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  4. Persistent scatterer pair interferometry: Approach and application to COSMO-skymed SAR data
 
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Persistent scatterer pair interferometry: Approach and application to COSMO-skymed SAR data

Author(s)
Costantini, M.
Falco, S.
Malvarosa, F.
Minati, F.
Trillo, F.
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Date Issued
2014
Publisher
Institute of Electrical and Electronics Engineers
Abstract
Persistent scatterer interferometry is a widely used technique to detect and monitor slow terrain movements, with millimetric accuracy, from satellite synthetic aperture radar (SAR) data. We have recently proposed a method, named persistent scatterer pair (PSP), aimed at overcoming some limitations of standard techniques. The PSP method is characterized by the fact of exploiting only the relative properties of neighboring pairs of points for both detection and analysis of persistent scatterers (PSs), intended in the general sense of scatterers that exhibit interferometric coherence for the time period and baseline span of the acquisitions, including both point-like and distributed scatterers. Thanks to the pair-of-point approach, the PSP technique is intrinsically not affected by artifacts slowly variable in space, like those depending on atmosphere or orbits. Moreover, by exploiting a very redundant set of pair-of-point connections, the PSP approach guarantees extremely dense and accurate displacement and elevation measurements, both in correspondence of structures and when the backscattering is weak or distributed as in the case of natural terrains. In all cases, the measurements keep the full resolution of the input SAR images. In this work, the qualifying characteristics of the PSP technique are described, and several application examples and validation tests based on COSMO-SkyMed data are reported, which demonstrate the validity of the proposed approach. © 2014 IEEE.
URI
https://hdl.handle.net/20.500.13025/5907
Journal
IEEE Journal of Selected Topics in Applied Earth Observations and Remote Sensing
Issue
7, July 2014
Volume
7
Start Page
2869
Start Page
2879
DOI
10.1109/JSTARS.2014.2343915
URL
https://ieeexplore.ieee.org/document/6881816
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