NovaSAR-1 — A low cost S-band SAR mission on a Minisatellite
NovaSAR-1 is a joint technology demonstration initiative of SSTL (Surrey Satellite Technology Ltd.), UK, and Airbus DS (former EADS Astrium Ltd, Stevenage, UK), funded by the UK Government via the UKSA (UK Space Agency). The overall objective is to make SAR (Synthetic Aperture Radar) observation missions more affordable to a customer base and to open up new application-oriented in the microwave region of the spectrum.
In the past decade, programs such as the DMC (Disaster Monitoring Constellation) have proven that a low cost, small satellite approach can provide solutions for medium resolution EO (Earth Observation) applications. However, these have all been optical missions. SAR missions have well known night time and all weather advantages over optical missions but have not yet made the same evolutionary step. To date, SAR satellites have mostly served large budget, institutional missions with a performance driven, rather than applications driven, design. 1) 2) 3) 4) 5) 6) 7) 8) 9)
A SAR payload design, which optimizes all imaging parameters (resolution, swath, sensitivity, duty cycle etc.), leads to a satellite design which is at odds with a low cost approach. An applications driven approach, focused on medium resolution applications, enables solutions that can make the evolutionary step to the low cost, small satellite arena. In the same way that low cost optical satellites have enabled numerous optical EO programs, a low cost approach can bring SAR solutions to a wider EO user community.
Rather than follow a traditional development with a flow down of requirements from an external customer, our approach has been to design a baseline mission which answers the question “what imaging performance can we achieve with a spacecraft that can be built and operated at low cost, and is compatible with low cost launches?” This approach leverages heavily SSTL’s experience of low cost optical EO missions and Astrium’s experience of SAR missions.
NovaSAR-1 provides medium resolution (6-30 m) imagery ideal for applications in the following fields:
- flood monitoring
- agricultural crop assessment
- forest monitoring (temperate and rain forest)
- land use mapping
- disaster management
- maritime applications (e.g. ship detection, oil spill monitoring, maritime safety, and security of defence applications). 10)
However, applications that can be served by a medium resolution (10-30 m) system are not limited to the list above.
In November 2011, the British government announced an investment of £ 21 M to SSTL to assist in the development and launch of the first NovaSAR spacecraft, an innovative and highly competitive new spaceborne radar remote sensing program, in the international market. 11) 12) 13)
The industrial team developing the NovaSAR spacecraft is led by SSTL. NovaSAR-1 combines heritage avionics (of the SSTL-300 bus) with a new structural design, to accommodate a payload, developed under a joint initiative between SSTL and Astrium. The design lifetime of the satellite is 7 years. A trade-off between imaging requirements, drag and propulsion subsystem mass/NRE/costs settled on an optimum orbital altitude of 580 km. 14) 15)
Figure 1: NovaSAR-1 spacecraft with payload antenna (left), component accommodation (center), and solar panel (right), image credit: SSTL, Airbus DS
EPS (Electrical Power Subsystem):
Super capacitor experiment: The objective is to test a new energy storage technology in space - by providing a high-power energy source for relatively short operating times (to make for instance a radar operation possible on a small spacecraft. 16)
To provide a highly reliable system with a high probability of meeting the 7+ year lifetime requirement, SSTL’s platforms make use of wide-ranging redundancy architectures. The EPS architecture is shown in Figure 2. There are two redundant CAN data buses and two of each of the key platform units, each connected to each data bus allowing cross strapping of units. Additionally some of the units provide internal redundancy e.g. triple redundant program memory and EDAC protection on the data memory.
Figure 2: Electrical architecture of the NovaSAR-1 platform (image credit: SSTL, Ref. 15)
SSTL is developing a prototype of a super-capacitor based power system, including a capacitor charge regulator (with maximum peak power tracking and control charging), a cell monitoring and management module (to monitor and protect each cell), and capacitor-bank (energy storage module). A COTS LIC (Lithium-Ion Capacitor) is employed in the capacitor-bank. The LIC uses activated carbon as a positive electrode that makes an electric double layer, and has lithium-ions pre-doped into a carbonaceous negative electrode.
