adv rm v6.2 lect 02a srf

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    Frame (SRF) Model

    Frame (SRF) Model

    Advanced FLUENT CFD TrainingAdvanced FLUENT CFD Training

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    Fluent User Services Center

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    Advanced FLUENT Training v6.3

    Rotating Machinery July 2008

    Outline

    ntro uct on to o e ng

    Navier-Stokes Equations for a Rotating Reference Frame Relative and Absolution Velocity Formulations

    SRF Problem Setup

    Solver

    Physical Models

    Material Properties

    Boundary Conditions

    Solver Settings Initialization

    Troubleshooting SRF Problems

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    Appendix

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    Advanced FLUENT Training v6.3

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    Introduction to SRF Modeling

    any pro ems w c nvo ve rotat ng components can e mo e e us ng a

    single moving reference frame. Why use a rotating reference frame?

    A flow field which is unsteady with respect to the stationary frame becomes

    steady with respect to the rotating frame.

    Steady-state problems are easier to solve...

    mp er s

    Lower computational cost

    Easier to postprocess and analyze

    e w scuss ssues re a e o mo e ng n s sec on, u many

    concepts (e.g. solver settings, physical models, etc.) will also apply to MRF,

    MPM, and SMM

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    Advanced FLUENT Training v6.3

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    Characteristics of SRF Models

    ov ng rame s assoc ate w t a s ng e u oma n.

    In FLUENT, you may divide this domain up into several connected fluid zones,but each fluid zone must have the same moving reference frame speed and axis

    Domain rotates with a constant, prescribed rotational speed about a specifiedax s o ro a on

    No translation considered (though this may be included)

    FLUENT only provides for a constant rotational speed in the user interface

    cce era ng rames o re erence can e mp emen e roug user e ne

    functions

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    Characteristics of SRF Models

    oma n typ ca y cons sts o

    Inlets and outlets Walls

    Rotationally periodic boundaries

    Boundaries which move with the fluid domain may assume any shape.

    Boundaries which are stationary (with respect to the laboratory or fixed

    frame must be surfaces of revolution.

    Rotationally periodic boundaries require spatial periodicity of all boundary

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    Illustration of a Typical SRF ModelShroud/casing

    Fluid domain

    sur ace

    Rotatingx

    frameAxis of rotation

    Hub surface

    z

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    Blade surface

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    Stationary Walls in SRF Models

    Stationary walla e

    Rotor

    Wron !

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    Wall with baffles nota surface

    of revolution!

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    Rotating Reference Frames

    e norma y escr e u mot ons w t respect to an a so ute or

    inertial reference frame We can define a rotating reference frame as a reference frame which is

    sp nn ng w t a prescr e or entat on an spee w t respect to an

    inertial reference frame

    The motion of the reference frame gives rise to additional accelerations

    Non-inertial reference frame

    The velocity of the fluid can defined with respect to either the absolute or

    Absolute velocity - Fluid velocity with respect to the stationary (absolute)

    reference frame

    Relative velocity - Fluid velocity with respect to the rotating reference

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    frame

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    The Velocity Triangle

    e re at ons p etween t e a so ute an re at ve ve oc t es s g ven y

    UWVrrr

    += velocityabsolute=Vr

    rUrrr

    velocityrelative=Wr

    In turbomachinery, this relationship can be illustrated using the laws of

    vector addition. This is known as the Velocity Triangle

    Wr

    Ur

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    Vr

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    Navier-Stokes Equations (Rotating Reference Frame)

    wo erent ormu at ons are use n

    Relative Velocity Formulation (RVF) Obtained by transforming the stationary frame N-S equations to a rotating reference frame

    Uses the relative velocit as the de endent variable in the momentum e uations

    Uses the relative total internal energy as the dependent variable in the energy equation

    Available for the Segregated Solver only!

    Absolute Velocity Formulation (AVF)

    Derived from the relative velocity formulation

    Uses the absolute velocity as the dependent variable in the momentum equations

    Uses the absolute total internal energy as the dependent variable in the energy equation

    Available for all solvers Se re ated and Cou led NOTE: RVF and AVF are equivalent forms of the N-S equations!

