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I / _i _ MPR-SAT-63-1 February 28, 1963 SPACE FLISHT HUNTSVILLE, ALABAMA CENTER SATURN SA-3 FLIGHT EVALUATION VOLUME II %.%6%'2" ' . NATIONAL AERONAUTICS ANDSPACEADMINISTRATION "_ i -_--'_' _.,,._ :- ./ °_'aa'6_ _" 'vPl_'J_r-&3-1 R <_'_,- _ " " *'" '''_ ,/.oc. RISFC -Fm 75'4 (Rev Pebe'ua_ *oP b_I_II_I_L'I_'_-IAL

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Page 1: Saturn SA-3 Flight Evaluation Volume II, MPR-SAT-63-1, …klabs.org/history/history_docs/jsc_t/sa03_flight_evaluation_vol_2.pdf · i / _i_ mpr-sat-63-1 february 28, 1963 space flisht

I

/ _i _

MPR-SAT-63-1

February 28, 1963

SPACEFLISHT HUNTSVILLE, ALABAMA

CENTER

SATURN SA-3 FLIGHT EVALUATION

VOLUME II

%.%6%'2"'

.

NATIONALAERONAUTICSANDSPACEADMINISTRATION

"_ i -_--'_' _.,,._:- ./

°_'aa'6_ _" 'vPl_'J_r-&3-1 • R <_'_,- _ " " *'" '''_ ,/.oc.

RISFC -Fm 75'4 (Rev Pebe'ua_ *oP b_I_II_I_L'I_'_-IAL

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SECURITY NOTE

This document contains information affectinE the national

defense of the United States within the meaning of the Espionage Law,

Title 18, U.S.C., Sections 793 and 794 as amended. The revelationof its contents in any manner to an unauthorized person is prohibited

by law.

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GEOP_E C. 14ARSlIAI_ SPACE FLZGI_ CENTER

MPR-SAT-63-1

VOLI.R4E _I

SATURN SA-3 FLIGHT EVALUAT'£ON

By Saturn Flight Evaluation Working Group

(4) ASSZP,

The evaluation of the Saturn SA-3 test flight is presented in

volumes. The first volume contains the results of the early

engineering evaluation and the second volume contains supporting in-formation and information related to the evaluation of the flight. In

these volumes the performance of each major vehicle system is discussed

with special emphasis on malfunctions and deviations.

The SA-3 flight test was a complete success with all missions of

the test being accomplished. No maJor malfunctlons or •deviationswhich _uld he considered a serious system failure or design deficiencyoccurred.

4 Any questions or comments pertaining to the information contained

in this report are invited and should be directed to

_!_i Director, George C. Marshall Space Flight Center

-_ Huntsville, AlabamaAttention: Chairman, Flight Evaluation Working Group,

M-AERO-F (Phone 876-2701)

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GEORGE C. MARSHALL SPACE FLIGHT CENTER

MPR -SAT- 63-1

VOLUME II

SATURN SA-3 FLIGHT EVALUATION (U)

_!_ SATURN FLIGET EVALUATION_ WORKING GROUP

il,

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b Acknowledgement is made to the various d_visions and elements of

MSFC and Launch _Operations Center for their contributions to this

report. Without the assistance and cooperation of these elements this

integrated report would not have been possible. The Saturn FlightEvaluation Working Group is especially indebted to the following

* branches (of MSFC) which have made major contributions:

Aeroballlstics Division

Aerodynamics Branch

Aerophysics and Astrophysics Branch

Dynamic Analysis Branch

, Flight Evaluation Branch

Astrionics Division

Electrical systems Integration Branch

Flight Dynamics BranchGuidance and Control Systems Branch

Gyro and Stabilizer BranchInstrumentation Development Branch

Computation Division

Data Reduction Branch

Launch Vehicle Operations Division

Electronic Engineering, Measuring and Tracking Office

• Mechanical, Structural and Propulsion Office

Propulsion and Vehicle Engineering Division

Propulsion and Mechanics BranchStructures Branch

Vehicle Engineering Branch

/

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(u) TABLE OF CONTENTS

Page

1.0 Vehicle Description 1

I.1 Su_mry I .1.2 S-I Stage 1

1.3 S-IV Dummy Stage 1

1.4 S-V Dummy Stage 4

1.5 Dummy Payload 4

2.0 Introduction 7

3.0 Launch Operations 8

3.1 Chronological Stm_mary of Prelaunch Checkout 83.2 Blockhouse Redline Values 9

3.3 Ground Sequence of Events 133.4 Enviroranental Measurements During Launch 15

3.4.1 Vehicle 15

3.4.2 Launch Complex 34 15

3.5 Atmospheric Smmnary For SA-3 233.5. I Introduction 23

3.5.2 General Synoptic Situation at Launch Time 233.5.3 Surface Observations at Launch Time 24

3.5.4 Time and Space Variations Between Vehlcle 26

Flight Path and Upper Air Measurementsby Rawlnsonde and Rocketsonde

3.5.5 Wind Data 26

3.5.6 Thermodyn_.Ic Data 31

4.0 Trajectory 38

4.1 Tracking Analysis 384.1.1 Data Sources 384.1.2 Data Utilization 38

4.1.3 Error Analysis of Actual Trajectory 434.2 Vehicle Liftoff Motion 45

5.0 Propulsion 48

5.1 Propulsion System Description 48

5.2 Individual Engine Performance 49

5.3 Flight Simulation of Cluster Performance 49

5.4 Pressurization System 59 •5.4.1 Fuel Tank Pressurization 59

5.4.2 LOX Tank Pressurization System 64

5.4.3 Control Pressure System 64

5.4.4 Air Bearlng Supply System 64

5.5 Propellant Utilization System 70

5.6 Hydraulic System 70

iv

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(u) -TABI OFCONTES(CON)

Page

6.0 Mass Characteris_Ics 81

- 6.1 Weight Measurement Accuracy 81

6.2 Propellant Loading 81

7.0 Control 85

7.1 _mmary 857.2 Control Simulation 85

7.2.1 Pitch Plane 85

7.2.2 Yaw Plane 85

7.2.3 Bending Oscillations After Cutoff 857.3 Control Accelerometers 92

7.4 Angle-of-Attack Meters 92

7.5 Propellant Sloshing 96

8.0 Guidance _ 103

8.1 Introduction 103

8.2 Description of Guidance Equipment 103

8.2.1 ST-90 System 103

8.2.2 ST-124P System 103

8.3 Guidance Intelligence Errors 1048.3.1 General 104

8.3.2 ST-124P Intelligence Errors 104

8.4 Platform and Vehicle Alignments 105

9.0 Vehicle Electrlcal System 107

9.1 Power Supply Description 107

9.2 Power Consumption 112

I0.0 Structures and Vibrations 114

I0.1 Summary 114

10.2 Bending Moments and Normal Load Factors 114

10.2.1 Instrumentation 114

10.2.2 Strain Gauge Measurement Adjustments 116

10.2.3 Time Points Evaluated 116

10.2.4 Longitudinal Loads 117

10.2.5 Moment Loads 117

10.2.6 Shear Loads 122

10.3 Bending Oscillations 122

10.4 Vibrations 12610.4.1 Introduction 126

10.4.2 General Discussion 126

* 10.4.3 Major Deviations Observed in Flight 132VihrationData

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(u) TABLEOF CONTENTS(CONCLUDED)

Page

10.5 Analysis of Ground Acoustic Measurements 13410.5. I Summary 13410.5.2 Near-Field Data 134

10.5.3 Mid-Field Data 136

10.5.4 Far-Field Data 137

I!.0 Environmental Temperatures and Pressures 141 *II. I Summary 141II.2 Tail Section 141

II. 2.I Base Enviroement 141

II.2.2 Calorimeter Loss Determination 148

11.2.3 Engine Compartment 156

11.3 Skin Temperature 160

• 11.3.1 Propellant Tank Temperatures 160

II.3.2 Interstage Skin Temperatures 160

11.3.3 S-IVD Skin Temperatures 160

12.0 Aerodynamics 166

12.1 Equation Derivations and Limitations 16612.2 Wind Tunnel Tests 168

12.3 Centaur Simulation Panels 168

13.0 Tnstrumentation 170

13.1 _nstrumentation Program 170

13.2 Telemetry Systems Description 170

13.3 Operation of Experimental Telemetry Systems 17313.4 Telemetry and Tracking Stations 174

13.5 Photographic Coverage 174

14.0 Data Reduction 178

14.1 Telemetry Data 17814.1.1 Telemetry Ground Station 178

14.1.2 •Analog to Digital Conversion 179

14. i.3 Experiments 17914.1.4 Vibration Data 180

14.1.5 OutputData 18014.2 UDOP Data 180

14.2.1 General 180 "

14.2.2 Quality of Cycle Data 181

14.2.3 Position Data 182

14.3 Meteorological Data 183

15.0 Bias Adjustment of Flight Mechanical Data 184

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LIST OF TABLES

"Table Page

3-I Blockhouse Redliae Values lO

" 3-_ Environmental Measurements on Launch Complex 34 16

3-Ill Vibrations on Complex 3¢ 19

4-_ _ _xternal Data Source 39'_-_I _"Supp6rting Flight Data 40

• 10-I SA-3 Flight Vibration Measurements 12713-_ Saturn SA-3 Telemetry Systems 171

15-_ .Flight Mechanical Data Pre-lgnition Bias for SA-3 185

•!

vii

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LIST OF FIGURES

Figure Page

l-I Saturn Configuration 2

I-2 Dummy Second Stage 3 .

I-3 Dummy Third Stage 5

1-4 Dmmny Payload 6

3-1 Comparison of Frequency Distribution on SA-2 and SA-3 21

Flights3-2" Launch Site Wind Measurements (Anemometers) for Saturn 25 *

SA-3 Launch

3-3 Low Altitude Launch Site, SA-3 Wind Speed by Rawinsonde 27

and Angle-of-Attack3-4 High Altitude Launch Site Wind Speed for SA-3 by 28

Eocketsonde, Rawinsonde, and Angle-of-Attack3-5 Launch Time Wind Components for SA-3 (Rawinsonde vs 29

Angle-of-Attack)3-5 Launch Time Wind Components for SA-3 at High Altitude 30

(Rocketsonde, Rawinsonde, and Angle-of-Attack)

3-7 Range and Cross Range Wind Shear (i000 m) For SA-3 32

by Rawlnsonde and Angle-of-Attack

3-8 High Level Range and Cross Range Component Wind Shear 33(1000 m) For SA-3 Launch

3-9 SA-3 Launch Time Range Components Wind Shear (250 m) 34

by A_le-of-Attack3-10 SA-3 Launch.Time Cross Range Component Wind Shear 35

(250 m) by Angle-of-Attack3-11 Relative Deviations of SA-3 Launch Site Temperature 36

and Density from PAFB Reference Atmosphere3-12 Absolute Deviation of the Index of Refraction and 37

Relative Deviation of Pressure from the PAFB Ref-

erence Atmqsphere for SA-3 Launch Site4-1 External Tracking Data 41

•-i:. 4-2 Separation Anvil vs Vehicle Support Block 42_ 4-3 Data Utilization 44

4-4 Tracking Comparisons (Tracking-Reference) 464-5 Altitude vs Distance to Tower 47

._r 5-1 H-I Engine Schematic 50

. 5-2 Thrust and Specific Impulse, Engine Position I 51

_:-: 5-3 Thrust and Specific Impulse, Engine Position 2 52

5-4 Thrust and Specific Impulse, Engine Position 3 53 •

_,i':" 5-5 ThruSt and Specific Impulse, Engine Position 4 54

¢. _ 5-6 Thrust and Specific Impulse, Engine Position 5 55

_;_ 5-7 Thrust and Specific Impulse, Engine Position 6 56'.__:i_. 5-8 Thrust and Specific Impulse, Evglne Position 7 57

_.'.,i._., 5-9 Thrust and Specific Impulse, Engine Position 8 58

viii

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LIST OF FIGURES (CONT)

Figure Page

5-10 Flight Simulation Results 60

" 5-11 Earth-Fixed Velocity and Slant Distance 61

(Tracking - Flight Simulation)

5-12 SA-3 Fuel System 62

5-13 Gas Pressure in High Pressure Spheres and Fuel Tank, F3 63

5-14 SA-3 LOX System 65

5-15 Pressure and Temperature in L0X Tanks 66

5-16 Control Pressure System Schematic 67

5-17 Control Equipment Pressure 68

5-18 Air Bearing GN 2 Supply System Schematic 695-19 Air Bearing Supply Pressure (ST-90 and ST-124) 7I5-20 Propellant Utilization System 72

5-21 Liquid Height Above Tank Bottom - LOX Tank 04 73

5-22 Liquid Height Above Tank Bottom - Fuel Tank F2 74

5-23 _Pressure PU Computer (fine), LOX and Fuel, and 75

Propellant Utilization Computer Output (fine)

5-24 Hydraulic Oil Temperature and Source Pressure (Engine 77

position ! through 47

5-25 Hydraulic Oil Level and Return Pressure 78

5-26 Hydraulic Source Pressure and Level 79

5-27 Hydraullc Source Pressure and Level 80

6-1 RP-I Specific Weight Versus Temperature 837-I Pitch Attitude minus Program, Free-Stream Angle-of 86

Attack (pitch), and Average Pitch Actuator Position

7-2 Yaw Attitude_ Free-Stream Angle-of-Attack (yaw), and 87Average Yaw Actuator Position

7/3 Pitch and Yaw Normal Acceleration After Outboard 88

- Engine Cutoff7-4 Root Locus Plot of Coupled First Bending Mode at Out- 90

board Engine Cutoff as a Function of VariableThrust Level

7-5 Comparison of Multi-Beam Coupled Bending Mode Shape 93for Zero Thrust With Flight Data (150-154seconds)

7-6 Pitch and Yaw Control Acceleration Comparisons 94

7-7 Error Factor For Q-Ball Angle-of-Attack Indicator 97

7-8 Baffle Configurations 99

- 7-9 Fuel Tank F2 Sloshing Amplitudes I00" 7/10 LOX Tank 04 Sloshi_ Amplitudes 101

:_ 7-11 Spatial Plots of Sloshing Motion 102

_. 8-1 ST-90 Platform Alignment With Respect to Vehicle Axis I06

9-I 28 Volt DC Power System 108* "9-2 Unit Locations 109

9-3 Propulsion and Control Distributor Network System 110

9-4 Current Cons,-,ption from Battery D20 113

ix

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LIST OF FIGURES (CONCLUDED)

Figure Page

I0-I SA-3 Strain Gauge Locations 115

10-2 Comparison of the Longitudinal Loads at Station 118979 For SA-2 and SA-3

10-3 Longitudinal Load at Station 979 11910-4 Load in LOX Studs at Station 869 120

10-5 Vehicle Bending Moment at Station 979 121 •

10-6 Bending Mode Accelerometer Locations 123

10-7 SA-3 Bending Mode- First Mode, Yaw (I0 to 13 sec) 124

10-8 SA-3 Bending Mode - First Mode, Pitch (32 to 36 sec) 12510-9 Saturn SA-3 Booster 128

I0-18 Saturn SA-3 Booster 129

I0-Ii Saturn SA-3 Booster 130

10-12 Maximum and Minimum Acceleration Times 131

I0-13 Launch Vehicle Operations and Test Division Near- 135Field. Measurements Locations on Fad 34A for SA-3

10-14 Far-Field Acoustic Measuring Points 139

10-15 Overall Time History of the Saturn SA-3 Launch I$011-1 Heat Shield Instrumentation Location for Saturn 142

SA-3 Flight

11-2 SA-I, SA-2, and SA-3 Radiation Calorimeters 14311-3 Calibration Factor 145

11-4 Total Heating Calorimeter 14611-5 Total Calorimeter on Flame Shield 147

11-6 Gas Temperature Probes for SA-2 and SA-3 14911-7 Heat Shield Instrumentation on Aft Side 150

11-8 Conduction Loss Coefficient 154

11-9 Comparisons of SA-I Heating Rate Calibrations 157

11-10 Comparison of SA-2 Heating Rate Calibration 158

11-11 S-I Stage Flight Measurements 159

11-12 S-I Stage Flight Measurements 16111-13 Measured and Estimated Skin Temperatures on Inter- 162

stage Conical Flare11-14 Measured and Estimated Skin Temperatures on S-IVD 163

Stage11-15 Measured and Estimated Skin Temperatures Around Fro- 164

tuherance on S-I-_D Stage12-1 Centaur Simulation Panels 169

13-1 Telemetry and Tracking Station Locations 175

x

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CONVERSION FACTORS FOR PREFERRED HSFC_ASURING UNITS

M'I':iPZZ Obtai.

. 1. Acceleratlon ft/s 2 3. 04800x10-1 m/s22. Area in2

6.4516xi0-4 m23. Density ib_s 2

5"25539XI01 m_

" slug/f t3 5.25539xi01 k__s 2-'T--

4. Energy BTU 2-51996xi0 "I m"5. Force kcal

Ib 4.53592x10-1 kg

6. Length in 2.54000xi0"2m

7. Mass lb.s 2

ft Z.48816 _ =m

8. Mass Flow Rate Ib-____s 1.48816ft

9. Pressure m•_'. ib/in 2

7.03067xi0-2 kg/cm2i0. Temperature OF.32o

5.55556xi0-1 oC

11. Velocity ft/s 3.04800xi0_i12. Volu_e m/s

gal (U.S.) 3. 78543x10-3 m3ft3

2.83168xi0-2 m3

" I3. Volume Flow ft3/si 2.83168xi0-2 m3/s

gal/s 3. 78543xi0-3 m3/s

xi

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GEORGE C. MARSHALL SPACE FLIGHT CENTER

MPR-SAT-63-1

VOLI_iE II

6 SATURN SA-3 FLIGHT EVALUATION

By Saturn Flight Evaluation Working Group

1.0 (U) VEHICLE DESCRIPTION

1.1 St_qMARY

Saturn SA-3 was the same basic configuration as previous Saturn

vehicles. The vehicle was made of a live S-I stage, a dummy S-IV stage,

a dummy S-V stage, and a dummy payload. A diagram of the overall Saturnconfiguration including some of the more important vehicle dimensions

is presented in Figure i-I.

1.2 S-I STAGE

The S-I stage was the only active stage of the Saturn SA-3 vehicle.

Propulsion was provided by a unique arrangement of eight clustered H-I

rocket engines. Propellants were supplied to the engines from a cluster

of nine propellant tanks. Most of the SA-3 instrumentation, including

guidance and control components, was located in the S-I stage. TheS-I stage was essentially the same as the S-I stage flown on SA-2; the

only important changes between the two vehicles being the addition of

one antenna panel and four retro rockets on the forward end of the S-I

stage and the addition of a fifth instrument canister, which housed a

laboratory model passenger guidance system that was flight tested forthe first time, to the S-I/S-IV interstage area.

1.3 S-IV DI_YSTAGE

The S-IV dummy second stage for Saturn SA-3 carried water ballast

" (41,102 kg) to simulate the weight and aerodynamic characteristics ofthe live S-IV stage. Dimensions of the S-IV stage are givenln Figures

I-i and 1-2.

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2

Sta° 195]-.90 A

Payload

t \

Sta. 1731.12.

3.05 m (3.20in)Diameter Dummy Stage

S-V

Sta. 1506 ......

_ _eo_ / \49.60m (162.7ft)Sta.1319.37 "....

5.59 m (220 in) _Diameter _ Dum_y Stage

S-Y_

%% ._o'

sta.889.3

_ r-= Booster S_ge

6.53 m (257 in)_Diameter _ %--

sooSA-3

FIGURE l-l SATURN CONFIGURATION

MPR-SAT-63-1

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13"9. 37

FIGURE 1-2 DL_fY SECOND STAGE ;MPR-SAT-63-1

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4

1.4 S-V DIn_4Y STAGE

The S-V dummy third stage was basically a Centaur cruiser .tank

modified by increased skin gauges. The tank carried water ballast

(46,312 k_) to simulate upper stage weight. Dimensions of the S-Vstage are given in Figures 1-I and 1-3. •

1.5 DI]_Y PAYLOAD

SA-3 carried a Jupiter type nose cone and aft unit as the dmmy

payload. An ad_pt.er section was required to rote the aft unit to theS-V stage. Dimensions of the payload are given in Figures i-i and 1-4.

• I

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FIGURE 1-3 D_ THIRD STAGE

MPR- SAT- 63 -i

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Sta. 1951.90

)iter Nose Cone

(With Insulation)

Angle-of'Attack Jupiter AftMeter (4 Places) Section

Angle-of-AttackMeter PressureManifolds

0.0143 m3 _ottle

Overflow Plpe!

& Hand Operated I,,, Sta. 1731.12

Valve LJ

/ ! erometerr _t, (2 Places)

I I

FIGURE i-4 DI_MMY PAYLOAD

MPR-SAT-63-1

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2 _0 - (U) INTRODUCTION

This volume of the Saturn SA-3 Flight Evaluation report contains

supporting information for Volume I.

• This report is published by the Saturn Flight Evaluation Working

Group, whose membership includes representatives of all Marshall Space

Flight Center Divisions. Therefore, the report represents the official

MSFC position at this time. This report will not be followed by a

• similarly integrated report unless continued analysis and/or new evi-

dence should prove the conclusions presented here partly or whollywrong. Final evaluation reports will, however, be published by the

MSFCDivislons covering some of the major systems and/or specialsubjects.

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3.0 (u) LAUNCHOPERATIONS

3.1 CHRONOLOGICAL S_4AEY OF PRELAUNCH CHECKOUT

Saturn vehicle SA-3 (consisting of the S-I first stage booster,

S-IV duchy second stage, S'V dummy third stage, and payload body)arrived by the barge 'Tromise" at Cape Canaveral on September 19, 1962.

The S-I booster was transferred to Complex 34 the same day. On Sep-

tember 21, 1962, the S-I booster was erected on Pad 34.

The following is a chronological summary of the work and mile-

stones accomplished duri_ the Saturn vehicle SA-3 erection and check-out.

September 21_ 1962 thru September 30_ 1962 - Electrical, mechani-cal, and pneumatic systems connected and checked. R1_ antennas installed

. and calibrated; R1_ subsystems tests begun. Stabilized platform (ST-90)lahorato_y test and calibration completed. Retract arms positioned

under the vehicle. Milestone - second and third dmmny stages (S-IV and

S-_, and dummy payload erected and mated to the S-I booster.

October I_ 1962 thru October 7_ 1962 - Mechanical systems and elec-tromechanical components tests completed. EBW checks and changes com-

.pleted. Stabilized platform (ST-124P) laboratory test and calibration

be@un. Destruct Co_nd Control Receivers received from MSFC and

checked out. l_light measurin E calibrations 40 percent complete.

Milestone - fuel and LOX simulated loading, functional and low pres-surization tests completed.

October 8_ 1962 thru October i_ 1962 - Stabilized platforms,ST-90 and ST-124P, installed in the vehicle and tests complete. Guid-

ance and ST-124P accelerometer monitors installed in blockhouse; EO's

installed in vehicle to permit blockhouse monitoring of the ST-124P.

Malfunction sequence and DCE tests completed. Heat and radiation

shields, Azusa transponder, and outstanding EO's on electrical supportequipment installed and checked out. Milestone - fuel and LOX full

pressurization tests complete.

+October 15_ 1962 thru October 21_ 1962 - Service structure func-tional tests completed satisfactorily. RF ranEe checks, navigstlon

system check, hydraulic system preparations completed. Service struc-

ture removed and sway tests and alignment tests completed. Cooling

tests cumpletedsatlsfactorily. EO's of EBW installed, upper stage

-leak tests started, dummy retro rocket tests begun. Measuring calibra-

tio,_ of flis,_t measurements 80 percent c_mpl.:te. Installation andcheckout of ground facilities measurements 50 percent complete.

Milestone - interstnge aligr_,ent, RF checks (with service structure re-

moved) performed satisfactorily.

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.... October 22 t 1962 thru October 28_ 1962 - Relay distributors £n-i spected aRd aligned. ST-90 and rate gyros aligned. Installation of

falrings and outboard curtains completed. Propellant utilization com-

puter replaced and checked. Meanurement calibration of fligh.C instru-ments and installation and checkout of ground facilities measurements

• about 90 percent complete. Milestone - overall tests numbers i, 2, and

3 completed and evaluated.

_ctober 29_ 1962 thru November 4_ 1962 - Acoustical drag cable in-• stalled and EB_ retro rocket initiators test fired. Sleeves on engine

• positions 2 and 4 replaced and umbilical faceplate pin installed.

Milestone - L0X loading and all associated tests completed.

November 5_ 1962 thru November 13_ 1962 - Overall test number 4completed; two angle-of-attack meters and telemeter transmitter munber

9 replaced. Retro rocket installation and prlmacord installation com-

pleted. Milestone- simulated flighttest and evaluation performed and

- completed satisfactorily.

November 14_ 1962 thru November 15_ 1962 - Preparations for launchCompleted.

November 16_ 1962 - Launch.

3.2 _LOCKHDUSE REDLyNE VALUES

Blockhouse redline values are defined as limits on critical meas-

urements, se_ to assure safe engine and vehicle operating conditions.

These measurements are monitored in the blockhouse, and the countdown

procedure could be stopped if these measurements show values outsidethe limits.

These redline values are shown in Table 3-I. All of the measure-

ments were within their specified limits and the countdown procedurewas normal.

