Boundary Layer Transition and Trip Effectiveness on an Apollo Capsule in the JAXA High Enthalpy Shock Tunnel (HIEST) Facility LindsayC.Kirk∗,RandolphP.Lillard† NASAJohnsonSpaceCenter,Houston,TX77058 JosephOlejniczak‡ NASAAmesResearchCenter,MoffettField,CA94035 HideyukiTanno§ JAXAKakudaSpaceCenter,Kakuda,Miyagi,9811525Japan ComputationalassessmentswereperformedtosizeboundarylayertripsforascaledApollocapsulemodelinthe HighEnthalpyShockTunnel(HIEST)facilityattheJAXAKakudaSpaceCenterinJapan. Forstagnationconditions between2MJ/kgand20MJ/kgandbetween10MPaand60MPa,theappropriatetripsweredeterminedtobebetween 0.2mmand1.3mmhigh, whichprovidedk/δ valuesontheheatshieldfrom0.15to2.25. Thetrippedconfiguration consistedofaninsertwithaseriesofdiamondshapedtripsalongtheheatshielddownstreamofthestagnationpoint. Surfaceheatfluxmeasurementswereobtainedonacapsulewitha250mmdiameter,6.4%scalemodel,andpres- suremeasurementsweretakenataxialstationsalongthenozzlewalls. Atlowenthalpyconditions,thecomputational predictionsagreefavorablytothetestdataalongtheheatshieldcenterline.However,agreementbecomeslessfavorable as the enthalpy increases conditions. The measured surface heat flux on the heatshield from the HIEST facility was under-predictedbythecomputationsinthesecases. Bothsmoothandtrippedconfigurationsweretestedforcompar- ison, and a post-test computational analysis showed that k/δ values based on the as-measured stagnation conditions rangedbetween0.5and1.2. Trippedconfigurationsforboth0.6mmand0.8mmtripheightswereabletoeffectively triptheflowtofullyturbulentforarangeoffreestreamconditions. I. Introduction A 6.4% scale model of the Apollo entry capsule was tested in the High Enthalpy Shock Tunnel (HIEST) facility at the Japan Aerospace Exploration Agency’s Kakuda Space Center (JAXA-KSC). A range of stagnation enthalpy and stagnation pressureconditionsweretestedtogatherdatatohelpimprovecomputationalsimulationaccuracyathighenthalpyconditions, toassessboundarylayertripeffectivenessathighenthalpyconditions, andtofurtherinvestigateanomaloussurfaceheatflux datapreviouslyobtainedintheHIESTfacilityandotherhighenthalpyfacilitiessuchastheT5facilityattheCaliforniaInstitute ofTechnology2. ThedetailsoftheHIESTtestcampaignwiththeApollocapsuleexaminedinthisworkhavebeenreportedby Tannoet. al. inaseparatepublication3. ForreentryvehiclesreturningthroughEarth’satmosphereonhighenergytrajectories,suchasthosefromthemoonorMars, chemistryeffectsplayasubstantialroleintheaerodynamicheatingtothevehiclesurface**REFERENCE**. Computational tools are able to predict the heating environments for these high enthalpy conditions where chemistry is important, but the accuracy of and the uncertainties inherent in these predictions are generally less understood than those of lower enthalpy conditions because there is less quality validation data available at the higher energy conditions. Ground test facilities are limited in the conditions that can be reached at higher pressure and enthalpy conditions, so much of the validation data for flight-like high enthalpy conditions comes from flight test data. Flight test data is able to measure the flight environment, but understanding the data and quantitatively assessing the uncertainties in computational predictions is hindered by larger measurement uncertainties such as those due to trajectory uncertainties, instrumentation installation uncertainties, and flight datareconstructionuncertainties. **ADDMOREHERE** ∗AerospaceEngineer,AIAAMember †Chief,ThermalDesignBranch ‡Manager,OrionMPCVAerosciences §Associate Senior Researcher, Space Transportation Propulsion Research and Development Center, Space Transportation Mission Directorates, [email protected],AIAAmember 1of11 AmericanInstituteofAeronauticsandAstronautics