Minimize ERS-2

ERS-2 (European Remote-Sensing Satellite-2)

ERS-2 is the follow-up ESA mission of ERS-1. It was in 1989 when ESA decided to continue the ERS program beyond the lifetime of ERS-1. The ERS-2 satellite is essentially a copy of ERS-1, except that it includes a number of enhancements; it is also carrying a new payload instrument to measure the chemical composition of the atmosphere, named GOME (Global Ozone Monitoring Experiment).

ERS-2 has a total mass of 2,516 kg at launch (about 200 kg more than ERS-1). The mission design life requirement was extended to 3 years. ERS-2 has also the same mission objectives as ERS-1, plus an atmospheric chemistry mission objective (with GOME). 1) 2)

The description of the ERS-2 spacecraft and of the common sensor complement can be found under the ERS-1 description.


Figure 1: Artist's view of the ERS-2 spacecraft in orbit (image credit: ESA)


Figure 2: Photo of the ERS-2 spacecraft at ESTEC in 1994 (image credit: ESA)


Figure 3: Basic view of the deployed ERS-2 spacecraft (image credit: ESA)

Launch: The launch of the ERS-2 spacecraft took place on April 21, 1995 from Kourou on an Ariane-4 vehicle.

Orbit: Sun-synchronous polar orbit (retrograde orbit). Altitude = 780 km (mean); inclination = 98.5º, local crossing time of the equator = 10:30 AM, orbital period is about 100 minutes. Repeat cycle = 3 days or 35 days.


ERS-2 mission status:

• The ERS-2 mission ended on Sept. 5, 2011, after the satellite's average altitude had already been lowered from 785 km to about 573 km. At this height, the risk of collision with other satellites or space debris is greatly reduced. - The final critical step was to 'passivate' ERS-2, ensuring that all batteries and pressurised systems were emptied or rendered safe in order to avoid any future explosion that could create new space debris. This primarily consisted of burning off the fuel, disconnecting the batteries and switching off the transmitters.

With the effects of natural atmospheric drag, ERS-2 is predicted to enter and largely burn up in the atmosphere in about 15 years. This is well within the 25-year-limit that is imposed to minimise the risk of collision before reentry. 3)

• ESA retired the ERS-2 spacecraft in early July 2011 to avoid ending up with the mission as a piece of space debris. ERS-2 has been delivering data right to the end. After orbiting Earth almost 85,000 times, the risk that the satellite could lose power at any time was clearly high. The deorbiting procedures were started on July 6, 2011 at ESOC with the goal to lower the satellite's orbit from its current altitude of 800 km to about 550 km, where the risk of collision is minimal. Eventually, ERS-2 will enter Earth's atmosphere and burn up.

ERS-2 spent 16 years in orbit, gathering a wealth of data that has revolutionized our understanding of Earth. This pioneering mission has not only advanced science, but also forged the technologies we now rely on for monitoring our planet. 4)

• The ERS-2 spacecraft is “operating nominally” in early 2011 (the approved mission extension goes up to the end of 2011).

However, ERS-2 will cease its operations in mid-2011, after 16 years of successful activity. Preparations for the subsequent decommissioning and deorbiting have started. Before the end of its mission, ERS-2 is being exploited to the maximum of its capabilities, within the constraints of its ageing equipment. Until the Envisat orbital change of October 2010, ERS-2 was used for specific SAR Interferometry (InSAR) campaigns in tandem with Envisat. - A new ERS-2 mission phase, with a three-day repeat cycle, is being prepared for the few months before the end of the mission. This phase will repeat the ERS-1 Ice Phases of 1992 and 1994, almost 20 years later, taking advantage of the availability of GPS network supporting atmospheric corrections for InSAR applications. 5)

• Adding to their unique information from previous tandem missions, ESA’s ERS-2 and Envisat satellites have been paired up again – for the last time. Data from this final duet are generating 3D models of glaciers and low-lying coastal areas. 6)

The fourth tandem interferometric campaign, from July to October 2010, focused on low-lying coastal areas, such as New Orleans in USA and the Po River Mouth in Italy. This information will be used for various applications in many different fields, in particular for creating accurate DEMs of coastal areas that could be used to help manage floods.

• On April 21, 2010, the ERS-2 celebrated its 15th anniversary on orbit. 7)

• The ERS-2 spacecraft is “operating nominally” in early 2010, more than 14.5 years after launch (nominal mission life of 3 years). A mission extension was approved to the end of 2011. 8) 9) 10) 11)

- The S/C performs gyroless operations since mid-2001

- The gyroless data are being Doppler screened removing the attitude uncertainty

- The SAR instrument works satisfactorily

- In June 2003, ERS-2 lost its onboard data storage capability, effectively ending its global coverage capability. However, a network of SAR data acquisition stations provides a good coverage (real-time data reception).

