The detailed algorithm for stack processing of TOPS data can be find here:
- Fattahi, H., P. Agram, and M. Simons (2016), A Network-Based Enhanced Spectral Diversity Approach for TOPS Time-Series Analysis, IEEE Transactions on Geoscience and Remote Sensing, 55(2), 777-786, doi:10.1109/TGRS.2016.2614925.
To use the sentinel stack processor, make sure to add the path of your contrib/stack/topsStack folder to your $PATH environment varibale.
The scripts provides support for Sentinel-1 TOPS stack processing. Currently supported workflows include a coregistered stack of SLC, interferograms, offsets, and coherence.
stackSentinel.py generates all configuration and run files required to be executed on a stack of Sentinel-1 TOPS data. When stackSentinel.py is executed for a given workflow (-W option) a configs and run_files folder is generated. No processing is performed at this stage. Within the run_files folder different run_#_description files are contained which are to be executed as shell scripts in the run number order. Each of these run scripts call specific configure files contained in the “configs” folder which call ISCE in a modular fashion. The configure and run files will change depending on the selected workflow. To make run_# files executable, change the file permission accordingly (e.g., chmod +x run_01_unpack_slc).
stackSentinel.py -H #To see workflow examples,
stackSentinel.py -h #To get an overview of all the configurable parametersRequired parameters of stackSentinel.py include:
-s SLC_DIRNAME #A folder with downloaded Sentinel-1 SLC’s.
-o ORBIT_DIRNAME #A folder containing the Sentinel-1 orbits. Missing orbit files will be downloaded automatically
-a AUX_DIRNAME #A folder containing the Sentinel-1 Auxiliary files
-d DEM_FILENAME #A DEM (Digital Elevation Model) referenced to wgs84In the following, different workflow examples are provided. Note that stackSentinel.py only generates the run and configure files. To perform the actual processing, the user will need to execute each run file in their numbered order.
In all workflows, coregistration (-C option) can be done using only geometry (set option = geometry) or with geometry plus refined azimuth offsets through NESD (set option = NESD) approach, the latter being the default. For the NESD coregistrstion the user can control the ESD coherence threshold (-e option) and the number of overlap interferograms (-O) to be used in NESD estimation.
The following calibration auxliary (AUX_CAL) file is used for antenna pattern correction to compensate the range phase offset of SAFE products with IPF verison 002.36 (mainly for images acquired before March 2015). If all your SAFE products are from another IPF version, then no AUX files are needed. Check ESA document for details.
The AUX_CAL file is available on Sentinel-1 Mission Performance Center. We recommend download it using the web brower or the wget command below, and store it somewhere (i.e. ~/aux/aux_cal) so that you can use it all the time, for stackSentinel.py -a or auxiliary data directory in topsApp.py.
wget https://sar-mpc.eu/download/ca97845e-1314-4817-91d8-f39afbeff74d/ -O S1A_AUX_CAL_V20140908T000000_G20190626T100201.SAFE.zip
mkdir MexicoSenAT72
cd MexicoSenAT72
Download of DEM (need to use wgs84 version) using the ISCE DEM download script.
mkdir DEM; cd DEM
dem.py -a stitch -b 18 20 -100 -97 -r -s 1 -c
rm demLat*.dem demLat*.dem.xml demLat*.dem.vrt
cd ..