    Identical solutions should be obtained from either formulation with equivalent boundary

    conditions

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    Relative Velocity Formulation

    (Continuity)0=+

    Wt

    r

    (Momentum)

    ( ) rWWWt

    W

    r

    rrrrrrrr

    +++

    )2(

    brp ++=

    &rrrr

    etr b trtr

    =r

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    TermSourceGenerationHeat=Q&

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    Relative Velocity Formulation

    (Relative total internal energy)( )22

    tr 2

    1

    UWee +=

    Viscous stress += 2T

    WWWvr rrr

    (Rothalpy)2

    22 UWpehtr

    +

    +=

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    RVF Accelerations Due to Rotating Frame

    or o s an centr uga acce erat ons are treate as source terms n t e

    momentum equationsrrrrr

    Coriolis

    acceleration

    Centrifugal

    acceleration

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    Absolute Velocity Formulation

    (Continuity)0=+ Wt

    r

    V rrrrrr

    omentumbp

    t++=++

    (Energy)( ) ( ) Qb &rrrrr+++=+

    VFVUpTkhWt

    et

    t

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    Absolute Velocity Formulation

    (Relative total internal energy)2t21Vee +=

    += 2T

    VVVrrr

    3

    (Total enthalpy)2

    2Vpehtr ++=

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    TermSourceGenerationHeatForcesBody

    ==

    QFb&

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    AVF Accelerations Due to Rotating Frame

    rrrrrrr=

    or o s an centr uga acce erat ons re uce to a s ng e term

    Coriolis

    acceleration

    Centripetal

    acceleration

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    Scalar Equations

    ener c sca ar transport equat on n a mov ng re erence rame

    ( ) ( )+=+

    SWt

    r

    tcoefficiendiffusionscalar

    iablescalar var

    =

    =

    The use of the relative velocity in the convective term implies that, for

    =

    - ,

    This form is employed for turbulence models, species and phase transport,

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    e c.

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    Summary of SRF Equations

    wo orms o t e av er- to es equat ons can e app e to pro ems

    (AVF and RVF) RVF only available for the pressure-based solver

    Scalar transport equations can be transformed to moving frame by modified

    convection term

    Source terms may require modification depending on dependent variables

    required (e.g. production term in turbulence model equation may need relative

    velocity gradients)

    Appropriate boundary conditions complete the problem specification

    Inlet / outlet flow boundaries, walls, periodics, etc.

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    SRF Problem Setup

    e w ocus on aspects o mo e setup rect y re ate to pro ems

    Topics SRF geometries (2D, 3D)

    Solver Choices

    Physical Models

    Material Properties

    Boundary Conditions

    Solver Settings

    Initialization

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    SRF Geometries (2D)

    p anar geometr es

    Geometries rotate about axis normal to xy plane with specified origin (periodicboundaries are permitted)

    ax symmetr c, ax symmetr c w t sw r

    Geometries rotate about the x axis

    y

    x

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    Planar Axisymmetric

    x

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    SRF Geometries (3D)

    ee to e ne ot

    rotational axis origin anddirection for the fluid

    Rotationally periodic

    boundaries permitted

    Origin

    Axis of

    r

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    ro a on

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    Choice of Solver for SRF Models

    ame cons erat ons or genera

    flow field modeling apply to SRFsolver choice

    egrega e o ver: ncompress e,

    low speed compressible flows.

    Fans

    Pumps

    Coupled Solvers: high speed

    com ressible flows where Machnumber is above 0.3

    High-pressure axial compressors

    Turbines

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    Turbochargers

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    Velocity Formulation Recommendations

    se w en n ow comes rom a

    stationary domain

    Absolute total pressure, total temperature,

    Use RVF with closed domains (all surfaces

    are moving) or if inflow comes from a

    rotating domain

    Relative total pressure, relative total

    temperature or relative velocities are known

    in this case

    As noted previously, RVF and AVF are

    equivalent, and therefore either can be used

    successfully for many problems

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    disappear with suitable mesh refinement.

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    Disk Cavity Example

    urpose ompare so u ons o a ne us ng ree eren pro emformulations

    Case 1 - Stationary frame, moving walls

    - ,

    Case 3 - SRF, AVF

    Disk cavity air flow study based on the experiments of Pincombe, 1981= = =

    Solutions obtained for following conditions : Cw = Q/b = 1092,Re

    = b2/ = 105

    All cases use the same mesh 20576 uad cells 2D se re ated solver(axisymmetric with swirl), incompressible flow, RKE turbulence model,second order discretization.

