineering
University of Maryland, College Park, MD-20740
Sponsors: DOE Of鍖ce of Science (INCITE - Innovative and Novel Computational Impact on Theory and
Experiment - Program); and National Science Foundation (CBET)
Friday, April 30, 2010
Scholastic background
Friday, April 30, 2010
Scholastic background
 PhD: Mechanical/Fire Protection Engineering
 University of Maryland, College Park (2005-present)
 Thesis topic: Direct Numerical Simulations of non-premixed 鍖ame extinction phenomena
 Advisers/collaborators: Dr. Arnaud Trouv辿 (UMD), Dr. Howard Baum (UMD), Dr. Hong
Im (UMich), Paul Arias (UMich)
Friday, April 30, 2010
Scholastic background
 PhD: Mechanical/Fire Protection Engineering
 University of Maryland, College Park (2005-present)
 Thesis topic: Direct Numerical Simulations of non-premixed 鍖ame extinction phenomena
 Advisers/collaborators: Dr. Arnaud Trouv辿 (UMD), Dr. Howard Baum (UMD), Dr. Hong
Im (UMich), Paul Arias (UMich)
 Batchelor and Master of Technology: Chemical Engineering
 Indian Institute of Technology Madras, Chennai, India (2000-2005)
 Masters thesis: Implementation of high order compact schemes for incompressible 鍖ows
Friday, April 30, 2010
Research overview
 Flame extinction` phenomena in non-premixed 鍖ames
 Background and motivation
 Phenomenological description
 Premise, hypothesis
 Problems investigated
 Solution approaches and results
 Future HPC research in 鍖re/combustion phenomena
Friday, April 30, 2010
Background and motivation
Friday, April 30, 2010
 What is a diffusion 鍖ame?
 Diffusion 鍖ames
(or non-premixed 鍖ames): fuel and
oxidizer initially unmixed
 Examples: 鍖res, diesel engines
Fuel
Flame
Air
Diffusion 鍖ames
Friday, April 30, 2010
Diffusion 鍖ame extinction
 Combustion science
 Impacts performance of non-premixed combustion
systems
 Determines turbulent 鍖ame structure and levels of
pollutant emission (NOx, soot, CO)
 Engine applications: extinction caused by high
turbulence intensities in diesel engines
(momentum driven, large Reynolds number 鍖ows
Diesel engine
Friday, April 30, 2010
Diffusion 鍖ame extinction
 Fire applications
 Extinction caused by air vitiation
in underventilated compartment
鍖res
 Forest 鍖res, oil spills
 Sprinkler systems
 Extinction caused by inert gaseous
agents or water spray suppression
systems
pool fire
sprinklers
Friday, April 30, 2010
Diffusion 鍖ame extinction
smoke
Air
Fuel
Air Extinction
Flame surface
(Sunderland et al)
 What is 鍖ame extinction?
 A hole` in 鍖ame: mixing without chemical reaction
 Examples: suppressing (or extinguishing) 鍖res from water spray,
blowing out candle
Friday, April 30, 2010
Phenomenology
Friday, April 30, 2010
Diffusion 鍖ame extinction
Fuel side Oxidizer side
Flame
Fuel side Oxidizer side
Flame
Fuel side Oxidizer side
Flame
Friday, April 30, 2010
Diffusion 鍖ame extinction
 Types of 鍖ame extinction phenomena
Fuel side Oxidizer side
Flame
Fuel side Oxidizer side
Flame
Fuel side Oxidizer side
Flame
Friday, April 30, 2010
Diffusion 鍖ame extinction
 Types of 鍖ame extinction phenomena
 Aerodynamic quenching: 鍖ame weakening due to
鍖ow-induced perturbations (insuf鍖cient
residence time-blowing out a candle)
Fuel side Oxidizer side
Flame
Fuel side Oxidizer side
Flame
Fuel side Oxidizer side
Flame
Friday, April 30, 2010
Diffusion 鍖ame extinction
 Types of 鍖ame extinction phenomena
 Aerodynamic quenching: 鍖ame weakening due to
鍖ow-induced perturbations (insuf鍖cient
residence time-blowing out a candle)
 Thermal quenching: 鍖ame weakening due to heat
losses (wall cooling, thermal radiation,
evaporative cooling in suppression systems)
Fuel side Oxidizer side
Flame
Fuel side Oxidizer side
Flame
Fuel side Oxidizer side
Flame
Friday, April 30, 2010
Diffusion 鍖ame extinction
 Types of 鍖ame extinction phenomena
 Aerodynamic quenching: 鍖ame weakening due to
鍖ow-induced perturbations (insuf鍖cient
residence time-blowing out a candle)
 Thermal quenching: 鍖ame weakening due to heat
losses (wall cooling, thermal radiation,
evaporative cooling in suppression systems)
 Quenching by dilution: insuf鍖cient fuel/oxidizer
concentration (air vitiation in under-ventilated
鍖res)
Fuel side Oxidizer side
Flame
Fuel side Oxidizer side
Flame
Fuel side Oxidizer side
Flame
Friday, April 30, 2010
Types of 鍖ame extinction
phenomena
 Aerodynamic quenching
 Blowout at large stretch rates (also known
as kinetic extinction)
 Extinction criterion
 Sources
 Linan, 1974, Acta Astronautica
 Williams, 1975, Combustion theory
 Carrier, Fendell & Marble, 1975, SIAM
Journal of Applied Mathematics
Friday, April 30, 2010
Types of 鍖ame extinction
phenomena
 Thermal quenching:
 Radiative extinction (large radiation heat losses)
 Extinction due to evaporative cooling
 Extinction criterion
 Sources
 Sohrab, Li単an & Williams (1982) Combustion Science and Technology
 Chao, Law & Tien (1992), Combustion and Flame
 Tien (1986), Combustion and 鍖ame
Friday, April 30, 2010
The premise: uni鍖ed extinction
criterion
Friday, April 30, 2010
Questions
Friday, April 30, 2010
Questions
 Whether extinction can be described in phenomenological terms with a
consistent mathematical model for cases with
Friday, April 30, 2010
Questions
 Whether extinction can be described in phenomenological terms with a
consistent mathematical model for cases with
 Stretch (due to turbulence)
Friday, April 30, 2010
Questions
 Whether extinction can be described in phenomenological terms with a
consistent mathematical model for cases with
 Stretch (due to turbulence)
 Radiative heat losses (soot, CO2, H2O, other gases)
Friday, April 30, 2010
Questions
 Whether extinction can be described in phenomenological terms with a
consistent mathematical model for cases with
 Stretch (due to turbulence)
 Radiative heat losses (soot, CO2, H2O, other gases)
 Evaporative cooling (suppression from water droplets)
Friday, April 30, 2010
Questions
 Whether extinction can be described in phenomenological terms with a
consistent mathematical model for cases with
 Stretch (due to turbulence)
 Radiative heat losses (soot, CO2, H2O, other gases)
 Evaporative cooling (suppression from water droplets)
 A combination of the above
Friday, April 30, 2010
Questions
 Whether extinction can be described in phenomenological terms with a
consistent mathematical model for cases with
 Stretch (due to turbulence)
 Radiative heat losses (soot, CO2, H2O, other gases)
 Evaporative cooling (suppression from water droplets)
 A combination of the above
 What kind of diagnostics may be developed to qualify (or quantify)
extinction?