Generate the run and configure files needed to generate a coregistered stack of SLCs. In this example, a pre-defined bounding box is specified. Note, if the bounding box is not provided it is set by default to the common SLC area among all SLCs. We recommend that user always set the processing bounding box. Since ESA does not have a fixed frame definition, we suggest to download data for a larger bounding box compared to the actual bounding box used in stackSentinel.py. This way user can ensure to have required data to cover the region of interest. Here is an example command to create configuration files for a stack of SLCs:
stackSentinel.py -s ../SLC/ -d ../DEM/demLat_N18_N20_Lon_W100_W097.dem.wgs84 -a ../../AuxDir/ -o ../../Orbits -b '19 20 -99.5 -98.5' -W slc
by running the command above, the configs and run_files folders are created. User needs to execute each run file in order. The order is specified by the index number of the run file name. For the example above, the run_files folder includes the following files:
- run_01_unpack_slc_topo_reference
- run_02_average_baseline
- run_03_extract_burst_overlaps
- run_04_overlap_geo2rdr_resample
- run_05_pairs_misreg
- run_06_timeseries_misreg
- run_07_geo2rdr_resample
- run_08_extract_stack_valid_region
- run_09_merge
- run_10_grid_baseline
The generated run files are self descriptive. Below is a short explanation on what each run_file does:
run_01_unpack_slc_topo_reference:
Includes commands to unpack Sentinel-1 TOPS SLCs using ISCE readers. For older SLCs which need antenna elevation pattern correction, the file is extracted and written to disk. For newer version of SLCs which don’t need the elevation antenna pattern correction, only a gdal virtual “vrt” file (and isce xml file) is generated. The “.vrt” file points to the Sentinel SLC file and reads them whenever required during the processing. If a user wants to write the “.vrt” SLC file to disk, it can be done easily using gdal_translate (e.g. gdal_translate –of ENVI File.vrt File.slc). The “run_01_unpack_slc_topo_reference” also includes a command that refers to the config file of the stack reference, which includes configuration for running topo for the stack reference. Note that in the pair-wise processing strategy one should run topo (mapping from range-Doppler to geo coordinate) for all pairs. However, with stackSentinel, topo needs to be run only one time for the reference in the stack.
run_02_average_baseline:
Computes average baseline for the stack. These baselines are not used for processing anywhere. They are only an approximation and can be used for plotting purposes. A more precise baseline grid is estimated later in run_10.
run_03_extract_burst_overlaps:
Burst overlaps are extracted for estimating azimuth misregistration using NESD technique. If coregistration method is chosen to be “geometry”, then this run file won’t exist and the overlaps are not extracted.
run_04_overlap_geo2rdr_resample:*
Running geo2rdr to estimate geometrical offsets between secondary burst overlaps and the stack reference burst overlaps. The secondary burst overlaps are then resampled to the stack reference burst overlaps.
run_05_pairs_misreg:
Using the coregistered stack burst overlaps generated from the previous step, differential overlap interferograms are generated and are used for estimating azimuth misregistration using Enhanced Spectral Diversity (ESD) technique.
run_06_timeseries_misreg:
A time-series of azimuth and range misregistration is estimated with respect to the stack reference. The time-series is a least squares esatimation from the pair misregistration from the previous step.
run_07_geo2rdr_resample:
Using orbit and DEM, geometrical offsets among all secondary SLCs and the stack reference is computed. The goometrical offsets, together with the misregistration time-series (from previous step) are used for precise coregistration of each burst SLC.
run_08_extract_stack_valid_region:
The valid region between burst SLCs at the overlap area of the bursts slightly changes for different acquisitions. Therefore we need to keep track of these overlaps which will be used during merging bursts. Without these knowledge, lines of invalid data may appear in the merged products at the burst overlaps.
run_09_merge:
Merges all bursts for the reference and coregistered SLCs. The geometry files are also merged including longitude, latitude, shadow and layer mask, line-of-sight files, etc. .
run_10_grid_baseline:
A coarse grid of baselines between each secondary SLC and the stack reference is generated. This is not used in any computation.
In the following example, the same stack generation is requested but where the threshold of the default coregistration approach (NESD) is relaxed from its default 0.85 value 0.7.
stackSentinel.py -s ../SLC/ -d ../DEM/demLat_N18_N20_Lon_W100_W097.dem.wgs84 -a ../../AuxDir/ -o ../../Orbits -b '19 20 -99.5 -98.5' -W slc -e 0.7
When running all the run files, the final products are located in the merge folder which has subdirectories geom_reference, baselines and SLC. The geom_reference folder contains geometry products such as longitude, latitude, height, local incidence angle, look angle, heading, and shadowing/layover mask files. The baselines folder contains sparse grids of the perpendicular baseline for each acquisition, while the SLC folder contains the coregistered SLCs
Generate the run and configure files needed to generate a stack of interferograms. In this example, a stack of interferograms is requested for which up to 2 nearest neighbor connections are included.
stackSentinel.py -s ../SLC/ -d ../../MexicoCity/demLat_N18_N20_Lon_W100_W097.dem.wgs84 -b '19 20 -99.5 -98.5' -a ../../AuxDir/ -o ../../Orbits -c 2
In the following example, all possible interferograms are being generated and in which the coregistration approach is set to use geometry and not the default NESD.
