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SCISEAL: A CFD CODE FOR ANALYSIS OF FLUID DYNAMIC FORCES IN SEALS Mahesh Athavale and Andrzej Przekwas CFD Research Corporation Huntsville, Alabama OUTLINE N95-13586 Objectives Status Report Code Capabilities Test Results Concluding Remarks and Future Plans Develop Verified CFD Code for Analyzing Seals Required Features Include: - Applicability to a Wide Variety of Seal Configurations such as: Cylindrical, Labyrinth, Face, and Tip Seals - Accuracy of Predicted Flow Fields and Dynamic Forces - Efficiency (Economy) of Numerical Solutions - Reliability (Verification) of Solutions - Ease-of-Use of the Code (Documentation, Training) - Integration with KBS 35 https://ntrs.nasa.gov/search.jsp?R=19950007173 2020-04-03T13:47:06+00:00Z

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Page 1: OUTLINE - NASA · 19. Turbulent compressible flow and heat transfer in turbine disk cavities Athavale et.al. 20. 3-D driven cavity flow with lid clearance and axial pressure gradient

SCISEAL:A CFD CODE FOR ANALYSIS OF FLUID DYNAMIC FORCES IN SEALS

Mahesh Athavale and Andrzej Przekwas

CFD Research CorporationHuntsville, Alabama

OUTLINE

N95-13586

• Objectives

• Status Report

• Code Capabilities

• Test Results

• Concluding Remarks and Future Plans

Develop Verified CFD Code for Analyzing Seals

Required Features Include:

- Applicability to a Wide Variety of Seal Configurationssuch as: Cylindrical, Labyrinth, Face, and Tip Seals

- Accuracy of Predicted Flow Fields and Dynamic Forces

- Efficiency (Economy) of Numerical Solutions

- Reliability (Verification) of Solutions

- Ease-of-Use of the Code (Documentation, Training)

- Integration with KBS

35

https://ntrs.nasa.gov/search.jsp?R=19950007173 2020-04-03T13:47:06+00:00Z

Page 2: OUTLINE - NASA · 19. Turbulent compressible flow and heat transfer in turbine disk cavities Athavale et.al. 20. 3-D driven cavity flow with lid clearance and axial pressure gradient

SCIENTIFIC CODE DEVELOPMENT

Task 1: Develop a 3D CFD Code (SCISEAL) forCylindrical Seals

- for Annular, Tapered, Stepped- Verification of Code Accuracy- Rotordynamic Coefficient Calculations

Future Tasks: Augmentation of SCISEAL

Incorporation of Multi-Domain CapabilitiesExtension to Labyrinth, Damper, Face, andTip Seals

Note: Starting CFD Code = REFLEQS (developed by CFDRCunder a contract from NASA MSFC/ED32)

STATUS: 1992 WORKSHOP

. Numerical Methodsin 3D Code

. Colocated Grids- High-Order Schemes. Rotating and Moving Grid Systems

Rotordynamic Coefficient Calculation Methods(CFD Solutions)

- Circular Whirl- Moving Grid (numerical shaker)

Seal Specific Interface

- Grid Generation. Pre-Processing

36

Page 3: OUTLINE - NASA · 19. Turbulent compressible flow and heat transfer in turbine disk cavities Athavale et.al. 20. 3-D driven cavity flow with lid clearance and axial pressure gradient

CURRENT STATUS

Augmentation Effort on SCISEAL:

• Implementation of Small Perturbation Model for Rotordynamics

Treat Eccentric as well as Centered SealsEfficient, Economic Solutions

• Addition of 2-Layer Turbulence Model

Very Small Seal Clearances --> Very Small y+

Standard k-E Model Inaccurate, Low Re Model Stiffness Problems, etc2-Layer Model Overcomes this Difficulty to Significant Extent

Code Validation

Rotordynamics: Long & Short Annular Seals, Eccentric SealsLabyrinth Seal Flow ComputationsEntrance Loss Coefficients

