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Proceeding Paper

Sentinel-1 GRD Preprocessing Workflow †

by
Federico Filipponi
Istituto Superiore per la Protezione e la Ricerca Ambientale, 48 - 00144 Roma, Italy
Presented at the 3rd International Electronic Conference on Remote Sensing, 22 May–5 June 2019; Available Online: https://sciforum.net/conference/ecrs-3.
Proceedings 2019, 18(1), 11; https://doi.org/10.3390/ECRS-3-06201
Published: 4 June 2019
(This article belongs to the Proceedings of 3rd International Electronic Conference on Remote Sensing)

Abstract

:
The Copernicus Programme has become the world’s largest space data provider, providing complete, free and open access to satellite data, mainly acquired by Sentinel satellites. Sentinel-1 Synthetic Aperture Radar (SAR) data have improved spatial resolution and high revisit frequency, making them useful for a wide range of applications. While few research applications need Sentinel-1 Ground Range Detected (GRD) data with few corrections applied, a wider range of users needs products with a standard set of corrections applied. In order to facilitate the exploitation of Sentinel-1 GRD products, there is the need to standardise procedures to preprocess SAR data to a higher processing level. A standard generic workflow to preprocess Copernicus Sentinel-1 GRD data is presented here. The workflow aims to apply a series of standard corrections, and to apply a precise orbit of acquisition, remove thermal and image border noise, perform radiometric calibration, and apply range Doppler and terrain correction. Additionally, the workflow allows spatially snapping of Sentinel-1 GRD products to Sentinel-2 MSI data grids, in order to promote the use of satellite virtual constellations by means of data fusion techniques. The presented workflow allows the production of a set of preprocessed Sentinel-1 GRD data, offering a benchmark for the development of new products and operational down-streaming services based on consistent Copernicus Sentinel-1 GRD datasets, with the aim of providing reliable information of interest to a wide range of communities.

1. Introduction

The establishment of the Copernicus Programme by the European Commission created a new paradigm in the availability and accessibility of data information, offering services based on Earth observation satellites and in situ data under six thematic Copernicus services. The Copernicus Programme has become the world’s largest space data provider, providing complete, free and open access to satellite data, mainly acquired by Sentinel satellites. The main advantages offered by Sentinel data are the improved spatial resolution and high revisit frequency, making them useful for a wide range of applications.
The Sentinel-1 mission is a constellation of two polar-orbiting satellites (Sentinel-1A and Sentinel-1B), which operate day and night, sensing with a C-band synthetic aperture radar instrument operating at a centre frequency of 5.405 GHz, allowing the acquisition of imagery regardless of weather and illumination conditions. Sentinel-1 satellite constellations acquire Synthetic Aperture Radar (SAR) data in single or dual polarization with a revisit time of 6 days. Sentinel-1 Level 1 data are distributed by the Copernicus Open Access Hub under two product types: Ground Range Detected (GRD) and Single Look Complex (SLC).
Sentinel-1 level-1 GRD products consist of focused SAR data that have been detected, multi-looked and projected to ground range using an Earth ellipsoid model. The ellipsoid projection of the GRD products is corrected using the terrain height, specified in the product general annotation, that varies in azimuth but is constant in range. After performing a multi-looking separately for each burst, a ground range detected image is generated merging all bursts in all sub-swaths. The Sentinel-1 GRD scene is composed of square pixels with reduced speckle, due to the multi-look processing, representing only the detected amplitude (the phase information is discarded).

2. Workflow

A standard generic workflow to preprocess Copernicus Sentinel-1 GRD data is presented here. The workflow was created in order to be used within the Sentinel application platform (SNAP), a common architecture for all Sentinel satellite toolboxes. The processing graph in ‘xml’ format allows the processing of Sentinel-1 GRD using the command line graph processing framework, which allows for batch processing of large datasets.
The preprocessing workflow consists of seven processing steps, designed to best reduce error propagation in subsequent processes, described hereafter in separate subsections. The code to perform the preprocessing workflow is available on the GitHub repository [1] and in the Supplementary Materials as Computer Code 1.