Friday, April 30, 2010
The extinction criterion
 The Damk旦hler number
 Code supplies both quantities
 Need to test if hypothesis holds
Friday, April 30, 2010
The extinction criterion
 The Damk旦hler number
 Code supplies both quantities
 Need to test if hypothesis holds
Mixing
Friday, April 30, 2010
The extinction criterion
 The Damk旦hler number
 Code supplies both quantities
 Need to test if hypothesis holds
Mixing
Chemistry
Friday, April 30, 2010
What is new about this work?
Friday, April 30, 2010
What is new about this work?
 Extinction studies with stretch -widely studied (Linan-1974)
Friday, April 30, 2010
What is new about this work?
 Extinction studies with stretch -widely studied (Linan-1974)
 Extinction studies with heat losses (primarily, radiation)
Friday, April 30, 2010
What is new about this work?
 Extinction studies with stretch -widely studied (Linan-1974)
 Extinction studies with heat losses (primarily, radiation)
 Some theoretical developments by Tien, Law, Chao, Liu
Friday, April 30, 2010
What is new about this work?
 Extinction studies with stretch -widely studied (Linan-1974)
 Extinction studies with heat losses (primarily, radiation)
 Some theoretical developments by Tien, Law, Chao, Liu
 Current study
Friday, April 30, 2010
What is new about this work?
 Extinction studies with stretch -widely studied (Linan-1974)
 Extinction studies with heat losses (primarily, radiation)
 Some theoretical developments by Tien, Law, Chao, Liu
 Current study
 Rigorous treatment of non-adiabatic environments (soot, radiation, water spray)
Friday, April 30, 2010
What is new about this work?
 Extinction studies with stretch -widely studied (Linan-1974)
 Extinction studies with heat losses (primarily, radiation)
 Some theoretical developments by Tien, Law, Chao, Liu
 Current study
 Rigorous treatment of non-adiabatic environments (soot, radiation, water spray)
 Theoretical developments validated with high quality numerical datasets
Friday, April 30, 2010
What is new about this work?
 Extinction studies with stretch -widely studied (Linan-1974)
 Extinction studies with heat losses (primarily, radiation)
 Some theoretical developments by Tien, Law, Chao, Liu
 Current study
 Rigorous treatment of non-adiabatic environments (soot, radiation, water spray)
 Theoretical developments validated with high quality numerical datasets
 Questions asked about soot leakage and connection with radiative extinction
Friday, April 30, 2010
What is new about this work?
 Extinction studies with stretch -widely studied (Linan-1974)
 Extinction studies with heat losses (primarily, radiation)
 Some theoretical developments by Tien, Law, Chao, Liu
 Current study
 Rigorous treatment of non-adiabatic environments (soot, radiation, water spray)
 Theoretical developments validated with high quality numerical datasets
 Questions asked about soot leakage and connection with radiative extinction
 Treatment of radiation absorption (with possible extension to optically thick media)
Friday, April 30, 2010
What is new about this work?
Friday, April 30, 2010
Pulications
 Radiation driven 鍖ame weakening effects in sooting turbulent 鍖ames (2008),
Narayanan & Trouv辿, Proceedings of the combustion institute
 Effects of soot addition on extinction limits of luminous laminar counter鍖ow
鍖ames, Narayanan, Baum & Trouv辿 (Accepted, Combustion symposium, 2010)
 Extinction of Nonpremixed Ethylene-Air 鍖ames by water spray, Arias, Im,
Narayanan & Trouv辿 (Accepted, Combustion symposium, 2010)
 Mixture fraction and state relationships in diffusion 鍖ames interacting with an
evaporating water spray, Narayanan, Trouv辿, Arias & Im (in preparation, presented
at the US Combustion meeting, Ann Arbor, 2009)
 Constructing extinction maps for diffusion 鍖ames predicated by radiation emission
in sooting turbulent 鍖ames, Narayanan, Lecoustre & Trouv辿 (in preparation,
presented at the International Seminar on Fire and Explosions Hazards, Leeds, 2010)
Friday, April 30, 2010
Tools/approach
Friday, April 30, 2010
Tools/approach
 Direct numerical simulations to generate datasets
 Massively parallel Combustion solver S3D
 NERSC machines (Franklin,Hopper)
Friday, April 30, 2010
Tools/approach
 Direct numerical simulations to generate datasets
 Massively parallel Combustion solver S3D
 NERSC machines (Franklin,Hopper)
 Mathematical modeling
 Canonical problems solved using singular perturbation techniques
Friday, April 30, 2010
Tools/approach
 Direct numerical simulations to generate datasets
 Massively parallel Combustion solver S3D
 NERSC machines (Franklin,Hopper)
 Mathematical modeling
 Canonical problems solved using singular perturbation techniques
 Model validation and analysis
Friday, April 30, 2010
Numerical approach
Friday, April 30, 2010
Numerical approach
 Use Direct numerical simulations (DNS)
Friday, April 30, 2010
Numerical approach
 Use Direct numerical simulations (DNS)
 Leverage DOE sponsored SciDac collaboration solver S3D
 Collaborators: Sandia Ntl. Laboratories (J. J. Chen), University of Michigan (H. G. Im)
Friday, April 30, 2010
Numerical approach
 Use Direct numerical simulations (DNS)
 Leverage DOE sponsored SciDac collaboration solver S3D
 Collaborators: Sandia Ntl. Laboratories (J. J. Chen), University of Michigan (H. G. Im)
 DNS solver S3D
 Navier-stokes solver; fully compressible 鍖ow formulation
 Higher-order methods: 8th order 鍖nite difference; 4th order Runge Kutta time
 Characteristic based boundary conditions (NSCBC)
 Structured cartesian grids
 Parallel, MPI based (excellent scalability)
 Flame modeling: detailed fuel-air chemistry (CHEMKIN compatible); simpli鍖ed soot formation model;
thermal radiation model (Discrete Ordinate/Discrete Transfer Method); Lagrangian particle model to
describe dilute liquid sprays
Friday, April 30, 2010
Flame modeling
Friday, April 30, 2010
Single step chemistry
 Ethylene-air chemistry model (Westbrook & Dryer, 1981)
 Used for simpli鍖ed extinction model (in asymptotic analysis and
numerical validation with DNS)

F = BRR (
YF
MF
)僚 F
(
YO2
MF
)僚O
exp(
Ta
T
)
Friday, April 30, 2010
Detailed Chemistry
 Used for more detailed calculations with water spray
 Reduced chemical kinetic mechanism (Lu & Law, 2009, Progress in
Energy and Combustion Science)
 Based on detailed chemistry mechanism for ethylene-air combustion (70 species,
463 elementary reactions, Wang et al., 2000, Proceedings of the Combustion Institute)
 Reduced chemistry mechanism using: the method of directed relations graphs
(DRG): sensitivity analysis; quasi steady-state assumption for fast reacting
radicals
 19 species, 15 semi-global reactions
Friday, April 30, 2010
Soot formation model
 Phenomenological, two equation model (Moss et al., Lindstedt et al.)