TheanalysispresentedherewillfocusonthecomputationalanalysisofthedataobtainedattheHIESTfacility. Apretest analysis supported the design of the model and the trip insert, which was comprised of a series of “pizza box” trip elements andlocateddownstreamofthestagnationpoint. Thepost-testanalysisconsistsofanevaluationofthepredictivecapabilityof thecapsulesurfacequantitiesforasmoothconfigurationathighenthalpyconditionsandanassessmentoftheeffectivenessof thetripsthatweredesignedinthepretestanalysis. Anadditionalassessmentoftheaccuracyofthepredictedpressuresonthe nozzlewallisincludedtohelpunderstandthecomparisonsonthecapsulesurface. A. HIESTFacilityOverview TheHIESThighenthalpyfacilityattheJAXA-KSCfacilityisafreepistonshock tunneldesignedtosimulatetherealgaseffectsathightemperaturessuchasthose seenbyspacecraftreenteringtheatmosphere1. Thefacilitymeasuresjustover 90 meters in length and has both a conical nozzle and a contoured nozzle to reach a range of velocities from 3 km/s to 7 km/s. The HIEST can operate at conditionsuptoamaximumstagnationenthalpyof25MJ/kgandamaximum stagnation pressure of 150 MPa, and test times are at least 2 msec. Figure 1 showstheshocktubeandinertiamassoftheHIESTfree-pistonshocktunnel. II. NumericalSimulationMethodology The computational analysis for this work was performed using the Data- Parallel Line Relaxation (DPLR)4 software v4.02.2 developed at the NASA Ames Research Center. DPLR is a finite-volume Navier-Stokes solver that is capable of modeling thermal and chemical non-equilibrium, both of which are important for predicting reentry flight conditions and high enthalpy flows in ground test facilities. All simulations for this analysis were completed using a five species air chemistry model, and diffusion and transport properties were modeledusingtheSelf-ConsistentEffectiveBinaryDiffusion(SCEBD)model and Gupta-Yos transport models, respectively. To reduce complexity, the noz- zleandcapsulesimulationswererunindependently. Bothsimulations,however, usedthesamephysicalmodelsinthesimulationforconsistency. A. NozzleCalculations Figure1.HIESTShockTubeFacility Freestream conditions for the Apollo capsule simulations were extracted from axisymmetricnozzlesimulationswheretheflowwasexpandedthroughthenoz- zlethroatfromasubsonicartificialwallextension.Theflowforeachrunwasas- sumedtobeinchemicalequilibriumatthestagnationpressureandenthalpypro- videdbythetestfacility. Equilibriumconditionsforafive-speciesairchemistry modelwerecomputedusingChemicalEquilibriumwithApplications(CEA)5. The grid resolution for the nozzle simulations was 178 cells in the axial direction and 600 cells in the radial direction for a totalof approximately105,000 cells. Figure2 showsa samplenozzlesimulation fora stagnationpressurefor 45MPa anda stagnationenthalpyof20MJ/kg. Astudyofthenozzlewallcatalycitywasperformedusingbothcatalyticandnon-catalyticboundaryconditions.Theresults showed that, for a case with a stagnation enthalpy of 20 MJ/kg and a stagnation pressure of 20 MPa, the wall catalycity had littleeffectonthecorefloworthewallboundarylayerparameters,specificallytheheightandmomentumthicknessReynolds number,Re . Asaresult,allsubsequentnozzlesimulationswererunwithanon-catalyticboundarycondition. θ A similar study of the effects of the chosen turbulence model on the core flow was completed using a laminar flow as- sumptionaswellasaturbulentflowassumptionusingtheSpalart-Allmaras(SA)andShearStressTransport(SST)turbulence models. Figure3showstheeffectofeachofthesemodelingassumptionsontheMachnumberattheassumedmodellocation. LittledifferenceintheMachnumberwasobservedbetweenthetwoturbulentsolutions,soallsubsequentsimulationswererun withtheSSTturbulencemodel. 