Minimize Interferometric Wide Swath

The Interferometric Wide swath mode is the main acquisition mode over land and satisfies the majority of service requirements. It acquires data with a 250 km swath at 5 m by 20 m spatial resolution (single look). IW mode captures three sub-swaths using Terrain Observation with Progressive Scans SAR (TOPSAR). With the TOPSAR technique, in addition to steering the beam in range as in ScanSAR, the beam is also electronically steered from backward to forward in the azimuth direction for each burst, avoiding scalloping and resulting in homogeneous image quality throughout the swath [1].

TOPSAR mode is intended to replace the conventional ScanSAR mode, achieving the same coverage and resolution as ScanSAR, but with a nearly uniform SNR (Signal-to-Noise Ratio) and DTAR (Distributed Target Ambiguity Ratio).

Figure 1: TOPSAR Sub-Swath Acquisition

Azimuth resolution is reduced compared to SM due to the shorter target illumination time of the burst. Using the sweeping azimuth pattern, each target is seen under the same antenna pattern, independently from its azimuth position in the burst image. By shrinking the azimuth antenna pattern, as seen by a target on the ground, scalloping effects on the image can be reduced. Bursts are synchronised from pass to pass to ensure the alignment of interferometric pairs.

IW SLC products contain one image per sub-swath and one per polarisation channel, for a total of three (single polarisation) or six (dual polarisation) images in an IW product.

Each sub-swath image consists of a series of bursts, where each burst has been processed as a separate SLC image. The individually focused complex burst images are included, in azimuth-time order, into a single sub-swath image with black-fill demarcation in between, similar to ENVISAT ASAR Wide ScanSAR SLC products.

Due to the one natural azimuth look inherent in the data, the imaged ground area of adjacent bursts will only marginally overlap in azimuth by just enough to provide contiguous coverage of the ground. The images for all bursts in all sub-swaths are resampled to a common pixel spacing grid in range and azimuth while preserving the phase information.

Figure 2: IW Sub-Swaths with Minimal Overlap

After de-bursting and merging the sub-swaths, a wide area product can be created. The TOPSAR technique greatly reduces scalloping effects over conventional ScanSAR.

Figure 3: Resulting De-Burst and Merged IW Product

The table below shows the main characteristics of the Interferometric Wide swath mode.

Characteristic Value
Swath width 250 km
Incidence angle range 29.1° - 46.0°
Sub-swaths 3
Azmiuth steering angle ± 0.6°
Azmiuth and range looks Single
Polarisation options Dual HH+HV, VV+VH
Single HH, VV
Maximum Noise Equivalent Sigma Zero (NESZ) -22 dB
Radiometric stability 0.5 dB (3σ)
Radiometric accuracy 1 dB (3σ)
Phase error

Table 1: Characteristics of Interferometric Wide swath mode

The table below shows the incidence and off-nadir angles for Interferometric Wide swath mode beams.

Beam IW1 IW2 IW3
Off-nadir angles at
min orbit altitude
27.53-32.48 32.38-36.96 36.87-40.40
Incidence angles at
min orbit altitude
30.86-36.59 36.47-41.85 41.75-46.00
Off-nadir angles at
max orbit altitude
26.00-30.96 30.86-35.43 35.35-38.88
Incidence angles at
max orbit altitude
29.16-34.89 34.77-40.15 40.04-44.28

Table 2: Angles for Interferometric Wide swath mode beams

[1] De Zan, F., & Guarnieri, A. M. (2006). TOPSAR: Terrain Observation by Progressive Scans. Geoscience and Remote Sensing, IEEE Transactions on, 44(9), 2352–2360. doi:10.1109/TGRS.2006.873853