Minimize Pleiades

Pleiades-HR (High-Resolution Optical Imaging Constellation of CNES)

Spacecraft     Launch    Mission Status     Sensor Complement    Ground Segment    References

Pleiades-HR is a two-spacecraft constellation of CNES (Space Agency of France), representing a long-term engagement with the introduction of advanced technologies in Earth observation capabilities. Starting with the first launch in 2009, the Pleiades program will follow the SPOT program satellite series services, with the following overall objectives:

• Provision of an optical high-resolution panchromatic (0.7 m) and multispectral (2.8 m) imagery with high quality product standards in terms of resolution, MTF (0.2 at system level), and a high image location accuracy

• Global coverage and a daily observation accessibility to any point on Earth

• Service provision of so-called "level-2 products" to customers consisting of a panchromatic image with a merged multispectral image orthorectified on a DTM (Digital Terrain Matrix)

• Provision of stereo imagery (up to 350 km x 20 km or 150 km x 40 km) and mosaic imagery of size up to 120 km x 120 km

• More than 250 images/day are expected from each spacecraft of the constellation

• The constellation is required to support risk management support services in terms of observation coverage (this requires an agile S/C design, a responsive operational concept, and a sufficient ground segment). 1) 2) 3) 4) 5) 6) 7)

Note: The name Pleiades refers to an open cluster of stars (about 35 light years in diameter) in the zodiacal constellation Taurus, about 400 light years from our solar system. It contains a large amount of bright nebulous material and several hundred stars, of which six or seven can be seen by the unaided eye and have figured prominently in the myths and literature of many cultures. In Greek mythology the Seven Sisters (Alcyone, Maia, Electra, Merope, Taygete, Celaeno, and Sterope, names now assigned to individual stars), daughters of Atlas and Pleione, were changed into the stars. The heliacal (near dawn) rising of the Pleiades in spring of the Northern Hemisphere has marked from ancient times the opening of seafaring and farming seasons, as the morning setting of the group in autumn signified the seasons' ends. Some South American Indians use the same word for "Pleiades" and "year." The cluster was first examined telescopically by Galilei Galileo, who found more than 40 members.


Figure 1: Artist's rendition of the deployed Pleiades spacecraft (image credit: CNES)


Since 1997 CNES is studying the use of smaller satellites (a medium spacecraft size of about 1000 kg instead of 3 tons as for the SPOT-5 S/C), resulting in the "3S" platform concept (Small Satellite System) standing for "Suite de Systeme SPOT" or for "SPOT Successor System." The focus is on cost reduction, technological innovation, user services, and performance upgrades for a new generation of optical imaging satellites, referred to as Pleiades. 8) 9)

In the same timeframe, the Italian Space Agency (ASI) performed also studies of a new program under the name of COSMO-SkyMed. Both countries had the same objectives in building a dual system, serving the civilian user community (institutional and commercial) and the defense users in each country. Recognizing the very similar goals of both programs, the two nations decided to cooperate to avoid duplications of civil and defense systems in Europe.

On Jan. 29, 2001, an intergovernmental agreement (memorandum of understanding) was signed during the Turin meeting between the heads of government of Italy (Guiliano Amato) and France (Lionel Jospin). The objective of this bilateral agreement, referred to as ORFEO (Optical and Radar Federated Earth Observation), is the cooperation of France and Italy on a "dual high-resolution Earth observation system," comprising a two-satellite constellation in the optical region under the leadership of France, and a four-satellite constellation under Italian leadership in the microwave region of the spectrum (initially X-band SAR). The intent of this agreement is to provide a long-term perspective on a number of high-quality data products and services on the commercial market for a wide range of applications in the fields of cartography, agriculture, forestry, hydrology, and geological prospecting. The dual service concept is seen in the data requirements of the defense and civilian communities with an option of a daily revisit capability. The agreement calls for funding and development of the space segment by each country and a common sharing of the ground segment. 10) 11)


Figure 2: Overview of organizations in ORFEO agreement (image credit: CNES)

In this framework, the Italian and French Governments started a cooperation with the goal of Earth observation for dual-use applications (military and civil) with SAR and optical instruments based on the on-going COSMO-SkyMed and Pléiades small satellite programs, respectively. This dual-use scenario calls for missions that offer advanced observation capabilities in several modes of operation, permitting to meet the objectives of the military and civil communities at the same time. The development of innovative and complementary instrumentation in the radar field (e.g., multi-mode and flexible-support SAR's offering high-resolution data) and in the optical field (e. g., hyperspectral sensor with capabilities of variable spatial resolutions as well as high detection sensitivities in the visible and infrared spectral regions) are major objectives of the programs.

The earlier memorandum of understanding was followed by a Memorandum of Agreement (MoA), for the ORFEO system definition step, between the French space agency (CNES) and the Italian space agency (ASI). The MoA was signed on June 22, 2002 at the Paris Air Show.

In 2005, CNES signed also Pleiades cooperation agreements with SNSB (Swedish National Space Board) with INTA (Instituto Nacional de Técnica Aeroespacial) of Spain, with ASA (Austrian Space Agency) of Austria, and with BELSPO (Belgian Science Policy Office) of Belgium. Belgium and France are already partners in the long-term SPOT program. Pleiades is with this action a multi-mission concept and a partnership program.

Thematic commissioning phase: 12)

The thematic part of the ORFEO accompaniment program covers a large range of applications, and aims at specifying and validating products and services required by users. An in-depth work of user needs assessments in eight domains (sea and coastline, risks and humanitarian aid, cartography and urban planning, geophysical hazards, hydrology, forestry, agriculture and defense) has given rise to a large number of feasibility studies from 2006 to 2011. Since 2006, more than 40 studies have been led by scientists and thematic experts from French and Belgium institutions, in close link with public end-users such as Ministry of Internal Affairs, Ministry of Ecology, French national cartographic institute, etc. Such studies, generally based on student internship, have been performed with imagery support provided by CNES both in the optical domain (WorldView-2, Formosat-2, QuickBird, Ikonos, GeoEye-1, Kompsat, aerial images) and in the radar domain (TerraSAR-X, COSMO-SkyMed, aerial images).

The third and last phase of the ORFEO program, the PUTC (Pleiades Users Thematic Commissioning) phase, started in March 2012. This phase is a direct follow-up of ORFEO program objectives and philosophy, aiming at supporting and encouraging institutional use of Pleiades, performing research, R&D and demonstration projects required by institutional actors. Free open source image handling and processing tools set up in the ORFEO methodological part will be provided, if needed, for easier access to data. Such activities are performed in complementary and in synergy with Astrium GEO-Information Services marketing activities, aiming at developing a Pleiades market among commercial users and at setting up certified and qualified commercial services.

The most promising studies since 2006 are being assessed with Pleiades imagery, in the eight domains of interest. Several key issues such as response to crisis, urban planning, human pressure on coastlines, watershed cartography, forest management are thoroughly studied. The parameters taken into account for the selection of the thematic studies were:

• Projects ready for operational applications (e.g. monitoring large gathering/summits, updating databases . .. )

• Projects still in demonstration but very mature (e.g. coastline detection and characterization, scrublands detection for fire prevention. . . )

• Projects of interest for institutional actors whatever their technical maturity is: research, Research & Development,demonstration (e.g. Green and Blue corridors, biodiversity, roof reconstruction . . . )

• Projects for operational demonstration capacity acquisition (e.g. IGN studies: department global coverage, MNT-Lidar assessment. . . ).

Major disasters and emergency events are covered with Pleiades imagery for Civil Protection needs. Since the beginning of 2013, Pleiades is fully operational in the International Charter "space and major disasters" process . The PUTC philosophy remains in the association of institutional users in the related projects. Indeed, studies in close interaction with public sector which answer to the requirements of the Ministry of Ecology specified in the Plan d'Applications Satellitaires, but also to other Ministries Requirements (Internal Affairs, Agriculture).

The importance of a collaborative work between the different thematic working groups has been privileged in order to maximize the efficiency for the key thematic studies (i.e Green and Blue Corridors) and to gather the data acquisition over multi-thematic sites. About 70 geographical sites related to almost 130 thematic studies have been selected in the framework of PUTC. More than 500 Pleiades acquisitions have been requested by users.

From its start in March 2012, the PUTC allowed the acquisition of more than 150 Pleiades images with a total surface of 40,000 km2. About 150,000 km2 are planned to be imaged by Pleiades for PUTC until the end of 2013. A total of 69 geographic sites around the world have been selected; their sizes vary from 100 km2 up to 3500 km2.

In the framework of the PUTC, more than 60 scientists or institutional teams are provided with the Pleiades images. Most of them are French but there are also some Belgian partners. As images are bought under DSP licence, institutional partners from France, Belgium, Spain, Sweden and Austria can access those images for free, thanks to their affiliation to ORFEO program.



Pleiades spacecraft:

The design of the Pleiades spacecraft employs a variation of the AstroSat platform, namely AstroSat-1000 of EADS Astrium SAS. The main design drivers for the S/C architecture were "satellite pointing agility and image location accuracy." Agility requires a very compact S/C design; hence, the imaging instrument is integrated inside the bus. A high degree of image location accuracy is achieved by minimizing the interface between the imager and the bus. The bus structure is of hexagonal shape, with three solar arrays positioned at 120º at the top of the platform (fixed mounting of solar arrays), and three star trackers in a quasi tetrahedron configuration, optimizing the attitude determination accuracy. The solar array size is minimized by using high-efficiency triple-junction cells. The satellite electrical architecture is organized around a central computer, based on a SPARC ERC 32 computer, communicating via MIL-STD-1553B buses to the onboard equipment. The computing, monitoring and reconfiguration functions are centralized in the OBMU (On Board Management Unit). The IMU (Instrument Management Unit) gathers the instrument interfaces: instrument thermal control hardware, mechanisms command, detection unit power conversion. All the other instruments have their own 1553 interface and directly interface with the OBMU. Two 1553 buses are nominally used: the first one for cyclic tasks, mainly allocated to AOCS and thermal control., the second one dedicated to burst exchanges, mainly payload instruments.


Figure 3: Schematic layout of the Pleiades outer structure (image credit: CNES)


Figure 4: Interior structure of the Pleiades spacecraft and instrument accommodation (image credit: CNES)

The S/C is three-axis stabilized; attitude is sensed by star trackers, SED36 of EADS Sodern, (capable of finding attitude starting from a "lost-in-space" condition) and by fiber-optic gyrometers (FOG)- the FOG device, a product of IXSPACE, is also referred to as AstrixTM. The S/C permits a body-pointing capability with roll and pitch maneuvers, each up to 60º, within a period of 25 s. The solar array design (each panel size of 2.3 m x 1.0 m) introduces LPS (Lightweight Panel Structure) and triple-junction GaAs solar cells (RWE-3G with integral diode, 27% efficiency); these new developments were supported by ESA/ESTEC. The spacecraft solar panels (GaAs cells of 5 m2) provides a power of 1.5 kW EOL of 33.6 V at summer solstice (mean power of 850 W). The Lithium-ion batteries have a capacity of 150 Ah. To ensure a balanced power budget over one day, the satellite points its arrays towards the sun before and after every imaging sequence. The S/C propulsion module employs hydrazine (50 l) and four 15 Nms thrusters for orbit control phases. The total dry mass of the S/C is 940 kg (compatible with Rockot, PSLV, and Soyuz launchers) + 75 kg of hydrazine. Hence, the mass of the new generation Pleiades spacecraft is only 1/3 that of its predecessor SPOT-5 with a mass of 3000 kg. 13) 14)

Attitude and orbit determination: An autonomous orbit determination is performed by a DORIS receiver. DORIS is the CNES tracking system, based on measurements between the satellite and dedicated ground stations at two frequencies (400 MHz and 2 GHz). The receiver raw measurements are filtered inside the receiver by a high order navigator, based mainly on Earth gravity potential modeling, to reach an accuracy of about 1m. The receiver can be cold started in any satellite orientation in less than 1 orbit, which eases the satellite operations. It also provides the onboard time and the PPS (Pulse Per Second) count needed to synchronize the system.

