Minimize ESEO

ESEO (European Student Earth Orbiter)

Overview    Spacecraft    Launch    Sensor Complement   Ground Segment   References

ESEO is the third mission within ESA's Education Satellite Program and builds upon the experience gained with SSETI (Student Space Exploration and Technology Initiative) Express (launched into LEO on Oct. 27, 2005) and the YES-2 tether and reentry capsule experiment (launch on Foton-M3 on Sept. 14, 2007). 1) 2) 3) 4)

ESEO is a microsatellite mission in LEO (Low Earth Orbit). The overall mission objectives are to:

• Take imagery of Earth's surface and/or other celestial bodies for educational outreach purposes

• Measure the radiation environment in Earth orbit

• Test technologies for future educational satellite missions.

The capability to ensure more global radio coverage for the satellite's operation will be achieved through cooperation with AMSAT, the Radio Amateurs Satellite organization, which has already cooperated with a few ESA missions in the past.

 

ESEO project history:

In early December 2008, ESA awarded a contract to CGS (Carlo Gavazzi Space) of Milan, Italy for the development ESEO spacecraft. CGS will lead a network of 12 universities and associations from various countries (France, Germany, Hungary, Italy, New Zealand, Poland, Portugal, Spain, UK) and will coordinate students work to design, build, test and launch the satellite. 5) 6) 7)

The first workshop of the B2 development phase of ESEO took place December 15-19, 2008 at ESA/ESTEC. The theme of the workshop involved in particular the ESEO spacecraft reconfiguration activity led by CGS. The workshop was also supported by AMSAT, an international group of amateur radio operators that is participating in ESEO by providing some of the satellite communication functions. 8)

After about 1.5 years, the ESEO project passed the PDR (Preliminary Design Requirements), ending the involvement of CGS for the ESEO project. During the preliminary design phase, known as Phase B, ESEO involved more than 200 students from 13 universities across Europe. At the end of this phase, the project was re-oriented to fit into a smaller spacecraft and a new invitation to tender was released to European companies to provide and test the ESEO satellite (Ref. 10).

A new open ITT (Invitation To Tender) was issued by ESA in early 2012 which resulted in a contract award for ALMASpace S.r.l. following ESA's tender evaluation. ALMASpace S.r.l. is a spin-off company from the Microsatellites and Space Micro systems Lab of the University of Bologna, Italy. ALMASpace was selected as the new system prime and a network of Universities participating in the project. 9) 10) 11) 12) 13)

The University of Bologna, in particular, has a critical role being the coordinator of the University Network and taking care of all educational activities (Lecture Courses, Training Courses and Internships) for students belonging the partner Universities and participating to the preparation of the payloads. ALMASpace and UniBO have now full responsibility of the spacecraft bus, and this is a significant change with respect to the previous phase of the ESEO project (under CGS guidance). 14) 15)

 

ESA's plans for this project were changed since the last project phase. It was realized that an organization where every single spacecraft subsystem was entirely designed, assembled, verified by a University team and then delivered to an industrial Prime Contractor, was probably too complex to be managed successfully, without increasing the costs and the development time.

In the new ESEO phase, the project philosophy is slightly changed in that the System Prime shall make use an existing microsatellite platform fitting ESA requirements in order to minimize the risk of a large effort being devoted to the design and harmonization of the spacecraft subsystems. On the contrary, the idea is now to maximize the participation of students belonging to the ESEO University Network to the AIV (Assembly, Integration and Verification) activities at subsystems and system level, plus participating to the spacecraft operations in orbit. While the subsystems will not be necessarily designed by students, by taking advantage of a pre-existing microsatellite platform design, the payloads are to be developed, qualified and provided by universities and their student teams. This approach still allows a direct participation of students to the design, procurement, assembly, qualification of a physical piece of hardware, but minimizes the risk that potential failures or delays in the completion of a single payload could jeopardize the entire spacecraft development plan and, potentially, its launch and operations in orbit.

The consortium assembled by ALMASpace brings together all necessary know‐how and expertise in the field of microsystems design, development and manufacturing. ALMASpace will act as prime contractor and be responsible for:

• Managing the project and, in particular, the formal interfaces to ESA/ESTEC

• Payload selection, qualification and integration onboard the spacecraft and mission implementation management.

The University of Bologna, apart from being involved in the spacecraft design and assembly, is responsible for the educational activities and the University Network coordination. The other universities belonging to the ESEO network are responsible for the scientific and technological payloads hosted onboard, the ground segment, and other support activities to the mission preparation. The overall consortium organization and the interfaces with ESA/ESTEC are shown in Figure 1.

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Figure 1: ESEO project organization (image credit: ALMASpace)

Eight European universities are now working with ALMASpace on the ESEO mission. Their contributions to the mission are shown in Figure 2.

