Beyond Brightness Constancy: Learning Noise Models for Optical Flow

TL;DR

This paper introduces a learned noise model for optical flow that outperforms traditional brightness constancy assumptions by explicitly modeling warp error patches with a GMM, leading to improved flow estimation.

Contribution

It proposes a generative approach to learn a data cost using GMMs for warp error patches, capturing spatial structure and improving optical flow accuracy.

Findings

GMM-based warp error modeling outperforms traditional constancy assumptions.

Using expected patch log-likelihood improves optical flow estimation.

Iterative optimization with denoising enhances flow accuracy.

Abstract

Optical flow is typically estimated by minimizing a "data cost" and an optional regularizer. While there has been much work on different regularizers many modern algorithms still use a data cost that is not very different from the ones used over 30 years ago: a robust version of brightness constancy or gradient constancy. In this paper we leverage the recent availability of ground-truth optical flow databases in order to learn a data cost. Specifically we take a generative approach in which the data cost models the distribution of noise after warping an image according to the flow and we measure the "goodness" of a data cost by how well it matches the true distribution of flow warp error. Consistent with current practice, we find that robust versions of gradient constancy are better models than simple brightness constancy but a learned GMM that models the density of patches of warp error gives a much better fit than any existing assumption of constancy. This significant advantage of the GMM is due to an explicit modeling of the spatial structure of warp errors, a feature which is missing from almost all existing data costs in optical flow. Finally, we show how a good density model of warp error patches can be used for optical flow estimation on whole images. We replace the data cost by the expected patch log-likelihood (EPLL), and show how this cost can be optimized iteratively using an additional step of denoising the warp error image. The results of our experiments are promising and show that patch models with higher likelihood lead to better optical flow estimation.