Avionics: NovaSAR-1 features the same avionics as those on the on the SSTL-300 bus of NigeriaSat-2.
The NovaSAR-1 spacecraft has a mass of 430 kg, a xenon propulsion system, and a design life of 7 years.
RF communications: The TT&C data are transmitted in S-band (2025-2110 MHz, 2200-2290 MHz); the payload data are downlinked in X-band (8.025-8.4 GHz) at a data rate of 500 Mbit/s. An onboard data storage capacity of 544 GByte is provided (Ref. 15).
Figure 3: Photo of the NovaSAR platform during assembly and integration in November of 2014 (image credit: SSTL) 17)
Figure 4: Artist's rendition of the NovaSAR radar platform in orbit (image credit: SSTL)
• August 16, 2018: SSTL has signed an agreement with Antrix Corporation Limited, the commercial arm of ISRO ( Indian Space Research Organisation), for the launch into a 580 km sun-synchronous orbit of NovaSAR-1 (also referred to as NovaSAR-1), a small Synthetic Aperture Radar (SAR) satellite, and SSTL S1-4, a high resolution Earth observation minisatellite. The two satellites will launch on PSLV-C42, due to lift-off in September 2018. 18)
- NovaSAR-1 is a technology demonstration satellite mission designed to test the capabilities of a new low cost S-band SAR platform. The spacecraft was designed and manufactured by SSTL, with an S-band SAR payload developed by Airbus Defence and Space in Portsmouth, and an Automatic Identification Receiver (AIS) supplied by COM DEV to track ships at sea. NovaSAR-1 will be operated from SSTL’s Spacecraft Operations Center in Guildford, UK.
- The UK Space Agency has invested £21M in the development of NovaSAR-1 and will benefit from access to data from the spacecraft, significantly boosting the UK’s sovereign Earth observation capabilities and leveraging additional inward investment to the UK by creating highly skilled jobs in the UK space industry, and stimulating the growth of data analysis services.
- Also on the PSLV-C42 launch will be the SSTL S1-4, a sub-meter resolution Earth observation satellite with a mass of 440 kg that will further enhance SSTL’s existing in-orbit observation capabilities.
• September 26, 2017: SSTL signed an agreement in Adelaide today at the IAC (International Astronautical Congress) to provide Australia’s CSIRO (Commonwealth Scientific and Industrial Research Organisation) a 10% share of the tasking and data acquisition capabilities from NovaSAR-1, a first-in-class small radar satellite due for launch later this year. 19)
- NovaSAR-1 is a technology demonstration mission designed to complement much larger, complex radar satellites with a smaller, lighter and more cost effective platform that delivers Earth observation Synthetic Aperture Radar imagery day and night, and through cloud cover. Managing the energy use on board the small SAR platform has been made possible by using a new, highly efficient S-band solid-state amplifier technology and flying an innovative S-band SAR payload developed by Airbus UK in Portsmouth .
- Speaking at the IAC in Adelaide, Luis Gomes, SSTL’s Commercial Director said “We are delighted to be here in Adelaide for the IAC, and to see the Australian government’s “Big Country, Big Sky, Big Ideas” slogan underpinned by today’s announcement of our partnership with CSIRO on the NovaSAR-1 mission. We anticipate that CSIRO will greatly enhance Australia’s sovereign Earth observation capability with the addition of SAR data, particularly for this continent which has a tropical climate and a large coastline territory.”
- Gomes also confirmed that further data shares on the mission are available, commenting “With the launch of the satellite due later this year, we have a number of discussions open with potential partners on the mission but we also welcome new partners looking to take a data and tasking share in NovaSAR-1.”
- The agreement gives CSIRO tasking priorities and the ability to access the raw data directly from the satellite, and a license to use and share the data with other Australian companies and organizations over an initial 7 year period.
• The NovaSAR-1 payload was delivered by Airbus DS UK to SSTL for platform integration in November 2015.
• The flight build commenced in January 2014 and was completed on schedule and on budget in July 2015.
• The Engineering Qualification program was completed in Q1 2014.
