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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-B5-69-2016</article-id>
<title-group>
<article-title>ACCURACY OF 3D RECONSTRUCTION IN AN ILLUMINATION DOME</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>MacDonald</surname>
<given-names>Lindsay</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>Toschi</surname>
<given-names>Isabella</given-names>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Nocerino</surname>
<given-names>Erica</given-names>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Hess</surname>
<given-names>Mona</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>Remondino</surname>
<given-names>Fabio</given-names>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Robson</surname>
<given-names>Stuart</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 Geomatic Engineering (CEGE), UCL, London, UK</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>3D Optical Metrology (3DOM) unit, Bruno Kessler Foundation (FBK), Trento, Italy</addr-line>
</aff>
<pub-date pub-type="epub">
<day>15</day>
<month>06</month>
<year>2016</year>
</pub-date>
<volume>XLI-B5</volume>
<fpage>69</fpage>
<lpage>76</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2016 Lindsay MacDonald et al.</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-B5/69/2016/isprs-archives-XLI-B5-69-2016.html">This article is available from https://isprs-archives.copernicus.org/articles/XLI-B5/69/2016/isprs-archives-XLI-B5-69-2016.html</self-uri>
<self-uri xlink:href="https://isprs-archives.copernicus.org/articles/XLI-B5/69/2016/isprs-archives-XLI-B5-69-2016.pdf">The full text article is available as a PDF file from https://isprs-archives.copernicus.org/articles/XLI-B5/69/2016/isprs-archives-XLI-B5-69-2016.pdf</self-uri>
<abstract>
<p>The accuracy of 3D surface reconstruction was compared from image sets of a Metric Test Object taken in an illumination dome by
two methods: photometric stereo and improved structure-from-motion (SfM), using point cloud data from a 3D colour laser scanner
as the reference. Metrics included pointwise height differences over the digital elevation model (DEM), and 3D Euclidean differences
between corresponding points. The enhancement of spatial detail was investigated by blending high frequency detail from photometric
normals, after a Poisson surface reconstruction, with low frequency detail from a DEM derived from SfM.</p>
</abstract>
<counts><page-count count="8"/></counts>
</article-meta>
</front>
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