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- W2103341738 abstract "Recently, the sparsity model has been applied to photometric stereo by modeling non-Lambertian artifacts as sparse components. As one of these efforts, we present l <sub xmlns:mml=http://www.w3.org/1998/Math/MathML xmlns:xlink=http://www.w3.org/1999/xlink>1</sub> -based photometric stereo for the non-Lambertian corruptions. A solution method was derived using the Augmented Lagrange Multiplier (ALM) method, which effectively solves the constrained problem by solving the sub-problems for surface normal and sparse corruptions iteratively. Experiments demonstrate the applicability of our method by comparing with the Least Square method and the l <sub xmlns:mml=http://www.w3.org/1998/Math/MathML xmlns:xlink=http://www.w3.org/1999/xlink>1</sub> baseline method." @default.
- W2103341738 created "2016-06-24" @default.
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- W2103341738 date "2013-10-01" @default.
- W2103341738 modified "2023-09-24" @default.
- W2103341738 title "L<inf>1</inf>-based photometric stereo via augmented lagrange multiplier method" @default.
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- W2103341738 doi "https://doi.org/10.1109/urai.2013.6677405" @default.
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