Launch: The NovaSAR-1 minisatellite, along with SSTL S1-4, a high resolution Earth observation minisatellite of SSTL, were launched on 16 September 2018 (16:38 UTC) on the PSLV-C42 vehicle of ISRO from SDSC (Satish Dhawan Space Center) from SHAR, ISRO's launch center on the south-east coast of India, Sriharikota. Launch provider: Antrix Corporation Ltd., the commercial arm of ISRO. 20) 21)
Sun-synchronous orbit: altitude of ~580 km, inclination of 97.5º, LTAN (Local Time on Ascending Node) = 10:30 hours.
For a description of the SSTL S1-4 mission, see the DMC3 file (Disaster Monitoring Constellation-3) / TripleSat Constellation of 21AT / Beijing-2 on the eoPortal. The SSTL S1-4 satellite is identical to the three DMC3 satellites in the TripleSat Constellation, launched in 2015. It has a mass of 440 kg and is capable of acquiring multiple targets in one pass and will utilize spot, strip and mosaic imaging modes and 45 degree off-pointing agility for a range of applications including urban planning, agricultural monitoring, land classification, natural resource management and disaster monitoring.
Figure 5: PSLV C42 launch of NovaSAR-1 and SSTL S1-4 on 16 September 2018 (image credit ISRO/Antrix)
• August 2019: The first NovaSAR image turned out to be a fortuitous anomaly and there followed a period of fixing bugs in mode definitions, tasking software, on board computer software and ground data processing. In parallel, commissioning activities, relating to both space segment and ground segment, progressed. The NovaSAR radar antenna is a planar phased array. Although the aperture is small for this type of system it has sufficient phase centers to support flexible modes of operation. A number of modes have been implemented and modes will be added through the mission at the request of mission partners. The following operational modes in Table 1 have so far been implemented and functionally tested. 22)
Figure 6: NovaSAR first image (image credit: SSTL)
- Being an S-band instrument, the NovaSAR payload provides data in an underutilized frequency band. With a wavelength between L- and C-band there is interest in seeing how much information is available relating to vegetation penetration and soil moisture. Proper studies are required to quantify these effects. To the eye images look information rich and multipolar examples in particular suggest there is plenty of information content to be exploited by classification techniques.
- From images captured so far there is good potential for exploitation by ocean applications (Figures 7, 8, 9, 10). Wave structure, bathymetry and sea ice all show up well (Figure 11). Responses from ships and ship wakes suggest a direct read across of ship detection techniques developed on other data. The darkness of calm sea areas suggests good potential for oil spill identification.
- A unique feature built into the NovaSAR payload is the ability to support long pulse durations. The bulk capacitance associated with the SSPA in each phase center of the antenna array has been oversized to support low pulse repetition frequencies with long duration pulses. Although not useful for normal SAR imaging, wider swaths can be captured at the expense of along-track ambiguities. When imaging open ocean areas in this mode NESZ exceeds ocean backscatter levels. Hence, if SAR focusing is applied to the data ships are represented as bright responses with ambiguities against a background which is the noise floor of the instrument modified by scalloping from radiometric correction. Tests to date have produced expected results. Since the resultant level 1 data is somewhat unique there are currently no bespoken ship detection algorithms but it is hoped mission partners will develop techniques to exploit this mode.
- As well as the primary SAR payload, NovaSAR also carries a secondary AIS payload. To make data handling convenient the AIS will capture AIS messages and store a separate file for each hour it is operational. AIS antennas are omnidirectional and transmissions are received anywhere within line of sight of the satellite. Analysis of data indicates many thousands of AIS transmissions are captured per hour, although many of these are coastal stations and static facilities. It is also apparent from lat/longs outside line of sight of the orbit that there are many erroneous or malicious rogue transmissions.