    Additional cases were computed using a fine mesh (82,304 cells) to examine the

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    mes n epen ence o e so u ons

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    Disk Cavity Mesh

    Bot wa s rotate

    Inlet tube

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    InletAxis

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    Disk Cavity Stream Function

    Case 1 Case 2 Case 3

    Separated flow

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    Nearly identical flow patterns observed for all three cases.

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    Radial Velocity Profile (r/b = 0.633)

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    Disk Cavity Results

    x a orce an moment resu ts

    Case Mesh Axial Force (103 N) Torque (103 Nm)

    Coarse 6.431 7.231a onary

    Fine 6.141 7.435

    2 (RVF)Coarse

    Fine

    6.681

    6.156

    7.195

    7.444

    3 (AVF)Coarse

    Fine

    6.449

    6.089

    7.241

    7.446

    onc us ons

    All three numerical approaches yield essentially the same results

    Closer agreement is obtained through mesh refinement

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    esu ts emonstrate t e equ va ence o stat onary, , ormu at ons

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    S i C

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    Heat Transfer

    ,

    SRF zone

    Note: BCs for stationary walls must be circumferentially uniform

    ,

    distributions relative to the rotating frame

    Conduction and radiation models can also be enabled with SRF models o e: or con uc ng so s w c are con a ne n a mov ng re erence

    frame, you shouldNOTactivate the Moving Reference Frame option!

    Reason MRF option activates convection terms in the solid, which arent

    relevant to SRF modelin

    ( ) ( ) ( )+=+ s STkCTVCTr

    Solid convection term

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    velocitysolid=sVr

    Fl t U S i C t

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    DPM and Pathline Modeling

    ou can use an

    pathline models for SRFproblems

    art c e pat s are compute

    in the relative frame

    If you want to see particlepat s n t e a so ute rame,

    you can select this option in

    the Pathlines panel.

    o e a par c es mov ng n

    absolute frame may hit wall

    surfaces, since the rotation of

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    Particle injection at fan blade tips

    Fl t U S i C td d FLUENT i i

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    Other Physical Models

    VOF, ASMM, Eulerian (Fluent 6), Cavitation models are all

    compatible with SRF (and MRF, Sliding Mesh) modeling in Fluent

    Exam les: mixin tanks cavitatin um s flows

    Real Gas Model

    Can model specific fluids using non-ideal gas equation of state-

    Two options are available (Fluent 6.1)

    NIST Library (REFPROP) - available fluids include: carbon

    , , , , , ,of refrigerants (e.g. R11, R134a)

    User-Defined Function user can write custom real gas propertylibrary

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    UDF source code available for Redlich-Kwong equation of state

    Fl t U S i C tAd d FLUENT T i i 6 3

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    Boundary Conditions For SRF Models

    u

    Inlet BCs Pressure Inlet

    Shroud

    Velocity Inlet

    Mass Flow Inlet

    Outlet BCs Blade

    Outle

    Pressure Outlet

    Non-reflecting BCs

    Mass flow outlet

    Inlet

    Walls

    Periodics

    Conformal

    Hub

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    Non-conformal Axial Pump IGV

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    Fluid Zone BCs

    se u to se ect rotat ona ax s

    origin and direction vector for rotatingreference frame

    o e: a rec on vec ors s ou e

    unit vectors, but FLUENT will

    normalize them if they are not

    Motion Type for SRF

    Enter rotational speed

    Can use negative value to reverse

    sense of rotation

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    Velocity Inlets

    se or ncompress e, m ycompressible flows when inlet

    velocity is known Can specify absolute or relative

    velocities using Reference Frameoption

    Can specify vector components orma nitude and direction in Cartesianor Cylindrical coordinates

    For 2D, axisymmetric with swirl and3D problems you can specify

    velocitntialuser tan e

    inin,

    =

    += V

    VV

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    locityangular veuserin

    n,

    =

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    Flow Direction

    ow rect on s e ne as

    the velocity vector normalizedby its magnitude Polar)-al(Cylindric

    )(Cartesian

    aarr

    zzyyxx

    d

    d

    ++=

    ++=

    nput a ows artes an or

    Cylindrical-Polar coordinate

    forms

    Frame)(AbsoluteV

    Vdabs

    r

    r

    r

    =

    ote t at t e ow rect ons

    differ in absolute and relative

    frames!