In 2009, the ERS-1 and ERS-2 missions have a cumulative 18 years of ERS-1/2 data in the archive, representing the most complete and consistent SAR archive.

Envisat / ERS-2 SAR tandem interferometry missions. The objective was to: a) measure the velocity of fast moving polar glaciers (> 200 m/year). ERS/Envisat SAR data should be suited to map velocities of 1 cm between the two 30 minute passes; and b) to generate accurate low relief Digital Elevation Models. This is of particular interest for many low elevation delta regions, in particular for polar areas (North Canada, North Russia) where there is no available SRTM DEM information. 12) 13)

- The second tandem mission started on Nov. 23, 2008 and ended in late April 2009 (both spacecraft acquired data over the same area just 28 minutes apart). The second campaign was due to end in late January 2009, but could be extended through to late April 2009 due to the excellent performance of the satellites and the strong teamwork between the mission data teams at ESRIN, and ESOC. -- After the completion of the tandem mission, ERS-2 drifted naturally (without maneuvering) to its reference orbit.

The second tandem mission also had perfect timing due to the occurrence of low solar activity, which is very favorable for ERS-2 attitude stability, and the fact that ERS-2 could be left to quickly drift back to its nominal orbit without using additional resources. 14)

- The first SAR tandem mission took place from September 2007 to February 14, 2008. This required a temporal modification of the ERS-2 orbit (2 km off-set versus nominal ground track) to have optimal interferometric baselines between ERS-2 and Envisat (30 min. separation).

• Status of the PRARE mission: On Dec. 31, 2007, the fully functional onboard PRARE instrument was retired. The reason: The design of the PRARE ground segment was conceived for an operational period of 4 years; only a lot of 29 ground stations was provided on a global scale. After the German national funding ran out at the end of 2002, it became increasingly difficult to operate the PRARE system when ground stations experienced a hardware failure. Eventually, this resulted in 2 fully functional ground stations at the end of 2006. As a consequence, the PRARE instrument was switched off at the end of 2007. 15)

• Instrument and spacecraft performance reviews took place in December 2006 with the main outcome that ERS-2 can be operated for several years - assuming that measures compensating for aging are being applied during 2007. The AOCS continues to be operated in Zero-Gyro mode for “fine mode” support and in mono-gyro mode for the “coarse mode” support.. The AMI SAR instrument is now being operated with an average duty cycle of 3.5 minutes per orbit.

• In late 2007, ESA approved a 3-year extension the ERS-2 mission operations to the end of 2011. In 12 years of operations, only 50% of the onboard fuel had been used (hence, a further extension might be granted). Since Sept. 2007, the ERS-2 orbit has been shifted for a four month trial of 30 minute ERS- Envisat interferograms (although this only works for high northern latitudes). One successful application has been measuring the fastest glacier in the world (14 km/year in Greenland) which could not be measured previously.

• The ERS-2 spacecraft reached 10 years in orbit on April 21, 2005, a remarkable engineering achievement. All platform subsystems and payload instruments are working “nominally” and are providing good data.

Close collaboration between ESA and EADS Astrium resulted in the successful implementation of a gyroless or ZGM (Zero-Gyro Mode) of operation. The ZGM software was loaded on June 6, 2001 and activated onboard. The first period of recommissioning lasted until the end of July 2001. In Nov. 2001, the tuning was improved to cover all data products. The ZGM represents a re-design of AOCS, making extended use of the platform's sensors and actuators to compensate for the lack of gyroscopes. The goal is to extend the ERS-2 mission until MetOp-1 becomes operational in 2006. However, one consequence of renewed ERS-2 operations is that ATSR-2 high-rate operations are suspended since the Wind/Wave mode is used for S/C attitude control (only within narrow limits can the ATSR-2 HR mode be operated).

• In June 2003, ERS-2 lost its onboard data storage capability, effectively ending its global coverage capability (tape recorder A stopped functioning June 22, 2003 while tape recorder B failed Dec. 20, 2002). - This implied that only real-time observations could be supported starting by the end of June 2003. From now on, the spacecraft returns data when in line of sight of an appropriately equipped ground station. And because the majority of such stations are found around Europe and Canada, ensuring good observation of the North Atlantic, ERS-2 coverage of these regions has been able to continue.