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lO

ioooooooo

ooooooooo

ioooo

IQIOOOtQ

_•

o__o_

___

_IIIIIIII

HH

g

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1..2

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_!t, 13

3.3 GROUND SEQUENCE OF EVENTS

Predicted Time Actual Time*

• Event Nominal (sec) (s.ec)

" F£rln E Command -369%10 -363.440

Fuel Vent Nr. 1 Closed -368_I0 -362.985

Fuel Vent Nr. 2 Closed -368__I0 -362.955

Fuel Pressurlzin E Command -368%10 -362.955

Fuel Pressurizing Valve Nr. 1 Open -368TI0 -362.915

l_uel Preskurizing Valve Nr. 2 Open -368_.I0 -362. 915

Fuel Pressurizing Valve Nr. 3 Open -368+10 -362.915

FUel Pressurizing Valve Nr. 4 Open -368TI0 -362.915Fuel Pressurized -364.+10 -358.655

LOX Pressurizing Valve Open -120_I0 -110.255LOX Relief Nr. 2 Closed -120+10 -109.855

LOX Relief Nr. I Closed -120T_I0 -109.855

" LOX Pressurized -35 -35. 220

Power Transfer Command -35 -35.220Umbilical Eject Co_nand -25 -25.555

Umbilical Retracted -13 -13. 715

Ignition Start Timer -0.06 -0.0Ignition Command O. 0 0.0

Eng. Nr. 5, Igniter _r. I Energized +0.015 +0.018

Eng. Nr. 5, Igniter Nr. 2 Energized +0.015 44).018Eng. Nr. 7, Igniter Nr. I Energized +0.015 +0.018

Eng. Nr. 7; Igniter Nr. 2 Energized +0.015 +0.018

Eng. Nr. 6, Igniter Nr. I Energized +0.1!5 +0.116Eng. Nr. 6, Igniter Nr. 2 Energized +0.115 +0.116

Eng. _r. 8, Igniter Hr. I Energized +0. 115 +0. 116

Eng. Nr. 8, Igniter Nr. 2 Energized +0.115 +0.116

Eng. Nr. 2, Igniter Nr. 1 Energized +0.215 +0.224

Eng. Nr. 2, Igniter Nr. 2 Energized +0.215 +0.22_

Eng. Nr. 4, Igniter Nr. I Energized +0.215 +0.224Eng,: Nr. 4, Igniter Nr. 2 Energized +0.215 +0.224

Eng. Nr. I, Igniter Nr. 1 Energized +0.315 +0.330

Eng. Nr. I, Igniter Nr. 2 Energized +0.315 +0.330

Eng. Nr. 3, IEnlter Nr. i Energized +0.315 +0.330

Eng. Nr. 3, Igniter Nr. 2 Energized +0.315 +0.330

All Igniters Energized +0 315 +0.346

All Engines Running +l 32 +l. 247

Thrust OK Timer +3 30 +3. 247Thrust Commit +3 34 +3.330

'-' Short Mast Nr. 2 Valve Nr. l_Open +3 39 +3.385

Short Mast Nr. 2 Valve Nr. 2 Open +3 39 +3.385

• Short Mast Nr. 4 Valve Nr. i Open +3 39 +3. 385

* Time referenced to ignitio]I command.

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14

3.3 GROIrN'DSEQUENCE OF EVENTS (CONCLUDED)

Predicted Time Actual Time*

Event Nominal (sec) (sec),

Short Rast Nr. 4 Valve _r. 2 Open +3.39 +3.385

Support Retract Command +3 44 +3.395Retract Valve Nr. 4 Open +3 57 +3.544

Retract Valve Nr. 3 Open +3,58 +3.605

Retract Valve Nr. 2 Open +3 59 +3.620

Retract Valve Nr. l Open +3,61 +3.610

Support Nr. 4 Not Supporting +3 63 +3.610

Support Nr. 3 Not Supporting +3 64 +3.680

Support Nr. 2 Not Supl_rtlng +3 65 +3.680

Support Nr. I Not Su_portlng +3 67 +3. 676Launch Commit +3 67 +3.692

H. D. Release Valve Nr. I Open +3 72 +3.745

H. D. Release Valve Nr. 2 Open +3 72 +3.745

Hi D. Release Valve Nr. 3 Open +3 72 +3.745

H. D. Release Valve Nr. 4 Open +3 72 +3.758

HolddownNr. i Released +3 74 +3.758

HolddownNr. 2 Released +3,74 +3.763

Rolddown Nr. 3 Released +3 74 +3.763HolddownNr. 4 Released +3 74 +3.768

Liftoff Switch Nr. i +3 86 +3.950Liftoff S_ritch Nr. 2 +3 86 +3.953

Liftoff Switch Nr. 3 +3 86 +3.955Liftoff Switch Nr. 4 +3.86 +3.953

Liftoff (Tall Plug Eject) +3.96 +4.110

The times presented in this section may differ somewhat from those

event times shown in Volume l, due to refinement of event times based

on telemetered data and other functions. Thi_ difference is small

h0wever, usually in the order of 0.01 to 0.03 seconds.

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15

3.4ENVIRO_MEASUREMENTSDUP_NGLAI_NCH

3.4.1 VEHICLE

The Combustion Stability Monitor equipment performed satisfactorily

" during the launch of SA-3. The following vibration levels were re-

corded during the period from ignition to launch commit.

Meas. . Engine No. Max. (peak-to-peak) Average (peak-to-peak)

XE57-1 I 72.5 g 30 g

XE57-2 2 60 g 27 g

XE57-3 3 60 g 30 g

XE57-4 4 73 g 33 g

XE57-5 5 60 g 20 g

XE57-6 6 47 g 30 g

XE57-7 7 58 g 25 g

XE57-8 8 50 g 20 g

Fire detection measurements XCII4 and xCII5 gave no indication of

a temperature rise during the period between ignition and launch commit.

Measurements XCII6 and XCII7 gave a very slight indication of a tempera-

ture rise during this period (approximately 12.5°C).

3.4.2 LAUNCH COMPLEX 34

During the SA-3 launch, there were 37 ground support equipmentmeasurements taken. These included 19 vibration measurements, 8 static

pressure measurements, and I0 temperature measurements. Most of themeasurements were taken on theumbilical tower. The measurements,

their locations, and their calibration ranges are listed in Table 3-11.

Vibration Measurements

The locations of six vibration measurements made on the launch

pedestal during the SA,2 launch were duplicated during the SA-3 launch.The other thirteen were new measurements, located on the umbilicaltower.

Low frequency oscillations, below 15 cps, were noted in measure-

ments YE-7, YE-8, YE-II, and YE-12. This frequency is below the linearbresponse of the measuring system and therefore, the amplitude of thedata is distorted. Further analysis was not •possible since the degree

_ of distortion'was not known. Data from measurements YE-13, and YE-16

through YE-24, exhibited the same frequency spectrums during both the• holddown and liftoff periods

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16

TABLE 3-If

ENVIRO}_4ENTAL MEAS_S ON LAUNCH COMPLEX 34

Vibration Measurements

Mess. Direction Frequency Calibration

No. Description of Mess. Response (cps> Range (_+G's_

YE-7 Limit Switch ]_rk't, R-2 Long't 330 50

-8 Retract Valve, R-2 Long't 80 50

-9 Vent Valve, R-2 Long't ii0 25

-I0 Pneumatic Separator, H-2 Long' t 330 50

-II Pneumatic Separator, H-4 Long't 440 50

-12 Release Valve, H-2 Long't 160 25

-13 Tower, 30.5 m Level, SE Face Vert. 600 10

-14 Tower , 30.5 m Level, SE Face West 60 I0

-15 Tower, 30.5 m Level, SE Face South 790 I0-16 Tower, 48.8 m Level, SE Face Vert. 220 i0

-1-7 Tower, 48.8 m Level, SE Face West 160 I0

-18 .Tower, 48.8 m Level, SE Face South 790 i0

-19 Swing Arm Vert. 1050 25

-20 Swing Arm West 600 25-21 Swing Arm South 60 i0

-22 Swing Arm Mount Vert. 80 I0-23 Swing Arm Mount West 220 i0

-24 Swing Arm Mount South 160 10

-25 Valve Panel #4 Perp. 1050 50

Pressure MeasurementsCalibration Range

Mess. No. Description (k_/cm 2)

YD-9 Tower, 8.2m Level, South Leg 0 to 2.11

-10 Tower, 8.2 m Level, North Leg 0 to 2.11

-II Tower, 30.5 m Level, South Leg 0 to 2.11

-12 Tower, 30.5 m Level, North Leg 0 to 2.11

-13 Tower, 48.8 m Level, South Leg 0 to 2.11

-14 Tower, 48.8 m Level, North Leg 0 to 1.41

-15 Tower, 73.2 m Level, South Leg 0 to 1.41

-16 Tower, 73.2 m Level, North Leg 0 to 1.41

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17

TABLE3-_ (CONCLUDED)

ENVIRONMENTAL MEASLqIEMENTS ON LAUNCH COMPLEX 34

" Temperature Measurements

Calibration Range

Meas. No: Description (°C)

. YC-19 Tower, 8.2 m Level, South Leg 0 to 600

-20 Tower, 8.2 m Level, North Leg 0 to 600

-21 Tower, 30.5 m Level, South Leg 0 to 600

-22 Tower, 30.5 m LeVel, North Leg 0 to 600

-23 Tower, 48.8 m Level, South Leg 0 to 600

-24 Tower, 48.8 m Level, North Leg 0 to 600

-25 Tower, 73.2 m Level, South Leg 0 to 600

-26 Tower, 73.2 m Level, North Leg 0 to 600

-27 Retract Solenoid Valve, R-4 0 to 600

-28 Release Solenoid Valve, H-4 0 to 600

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18

It should be noted that the composite vibration magnitude (shown

in Table 3-111) is related to the cutoff frequency (Table 3-11) of the

particular measurement. For example, if the cutoff frequency of YE-7

was 790 cps instead of 330 cps, it is quite possible that this measure-ment would record a much higher composite value than was actually re-

corded. The reason for this is that more vibration, consisting of

higher frequency components, would be measured. However, this does

not preclude a comparison of the amplitude of the frequency spectrumsof the measurements. The amplitude of any frequency component, below

the cutoff frequency of the measurement, is influenced only by the elec-

tronic analyzing equipment. All the data has been analyzed such that

the frequency spectrum amplitudes are comparable.

Table 3-!II gives the frequency and amplitude of the major com-

ponent of the vibration energy concentration and the composite vibra-

tion magnitude of each measurement, during the holddown and liftoff

period§.

Measurement YE-18, located adjacent to YE-16 and YE-17, indicated

the energy to be concentrated at a higher frequency and with a higher

amplitude than either YE-16 or YE-17. However, this is probably only

due to the higher frequency response of YE-18.

Measurement YE-21, located adjacent to YE-19 and YE-20, did not

exhibit the higher frequency energy components as did YE-19 and YE-20.

This may be attributed to the lower (60 cps) cutoff frequency of YE-21.

The vibration energy of measurement YE-25 remained at essentially

the same frequencies during liftoff, as during holddown; however, the

amplitude was considerably magnified when the vehicle lifted off and

the exhaust gases impinged on the pedestal surface.

A comparison of the frequency distribution of the data taken onthe launch pedestal during the SK-2 and SA-3 flights is shown in Figure

3-1. The YE-7 spectrum for the holddown period of SA-2 was flat, where-

as the spectrum for SA-3 showed energy concentrations at 180, 280, and420 cps. However, since the frequency response of the SA-2 measurement

YE-7 was limited to 160 cps, no comparison can be expected above this

frequency. A similar situation exists for measurement YE-9; the fre-

quency response of the SA-3 measurement was limited to II0 cps, pre-

cluding any comparison of the data above this frequency.

The spectrum of measurements YE-10 and YE-II, for the liftoff

period, shows that the energy is concentrated at the same frequency,

but at a much higher amplitude on SA-3 than on SA-2. This higher ampli-tude of the SA-3 data may be attributed to higher excitation levels,

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19

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2O

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_ 21

GRMS YE- 7 GRM S YE -7

I.0 1.0

0.5 0.5-0 : : : : : 0 : : _ ' :

0 500 0 500

* Frequency (cps) Frequency (cps)

HOLDDOWN LIFTOFF

--SA-3

----SA- 2

Cm_s YE-Zz Gm_s YE-9

1.o _.o f,..,.

0 ------: : : : 0 i0 500 0 500

Frequency (cps) Frequency (cps)

LIFTOFF LIFTOFF

c_m_s rs-lo ¢n_s YE-IO

5.0 5.0

,, 2.5 2.5

o •."_--_-_--'--., • o0 500 0 500

s Frequency (cps) Frequency (cps)

HOLDDOWN LIFTOFF

FIGURE 3-1 COMPARISON OF FREQUENCY DISTRIBUTIONON SA-2 AND SA-3 FLIGHTS

MPR-SAT- 63-i

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22

during SA-3 liftoff, rather than a difference between the cutoff fre-

quencies of the measurements for the two flights.

Pressure Measurements

Eight pressure measurements were located on the umbilical towerat various levels.

Measurements YD-9 and YD-10 recorded an underpressure condition

from I sec after liftoff until 2.8 sec after liftoff, when the measure-

ments were lost. The magnitude of the pressure at the time the measure-

ments were lost was approximately 0.886 and 0.879 kg/cm 2, on YD-9 and

YD-10 respectively.

Pressures of 0.297 and 0.949 kg/cm 2 (underpressures) were re-

corded, by measurements YD-11 and YD-12 respectively, at 5.5 sec afterliftoff. These values give a net underpressure condition of approxi-

mately 0.652 kg/cm Z acting across the tower from north to south at thist_me. Measurement YD-12 also recorded an underpressure condition of

0.357 kg/cm 2 at I0 sec after liftoff. 2Measurement YD-13 recorded anunderpressure condition of 0.254 kg/cm at 7.2 sec after liftoff. Allthree of these measurements (YD-II, YD-12, and YD-13_ show that the

underpressure condition existed for about 30 seconds.

Measurements YD-14, YD-15, and YD-16 did not exhibit any slgnifi-cant data trends and these measurements were lost 3 sec.after llftoff.

Temperature Measurements

Eight temperature measurements were located on the tower at the

same levels as the pressure measurements. Two additional measurementswere taken on the pedestal. All temperature measurements were com-

mutated at the rate of ten samples per second.

None of the measurements YC-19 through YC-26 indicated any appre-

ciable rise above 24°C, and all of these measurements stopped recording

data at the same time (3.5 sec after liftoff). Measurement YC-2_ re-

corded a maximum temperature of 38°C at 4.7 sec after liftoff. After

this time, no more data was recorded. Measurement YC-28 recorded a

maximum temperature of 630°C at 3.8 sec after liftoff. Since the tem-

perature rose from 32°C to 630°C in 0.3 sec, it is suspected that the

temperature of the exhaust gases_rather than the valve, was beingmeasured. This measurement did not record any data beyond 3.8 sec afterllftoff.

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23

Possible Causes of Signal Loss and Erroneous Data

Investigation of possible causes of signal loss revealed that 23

measurements_ including all vibration measurements (except YE-11, YE-14,• E-21, and YE-22) and all temperature measurements on the towerp

utilized the s_,e voltage power supply. It was found that signal drop-

out in these measurements could be duplicated by short circuiting the

output of the power supply. A short circuit could be caused by sub-

jecting one of the accelerometers to intense heat. Physical evidence" showed that the accelerometer cables of measurements YE-7, YE-8, and

YE-9 weTe burned, thus the probability of a short circuit was very high.

It was also found that an intermittent short circuiting of the

power supply would introduce noise and erroneous data into some of the

measurements. This occurred for pressure measurements YD-14 and YD-15.

3.5 A_SPHEEIC SI_IARY FOR SA-3

3.5_ I INTRDDUCTION

This section contains information concerning the more important

aspects of the atmospheric environment for the flight of Saturn SA-3.

The atmospheric data are presented in a form which will allow easy com-

parison with similar data for ot_er space vehicle flights from the

Atlantic Missile Range. Wind and thermodynamic data are shown as a

function of both flight time and altitude. The general weather situa-

tiou for the flight area is discussed, surface observations at launch

time are given_ and upper air conditions near launch time, as measured

by rawinsonde and rocketsonde_ are given.

3.5.2 GENEEAL SYNOPTIC SITUATION AT LAUNCH T]24E

Pressure Distribution and Fronts. A high pressure cell_ with cen-

tral pressure near 1.04011 kg/emZ (1020 mb), dominated the launch area

at flight ti_2. A low pressure cell, with central pressure near1.02481 kg/cm (1005 mb), was centered ever the lower Ohio Valley; and

a cold front, embedded in a trough of low pressure, extended southwest-

ward across eastern Texas into Mexico. These pressure cells gradually

tilted westward with increasing altitude. There were no fronts in the

launch area,

Jet Streems and Associated Weather. Two Jet streams accompanied

the pressure distribution. The stronger jet stream swept eastward

across Kentucky and Virginia at about 55 Ks near ii km altitude. To

the south_ at about 12 km altitude_ a weaker jet stream moved eastward

through the Florida straits at about 35 m/s.

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L 24

Scattered high thin cirrus (ice-crystal) and scattered cumuliform

clouds, with bases near I km, were reported throughout the launch area

at launch time, but the combined clouds did not exceed 0.6 sky cover

at any point. Clouds did not obscure the vehicle flight path during

launch time except for the brief cloudiness caused by Project Highwater. •

Light (less than 5 m/s) winds, mostly southwesterly, prevailed near thesurface in the launch area.

3.5.3 SURFACE OBSKRVATIOHS AT LAUNCH TIME

Blockhouse Observations. Surface observations have been discon-

tinued at the blockhouse.

Launch Pad Observations. A recording anemometer on the launch pad,

13.4 m above ground level and 38 m north of the launch pedestal, showedthe wind to be about 3 m/s from the southwest, both before and after

the SA-3 launching (see Figure 3-2). The launch blast caused the winds

to shift rapidly through all directions for about 45 sec after ignition.

During this period, wind speed also fluctuated rapidly, varying fromzero to 14 m/s. The 14 m/s gust occurred at 12:45:08EST. These launch

time wind fluctuations are greater than those shown for the SA-I launch,

and are very similar to the fluctuations during the SA-2 launch, exceptthat the maximum launch gust was 2 m/s greater for SA-3.

Service Structure Observations. A recording anemometer on the

service structure, 95 m above ground level and 207 m southwest of the•Saturn launch pedestal, sho_ed the wind to be rather steady from the

southwest at about 3 n_s throughout the launch period. As on the SA-2

flight, no effects from the launch blast could be detected at this lo-cation. This is due to the fact that the surface winds blew from the

service structure toward the launch pedestal, in both cases. During

the SA-I launch, the winds on the service structure were moderately

disturbed, dropping from 9.2 to 4.1 m/s 10 sec after T-0.

Recording i_struments on the ground near the pad showed the launch

time ambient temperature to be 24.7°C, relative humidity 36 percent,

and the air pressure 1.03858 kg/cm 2. At 13.4 m above the ground, on

the service structure, the launch time ambient temperature was 20. I°C "

and the relative humidity was 48 percent. At 79 m above the ground, on

the service structure, the launch time ambient temperature was 21.4°Cand the relative humidity was 66 percent. The launch blast caused

minor vibrations of the self-recording instruments at both the 13.4 m

and 79 m levels.

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MPR

-SAT

-63-1

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.... 26

3.5,4 TIME AND SPACE VARIATIONS BETWEEN VEHICLE FLIGHT PATHAND

UP'PERAIR_UREHEN_ BY RAWI'NSONDEANDROCKETSONDE

Rawinsonde Path. A rawinsonde was released 5 km south of the

Saturn pedestal 35 min prior to T-0. The rawinsonde drifted 74 km east •

by south of the Saturn launch pedestal where it burst, at 32.25 km

altitude, 67 min after T-0, thus ending the observation. At that time,

it was 63 _=n east of the Immsition reached by SA-3, when SA-3 was at

the altitude where the balloon burst.

Rocketsonde Path. A meteorological rocket was fired, 122 min after

T-0, on almost the same heading as SA-3. The target was acquired 32 kmeast-southeast of the SA-3 launch pedestal, at 52 km altitude. At that

time, it was 7 km east-southeast of the SA-3 position, when SA-3 wasat the same altitude. While falling to 23.75 km altitude, the rocket-

sonde target drifted 28 km to the northeast, where it was lost 146 min

after T,0. At that time, the rocketsonde target was 33 km northeast

of the position reached by SA-3, when SA-3 was at the same altitude.

3.5.5 WIND DATA

Wind Speed and Direction. Wind speed and direction are in good

. agreement by rawinsonde, rocketsonde, and angle-of-attack measurements,

as shown in Figures 3-3 and 3-4. Winds were mostly from the southwest

quadrant and less than I0 m/s up to 4 km altitude. From 4 to 19 km

altitude, the winds were westerly and reached a peak speed, by rawinsode

and angle-of-attack measurement, of 31.3 m/s at 14 km altitude (83 sec

range time). Above 14 km, the wind shifted to southeasterly and the

speed decreased to near calm in the 21 km region. In the i0 to 14 _m

region of high dynamic pressure, winds averaged about 5 m/s less than

for the SA-2 launch. Above 22 km, the wind shifted back to southwest

and west, and increased in speed to reach an extreme of 68 m/s from the

west at 42 km altitude (123 sec range time), by rocketsonde measurement.

Wind speeds were near the 95 percent probability of occurrence level

from 30 to 42 km altitude. Angle-of-attack winds show speed and direc-

tion profiles similar to the rocketsonde wind profiles.

The SA-I winds reached 47 m/s from the west-southwest at 12 km

altitude (64 sec range time).

Wind Components. Range component winds were mostly from the rear

except in the low wind speed region from 20 to 25 km altitude, and

near the surface (Figure 3-5). The strongest range component, in the

high dynamic pressur,, region, was 30.7 m/s from the re r at 14 km

altitude (83 sec range time); but an extreme tail wind of 60 m/s was

measured at 42 km altitude by rocketsonde (Figure 3-6). SA-I had a

maximum tailwind of 36.8 m/s at 13 km altitude, and SA-2 had a 31.8 m/s

tailwindat 14 km altitude.

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27

_wlnsonde (17:10 to i8:42 Z)

Altitude (_) Angle-of-Attack Range T_e (sic)

35 _ "I16.5

. 30 -_'-" Z uo

_ --9_ probability

envelope

I00

- L_it Cu_e Based on 3o /variation in control fac- / i 80

no limitations occurred

I0 _ . for winds under the 95_envelope. --_ 70

_ 6o

' S _i 403020500 i00 I0 20 30 40 50 60 70 80

Wind Speed (m/s)

FIGURE 3-3 LOW ALTITUDE _ SITE_ SA-3 WIND SPEEDBY _W_SO_R _D _G_-OF-A_A_

I

MPR-SAT-63- I

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28_mRocketsonde (19:47 to 20:01 Z)

Rawinsonde (17:10 to 18:42 Z)

Altitude (km) Angle-of-Attack Range Time (sec)

55

135

50 " _b

130

45 __

I20

35

95% Probability

envelope

25 _ L.-._

I00

20 95

0 i0 20 30 40 50 60 70

Wind Speed (m/s)

FI_ 3-4 HIGH ALTITUDE LAUNCH SITE wIND SPEED FO_ SA-3 BY

BJOCKETSONDE, RAWINSONDE, AND ANGLE-OF-ATTACK

MPR-SAT-63- I

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-- gawlnsonde (17:10 to 18:42 Z)

.... Angle-of-Attack 29

Altitude Altitude (km) Range Time (set)

35 I. ,,_, 35 _.... 116.5

_r

El •I0020 20

_._ "_"'" ._o

• 115 ' 15 p

, :- | _. 8o

<. /I0 I0

Head' ". Wind From $_[.n'd from /eft

Wind 7 Wind _ right

j 6o

5 .¢" _, 5 _.2 r:_ fF !__ 50'40

-30• 200 0 _ i0

• -20 -I0 0 I0 20 30 40 -30 -20 -I0 0 I0 20 30 40;._ Wx Range Component (m/s) W z Cross Range Component (m/s)

FIGDRE 3-5 LALr_CH TIME WIND COMPONENTS FOR SA-3

_: _ (Rawinsonde vs Angle-of-Attack)

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--Rocketsoude (19:47 to 20:01 Z)

Rawinsonde .(17:10 to 18:42 Z)30 Angle-of-Attack

(km) Altitude (km) Range T (sec)

55

'135

so _ ___ -130

35 ..._-

_,. .Head Tail Jind Wind

Wind Wind from fromrigh! left

._ t.'K

L 1°°20 '95-I0 0 10 20 30 40 50 60 -60 -50 -40 -30 -20 -i0 0 i0

WX Range Component (m/s) Wz Cross Range Component (m/s) #

FIGURE 3-6 LAUNCH TIME WIND COMPONENTS ]FOR SA-3 AT HIGH ALTITUDE

(ROCKETSONDE_ RAWINSONDE, AND ANGLE-OF-ATTACK)

l_R-SAT-63-1

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: 31

Cross range components were mostly from the right above 25 km

(Figure 3-6) and reached a maximum of 57 m/s at 49 km altitude, by

roeketsonde measurement. In the high dynamic pressure region, the

strongest cross range component, by rawlnsonde measurement, was 11.3

m/s from the left at 12 km altitude. The maximum cross range component

for SA-2 was 13.3 m/s from the right at 12 km, and SA-I had 29.2 m/sfrom the right at 12 km.

Wind Shear. Wind shear profiles are shown in Figures 3-7 through

* 3-10. The wind shear discussed here is for the modulus of shear; that

• is, the absolute shear value. Because of their greater accuracy, it

is recommended that I000 m interval shears be used, in preference to

250 m interval shears, wherever possible. A table comparing extremeshears in the high dynamic pressure region, for SA-1, SA-2, and SA-3,is shown below.

Extreme Wind Shear (Rawinsonde) In High Dynamic Pressure Re_ion%

250 m interval I000 m interval

"-Pitch Yaw " Pitch Yaw

Space Plane Air Plane Alt Plane Aft Plane Aft

Vehicle (sec -I) (kin) (sec -I) (kin) (sec -1) (kin) (sec -I) (kin)

SA'i 0.0415 15 0.0350 16 ..........

SA-2 0.0261 14 0;0196 12 0.0144 15 0.0083 16

SA-3 0.0555 14 0.0205 13 0.0105 14 0.0157 13

High Resolution Wind Measurements. High resolution wind profilemeasurements were made, employing the FPS-16 Radar/Spherical Balloon

method, beginning at 19:56 Z (2 hr and Ii min after T-O). In view oftime (more than 2 hrs) and space differences, these wind measurementscompare favorably with the rawinsonde and angle-of-attack wind measure-ment s.