Attitude determination is performed by a gyro-stellar system. Three high-accuracy star trackers (STR) are used for attitude sensing, with separate optical heads. STR measures the direction of 12 stars to estimate a 3 axis attitude at a frequency of 8Hz. Each star tracker operates autonomously, its pointing accuracy is better than 2 arcsec in FOV error, and 10 arcsec (max) in noise which translates to 200 m on the ground. Only the axes perpendicular to the boresight axis are used to improve the accuracy. The ground location accuracy of the imagery is 10 m for a 90% probability ground circular error without GCP (Ground Control Points). Solid state FOG (Fiber Optic Gyrometers), Astrix 200 of EADS Astrium-Xspace, are used to ensure high-accuracy attitude determination while maneuvering. 15)


Figure 5: Optical head configuration of the FOG inertial measurement unit (image credit: CNES)

Actuator system: A newly developed CMG (Control Moment Gyro) technology is being introduced to perform the very demanding requirements of rapid slewing spacecraft maneuvers (i.e. body pointing of the S/C within ±60º). A cluster of four CMG actuators is being used, positioned in a pyramid configuration. The patented actuator system, developed by EADS Astrium-Teldix, is referred to as CMG 15-45S (15 Nms, 45 Nm, standard): it delivers a torque up to 45 Nm with a wheel of 15 Nms (angular momentum), sufficient to point a satellite in the 1000 kg class at more than 3º/s of slew rate within < 2 s; the compact architecture can be used for satellites from 1000 kg down to mini- and microsatellites. For Pleiades program applications, the requirements call for CMG fatigue failure modes in excess of 1.8 x 106 cycles under an average output torque of 19 Nm. 16) 17) 18) 19) 20)

Output torque

45 Nm

Angular momentum

15 Nms

Data bus interface

MIL-STD-1553 (or RS-422)

CMG mechanism mass; volume

15.7 kg; diameter = 270 mm, height = 350 mm

CMG mechanism footprint

200 mm diameter

Electronics mass (1 box for 4 CMGs); volume

2.7 kg per channel; 310 mm x 300 mm x 150 mm

Power use per CMG (including electronics)

25 W at max speed (@15 Nms)

Input bus voltage range

22-37 V


120 Hz

Table 1: Characteristics of the CMG 15-45S (for S/C in the 1000 kg class)


Figure 6: Illustration of the CMG 15-45S actuator (image credit: EADS Astrium SAS, CNES)


Figure 7: Pleiades-HR1 undergoes radiometric testing (image credit: CNES)


Figure 8: Photo of the flight payloads in the integration facility in the Kourou Spaceport (image credit: Arianespace)

Legend to Figure 8: The payloads of the Soyuz launch vehicle include the Pleiades 1A satellite, pictured at top, and four ELISA satellites, two of which are seen at bottom. Chile's SSOT satellite is not visible because it is inside the adapter's central cylinder.


New ASAP-S dispenser structure developed for Soyuz:

Arianespace enhanced the Soyuz mission flexibility with its development of a structure to accommodate small secondary payloads. Called the ASAP-S (Arianespace Structure for Auxiliary Payloads-Soyuz) this system continues the ASAP (Arianespace Structure for Auxiliary Payloads) concept previously developed for missions with members of the Ariane family, which have enabled "piggyback" passengers to be flown for the past 20-plus years. With the availability of ASAP-S on Soyuz, the ASAP launch capability on Ariane vehicles has been retired. 21)

The ASAP-S system for Soyuz has external positions for four microsatellites, along with volume inside the center structure for a fifth payload. The ASAP-S external configuration accommodates spacecraft weighing up to 200 kg, while the internal position is designed to accept a payload with a maximum mass of 400 kg.

The launch of the Pleiades-1A spacecraft was the first launch with the new ASAP-S dispenser structure.


Figure 9: Photo of the ASAP-S dispenser structure (image credit: Arianespace)

Legend to Figure 9: The ASAP-S structure is based on a massive rigid low plate made of alloy, which provides the interface with the launcher and supports the propulsion system. This plate provides the vertical stiffness required by the launcher. The structure is completed by four vertical struts at each angle of the satellite and by four lateral panels made of alloy honeycomb, which concur to the lateral stiffness. The ASAP-S structure has a total mass of 425kg, a total height of 1.841 m, and a diameter of 1.875 m. 22) 23)


Launch: The Pleiades-1A spacecraft was launched on December 17, 2011 on a Soyuz ST launcher (with Fregat upper stage) from Europe's spaceport in Kourou, French Guiana (launch provider: Arianespace). The flight was designated as VS02 (Vehicle Soyuz 02) in the Arianespace launcher family numbering system. The mission involved four burns of the Soyuz' Fregat upper stage, which enabled the six satellites to be released for operations at altitudes ranging from 700 km to 610 km. The Fregat upper stage performed a 3 hour, 26 minute flight to deploy its payload. The Fregat upper stage used a new purpose-built payload dispenser developed for Arianespace's Soyuz missions. Flight deployment sequence (Figure 11): 24) 25)

- The Pleiades-HR1 (primary payload) was deployed first after 55 minutes at an altitude of ~694 km

- The 4 ELISA satellites (secondary payloads) were released at ~ 700 km, 59 minutes after lift-off.
ELISA-1, ELISA-2, ELISA-3, ELISA-4 (Electronic Intelligence Satellite). A constellation of 4 ELINT (Electronic Intelligence) spacecraft of CNES/DGA, France. The ELISA demonstration constellation of microsatellites is based on the Myriade platform of CNES and was developed by by EADS/Astrium SAS and TAS-F (Thales Alenia Space-France) as co-prime contractors. Each spacecraft has a mass of 120 kg.

- This was followed by another orbit maneuver after which the SSOT satellite (secondary payload) separated from the Fregat stage, 3 hrs. 26 min. after lift-off at an altitude of 610 km.
SSOT (Sistema Satelital para Observación de la Tierra) of ACE (Agencia Chilena del Espacio - Chilean Space Agency), Chile. SSOT is a high resolution optical Earth observation satellite which was designed, built, integrated and tested by EADS Astrium SAS of France. SSOT has a mass of 117 kg.


Figure 10: Image of the Soyuz launch site ELS (Ensemble de Lancement Soyouz) in Kourou French Guinea which launched the Pleiades-HR1 spacecraft (image credit: ESA)


Figure 11: Flight sequence of the Soyuz launcher from the Guiana Space Centre to orbit the Pleiades, ELISA and SSOT satellites (image credit: Arianespace)


Launch: The Pleiades-1B spacecraft was launched on December 02, 2012 (UTC) on a Soyuz STA/Fregat launcher from Europe's spaceport in Kourou, French Guiana (launch provider: Arianespace). The flight was designated as VS04 (Vehicle Soyuz 04) in the Arianespace launcher family numbering system. 26) 27)

Orbit: Sun-synchronous phased orbits (180º phasing, 14 and 15/26 rev./day), altitude = 694 km, inclination = 98.2º, local equator crossing time on a descending node at 10:30 hours. The nominal repeat cycle is 26 days. With a roll "pointing" capability of 30º with respect to the track, world access can be achieved in 5 days with one satellite, and in 4 days with the system's 2 satellites. 28)

Naturally, with two agile spacecraft in orbit (and a FOR of 47º into any direction from nadir), there is the potential to revisit any point on Earth within 1 day (Ref. 28). 29)

RF communications: An X-band downlink provides a nominal payload transmission rate of 465 Mbit/s in 3 channels, each of 155 Mbit/s capacity. All source data are compressed prior to on-board (mass memory of 600 Gbit EOL). The CCSDS protocol is used for all S/C communications. An S-band link is being used for the support of all TT&C services.


Figure 12: Artist's conception of the Pleiades spacecraft in orbit (image credit: CNES)



Status of the Pleiades-1A and -1B missions:

• January 9, 2017: How do you deliver supplies to one of the remotest research stations on Earth? Put the equipment and food on skis and pull them by tractor across the ice and snow in a long caravan. The image of Figure 13 was taken by France's Pleiades satellite orbiting 700 km high. The convoy of supplies can be seen on the 1000 km trek from Dumont d'Urville on the Antarctic coast to the Concordia research station. 30)

- The traverse across Antarctica takes 10 days, climbing more than 3000 m to reach Concordia's plateau. Pulled by heavy-duty tractors, the caravans carry up to 300 tons of fuel, food and heavy equipment in 300 m-long convoys organized by France's IPEV (Institut Polaire Français Paul Emile Victor) polar institute.

- Once at Concordia, three days are spent unpacking and preparing for the return trip. The trip back to the coast generally takes two days less because it is downhill most of the way.

- Concordia sits on a plateau 3200 m above sea level. A place of extremes, temperatures can drop to –80°C in the winter, and the Sun does not rise above the horizon in the winter, forcing the crew to live in isolation without sunlight for four months of the year.

- For ESA, the isolation and extreme weather offer interesting parallels with spaceflight and living on another planet. Each year an ESA-sponsored medical doctor joins the crew of the Italian–French station to monitor and run experiments on the crew of up to 15 persons.

- In addition, the area around Concordia is also used as a validation site for a number of ESA's Earth observation missions such as the SMOS (Soil Moisture and Ocean Salinity) satellite.


Figure 13: This image of the Antarctic caravan was taken by the Pleiades satellites of CNES, acquired in late 2016 during the Antarctic summer (image credit: Pleiades–CNES 2016, Distribution Airbus DS)

• On December 17, 2016, Airbus DS is celebrating five years of the Pleiades-1A spacecraft on orbit. The Pleiades-1B satellites was launched almost a year later, making up the Pleiades constellation, an ambitious service that creates an imagery product of every point of the globe at a 50 cm resolution within a few hours and guarantees a daily revisit, with more than 1 million km2 acquired each day. 31)

- The Pleiades constellation has demonstrated its reactivity during the earthquake that rocked Ecuador on April 16, 2016, providing an image on the town of Pedernales in just four hours after being acquired. Immediately delivered to the local authorities, it enabled organizers to provide the various relief operations, and to carry out a rapid assessment of the damage.

- The precision of the Pleiades imagery, coupled with the speed of acquisition over large regions, also played a key role in demonstrating the demolition of the ancient city of Palmyra in Syria by the Islamic State in 2015 and thereby creating a consciousness for the need of preservation of this UNESCO world heritage site.

- The two satellites, built and operated by Airbus Defence and Space on behalf of CNES (French Space Agency), are the first European satellites to observe the Earth in very high resolution. Providing imagery products at 50 cm resolution with a 20 km swath, they are positioned 180° apart in a same near-polar, sun-synchronous orbit at an altitude of 694 km. They also have remarkable agility which allows them to aim a point up to 1500 km on either side of their track. This gives them a fast zone-pointing capability and multiple shooting modes (stereo, mosaics, corridor, targets).