• Some control mode changes were required after the failure of the onboard tape recorders. The new strategy, referred to as R-YCM (Regional Yaw Control Monitoring) is based on a limited set of data. Orbit and attitude control are sufficient to support ERS-2 data use. However there are some limitations for InSAR use. 16) 17)

• The ERS-2 satellite was piloted in the nominal yaw steering mode, using 3 gyroscopes out of 6 available, from launch until Feb. 2000. During this period, there were several problems with the gyroscopes. [in 1997, the S/C lost gyro #2 and in 1998 a pointing anomaly on gyro #3 made it unreliable]. The measures implemented in Feb. 2000 to protect the satellite against further gyroscope failures have allowed the continuation of the ERS-2 operations, despite two major anomalies that took place in Jan. 2001 (during this period, the S/C was piloted using one gyroscope). Under normal conditions these would have meant the end of the ERS-2 mission, but the measures implemented meant that the effects were limited to the interruption of service for about one month and temporary degradation of data quality. 18) 19) 20)


Sensor complement: (AMI, ATSR-2, RA-1, LRR, PRARE, GOME)

The descriptions of AMI, RA-1 and LRR can be found under the ERS-1 mission. Here, only ATSR-2, GOME and PRARE are being described.


ATSR-2 (Along-Track Scanning Radiometer and Microwave Sounder-2):

The IRR instrument of ATSR-2 was upgraded for the ERS-2 mission by adding three more bands in the visible range to provide data for vegetation studies. The channels are accommodated by the addition of a second focal plane assembly (FPA). The center wavelengths of the VIS channels are at 0.555, 0.659, and 0.865 µm (the IR channels are at 1.6, 3.7, 10.85 and 12 µm). The VIS channels are calibrated through a complex procedure using sunlight.21)

Major mechanical modifications were made to the ATSR-2 Infrared Radiometer (IRR). The carbon-fiber structure has been substantially re-designed, the vestigial ATSR-1 optical bench has been removed, and all optical elements are now mounted directly onto the structure.

With the addition of GOME (Global Ozone Monitoring Experiment) for the ERS-2 mission, and the need to interface this experiment to the satellite via the ATSR-2's DEU (Digital Electronics Unit), it became important to add more redundancy to the latter as it now interfaces with the IRR, the MWR and GOME. A second identical DEU was therefore added to the payload module, together with a DEU Switching Unit (DSU).


Figure 4: Schematic of the configurations of the IRR, MWR and DEU aboard ERS-1 and ERS-2 (image credit: ESA)


Figure 5: The measurement principle of the ATSR-2 instrument (image credit: ESA)


Figure 6: Schematic view of the ATSR-2 optical components (image credit: ESA)

The visible channels are calibrated with a visible calibration unit, as shown in Figure 7. Calibration takes place close to the time of local satellite sunset, when the sun is 13º below the tangent to the Earth's surface at the satellite's nadir point. The nadir- and forward-viewing baffles are designed to exclude stray radiation from entering the calibration system, which would degrade its accuracy.


Figure 7: Optical components of the visible calibration system (image credit: ESA)

The increased data flow on ATSR-2 called for a new set of data compression algorithms. In addition, uncompressed infrared and visible data can be transmitted in a high-data-rate mode, which provides double the normal throughput. This mode is limited, however, to the periods when other payload instruments are not making full use of the X-band data capacity.


GOME (Global Ozone Monitoring Experiment):

GOME (also referred to as GOME-1) is an ESA-funded instrument developed and built by an industrial consortium in the time frame 1990-1994. The industrial consortium consisted of the Italian firms Officine Galileo and Laben (main electronics and electronic interface with ERS-2), British Aerospace (joint usage of the ATSR digital electronic interface), and the Dutch firm TPD (optical concept, calibration unit, pre-flight calibration). The German Remote Sensing Data Center (DFD) of DLR got the mandate to develop the GOME data processor system in collaboration with other institutes involved in the GOME Science Advisory Group.

GOME is a cross-track scanning optical double spectrometer (or double monochromator), a nadir viewing instrument. The double spectrometer operates in the spectral range of 240 - 790 nm with a good spectral resolution of 0.2 - 0.4 nm; this decomposition is done in two steps: first by a quartz predisperser prism, from which the light is split into four different channels. Each of the four channels is equipped with a 1024-pixel linear diode array detector. The resulting spectral resolution is 0.2 nm in UV and 0.4 nm in the VNIR spectrum.

The gooal of GOME is to observe upwelling solar radiation reflected or scattered in the Earth's atmosphere and from its surface. The measured spectrum contains absorption features which can be used to derive quantitative information on the presence of ozone, and of a number of other atmospheric species. In addition to the improved backscattering technique, GOME exploits the full capabilities of the enhanced ATSR-2. The GOME measurement concept is based on `Differential Optical Absorption Spectroscopy' (DOAS), a technology proven in balloon flights. 22) 23) 24) 25) 26) 27) 28) 29) 30) 31)

GOME science objectives: measurement of total column amounts and stratospheric and tropospheric profiles of ozone on a daily basis. - In addition: measurement of column amounts of H2O and other gases involved in ozone photochemistry (like NO2, OClO, BrO, and possibly ClO in anticyclonic conditions, and pollutants like SO2 and HClO). GOME can also be used to investigate the distribution of atmospheric aerosols and clouds-plus-surface spectral reflectance.

