Help Content > Interferometry Module > Clustered Processes

Purpose

Single-date and multi-temporal features based on first order statistics Intensity image(s) or interferometric image pairs can be derived from SAR data. These features enable, depending upon the targeted product, to detect and extract structures or temporal changes, which can be additionally used for segmentation and/or classification purposes. This process will exploit the capabilities of SARscape cluster (if enabled and licensed). As a function of cluster nodes, the full area is splitted in more subareas and each subarea is processed. A mosaiced final result is obtained.

Technical Note

Given two coregistered complex SAR images (S1 and S2), one calculates the interferometric coherence (γ) as a ratio between coherent and incoherent summations. Note that the observed coherence - which ranges between 0 and 1 - is, in primis, a function of systemic spatial de-correlation, the additive noise, and the scene de-correlation that takes place between the two acquisitions.

The estimated coherence - which ranges between 0 and 1 - is function of:

-	Systemic spatial de-correlation (i.e. the additive noise).

-	Temporal de-correlation between master and slave acquisitions.

The coherence product has essentially a twofold purpose:

-	To determine the quality of the measurement (i.e. interferometric phase). As a rule of thumb, InSAR pairs with low coherence should not be used to derive reliable phase related measurements.

-	To extract thematic information relevant to the ground features properties and their temporal changes. This information is enhanced when coupled with the backscattering coefficient (σo) of the master and slave Intensity data.

As a general rule it can be assumed that the coherence decreases with increasing master-slave acquisition time distance. The relationship between the coherence (γ) and the Signal to Noise Ratio (SNR) is:

SNR = γ2/1-γ2

In case the two images are very much different in terms of areal coverage, the smallest one should be used as "Input Master file" in order to avoid the coregistration windows to be located in areas with null pixel values, which can eventually cause the coregistration process to fail. For details about the coregistration process, refer to the relevant Technical Note.

In case of baseline conditions - or topographic conditions - which cause the coherence to get lost due to the very fast change of the interferometric phase, it is suggested to over sample the range pixel size by entering negative values in the Range Multilooking (Preferences>Interferometry>Multilooking). As an example using ERS-ASAR interferometric tandem pairs, which are characterized by a very small ambiguity height (hence very dense/frequent interferometric fringes), the Interferometric multilooking factors shall be set to -2 and 3 (respectively in Range and Azimuth).

The use of the Digital Elevation Model in input (optional) enables to generate the coherence image using the interferogram flattened on the basis of the known topography.

In case of inaccuracy in the satellite orbits or in the Digital Elevation Model geolocation, a Ground Control Point (i.e. "GCP" file) is required to correct the SAR data (i.e. "Input Master SLC" file) with respect to the reference Digital Elevation Model. In this case the shift calculated in the coregistration process is combined with the Ground Control Point shift in order to correct the data of the Input file list according to the Input reference file.

It is important to note that:

❖the master file should be the image characterized by the higher spatial resolution (as a consequence of the higher incidence angle)

❖In case the "Input Master SLC file" has already been corrected with the manual or the automatic procedure the GCP is not needed.

❖In case the "Input Master SLC file" is correct (i.e. the nominally geocoded image fits with the DEM), while the orbital parameters of the "Input Slave SLC file" are not accurate (i.e. the nominally geocoded image does not fit with the DEM), the GCP is not needed but the flag "Automatic Slave Orbit Correction", in the Preferences>Flattening, must be checked.

The coherence image can be generated from the input unfiltered interferogram or from the filtered one, using one of the available filtering methods. The selected option can be specified in the relevant Preferences.

Cluster:

The processing for the geocoded coherence map generation is divided among different machines: by splitting the input pair into smaller parts accordingly with the cluster node number in case of Stripmap data or sending the ScanSAR/TOPSAR bursts to the cluster nodes directly. Each node will perform the coregistration, the interferogram generation and flattening the coherence generation and the geocoding. The orchestrator will have the tasks to split the input data, join toghether the coregistration parameters of each patch, and assemble the geocoded parts coming from the nodes. The entire process is then parallelized with a small additional overhead for the orchestrator tasks.

