Sentinel-1 Bursts
Table of contents
Instrument
Launches:
- Sentinel-1B: Soyuz rocket, launched 25 April 2016, from Kourou, French Guiana
- Sentinel-1A: Soyuz rocket, launched 3 April 2014, from Kourou, French Guiana
Orbit: Polar, sun-synchronous at an altitude of 693 km
Revisit time: Six days with two-satellite constellation of Sentinel-1A and 1B. Before 1B launched, revisit time for Sentinel-1A alone was 12 days.
Instrument: C-band synthetic aperture radar (SAR) at 5.405 GHz
- Interferometric wide-swath (IW) at 250 km and 5×20 m resolution, using TOPSAR
- Wave (WV) images of 20×20 km and 5×5 m resolution (at 100 km intervals)
- Stripmap (SM) at 80 km swath and 5×5 m resolution
- Extra wide swath (EW) of 400 km and 20×40 m resolution, using TOPSAR
- Supports operation in single polarization (HH or VV) and dual polarization (HH+HV or VV+VH)
- Polarization implemented through one transmit chain (switchable to H or V) and two parallel receive chains for H and V polarization
- SM, IW and EW are available in single (HH or VV) or dual polarization (HH+HV or VV+VH)
- WV is single polarization only (HH or VV)
Receiving stations: SAR data: Svalbard, Norway; Matera, Italy; Maspalomas, Spain; and via laser link through EDRS (European Data Relay System)
Telemetry, tracking and command: via Kiruna, Sweden
Main applications: Monitoring sea ice, oil spills, marine winds and waves, land-use change, land deformation, and to respond to emergencies such as floods and earthquakes
Mission: Developed, operated, and managed by various ESA establishments
Life: Minimum of seven years
Satellites: 2.8 m long, 2.5 m wide, 4 m high with 2×10 m-long solar arrays and a 12 m-long radar antenna
Mass: 2300 kg (including 130 kg fuel)
Funding: ESA Member States and the European Union Prime contractors: Thales Alenia Space, Italy, for the satellite; Airbus Defence and Space, Germany, for the SAR instrument
Content on ASF’s Sentinel web pages is adapted from the European Space Agency (ESA) Sentinel website.
SAR Modes
Links in the table below open to ESA’s website for more information.
| SAR Mode | Interferometric Wide Swath (IW) | Extra Wide Swath (EW) |
|---|---|---|
| Details | Acquired with TOPSAR. Default mode over land; 250km swath width; 5m-x-20m ground resolution. | Acquired with TOPSAR using 5 sub-swaths instead of 3, resulting in lower resolution (20m-x-40m). Intended for maritime, ice, and polar-zone services requiring wide coverage and short revisit times. |
Extractor API
Single-burst SLC datasets are virtual datasets, meaning that they are not extracted until a user requests them. For developers wishing to interact directly with the extractor application program interface (API) that is responsible for creating these datasets, documentation on the extractor API can be found at https://sentinel1-burst-documentation.asf.alaska.edu.
Image Quality
Users of Sentinel data may see quality issues similar to those below. Users are encouraged to submit examples of image-quality issues to [email protected].
Images from data close to the noise floor
Images that contain a great deal of noise have often been processed close to the noise floor (the data closest to the point where it is too noisy to be useful). The noise can look like repeating lines across an image, something like horizontal window blinds, as in the left image below. Those repeating lines are not the same as the bright spots in these images, which appear in the image below and to the right as a line of repeated bright spots or bursts. Those bright bursts are image anomalies that are not yet well understood. Also visible in these images are beam seams (see the next section).
Empty heading
Beam seams
When one image is made up of several beams, the seams can show, particularly in dark data. Beam seams are visible in many of the images on this page, including the one to the right.
Empty heading
Offsets between channels
Beams that seem to have noisy or missing data at one end, such as the dark blue edge at the top of the image, have been processed in one channel more than another (such as the HV or VH channels).
Stepped edges
Stepped ends, as in this image, are an artifact of the multi-beam scanning technology of TOPSAR and the way that ESA “slices” a data take into discrete, manageable units.
Bright burst
Bright bursts are processing anomalies that are not well understood. Bright bursts are in the upper left corner of the image below at left and in the light stripe across the image below right. Also visible in the image on the left are noise (window-blind effect), beam seams, and a bit of blue on the far left that may indicate an offset between channels.
Documents and Tools
Sentinel-1-Documents
Links and descriptions for key Sentinel-1 documents| Name | Description |
|---|---|
| Product Specification Document, ASF | Defines the ISO-compliant XML metadata for ESA’s Sentinel-1A data. |
| Sentinel-1 SAR User Guide Introduction | High-level description of instrument modes and products. Also introduction to relevant application areas, information on data distribution, product formatting, and software tools available from ESA. |
| Sentinel-1 Technical Guide | Covers an in-depth description of the mission’s products and algorithms as well as details of the SAR instrument and its performance. |
| Sentinel High Level Observation Plan, Issue 2, Revision 1 | Provides the top-level operations plan of the Sentinel missions, including space and ground segments. |
| Sentinels POD Service File Format Specifications | Useful for InSAR. Users who consult this document may also want Precision State Vectors, available from ASF from 3 September 2015. The product handbook describes the products generated as part of the provisioning of the Copernicus POD Service. |
| Sentinel Document Library | The full document library is available on the ESA website. |
Sentinel-1-Tools
links and descriptions for key Sentinel-1 tools| Name | Description |
|---|---|
| ESA Sentinel App, for iOS and Android | Powerful visualization of Sentinel product availability. Track the satellites in real time over a 3D globe, see the last and next time they have been and will be over the user’s location, and more. |
| HyP3-ISCE2 | HyP3-ISCE2 is a burst-based Python package for creating burst InSAR products using ASF’s burst SLC products. This Python package can be installed and run locally, or burst InSAR products can be requested through HyP3, ASF’s on-demand processing tool. |