Figure 12: NovaSAR AIS data showing “suspect”transmissions (white), image credit: SSTL
- An obvious advantage of having both SAR and AIS payloads on the same spaceborne platform is the potential to associate the two types of data. An initial attempt shows that a close correlation can be achieved if the time delta is favorable. In the example the offset between the ship response in the SAR image and the lat/long pair of the AIS messages is consistent highlighting an error in the geo-referencing of the SAR data. Since the data was captured near a port the ships’ AIS transceivers are transmitting every few seconds. Hence, multiple successive lat/long pairs are captured for each ship showing a nice correlation with the direction indicated by the shape of the ship response in the SAR image.
Figure 13: NovaSAR AIS data in Sydney Harbor (image credit: SSTL)
- Post launch commissioning activities have included a calibration campaign on the SAR payload to optimize and characterize its performance. Typical measurements using passive targets where carried out: corner reflectors for known radar cross section point targets; rain forest for wide area homogenous targets; calm water, salt flats and airport runways for low backscatter dark targets. Radiometric stability looks good with a standard deviation of <0.4 dB. The mission requirement for geolocation error is 50 m. When a correction is made to account for the difference between the ellipsoid height used to generate the level 1 product and the actual terrain height the geolocation requirement is easily achieved and is typically <10 m.
Figure 14: NovaSAR-1 ship detection mode (image credit: SSTL)
- Future plans: CarbSAR — Based on experience with NovaSAR, and leveraging improvements in technology, SSTL has developed a follow-on SAR spacecraft product. ”CarbSAR” is an ultra-low cost SAR satellite intended for operation in SAR or mixed service Earth Observation constellations, providing very high resolution across relatively small scenes with the potential for high temporal resolution. CarbSAR utilizes the platform heritage of the Carbonite optical satellite series and combines it with an innovative deployable X-band SAR antenna and payload.
Table 2: CarbSAR specifications
Figure 15: CarbSAR is part of a series of small EO spacecraft (image credit: SSTL)
- In summary, as SAR systems become more popular with commercial companies supporting data analytics applications, there is significant room for a variety of systems that utilize small SAR spacecraft in order to address some specific markets. These system require low-cost SAR systems with payload characteristics matched to the specific market, rather than the general purpose SAR spacecraft launched under some national and space agency projects. Such small SAR spacecraft may need to be deployed into multi-plane constellations in order to observe targets at different times of the day.
- NovaSAR-1, and its follow-on SAR concept CarbSAR address two particular variants of small SAR spacecraft addressing very specific applications, and have been presented as examples of how small SAR missions can help address specific markets and end-users. NovaSAR-1 results from the first year of operations show significant promise in the use of S-band radar for a range of commercial applications including maritime surveillance.
• November 23, 2018: SSTL has today released the first SAR (Synthetic Aperture Radar) images taken from orbit by NovaSAR-1, a technology demonstration mission launched into a 580 km sun-synchronous orbit on 16 September 2018. 23)
- The S-band SAR sample images released today have been acquired using the satellite’s stripmap mode at 6 m resolution and are 20 km wide by 87km long. They were taken over Sydney Harbor and Cairo, Egypt.
Figure 16: NovaSAR-1 SAR image of size 20 x 87 km at 6 m resolution of Sydney Australia, acquired at night in November 2018 (image credit: SSTL)
Figure 17: NovaSAR-1 SAR image at 6 m resolution of Cairo, Egypt (image credit: SSTL)
- Sam Gyimah, the UK’s Science and Education Minister, visited SSTL today where he toured the Company’s satellite assembly and operations facilities, and viewed the new images from NovaSAR-1. The Minister said: “Yet again we can see UK research and innovation that is truly out of this world. This ‘eye in the sky’ can capture an image a dozen times wider than the Strait of Dover and the data it provides can help crack problems from illegal shipping to alerting us to damaging pollution that needs to be countered. This satellite, backed by a £21 million investment from the UK Government, is a great example of how we are working with the space sector through our modern Industrial Strategy to remain at the forefront of pioneering science and exploration.”
- Andrew Cawthorne, Director of Earth Observation at SSTL said “We have worked closely with the SAR experts at Airbus in Portsmouth to develop NovaSAR-1 and the whole team is delighted with these first results - the outcome of space engineering expertise, ingenuity and collaboration. Over the coming weeks our spacecraft operators will continue to test the capabilities of the spacecraft as we task the satellite to image locations around the world, working towards the start of service delivery to our mission partners in the near future.”
