Description • Installation • Dependencies • Example • Notes • Authors
The pyroSAR package aims at providing a complete solution for the scalable organization and processing of SAR satellite data:
- Reading of data from various past and present satellite missions
- Handling of acquisition metadata
- User-friendly access to processing utilities in SNAP and GAMMA Remote Sensing software
- Formatting of the preprocessed data for further analysis
Here you can find the documentation.
For the installation we need the Python tool pip and the version control system git. On Windows pip is installed together with Anaconda, git can be downloaded from here. On Linux you can easily install both via command line:
sudo apt-get install python-pip
sudo apt-get install gitOnce everything is set up, pyroSAR is ready to be installed:
sudo pip install git+https://github.com/johntruckenbrodt/pyroSAR.gitOn Windows you need to use the Anaconda Prompt and leave out sudo in the above command.
If you are using Windows, the easiest way to work with pyroSAR and Python in general is by using Anaconda. It comes with all basic requirements of pyroSAR. The more specific instructions below are intended for Linux users.
pyroSAR requires GDAL version 2.1 with GEOS and PROJ4 as dependencies as well as the GDAL Python binding. Alternatively, one can use pygdal, a virtualenv and setuptools friendly version of standard GDAL python bindings.
Starting with release Yakkety (16.10), Ubuntu comes with GDAL >2.1. See here. You can install it like this:
sudo apt-get install python-gdal python3-gdal gdal-binFor older Ubuntu releases you can add the ubuntugis repository to apt prior to installation to install version >2.1:
sudo add-apt-repository ppa:ubuntugis/ppa
sudo apt-get updateThis way the required dependencies (GEOS and PROJ4 in particular) are also installed. You can check the version by typing:
gdalinfo --versionStarting with Debian 9 (Stretch) GDAL is available in version >2.1 in the official repository.
Alternatively, you can build GDAL and the dependencies from source. The script pyroSAR/install/install_deps.sh
gives specific instructions on how to do it. It is not yet intended to run this script via shell, but rather to
follow the instructions step by step.
While sqlite3 and its Python binding are usually already installed, the spatialite extension needs to be added. Two packages exist, libspatialite and mod_spatialite. Both can be used by pyroSAR. mod_spatialite has been found to be easier to setup with sqlite and can be installed via apt:
sudo apt-get install libsqlite3-mod-spatialiteThe following can be run in Python to test the needed functionality:
import sqlite3
# setup an in-memory database
con=sqlite3.connect(':memory:')
# enable loading extensions and load spatialite
con.enable_load_extension(True)
try:
con.load_extension('mod_spatialite.so')
except sqlite3.OperationalError:
con.load_extension('libspatialite.so')In case loading extensions is not permitted you might need to install the package pysqlite2.
See the script pyroSAR/install/install_deps.sh for instructions.
There you can also find instructions on how to install spatialite from source.
To test pysqlite2 you can import it as follows and then run the test above:
from pysqlite2 import dbapi2 as sqlite3Installing this package is likely to cause problems with the sqlite3 library installed on the system. Thus, it is safer to build a static sqlite3 library for it (see installation script).
Now that everything is installed, we can start working with our satellite data. Let's assume you have a Sentinel-1 scene in a local directory. At first we load the scene into pyroSAR for analysis of the metadata:
from pyroSAR import identify
name = 'S1A_IW_GRDH_1SDV_20150222T170750_20150222T170815_004739_005DD8_3768.zip'
scene = identify(name)
scene.summary()This will automatically identify the scene, scan it for metadata and print a summary of selected metadata entries.
The names of the attributes (e.g. sensor and acquisition_mode) are standardized for all SAR scenes.
Further entries, whose names are not standardized, can be found in a dictionary scene.meta.
Now that we have made ourselves familiar with the scene, we import it into a sqlite database:
from pyroSAR import Archive
dbfile = 'scenes.db'
with Archive(dbfile) as archive:
archive.insert(scene)dbfile is a file either containing an already existing database or one to be created.
Let's assume our database contains a number of scenes and we want to select some for processing.
We have a shapefile, which contains a geometry delimiting our test site for which we want to
process some Sentinel-1 scenes.
We already processed some scenes in the past and the results are stored in a directory
outdir. We only want to select scenes which have not been processed to this directory before.
Furthermore, we are only interested in scenes acquired in Ground Range Detected (GRD) Interferometric Wide
Swath mode (IW), which contain a VV band.
from spatialist import Vector
archive = Archive('scenes.db')
site = Vector('site.shp')
outdir = '/path/to/processed/results'
maxdate = '20171231T235959'
selection_proc = archive.select(vectorobject=site,
processdir=outdir,
maxdate=maxdate,
sensor=('S1A', 'S1B'),
product='GRD',
acquisition_mode='IW',
vv=1)
archive.close()Here we use pyroSAR's own vector geometry driver for loading the shapefile and pass it, together with the other parameters,
to the method Archive.select. You can also use the with statement like in the code block above.
