Flying Laptop (FLP) is the first minisatellite of the IRS (Institute of Space Systems - Institut für Raumfahrtsysteme) at the University of Stuttgart, Germany. The primary mission objective is to demonstrate and qualify new small-satellite technologies for follow-up missions as summarized in Table 1.
The Flying Laptop project is being developed at IRS. The satellite's subsystems and key functions such as the on-board software and the FDIR (Failure Detection, Isolation and Recovery) concept are allocated to about 10 doctoral candidates. All components, except the ACS (Attitude Control Subsystem ) units, are new developments and mostly engineered in cooperation with industry. While specifications are composed according to mission and project requirements by the students, the satellite component quality benefits from the experience and the industrial procedures that are applied at a professional supplier company. The project progress is observed and supported by the project manager at IRS. In addition, two project advisors (former IRS students) from Airbus DS in Friedrichshafen, and one from Tesat-Spacecom GmbH in Backnang, Germany, support the satellite development with their technical knowhow and management advice.
The mission objectives of Flying Laptop include also scientific observations. 2)
• One goal is to use MICS (Multispectral Imaging Camera System) for various scientific Earth observation experiments. Particular targets will be imaged in multispectral bands from different angles in support of BRDF (Bi-directional Reflectance Distribution Function) studies. This in turn implied the introduction of a "spotlight" attitude mode, in which the complete spacecraft is rotated in its orbital path for target fixation. In Flying Laptop notation, the spotlight mode is also referred to as "Target Pointing Mode." 3) 4) 5)
• A further scientific mission goal, conducted in cooperation with the DTU (Technical University of Denmark), is to utilize the satellite's star trackers for the detection of NEOs (Near Earth Objects). NEOs are asteroids and meteoroids whose trajectories are passing Earth in relatively close orbits.
• A further scientific mission goal is the observation of ship traffic. By means of an AIS Receiver in combination with the optical observation of MICS the spaceborne ship surveillance shall be evaluated.
Figure 1: Artist's rendition of the deployed Flying Laptop spacecraft (image credit: IRS Stuttgart)
Like most satellite projects, the Flying Laptop experienced several reconfigurations throughout its development life. Reshaping the design was necessary due to payload changes, but also due to changing mission requirements . The new configuration is shown in Figure 2 (Ref. 2).
The spacecraft structure is a box of size 60 cm x 70 cm x 90 cm with a total mass of ~ 120 kg and a design life of 2 years. The design is modular. The mechanical structure of the satellite allows a convenient access to the internal components and ensures simultaneous integration of the modules. The lower part consists of integral aluminum parts and therefore offers a cost-effective and precise assembly, adjusted force transmission and good thermal properties. The upper part, where the optical systems are installed, consists of carbon‐fibre reinforced sandwich structures. These offer a low mass, high stiffness as well as low thermal longitudinal expansion to provide a stable calibrated alignment of the cameras in the satellite and to each other. The system design is one-failure tolerant to provide secure operations and to preserve system functions. All optical instruments are mounted onto an optical bench, consisting of a CFRP (Carbon Fiber-Reinforced Plastic) sandwich with an aluminium honeycomb core, to insure optical alignment and to minimize thermal expansion effects. Flying Laptop is a low-cost project by using COTS (Commercial-Off-The-Shelf) components whenever possible. 6) 7) 8) 9) 10) 11) 12)
Figure 2: Two views of the Flying Laptop satellite configuration (image credit: IRS Stuttgart)
Table 2: Summary of the spacecraft subsystems and payloads (Ref. 2)
OBC (On-Board Computer): A main requirement is the development of an ultra compact and high-performance OBC, intended to support a RTEMS (Real-Time Executive for Multiprocessor Systems) operating system, a PUS (Packet Utilization Standard) standard based onboard software (OBSW) and a ground/space communication standard based on CCSDS (Consultative Committee for Space Data Systems) protocols. The OBC system consists of four functionally differing boards (Table 3). Each board is available twice for redundancy reasons. All boards are cross-coupled via SpaceWire with a maximum transfer rate of 10 Mbit/s (Ref. 2). 13) 14)
Table 3: Spacecraft OBC composition and properties
The C&DH (Command and Data Handling) functions in the on-board S/W are based on ESA's PUS implementation. PUS describes the transfer of TC and TM data between ground and satellite. In nominal support operations, only one OBC core board and one I/O board are activated controlling the satellite. Since both OBC core boards are cross-coupled to both I/O boards, every link configuration of the boards can be applied for operations. Hence, there are 4 connections available for Flying Laptop to provide failure tolerance against failing boards. To safeguard the accessibility of FLP, two CCSDS boards are available. Both CCSDS boards are operated in parallel and are each connected to one transceiver. As the designation of the boards indicate, the FLP is applying the CCSDS standard as communication protocol for S/C telecommands (TCs) uplinked from ground as well as telemetry (TM) transmitted to ground. All PCBs (Printed Circuit Boards) of the OBC are scaled according to a 3U Eurocard size and mounted into an aluminum frame. The single frames are stacked together and cross-strapped under the front panel (Figure 3). All interfaces that connect to the remaining S/C components are located on top of the stack.