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Figure 2: ESEO University Network and Roles (image credit: ALMASpace)

Educational approach: Educational activities play an important role in the ESEO project involving more than 60 students selected from the University Network. Student training allows the participants to gain both theoretical knowledge and practical experience in the field of space system design, and integration. The plan of student training includes the following three segments:

1) Lecture Course

2) Training Course

3) Student Internships.

Three cycles of student training are foreseen starting after about six months from kick-off, where the first group of 20 students attends the Lecture Course (2 weeks) and the Training Course (1 week). Then, students will participate, in small groups of 5 students each, in the Student Internship at ALMASpace facilities (4 weeks). Once the 4 groups of five students have completed the Internship, the second cycle and the third cycle of Student Training will start at month 13 and month 20, respectively. A total of 18 credits, according to the ECTS European Credit Transfer and accumulation System), are granted by the University of Bologna for the three segments of the Student Training (Ref. 11).

In October 2013, after the successful completion of Preliminary Design Consolidation Review (PDCR), the ESEO (European Student Earth Orbiter) program moved to Phase C1, with the objective of entering in the process of the CDR (Critical Design Review) during the Summer 2014.

 


 

Spacecraft:

The ESEO spacecraft is a microsatellite with an allocated mass of ~45 kg and a size of 33 cm x 33 xm x 63 cm. The ESEO platform architecture is based on both ALMASat-1 heritage (launch Feb. 13, 2012) and ALMASat-EO . Two modules, namely the bus module and the payload module, contain all the subsystems and payloads. In particular, based on the heritage of past missions, most of the subsystems and their units are arranged inside aluminum trays in order to provide physical separation and flexibility. The main bus is physically separated from the payloads and integration can be performed separately. In order to increase the overall reliability level, redundancy is implemented for most subsystems and units. The composite payload module is installed under the bus module and contains most of the payloads.

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Figure 3: Illustration of the ESEO microsatellite with its DOM (De-Orbit Mechanism) in its stowed (left) and deployed (right) configuration (image credit: ALMASpace, ESA)

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Figure 4: Functional block diagram of ESEO (image credit: ALMASpace)

The ESEO platform layout is represented in Figure 5. The composite payload module, containing most of the payloads, has been inherited from ALMASat-EO and the payload arrangement is based on the following constraints: volume and mass, payloads performance and functional requirements, environment, stay-out zones and instrument FOV, accessibility during ground operations.

Most of the subsystems and their equipment are installed inside aluminum trays in order to provide physical separation, flexibility and reduced MAIT (Manufacturing Assembly, Integration and Test) effort. Once stacked, the trays compose a solid cubic structure similar to the design solution that was adopted for ALMASat-1. This ensures that the main bus is physically separated from the payloads, and the system integration can be performed separately for subsystems and payloads. In order to increase the overall system reliability, redundancy is implemented for most subsystems and units. The composite payload module is installed under the bus module and it contains most of the payloads.

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Figure 5: Illustration of the ESEO spacecraft bus layout (image credit: ALMASpace)

AOCS (Attitude and Orbit Control Subsystem): The spacecraft is 3-axis stabilized. Attitude information is provided by 2an assembly of 2 redundant sun sensors, 2 redundant 3-axes magnetometers and an Earth horizon sensor. A set of 3 orthogonal gyroscopes are included to provide an accurate estimation of the spacecraft angular velocities. The actuator system features 3 redundant orthogonal magnetic coils for attitude acquisition maneuvers and coarse attitude pointing. An assembly of 4 redundant momentum-biased/reaction wheels is used for fine pointing. Both the magnetic coils and the momentum/reaction wheels have been designed and developed by ALMASpace. In addition, a MPS (Micropropulsion System) is provided to provide orbital control and small orbital maneuvers. - Communication between all elements of the AOCS is performed by a CAN bus with a CANopen protocol.

An attitude determination quaternion filter experiment has been designed and developed by students of the Technical University of Delft. It uses sensor and control signal outputs to perform several spacecraft attitude tests in LEO (Low Earth Orbit). Four algorithms from different families of estimators are run in parallel and generate telemetry for further analysis and comparison. One of the four algorithms makes use of a maximum information rate filter which computes the information rates of six possible reduced measurement matrices. It selects one for use in the estimation process based on the maximum trace of the associated information rate matrix. The payload shall provide probability distributions for the selection of each different measurement matrix within the telemetry in order to determine the causality underlying the selection of a particular reduced measurement matrix based on features of the orbit and the used measurements. The software experiment will be loaded onto the OBDH. 16)

OBDH (On-Board Data Handling subsystem): The OBDH consists of one main and one redundant computer unit, based on the STM32F107 ARM microcontroller. The computer hosts both, the AOCS and OBDH functionalities, therefore it is equipped with the necessary interfaces to communicate with the subsystems and payloads. The computer unit communicates with all subsystems with two independent CAN interfaces, while an additional pair of CAN interfaces is dedicated to the data exchanges with the payloads. Finally the computer unit is connected with TMTC main and TMTC redundant strings using two independent UART (Universal Asynchronous Receiver/Transmitter) interfaces implemented with the RS-422 standard. Moreover, open collector digital inputs are used to let the TMTC main and redundant set the unit in programming mode, and to select which of the OBDH main and redundant shall be powered on.

