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EG 2011 | Computational Plenoptic Imaging STAR | I. Introduction1 Computational Plenoptic Imaging Gordon Wetzstein 1 Ivo Ihrke 2 Douglas Lanman 3 Wolfgang.

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Presentation on theme: "EG 2011 | Computational Plenoptic Imaging STAR | I. Introduction1 Computational Plenoptic Imaging Gordon Wetzstein 1 Ivo Ihrke 2 Douglas Lanman 3 Wolfgang."— Presentation transcript:

1 EG 2011 | Computational Plenoptic Imaging STAR | I. Introduction1 Computational Plenoptic Imaging Gordon Wetzstein 1 Ivo Ihrke 2 Douglas Lanman 3 Wolfgang Heidrich 1 1 University of British Columbia 2 Saarland University 3 MIT Media Lab Eurographics 2011 – State of the Art Report I. Introduction

2 EG 2011 | Computational Plenoptic Imaging STAR | I. Introduction2 The Mantis Shrimp 3 bands = trinocular vision with each eye! Up to 16 different photoreceptors: 12 for color (4 UV, visible, IR) 4 for polarization (linear & circular)

3 EG 2011 | Computational Plenoptic Imaging STAR | I. Introduction3 Cameras are modeled as one Human Eye http://en.wikipedia.org/wiki/Bayer_filter webvision.med.utah.edu [Williams 91] How would a camera look like if it was modeled as a mantis shrimp eye?

4 EG 2011 | Computational Plenoptic Imaging STAR | I. Introduction4 The Plenoptic Function Ray-based model for light Includes variations in space, time, wavelength, and directions [Adelson & Bergen 91] More common angular parameterization Light field is

5 EG 2011 | Computational Plenoptic Imaging STAR | I. Introduction5 Plenoptic Information Sampled Allan Brooks, EE421, 2003 HVS Consumer Video Camera 1 continuous, ~30fps (band-limited) 3, Bayer color filter array 1920x1080 (HD) 4 Plenoptic Parameters Sampled (no V x,y,z )

6 EG 2011 | Computational Plenoptic Imaging STAR | I. Introduction6 Computational Photography and Plenoptic Imaging CPI: joint optical modulation & computational processing of plenoptic dimensions CP: computational optics, illumination, probes, reconstruction, image processing, sensors, etc. [Raskar & Tumblin]

7 EG 2011 | Computational Plenoptic Imaging STAR | I. Introduction7 Taxonomy and Overview II. High Dynamic Range Imaging – 10 minutes, Wetzstein III. Spectral Imaging – 10 minutes, Wetzstein IV. Light Field Acquisition – 25 minutes, Lanman V. Space & Focal Surfaces – 15 minutes, Wetzstein VI. Temporal Multiplexing – 10 minutes, Wetzstein VII. Further Light Properties – 10 minutes, Wetzstein VIII. Discussion – 5 minutes, Wetzstein

8 EG 2011 | Computational Plenoptic Imaging STAR | I. Introduction8 Next: High Dynamic Range Imaging


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