CURR, ENT CODE CAPABILITIE S

• Seals Code has:

- Finite Volume, Pressure-Based Integration Scheme- Colocated Variables with Strong Conservation

Approach- High-Order Spatial Differencing - up to Third-Order- Up to Second-Order Temporal Differencing- Comprehensive Set of Boundary Conditions- Variety of Turbulence Models (k-E, Low Re k-_,

multiple scale k-_, 2-Layer Model), Surface RoughnessTreatment

- Moving Grid Formulation for Arbitrary Rotor Whirl- Rotordynamic Coefficient Calculation Methods, CFD

Based Centered Seals: (i) Circular Whirl (ii) NumericalShaker

- Small Perturbation: Centered & Eccentric Seals

37

Page 4: OUTLINE - NASA · 19. Turbulent compressible flow and heat transfer in turbine disk cavities Athavale et.al. 20. 3-D driven cavity flow with lid clearance and axial pressure gradient

=

SEAL SPECIFIC CAPABILITIESI I II

• GUI and Preprocessor- Geared for Seals Problems

• Easy, Quick Geometry Definition and Grid Generation

• Four Types of Cylindrical Seals:

- Annular, Axial Step-Down, Axial Step-Up,and Tapered

• Pull-Down Menus for Problem Parameter Specification

• One Line Commands for

- Automatic Grid Generation- Integrated Quantities: Rotor Loads, Torque, etc.- Rotordynamic Coefficients

ROTORDYNAMIC COEFFICIENTSIII I II I I

• Relation Between Fluid Reaction Forces and Rotor Motion

Stiffness Damping

• Fy

M w M_

Inertia (mass)

38

Page 5: OUTLINE - NASA · 19. Turbulent compressible flow and heat transfer in turbine disk cavities Athavale et.al. 20. 3-D driven cavity flow with lid clearance and axial pressure gradient

- Rotor Undergoes Circular Whirl- Rotating Frame _ Quasi-Steady Solution- CFD Solutions at Several Whirl Frequencies- Pressure Integration to Yield Rotor Loads- Curve Fit to Force vs Whirl Frequency

*For Centered Rotor with Skew Symmetry Coefficient Matricesz

Y

ROTORDYNAMIC ,COEFFICIENTS

° Numerical Shaker Method

- Rotor Motion Along a Radial Direction- Time-Dependent Solutions- Moving Grid Algorithm for Grid Deformation- Time-Dependent Pressure Loads --> Rotordynamic

Coefficients- Can Treat Centered as well as Eccentric Seals- Time Accurate Solutions -> Computationally Slower

39

Page 6: OUTLINE - NASA · 19. Turbulent compressible flow and heat transfer in turbine disk cavities Athavale et.al. 20. 3-D driven cavity flow with lid clearance and axial pressure gradient

ROTORDYNAMiC COEFFICIENTCALCULATIONS

Small Perturbation Method

- For Centered or Eccentric/Misaligned Seals- Rotor Undergoes Circular Whirl with Very Small Radius. Resulting Perturbations in Flow Variables:

¢=¢0 +E01Generate Oth and 1st Order Flow Equations

. Use Fournler Series In Time for Perturbations:-- Complex Form of 1st Order Variables;-- Flow Equations are Quasi-SteadyComplex Flow Perturbations Solved at Several WhirlFrequencies

- Integrate Pressure Perturbations for Rotor Loads- Curve Fit for Rotordynamic Coefficients

t=nT t = nT÷T/8 t. nT÷TI4 t,, nT ÷ 3T/8

t.nT+T/2 t. nT,_ST/B t - nT • 3T/4

Time-dependent solutions of the perturbation pressure

- 0.0, Plane at half seal length, .Q-.2.0(o

t. nT ÷TTR

Page 7: OUTLINE - NASA · 19. Turbulent compressible flow and heat transfer in turbine disk cavities Athavale et.al. 20. 3-D driven cavity flow with lid clearance and axial pressure gradient

tm nTt • nT+T/8 t - nT+TN t - nTq_3T/e

t = nT+T/2 t - nT*ST/B t • nT_TI4 t : nT+Tr_

Time-dependent solutions of the perturbation pressure

c - 0.7, Plane at half seal length, _- 2 Se)

