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Numerical
Equations
Objects
Modelling
Results
Future plans
Experimental
Facility
LC probes
TFG probes
Sizes
Processing
Improvements to the aerothermal modelling ofobject-oriented debris re-entry codes
Numerical and experimental progress
Nathan L. Donaldson
Osney Thermofluids LaboratoryUniversity of Oxford
4th International Workshop on Space Debris Re-entryThursday, 1st March 2018
Numerical
Equations
Objects
Modelling
Results
Future plans
Experimental
Facility
LC probes
TFG probes
Sizes
Processing
Contents
1 Numerical modelling of debris aerodynamicsEngineering level modellingCommon debris objectsMultidimensional correlationCorrelation errorsFuture modelling
2 Experimental studies of thermal fluxesExperimental facilityThermochromatic liquid crystal studiesPlatinum thin film gauge heat transfer probesProbe sizes and gauge arrangementsPost processing of thermal flux data
Nathan L. Donaldson 4th International Workshop on Space Debris Re-entry 1 / 19
Numerical
Equations
Objects
Modelling
Results
Future plans
Experimental
Facility
LC probes
TFG probes
Sizes
Processing
Numerical modelling of debris aerodynamicsEngineering level modelling
RAC (Re-entry Aerodynamic Calculator) is used for analysesStandard multi-regime panel method formulation
Continuum: Modified NewtonianFree molecular: Schaaf & ChambreTransition: Wilmoth
Ma
5 10 15 20 25 30 35
Kn1e-04
1e-021e+00
1e+02
CD
1.41.61.82.02.22.4
(a) Unit cylinder, α = 90o
Ma
5 10 15 20 25 30 35
Kn1e-04
1e-021e+00
1e+02
CD
2.0
2.2
2.4
2.6
2.8
(b) Unit cuboid, α = 90o
Figure 1: Mach-Knudsen surfaces for drag coefficient
Nathan L. Donaldson 4th International Workshop on Space Debris Re-entry 2 / 19
Numerical
Equations
Objects
Modelling
Results
Future plans
Experimental
Facility
LC probes
TFG probes
Sizes
Processing
Numerical modelling of debris aerodynamicsCommon debris objects
Triangulated surface meshes of a unit cylinder and cuboid
Different aspect ratios are achieved by scaling along thelongitudinal axis
(a) 1:10 (b) 1:1 (c) 10:1
Figure 2: Cylindrical meshes
Nathan L. Donaldson 4th International Workshop on Space Debris Re-entry 3 / 19
Numerical
Equations
Objects
Modelling
Results
Future plans
Experimental
Facility
LC probes
TFG probes
Sizes
Processing
Numerical modelling of debris aerodynamicsCommon debris objects
Triangulated surface meshes of a unit cylinder and cuboid
Different aspect ratios are achieved by scaling along thelongitudinal axis
(a) 1:10 (b) 1:1 (c) 10:1
Figure 2: Cuboidal meshes
Nathan L. Donaldson 4th International Workshop on Space Debris Re-entry 3 / 19
Numerical
Equations
Objects
Modelling
Results
Future plans
Experimental
Facility
LC probes
TFG probes
Sizes
Processing
Numerical modelling of debris aerodynamicsMultidimensional correlation
Kriging (1), a modified version of a Gaussian radial basisfunction, is utilised for correlative modelling
Models are currently trained with calculations performedusing RAC, but may be trained with data from any source(CFD, DSMC, experiments, etc.)
A single model is used for each aerodynamic coefficient
Prediction time varies depending on the complexity of themodel
Number of training pointsNumber of dimensions
ψ(i) = exp
− k∑j=1
θj |x(i)j − xj |pj
(1)
Nathan L. Donaldson 4th International Workshop on Space Debris Re-entry 4 / 19
Numerical
Equations
Objects
Modelling
Results
Future plans
Experimental
Facility
LC probes
TFG probes
Sizes
Processing
Numerical modelling of debris aerodynamicsMultidimensional correlation
Two different types of Kriging models are being explored:
Pure models, wherein a single model with a high numberof training points is used for each aerodynamic coefficientAugmented models, wherein the Mach-Knudsen surface ismodelled for each coefficient using a set of analyticalexpressions. The parameters of these surfaces are thencorrelated using a series of smaller Kriging models.