Figure 3: Illustration of the Flying Laptop OBC stack assembly (image credit: IRS Stuttgart)
The OBC boards are SBC (Single Board Computers) designed around the Aeroflex LEON3FT (Fault Tolerant) processor. The LEON3FT is a 32 bit SPARC TM V8 microprocessor with a number of available on chip interfaces including cPCI, SpaceWire and CAN. The OBC boards are implemented with the SpaceWire interface as the primary method of in flight communication. OBC memory resources include 8 MB of on board SRAM and 4 MB of non-volatile memory. Both the SRAM and non-volatile memory interfaces have the LEON3FT on chip EDAC (Error Detection and Correction) designed into the board. The EDAC is capable of detecting two errors on the SRAM or NV memory bus and correcting one. All 4 of the LEON3FT SpaceWire ports have been implemented on the OBC and the data rate is set to 10 Mbit/s. 15) 16)
In addition, ports 3 and 4 support the RMAP (Remote Memory Access Protocol) that gives the user the ability to DMA data directly into SRAM from either port 3 or port 4 SpaceWire interfaces.
Figure 4: Block diagram of the OBC processor board (image credit: Aeroflex, IRS Stuttgart)
EPS (Electrical Power Subsystem): Electrical power is being provided by three solar panels, two of which are deployable (total area of approx. 1 m2). Use of triple-junction GaAs solar cells with an efficiency of 25.3%. In addition, the satellite is being used as an on-orbit testbed for atest string of a new generation of 100 µm 3G triple junction solar cells.
Battery: To achieve a low total cost of the battery system, commercial off-the-shelf Lithium iron phosphate cells manufactured by A123 Systems are used. The system consists of three battery cell strings, yielding a total nominal voltage of 23.1 V and a total nominal capacity of 35 Ah. As the battery cells are susceptible to overcharging, a charge control system to report overvoltages to the PCDU (Power Control and Distribution Unit) is part of the battery system. Furthermore, a simple cell balancer design using bleed resistors is implemented. In order to keep the temperature within the operational temperature range of the cells, the battery system is thermally isolated from the rest of the satellite system by means of multi-layer insulation and glass fiber reinforced plastic parts. 17)
The battery system consists of three battery strings, one for each solar panel. The battery strings for the two deployable solar panels consist of 35 battery cells each, with blocks of five cells in parallel and seven of these blocks in series , yielding a total nominal capacity of 12.5 Ah at a voltage between 18.9 V and 25.2 V. For the string connected to the body mounted solar panel, there are only four cells in parallel, reducing the nominal capacity to 10 Ah, because of the fewer solar cells and the higher temperature of this panel. Thus the whole battery has a nominal capacity of 35 Ah. The mass of the battery system is ~10 kg, its dimensions are 21 x 20 x 20 cm.
Figure 5: Illustration of the battery system (image credit: IRS Stuttgart)
The PCDU (Power Control and Distribution Unit) functions exceed the conventional functional scope of power distribution units. Besides the classic power distribution and regulation functions ,the PCDU serves additionally as the reconfiguration unit for the OBC sub units - processor boards, I/O- and CCSDS boards. The communication between OBC and PCDU is performed via CCs (Common Commands) with a working OBC core board, I/O board and PCDU (Figure 6).
For CC communications, the PCDU provides nominal and redundant cross-coupled, fullduplex communication interfaces in RS422 level (8-N-1) with a baud rate of 115200. The PCDU confirms the proper reception of every command sent by the OBC with a confirmation return. In this way, the OBC supervises power regulation and can request PCDU acquired TM.