2-LAYER TURBULENCE MODEL

• Small Seal Clearances -_ very Low y+ Values

• Standard Wall Functions _ Inaccurate

• Low Re k-E Model for Very Low y+- can generate very stiff systems

2-Layer Model Uses

- wall functions for large y+

- Low Re k-_ model for very low y+

• A Buffer Zone Used to Smoothly Merge the TwoTreatments

• Model has been Tested for a Number of Seal andRotating Flow Problems

"Work Performed by Drs. Avva and Lai of CFDRC

41

Page 8: OUTLINE - NASA · 19. Turbulent compressible flow and heat transfer in turbine disk cavities Athavale et.al. 20. 3-D driven cavity flow with lid clearance and axial pressure gradient

SAMPL E RESULTS

Computation of Flow in Enclosed RotorSystem (Dailey and Nece)

b st a for

rotor

Torque coefficients,

Experimental value ~ 4x10 "3

k-e with wall function 2-layer model

near wall

16

0.7

0.04

Cm

3.58x10 .3

5.28x10 -3

S.SgxlO-3

near well C my+

3.9x10 .321

0.7 4.64xl 0.3

0.04 4.25x10"3

CODE VALIDATION AND

DEMONSTRATION

Code has been Validated for a Large Number of BenchmarkProblems

- A List of 29 Relevant Problems Included in the InterimReport

• Extensive Validation Effort Conducted for Practical Seals:

- Annular and Tapered Seals- Labyrinth Seals

Annular Incompressible Seals (Dietzen and Nordmann, 1987)

i Long Incompressible Seals (Kanemori & Iwatsubo, 1992)

Eccentric Annular Seal (Simon & Frene, 1991)Annular and Tapered Gas Seal (Nelson, 1985)Labyringth Seals Planar, (Wittig et al, 1987)Labyrinth Seals, Tapered Knives; stepped(Tipton et al, 1986)

42

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.

2.

.

1

1

.

7.

.

9.

10.

13.

14.

15.

VALIDATION CASESI I

Fully-developed flow in a pipe and channel.

Developing laminar flow in a narrow annulus between two cylinders.Slug flow at inlet, fully-developed flow at outlet.

Laminar flow between rotating cylinders. Below critical Taylor number,tangential flow only.

Flow between two cylinders, rotating Inner cylinder. Taylor vortex flow,Laminar and turbulent.

2-D driven cavity flow, Reynolds number up to 10,000. Comparisons withnumerical results by Ghia eLai.

3-D driven cavity flow.

Couette flow under different pressure gradients. With and without heattransfer.

Planar wedge flow in a slider bearing.

Laminar flow over a back step. Reattachment length comparison withexperiments by Armaly and Durst.

Laminar flow in a square duct with a 90 ° bend. Comparison withexperimental data by Taylor et.al.

Shock reflection over a flat plate.

Turbulent flow in a plane channel. Fully-developed solution at exitcompared with experiments by Laufer.

Turbulent flow induced by rotating disk in a cavity. Comparison withexperiments by Dally and Nece.

Centripetal flow in a stator-rotor configuration. Comparison withexperiments by Dibelius et.al.

Flow between stator and whirling rotor of a seal. 2-D results for 0, 0.5, andsynchronous whirl frequencies

43

Page 10: OUTLINE - NASA · 19. Turbulent compressible flow and heat transfer in turbine disk cavities Athavale et.al. 20. 3-D driven cavity flow with lid clearance and axial pressure gradient

VALIDATION CASES

16. Flow over a bank of tubes.

17. Turbulent flow in an annular seal. Comparison with experiments byMorrison et.al.

18. Turbulent flow in a 7-cavity labyrinth seal. Comparison with

experiments by Morrison et.al.

