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InSAR Stack Processing — Deformation Mapping in the Area of ...

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Chapter 3Methodology3.1 Interferogram creationThe first step <strong>of</strong> <strong>the</strong> process<strong>in</strong>g is <strong>the</strong> <strong>in</strong>terferogram creation. It consists <strong>of</strong> <strong>the</strong> follow<strong>in</strong>g important steps:• coregistration <strong>of</strong> <strong>the</strong> two scenes,• resampl<strong>in</strong>g <strong>of</strong> <strong>the</strong> slave scene <strong>in</strong> order to correspond exactly to <strong>the</strong> master,• subtraction <strong>of</strong> <strong>the</strong> slave phase from <strong>the</strong> master phase (<strong>in</strong>terferogram creation),• subtraction <strong>of</strong> <strong>the</strong> flat-Earth phase (i.e. <strong>the</strong> phase correspond<strong>in</strong>g to <strong>the</strong> Earth surface withouttopography) from <strong>the</strong> <strong>in</strong>terferogram. For <strong>the</strong> flat-Earth phase computation, orbital <strong>in</strong>formation isused.3.2 Topography subtractionA significant component <strong>of</strong> <strong>the</strong> phase <strong>in</strong>formation is <strong>in</strong>fluenced with topography. The coefficient <strong>of</strong>proportionality is <strong>in</strong>fluenced by <strong>the</strong> spatial basel<strong>in</strong>e between <strong>the</strong> two scenes, particularly by <strong>the</strong> componentperpendicular to <strong>the</strong> radar ray (perpendicular basel<strong>in</strong>e).There are two basic methods <strong>of</strong> topography subtraction:• 2-pass method, i.e. us<strong>in</strong>g an external digital elevation model (DEM) as a topography <strong>in</strong>formation.Us<strong>in</strong>g orbital <strong>in</strong>formation, <strong>the</strong> DEM is converted <strong>in</strong>to <strong>the</strong> radar system (i.e. a syn<strong>the</strong>tic <strong>in</strong>terferogramis created) and this is subtracted from <strong>the</strong> real <strong>in</strong>terferogram. GAMMA s<strong>of</strong>tware allowsto create also a syn<strong>the</strong>tic magnitude image to be coregistered with <strong>the</strong> magnitude image from <strong>the</strong>satellite; however, this possibility was not used for <strong>the</strong> processed scene crops. The syn<strong>the</strong>tic magnitudeimage is created from <strong>the</strong> DEM <strong>in</strong>formation only and <strong>the</strong>refore does not conta<strong>in</strong> man-madefeatures, which are most significant <strong>in</strong> <strong>the</strong> satellite magnitude image. Due to this fact <strong>the</strong> coregistration<strong>of</strong> <strong>the</strong> small scene crops fails. However, as proven <strong>in</strong> <strong>the</strong> whole scene process<strong>in</strong>g, <strong>the</strong> orbitsare <strong>in</strong> most cases precise enough such that <strong>the</strong> difference between <strong>the</strong> syn<strong>the</strong>tic and real magnitudeis not higher than one pixel. We use <strong>the</strong> SRTM (Shuttle Radar Topography Mission) DEM, whichis created by <strong>InSAR</strong> method, and <strong>the</strong>refore some properties may be similar.• 3-pass method, i.e. us<strong>in</strong>g a different <strong>in</strong>terferogram for topography subtraction. The phase <strong>of</strong> this<strong>in</strong>terferogram must be unwrapped which may be a problem <strong>in</strong> <strong>in</strong>coherent areas. We decided not touse this method <strong>in</strong> <strong>the</strong> project.13

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