 Soot formation process included into phenomenology
 nucleation, surface growth, coagulation, oxidation
Friday, April 30, 2010
Lagrangian spray model
 Adapted from Wang
and Rutland (2007),
Combustion and
Flame
 Spherical,
monodisperse droplets
 Particle in cell
 Dilute liquid phase
assumption
 Lagrangian-Eulerian
coupling
Position
Mass
Momentum
Energy
Lagrangian droplet
equations
Droplet source terms in
Eulerian gas equations
Mass
Momentum
Energy
Friday, April 30, 2010
Thermal radiation model
 Non-scattering, gray gas assumption; Discrete Transfer Method
(Lockwood & Shah, 1981)
 Solve radiative transfer equation
 Mean absorption coef鍖cient (ap,i)
Friday, April 30, 2010
Problems investigated
Friday, April 30, 2010
Problems investigated
 Turbulent sooting/radiating wall 鍖ames
Friday, April 30, 2010
Problems investigated
 Turbulent sooting/radiating wall 鍖ames
 Radiative weakening and extinction 鍖rst come to light in turbulent simulation
Friday, April 30, 2010
Problems investigated
 Turbulent sooting/radiating wall 鍖ames
 Radiative weakening and extinction 鍖rst come to light in turbulent simulation
 Laminar counter鍖ow sooting/radiating 鍖ames
Friday, April 30, 2010
Problems investigated
 Turbulent sooting/radiating wall 鍖ames
 Radiative weakening and extinction 鍖rst come to light in turbulent simulation
 Laminar counter鍖ow sooting/radiating 鍖ames
 Attempts in understanding radiative extinction through asymptotic analysis and
numerical simulations
Friday, April 30, 2010
Problems investigated
 Turbulent sooting/radiating wall 鍖ames
 Radiative weakening and extinction 鍖rst come to light in turbulent simulation
 Laminar counter鍖ow sooting/radiating 鍖ames
 Attempts in understanding radiative extinction through asymptotic analysis and
numerical simulations
 Turbulent counter鍖ow 鍖ames weakened by water spray
Friday, April 30, 2010
Problems investigated
 Turbulent sooting/radiating wall 鍖ames
 Radiative weakening and extinction 鍖rst come to light in turbulent simulation
 Laminar counter鍖ow sooting/radiating 鍖ames
 Attempts in understanding radiative extinction through asymptotic analysis and
numerical simulations
 Turbulent counter鍖ow 鍖ames weakened by water spray
 More complex problem with detailed chemistry, explored via numerical
simulations and application of asymptotic model developed
Friday, April 30, 2010
Turbulent sooting 鍖ames
 Simpli鍖ed turbulent con鍖guration
 Two dimensional (8 x 4 cm2); grid size: 1216 x 375 (uniform x stretched); prescribed in鍖ow
turbulent 鍖uctuations (u = 1-2.5 m/s, Lt = 1.7 mm)
Air
Fuel
Solid Wall
2.5-5 m/s y  50 袖m
x  66 袖m
Friday, April 30, 2010
Turbulent sooting 鍖ames
 Observations
 radiative cooling region is not
thin
 soot region is not thin
 weak 鍖ame events correlated
with soot mass leakage across
the 鍖ame
radiation cooling rate
soot mass fraction extinction
extinction
 Analysis of 鍖ame structure (case, Tw=300 K, with soot/radiation,
Csoot= 7000 m-1 K-1)
Friday, April 30, 2010
Turbulent sooting 鍖ames
 Analysis of 鍖ame structure (case, Tw=300 K, with soot/radiation,
Csoot= 7000 m-1 K-1)
weak spots
weak flame events occur at low values of
flame stretch (slow mixing limit)
Friday, April 30, 2010
Radiative extinction under
external soot loading
Friday, April 30, 2010
Overview
 Explore connection between 鍖ame extinction and soot leakage
 Relevance in radiating/sooting environments
 Pool鍖res
 Connection with smoking candle 鍖ames
Cold Soot
Hot Soot
Friday, April 30, 2010
Problem formulation
 Asymptotic 鍖ame structure with soot loading
 External soot loading to simulate multi-dimensional 鍖ame structure in a one-
dimensional framework
 Soot loading from air side
Fuel
Air Air
Flame
Soot region
Flame
Sootinjection
Friday, April 30, 2010
Problem formulation
 Approach: setup counter鍖ow 鍖ame with radiative heat loss
 Analytical setup (transform to one-dimensional scalar 鍖elds)
 Numerical setup (DNS) for validation (two dimensional counter鍖ow 鍖ame)
 Outputs: Flame structure (鍖ame variables such as temperature,
mixing rate, radiation cooling rate)
 Effect of soot loading on extinction properties
 how are the limits changed with radiation heat loss?
Friday, April 30, 2010
Activation Energy Asymptotics
 Convert governing equations into one-dimensional coordinates using
Howarth transformation for variable density
 Constant speci鍖c heat, single step Arrhenius Chemistry
 Conventional solution using singular perturbation: split domain into
 Outer radiating zone-to obtain radiation corrected outer temperatures
 Full treatment-both emission and absorption handled (radiation transport equation solved)
 Inner reacting zone -complete 鍖ame structure and extinction conditions
 Solve using two point BVP solver
 Patch outer and inner solutions to obtain complete 鍖ame structure
 Solve for soot 鍖eld using completed 鍖ame structure with BVP solver (but do not have
bene鍖t of asymptotic expansions here!)
