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Presented By Stephen W. Miller Thermal & Fluids Analysis Workshop TFAWS 2011 August 15-19, 2011 NASA Langley Research Center Newport News, VA TFAWS Passive Thermal Paper Session Improvements to a Response Surface Thermal Model for Orion Stephen W. Miller – NASA JSC William Q. Walker – West Texas A&M

Presented By Stephen W. Miller Thermal & Fluids Analysis Workshop TFAWS 2011 August 15-19, 2011 NASA Langley Research Center Newport News, VA TFAWS Passive

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Page 1: Presented By Stephen W. Miller Thermal & Fluids Analysis Workshop TFAWS 2011 August 15-19, 2011 NASA Langley Research Center Newport News, VA TFAWS Passive

Presented By

Stephen W. MillerThermal & Fluids Analysis WorkshopTFAWS 2011August 15-19, 2011NASA Langley Research CenterNewport News, VA

TFAWS Passive Thermal Paper Session

Improvements to a Response Surface Thermal Model for Orion

Stephen W. Miller – NASA JSCWilliam Q. Walker – West Texas A&M

Page 2: Presented By Stephen W. Miller Thermal & Fluids Analysis Workshop TFAWS 2011 August 15-19, 2011 NASA Langley Research Center Newport News, VA TFAWS Passive

TFAWS 2011 – August 15-19, 2011 2

Talking Points

• Simple Design of Experiments (DOE) introduction

• Goals of Study• Orion Outer Mold Line Model Overview• Response Surface Equation Development

– Factors– Responses– Case Matrix

• Results• Conclusions• Summary

TFAWS2011-PT-006

Page 3: Presented By Stephen W. Miller Thermal & Fluids Analysis Workshop TFAWS 2011 August 15-19, 2011 NASA Langley Research Center Newport News, VA TFAWS Passive

DOE/RSM Introduction

• What is Design of Experiments?– Mathematical/Statistical approach to complex problems– Identify quantifiable measurements and controllable factors (or

variables)– Then implement purposeful changes in factors and measure

changes in response– Can then use statistical analysis to quantify the effect of each

factor (and combination of factors) on the response• What is Response Surface Methodology?

– Extension of DOE to produce a polynomial equation that can be used to create a surface of the response for any combination of identified factors

– Note that extrapolation beyond defined factor limits is inherently dangerous due to the behavior of polynomials

TFAWS2011-PT-006 TFAWS 2011 – August 15-19, 2011 3

Page 4: Presented By Stephen W. Miller Thermal & Fluids Analysis Workshop TFAWS 2011 August 15-19, 2011 NASA Langley Research Center Newport News, VA TFAWS Passive

Introduction, Continued

• DOE is different from changing one factor at a time– Changing one factor each case leads to a large number of cases

and doesn’t do a good job highlighting how factors interact

• DOE reduces the number of cases by looking at how simultaneous changes in variable effect the response.– For example, just changing Yaw alone may not be that

important, but changing Yaw and Roll together could be vital

TFAWS2011-PT-006 TFAWS 2011 – August 15-19, 2011 4

Page 5: Presented By Stephen W. Miller Thermal & Fluids Analysis Workshop TFAWS 2011 August 15-19, 2011 NASA Langley Research Center Newport News, VA TFAWS Passive

Goals of Study

• Build on previous work by incorporating the following:– Simplify the model geometry– Use minimum and maximum orbital temperature variations as

the responses– Evaluate RSEs up to a 5th order polynomial

• Generate an RSE that predicts temperatures within ±10°F of the of the engineering model prediction

TFAWS2011-PT-006 TFAWS 2011 – August 15-19, 2011 5

Page 6: Presented By Stephen W. Miller Thermal & Fluids Analysis Workshop TFAWS 2011 August 15-19, 2011 NASA Langley Research Center Newport News, VA TFAWS Passive

Orion Outer Mold Line (OML) Model Overview

• Developed by Lockheed Martin for the Orion project– A simplified version of the more

detailed Orion thermal model• Purpose of the model is to screen

attitudes to determine radiator thermal environments– The full Orion thermal model is then

run in the identified hot/cold environments to determine the vehicle level response

• The radiators are modeled with the most detail, including a simulated fluid loop with varying heat loads

• Other model geometry is present to provide the correct radiation environment– Not intended to predict temperatures for

these components

TFAWS2011-PT-006 TFAWS 2011 – August 15-19, 2011 6

Solar Arrays

Crew Module

Docking Port

Radiators

Service Module

Page 7: Presented By Stephen W. Miller Thermal & Fluids Analysis Workshop TFAWS 2011 August 15-19, 2011 NASA Langley Research Center Newport News, VA TFAWS Passive

RSE Development – Factors

• Used the main factors that affect on-orbit thermal analysis– Attitude (Yaw, Pitch, Roll)– Beta Angle– Environment