Augmented models have been shown to have higheraccuracy for a lower training point count
Pure Kriging models are faster to evaluate (very useful ifthey are to be queried as part of a Monte Carlo calculation)
Results presented today are produced using augmentedmodels (pure models are still undergoing training)
Nathan L. Donaldson 4th International Workshop on Space Debris Re-entry 5 / 19
Numerical
Equations
Objects
Modelling
Results
Future plans
Experimental
Facility
LC probes
TFG probes
Sizes
Processing
Numerical modelling of debris aerodynamicsCorrelation errors
Cylindrical modelsare trained on 4parameters
Mach, MaKnudsen, KnPitch, αAspect, L
�A vector transformis used to convertEuler angles to asingle equivalentpitch
Absolute errorshave been shownto be < 6%
5101520253035
= 0o = 15o
5101520253035
= 30o = 45o
5101520253035
= 60o = 75o
10 5 10 3 10 1 101 1035
101520253035
= 90o
10 5 10 3 10 1 101 103
Mean
0.0 0.2 0.4 0.6 0.8 1.0Knudsen number Kn
0.0
0.2
0.4
0.6
0.8
1.0
Mac
h nu
mbe
r Ma
0.000
0.123
0.245
0.368
0.491
0.613
0.736
0.859
0.981
1.104
1.227
1.349
1.472
1.595
1.717
1.840
1.963
2.085
2.208
2.331
Erro
r (%
)
Figure 3: CD errors for L� = 1
Nathan L. Donaldson 4th International Workshop on Space Debris Re-entry 6 / 19
Numerical
Equations
Objects
Modelling
Results
Future plans
Experimental
Facility
LC probes
TFG probes
Sizes
Processing
Numerical modelling of debris aerodynamicsCorrelation errors
Cylindrical modelsare trained on 4parameters
Mach, MaKnudsen, KnPitch, αAspect, L
�A vector transformis used to convertEuler angles to asingle equivalentpitch
Absolute errorshave been shownto be < 6%
5101520253035
= 0o = 15o
5101520253035
= 30o = 45o
5101520253035
= 60o = 75o
10 5 10 3 10 1 101 1035
101520253035
= 90o
10 5 10 3 10 1 101 103
Mean
0.0 0.2 0.4 0.6 0.8 1.0Knudsen number Kn
0.0
0.2
0.4
0.6
0.8
1.0
Mac
h nu
mbe
r Ma
0.000
0.170
0.339
0.509
0.678
0.848
1.017
1.187
1.357
1.526
1.696
1.865
2.035
2.204
2.374
2.543
2.713
2.883
3.052
3.222
Erro
r (%
)
Figure 3: CD errors for L� = 5
Nathan L. Donaldson 4th International Workshop on Space Debris Re-entry 6 / 19
Numerical
Equations
Objects
Modelling
Results
Future plans
Experimental
Facility
LC probes
TFG probes
Sizes
Processing
Numerical modelling of debris aerodynamicsCorrelation errors
Cylindrical modelsare trained on 4parameters
Mach, MaKnudsen, KnPitch, αAspect, L
�A vector transformis used to convertEuler angles to asingle equivalentpitch
Absolute errorshave been shownto be < 6%
5101520253035
= 0o = 15o
5101520253035
= 30o = 45o
5101520253035
= 60o = 75o
10 5 10 3 10 1 101 1035
101520253035
= 90o
10 5 10 3 10 1 101 103
Mean
0.0 0.2 0.4 0.6 0.8 1.0Knudsen number Kn
0.0
0.2
0.4
0.6
0.8
1.0
Mac
h nu
mbe
r Ma
0.000
0.308
0.616
0.925
1.233
1.541
1.849
2.158
2.466
2.774
3.082
3.391
3.699
4.007
4.315
4.623
4.932
5.240
5.548
5.856
Erro
r (%
)
Figure 3: CD errors for L� = 10
Nathan L. Donaldson 4th International Workshop on Space Debris Re-entry 6 / 19
Numerical
Equations
Objects
Modelling
Results
Future plans
Experimental
Facility
LC probes
TFG probes
Sizes
Processing
Numerical modelling of debris aerodynamicsCorrelation errors
Cuboidal models are the most complex, and are trained on6 parameters:
Mach, MaKnudsen, KnPitch, αYaw, θRoll, βAspect, L
�
Nathan L. Donaldson 4th International Workshop on Space Debris Re-entry 7 / 19
Numerical
Equations
Objects
Modelling
Results
Future plans
Experimental
Facility
LC probes
