The Sentinel-1 Constellation – A new era of operational InSAR
Abstract:
Sentinel-1 acquires radar data in a novel mode, known as Interferometric Wide Swath or TOPS (Terrain Observation with Progressive Scans in azimuth) mode. TOPS mode has some advantages, the most significant of which is that a 250 km wide image can be acquired without the scalloping effect that is seen in conventional ScanSAR amplitude images. However, because the Doppler centroid varies in azimuth, phase artefacts are introduced in TOPS-mode interferograms unless the images are co-registered with an azimuth accuracy of ~5 cm. This, and the bursted nature of TOPS data, introduces new challenges and opportunities to InSAR processing. We show how the required coregistration accuracy can be achieved with an end-to-end geometric approach, and by exploitation of the view angle diversity in burst and swath overlap regions. We also discuss different strategies for when and how to stitch the bursts, which depend on the application domain and processing methodology.
The systematic acquisitions and free and open data policy provide new opportunities for routine analysis and operational applications of InSAR. COMET (* http://comet.nerc.ac.uk) aims to provide processed results for all the tectonic and volcanic regions of the planet, and we will present preliminary results of our processing system from test regions in Turkey and Mexico. By 2034, there will be a 20 year archive of systematic radar acquisitions from the Sentinel-1 program. We will end this presentation with a speculative view from 2034 on the main achievements of the program.
*COMET is the UK NERC's Centre for the Observation and Modelling of Earthquakes, Volcanoes and Tectonics.