Outer
Outer
Inner
Friday, April 30, 2010
Governing equations
Only contributes near thin reaction zone (inner region)
Zero far from reaction zone (outer region)
Fuel
(Ethylene)
Outer layer
(radiatively active)
Thin 鍖ame (inner layer)
Oxidizer
(air)
Friday, April 30, 2010
Outer solutions
 Solve for leading order solutions far from 鍖ame
Algorithm
Solve on either side of 鍖ame using
Greens functions
Get temperature at 鍖ame location
Solve Inner equation
Obtain complete solution
Howarth
Transform
Friday, April 30, 2010
Inner solutions
 Solve for inner solutions by zooming in at 鍖ame zone

Transform
Outer
Outer
Inner
Friday, April 30, 2010
Inner solutions
 Solve for inner solutions by zooming in at 鍖ame zone

Transform
Outer
Outer
Inner
Reduced Damk旦hler number
Friday, April 30, 2010
What is the effect of radiation in
all this?
 Radiation free 鍖ame: (outer)
temperature is the adiabatic 鍖ame
temperature
 With radiation: (outer) temperature is
lowered!
 Effects of radiation felt when
 Large amounts of soot
 Small strain
 Radiation corrected 鍖ame temperature
feeds into inner equation
Radiation correction to give new
Burke-Schumann temperature
Text
Solve RTE
Friday, April 30, 2010
What is the effect of radiation in
all this?
 Radiation free 鍖ame: (outer)
temperature is the adiabatic 鍖ame
temperature
 With radiation: (outer) temperature is
lowered!
 Effects of radiation felt when
 Large amounts of soot
 Small strain
 Radiation corrected 鍖ame temperature
feeds into inner equation
Radiation correction to give new
Burke-Schumann temperature
Radiation
Text
Solve RTE
Friday, April 30, 2010
What is the effect of radiation in
all this?
 Radiation free 鍖ame: (outer)
temperature is the adiabatic 鍖ame
temperature
 With radiation: (outer) temperature is
lowered!
 Effects of radiation felt when
 Large amounts of soot
 Small strain
 Radiation corrected 鍖ame temperature
feeds into inner equation
Radiation correction to give new
Burke-Schumann temperature
Radiation
Strain
Text
Solve RTE
Friday, April 30, 2010
On radiative emission and
absorption
 Emission: local function of temperature
 Absorption: non-local convolution
integral
 Depends on optical thickness of surroundings
 Can develop asymptotic measures for
radiating regimes (thick (Szoke, LLNL),
thin (the optically thin assumption),
intermediate)
 Possibilities of regime based approximations
(thick and thin somewhat amenable to
analytical solutions (!?), intermediate needs
computation)
Radiation
source term
Optically thin
Optically thick
Friday, April 30, 2010
Laminar counter鍖ow 鍖ames
 Reference counter鍖ow
鍖ame
 Flamelet perspective: study
鍖ame structure as a function
of 鍖ame stretch ranging
from ultra-low to ultra-high
values
 No soot injection
Flame
Friday, April 30, 2010
Laminar counter鍖ow 鍖ames
 Reference counter鍖ow
鍖ame
 Flamelet perspective: study
鍖ame structure as a function
of 鍖ame stretch ranging
from ultra-low to ultra-high
values
 No soot injection
kinetic
extinction
limit
radiation
extinction
limit
DNS
AEA
Friday, April 30, 2010
Laminar counter鍖ow 鍖ames
 Reference counter鍖ow 鍖ame
 Flamelet perspective: study 鍖ame structure as a function of 鍖ame
stretch ranging from ultra-low to ultra-high values
Friday, April 30, 2010
Laminar counter鍖ow 鍖ames
 Extinction values correspond to critical value of Damk旦hler number
Friday, April 30, 2010
Laminar counter鍖ow 鍖ames
 Extinction values correspond to critical value of Damk旦hler number
adiabatic
soot-free
with
soot
with external
soot loading
approximate
critical value
Extinction
Flammable
Friday, April 30, 2010
Flammability maps
 Extinction limits
 Flammability maps with mixing rate and 鍖ame temperature as coordinates
Extinction
Flammable
Engine
extinction event
Fire
extinction event
Friday, April 30, 2010
Analysis of turbulent 鍖ame data
 Extinction limits
 Flammability maps with mixing rate and 鍖ame temperature as coordinates
Extinction
representative conditions of
flame weakest spots in DNS
Apparently, the 鍖ames weakest
spots are not actually quenched
Soot leakage events may have more
to do with cessation of soot
oxidation chemistry than radiative
extinction
soot mass fraction extinction
Friday, April 30, 2010
Conclusions on sooting 鍖ames
Friday, April 30, 2010
Conclusions on sooting 鍖ames

Activation energy asymptotics and DNS have been used to make fundamental
observations on non-adiabatic turbulent sooting diffusion 鍖ames
Friday, April 30, 2010
Conclusions on sooting 鍖ames

Activation energy asymptotics and DNS have been used to make fundamental
observations on non-adiabatic turbulent sooting diffusion 鍖ames

Two extinction limits are encountered
 Kinetic extinction (at high stretch)
 Radiative extinction (at low stretch)
Friday, April 30, 2010
Conclusions on sooting 鍖ames

Activation energy asymptotics and DNS have been used to make fundamental
observations on non-adiabatic turbulent sooting diffusion 鍖ames

Two extinction limits are encountered
 Kinetic extinction (at high stretch)
 Radiative extinction (at low stretch)

Extinction occurs at a single critical value of the reduced Damk旦hler number
equalling unity
 Can construct maps to gauge extinction propensity of 鍖ames
Friday, April 30, 2010
Conclusions on sooting 鍖ames

Activation energy asymptotics and DNS have been used to make fundamental
observations on non-adiabatic turbulent sooting diffusion 鍖ames

Two extinction limits are encountered
 Kinetic extinction (at high stretch)
 Radiative extinction (at low stretch)

Extinction occurs at a single critical value of the reduced Damk旦hler number
equalling unity
 Can construct maps to gauge extinction propensity of 鍖ames

Turbulent 鍖ame data indicate that soot leakage events are not necessarily radiative
extinction events. Further investigation of soot oxidation chemistry is warranted
Friday, April 30, 2010
DNS of turbulent spray 鍖ames
Friday, April 30, 2010
Turbulent spray 鍖ames
 Counter鍖ow laminar/turbulent
diffusion 鍖ames with water spray
injection
 Two dimensional, domain size (1 cm x 2
cm), 480 k grid points (400 procs on
Franklin)
 Detailed chemistry
 Strain rate of 440 s-1 (extinction: 1300 s-1)
 Turbulence injection at inlet (u/U=0.85,
L11=0.5 cm)
1 cm
x = 16 袖m
y= 25 袖m
 Droplet diameter: 10 亮m, mist
regime
 Injection at local gas velocity
Friday, April 30, 2010
Unexplored areas
 Extinction and soot leakage
 If soot leakage precedes radiative extinction, can one come up with a description based
on soot chemistry
 Damk旦hler number criterion for cessation of soot oxidation chemistry
 Could have rami鍖cations in smoking 鍖res
 Strongly radiating, but not quenched
 Development of approximations in thick media (and thin) and its application
to radiating solvers
 Envisage cost reduction if only intermediate regions need to be computed
 How do we incorporate chemistry effects in complex 鍖ames?
