Near-light Photometric Stereo with Symmetric Lights
Organizations: Graduate School of Information Science and Technology, Osaka University, Japan.
Abstract
This paper describes a linear solution method for near-light photometric stereo by exploiting symmetric light source arrangements. Unlike conventional non-convex optimization approaches, by arranging multiple sets of symmetric nearby light source pairs, our method derives a closed-form solution for surface normal and depth without requiring initialization. In addition, our method works as long as the light sources are symmetrically distributed about an arbitrary point even when the entire spatial offset is uncalibrated. Experiments showcase the accuracy of shape recovery accuracy of our method, achieving comparable results to the state-of-the-art calibrated near-light photometric stereo method while significantly reducing requirements of careful depth initialization and light calibration.
Figures & tables
| Light model | Method | Light calibration | Light arrangement | Optimization | Additional requirements |
| Distant | [ 1 ] | Calibrated | N.A | Convex | N.A |
| [ 2 ] | Partially calibrated | Axis-aligned symmetric | Convex | Constant albedo | |
| [ 3 ] , [ 4 , 5 ] | Partially calibrated | Ring | Convex | Integrability | |
| [ 6 ] | Uncalibrated | N.A. | Convex | Integrability, diffuse maxima detection | |
| Near | [ 7 ] , [ 8 , 9 , 10 ] | Calibrated | N.A | Non-convex | Depth initialization |
| [ 11 ] | Calibrated | Ring | Non-convex | Depth initialization |
Surface Normal Estimation
Surface Normal Estimation recovers the orientation of visible 3D surfaces from images and other sensor data for shape understanding and reconstruction.
See all 26 papers