- Mission partners signed up for capacity from NovaSAR-1 include the UK Space Agency, Australia’s Commonwealth Scientific and Industrial Research Organization (CSIRO), and the Indian Space Research Organization (ISRO).
- The image of Sydney was taken at night and cropped images taken from the original show Sydney Harbor Bridge, Sydney Opera House, The Royal Botanic Garden, Bondi beach and several boats crossing the harbor. A second close up from the original image shows small boats moored in the natural harbor at Church Point, north of Sydney in a demonstration of the usefulness of SAR for detecting vessels of many different sizes and types, particularly at night or through cloud cover.
- The image of Cairo shows the River Nile flowing from Upper Egypt through Cairo and down towards Beni Suef. Urbanization, cultivation along the Nile, and the non-irrigated desert areas are clearly distinguishable. Cropped images taken from the original show The Great Pyramids of Giza, and the Red Pyramid and Bent Pyramid near Dahshur.
- Synthetic Aperture Radar is a powerful tool for monitoring the Earth from space due to its ability to see through clouds and image the Earth night and day, and NovaSAR-1 is the world’s first commercial SAR satellite to be operated at a 10:30 equator crossing time, providing time diversity for radar observations by affording increased daylight imaging opportunities in addition to night acquisitions.
- NovaSAR-1 was designed and manufactured by SSTL, with an S-band SAR payload developed by Airbus Defence and Space in Portsmouth and an AIS (Automatic Identification System) receiver supplied by Honeywell Aerospace. The SAR payload has a dedicated maritime mode designed with a very wide swath area of 400 km to enable the monitoring of the marine environment, and will provide direct radar ship detection information simultaneously with AIS ship tracking data to assist with the identification and tracking of sea-going vessels. In addition to operating in maritime mode, NovaSAR-1 has been optimized with three additional imaging modes, including a six meter resolution imaging mode, for a range of other applications such as flood monitoring and agricultural and forestry applications. The satellite has been designed to offer a high throughput of data, observing in a variety of polarization combinations to add additional information to acquisitions in the form of ‘color’.
- NovaSAR-1 is operated in orbit from SSTL’s Spacecraft Operations Centre in Guildford UK.
Sensor complement: (S-SAR, AIS)
S-SAR (S-band Synthetic Aperture Radar):
The innovative S-SAR payload is being developed collaboratively by Airbus Defence & Space Ltd (formerly EADS Astrium Ltd.) of Portsmouth, UK, and SSTL, the payload activities are led by Airbus DS, UK. 24) 25) 26) 27) 28)
Background: The S-SAR payload is a derivative from Astrium’s airborne radar demonstrator technologies with the benefit of significant heritage and risk reduction from the airborne demonstrator development: 29)
• architecture and implementation of back end radar electronics
• development and demonstration of imaging modes
• provision of data sets to support proving of SAR applications
• key enabler for low cost approach to space-based radar instruments.
Demonstrator developed by Astrium over the last decade:
• designed and built under UK government contract and Astrium R&D
• system/instrument exercised on extensive flight trials campaigns
• has been an important tool as a radar test bed to provide support to SAR research and development
• SAR image processor developed to evaluate acquired imagery.
Detailed trade-off analyses were performed to ascertain the performance of an S-band Phased Array Antenna of this architecture, with many phase-center configurations considered. The result is an innovative Front-End Architecture (low phase center count) with 18 x 100 W phase centers, arranged in a 3-column by 6-column configuration, all accommodated in a 3 m x 1 m panel.
Figure 18: Low phase center count antenna (image credit: Airbus DS)
The S-band antenna is a microstrip patch phased array of ~ 3 m x 1 m in size. The antenna size drives the satellite size which has been deliberately constrained to meet low cost launch vehicle requirements.
The payload can transmit and receive on both horizontal and vertical polarizations. The baseline payload configuration can be operated to produce imagery in polarimetric mixes that include single polar (HH, VV), dual polar (any 2 from HH, VV, HV or VH), tri-polar (any 3 from HH, VV, HV or VH), or quad polar (HH, VV, HV & VH) .