The PCDU is being developed in cooperation with an experienced industrial partner (Vectronic Aerospace, Berlin). The device represents the independent monitoring unit for the OBC system and facilitates its operational recovery. Important housekeeping data that is collected at the PCDU is polled by the OBC in a regular interval of 10Hz by a Common Command. If the PCDU is not being polled as specified, a fault of the OBC system is probable.
The PCDU has a size of 220 mm x 160 mm x 118 mm and a mass slightly over 4 kg. Five frame stacks, each corresponding to one PCB, are assembled to a single unit and closed by a cover plate. The PCDU is designed radiation tolerant to at least 20 krad in order to account for the radiation load that is to be expected for a mission life of 2 years. A PCB internal heating for the CPU PCB facilitates the fast warming up to -20ºC in order to prevent damaging of electronic parts due to thermal tension over high temperature gradients. The PCDU is qualified to a lower temperature limit of -40ºC for operational use in order to increase the availability of the PCDU and thus S/C system safety.
Figure 7: Photo of the EM (Engineering Model) PCDU (image credit: Vectronic Aerospace)
Considering the importance of the PCDU for satellite operations a single-point failure tolerant design is particularly realised for C&DH functions inside the unit. Two redundant Central Processing Units (CPUs) are implemented in the PCDU. Both are operated in a hot-redundant concept with a master and a slave unit. The master unit performs all actions, whereas the slave monitors the master. Both CPUs are connected by a toggle logic, which switches the master unit as soon as the currently operating CPU is not responding any more. The master CPU is sending a confirmation signal in a specified period in order to confirm its operability. If this condition is not met, the slave unit commands the toggle-logic to switch the master unit (Figure 8).
Figure 8: Functional design of the CPU toggle-logic (image credit: IRS Stuttgart)
ACS (Attitude Control Subsystem): Flying Laptop is 3-axis stabilized. The requirements call for high-accuracy pointing (150 arcsec or 0.042º) and agile maneuvering capabilities for the imaging mission. The ACS actuators feature four reaction wheels and three magnetic torquers (these are torque rods for momentum dumping of the reaction wheels). Attitude sensing is provided by two 3-axis magnetometers, eight coarse sun sensors (6º rms pointing), four fiber-optic rate sensors, one autonomous star tracker (fine pointing accuracy of < 2 arcsec), and three GPS receivers (GENIUS). 19) 20) 21)
Table 4: Pointing parameters of the ACS
Following is a description of the various ACS and S/C subsystem components:
• In this context, GENIUS (GPS Enhanced NavIgation system for the University of Stuttgart microsatellite) is an onboard experiment being conducted in cooperation with DLR/GSOC (Figures 9 and 10). GENIUS consists of three COTS Phoenix GPS boards. Each of the receivers is connected to separate GPS antenna via a low noise amplifier. The antennas of three separate GPS receivers are being placed on three corners of the body-mounted central solar array in an L-shape configuration. The GENIUS performance offers real-time position, velocity and timing information with estimated accuracies of 10 m, 0.1 m/s and 1 µs, respectively (in addition attitude is being provided). The Phoenix GPS receiver is a commercial GPS receiver board with a new DLR/GSOC developed firmware for space and high dynamics applications. The receiver has 12 tracking channels and is able to measure phase and Doppler shift of the GPS-L1 carrier signal.
Figure 9: Configuration of the GENIUS system (image credit: DLR/GSOC)
Figure 10: Illustration of GPS antenna allocations (image credit: IRS)
The GENIUS GPS system consists of three independent GPS receiver boards, each connected to a separate antenna and low noise amplifier (LNA) as shown in Figure 9. The GPS Box is connected to the on-board computer (OBC) and the power control and distribution unit (PCDU). The used Phoenix boards are commercial 12-channel GPS L1 receivers with a DLR/GSOC developed firmware for space and high dynamics applications. Three GPS antennas are mounted on the middle solar panel in an L-shaped arrangement, creating two baselines with a length of 440 mm and 610 mm respectively (Figure 10). The three GPS receivers are integrated in a single 100 mm x 80 mm x 67 mm box together with an interface board for RS-422 conversion. To achieve a high level of redundancy, each receiver can be switched on/off independently varying the system input power from 0.9 W for 1 receiver to 2.6 W for all 3 receivers according to measurements at the testing model.