    Frame)(RelativeW

    drel r=

    e oc y r ang e ru e

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    Pressure Inlets

    ressure n ets can e use w t e t er ncompress e or compress e ows

    Definitions of total pressure and total temperature depend on velocityformulation and compressibility:

    Incompressible, AVF+=+=

    2

    22

    2

    2

    1

    p

    ttC

    VTTVpp

    Neglected for

    incompressible flow

    Incompressible, RVF+=+= 2 2

    2 p

    trtrC

    TTWpp

    Incompressible, AVF

    +=

    +=

    1

    22

    11

    21

    21 tt MTTMpp

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    Incompress e, RVF

    += += 2121 rtrrtr TTpp

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    Pressure Inlets

    pec y appropr ate tota pressure

    and total temperature

    If inlet flow is supersonic, you

    such that desired the Mach number

    corresponds toptotal/pstatic

    Specify flow direction vector

    Frame of flow direction depends

    on velocity formulation!

    If using AVF: absd

    Specify other scalar BCs as

    appropriate (energy, turbulence,

    species, etc.)

    re

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    Mass Flow Inlets

    ass ow n ets can e use w t

    incompressible or compressible

    flows

    flux

    Same flow direction options as

    Velocity Inlet

    Specify other scalar BCs as

    appropriate (energy, turbulence,

    species, etc.)

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    Flow Direction and Mass Flow Inlets

    ow o you eterm ne t e ve oc ty magn tu e now ng t e mass ow rate

    and flow direction?

    dVV=r&

    r

    )( ndVnVA

    Vn ===

    V

    tV

    d)( ndA

    mV

    =

    &

    n

    areafaceboundary

    rateflowmass

    =

    =

    A

    m& NOTE: For relative frame, substitute

    relative velocity and direction (W) for

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    velocitytangentialvelocitynormal

    ==tn

    VV absolute velocity (V)

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    Pressure Outlets

    pec y stat c pressure constant or pro e at t e out et.

    Can employ a simple radial equilibrium assumption which computes a radialpressure variation from

    The specified pressure is then

    R

    V

    R

    p =

    assumed to be the hub static

    pressure.

    Appropriate for axial compressors

    an ur nes, w ere e ow sparallel to rotational axis.

    You must also specify appropriate

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    Backflow

    ac ow reverse ow at a oun ary typ ca y occurs w en t e stat c

    pressure in a cell adjacent to a pressure boundary (Pc) forces the flow in adirection opposite to what is intended

    or a ressure n e b < c : oun ary o a pressure s assume o e a

    static pressure for the purposes of determining the flow velocity

    Backflow scalars (temperature, species, etc.) are obtained from the solution b c

    total pressure for the purposes of determining the flow velocity

    Backflow scalars (temperature, species, etc.) are prescribed in the GUI panel

    P < P P > P c

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    cb

    Pressure Inlet

    c b

    Pressure Outlet

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    Backflow

    or a pressure n e , e ow rec on comes rom e ve oc y componen scalculated in the cell

    For a pressure outlet, there are three methods for determining the direction of reversedflow:

    Normal to boundary

    From adjacent cell

    Prescribed direction vector,

    relative to the boundary in the absolute frame if AVF is used

    relative to the boundary in the relative frame if RVF is used

    Recommendations

    As some backflow may occur during the solution process, prescribe reasonable values forall backflow quantities

    Try to minimize (or eliminate) backflow by extending your boundaries further upstream ordownstream

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    Target Mass Flow BC

    or some pro ems t e n et mass ow rate an n et tota pressure an

    temperature are known, and the exit pressure is unknown Example: fans and compressors for which the pressure rise is unknown

    Fluent can address this situation with the target mass flow outlet BC

    How it works

    User sets the exit BC to a pressure outlet

    Desired mass flow rate is prescribed

    As calculation proceeds, exit pressure is adjusted automatically to achieve desired

    mass flow rate

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    Target Mass Flow Methods

    wo met o s are ava a e or comput ng t e pressure or a prescr e mass

    flow Method 1 (best suited for turbomachinery applications)

    ass ow rate at t e out et oun ary s compute an compare to t e es re

    mass flow rate

    A pressure increment is determined based on the required change in mass flowrate the basic behavior is to:

    Increase the exit pressure if computed mass flow > desired mass flow

    Decrease the exit pressure if computed mass flow < desired mass flow

    Method 2 (best suited for incompressible flows)

    Same basic algorithm except the pressure increment is determined from a

    linearized form of Bernoullis equation

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    Target Mass Flow Outlet Setup

    o act vate target mass ow

    outlet , simply enable the Targetmass-flow rate option in pressure

    desired mass flow rate

    ou can spec y t e mass ow

    outlet method in the text interface:

    - -mass-flow-rate-settings>

    enable? set method verbosity?