stackSentinel.py -s ../SLC/ -d ../../MexicoCity/demLat_N18_N20_Lon_W100_W097.dem.wgs84 -b '19 20 -99.5 -98.5' -a ../../AuxDir/ -o ../../Orbits -C geometry -c all
When executing all the run files, a coregistered stack of slcs are produced, the burst interferograms are generated and then merged. Merged interferograms are multilooked, filtered and unwrapped. Geocoding is not applied. If users need to geocode any product, they can use the geocodeGdal.py script.
Generate the run and configure files needed to generate a stack of coherence. In this example, a correlation stack is requested considering all possible coherence pairs and where the coregistration approach is done using geometry only.
stackSentinel.py -s ../SLC/ -d ../../MexicoCity/demLat_N18_N20_Lon_W100_W097.dem.wgs84 -b '19 20 -99.5 -98.5' -a ../../AuxDir/ -o ../../Orbits -C geometry -c all -W correlation
This workflow is basically similar to the previous one. The difference is that the interferograms are not unwrapped.
Ionospheric phase estimation can be performed for each of the workflow introduced above. Generally, we should do ionospheric phase estimation for data acquired at low latitudes on ascending tracks. However, ionospheric phase estimation only works well in areas with high coherence since it requires phase unwrapping. Details about Sentinel-1 ionospheric correction can be found in
- C. Liang, P. Agram, M. Simons, and E. J. Fielding, “Ionospheric correction of InSAR time series analysis of C-band Sentinel-1 TOPS data,” IEEE Transactions on Geoscience and Remote Sensing, vol. 57, no. 9, pp. 6755-6773, Sep. 2019.
Ionospheric phase estimation has more requirements than regular InSAR processing. The most important two requirements include
-
All the acquistions need to be connected in the entire network.
-
The swath starting ranges need to be the same among all acquistions; otherwise a phase offset between adjacent swaths need to be estimated in order to maintain consistency among the swaths, which might not be accurate enough.
In stack ionospheric phase estimation, acquistions with same swath starting ranges are put in a group. A network is formed within a group. Extra pairs are also processed to connect the different groups so that all acquistions are connected. But we need to estimate a phase offset for these extra pairs, which might not be accurate. Therefore, for a particualr swath starting ranges, if there are only a few acquistions, it's better to just discard them so that we don't have to estimate the phase offsets.
s1_select_ion.py -dir data/slc -sn 33.550217 37.119545 -nr 10
Acquistions to be used need to fully cover the south/north bounds. After running this command, acquistion not to be used will be put in a folder named 'not_used'. It's OK to run this command multiple times.
In stackSentinel.py, two options are for ionospheric phase estimation
- --param_ion
- --num_connections_ion
An example --param_ion file 'ion_param.txt' is provided in the code directory. For example, we want to do ionospheric phase estimation when processing a stack of interferograms
stackSentinel.py -s ../data/slc -d ../data/dem/dem_1_arcsec/demLat_N32_N41_Lon_W113_W107.dem.wgs84 -b '33.550217 37.119545 -111.233932 -107.790451' -a ../data/s1_aux_cal -o ../data/orbit -C geometry -c 2 --param_ion ../code/ion_param.txt --num_connections_ion 3
Note in 'ion_param.txt', if 'consider burst properties in ionosphere computation' is True, Coregistration options '-C', '--coregistration' in stackSentinel.py must be NESD.
If ionospheric phase estimation is enabled in stackSentinel.py, it will generate the following run files. Here ns means number of steps in the original stack processing, which depends on the type of stack (slc, correlation, interferogram, and offset).