• May/June 2016: The PHR (Pleiades High Resolution) system is a constellation of two Earth-observation satellites (PHR-1A and PHR-1B), with very high resolution capability delivering resampled 50 cm ortho color products as standard. The PHR system is operated by the French Space Agency (CNES) in a dual mission for civilian and defense needs: the imagery requests could be for a military user (the French Defense), a governmental or an institutional user, or a customer of a commercial operator (Airbus Defense & Space - Intelligence). 32)

- The system is designed on a chronology based on the preparation of three working plans (mission plans) per day, each covering 24-hour shifting mission programming. The Mission plans are processed simultaneously for the two satellites ensuring an overall optimization of the system. This process reduces the system reaction delays for all the user entities, taking into account the latest up-to-date meteorological data and including optimization of the reactivity over the interest area for both defense and civilian operators. To improve the system reactivity and reduce the reaction delays for specific customers, the DT (Direct Tasking) concept has been implemented. The Direct Tasking is a specific mission planning mode that uses a dedicated RIRS (Regional Image Receiving Stations), including S and X band capability (called Direct Tasking S+X), to have a "last minute" access to the satellites during an allocated slot. For this mode, a specific DT mission plan is computed in the PHR ground segment just before the station fly-by and is uploaded during the first seconds of the satellite visibility.

- As an extension of the DT function, called Direct Tasking S- and X-band, DT could be performed on a standard PHR RIRS (only X-band station) complemented by a standard S- band ground station, managed by the NOC (Network Operation Center) of the French Space Agency, having a visibility with PHR satellite few minutes before the X-band RIRS pass. For each mode, The Direct Tasking plan has to be performed on a specific short time of period slot and specific constraints, and has to be inserted in the default 24-hour plan already onboard.

- The PHR configuration offers a daily revisit capability over any point on the globe (repeat cycle of 26 days by satellite). The system is operated in a dual program for a commercial operator (Airbus Defense and Space Intelligence – Airbus DS Intelligence, formerly SPOT Image) and for the French Defense (FD).

- The instrument consists of 5 acquisition tracks (one panchromatic and four multispectral tracks) for a 70 cm resolution. The system delivers resampled 50 cm ortho color products as standard. The swath on the ground is 20 km, meaning a simple acquisition represents a 20 km x 20 km square at nadir. Equipped with innovative fiber-optic gyros and control moment gyros, the two satellites offer high agility performances in roll, pitch and yaw, enabling the system to maximize the number of acquisitions above a given area. All these characteristics and the high agility performances of the satellites in the three axes, represent about 1300 image acquisitions carried out by the constellation every day.

- The PHR system uses the network of CNES S-band stations to upload the dual working plan onto the satellites. No CNES X-band station is used to download images because no image downloading is performed in the CNES programming center. The few acquisitions requested by CNES for the instrument calibration are downloaded onto the Airbus DS Intelligence station and transferred to the CNES via secured links. The different centers are linked as presented in Figure 14.

- The Pleiades civilian ground segment is composed of a set of user centers mainly located in France and in Sweden, and other stations (Direct Receiving Station and RIRS). All of these centers are interfaced with the SDGC (Secure Dual Ground Center, the PHR Command / Control and CNES programming center) located at CNES, in Toulouse, France. Each user center is able to manage the user image acquisition requests and the image productions, including:

a) A X-band antenna for data acquisition, 3-channel signal demodulation and ingestion system.

b) An image processing unit to make the inventory, the catalogue, to archive the data and to produce imaging products.

c) A programming unit to manage the mission planning requests.

d) A set of access units permitting the users to browse the image catalogue, to submit requests and to receive the ordered products.


Figure 14: Users centers interfacing with SDGC (Secure Dual Ground Center, the PHR Command / Control and CNES programming center) located at CNES, in Toulouse, France (image credit: CNES)

CNES in Toulouse hosts the SDGC, the dual center which deals with the following functions and service requests:

- Monitoring and control of the Pleiades spacecraft.

- Hosting of the defense coordination function in support of an optimized mission plan for the different partners, taking into account the priorities of each national work plan.

- It performs the planning of all the programming requests, by collecting and analyzing all the demands of the civilian and defense users.

- It implements and oversees the periodic calibration function of the imaging instrument, for the benefit of all the users. The instrument calibration is requested by the ICC (Image Calibration Center, located at CNES).

- Airbus DS Intelligence deals with the civilian customers in their ground center located in Toulouse,France. The customers can consult the civilian images catalog, submit requests and receive the ordered products. All civilian image requests are centralized by Airbus DS Intelligence. It ensures the civilian antenna management as well as the reception and the archiving of raw data received from satellites. Airbus DS Intelligence also manages a network of regional image receiving stations (RIRS). The Kiruna station enables the daily reception of the Pleiades images, in addition to the Toulouse station; it is operated as a RIRS. The RIRS can be eligible for Direct Tasking activities (station JP1, JP2 in Japan and PS1 in Peru). A very important operational criterion is the delivery of the data products for the commercial customers quickly. This speed represents a key element of the space and ground segment components, built to comply with the user requirements.

- The French defense programming center looks after the defense images requests. The basic functions of the defense programming centers are similar to those of the civilian ground segment with some differences in the interfaces, and the security aspects.

Direct Tasking principles (Figure 15):
In addition to the centralized programming mode as previously explained, the PHR system offers a Direct Tasking mode to the dedicated RIRS (Regional Receiving Stations) equipped with X- and S- band capabilities in order to improve the overall system reactivity. The objective of Direct Tasking is to provide a "direct" access to the satellite, by processing a specific Direct Tasking plan (or DT working plan or DT plan) just before the satellite flyby over the station. The DT mode provides better reactivity for the near-real time applications. The access to the satellite is not a completely direct access due to security reasons and because the Direct Tasking plan is computed in the CNES programming center, considering the potential defense acquisitions which have priority over other acquisitions.

An ADS customer can reserve an orbit slot during the satellite flyby of its RIRS, this slot is called a "DT slot". The image acquisition and downloading have to be performed during the DT slot. The customer has image downloading exclusivity during the slot. No other image downloading can be done if the DT slot is at an intersection of many station visibilities.

There are two kinds of Direct Tasking mode: the DT S+X mode and the DT S&X mode. In the first mode, the station has image reception means (X-band system and antenna) and a system to ensure the uploading of the DT plan (S-band system and antenna). The X- and S-band systems and antennas are collocated. In the second mode (DT S&X), the station only has the image reception equipments (X-band system and antenna) and the RIRS customer uses a S-band station of CNES network located just before the satellite flyby of the RIRS. In this mode, the X-band station and S-band station are not located in the same place.

Nowadays, the DT S+X mode is fully operational with three RIRS eligible for the Direct Tasking mode: in Japan with JP1 (Hokkaido) and JP2 (Okinawa) stations; and a station in Peru, PS1. This article is focused on the DT S+X mode. The DT S&X mode is not currently used by customers of Airbus DS Intelligence but this mode has been tested and validated during in-orbit validation in the PHR-1A beginning of life, in 2012; only general principles of this mode which are near from DT S+X mode, will be explained.

The Direct tasking S+X mode process follows this sequence of events:

- An orbit slot (typically 2 minutes) is reserved up to 24 hours by the RIRS customer before the satellite flyby over the station.

- The customer could generate a "local" Direct Tasking plan on its local programming unit up to 30 minutes before the beginning of the DT slot (considering the latest weather conditions or urgent requests). The image acquisition request list resulting from this phase (prioritization phase) is sent to the CNES programming center via Airbus DS Intelligence (secured links).

- The Direct Tasking plan is compiled into command plans, checked then ciphered into the CNES programming center for security reasons and takes into account potential defense image acquisition requests or technological operations.

- Then, the DT plan is sent back to Airbus DS Intelligence and returns to the RIRS station through secured link [ISDN (Integrated Services Digital Network) or VPN (Virtual Private Network) links)]. The DT plan is uploaded to the satellite using the CRT equipment (Command and Ranging Telemetry) and the RIRS S-band equipments.

- The satellite runs the recently uploaded DT plan by simultaneously acquiring and downloading the images to the Direct Tasking station during the DT slot. This sequence represents a near-real time service. The satellite keeps the potential defense image acquisitions taken during the DT in its onboard memory. They will be downloaded to the defense station later.

- The data is automatically produced in the RIRS: 30 minutes from the image reception to the final product. The RIRS has two actions: to reserve the DT slots up to D-1 and to establish the DT prioritized list which will be considering by the CNES programming center up to 30 minutes of the DT slot.

The other operations managed by Airbus DS Intelligence and CNES are automatic actions. They update the interfaces: reservation confirmation of the slots via the pass plan allocated interface and DT plan transfer to the RIRS for automatic uploading just before the DT slot. They also send the new receiving and inventory plans (about 10 minutes before the DT slot) to allow the station able to receive and archive image telemetry. The detailed chronology from creation of the acquisition list to the reception of images telemetry will be presented in the next paragraph.

The main difference between DT S+X and DT S&X modes is that the orbit slot must be reserved 72 hours beforehand, for the S&X mode. This mode uses the CNES S-band station network to upload the mission plan. The S-band station must be located in the same orbit and just before the RIRS flyby. However, image acquisition and downloading are only possible during the DT slot. In the DT S&X mode, the concept is less reactive than the DT S+X mode but always more reactive than the centralized programming mode (Ref. 32).


Figure 15: Direct Tasking interfaces (image credit: CNES)

• May 2016: Airbus DS released the Pleiades image of Paris, France (Figure 16) as image of the week. 33)


Figure 16: Pleiades Satellite Image - Stade Parc Des Princes, Paris (image credit: Airbus DS)

• In Dec. 2015, Pleiades-1A was 4 years on orbit and Pleiades-1B was 3 years on orbit. Both satellites and their payloads are operating nominally.

• Sept. 14, 2015: Thales Alenia Space (TAS) has signed a contract with CNES, the French space agency, for a feasibility study regarding the development of a high-resolution optical remote sensing satellite system designed as a follow-on to the Pleiades satellites, planned for launch early in the next decade. Through the second half of 2016, this study will define the system's optimal design and select the technologies to be applied. 34)

- As the provider of all of Europe's high-resolution optical instruments in Europe since Helios-1, launched in 1995, Thales Alenia Space, under a co-contractorship with Airbus Defence & Space will contribute to the design selection at system level for the satellites and will be more particularly in charge of the payloads and associated systems.

- The satellite will enable in-flight qualification of advanced technologies developed by TAS on behalf of R&D efforts funded by DGA (Délégation Générale pour l'Armement), the French ministry of Defense's procurement agency, and CNES, such as the OTOS (Observation de la Terre Optique Super-Résolue) program of CNES.

• Sept. 11, 2015: Airbus Defence and Space has just signed a feasibility study contract with CNES, the French space agency, for future French space-based civil and military Earth observation systems. This contract was announced by CoSpace, the joint government-industry committee on space, which met today in Paris, in the presence of Emmanuel Macron, Minister for the Economy, Industry and Digital Affairs, Jean-Yves Le Drian, Minister of Defence, and Thierry Mandon, Minister of State for Higher Education and Research, along with representatives of the ministries concerned. 35)

• Sept. 2015: Moscow is Russia's largest city and one of the largest in Europe as a whole. Over twelve million people live in Moscow, and Istanbul (Turkey) is the only other city on the continent to exceed that. Moscow is located on the Moskva River, from which the city gains its name, and this can be seen as a clear white line running through the city in the image (Figure 17). 36)

- Another landmark visible in this image are Moscow's Rings. A series of roads ring the city, and news ones have been constructed over the centuries to help traffic. The older roads conform to the ancient walls that once surrounded Moscow but now form part of the city's core.