The OBDH functionalities are: collecting platform and payloads housekeeping data, and generate periodic reports to be transmitted to the ground segment; record historical housekeeping data, for a maximum of 7 orbit periods, to be transmitted to the ground upon request; monitor a subset of relevant housekeeping parameters to generate errors and warnings; receive, execute or route telecommands from the ground segment; generate internal telecommands to manage the subsystems.

EPS (Electrical Power Subsystem): The EPS comprises the SA (Solar Array), BP (Battery Packs) and PMB (Power Management Board). An unregulated power bus is used. Based on the ALMASat heritage, the solar array will be body fixed and the battery will be based on Li-ion cells. The main tasks of the PMB are to control and monitor the power distribution and power consumption of the units, to monitor the status of the solar arrays, and to monitor the status, charge process and temperature of the battery. The design of the PMB includes redundancy for critical functions and interfaces with both the OBDH and TMTC.

RF communications: The TMTC subsystem consists of a digital transceiver electronic board (RTx), RF front-end and the antenna network. The digital transceiver consists of a redundant board managed by a microcontroller device whose main goals are to receive digital telemetry data from the OBDH board and generate the downlink signal for transmission operations, to receive telecommands from the GS (Ground System) and to send to the OBDH board the digital bit stream. The RF front-end consists of the RF distribution unit based on a passive six-ports hybrid coupler and a circulator while the HPA (High Power Amplifier) and LNA (Low Noise Amplifier) will introduce the appropriate RF signal amplification to establish a reliable link with the GS. The antenna network is a vase turnstile antenna consisting of an array of four dipoles placed in the zenith facet of the spacecraft.

The TMTC subsystem exchanges its data with the OBDH subsystem through a dedicated UART interface included in the electronic board design. As each TMTC board needs to be connected to both OBDH boards, two UART interfaces are included. Furthermore, the redundant CAN bus is used for communication with the PMU (Power Management Unit) board and reboot operation. The TMTC subsystem guarantees a cold redundancy of the transmitter and a hot redundancy of the receiver.

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Figure 6: ESEO Functional Block Diagram: fully redundant platform (image credit: ALMASpace)

ESEO technology demonstrations and tests conducted:

• At platform level the following items are implemented as in-orbit technological demonstrators:

- In house developed cold-gas micro-propulsion subsystem

- In house developed momentum wheel

- Integrated Current Limiter for power distribution unit (ESA CFI)

- Integrated Single Event Latch-up protection for digital devices (present in particular in OBDH and TMTC subsystems)

• The model philosophy foresees Elegant Breadboard (EBB) and Proto-flight models (PFM)

• EBBs implemented with COTS components and going to face qualification tests (including environmental)

• Confidence tests (VFT) are performed before CDR

• A set of electrical and functional confidence tests (included in the VFT category) were agreed with ESA and successfully completed

• The following verifications were performed:

- Envelope and mass measurement, mechanical interface check

- Signals verification on electrical interfaces (power supply, CAN, RS-232/RS-422/RS-485, pulse command, dedicated data I/F)

- Power consumption measurement, including in-rush current, ripple and DC-DC secondary output measurement in idle and working conditions

- Over-voltage protection circuit activation on secondary power buses

- Pulse command interface (inhibit, reset, re-programming mode) verification.

• Tests have been repeated at -25°C and 70°C

• TID (Total Radiation Dose) and SEE (Single Event Effect) tests were performed on the selected microcontroller

• DOM (De-Orbit Mechanism) performed more than 20 successful consecutive deployments after environmental testing

• GPS successfully completed verification functional test and interface check including a specific test campaign at ESA/ESTEC dedicated to the verification of the two redundant front-ends

• TRITEL (Three-Dimensional space dosimetric Telescope) unit successfully completed electrical and functional tests at ambient, minimum and maximum temperatures

• HSTx (High Speed Transmitter) completed several transmission tests in order to verify data-rates, bandwidth and power consumption at the different operational modes

• ADE (ADCS S/W Experiment) completed algorithms coding, test on the OBDH hardware representative model and measurement of the performance

• AMSAT successfully completed electrical verification and functional tests.

 

Launch: A launch of ESEO is planned for the timeframe 2016. ESA is considering of using one of the VERTA (Vega Research and Technology Accompaniment) qualification flights of the new Vega launcher. Possible alternative launcher candidates are: Dnepr, Rockot, and PSLV.