3.5.6 "THERMODYNAMIC DATA

Thermodynamic data were measured by rawinsonde to 33.25 km alti-

tude. Deviations of temperature, pressure, density, and index of re-

* fraction, from the Patrick AFB reference atmosphere, are shown in

Figures 3-11 and 3-12. Temperature, pressure, and density vary less

than 3 percent from the reference atmosphere at any level, and depar-tures are less than 2 standard deviations in all cases. The lowest

. ambient temperature measured was -73°C at 17 km altitude. The indexof refraction exceeded the PAFB reference atmosphere values by as much

as 36(n-l)106 units in the first 2 km above the surface. Above 4 km,

the index of refraction did not vary from the PAI_B reference atmosphere

by as much as 3(n-l)106 units, at any level.

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32]_esonde

A_le-o_-Attack

Altitude {km) Altitude (km) . Itange Time (sec)

99"/. Probability r99I '100Probeblllty

envel° 7 envelo_" 20

-J 90

_, \ \\

J ,. J0

0 0.01 0.02 0.03 0.04 0 0.01 0,02 0,03 0.0_

S x Wind Shear [_(sec -1) 8 z Niucl Sheer I_)(sec-1)

1;'ZGUIt]I 3-7 ILi.I_Z _ _ ]U,NCE _ WIND SHF,AR (1000 m)FOR 5A-3 BY _E AND ANG_E-OF-ATTAC_

Q

HPR-SAT-63-1

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33

Rocketsonde (19:47 to 20:01 Z)

Rawlnsonde (17:10 to 18:42 Z)..............Angle-of-Attack

Altitude (km) Altitude (km) Range Time (sec)

55 55

13.5

- I

50 50 _ -

_ 1so

<545 - _.,r-"-" 45 ,.- "_-I _

_-';._. _ I _ "---7 i40 f"'_;_'-.

/ /_ 120

• _. ._

""_--- _ 9/9% probability35 ....._ 35

k-c- I00

20 20 "_ 950 O. 01 0.02 0, 03 0 O. O1 0.02 0.03

, _ , IAh/ |AhJ

FIGURE 3-8 HIGH LEVEL RANGE AND CROSS RAI_E COMPONENTWIND SHEAR(i000 m) FOR SA-3 LAUNCH

MPR-SAT-63- i

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_- Altitude (kin) Range Time (sec)

4O

120

35 _ ,, ,

30 _ 11o

_-- f 99% i_robabilltyenvelope

• I00

20 _""

: 15

_ _ 8O

lo __ "_ 70

• oo

4O

0 100 0.Ol 0.02 0.03 0.04 0.05 0.06 0.07

Wl_d Shea_ I/_w:l<se¢-I) .. r

l"hlFIGqYRE3-10 SA-3 LAD_OI TIME CROSS RANGE COIqPO_NT WIND SHEAR

(250 m) ]PIAI_I.E-OF-AT_ACg MPR.-_AT-63-1

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36

Altitude (_ Altitude (_)

35 35

,J •3Ol ao ! /

i_ / _ J -! I _ /2_ 1 ( /

-20 , , +20

15 15

i/< \ "' h

\. !

_'' [ ' I

& ,\ / \,0 ¢ 0 "

0 4 -8 -4 0 4 8Perce_ _elati_e _iation Percent Relat_e Deviation

Of T_erature (_) of Density .

_CUEE 3-11 ItELET_ DEVIATZ_S OF _-3 _ SI_ TD_ERATUREO_ _ ¥_ _CE A_OSPHEEE

MPR- SAT-63 - I

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_:.._ Altltude (km Altitude (kin) 37

! 40 40

35 35

4

. 30 30 _ l

_.2o +2oI

!\ i_o _o \ !

15 _ 15

|If/

lO 1o \ /

\ /\ /

I5 5 _ Ii II| I

Q 0 0-20 0 20 40 -8 -4 0 4 8

_i Absolute Deviation of the Index Percent Relative Deviation" of Refract£on (n-1)106 of Pressure

• FIGIIRE 3-12 ABSOLUTE DEVIATION OF THE INDEX OF REFRACTION AND RELATIVE DEVIATIONOF PEESSURE FROM THE PAFB REFERENCE A_MOSPHERE FOR SA-3 LAUNCH SITE

MPR-SAT-63 -I

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4.0 JrscToRY

4.1 TRACKING ANALYSIS

4.1. I DATA SOURCES •

The data available for establishing the postflight trajectory onSA-3 are shown in Tables 4-I and 4-II. These tables include the

various types Of external tracking, the onboard measurements that areuseful in determining transients, and meteorological data. Tracking

from several systems was available throughout the powered flight (seeFigure 4-I). A sufficient amount of high quality tracking data was

available to establish a ballistic trajectory representing the vehicle

path from retro rocket burnout to water release. Some radar sites

even provided tracking beyond water release, thus indicating that the -

:: _ooster and _nstrument compartment retained structural integrity for:_ a. period of time after water release.

The electronlc tracking data obtained on this flight was somewhat

poorer than on the first two vehicles. Although no simple rule can be

given at this time for determining the relative quality of external

tracking that wily be appllcable to each flight, the random error of

the acceleration components during powered flight should certainly be

less than 1.0 m/s 2. This error is about i0 times larger than the

requested metric requirements for this flight. Periods of usable ac-

celeration components, from the electronic tracking data, during pow-

ered flight were:

' Trackln_ System Time Available

Azusa 76 to 160 sec;_ UDOP -MSFC 35 to 120 see

: UDOP - RCA 30 to 125 sec

: Radar None

_:" FPS-16 radar data was intermittent during the entire flight from

all stations. Retro rocket operation and the roll resulting from the

#_: firing of the retro rockets adversely affected all of the electronic

tracking data.

4.1.2 DATA IPEILIZATION

_;i The relative motion between the vehicle and support arms was deter-

:! mined from pad measurements YL-1 and YL-2, which were mounted on sup-,_' port arms R-2 and R-4 respectively. These were plunger type relative .-_i distance measurements. The results of the measurements are shown in

l_gure 4-2. First motion was determined from these measurements to be

O.I0 see range time.

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.__ 39

. _ TABLE 4-I

_gl_AI, DA_/_ SOURCE

Data Sourc_ Interval

"Close-in" Fixed Camera (light) 0.036 to 5.573 sec

6.774 to 10.910 sec

"Regular" Fixed Camera (nose) 0.338 to 27.237 sec

Theodolite 20.0 to 133.6 secL

Azusa 18.0 to 168.4 sec

211.3 to 254.4 sec

ODO£ (HSFC) 22.0 to 120.0 sec%

FPfl-16 Radar i.16 (Cape) Auto Beacon 0.0 to 92.0 sec

Auto Beacon 105.1 to 195.7 sec

Auto Beacon 202.0 to 235.9 sec

Auto Skin 244.4 to 312.8 sec

FPS-16 Radar 0.16 (PAFB) Auto Beacon 22.0 to 132.4 sec

....... AUtO Skin 186.0 to 323.0 sec

Auto Skin 368.0 to 456.0 sec/

FPS-16Radar 3.16 (GBI) Auto Beacon 84.0 to 191.0 sec

Auto Skin 191.i to 228.0 sec

Auto Beacon 239.0 to 260.0 sec

Auto Beacon 286.0 to 289.0 sec

Auto Skin 289. i to 408.0 sec

Auto Skin 432.0 to 471.0 sec

. FPS-16 Radar 42.16 Auto Beacon 90.0 to 190.6 sec(Carter Cay)

Auto Skin 202.0 to 278.6 sec

Auto Skin 325.0 to 352.0 sec

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_ 40

TABLE 4-11

•SUPPORTING FLIGHT DATA

Tilt Program Powered Flight Interval

Guidance Outputs 0.0 to 158.4 sec

Meas: 11-15, 12-15, 13-15, and 14-12

Longitudinal Acceleration 4Meas: F5-13 0.0 to 154.0 sec

F6-13 0.0 to 160.0 sec

F7-13 Decay to 160.0 sec

Cutoff Signals

,_ Observed Meteorological (to 33.4 km Alt.) 0.0 to 114.5 sec

Chamber Pressure

Meas: DI-I, DI-2, D1-3, DI-5, DI-6, DI-7,DI-8 0.0 to End Outboard DecayD1-4 0.0 to 73.6 sec

_pp, Hl-i5 0.0 to 158.4" s_c

_y, H2-15 0.0 to 158.4 sec

Separation, Anvil vs Vehicle Support Block:YL-I, YL-2 -4.0 to 1.0 sec

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:_-.

MP

R-SA

T-63-1

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_ 43

The trajectory, as shown in Volume I, was established in the

following manner (also see Figure 4-3):

&0.0 to 35.0 sec: "Close-in" and "Regular" Fixed Camera, and

Theodolite data used in a least squares curve

fit, assuming that an eighth degree polynomial

represents the flight path for that period of

time. The resulting curve fit of the data is

almost identical wg.th the original input track-

ing data. This procedure was followed to

establish smooth acceleration components dur-

ing the launch phase of flight.

35.0 to 62.0 sec: Theodolite data processed through a digital

, smoothing and differentiation program.

62.0 to 78.0 sec: Azusa position data processed through a

digital smoothing process. Velocity and ae-

" celeration components were calculated from on-board accelerometer and attitude data. These

calculated velocity and acceleration data

were corrected tO fit theodolite data at 62.0

sec and Azusa data at 78.0 seconds.

78.0 to 130.0 sec: Azusa position data processed through a

digital smoothing and differentiation program.

130.0 to 160.0 sec: The same procedure as use 4 in the Mach I

area (62 to 78 sec) to maintain the true

: characteristics of the large transients that

occur in the cutoff and decay sequence.

160.0 to 292.0 sec: A ballistic trajectory calculation using

Azusa data as initial conditions at 160.0 Sec,

_- and adjusted to be compatible with the avail-

able external tracking data after 160 seconds.

Measured meteorologlcal data and winds were used in the calcula-

tion of the trajectory from liftoff to 33.4 km altitude. Between

33.4 km and 47.0 km altitude, the measured data was adjusted to the

_i_ 1959 ARDC atmosphere. The 1959 ARDC _as used above 47.0 kilometers.

i%q 4.1.3 ERROR ANALYSIS OF ACTUAL TRAJECTORY

_' Good coverage for the launch phase was provided by the "Close-in"

and'%egular" Fixed Camera and the Theodolite Cameras. There was some

degradation in quality of the Radar and Azusa data during the first

_:

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MPR-SAT-63-1

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45

40 tO 50 sec of flight, because of surface environmental conditionsand multipath effects. All electronic tracking data were adversely

affected by retro rocket operation and the vehicle roll resulting fromretro rocket firing. All of the electronic systems appeared to resaln

good track for about 20 to 30 sec around 250 sec range time.

Figure 4-4 Shows a time history of the relationship between the

established trajectory and the available external tracking data duringthe first 170 sec of flight. Comparisons of the external tracking data

iwlth the established trajectory near cutoff and midway of the free

flight are shown in the following table.

Tracking System 150 sec 240 sec

_X(m) AY(m) AZ(m) L_X(m) AY(m) AF.(m)

Azusa 0 0 0 15 20 3

IIDOP -16 3 -I -i0 34 -22

Radar I. 16 -8 -18- 16 -0.16 - 3 4 92

3.16 404 -13 -97 16 31 30

...... 42.16 -12 61 -70 35 21 80

This table indlcates that the FPS-16 radar on GBI (3.16) was able

to track the vehicle much better during free flight than during powered

flight.

4.2 VEHICLE LIFTOFF I_0TION

Figure 4-5 shows the distance the vehicle traveled toward theumbilical tower, used on SA-3 for the first time, versus altitude.The vehicle attained an altitude higher than the umbilical tower at i0

sec range time .... :

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46

, _. 16 Radar

--Azusa / _"--UDOP /e--l. 16 Radar

o ___ ,{,/ --IX , I

-40 -0 20 40 60 80 I00 120 140 160 180

Range Time (sec)

FFi_ed Camera

I ¢-I. 16 Radar -. 16 Radar Theodollte.. .l J I. I_O

20 40, 60 80 - 100 120 140 160 180

]_mge Time (sec)

/

_z¢-)J,o

- ,--. 16_dar r [

__o . .:,u.. i___._o._.I .0 "_"20 40 60 80 100 120 140 160 180

Raltge T:L¢_ (see)

I_G01_ 4..4 Tg&CCINCCOl_Alttl_lS (I_AQ_NG_-REFER_CE)

MPI_-SAT-63-1

J

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@_ 47_?" Altitude (m)

-_ , 70

60

50

i 40

• .= 30

2O

::Cb; 0

-5 0 5 I0 15 20 25_ Distance to Tower (m)i FIGURE 4-5 ALTITUDE _rSDISTANCE TO TOWER

MPR-SAT-63-1

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!_c_. 48

. 5.0 (C) PROPULSION

5.1 PROPULSION SYSTEHDESCP.IPT_ON

_ The S-_ or booster stage of the SA-3 vehicle was powered by eight ,

i clustered H-I liquid propellant engines. Engines I through 4 were

designated outboard, while engines 5 through 8 were designated inboard.

The four inboard engines were fixed mounted on a 1.63 m (64 inch)

diameter circle with a 3 deg cant angle. The four outboard engines

were glmbal mounted to provide pitch, yaw, and roll control with a null

position cant angle of 6 degrees. The outboard engines hada maximum

gimbal angle of 7 deg in the pitch and yaw planes.

:i_- The SA-3 flight test was the first flight with a propellant load

i._ : of 355,300 kg (783,300 Ib) from discrete level calculations. This pro-pellant IDEW, which was larger than previous flights, was flight testedto simulate C-I Block }I ullage volumes in the S-I propellant tanks.

_i.:/ " The H-1 engine is a fixed thrust, single start type, bi-propellant

rocket engine. It is a derivative of the Thor-Jupiter-Atlas family of

_;!_ rocket engines manufactured by Rocketdyne Division of North American

_:_ Aviation..The SA-3 version of the engine produces a nominal 74,800 kg(165,000 ib) of thrust and has a nominal sea level specific impulse of252.7 seconds.

Liquid oxygen (LOX) and RP-I fuel are the propellants used as the

:_: main po_er source. A hypergolic fuel mixture is used for combustion -"

chamber ignition, and a solid propellant charge provides initial gas

to spin the turbine.

Major components of the H-I ehgine are a thrust chamber assembly,

:_ turbopump assembly_ gas generator assembly, hydraulic system (outboard

_i_: engines only), and a hypergolic ignition system.

The exhaust gases from the turbine are handled differently in the

' outboard and inboard engines. In the case of the outboard engines,

_ the exhaust is routed rearward through the heat exchanger and into an

_!_ aspirator. The aspirator is welded around the periphery of the expan-

d. slon nozzle ex£t to fom an integral part of the thrust chamber. Use

_,i_ of the aspirator on the gimbaled engines allows removal of the hot. gases from. the engine compartment without the need for flexible Joints_: in the turbine exhaust ducts. The exhaust gas from the inboard engine

turbine is routed laterally from the heat exchanger through the outer

_:_ vehicle skln_ then ejected rearward.,_:_,:_.'-_'_ Propellants were supplied to the engines through suction lines

_i, from an arrangement of nine propellant tanks. These tanks consist of

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_i_ __ ._.__t_r_Wl_l_l_, 49

four 1.778 m (70 inch diameter) LOX tanks, four 1.778 m (70 inch diam-eter) fuel tanks, and one 2.667 m (105 inch diameter) LOX tank. The1.778 m fuel and LOX tanks are mounted alternately around the circum-

ference of the center LOX tank, Each outboard tank (LOX and fuel) sup-

plies propellant to one inboard and one outboard engine. The center

LOX tank is used to supply the outboard tanks through the L0X inter-

=hange system and does not supply LOX directly to any engine.

• LOX tank pressurization was provided by gaseous oxygen (GOX). The

• COX, whichwas obtained by passing L0X through a heat exchanger (one

for each engine), was routed to a COX manifold and distributed to allLOX tanks. Pressurization of the fuel tanks was provided by gaseous

nitrogen (GN2) Supplied from 48 storage spheres located atop the pro-pellant tanks.

Eight outriggers and a spider beam assembly support the outer pro-

pellant tanks. The LOX tanks form the basic structure, with the fueltanks mounted to allow for thermal contraction of the S-I stage struc-

tural elements. All four fuel tanks are interconnected at the base

through the fuel interchange system. Baffles, used to prevent propel-

lant sloshing in the tanks, may be seen in Chapter 7.0.

A propellant utilization (PU) system was flown as a passenger on

this flight to obtain flight data for performance evaluation of the

system. The system utilized two (one for LOX and one for fuel) differ-ential pressure transducers for propellant weight information. Signals

from the transducers were sent to a computer for mass ratio determina-tions.

5.2 INDMDUAL ENGINE PERFORMANCE

A schematic of the H-I engine is shown in Figure 5-1.

Total thrust and specific impulse for each engine is shown in

Figures 5-2 through 5-9. These curves indicated that the flight data

showed no significant deviation from predicted data. A more detaileddiscussion of the individual engine performance is given in Volume I.

5.3 FLIGHT SIMULATIO_ OF CLUSTER PERFORMANCE

qThe vehicle •specific impulse, thrust, and total weight loss rate

; were derived from the telemetered propulsion system measurements in a

simula_tlon of the tracked trajectory. Measured values, or best esti-

i mates, of the liftoff weight and propellant tanking weights are partof the inputs required, in addition to the propulsion system measure-

ments that are used as inputs, for the differential equations which

represent the vehicle's powered flight motion.

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r

•. " " • _R-SAT-63-1

_, -"..

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Specif'Lc _mpulee (see)30O

280 " I

OECO

260 /

_s Reconstructed." ]Predicted

240

220-;' 0 20 40 60 80 100 120 140 160

Range Time (sec)

Thrust (1000 kg) Thrust (1000 lb)88

190

: ,-" 180

80 /

OECO 170

76 /

•• .- Calculated from

S Measured Data' Predlcte_ 160

72

68 150:0 20 40 60 80 I00 120 140 160

Range Time (sec)

"FIGURE 5-2 THRUST AND SPECIFIC IMPULSE, ENGINE POSITION I

.... l_R-SAT-63- I

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, • - £

52Specific Impulse (see)_oo

|

280 f J""" ""

/_/. ,J OEC0

260' /,/.J"_" ....--" Reconstructed---'-'--"" -------- Predicted

240 ,,

2200 20 40 60 80 I00 120 14( 160

Kanse Time (sec)

•Thrus¢ (1000 kE) Thrust (I000 Ib)88

.... 190

• 180

80

OECO 170

76 j ........ -- Calculated from

f Measured Data.... Predicted 16072 r:.

68 , 1500 20 40 60 80 I00 120 1441 160

5-3 THRI]STAND S_ECI'FZCD_PULSE,ENGXNEPOSITION 2

MPR-SAT-63-i

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3O0

z8o /

" _ '// .... OECO260

_._ Reconstructed.... Predicted '

i _ . -

240o.

22020 40 60 80 100 120 140 160. Range Time (see) .

Thrust (I000 kg) 'thrust (1000 Ib)

88 . ,.

190

...... _ . .180

1

8o _

,e_ '_/ OECO 170

76 _'_/ , Calculated from

" .Measured Data

i" Predicted :'72 / 160

' ! f

If 68 zs0i " _ 0 20 40 60 .. 80 100 120 140 160

I: Range Time (see),FIGURE 5-4 THRUST AND SPECIFIC IMPULSE _ENGII_ POSITION 3

i

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Speciflc Impulse (sec)300

280

.j" OECO

260 _'7"_Reconstructed(extrapolated after 73 sec).... Predicted

240

2200 20 40 60 80 100 120 140 160

Range Time (met)

88

0EC0. 190

I

; 170

.'_ _ _ Calculated from Heasured Data i(extrapolated after 73 sec) i

_ _ --_-- Predicted

" / 160 .72

'_, 68 150o 20 40 60 80 IO0 120 X40 t60

Range Time . (see..)

5-szmws__ se,,ci_c __rs msrrr_ 4• _ ..._j_ -

.i

MPR-SAT- 63-i

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_, - o . 55

Specific Impulse (sec)

300

280 I_-_-"_"

- _ECO

260

Reconst_cted. Predicted

240

-22020 40 60 80 100 120 140 160

Range Time (see)

Thrust (lO00kg) _nz_zst (I000 Ib)

88

190

-2' "/ 180y80 /!

170

76 " ..e'

': Calculated from

////_ Neasured Data "Predicted 160

72 •

[ " 150I 68I 0 20 40 60 80 100 120 140 160

RangeTime (sec)

H]FR-SAT-63-1

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565!

• Specific _r.mpulse (see)" 300

280

_ECO

J• 260 "_

/ _ Reconstructed.... Predicted

240 '-

2200 20 40 60 80 I00 120 140 160

Range Time (sec)

Thrust (lO00 kg) Thrust (1000 lb)88

190

//_/ 180

80 / _j/

,/ 170

76 Z

Calculated from

J Heasured DataPredicted 16072 _,

_, 68 1500 20 40 60 80 I00 120 140 160

Range Time ($ec)

Ir£G_E 5-7 THRUST AND SPECIF£C _4PU_E ,ENGINE POSI_ON 6

: " ._ ""*_. f._.;, :_" _'_'2,:,':. MPR-SAT-63 - I

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Specific I_pulse (see)3O0

i,

280

.j IEO_

260 jReconstructedPredicted

240

2200 20 40 60 80 100 120 140 160

Range Time (see)

Thrust (I000 kg) Thrust (I000 ib)

88

190

i /

80 // _ 180

/_ IECO

- 170

75

• Calculated from

, _._ Measured Data

72 /_ Predicted 160\

68 1500 20 40 60 80 100 120 140 160

Range Time (sec)

FIGURE 5-8 THRUST AND SPECIFIC D_ULSE ,ENGINEPOSITION 7

MPR -SAT -63 -i

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Specific T_pulse (see)3OO

-° jj-I . IECO

260 y"ReconstructedPredicted

240

2200 20 . 40 60 80 100 120 140 160

Range Ti--=e (see)

Thrust (1000 k8) Thrust (1000 Ib)88

190

J/_/ ZECO 180

76 r_,-'_/J _'/ 170

Calculated from

Measured Data

Pred'[cted 16072

68 1500 20 40 60 80 100 120 140 160

Range Tlme (sec)

I_GIIRE 5-9 THRUST AND SPECZI_C ;]_'LSE,ENG'INE POSITION-8

lq1_!_ _ _: A,,V_ _":t 1_

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'_'. ' : i " " ., %':'..,

_, .. _ :.....• 59

Many combinations of specific impulse, thrust, and flow rates,

which will satisfy the tracked trajectory within its accuracy limita-

" tions_ can be derived if the llftoff weight and propellant tanking

weights are allowed to vary.

Mean sea level vehicle specific impulse is shown versus liftoff

- weight in the upperportlon of Figure 5-10. All the values of specific

impulse and liftoff-weightwhich fall on the solid line will satisfy

the trackedtrajectory very closely. Those values which lie within

the dashed lines will satisfy the tracked trajectory within its accu-racy limitations.

Mean vehicle total weight loss rate is shown versus mean sea level

vehicle thrust in the lower portion of Figure 5-10. Points correspond-

" ing to a variation of T 0.5_ in liftoff weight are also shown in th_s

figure.

The differences between the earth-fixed velocities and slant dis-

tances_ determined from the computed and tracked trajectories, are

shown versus range time in Figure 5-11. The maximum difference between

the velocity for the actual and simulated trajectories was less than

0,5 m/s. This can he used to judge the quality of the simulation of

the cluster performance. - •

5,4 PR ssm ZATZOSYSTm

- 5.._.i..1_. t TANK PRESSURIZATIOn

Figure 5-12 sh&ws a schematic of the SA-3 fuel system. This sys-

tem is identical to that used on SA-I and SA-2, and performed satis-

factorily during flight. Fuel tanks were initially pressurized during

automatic seque,ce, which started with firing command. Initial pres-

surization was aehi@ved in approximately 4 sec_ which was 15 sec shorter

than the pressurizing time for SA-2, and was due to the decreased inltialullage volumes. Fuel tank pressure throughout flight was limited to amaximum of 1.20 _ 0.04 kg/cm 2 (17,0 T 0.6 psi gauge) by a pressure

switch sensing fuel tank_F-I ullage pressure. Ullage pressure decayedfrom 1.185 kg/em z (16.85 psi gauge) after initial pressurization to

" \ 1.15 kg/cm 2 (16.4 psi gauge) at liftoff. During flight, a maximum

ullage pressure of 1.17 kg/cm 2 (16.6 psi gauge) was reached at 60 secand a minimum of 1.02 kg/cm z (14.5 psi gauge) at 30 sec (Figure 5-13).

After cutoff, ullage pressure increased to 1.18 kg/cm 2 (16.8 psi gauge)at 160 sec, and activated the ullage pressure switch which stopped

nitrogen flow into the fuel tanks.

-'_ . _ :: '_: _" i:_I_ _"_."_i ._ _ "

.'j _, ,...; ,= , '_.._.'_

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: 63

Pressure (kg/cm 2 gauge) . Pressure (psi gauge)

210

• \... :._. : : 2800

190

2600

High Pressure Spheres

170 2400

150 __. 2200

2000

130 . _ , 1800

\ * " 1600

II0

1400

90 '_1200

70 i0000 20 40, 60 80 I00 120 140 160

Range Tfme (eec)

Pressure (kg/cm 2 gauge) Pressure (psi gauge) •

1.6 .... I 22

• Fuel Tank,/ F3 _Predicted 20

" Max _S_rit h Pickup : | ___ 18

I., , 16%,

-=-=-4_ \ 14. Max Switch Dropout Measure a-_

I | 120,8

0 " 20 40 60 80 100 120 140 160Range :rime (sec)

I_GURE 5-13 GAS PRESSURE IN HIGH PRESSURE SPHERES AND FUEL TAI_, F3

IMPR-SAT-63- I

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64

$,4.2 LOX TANK PRESSURIZATION SYSTH4

Figure 5-14 shows a schematic of the SA-3 LOX system. The initial

pressurizatio n of this system was provided by helium from a ground

source. In flight, the LOX tank pressur_zatlon is provided by gaseous

oxygen (GOX). The simulation of Block @I ullage volumes and the effect

of this reduced volume on the LOX pressurization system was one of thespecial missions of SA-3.