Figure 17: This Pleiades image, acquired on 11 August 2013, shows Moscow, the capital city of Russia (image credit: CNES, Airbus DS)

• April 10, 2015: The SPOT-1 to -5 mission archive, the SPOT-6 and -7 mission archive and new acquisitions, the Pleiades mission archive and new acquisitions, and the SPOTMAPS 2.5 complete dataset are now available to the scientific user community. 37)

- The products are available in level 1 and level 3 (levels 1A/1B and orthorectified level 3 for SPOT-1 to -7, primary and orthorectified levels for Pleiades). Stereo and Tri-Stereo modes available on SPOT-6 and -7 and Pleiades are also available.

- The products can be made available for free through a project proposal submission via the SPOT information area and Pleiades information area on ESA's Earth Online Portal.

Pleiades is a TPM (Third Party Mission) of ESA. ESA is offering free of charge for scientific research and application development access to the following PLEIADES collections: 38)

- Archived PLEIADES Panchromatic,Multispectral, Bundle and Pan-Sharpened all production levels (on demand)

- New acquisitions PLEIADES in single,stereo or tri-stereo acquisition mode (standard service).

• January 2015: Pleiades, the very high resolution satellite operated by Airbus Defence and Space, witnessed the birth of a new island in the Tonga archipelago in Polynesia, in the timeframe July 2014 to January 2015. 39)

- Hunga Tonga is located between two small islands in the Tonga archipelago; Hunga Tonga and Hunga Ha'apai. This region is located within the "Ring of Fire", an area of the Pacific Ocean which experiences a great deal of seismic activity. As such, activity has been recorded at the volcano for centuries, and even plays a role in Tongan mythology.

- The underwater volcano Hunga Tonga, awoke on December 20, 2014 and a huge crater emerged between two islands.. The enormous volumes of rock and ash expelled by the volcano joined the crater to one of the two islands and all vegetation disappeared. The diameter of the new crater is about 1.5 km. On 19th January 2015, the Pléiades satellite image enabled Tongan geologists to observe that the volcanic eruption was weakening.


Figure 18: This image from the Pleiades satellite, acquired on 19 January 2015, shows a new island that has formed from the eruption of the Hunga Tonga underwater volcano, in Tonga (image credit: CNES, Airbus DS)

• April 2014: Owing to their agility and capacity to capture a large collection of images, Pléiades-1A and Pléiades-1B become key elements within crisis management and military operations. Phased in 180º co-planar orbits, the twin satellites have daily revisits over most locations on Earth. Due to their CMG (Control Moment Gyroscope) actuation capability, the satellites can pitch and roll forward, backward and sideways up to 45º very quickly. This remarkable agility enables them to capture a multitude of individual scenes, long strips, or broad contiguous areas of interest on a single pass. The CMG effectively extends the swath widths from 20 to 120 km. 40)


Figure 19: Pleiades image of Sevastopol Ukraine on March 3, 2014 (image credit: Airbus Defence and Space)

Legend to Figure 19: Following the first Russian troops movements in the Crimean region, Pleiades was tasked to prioritize collection on the most important hot spots: airbase, naval base, military barracks, roads and strategic bridges and railways. Within less than 24 hours from receipt of the tasking request on 3 March to the satellite imagery delivery on 4 March, Pleiades provided a 50 cm detailed level on Sevastopol, allowing objective situation analysis. The accuracy of the information contained in each pixel allows identifying what type of boats are present in the harbor, and therefore, their nationality.

• Pleiades - A dual system: A success story for defense and civil users

• A Public Service Delegation

- Airbus DS provides the service for institutional users (tasking and production)

- Synergy with commercial market allows to minimize the costs for institutional users

- Fair balance to be maintained between the institutional and commercial sectors

• A specific organization in France

- IGN (Institut Géographique National, Paris) will ensure overall coordination and optimization

- CNES will ensure the overall supervision of the system

• Challenges remain on the User side in processing the high volume of Pleiades products

- It is important to maintain activities to improve tools and software

• Technology development activities "OTOS": 2013 to 2016. OTOS is a demonstrator of technologies needed for EHR imagery.

- To improve the performance by a factor 2 and maintain acquisition capability

- To improve the maturity of technologies and be ready for a launch in 2021

• A new mission study (Phase 0) "Arctos" :

- Mission Definition Review mid 2014

- To find the best compromise for the various actors (technique, economic and calendar)

The objective is to start the post Pleiades phase A study in September 2014

Table 2: Pleiades for the institutional users 41) 42) 43)


Figure 20: Pleiades image of Rotterdam Harbor (The Netherlands) acquired in 2013 and released at the Pleiades Days, April 1-3, 2014 (image credit: CNES, Airbus DS/Geo-Intelligence) 44)

• 2014: The Pleiades-1A and -1B missions are operating nominally. 45)

• Pleiades-1B image quality status after commissioning and 1st year in orbit. This applies to the geometric performances such as pointing, location, planimetric and vertical accuracy. 46)

1) Pointing Accuracy Performance: The capability to target the instrument toward the desired point when tasking the satellite.

- Pleiades-1B performance: requirement reached with a comfortable margin
- Performance across track: 275 m LE99.7 vs. requirement 500 m LE99.7
- Performance along track: 520 m LE99.7 vs. requirement 1000 m LE99.7


Figure 21: Spacecraft fleet operated by Airbus Defense and Space (image credit: Airbus Defence and Space)

2) Location Accuracy Assessment: Products location with on-board data only ⇒ Rigorous Geometric Model accuracy without GCP

- On board ephemeris
- On board raw attitudes and accurate attitudes for Pleiades (orbitography refined twice a day)

Geolocation assessment (both for commissioning and current monitoring) performed with several hundreds of acquisitions over fully qualified GCPs (Ground Control Points) distributed worldwide in order to reflect the performance all along the orbit and the nominal acquisition domain (OZA < 30º).

3) Location Accuracy Performance:

- Excellent location accuracy already confirmed at commissioning: 8.5 m CE90 @30º
- Better than satellite requirement (12 m CE90 @30º). Measurement during the commissioning phase (Jan – May 2013).

4) Focal Plane Calibration and Planimetric Accuracy Assessment:

Planimetric accuracy: residual error of all Line Of Sight contributors after geometric model reset on a Ground absolute reference:

- Assessment on reference site, image auto calibration (cross acquisition)
- Reference sites: correlation on nearly perfect reference sites covering the full swath
- Supersites of Toulouse (France), Bouches du Rhône (France), Napier (New Zealand)
- XY accuracy <0.2 m ; Z accuracy<0.3 m

- Auto calibration without reference site
- Cross acquisition of 2 images (or more) on a same orbit, viewing the same site with opposite viewing angles of 90º
- Correlation of image couple gives static and dynamic residues along lines and columns.


Figure 22: Schematic view of the Pleiades-1B focal plane (image credit: Airbus Defence and Space)

• October 2013: More than 1 ½ years after the first satellite's launch, the Pleiades system is in very good health and the two satellites are fully operational offering a very good image quality. The system offers a very high acquisition capability (more than 500 images per day and per satellite) and its availability is close to 100%. Regional image receiving stations have been installed (Japan, China and Canada). 47) 48)

The use of both satellites simultaneously in orbit shifted by 180º permits to ensure:

- the daily accessibility to any point of the Earth and a prompt imaging required by Defense and Civil Security missions.

- the high coverage capability required for mapping and land planning needs.

Given the dual nature of this system, two types of access are defined to schedule the satellites' tasks:

- The Defense channel used by Ministry of Defense beneficiaries for High Priority Defense programming requests.

- The Civil channel used by civilian users. It is operated by a civilian operator.

The civilian data distribution is delegated to Astrium Geo-Information Services (formerly Spot Image) through a Public Service Delegation: 40% of the resources of the system are reserved for institutional users of the cooperative countries for no-commercial activities. CNES has granted an exclusive license to the Civilian Operator allowing him to process, distribute and commercialize the data and products on the worldwide market.

Table 3: Data distribution concept of the Pleiades program

Each Pleiades satellite is capable of targeting images along any ground direction within 47° of vertical viewing position, with very low maneuvers durations between two consecutive images. This high agility permits (Ref. 47):

- to ensure a good reactivity of the system in order to satisfy the urgent needs

- to minimize scheduling conflicts within the dual use framework

- to acquire image in any direction following, for example, coastlines or river routes as so to optimize programming for instance in a crisis case (flooding, tsunami, etc.)

- to enlarge the swath by taking in the same pass adjacent stripes, mosaic images covering up to 140 km x 105km (6 strips) can be acquired

- to acquire in the same pass stereoscopic pairs or tri-stereoscopic triplets even with low base over height ratio, a very important improvement in order to avoid hidden objects in an urban area (occlusions), see Figures 23 and 24 acquired in 2013.

- To perform calibrations on stars or moon images or using "exotics" guidance methods.


Figure 23: Three pictures on the Mecca "tower clock" acquired by Pleiades 1B every 90 s in a single pass to see the minutes needle moving ! (image credit: CNES)


Figure 24: Three pictures on the Mecca "tower clock" acquired by Pleiades 1B every 90 s in a single pass to see the minutes needle moving ! (image credit: CNES)

In addition to stereoscopic acquisitions, during commissioning, Pleiades agility has been pushed to its limits in order to acquire more than 30 images in a single pass to produce a sequence of animated images allowing to highlight human activities on the targeted area. This high acquisition capability is accompanied by a revisit interval of less than 24 hours to meet both civil and military requirements.

The orbit has been selected in order to minimize the revisit time with either one or two satellites in orbit.

Viewing angle

1 satellite

2 satellites

26 days

13 days


7 days

5 days


5 days

4 days

Table 4: Revisit time scenario

Pleiades has demonstrated its capability to acquire cloud-free images very quickly (more than 50% of the images have a cloud cover better than 10%). As an example on climatological difficult areas (Figure 25), 94% of Burundi have been acquired and validated within 4 weeks and 3 segments of 90 km have been acquired cloud-free over Amazonia on a single pass....


Figure 25: Pleiades constellation coverage of Burundi in 4 weeks (image credit: CNES, Ref. 47)

• Sept. 19, 2013: The 50,000 ton Italian cruise ship, Costa Concordia, which ran aground on January 13, 2012 due to error made by its Captain was righted after massive salvage efforts by a team of engineers and mariners. This has been the most expensive salvage operation in marine history. 49) 50)

- The very high resolution Pleiades satellite, captured the refloating on 17 September of the Costa Concordia (Figure 27), wrecked off the Island of Giglio, Italy.


Figure 26: Pleiades image acquired on July 12, 2013 showing the wrecked Costa Concordia off the coast of Giglio, Italy. (image credit: CNES Distribution Astrium/SPOT Image)


Figure 27: Re-floating operation of the Costa Concordia. This Pleiades-1A image was captured on September 17, 2013 (image credit: CNES Distribution Astrium/SPOT Image)

• March 2013: Pleiades-1B has completed its technical commissioning and is now commercially available. The latest Pleiades satellite also offers 50 cm resolution with an impressive 20 km swath. Like its twin, orthorectified imagery is standard and several tasking options are available. - The Pleiades twins now operate as a true constellation on the same orbit, allowing a daily revisit capability to guarantee the customer the right information at the right time. 51) 52)

Astrium Geo-Information Services is the civil operator of the Pleiades constellation (Pleiades-1A and -1B) as well as the operator of the SPOT-6 and SPOT-7 constellation. When SPOT-7 is launched in 2014, there will be 2 x 2 satellites, a true constellation with all spacecraft in the same orbital plane, coherently operated (90° one from the other on the same orbit) through a single interface. 53)


Figure 28: Astrium GEO-Information Services is operating the Pleiades constellation and the SPOT-6&7 constellation (image credit: Astrium)


Figure 29: The Pleiades and SPOT-6/-7 Pleiades satellite constellation configuration (image credit: Astrium GEO-Information Services)

• February 22, 2013: Astrium Geo-Information Services and ESA are pleased to announce the availability of Pleiades-1A data for GMES users starting on March 4, 2013. Orders received after that date will be fulfilled taking into account the contribution of Pleiades as described in the Data Access Portfolio 2.6.1, archived data being available since 1st of March 2012. 54) 55)

The Pleiades-1A satellite will enlarge the portfolio of missions available in response to emergency activations. The initial setting benefits from the service coverage already available for SPOT satellites and will be extended if needed in the future.