An algorithm based on a Kalman Filter is used to process the measurement data and produce an offline attitude solution which will be compared to the attitude information available from the satellite's star camera. The algorithm uses the lambda-method to resolve the integer ambiguities of the double differences of the carrier phase measurements. These resolved double difference ambiguities are then used to fix the single difference ambiguities in the filter. Hence, the algorithm provides a seamless transition from the ambiguity resolution to the attitude determination.
• STR (Star Tracker): The autonomous star tracker in the ACS configuration is the newly developed µASC (micro Advanced Stellar Compass) of DTU (Technical University of Denmark), Lyngby, Denmark. In fact, µASC is of ASC heritage flown on Ørsted, SAC-C, CHAMP, GRACE, ADEOS-2, SMART-1, GOCE, etc. The µASC instrument is physically divided into a µDPU (micro Data Processing Unit) with hot/cold redundancy and CHU (Camera Head Unit), a µDPU may drive up to 4 CHUs (2 CHUs are being used on Flying Laptop). The intrinsic accuracy of an attitude measurement from a single CHU is better than 1 arcsec at an integration time of 0.5 s. This attitude is autonomously calculated based on all brighter stars in the FOV of the CHU. The µASC on Flying Laptop provides a pointing knowledge within 2 arcsec. Furthermore, µASC delivers attitude information at S/C angular rates of up to 10º/s and thus enables rapid repointing of the platform to any object. This attitude is autonomously calculated based on all brighter stars in the FOV of the CHU. The µASC on Flying Laptop needs to provide a pointing knowledge of one pixel at 7.4 arcsec.
The use of µASC on Flying Laptop is an early spaceborne demonstration of this instrument. Currently PROBA-2 is another mission under development using the µASC device. 22)
Figure 11: Illustration of the µASC instrument (image credit: IRS)
Figure 12: View of a camera head unit and baffle (image credit: IRS)
• The three magnetic torque rods employed are developed by ZARM Technik, Bremen, with a linear dipole moment of 6 Am2. The torquers are connected to a power box that includes two I2C buses for connection to the OBC. The whole system is single redundant.
• Magnetometer: ZARM Technik provides also the AMR (Anisotropic-Magneto-Resistive) magnetometer, a microcontroller-based 3-axis magnetometer with digital output. Two magnetometers are being installed on the microsatellite. The Earth's magnetic vector field is being used as input information for the magnetic torquers (detumbling after launcher separation, etc.). The ARM sensor is the HMC-1023 model of Honeywell.
• The angular rate of the S/C is measured with 4 single-axis COTS fiber optic rate gyros (FOGs) in a tetrahedron configuration. The sensors employed are C-FORS (Commercial Fiber Optic Rate Sensor) of Litef. The complete FOG assembly has a mass of ~1.7 kg.
Figure 13: Functional architecture of the spacecraft (image credit: IRS Stuttgart)
Figure 14: Overview of the ACS sensors and actuators (image credit: IRS Stuttgart)
RF communications: For telemetry and telecommand, S-band (low and high gain) antennas are being installed on the satellite. The S-band command uplink has a frequency at 2.068 GHz, a telemetry downlink at 2.245 GHz, and a data downlink at 2.425 GHz.
Flying Laptop also features commanding by so-called HPCs (High Priority Commands) of the PCDU in case of an emergency, indicated by the red colored communication path in Figure 15.
Figure 15: Block diagram of the communications system (image credit: IRS Stuttgart)
The microsatellite will be operated by students at IRS (Institut für Raumfahrtsysteme), of the University of Stuttgart. The existing ground station on campus is being upgraded to permit satellite communications in the following frequency bands: UHF, and S-band.
Figure 16: Block diagram of TM/TC FPGA device (image credit: IRS Stuttgart)
Figure 17: Sensor positions during vibration test (image credit: IRS Stuttgart)
Project development status:
• March 9, 2017: The Flying Laptop passed its Flight Readiness Review as well as its Operational Readiness Review on Tuesday, March 7, 2017! The review board, consisting of representatives from DLR, Airbus, Tesat and Thales, confirmed the success of the reviews, provided that the actions for launch and operation preparation are completed and documented as planned before the satellite is shipped, and therefore also before its launch. 23) 24)
Figure 18: Photo of the Flying Laptop Team in 2017 (image credit: IRS Stuttgart)
• As of the summer of 2015, the flight software of the Flying Laptop is being finalized and the last functional system tests will be prepared and executed. Thus, by the end of 2015 the satellite will be completed.