Input Files

Input Master file

Input file name of the (not coregistered) Single Look Complex (_slc) Master data. This file is mandatory.

Input Slave file

Input file name of the (not coregistered) Single Look Complex (_slc) Slave data. This file is mandatory.

Optional Files

ScanSAR-TOPSAR Spectral Diversity Avoid Area

In case of large displacement (like an earthquake) it is suggested to create a shapefile (.shp) which contains the movement area, this shapefile must be geocoded (lat-long). All the ScanSAR or TOPSAR bursts which intersect this shapefile will be avoided during the Spectral Diversity estimation step. This file is optional.

DEM/Cartographic System

Digital Elevation Model file

Name of the Digital Elevation Model file. This should be referred to the ellipsoid. This file is optional.

Output Projection

In case that the Digital Elevation Model is not used, the following parameters are compulsory to define the Cartographic System:

State

Definition of the country or general projection systems.

Projection

Definition of the projection system of the selected State. In case that a general projection system is selected in State, the Projection is automatically set.

Ellipsoid

Definition of the ellipsoid. This is chosen according to the selected State and Projection.

Hemisphere

Definition of the hemisphere. This is chosen according to the selected State and Projection.

Zone

Definition of the zone. This is chosen according to the selected State and Projection.

Datum Shift Parameters

Definition of the datum shift parameters. These are chosen according to the selected State and Projection.

Reference Height

In case that the Digital Elevation Model is not used, a constant ellipsoidal height must be provided. Default Reference Height is 0.

Cartographic Parameters

The reference parameters for some projection systems (e.g. Stereographic, Polar Stereographic, Gnomonic, Mercator, Miller, Albers, etc.) can be set.

Parameters - Principal Parameters

Range looks

Number of looks in range.

Azimuth looks

Number of looks in azimuth.

Grid Size for Suggested Looks

The grid size, in meters, used to tune range and azimuth looks. If the other parameters are manually set, the grid size will not imply a change in their values.

X and Y Grid Size

The grid size of the output data must be defined; the default unit of measure is meters.

Coregistration with DEM

By setting this flag, the input Digital Elevation Model is used in the coregistration process.

Filtering method

The filtering methods can be selected:

•Boxcar

•Adaptive Non-Local

Coherence AZ Box Range

Window Size in Azimuth direction for Boxcar method.

Coherence RG Box Range

Window Size in Azimuth direction for Boxcar method.

Parameters - Cluster

It brings to the general section of the Preferences parameters. Any modified value will be used and stored for further processing sessions.

Parameters - Global

It brings to the general section of the Preferences parameters. Any modified value will be used and stored for further processing sessions.

Parameters - Interferogram

It brings to the Interferometry section of the Preferences parameters. Any modified value will be used and stored for further processing sessions.

Parameters - Flattening

It brings to the Flattening section of the Preferences parameters. Any modified value will be used and stored for further processing sessions.

Parameters - Filtering

It brings to the Adaptive Filtering section of the Preferences parameters. Any modified value will be used and stored for further processing sessions.

Parameters - Coregistration

It brings to the coregistration section of the Preferences parameters. Any modified value will be used and stored for further processing sessions.

Parameters - Other Parameters

It brings to the general section of the Preferences parameters. Any modified value will be used and stored for further processing sessions.

Output Files

Output Root Name

Name of the output root. This file is mandatory.

_cc

Coherence and associated header files (.sml, .hdr).

Details specific to the Units of Measure and Nomenclature of the output products can be found in the Data Format section.

General Functions

Exec

The processing step is executed.

Store Batch

The processing step is stored in the batch list. The Batch Browser button allows to load the batch processing list.

The window will be closed.

Help

Specific help document section.

Specific Function(s)

None.

Interferometry - Clustered Processes - CCD Cluster

Interferometry - Clustered Processes - CCD Cluster