The GOME instrument consists of the following functional modules:

- the spectrometer

- the four FPAs (Focal Plane Assembly)

- the calibration unit

- the scan electronics unit assembly

- the PMD (Polarization Measurement Device)

- the DDHU (Digital Data Handling Unit)

- the optical bench structure

- the thermal control unit.


Figure 8: Schematic view of the GOME instrument elements


Figure 9: Spectrometer optics layout of the GOME instrument (image credit: ESA, SRON)


Figure 10: Partial view on the spectrometer optics (image credit: ESA, SRON)


Figure 11: Schematic layout of the GOME optics elements (image credit: (image credit: University of Bremen, ESA)

Its main mode of operation is nadir looking, but it is also able to look at the sun and the moon for calibration purposes. For onboard calibration, GOME does not depend on one technique, but seeks to exploit several. Both absolute radiometric and wavelength calibrations are performed. This means that GOME retrieves ozone distributions by exploiting the traditional backscatter approach, as well as by the more novel differential optical absorption spectroscopy.

The IFOV (2.8º x 0.14º), corresponding to the projection of the spectrometer slit on the Earth, is a narrow rectangle 40 km (along-track) x 2 km (across-track). A scan mirror sweeps the IFOV in the cross-track direction in three steps (normal mode), a ±31º scan (max). Maximum swath width = 960 km with corresponding pixel sizes of 40 km x 320 km. Smaller pixel sizes of 40 km x 40 km can be commanded (resulting smaller swath). With the 960 km swath global coverage can be achieved within three days. Calibration is performed with regular views of the sun; in addition, a wavelength calibration lamp is used for wavelength stability. As the instrument is sensitive to polarization of incoming radiation, a polarization detector monitors one polarization direction in the broadband channels corresponding essentially to detectors 2-4. GOME data rate = 40 kbit/s. GOME data are processed, archived and distributed at DLR/DFD.

GOME spectral bands:

- Channel 1A + 1B (237 -316 nm), 512 channels; [the Hartley bands of O3 and NO emission are the dominant features]

- Channel 2 (311 - 405 nm), 1024 channels; [a variety of target species absorbs in regions such as O3 (Huggin's band), O4, NO2, HCHO, SO2, BrO and OClO]

- Channel 3 (405 - 611 nm), 1024 channels; [the target molecules for this region are: NO2, OClO, O2, O3, (Chappius band), O4 and H2O]

- Channel 4 (595 - 793 nm), 1024 channels; [the target molecules are: O3 (Chappius band), NO3, H2O, and O2]

A combination of channels 2 to 4 can be used to make measurements of O2 and O4 column amounts (radiation penetration depths, cloud top heights).





Spectral range

240 - 790 nm

Spectral resolution

0.2 - 0.4 nm

Spatial resolution

320 km x 40 km

No of spectral channels


Swath width

120 - 960 km

Polarimetric channels


Calibration system

spectral lamp,
solar diffuser

Instrument size

60 cm x 70 cm x 50 cm

Instrument mass

50 kg

Power, bus voltage

50 W, 22 V

Table 1: Overview of some GOME characteristics


Figure 12: The mechanical assembly of the scan unit (image credit: ESA)


Figure 13: Illustration of the GOME calibration unit (image credit: ESA)


Figure 14: The GOME instrument package during an instrument vibration test (image credit: ESA)


PRARE (Precise Range And Range-Rate Equipment) tracking system

PRARE is a microwave tracking system operating at centimeter accuracy levels for the measurement of satellite to ground range and range rate. The concept is based on an autonomous spaceborne two-way and dual frequency microwave tracking system with its own telemetry, telecommand, data storage, timing and data transmission capabilities. This allows data analysis on a global basis within a very short time delay. Due to the microwave transmission concept, the system operates independently from weather and daylight conditions.

Background: The initial PRARE system development started in 1982 in Germany as a response to ESA's announcement of opportunity for exploitation of Europe's new Earth-remote sensing satellite series starting with ERS-1. The project was funded by BMFT and DARA, defined/designed by Ph. Hartl (University of Stuttgart) and Ch. Reigber of DGFI (German Geodetic Research Institute), Munich and since 1992 of GFZ (GeoForschungsZentrum), Potsdam. The space segment was built by Kayser Threde of Munich, and TimeTech GmbH of Stuttgart; the ground stations were developed by Dornier GmbH, Friedrichshafen. 32) 33) 34) 35) 36)

On ERS-1, the PRARE onboard instrument suffered a destructive RAM latch-up - resulting in a complete loss of the instrument operations about a week after the spacecraft launch. However, PRARE was successfully flown on the Russian mission Meteor-3-7 (launch: Jan. 25, 1994) as a passenger payload and a proof-of-concept mission for all PRARE subsystems. PRARE operations onboard Meteor-3-7 lasted for over a year providing excellent results; the operations were terminated in 1995 after completion of all tests.