19. Turbulent compressible flow and heat transfer in turbine disk cavitiesAthavale et.al.

20. 3-D driven cavity flow with lid clearance and axial pressure gradient.Control of flow through vortex imposition.

21. Flow in cavities on a rotor for an electrical motor. Interaction of Taylorvortices with driven cavity flow.

22. Flow in infinite and finite length bearings (without cavitation).Comparison of calculated attitude angles with theory.

23. Flow and rotordynamic coefficient calculation for straight,incompressible seals. Comparison with results from other numericaland analytical solutions; Dietzen and Nordmann.

24. Flow and rotordynamic coefficients in tapered compressible flow seals.Comparison with bulk-flow theory results; Nelson.

25. Rotordynamic Coefficients in a long annular incompressible flow seal.Comparison with experimental data; Kanemori and Iwatsubo.

26. Calculation of entrance loss coefficients in the entrance region of ageneric seal. Effect of flow and geometry on the loss coefficientvalues; Athavale et.al.

27. Flow coefficient and pressures in a 5 cavity, straight knife, look-throughlabyrinth seal. Comparison with experimental data ; Witting et.al.

28. Flow coefficients and pressures in a 3 cavity, tapered knife, look-through labyrinth seal. Comparison with experimental data; Tiptonet.al.

29. Flow coeffients and pressures in a 2 cavity, straight-knife, stepperdiabyyrinth seal. Comparison with experimental data; Tipton et.al.

44

Page 11: OUTLINE - NASA · 19. Turbulent compressible flow and heat transfer in turbine disk cavities Athavale et.al. 20. 3-D driven cavity flow with lid clearance and axial pressure gradient

LONG ANNULAR SEALS

• Experimental Data by Kanemorl & Iwatsubo (1992)

• R = 39.656 mm, L = 240 mm, Rotor Speed [] 600-3000 rpmClearance = 0,394 mm, _p = 20 kPa - 900 kPaSpecified Inlet Loss Coefficient, Ra [] 1000-18000

• Various Models Checked:

- Whirl Method, Perturbation Method- Low Re k-_ Model, 2-Layer Model- 20x15x30 grid

DIRECT & CROSS-COUPLED STIFFNESS

1.0Bd)71 K 1.0EtO7-

1.0E,06 _' ,.._ ._.,,.._ _

1.0E_05 1

(-ve_//

1.0E+041.0Ed)4 1.0_ 1 1.0E_51.0Ed_

AP Pa

k

..._..t_..._._f _'''r'_ _

Ref PmNnt rpm

a -'-"'-- 1080- - - 1980

• _ _ 3000

I ]

1.0E_4 1.0E+05 1,0E+06AP Pa

Symbols:Lines:

Experimental Data by Kanemori and IwatsuboNumerical Results from SCISEAL

45

Page 12: OUTLINE - NASA · 19. Turbulent compressible flow and heat transfer in turbine disk cavities Athavale et.al. 20. 3-D driven cavity flow with lid clearance and axial pressure gradient

DIRECT & CROSS-COUPLED DAMPING

1.0_..05 "-C 1.0E*05

Ns/m

1.0E+0.4

. • _.._,_ Nstm

: " •_,____--__>._-_1.0Ed)4

Ref Present rpm

g ------- 1080

__ _ --- 1980A _ _ 3000

I"OE_I. OE_4 1. _:_05 1.0_Ap Pa

C

._.,=._._&_._._...___ _.-..#-----*** ..2 _ ..-*------t-----_- ---_

• • • • • m

Ref Present rpm

a ---'---" 1080- - - 1980

,& -- -- 3000I

1.0E+03.0E+04 1.0E+05&P Pa

1.0E_06

::z

DIRECT MASS (INERTIA) ,

1.0E_3

kg

1.05d_

1.0E_01

1.0E_04

M

Ref. Present rpm[] _ 10800 ....... 1980_, ........ 3000

i

1.0Ez.0S

z_PPa

I

1.0E_06

_ _ mr1

46

Page 13: OUTLINE - NASA · 19. Turbulent compressible flow and heat transfer in turbine disk cavities Athavale et.al. 20. 3-D driven cavity flow with lid clearance and axial pressure gradient

