Chapter 5 Robust Performance Tailoring with Tuning - SSL - MIT

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x,y,p Build NASTRAN model [MATLAB] Mirrors.bdf + Model_Cbars_19TraiBays.bdf docs_acs.m [DOCS/MATLAB] RWADist.mat DIST ACS Model.bdf run NASTRAN Read modal data into MATLAB [Perl] replace/remove rigid body modes [MATLAB] Generate DOCS model [DOCS/MATLAB] PLANT Integrate model components [DOCS] SYS(x,y,p) ISO y Generate isolator model [DOCS/MATLAB] Figure 6-10: Implementation flow for generating integrated TPF model. 202
does not change with the design parameters, so it is generated a priori and then loaded into the workspace at each iteration. The model components are integrated with DOCS to form the fully-integrated system model and evaluate the performance. It is important to keep in mind that the process outlined in Figure 6-10 is exe- cuted once for each iteration, or random guess, in the SA algorithm. Therefore, the NASTRAN model must be built and a finite element analysis run thousands of times. This operation is computationally expensive and becomes more so as the model fidelity and number of degrees of freedom are increased. In addition, as the design space grows, a greater number of SA iterations are required. It is clear that a brute force method such as the one outlined here may not be appropriate for a model of this fidelity and further investigation into the optimization implementation is war- ranted. There are known methods for reducing the computational effort required for these types of optimizations [28, 39] that are appropriate for this application, such as reduced-order modeling [37] and response surface approximation [22, 11]. 6.4 Results The TPF SCI structure is designed through a SA stochastic search using the PT, RPT and RPTT cost functions (Equations 2.1, 3.5, and 5.5, respectively). In the RPT and RPTT optimizations the uncertainty space is searched with the vertex method. Since there are three uncertainty parameters, there are eight vertices at which performance must be evaluated during each iteration. The RPTT cost is considered with α =0 to obtain the most tunable design. In the PT and RPT optimizations both the tailoring, �x and tuning, �y parameters are used as tailoring parameters to provide for a fair comparison with the RPTT design. In this way all three optimizations have the same design variables available to them and the only difference lies in the manner in which the tuning parameters are incorporated. The tailoring parameters for the nominal and optimized designs are listed in Ta- ble 6.13 along with the mass of the structures. The three designs are distinct from each other and very different from the nominal design. In each case the truss bays 203
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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
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tained by randomly choosing paramet
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p [GPa] y ∗ [kg] Performance [µm
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# Func. Evals Performance RMS (µm)
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tion changes in the updated solutio
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Data: initial iterate, p0, performa
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the new tuning configuration is ver
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Performing an AO tuning optimizatio
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Uncertainty Bounds Test �y [kg] S
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Table 4.6: Tuning results on fifty
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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
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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
Page 175 and 176: have a very small nominal performan
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Page 181 and 182: Chapter 6 Focus Application: Struct
Page 183 and 184: optical path differences between th
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: complex and the normal modes analys
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
Page 233 and 234: AIAA/ASME/ASCE/AHS/ASC Structures,
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