• Attitude– Kept Y/P/R as 3 independent variables

• Yaw and Roll: -15° to +15°• Pitch: -20° to +15°

• Beta Angle– Looking only at positive beta angle from 0 to +75°

TFAWS2011-PT-006 TFAWS 2011 – August 15-19, 2011 7

Page 8: Presented By Stephen W. Miller Thermal & Fluids Analysis Workshop TFAWS 2011 August 15-19, 2011 NASA Langley Research Center Newport News, VA TFAWS Passive

RSE Development – Factors, Continued

• Environment– Lumped all of the following into a single parameter called

Environment– Scaled from cold values (-1) to hot values (+1)

• To simplify the DOE process, each factor was normalized to values between -1 and +1– This simplifies the creation of the RSEs– Also helps to reuse the DOE case matrix if you want to change

the range of the factors

TFAWS2011-PT-006 TFAWS 2011 – August 15-19, 2011 8

Parameter Hot Case Cold CaseSolar 451 BTU/(hr-ft2) 419 BTU/(hr-ft2)Albedo 0.53 0.20Planetary IR 110.7 BTU/(hr-ft2) 48.5 BTU/(hr-ft2)Altitude 173 miles 286 miles

Page 9: Presented By Stephen W. Miller Thermal & Fluids Analysis Workshop TFAWS 2011 August 15-19, 2011 NASA Langley Research Center Newport News, VA TFAWS Passive

Radiators

RSE Development – Responses

• To align with the purpose of the model and the goals of the study, the minimum and maximum temperature of each radiator was selected as a response

• Each radiator consists of 32 nodes.– A simple min/max survey of the nodes on each radiator provided

the response for each case– Different nodes can supply the min/max temperatures for

different cases

• A total of 8 responses are used– Radiator 1 Min/Max– Radiator 2 Min/Max– Radiator 3 Min/Max– Radiator 4 Min/Max

TFAWS2011-PT-006 TFAWS 2011 – August 15-19, 2011 9

Page 10: Presented By Stephen W. Miller Thermal & Fluids Analysis Workshop TFAWS 2011 August 15-19, 2011 NASA Langley Research Center Newport News, VA TFAWS Passive

RSE Development – DOE Case Matrix

TFAWS2011-PT-006 TFAWS 2011 – August 15-19, 2011 10

• With factors and responses defined, a case matrix can now be produced

• Used Design Expert 8 to create the matrix– Used a 5 Factor user-defined response surface with test points

(cases) as follows:• Vertices – Corners of the 5-dimensional space (32 cases)

– All factors set at either +1 or -1• Centers of Edges – Mid-point of each edge line (80 cases)

– Four factors set at either +1 or -1, and the fifth at 0• Axial Checkpoints – Internal test points (32 cases)

– All factors set at either +0.5 or -0.5• Overall Centroid – Center of the design space (1 case)

– All factors set to 0– This produced 145 cases

Page 11: Presented By Stephen W. Miller Thermal & Fluids Analysis Workshop TFAWS 2011 August 15-19, 2011 NASA Langley Research Center Newport News, VA TFAWS Passive

RSE Development – DOE Case Matrix, Cont.

TFAWS2011-PT-006 TFAWS 2011 – August 15-19, 2011 11

• The figure below shows example test points for a problem with 2 factors

-Vertices-Center of Edges-Axial Checkpoints-Overall Centroid

Factor A

Fac

tor B

-1

-1

0

+1

+1

0

Page 12: Presented By Stephen W. Miller Thermal & Fluids Analysis Workshop TFAWS 2011 August 15-19, 2011 NASA Langley Research Center Newport News, VA TFAWS Passive

Thermal Desktop Runs

• DOE case matrix was run in Thermal Desktop (TD)– Radiation and heating rates were calculated by shooting 100k rays per

node for each radiation task• Radks were determined once and then that file is inserted into all

subsequent runs– The SINDA model was solved using a steady-state solution solver

followed by a transient run for 4 orbits• Wrote a dynamic SINDA code to read in factor values from arrays and run

cases (radiation analysis and SINDA) autonomously– Data was captured over the final 2 orbits and the min/max temperature

pair for each radiator was determined• Case run time

– All cases were run on dual quad-core processor with 8 GB of RAM• Cases allowed to execute without any other processes

– Solution time for heating rate calculations and SINDA was approximately 1 hour per case

TFAWS2011-PT-006 TFAWS 2011 – August 15-19, 2011 12

Page 13: Presented By Stephen W. Miller Thermal & Fluids Analysis Workshop TFAWS 2011 August 15-19, 2011 NASA Langley Research Center Newport News, VA TFAWS Passive

Producing the RSE

• After completing the runs, the temperatures are entered into Design Expert 8 for regression– Takes a matter of seconds to perform and the

software helps provide suggestions for what level of fit is appropriate based on how each factor contributes.

