Radiative Heat Transfer in CFAST Martin Clouthier Introduction

Radiative Heat Transfer in CFAST

Concepts Conservation Equations

Martin Clouthier

Mass Species Energy Assumptions & Limitations

January 2013

Assumptions Veri ication Radiative heat transfer Conclusions

Martin Clouthier

Radiative Heat Transfer in CFAST

Outline Radiative Heat Transfer in CFAST Martin Clouthier Introduction Concepts Conservation Equations Mass Species Energy Assumptions & Limitations Assumptions

1 Introduction 2 Concepts 3 Conservation Equations

Mass Species Energy 4 Assumptions & Limitations

Assumptions

Veri ication

5 Veri ication

Radiative heat transfer

6 Radiative heat transfer

Conclusions

7 Conclusions Martin Clouthier

Radiative Heat Transfer in CFAST

The purpose of this presentation is to provide… Radiative Heat Transfer in CFAST Martin Clouthier

1

Understanding of basic concepts underlying a zone ire model

2

Exposure to conservation equations and submodels

3

Knowledge of the major assumptions and limitations

4

Familiarity with veri ication of CFAST, and results for Version 6.2.0

5

Awareness of how CFAST deals with radiative heat transfer

Introduction Concepts Conservation Equations Mass Species Energy Assumptions & Limitations Assumptions Veri ication Radiative heat transfer Conclusions

Martin Clouthier

Radiative Heat Transfer in CFAST

What is CFAST? Radiative Heat Transfer in CFAST Martin Clouthier Introduction Concepts Conservation Equations Mass Species Energy Assumptions & Limitations Assumptions Veri ication Radiative heat transfer

CFAST is a two-zone ire model developed by NIST, used to calculate the evolving distribution of smoke, ire gases and temperature throughout compartments of a building during a ire. The software solves conservation equations for mass and energy in two control volumes Accounts for the effects of User speci ied ire(s) in multiple connected compartments Natural low between compartments through vents Mechanical ventilation Heating and ignition of objects

Conclusions

Martin Clouthier

Radiative Heat Transfer in CFAST

Extensive validation from literature and comparisons with experiments Radiative Heat Transfer in CFAST Martin Clouthier Introduction Concepts Conservation Equations Mass Species Energy Assumptions & Limitations Assumptions Veri ication

Predictions of HGL temperature, HGL height, ceiling jet temperature, plume temperature, lame height, gas concentration, smoke concentration, and room pressure are typically within or near experimental uncertainty Zone model predictions of target/wall lux or target/wall temperature require care and an understanding of the capabilities and limitation of zone models when used for analysing ire scenarios

Radiative heat transfer Conclusions

Martin Clouthier

Radiative Heat Transfer in CFAST

A zone model divides the compartment into control volumes Radiative Heat Transfer in CFAST Martin Clouthier

��

Introduction Concepts Conservation Equations

�̇

Mass Species Energy Assumptions & Limitations Assumptions Veri ication Radiative heat transfer

�̇

��

�̇ �̇

�̇

�̇

.

Figure 1: Control volumes selected in zone ire modelling

Conclusions

Martin Clouthier

Radiative Heat Transfer in CFAST

Conservation Equations Radiative Heat Transfer in CFAST Martin Clouthier Introduction Concepts Conservation Equations

Governing equations based on First law of thermodynamics (energy conservation)

Mass

Continuity equation (mass conservation)

Species

Newton’s second law of motion → Bernouilli’s equation (momentum)

Energy Assumptions & Limitations Assumptions Veri ication Radiative heat transfer Conclusions

Martin Clouthier

Radiative Heat Transfer in CFAST

Conservation of mass Radiative Heat Transfer in CFAST Martin Clouthier

∑ d ˙j=0 A (ρzl ) + m dt J

��

Introduction Concepts

j=1 (net out)

Conservation Equations �̇

Mass Species Energy Assumptions & Limitations Assumptions Veri ication

�̇

��

�̇

dml ˙ in − m ˙ out − m ˙e =m dt

�̇ �̇

.