LOX tank pressures and temperatures are presented in Figure 5-15.

The temperatures were as expected; however, the reduced ullage volumeaffected the accuracy of the predicted characteristics of LOX tank

pressures. Therefore, the prediction technique will he refined forBlock II _hicles based on results of this fllght.

5_4.3 CONTROL PRESSURE SYST_4

The control pressure system, shown in _IEure 5-16, operated satis-

factorily during flight. This system consists of a high pressure,

21i kg/cm 2 (3000 psi gauge), GN2 supply; a 53 l_/cm Z (750 psi gauge)regulatoT; and a regulated pressure manifold, from which is taken con-t_ol pressure for the control valves, vent valves, and prevalves. This

manifold also supplies 53 T i kg/cm 2 (750 T 15 psi gauge) pressure for

gearboxpressurlzation, LOX seal, and calorlmeter purge. The controlsystem pressure decay over flight is shown in Figure 5-17. This regu-

lated pressure decayed over flight, as was expected with a gauge typeregulator.

14.4 sm, sYs .

:_ The purpose of the air bearing supply is to provide clean gaseous

nitrogen at a predetermined flow, temperature, and pressure to the airhearings of the ST-90 and ST-124P stabillzed platforms. This pressure

was supplied to the ST-90 and ST-124P by two separate but identical

system_

Prior to flight, the O.O14m 3 (0.5 ft3) spheres were charged and

_eplenished tO a pressure of approximately 211 kg/cm 2 (S000 psi gauge)

by ground support equipment. The GN 2 then flowed from the sphere_hrough a filter to the pressure regulator, where the high pressure

was regulated to a predetermined Io_ pressure. From this pressure

Kegulator, the low pressure GN 2 wasdirected through the orifice and_he normally open solenoid valve in the regulator assembly, to the

_hermostatlcally controlled heater, where it was maintained at a con-

stant temperature (25 T I°C). The GN 2 flowed from the heater, through

i_,other filter, to the air bearings (see Figure 5-1S). Sphere pressure

i

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MP

R-SA

T-63-1

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66

Gas Pressure in LOX Tanks (kg/cm 2) (psi)

6

80

S ...... L7O

t-_3-°c__/-- ._-o_

--PredlccedD3-0eD3-03_

3 . I0 20 40 60 80 I00 120 140 _60

Range Ti_e(sec)

Temperature in _ tanks (°C) (oF)

150 300

FIGURE 5-15 EtlISSURE AND _ERA_IRE IN LOX

IqPR-SAT-63-1

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!HPR-SAT-63-i

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68

Pressure Control EqulpmenttSupply (kg/cm 2) (psi)

3004000

3000,200 "-

2000

loo1000

" 0 ' 00 20 40 60 80 100 120 140 160

Range Time (sec)

rressure Control Equ£pmenc, Regulated (kg/cm 2) (psi)8O

UO0

70 .... 1000

9OO

6O

800

50 '- ' • ...... 7OO

60040

0 20 40 60 " 80 100 120 140 160Range Time (lec)

1_ 5-17 CONTROLP.qUTlq4_T PRESSU_

141_-SAT-63-I

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69

iMPR-SAT-63-!

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7O

was monitored during preflight by a high pressure OK switch. This

switch was set to maintain a sphere pressure between 225 kg/cm 2

(3200 psi gauge) and 183 kg/cm2 (2600 psi gauge). A low pressure OK

switch was in the system to shut off electrical power to the stabilized

platform and close the solenoid valve in the regulator assembly if

sphere pressure dropped below the switch setting. The switch was setto actuate on decreasing pressure at 103.7 T 4.9 kg/cm 2 (1475 T 70 psi

gauge) with a maximum actuation differential pressure of 5 kg/cm 2.This assured an adequate flow of GN 2 through the orifice to the air

bearings, to prevent damage while the gyroscopes decelerated.

Figure 5-19 shows the air bearing supply pressure actually suppliedto the air hearing. This low pressure air to the air bearing of the

ST-902decayed slightly from 2.41 kg/cm 2 (34.3 psi) at 32 sec to 2.37kg/cm (33.7 psl) at 150 seconds. The low pressure to the ST-124P re-maimed constant at 2.24 kg/cm 2 (31.8 psi).

5.5 PROPEILANTOTILIZATIONSYSTEM

A schematic of the propellant utilization (PU) system is presented

in Figure 5-20. This system was flown as a passenger on this flight

to obtain flight data for performance evaluation of the system. The

system utillzed two (one for LOX and one for fuel) differential pres-sure transducers for propellant weight information. Signals from thetransducers were sent to a computer for mass ratio determination.

LOX level in tank 04 and fuel level in tank F2, shown throughout

powered flight in Figures 5-21 and 5-22 respectively, are indicativeof the rate of propellant utilization as well as total utilization.The levels were calculated using the propellant tank differential pres-

sure data, the propellant densitites, and the vehicle longitudinal ac-celeration. The calculated LOX level Was higher than predicted except

from ii0 to 135 seconds. The calculated fuel level was at or above

the predicted value throughout flight.

:The LIP measurements from the PU system, for the LOX and fuel con-

tainers, are compared to the predicted differential pressures in

Figure 5-23. Also shown is a comparison of the calculated AP ratio,from the measured LOX and fuel container _P data, with predicted.

5.6 }P/DRAOLIC_S_

The performance of the hydraulic system is monitored by the fol-lowing groups of measurements, one group for each independent system:

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71

Air Bearing Supply Pressure (kE/cm 2) (ps£)3.0

42

2.8 40

I 38

2.6

36--ST-90

2.4 _ -- 34

32

,7-,--ST-124 30

2.00 20 40 60 80 100 120 140 160

Range Time (sec)

FIGURE 5-19 AIR BEARING SUPPLY PRESSURE (ST-90 AND ST-124)

MpRmSAT-63-1

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F-2 0-4

__/FIGURE 5-20 PROPELLANT UTILIZATION SYST_4

MPR-SAT-63- i

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73

00

00

0

I.,

,,

,o

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74

00

00

00

oo

=o

oo

II

,,

,,

MPR-SAT-63-I

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75

A p, FU Computer, LOX, Fine (kg/cm 2 ) (psi)

3 40

Measured

* _ 30Predicted _ 20

1 _"_,_ I0

0 00 20 40 60 80 i00 120 140 160

Range Time (sec)

AP PU Computer, Fuel, Pine (kg/c_ 2) (psi)

340

302

m---Measured

i _ --_ I0Predicted

0 00 20 40 60 80 i00 120 140 160

Range Time (sec)

Ratio (Ap LOX/_P Fuel)

2" iPredicted

. • /Calculated from Measured

•, Propellant Tank dF's ------

o l [20 40 60 80 I00 120 140 160

_ Range Time (sec)

._ FEGUEE 5-23 _ PRESSURE PU COMPUTER(FINE), LOX AND FUEL,AND PROPELLANT trfILIZAT_ON COm_Y_R o_nYr (_)

i

___ MPR-SAT-63-1

_.

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76

Meas. No. Measurement

C59-(I-4) Temperature, Hydraulic 0il

D29-(I-4) Pressure, Hydraulic Source

D32-(I-4) Pressure, Hydraulic Return

G8-(I-4) Level, Hydraulic Oil

The telemetered data from the SA-3 flight indicated that operation

of all four hydraulic systems was satisfactory. All temperature, level,

and pressure measurements remained within acceptable operating limits.

Source pressures remained within the band indicated in Figure

5-24. Fluid temperatures (Figure 5-24 for engine positions I through

4) agreed with all previous data, and showed a gradual 6°C (10oF) to8oc _lb°F) decrease from approximately 40.6°C (105 F) at ignition.

Specified fluid temperatures were between -17.8 and 98.9°C (0 and 210°_." The hydraulic oil levels (Figure 5-257 remained constant throughout

flight, with a high of 53 percent for engine position 3 and a low of

40 percent for engine position 4. All of these levels are within the18 to 68 percent specifications. The hydraulic oil return pressures

(Figure 5-25) remained constant throughout fllght. Constant levels and

source pressures indicate that the average actuator demand during flightwas well within the pump capacity.

Figures 5-26 and 5-27 show the hydraulic source pressure and level

after outboard engine cutoff. These curves indicate that an engine

glmbaling capability exists for approximately 9 sec after engine cut-off.

J

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•i_'_;"

77

• TemperatureHydraulic Oil (°C) (°F)

100

200

80

150

60

Band Determined by FourOil Temperatures

20

•50

00 20 40 60 80 i00 120 14o 16o

Range Time (eec)

Pressure Hydraulic Source (kg/cm 2) (psi)

300 ! _ ,4000Band De_ermined by Four

Source Pressuresi

200

2000

o i00"i000

0 0• 0 20 40 60 80 I00 120 140 160

Range Time (sec)

FIGURE 5-24 HY])RAS'L_COZL_EBATHREAh'D SOURCEPRESSURE(ENGINE POSITIONS 1 THROUGH4)

MPR-SAT-63-1

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78

l_.eservoSr Level (7.)

6O i

_ _ _-:_............_._ .....

Band Determlnedby l_our0£1 Levels

20

O ....

0 20 40 60 80 100 120 140 160Range Time (sec)

Fressure Hydraulic 0ii Re_urn (k_/an 2) (psi)I0 140

1208

100

680

R_urn l_ressures

, 60

_"_ 2

20°

0 00 20 40 6 0 80 100 . 120 140 1160

. Range Time (sec)

I_GUR_ 5-2.5 HYDRAULZC OIL LEVI_ ARD R_JL'Ui_N_SSURE

_ ' MPR-SAT-63-_

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r _._

!;' Pressure

Level _) Hydraulic Source Pressure (kg/cm2 gauge) (psl gauge)

100 50( -- 7000

G8-1 Level

6000

80 40( , |

• Retro Rockets J 50000ECO Ignite

60 30C / 4000

i

40 200 -'_=- 3000

.2000

20 100

i000

D29-I SourcePressure

0 0 I "- 0148 150 152 154 156 158 160

Range T_me (set)

Pressure

• Level (%) Hydraulic Source Pressure (kg/cm2 gauge) (psi gauge)

100 T 7000. Level

6000.. 80

Retro Rockets

: 500O

OEC0

60

4000

_: 40 3000

.. 2000it, 20

_: 1000D29-2 Source

Pressure

0 0148 150 152 154 156 158 160

Range Tl.me (set)

'_ FIGIIRE 5_26 HYDRAULIC SOL_ECE PRESSt_JE AND LEVEL

L£ _R-SAZ-63-Z

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,;7 .-%..:_ - _.. _ _.': _. _ : .- .

Pressure

Level (%) Hydraulic Source Pressure (kg/cm 2 gauge) (psi 8auEe )

100

G8-3 Level / 7000

1%eCro Rockets I

Ignite 6000J

80 /OECO J 5000

60 I r_ "' 4000

40 _'_ 30002000

20 i_ _ I000D29-3 Source

Pressure

• 1 h o148 150 152 154 156 158 160

Range Tlme (see)

Pressure

Level (%) Hydraulic Source Pressure (kg/cm 2 gauge) (psi gauge)

100 _ T 7000!

G8-4 Level

. 6000_: 80

e

,.. Retro Rockets 5000Ignite

. OECO60'

•_ 4000

30OO_ 40

2OOO

20

D29-4 Source I000•_" Pres sure

0 0148 150 152 154 156 158 160

Range Time (sec)

FIG_T.E 5-27 HYDRAITr_tcSOUgEE PRESSURE AND LEVEL

• : MPE- SAT -63-1

.;/_ _ _'_ . . _ _ " , _:..

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• _ 6.0 (c) MASS_CTERISTICS

6.1 WEIGHTMEASUREMENTACCURACY@

• The .weight measurements for vehicle total weight (on-pad) consistof component dry weights, propellant loading weights, ice accumulation,

auxiliary fluids, and other miscellaneous weight items.

For flight simulation and flight reconstruction programs, the

agreed liftoff weight is assumed to be accurate to within T 0.25_ ofthe actual value.

6.2 PROPELLANT LOADING

The Saturn propellant loading system is designed to tank propel-

lants to a given total weight, at a ratio to give simultaneous deple-tion at cutoff. By design_ it is easier to drain fuel and tank LOX,

than to tank fuel and drain LOX, for final adjustments. A final fuel

density check is made prior to flight. Fuel is drained and LOX is

tanked to the proportions necessary to give the desired total propel-lant load based on the final fuel density check. The design goal for

the system was to load propellants to an accuracy of 0.25 percent total

weight load. Tanked propellants of 355,600 kg (784,000 Ib) agreed wellwith the discrete level calculations of 355,300 kg (783,300 Ib), or

within approximately 0.i percent.

The following is a summary of the fuel (RP-I) and liquid oxygen

(LOX) loading operations performed and a list of the malfunctions anddeviations observed in the propellant loading system. Also included

are final settings of the tanking computers and readings of the backup_; manometers. The SA-3 vehicle was flown with approximately the same

propellant tank ullage that is expected on SA-5.

i. Fuel (RP-I). RP-I fuel was loaded on T-2 days. The tanking

was accomplished similar to SA-I and SA-2, with the following excep-: tions. The tanks were filled to less than I00 percent (based on a com-

puter ZIP of 1.0873 kg/cm2). At this level, the overfill pressure'.__ switch was "Jumpered out" (because of a previous difficulty), and the

• level was raised to above I00 percent (based on a computer _P of

1.1189kg/cm 2) by using the replenish sequence. Upon completion of

__ the EP-I tanking, the density computer indicated 99.05 percent of nomi-_' nal density.

_o . No coarse adjust level drain was made, due to the small over-

_iiii_ " fill above I00 percent. The final level adjustment, made at T-90

minutes, was an adjust level drain.•

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At T-90 minutes, the density computer indicated 99.53 per-

cent of nominal densit_ and, according to the loading tables, a correc-tion of -'0.00738 kg/cm _ was to be used in the level adjustment. When

this value was dialed into the computer, the "out of tolerance" llght

illuminated on the Computer. _t wa_ attempted several times to dialin the correction of -0.00738^kg/um ; however, the closest that was

attainable was -0.00668 kg/cmZ. During the remainder of the countdown,the density increased to 99.59 percent, which calls for a correction

of -0.00668 kg/cm 2 (the same as that used for the final adjustment).

Fuel density versus fuel temperature, as shown in Figure 6-1,

was detemined from fuel analysis data. Blockhouse fuel temperature

data, fuel density probe data, and fuel pump inlet temperature data

are also shown in Figure 6-1.

, 2. Li_uld OxTsen (LOX). Launch day LOX tanking was accomplishedsimilar _ SA-I and SA-2, with the 100 percent LOX level set at a

computer AP of 1.4543 kg/cm 2.

The LOX replenish system was used for the final LOX level

adjustment. A correction of +0.00422 kg/cm 2 was dialed into the LOX

computer, and the new 100 percent level (based on a computer _P of

1.4585 kg/cm 2) was maintained by automatic replenishing. The replenlshrate control setting was 0.400.

3. Propellant Loadln_ Computer System. Listed below are thefinal settings for the tanking computers and the readings of the backupmanometers at T-15 minutes.

Backup

Computer Manometers Deviation

(kg/em2) _kg/_ 2) ,_),

L0X AP 1.4585 1.4594 0..06

Fuel Ap 1.0982 I.1003 0.2

Fuel Density AP I.0226 i.0224 0.02

4. Loadln $ System Malfunctions and Deviations°

a. The fuel loading computer pressure correction readout

indicated"out of tolerance" when a -0.00738 kg/cm 2 correction factorwas dialed.

b. When the IEX replenish tank pressurization valve was

closed, the stem remained approximately 0.08 cm above the seat, causing

intermittent venting of the replenish tank. This did not impair normal

LOX loading.

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_'_:_;:"_::"_

_""__'_

__.;_"__""

MPR

-SAT

-63-1

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_84

c. The replenish llne vent valve was freezing open and hadto be thawed to allowuorma_ operation.

d. The replenish vaporizer experienced heavy icing on thefinned tubes and the excess ice had to be thawed to allow continued

sto_age tank pressurization.

e. A deviation occurred, in that the fuel system slow fill

push button was pressed at 78 percent to allow the uneven levels in

the fuel tanks :to settle before the tanks were completely full, and to

provide a slow fill condition (about 0.757 m3/mln) as the tank filled

to i00 percent.

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_" 85

7.0 (U) CONTROL

7.1 SUMMARY

The basic flight results of the control system performance are

given in Volume I of this report. Here in Volume II are presented

• supporting data for Volume I.

Pitch and yaw simulations of the vehicle dynamics are compared

with flight results. A discussion of the control aspects of the bending

oscillations after OEC0 is also presented. Functional analyses of the

angle-of-attack meters, controlaccelerometers, and sloshing measurements

are presented to supplement the discussion made in Volume I.

' 7.2 CONTROL SIMULATION

7.2.1 PITCH PLANE

The results of the digital simulation for the pitch plane are

compared with telemetered attitude, average actuator position, and

free-streamangle-of-attack in Figure 7-1. The mathematical model used

for the digital simulation includes the dynamics of the first elasticmode and the first sloshing mode. The control system filter network

and swivel engines are represented by the appropriate transfer functions.

Close agreement of the simulation trajectory with the tracking trajectory

was obtained by using the best estimate of the actual weight and engine

performance. The wind input data was obtained from the angle-of-attackwinds calculated from onboard measurements (see Figures 7-3 and 7-6 in

Volume I). The simulation gives a good representation of the actual

control system response during the oscillations, which are primarily

due to wind gusts. Some of the small oscillatory motion, appearing

in the engine deflection and angle-of-attack, may be due to propellantsloshing. No attempt was made to phase the sloshing, in the calculations,

with the actual flight history of propellant sloshing.

7.2.2 YAW PLANE

• A comparison of the yaw plane simulation with actual flight results

is shown in Figure 7-2 from 50 to Ii0 seconds. Again, the attitude,

free-stream angle-of-attack, and average actuator position show close

agreement with the simulation program.

• 7.2.3 BENDING OSCILLATIONS AFTER CUTOFF

As mentioned in Volume I, the cutoff of the outboard engines at

149.09 sec excited vehicle bending in both pitch and yaw. Figure 7-3shows the oscillations as measured by the pitch and yaw control

h

7_

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HP

R-SA

T-63

-1

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accelerometers. The pitch plane bending indicates neutral, and even

• negative stability, between OECO and ignition of the retro rockets;whereas more normal damping is indicated in the yaw plane.

An examination of the flight data showed that during the period

• between OECO and retro rocket ignition, the engine deflections in

pitch lagged the vehicle angular rate by about 200 degrees. This iswhat would have been expected from the control system.

In order to examine the expected behavior during and after thrust

decay, a study was made of the roots of the system with decreasing

thrust force. The study included the following degrees of freedom:

a. rigid body rotation

b. rigid body translationc. first few vehicle bending modes

d. first engine mode (all engines in phase)e. control equation for engine (including actuator transfer

function).

The results of this root locus study for both the pitch and yaw

planes, based on certain assumptions, are shown in Figure 7-4. Thevariations of the first bending mode coupled roots, for pitch and yaw,

with decreasing thrust are shown. The circle represents the locus of

the pitch plane root at the zero thrust level, for phase lags introducedin addition to what was assumed in the basic information.

For the theoretical analysis, the first natural bending mode

frequency of 2._4 cps was assumed. Two significant differences wereassumed for the theoretical analysis. First, a difference in the

mounting constraint 5etween the pitch and yaw directions of the instru-ment canister containing the stabilized platform was considered, From

this effect, the gain of the yaw feedback signal at the first bending

_ode frequency was 0.5 to 0.6 of the gain in pitch. This was determinedfrom the full scale dynamic tests of SA-DI, and was also verified by

the rate gyro flight data in the canister of SA-3. Another factor

$ considered was a difference between the pitch and yaw directions forthe structural damping. This was also indicated from the dynamic tests,

as given in MI_P-P&VE-S-62-3, Experimental Vibration on a Full Scale

Saturn Space Vehicle, where the damping factor in yaw was twice that in

. pitch. These tests indicated a structural damping, for the emptycondition, of 2.5 percent of critical damping for yaw, compared to 1.2

L percent for the pitch plane.

Whether or not the above assumptions with respect to the structural

_:_7!' damping can be considered valid is difficult to determine. However,

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9O

i.

(tad/s) o

(Imaginary Part)

18.0

Pitch Plane

Plane _T 240 ° 17.8

Yaw _0T 300°

0.5T17.6

0.5T

o0

17.4

12( Actual Pitchroot

[_ D =60 °

Actual Yaw17.2

Root

FIGERE 7-4 ROOT LOCUS PLOT OF COUPLED FIRST BENDINGMODE AT OUTBOARD ENGINE CUTOFF AS A

FUNCTION OF VARIABLE THRUST LEVEL

MPR-SAT-63-1

_r

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i='¸.._

there are some indications, from the SA-3 flight data, that the

structural damping in yaw may be greater than expected. There arealso some nonlinear effects, which are a function of amplitude, that

# have not been considered because of the difficulty in incorporating

them. One such effect is the nonlinearity of the servo system, which

gives an increased phase lag at small amplitudes.

The actual roots of the coupled first bending mode, as deduced. from the telemetered information, are shQwn for comparison with the

theoretical results in Figure 7-4. The uncertainty in the actual

frequencies is quite largewith respect to the scale shown. The

apparent variation in the damping in pitch is shown by the spread in-

dicated in the figure.

The basic reason for the trend towards a decrease in stability,

during-the thrust decay period• can be explained as follows. The

control system is designed to phase-stabilize the first bending modewith full thrust. The force felt by the gimbal point• for a given

bending mode, can be expressed as:

where;

T = thrust force

me = engine mass

ie : = distance of engine c.g. from gimbal point

Ie = engine m°nmnt of inertia about gimbal point

Y(XT) = bending mode shape at gimbal point

Y' (XT) = bending mode slope at gimbal point

c_B = bending mode natm0cal frequency

./

When;

:i} T = _B 2 ie + Ie Y(XT)I

_i_ the force changes sign and reverses the stability trends of the system.For the Saturn vehicle, this occurs at about 40 percent of full thrust

of the outboard engines. A further decrease moves the coupled root

closer to the unstable region.-_:#

c-2:.;i_

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92

As can be noted in the above equations, the stability is a function

of, among other things, the bending mode shape. Figure 7-5 shows the

theoretical coupled first bending mode shape after cutoff for zero

thrust, as determined from a molti-beam theoretical analysis. Some

points determined from the SA-3 accelerometer measurements are shown

for comparison. The results are basically in good agreement, which

helps to support one of the inputs used in the theoretical analysis.

There may be other possibilities, other than a difference in

structural damping, that might explain the different behavior between

pitch and yaw bending observed on SA-3. It is not intended that this

present analysis proves that a difference in structural damping actually

exists. More direct proof should be obtained before this hypothesis

is accepted.%

7.3 CONTROL ACCELERC_IETERS

The calculated pitch and yaw normal accelerations, for the control

accelerometers, are compared with the telemetered values in Figure 7-6.The control accelerometers were located at station 879 on the web of

the spider beam s 1.13 m from the longitudinal axis of the booster. The

pitch accelerometer was located in line with Fin III, while the yawaccelerometer was in llne with Fin IV.

The telemetered accelerations had a considerable amount of higher

frequency (approximately I0 to 15 cps) oscillations, but these were

filtered out for the purpose of this comparison. All oscillationsabove approximately 2 ¢ps were removed by a numerical Fourier filtering

technique. The calculated accelerations were computed from telemetered

angles-of-attack and engine positions, and were corrected to the

accelerometer location by means of the telemetered rotational motionof the vehicle.

The agreement between the two results is good with the exception

_of a sllght bias shift, that seems to appear in both functions at

approximately 110 seconds. The telemetered values are slightly morepositive, in both cases, until cutoff of the outboard engines. The

calculated results may be in some error, due to small erroneous biases

in some of the telemetered functions. However, this may also be an

indication of some small thrust vector misalignments (Z_ :0.3 deg).

7.4 ANGLE-OF-ATTACK METERS

A Q-ball angle-of-attack indicator was flown as a passenger on

SA-3. ,Dynamic pressure, angle-of-attack in pitch, and angle-of-attackin yaw were determined from differential pressure measurements made on

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93

,#

Vehicle Station6

2000 t E66-30

1800 I16001400

E64-20

1200

E62-201000

800 i FIO-II

6OO

400

I

200 E251-9

0._ ! ! I I I : : : : :

-I 0 i

Q From flight measurements (f=2.7 cps)o./

Multi-Beam Theoretical Mode Shape(f=2.77 cps)

-t

FZGDRE 7-5 COMPARISON OF MULTI-BEAMCOUPLED BENDINGMODE SHAPE FOR ZERO THRUST WITH FLIGHT

DATA (150 - 154 SECONDS)

MPR-SAT-63-1

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0'_

i

_-

_'._

o

!

ltPll-,_'£-63-

I

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_ 95

the spherical Segment of the nose. The angle-of-attack differential

pressure measuring ports were located on opposite sides of the surfacein the pitch and yaw planes, 45 deg from the longitudinal axis of thevehicle. Differential pressure ports, for dynamic pressure measurements,

were located midway between the Fin I and Fin II planes, 39 deg and

51 deg measured as above. The pressures from the pitch plane ports" were led to a differential pressure transducer in the model F-13 Q-ball

electronics package. The same thing was done in the yaw plane. Inthis manner, differential pressures are produced proportionally to

(i) the product Of the angle-of-attack and the dynamic pressure and (2)the dynamic pressure. The differential pressures were telemetered andalso fed into the computing portion of the F-13 circuitry, from which

signals were produced corresponding to the angle-of-attack in pitchand yaw, and also to the dynamic pressure.. By using the differentialpressures, the angle-of-attack and dynamic pressure may be comp,xted by the

following equations.