Friday, April 30, 2010
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LBNLppt

  • 1. 30th April 2010 Friday, April 30, 2010
  • 2. 30th April 2010 Non-premixed 鍖ame extinction phenomena: analytical and numerical investigations Friday, April 30, 2010
  • 3. 30th April 2010 Non-premixed 鍖ame extinction phenomena: analytical and numerical investigations Praveen Narayanan Department of Fire Protection Engineering University of Maryland, College Park, MD-20740 Sponsors: DOE Of鍖ce of Science (INCITE - Innovative and Novel Computational Impact on Theory and Experiment - Program); and National Science Foundation (CBET) Friday, April 30, 2010
  • 5. Scholastic background PhD: Mechanical/Fire Protection Engineering University of Maryland, College Park (2005-present) Thesis topic: Direct Numerical Simulations of non-premixed 鍖ame extinction phenomena Advisers/collaborators: Dr. Arnaud Trouv辿 (UMD), Dr. Howard Baum (UMD), Dr. Hong Im (UMich), Paul Arias (UMich) Friday, April 30, 2010
  • 6. Scholastic background PhD: Mechanical/Fire Protection Engineering University of Maryland, College Park (2005-present) Thesis topic: Direct Numerical Simulations of non-premixed 鍖ame extinction phenomena Advisers/collaborators: Dr. Arnaud Trouv辿 (UMD), Dr. Howard Baum (UMD), Dr. Hong Im (UMich), Paul Arias (UMich) Batchelor and Master of Technology: Chemical Engineering Indian Institute of Technology Madras, Chennai, India (2000-2005) Masters thesis: Implementation of high order compact schemes for incompressible 鍖ows Friday, April 30, 2010
  • 7. Research overview Flame extinction` phenomena in non-premixed 鍖ames Background and motivation Phenomenological description Premise, hypothesis Problems investigated Solution approaches and results Future HPC research in 鍖re/combustion phenomena Friday, April 30, 2010
  • 9. What is a diffusion 鍖ame? Diffusion 鍖ames (or non-premixed 鍖ames): fuel and oxidizer initially unmixed Examples: 鍖res, diesel engines Fuel Flame Air Diffusion 鍖ames Friday, April 30, 2010
  • 10. Diffusion 鍖ame extinction Combustion science Impacts performance of non-premixed combustion systems Determines turbulent 鍖ame structure and levels of pollutant emission (NOx, soot, CO) Engine applications: extinction caused by high turbulence intensities in diesel engines (momentum driven, large Reynolds number 鍖ows Diesel engine Friday, April 30, 2010
  • 11. Diffusion 鍖ame extinction Fire applications Extinction caused by air vitiation in underventilated compartment 鍖res Forest 鍖res, oil spills Sprinkler systems Extinction caused by inert gaseous agents or water spray suppression systems pool fire sprinklers Friday, April 30, 2010
  • 12. Diffusion 鍖ame extinction smoke Air Fuel Air Extinction Flame surface (Sunderland et al) What is 鍖ame extinction? A hole` in 鍖ame: mixing without chemical reaction Examples: suppressing (or extinguishing) 鍖res from water spray, blowing out candle Friday, April 30, 2010
  • 14. Diffusion 鍖ame extinction Fuel side Oxidizer side Flame Fuel side Oxidizer side Flame Fuel side Oxidizer side Flame Friday, April 30, 2010
  • 15. Diffusion 鍖ame extinction Types of 鍖ame extinction phenomena Fuel side Oxidizer side Flame Fuel side Oxidizer side Flame Fuel side Oxidizer side Flame Friday, April 30, 2010
  • 16. Diffusion 鍖ame extinction Types of 鍖ame extinction phenomena Aerodynamic quenching: 鍖ame weakening due to 鍖ow-induced perturbations (insuf鍖cient residence time-blowing out a candle) Fuel side Oxidizer side Flame Fuel side Oxidizer side Flame Fuel side Oxidizer side Flame Friday, April 30, 2010
  • 17. Diffusion 鍖ame extinction Types of 鍖ame extinction phenomena Aerodynamic quenching: 鍖ame weakening due to 鍖ow-induced perturbations (insuf鍖cient residence time-blowing out a candle) Thermal quenching: 鍖ame weakening due to heat losses (wall cooling, thermal radiation, evaporative cooling in suppression systems) Fuel side Oxidizer side Flame Fuel side Oxidizer side Flame Fuel side Oxidizer side Flame Friday, April 30, 2010
  • 18. Diffusion 鍖ame extinction Types of 鍖ame extinction phenomena Aerodynamic quenching: 鍖ame weakening due to 鍖ow-induced perturbations (insuf鍖cient residence time-blowing out a candle) Thermal quenching: 鍖ame weakening due to heat losses (wall cooling, thermal radiation, evaporative cooling in suppression systems) Quenching by dilution: insuf鍖cient fuel/oxidizer concentration (air vitiation in under-ventilated 鍖res) Fuel side Oxidizer side Flame Fuel side Oxidizer side Flame Fuel side Oxidizer side Flame Friday, April 30, 2010
  • 19. Types of 鍖ame extinction phenomena Aerodynamic quenching Blowout at large stretch rates (also known as kinetic extinction) Extinction criterion Sources Linan, 1974, Acta Astronautica Williams, 1975, Combustion theory Carrier, Fendell & Marble, 1975, SIAM Journal of Applied Mathematics Friday, April 30, 2010
  • 20. Types of 鍖ame extinction phenomena Thermal quenching: Radiative extinction (large radiation heat losses) Extinction due to evaporative cooling Extinction criterion Sources Sohrab, Li単an & Williams (1982) Combustion Science and Technology Chao, Law & Tien (1992), Combustion and Flame Tien (1986), Combustion and 鍖ame Friday, April 30, 2010
  • 21. The premise: uni鍖ed extinction criterion Friday, April 30, 2010
  • 23. Questions Whether extinction can be described in phenomenological terms with a consistent mathematical model for cases with Friday, April 30, 2010
  • 24. Questions Whether extinction can be described in phenomenological terms with a consistent mathematical model for cases with Stretch (due to turbulence) Friday, April 30, 2010
  • 25. Questions Whether extinction can be described in phenomenological terms with a consistent mathematical model for cases with Stretch (due to turbulence) Radiative heat losses (soot, CO2, H2O, other gases) Friday, April 30, 2010
  • 26. Questions Whether extinction can be described in phenomenological terms with a consistent mathematical model for cases with Stretch (due to turbulence) Radiative heat losses (soot, CO2, H2O, other gases) Evaporative cooling (suppression from water droplets) Friday, April 30, 2010
  • 27. Questions Whether extinction can be described in phenomenological terms with a consistent mathematical model for cases with Stretch (due to turbulence) Radiative heat losses (soot, CO2, H2O, other gases) Evaporative cooling (suppression from water droplets) A combination of the above Friday, April 30, 2010