2.1. Apply Orbit File

Orbit state vectors, contained within the metadata information of SAR products, are generally not accurate. The precise orbits of satellites are determined after several days and are available days-to-weeks after the generation of the product. The operation of applying a precise orbit available in SNAP allows the automatic download and update of the orbit state vectors for each SAR scene in its product metadata, providing an accurate satellite position and velocity information.

2.2. Thermal Noise Removal

Sentinel-1 image intensity is disturbed by additive thermal noise, particularly in the cross-polarization channel [2]. Thermal noise removal reduces noise effects in the inter-sub-swath texture, in particular, normalizing the backscatter signal within the entire Sentinel-1 scene and resulting in reduced discontinuities between sub-swaths for scenes in multi-swath acquisition modes. The thermal noise removal operator available in SNAP for Sentinel-1 data can also re-introduce the noise signal that could have been removed during level-1 product generation, and update product annotations to allow for re-application of the correction [3]. Sentinel-1 level-1 products provide a noise look-up table (LUT), provided in linear power, for each measurement data set and used to derive calibrated noise profiles matching the calibrated GRD data [3].

2.3. Border Noise Removal

While generating level-1 products, it is necessary to correct the sampling start time in order to compensate for the change of the Earth’s curvature. At the same time, azimuth and range compression leads to radiometric artefacts at the image borders. The border noise removal algorithm [4], available as an operator in SNAP, was designed in order to remove low intensity noise and invalid data on scene edges.

2.4. Calibration

Calibration is the procedure that converts digital pixel values to radiometrically calibrated SAR backscatter. The information required to apply the calibration equation is included within the Sentinel-1 GRD product; specifically, a calibration vector included as an annotation in the product allows simple conversion of image intensity values into sigma nought values. The calibration reverses the scaling factor applied during level-1 product generation, and applies a constant offset and a range-dependent gain, including the absolute calibration constant.
In the proposed preprocessing workflow, a LUT to produce sigma nought values is proposed, in order to generate radiometrically calibrated SAR backscatter with respect to the nominally horizontal plane. Sigma specifies the strength of reflection in terms of the geometric cross section of a conducting sphere, and represents the radar cross section of a distributed target over that expected from an area of one square meter. The sigma nought has a significant variation with the incidence angle, wavelength, and polarisation, as well as with properties of the scattering surface.
Figure 1. Sentinel-1 Ground Range Detected (GRD) preprocessing workflow.
Figure 1. Sentinel-1 Ground Range Detected (GRD) preprocessing workflow.
Proceedings 18 00011 g001

2.5. Speckle Filtering

Speckle, appearing in SAR images as granular noise, is due to the interference of waves reflected from many elementary scatterers [5]. Speckle filtering is a procedure to increase image quality by reducing speckle. When such a procedure is done at an early processing stage of SAR data, speckle is not propagated in ongoing processes (i.e., terrain correction or conversion to dB). Speckle filtering is not advisable when there is an interest in the identification of small spatial structures or image texture, since it might remove such information. The refined Lee filter has been found to be superior, with respect to other single product speckle filters, for visual interpretation, because of its ability to preserve edges, linear features, and point target and texture information [5]. More recently, multitemporal speckle filters have been developed to reduce speckle, taking advantages from multiple SAR observations in time. The proposed preprocessing workflow includes a speckle filtering step, which could be skipped by selecting ‘None’ as the filter type. Currently, one of the following filters is available in the SNAP single product speckle filter operator: ‘Boxcar’, ‘Median’, ‘Frost’, ‘Gamma Map’, ‘Lee’, ‘Refined Lee’, ‘Lee Sigma’, ‘IDAN’.