• January 2013: The Pleiades-1A spacecraft is operating nominally in 2013. The Pleiades-1B spacecraft is in the commissioning phase.

• On Dec. 5, 2012, Pleiades-1B acquired its first images. 56)


Figure 30: Pleiades-1B acquired this pansharpened, high-resolution image of Istanbul (Turkey) on Dec. 5, 2012 (image credit: Astrium Services)


Figure 31: First image of the Pleiades-1B mission showing Lorient, France, acquired on December 5, 2012 (image credit: CNES) 57)

• December 02.2012: CNES is reporting that operations on the Pleiades-1B are nominal; the solar panels are deployed, the attitude is stabilized, the thermal and power balance is reached. 58)

• In August 2012, Pleiades-1A has already acquired more than 10,000 images, the system is very robust and the availability of the satellite is excellent. The success of the Pleiades mission is now in the hands of operational teams that will focus their energies to satisfy the users needs and keep Pleiades in good health throughout the years to come (Ref. 7).

• June 26, 2012 marked the end of the Image Quality in-flight commissioning. 59) 60)

The assessment of the image quality and the calibration operation have been performed by the CNES Image Quality team during the 6 month commissioning phase that followed the satellite launch. These activities cover many topics gathered in two families : radiometric and geometric image quality. The new capabilities offered by PLEIADES-HR agility allowed to imagine new methods of image calibration and performance assessment. 61)

The radiometric activities dealt with the following main topics:

- MTF assessment and refocusing operations

- Absolute calibration

- Inter-detector normalization

- Signal-to-noise ratio assessment

- Onboard compression bit rate optimization

- Clouds auto-detection

The geometric activities evaluated were:

- Localization performance

- Focal plane cartography

- Line-of-sight dynamic stability

- 3D rendering capabilities (Ref. 61).

• In early June 2012, all the calibrations were performed; the precise measurement of the performances are still ongoing satisfactorily: the end of the Image Quality Commissioning Phase is scheduled for the end of June 2012. 62)

- The launch of the Pleiades-1B spacecraft is planned for the end of 2012 (Ref. 62).


Figure 32: Pleiades-1A image of Melbourne acquired during commissioning (image credit: CNES, Ref. 7)

• Astrium GEO-Information Services (see Table 5) is the official distributor of the Pleiades high-resolution commercial imagery products. 63)

- In return for financing 90% of the Pleiades program, the French government has reserved access to specific percentages of Pleiades' output of 900 images per day once both satellites are in their 694 km orbit, spaced 180º apart.

- The French Defense Ministry has priority access to 50 images per day from the two-satellite Pleiades constellation.

- Civil agencies of the French government have access to 40% of the remaining Pleiades output, with Astrium Geo-Information Services claiming 60%.

• The commissioning phase ended on March 2, 2012. The main image quality performances had been assessed and appeared to be very good; even if some of them were not considered to be accurately measured the Pleiades-1A system was declared fully operational (Ref. 62). 64)

• The Pleiades-1A spacecraft is in the commissioning phase in early 2012 (the commissioning phase is led by CNES).


Figure 33: Image of Bora Bora Island in Polynesia observed by Pleiades-1A on January 3, 2012 (image credit: CNES) 65)

• The Pleiades-1A satellite imager captured the first panchromatic satellite images 3 days after its successful launch from the Kourou launch site (French Guiana) via a Russian Soyuz ST rocket on December 16, 2011. 66)

Pleiades-1A represents the first very high-resolution satellite of the SPOT family and will be capable of providing orthorectified color data at 0.7 m resolution and revisiting any point on Earth as it covers a total of 1 million km2 daily. Perhaps most importantly, Pleiades-1A will be capable of acquiring high-resolution stereo imagery in just one pass, accommodating large areas (up to 1,000 km x 1,000 km).


Figure 34: Three days after its launch, Pleiades-1A returned this image of the Hassan II Mosque in Casablanca, Morocco (image credit: CNES, Astrium, Ref. 66)

Spot Image and Infoterra joined forces within Astrium Geo-Information Services to offer a consolidated product and services portfolio under the Astrium brand. The merger took place in May 2010 and was fully integrated in December 2010. 67)

A single operational management structure started on January 1, 2011, bringing closer together the satellite imagery and geo-information specialists Spot Image and Infoterra to form the GEO-Information division of Astrium Services. As a global, integrated company, the GEO-Information division of Astrium Services implemented this new organization with a single vision in mind: to better respond to the needs of customers.

The GEO-Information Services division will offer:

• A one-stop shop for data from the SPOT-4 and -5 missions, from the TerraSAR-X/TanDEM-X satellites, from FormoSat-2, and from the Pleiades constellation. This will also include the imagery of the SPOT-6/7 constellation.

• A wide range of other satellite and aerial data

• A single product and services portfolio covering the entire geographic information value chain from satellite imagery to value-added services and turnkey solutions.

As Pleiades is a dual-service system - there are also two operators sharing the system according to predetermined quotas. 62)

5) Astrium Geo-Information Services is the civil operator of Pleiades

6) The French defense system (DGA) is the defense operator of the system.

Astrium Geo-Information Services takes over the spacecraft operations of the civil channel with an exclusive license once each Pleiades satellite has been commissioned.


As of January 1, 2014, former EADS rebranded itself as the Airbus Group, with three divisions that include: 68)

- Airbus, focussing on commercial aircraft activities

- Airbus DS (Airbus Defence & Space), integrating the Group's defence and space activities from Cassidian, Astrium, and Airbus Military

- Airbus Helicopters,comprising all commercial and military helicopter activities.
The former Astrium subsidiary was merged into the Airbus DS in late 2013. The new Airbus DS started operating at executive level as of January 1, 2014. The GEO-Information Division of Astrium Services became the program line "Geo-Intelligence", of Airbus DS.

After the consultation process with the works councils, expected to be concluded by mid-2014, the three entities – Airbus Military, Astrium and Cassidian – will be fully integrated and operational at all levels as Airbus DS. 69)

Table 5: Geo-Information Services of Astrium 67) 68) 69)

As of January 1, 2014, former EADS rebranded itself as the Airbus Group, with three divisions that include:

- Airbus, focussing on commercial aircraft activities

- Airbus DS (Airbus Defence & Space), integrating the Group's defence and space activities from Cassidian, Astrium, and Airbus Military

- Airbus Helicopters,comprising all commercial and military helicopter activities.
The former Astrium subsidiary was merged into the Airbus DS in late 2013. The new Airbus DS started operating at executive level as of January 1, 2014. The GEO-Information Division of Astrium Services became the program line "Geo-Intelligence", of Airbus DS.

After the consultation process with the works councils, expected to be concluded by mid-2014, the three entities – Airbus Military, Astrium and Cassidian – will be fully integrated and operational at all levels as Airbus DS.



Sensor complement: (HiRI)

HiRI (High-Resolution Imager):

HiRI of CNES with Thales Alenia Space (TAS-F) as the prime contractor for this instrument (formerly Alcatel Alenia Space). The objective is to provide high-resolution multispectral imagery with high geo-location accuracy. The camera design employs a pushbroom imaging concept. Extensive use of existing state-of-the-art technologies is made regarding such items as: a) camera alignment procedures, b) telescope thermal control and mechanical assembly principles, c) video processing techniques. 70) 71) 72) 73) 74)

The industrial team consists of the following partners:

• Thales Alenia Space, France: Instrument, telescope, detection unit, telescope structure & thermal control, video electronics, video power supply, harness

• Thales Alenia Space España: Instrument service module

• Sener: Shutter, detection unit structure & thermal control

• E2V (Chelmsford, UK): Pan & MS CCD imaging detectors

• SESO (Société Européenne de Systèmes Optiques), France: telescope mirror manufacturing

• EADS Sodern: FPA (Focal Plane Assembly)

• Sagem: Spectral filters.


Figure 35: Illustration of the HiRI instrument (image credit: CNES)




Panchromatic detector

CCD detector array with TDI (Time Delay Integration) mode of operation and anti-blooming structure

High resolution imaging without satellite slowing. No light spreading due to blooming.

Very long multispectral stripe filters

Assembly of a single substrate with 4 stripe filters over the detector window

Separate the different spectral bands in the FOV. Minimize chromatic aberrations

Highly integrated detection unit

Integrated focal plane and video electronics. Highly integrated ASIC technology

Compact detection function integrated in the camera


Carbon / carbon structure and light-weighted Zerodur optics

Low mass/high thermal stability, highly polished mirror surfaces

Table 6: Introduction of technologies into camera design


Figure 36: Optical configuration of HiRI (image credit: TAS)

Optical assembly: The instrument employs a Korsch all-reflective 4 mirrors telescope design with TMA (Three Mirror Anastigmatic) optics. An additional plane mirror (MR) is used to enhance the instrument compactness. The imaging geometry optimization features a primary mirror size of 650 mm diameter, which suits well to the detectors performance and the orbit characteristics. The instrument architecture chosen is organized around a central plane structure supporting the primary mirror, the tertiary mirror, the plane mirror (MR), and a central cylinder that supports the secondary mirror. The optical assembly consists of an on-axis part (M1 + M2 collector mirrors) and an off-axis part (M3 + MR mirrors) feeding the different focal planes. 75) 76) 77)

The Korsch TMA telescope has a focal length of 13 m and an aperture diameter of 65 cm.


Figure 37: Schematic view of the HiRI instrument elements (image credit: CNES)


Figure 38: Illustration of the FPA (image credit: (TAS)

The optics system of the instrument uses state-of-the-art techniques such as SiC-100 (silicon carbide) material for the mirrors and the telescope structure, specific detectors, and a modular video chain design. EADS Sodern is responsible for the development of the FPA. The FPA is offering a wide variety of new technologies for the imaging function. The size of the observed image is close to 400 mm and is analyzed in 30,000 samples in Pan and 7,500 in MS.. The focal plane assembly consists of two symmetrical arrangements of Pan and MS detectors. The beam splitter is made of a set of mirrors (Figure 38).

The spectral selection is made by optical filters placed very close in front of the detectors. Pan filters and MS stripe line filters are space-qualified multi-layer coatings deposited on glass substrates. Each filter is composed of a high-pass filter and a low-pass filter. An absorbing material deposited between the MS filters isolates each band from the others to avoid interband straylight.


Figure 39: Exploded view of the HiRI camera (image credit: TAS, CNES)

Attitude sensors (star tracker heads and gyroscope heads) are placed on this central instrument structure to improve the performance. A dedicated supporting truss structure ensures the instrument interface with respect to the bus. The detector thermal radiator has its own supporting structure. The instrument design employs carbon material for the structure (the carbide characteristics are: very low coefficient of thermal expansion, very low density, resulting in a light telescope, and a simple thermal control) and Zerodur material for the mirrors.