ECCENTRIC SEAL

• Experimental Data by Falco et al (1984)Numerical Data by Nordmann (1987), Simon & Frene (1991)

Radius = 80 mm, Length = 40 mm, E - 0. 1-->0.74000 rpm, Ap [] 1MPa, Entrance Loss Coefficient [] 0.5

Physical Models

- Standard k-E Model- Small Perturbation Method- 12x6x30 grid

DIRECT STIFFNESS

COEFFICIENT, Kyy, Kzz

8. r_06,

N/m

6.Ed)6-

4.E_06_

2.F=_6-

Kyy e.r:,e6-Wm

6E _.06-

QCO0

4. E+06-

_.Ed]

_= o_4 _s o'e ooGO

Eccentricity, e

Kzz

_E--_ m

O Experiment, Faleo

- _ Neleon and Nguyen...... 81mort and Frene

Nordmann

I !• = Q'4 o_s oeEccentrlclW, e

47

Page 14: OUTLINE - NASA · 19. Turbulent compressible flow and heat transfer in turbine disk cavities Athavale et.al. 20. 3-D driven cavity flow with lid clearance and axial pressure gradient

CROSS-COUPLED STIFFNESS,

3. 0E+08"

2.5Ed)6"

Him9_0Ed)6"

1.5Ed_"

5.0E_05-

O.O-OO

Kyz

O Experiment, FetcoSCISEAL

---Nelson and NguyenSimon and FreneNordmenn

5. N/Ed)6m_ Kzy

Eccentricity e (10 (12 (14 (16Eccentricity g

Q8

DIRECT DAMPING, Cyy, Czz

2. 0E+04 - 2. 01_l_-

1.5_- 1.55,04-

1._., 1._-

5.01N03-5. OB_-O3"

O.B,O0 0_2 11'4 (16 Q8Eccentricity,

-_ Nelson and Nguyen...... Simon and Fmne

Nordmsnn

QO _2 (1'4 0.6Eccentricity,

I

Q8

48

Page 15: OUTLINE - NASA · 19. Turbulent compressible flow and heat transfer in turbine disk cavities Athavale et.al. 20. 3-D driven cavity flow with lid clearance and axial pressure gradient

CROSS-COUPLED DAMPING, C z, Cz

N-slm

500-

0OO

41XO-

CyzN-s/m

==_._ .... _,K_'_. _ _"_

SClSEAL 1000-m. _ Nelson and Nguyen

...... Slmon end Frene..... Nordmenn

Eccentdcity, e

Czy

Eccentricity, E

I

Q8

DIRECT,,INERTIA Myy, M:,?Ii ii

8"

Kg

6-

4-

2-

0QO

8-

MyyKg

" .-..___.- _-'_---_.-._'_

Eccentricity, z

Mzz

_ ._....m.. _ ._ _P

2 _ SClSEAL- _ Nelson and Nguyen

..... Slmon and FreneNordmsnn

Ioo o_2 o_4 o_6 08Eccentricity,

49

Page 16: OUTLINE - NASA · 19. Turbulent compressible flow and heat transfer in turbine disk cavities Athavale et.al. 20. 3-D driven cavity flow with lid clearance and axial pressure gradient

''7

:z

STRAIGHT LABYRINTH SEAL

• Experimental Data by Wittig et al (1987)