The angle-of-attack: _(AP) = 6 AP____t(1)Z_Pq

The dynamic pressure: q(Z_P) = __Z_Pq (2)Cp

where;

_(_p) = Angle-of-attack computed from the differential pressuresmeasured with the Q-ball.

_P_ = Differential pressure proportional to the product ofangle-of-attack and dynamic pressure. _easurementsD64"30 and D65-30_)

pq = Differential pressure proportional to the dynamicpressure. (Measurement D66-30.)

q(AP) = Dynamic pressure computed from the telemetered differ-•" ential pressure. (Measurement D66-30.)

- = Wind tunnel determined pressure coefficient.

A comparison of the angles-of-attack measured from the locals, the

Q-ball, and those calculated from rawinsonde and rocketsonde winds is

_ presented in Volume I (Figures 7-3 and 7-6). The agreement between the

!_ calculated angle-of-attack from the Q-ball differential pressures, and_' the direct measurement of angle-of-attack from the F-13 Q-ball electronics

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96

package is quite good. A bias of approximately 0.25 deg, between the

direct Q-ball measurement (F23-30) and the calculated values from the

differential pressures (D64-30 and D66-30), starts at about 65 secand continues for the remainder of the time. A nonlinear time shift

of the telemetered data could possibly explain this deviation. The

agreement in the yaw plane is good to approximately 105 sec, where thedirect measurement (F24-30) starts to deviate from all other determln-

ation_ of angle-of-attack. This deviation can most likely be attributed •

"to the operation of the servo.

The angles-of-attack from the Q-ball and the free-stream angles-of-attack calculated from the locals were not in good agreement prior

'to Mach I (68 seconds). This deviation is suspected to be due to an

error in the dynamic pressure _P measurement of the Q-ball. The factor,

, representing this error_ was computed by taking the ratio of the directmeasurement of angle-of-attack from the Q-ball, and dividing by the

_ree-stream angle-of-attack from the locals. This ratio is shown in

Figure 7-7 as a dashed line for the yaw plane and a solid line for the

pitch plane. To further substantiate this, equation (I) above wasused, by substituting the dynamic pressure from the trajectory_ along

with the wind tunnel determined pressure coefficient for Apq, andcomputing a free-stream angle-of-attack in the pitch plane. The ratio

of this angle-of-attack and the angle-of-attack computed from the

differential pressure, using equation (1)_ was determined and is shown

as the solid points in Figure 7-7. The agreement was very good, and

verified that this error does exist for the Q-ball angle-of-attackindicator in the subsonic region, varying from about 2.0 at Mach 0.2

to 1.0 shortly after Mach 1.0.

.5 PROPELLANT SLOSHING

Sloshing was measured by means of differential pressure measurements

in three of the nine propellant tanks. Slosh measurements were made inthe center LOX tank, LOX tank 04, and fuel tank F2. Locations of the

tanks and the polarity of the measurements are shown below.

+ Pitch

II _V _ + Yaw

I

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_._

97!

i:-,

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98

The ring frame and baffle locations, as well as the locations of

some of the measurements, are shown in Figure 7-8.

The telemetered sloshing differential pressure measurements mustbe multII_lied by a conversion factor, to obtain the sloshing amplitude

in terms of height. At the present time, this conversion facto.r is

based on a theoretinal correlation. Some recent ground tests, to a

determine the adequacy of this approach, indicate that this approach"may not be very accurate. However, the analysis of these test results

has not been completed as yet.

= The converted propellant sloshing amplitudes, for the fuel tank F2

_d the LGX tank 0¢, are shown in Figures 7-9 and 7-10 respectively,

for the later portion of the powered flight. The small sloshing

,. amplitudes indicate the effectiveness of the additional baffles in the

lower portion of the propellant tanks, added after the flight of SA-I.The sloshing in the center tank (see Volume I) was slightly more

siguificant.

Figure 7-11 shows a comparison, in the form of polar plots, of the

_ propellant motion in L(_ tank 04 for SA-2 and SA-3. These plots areboth comparable with respect to the passing of the propellant surface

:_ below the last baffle. Both vehicles showed motion which took place

"__ more predominantly in the pitch plane direction, SA-2 being of a more_c planar motion than SA-3. On SA-3, it does not appear that vortexlng

!'_ occurred as the propellant reached the bottom of the tank.

This flight has again demonstrated that the baffling arrangement

j being used is sufficient to keep the sloshing small and therefore, ithas no significant effect on the vehicle's performance.

L _s

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99

784.99

775.75 --763.78 --

. >>.... f n__ v 4f

> Center Tank Cross Section _ I, I_,Showing Baffles _ v Y

{_. _ 0.737= 7 A _.

,q'_.",vvx_. T > 523.99-- =

514.75 -- " ....

_> _J_o_,+r_:_n_+;:;_::_oof "

/-_" 0.737m

_ >> r

" _ --369.75 -- _ q A _',

> '311.75 -- " .... 299.78-- / 291.99 _ _" "/_"_

287.25 --'_ -- _ 285.28-- 276.25 -- _ O

270.13 -- --_ _ j 264.25 -- ----T246- 235 _ _235

o-- Ap Slosh Probe

T Level C. O.

..... Note: Numbers Indicate'e Station Locations

FIGURE 7-8 BAFFLE CONFIGURATIONS

_ MPR- SAT-63- I

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MPR-SAT-63-1

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101

MPR-

SAT-63-I

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102Slosh Amp. Pitch Slosh Amp, Pitch

(_) (_)

0.5

-o.5 II .0.5 (cm)

I1o136 - 138 sec /

106 - 108 sec

Last Baffle SA-2 106 secCrossed SA-3 136 sec

Slosh Amp. Pitch

' (c_)

| Slosh Amp. PlZch

| 0.5-(cm)

__ / l_B ._.__Slosh Amp. Yaw losh Amp. Yaw

138 - 140 sec _10_8__1.0 5

Q

108 - I10 sec

1,778m (70") _ Tank 1.778m (70") LOX TankSA-3 SA-2

0.1 See Time Interval

_G_tE 7-11 SPATIAL IFLOTS OF SL{_RING MOTION

MPR- SAT- 63 -l

,;;__:_4_;a_' _" . -,_-_= .v_ . _;_:

_. .

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_!'_ I03

• .. 8.o (c) CUn)ANCE

8.I INTRODUCTION

f

,Two guidance systems were carried on the Saturn SA-3 vehicle as

passenger equipment. The flight-proven ST-90 platform and associatedhardware furnished a reference for the control system. Data telemetered

from the BT-90 system were also used as reference data for evaluation

" of the functional operation of the ST-124P system.

8.2_ DESCRIPTION OF THE GUIDANCE EQUIPMENT

8.2.1 ST-90 SY_

The ST-90 guidance hardware included three pendulus integrating

gyro aecelerometers (AMAB-3) mounted on the ST-90 stabilized platform.These accelerc,,_eters were mounted to sense forces along a set of inertial

axes, oriented with respect to the stable platform X, Y, and Z axes.The slant range axis was directed downrange and elevated 41 deg up from

the horizontal plane at launch; the slant altitude axis was directed up

and 41 deg counter-clockwlse from the local plumbline at launch, when

viewed from the positive cross range direction; the cross range axis

was parallel to the local horizontal plane at launch and normal to therange-altltude plane, completing a right-handed cartesian coordinate

system. The platform axes were maintained in orientation by three AB-7

air bearing gyros. No second integrators were carried and the velocity

sIEmals were used for measuring purposes only.

Velocity Encoders mounted on the individual accelerometers are

driven by the precession of the accelerometer measuring head. Each en-

coder generates two variable frequency output signals. The zero cross-

ings of each signal indicate an incremental change in velocity of 0. i m_s.

The polarity of the velocity increment is determined by the phase rela-tion of the two signals.

The Guidance Signal Processor accepts the two sine wave signals

from the enco_er, determlnes the phase of the signals and zero cross

points, and then sends a polarized, 350 _s pulse to the telemetry sys-tem. With each 64th incremental pulse, the Signal Processor shifts the

_ bias level of its respective telemeter channel. The bias shift is nor-

mally'iused as a coarse velocity count of 6.4 m/s for data reduction

purposes _. . ..

, 8.2.2 ST-124P SY_

The ST-124P guidance system, flown for the first time on Saturn

SA-3, was a prototype or engineering test model of the system to be

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104

flown in the Saturn Block II vehlcles. The ST-124P is a four gimbal system,utilizln E twO p_du_s integrating accelerometers (AMAB-3) mounted on

_i the stable element. Platform orientation is maintained by three AB-5

air bearing gyros.

The accelerometers were mounted to sense the forces acting alon E

inertial axes oriented with respect to the stable platform Y and Z axes.

The altitude axis was directed up along the local plumbline at launch;

the cross range axis was parallel to the local horizontal plane at

launch and normal to the platform X axis.

The Guidance Signal Processor Repeater and two Velocity Encoders_

used with the ST-124P, were similar to those used with the ST-90 system.

8.3 GUIDANCE INTELLIGENCE ERRORS

8.3 _1 GENERAL

Guidance intelligence errors are defined as deviations in the

guidance measurements resulting from platform and accelerometer errors.

_ntelllgence errors are obtained by comparing the telemetered outputs

of the guidance system with corresponding values computed from trajec-

tory data. The earth-fixed trajectory, established from external track-

ing data, is mathematically transformed into inertlal_ space-flxed guid-

ance indications. Hardware alignments established at liftoff are as-

Sumed to be ideal for the data.transformation. Telemetered and calcu-

lated guidance values are compared to establish their agreement.

The guidance intelligence errors _ as presented in Volume I, include

small errors in tracking and data reduction as well as guidance hard-

ware errors. The errors shown for the ST-90 system are well within the

data noise level and/or one sigma hardwaTe errors. Errors observed in

the two guidance measurements from the ST-124P system are discussed be-

:_ : IOW.

_:_- 8.3.2 ST-124P L_EELLIGENCE ERRORS

Velocity differences_ shown in Volume I for the ST-124P system,

present no particular problem. This system was a prototype model flown

@s an engineering test to observe its functional operation and for

familiarization with the resolver chain and 5 kc/s servo systems in an

operational enviromnent. Accuracy was only secondary and a considerable

_i/ savings in both cost a_d time wa s accomplished by using equipment thatwas !ess accurate, yet fulfilled the prime objectives.

The altitude Intelligence errors resulted from some combination

of errors in scale factor_ data reduction, and difference in allgx_ents

T

L,

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:_ . , . I05

..i. ..---_'_."_:.... _ .

of the ST-124P platform, with respect to the ST-90 system which wasactive in the control loop.

Cross range velocity errors for the ST-124P system resulted from

a difference in alignments of the ST=I24P platform and data reductionerrors. The ST-124P platform was aligned within approximately 0.27 deg

of the ST-90, or within approximately 0.I deg of the vehicle axes.

This difference in azimuth contributes the major portion of the cross

_ range velocity differences. However, errors in data reduction and otheralignment differences contribute to the total velocity deviations.

Malfunctions in the Guldance Signal Processor Repeater, used with

the ST-124P system, are discussed in Volume I. One malfunction, affect-

ing the cross range outputs, occurred before firing command. A second,affecting both guidance measurement outputs, occurred intermittently

between if3 and 120 seconds. The accuracy of the data reduction was

": affected to some extent by the malfunctions. Errors made in interpret-

ing the telemetered velocity data are reflected in the ST-124P velocity

differences presented in Volume I.

8.4 PLATlq)RM AND VEHICLE ALIGNMENTS

The vehicle axes, as defined by the ST-90 stabilized platform,

with respect to the actual SA-3 vehicle axes are shown in Figure 8-1.

The ST-124P platform was aligned in azimuth approximately the sane asthe vehicle.

Azimuth of the ST-90 platform was 100.011 deg E of N, while the

vehicle Fin I v Fin III position was 100.381 deg E of N. The view in

Figure 8-1 is from the rear_ with the solid lines and circles represent-

_ ing the vehicle axes and engin e positions respectively. Dashed lines

and circles represent the position of the vehicle axes and engines, if

aligned at launch with the ST-90 platform. Alignment differences for

the ST-90 system were hulled out before launch and the vehicle flewwith offset axis reference. These alignment differences contribute to

!

the actual cross range velocity buildup observed on the three Saturn

flights, and also contribute to the attitude differences between thetwo platforms flown on SA-3.

The operation of the ST-90 system was completely satisfactory.

The prime objectives of the ST-124F test were satisfactorily accom-

pllshed; the deviations in th@ measurements telemetered from this sys-tem result primarily from the less-than-optimum hardware used and the

.., difference in platform alignment.

?

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106

Fin III

Position

• Fin IV:ion

Fin II

Posit_ow

Fin IPosition

8-I ST°90 PLATFORM ALIGNMENT WITH RESPECT TO VEHICLE AXES

MPR- SAT -63 -I

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z_ 107

9.o (u)iv IcLzELZCZ ZCALS STm

9.1

* The power supply for SA-3 ,=(Figure 9-I) consisted of two identical

28 volt zinc-silver.oxide batteries, designated DI0 and D20, locatedin instrument canister 14 (canister and unit locations are shown on

Figure 9-2). These hatterles supplied power to nine inflight distri-

Q butors_ a power distributor, control distributor, propulsion system

distributor, main distributor, and five measuring distributors. The

capacity of each battery is 2650 amp-mln, which is approximately three

times that required for the flight.

Power Distributor

The twe 28 volt batteries supply main power to the power distri-

. butor, located in canister 14, which is used to switch and distribute

ppwer as required for operating all inflight subsystems. Three buss

systems (DII, D21, and 400 cycle) are used as junction points to dis-tribute the power from the power distributor to the eight other distri-

butors.

Control Distributor

This distributor (Figure 9-3), which contains busses to receive28 volt power from the power distributor, distributes this power to

control the functions as required by the program device, flight se-

quencer, control computer, and the pressurization system. The 60 voltdc control voltage supply converts the three-phase, i15 volt, 400 cycle

ac power to 60 volts dc and feeds it to the control distributor for

distribution to the actuators. Three-phase, 115 volt, 400 cycle acpower is also distributed directly through the control distributor to

the stabilized platform, servo amplifiers, and guidance repeater. The

control distributor is located in canister 15.i

Propulsion System Distributor ..

The propulsio_ distributor (Figure 9-3) _ontains the relays and

circuitry which control the functions of all eight engines according

to a preset, progr_mned sequence. This distributor is located in unit9 of the vehicle.

_The propulsion distributor receiVeS_ through its busses, 28 volt

power from the power distributor and distributes this power to the cir-

• cults and relays which control the engine functions. Part of the relaysactuate fueland LOX prevalves for controlling the flow of propellant

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_' 109

I III

L

Unit 11

.. . |

I Canisters I

!

i-

ra _ _

" :'2 ::

" - ,Unit I0

. . } ":-

e .

2

!. ._ Unlt 9

: ... _R-_T-63-1i

_6qJl_ 9-2 UNIT _CATT_S

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11o

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._: III_:_

to the engines.: Some of the relays are used to activate the conaxvalve for engine'cutoff. The engine cutoff relays are activated when

slguals are received from the flight sequencer, or from sensors indlca-

tiug log liquid level and low thrust. There are also relays which

* Operate fuel and LOX fill-draln and replenishing valves.

Main Distributor

, The main distributor contains relays for control of the retro rocket

EBW firing units. Other relays control the horizon sensqr, the guidance

signal processor, the heaters for the gyros, and the air bearing for

the ST-124P passenger platform system. This distributor, located in

canister 12, also has relays to turn the measuring racks on and off.

Measurin_ Distributors

The Saturn SA-3 vehicle was equipped with five measuring distri-

butors. All five of these distributors are identical in configuration

and size, but differ electrically. The measuring distributors serve

to dlstribute measurement signals to the telemeter channels from the

engines, tail area, and the upper portion of the vehicle. The maln

distributor also functioned, for SA-3, as the measuring distributorfor canister 12. The location and function of these distributors are:

Measuring Distributor 9A3 - located in unit nine - controls

measurements which do not require signal conditioning on

engines I, 2, 5, 6, and a portion of the thrust frame area.

Measuring Distributor 9A4 - located in unit nine - controls

measurements which do not require signal conditioning on

.." engines 3, 4, 7, 8, and a portion of the thrust frame area.

MeasurementDistrlbutor 9A5 - located in unit nine - controls

measurements which require .signal conditioning on engines

i_ 2, 5, 6, and a portion of the thrust frame area.

Measurement Distributor 9A6 - located in unit nine - controls

measurements which require signal conditioning on engines

3, 4, 7, 8, and a portion of the thrust frame area.

Main Distributor 12Al - located in canister 12 - controls

measurements associated with the ST-124P passenger platform.

Measurement Distributor 13A1 • located in canister 13 -

controls measurements located in the upper portion of the

vehicle, except for the measurements in canister 12. It

also controls all telemeter and tracking equipment.

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:._ 112

The 28 volt dc power from the vehicle batteries is supplied

through the power distributor to busses in the measuring distributors.

This 28 volt supply is fed to the measuring power supplies, converted

to a 5 volt output, and is routed to the measuring voltage busses (Dglthrough D89). From these 5 volt busses, energy is supplied to the

various measuresnent pickups throughout the vehicle. Busses Dgl through

Dgg distribute 5 volt power through the vehicle measuring network to

the measurements in the eight engine compartment areas. The D89 buss

supplies 5 volt power to all remaining measurementsthroughout the,vehlcle.

9.2 POWEE CONSIRdPTION

The capacity of Battery D20 was 2650 amp-min. The loads on Bat-

tery D20 were continuous and a current of 165 amps was supplied from

T-35 sec until Project Highwater at 292 seconds. A total of ap_roxl-" mately 898 _np-min was used for the flight (Figure 9-4) or approximately

33.9_ of the total battery capacity.

The capacity of Battery DI0 was also 2650 amp°rain. The loads

varied, during flight, from 165 to 95 amps and the total consumption

cannot be accurately determined; however, the consumption was less than

for Battery D20.

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g,

',"4

o.,-,

113

(_hU

•.

.N°

r\

....iJ

,..:..,.-..._-.:.,

::-..:....'.::.

._

°^!

!';'"-".'='-"2'2

,(,"

,e.,,4

V

I,wO,u,n

_

uo

'p]fJ,

•..

.-:..._

_,_,

"To,

•o.o-.H

oj

<_

4.1

I._•

|.

e_

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114

I0.0 (U) STRUCTURES AND VIBRATIONS

i0.1 S_L_RY

The instantaneous longitudinal loads, bending moments, and shears

al_ng the pitch and yaw axes were determined from 8 truss compression

member strain gaugesj !6 truss tenslon member stralngauges, and 8

LOX tank stud strain gauges. The strain gauge data showed a very

smoot_ flight, as was evidenced by the relatively low bending moments,

and generally agreed very closely with trajectory values.

Instrumentation for detectlngvehlcle body bending consisted of10 bending accelerometers at five vehicle stations. All acceleremeters

appeared to respond properly and have polarity as reported beforeflight.

• The vibration data received from the SA-3 flight was transmitted

by two telemetry systems, FM/FM and single sldeband. Data in general

was smooth and within the expected range with respect t_ vibration

amplitudes. Transients and irregularities were noted in some of themeasurements.

10.2 BENDING M_4ENTS AND NORMAL LOAD FACTORS

10.2.1 INS_TION

Instrumentation for determining bending moment and normal load

factors consisted of eight truss compression member strain gauges

(E13-11 thru E20-11), sixteen truss tension member strain gauges (E229-

11 thru E2_-II), and eight LOX tank stud strain gauges (E21-01 thruE21-04 and E22-01 thru E22-04). _?nese gauges were located as shown

in Figure I0-I. Flight evaluation consisted of determining, for nu-

merous time slices, the instantsueous longitudinal loads s bending mo-ments, and shears about the pitch and yaw axes. The strain gauge dataindicated a very smooth flight, as was evidenced by the relatively low

! bending moments whichwere encountered.

The eight LOX stud straiD gauges were located at station 869 (see

Figure i0-I). Of the eight gauges., five were lost prior to ignition;:

therefore, no bending moments: about the pitch and yaw axes could be

calculated for this station. The three gauges which functioned pro-

perly served as a check on the vehicle longitudinal load. These three

gauge readings were found to closely agree with predicted values.

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_ 10.2.2 STRAI_ GAUGE H]_J_S_ Ag.TU$_2_$

Several days before the SA-3 flight, each strain gauge ws_ set to

a zero reading wltha total of 101,290 kg of load existing above sta-

• tion 979; howe_eE, telemetry data recorded 30 sec prior to engine _gni-

tion indicated that the gauges might have drifted. An average of eachtZ_ss strain gauge during this time interval indicated a total of

3026 kg compression load from the dummy stages, instead of zero. The

actual- strains used were obtained as followe:

(a) The average of I00 strain readings recorded prior to ignition

•ras computed for each strain gauge. This average constituted a "drift"value for eac h strain gauge.

(b) Thes e "drift" values were subtracted from their respectiv e

• strai n measurements recorded at any time point during flight to obtaindifferential strain values to use in the calculation of bending moments

and 10ngitudinal loads at station s 979 and 869. Hence, the zero read-

ings were essentially reset (,the 3026 kg load was subtracted) and anymoment present prior to ignition was neglected. (Note: Low wind veloc--

_ty Just before liftoff generates extremely small bending moments atstation 979.)

I#olarlty of the gauges on the 16 tenslon members of the trussas _elemetered was reversed. Verification of this was obtained several

week s after the evaluation was started.

I0_ 2,3 TIME POINTS EVALUATE D

]_ending moments and 10ngitudinal loads were calculated in 0_2 sec

_" intervals for the fQ!lowing t.ime Slices:

Seconds from Range Zero Significant Event

_' -4.O to II.0 Tgn.ltlon and liftoff_ ]_eg_nning of tilt progr_

60.0 to i15.0 _ach i

_: Maximum _Q_ _ _ntermediate time slice.

_: 139,0 to 155.0 Engine cutoff

_ _ Retro Rocket firing

_ _ddltional time points were consldered for the construction of the_ . longitudinal load vs time curve.

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._::. 117

i0.2.4 LONGITUD_ LOAD_

Multiplication of the actual telemetered strain by the calibration

factor results in the loads shown in Figure i0-3 of Volume I. The

solid line in this figure was obtained by using the differential strains

and addlng the 101,290 kg load which was lost when the ganges were setto zero. This latter curve is also shown in Figure 10-2 of Volmne _

and is comphred to the corresponding curve for the SA-2 flight. Al-

though both curves are seen to pass from their calibration range, it is

known that they go to zero as the thrust decays. The SA-3 curve is

also known to drop below zero load (go inCo tension) during retro rocket

flriRg. L

Figure 10-3 shows the longitudinal load at station 979 versus time

in the cutoff @egion. Of primary importance is the agreement betweenthe times of cutoff as given by trajectory data and that given by the

strain gauge data. The cutoff accelerations determined from the strain

:gauge data also agree with those determined using trajectory data.

The loads in the three functioning LOX stud gauges versus time in

the cutoff region are shown in Figure 10-4. These gauges were the only

source of data presenting the longitudinal loads during the outboardengine thrust decay and retro rocket firing periods. They are in close

agreement with expected values.

!0.2.S mArS

_ Maximum bending moment at station 979 occurred at 69.2 sec after

range zero (" aQ" max). High •bending moments were also experienced at

64.8, 67.0 and 81.6 seconds. _igure 10-5 presents the bending moments

.=:: versus time throughout the above interval and includes the time pointfor Math 1 (68.I seconds). These moment values vary to such a degree

as to make it difficult :to detect any natural bending frequencies. A

portion of the pitch moment shown in Figure 10-5 was previously pre-

sented with the corresponding c_ and _ measurements in Figure 10-2 of

_ _rolt_e _. GOod agreement _n frequency of oscillatlon was noted.

The decommutated oscillograph traces showed small oscillations in

the vehicle in the time interval of 80 thru 105 sec after range zero.

The bending moment values corresponding to these oscillations provedto be of relatively low magnitude and hence_ are not considered serious.

Maximum yaw moment at station 979 occurred at 103.5 sec after

range zero. This moment was somewhat less than the maximum pitch mo-• ment and was found not to be crltlcal.

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I_R-SAT-63-1

iLt

,

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r+ ,

120

Load (_000 kg)

140

120

End of 2ndThrust.

100

Retro RocketFiring:

8O

L6O

FIPR-SAT- 53 J_ _

!:

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"_

MPR-SAT-63-1

.i

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122

10.2.6 S__ARL0_S

Shear loads perpendicular to Fin I-III and Fin II-IV were inves-tigated throughout the flight and found to be erratic but of very lowmagnitude. Since the oscillations were irregular, no bending frequen-cies could be determined. However_ the shears were found to lle in a

re!atively narrow band of T 5000 kg. Because no significantly impor-tant information could be shown_ no graphical results are presented

for shear. .

I0._ SEN_n_ OSCILLATIONS

Instrumentation to detect vehicle bending frequencies and deflec-

tions consisted of four pitch and four yaw accelerometers located at

stations 189 (thrust frame), 1050 (2nd stage), 1310 (2nd stage), and

1900 (nose cone). _n addition to these four positions on the vehicle

"" proper, accelerometers were locate d on fuel tank F1 at vehicle station

814, in both pitch and yaw directions (Figure 10-6). The measuring

range of these low frequency accelerometers (0 to 25 cps ) was T 0.5 g's.All accelerometers appear to respond properly and have polarity as re-

ported before flight.

' The frequencies presented here vary sllghtly in accuracybut allare considered to he wlthln T 0.15 cps.

The oscillographs showed s gredominaut frequency content of ap-

proximately 12 to 20 cps throughout flight, with increased amplitudes

at llftoff and the two engine cutoffs.. The natural frequencies of theaccelerometers vary from approximately 13 to 18 cps.