TFG probes
Sizes
Processing
Numerical modelling of debris aerodynamicsCorrelation errors
10 5
10 1
103
= 0.00o,= 0.00o
= 7.50o,= 0.00o
= 15.00o,= 0.00o
= 22.50o,= 0.00o
= 30.00o,= 0.00o
= 37.50o,= 0.00o
= 45.00o,= 0.00o
10 5
10 1
103
= 7.50o,= 7.50o
= 15.00o,= 7.50o
= 22.50o,= 7.50o
= 30.00o,= 7.50o
= 37.50o,= 7.50o
= 45.00o,= 7.50o
= 15.00o,= 15.00o
10 5
10 1
103
= 22.50o,= 15.00o
= 30.00o,= 15.00o
= 37.50o,= 15.00o
= 45.00o,= 15.00o
= 22.50o,= 22.50o
= 30.00o,= 22.50o
= 37.50o,= 22.50o
10 20 3010 5
10 1
103
= 45.00o,= 22.50o
10 20 30
= 30.00o,= 30.00o
10 20 30
= 37.50o,= 30.00o
10 20 30
= 45.00o,= 30.00o
10 20 30
= 37.50o,= 37.50o
10 20 30
= 45.00o,= 37.50o
10 20 30
= 45.00o,= 45.00o
0.0 0.2 0.4 0.6 0.8 1.0Mach number Ma
0.0
0.2
0.4
0.6
0.8
1.0Kn
udse
n nu
mbe
r Kn
0.000
0.415
0.829
1.244
1.658
2.073
2.487
2.902
3.317
3.731
4.146
4.560
4.975
5.389
5.804
6.218
6.633
7.047
7.462
7.876
Erro
r (%
)
Figure 4: CD errors for L� = 1
Nathan L. Donaldson 4th International Workshop on Space Debris Re-entry 8 / 19
Numerical
Equations
Objects
Modelling
Results
Future plans
Experimental
Facility
LC probes
TFG probes
Sizes
Processing
Numerical modelling of debris aerodynamicsCorrelation errors
10 5
10 1
103
= 0.00o,= 0.00o
= 15.00o,= 0.00o
= 30.00o,= 0.00o
= 45.00o,= 0.00o
= 60.00o,= 0.00o
= 75.00o,= 0.00o
= 90.00o,= 0.00o
10 5
10 1
103
= 15.00o,= 15.00o
= 30.00o,= 15.00o
= 45.00o,= 15.00o
= 60.00o,= 15.00o
= 75.00o,= 15.00o
= 90.00o,= 15.00o
= 30.00o,= 30.00o
10 5
10 1
103
= 45.00o,= 30.00o
= 60.00o,= 30.00o
= 75.00o,= 30.00o
= 90.00o,= 30.00o
= 45.00o,= 45.00o
= 60.00o,= 45.00o
= 75.00o,= 45.00o
10 20 3010 5
10 1
103
= 90.00o,= 45.00o
10 20 30
= 60.00o,= 60.00o
10 20 30
= 75.00o,= 60.00o
10 20 30
= 90.00o,= 60.00o
10 20 30
= 75.00o,= 75.00o
10 20 30
= 90.00o,= 75.00o
10 20 30
= 90.00o,= 90.00o
0.0 0.2 0.4 0.6 0.8 1.0Mach number Ma
0.0
0.2
0.4
0.6
0.8
1.0Kn
udse
n nu
mbe
r Kn
0.000
0.509
1.018
1.527
2.036
2.544
3.053
3.562
4.071
4.580
5.089
5.598
6.107
6.615
7.124
7.633
8.142
8.651
9.160
9.669
Erro
r (%
)
Figure 4: CD errors for L� = 5
Nathan L. Donaldson 4th International Workshop on Space Debris Re-entry 8 / 19
Numerical
Equations
Objects
Modelling
Results
Future plans
Experimental
Facility
LC probes
TFG probes
Sizes
Processing
Numerical modelling of debris aerodynamicsCorrelation errors
10 5
10 1
103
= 0.00o,= 0.00o
= 15.00o,= 0.00o
= 30.00o,= 0.00o
= 45.00o,= 0.00o
= 60.00o,= 0.00o
= 75.00o,= 0.00o
= 90.00o,= 0.00o
10 5
10 1
103
= 15.00o,= 15.00o
= 30.00o,= 15.00o
= 45.00o,= 15.00o
= 60.00o,= 15.00o
= 75.00o,= 15.00o
= 90.00o,= 15.00o
= 30.00o,= 30.00o
10 5
10 1
103
= 45.00o,= 30.00o
= 60.00o,= 30.00o
= 75.00o,= 30.00o
= 90.00o,= 30.00o
= 45.00o,= 45.00o
= 60.00o,= 45.00o
= 75.00o,= 45.00o
10 20 3010 5
10 1
103
= 90.00o,= 45.00o
10 20 30
= 60.00o,= 60.00o
10 20 30
= 75.00o,= 60.00o
10 20 30
= 90.00o,= 60.00o
10 20 30
= 75.00o,= 75.00o
10 20 30
= 90.00o,= 75.00o
10 20 30
= 90.00o,= 90.00o
0.0 0.2 0.4 0.6 0.8 1.0Mach number Ma
0.0
0.2
0.4
0.6
0.8
1.0Kn
udse
n nu
mbe
r Kn
0.00
0.61
1.22
1.83
2.43
3.04
3.65
4.26
4.87
5.48
6.09
6.69
7.30
7.91
8.52
9.13
9.74
10.35
10.95
11.56
Erro
r (%
)
Figure 4: CD errors for L� = 10
Nathan L. Donaldson 4th International Workshop on Space Debris Re-entry 8 / 19
Numerical
Equations
Objects
Modelling
Results
Future plans
Experimental
Facility
LC probes
TFG probes
Sizes
Processing
Numerical modelling of debris aerodynamicsFuture modelling