Target orbit: Sun-synchronous near-circular orbit, altitude = 524 km, inclination = 97.47º, LTAN (Local Time on Ascending Node) = 10:30 hours.

Mission profile: The identified orbit produces a cycle of 106 orbits in a week, about 15 orbit per day, in order to complete the coverage of the selected areas of interest (Europe and South Atlantic Anomaly). The definition of the areas of interest was driven by the optical payload and the scientific instruments requirements.

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Figure 7: ESEO requested coverage of the areas of interest - namely over Europe and the South Atlantic Anomaly (image credit: ALMASpace)

 


 

Sensor complement: (µCAM, LMP, TriTel, HSTx, GPS receiver, DOM, AMSAT)

The ESEO microsatellite carries six payloads: µCAM (micro Camera), LMP (Langmuir Probe), Dosimeter instrument (a 3D silicon detector telescope - Tritel-S), Star tracker, Reaction Wheel, AMSAT payload (UHF/VHF, S-band transponder).

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Figure 8: Layout of the ESEO payload accommodation (image credit: ALMASpace)

 

µCAM (micro Camera):

The objective of µCAM is to provide ESEO with Earth imaging capabilities. The subsystem will be configured for wide angle, color imaging and must produce images of sufficient quality for FOV features to be recognizable.

 

LMP (Langmuir Probe):

The objective of LMP is to provide ESEO with plasma measurements capabilities and to investigate the solar activity. Besides analyzing the normal characteristics of the plasma, the LMP payload will acquire scientific data of the geomagnetic disturbances induced by solar eruption and CME (Coronal Mass Ejection). These phenomena are accompanied by ionospheric storms, characterized by abrupt changes of the electron density. Another important objective is to obtain more information about plasma anomalies. The effects of the solar wind can be analyzed by investigating the magnetic disorders and observing the spatial and temporal extent of plasma anomalies. Different types of anomalies are to be observed, including the South-Atlantic anomaly, the Equatorial anomaly, etc. These irregularities influence the function of electrical instruments, and the density of charged particles play an important role in heat transfer, thus it has effect on both the space and Earth weather.

The Langmuir probe is a metallic electrode immersed to the plasma. The experiment is based on measuring the current-voltage curve of the probe. The expected voltage-current curve depends on the density of ionized particles, electron temperature and floating potential. LMP is developed by the Budapest University of Technology and Economics team.

 

TriTel (Three-Dimensional space dosimetric Telescope):

TriTel is an instrument provided by students of the Budapest University of Technology and Economics (BUTE), Budapest, Hungary. The objective of TriTel is to measure the cosmic radiation field and plasma processes in the near-Earth region, in particular in the SAA (South Atlantic Anomaly), on the variations in space weather and the effects of solar activity on the Earth's magnetic field. 17) 18)

Background: The development of the TriTel 3D silicon detector began in the KFKI (Atomic Energy Research Institute) of the Hungarian Academy of Sciences several years ago. By evaluating the deposited energy spectra recorded by the instrument the absorbed dose, the LET (Linear Energy Transfer) spectra in three directions, the average quality factor of the cosmic radiation and the dose equivalent can be determined for different segments of the orbit. The instrument, comprising three mutually orthogonal, fully depleted PIPS (Passivated Implanted Planar Silicon) detector pairs is designed to measure the energy deposit of charged particles (Figure 9).

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Figure 9: The TriTel telescope geometry (image credit: BUTE)

The detectors are connected as AND gate in coincidence in pairs forming the three orthogonal axes of the instrument. By evaluating the deposited energy spectra recorded by TriTel, the absorbed dose, the LET spectra in three directions, the quality factor and the dose equivalent can be determined. Since we are interested in the equivalent dose in tissue, the LET spectra in silicon will be converted to LET spectra in human tissue.

Although the instrument cannot determine the arrival direction of the individual particles, due to the three-axis arrangement, an assessment of the angular asymmetry of the radiation might be possible. The effective surface of each detector is 220 mm2 with a nominal thickness of 300 µm. The most important geometrical parameters of the TriTel telescope are summarized in Table 1.

Radius of the detectors (r)

8.4 mm

Effective surface of the detectors (A)

220 mm2

The gap between the detectors in one telescope axis (p)

8.9 mm

Ratio of the separation between the detectors and the radius (q = p/r)

1.06

Geometric factor, G (for one telescope axis in 4π)

5.1 cm2 sr

Maximum angle of incidence (for one detector pair)

62.1º

Minimum path length in the detector (depletion layer thickness, w)

300 µm

Average path length in the detector (for an isotropic field)

361 µm

Maximum path length in the detector (for maximum angle of incidence)

641 µm

Ratio of the maximum and minimum path lengths

2.14

Table 1: Geometrical parameters of the TriTel telescopes

Since the spectrum of the trapped radiation inside the SAA (South Atlantic Anomaly) is significantly softer, it is worth collecting the SAA and non-SAA spectra separately.

