Chapter 5 Robust Performance Tailoring with Tuning - SSL - MIT

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Controls Structure) tools [24]. The model is based largely on one created at the MIT Space Systems Laboratory by D. Lobosco [76] with some updates resulting from communication with the Jet Propulsion Laboratory 1 . A schematic of the integrated model is shown in Figure 6-1. The main model components are the plant, attitude RWA Disturbances (3 wheels) Σ Σ Σ RWA Isolator LPF LPF LPF LPF LPF LPF bus Isolator LPF LPF LPF LPF LPF LPF Fx Fy Fz Tx Ty Tz Figure 6-1: Schematic of TPF SCI Model. PLANT ACS OPD12 OPD13 OPD14 ACS Tx ACS Ty ACS Tz control system, disturbance model and vibration isolation stages. The inputs to the integrated model are reaction wheel assembly (RWA) disturbances, shown at the left- hand side of the figure. The disturbances are combined with torque commands from the attitude control system (ACS) and pass through a two-stage vibration isolation system. The first stage represents an isolator between the RWA and the bus, and the second stage models isolation between the bus and the supporting structure. The isolated disturbances then pass through the plant. This component has the highest fidelity and includes the structural finite element model and optical sensitivities. The structural model consists of four evenly-spaced collectors mounted to a truss with a triangular cross-section as shown in Figure 6-2. The plant has six outputs, three 1personal communication with Douglas Adams, Member of Technical Staff, Jet Propulsion Laboratory 182
optical path differences between the collector pairs and three angular torque mea- surements from the bus that drive the ACS. Since the ACS commands are fed back to the plant torque inputs, the only outputs of the integrated model are the three optical performance metrics. The model components are described in detail in the following sections. (a) (b) (c) (d) Figure 6-2: Nominal SCI TPF plant finite element model (a) Isometric view (b) top view(XY)(c)sideview(ZY)(d)frontview(XZ). 6.1.1 Reaction Wheel Assembly Disturbances The inputs to the integrated model are the disturbances. The are many possible sources of disturbances that may impinge on a spacecraft such as TPF. Some are functions of the environment, such as gravity gradients and solar torque. Other disturbances are from on-board mechanisms such as fast-steering mirrors or thrusters. Vibrations from the reaction wheel assembly (RWA) are anticipated to be the dom- 183
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Dynamic Tailoring and Tuning for Sp
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Acknowledgments This work was suppo
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3.2 RPT Formulation . . . . . . . .
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List of Figures 1-1 Timeline of Ori
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List of Tables 1.1 Effect of simula
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Nomenclature Abbreviations ACS atti
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dk optimization search direction f
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1.1 Space-Based Interferometry NASA
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unfettered by the Earth’s atmosph
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the SCI, both the size and flexibil
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maybethatitbecomescertain that the
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Table 1.1: Effect of simulation res
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Table 1.2: Effect of simulation res
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has been found that structural desi
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precision telescope structure for m
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attractive, and more conservative a
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to solve the performance tailoring
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Chapter 2 Performance Tailoring A c
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ometer (SCI). In the following sect
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The equations of motion of the unda
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The frequency response functions fr
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the output covariance matrix, Σz,
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where the subscript indicates the i
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2.3.3 Design Variables The choice o
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and then, by inspection, the inerti
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algorithms begin at an initial gues
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at least locally optimal, and the s
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initial design variable state, x =
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and the RMS OPD is computed using E
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# Designs 25 20 15 10 5 Accepted, b
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does not provide information on why
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energy is distributed almost evenly
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also symmetric as seen in the figur
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Chapter 3 Robust Performance Tailor
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through careful and experienced mod
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described above. However, one can r
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ic, σz(�x, �p), that is depend
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Magnitude, OPD/F x [µm/N] Magnitud
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% Energy 100 90 80 70 60 50 40 30 2
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metric to the cost function. Note,
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tion: ∂hi (z,�x, �pi) ∂�x
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values are chosen from their statis
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Table 3.3: Algorithm performance: a
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Statistical Robustness The statisti
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Performance [µm] 1400 1200 1000 80
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(Figure 3-6(b)). The nominal perfor
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Norm. Cum. Var. [µm 2 ] PSD [µm 2
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energy by mode for easy comparison.
