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Heat Transfer and Thermal Boundary Conditions

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Headlamp modeled with Discrete Ordinates Radiation Model Outline Introduction Thermal Boundary Conditions Fluid Properties Conjugate Heat Transfer Natural Convection ... – PowerPoint PPT presentation

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Title: Heat Transfer and Thermal Boundary Conditions


1
Heat Transfer and Thermal Boundary Conditions
  • Headlamp modeled with
  • Discrete Ordinates
  • Radiation Model

2
Outline
  • Introduction
  • Thermal Boundary Conditions
  • Fluid Properties
  • Conjugate Heat Transfer
  • Natural Convection
  • Radiation
  • Periodic Heat Transfer

3
Introduction
  • Heat transfer in Fluent solvers allows inclusion
    of heat transfer within fluid and solid regions
    in your model.
  • Handles problems ranging from thermal mixing
    within a fluid to conduction in composite solids.
  • Energy transport equation is solved, subject to a
    wide range of thermal boundary conditions.

4
Options
  • Inclusion of species diffusion term
  • Energy equation includes effect of enthalpy
    transport due to species diffusion, which
    contributes to energy balance.
  • This term is included in the energy equation by
    default.
  • You can turn off the Diffusion Energy Source
    option in the Species Model panel.
  • Term always included in the coupled solver.
  • Energy equation in conducting solids
  • In conducting solid regions, simple conduction
    equation solved
  • Includes heat flux due to conduction and
    volumetric heat sources within solid.
  • Convective term also included for moving solids.
  • Energy sources due to chemical reaction are
    included for reacting flow cases.

5
User Inputs for Heat Transfer (1)
  • 1. Activate calculation of heat transfer.
  • Select the Enable Energy option in the Energy
    panel.
  • Define ? Models ? Energy...
  • Enabling reacting flow or radiation will toggle
    Enable Energy on without visiting this panel.

6
User Inputs for Heat Transfer (2)
  • 2. To include viscous heating terms in energy
    equation, turn on Viscous Heating in Viscous
    Model panel.
  • Describes thermal energy created by viscous shear
    in the flow.
  • Often negligible not included in default form of
    energy equation.
  • Enable when shear stress in fluid is large (e.g.,
    in lubrication problems) and/or in high-velocity,
    compressible flows.
  • 3. Define thermal boundary conditions.
  • Define ? Boundary Conditions...
  • 4. Define material properties for heat transfer.
  • Define ? Materials...
  • Heat capacity and thermal conductivity must be
    defined.
  • You can specify many properties as functions of
    temperature.

7
Solution Process for Heat Transfer
  • Many simple heat transfer problems can be
    successfully solved using default solution
    parameters.
  • However, you may accelerate convergence and/or
    improve the stability of the solution process by
    changing the options below
  • Underrelaxation of energy equation.
  • Solve ? Controls ? Solution...
  • Disabling species diffusion term.
  • Define ? Models ? Species...
  • Compute isothermal flow first, then add
    calculation of energy equation.
  • Solve ? Controls ? Solution...

8
Theoretical Basis of Wall Heat Transfer
  • For laminar flows, fluid side heat transfer is
    approximated as
  • n local coordinate normal to wall
  • For turbulent flows, law of the wall is extended
    to treat wall heat flux.
  • The wall-function approach implicitly accounts
    for viscous sublayer.
  • The near-wall treatment is extended to account
    for viscous dissipation which occurs in the
    boundary layer of high-speed flows.

9
Thermal Boundary Conditions at Flow Inlets and
Exits
  • At flow inlets, must supply fluid temperature.
  • At flow exits, fluid temperature extrapolated
    from upstream value.
  • At pressure outlets, where flow reversal may
    occur, backflow temperature is required.

10
Thermal Conditions for Fluids and Solids
  • Can specify an energy source using Source Terms
    option.

11
Thermal Boundary Conditions at Walls
  • Use any of following thermal conditions at walls
  • Specified heat flux
  • Specified temperature
  • Convective heat transfer
  • External radiation
  • Combined external radiation and external
    convective heat transfer

12
Fluid Properties
  • Fluid properties such as heat capacity,
    conductivity, and viscosity can be defined as
  • Constant
  • Temperature-dependent
  • Composition-dependent
  • Computed by kinetic theory
  • Computed by user-defined functions
  • Density can be computed by ideal gas law.
  • Alternately, density can be treated as
  • Constant (with optional Boussinesq modeling)
  • Temperature-dependent
  • Composition-dependent

13
Conjugate Heat Transfer
  • Ability to compute conduction of heat through
    solids, coupled with convective heat transfer in
    fluid.
  • In 2D Cartesian coordinates
  • Solid properties may vary with location, e.g.,
  • Density, ?w
  • Specific heat, cw
  • Conductivity, kw
  • Solid conductivity, kw, may also be function of
    temperature.
  • is a uniformly distributed volumetric heat
    source.
  • May be function of time and space (using profiles
    or user-defined functions).

14
Conjugate Heat Transfer in Fuel-Rod Assembly
  • Fluid flow equations not solved within solid
    regions.
  • Energy equation solved simultaneously in full
    domain.
  • Convective terms dropped in stationary solid
    regions.

15
Natural Convection - Introduction
  • Natural convection occurs when heat is added to
    fluid and fluid density varies with temperature.
  • Flow is induced by force of gravity acting on
    density variation.