The main design goal in the frame of the ESEO mission is to design, develop, manufacture and verify through an intensive test campaign a new, satellite version of the TriTel three dimensional dosimetric telescope.

The first level of the proposed design work is to study the expected radiation environment in order to draw conclusion about the measurement behavior of the original TriTel instrument (saturation, low noise level, shielding thickness in front of the silicon detectors, optimal measurement parameters, etc.). The second level of the design work is the mechanical and electrical design changes and implementation. The mechanical design work is based on a model approach in which the ESEO-TriTel payload design should build up in a 3D modelling environment together with the satellite structure and simulate based on the input parameters provided by ALMASpace. The thermal design is an important part of the mechanical design work and should be well simulated using the 3D mechanical model and the environmental conditions provided by ALMASpace.

Based on the results of the simulation the mechanical structure of the ESEO-TriTel EQM will be manufactured and verified according to the ESEO verification and test plan to make it flight proven. The electrical design work focuses on the electrical interfaces to the ESEO satellite system: power and data interfaces. In case of the power interface according to the new ESEO design some modifications might be needed on the original TriTel PS (Power Supply) board. In case of the data interface the communication will be based on the CAN (Controller Area Network) open protocol. The CAN interface shall be implemented into the electrical system of the original TriTel instrument.

The TriTel CPU ( Central Processing Unit) software shall be rewritten to implement the CAN communication protocol according to the ESEO requirements. The behavior of the TriTel electrical system, connected to the ESEO system, will be well studied and modified if needed (additional input EMC (Electromagnetic Compatibility) filtering circuits, electronic fuses inside the TriTel, 60 V high voltage for silicon detectors and its influences, etc.). The modified TriTel electrical system shall be manufactured and built into the ESEO-TriTel EQM.

The third level of the engineering work is to carry out the verification process of the ESEO-TriTel payload on the ESEO-TriTel EQM following the ESEO verification and test plan. The EQM will be calibrated and functionally tested as well in different radiation environment tests.

Mass, size

0.95 kg, 155 mm [L] x 107 mm [W] x 83 mm [H]

Power consumption

2.8 – 2.9 W

Input voltage range

15.5 – 34.0 V

Operational temperature range

-40 to +30ºC

Table 2: Parameters of the TriTel instrument

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Figure 10: View of the internal structure of TriTel-S (image credit: BUTE)

 

HSTx (High Speed Transmitter):

An S-band HSTx is provided as a technology demonstration device to allow a high data rate downlink of the payload data. The S-band communication system is capable to transmit data to the ground segment in the 2200-2290 MHz frequency range with data rates ranging up to 8 Mbit/s. The objective is to enable the downloading of data stored in the payload memory for a time of up to 7 no-contact orbits. The S-band HSTx is developed by the student team of Wroclaw University of Technology.

 

GPS receiver:

The student team of the University of Bologna is providing the GPS receiver for orbit determination. The instrument is composed of three units: the receiver antenna, mounted on the satellite top surface; the GPS based-band processor, a COTS component which generates the GPS observables, pseudoranges and carrier phases; the navigation unit, a computer that executes the navigation algorithm and provides satellite position and velocity. The navigation algorithm is a sophisticated software that puts together the GPS measurements with a detailed model of the satellite orbit, in order to generate sub-meter satellite positioning.

The main objectives of the GPS receiver development are to test COTS technologies for the reception of the GPS signal in space environment, and to test the on board navigation algorithm based on Kalman filter and single frequency observations. The purpose of the ESEO GPS receiver is to provide proof of reliable meter-level 3D RMS positioning in a real-time mission environment, using a single frequency GPS L1 C/A receiver coupled with a sophisticated on-board navigation algorithm. This paper describes the receiver design details, with focus on the software navigation algorithm. An effort has been made to formalize the approach to the GPS-based navigation filter tuning which, among others, is one of the most complex tasks in filter design. Although the receiver architecture is based on terrestrial technology, various design techniques are applied to improve its reliability in the space environment. Apart from cold redundancy of the front-end, the unit is equipped with a high-reliability isolated DC-DC converter, and each front-end is monitored for current absorption and equipped with a current limiter. The navigation filter is based on single frequency C/A code and GRAPHIC observations. It is a variable state dimensions filter, since for each satellite in-view an ambiguity is included in the state vector. The filter is then completed with a detailed orbital acceleration model. 19)

The ESEO GPS receiver is composed of four functional units connected together (Figure 11):

• The based-band processor: it is a OEM615 receiver, from NovAtel, that performs GPS signal acquisition, tracking and data demodulation. It provides the raw GPS measurements together with the GPS satellite broadcasted navigation data that is required to compute the navigation solution. The unit is provided by the manufacturer with removed COCOM limitations. Two of these devices are included inside the payload configured to work in cold double redundancy.

