derived from Sentinel-1 image collections (2016) and 
resolution will be about 20 meters. Since these data 
has not been available yet, it could not be considered 
for a visual comparison nor an accuracy assessment 
in this study. 
By launching the Sentinel mission in 2014, the 
European Space agency ESA aimed to satisfy the 
need of the Copernicus program. Sentinel-1 is the first 
of five missions that ESA developed for the 
Copernicus initiative. Sentinel-1 comprises a 
constellation of two polar-orbiting satellites 
(Sentinel-1A, Sentinel-1B), operating day and night 
performing C-band synthetic aperture radar imaging, 
enabling them to acquire imagery regardless of 
weather conditions or light conditions (D’Aria et al., 
2016).  
This work presents the comparison of Sentinel-1 
data used for the development of two automatically 
derived settlement layers differentiating between 
built-up and non-built up area and the Copernicus 
high-resolution layer ‘Imperviousness Degree’ and 
the European Settlement Map (ESM) 2016. In 
contrast to CLC data that are confined for Europe, 
satellites of the Sentinel mission collect data globally. 
The Sentinel-1 data coverage makes it possible to 
establish a global settlement layer. 
2  DATA 
This study uses Sentinel-1 image data, collected from 
the first 7 months of the year 2016, the Compernicus 
HRL imperviousness for the year 2012 and European 
Settlement Map 2016. Additionally a Sentinel-2A 
scene (date of acquisition: 02.07.2016) is used for 
visual interpretation of the results. 
2.1 Sentinel-1 Data 
The Sentinel program is the most comprehensive and 
ambitious European Earth Observation program. The 
Sentinel satellites provide unique operational sensing 
capabilities across the whole measurement spectrum, 
covering a broad range of applications. Thanks to 
their advanced sensing concepts and outstanding 
spatio-temporal sampling characteristics, the Sentinel 
satellites will collect more data than any earth 
observation program before (Attema et al., 2007). 
The first of the Sentinel satellite series, Sentinel-1A 
was launched on 3 April 2014. Seninel-1 (S-1) is a 
Synthetic Aperture Radar (SAR) mission for ocean 
and land monitoring. S-1 is the continuity mission to 
the SAR instruments flown on board of ERS and 
ENVISAT. The S-1 mission is implemented through 
a constellation of two satellites. The S-1B was 
launched on 25 April 2016. The S-1 data over the land 
masses are mainly acquired in Interferometric Wide 
swath (IW) mode. The S-1 Level-1 Ground Range 
Detected (GRD) products, which are suitable for the 
most of the land applications, consist of focused SAR 
data that has been detected, multi-looked and 
projected to ground range using an Earth ellipsoid 
model such as WGS84. The IW GRD products are 
provided in two High (20 m x 22 m)  and Medium (88 
m x 87 m) spatial resolutions resampled to 10 m and 
40 m pixel spacing grids respectively (European 
Space Agency, 2013, p. 1).  
Despite all corrections from Level-0 up to Level-1 
data, the GRD data still need to be processed further 
before generating level-2 products. The S-1 Level-1 
GRD data used in this study were pre-processed using 
the TU Wien SAR Geophysical Retrieval Toolbox 
(SGRT) (Naeimi et al., 2016). The pre-processing 
workflow include calibration, noise removal, 
georeferencing and terrain correction using a Digital 
Elevation Model (DEM), shadow mask generation, 
data conversions, and data resampling and tiling to a 
regular grid using an appropriate cartographic map 
projection. For the calibration, georeferencing and the 
terrain correction, the ESA’s Sentinel-1 toolbox 
(S1TBX) is employed. The S1TBX operators are 
called via SGRT to perform the georeferencing using 
the S-1 precise orbit files provided externally by ESA. 
In this study the S1TBX Range Doppler algorithm 
and SRTM digital elevation data are used for terrain 
correction of the SAR scenes. After some further 
preprocessing steps like thermal noise removal, data 
format conversion and shadow mask generation the 
geocoded SAR scenes are resampled to the TU Wien 
Equi7 Grid. The TU Wien Equi7 Grid is designed to 
minimize the oversampling rate of the high resolution 
satellite data globally, while keeping its structure 
simple (Bauer-Marschallinger et al., 2014). After the 
pre-processing step, the S-1 backscatter time series 
were used to generate composites of monthly mean of 
backscatter for each polarization separately over the 
test site. In this study high resolution S-1 image stacks 
collected from 7 months (January – July) of the year 
2016 are used. 
2.2  Copernicus High Resolution Layer 
Imperviousness Degree 
The HRL imperviousness is produced using an 
automatic algorithm based on calibrated NDVI. 
Similar to other HRLs of the Copernicus program, the 
imperviousness HRL is derived from 20 m resolution 
optical satellite imagery. The layer has 20 m