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    Target Mass Flow Outlet Example

    Convergence HistoryMass flow outlet BCapplied at compressor

    outlet

    Target mass flow:

    . g s

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    Eckardt centrifugal compressor

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    Non-Reflecting Boundary Conditions

    tan ar pressure s or compress e ow x spec c ow var a es at

    the boundary (e.g. static pressure at an outflow boundary)

    Result: pressure waves incident on the boundary will reflect in an unphysical

    Can lead to local errors and convergence degradation

    Effects are more pronounced if the boundary is close to the blade (e.g. truncated,

    Non-reflecting boundary conditions (NRBCs) permit waves to pass through

    the boundaries without spurious reflections

    Turbo-specific NRBCs

    General NRBCs

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    Turbo-Specific NRBCs

    ur o-spec c s are ase on t e axer- es stea y-state ormu at on

    NRBCs are available for pressure inlets and pressure outlets only All pressure boundaries will be affected (cannot selectively activate NRBCs for

    specific boundaries)

    can coexist with other BCs (e.g. mass flow inlet)

    NRBCs require the use of the steady-state, coupled solver Mesh requirements

    The mesh at the pressure inlet/outlet boundaries must be a structured quad (2D)

    or hex (3D) mesh

    Note that away from the boundaries, any mesh type is permissible (e.g. hybrid tri-

    quad mesh is permitted in 2D)

    You can use NRBCs with mixing planes!

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    Using the Turbo-Specific NRBCs

    ur o- pec c s areactivated using the TUI

    select enable? and answeres

    /define/boundary-conditions/non-reflecting-

    bc/turbo-specific-nrbc>enable? show-status

    NRBC Controls (under the set/menu in the TUI)

    discretization option to

    /define/boundary-conditions/non-reflecting-

    bc/turbo-specific-nrbc> enable

    enable non-reflecting b.c.'s [no] yes

    permit first or second orderreconstruction at boundary faces

    under-relaxation sets

    the under-relaxation factor for

    - - -

    bc/turbo-specific-nrbc>

    enable? set/

    initialize show-status

    NRBCs (0 < URF < 1)

    verbosity option to enableprinting of debugging messages

    /define/boundary-conditions/non-reflecting-

    bc/turbo-specific-nrbc>

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    Turbo-Specific NRBC Example: 2D Turbine Vane

    mp e vane c or = . m

    Compressible flow, ideal gas (air)

    Boundary conditions

    n e o a pressure = . a m

    Inlet total temperature = 300 K

    Inlet turbulence intensity = 1%= .

    Hybrid quad-tri mesh used (quad block at inlet)

    Solutions on two meshes compared

    - - Short mesh - mesh truncated near trailing edge - NRBCs required

    Compare solutions on long mesh with solutions on the short mesh with andwithout NRBCs

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    2D Vane Long Mesh

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    2D Vane Short Mesh

    Truncated downstream

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    boundary

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    2D Vane Long Mesh

    Shock wave at

    vane trailing edge

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    2D Vane Short Mesh NBRCs Off

    onstant pressure

    results in incorrect shock

    location

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    2D Vane Short Mesh NRBCs Activated

    Non-reflecting boundary

    conditions permit shockwave to pass t roug t e

    boundary - shock location

    is correctly predicted!