• The passive antenna amplification stage: it is the PCB (Printed Circuit Board) designed to provide the correct interface between the passive antenna and the based-band processors.

• The navigation processor: it is a custom on board computer that hosts the navigation filter and manages the power for the entire payload and antenna. It also collects positioning data and distributes them to the other subsystems (Figure 12).

• The GPS antenna: a passive antenna from Sensor Systems, model S67-1575-20, mounted on the satellite top panel (Figure 13).

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Figure 11: ESEO GPS receiver units and connections (image credit: ALMASpace)

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Figure 12: Photo of the navigation computer (image credit: ALMASpace)

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Figure 13: Sensor systems passive antenna (image credit: ALMASpace)

Electronic design: The electronic design of the navigation computer is based on the ARM Cortex microcontroller STM32F407, equipped with single precision FPU, capable of 1.25 DMPIS/MHz, with maximum clock frequency up to 168 MHz. Two DC/DC converters are included and supported by an overvoltage protection circuit that continuously monitors the voltage of the circuit. An overvoltage sensing circuit activates a latch through an optoisolator, once a voltage higher than 3.3 V or 5 V is detected, that disables the output on both voltage regulators.

Also a current limiter stage was implemented in order to avoid that a wrong behavior of one of the two front-end, due to the effect of space radiations, could damage the navigation computer. This limitation circuit is placed between both main and redundant front-end and the power source. It can be activated with a digital output from the microcontroller and once an excessive current absorption is detected, the voltage drop on the sensing resistor is used by an amplifier stage to reduce exponentially the current that flows into the front end. At the same time the limiter status is monitored by the microcontroller with a digital input, so that the microcontroller can disable the malfunctioning front end and enable the redundant one.

Satellite position determination: The selected microcontroller hosts the navigation filter, a sophisticated algorithm that combines the raw measurements provided by the baseband processor with a detailed model of the satellite orbit. In order to test codes with different level of complexity, two different algorithms will be hosted by the navigation computer:

• Kinematic solution: it is the simplest algorithm, a direct computation of the receiver position from the raw observables, without filtering it by an orbit dynamic model. The provided accuracy is the typical accuracy of ground application, between 10-15 m 3D RMS (Root Mean Square). The method used to determine the position is based on Least Square Algorithm.

• Reduced dynamic solution: this algorithm is based on the integration of the raw observations within an accurate orbit dynamics model. According to the complexity of the model and to the selected observation combination, this algorithm 3D RMS accuracy is between 60 and 80 cm.

The data produced by the navigation algorithm, which can be communicated to other satellite subsystems or transmitted to the ground station are: (a) position, velocity and time offset fixes, that are either communicated in real-time upon requests or recorded inside the unit as daily records, in order to be transmitted to the ground infrastructure as mass memory data; (b) daily raw observation records (pseudoranges and carrier phases) provided directly by the COTS front-end, that can be also used to compute the satellite orbit off-line, using POD software, in order to have an accurate reference orbit for on board solution comparison (generally the POD orbit accuracy is around 4cm 3D RMS). In default conditions, both fixes and raw data are recorded every 30 seconds.

Receiver test and verification: A functional test was performed on the COTS front end at the ESA/ESTEC facilities in Noordwijk (the Netherlands), in order to ensure that the receiver is suitable for operation on-board the satellite. The receiver has been connected to the development board which in turn was connected to a GPS signal simulator at ESTEC. Thanks to this simulator, it was possible to reproduce in the realistic ESEO mission scenario in order to verify the capability of the receiver to work with Doppler frequencies typical of space missions. The test demonstrated the need for a setting of the receiving channel's frequency scanner, in order to directly address the receiver to search space frequencies and reduce first acquisition time. After the correct setting, the receiver was able to lock the signal of several satellites in view. From this moment on the receiver started tracking the satellites automatically and maintained the GPS link in time, setting the frequency to the correct values. The test was performed for several minutes and it demonstrated that, after the previous tracked satellites disappeared from the field of view, the receiver was able to automatically rearrange the channels to search and track new satellites with the right Doppler. Then several commands were sent to the receiver through the laptop, in order to validate the generated data about position and other mission-related values.

To verify the performance of the navigation algorithm in a real scenario, it was implemented and used to process GRACE-A raw observations. Although the GRACE receiver and orbit are substantially different from the ESEO ones, this verification was used to prove the correct design of the algorithm which can then be tuned to match the ESEO mission needs. The offline processing showed a positioning error of about 80 cm 3D RMS when using broadcasted GPS ephemeris and clocks. It is expected that the ESEO positioning error will be worse, between 1 and 1.2 meters, due to the lower quality of the receiver oscillator.