  • 28. Questions Whether extinction can be described in phenomenological terms with a consistent mathematical model for cases with Stretch (due to turbulence) Radiative heat losses (soot, CO2, H2O, other gases) Evaporative cooling (suppression from water droplets) A combination of the above What kind of diagnostics may be developed to qualify (or quantify) extinction? Friday, April 30, 2010
  • 29. The extinction criterion The Damk旦hler number Code supplies both quantities Need to test if hypothesis holds Friday, April 30, 2010
  • 30. The extinction criterion The Damk旦hler number Code supplies both quantities Need to test if hypothesis holds Mixing Friday, April 30, 2010
  • 31. The extinction criterion The Damk旦hler number Code supplies both quantities Need to test if hypothesis holds Mixing Chemistry Friday, April 30, 2010
  • 32. What is new about this work? Friday, April 30, 2010
  • 33. What is new about this work? Extinction studies with stretch -widely studied (Linan-1974) Friday, April 30, 2010
  • 34. What is new about this work? Extinction studies with stretch -widely studied (Linan-1974) Extinction studies with heat losses (primarily, radiation) Friday, April 30, 2010
  • 35. What is new about this work? Extinction studies with stretch -widely studied (Linan-1974) Extinction studies with heat losses (primarily, radiation) Some theoretical developments by Tien, Law, Chao, Liu Friday, April 30, 2010
  • 36. What is new about this work? Extinction studies with stretch -widely studied (Linan-1974) Extinction studies with heat losses (primarily, radiation) Some theoretical developments by Tien, Law, Chao, Liu Current study Friday, April 30, 2010
  • 37. What is new about this work? Extinction studies with stretch -widely studied (Linan-1974) Extinction studies with heat losses (primarily, radiation) Some theoretical developments by Tien, Law, Chao, Liu Current study Rigorous treatment of non-adiabatic environments (soot, radiation, water spray) Friday, April 30, 2010
  • 38. What is new about this work? Extinction studies with stretch -widely studied (Linan-1974) Extinction studies with heat losses (primarily, radiation) Some theoretical developments by Tien, Law, Chao, Liu Current study Rigorous treatment of non-adiabatic environments (soot, radiation, water spray) Theoretical developments validated with high quality numerical datasets Friday, April 30, 2010
  • 39. What is new about this work? Extinction studies with stretch -widely studied (Linan-1974) Extinction studies with heat losses (primarily, radiation) Some theoretical developments by Tien, Law, Chao, Liu Current study Rigorous treatment of non-adiabatic environments (soot, radiation, water spray) Theoretical developments validated with high quality numerical datasets Questions asked about soot leakage and connection with radiative extinction Friday, April 30, 2010
  • 40. What is new about this work? Extinction studies with stretch -widely studied (Linan-1974) Extinction studies with heat losses (primarily, radiation) Some theoretical developments by Tien, Law, Chao, Liu Current study Rigorous treatment of non-adiabatic environments (soot, radiation, water spray) Theoretical developments validated with high quality numerical datasets Questions asked about soot leakage and connection with radiative extinction Treatment of radiation absorption (with possible extension to optically thick media) Friday, April 30, 2010
  • 41. What is new about this work? Friday, April 30, 2010
  • 42. Pulications Radiation driven 鍖ame weakening effects in sooting turbulent 鍖ames (2008), Narayanan & Trouv辿, Proceedings of the combustion institute Effects of soot addition on extinction limits of luminous laminar counter鍖ow 鍖ames, Narayanan, Baum & Trouv辿 (Accepted, Combustion symposium, 2010) Extinction of Nonpremixed Ethylene-Air 鍖ames by water spray, Arias, Im, Narayanan & Trouv辿 (Accepted, Combustion symposium, 2010) Mixture fraction and state relationships in diffusion 鍖ames interacting with an evaporating water spray, Narayanan, Trouv辿, Arias & Im (in preparation, presented at the US Combustion meeting, Ann Arbor, 2009) Constructing extinction maps for diffusion 鍖ames predicated by radiation emission in sooting turbulent 鍖ames, Narayanan, Lecoustre & Trouv辿 (in preparation, presented at the International Seminar on Fire and Explosions Hazards, Leeds, 2010) Friday, April 30, 2010
  • 44. Tools/approach Direct numerical simulations to generate datasets Massively parallel Combustion solver S3D NERSC machines (Franklin,Hopper) Friday, April 30, 2010
  • 45. Tools/approach Direct numerical simulations to generate datasets Massively parallel Combustion solver S3D NERSC machines (Franklin,Hopper) Mathematical modeling Canonical problems solved using singular perturbation techniques Friday, April 30, 2010
  • 46. Tools/approach Direct numerical simulations to generate datasets Massively parallel Combustion solver S3D NERSC machines (Franklin,Hopper) Mathematical modeling Canonical problems solved using singular perturbation techniques Model validation and analysis Friday, April 30, 2010
  • 48. Numerical approach Use Direct numerical simulations (DNS) Friday, April 30, 2010
  • 49. Numerical approach Use Direct numerical simulations (DNS) Leverage DOE sponsored SciDac collaboration solver S3D Collaborators: Sandia Ntl. Laboratories (J. J. Chen), University of Michigan (H. G. Im) Friday, April 30, 2010
  • 50. Numerical approach Use Direct numerical simulations (DNS) Leverage DOE sponsored SciDac collaboration solver S3D Collaborators: Sandia Ntl. Laboratories (J. J. Chen), University of Michigan (H. G. Im) DNS solver S3D Navier-stokes solver; fully compressible 鍖ow formulation Higher-order methods: 8th order 鍖nite difference; 4th order Runge Kutta time Characteristic based boundary conditions (NSCBC) Structured cartesian grids Parallel, MPI based (excellent scalability) Flame modeling: detailed fuel-air chemistry (CHEMKIN compatible); simpli鍖ed soot formation model; thermal radiation model (Discrete Ordinate/Discrete Transfer Method); Lagrangian particle model to describe dilute liquid sprays Friday, April 30, 2010