Table 3: S-SAR payload parameters
The payload front-end RF electronics are mounted on the reverse side of the antenna panel making the payload front-end self-contained. The NovaSAR platform has been designed to support payloads that operate in different frequency bands.
Traditional space qualified TWTA (Traveling Wave Tube Amplifier) reflectors offer good efficiency but are relatively expensive. GaAs SSPAs (Solid-State Power Amplifiers) can be implemented using COTS technology but do not offer such good efficiency. Recently, the terrestrial use of GaN (Gallium Mitride) technology in SSPAs has become mature at frequencies up to S-band and offers efficiencies > 40%. Therefore, our payload has been designed around S-band GaN SSPAs.
By using GaN SSPAs and designing for an imaging duty cycle of ≥ 2 minutes/orbit (~2%) the orbit average power consumption of the payload is in the region of 100 W. This greatly helps to reduce the overall spacecraft mass and volume, and hence costs associated with manufacturing, test, transportation, launch etc. The 2 minute imaging period has been selected as a baseline to enable an 800 km long strip of imaging each orbit that is well suited to regional observations, comparable with the size of many nation states. In fact, depending on operational mode and downlinking opportunities, larger payload duty cycles can also be supported by the NovaSAR-1 satellite providing the overall 2% duty is respected across a number of orbits.
The payload can transmit and receive on both horizontal and vertical polarizations. The baseline payload configuration can be operated to produce imagery in polarimetric mixes that include single polar (HH, VV), and then by trading swath width and/or resolution for more diverse polarimetric capability, dual polar (any 2 from HH, VV, HV or VH) or tripolar (any 3 from HH, VV, HV or VH).
The front surface of the payload frontend consists of the SAR antenna panel with a total of 18 pairs of sub-arrays, each pair forming an individually controllable phase center. The payload frontend RF electronics are mounted on the reverse side of the antenna panel, making the payload frontend self-contained. Six beam control units apply transmit and receive phase adjustments to the eighteen phase centers. Each phase center consists of a transmit unit (100 W RF o/p), a power conditioning unit, a receive unit and a radiator unit. The radiator units are arranged in three columns of six sub-array pairs, each having 24 patches (Figure 19).
This arrangement enables ScanSAR modes with up to around five subswaths with acceptable grating lobe performance. In fact, the use of the longer wavelength at S-band improves the grating lobe performance, enabling more elevation steering than would be possible with just six elevation phase centers at shorter wavelengths. With each phase center delivering around 100 Watts of peak RF power, GaN devices were readily available, and measures to avoid multipaction remained practicable. The total DC power demand was also kept within achievable limits for the small satellite platform with this arrangement.
Bandwidth: With an ITU regulation bandwidth limit of 200 MHz at S-band, the six-element subarrays are sufficiently short for this bandwidth to be readily achieved. However, in terms of power aperture product, the need for credible sensitivity performance limited the bandwidth used on NovaSAR-1 to around 100 MHz, even though the payload can implement up to 200 MHz.
Antenna size considerations: Clearly a 3m2 antenna will be restricted in terms of access capability due to early range ambiguity degradation with increasing incidence angle. Indeed, an S-band SAR solution to access out to 50° incidence (single-polar) would typically need around 14m2 of antenna area. However with careful tuning of the processed Doppler bandwidth and the pulse repetition frequency, an antenna area of just 3m2 can deliver access out to 31° with acceptable ambiguity performance, achieving an access width of around 125 km for 20-31° incidence. Additional access width can be achieved (for compatible applications) by venturing below the traditional 20° incidence angle lower limit. Extending down to 16° incidence, for example, widens the access to 165 km.
It is important to note that the design of the front-end for NovaSAR-1 provides a fully scalable solution, so that a larger antenna can easily be realized simply by building more of the same phase center units and configuring them with the required number of rows and columns. The performance and access will then improve accordingly.