 

DOM (De-Orbit Mechanism):

The DOM assembly will be deployed at the end of the mission lifetime to enlarge the effective satellite area, thereby reducing the required de-orbiting time. In the case of the present device, this is achieved by deploying a sail which is attached to coilable boom arms. The boom arms as well as the sail are rolled up around a central spool in the middle of the device and held in position by three kevlar chords. Thus, the device is compactly stored in a single unit of 100 x 100 x 60 mm before actuation. On deployment, the kevlar chords are cut and the strain energy stored in the boom arms during the coiling process is transferred into kinetic energy about the central spool, resulting in deployment. The de-orbit mechanism is developed by the student team of Cranfield University, UK.

 

AMSAT payload:

The objective of the AMSAT payload is to provide downlink telemetry that can be easily received by schools for educational outreach purposes and to encourage students to become interested in all STEM (Science Technology Engineering Mathematics) subjects. It will provide "signals from space directly to the classroom." This telemetry will be gathered by the payload monitoring all of the required telemetry packets being transmitted by the OBDH on the CAN bus or via a separate interface. The AMSAT-UK team will develop the payload.

The project includes the development of a simple and cheap "ground station" operating on VHF frequencies in the Amateur Satellite Service. This station is an omnidirectional antenna feeding a FUNcube USB DonglePRO+ SDR receiver which will receive the signals directly from the satellite and transfer the data to a specially developed graphical software running on any Windows laptop. 20)

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Figure 14: Photo of FUNcube Dongle Pro+ SDR (Software Defined Radio), image credit: AMSAT-UK

Using such equipment, the link budget will be sufficient to enable reception of signals at a satisfactory level on all passes where the elevation exceeds 15º. For radio amateur users, similar simple equipment will suffice to listen to the FM voice downlink. Those users who wish to use the FM transponder will require about 100 W EIRP, e.g. 10 W to an 8 element Yagi on the 1260 MHz uplink.

To display the telemetry, suitable display software will be developed together with a central data warehouse to enable schools to access data from prior orbits over the Internet. The AMSAT-UK team will also assist the development of the software for schools and support the creation of teacher aids and lesson plans to ensure the best possible benefits for school students.

 


 

Ground Segment:

The ESEO ground segment basic functions necessary to establish reliable radio link for uplink and downlink communication for the ESEO mission are (Ref. 12):

1) Support to the space segment in terms of command and control of the satellite, monitoring of the telemetry data and management of the communication link. In particular, this is performed through a bidirectional link at UHF band.

2) Support to the space segment in terms of reception of the data collected by payloads on-board the spacecraft during the orbiting phase. In particular, this is performed through a downlink connection performed at S-band.

3) Management of the overall mission, in terms of planning of the activities problem/conflict solving, resource optimization, user priority handling.

4) Management of user requests, data acquisition, archiving and delivery of the data received from the ESEO satellite by means of co-located and/or remotely located acquisition stations.

The ground segment infrastructure comprises the following functional areas: Mission Exploiting Area and Mission Programming and Control Area. Each functional area is devoted to perform and exploit the ESEO mission from the ground segment side.

The mission exploitation area includes the Mission Exploitation System MIEX) and User Segment while the Mission Programming and Control Area includes the MCC (Mission Control Center), MPS (Mission Planning System), FDS (Flight Dynamics System) and the following ground stations:

• GSF (Ground Station Forlì), Italy, as the main station for telemetry and command of the spacecraft at UHF

• GSV (Ground Station Vigo), Spain, as a backup station for GSF

• GSM (Ground Station Munich), Germany, dedicated to the reception of data collected by the on-board payloads at S-band.

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Figure 15: Overview of the ESEO ground segment (image credit: ALMA Space)

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Figure 16: ESEO ground segment physical architecture (image credit: ALMASpace)

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Figure 17: Uplink chain functionalities (image credit: ALMASpace)

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Figure 18: Downlink chain functionalities (image credit: ALMASpace)

 


1) ESEO - The European Student Earth Orbiter, ESA, URL: http://esamultimedia.esa.int/docs/LEX-EC/ESEO_fact_sheet_20080228.pdf

2) Francesco Emma, Javier Ventura-Traveset, Roger Walker, Helen Page, Carlos Lopez de Echazarreta, Thomas-Louis de Lophem, Matthew Cross, Per Berglund, Victor Nikolaidis, "ESA hands-on projects education strategy," Proceedings of the 59th IAC (International Astronautical Congress), Glasgow, Scotland, UK, Sept. 29 to Oct. 3, 2008, IAC-08.E1.1.2

3) http://esamultimedia.esa.int/docs/edu/ESEO_fact_sheet_20090612.pdf

4) http://www.esa.int/Education/ESEO_mission

5) "Development of the ESEO student satellite gets under way," ESA, Dec. 9, 2008, URL: http://www.esa.int/SPECIALS/Education/SEMYQ2STGOF_0.html

