The phase noise can be computed from the InSAR pair with the help of the local coherence γ.
The γ is the cross- correlation coefcient of the InSAR pair computed on a moving window of few
pixels in range and azimuth, after all the deterministic phase components due to the terrain eleva-
tion are corrected. As a rst approximation, the deterministic phase components in a small window
are linear, in both slant- range and azimuth direction. This can be estimated from the interferogram
using the frequency detection of complex sinusoids in noise. The coherence image of the data is
then generated by calculating the absolute value of γ on ...
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