16
Natural Convection - Boussinesq Model
  • Makes simplifying assumption that density is
    uniform.
  • Except for body force term in momentum equation,
    which is replaced by
  • Valid when density variations are small.
  • When to use Boussinesq model
  • Essential to calculate time-dependent natural
    convection inside closed domains.
  • Can also be used for steady-state problems.
  • Provided changes in temperature are small
  • You can get faster convergence for many
    natural-convection flows than by using fluid
    density as function of temperature.
  • Cannot be used with species calculations or
    reacting flows.

17
User Inputs for Natural Convection (1)
  • 1. Set gravitational acceleration.
  • Define ? Operating Conditions...
  • 2. Fluid density
  • (a) If using Boussinesq model
  • Select boussinesq as the Density method and
    assign a constant value.
  • Set the Thermal Expansion Coefficient.
  • Define ? Materials
  • Set the Operating Temperature in the Operating
    Conditions panel.
  • Define ? Operating Conditions...
  • (b) Otherwise, define fluid density as function
    of

    temperature.

18
User Inputs for Natural Convection (2)
  • 3. Optionally, specify Operating Density.
  • Does not apply for Boussinesq model.
  • 4. Set boundary conditions.
  • Define ? Boundary Conditions...

19
Radiation
  • Radiation intensity along any
    direction
    entering medium
    is reduced by
  • Local absorption
  • Out-scattering (scattering away

    from the direction)
  • Radiation intensity along any
    direction
    entering medium is
    augmented by
  • Local emission
  • In-scattering (scattering into the direction)
  • Four radiation models are provided in FLUENT
  • Discrete Ordinates Model (DOM)
  • Discrete Transfer Radiation Model (DTRM)
  • P-1 Radiation Model
  • Rosseland Model (limited applicability)

20
Discrete Ordinates Model
  • The radiative transfer equation is solved for a
    discrete number of finite solid angles
  • Advantages
  • Conservative method leads to heat balance for
    coarse discretization.
  • Accuracy can be increased by using a finer
    discretization.
  • Accounts for scattering, semi-transparent media,
    specular surfaces.
  • Banded-gray option for wavelength-dependent
    transmission.
  • Limitations
  • Solving a problem with a large number of
    ordinates is CPU-intensive.

21
Discrete Transfer Radiation Model (DTRM)
  • Main assumption radiation leaving surface
    element in a specific range of solid angles can
    be approximated by a single ray.
  • Uses ray-tracing technique to integrate radiant
    intensity along each ray
  • Advantages
  • Relatively simple model.
  • Can increase accuracy by increasing number of
    rays.
  • Applies to wide range of optical thicknesses.
  • Limitations
  • Assumes all surfaces are diffuse.
  • Effect of scattering not included.
  • Solving a problem with a large number of rays is
    CPU-intensive.

22
P-1 Model
  • Main assumption radiation intensity can be
    decomposed into series of spherical harmonics.
  • Only first term in this (rapidly converging)
    series used in P-1 model.
  • Effects of particles, droplets, and soot can be
    included.
  • Advantages
  • Radiative transfer equation easy to solve with
    little CPU demand.
  • Includes effect of scattering.
  • Works reasonably well for combustion applications
    where optical thickness is large.
  • Easily applied to complicated geometries with
    curvilinear coordinates.
  • Limitations
  • Assumes all surfaces are diffuse.
  • May result in loss of accuracy, depending on
    complexity of geometry, if optical thickness is
    small.
  • Tends to overpredict radiative fluxes from
    localized heat sources or sinks.

23
Choosing a Radiation Model
  • For certain problems, one radiation model may be
    more appropriate in general.
  • Define ? Models ? Radiation...
  • Computational effort P-1 gives reasonable
    accuracy with
    less effort.
  • Accuracy DTRM and DOM more accurate.
  • Optical thickness DTRM/DOM for optically thin
    media (optical
    thickness ltlt 1) P-1 better for optically thick
    media.
  • Scattering P-1 and DOM account for scattering.
  • Particulate effects P-1 and DOM account for
    radiation exchange between gas and particulates.
  • Localized heat sources DTRM/DOM with
    sufficiently large number of rays/ ordinates is
    more appropriate.

24
Periodic Heat Transfer (1)
  • Also known as streamwise-periodic or
    fully-developed flow.
  • Used when flow and heat transfer patterns are
    repeated, e.g.,
  • Compact heat exchangers
  • Flow across tube banks
  • Geometry and boundary conditions repeat in
    streamwise direction.

Outflow at one periodic boundary is inflow at the
other
25
Periodic Heat Transfer (2)
  • Temperature (and pressure) vary in streamwise
    direction.
  • Scaled temperature (and periodic pressure) is
    same at periodic boundaries.
  • For fixed wall temperature problems, scaled
    temperature defined as
  • Tb suitably defined bulk temperature
  • Can also model flows with specified wall heat
    flux.

26
Periodic Heat Transfer (3)
  • Periodic heat transfer is subject to the
    following constraints
  • Either constant temperature or fixed flux bounds.
  • Conducting regions cannot straddle periodic
    plane.
  • Properties cannot be functions of temperature.
  • Radiative heat transfer cannot be modeled.
  • Viscous heating only available with heat flux
    wall boundaries.
  • Flow must be specified by pressure jump in
    coupled solvers.

Contours of Scaled Temperature
27
Summary
  • Heat transfer modeling is available in all Fluent
    solvers.
  • After activating heat transfer, you must provide
  • Thermal conditions at walls and flow boundaries
  • Fluid properties for energy equation
  • Available heat transfer modeling options include
  • Species diffusion heat source
  • Combustion heat source
  • Conjugate heat transfer
  • Natural convection
  • Radiation
  • Periodic heat transfer
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