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    General NRBC Formulation

    new genera ormu at on as een eve ope or

    Uses general characteristics-based algorithms from the literature Applies to pressure outlets only

    Benefits

    Can be used for both steady-state and unsteady flows

    No geometry or mesh restrictions

    Limitations

    Can only be used with the coupled-explicit or coupled-implicit solvers (no

    segregated solver implementation at this time)

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    General NRBC User Interface

    pt on se ecte n pressure out et pane

    Permits selected enabling of the NRBCs (unlike Turbo-Specific NRBCs). Two options available

    Pressure at Infinity

    Assumes specified pressure

    is defined downstream of-

    Example: rocket nozzle

    Average Boundary Pressure

    is an average pressure at the

    outlet boundary

    Example: turbine blade row

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    ex t oun ary

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    General NRBCs: 2D Stator Vane

    Constant Pressure BC Non-Reflecting Pressure BC

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    Contours of Static Pressure (atm)

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    Wall Boundary Conditions

    a s en orce zero normavelocity at all wall surfaces

    no slip (zero velocity) forviscous flows

    For moving reference frames,you can specify the wallmotion in either the absolute

    or relative frames

    Recommended specificationof wall BCs for all movingreference frame problems

    lab frame) use zeroRotational speed, Absolute

    For moving surfaces, usezero Rotational s eed,

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    Relative to Adjacent CellZone

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    Conformal Periodic Boundary Conditions

    on orma per o c s requ re t at t e oun ary ace mes

    element match one-for-one on the periodic boundary.

    Rotationally periodic BCs rely on the rotational axis

    .

    Rotationally periodic boundaries can be used in SRF

    problems to reduce mesh size, provided that both the

    geometry and flow are periodic.

    If you are using themake-periodic TUI command,

    make sure you set the rotational axis

    in the Fluid BC anel first beforecreating the periodic boundaries.

    Once the periodic BCs have

    been set, perform a grid check to see

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    correct.

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    Non-conformal Periodic Boundary Conditions

    perm ts t e use o non-con orma rotat ona y per o c s.

    Non-conformal periodics do not require a matching mesh on the boundaries. Coupling of the periodic zones is accomplished using the same algorithms

    employed in non-conformal interfaces.

    Setting up a non-conformal periodic BC is performed in the TUI:

    define/grid-interfaces/make-periodic.

    Shadow zone [()] interface.5

    Rotational periodic? (if no, translational) [yes] yes

    Rotation angle (deg) [0] 90

    Periodic zones

    Create periodic zone? [yes] yes

    grid-interface name [] int1

    er o c ang e

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    Conformal vs. Non-Conformal Periodic Boundaries

    Conformal

    -

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    Pressure-Based Solver Settings

    ressure- e oc y oup ng e o

    Coupled

    Recommended (provides robust, fast convergence) Requires twice the memory relative to other schemes

    SIMPLE, SIMPLEC, PISO

    Use when computer memory is an issue (large mesh)

    Pressure Interpolation

    For highly swirling flows, use PRESTO! scheme

    Other equations - use second order discretization

    Can start with first order for stability, especially for problems with high rotational

    spee s Compressible flows with Pressure-based solvers

    May need to under-relax Density (0.1 is recommended)

    Can also run with energy equation initially turned OFF enable the energy equation

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    after establishing a reasonable, isothermal flow field.

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    Density-Based Solver Settings

    mp c t sc eme s recommen e un ess computer memory s an ssue

    Flux type options Roe-FDS baseline methods

    AUSM can provide enhanced accuracy for strong shocks

    Use first order discretization to begin your calculation, then switch to second

    order when the solution is close to convergence

    Use default Courant numbers as a start (1 for explicit solver, 5 for implicit

    solver)

    For coupled-explicit solver

    Use 4 levels of FAS MultiGrid for most problems

    helps propagate solution more rapidly through the domain

    Use more levels of you have a very large mesh

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    Initialization

    oo n a za on o e so u on s o en e ey o o a n ng rap anrobust convergence of turbomachinery problems

    Less of an issue for

    Fixed flow rate provides stability to the calculation

    Problems with favorable pressure gradients (e.g. turbines)

    Less propensity for reverse flow at boundaries Often critical for

    Compressible flows with adverse pressure gradients (e.g. compressors, diffusers)

    Adverse pressure gradient leads to reverse flows, solution instability

    Use grid interpolation to patch a coarse mesh solution onto a fine mesh.

    Use Full Multigrid (FMG) initialization technique.