PRARE is also flown on ERS-2 (ESA procurement). It is in “operational status” as of Jan. 1, 1996 (i.e. the routine range and range rate product generation started on Jan. 1, 1996) providing measurement accuracies between 2.5 and 6.5 cm (two-way range data) and 0.1 mm/s (two-way range-rate data) respectively. PRARE operations are fully autonomous and separate from ERS-2 operations. 37) 38)

The PRARE system consists of three major components:

1) Space Segment: This is a small self-contained hardware unit with a mass of 19 kg, power consumption of 39 VA (operational), or 8 VA in standby mode, and communication links independent of the host satellite.

2) Ground Station Network: The network consists of small automated and transportable ground stations (whose positions are known or can be determined from PRARE data to high precision). At X-band a ground station works as a regenerative and coherent transponder, at S-band a station acts as a receiver for the transmitted signals and measures the difference of the time of arrival of both signals.

3) Control Segment consisting of:

- GFZ's Master Station located at DLR in Oberpfaffenhofen, Germany

- TimeTech's Monitoring and System Command Station in Stuttgart, Germany

- A Calibration Station in Potsdam, Germany

These stations have special data evaluation, system control, and communication capabilities, which allow to fully control the space segment on ERS-2 as well as each individual ground station via the primary PRARE microwave links. This unique feature makes the PRARE system operations independent from the host satellite (except for power) and adaptable for any near-Earth communication, navigation, or observation satellite system.

Applications: The high quality measurement of the PRARE data as well as their good global repeatability, density, and spatial distribution suit the data for deriving several higher-level geodynamic products for such applications as: 39)

- Precise satellite orbits

- Ground station coordinates

- Earth gravity field and Earth orientation parameters

- Ionospheric parameters

- Ultra-stable clock time information.

PRARE measurement principle:

Two continuous signals are emitted from the space segment to the ground, one of which is in S-band (2.2 GHz), the other in X-band. Both signals are modulated with a PN-code (pseudo random noise, 1 MChirp/s for the S-band and 10 MChirp/s for the X-band) used for the distance measurement and containing data signals (broadcast information) for ground station operation (prediction of orbit visibility, etc.). The time delay in the reception of the two simultaneously emitted signals is measured at the ground stations with an accuracy of better than 1 ns; the result is retransmitted and stored in the on-board memory of PRARE for later ionospheric correction of the data.

In the ground station the received X-band signal is transposed to 7.2 GHz, coherently modulated with the regenerated PN code (or with one of three orthogonal copies for code multiplexing) and including the two-frequency delay data as well as housekeeping and meteorological ground data is retransmitted to the PRARE space segment.

X-band uplink

- 7225.296 MHz (carrier frequency)
- PN-code = 10 Mbit/s, BPSK (bandwidth = 10 MHz)
- Low rate data = 16 bit/s code-biphase modulation
- High rate data = 1 kbit/s mod(2)-add.

Ground transponder power

60 cm parabolic dish, 5 watts transmit

X-band downlink

- 8489 MHz (carrier frequency)
- PN code =10 Mbit/s, BPSK (bandwidth = 10 MHz)
- Low rate data = 16 bit/s code-biphase modulation
- High rate data = 2/4/10 kbit/s mod(2)-add.

S-band downlink

- 248 MHz (carrier frequency)
- PN-code = 1 Mbit/s, BPSK (bandwidth = 1 MHz)
- Low rate data 16 bit/s code-biphase modulation
- High rate data 2/4/10 kbit/s mod(2)-add.

Satellite antennas

Crossed dipoles at X-band and S-band, 1 W in downlink and 5 W in uplink transmission power

Noise values

±1.5 cm rms for X-band ranging (1 measurement/s)
±0.05 mm/s rms for X-band Doppler (30 s integration time, 90º elevation)

Bias values

<1 cm for X-band; <3 cm for S-band (after post-processing)

Range-error estimation

Tropospheric error: 2-7 cm; ionospheric error <1 cm;
Thermal noise and calibration error: 2-3 cm;
Antenna phase center uncertainty <1 cm

Total ranging accuracy

2.5-6.5 cm (root squared sum)

Total range-rate accuracy

0.1 mm/s rms (root squared sum)

Table 2: PRARE system characteristics and measurement precision parameters

The bandwidth-spread PRARE signals serve simultaneously for the primary ranging purposes and for transmission of all necessary data among the system components. Both the user ground station network and the control segment can decode these superimposed data and react according to the information contained.