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Y−coordinate [m] Y−coordinate [
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RMS performance, [µm] 400 350 300
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The requirement chosen here is some
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Chapter 4 Dynamic Tuning Robust Per
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on a physical truss. Since tailorin
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Table 4.1: Tuning parameters for SC
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m 2 [kg] J ∗ # # time y ∗ [kg]
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m 2 [kg] 800 700 600 500 400 300 20
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configuration than the untuned, but
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Norm. Cum. Var. [µm 2 ] PSD [µm 2
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Performance Requirement [µm] 400 3
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is considered. 4.2.1 Hardware-only
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and added to the objective function
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using either a decreasing step-size
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for tailoring, but tuning parameter
Page 131 and 132: tained by randomly choosing paramet
Page 133 and 134: p [GPa] y ∗ [kg] Performance [µm
Page 135 and 136: # Func. Evals Performance RMS (µm)
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Page 139 and 140: Data: initial iterate, p0, performa
Page 141 and 142: the new tuning configuration is ver
Page 143 and 144: Performing an AO tuning optimizatio
Page 145 and 146: Uncertainty Bounds Test �y [kg] S
Page 147 and 148: Table 4.6: Tuning results on fifty
Page 149 and 150: eters are discussed. The optimizati
Page 151 and 152: Chapter 5 Robust Performance Tailor
Page 153 and 154: MPC optimization by allowing a diff
Page 155 and 156: where the notation yij indicates th
Page 157 and 158: (Table 4.1), and the uncertainty pa
Page 159 and 160: Table 5.2: Performance and design p
Page 161 and 162: it in the worst-case uncertainty re
Page 163 and 164: The data in Figure 5-2 indicate tha
Page 165 and 166: configuration. The tuned configurat
Page 167 and 168: same requirement. The effect become
Page 169 and 170: indicating that this requirement is
Page 171 and 172: E 2 [Pa] 7.8 7.6 7.4 7.2 7 6.8 6.6
Page 173 and 174: than the RPT design, 155.45µm to 5
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Page 177 and 178: of these simulations fail to meet r
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Page 181: Chapter 6 Focus Application: Struct
Page 185 and 186: Table 6.1: RWA disturbance model pa
Page 187 and 188: FRF Magnitude 10 1 10 0 10 −1 10
Page 189 and 190: Y Z Z X Y (a) w (c) w Y h Z Figure
Page 191 and 192: Table 6.6: Primary mirror propertie
Page 193 and 194: OP1 STAR Z OP2 OP3 Coll 1 Coll 2 Bu
Page 195 and 196: PSD OPD14 [m 2 /Hz] CumulativeOPD14
Page 197 and 198: 6.2 Design Parameters In order to a
Page 199 and 200: 6.2.2 Tuning The tuning parameters
Page 201 and 202: complex and the normal modes analys
Page 203 and 204: does not change with the design par
Page 205 and 206: (a) (b) (c) Figure 6-11: SCI TPF PT
Page 207 and 208: Table 6.14: Performance predictions
Page 209 and 210: performance trends similar to those
Page 211 and 212: Chapter 7 Conclusions and Recommend
Page 213 and 214: a statistical robustness measure su
Page 215 and 216: and the worst-case performance is a
Page 217 and 218: - Consider uncertainty analysis too
Page 219 and 220: Appendix A Gradient-Based Optimizat
Page 221 and 222: such that the gradient direction is
Page 223 and 224: the descent direction. In some case
Page 225 and 226: Bibliography [1] Jpl planet quest w
Page 227 and 228: [24] Nightsky Systems Carl Blaurock
Page 229 and 230: [48] S. C. O. Grocott, J. P. How, a
Page 231 and 232: [74] M. Lieber. Development of ball
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AIAA/ASME/ASCE/AHS/ASC Structures,
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