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    Solution Interpolation

    roce ure

    Run coarse grid version of your

    model

    r e a a o n erpo a on e

    Set up fine mesh model

    Read interpolation file to initialize

    Advantages

    Can be applied to nearly any

    , Easy to use

    Disadvantage

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    equ res eve opmen o coarse mes

    model

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    Full Multigrid (FMG) Initialization

    n t a zat on opt on n uses t e u u t gr a gor t m n

    FLUENTs Coupled Explicit solver to generate a system of coarse meshes

    Solves the inviscid equations on coarsest mesh, interpolates to next finest, and so

    Inviscid solution used as initial condition for subsequent full Navier-Stokes

    calculation

    Benefits

    Convenient for user (no separate meshes or solutions required)

    ny so ver can e use segrega e , coup e -exp c or mp c

    Permits very large Courant numbers for coupledimplicit solver

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    FMG Interface (TUI) FMG controls can be set in TUI usin

    solve/initialize/set-fmg-

    initialization

    Permits setting of convergence

    ,

    on each coarse grid level, Courant

    number, verbosity

    Once FMG arameters set the

    initialization can be started using the

    text command

    solve/initialize/fmg-

    n t a zat on

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    FMG Initialization Eckardt Rotor

    With FMG

    Initialization

    Without FMG

    Initialization

    ~

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    ,

    Number of iterations reduced by a factorof 5 using FMG initialization!

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    Troubleshooting SRF Problems

    pro ems may e cu t to so ve ecause o arge ow gra ents

    resulting from the rotation of the fluid domain

    May need to use lower under-relaxations than default

    Some things to consider for troublesome cases

    Make sure the mesh quality is good (max cell skewness < 0.9 0.95)

    Use FMG initialization for hard-to-start problems

    Reduce under-relaxation factors and/or Courant numbers

    Consider running the problem as a transient calculation

    Can provide more robust convergence versus the standard steady-state approach

    Use first order discretization in time and about 2-3 time steps per iteration

    Run until steady-state is achieved

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    Summary

    mo e ng s t e s mp est mo e ng approac or rotat ng mac nery

    Applications typically involve a single passage of a rotating machine (e.g.

    single compressor blade row)

    Some example applications are provided in Appendix A

    FLUENT provides two formulations of the Navier-Stokes equations for

    rotating reference frames

    Absolute Velocity Formulation

    Relative Velocity Formulation

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    which are compatible with SRF modeling.

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    SRF Examples

    SRF Examples

    3D propeller fan

    3D cavitating centrifugal pump

    3D propeller fan

    3D cavitating centrifugal pump

    2D axisymmetric flow in a labyrinth seal

    3D flow in a transonic axial compressor blade row

    2D axisymmetric flow in a labyrinth seal

    3D flow in a transonic axial compressor blade row

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    Propeller Fan

    mo e o a our a e prope er an

    Results compared with data from open literature:

    , . . an ang, . ., umer ca nves ga on o e ua er ormanceCharacteristics of a Small Propeller Fan Using Viscous Flow Calculations,Computers and Fluids, 28 (1999), pp. 815-823.

    Solutions obtained for a range of flow rates at 2000 rpm.

    Numerical model Mesh size = 269265 cells (tets + wedges)

    Segregated solver with moving reference frame

    Incompressible flow (air)

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    Realizable k model with non-equilibrium wall functions

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    Propeller Fan - Mesh

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    Comparison to Data: Head Coefficient

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    Comparison to Data: Power Coefficient

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    Fan Flow Field: Flow Coefficient = 0.1Significant flow reversalu stream of fan face

    Static pressure contoursdisplayed on fan surfaces

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    Fan Flow Field: Flow Coefficient = 0.35

    Strong radial outflow

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    Fan Flow Field: Flow Coefficient = 0.5Strong axial outflow

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    Cavitating Centrifugal Pump

    was use to s mu ate ow n a centr uga pump w t cav tat on

    effects

    Geometry based on pump design reported in paper by Hoffman et al. (2001):o man, ., o e , ., r e r c s, ., osyna ., m ar es an eome r ca

    Effects on Rotating Cavitation in Two Scaled Centrifugal Pumps, Proc. 4th

    International Symposium on Cavitation, Pasedena, CA, June 2001.

