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Munch's paintings Separation and Portrait of Friedrich. Nietzsche dated 1893 and 1905 respectively [1]. table. 1 indicates all the pigments
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Actinide Separation from MAW Process Streams via Ion-Exchange
R. Oldenbourg Verlag München 1984. Actinide Separation from MAW Process Streams via Ion-Exchange Techniques. By SAMEH A. ALI and HANS J. ACHE
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Stage Separation Aerodynamics of Future Space Transport Systems
Universität München zur Erlangung des akademischen Grades eines. Doktor-Ingenieurs 3 Progress in Analysis of Unsteady Stage Separation of.
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Mochammad Agoes Moelyadi
Stage Separation Aerodynamics of
Future Space Transport Systems
Lehrstuhl
fürAerodynamik
aerLehrstühl für Aerodynamik
Lehrstuhl für Aerodynamik
Stage Separation Aerodynamics of
Future Space Transport Systems
Mochammad Agoes Moelyadi
Doktor-Ingenieurs
genehmigten Dissertation. Vorsitzender : Univ.-Prof. Dr. rer. nat. Ulrich WalterPrüfer der Dissertation :
1. Univ.-Prof. Dr. -Ing. Boris Laschka, em.
2. Univ.-Prof. Dr. -Ing. habil. Nikolaus A. Adams
3. Prof. Dr. i.r. H. R. Harijono Djojodihardjo, Sc.D.,
Univ. Al Azhar, Jakarta / Indonesien
ACKNOWLEDGEMENTS
Many thanks need to go out, it is a monumental accomplishment for me to graduate. I would like to express firstly my utmost gratitude to God for His Help and Bounty and to my loving parents, Mochammad Sutadi and Murdaningsih, as well as my parents in law, Mochammad Faisal and Nuriah. I am very thankful to my supervisor, Univ.-Prof. Dr.-Ing. Boris Laschka, em., for giving me opportunity to work on this interesting research field and for his pioneering work on unsteady aerodynamics which served as a starting point for my doctoral research at Technical University München and also for his invaluable advice and discussion during the research time. My honourable thanks must also go out to Univ.-Prof. Dr. -Ing. Gottfried Sachs for his encouragement and support and for his valuable advice and discussion. It is also my worthy thanks to Prof. Dr. Harijono Djojodihardjo for kindly help to conduct the research here and for his advice and discussion in the beginning research time. My special thanks go to Univ.-Prof. Dr.-Ing Nikolaus A. Adams who heads of the institute of Aerodynamics giving me the support during the final time of my writing. I would also like to thank Dr.-Ing. Christian Breitsamter for spending countless hours trying to help me understand the space vehicle problems and for his generosity and help. I would also like to thank all my friends at Technical University München, Dipl.- Ing. A. Allen, Dipl.-Ing. M. Iatrou, Dipl.-Ing. L. Jiang, W. Sekar, M.Sc., Dr.-Ing. U. Sickmüller, Dipl.-Ing. A. Pechloff, Dipl.-Ing. C. Bellastrada, Dipl.-Ing. A. Schmid, Dipl.-Ing. R. Reß and also all my colleges in the Institute of Aerodynamics. This work would not have been possible without their friendship and their helpful discussions and suggestions on both the technical and non- technical topics. Most importantly, I cannot thank enough my loving wife, Ratna Dewi Angraeni for her endless support and patience. To my son, Ihsanuddin, and my daughters, Qonita and Tazkiya, thank you for giving me so much happiness. München, September 2006 Mochammad Agoes Moelyadi iABSTRACT