Both augmented and pure Kriging models of a simplifiedATV geometry are planned
These will be trained on variances in pitch, α and yaw, θ
Y
Z
X
Figure 5: Surface mesh of a simplified ATV geometry
Nathan L. Donaldson 4th International Workshop on Space Debris Re-entry 9 / 19
Numerical
Equations
Objects
Modelling
Results
Future plans
Experimental
Facility
LC probes
TFG probes
Sizes
Processing
Experimental studies of thermal fluxesExperimental facility
The experimentalfacility being used isthe Oxford LowDensity Wind Tunnel(LDWT)
3 stage continuousvacuum pumpingsystem (22000 l/s)
Knudsen numbers ofthe order of ∼ 0.001(slip regime)
Mach numbersranging from 3− 10
Figure 6: The low density wind tunnel(LDWT)
Nathan L. Donaldson 4th International Workshop on Space Debris Re-entry 10 / 19
Numerical
Equations
Objects
Modelling
Results
Future plans
Experimental
Facility
LC probes
TFG probes
Sizes
Processing
Experimental studies of thermal fluxesExperimental facility
Working gas (air or nitrogen) is heated in an insulatedstagnation chamberThe gas is then expanded through a contoured Mach 6nozzle into the test sectionAutomated traverses control model position, and flowinitialisation
Figure 7: LDWT test section diagram
Nathan L. Donaldson 4th International Workshop on Space Debris Re-entry 11 / 19
Numerical
Equations
Objects
Modelling
Results
Future plans
Experimental
Facility
LC probes
TFG probes
Sizes
Processing
Experimental studies of thermal fluxesExperimental facility
The LDWT iscurrentlyundergoingcharacterisa-tion activitiesfollowing anextensiverenovation
These are setto concludewithin thenext fewweeks
Figure 8: Total pressure pitot survey in theMach 6 plume
Nathan L. Donaldson 4th International Workshop on Space Debris Re-entry 12 / 19
Numerical
Equations
Objects
Modelling
Results
Future plans
Experimental
Facility
LC probes
TFG probes
Sizes
Processing
Experimental studies of thermal fluxesThermochromatic liquid crystal studies
Thermochromatic liquidcrystal studies have been usedat Osney for decades
Current probes have beenmanufactured from Rohacell
Three crystal solutions havebeen applied, with transitiontemperatures: 25oC , 30oC ,and 35oC
Figure 9: Hemisphere LCprobe undergoing atemperature change
Nathan L. Donaldson 4th International Workshop on Space Debris Re-entry 13 / 19
Numerical
Equations
Objects
Modelling
Results
Future plans
Experimental
Facility
LC probes
TFG probes
Sizes
Processing
Experimental studies of thermal fluxesPlatinum thin film gauge heat transfer probes
Thin film gauge probesare manufactured usingMacor glass ceramic
Originally, gauges werepainted onto thesubstrate by hand
This arrangement led totransverse conductionissues inside thesubstrate, skewingthermal readings
Figure 10: Original platinum paintTFG probe
Nathan L. Donaldson 4th International Workshop on Space Debris Re-entry 14 / 19
Numerical
Equations
Objects
Modelling
Results
Future plans
Experimental
Facility
LC probes
TFG probes
Sizes
Processing
Experimental studies of thermal fluxesPlatinum thin film gauge heat transfer probes
The new design utilisesprecision printed gauges(details are accuratedown to 5 µm)
Gauges are sputteredusing a vacuumdeposition process
Gauges are double-sidedwith a sheet of kaptonbetween the twoplatinum layers,removing dependenceon the substrateproperties
Figure 10: New sputtered TFG probe
Nathan L. Donaldson 4th International Workshop on Space Debris Re-entry 14 / 19
