1. Introduction

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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

I. Introduction

Eurographics 2011 – State of the Art Report

EG 2011 | Computational Plenoptic Imaging STAR | I. Introduction 1

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)

EG 2011 | Computational Plenoptic Imaging STAR | I. Introduction 2

Cameras are modeled as one Human Eye webvision.med.utah.edu

How would a camera look like if it was modeled as a mantis shrimp eye?

[Williams 91] http://en.wikipedia.org/wiki/Bayer_filter

EG 2011 | Computational Plenoptic Imaging STAR | I. Introduction 3

The Plenoptic Function

• Ray-based model for light

• Includes variations in space, time, wavelength, and directions

• Light field is

P

P

   t V V V x y z

)

P

P

 

, x y

)

V y

V x

More common angular parameterization

EG 2011 | Computational Plenoptic Imaging STAR | I. Introduction

[Adelson & Bergen 91]

4

Plenoptic Information Sampled

HVS

Consumer

Video Camera

4 Plenoptic Parameters

Sampled (no V x,y,z

)

1920x1080 (HD)

3, Bayer color filter array continuous, ~30fps

(band-limited)

1

Allan Brooks, EE421, 2003

EG 2011 | Computational Plenoptic Imaging STAR | I. Introduction 5

Computational Photography and Plenoptic Imaging

• CPI: joint optical modulation & computational processing of plenoptic dimensions

• CP: computational optics, illumination, probes, reconstruction, image processing, sensors, etc.

EG 2011 | Computational Plenoptic Imaging STAR | I. Introduction 6

Taxonomy and Overview

II.

III.

High Dynamic Range Imaging

Spectral Imaging

– 10 minutes, Wetzstein

– 10 minutes, Wetzstein

– 25 minutes, Lanman IV. Light Field Acquisition

V. Space & Focal Surfaces

VI. Temporal Multiplexing

– 15 minutes, Wetzstein

– 10 minutes, Wetzstein

VII. Further Light Properties

VIII. Discussion

EG 2011 | Computational Plenoptic Imaging STAR | I. Introduction

– 10 minutes, Wetzstein

– 5 minutes, Wetzstein

7

Next: High Dynamic Range Imaging

EG 2011 | Computational Plenoptic Imaging STAR | I. Introduction 8

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