    TFA pump design used in the present study

    Impeller diameter = 278 mm

    Number of blades = 5

    Speed = 2160 rpm

    Single blade passage modeled with rotationally-periodic boundaries

    Mesh Type: Hex mesh, 284,955 cells

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    Pump Geometry

    diffuser

    impeller

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    inlet tube

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    Pump Model Mesh

    Single blade

    passage

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    Physical / Numerical Models

    tea y-state so ut ons, segregate so ver

    Incompressible flow, SRF, AVF

    Multiphase cavitation model enabled

    Mixture model used

    Primary phase = water (density = 1000 kg/m3)

    Pvap = 2620 Pa; surface tension = 0.0717 N/m,

    Non-condensible gas = 1.510-5

    Secondary phase = water vapor (density = 0.01927 kg/m3,

    viscosity = 8.810-6Ns/m2)

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    Realizible k turbulence model with standard wall functions

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    Case Studies

    on-cav tat ng cases

    Model run over a range of flowrates (100 275 m3/hr) to obtain non-cavitating

    pump curve

    ump ea r se pressure r se pre c e an compare o non-cav a ng a a

    Cavitating Cases Flow rate fixed at design flow (210 m3/hr)

    Exit pressure initial set to 600 kPa to ensure non-cavitating flow

    Exit pressure decreased in 50 kPa increments to gradually develop cavitating

    con t ons

    Predicted head rise vs NPSH compared with data

    NPSH =PinletPvapor

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    Non-Cavitating Flow Comparison with Data

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    Midspan Pressure Non-Cavitating Flow

    Design Flow rate

    03.0=

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    Midspan Relative Velocity Non-Cavitating Flow

    Design Flow rate

    03.0=

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    Cavitating Flow Comparison to Data

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    Cavitating Midspan Pressure

    Exit Pressure: 500 kPa

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    Cavitating Midspan Pressure

    Exit Pressure: 400 kPa

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    Cavitating Midspan Pressure

    Exit Pressure: 300 kPa

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    Cavitating Vapor Volume Fraction

    Exit Pressure: 500 kPa

    Cavitation

    inception

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    Cavitating Vapor Volume Fraction

    Exit Pressure: 400 kPa

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    Cavitating Vapor Volume Fraction

    Exit Pressure: 300 kPa

    Significant

    cavitation on

    pressure side

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    Illustration of Cavitation Induced Separation

    Separation bubble

    downstream of

    vapor cavity

    Exit Pressure

    300 kPa

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    Labyrinth Seal

    ax symmetr c mo e o ve-toot a yr nt sea

    Results compared with experimental data of Millward and Edwards (ASME

    94-GT-56)

    Numerical model Steady state, incompressible flow

    2D axisymmetric with swirl and viscous dissipation

    Se re ated solver

    Realizable k turbulence model

    Solutions calculated over a range of rotational speeds (3000 13000 rpm)

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    Labyrinth Seal - Mesh

    InletOutlet

    -

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    straight seal

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    Labyrinth Seal - Stream FunctionPR = 1.5 , N = 13000 rpm

    Seal leakage flow

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    Labyrinth Seal - Total Temperature

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    Total Temperature

    Windage heating due

    to viscous dissipation

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    Comparison with Data

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    Transonic Axial Compressor

    ranson c compressor rotor otor

    36 blades

    Design conditions

    17188 rpm, PR = 2.1, mass flow = 20.2 kg/s

    Numerical model

    steady-state, compressible flow

    coupled implicit solver

    mesh: ~90,000 hex cells

    standard KE turbulence model inlet TU=3.5%

    inlet profiles from test data

    back pressure varied to obtain speed line

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    Rotor 37 - Mesh

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    Comparison with Data - Pressure Ratio

    Choked mass flow

    predicted: 20.80 kg/s

    data: 20.93 kg/s

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    Pressure Ratio (Choked Flow)

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    Relative Mach Number (Choked Flow)

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    Pressure Ratio (94.3% Relative Mass Flow)

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    Relative Mach Number (94.3% Relative Mass Flow)

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    Centrifugal Compressor

    c ar t otor otor- geometry

    20 blades

    Design conditions

    14000 r m PR = 2.0 mass flow = 5.31 k /s

    Numerical model

    - , Coupled implicit solver

    Mesh: 199,480 hex cells

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    -

    Inlet profile from 2D axisymmetric solution

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    Centrifugal Compressor Mesh

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    Centrifugal Compressor Surface Pressure

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    Centrifugal Compressor esu ts es gn on t on

    Mass flow Pressure Efficiency

    Fluent 5.31 2.08 88.8

    Test Data 5.284 2.066 89.2