2.6. Range Doppler Terrain Correction

SAR data are generally sensed with a varying viewing angle greater than 0 degrees, resulting in images with some distortion related to side-looking geometry. Terrain corrections are intended to compensate for these distortions so that the geometric representation of the image will be as close as possible to the real world. Range Doppler terrain correction is a correction of geometric distortions caused by topography, such as foreshortening and shadows, using a digital elevation model to correct the location of each pixel. The range Doppler terrain correction operator available in SNAP implements the Range Doppler orthorectification method [6] for geocoding SAR scenes from images in radar geometry. It makes use of available orbit state vector information in the metadata, the radar timing annotations, and the slant to ground range conversion parameters together with the reference digital elevation model data to derive the precise geolocation information [3]. The target Coordinate Reference System (CRS) can be selected and optionally set to match the UTM zone of the overlaying Sentinel-2 granules. The operator allows the selection of the image resampling method and the target pixel spacing in the target CRS. This processing step allows the spatial snapping of Sentinel-1 GRD products to Sentinel-2 MSI data grids, in order to geolocate data to a common spatial grid and promote the use of satellite virtual constellations.

2.7. Conversion to dB

As a last step of the preprocessing workflow, the unitless backscatter coefficient is converted to dB using a logarithmic transformation.

3. Conclusions

A standard generic workflow to preprocess Copernicus Sentinel-1 GRD data was presented. The workflow aims to produce a set of preprocessed Sentinel-1 GRD data, offering a benchmark for the development of new products and operational down-streaming services based on consistent Copernicus Sentinel-1 GRD data.
The workflow applies a series of standard corrections, and to apply a precise orbit of acquisition, remove thermal and image border noise, perform radiometric calibration, and apply range Doppler and terrain correction. Additionally, Sentinel-1 GRD products can be spatially coregistered to Sentinel-2 MSI data grids, in order to promote the use of satellite virtual constellations by means of data fusion techniques.

Supplementary Materials

The following are available online at www.mdpi.com/2504-3900/18/1/11/s1.

Acknowledgments

This work contains modified Copernicus Sentinel data (2019). The author is grateful to the many individuals working on the development of free and free open-source SNAP software for supporting the sharing of knowledge.

Conflicts of Interest

The author declares no conflict of interest.

References

  1. github.com, Ffilipponi Repository—Sentinel-1_GRD_Preprocessing: Standard Workflow for the Preprocessing of Sentinel-1 GRD Satellite Data. Available online: https://github.com/ffilipponi/Sentinel-1_GRD_preprocessing (accessed on 21 May 2019).
  2. Park, J.W.; Korosov, A.; Babiker, M. Efficient thermal noise removal of Sentinel-1 image and its impacts on sea ice applications. In Proceedings of the EGU General Assembly Conference Abstracts, Vienna, Austria, 23–28 April 2017; Volume 19, p. 12613. [Google Scholar]
  3. SNAP Software, Help Document 2019. Available online: https://step.esa.int/main/toolboxes/snap (accessed on 1 May 2018).
  4. Guillaume, H. Masking “No-value” Pixels on GRD Products generated by the Sentinel-1 ESA IPF. ESA Tech. Rep. 2015; Reference MPC-0243, Issue 1.0. [Google Scholar]
  5. Lee, J.S.; Jurkevich, L.; Dewaele, P.; Wambacq, P.; Oosterlinck, A. Speckle filtering of synthetic aperture radar images: A review. Remote Sens. Rev. 1994, 8, 313–340. [Google Scholar] [CrossRef]
  6. Small, D.; Schubert, A. Guide to ASAR Geocoding; ESA-ESRIN Technical Note RSL-ASAR-GC-AD; University of Zurich: Zurich, Switzerland, 2008; Volume 1, p. 36. [Google Scholar]

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MDPI and ACS Style

Filipponi, F. Sentinel-1 GRD Preprocessing Workflow. Proceedings 2019, 18, 11. https://doi.org/10.3390/ECRS-3-06201

AMA Style

Filipponi F. Sentinel-1 GRD Preprocessing Workflow. Proceedings. 2019; 18(1):11. https://doi.org/10.3390/ECRS-3-06201

Chicago/Turabian Style

Filipponi, Federico. 2019. "Sentinel-1 GRD Preprocessing Workflow" Proceedings 18, no. 1: 11. https://doi.org/10.3390/ECRS-3-06201

APA Style

Filipponi, F. (2019). Sentinel-1 GRD Preprocessing Workflow. Proceedings, 18(1), 11. https://doi.org/10.3390/ECRS-3-06201

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