Figure 15: The signal structure of PRARE measurements (image credit: GFZ Potsdam)

PRARE space segment:

The PRARE space segment has been developed and partly manufactured by the University of Stuttgart's Institute of Navigation (INS), later by the private company TimeTech GmbH, Stuttgart. It consists of a compact electronics box (dimensions 400 x 210 x 180 mm, power consumption 30 W in operational mode and 8 W in stand-by) and two crossed dipole antennas for transmission of the X-band and S-band signals. The X-band antenna also receives the microwave signal after it has accomplished the round-trip transmission.

The space segment design features four independent, parallel, strictly coherently operating receiver channels which track up to four PRARE ground stations that are in view of the satellite simultaneously. This allows to generate overlapping measurement data used for internal calibration and for back-up of the main orbit solution. This required a very careful internal hardware design and sophisticated control of all modules.

The very heart of the whole PRARE system is the internal oscillator of the space segment which is not only responsible for time tagging of the signal generation and communication processes, but in fact controls the complete system synchronization in ultra-short- (up to 1 second), in short- (up to 1000 seconds) and in long-term (more than 1000 seconds):

• Control of the internal coherency of the space segment signals, both for range and range-rate measurement data as well as for inter-channel coherency

• Time control of the whole ground station network by periodic synchronization pulse generation and transmission.

The PRARE space segment oscillator is an ultra-stable voltage controlled quartz-crystal oscillator (VCXO) designed in BVA technique, and a state-of-the-art type of quartz oscillator. The primary output frequency is 5 MHz, which is divided/multiplied by the space segment electronics to generate all the frequencies necessary within the system.


Figure 16: The PRARE-2 instrument during integration (image credit: GFZ Potsdam)

PRARE ground segment:

Dedicated ground stations are used, which are acting basically as a regenerative transponders. A PRARE ground transponder consists of:

- An antenna unit with an offset antenna of 60 cm diameter (parabolic dish), fronted electronics and tracking system. The antenna s fully movable in azimuth and elevation to track the satellite from horizon to horizon (weight 42 kg including gearing unit)

- An electronics unit including RF-modules (dimensions 560 x 560 x 300 mm, weight 35 kg), linked together by RF-signal and data cables. The electronic tracking loops filter the received microwave signal, decode the superimposed data (low-rate modulation), which contain dedicated information for each individual ground station, transpose the microwave frequency to the uplink (fixed frequency ratio 749/880), re-modulate new site-specific low-rate information, and send the signal back to the satellite.

The PRARE ground station tracking network consists of 29 PRARE transponders in total (globally distributed), which are owned by 10 different international geodetic research groups (plus GFZ) and operated locally by co-operating scientific institutions.


Figure 17: View of a PRARE ground station (image credit: GFZ Potsdam)


Figure 18: External PRARE system calibration by simultaneous SLR observations (image credit: GFZ Potsdam)

During satellite contact, the main tasks of the ground station modules are:

- X-band signal transponding

- Measurement of the delay difference between the quasi-simultaneously transmitted S- and X-band signals

- Measurement of the internal X-/X-signal path delay

- Meteorological data handling, acquired at the ground station site

- Clock pulse and time generation and synchronization

- Low-rate and high-rate data reception and interpretation

- Low-rate data transmission

- Setup and calibration data interpretation and storage.


ERS Tandem Mission (Oct. 1995 to June 1996)

In 1993, the ERS science community realized that a future tandem mission of the healthy ERS-1 spacecraft and a planned launch of the ERS-2 satellite in 1995 would be a great possibility for interferometric experimentation in SAR observations. As a consequence, the ESA Council adopted a resolution in March 1995 - with the objective to provide ERS-1/2 tandem mission operations for a nominal period of 9 months (starting with the ERS-2 operational phase) and to keep ERS-1 operational at least until April 1997. 40) 41) 42)

In the orbital tandem configuration has both spacecraft in the same orbit, ERS-2 follows ERS-1 with an approximate delay (referred to as orbit phasing) of 35 minutes. The configuration was that of two-pass measurements of a single-antenna SAR platform (the same SAR instrument on both satellites observing the same area on the ground), permitting the superposition technique of imagery (in data processing) of fairly close repeat tracks. Due to the phasing and the Earth's rotation, the ground-track patterns of ERS-2 are slightly shifted westwards with respect to those of ERS-1. The orbit phasing is adjusted in such a way that the ERS-2 track coincides exactly with that of ERS-1, however 24 hours earlier. The benefits of tandem operations are the following:

• When the same area of the Earth is observed by the same instrument on both satellites with a ground-site revisiting interval of 1 or 8 days, the improvements compared to a single satellite are:

- the number of acquisitions in a repeat cycle (35 days) is doubled

- the time interval between two successive acquisitions is shorter, being 1 to 8 days rather than 35 days

• For global applications, such as wind scatterometer data, coverage is doubled within a given time period

• When the ground-track pattern of nadir-looking instruments on one satellite overlap ground tracks of side-looking instruments on the other satellite, then their information can be combined, providing synergistic benefits.