  • 52. Single step chemistry Ethylene-air chemistry model (Westbrook & Dryer, 1981) Used for simpli鍖ed extinction model (in asymptotic analysis and numerical validation with DNS) F = BRR ( YF MF )僚 F ( YO2 MF )僚O exp( Ta T ) Friday, April 30, 2010
  • 53. Detailed Chemistry Used for more detailed calculations with water spray Reduced chemical kinetic mechanism (Lu & Law, 2009, Progress in Energy and Combustion Science) Based on detailed chemistry mechanism for ethylene-air combustion (70 species, 463 elementary reactions, Wang et al., 2000, Proceedings of the Combustion Institute) Reduced chemistry mechanism using: the method of directed relations graphs (DRG): sensitivity analysis; quasi steady-state assumption for fast reacting radicals 19 species, 15 semi-global reactions Friday, April 30, 2010
  • 54. Soot formation model Phenomenological, two equation model (Moss et al., Lindstedt et al.) Soot formation process included into phenomenology nucleation, surface growth, coagulation, oxidation Friday, April 30, 2010
  • 55. Lagrangian spray model Adapted from Wang and Rutland (2007), Combustion and Flame Spherical, monodisperse droplets Particle in cell Dilute liquid phase assumption Lagrangian-Eulerian coupling Position Mass Momentum Energy Lagrangian droplet equations Droplet source terms in Eulerian gas equations Mass Momentum Energy Friday, April 30, 2010
  • 56. Thermal radiation model Non-scattering, gray gas assumption; Discrete Transfer Method (Lockwood & Shah, 1981) Solve radiative transfer equation Mean absorption coef鍖cient (ap,i) Friday, April 30, 2010
  • 58. Problems investigated Turbulent sooting/radiating wall 鍖ames Friday, April 30, 2010
  • 59. Problems investigated Turbulent sooting/radiating wall 鍖ames Radiative weakening and extinction 鍖rst come to light in turbulent simulation Friday, April 30, 2010
  • 60. Problems investigated Turbulent sooting/radiating wall 鍖ames Radiative weakening and extinction 鍖rst come to light in turbulent simulation Laminar counter鍖ow sooting/radiating 鍖ames Friday, April 30, 2010
  • 61. Problems investigated Turbulent sooting/radiating wall 鍖ames Radiative weakening and extinction 鍖rst come to light in turbulent simulation Laminar counter鍖ow sooting/radiating 鍖ames Attempts in understanding radiative extinction through asymptotic analysis and numerical simulations Friday, April 30, 2010
  • 62. Problems investigated Turbulent sooting/radiating wall 鍖ames Radiative weakening and extinction 鍖rst come to light in turbulent simulation Laminar counter鍖ow sooting/radiating 鍖ames Attempts in understanding radiative extinction through asymptotic analysis and numerical simulations Turbulent counter鍖ow 鍖ames weakened by water spray Friday, April 30, 2010
  • 63. Problems investigated Turbulent sooting/radiating wall 鍖ames Radiative weakening and extinction 鍖rst come to light in turbulent simulation Laminar counter鍖ow sooting/radiating 鍖ames Attempts in understanding radiative extinction through asymptotic analysis and numerical simulations Turbulent counter鍖ow 鍖ames weakened by water spray More complex problem with detailed chemistry, explored via numerical simulations and application of asymptotic model developed Friday, April 30, 2010
  • 64. Turbulent sooting 鍖ames Simpli鍖ed turbulent con鍖guration Two dimensional (8 x 4 cm2); grid size: 1216 x 375 (uniform x stretched); prescribed in鍖ow turbulent 鍖uctuations (u = 1-2.5 m/s, Lt = 1.7 mm) Air Fuel Solid Wall 2.5-5 m/s y 50 袖m x 66 袖m Friday, April 30, 2010
  • 65. Turbulent sooting 鍖ames Observations radiative cooling region is not thin soot region is not thin weak 鍖ame events correlated with soot mass leakage across the 鍖ame radiation cooling rate soot mass fraction extinction extinction Analysis of 鍖ame structure (case, Tw=300 K, with soot/radiation, Csoot= 7000 m-1 K-1) Friday, April 30, 2010
  • 66. Turbulent sooting 鍖ames Analysis of 鍖ame structure (case, Tw=300 K, with soot/radiation, Csoot= 7000 m-1 K-1) weak spots weak flame events occur at low values of flame stretch (slow mixing limit) Friday, April 30, 2010
  • 67. Radiative extinction under external soot loading Friday, April 30, 2010
  • 68. Overview Explore connection between 鍖ame extinction and soot leakage Relevance in radiating/sooting environments Pool鍖res Connection with smoking candle 鍖ames Cold Soot Hot Soot Friday, April 30, 2010
  • 69. Problem formulation Asymptotic 鍖ame structure with soot loading External soot loading to simulate multi-dimensional 鍖ame structure in a one- dimensional framework Soot loading from air side Fuel Air Air Flame Soot region Flame Sootinjection Friday, April 30, 2010
  • 70. Problem formulation Approach: setup counter鍖ow 鍖ame with radiative heat loss Analytical setup (transform to one-dimensional scalar 鍖elds) Numerical setup (DNS) for validation (two dimensional counter鍖ow 鍖ame) Outputs: Flame structure (鍖ame variables such as temperature, mixing rate, radiation cooling rate) Effect of soot loading on extinction properties how are the limits changed with radiation heat loss? Friday, April 30, 2010
  • 71. Activation Energy Asymptotics Convert governing equations into one-dimensional coordinates using Howarth transformation for variable density Constant speci鍖c heat, single step Arrhenius Chemistry Conventional solution using singular perturbation: split domain into Outer radiating zone-to obtain radiation corrected outer temperatures Full treatment-both emission and absorption handled (radiation transport equation solved) Inner reacting zone -complete 鍖ame structure and extinction conditions Solve using two point BVP solver Patch outer and inner solutions to obtain complete 鍖ame structure Solve for soot 鍖eld using completed 鍖ame structure with BVP solver (but do not have bene鍖t of asymptotic expansions here!) Outer Outer Inner Friday, April 30, 2010
  • 72. Governing equations Only contributes near thin reaction zone (inner region) Zero far from reaction zone (outer region) Fuel (Ethylene) Outer layer (radiatively active) Thin 鍖ame (inner layer) Oxidizer (air) Friday, April 30, 2010
  • 73. Outer solutions Solve for leading order solutions far from 鍖ame Algorithm Solve on either side of 鍖ame using Greens functions Get temperature at 鍖ame location Solve Inner equation Obtain complete solution Howarth Transform Friday, April 30, 2010