– The resulting polynomial can be anything from a linear equation up to an nth power polynomial, where n is the number of factors• For this study, produced cubic, quartic and 5th-order

polynomial for comparison• Focused mainly on the 5th-order polynomial, as outlined

in the study’s goals

TFAWS2011-PT-006 TFAWS 2011 – August 15-19, 2011 13

Page 14: Presented By Stephen W. Miller Thermal & Fluids Analysis Workshop TFAWS 2011 August 15-19, 2011 NASA Langley Research Center Newport News, VA TFAWS Passive

Evaluating the RSE

• For each of the 145 cases the RSE prediction was compared against the TD output– Took the difference between the RSE and TD values and found a ±3s

value for the 145 cases

– Good agreement should be expected since the Thermal Desktop values were used to create the RSEs

• An additional 70 verification cases were run using randomly generated values for the factors– Only the 5th order RSE was used– The largest difference for all 8 responses over the 70 cases was 3.5 F,

higher than the 3s values, but well within the desired ±10 F goal.– Provides confidence that the RSE is performing well.

TFAWS2011-PT-006 TFAWS 2011 – August 15-19, 2011 14

Response ±3 – Cubic (°F)

±3 – Quartic (°F)

±3 – 5th Order (°F)

Radiator 1 Min/Max 0.7 / 1.9 0.2 / 1.1 0.2 / 0.3 Radiator 2 Min/Max 0.6 / 0.4 0.2 / 0.2 0.2 / 0.1 Radiator 3 Min/Max 0.5 / 0.5 0.1 / 0.2 0.1 / 0.1 Radiator 4 Min/Max 1.1 / 0.6 0.3 / 0.4 0.1 / 0.1

Page 15: Presented By Stephen W. Miller Thermal & Fluids Analysis Workshop TFAWS 2011 August 15-19, 2011 NASA Langley Research Center Newport News, VA TFAWS Passive

Rad1 Min Temp “Truth Plot” for DOE Case Matrix

TFAWS2011-PT-006 TFAWS 2011 – August 15-19, 2011 15

-50

-45

-40

-35

-30

-50 -45 -40 -35 -30

RS

E T

emp

erat

ure

(D

eg. F

)

Thermal Desktop Temperature (Deg. F)

RSE Regression Results for Rad1 Min Temp

Error bars represent 2 deg F.

Page 16: Presented By Stephen W. Miller Thermal & Fluids Analysis Workshop TFAWS 2011 August 15-19, 2011 NASA Langley Research Center Newport News, VA TFAWS Passive

Results – Using the RSE

• Tested the RSE by screening for hot radiator temperatures– Varied all factors from -1 to +1 in 0.25 increments

• Creates 59,045 case– Used the RSE to evaluate all of these cases

• Took approximately 15 minutes– Selected 55 cases that produced hot temperatures– Ran these 55 cases in Thermal Desktop and compared the

output to the RSE predictions

• The largest difference between the RSE and TD result for all 8 responses over the 55 cases was 1.8 F– Indicates the RSE is quite capable of being used for screening

and goal-seeking

TFAWS2011-PT-006 TFAWS 2011 – August 15-19, 2011 16

Page 17: Presented By Stephen W. Miller Thermal & Fluids Analysis Workshop TFAWS 2011 August 15-19, 2011 NASA Langley Research Center Newport News, VA TFAWS Passive

Rad1 Max Temp “Truth Plot” for Hot Case Screening

TFAWS2011-PT-006 TFAWS 2011 – August 15-19, 2011 17

-30

-25

-20

-15

-10

-30 -25 -20 -15 -10

RS

E T

emp

erat

ure

(D

eg. F

)

Thermal Desktop Temperature (Deg. F)

Hot Case Screening Results for Rad1 Max Temp

Error bars represent 2 deg F.

Page 18: Presented By Stephen W. Miller Thermal & Fluids Analysis Workshop TFAWS 2011 August 15-19, 2011 NASA Langley Research Center Newport News, VA TFAWS Passive

Conclusions

• DOE/RSM was successfully applied to on-orbit thermal analysis– Must be careful to consider the appropriate responses in the thermal

model– DOE is powerful, but must be used correctly

• RSE cannot replace detailed thermal models– Detailed engineering models are needed to supply regression data to

DOE/RSE programs– RSEs cannot predict thermal “singularities” such as solar entrapment or

geometric shadowing• Must have detailed analysis to find these areas• Once discovered, the RSE can be “patched” around these points

• RSEs have several uses for on-orbit thermal analysis– Screening a large number of cases quickly– Optimizing an RSE to locate an “absolute” hot or cold case– Fulfilling requirement verification tasks that a large number of analysis

cases to be run

TFAWS2011-PT-006 TFAWS 2011 – August 15-19, 2011 18

Page 19: Presented By Stephen W. Miller Thermal & Fluids Analysis Workshop TFAWS 2011 August 15-19, 2011 NASA Langley Research Center Newport News, VA TFAWS Passive

Summary

• Goals of the study were met– Simplify the model geometry

• Used only the Orion OML– Use minimum and maximum orbital temperature variations as

the responses• Responses identified as min/max radiator temperatures

– Evaluate RSEs up to a 5th order polynomial• Used Design Expert 8 to produce a 5th order RSE

– Generate an RSE that predicts temperatures within ±10°F of the of the engineering model prediction

• 5th order RSE predicted Thermal Desktop

TFAWS2011-PT-006 TFAWS 2011 – August 15-19, 2011 19