The returned selection_proc is a list of file names for the scenes we selected from the database, which we can now
pass to a processing function:
from pyroSAR.snap import geocode
# the target pixel resolution in meters
resolution = 20
for scene in selection_proc:
geocode(infile=scene, outdir=outdir, tr=resolution, scaling='db', shapefile=site)The function geocode is a basic utility for SNAP. It will perform all necessary steps to subset, resample, orthorectify,
topographically normalize and scale the input image and write GeoTiff files to the selected output directory.
All necessary files like orbit state vectors and SRTM DEM tiles are downloaded automatically in the background by SNAP.
SNAP is most conveniently used with workflow XMLs. The function geocode parses a workflow for the particular scene,
parametrizes it depending on the scene type and selected processing parameters and writes it to the output directory.
It then calls the command gpt, which is SNAP's command line interface, on the workflow to execute the processing steps.
pyroSAR internally uses a fixed naming scheme to keep track of processed results. For each scene an identifier is created,
which contains the sensor, acquisition mode, orbit (ascending or dsescending) and the time stamp of the acquisition start.
For the example above it is S1A__IW___A_20150222T170750, which can be created by calling scene.outname_base(). For each
attribute a fixed number of digits is reserved. In case the attribute is shorter than this number,
the rest of the digits is filled with underscores. I.e., the sensor field is four digits long, but 'S1A' only three.
Thus, S1A_ is the sensor slot. In the same way, IW__ is the acquisition mode slot, which is also four digits long.
A denotes ascending orbit, the time stamp is in format YYYYmmddTHHMMSS.
Processing functions like geocode add suffixes to this identifier to further keep track of individual processing
steps performed on the dataset.
This core concept is used by many pyroSAR functions internally to keep track of which scenes have been processed before.
The launch of recent satellite missions, the Sentinel fleet of ESA’s Copernicus programme in particular, has led to a tremendous increase in available earth observation data provided at no cost. The increase in data availability opens up new opportunities for analysing data not only in the spatial but also temporal domain by observing time series and thus the possibility to visualise processes on the earth’s surface. Although this is not entirely new to optical satellite data, Synthetic Aperture Radar (SAR) data was only infrequently acquired in the past. With the new ESA SAR satellites Sentinel-1A and Sentinel-1B there is now the possibility to observe the earth’s surface with a repeat rate of up to six days and a spatial resolution of 20 m independent of atmospheric effects and sun illumination. Together with the increase in data availability comes the challenge of organizing data and preparing it for scientific analysis. While traditional software aimed at analysing single images, the need arises for fully automated organization of large image archives with thousands of images together with a highly capable processing framework to make full use of available hardware resources. The pyroSAR environment aims at providing a complete solution for the organization and processing of SAR satellite data for applications scalable from personal computers to large server infrastructures using various open source tools and libraries. Its purpose is to provide complex functionality for reading various data formats from past and present satellite missions, handling metadata about acquisition characteristics in a database, and providing homogenised user-friendly access to processing utilities in ESA’s Sentinel Application Platform (SNAP) as well as GAMMA Remote Sensing software. The data reader uses the Geo Data Abstraction Library (GDAL) where possible and own implementations otherwise. The metadata attributes are homogenised to enable database access of specific acquisition characteristics across different sensor platforms. The metadata is ingested into a SpatiaLite database from which the original imagery can be selected for processing. The SAR processor provides functionality to distribute the tasks on different computing cores as well as different server nodes. By following a stringent naming scheme of processed images as well as annotated metadata XMLs, processing can be organized to be performed by several operators in a server network. This way, redundant usage of disk space and processing resources can be reduced. Once the images are processed, further functionalities are available for mosaicking and resampling images to common pixel boundaries suited for time series analysis. Thus, the scientist is provided with data stacks cropped to the study area and directly formatted for analysis without spending time with SAR-specific processing and general data management issues. This software is currently being developed within EU Horizon-2020 project ‘Satellite-based Wetland Observation Service (SWOS)’. In an effort to better monitor wetlands from space with both optical and radar data, the dense time series of the Sentinel-1 satellites is exploited in order to derive high temporal resolution surface water dynamics maps. This is realized by applying clustering techniques in the temporal image domain of all available datasets.
- John Truckenbrodt ([email protected])
- Felix Cremer ([email protected])
- Ismail Baris ([email protected])