The instrument focus mechanism is placed onto the tertiary mirror. This position offers an optimum between mechanism and accuracy. The instrument includes also an internal shutter to protect it from sun radiation in non-operational phases such as launch, attitude acquisition, or safe modes. The shutter is placed behind the primary mirror to protect only the tertiary mirror and the detection cavity.

Spectral bands

Pan: 480-820 nm; TDI is only used for Pan data
MS bands in nm
B0= 450-530 (blue),
B1= 510-590 (green),
B2= 620-700 (red),
B3= 775-915 (NIR)

Optical system

65 cm aperture diameter, focal length of 12.905 m, f/20, TMA optics

Spatial resolution, GSD

0.7 m for Pan, 2.8 m for MS bands

Swath width, FOR

20 km at nadir, 60º (FOR=Field of Regard); Each satellite will be able to collect imagery anywhere within an
800 km wide ground strip, covering 200 km in 11 s or 800 km in 25 s, including stabilization time.


> 147 (Pan), > 130 (MS)

MTF in Pan band

0.07 at Nyquist frequency fe/2 (1/2 x 0.7 m-1) Note: "fe" is the sampling frequency (fréquence d'échantillonnage)


Pan array assembly: 5 x 6000 (30,000 pixels cross-track) pixel size: 13 µm
MS array assembly: 5 x 1500 (7500 pixels in cross-track) pixel size: 52 µm

TDI detector data rate

290 Mpixel/s (total) or about 700 Mbit/s per detector; or 3.5 Mbit/s (max)

Data quantization

12 bit per pixel (correlated dual sampling)

Image location accuracy

1 m (with ground control points), 20 m without GCP (99.7%), 10 m (90%)

Image location accuracy

<0.9 pixel Pan over 12 s with a time linear error model (with GCPs)

Line-of-sight frequency

<0.1 pixel (dynamic stability)

Source data rate, downlink

4.5 Gbit/s (max), 465 Mbit/s in 3 x 155 Mbit/s X-band channels

Data compression

Wavelet compression algorithm with an average compression factor of 4

Instrument mass, power

~ 195 kg (< 14 service electronics), ~ 400 W

Instrument size

L < 1594 mm
W < 980 mm
H < 2235 mm

Pointing agility of S/C

Roll of 60º within 25 s; Pitch of 60º within 25 s

Table 7: Characteristics of the HiRI instrument


Figure 40: Pleiades spectral bands (image credit: CNES)

The Pan band of the detector array makes use of back-thinned TDI (Time Delay Integration) with 5 selectable levels from 7 to 20. The size of the detector array assembly is 5 x 6000 (30,000 pixels or samples in cross-track) with a pixel size of 13 µm. The Pan band employs PhotoMOS-type CCDs [note: the PhotoMOS relays have LED inputs and MOSFET outputs that provide input-to-output isolation - comparing favorable with the isolation obtained from EMRs (Electromechanical Relay)]. The detector array is clocked continuously to give a time-delay-and-integrate (TDI) function. The transfer of charge along the CCD is made synchronous with the velocity of the scan image. The integration time is m times longer than a single-detector integration time, where m is the number of stages in a row.

MS bands: Five detector line arrays, each of 1,500 elements (7,500 pixels in cross-track), are utilized for the four MS bands (line arrays). The spacing between the centers of two consecutive lines is 936 µm. Each line array has a pixel pitch of 52 µm.

Each TDI detector outputs data at 58 Mpixel/s (or 290 Mpixel/s total), which amounts to a data rate of about 700 Mbit/s per detector (or 3.5 Gbit/s total in worst case). The MS detectors output at the same frequency their video data. Those video signals are converted in numerical data with individual chains at about 7 Mpixel/s, for maximum SNR performance. The focal plane is physically coupled with the detection electronics to form the integrated detection unit. The overall unit realizes the functions of detection and conversion of video signals in numerical data. The highly integrated design allows a simplification of the data transmission between the focal plane and the detection electronics.
Note: The spectral band definition deviates somewhat from the SPOT instrument series. The Pan band is enlarged, the MS bands are also wider. The MS and Pan viewing planes are separated only by 1.5 mrad in the field (provided by a separation mirror), thus making Pan and MS channel registration possible by a rather simple ground processing (resampling) step.

Detector electronics: The camera system design employs the newly developed SEDHI (Highly Integrated Detection Electronics Subsystem) architecture to support such functions as: a) integrated video processing in the focal plane, b) provision of a high-speed data link, and c) digital onboard processing. 78) 79)

The modular SEDHI concept is implemented on a single board and provides all electronic functions associated to 1 or 2 detectors, from video signal pre-amplification to the digitization of video frame - including various functions such as video signal processing, detector low noise power supply and polarization generation, detector and video processing chain sequencer, detector clock drivers, synchronization interface, command and control interfaces.

The SEDHI concept uses a number of MVPs (Module Video de Proximité) to organize the detection function in the FPA (Focal Plane Array). One MVP is able to process up to 10 CCD outputs, at a maximum pixel rate of 10 Mpixel/s. The high output data rate of a MVP (up to 1.2 Gbit/s) is transmitted downstream through 2 LNTHD (Liaison Numérique Très Haut Débit), which are serial integrated digital interfaces. Two types of hybrid ASICs were developed, a video processing hybrid, and a CCD phase driver hybrid, in support of all processing functions required.


Figure 41: Overview of elements in the integrated detection unit (image credit: TAS)


Figure 42: Illustration of the focal plane assembly (image credit: CNES)


Figure 43: Views of the Pleiades FPA (top and bottom faces), image credit TAS

The full detection electronics consist in 5 panchromatic MVPs, 3 multispectral MVPs, 3 panchromatic MSP (embedded in a single mechanical module) and 1 multispectral MSP. The Pléiades instrument electronics include the MVP functions, the MSP (Module de Servitude de Proximité) and the MSI (Module de Servitude Instrument) dedicated to command / control. The PAN detection electronics is divided in 3 blocks:

• 1 block which includes 2 MVPs and 1 MSP

• 1 block which includes 1 MVP (associated to the panchromatic detector in the center of the focal plane) and 1 MSP

• 1 block which includes 2 MVPs and 1 MSP

The modular SEDHI concept has the potential to support the new generation of Earth observation optical systems (large swath width, reduced ground sampling distance, number of spectral bands, etc.), the modularity, the compatibility - for a large number of missions. This "photon in - bit out" concept may be summarized by: radiometric performance optimization at lowest costs.



Number of PAN video chains

50 at 6.5 Mpixel/s each

Number of multispectral video chains

20 at 3.7 Mpixel/s each

Output data rate

6.2 Gbit/s (useful rate 4.3 Gbit/s)

Size of electronics

463 mm x 237 mm x 246 mm

Mass, power consumption

17 kg (typical), 218 W

Table 8: Overview of the SEDHI detection electronics

Payload data handling: The MS (Multispectral) video data are output from the instrument, at about 4.5 Gbit/s total output rate, and are compressed in the Payload Data Compression Unit. A wavelet algorithm is used, that enables the compression ratio to go up to 7, while in standard operation the ratio is 4.8. Image data are time-tagged in this unit. The compressed data are stored in SSR (Solid State Recorder) with a capacity of 600 Gbit (EOL). The compression module and the SSR are physically in one equipment referred to as COME (COmpresseur MEmoire). The COME output data rate is nominally 465 Mbit/s on three channels at 155 Mbit/s each. The data cyphering, civil and military, is performed in another equipment, namely the DCU (Deciphering and Ciphering Unit). The data are packetized according to CCSDS standards.


Figure 44: Functional block diagram of the HiRI instrument (image credit: TAS)

The data are coded following a trellis-coding scheme in 8-PSK-type modulators that include their own SSPA (Solid State Power Amplifiers). They are then multiplexed, and downlinked with an X-band antenna. The X-band antenna employs a corrugated horn (omni-directional) with a 64º aperture. It is mounted on a 2-axis gimbal mechanism to ensure image downlink during imaging and maneuvering sequences (gimballed gyroscopic actuators give the S/C a high degree of agility). This mechanism is not used during imaging periods to minimize any dynamic disturbances. A dedicated antenna pointing algorithm is developed to orient the antenna during satellite maneuvers so that the ground station always stays in the antenna lobe. In this way, the complete ground station visibility is used to downlink imagery.

Pleiades data acquisition modes and performance capability:

The agile Pleiades satellites are capable to image targets along any ground direction within 47º of a vertical viewing position (with very low maneuver durations between two consecutive imaging scenes. Several types of acquisition modes are defined:

• One-pass acquisition mode: The satellite agility offers the possibility to locally enlarge (widen) the swath by realizing from the same orbit and thus quasi simultaneously the acquisition of several adjacent swaths within the field of regard (FOR). Hence, it should be possible to acquire imagery with an area of approximately 120 km long, and 110 km wide, using the S/C pointing capability (maximal) in roll of 30º.

• Simultaneous stereoscopic or tri-stereoscopic acquisitions mode: This acquisition mode employs a variation of the one-pass mode. Instead of using the agility capabilities to acquire contiguous imagery, the same scene is acquired with two (or three) different view angles as shown in Figure 45.

• Multi-spot mode: Refers to a support mode in which the S/C acquires many spot targets around the S/C ground track, even fore and aft stereoscopic mode if needed. In this mode, the agility capabilities of the satellite are used to acquire the maximum of scenes on a given surface, in one day.


Figure 45: Illustration of various acquisitions modes with HiRI due to the agility of the spacecraft (image credit: Spot Image) 80)

The basic data products of Pleiades are level 0 and level 1 imagery (up to orthorectified imagery). Intermediate products (level-2) are: Mosaicked imagery, DTM (Digital Terrain Model) extracted from stereo pairs.

The main application fields identified for the Pleiades program data fall into the following categories: Cartography, agriculture, forestry, hydrology, geological prospecting, dynamic geology and risk management.

Pleiades is a multi applications, multi sensor and multi partnership program. The first generation will only be furnished with an optical high-resolution imager. Wide-field, superspectral, hyperspectral and thermal (TIR) system observation capabilities are options for future Pleiades implementations (with launches well beyond 2009).


Resolution (m)

Swath Width (km)

Nr. of Bands

Revisit Time (days)

Main applications

Wide Field





Cartography, geology, agriculture, forest, hydrology

Optical HR

≤ 1




Cartography, risk, forest, geology






Agriculture, forest, geology












Forest fires, geology, ocean

Table 9: Optical system identification for possible user needs



Ground segment:

The Pleiades ground segment is composed of a set of user centers located in France, Sweden, Spain and, optionally, in Italy, all of them being interfaced with a dual center in France. Each user center is able to manage the user image acquisition requests and product generations, they include: 81) 82) 83) 84) 85)

- An X-band antenna for data acquisition, 3-channel signal demodulation and ingestion system

- An image processing unit to inventorize, catalog, and archive the data, and to produce imaging products

- A programming unit to manage the mission planning requests

- A set of access units permitting the users to browse the image catalog, submit requests and to receive the ordered products.

1) Astrium Geo- Information Services (formerly SPOT Image) serves the civilian clients.

• Users can consult the civilian images catalog, submit requests and receive the ordered products

• All civilian requests are centralized by Astrium Geo- Information Services

• Astrium Geo- Information Services insures the civilian antenna management as well as the reception and the archiving of raw data received from satellites

• Astrium Geo- Information Services also manages a network of regional image receiving stations (RIRS). The Kiruna station enables to daily receive the Pleiades images, in complement of the Toulouse station; it is managed as a RIRS.