Steady and unsteady Euler investigation is carried out to simulate the unsteady flow physical phenomena on the complex geometry of two stage space transportation system during a separation phase. The dynamic computational grids and local smoothing techniques as well as the solution of unsteady Euler equations based on the finite explicit finite volume shock capturing method are used to obtain accurate unsteady flow solution. The staging path is approached with the one-minus-cosine function applied for the relative angle of attack and relative distance. The effects of numerical factors on flow solution including grid density and grid smoothing are investigated. The results obtained include the static pressure contours on symmetry plane as well as on the aerodynamic coefficients of the orbital and carrier stages that are compared to the corresponding experimental data.Zusammenfassung
Die erzielten Resultate schließen die Druck Verteilungen in der Symmetrieebene sowie die aerodynamischen Beiwerte der Ober- und Unterstufe ein. Sie werden mit entsprechenden experimentellen Daten verglichen. iiLIST OF CONTENTS
CHAPTER Page
ACKNOWLEDMENTS i
ABSTRACT / Zusammenfassung ii
LIST OF CONTENTS iii
LIST OF FIGURES vii
LIST OF TABLES xii
NOMENCLATURE xiii
GLOSSARY xviii
I INTRODUCTION
1 Overview
12 Problems and Challenges in the Simulation of Unsteady
Stage Separation of Two-Stage Space Transport Systems 53 Progress in Analysis of Unsteady Stage Separation of
Hypersonic Space Transport Systems 8
4 Objectives and Scope of the Study
95 Problem Solution and Methodology
106 Outline of the Present Analysis
137 Research contributions
14II COMPUTATIONAL AERODYNAMIC SIMULATION
171 Simulation of Stage Separation of TSTO
SpaceTransportation Systems 17
2 The Computational Approach to Physics of Stage
Separation of the TSTO Space Vehicle System 19
3 Basic Mathematical Flow Models
223.1 The Unsteady Euler equations
224 Geometry Models of TSTO Space Transportation System
255 The Model of Separation Path of the Orbital Stage
27Two Stage to Orbit
iii6 Aerodynamic Forces and Moments
29III COMPUTATIONAL GRID
311 Grids in Computational Fluid Simulations
312 Grid Generation Methods for Stage Separation of TSTO
Space System 32
2.1 Structured Grid Generation Techniques
342.2 Dynamic Grid Technique for TSTO Space Vehicle
System 36
IV NUMERICAL METHOD
381 Numerical Solutions for Euler Equations
382 Numerical Methods for Stage Separation of TSTO Space
Vehicle Systems 40
2.1 Finite Volume Discretization Method
402.2 Evaluation of Convective Fluxes
412.3 Initial and Boundary Conditions
462.3.1 Body boundary condition
472.3.2 Farfield boundary condition
482.3.3 Symmetry boundary condition
492.3.4 Boundary between grid block
502.4 Temporal Discretization
503 Unsteady Flow Simulations
53V STEADY AERODYNAMIC OF STAGE SEPARATION OF
TSTO SPACE VEHICLE SYSTEM ANALYSIS 55
1 Experimental Test: Model and Conditions
552 Computational Test: Facilities, Procedures and Test Cases
592.1 Computational Facilities
592.2 Computational Procedures
602.2.1 Topology and Mesh Generation
602.2.2 Obtaining Numerical Flow Solutions
652.3 Computational Test Cases
66iv
3 Effects of Numerical Grids
673.1 Effects of Grid Smoothing
673.2 Effects of Grid Density
724 Validations
764.1 Simplified Configuration
764.2 Fully Two-Stage-to-Orbit Configuration
825 Detailed Analysis of Quasy Steady Stage Separation of
TSTO vehicle system 90
5.1 Flat Plate / EOS Configuration
905.1.1 Effects of Orbital Stage Position
905.1.2 Effects of Mach number
955.2 ELAC1C /EOS Configuration
995.2.1 Effects of Angle of Attack of Carrier Stage
995.2.2 Effects of Separation Distance between the
Stage 104
5.2.3 Effects of Orbital Stage Angle of Attack
108VI ANALYSIS OF UNSTEADY AERODYNAMICS OF STAGE
SEPARATION OF TSTO SPACE VEHICLE SYSTEM 114
1 Computational Test
1142 Simulation Results of Unsteady Stage Separation of Fully
Two-Stage-to-Orbit Configuration 117
2.1 Aerodynamic Characteristics of Unsteady Stage
Separation 117
2.2 Instantaneous Flow Features of Stage Separation
1202.2.1 Instantaneous Flow Features at reduced
frequency of 0.22 1202.2.2 Instantaneous Flow Features at reduced
frequency of 0.5 1242.2.3 Instantaneous Flow Features at reduced
