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Near-light Photometric Stereo with Symmetric Lights

arXiv cs.CV / 3/18/2026

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Key Points

  • The paper describes a linear, closed-form solution for near-light photometric stereo that uses symmetric light source pairs, avoiding non-convex optimization and initialization.
  • The method works with symmetric light distributions around an arbitrary point and does not require calibrated spatial offsets.
  • Experiments show surface normal and depth recovery with accuracy comparable to calibrated near-light photometric stereo methods while reducing depth initialization and light calibration requirements.
  • The approach enables simpler hardware setups for near-light photometric stereo and could speed up shape recovery in practical imaging systems.

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.