The NovaSAR-1 platform has been designed to support payloads that operate in different frequency bands. Efficient SSPA technologies in other bands are being investigated so that alternate payload frontends can be implemented in the future.
The applications focused approach to the NovaSAR-1 system design has resulted in a platform where both solar panels and the payload antenna can follow fixed, body mounted forms. Hence, the satellite is without deployable appendages, a unique achievement for a SAR satellite.
Baseline imaging modes: An orbit altitude of 580 km has been used to derive the baseline imaging modes given in Table 4. Mode 1 is expected to be the mode most commonly used for the target applications identified. Mode 2 is an unconventional, ultra-wide swath mode intended for ship detection. Modes 1, 2 and 4 are ScanSAR modes. Mode 3 is a Stripmap mode which trades swath width for an improved resolution. However, this reduced swath can be selected from a 150 km access range. Mode 4 is similar to mode 1, but trades resolution to get a wider swath. Modes 1, 3 and 4 have options to increase the available incidence angles and reduce revisit times.
Maritime Mode: An additional, experimental, mode was also defined, known as Maritime Mode, which implements a novel low PRF mode for wide-area ship detection in the open ocean. This is expected to enable effective ship detection via deliberately azimuth ambiguous ScanSAR imaging over a swath more than 400 km wide in the 32-56° incidence angle range. Analysis of S-band airborne imagery of ships using the Airborne SAR Demonstrator developed at Airbus DS in Portsmouth has enabled tuning of the baseline mode design to maximize detection probability and swath width, while maintaining an acceptable false alarm rate of less than 1 image pixel in 107.
Polarimetric capability: Since the antenna is dual polarized (H and V), the instrument is capable of transmitting H or V pulses. To keep cost low, a single receive chain is implemented, but this can receive either H or V in any given echo window, enabling incoherent polarimetric imaging to be acquired. Sensitivity is compatible with primarily using HH and/or VV imaging, since signal to noise ratios will be limited in cross-polar operation for typical rural distributed scenes. However cross-polar operation is available and may also be useful in some circumstances, for example for detecting ships at low incidence angles where unwanted sea clutter will be heavily attenuated in cross polar imagery while the target cross section remains high.
The payload is highly flexible and is capable of delivering a wider range of imaging modes than those baseline modes presented in Table 4 which have been designed for maximum coverage. In-orbit tuning of beam shape and PRF (Pulse Repetition Frequency) can be used to define new modes.
Ship detection is one of the main SAR applications since the ships are usually built from large metal sheet and therefore detectable in SAR imagery; commonly a ship detection algorithm consists of three stages: pre-processing (land masking), detection (also known as prescreening) and discrimination. The flow-chart of the ship detection scheme is shown in Figure 20, where all the steps are highlighted and elements of novelty are introduced in each stage Ref. 30).
In the pre-processing, a land mask is obtained considering the different statistics between the sea and the land’s backscattered field; the detection stage isolates the bright points over the sea background employing a CFAR (Constant False Alarm) method; while the ships are retrieved, in the discrimination step, by evaluating the scattering contributions of the possible targets detected in the previous stage.
Figure 20: Ship detection flow-chart. The rounded rectangles represents input and output data, while the rectangles are all the processes needed to perform the algorithm. The scheme is divided into three sections: pre-processing (masking), detection (CFAR) and discrimination (clustering, ambiguities removal and scattering evaluation), image credit: SSC, SSTL
Calibration: The architecture of the front-end subsystem is shown in Figure 21. Calibration paths have been included to enable characterization of the phase center distortions for replica generation, antenna beam pattern maintenance, and system diagnostics. The calibration scheme is based on the scheme developed for ASAR on ENVISAT, with a P1 path that includes the transmit electronics but bypasses the receive electronics, a P2 path that includes the receive electronics but bypasses the transmit electronics, and a P3 path that bypasses both the transmit and the receive electronics. The P1 and P2 paths each have an H and a V variant.