;_: Analysis of the data by a _Igltal computer program revealed the

_ presence of frequencies in the control frequency range of 0.25 to 0.50

cps_ and also in the propellant sloshing range of 0.6 to 1.5 cps. TheJ frequency trend of the vehicle first mode follows the first mode of

the SA-D tests for similar fill conditions (see ¥olume I, Figure 10-5)

and this trend _s s_hstantlated by the mode shapes shown in Vol,--e I,

Figures 10-6_ 10,7 and 10-8. Addltlonal mode shapes for time slices

at !0 to 13 sec, and 32 to 36 sec are presented here in Figures 10-7and 10-8, The _econdmode Shapes are not shown due to their low ampll-

tude-of response. The'response of the vehicle structural modes was •16wet on this flight than on SA- 2. The only outstanding difference

Inthls fllght was the forced response after OECO which was caused by

_ the inertia of the e.nglne gimballing after cutoff.

o

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, Sta. 1050

E62-20 Pitch

E63-20 Yaw

• _t a. 814

6o-ioPitchI_ __ E61-10 Yaw

! ---_ _ Fuel Tank #i

|

I

I Sta. 189E251-9 Pitch

I E252-9 YawThrust Frame

FIGURE 10-6 ]IENDING MODE ACCELEROMEYgR LOCATIONS

"MPR-SAT- 63- I._ i•

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124

Vehicle Station

2000'

E67-30

180C T_e ($ec) Freq (cps)

tt 10-13 2.0 !

1600 I

: SA-3 St_le _p

A E'S In_00 E67-30 O.0060 O.0_6 _:3

E65-20 0 0 0E65-20 E63-20 0.0017 0.0043 0.1

E61-I0 0.0025 0.0062 0.1

1200 E252-9 0.0026 0.0063 0.1

/E63-20

I_0

• 800 E61-IO

I

600 I

\ ,|

4O0

200 E252-9 _ _

J | | i •"_.!_ ...._.,..:' .l...,l._,._'.__._-.....

-1,0-.8-,.6,.4-.2 0 ._ ,4 ,6.8 1.0

ge_.ariv_ _$itpd_

j FIGURE I0-7 SA-3 B_21DIN_ I_DDE-_ MODE, YAW (10 to 13 sec)

MPR-SAT-63-1

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?

_: Vehicle Station 125

2000 T• . E66-30

_ I " " Time32_36(sec_ Freq.2.50(cps3

1800 1

•, , 1600 _ SA-3 Sln_le Amp.

t g_s Ip . mm

: // E66-30 0.0050 0.0079 0.20

E64-20 0.0012 0.0019 0.05

_ '_, 1400 E62-20 0.0018 0.0029 ,0.07: E251-9 0.0026 0.0041 0, i0

E64-20 ?

_:_ 12oo

E62=20,_.i 1000

\:' 800

_ _, 600i !

_!:} , 400

__ ' ; 200 ' E251-9 _'_

•: " I I I : : : : : ! l I_::- -1.0-.8-.6-.4-.2 0 .2 .4 .6 .8 1.0

_'_,_ ' : Eelattve Amplitude

:i lr_b"0RE 10-8 SA-3 BENDING MODE-FIRST MODE, PITCH -(32 TO 36 SEC)_i_'_;_, ,, HPR-SAT-63-1

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126

10.4 VIBRATIONS

10.4.1 INTRODUCTION

The SA-3 fllght vehicle was instrumented with 40 vihratlonmeas-

urements, Their description, axis of sensitivity , and frequency rangeare listed in Table 10-I. Measurement locations are shown in Figures

10-9 through 10-11. The accelerometers were divided into three major

monitoring groups : structural measurements, engine compartment measure-

menEs s and component measurements.

RMS acceleration time histories were obtained for all measurements.

' Data envelopes are presented for the major monltoringgroups and for

individual components whenever possible.

10.4.2 GENERAL DISCUSSION

The vibration data received from the SA-3 flight were transmitted

by t_o telemetry systems, FM/FM and single sldeband. Data in general

were smooth and within the expected range with respect to vibration

amplitudes. Transients and irregularities were noted in some of the

measurements. A discussion on the investigation of these transientsis included in this section.

The vibration data was divided into three major categories accord-

ing to the location of measurements; i.e., structural, engine compart-

ment, or component measurements. Measurement E85-II, located at thebase of canister 14 on the spider beam, was an exception. It was ana-

lyzed as a component measurement instead of a structural measurement

because it recorded the v_bration input to the canister.

The five structural measurements represent both the upper and

lo%_rstructure of the booster. Three measurements were located onthe lower strucEure_ two being on the gimbal point support and one on

the heat shlelS. The trend of these data is displayed in the upper

part of Figure 10-12. The two upper structure measurements were on

the spider beam. The acceleration time history envelope of these

measurements is shown in the center portion of Figure I0-12.

Twelve engine vibration measurements weremonltored during the

fllght of the SA-3 vehicle. The results of these measurements are pre-

sented in Volume _, Figure 10-9; The data from measurement E45-8 was

plot_ed separately because of its comParatlvely high levels as indi-

cared on the figure.

_ A total of 22 vlbratlonmeasurements monitoredcomponent vibrationduring the flight of the SA-3 vehicle. An aceeleratlon time history

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127

TABLE 10-I!

SA-3 FLIGHT VIBRATION MEAB_S

Meas. Direction of Frequeney

No_____. Description Sensitivity Response (.cps)

LI0-11 Sound Intensity 3 kcE4-15 Vibr. ST-90 Y Axis 790

Eli-4 Vibr. Thr. Chain. Dome Lateral 3 kc

_ E12-2 Vibr. Turbine Gear Box 3 kc

E12-3 Vlbr. Turbine Gear Box 3 kc

E12-4 Vibr. TurSine Gear Box 3 kc

E12-6 Vibr. Turbine Gear Box 3 kc

E12-7 Vibr. Turbine Gear Box 3 kc

E12-8 Vibr. Turbine Gear Eox 3 kc

E33-1 _ Vibr. Thr. Chain. Dome Long't 3 kc

• E33-3 Vibr. Thr. Chain. Dome Long't 3 kc

E33-5 ._ Vibr. Thr. Chin,. Dome Long't 3 kcE34-I Vibr. Pitch Actuator Pitch 3 kc

E34-2 Vibr. Pitch Actuator Pitch 3 kc

E34-3 Vlhr. Pitch Actuator Pitch 3 kc

E34-4 Vibr. Pitch Actuator Pitch 3 kc

E37-I Vibr. Yaw Actuator Yaw 3 kcE37-2 _lhr. Yaw Actuator Yaw 3 kc

E37-3 Vibr. Yaw Actuator Yaw 3 kc

E37-4 Vibr. Yaw Actuator Yaw 3 kc

E40-1 Vibr. Gimbal Pnt. Support Long't 3 kc

E40-7 Vibr. Gimbal Pnt. Support Long't 3 kcE42-2 Vibr. Fuel Cracking Valve Long ' t 3 kcF/+3-4 Vibr. Hydraulic Pkg. _ Lateral 3 kcE45-8 ¥ibr. Fuel Suction Line Long't 3 kc

_ E46-9 Vibr. Prop. unit Distr_ 9AI Long't 3 kcEA7-1 Vihr. Radiation Shield Long't 3 kc

E48-14 Vibr. I_str. Panel Lateral 3 kcEBS-II Vlbr. Lower_Suppor_ L_'t 3 kcE86-14 Vibr. Instr. Panel Pitch 3 kc

E90-12 Vibr. Roll Gimbal ST-124P X-Axis 3 kc

E91-12 Vibr. Roll Gimbal ST-124P Y-Axls 330

E92-12 Vihr. Roll Gimbal ST-124P Z-Axis 3 kc

E93-12 Vibr. ST-124P Mtg. Frame Long't 600

- E94-!2 Vlbr. ST-124P Mtg. Frame Pitch 1050

E95-12 _ibr. ST-124P Mtg. Frame Yaw 790

E96-11 Vibr. Retro Rocket #1 _ Long't 3 kcE97-11 Vibr. Retro Rocket #1 Pitch 3 kc

E98-II Vibr. Retro Rocket #i Yaw 3 kcE99-II Vibr. Spider Beam Long't 3 kcEl00-11 Vibr. Spider Beam Pitch 3 kc

XL24-9 Sound Intensity, Sta. 167-_..... XL25-9 Sound Intensity, Sta. 167

XL26-9 Sound Intensity, Sta. 889_L27-13 Sound Intensity, Sta. 889

/

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12_

VIEW A

[=3.3-..A

ImZ_ ,& -4/. 4ILh]_.llIL _OJ 1_2 1_41 .A

F.Z3t-41.A

R41-11.&

IE_. I!, o E24441 •

IIW,_.I2.o

E48-14, LAT,O|m6-Ji4op. 0

t4*n_,o

: _MiISTIO;/ 14 :lt&i_tl_q*r! _II,L,O

u=-,,., VIEW A

.-E4_- I,L.O £_-_t. #*0_4,n,oI[m*4,11,oEII_-41,11.oIEI_-?.11,0EI_,.I,#, 0

:_'40-=* t40-1 ,L,O1 E40_7,L,O•E3?.-P_T.O _E4_-2_L .0

,=.,.,.oo..1DETA'LA' A/ [41.. J-_ E_t-_ ,P.o "

1£34.-4.O, 0Lr'_?.| tY, O

o ° VIII_ATI_u - I[l_kOll_A- STR/_

p- I_'CH

T- T_INT1M._- 1 TO FtOW

FIGURE I0-9 SATI/IOISA-3 BOOSTER _,T._.,

MPR-S_T-63-1

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].29

•" M_R-SAT-63-_

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13.0

VIEW A

[I;t...4.l10 OI_-&,U, 0I[1-?°11. O

• lille.411.11,0

,_. 1140-1,L,O[40-7.L *0

I[ll?,_,Y,O 4 -2 I,, 0EII?-4_Y,O I[ ! , ,

a3.s,L,o DETAIL AE_4-2 ,P*o •

h 1[:II4-4.P,oP_- EST-i I_,0

[;r/4..YDoA. AG'Ous'f';¢o - VISRAT_o - 8[NOmGA- SCrAAmL" (._LI_ pITCN **/I.o _J2A¢T- TANGENTIAl..L- JL"ro _"|1.1[ TORffy. yAWLAT* LAY

I_GIJICEI0_]_I SATURN SA-3"BOOSTZll

I_R-SAT-63_i

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G_ 131

Eng J.ne CompartmentStruc£ural Measurement: Re

-_ , FAO-I20 E40-7

E47-1f

to -:- II

. , ,!2t(0

-20 20 40 60 - 80 100 120 140 160Range Time (sec)

I_. 8p£der Beam i

_tructural Measurements _ _;::'.._.,_

_ ,_99-11 _ _ _..

o X__.-20 0 20 40 60 .80 100 120 140 160

_S Range Time (sec)

.o., ,Retro Rocket Measurements ._ _._E96-11 _._L_:__

8 , E98-1I

_-_-_t,.,,-__,"_,__,•'_ -,.__

_! .,_e:.-. _ _,._.2

., .i!,_ I

0-20 20 40 60 80 100 120 140 160

Range Time (sec) ...

FIGURE 10-12 MAX]Ht_ AND _ ACCELERATION TIMES

e

MPR-SAT-63-1

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fenvelope for the canister area is shown in Volume I, Figure I0-9. Thelower part of Figure 10-12 exhibits the acceleration time history

_ envelope for the retro rocket measurements. Data envelopes for the

_ hydraulic actuators and the propulsion unit distributor are not in-

_ cl_ded because of an insufficient amount of data.

10.4.3 MAJOR DEVIATIONS OBSERVED IN FLIGHT VIBRATIONS DATA

1. Three engine measurements, E33-1_ E33-3, and E33-5_ transmitteddata only intermittently throughout flight.

2. The SA-3 flight data revealed a great number of data points

of questionable origin, which are termed transients. Most of these

transients are similar to those resulting from a severe or high mechan-

ical input to the vibration transducers. However, it is felt that dur-

ing this flight there were no mechanical inputs great enough to satu-

" rate the telemetry circuit temporarily, except at ignition, liftoff,Mach i, max q, cutoff s and retro rocket firing.

There were 3,869 transients observed in the vibration measurements

on links 7 and 8, and on _FM. Of the recorded transients_ 90_ can

be classified in the following four categories:

I. Transients caused by the two commutators.

2. Transients having periods between 6.I and 6.2 seconds.

3. Transients having periods between 7.0 and 12.0 seconds.

4. Transients having periods between 0.09 and 0.60 seconds.z

Transients in category 1 occurred on links 7 and 8, but not on

_ _M/I_M. Transients in categories 2, 3_ and 4 occurred on links 7 and 8,"_: and on I_M/I_M._.

_: ApProximately 57. of the recorded transients were in category I,

:_i The sources of these transients were separated into two groups:

_ (a) Those produced by the Master Pulse of the commutator, occur-

red, ring approximately every 13.86 seconds. .

i (b) Those produced by the commutator when it switched from record-

_ lug one channel to the next, occurring approximately every 3.45 seconds.

*-. The majority of the transients in category I resulted from source

¢,.: (b). Source (a) affected measurements E40-1, E40-2, E42-2, E43-4,

_ L10-11,E96-11, and E97-11.

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133

Approximately 8Z of the recorded transients were in category 2

and were of a cyclic nature, occurring every 6.13 _ 0.04 sec, or a mul-

tiple thereof. These transients have been correlated with the turning

on of the air heaters for the ST-124P. It appears that the resulting

electrical transients induced a disturbance in the electrical wiring

associated with the particular accelerometers affected.

The measurements seriously affected by the transients in category

2 are E96-II, E97-II, E98-II, LI0-11, E90-12, E92-12, E93-12, E94-12,

E95-12, E91-12, E99-II, and EIO0-11.

Approximately 3_of the recorded transients were in category 5 and

were also of a cycllcnature; however, there was a rather large devia-

tion from any particular assumed period. During and after powered

flight, up to 180 sec, the period of occurrence remained near 7 or 8

sec, or a multiple thereof. After 180 sec, the period increased stead-

ily to almost 12 sec at Project Highwater. The source of these tran-sients was active at least 8 minutes before liftoff.

The measurements most likely to be seriously affected by the tran-

sients in this category are E4-15, LlO-ll, E96-II, E97-11, and E98-II.

Approximately 74_ of the recorded transients were in category 4,

making this the must significant category. Similarly to category 3,

the source, or sources, adopt a near periodic pattern, the frequency

decreasing with respect to time. The average period of occurrence

increases steadily from 0. I0 sec at 100 sec range tim.e, to 0.19 sec

at 200 seconds. Beyond 200 sec, the period increases sharply to ap-:

proximately 0.60 sec at 240 sec range time.

As yet, the source of the transients in this category is unknown,

but characteristics have been determined. In categories 3 and 4 (un-

llke i and 2), the cause is not a "time_' function, but is somewhat

variable with time, perhaps contingent on conditions requiring or effect-

ing correction or adjustment; such as the operation of a thermostat,

or a condenser discharge or breakdown.

The measurements most seriously affected by the transients in cat-

egory4 are E96-11, E97-11, E98-11, E99-11, E100-11, E90-12, E92-12,

• LI0-11, and E91-12. Transients in category 4 are capable of affecting

other measurements slightly.

The remaining 107. of the recorded transients, which are not in

these four categories, are termed "residual transients". A series of

these transients appeared between -1.40 sec and +2.35 sec range time

in measurements E96-II, E97-11, E98-11, and E99-11. They were similar

k

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_'t

•" 134

.if!:

to the transients in category 4 in all respects, except that they lacked

the cyclic feature so predominant in category4. Because many of these

residuals appeared at periods of high vibration levels, such as ignl-

tion, llftoff, Math I, max q, cutoff, and retro rocket firing, they

could be a result of a mechanical input to the vibration transducer.

10.5 ANALYSIS OF GROUNDACOUSTICMFAS_

10.5.1 SUMMARY

Sound measurements made on the SA-3 vehicle were used to determine

the acoustic environment created during launch. These measurements

were made in a similar position to those of previous Saturn flights; in

the near-fleld, mid-field, and far-fleld; such that both specific envl-ronmental characteristics were known and general acoustic evaluations

could be made.

I0.5.2 NEAR-FIELD DATA

Four measurements were made on the vehlcle itself with the micro-

phone signals transmitted to the blockhouse through trailing wires,which were cut when the vehicle was approximately 33 m above the pad.

The results of the near-fleld acoustic measuring program are shown

below compared with the results of SA-2. For SA-3, the values _ere

recorded between ignition and approximately T+5 sec within 60 m of the

vehicle, giving an indication of the magnitude of the sound pressure

at critical points on launch complex. The on-pad measurement locations

are shown in Figure 10-13.

Near-Field Acoustic Measurements

Microphone Location Max. Overall Sound Pressure Leve'l (db)

: Vehicle Enviror_ment Meas. (db re: 0.0002 microbar_SA-2 SA-3

_b. Tower, Sta. 167 16"7 163

Umb. Tower, Sta. 860 45 162

Holddown Arm Nr. 4 (inside) - 151

Swing Arm Nr. I, control panel - 155

On Vehicle Meas.

Outside Shroud_ Sta. 167 156 149.0Inside Shroud, Sta. 167 135 157.5 "

Outside Can. Nr. 13, Sta. 889 141 149.5

Inside Can. Nr. 13, Star 889 130 132.0

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: - 135

Directionof Exhaust

130 °

115 °

Direction66 ° of Exhaust

.': 58° 50o45040 °

O°LVOMeasurement Location Degrees are in Angular CoordinatesA-T_ Division Measurement Location from Direction of Exhaust.I-L_O.and Teat Division Location

- A-Inslde NolddownArmNumber 4 Direction of Exhaust is 132 ° With

_-Above Large Uti1_ty Room (Outside),. Respect to True North.C-Umbilical Tower Station 167

I_abilical Tower Station 860 •

SwlngArmControl Panel Nu_aber I

'" FIGURE I0-13 LAUNCIIVEHICI_ OPERATIONS AND TEST DI'VISTON_: NEAR-FIEI_ MF,AS_ LOCATIONS ON PAD 34A FOR SA-3

M?R-SAT -63 -i

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136

GSE Environment Meas. Max. Overall Sound Pressure Level (db)

(db re: 0.0002 microhar)SA-2 SA-3

Small Utility Room (underground) 120

Large Utility Room (inside) 125

Large Utility Room (outside) 157Blockhouse 34 (inside) ii0 113

Blockhouse 34 (outside) 139 141

On-Pad Environmental Mess. Max. Overall Sound Pressure Level (db)

Radius (m) AC* (deg) SA-3

•15 66 161

15 80 157

"15 90 157

22.5 75 152

,: 22.5 90 15530 80 153

30 I00 - 154

32 45 154

45 40 154

45 50 150.5

45 58 15345 90 153

_ 45 130 156

60 66 15160 30 154

60 90 149

*AC - Angular Coordinates are measured in degrees from centerline of_ the direction of exhaust. Direction of exhaust is 132 deg with respect

to the true north.

10.5.3 MID-FIELD DATA-_

;_ The mld-field data represents measurements ranging from 0.090 _n":_: to 0.366 km from the launch site. The results obtained from these

_!_ measurements are compared with SA-I and SA-2 results below.

Mid-Field Acoustic Data

Microphone Location Max. Overall Sound Pressure Level (db)(db re:0.0002 microhar)

SA-1 SA-2 SA-3

0.046 fun,Az 182 °, A.C. 50° 15---_ ---f--- _-'i--

_ 0.061 ks, Az 162 °, A.C. 30° - - 154

_=_ 0.061 km, Az 198 ° , A.C. 66 ° ....

_: 0.061 kin; Az 222 ° , A.C. 90 ° - -1.49

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_'i'_:_ 137

Mid-Field Acoustic Data (Cont)

_Microphone Location- Max. Overall Sound Pressure Level (db)'_ : . ",: (db re: 0.0002 microbar)

B : 4 SA- I SA- 2 SA-3

0.091-_=, As i72('-,";(.C. 40 ° -- -0.091 km, Az 182°, A.C. 50° 140

0.091 kin,Az 198° , A.C. 66° 145 155d& _"

. 0.183 km, Az 142° , A.C. i00 137.5 - 135

0.183 kin,Az 152°, A.C. 20°

0.183 km, Az 162°, A.C. 30° 143 148" 150

0.183 kin, Az 172°, A.C. 40 ° - 139

0.183 kin, Az 182 °, A.C. 50° 141 -

0.183 kin,Az 198°, A.C. 66° - 146" 149

0.183 km, Az 222 °, A.C. 90° 142 - 142

" 0.183 kin,Az 232 °, A.C. I00° - - 143

0.183 kin, Az 242 °, A.C. 110° 145 -

0.183 kin,Az 262 °, A.C. 130° - - 143.5

0.366 kin,Az 142 °, A.C. I00 - 139" 134

0.366 kin,Az 162° , A.C. 30° 143 137" 139

0.366 km, Az 182° , A.C. 50° 138" 137" 136.5

, 0.366 km, Az 198° , A.C. 66° 135" 139" 142

-- Indicates that no launch maximum value was obtained from measure-ment record.

* Measurement made 2 m above grade level.

10.5.4 FAR-FIELD DATA

To determine the variation of sound levels, frequency, spectral

characteristics, and effects of meteorological conditions over the

acoustic ray path, ten data collection points were established. These

points were chosen to fall along three azimuths running through the

major population centers of Brevard County, as shown in Figure 10-14.

The maximum overall sound pressure levels measured_for all far-field

• monitoring points are shown compared to those recorded for SA-I andSA-2. Sound pressure levels were also determined at other points ofinterest. These levels are included in the following table. Figure

10-15 shows an overall sound pressure level for two far-field positions

with respect to range time.

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138

Far-Field Acoustic Data

Measurement Site Ground Max. Overall Sound Press. Level (db)

With Code Name Range (db re: 0.0002 microbar)

_eters) SA-I . SA-2 SA-3 "

North Cape (C) 1,524 122 126 124

Hangar D (Jade) 4_294 --- 112 116

Barge Dock (D) 4,511 122 122 117 •

.Mandy Facility 7,523 --- ll0 115

South Cape (G) 9,022 --- 121 i12

North Merritt Island (B) 10,302 102 109 112

Playallnda Beach (Sierra) 14,794 --- 103 104East Merrltt Island (E) 15,774 102 107 105

Winslow Beach (H) 16,551 105 105 90Cocoa Beach (1) 21,717 --- 102 109

South Merritt Island 22#037 93 103 ---

Titusville-Cocoa Airport 22,877 --- 93 108

(Tango)

Merritt Island Airport 23_579 --- 90 105

.(Metro)Cocoa (F) 24,262 86 100 Iii

Titusville (A) 26,441 94 I00 i00

Rockledge 28,000 84 ......

Eau Gallie (J) 43,434 ...... 86

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140

.!

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_ 141

ll.0 (u) ENVIRONMENTALTEMPERATURESAND PRESSURES

Ii. 1 SI_MAEY6

Base regio_ environment during the SA-3 flight was similar to thatencountered on the two previous flights. Evaluation of the heating

rates on SA,3again indicated that major differences existed betweenthe two methods of evaluation. Sunxnation of sources of possible uncon-

sidered losses is made in this chapter and it is indicated that

add£tlonal experimental testing in this area must be accomplished

prior to the SA-4 fllght.j."

Evaluation of interstage and S-IVD stage skin temperatures was

accomplished with an unexpected low temperature level existing on theleeward side of the interstage. This was possibly due to boundary layer

"_ buildup which would reduce the heat flux due to aerodynamic heating.' Measured and estimated temperatures on the S-IVD stage were within the

expected degree of agreement. This agreement deviated at about 85 secrange time, although final temperatures w_re within the expected range.

II. 2 TAIL SECTION

11.2.1 BASE ENVIRONMENT

Instrumentation used to measure the base region environment on SA-3

consisted of five absolute pressure taps, two radiation calorimeters,

four total calorimeters, and six gas temperature probes. Of the above

measurements, _ne pressure tap, one total calorimeter, and one gas temp-.,erature were mounted on the flame shield.. The locations of the above

measurements are shown in Figure Ii-i.L- "

This instrumentation differed from that on the two previous vehicles,in that the total calorimeter C77-5 was mounted flush with the heat

shield on SA-3 instead of on a stand-off mount, while C63-I was the

reverse (i.e., stand-off mounted on SA-3).

For each of the C-I vehicles, two radiation calorimeters have been

mounted on the heat shield (C79-2 and C64-4), For the SA-2 and SA-3

. flights, improved versions of the slug type calorimeter used on SA-Iwere flown (see Figure ii-2). The SA-I calorimeter had the smallest

view angle (114 deg total angle) and the slug temperature was greatly

influenced by the window nitrogen purge flow. The SA-2 version had a

larger sapphire window, which increased the view angle to approximately

• 130 deE, and the slug had improved isolation from the nitrogen purge

flow. Another modification was made to the calorimeter, decreasing the

influence of the nitrogen purge on the slug losses (better slug isolation

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U-1 HEAT SHIELd. __QI_J_61'_OR_FOR SATUR_ SA-3 ln_..IG'I_

MPR-SA_r63-1:

.!

!/.:

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I

FIGURE 11-2 SA-I, SA-2, AND SA-3 RADIATION CALORIMETERS

MPR- SAT - 63 - I

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144

was obtained) and, the ,view angle was increased to 150 degrees. This

calorimeter was used for measurement C79-2 on SA-3, and the same designas used on SA-2 was retained fur measurement C64-4.

Figure 11-3 indicates the change in the performance of the. radla-

tlon_ calorimeters as. the _lew angle was increased. The calorimeters:

were placed under an infrare_ heat source and their resulting heat flux

was compared-with the measured heat flux from a standard- slug with a

180 deg view angle. This" correction factor was plotted as a _wnc_iO_.

of the distance from the. radiant source. As shown in Figure 11-3:,.the

SA-I calorimeter had a-rather large correction factor which varied

widely with .distance from the source, The improved SA-3 calorimeter,

at IOw sensor temperatures, had a_correction factor near unity, and was

relatively unaffected by Its_ distance from the radiant heat source.

_i_ Taking a view area of unity for the SA-I calorimeter, the S&-2 c_!o_i--,, meter, due to its increased view angle, would cover an area• 1.94 times

larger. Similarly, the SA-3 view area would be 5.87 times greater than

SA-I. However_ this is not intended to imply that SA-1 or SA-2 radla-

= tlon results are in error by this magnitude. It does indicate that the

_ present design of the SA-3 radiation calorimeter will be responsive tothe major portion of the radiation present from the Jet exhaust.

i

The problem of the slug conduction losses (reradiat.lon ca__be

evaluated with reasonable valldity) is still a major one. Slug losses

will tend to cause a negative slope in the temperature - time curve

prior •to engine cutoff. A comparison of the negative slopea of thethree calorimeter types indicates that the SA-3 type calorlmeterconduction loss has been reduced.