2of11 AmericanInstituteofAeronauticsandAstronautics Figure2.NozzlesimulationforP0=45MPaandH0=20MJ/kgwithMachnumberontopandtranslationaltemperatureonbottom. Figure3.NozzleTurbulenceModelEffectonCoreMachNumber 3of11 AmericanInstituteofAeronauticsandAstronautics B. CapsuleCalculations ThetestarticleusedinthetestserieswasanaxisymmetricidealizedmodeloftheApollocapsulewithheatfluxinstrumentation along the heatshield centerline and off-centerline on the leeside of the heatshield. All simulations were run with a smooth, heatshield only, half-body grid to reduce the computational cost. The heatshield only approximation was made due to the lack of instrumentation on the model backshell, and all conditions were tested at 28◦ angle of attack with no side slip so a symmetricalsimulationwasalsoanappropriateapproximation. Thisresultedinagridsizeofapproximately2.5Mcells,with 160cellsintheoff-bodydirection. Thenozzlesimulationsshowedthattheflowatthelocationofthetestarticlewasapproximatelyuniformacrossthenozzle crosssection,andthiswasseeninFigure3. Asaresult,thefreestreamconditionsforthecapsulesimulationswereextractedat thenozzlecenterline. Figure4showstheassumedmodellocationwithinthenozzle. Figure4.Assumedtestarticlelocationwithinthenozzle Once the freestream conditions for each run were extracted from the nozzle simulations, the capsule simulations were completed assuming both laminar and turbulent flow assuming an isothermal wall boundary condition of 300 K. Turbulent simulationswererunwiththeBaldwin-LomaxandSSTturbulencemodels. Thewallboundaryconditionwasinitiallyassumed to be non-catalytic, but it was also expected that catalytic effects would become more important as the enthalpy increased. For a higher enthalpy run, H = 20 MJ/kg, at a high stagnation pressure of 40 MPa, an additional simulation with a fully 0 catalytic wall boundary condition was completed for comparison. Figure 5 shows this comparison and the nearly negligible difference between the wall heat transfer resulting from the non-catalytic boundary condition and that of the fully catalytic boundary condition. The largest differences, which are still minimal, are seen near the windside shoulder. When comparing thecomputationalresultstothedatameasuredattheseconditions,bothwallcatalycityassumptionssignificantlyunder-predict thedata. Fromthisresult,wallcatalycityappearstoprovideasmallamountofuncertaintyinpredictingthesurfaceheatflux measuredinthetunnel.However,somephenomenonappearstobemissingfromthesimulationsthatiscontributingtothelarge discrepancybetweenthecomputationalpredictionsandthemeasureddata.Thisresultisconsistentwithsometestingshownby Marineau,et. al. intheT5highenthalpyfacilityatCalTech2. AdditionalinvestigationattheHIESTfacility,particularlywith respecttosourcesofradiationthatcouldbecausingthisincreasedheating,iscurrentlyunderwayandresultswillbepublished atalaterdate. Asampleofthecapsulesimulationsforahighpressure(P =50MPa)andlowenthalpy(H =10MJ/kg)conditioncanbe 0 0 seeninFigure6. Thelaminarandtwoturbulentsolutionscanbeseeninseparatesurfaceheatfluxmapsinadditiontoaplot comparingthecomputationalpredictionsalongthecenterlinetothesmoothandtrippeddatameasuredinthetunnel. 4of11 AmericanInstituteofAeronauticsandAstronautics Figure5.Shot2220withNon-catalyticandFullyCatalyticWallBoundaryConditions,H0=20.75MJ/kg,P0=41.54MPa Figure6.LaminarandturbulentcapsulesimulationsforP0=50MPaandH0=10MJ/kgwithsmoothandtrippedmeasureddatacomparisons. 