2) The French and Spanish Defence Mission Centers serve the defence users of each country. The basic functions of the Defence Mission Centers are similar to those of the civilian ground segment with some differences in the interfaces, and the security.

3) CNES hosts the dual control center (civil and military). The control center manages the following functions and service requests:

• Monitoring and control of the Pleiades spacecraft

• Hosting of the defence coordination function in support of an optimized work plan to the different partners, taking into account the priorities of each national work plan

• It realizes the planning of all the programmatic requests, by collecting and analyzing all the requests of the civilian and defence users

• It implements and oversees the periodic calibration function of the imaging instrument, for the benefit of all the users.

A very important operational criteria is the devivery of the data products for the commercial customers in record time. This speed represents a key element of the space and ground segment components, built to comply to the user requirements.


Figure 46: Architecture of the Pleiades ground segment (image credit: CNES)

The ground segments were entrusted to CapGemini and CS-SI (programming system), Thales services (image system) and a consortium involving EADS Astrium, Cap Gemini, CS-SI and Thales services (integration of user centers), while INDRA has been given responsibility for the Spanish Defense mission center. The receiving stations have been developed by Zodiac.


Figure 47: Overview of the major ground segment partners of the Pleiades program (image credit: CNES)


Figure 48: Alternate view of the Pleiades ground system architecture (image credit: CNES)


HMA (Heterogeneous Mission Access) implementation:

CNES is in the process to implement the HMA data services, a European initiative by the GSCB (Ground Segment Coordination Body), to the following projects of CNES: 86)

• Catalog Service: SPOT & Pleiades

• Ordering Service: Pleiades, SPOT (in planning)

• Programming Service: Pleiades prototype based, SPOT (in planning)

• Online Data Access Service (future): SPOT & Pleiades

The overall objective of HMA is to establish a harmonized access to heterogeneous EO (Earth Observation) missions' data from multiple mission ground segments, including national missions and the Copernicus/Sentinel missions. HMA's goal is to standardize the ground segment interfaces of the satellite missions to enable easier access to EO data. HMA is managed by GMES (Global Monitoring for Environment and Security) - the European program for the implementation of information services to support decisions concerning environment and security.


Figure 49: Schematic view of HMA implementation at CNES (image credit: CNES)

The long-term HMA goal are rapid and reliable access to time-sensitive information is a significant strategic resource for any community. The EO interoperability benefits are linked to the following high-level objectives:

- Manage and reduce technical risks in EO systems and operations

- Manage and reduce cost of EO systems and operations

- Establish the baseline for the development of the European Space infrastructure capable of harmonizing and exploiting relevant national initiatives and assets

- Allow interoperability within and across organizations

- Increase competitiveness of European Space (and downstream) industries

- Maintain the leadership in EO systems and operations, and avoid the emergence of undesirable standards

- Ensure that technology drivers for the European Guaranteed Access to Space are lead by European requirements.

The HMA project focuses on defining and providing five interfaces:

1) Catalog Service: browsing and retrieving metadata on collections and products across collaborating HMA catalogs

2) Ordering Service: for products identified in a catalog

3) Programming Service: submitting requests for new acquisitions to the HMA partner missions' ground segments

4) Mission Planning Service: facilitating preparation of programming requests

5) Online Data Access Services: retrieving products from the online access archives offered through the HMA.


The GMES program, an EU and EC initiative, with its multiple EO missions and data handling concepts by the various national entities within this program, implied no other way but to start the HMA initiative, a coordination effort of standard interfaces for the benefit of all parties involved (ESA, CNES, DLR, EUMETSAT, ASI, INTA, CSA, DMCii, etc.) including TPM (Third Party Missions) and of course the data user community. 87) 88) 89) 90)

• About 15 European Entities (+ their partners)

• More than 40 EO satellites

• More than 60 instruments — and related ground segments, operations, infrastructure

• Plus around 20 data policies.



Calibration methods of the Pleiades program:

For an earth observing satellite with no on-board calibration source like Pleiades, the commissioning phase is a critical quest of well-characterized earth landscapes and ground patterns that have to be imaged by the camera in order to compute or fit the parameters of the viewing models. It may take a long time to get the required scenes with no cloud, whilst atmospheric corrections need simultaneous measurements that are not always possible. 91) 92)

Performance assessment:

Like other Earth observing space systems, Pleiades has been designed to meet its performance requirements throughout its lifetime. The performance compliance depends on a good knowledge of all parts of the system, from low-level equipment to global chains. This engineering knowledge is used to define useful physical models dedicated to image quality:

• The geometric model is used to compute the location on the Earth of any pixel. It takes into account a geometric modelization of the satellite: orbit determination, attitude estimation, datation, viewing frame determination, focal length adjustment, viewing directions of all detectors, and a ground reference frame.

• The radiometric model is used to convert raw digital counts to TOA (Top-of-Atmosphere) radiance and to normalize the inter-detector sensitivities. It is applied to the pushbroom acquisition principle, since each elementary detector has its own sensitivity to input radiance and its own dark current.

• The resolution model is used to master how details are filtered by the imaging chain, and involves a convolution model by the point-spread function. This model can be handled easily in the Fourier domain where the MTF (Modulation Transfer Function) plays a major role.

Some contributors cannot be modelled and must be minimized by design, like sensor noises. But many parameters can be modelled and calibrated, either during on-ground validation tests or during in-flight operations.

On-ground calibration:

Before launch, the satellite manufacturer runs many tests in order to check the behavior of all the satellite components, and to demonstrate that the requirements are fully compliant. For example, the geometric model is built step by step by combining the different reference frames of the attitude control loop – including sensors and actuators - and the instrument line of sight model. In spite of very accurate measurement instruments like theodolites, this kind of model cannot reach the level of accuracy that is needed for the image location performance where one PAN pixel defines an angle of 1 µrad . That is why a frame correction is scheduled at system or satellite level, in order to compensate for all the uncertainties due to ground conditions or to launch.

Even if a ground sequence test can be considered accurate enough or very representative, the instrument behavior may change after the launch and throughout its lifetime on orbit: on-ground calibration has to be considered as the first characterization before launch. For example, detectors non-uniformity can be measured in front of a integrating sphere during on-ground tests, and the camera best focus can be determined using a collimator on an optical facility, but both of these parameters are expected to vary slightly in orbit and therefore must be updated after launch.

Ground tests are also mandatory to check the right signs of all the signed data : for example, the right sign of the TDI line transfer is compared to the expected velocity of the scene due to the satellite motion.

In-flight calibration:

During the satellite development, the useful parameters of the three image quality models are identified and at least one dedicated calibration procedure has to be defined and validated before launch thanks to simulated images. A lot of experience has been gathered by CNES in the Earth observing systems domain and many calibration procedures rely on this basic principle: if one gets an image of a well-known reference pattern, then one is able to identify the unknown parameters of the model, which links the input scene to the output image.

In radiometric image quality, in-flight normalization and signal-to-noise ratio are classically performed thanks to uniform expanses of snow-covered scenes, absolute calibration is computed on reference photometric sites with a simultaneous atmosphere characterization, the MTF is measured on knife-edge ground patterns.

The geometric model parameters are estimated in two steps. First, the image location biases are tuned thanks to location sites on which many GCPs (Ground Control Points) are available. As these landmarks give the true location of the line of sight, a block adjustment of several images is performed to determine the alignment bias that minimize the location error. Then, the viewing directions of each detector are computed with several methods using inter-images correlation, either relatively between images given by different retinas, or absolutely between an image and a ground orthorectified reference equivalent to thousands of GCPs.

All these calibration methods are very demanding in dedicated images of specific sites, because they may need a lot of images to make an accurate least-square estimation possible, and because it is not easy to get cloud-free images over these sites. The project team can manage the resource sharing during the commissioning phase but the system unavailability during the operational mission must be strictly minimized. Looking for alternate methods that need less usage of ground references is therefore an issue of importance.

Looking from different points of view:

To reduce the in-flight operations, the so-called AMETHIST method has been processed for the first time to be able to compute the parameters of the radiometric model in case of non-linear behavior. An efficient way to bypass the quest of uniformity is to use the satellite agility in order to align the ground projection of the scan-line on the ground velocity. This weird viewing principle (Figure 50) allows all the detectors to view the same landscape. After a pre-processing, that globally shifts each column of the raw image, an image is obtained that contains all needed information. This means that every row contains the set of detector responses to the same landscape. Thus, non-linear normalization coefficients can be computed by a histogram matching method.


Figure 50: AMETHIST acquisition principle (image credit: CNES)

The Pleiades spacecraft is not only capable to be controlled at a specific 3D attitude, but also with a tunable rotation rate. This ability can be used to stop the scanline projection on the ground during the satellite overpass, so that each detector sees the same landscape during the image capture: this is called the steady-mode (Figure 51). This kind of image can be used to compute the SNR, and, combined with a single reference image in the same overpass, can deliver geometrical stability information.


Figure 51: Schematic of the steady-mode guidance principle (image credit: CNES)

Detector normalization:

Several AMETHIST calibration campaigns were performed during the commissioning phase, over a large collection of landscapes that mix Earth, ocean surfaces and clouds in order to get a large set of pixels at different radiance levels.


Figure 52: Example of AMETHIST PAN and XS images (image credit: CNES)

The AMETHIST calibration method gives the same magnitude of residuals as the direct method that compute normalization parameters on uniform snowy expanses, with far less operational constraints. Moreover, it allows a fine monitoring of the in-flight performance that can be compared to pre-flight expectations: up to now, the normalization monitoring confirms the need for an update of the parameters every 6 months, as expected on-ground.

Absolute calibration:

In addition to images of well-characterized landscapes that have been used for years and continuously improved thanks to previous satellites commissioning, the Pleiades project has been taken many images of the Moon since the launch. In a nominal calibration mode, the moon is observed once a month during the descending phase in order to follow the stability of the absolute calibration of the different spectral bands.

The Pleiades project has also regularly acquired imagery of stars since the launch. It is planned to follow the temporal evolution of the absolute calibration of the instrument with these well-known and stable sources without any access conflict of the mission.

Thanks to its total lack of atmosphere and the perfect stability of its surface and thus optical properties, the Moon constitutes an ideal calibration site for Earth observation missions for which the radiometric quality of the data is crucial. In the framework of the Pleiades- 1A and Pleiades-1B in-flight calibration, studies took place in order to determine the calibration precision that could be reached from the acquisitions realized during the different lunar cycles. The POLO data set (Pleiades Orbital Lunar Observations) was born: over 1000 images of the Moons acquired over 6 months for viewing angles varying from -115º to +115º (0º corresponding to the full Moon, 180º, to the new Moon). 93)

The commissioning phase of Pleiades-1A and Pleiades-1B represented the opportunity: 94)

• To acquire a unique dataset of Moon images with a very high spatial resolution (~300 m)

• More than 800 images of the Moon were acquired in only 6 months (guaranty of the stability of the instrument over this time slot)

• An intensive analysis was performed to determine the sensitivity of the method to the different parameters: precision better than 0.5%.

The short term objective is now to use this POLO data set to improve the ROLO (Robotic Lunar Observatory) lunar model, developed by USGS (United States Geological Survey) which is internationally accepted and used by every space agency for the calibration of satellite which are able to aim at the Moon. This new model should then be available to the international community through the CNES participation to the GSICS (Global Space-based Inter-Calibration System).