• 5 Cavity, Planar Look Through Seal

• Physical Models

- 30x30 Cells In each Cavity, 8/12 Cells in Gap. Compressible Flow, Standard k-s Model- Specified Pressure Ratio Across Seal

• Results: Numerical Results Compared withExperimental Data

. Pressure Along the Seal Length for Different TipGaps

- Mass Flow Rates at Different Tip Gaps and PressureRatios

RESULTS FOR STRAIGHT LABYRINTHSEAL

1.0_

08

06-

(14

(12-

(10

ii i

Pressure

_Exoerlmentai data

_\\_ • tip gap = 0.5 mm\\\_ . tip gap : 1.02 mm

• tl gap=151mm

2:52 mmp "

"_ t _ I t0 2 3 4 5cavity number

1.0-

nB-

(16-

(14-

Mass Flow

Experl .mentaldata_ymDOlS:• seal gap =0.5 mm• seal gap = 1.51 mm• seal gap = .2.52 mm

(12-

(10- _, 30to - 10 15""seal pressure ratio

==c:>

5o

Page 17: OUTLINE - NASA · 19. Turbulent compressible flow and heat transfer in turbine disk cavities Athavale et.al. 20. 3-D driven cavity flow with lid clearance and axial pressure gradient

STEPPED LABYRINTH SEAL

• Experimental Data by Tipton et al (1986)

• 2 Cavity, Planar, Stepped Labyrinth Seal

• Physical Models:

- CompressibleFlow, Specified Pressure Ratio- Standard k-_ Model

- 26x53, 26x62 Cells in Cavities; 10 Cells in Tip Gap

• Results: Numerical Results Compares withExperimental Data

- Pressure Along Stator and Rotor Surfaces at OnePressure Ratio

- Mass Flow Rates at Different Pressure Ratios

*Work Performed by Dr. Makhijani of CFDRC

RESULTS FOR STEPPED LABYRINTHSEAL

10

0.8-

8.6

0.4

0.2

Pressure

Mass Flow

t,"

Experimental 0._ 'Numerical Experimental

• Numerical0.m

zHorizontal Distance from Inlet Plane, m

IOI H _'=

II

=i= a¢_

I I_ 5 6Pressure Ratio (Pinlet/Pexit)

51

Page 18: OUTLINE - NASA · 19. Turbulent compressible flow and heat transfer in turbine disk cavities Athavale et.al. 20. 3-D driven cavity flow with lid clearance and axial pressure gradient

ENTRANCE LOSS COEFFICIENTS

• Measure of Flow Losses at Entrance Region

• SClSEAL Used to Compute P,with CFD Solution

Variation of P,with

. Axial Reynolds Number Flow- Seal Clearance-to-Radius Ratio. Entrance Gap-to-Clearance Ratio

entrance_

region

seal

Physical Models

. Incompressible Flow, Standard k-_ Model- Fully Developed Flow Upstream, Pressure

Downstream50 Cells In Axial Direction, 5 in Clearance, 30 or 50 in

Entrance Region

FLOW GEOMETRYFOR ENTRANCE LOSS

Inlet

Entrance .._, _.,"-" / # ' "- I_

Sealv

Clearance

52

Page 19: OUTLINE - NASA · 19. Turbulent compressible flow and heat transfer in turbine disk cavities Athavale et.al. 20. 3-D driven cavity flow with lid clearance and axial pressure gradient