Backend (central electronics): A separate, but directly relevant, development at Airbus DS in Portsmouth is the NIA (New Instrument Architecture) generic space radar central electronics. This equipment exploits the power and flexibility of the Xilinx Virtex 5 (XQR5V) FPGA (Field Programmable Gate Array). The XQR5V is the first high performance RAM based FPGA to integrate effective single event effect mitigation into its core architecture. This has created the opportunity to develop a truly generic backend solution that can easily be applied to a very wide range of space radar missions with minimal non-recurring cost. In addition, the power of the Virtex 5 enables functionality that would normally be implemented within a dedicated CPU module within the central electronics to be moved into the FPGA, making the CPU module potentially unnecessary. Missions which are able to omit the CPU module from the central electronics not only save the mass, power, cost and size of the CPU module itself, but also have a fully functional equipment that requires no flight software, which is a major cost saving factor. NovaSAR-1 is an example of such a mission, and is fully functional without the need for a CPU module or any flight software. The NIA central electronics is compact, lightweight (10.9 kg on NovaSAR-1) and consumes just 46 W, the size of the instrument is 211 mm (H) x 265 mm (W) x 272 mm (D). NIA's first mission is NovaSAR-1. 31) 32) 33)
Figure 23: Nominal architecture of NIA (image credit: Airbus DS)
S-SAR payload qualification campaigns:
An extensive development program has been in progress for 3 years. This involves four stages of development for the NovaSAR-1 payload equipment:
1) Prototype hardware ground based inverse SAR test which imaged the ISS (International Space Station).
2) Airborne demonstrator using prototype hardware for providing sample imagery. 34)
3) In-orbit validation of payload technology by flying one phase center as a radar altimeter on the TechDemoSat-1 (Technology Demonstration Satellite-1) / TDS-1 mission of SSTL (a launch of TechDemoSat-1 is scheduled for late 2013).
4) Qualification of the payload via an EQM test campaign.
AIS (Automatic Identification System) payload:
AIS is a secondary payload on the NovaSAR-1 mission provided by COM DEV.
When the AIS instrument is being used to collect data simultaneously with SAR imagery of the same area, this will provide additional information on the identification of detected ships and highlight non-AIS transmitting vessels located in restricted areas. AIS is required to be carried for any ship over 300 tons, or for any passenger carrying ship, and the transmitted messages include unique identification, position, course, and speed data.
Note: The instrument will be described when information is available.
Philip Whittaker, Martin Cohen, David Hall, Luis Gomes, “An
Affordable Small Satellite SAR Mission,” 8th IAA (International
Academy of Astronautics) Symposium on Small Satellites for Earth
Observation, Berlin, Germany, April 4-8, 2011; URL of the presentation,
IAA-B8-0203, URL: http://media.dlr.de:8080
NovaSAR - setting a new benchmark in affordability and performance for
spaceborne Synthetic Aperture Radar (SAR) systems,” SSTL, URL:.http://www.sstl.co.uk
3) Philip Whittaker, Martin Cohen, David Hall, Rachel Bird, Luis Gomes, “NovaSAR – A Novel, Low Cost, Medium Resolution Spaceborne SAR System Development,” Proceedings of the 3rd Workshop on Advanced RF Sensors and Remote Sensing Instruments (ARSI), Noordwijk, The Netherlands, Sept. 13-15, 2011, URL: http://www.congrex.nl/11c11/ARSI%20papers/WHITTAKER_ARSI_Paper.pdf
4) Philip Whittaker, Rachel Bird, Martin Cohen, David Hall, Luis Gomes, Alex da Silva Curiel, Philip Davies, “A Low Cost SAR Solution for Disaster Management and Environmental Monitoring Applications,” Proceedings of IAC 2011 (62nd International Astronautical Congress), Cape Town, South Africa, Oct. 3-7, 2011, paper: IAC-11-B4.4.10
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Philip Davies, Alex da Silva Curiel, Rachel Bird, Philip Whittaker,
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The information compiled and edited in this article was provided by Herbert J. Kramer from his documentation of: ”Observation of the Earth and Its Environment: Survey of Missions and Sensors” (Springer Verlag) as well as many other sources after the publication of the 4th edition in 2002. - Comments and corrections to this article are always welcome for further updates (firstname.lastname@example.org).