Title | ||
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Use of scaling information for stochastic atmospheric absolute phase screen retrieval |
Abstract | ||
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Scaling information is an important tool for the description of natural processes. Many applications of SAR (differential) interferometry lead to a set of sparse phase measurements, e.g. the monitoring of permanent scatterers. In this case, the atmospheric phase screen component of a given SAR image can be estimated over the PS sparse grid. Usually such data have to be unwrapped and then interpolated on a regular grid. We investigate the utility of the scaling information, valid for atmospheric phase screen data, in the process of unwrapping a set of sparse measurements. We show how the power-law behaviour of the data variogram can be used as an a priori constraint for optimization through techniques such as simulated annealing. The results are interpreted in view of operational applications to real data. |
Year | DOI | Venue |
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2002 | 10.1109/IGARSS.2002.1026235 | IGARSS |
Keywords | Field | DocType |
geophysical techniques,radar theory,remote sensing by radar,synthetic aperture radar,terrain mapping,insar,ps sparse grid,sar,sar image,sar interferometry,atmospheric phase screen,geophysical measurement technique,land surface,permanent scatterers,radar remote sensing,scaling data,sparse phase measurements,stochastic atmospheric absolute phase screen retrieval,unwrapped,unwrapping,interferometry,simulated annealing,atmospheric modeling,information retrieval,sparse grids,power law,scattering,constraint optimization,stochastic processes | Simulated annealing,Absolute phase,Computer vision,Regular grid,Computer science,Synthetic aperture radar,Remote sensing,Feature scaling,Artificial intelligence,Sparse grid,Scaling,Constrained optimization | Conference |
Volume | Citations | PageRank |
3 | 0 | 0.34 |
References | Authors | |
2 | 4 |
Name | Order | Citations | PageRank |
---|---|---|---|
Alberto Refice | 1 | 46 | 12.80 |
Fabio Bovenga | 2 | 70 | 19.41 |
Sebastiano Stramaglia | 3 | 169 | 18.42 |
Domenico Conte | 4 | 2 | 1.66 |