:i

The total calorimeter shown in Figure 11-4 has been used on the

first three Saturn flights without modification or improvement. _f

the calorimeter slug is not well isolated from the surrounding basei

structure, the conduction losses could be quite high. If the heat

_ barrier groove has not been effective in isolating the slug, a sizeable

",_- conduction loss through the twelve mounting bolts into the metal

!.__: support structure of the heat shield would result_ This calorimeter

_,_i is being evaluated, and modified if necessary, for flights in the_$%_ near future and will be replaced as soon as possible.C

The calorimeter mounted on the flame shleld was also a sluE type_

:: (see Figure I_-5) _. The larger copper sluE (7.6 cm diameter x 1.5 cm)

:_ was mounted in a transits housing and was _solated from direct cO_t;_¢t_ with the flame shield structure. This calorimeter has bee_ uged_ QD_:al_

three Saturn flights, and has g_e_-rather _nslstent results, _e_though subjected to significant reradlat_on l_ssel on the orde_ _E a

/. to' 1"7kcal/m2-sec. These losses_ were evaluated from the infllgh_

_, .

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:IqPR

-SA.T

=63-

I

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MPR-SAT-63-i

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148

cooloff rate after engine burnout. Results indicate that percentage-wise, the losses on this calorimeter were less than on the heat shield

calorimeters. Calibration of this instrument, mounted in a simulated

flame shield panel_ would greatly assist in the closer evaluation ofthe losses.

On SA-2, three of the gas temperature probes (CI0-2, CI0-4 and

C10-7) had protective shields which were not present on the SA-3 vehicle

(see Figure 11-6). Although the total temperature varied by i00 to 200

deg between SA-2 and SA-3, it can be considered that good agreement

between the gas temperatures was obtained (see Figure 11-4, Volm,e I).

The thermocouples on the forward side (cold side) of the heat

shield are shown in Figure 11-7. It should be noted that measurement C69-5,

mounted on the Block II heat insulation material (M-31), failed prior to. 1if toll.

11.2.2 CALORIMETER LOSS DETERMINATION

Two independent methods have been used in the evaluation of Saturn

base heating rates. Both methods,the inflight loss determination and

the preflight calibration, are presente_ here in some detail.

The inflight loss determ_natlon method was developed as a possiblemeans to calculate inflight calorimeter loss rates, without the use of

preflight calibration of the Instr,-,ents. This method has not been

fully exploited at this time and several known shortcomings are pointedout in the following section. _Ex_ever, additional analytical and

experimental studies are being -,,de in an attempt to develop this

method for use on applicable calorimeters.

The preflight calibration method, which is also presented, is

rather typical in scope for calorimeters of this type. Heating rates

obtained from Infllght temperature-time data, using the preflightlaboratory calibration results, are compared with results obtained from

a postfliEht simulation. Generally, good agreement was obtainedbetween these two methods.

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?:

149

@

Guard Ring

Shield Bracket

/-- Thermocouple , , / 3. 175 cm Wide' [., • ,[

"-- llllf" o )0(

0 )0(

Base J /

_\\'_

. .. . .

Unsh_elded SA-3 .... Shielded SA°2

FIG_rKE 11-6 GAS _ERATURE PROBES FOR SA-2 AND SA-3

ii_ .-. 7 . . MPR-SAT-63-1

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150

}III

\ .O C70-7 Eng. 3

Eng. 2

Eng, 5C61~4

Eng. 1 C71-4

c61-1 • C6i-5

I[3:lr C69-5 (_)| Eng. 4I!

C72-I

I

M-31 Panel NOTE: Instrmnentation is attached tobackside of surface shown.

r:] Gas Temperature

O Skin Temperature

]_IGgRE 11-7 ?HEAT_,D'_P3TRI_SNTATLrON-OR'AFT_SIDE

++ MPR'SAT_63-1

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_i 151

11.2.2._I. INFLIGHT _LOSS DETERMINATION

This method is based on the definition of a heat balanc_ just

• after inboard engine cutoff. The assumed heat balance i's defined as

shown in t_e following sketch:

# --,;:.- q_ /qrr

;3: ; .... I

' qLr-

Such that _qln = qs + qL + qrr (kcal/m2"sec) (I)

where ':qin = incoming heat flux to sensor.!- . . ,:.

_::r ";'- qs = pCp _ (dTs/dS) = heat stored in sensor

...._"_ " qL = K(To-Ts)= heat loss by conduction

qrr = Be°T4 = heat reradiated from sensor surface/, s

,'-;-_ " p =isensing element density (kg/m3)

_:ii Cp = specific heat (kcal/kg-°C)

= sensing element thickness (m)

= absorptivity of sensor surface

:_ Ts = sensing element temperature (°C)

_' 8 = time (sec)

_' 5 = transmissivity of the medium between source and sensor

_!i_ _"_" K = conduction loss coefficient (kcal/m2-sec-°C)

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152

To ffistructure temperature to which heat is conducted (°C)

c ffiemlssivity of sensing element

u = Boltzmann constant (kcal/m2-sec-°C ¢)

Making the appropriate substitutions, Equation 1 can be written as .

_qln = PCp _ (dTs/dS) + K(To-T s) + _OTs 4 (2)

The conduction loss coefficient (K) is now evaluated just after inboard

engine cutoff, where the incoming heat flux (qin) is assumed equal tozero.

P,CE,_ (dTs/dS) + 5e°Ts4 qs + qrrx = - = (3)(To'Zs) To-Ts

In Equation 3, the sensor surface emissivity (e) and the transm/ssivity(8) are assumed to be unity, and the structure (casing) temperature

(To) is assumed to be equal to the ambient value just prior to liftoff.The temperature-time slope (dTs/dS) is evaluated at a point just after

inboard engine cutoff (e.g., see sketch on Page I15 of Volume I). The

sensor temperature (Ts) is eva_uated at the point where the temperature-time slope is derived. All other parameters in Equation 3 are knownsensor material properties.

._±'

•; Substitution of the conduction loss, evaluated from Equation 3,

into Equation 2 ylelds the follc_Ing expresslon for the heat rate atcutoff

,,_ qs + qrr_ _qin = qs (To-Ts) + 5coT4 (4)(Zo-Ze) •_ ECO

_ where ECO indicates engine cutoff.

;_ = 5e uT4At engine cutoff qrr s

_; and Equation 4 becomes _qln = .qs- (qs)ECO (5)(

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_ 153

The Conduction loss coefficient (K), evaluated just after inboard

engine cutoff, is assumed to be constant throughout flight and is

applied to Equation 2 in the calculation of the incoming heat flux.• The calorimeter case "temperature (To) has been assumed constant

throughout flight and equal tO the temperature just prior to ignition.

As shown by Equation 5, the heat flux just prior to cutoff can be

evaluated independent of the term (TO - Ts). However, the heat flux" for the remainder of flight depends entirely upon the assumed value of

To. No guidelines exist which might aid in assessing a realistic

value of TO except for membrane type calorimeters where a well definedheat sink exists, and since the present Saturn type calorimeters were

not designed to operate under this condition, it is suspected that in

part the disagreement between this method and the preflight calibra-

tion method may be a result of an incorrect To. Additional calibrations

will be performed to determine variations of initial temperature (To)

as used in the cutoff calibration technique and variations of loss

coefficient (K) during the flight history. These additional tests willbe oriented to determine the effects of mounting structure on the

calibration, and to obtain further information of conduction path

losses thr0ug h thermocouple wires, supporting structure, insulation,etc._ ....... i.-- - • -

Figure 11-8 compares conduction loss coefficients (K) derivedfrom laboratory calibration data and the inflight temperature-time

slope at cutoff. Equation 4 was used in both calculations to definethe loss coefficients for a total: calorimeter, C77-5, and a radiation

calorimeter, C79-2. The slope of the temperature-time curve was

evaluated for known slug temperatures and heat inputs from the labora-

tDry calibration data. For comparison with the calculated inflight

:i_" determined loss coefficient, TO was assumed constant at 46 ° C in bothcases, The inflight (cutoff slope) calibration loss coefficient wasevaluated at sensor temperatures of 605°C and 374°C, for the total and

: radiation calorimeters respectively.

• : The dashed and solid curves for C79-2 shown in Figure 11-8,

illustrate the effect of the transmlssivity of the sapphire window.

The dashed curve, which shows the best agreement with the inflight

calibration value, was obtained by reducing the incident heat flux,

, measured during Calibration, by the appropriate transmissivity.

The curves obtained from the laboratory calibration (see Figure

11-8), show that the conduction loss coefficient (K) is not a constant,

las determined using the inflight calibration, but varies with sensori

temperatures and heat flux.

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1.54

Conduction Los8 Coeff£cient(kcal/mZ-sec-°C) SA-3 Total Calo. 77-5

0 F_ro,.l Cutoff Slope u -

-0.04 "I / •

• qI " 27.1

-0. US / /---- La/'_ b "*. Calib.

ql " 67.6#

-0.12. I50 100 150 200 250 300 350

_!i Sensor Temperature (°C)

. Conduction LOSS Coefficient•. (kcal/m2-sec.OC) SA-3 Radiation Calo. C79-2

. o I I

_--_I " 0.8,.(27.6, ,tom Cutoff Slope 7

.0.02 i_'-_-- _

Lab. Cel£b.-

ql " 27.6Ithout Structure

/ --._= o.s_.(log)/

-0.{)4

ql I09 -_ chout Structure

/-0.06

_: /-0.08 ........

_" /v

-0. I00 50 100 150 200 250 300 350

Sensor Temperature (°C)

:: FICI)I_E II-8 _DUCTION LOss COEFFJECT_T

MPR-SAT- 63 - 1

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> " 155

Neither this method, nor the preflight calibration method, takes

into account effects such as surface contamination (deposits of carbon,

etc.) or change of emissivity of sensor surface during flight.

The absorptivity and transmissivity of the radiation calorimeter

windows are not considered, using the cutoff calibration method, when

evaluating flight data. This would cause an error in the corrected

heat rates of approximately 15 to 20 percent. If these quantities had

been included in the inflight calibration method, the correction would

have been in the proper direction. Since both the absorptivity and the

transmissivity are functions of source temperature and wave length, the

variation throughout flight cannot be fully evaluated without further

_xperlmental investigation.

i

Another assumption , which must be experimentally verified, is that_ the cooloff behavior of the calorimeter sensors is identical to the

behavior due to heating during flight.

Although the inflight loss determination method has several

shortcomings, which have been stated previously, it is concluded that

this method should produce reasonably accurate results just prior tocutoff. For other flight times however, the results will depend

entirely upon the validity of the necessary assumptions. Future

analytical and experimental programs should tend to reduce the number

of uncertainties in this method, and produce a means of evaluating

. heating rates independent of preflight calibration methods.

11,2.2.2 PREFLIGHT CALIBRATION METHOD

:; The preflight or laboratory calibration technique for both thetotal and the radiat%on calorimeters is performed in the followingmanner:

(i) A standard calorimeter and a test calorimeter are simul-

ate: "t'aneously exposed to a constant radiant heat source from a bank of

quartz lamps, such that their geometric location with respect to the

_ lamps is approximately the same.

o (2) The temperature-time history of both calorimeters is recorded.

Knowing the thermal characteristics of the reference calor_eterj theincident heat flux is calculated using the derivative of the temperature-

_: time history curve. Because of the geometric symmetry between thereference and the test calorimeter, the heat flux to the external

_ Dsurface of the calorimeter is approximately the same.

_ (3) With the heat flux and the temperature-time history known,_:_ the thermal and optical characteristics of the test calorimeter can_ be evaluated.

_:

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1.56

(4) The thermal and optical characteristics, thus obtained, can

then be used to evaluate the heat flux incident upon the same calorimeter

durin 8 flight. The laboratory calibration, as described above, is used

to determ/ne the calorimeter loss, as a function of its temperature, •

prior to use.

Following each flight, a postflight simulation of the calorimeter

types is performed. This postfllght simulation involves the duplicationof the infllght temperature-time history, measured by the calorimeter

by means of a variable power source lamp bank. The heating rates_required to duplicate this infllght temperature-tlme history, are

compared to the values obtained using the preflight calibration data.

.Shown in Figures 11-9 and II-i0 are comparisons of heating rates

corrected by the preflight calibration data with heating rates obtained

" from postflight simulation. It should be noted that nitrogen purge

effects _emain small for the radiation calorimeter, even though the

preflight calibration is of short duration, as compared with the post-

flight slmulation. Approximately i0 to 15 percent of the deviation

that remains between the two heating rate curves can be attributed to

differences in the surface and physical properties of the inflight and

postflight calorimeters. Conduction losses to the surrounding structure,if appreclable, will be evaluated during additional experimental testing.

Additional testing is being performed, on both the radiation and

the total heating calorimeters, to evaluate the magnitude of theconduction losses. Since results of these tests are not available at

tb/s time_ no conclusions can be drawn about the overall accuracy of

the inflight loss determination or the preflight laboratory calibration

methods of evaluating the infllght heating rates.

11.2.3 ENGINE CGMPARTMENT

Locations of measurements in the engine compartment are shown in

Figure 11-II. Nine thermocouples measured bulk temperatures of various

structural members, and 32 thermocouples were located in the firewall,to indicate the existence of fires in one or more engine areas prior

to liftoff. This latter system consisted of four circuits of eightthermocouples each, with each thermocouple wired in series within the

circuit. ,_ese measurements were monitored from the blockhouse prior

to liftoff_and would have given cutoff if any excessive rise intemperature had occurred.

_.

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MPR-SAT-63-1

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159

FIGURE Ii-Ii S-I STAGE FLIGHT _S_S

MPR- SAT -63-1

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,4_i" 160

11.3 SKIN TEMPERATURE

11.3.1 PROPELLANT TANK TEMPERATURES

The skin temperatures, at various positions on the propellant tanks

for the SA-3 vehicle, were measured by ten thermocouples located as shown •

in Figure 11-12. The largest difference in temperature between the

three flights •occurred at Station 745. This difference however, has

been attributed to the LOX level. On the first two flights _ the oxygen -

llquld vapor interface was located below Station 745, exposing the tankwall to the warmer ullage gas; while on SA-3, the liquid-vapor interfacewas above Station 745.

II. 3,2 INTERSTAGE SKIN TEMPERATbqtES

Measurements C128-11 and C133-11 (Station 954), located on the

, 25 deg conical portion of the Interstage fairing, indicated maximum

temperatures of 71°C and 160°C, respectively (Figure 11-13). Two

methods have been utilized to estimate the temperatures for these two

measurements, with similar results. The one-shock flow field approxima-

tion considered the angle-of-attack of the vehicle; while in the two-

shock:'flow field approxlmatlonj the angle-of-attack effects were

neglected,

'Both prediction methods estimate the windward (compression) sidetemperature values quite well, considering heat conduction and radiationthrough the corrugated-core sandwich panel, Under the same conditions,the temperatures predicted by the One-shock method for the leeward sideare overestimated by approximately 80 percent.

<! Since the instrumentation drawings show that measurements C128-11

:'_ and C133-II, except for being on opposite sides of the vehicle, were

,_. located similarly with respect to surrounding structure, they would be%,_: expected to exhibit similar temperature responses. No explicit reason

_. for the temperature difference between measurements C128-ii and C133-ii_ is readily discernible_ however, one possible explanation might be that

_. the boundary layer on the leeward side of the vehicle is thickening,_'_-_. due to the angle-of-attack, thus reducing the aerodynamic heat flux,"_' resulting in a lower skin temperature. Further investigation in this

area is, of course, warranted before any tenable conclusion can be

reached.

11.3.3 S-IVD SKIN TEMPERATURES

Measured and estimated temperatures on the S-IVD stage are shown

,.:; in Figures If-14 and II-15. The measuremenEs _all show expected

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# FIGURE 11-12 S-I STAGE FLIGHT __ASUR_TS

MPR-SAT-63-1

7r,

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MPR-SAT-63-1

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165

temperature rises, and although the estimated curves do not correspondto the more extreme dip in the measured temperatures at about 85 sec

. flight time, the agreement at cutoff shows that the final temperatures

can be reasonably predicted.

Two different theoretical approaches were again taken tu predict

I the protuberance effects. The one,shock flow field estimate did not

consider any protuberance effects, but did consider the conduction

through the 0.64 cm thick aluminum skin; while protuberance effectswere considered in the two-shock flow field estimate. Ratios of the

film coefficient, in the vicinity of the protuberance, to that for a

flat plate were obtained from experimental data as a function of

Reynolds nmnber and local Mach number. The flat plate film coefficient

was obtained using Van Drlests' method. This film coefficient, based

on protuberance heating, was then utilized to predict the temperature

history around the protuberance. Again, both prediction methods give

comparable results and agree reasonably well with the measured values.

St should be kept in mind that the range of these temperatures wasfrom O°C to 825°C, and that the measured temperatures were all between

approximately 0°C and 40°C, which is within the range of possible error.

Although the measurements around the protuberance (Figure 11-15) indicate

a steeper slope during the heating phase than the estimated curve, it

is questionable whether this indicates greater heating rates attributableto the protuberance. Measurements shown in Figure 11-14 indicate the

same trend, even though they are well away from the protuberance.

o

• ......

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166

12.0 _ (U) AERODYNAMICS

12.1 EQUATION DERIVATIONS AND LIMITATIONS

Determination of

(I) Ratio of Gradients of Angular Acceleration (stability ratio).

The Stability equation is:

_+ d_+ C_p + _p --0

assuming _ _ 0 and_ = 0 (For small oscillations)

Cl_p+ _o_p= o

C1 -_pJ If

- Bo. O:P

: _ Notations:

_= Angular acceleration, pitch or yaw

I Angular veloc£ty, pitch or yaw

d _ Aerodynamic and fuel flow damping coefficient

CICXp I Angular acceleration due to angle-of-attack

_i B°_p - Angular acceleration due to outboard engine

deflections

(2) Gradient of normal force coefficient and center of pressure

i. location:Z

To

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167

TO = Thrust of outboard engines

Cz = Normal force coefficient, Z___• qS

Q Cz'= Gradient Of normal force coefficient with

respect to angle-of-attack

C2 = Center of pressure location (calibers from base)• D

D--_.= Center of gravity location (calibers from base)

q = Dynamic pressure

S = Reference area (33.47 m2)

, _p m Body fixed normal acceleration

m = Mass

ZF = Cz'C_pqS + I_o sin _ = m_p

Since _ is small, sin B_B in radians

Cz'_qS + _ro _ = mTp

Cz' = m_p_ro_

c_qs

Z Moments CG = I_

z (cP-cc)d_ ZZQB(CG)= _"qSD qSD qSD qSD

c_' _ _ . f_" + _Zo_ CoG)+ d!D " qSD q_v qSD

D D qSD qSD qSD

cP cG 1 [I_"+ zro {_(c_)+ d_)_-=_-+ c__--2-_-_

• When _ ~0 and _~0

c_=c_ [i+ ____. ]D D Cz czqS

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12. 2 WIND TUNNEL TESTS

Wind t_nnel tests were conducted at the Ames 14-foot transonic

tunnel on a 7.4 percent scale model of the Centaur nose configuration,

and at the Langley 8-foot TPT and 4-foot UPWT on a 1.6 percent scalemodel o_; the Saturn Block I vehicle. These tests generally agreed

very well with the 'SA-'3flight test results, the data being within the

eTror margin of the telemetered flight data.

T2.3 CENTAUR S_JLATION PARELS

_gure 12-i :shows a sketch of the modified SA-3 payload showing

•-he basic features of the added panels. Also shown is the station

location of each pressure orifice with its respective measurement num-

ber. _The fl_gh't Tesults of these measurements are shown in Figures12-6 and 12-7 "of Volume I.

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Ill_ t..

= 305cm Dia--_

Sta. 1699.40 [t

II

1727.03 _ .......1731.12 I

" i

Sta. 1699.4

Measurement No.

D152-30 D153o30 D154-30 DL55-30 D1._-3_ 2.3 cm-_o_;' -_--I I I '1 I

•- riii|ta. 173L_ 1726 1720 1714 1707 1701 Base Vent (D147-30)

I-I• _" " "

i_ /- _Ba_eVe_t(D146-30_Measur No D148 30 DI 9 30 50-30

Section A-A

FIGURE 12-1 CENTAUR SIMULATION PANELS

HPR-SAT-63- I

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_i_:! 170

_' 13.0 (I]) _ATI_I'Z

'? 13.1 _'B, SmTATI0Z_ Z'ROGZ_M.

_; There were 607 flight measurements made on the Saturn SA-3 vehicle.

/_ In addition, 87 blockhouse and 16 fire detection measurements were made, "giving a total of 710 measurements. The inflight instrumentation was

_ as follows:

_ T_e of Measurement Number

!_ l_ropulsion 57._ Temperature 169__ Fre ssure 163

::_!_ Strain and "_Ibration 78

ni t echanics n:,,:_ Steering Control 22_ Stabilized Platform 18

'!_, Guidance 5

Signals 3 7;. Voltage, Current, and Frequency 25!:! Mis cellaDeous 2

_ Total Measurements 6.07

]3.2 T_ SYSTemS DESCRIPTXON

Data transmission for flight resting Saturn vehicle SA-3 was ef-

;: fected by eight radlo _e_me_ry systems links and a _ auxiliary equip-

ment assembly. In ad_tlon, _ experimental systems, a PCM system

_::_ (link 6) and a _H_ RF assembly (llnk 9), were flight tested for the

:_ f_rst t/me. _he systems tha_ were utilized were as follows (see also

i Table 13-I):

A. One XO-4 system (link 10)

B, Four XO-4_ systems (l_nks 2, 3, 4, amd 5) -- Triple FM sub-

. systems _ere used in conjunction with these systems.

_. One XO-6C system <link I) -- This system was used to transmit •

_:ii' _ontlnuous data and a high-capacity commutatio_ system was used to_ transmit static and low frequency _ata.

_ D. _wo XO-7 systems <lluks _ and 8) -- These systems were s_n_le- ,

a_deband systems that were used to transmit _,Ibra_i_n data.

5"

_.

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i i

172

E. One PCM system (l!n k 6) -- Because this was the first P(M":_ system to be flight tested, this system was used to transmit redundant

data (commutator output of link l).

F. One LTiF RF assembly (link 9) -- Because this was the ffrst L_iF

RF assembly to be flight tested, this assembly was used to transmit

redundan t data (mixer amplifier of link I0).

Commuta tion

Coummtators on links 2, 3, 4, 5, and I0 were 30 channel hy I0

sampl@s/s , electronic, solid-state commutators. Link 1 used a high-

data-capacity electronic commutator. All commutators performed satis-

factorily with no deviation from normal operation.

PreflibhtCalibration

A

Link. 1 commutated channels received preflight calibration from the

calibrator located within the commutator. Links 7 and 8 received pre-

flight calibration from th_ sweep-frequency calibrator located in the

groun d support equipment rack under the launch pad. The central cali-

brator, located in TM auxiliary equipment assembly, supplied preflight

ealibr,ation tO links 2, 3, 4, 5_ _, 9, 102 and the continuous datachannels of lir_/¢I_ All preflight calibrations were normal and satis-factory.

Infli_ht Calibration

Link I commutat e_ ch_amnels received inflight calibration from the

calibrator located wfthln the ccmmmtater. The central calibrator,

_:_. locate d i_.TM: auxiliary eq_i_men_ assembly_ supplied inflight calibra-

tion to links 2, 3, 4,. 5, 6,. 9_. IO, and. the continuous data channelsnf link I. Links 7 and 8 dld: not receive inflight calibration. All

i! inflight calibzations were n_rma! and aatisfactory.

Antenna Systems

The ni:ue _ telemetry.,l_inks:were transmitted over three antenrr_systems. Links I, 32 5, an_ 7:were tral_smltted by a group of three-

_:,_, _: antennas, spaced around the _ehlcle, on the S-I/S-IVD interstage fair-

._ inE. Links 22 4., 6, and 8 were _ransmitted by an identical antenna

_i syste m. Link I_ was _ransmi_Ee4 by an an_en_ Located on. a.panel Justaft of the second 8.ta_e:ada_em section at. the:l_in l_ position_.. _ washql_.d': that this location; woadS: produce less- s_gna_ attenuatiotr, at_retro

r:ocket fi_in_,, b_tt. thee.; wa_ no- ai_re¢_mb_e_ d_¢e. i_ this= llnk= '

and other Links at, _his. time:. Howevem,., the overal_l:perfbrmance of _His

system= a_pea=a to b_ exeeptio,nel_y/good,,, c_S._rlnE tha_- only one:

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173

The UHF telemetry link was transmitted over one antenna, located

25 deg off Fin I toward Fin IV, on the adapter section of the payload.

13.3 OPERATION OF EXPERIMENTAL TELEMETRY SYSTemS

PCM STstem (link 6)

The PCM system received the output wavetrain of the link I commu-

'J tator and digital information from the horizon sensor. The function

of this system was to convert multiplexed analog information to digitalinformation. The system contained an analog-to-digital converter, a

programmer, and an FMtransmitter.

The commutator wavetrain was applied to the A-D converter which

converted the analog information to digital information in the form of

a serial, binary-coded wavetrain.

The programner received timing information from the link i co_u-

tator and supplied the A-D converter with this information at the pro-

per time; this caused proper formating of the binary-coded wavetrain.

The programmer was programmed to present information from the horizonsensor to the A-D converter. The serial, binary-coded wavetrain outputof the A-D converter is used to modulate the transmitter.

A statistical study was made of the inflight calibrations applied

to the system. The results pertaining to accuracy of the system wereas follows:

•Sixty-eight percent of the information was within _ 0.16 percentof the mean value; a confidence level of 99 percent exists, that the

tolerance (T 0.16 percent) will not vary more than T 0.02 percent.