�̇

Figure 1: Control volumes selected in zone ire modelling

dmu ˙e+m ˙f−m ˙u =m dt

Radiative heat transfer Conclusions

Martin Clouthier

Radiative Heat Transfer in CFAST

Conservation of Species Radiative Heat Transfer in CFAST Martin Clouthier Introduction Concepts Conservation Equations Mass Species

dYi ∑ ˙ j (Yij − Yi ) = ω˙ i ρzl A + m dt J

j=1

Energy Assumptions & Limitations Assumptions Veri ication Radiative heat transfer Conclusions

Martin Clouthier

Radiative Heat Transfer in CFAST

Conservation of Energy Radiative Heat Transfer in CFAST Martin Clouthier Introduction Concepts Conservation Equations Mass Species Energy Assumptions & Limitations Assumptions Veri ication Radiative heat transfer

   rate of change of  { } enthalpy energy of the =+   low in layer { } enthalpy −  low out  heat   + transferred   to the layer { } work done − by the layer

Conclusions

Martin Clouthier

Radiative Heat Transfer in CFAST

Conservation of Energy Radiative Heat Transfer in CFAST Martin Clouthier Introduction Concepts Conservation Equations Mass Species Energy

∑ dT dp ˙ j (Tj − T) = ω˙ F ∆H − Q˙ net loss ρcp zl A − zl A + cp m | {z } dt dt J

j=1 (net out)

Assumptions & Limitations Assumptions Veri ication Radiative heat transfer Conclusions

Martin Clouthier

Radiative Heat Transfer in CFAST

submodels

Major Assumptions Radiative Heat Transfer in CFAST Martin Clouthier Introduction

1

Gas is treated as ideal gas with constant values for molecular weight and speci ic heats (i.e., cp and cv ).

2

Exchange of mass at free boundaries is due to pressure differences or shear mixing effects.

3

Combustion is treated as a source of mass and energy.

4

Plume instantly arrives at the ceiling. Transport times are not explicitly accounted for in zone modelling.

5

Pressure is considered uniform in the energy equation, but hydrostatic variations account for pressure differences at free boundaries.

6

Mass low into the ire plume is to to turbulent entrainment.

Concepts Conservation Equations Mass Species Energy Assumptions & Limitations Assumptions Veri ication Radiative heat transfer Conclusions

Martin Clouthier

Radiative Heat Transfer in CFAST

Veri ication vs. Validation Radiative Heat Transfer in CFAST Martin Clouthier Introduction Concepts Conservation Equations Mass Species Energy Assumptions & Limitations Assumptions Veri ication Radiative heat transfer Conclusions

ASTM E 1355 Standard Guide for Evaluating the Predictive Capability of Deterministic Fire Models Veri ication—the process of determining that the implementation of a calculation method accurately represents the developer’s conceptual description of the calculation method and the solution to the calculation method. Is the Math right? Validation—the process of determining the degree to which a calculation method is an accurate representation of the real world from the perspective of the intended uses of the calculation method. Is the Physics right?

Martin Clouthier

Radiative Heat Transfer in CFAST

Veri ication of proper installation Radiative Heat Transfer in CFAST Martin Clouthier

Table : Results at

Introduction Concepts Conservation Equations Mass Species Energy Assumptions & Limitations Assumptions

Value

C Upper Temp. C Upper Temp.

Units ∘



C C

Case

Version . . . .

seconds Case

Version . . . .

Veri ication Radiative heat transfer Conclusions

Martin Clouthier

Radiative Heat Transfer in CFAST

Case

Version . . . .