6) E. Razzano, T. Lupi, P. Sabatini, "Micro-Satellite Platform with Building-Block Approach for Leo Missions," Proceedings of the Symposium on Small Satellite Systems and Services (4S), Funchal, Madeira, Portugal, May 31-June 4, 2010

7) E. Razzano, T. Lupi, P. Sabatini, "Flexible Building-Block Architecture For LEO Microsatellite Platforms," Proceedings of the 61st IAC (International Astronautical Congress), Prague, Czech Republic, Sept. 27-Oct. 1, 2010, IAC-10.B4.7.5

8) "ESEO workshop begins reshaping at start of phase B2," ESA, Dec. 22, 2008, URL: http://www.esa.int/SPECIALS/Education/SEMYNCTTGOF_0.html

9) Paolo Tortora, Davide Bruzzi, Fabrizio Giulietti, Piero Galeone, "European Student Earth Orbiter: ESA's Educational Microsatellite Program," Proceedings of the 2nd IAA Conference on University Satellite Missions and CubeSat Workshop, IAA Book Series , Vol. 2, No 2, Editors: Filippo Graziani, Chantal Cappelletti, Rome, Italy, Feb. 3-9, 2013, IAA-CU-13-01-06

10) "ESA's Student Satellite Takes Important Step Towards Space," ESA, January 29, 2013, URL: http://www.esa.int/Education/ESA_s_student_satellite_takes_important_step-towards_space

11) Davide Bruzzi, Paolo Tortora, Fabrizio Giulietti, Piero Galeone, "European Student Earth Orbiter: ESA's educational Microsatellite Program," Proceedings of the AIAA/USU Conference, Small Satellite Constellations, Logan, Utah, USA, Aug. 10-15, 2013, paper: SSC13-IX-3, URL: http://digitalcommons.usu.edu/cgi/viewcontent.cgi?article=2974&context=smallsat

12) Davide Bruzzi, Paolo Tortora, Fabrizio Giulietti, Piero Galeone, Antonio De Luca, "The ESEO Development: Merging Technical with Educational Challenges," Proceedings of the 4S (Small Satellites Systems and Services) Symposium, Port Petro, Majorca Island, Spain, May 26-30, 2014

13) "European Student Earth Orbiter," ESA, URL: http://www.esa.int/Education/European_Student_Earth_Orbiter

14) Information provided by Paolo Tortora of the University of Bologna, Italy.

15) Davide Bruzzi, Nicola Melega, Paolo Tortora, Fabrizio Giulietti, Piero Galeone, Antonio De Luca, "The ESEO mission: current status and achievements," 10th IAA Symposium on Small Satellites for Earth Observation, Berlin, Germany, April 20-24, 2015, paper: IAA-B10-0703, URL of presentation: http://www.dlr.de/iaa.symp/Portaldata/49/Resources/dokumente/archiv10/pdf/0703-ESEO_SSEO_Davide_Bruzzi.pdf

16) Martijn Geers, Hans Kuiper, Daniel Choukroun, Manuel Salvoldi, Duarte Rondao, "A novel attitude quaternion filter for the ESA European Student Earth Orbiter (ESEO)," Proceedings of the 66th International Astronautical Congress (IAC 2015), Jerusalem, Israel, Oct.12-16, 2015, paper: IAC-15-C1.IP.12

17) ,Balazs Zabori, Attila Hirn, "TriTel 3 dimensional space dosimetric telescope in the European Student Earth Orbiter project of ESA," Proceedings of the 61st IAC (International Astronautical Congress), Prague, Czech Republic, Sept. 27-Oct. 1, 2010, IAC-10.A1.4.4

18) Balazs Zabori, Attila Hirn, Tamas Hurtony, Agnes Gyovai, Sandor Deme, Tamas Pazmandi, Istvan Apathy, Antan Csoke, Peter Szegedi, Andras Gerecs, "TRITEL satellite version silicon detector telescope development for the ESEO spacecraft," Proceedings of the 66th International Astronautical Congress (IAC 2015), Jerusalem, Israel, Oct.12-16, 2015, paper: IAC-15-A1.5.12

19) Alessandro Avanzi, Alfredo Locarini, Paolo Tortora, "Real-time precise orbit determination of the ESA ESEO spacecraft," 10th IAA Symposium on Small Satellites for Earth Observation, Berlin, Germany, April 20-24, 2015, paper: IAA-B10-1405P

20) "AMSAT-UK to provide Amateur Radio payload for ESEO satellite," AMSAT-UK, Feb. 2, 2013, URL: http://amsat-uk.org/2013/02/02/amsat-uk-to-provide-amateur-radio-payload-for-eseo-satellite/
 


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 (herb.kramer@gmx.net).

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