The Sentinel-1 SAR is a C-band radar on sun-synchronous polar orbit (Fletcher, 2012). Sentinel-1A has been on the orbit since 3 April 2014 and Sentinel-1B since 25 April 2016, while the 1B is not functional since December 2021 due to technical problems (ESA, 2022). The radar measures microwave backscatter using the Terrain Observation with Progressive Scans SAR (TOPSAR) method by electronically steering the radar antenna over target area while the satellite is moving in azimuth direction. Measurements are done using one of four configurations. The Interferometric Wide swath (IW) mode is commonly used for land surface targets. The full ground range swath of Sentinel-1 SAR in the IW-mode is divided into three sub-swaths (Fletcher, 2012; Hajduch
The long Sentinel-1 SAR time series are used for prediction of soil moisture dynamics, for mapping of forests and other vegetation phenology (Van doninck
A frequently used method for normalizing SAR backscatter is to assume a linear relationship and convert the
where
The orbits of Sentinel-1 converge towards Earth poles and at higher latitudes it is possible to observe target objects from different orbits. In Estonia the image swaths from four to six orbits intersect on the ground. With the Sentinel-1A/1B pair on the orbit it is therefore possible during 72 hours to get three nighttime measurements and three daytime measurements for a forest stand so that an almost fullview angle range of Sentinel-1 SAR is covered in the triplets. We selected a 15 by 15 km test site near Laeva village, Estonia, in managed hemiboreal forests to study the applicability of the linear normalization (1) for the compilation of dense SAR time series.
The 15×15 km test site centre coordinates are 26° 26’ 43’’ E and 58° 31’ 56’’ N. Within the area are two larger forested regions separated by river Laeva (map in Appendix 1). The topography of the area is flat. Forests in the northern bank of the river are regularly managed, but the southern region has common management history until 2019 when Raja-Kärevere nature reserve was established. Most soils in the forest land are fertile corresponding to
We used a stack of analysis-ready radar satellite data provided by the company KappaZeta (Kastani 42, 50410 Tartu, Estonia). The stack included interferometric coherence: 6- or 12-day repeat pass for VH and VV polarization, backscatter in VH and VV polarization mode and VH/VV backscatter ratio and local incidence angle data. Data were in raster files; pixel size 5 m. Backscatter values were computed as
The local incidence angle map was included in the data stack. It is based on satellite ephemeris data and Copernicus 30 m digital elevation model (DEM) (Fahrland
We used all Sentinel-1 SAR measurements that were available from the beginning of operation until the end of March 2022. From each orbit there were more than 200 images available (Table 1) for the entire study period. In this study we analysed VV polarised backscatter.
Sentinel-1 images over Laeva test site. θ is the local incidence angle.
Relative orbit |
Time, UTC |
Direction |
Images |
|
---|---|---|---|---|
058 | 45.5 | 16:00 | W | 254 |
153 | 31.3 | 04:30 | E | 217 |
160 | 39.3 | 16:00 | W | 281 |
080 | 38.9 | 04:30 | E | 281 |
087 | 31.7 | 16:00 | W | 233 |
007 | 45.3 | 04:30 | E | 280 |
The average value of pixels found within stand border was calculated for each stand from the VV-polarized band of each image. Out of the 4,995 stands we found triple SAR measurements, i.e. sequences from three orbits for 3,159 stands at nighttime and for 1,105 stands at daytime.
We compared data from nighttime {153;080;007} and daytime {087;160;058} orbit triplets and found that daytime VV-polarized backscatter
A mixed species stand (ID=2499). The mean value of VV-polarized backscatter
VV-polarisatsiooniga tagasihajumine
We separated daytime and nighttime measurements and then combined measurements according to data from orbit pairs {153–080; 080–007; 087–160; 160–058} and fitted each combination with the linear model
where
By comparing the values of
Slope β×104 values for model (2) fitted on VV polarized backscatter time series. Each symbol represents a single stand.
Puistute aegridadele lähendatud mudeli (2) parameetri β×104 väärtused VV-polarisatsiooniga tagasihajumise korral.
The reason for the dependence of the angular correction coefficient
Our empirical finding may have importance for the construction of the normalized incidence angle of Sentinel-1 SAR backscatter time series for vegetation mapping and phenology studies. Fitting just a linear model on all Sentinel-1 SAR backscatter measurements over target to correct for incidence angle is not sufficient to remove the signal dependence on the influence of scanner subswath. In mapping and change detection applications the processing and decision-making accuracy may be increased if the effect of Sentinel-1 SAR subswath characteristics and the nighttime and daytime backscatter difference on the registered microwave pulse backscatter will be taken into account. Also, the 1B is not functional since December 2021 and this can create artefacts in long time series as the combination of sub-swaths over the targets is now different compared to the operational pair of Sentinel-1A and Sentinel-1B.