The greatest benefit of the tandem mission is seen in SAR interferometry providing excellent temporal (1 day interval) and spatial coherence. This technique requires two separate images taken of the same ground track by two spatially-separated antennas (the interferometric baseline) to produce phase differences from slightly different viewing angles. For each pixel corresponding to the same area of the ground in both images, the phase values (depending on the satellite-to-ground pixel length) are subtracted to produce a phase difference image known as the `interferogram.' With the orbit of both satellites known, the phase interferogram can be used to generate a DEM (Digital Elevation Model) of the surface with an accuracy of about 10 m. An additional product of interferometry is the so-called `coherence image,' which shows bright areas where the coherence between to SAR images is high, indicating no variation in backscatter between the acquisition times of the two images. Dark regions indicate areas where changes have occurred.

ERS-1 and ERS-2 have been in tandem operations since about September 1995. The tandem mission was completed after nine months of successful operation in May/June 1996. About 110,000 ERS SAR pairs of data were acquired during the tandem mission, covering nearly the whole global land surface. Over South America and part of Southeast Asia, just one data pair was acquired. As many as five or six interferometric pairs are available for Europe and North America, allowing greater accuracies to be achieved. 43) 44)

The ERS Tandem Mission encompassed the following combinations of instrument data:

• The same instrument on both satellites observing the same area on the ground with a one-day interval, e.g. for SAR interferometry and/or change detection. ERS SAR interferometry had already been validated using ERS-1 data only, with a 3 or 35-day repeat cycle. The one-day offset offered by the tandem mission increased the probability of having high coherence between the acquired data

• The same instrument on both satellites observing different areas on the ground on the same day, to provide increased spatial sampling

• Different instruments observing the same areas on the ground with a very short interval (less than 1 hr), e.g. the AMI-SCAT (wind scatterometer mode) and the Radar Altimeter for comparison of wind measurements.

The ERS tandem mission generated a large resource of interferometric SAR data (InSAR) for analysis in the geosciences.

Nominal observation services of each mission (ERS-1 and -2) commenced after completion of the tandem mission in June 1996.

1) C. R. Francis, G. Graf, P. G. Edwards, M. McCaig, C. McCarthy, A. Lefebvre, B. Pieper, et al., “The ERS-2 Spacecraft and its Payload,” ESA Bulletin, No. 83, Aug. 1995, pp. 13-31,

2) G. Duchossois, P. Martin, “ERS-1 and ERS-2 Tandem Operations,” ESA Bulletin, No. 83, August 1995, pp. 54-60

3) “ERS satellite missions complete after 20 years,” ESA, Sept. 12, 2011, URL:

4) “Pioneering ERS environment satellite retires,” ESA, July 5, 2011, URL:

5) “ERS-2 status,” ESA Bulletin, No 145, Feb. 2011, p. 81

6) “Last 'tango' in space,” ESA, Nov. 2, 2010, URL:

7) “ERS-2 Satellite Celebrates 15th Anniversary,” April 21, 2010, URL:




11) Henri Laur, “SAR Interferometry opportunities with the European Space Agency: ERS-1, ERS-2, Envisat, Sentinel-1A, Sentinel-1B, ESA 3rdParty Missions (ALOS),” Fringe 2009 Workshop - Advances in the Science and Applications of SAR Interferometry, Frascati, Italy, Nov. 30-Dec. 4, 2009, URL:

12) “ESA satellites flying in formation,” Dec. 3, 2008, URL:

13) M. A. Martín Serrano, M. A. García Matatoros, M. E. Engdahl, “Achieving the ERS-2 - Envisat inter-satellite interferometry tandem constellation,” URL:

14) “ESA's old EO missions perform sophisticated new tricks,” April 29, 2009, URL:

15) The information was provided by Franz-Heinrich Massmann of GFZ (GeoForschungszentrum), Berlin, Germany

16) N. Miranda, B. Risich, C. Santella, M. Grion, “Review of the Impact of the ERS-2 Piloting Modes on the SAR Doppler Stability,” Envisat and ERS Symposium, Salzburg, Austria, Sept. 6-10, 2004, ESA publication SP-572

17) W. Lengert, “ERS missions overview,” Fringe Workshop 2003, ESA/ESRIN, Frascati, Italy, Dec. 1-5, 2003

18) Project News, ERS, ESA Earth Observation Quarterly No 69, p.4, June 2001

19) Project News, ERS, ESA Earth Observation Quarterly No 70, p.4, January 2002

20) X. Neyt, P. Pettiaux, M. Acheroy, “Scatterometer Ground Processing Review for Gyro¿Less Operations,” Proceedings of SPIE, Vol. 4881, 9th International Symposium on Remote Sensing, Aghia Pelagia, Crete, Greece, Sept. 23¿27, 2002