5of11 AmericanInstituteofAeronauticsandAstronautics III. AnalysisResults A. BoundaryLayerTripSizingandEffectiveness Apretestcomputationalanalysiswasperformedtodeterminethetripheightstobemanufacturedfortesting. Tripheightsthat would effectively cause the flow to transition from laminar to turbulent were desired. A range of stagnation enthalpies and stagnationpressures,showninTable1,wereconsidered. Table1.StagnationConditionsUsedinTripSizingStudy Case P [MPa] H [MJ/kg] 0 0 A 20.0 5.0 B 20.0 10.0 C 20.0 20.0 D 40.0 5.0 E 40.0 10.0 F 40.0 20.0 G 60.0 5.0 H 60.0 10.0 I 60.0 20.0 Figure7showsthecomputedboundarylayerthickness,δ,andmomentumthicknessReynoldsnumber,Re ,onthecapsule θ heatshield for the conditions selected. Also noted is the planned location of the trip elements on the test article. Case F was chosenasthebaselineconditiontosizethetripsforallotherconditions.Table2showsthek/δvalueschosenfortheassessment aswellastheresultingtripheightsrequiredtoobtainthedesiredk/δ fortheboundarylayerthicknesspredictedforCaseFat thedesiredtriplocation. Herek istheheightofthetripandk/δ isanon-dimensionalscalingparameterusedtomeasurethe tripeffectivenessfordifferentflowconditions. (a) BoundaryLayerThickness (b) BoundaryLayerMomentumThicknessReynoldsNumber,Reθ Figure7.Boundarylayerparametersusedintripsizingstudy Table2.CaseFBoundaryLayerScalingParameters,δ=1.103mm k/δ 0.2 0.3 0.5 0.7 1.0 1.2 k[mm] 0.22 0.33 0.55 0.77 1.10 1.32 From previous experience ***FIND REFERENCES***, the boundary layer is expected to trip at values of k/δ between 0.3and1.0,dependingonthevalueofRe . Thesixtripheightschosenforthistestingprovidedawiderangeofk/δ options θ 6of11 AmericanInstituteofAeronauticsandAstronautics acrossthedesiredtestconditions. ForCaseCwiththethickestboundarylayer, thelargesttripwouldprovideak/δ valueof 0.86,andforCaseGwiththethinnestboundarylayer,thesmallesttripwouldprovideak/δ valueof0.41,bothofwhichare withintherangeexpectedtotriptheboundarylayer. Post-testanalysisshowedawiderangeofk/δ valueswereachievedduringtesting. Boundarylayerthicknessvalueswere computedbasedontheas-measuredreservoirstagnationconditionsfromthetestingaccordingtotheproceduresdiscussedin SectionII.Forthelowenthalpy3MJ/kgcondition,a0.6mmtripwasusedandak/δof0.93wasachieved. Asaresultofthe highk/δ, fullyturbulentflowwasattaineddownstreamofthetrip. However, atahighenthalpyandhighpressurecondition, (40MPaand20MJ/kg),thetaller0.8mmtripwasnotaseffective. Thek/δvaluecomputedforthesetestconditionswas0.75, butthelowfreestreamReynoldsnumberof1.8×105,basedontheheatshielddiameter,preventedtheflowfromtransitioning tofullyturbulentwiththelargetrip. A high pressure, low enthalpy condition was tested with two different trip heights of 0.6 mm and 0.8 mm. At these conditions,theboundarylayerwasthinenough(0.7mm)thatbothtripheightseffectivelytrippedtheboundarylayertofully turbulent. Thesetripsresultedink/δvaluesof0.84and1.13,respectively. **ANYTRENDSINEFFECTIVENESSVS.RE THETA??*** B. ValidationofCapsuleSurfaceHeatFluxPredictions ForeachoftheconditionstestedintheHIESTfacilityduringtheApollocapsuletestcampaign,thecomputationalresultsalong theheatshieldcenterlinewerecomparedwiththeheatfluxdatameasuredinthetunnel.Datawasobtainedforbothsmoothwall conditionsandtrippedconditions,somewithmultipletripheightsforagivenfreestreamcondition. Table3showsthenozzle stagnationconditionsexaminedfortheApollocapsuleduringthistestseries,aswellasthecomputedfreestreamconditionsfor thecapsuleanalysis. Table3.NozzleStagnationandCapsuleFreestreamConditionsAnalyzedforCapsuleTestSeries Shot P [MPa] H [MJ/kg] ρ [kg/m3] V [m/s] T [K] T [K] Re ×10−5 0 0 ∞ ∞ ∞ v,∞ D 2216 31.86 6.22 0.0204 3299.33 569.62 606.70 5.497 2218 31.08 3.64 0.0264 2716.69 315.18 479.03 8.875 2220 41.54 20.76 0.0103 5631.80 2190.24 2194.60 1.823 2221 60.02 9.39 0.0278 3986.06 1024.39 1029.62 6.029 2232 12.72 4.63 0.0102 2864.18 368.36 588.61 3.251 2233 15.44 2.98 0.0168 2330.92 206.61 519.36 6.733 One test condition at a low stagnation enthalpy and high stagnation pressure showed natural boundary layer transition