frequency of 1.0 127 v2.3 Comparison between the Steady and Unsteady State
Solutions130
VII CONCLUSIONS AND RECOMMENDATIONS
136REFERENCES
139APPENDICES
ACONSERVATIVE DIFFERENTIAL FORM OF EULER
EQUATION
146B EULER EQUATIONS FORMULATED FOR MOVING
GRIDS 150
C TRANSFINITE INTERPOLATION ALGORITHMS FOR
GRID GENERATION 152
D POISSON AND LAPLACE ALGORITHMS FOR GRID
GENERATION 155
E UPWIND DISCRETIZATION SCHEMES
158E.1 Flux Vector Splitting
158E.2 Flux Difference Splitting
160F
AERODYNAMIC FORCE AND MOMENT COEFFICIENTS
DATA SET FOR STEADY FLOWS OF TWO-STAGE
SPACE TRANSPORT SYSTEM WITH THE IDEALIZED
FLAT PLATE
162G
AERODYNAMIC FORCE AND MOMENT COEFFICIENTS
DATA SET FOR STEADY FLOWS OF FULL
CONFIGURATION OF TWO-STAGE SPACE TRANSPORT
SYSTEM
163H AERODYNAMIC FORCE AND MOMENT COEFFICIENTS
OF THE COMPUTATIONAL DATA SET FOR UNSTEADY
FLOWS 164vi
LIST OF FIGURES
FIGURE Page
I.1 Layout of two-stage to orbit (ELAC-EOS) configuration 2 I.2 A flight mission of the two stage space transportation system 2 II.1 Structure of computational aerodynamic simulations 18II.2 Flow Approximation levels
21II.3 Basic geometry of EOS and flat plate
25II.4
Configuration and geometric reference values of
the EOS-ELAC1C two-stage transportation system 26II.5 The trajectory of stage separation of TSTO space vehicle system 27 II.6 The parameters of stage separation of the TSTO space vehicle system 27
II.7 The components of force and moment acting on the space vehicle 29
III.1 Block segmentation
33III.2 Schematic block connection
34III.3 Computational domain for dynamic grids
37IV.1 Farfield boundary conditions
48IV.2 Exchange of flow variables between two blocks A and B 50
IV.3 The flow chart of the unsteady calculation
54V.1 The test model of orbital EOS and flap plate
56V.2 The test model of ELAC1C and EOS
56V.3 The test model of EOS and flap plate for
the Shock Tunnel TH2-D 58 V.4 Pressure measurement sections at x = 0.6L, 0.75L, and y = 0 59V.5 Topology and blocks for the EOS - Flat Plate configuration 61
V.6 Topology and blocks for the EOS - ELAC1C configuration 61
V.7 Points distributions along the edge of the block 62
V.8 The initial generated grid for the standard grid 63
V.9 The smoothed grid of the EOS - flat plate configuration 64
vii V.10 Initially generated mesh for EOS and ELAC1C configuration 64
V.11 The smoothed grids of the EOS and ELAC1C configuration 65
V.12 The effect of grid smoothing on the grid quality 68
V.13 Convergence History for the smoothing grid effects 69
V.14
Mach contours with
for the different smoothed grids at = 0 , h/L EOS = 0.150. 70V.15 Pressure coefficient distribution on the symmetry line of the flat plate 71
V.16 The layout of three different grid density
73V.17 Density contours for the different grid densities. 74
V.18 Pressure coefficient distribution on the symmetry line of the flat plate for three different grid densities 75
V.19 Comparison between experiment and numerical computation at = 0.0, h/l EOS = 0.150 77
V.20 Comparison between experiment and computation at = 0.0, h/l EOS = 0.150. 79
V.21 Pressure coefficient distribution on the symmetry line of the lower surface of the EOS, at = 0.0, h/l EOS = 0.150 80
V.22 Pressure coefficient distribution on the cross section of the lower surface at x/L EOS = 0.6, for = 0.0, h/l EOS = 0.150 81
V.23 Pressure coefficient distribution on the cross section of the lower surface at x/L EOS = 0.75, for = 0.0, h/l EOS = 0.150 82
V.24 Schlieren picture of flow features observed in wind tunnel test for the ELAC1C/EOS configuration at Re m = 48.0x10 6 = 0.0, = 0.0, h/l EOS = 0.225 83
V.25 Density contour for the ELAC1C/EOS configuration at = 0.0, = 0.0, h/l EOS = 0.225 (case b1) 84
V.26 Density contour for the ELAC1C/EOS configuration at Re m = 48.0 x 10quotesdbs_dbs47.pdfusesText_47
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