21) N. Stricker, A. Hahne, D. L. Smith, J. Delderfield, M. B. Oliver, T. Edwards, “ATSR-2: The Evolution in its Design from ERS-1 to ERS-2,” ESA Bulletin No. 83, August 1995, pp. 32-37

22) ESA 1998: GOME Special, Earth Observation Quarterly No. 58, March 1998

23) “The GOME Spectrometer,” URL:

24) C. Zehner, G. Pittella, “Preparing atmospheric applications for future ESA Earth-observation missions in the frame of the data user program, ESA Earth Observation Quarterly No. 61, Feb. 1999, pp. 1-6

25) C.J. Readings, `The Interim GOME Science Report,' Feb. 1990,

26) `The Global Ozone Monitoring Experiment (GOME) and ERS-2,' Earth Observation Quarterly, ESA periodical No. 32 Dec. 1990

27) A. Hahne, et al., “GOME: A New Instrument for ERS-2,” ESA Bulletin, No. 73, February 1993, pp. 22-29

28) GOME Global Ozone Monitoring Experiment, Interim Science Report, ESA SP-1151, September 1993

29) J. P. Burrows, M. Weber, M. Eisinger, “The Global Ozone Monitoring Experiment - GOME,” SPARC Newsletter 09, July1997

30) J. P. Burrows, M. Weber, M. Buchwitz, V. Rozanov, A. Ladstätter-Weissenmayer, A. Richter, R. DeBeek,R. Hoogen, K. Bramstedt, K.-U. Eichmann, M. Eisinger, D. Perner, “The Global Ozone Monitoring Experiment (GOME): Mission concept and first scientific results,” Journal of Atmospheric Science, Vol 56, January 15, 1999, pp. 151-175 , URL:

31)) A. Hahne, A. Lefebvre, J. Callies, B. Christensen, “GOME - The Development of a New Instrument,” ESA Bulletin No. 83, August 1995

32) P. Hartl, C. Reigber, “Das PRARE-System der ERS-1 Mission,” Geowissenschaften Vol. 9, No. 4/5, 1991, pp. 156-162

33) P. Hartl, C. Reigber, “Das Satellitenbeobachtungssystem PRARE. Zeitschrift für Vermessungswesen, Vol. 12, 1990, pp. 512-519

34) F. Flechtner, K. Kaniuth, Ch. Reigber, H. Wilmes, “The Precise Range and Range Rate Equipment PRARE: Status Report on System Development, Preparations for ERS-1 and Future Plans,” Second International Symposium on Precise Positioning with the Global Positioning System (GPS '90), Sept. `90, Ottawa, Canada

35) P. Hartl, C. Reigber “Das PRARE-System der ERS-1 Mission,” Die Geowissenschaften, 9. Jahrgang, Heft 4-5, April-Mei 1991, pp. 156-162.

36) W. Schäfer, W. Schumann, “PRARE-2 - Building on the Lessons Learnt from ERS-1,” ESA Bulletin No 83, August 1995

37) Ch. Reigber, F.-H. Massmann, F. Flechtner, “The PRARE System and the Data Analysis Procedure,” CSTG Bulletin Vol. 14, 1997, pp. 11-19

38) F.-H. >Massmann, F. Flechtner, J.-C. Raimondo, C. Reigber, “Impact of PRARE on ERS-2 POD,” Advances in Space Research, Vol. 19, No 11, 1997, pp. 1645-1648

39) P. N. A. M Visser, R. Scharroo, R. Floberghagen, B. A .C. Ambrosius, “Impact of PRARE on ERS-2 orbit determination.,” Proceedings of the 12th International Symposium on Space Flight Dynamics, ESA-SP403, pp. 115-120, 1997

40)) G. Duchossois, P. Martin, “ERS-1 and ERS-2 Tandem Operations,” ESA Bulletin No 83, Aug. 1995

41) G. Duchossois, G. Kohlhammer, P. Martin, “Completion of the ERS Tandem Mission,” ESA Earth Observation Quarterly, June 1996

42) J. M. Dow, M. Rosengren, X. Marc, R. Zandbergen, R. Piriz, M. Romay Merino, “Achieving, Assessing and Exploiting the ERS-1/2 Tandem Orbit Configuration,” ESA Bulletin, No 85, February 1996

43) “Case Study 16: SAR Interferometry,” pp. 107-115, in `Further Achievements of the ERS Missions,' ESA SP-1228, Dec. 1998, ISBN: 92-9092-508-6

44) L. Timmen, X. Ye, C. Reigber, R. Hartmann, T. Fiksel, W. Winzer, J. Knoch-Weber, “Monitoring of Small Motions in Mining Areas by SAR Interferometry,” Proceedings of FRINGE 96, ERS SAR Interferometry Workshop 1996, University of Zürich, Switzerland, Sept. 30, Oct. 2, 1996

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.