- run_ns+1_subband_and_resamp
- run_ns+2_generateIgram_ion
- run_ns+3_mergeBurstsIon
- run_ns+4_unwrap_ion
- run_ns+5_look_ion
- run_ns+6_computeIon
- run_ns+7_filtIon
- run_ns+8_invertIon
Note about 'areas masked out in ionospheric phase estimation' in ion_param.txt. Seperated islands or areas usually lead to phase unwrapping errors and therefore significantly affect ionospheric phase estimation. It's better to mask them out. Check ion/date1_date2/ion_cal/raw_no_projection.ion for areas to be masked out. However, we don't have this file before processing the data. To quickly get this file, we can process a stack of two acquistions to get this file. NOTE that the reference of this two-acquisition stack should be the same as that of the full stack we want to process.
run_ns+1_subband_and_resamp
Two subband burst SLCs are generated for each burst. For secondary acquistions, the subband burst SLCs are also resampled to match reference burst SLCs. If the subband burst SLCs already exists, the program simply skips the burst.
run_ns+2_generateIgram_ion
Generate subband burst interferograms.
run_ns+3_mergeBurstsIon
Merge subband burst interferograms, and create a unique coherence file used in ionospheric phase estimation. This will be done swath by swath if the two acquistions of the pair has different swath starting ranges.
run_ns+4_unwrap_ion
Unwrap merged subband interferograms. This will be done swath by swath if the two acquistions of the pair has different swath starting ranges.
run_ns+5_look_ion
Take further looks on the unwrapped interferograms, and create the unique coherence file based on the further number of looks. This will be done swath by swath if the two acquistions of the pair has different swath starting ranges.
run_ns+6_computeIon
Compute ionospheric phase. This will be done swath by swath if the two acquistions of the pair has different swath starting ranges, and then the swath ionospheric phase will be merged.
run_ns+7_filtIon
Filter ionospheric phase.
run_ns+8_invertIon
Estimate ionospheric phase for each date. We highly recommend inspecting all pair ionospheric phases ion/date1_date2/ion_cal/filt.ion, and exclude those with anomalies in this command.
Typical anomalies include dense fringes caused by phase unwrapping errors, and a range ramp as a result of errors in estimating phase offsets for pairs with different swath starting ranges (check pairs_diff_starting_ranges.txt).
run_ns+9_filtIonShift
Filter azimuth ionospheric shift.
run_ns+10_invertIonShift
Estimate azimuth ionospheric shift for each date. As in step run_ns+8_invertIon, check if there are anamolies.
run_ns+11_burstRampIon
Compute azimuth burst ramps as a result of ionosphere for each date.
run_ns+12_mergeBurstRampIon
Merge azimuth burst ramps.
Run the commands sequentially.
Results from ionospheric phase estimation.
- reference and coreg_secondarys: now contains also subband burst SLCs
- ion: original ionospheric phase estimation results
-
ion_azshift_dates: azimuth ionospheric shift for each acquistion -
ion_burst_ramp_dates: azimuth burst ramps caused by ionosphere for each acquistion -
ion_burst_ramp_merged_dates: merged azimuth burst ramps caused by ionosphere for each acquistion - ion_dates: ionospheric phase for each acquistion
- ion/date1_date2/ion_cal/azshift.ion: azimuth ionospheric shift
- ion/date1_date2/ion_cal/filt.ion: filtered ionospheric phase
- ion/date1_date2/ion_cal/raw_no_projection.ion: original ionospheric phase
- ion/date1_date2/lower/merged/fine_look.unw: unwrapped lower band interferogram
- ion/date1_date2/upper/merged/fine_look.unw: unwrapped upper band interferogram
If ionospheric phase estimation processing is swath by swath because of different swath starting ranges, there will be swath processing directories including
- ion/date1_date2/ion_cal_IW*
- ion/date1_date2/lower/merged_IW*
- ion/date1_date2/upper/merged_IW*
Unit of azimuth ionospheric shift is number of single look azimuth lines. After processing, we can plot ionospheric phase estimation results using plotIonPairs.py and plotIonDates.py. For example
plotIonPairs.py -idir ion -odir ion_plot
plotIonDates.py -idir ion_dates -odir ion_dates_plot
Relationships of the ionospheric phases:
ion_dates/date1.ion - ion_dates/date2.ion = ion/date1_date2/ion_cal/filt.ion
ion_dates/date1.ion - ion_dates/date2.ion = ionospheric phase in merged/interferograms/date1_date2/filt_fine.unw
ion_burst_ramp_merged_dates/date1.float - ion_burst_ramp_merged_dates/date2.float = azimuth burst ramps caused by ionosphere in merged/interferograms/date1_date2/filt_fine.unw