alongtheheatshieldcenterline. Figure9showsthecomparisonofthedatafromshot2218withouttrips,shot2242atsimilar conditions with an array of trips 0.6 mm tall, as well as the computational simulations for a non-catalytic wall boundary at laminarandturbulentconditions. Theheatfluxinthelaminarregionpriortotransitionisunder-predictedbythelaminarflow prediction,andaswasshownpreviously,catalycityhasaminimaleffectonthewallheatfluxattheseconditions,sodifferences arelikelyduetootherinaccuraciesinthemodeling. TheturbulentpredictionswereagainperformedwiththeBaldwin-LomaxandSSTturbulencemodels. Thetransitionaldata fromshot2218betweenz=-0.05mandz=-0.02miswellpredictedbytheSSTturbulencemodel,butthefullyturbulentdata frombothtestrunsforzgreaterthan0.0misbetterpredictedbytheBaldwin-Lomaxturbulencemodel,butstilloverpredicted by both models in this region. Due to the complex nature of predicting boundary layer transition, it is likely serendipitous thatthetransitionlocationandtransitionaldataaresowellpredictedbytheSSTturbulencemodel. Themomentumthickness Reynoldsnumber,Re ,wasextractedfromtheCFDpredictionatthesensorlastobservedtobelaminar(z=-0.05m).TheRe θ θ valuewascomputedtobe76.7,whichislowerthanthetransitionRe valuesobservedinothercapsuletestingfromarangeof θ testfacilities6. DatafromhigherenthalpyfacilitiessimilartoHIESTwerealsoincludedinthestudy,althoughwithaCO test 2 gas,butthetransitionRe predictedfordataobtainedinthesefacilitiesagreedwellwiththatofthedataobtainedinfacilities θ withanairtestgas. 7of11 AmericanInstituteofAeronauticsandAstronautics Figure8.HeatshieldCenterlineData Figure9.Shot2218NaturalTransition,H0=3.64MJ/kg,P0=31.08MPa 8of11 AmericanInstituteofAeronauticsandAstronautics C. ComputationalPredictionsofNozzleWallPressure FortherunsinTable4,pressuresmeasuredataxialstationsalongthenozzlewallwereprovided. Thelocationsofthepressure sensorscanbeseeninFigure10. Thecomputationalpredictionswereextractedalongthenozzlewallatthesensorlocations andcomparedtothepressuretracesmeasuredinthetunnel. Table4.StagnationConditionsAnalyzedforNozzlePressureSensors Shot P [MPa] H [MJ/kg] 0 0 2341 44.62 20.49 2346 45.05 22.23 2347 56.59 8.05 Figure10.NozzlePressureSensorLocations Thecomputationalpredictionsfortheseconditionswererunwithasteady-stateassumption,sotherewasnophysicaltime componenttothesimulations. Forthisreason,atimewhentheshockpassedbythepressuresensorshadtobeassumedforthe computationalpredictionsinorderforthetestdataandcomputationalpredictionstobecompared. Thistimewasselectedby examinationofthetimetracesintheexperimentaldataandselectingthetimethattheshockpassedtocorrespondtothefirst spikeinpressureseeninthefirstpressuresensor. Thistimewasimposedonallsensorsdownthenozzlewithouttakinginto accounttheshockspeed. Whiletheshockwavemovesquicklydownthenozzle,thetimethattheshockpasseseachsensorwill vary. Itisrecognized,therefore,thattheassumptionofaconstanttimeofshockpassageforeachsensorisnotaccurate,butis sufficientforthisanalysis. Figure 11 shows the comparison of the pressures measured at each of the nozzle sensor locations, shown in the black lines, with the computationally predicted pressures at the discrete points. The high pressures measured near the throat of the nozzle are predicted well with the computations, but farther down the nozzle, the predicted pressures are less accurate andgenerallyoverpredictthemeasurements. **CALCULATEPERCENTAGEDIFFERENCEINPRESSURES**Different assumptions for catalycity and chemistry models were made in an attempt to understand these differences. However, these modelingassumptionshadlittleeffectonthepredictedpressures. 9of11 AmericanInstituteofAeronauticsandAstronautics Figure11.Shot2341NozzleWallPressureComparison 10of11 AmericanInstituteofAeronauticsandAstronautics