SNR (Signal-to Noise Ratio):

The radiometric noise behavior has been modelled for years: its variance is equal to an offset plus a linear function of the input radiance. The offset represents the variance of the noise in darkness and can be directly computed on darkness images. The linear part can be computed by different calibration techniques. One of them is the steady-mode, that provides a full set of couples (i.e., radiance mean, radiance standard deviation).


Figure 53: Variance of the radiometric noise computed on steady-mode image (image credit: CNES)

MTF (Modulation Transfer Function):

Three days after the launch, the Pleiades satellite MTF was computed thanks to images of stars in the Pleiades constellation, as a sign of destiny. MTF is the Fourier Transform of the point-spread function, but the actual images of stars undergo aliasing effects because of the sampling and the high level of MTF, especially in the XS bands. Therefore, a preprocessing is applied on a large number of stars to interlace each elementary response to produce a well sampled one. This method delivers a very accurate MTF in two dimensions, whereas previous methods were able to measure the MTF only along one axis.


In conclusion, the Pleiades technological breakthrough has given the opportunity to imagine new methods in a way that serve not only the calibration accuracy, but also the relaxation of operational constraints. These new calibration methods will reduce many time-consuming activities because they often provide a closer access to the final performance without external data. The Pleiades commissioning phase has been an unforgettable experience in engineering enthusiasm; hence, many new ideas and concepts turned into reality. It is time now to keep on looking ahead and up above in order to face the next challenge of high resolution optics — the design and the calibration process of the next generation cameras with embedded active optics control loops (Ref. 91).


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48) M. Benoit Boissin, Alain Gleyzes, Claire Tinel, "The Pleiades system and data distribution," Proceedings of IGARSS (IEEE International Geoscience and Remote Sensing Symposium), Melbourne, Australia, July 21-26, 2013

49) Amit Kumar, "Pleiades Captures Massive Salvage Operation of Costa Concordia," Sept. 19, 2013, URL:

50) "The Costa Concordia salvage operation by satellite," Sept. 18, 2013, URL:

51) "Pleiades Constellation Complete," Astrium, March 2013, URL:

52) "Astrium: operational and commercial launch of the fully complete Pléiades constellation," Astrium, March 19, 2013, URL:

53) Drew Hopwood, "Pleiades-1A and -1B, SPOT-6 & -7 — Status of Astrium GEO-Information Services' EO Satellite Constellation," 12th Annual JACIE (Joint Agency Commercial Imagery Evaluation) Workshop, St. Louis, MO, USA, April 16-18, 2013, URL:

54) "GMES Space Component Data Access Portfolio: Data Warehouse 2011-2014," GSC data access, ESA/ESRIN, Dec. 15, 2012, URL:

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57) Laurent Lebegue, Daniel Greslou, Gwendoline Blanchet, Francoise Delussy, Sebastien Fourest, Vincent Martin, Christophe Latry, Philippe Kubik, Jean-Marc Delvit, Cecile Dechoz, Virginie Amberg, "Pleiades satellites image quality in-orbit calibration and assessment," JACIE (Joint Agency Commercial Imagery Evaluation)Workshop , Tampa, FL, USA, May 4-8, 2015, URL:

58) "Successful launch of Pleiades-1B," CNES, Dec. 02,2012, URL:

59) http://misconceive/PLEIADES/GP_actuality's

60) Jean-Michel Achiever, "Pleiades: operational programming first results," Proceedings of SpaceOps 2012, The 12th International Conference on Space Operations, Stockholm, Sweden, June 11-15, 2012, URL:

61) Laurent Lebègue, Daniel Greslou, Françoise de Lussy, Sébastien Fourest, Gwendoline Blanchet, Christophe Latry, Sophie Lachérade, Jean-Marc Delvit, Philippe Kubik, Cécile Déchoz, Virginie Amberg, Florence Porez-Nadal, "Pleiades-HR Image Quality Commissioning," Proceedings of the 22nd Congress of ISPRS (International Society of Photogrammetry and Remote Sensing), Melbourne, Australia, Aug. 25 - Sept. 1, 2012, International Archives of the Photogrammetry, Remote Sensing and Spatial Information Sciences, Volume XXXIX-B1, 2012, URL:

62) Information provided by Benoit Boissin of CNES, Toulouse, France

63) Peter B. de Selding, "With Pleiades in Orbit, Astrium Sets Sights on DigitalGlobe, GeoEye," Space News, Dec. 19, 2011, URL:

64) Drew Hopwood, "Post Launch Commissioning and Testing of Pleiades 1," Astrium GEO-Information Services, April 2012, URL:

65) URL:

66) "First Pleiades 1A Imagery," Astrium GEO-Information Services, Dec. 22, 2011, URL:

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68) "Airbus Group Takes Off Into 2014 With Joint Brand," Airbus Group, January 2, 2014, URL:

69) "Enhancing Competitiveness – EADS Outlines Plan for Defence and Space Restructuring," EADS, Dec. 9, 2013, URL:

70) Catherine Gaudin-Delrieu, Jean-Luc Lamard, Philippe Cheroutre, Bruno Bailly, Pierre Dhuicq, Oliver Puig, "The High Resolution Optical Instruments for the Pleiades Earth Observation Satellites," Proceedings of the 7th ICSO (International Conference on Space Optics) 2008, Toulouse, France, Oct. 14-17, 2008

71) J.-L. Lamard, C. Gaudin-Delrieu, D. Valentini, C. Renard, T. Tournier, J.-M. Laherrere, "Design of the High Resolution Optical Instrument for the Pleiades HR Earth Observation Satellites," Proceedings of 5th International Conference on Space Optics," March 30 - Apr. 2, 2004, Toulouse, France

72) J.-L. Lamard, L. Frecon, B. Bailly C. Gaudin-Delrieu, P. Kubik, J.-M. Laherrere, "The High Resolution Optical Instruments for the Pleiades HR Earth Observation Satellites," Proceedings of the 59th IAC (International Astronautical Congress), Glasgow, Scotland, UK, Sept. 29 to Oct. 3, 2008, IAC-08- B1.3.5

73) Hélène Ducollet, Christian du Jeu, Jean-Jacques Fermé, "Manufacturing & Control of the Aspherical Mirrors for the Telescope of the Satellite Pleiades," Proceedings of the 7th ICSO (International Conference on Space Optics) 2008, Toulouse, France, Oct. 14-17, 2008

74) Vincent Costes, Guillaume Cassar, Laurent Escarrat, "Optical design of a compact telescope for the next generation Earth Observation system," Proceedings of the ICSOS (International Conference on Space Optical Systems and Application) 2012, Ajaccio, Corsica, France, October 9-12, 2012, URL of paper, : , URL of presentation:

75) P. Pranyies, D. Deswarte, I. Toubhans, R. Le Goff, "SiC focal plane assembly for the Pleiades HR Satellite," Proceedings of SPIE , 'Sensors, Systems, and Next-Generation Satellites VIII,' Roland Meynart, Steven P. Neeck, Haruhisa Shimoda, Editors, Vol. 5570, November 2004, pp. 568-576

76) "Pleiades focal plane technology breakthroughs," Proceedings of the 7th ICSO (International Conference on Space Optics) 2008, Toulouse, France, Oct. 14-17, 2008

77) Bruno Cugny, Benoit Boissin, "CNES Developments in Space Optics," Proceedings of the ICSOS (International Conference on Space Optical Systems and Application) 2012, Ajaccio, Corsica, France, October 9-12, 2012, URL:

78) D. Dantes, J.-M. Biffi, C. Neveu, C. Renard, "SEDHI: Development Status of the Pleiades Detection Electronics," Proceedings of 5th International Conference on Space Optics," March 30 - Apr. 2, 2004, Toulouse, France

79) Christophe Renard, Didier Dantes, Claude Neveu, Jean-Luc Lamard, Matthieu Oudinot, Alex Materne, "From SED HI Concept to Pleiades FM Detection Unit Measurements," Proceedings of the 7th ICSO (International Conference on Space Optics) 2008, Toulouse, France, Oct. 14-17, 2008



82) S. Baillarin, J. Gasperl, C. Dabin, C. Panem, B. Chausserie-Lapree, J.-P- Gleyzes, P. Kubik, C. Lathry, P. Floissac, E. Hillairet, "Remote Sensing Image Ground Segment Interoperability: PLEIADES-HR case study," Proceedings of IGARSS 2006 and 27th Canadian Symposium on Remote Sensing, Denver CO, USA, July 31-Aug. 4, 2006

83) Simon Baillarin, Laurent Lebegue, Philippe Kubik, "Pleiades-HR System Qualification: A Focus on Ground Processing and Image Products Performances, a few months before launch," Proceedings of IGARSS 2009 (IEEE International Geoscience & Remote Sensing Symposium), Cape Town, South Africa, July 12-17, 2009

84) A. Gleyzes, "Ground segment and products," ORFEO Seminar, Paris, Aril 2, 2003, URL:

85) C. Panem, F. Bignalet-Cazalet , S. Baillarin, "Pleiades-HR System Products Performance after in-orbit Commissioning Phase," Proceedings of the 22nd Congress of ISPRS (International Society of Photogrammetry and Remote Sensing), Melbourne, Australia, Aug. 25 - Sept. 1, 2012, URL:

86) C. Dabin, D. Giacobbo, A. Meygret, "Ground Segment Interoperability in the GSCB Missions, Pleiades & SPOT," GSCB Workshop, June 18-19, 2009, ESA/ESRIN Frascati, Italy, URL:

87) M. Eugenia Forcada, H. Laur, B. Hoersch, J. Martin, P. Goryl, G. Ottavianelli, G. Buscemi, S. Badessi, "ESA Missions and Sentinels ground segment interoperability," GSCB Workshop, June 18-19, 2009, ESA/ESRIN Frascati, Italy, URL:

88) "Ground Segment Coordination Body (GSCB)," 2nd Plenary Workshop 2009, June 18-19, 2009, ESA/ESRIN Frascati, Italy, URL:

89) Jolyon Martin, R. Smillie, "DAIL Implementation," 2nd Plenary Workshop 2009, June 18-19, 2009, ESA/ESRIN Frascati, Italy, URL:

90) P. G. Marchetti, Y. Coene, "HMA Standardisation Status," 2nd Plenary Workshop 2009, June 18-19, 2009, ESA/ESRIN Frascati, Italy, URL:

91) Philippe Kubik, Laurent Lebègue, Sébastien Fourest, Jean-Marc Delvit, Françoise de Lussy, Daniel Greslou, Gwendoline Blanchet, "First in-flight results of Pleiades-1A innovative methods for optical calibration," Proceedings of the ICSO (International Conference on Space Optics), Ajaccio, Corsica, France, Oct. 9-12, 2012, URL:

92) Gwendoline Blanchet, Laurent Lebègue, Sébastien Fourest, Christophe Latry, Florence Porez-Nadal, Sophie Lacherade, Carole Thiebaut, "Pleiades-HR Innovative Techniques for Radiometric Image Quality Commissioning," Proceedings of the 22nd Congress of ISPRS (International Society of Photogrammetry and Remote Sensing), Melbourne, Australia, Aug. 25 - Sept. 1, 2012, URL:

93) "Pleiades: towards a new radiometric model of the Moon?," CNES, Nov. 2013, URL:

94) Sophie Lachérade, Ouahid Aznay, Bertrand Fougnie, "POLO (Pleiades Orbital Lunar Observations) - Intensive Study of the Moon and Comparison to ROLO Mode," 22nd CALCON Technical Conference, August 2013, Logan, UT, USA, URL:

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 (

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