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<front>
<journal-meta>
<journal-id journal-id-type="publisher">ISPRS-Archives</journal-id>
<journal-title-group>
<journal-title>The International Archives of the Photogrammetry, Remote Sensing and Spatial Information Sciences</journal-title>
<abbrev-journal-title abbrev-type="publisher">ISPRS-Archives</abbrev-journal-title>
<abbrev-journal-title abbrev-type="nlm-ta">Int. Arch. Photogramm. Remote Sens. Spatial Inf. Sci.</abbrev-journal-title>
</journal-title-group>
<issn pub-type="epub">2194-9034</issn>
<publisher><publisher-name>Copernicus Publications</publisher-name>
<publisher-loc>Göttingen, Germany</publisher-loc>
</publisher>
</journal-meta>
<article-meta>
<article-id pub-id-type="doi">10.5194/isprs-archives-XLI-B3-137-2016</article-id>
<title-group>
<article-title>STRUCTURED LIGHT BASED 3D SCANNING FOR SPECULAR SURFACE BY THE COMBINATION OF GRAY CODE AND PHASE SHIFTING</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Zhang</surname>
<given-names>Yujia</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Yilmaz</surname>
<given-names>Alper</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Dept. of Civil, Environmental and Geodetic Engineering, The Ohio State University 2036 Neil Avenue, Columbus, OH 43210, USA</addr-line>
</aff>
<pub-date pub-type="epub">
<day>09</day>
<month>06</month>
<year>2016</year>
</pub-date>
<volume>XLI-B3</volume>
<fpage>137</fpage>
<lpage>142</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2016 Yujia Zhang</copyright-statement>
<copyright-year>2016</copyright-year>
<license license-type="open-access">
<license-p>This work is licensed under the Creative Commons Attribution 3.0 Unported License. To view a copy of this licence, visit <ext-link ext-link-type="uri"  xlink:href="https://creativecommons.org/licenses/by/3.0/">https://creativecommons.org/licenses/by/3.0/</ext-link></license-p>
</license>
</permissions>
<self-uri xlink:href="https://isprs-archives.copernicus.org/articles/XLI-B3/137/2016/isprs-archives-XLI-B3-137-2016.html">This article is available from https://isprs-archives.copernicus.org/articles/XLI-B3/137/2016/isprs-archives-XLI-B3-137-2016.html</self-uri>
<self-uri xlink:href="https://isprs-archives.copernicus.org/articles/XLI-B3/137/2016/isprs-archives-XLI-B3-137-2016.pdf">The full text article is available as a PDF file from https://isprs-archives.copernicus.org/articles/XLI-B3/137/2016/isprs-archives-XLI-B3-137-2016.pdf</self-uri>
<abstract>
<p>Surface reconstruction using coded structured light is considered one of the most reliable techniques for high-quality 3D scanning. With
a calibrated projector-camera stereo system, a light pattern is projected onto the scene and imaged by the camera. Correspondences
between projected and recovered patterns are computed in the decoding process, which is used to generate 3D point cloud of the surface.
However, the indirect illumination effects on the surface, such as subsurface scattering and interreflections, will raise the difficulties in
reconstruction. In this paper, we apply maximum min-SW gray code to reduce the indirect illumination effects of the specular surface.
We also analysis the errors when comparing the maximum min-SW gray code and the conventional gray code, which justifies that
the maximum min-SW gray code has significant superiority to reduce the indirect illumination effects. To achieve sub-pixel accuracy,
we project high frequency sinusoidal patterns onto the scene simultaneously. But for specular surface, the high frequency patterns are
susceptible to decoding errors. Incorrect decoding of high frequency patterns will result in a loss of depth resolution. Our method to
resolve this problem is combining the low frequency maximum min-SW gray code and the high frequency phase shifting code, which
achieves dense 3D reconstruction for specular surface. Our contributions include: (i) A complete setup of the structured light based 3D
scanning system; (ii) A novel combination technique of the maximum min-SW gray code and phase shifting code. First, phase shifting
decoding with sub-pixel accuracy. Then, the maximum min-SW gray code is used to resolve the ambiguity resolution. According to
the experimental results and data analysis, our structured light based 3D scanning system enables high quality dense reconstruction of
scenes with a small number of images. Qualitative and quantitative comparisons are performed to extract the advantages of our new
combined coding method.</p>
</abstract>
<counts><page-count count="6"/></counts>
</article-meta>
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