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Reconstruction with Adaptive Feature-Specific Imaging Jun Ke 1 and Mark A. Neifeld 1,2 1 Department of Electrical and Computer Engineering, 2 College of Optical Sciences University of Arizona Frontiers in Optics 2007
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Outline Frontiers in Optics 2007 Motivation for FSI and adaptation. Adaptive FSI using PCA/Hadamard features. Adaptive FSI in noise. Conclusion.
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Motivation - FSI Reconstruction with Feature-specific Imaging (FSI) : Frontiers in Optics 2007 FSI benefits: Lower hardware complexity Smaller equipment size/weight Higher measurement SNR High data acquisition rate Lower operation bandwidth Less power consumption Sequential architecture: Parallel architecture: LCD G (NxM) Reconstruction matrix G (NxM) object object reconstruction DMD Imaging optics light collection single detector feature projection vector
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Motivation - Adaptation Frontiers in Optics 2007 Acquire feature measurements sequentially Use acquired feature measurements and training data to adapt the next projection vector The design of projection vector effects reconstruction quality. Using Principal Component Analysis (PCA) projection as example Testing sample Training samples Projection axis 2 Static PCA Projection axis 1 Reconstruction Adaptive PCA Projection axis 2 Projection value Training samples for 2 nd projection vector Projection axis 1 Reconstruction
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Frontiers in Optics 2007 Object estimate y i = f i T x Calculate f i+1 Reconstruction Object x Update A i to A i+1 according to y i Computational Optics Calculate f 1 R i+1 Calculate R 1 from A 1 Adaptive FSI (AFSI) – PCA: i: adaptive step index A i : i th training set K (i) : # of samples for A i+1 High diversity of training data helps adaptation PCA-Based AFSI Testing sample K (1) nearest samples Projection axis Testing sample K (1) nearest samples Selected samples According to 1 st feature According to 2 nd feature K (2) nearest samples Projection axis 2 Projection axis 1 R i : autocorrelation matrix of A i f i : dominate eigenvector of A i y i : feature value measured by f i
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Object examples (32x32): Reconstructed object: RMSE: Feature measurements: where, is the total # of features PCA-Based AFSI Frontiers in Optics 2007 Number of training objects: 100,000 Number of testing objects: 60
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RMSE reduces using more features RMSE reduces using AFSI compare to static FSI Improvement is larger for high diversity data RMSE improvement is 33% and 16% for high and low diversity training data, when M = 250. Frontiers in Optics 2007 AFSI – PCA: PCA-Based AFSI K (i) decreases iteration index i Reconstruction from static FSI (i = 100) Reconstruction from AFSI (i = 100)
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Projection vector’s implementation order is adapted. Frontiers in Optics 2007 AFSI – Hadamard: Hadamard-Based AFSI Selected samples K (1) nearest samples testing sample projection axis 1 K (1) nearest samples testing sample projection axis 2 K (2) nearest samples sample mean First 5 Hadamard basis ←Static FSI AFSI→ according to 1st feature according to 2nd feature sample mean projection axis 1 Sample mean for training set A i is y j = f i T j = 1,…,M max{y j } corresponds to the dominant Hadamard projection vector
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L : # of features in each adaptive step Frontiers in Optics 2007 : sample mean of A i f i : i th Hadamard vector for A i AFSI – Hadamard: Hadamard-Based AFSI K (1) nearest samples testing sample projection axis 1 sample mean projection axis 2 Selected samples according to 1st 2 features Object estimate y iL+j = f iL+j T x (j=1,…,L) Choose f iL+1 ~ f (i+1)L Reconstruction Object x Update A i to A i+1 according to y iL+j Computational Optics Choose f 1 ~f L <Ai><Ai> Sort Sort Hadamard basis vectors
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RMSE reduces in AFSI compared with static FSI RMSE improvement is 32% and 18% for high and low diversity training data, when M = 500 and L = 10. AFSI has smaller RMSE using small L when M is also small AFSI has smaller RMSE using large L when M is also large Hadamard-Based AFSI Frontiers in Optics 2007 AFSI – Hadamard: K (i) decreases number of features M = Li L decreases L increases number of features M = Li Reconstruction from adaptive FSI Reconstruction from static FSI
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Hadamard-Based AFSI – Noise Frontiers in Optics 2007 AFSI – Hadamard: Hadmard projection is used because of its good reconstruction performance Feature measurements are de-noised before used in adaptation Wiener operator is used for object reconstruction Auto-correlation matrix is updated in each adaptation step T : integration time σ 0 2 = 1 detector noise variance: σ 2 2 = σ 0 2 /T Object estimate y iL+j = f iL+j T x+n iL+j (j = 1,2,…L) Choose f iL+1 ~f (i+1)L Reconstruction Object x Update A i to A i+1 according to Computational Optics Choose f 1 ~f L from de- noising y iL+j Calculate R i for A i Sort Hadamard bases Sort
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Frontiers in Optics 2007 RMSE in AFSI is smaller than in static FSI RMSE is reduced further by modifying R x in each adaptation step RMSE improvement is larger using small L when M is also small RMSE is small using large L when M is also large Hadamard-Based AFSI – Noise High diversity training data; σ 0 2 = 1 K (i) decreases L decreases L increases High diversity training data; σ 0 2 = 1 AFSI – fixed R x AFSI – adapted R x Static FSI
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T : integration time/per feature; M 0 : the number of features Total feature collection time = T × M 0 Reducing Measurement error Losing adaptation advantage Hadamard-Based AFSI – Noise Frontiers in Optics 2007 High diversity training data; σ 0 2 = 1 Minimum total feature collection time Increasing T Trade-off
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Conclusion Frontiers in Optics 2007 Noise free measurements: PCA-based and Hadmard-based AFSI system are presented AFSI system presents lower RMSE than static FSI system Noisy measurements: Hadamard-based AFSI system in noise is presented AFSI system presents smaller RMSE than static FSI system There is a minimum total feature collection time to achieve a reconstruction quality requirement
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