RESULTS

Table 1. Entrance Loss Coefficients, Radius/Clearance = 50

Entrance Gap/Clearance = 50

Uax rrVs Reax

10.814 1,037716.232 121.619 2074626.942 25854

J

0.4710.4310.4140.466

....,,

Entrance'O__NClearance = 100

Uax rrVs Reax _,

10.82 10384 0.49010.24 15584 0.48821.66 20785 0.48227.06 25970 0.48

Table 2. Entrance Loss Coefficients, Radius/Clearance = 100

Entrance Gap/Clearance = 50

Uax nYs

10.8016.5621.59526.6732.2743.062

Reax

5181794510361127961548420667

0.5620.540.5260.510.4930.478

Table 3. Entrance Loss

Entrance Gap/Clearance = 100

Uax m/s

10,79716.17621.5526.93432.2442.533

Reax

5167 0.5677761 0.55810339 0.5512664 0.5415469 0.537

20408 0.524

Coeffidents, Radius/Clearance = 150

Entrance Gap/Clearance = 50

Uax rrVs Reax

10.82 346116.19 517821.49 687426.74 855332.25 1031546.33 1546164.467 20630

0.660.650.6470.6370.6280.6060.595

Uax m/s

i

Entrance O_Clearance. 100

Reax

10.75 343816.09 514621.47 687426.81 855332.176 1029247.87 1531564.165 20630

0.680.660.650.6480.540.630.624

RELATED CFD RESULTS

REFLEQS-3D Used for Rotating Flows

- Flows in Inducer & Centrifugal Impeller (For MSFCPump Consortium)

- REFLEQS-3D & SCISEAL have Similar NumericalTechniques

• SCISEAL in Narrow, Long Channels

- Suitable for Cooling Channels In Rocket Nozzles- Heat Transfer & Flow Calculations

53

Page 20: OUTLINE - NASA · 19. Turbulent compressible flow and heat transfer in turbine disk cavities Athavale et.al. 20. 3-D driven cavity flow with lid clearance and axial pressure gradient

z

k •

54

Page 21: OUTLINE - NASA · 19. Turbulent compressible flow and heat transfer in turbine disk cavities Athavale et.al. 20. 3-D driven cavity flow with lid clearance and axial pressure gradient

_..,lllr1_,,_. I _'.,trlI11_,, "_ ............... :::: - .

Secondary flow patterns In a long, narrow channel

(Velodty vecto_sizeand c_ou-Jecth_ dzw notto Jcale)

CONCLUDING REMARKSI I

• A 3D CFD Code, SClSEAL, Being Developed and Validated

- Current Capabilities Include Cylindrical Seals

• State-of-the-Art Numerical Methods

- Colocated Grids

- High-Order Differencing

- Turbulence Models, Wall Roughness (in progress)

• Seal Specific Capabilities

- Rotor Loads, Torques, etc

Rotordynamice Coefficient Calculations

- Full CFD Based Solutions - Centered Seals- Small Perturbations Method - Eccentric Seals

Extensive Validation Effort

55

Page 22: OUTLINE - NASA · 19. Turbulent compressible flow and heat transfer in turbine disk cavities Athavale et.al. 20. 3-D driven cavity flow with lid clearance and axial pressure gradient

al

=

WORK PLANS FOR NEXT YEAR

• Consolidate Current Models

• Include Multi-Domain Solution Methodology

Efficient Solutions for Complicated Flow Geometries-- entrance region & seal clearance- stepped and straight labyrinth seals- face seals-- tip seals-- conjugate heat transfer

Increases Code Flexibility

Technology Already Developed but RequiresAdaptation and Testing for Seals

• Continue Work on Labyrinth Seals

ValidaUon/Demonstration for Practical Seal

Configurations

Entrance Loss Calculations =_,_ __ ...... ,

Single Domain Grid

Multidomain Grid

56

Page 23: OUTLINE - NASA · 19. Turbulent compressible flow and heat transfer in turbine disk cavities Athavale et.al. 20. 3-D driven cavity flow with lid clearance and axial pressure gradient

Stepped Labyrinth Seal grids

......................... _ ............. L ......

.............................. Illlllllt_

iiiiitlll ill .....

Single Domain grid

B

Mullidomlin grid

57

Page 24: OUTLINE - NASA · 19. Turbulent compressible flow and heat transfer in turbine disk cavities Athavale et.al. 20. 3-D driven cavity flow with lid clearance and axial pressure gradient