  • 74. Inner solutions Solve for inner solutions by zooming in at 鍖ame zone Transform Outer Outer Inner Friday, April 30, 2010
  • 75. Inner solutions Solve for inner solutions by zooming in at 鍖ame zone Transform Outer Outer Inner Reduced Damk旦hler number Friday, April 30, 2010
  • 76. What is the effect of radiation in all this? Radiation free 鍖ame: (outer) temperature is the adiabatic 鍖ame temperature With radiation: (outer) temperature is lowered! Effects of radiation felt when Large amounts of soot Small strain Radiation corrected 鍖ame temperature feeds into inner equation Radiation correction to give new Burke-Schumann temperature Text Solve RTE Friday, April 30, 2010
  • 77. What is the effect of radiation in all this? Radiation free 鍖ame: (outer) temperature is the adiabatic 鍖ame temperature With radiation: (outer) temperature is lowered! Effects of radiation felt when Large amounts of soot Small strain Radiation corrected 鍖ame temperature feeds into inner equation Radiation correction to give new Burke-Schumann temperature Radiation Text Solve RTE Friday, April 30, 2010
  • 78. What is the effect of radiation in all this? Radiation free 鍖ame: (outer) temperature is the adiabatic 鍖ame temperature With radiation: (outer) temperature is lowered! Effects of radiation felt when Large amounts of soot Small strain Radiation corrected 鍖ame temperature feeds into inner equation Radiation correction to give new Burke-Schumann temperature Radiation Strain Text Solve RTE Friday, April 30, 2010
  • 79. On radiative emission and absorption Emission: local function of temperature Absorption: non-local convolution integral Depends on optical thickness of surroundings Can develop asymptotic measures for radiating regimes (thick (Szoke, LLNL), thin (the optically thin assumption), intermediate) Possibilities of regime based approximations (thick and thin somewhat amenable to analytical solutions (!?), intermediate needs computation) Radiation source term Optically thin Optically thick Friday, April 30, 2010
  • 80. Laminar counter鍖ow 鍖ames Reference counter鍖ow 鍖ame Flamelet perspective: study 鍖ame structure as a function of 鍖ame stretch ranging from ultra-low to ultra-high values No soot injection Flame Friday, April 30, 2010
  • 81. Laminar counter鍖ow 鍖ames Reference counter鍖ow 鍖ame Flamelet perspective: study 鍖ame structure as a function of 鍖ame stretch ranging from ultra-low to ultra-high values No soot injection kinetic extinction limit radiation extinction limit DNS AEA Friday, April 30, 2010
  • 82. Laminar counter鍖ow 鍖ames Reference counter鍖ow 鍖ame Flamelet perspective: study 鍖ame structure as a function of 鍖ame stretch ranging from ultra-low to ultra-high values Friday, April 30, 2010
  • 83. Laminar counter鍖ow 鍖ames Extinction values correspond to critical value of Damk旦hler number Friday, April 30, 2010
  • 84. Laminar counter鍖ow 鍖ames Extinction values correspond to critical value of Damk旦hler number adiabatic soot-free with soot with external soot loading approximate critical value Extinction Flammable Friday, April 30, 2010
  • 85. Flammability maps Extinction limits Flammability maps with mixing rate and 鍖ame temperature as coordinates Extinction Flammable Engine extinction event Fire extinction event Friday, April 30, 2010
  • 86. Analysis of turbulent 鍖ame data Extinction limits Flammability maps with mixing rate and 鍖ame temperature as coordinates Extinction representative conditions of flame weakest spots in DNS Apparently, the 鍖ames weakest spots are not actually quenched Soot leakage events may have more to do with cessation of soot oxidation chemistry than radiative extinction soot mass fraction extinction Friday, April 30, 2010
  • 87. Conclusions on sooting 鍖ames Friday, April 30, 2010
  • 88. Conclusions on sooting 鍖ames Activation energy asymptotics and DNS have been used to make fundamental observations on non-adiabatic turbulent sooting diffusion 鍖ames Friday, April 30, 2010
  • 89. Conclusions on sooting 鍖ames Activation energy asymptotics and DNS have been used to make fundamental observations on non-adiabatic turbulent sooting diffusion 鍖ames Two extinction limits are encountered Kinetic extinction (at high stretch) Radiative extinction (at low stretch) Friday, April 30, 2010
  • 90. Conclusions on sooting 鍖ames Activation energy asymptotics and DNS have been used to make fundamental observations on non-adiabatic turbulent sooting diffusion 鍖ames Two extinction limits are encountered Kinetic extinction (at high stretch) Radiative extinction (at low stretch) Extinction occurs at a single critical value of the reduced Damk旦hler number equalling unity Can construct maps to gauge extinction propensity of 鍖ames Friday, April 30, 2010
  • 91. Conclusions on sooting 鍖ames Activation energy asymptotics and DNS have been used to make fundamental observations on non-adiabatic turbulent sooting diffusion 鍖ames Two extinction limits are encountered Kinetic extinction (at high stretch) Radiative extinction (at low stretch) Extinction occurs at a single critical value of the reduced Damk旦hler number equalling unity Can construct maps to gauge extinction propensity of 鍖ames Turbulent 鍖ame data indicate that soot leakage events are not necessarily radiative extinction events. Further investigation of soot oxidation chemistry is warranted Friday, April 30, 2010
  • 92. DNS of turbulent spray 鍖ames Friday, April 30, 2010
  • 93. Turbulent spray 鍖ames Counter鍖ow laminar/turbulent diffusion 鍖ames with water spray injection Two dimensional, domain size (1 cm x 2 cm), 480 k grid points (400 procs on Franklin) Detailed chemistry Strain rate of 440 s-1 (extinction: 1300 s-1) Turbulence injection at inlet (u/U=0.85, L11=0.5 cm) 1 cm x = 16 袖m y= 25 袖m Droplet diameter: 10 亮m, mist regime Injection at local gas velocity Friday, April 30, 2010
  • 94. Unexplored areas Extinction and soot leakage If soot leakage precedes radiative extinction, can one come up with a description based on soot chemistry Damk旦hler number criterion for cessation of soot oxidation chemistry Could have rami鍖cations in smoking 鍖res Strongly radiating, but not quenched Development of approximations in thick media (and thin) and its application to radiating solvers Envisage cost reduction if only intermediate regions need to be computed How do we incorporate chemistry effects in complex 鍖ames? Friday, April 30, 2010