Numerical
Equations
Objects
Modelling
Results
Future plans
Experimental
Facility
LC probes
TFG probes
Sizes
Processing
Experimental studies of thermal fluxesProbe sizes and gauge arrangements
9 LC probes have been manufactured
3 shapes (hemisphere, cylinder, cuboid)3 sizes (�10 mm, �15 mm, �20 mm)
12 TFG probes have been manufactured
2 shapes (cylinder, cuboid)3 sizes (�10 mm, �15 mm, �20 mm)2 probe arrangements (line over corner, line around edges)
Differing sizes allow various Knudsen numbers to beexamined without altering the freestream conditions
Nathan L. Donaldson 4th International Workshop on Space Debris Re-entry 15 / 19
Numerical
Equations
Objects
Modelling
Results
Future plans
Experimental
Facility
LC probes
TFG probes
Sizes
Processing
Experimental studies of thermal fluxesPost processing of thermal flux data
Constant current is applied to gauges from an amplifier
Voltage changes are recorded as gauge temperatures change
Calibration curves allow accurate conversion of change involtage to change in temperature
0 2 4 6 8 10 12 14 16 180
1
2
3
4
5
6
7
Tempera
ture
rise,∆T(K
)
T ime, t(s)
Gauge 1Gauge 2Gauge 3
Figure 11: Typical temperature rise profile for thin film gauges
Nathan L. Donaldson 4th International Workshop on Space Debris Re-entry 16 / 19
Numerical
Equations
Objects
Modelling
Results
Future plans
Experimental
Facility
LC probes
TFG probes
Sizes
Processing
Experimental studies of thermal fluxesPost processing of thermal flux data
An impulse response filter is designed based upon thesampling frequency of the gauge dataTemperature profiles are then processed through this filter,producing a heat flux profileDouble-sided gauges remove all dependence on substrateproperties
0 2 4 6 8 10 12 14 16 18−500
0
500
1000
1500
2000
2500
3000
Heatflux,q̇(W m
2)
T ime, t(s)
Gauge 1Gauge 2Gauge 3
Figure 11: Typical heat flux profile for thin film gauges
Nathan L. Donaldson 4th International Workshop on Space Debris Re-entry 16 / 19
Numerical
Equations
Objects
Modelling
Results
Future plans
Experimental
Facility
LC probes
TFG probes
Sizes
Processing
Experimental studies of thermal fluxesPost processing of thermal flux data
Thermochromatic surveys are processed in a similar fashion
Experimental runs are recorded visually using standard CCDor CMOS cameras
An in-house code is used to analyse the colour changesagainst time
A similar impulse response method is then used to convertthese temperature changes into heat flux distributions
Nathan L. Donaldson 4th International Workshop on Space Debris Re-entry 17 / 19
Numerical
Equations
Objects
Modelling
Results
Future plans
Experimental
Facility
LC probes
TFG probes
Sizes
Processing
Conclusions
Multidimensional correlative models are being generated forsome common debris shapes
These have been shown to have good accuracy and low runtimes
They may be trained with cheap or expensive data (or anycombination thereof)
Experimental facility characterisation is almost completefollowing an extensive refit
Experimental probes have been manufactured and arecurrently being assembled and tested
Nathan L. Donaldson 4th International Workshop on Space Debris Re-entry 18 / 19
Numerical
Equations
Objects
Modelling
Results
Future plans
Experimental
Facility
LC probes
TFG probes
Sizes
Processing
Thank you for your attention
Questions?
Nathan L. Donaldson 4th International Workshop on Space Debris Re-entry 19 / 19