Ninety-five percent of the information was within T 0.32 percent of themean value; a confidence level of 99 percent exists, that the tolerance

(T 0.32 percent) will not vary more than T 0.04 percent. Ninety-nine

percent of the information was within T 0.48 percent of the mean value;a confidence level of 99 percent exists, that the tolerance (T 0.48

percent) will not vary more than T 0.06 percent_

The overall performance of PCM/FM link 6 was found to be excellent,and indications are that the PCM/FM system will provide very accurate

data.

UHF RF Assembly (link 9)

The 5qlF RF assembly received the modulation output of the mixer

amplifier and modulated the LrHF RF assembly. The assembly consists ofan automatic frequency stabilizer, UHF oscillator, crystal oscillator,

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174_: buffer amplifier, drive amplifier, and an RF power amplifier with an

_i output of i0 watts..

The purpose of this assembly was to transmit at UKF frequencies

in order to evaluate and improve the UHF system. Possibly, the UHF" a

bard will be used more exte=sively in the future for transmitting te-

lemetry data.

The data reduction analog oscillograms of links 9 and i0 were I

compared. These oscillograms indicated that the difference between

links 9 and I0 was insignificant to the extent of resolution possib-le

with the osci]_lograms. Lower RF output power from I/HF link 9 accounts

for the poorer signal-to-noise ratios during flame attenuation periods

and at other times during the flight test.

The overall performance of UHF link 9 was found to be satisfactory.

13.4 TELEMETRY AND TRACKING STATIONS

The locations of some of the ground telemetry and tracking stations

used for the. SA-3 flight are shown in Figure 13-1. The performance of

these stations and the quality of the signals received are discussed

in Voltmae ! of this report.

13.5 PHOTOGRAPHIC COVERAGE

Engineering Sequen_ial_ Camera Coverage (ESCC) was used toprovide

engineering surve_llance of the launch opera_ion and the vehicle during

powered and: coast flight. The film was used to provide records of_ the

various ground support equipmen_ (GSE) operation, heat shield environ-

i m_nt, v ehicl_ motions during launch and flight, and various malfunc-tiQns which occur=ed.

The ESCC for the S_%.-3 flight_ was comparable to that of SA-2.

Sixty-eight cameras were used to fulfill the requirements of observing

launc h preparation, launch,, powered and coast flight, retro firing,

an(_ "_roject _Highwater". These cameras included both fixed and track+

ing _nstruments located on the launch pedestal, around the complex,

_: and at •various, tracking sites. Of the 68 cameras used for the test,:66 provided satisfactory coverage.

Sixteen-cemora_: were: lo.¢ated on the launch pedestal to. observe

GSEi operat£on an_ th_ vehic/¢;_ duri,g ignitions: and' liftoff. Four cameras

o.b__e_z_ed-:the_, retr_,_.l_:: stt_R_x_- arms, fOur_ _observed the holddm_: arms,.

and two. obseawed" t_- short_ c_bl'e..masts:,. F_z_- cameTas_ were mouate_: *

under the tDrus zing- to ph_tographensine ope_stlon and the beet s_leld

area during ignit-_on: and liftolf_ One camera-o_served the LOX fill: and

dr_s_

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175

'Q 9 Pad 34

0 1 2 3 Ion • (:apeTelemetryStation

• Hanger D Station

• C-Band RadarStation 1.16

• Cape Telemetry 3 Station

• Mandy Telemetry and IrDOP Station

• Mk II Station

F_GtrRE 13-I TEL_dETRY AND TRACKING STATION LOCATIONS

MPR-SAT-63- I

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i_:: The five cameras viewing the engine operation and heat shield area

provided coverage comparable to that obtained on SA-2. This film: showed that the heat shield stayed intact much better than on SA-I and

SA-2. Although some movement or pulsation of the heat shield during

engine ignition _as evident, the amplitude was much less than that ofSA-I and SA-2.

The retractable support arms, the holddown arms, and the short

cable masts appeared to operate properly. The high frequency rippling

of the vehicle skin, observed on previous flights, was not _pparent;

however, movement in the form of lower frequency undulation was visible.No failures in GSE connect fittings were observed, such as occurred on

SA-2.

The LOX fill and drain mast did not retract as expected before

vehicle llftoff. Because of smoke and debris, it could not be deter-

:,: mined if any contact between the mast and the vehicle occurred during

liftoff. Approximately 6.7 sec after liftoff, the mast collapsed dueto heat and blast.

Five cameras were located on the umbilical tower oriented to view

the vehicle and the GSE during ignition, lif_off, and after liftoff.

One camera, located at the 12.2 m level, viewed the fuel fi_l and drainmast. The mast appeared to operate properly. Another camera, locatedat the 30.5 m level and oriented to view the top of the booster, oh-

m: rained excellent coverage. :No malfunctions _ere observed by thiscamera. Two cameras were located at the 48.8 m level and one at the

64.0 m level to view the swing arm disconnect aridthe condition of the

launch pedestal after liftoff. _ The swine arm appeared to function pro-

perly. The LOX fill and drain mast collapse was shown by this coverage.

Opening of the LOX vent 'valve at 2.3 sec range time on LOX tank 02 was_?.... also covered by this camera.

Two cameras were oriented to view targets on the vehicle nose

cone to determine the sway of the vehicle. Coverage obtained indi-

cated that no apparent sway occurred during the 5 min prior to launch.

Fifteen cameras provided tr_cking coverage of the vehicle from

launch through retro rocket firing, and coast flight to vehicle de-

!_" Struct,

:Discoloration of _the bottom portion of the vehicle was observed

,approximately 20 sec prior :to outboard engine cutoff. This discolora-tion was similar to _hat o_sez_ed on the SA-I flight. Eetro rocket

:_i_ion was also =_obmarwed _y .the tracki_ .cameras. I

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177

"Project Highwater" was observed both during and after the explo-sion. The image size from the camera was very small at the time of

the explosion and a detailed analysis would be hard to make; however,

tumbling of the booster and parts of the S-IV dummy stage could be seen8 after the destruct.

Tracking coverage from approximately T+25 to T+80 sec range time

was also obtained by a camera located in an aircraft flying at approxi-

_ mately 4.6 kilometers. This camera provided excellent coverage of the

vehicle during this portion of flight.

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178

14.0 (10 DATA REDUCTION

14.1 TELDSmU_ DATA

14. I.1 _Y GROUND STATION

Real Time Experiment

As on the SA-2 flight, an attempt was made to record telemetry

data at Green Mountain when the vehicle rose above radio horizon. The

experiment was again successful and was performed essentially the same

as before, except that for the first time a microwave link was employedbetween Green MoUntain and the Computation Division. Five measurements

were displayed in real time for members of the Flight Evaluation Work-

ing Group by means of closed circuit television. The measurements dis-

played were Inboard Engine Cutoff, Outboard Engine Cutoff, PlatformPitch Position minus Program, Platform Yaw Position, and Platform Roll

Position. Various parameters were displayed by oscillograph immediately

after the firing. The recorded signals were of good quality, and the

effects of the retro rocket firing were clearly visible, both during

and after firing.

Class I Data

The attempt to make system-grouped oscillographs from Hangar D

and RCA recorded telemetry was unsuccessful. The requested groupings

were made available five days after the launch as opposed to expected

delivery of these groupings approximately twelve hours after receipt

of telemetry tapes. Factors contributing to the lack of success in

making oscillograph recordings were as follows:

a. Failure of RCA to provide the link arrangement requested

_i Dn ½" magnetic tape. This failure was attributed to conflicting re-

quirements by RCA; that is, a request for two original single sideband

tapes and the request for specific telemetry link groupings exceeded

the nt_nber of tape transports committed to the launch. This situation

is being investigated and will be resolved before the SA-4 launch.

!_iI b. The assigmnent of too few qualified personnel by Computa-

tion Division to a new telemetry ground station. Computation Division

Was an the process of accepting a new telemetry ground station at the

! time of the SA-3 launch, while the old ground station was inoperative.

Addlt_onal qual_ed _ersom_el will be checked-out on the new facility

before the SA-4 laumth_ !

Two recently acquired systems were used for the first

t_me by Computation Division. These were a Gulzon Industries tape

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r

_ 179

" synchronizer and combiner which combines two ½" tape outputs into asingle 1" tape recording. It was by this method that an input tapewas finally provided for the oscillograph groupings. A second systemused for the first time was a device manufactured by Recordak which

$ reduces documents to microfilm.

14.1.2 ANALOG TO DIGITAL CONVERSION

RCC'3 Cycle Counter ""

Frequency dependent telemetry measurements were processed by the

RCC-3 cycle counter..These measurements were chamber pressure, turbine

:_ rpm, flow rates, for each of the eight engines, and inverter frequency:_ for the vehicle. No difficulties were experienced in processing any

of these data and results were available approximately twelve hours

after receipt of telemetry tapes.

Microsadlc

Operation of the analog-to-digital converter was unsatisfactory

due to the time required to obtain digital data. Difficulty was ex-

perienced in the cireultry controlling the buffer in which digital data

is St0red prior to writing on magnetlc tape. Three days were spent

in correcting this problem; the first linearized and calibrated data

were made available four days after receipt of data and continued at a

satlsfactory pace thereafter. After reduction of data was complete,it was determined that all PAM data were in error by one second; the

trouble was determined to be programmer error and these data were subse-

quently re-run. An effort is underway at the present time to modernize

the buffer circuitry; this effort, in addition to delivery of a second

_.. analog-to-digital converter, should preclude difficulties of thisnature in the future.

i 14.1.3 EXPERIMENTS

Two experimental packages were carried on the SA-3 flight; these

were PCM and l_I_. Outputs of these packages were recorded by AstrlonicsDivision in an instrumentation trailer. The PCM information paralleled

the 216 package on Link I, except for horizon sensor informationwhich

was also a passenger. The P_ information was processed by a Dyna-tronlcs ground station and the horizon sensor information was processed

in the I_M 7090 Computer. The remainder of the PCM link is at the

present time being compared wlth the 216 package by the 7090 computer.

The lIHF informatlon paralleled link I0. UHF data were digitized by

Microsadlc, and a comparison with link I0 data is now underway.

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I4.1.4 vICION DATA

In most cases, the vibration data reduction was routine and was_pleted as scheduled with little difficulty. Even though this was

the first time that Ehe SSB _emoduiatlon station was used, the compO-site data compared favorabl-y w_th the composites from LOC.

Generally, le_s work Wa@ required on SA-3 because personnel are

more familiar with :_he _SSB-data. Also, on the SA-I and _A-2 f_Ights,much _time was d_voted to reduCing static data for comparison purposes.

Consequently, a _ufficlent _m0unt of data has been backiogged, such

that a minim,-- o_ reduction Was required of previous tests, both stati'c

and flight. _n-addition, some new equipment was available, such as

averagers and detectors, that simplified much of the routine reduction,

and the dupllcatiOn of certain prodesses was eliminated.

"- 14. t. 50UT_IE DATA

Output data were presented in tabuia_ed fOrm, in plotted form on

'the EAI plotter, and for the first time on the sC-4020 _,icrofilm re-

Corder. Plotting, as usual, was a bottleneck due to the large volum_of data; however, Operatlo_ of the EAI plotter was considered satisfac-

tory. It is anticipated that the SC-4020 will relieve the workload Onthe EAI plotte_ in the future.

14.2 DATA

14.2.i ¢ ERA5

Analog doppler data Were _Athered by the UDOP system at the fol-

_i lowing sites :

I. Playa1_nda _Beach _ pha@_-lock and open-ioo p

2. Merritt Island . phase-lock and open-loop

.: 3, Titusville _ phas_-loek a_d open-loop

Cape ..'sites

i. Blockhouse 34 - phdS_-io'ek only

_: / 2. :Mati_y sit_- -phas_--loek Only

_ _-

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Capesites (cont)

3. Blockhouse 26 - open-loop only

f 4. Site C - open-loop only

5. Site B - open-loop only

t 6. Hangar D - open-loop only

Downrange sites

I. Walker Cay - phase-lock and open-loop

2. Great Sale - phase-lock and open-loop

3. Allans Cay - phase-lock and open-loop

4. Bassett Cove - phase-lock and open-loop

5. Carter Cay - open-loop only

The uprange transmitter-receiver complex operated in the interim

offset mode (doppler bias) for the first time on a Saturn flight. The

i kc bias was recorded on the flight tapes for data reduction purposes.

No switch-over of the interrogating transmitter was planned or per-

formed. Therefore, the uprange complex (Mainland and Cape receivers)

operated in the sum mode, and the downrange complex in the difference

mode, for the entire flight.

The doppler data were digitized on the Data Reduction Branch's

automatic cycle counter (RCC-3). The RCC-3 employs a phase-locked

tracking filter with optional bandwldths of 2_5, 5.0, 10.0, 25.0, 50.0,and 100.0¢ps. The data cou_ted for determining position data were

tracked primarily with a 25 cps bandwidth. However, several band-

Widths were used for evaluation purposes.

14.2.2 QUALITY OFCYCLE DATA

_efore cutoff, the LrDOP suffered most in the interval between 125

and 135 seconds. Both the duration and intensity of noise in the cycle

data varied widely with the various receivers. The signal noise char-

aoteristics were such that no phase-locked receiver appeared to com-pletely drop lock in this interval; the same was true with the RCC-3tracking filter during the counting operation. Nevertheless, all cycledata contain prohibitive noise somewhere within the interval. The

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182 .-

least disturbed cycle data were obtained from the Mandy site. It hadexcessive noise for a total of about 3 sec over the entire 10 sec in-

terval of poor quality data. The maximum error in the filtered data ,

remained less than 2.0 cycles in a given 0. i sec readout period. Theaccumulated error was about 3 cycles. In contrast, the filtered

Merritt Island data were noisy for a total of 5 or 6 sec in the I0 sec

interval, and had 0. I sec readout errors as large as 4 cycles. The

accumulated error however, appears to be comparable to that for Mandy.

Between 125 and 135 sec, the remaining data are of a general

quality somewhere between that for Mandy and Merritt Island. But thenoise before cutoff was not limited to that interval. The Blockhouse

34 data contain prohibitive noise from about 12 to 25 seconds. The

Playalinda data contain excessive jitter until after 70 sec and ex-

hibited excessive noise, similar to the 125 to 135 sec interval, as

• early as 118 seconds.

Probable receiver drop-lock conditions, as indicated by the mag-

nitude of cycle data errors obtained from data counted without post-

flight filtering, occurred as follows:

a. Merritt Island between 20,0 and 21.8 and between 83.6 and

::, 85.3 seconds.

b. Titusville between 135 and 137.4 seconds.

c. All receivers through the area of retro rocket burning.

In general, comparisons between phase-lock and open-loop data,

derived from common sites, indicate that the data are comparable. How-.: ever, in isolated instances, each type of data are somewhat superior.

14.2.3 POSITION DATA

The solution for position data utilized the vehicle launch positionas a tie-in. The Cape data which contains the I kc bias were auto-

matically counted from llftoff time, and produced the trajectory from_'_ liftoff to about 30 sec, where Merritt Island and Titusville were added

to the solution. The Playallnda data were not usable before 20 secand the Blockhouse 34 data were deleted after 12 seconds. Several com-

u: binations of stations were used between 120 and 135 sec in an effort

_ :- " to minimize the overall position degradation. After 135 sec, attempts

_i!!i were made to use the downrange data in the difference mode, but a large• inconsistency in the least squares solution rendered the data unusable.

_ A triangulation for position after retro rocket burning requires a

tierln point from other instrumentation. Due to a lower priority, this_:: solution is not completed.

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183

From:the Standpoint of data accuracy, the solution for vehicle

. . data before wasposition cutoff hurt most by the interval of noise

between12_ and 135 seconds. The position data were computed throughthis intervai:at the expense of extensive cycle data correction, based

essential!y:6n an assumption of constant acceleration over a shorttime period. The internal consistency of the least squares solution

increases from about 0.l to about 0.8 m in this interval. Thus, the

probable position error is increased by about a factor of eight for the

remaining position data, since a tie-in with other instrumentation at135set was not made.

From the standpoint of position data smoothness, and consequently,

:_ accuracy of velocity and acceleration data, the trajectory sufferednot only between 120 and 135 sec, but also between about 12 and 30

seconds. This is apparently due to the deletion of the Blockhouse 34

data at 12 seconds. The Blockhouse 34 receiver is much closer to the

vehicle than the other receivers in this period. Therefore, the geo-metry of the solution for the vertical coordinate is much weaker with-

out the Biockhouse 34 data (by about a factor of 25).

14_ 3--'METEOROLOGI CAL DATA

The:SA-3 Radi0sondeData were transmitted from Cape Canaveral toComputation Division by transceiver. Transmission began at 0030 hours

_:on _November :16 and stopped at 2030 hours on November 16. In all, six

releases_ere transmlttedwhich took approximately seven hours. TheRadiosonde T-0 release was received at 2000 hours on November l6 and

was two hours off schedule.

_:: The Rocketsonde data tape was received on November 26, approxi-_ mately 3 or 4 days off schedule. The angle-of-attack data was received

on December 3.

!_

S

&

i _

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184

15.0 (U) BL SADJUS OF FLIGHTMECHANICALDATA

Flight data contains certain errors due to telemetering and data

reduction processes, slight misalignments of sensors, and electronic

noise. On SA-I and SA-2, biases of flight data were determined by a |

least squares solution of the primary control functions, using the

linearized forms of the moment, normal force, control, and wind equa-

tions in the pitch and yaw planes. These biases were compared to an

average of the data over a i0 see period prior to engine ignition, and )were found to agree with this bias to within 0.I deg or less. This

bias program did not work on SA-3 for unkno_n_ reasons. Therefore, the

average of the flight mechanical data prior to engine ignition Was

used to establish the biases. The angle-of-attack biases were hand-

computed from the wind equation after the other biases had been deter-mined.

" Shifts in differential pressures were obtained by making the dif-

ferential pressures zero prior to ignition, where the instruments weremeasuring a static condition, and also shifting them into zero after

cutoff, where the ambient pressu_re is zero. Direct pressure measure-ments were shifted into agreemeBt with the ambient pressure prio_ to

ignition, and to zero Where the ambient pressure was zero. All of

these shifts were either constants or o_ first degree with time.

Table 15-I contains the more important shifts of flight mechanical

measurements, along with the s_ndard deviation of the random errorcomponent.

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TABLE 15-I185

FLICRT _gCI_CAL .DATAPRg-I_I_luq'lT_kS I_R SA-3

Telemetered 14easu_ement Standard Deviation l_e- i_nitton CalculatedVariable N_ber o£ Random Error Observed Bias Bias

"Local Angle-of- "P16-30 "0_05 (deE) O.12 (de_/Attack I

Locat Angle-o£_ P17-30 0.OS (deE) -0.47 (deE)Attack _I

Local AnEle-o£- F18-30 0.05 (deE) -0.22 (de_Attack III

Local _le-of- P19-30 0.05 (deE) -0.03 (de_Attack IV

,/, Pitch Actuator O1-1 0.06 (deE) 0.21 (deE)position 1

Pitch Actuator 01-2 0.04 (des) -0.25 (deE)Position 2

Pitch Actuator 01-3 0:0_ (deE) -0.19 (deg)Position 3

Pitch Actuator 01-4 0.04 (deE) 0.29 (deE)Position 4

Yaw Actuator 02-1 0.03 (deg) 0.09 (deg)Position 1

Yaw Actuator G2-2 0.12 (deE) O.0& (deg)Position 2

;.i Yaw Actuator 02-3 0.06 (de8) =0.16 (de8)Position 3

Yaw Actuator 02-4 0.02 (deE) -0.1& (deE)'Position 4

Platform Pitch Hl-l$ 0.09 (des) 0.19 (des)"Position MinusProEram

Yaw Attitude H2-15 0.08 (deg) 0.02 (de8)Zrror Angle

Pitch Normal YlO-I1 0.09 (=/s 2) 0.03 (m/s 2)Acceleration

Yaw Normal Pll-ll 0.08 (m/s 2) 0.03 (_/s 2)_: Acceleration

,_'.-.

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_ 186

SA-3 FLIGHT EVALUATION REPORT

(U) DISTRIBUTION

Dr. yon Braun, MrDIR ._ r _ Mr. Boehm, M-ASTR-M

Dr. Rees, M-DEP-R&D Mr. Hosenthien, M-ASTR-F

Mr. Gorman, M-DEP-AI_4 Mr. Blackstone, M-ASTR-FF

•. ..... _ Mr. Mandel, M-ASTR-GM-AERO , ::_ Mr. Hoberg, M-ASTR-I

" Dr. Gelssler, M-AERO-DIR Mr. Bell, M-ASTR-IM

Mr. Jean, M-AERO-]_S (4) , _ Mr. Moore, M-ASTR-N

Mr. Dahm, M-AERO-A (2): Mr. McMahen, M-ASTR-NT (5)

Mr. Vaughan, M-AERO-G (3)' •Mr. Ryan, M-AERO-D _ M-LVOD

Mr. l{olderer, M-AERO-E Dr. Gruene, M-LVO-DIR

, Dr. Speer, M-AERO-F (25) Mr. Zeiler, M-LVO-M (3)Dr. Hoelker, M-AER0-P Mr. Sendler, M-LVO-E (4)

Mr. R. Cummings, M-AEEO-TS Mr. Collins, M-LVO-EP

Mr. D. Douglas, M-AERO-TS

Mr. H. Horn, M-AERO-D M-RELMr. Schulze, M-REL (3)

M-L&M

Mr. Hueter, M-IZeM-DIR (2) M-QUALMr. Grau, M-QUAL-DIR

M-COMP Mr. Klauss, M-QUAL-TS

Dr. Hoelzer, M-COMP-DIR Mr. Wittmann, M-QUAL-E

Mr. Fortenherry, M-COMP-A Mr. Urbanski, M-QUAL-M

Mr. Cochran, M-COMP-R Mr. Brooks, M-QUAL-P

Mr. Shaver, M-COMP-S Mr. Peck, M-QUAL-PSMr. Smith, M-QUAL-Q

• M-ME

Mr. Kuers, M-ME-DIE M-RP

Mr. Groth, M-ME-TS (4) Dr. Stuhlinger, M-RP-DIRMr. Miles, Jr., M-RP-R

M-FPO Dr. Shelton, M-RP-N

Mr. Koelle, M-FPO-DIR (2) Dr. Heller, M-RP-T

Mr. Weaver, M-FPO Mr. Thompson, M-RP-I

M-ASTR

Dr. Haeussermann, M-ASTR-DIR M-SAT

Mr. Noel, M-ASTR-TSJ Dr. Lange, M-SAT-DIR

Mr. Wagnon, M-ASTR-TSR Dr. Kuettner, M-SAT-AP

Mr. Digesu, M-ASTR-A Mr. Vreuls, M-SAT (5)

Mr. Taylor, M-ASTR-R Mr. D. R. Bowden, M-SAT-SIT (Downey)

Mr. Fichtner, M-ASTR-E

Mr. Baggs - Mr. Stroud, M-ASTR-E M-H

Dr--?Rudolf, M-BME-DIR

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} :: Dr--_azek, M-P&VE.DIR Mr. Warden, M-PATi Mr. Weidner, M-P&VE-DIR

__'. Mr. Burrows, M-P&VE-REL M-MI_Mr. Palaoro, M-P&VE-V Mr. Robert L. Riemer, M-MICH-QA j

J:" Mr. Glover, M-P&VE.VA Dr. Constan, M-MICH

_ Mr. Stein, M-P&VE-VE

Mr. Rothe, M-P&VE-VG LO

Mr. Barraza, M-P&VE-VK Dr. Debus, LO-DIR )

_: Mr. Seymour, M-P&VE-O}I (2) Dr. Knothe, LO-TSMr. Sehulze, M-P&VE-E (2) Col. Bidgood, LO-F

if: Mr. Harber, M,P&VE-EA Lt. Col. Petrone L0-H (3)

Mr. Kistler, M-p&VE-EF Mr. Peppel, LO-D

_ Mr. Hoffman, M-P&VE-ES Mr. Darby, LO-DHE

:_ Mr. Goerner, M.P&VE-F Mr. Body, LO-DS

Dr. Lucas, M_P&_E-M

:_;_ Col. Fellows, M-P&VE-NP (4)Mr. Paul, M-P&VE-P (2)

Mr. Thompson, M-P&VE-PA

Mr. Reed, M-P&VE-PL

Mr. Furman, M-P&VE-PM

Mr. Wood, M-P&VE-PTMr. Connell, M-P&VE-PH

Mr. HeusinEer, M-P&VE-PP (3)

Mr. Kro11, M-P&VE-S

Mr. ollunt,M-P&VE-S

Mr. Verble, M.P&VE-SB

Mr. Farrow, M-P&VE-ST (4)

Mr. Sterett, M-P&VE-SS

Mr. Showers, M-P&VE.SL

M'TPC

ii Mr. Smith, M-TPC

_ _ M.TESTMr. Heimburg, M-TEST-D_R

Mr. Auter, M.TEST-E

Mr. Sieber, M-TEST-M

Mr. Thornton, M.TEST-MC[

_ Mr. Driseoll, M-TES_T-T " ),i_ " Mr. Tessmann, M-TEST-C

M-MS-IFL(8) 7(4)

i]ill

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!188

DISTRIBUTION (CONCLUDED)

EXTERNAL

i Headquarters, National Aeronautics & Space Administration

Washington 25, D. C.

Offices of Space Sciences

Director: Mr. H. E. Newell

Office of Manned Space Flight

Director of Launch Vehicles and Propulsion

Mr. Milton W. Rosen (4)

Douglas Aircraft Company, Inc.

Missile and Space Systems Engineering

Santa Monica, CaliforniaAttn: H.M. Thomas

A. J. German (5)

The Boeing CompanyHIC Bldg.

Attn: A. H. Phillips

North American Aviation

Space & Information Division Systems12214 Lakewood Boulevard

Downey, CaliforniaAttn: A. Shimizu

•._. Rocketdyne6633 Canogo Avenue

Canogo Park, CaliforniaAttn: O. I. Thorsen

• Chrysler Space Division

Michoud OperationsAttn: B. Helnrich