CFAST simulations show the effects of increased soot yield Radiative Heat Transfer in CFAST Martin Clouthier Introduction

Table : Single Compartment at

Concepts Conservation Equations Mass Species Energy Assumptions & Limitations

Value

Upper Temp Lower Temp

Units ∘



C C

Methane �̄ =

Absorbtion incorrect

Absorbtion corrected

s

Methane �̄ = . kg/kg

Absorbtion incorrect

Absorbtion corrected

Assumptions Veri ication Radiative heat transfer Conclusions

Martin Clouthier

Radiative Heat Transfer in CFAST

Radiation network for two zones Radiative Heat Transfer in CFAST



Martin Clouthier

�walls

��

Introduction

�walls

Concepts Conservation Equations

�̇

Mass Species Energy Assumptions & Limitations Assumptions Veri ication

,walls

�̇

��

�̇ �̇

�̇

�̇

.

Figure 1: Control volumes selected in zone ire modelling

Radiative heat transfer

�walls to



loor

to w alls r to

� loo

� loor � loor .�

, loor

Figure 2: Radiation network

Conclusions

Martin Clouthier

Radiative Heat Transfer in CFAST



,

Equations used by CFAST to calculate radiative heat transfer Radiative Heat Transfer in CFAST Martin Clouthier

Q˙ net loss = hAs (Tgu − Twu ) + q˙ CV1 to Walls + q˙ CV1 to Floor {z } | {z } | radiative

convective

Introduction Concepts Conservation Equations

q˙ CV1 to Walls =

Ebgu − Ebw Rwg + Rw

Mass Species Energy

Rwg = (Aw Fwg ϵgu )−1 ,

Rw =

Assumptions & Limitations Assumptions Veri ication

q˙ CV1 to Floor =

Radiative heat transfer Conclusions

Ebgu − Ebflr Rflrg + Rflr

Rflrg = (Aflr Fflrg ϵgu )−1 , Martin Clouthier

1 − ϵw ϵw Aw

Rflr =

1 − ϵflr ϵflr Aflr

Radiative Heat Transfer in CFAST

Equations used by CFAST to calculate gas layer emissivity Radiative Heat Transfer in CFAST Martin Clouthier

ϵgu = 1 − e−Km S + ϵg e−Km S

Introduction Concepts Conservation Equations

Km = 3.72

Mass

Co fv Tgu C2

Species Energy Assumptions & Limitations

fv =

˙ s ∆t ¯ysoot m ρsoot (WLzl )

Assumptions Veri ication Radiative heat transfer

ϵg ≈

Conclusions

1 ϵH2 O + ϵCO2 |{z} 2

code error

Martin Clouthier

Radiative Heat Transfer in CFAST

Put simply Radiative Heat Transfer in CFAST Martin Clouthier Introduction Concepts Conservation Equations Mass Species

Q˙ net loss = f(Tg , Tw , ¯ysoot , zl , ϵg , ϵw , ϵflr )

Energy Assumptions & Limitations Assumptions Veri ication Radiative heat transfer Conclusions

Martin Clouthier

Radiative Heat Transfer in CFAST

There was a coding subscript error in CFAST Radiative Heat Transfer in CFAST Martin Clouthier Introduction Concepts Conservation Equations

Source code from the SVN repository, ‘radiation.f90’

Mass Species Energy Assumptions & Limitations Assumptions Veri ication Radiative heat transfer Conclusions

Martin Clouthier

Radiative Heat Transfer in CFAST

Conclusions Radiative Heat Transfer in CFAST Martin Clouthier Introduction Concepts Conservation Equations Mass Species

Soot yield has an important effect on upper layer gas temperature and radiative heat loss.

Energy Assumptions & Limitations Assumptions Veri ication Radiative heat transfer Conclusions

Martin Clouthier

Radiative Heat Transfer in CFAST

Radiative Heat Transfer in CFAST -

Conclusions. Conservation of Energy... rate of change of .... Source code from the SVN repository, 'radiation.f90'. Martin Clouthier. Radiative Heat Transfer ...

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