Abstract

Topographic mapping, e.g. the generation of Digital Elevation Models (DEM), is of general interest to the remote sensing community and scientific research. Commonly, photogrammetric methods, e.g. stereo image analysis methods (SIAM) or bundle adjustment methods (BAM), are applied to derive 3D information based on multiple images of an area. These methods require the detection of control points, i.e. common points within multiple images, which relies on a similarity measure and usually yields a sparse map of 3D points. The full spatial DEM is then obtained by interpolation techniques or imposed restrictions, e.g. smoothness constraints. Since BAM utilizes all images of the area, it is assumed to provide a more accurate DEM than SIAM which utilizes only pairs of images. Intensity-based shape recovery, e.g. shape from shading (SfS), utilizes the reflectance behavior of the object surface and thus provides a dense map of relative height changes, which provide the possibility to refine the photogrammetric DEMs. Based on Rosetta NavCam images of 67P/Churyumov-Gerasimenko we compare intensity-based DEM refinement methods which use DEMs obtained based on SIAM and BAM as a reference. We show that both the SIAM based DEM refinement and the BAM based DEM refinement are of similar quality. It is thus possible to derive DEMs of high lateral resolution by applying the intensity-based refinement to the less complex SIAM.

Highlights

  • In 2004, the spacecraft Rosetta was launched by the European Space Agency in order to analyze the comet 67P/ChuryumovGerasimenko (Churyumov, 2005)

  • Based on Rosetta NavCam images of 67P/ChuryumovGerasimenko we compare intensity-based Digital Elevation Models (DEM) refinement methods which use DEMs obtained based on stereo image analysis methods (SIAM) and bundle adjustment methods (BAM) as a reference. We show that both the SIAM based DEM refinement and the BAM based DEM refinement are of similar quality

  • Since both DEMs show “spikes” that originate from false matches, we apply a median filter of width 15 pixels prior to the computation of the reflectancebased surface refinement

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Summary

Introduction

In 2004, the spacecraft Rosetta was launched by the European Space Agency in order to analyze the comet 67P/ChuryumovGerasimenko (Churyumov, 2005). The shape of 67P/Churyumov-Gerasimenko has been analyzed by Sierks and 65 coauthors (2015) based on images of the OSIRIS camera (Keller and 68 coauthors, 2007). Photogrammetric methods, e.g. stereo image analysis methods (SIAM) or bundle adjustment methods (BAM) (McGlone et al, 2004), are applied to derive 3D information based on multiple images of an area. These methods require the detection of control points, i.e. common points within multiple images, which relies on a similarity measure and usually yields a sparse map of 3D points. The DEMs originating from both types of methods, have a lower resolution than the underlying image data (Kirk et al, 2003a; Schenk, 2008; Scholten et al, 2012)

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