• Since mid-2014, the fully integrated small satellite Flying Laptop is in the system testing phase at the Institute of Space Systems located at the University of Stuttgart in Germany.
Launch: The Flying Laptop satellite was launched on July 14, 2017 (06:36:49 UTC, 09:36:49 Moscow time) as a secondary payload on a Soyuz -2.1a Fregat-M vehicle configuration from Baikonur, Kazakhstan. The primary payload on this flight was the Kanopus-V-IK (IK =Infra-Krasny, means "infrared" in Russian) mission of Roscosmos. 26) 27) 28) 29) 30)
Orbit: A sun-synchronous polar circular orbit with an altitude of 600 km, inclination = 97.6º.
Secondary payloads: In total, 72 secondary satellites will be launched on the Kanopus-V-IK mission, including spacecraft for four separate commercial remote sensing and weather constellations.
Glavkosmos, a subsidiary of Russian state space corporation Roscosmos, is seeking to become a larger provider of rideshare launch services for small satellites. In addition to this upcoming launch, Glavkosmos is planning to fly about 40 more small satellites on two Soyuz missions from the new Vostochny Cosmodrome in Russia's Far East region late this year, with additional launch opportunities planned for 2018 and beyond.
In addition, the German Orbital Systems company of Berlin, ECM Space Technologies GmbH, actively participates in the launch, by supplying a DCSM (Deployment Control and Separation Sequence Management) unit. Integration of two secondary satellites built in Germany, three from Russia and 12 from the USA. GlavKosmos subcontracted this task to ECM. 31)
• Forty-eight (48) Dove satellites (Flock 2k) of Planet will be launched into an SSO of 475 km altitude. 32) Planet of San Francisco is the biggest single customer for the upcoming launch. This "flock" of 48 satellites will go into a sun-synchronous orbit, but one slightly different from those of 88 similar satellites launched on an Indian Polar Satellite Launch Vehicle in February. Those satellites went into a sun-synchronous orbit that crosses the equator at 9:30 hours local time. The new satellites will launch into an orbit that crosses the equator at about 11:00 hours local time.
• Spire Global of San Francisco, which is deploying a fleet of CubeSats to collect GPS radio occultation and ship tracking data, has eight (8) of its Lemur CubeSats on this launch.
• GeoOptics of Pasadena, CA, is flying its three CICERO 6U CubeSats (CICERO-1, -2,- 3), designed to collect GPS radio occultation data to support weather forecasting.
• Flying Laptop, a minisatellite (120 kg) of IRS (Institute of Space Systems), University of Stuttgart, Germany.
• WNISAT- 1R (Weather News Inc. Satellite 1R), a microsatellite (43 kg) for north arctic routes and atmosphere monitoring. The project is started from the commercial objects between Weathernews and Axelspace, Japan. The object of the WNISAT-1R mission is monitoring of the Northern sea routes and of the CO2 content of the atmosphere. 33)
• NorSat-1 and NorSat-2 of the Norwegian Space Center, built by UTIAS/SFL (Canada) on GNB (Generic Nanosatellite Bus), each with a mass of 15 kg. The NORSAT-2 satellite will carry a next generation Automatic Identification System (AIS) receiver from Kongsberg Seatex, along with a VDE (VHF Data Exchange) payload that will enable two-way communication at higher data rates than possible with AIS. NorSat-1 (< 30 kg) carries three instruments: An AIS receiver, a Langmuir Probe Instrument, and CLARA (Compact Lightweight Absolute Radiometer), intended to observe total solar irradiation and variations over time.
• TechnoSat is a nanosatellite project (18 kg) of the Technical University of Berlin. Test of new nanosatellite components, including a camera, a new reaction wheel system, a star tracker, a transmitter, a fluid dynamic actuator, and commercial laser retro-reflectors.
• Corvus-BC 1 and Corvus-BC 2: Astro Digital, formerly known as Aquila Space, (formed from the core team of the former Dauria Space daughter Canopus Systems) developed the Corvus-BC Earth observation CubeSats (6U, 10 kg). The Landmapper-BC spacecraft, also known as Corvus-BC1 and Corvus-BC2, have color and infrared cameras for wide-area imaging.
• MKA-N 1, 2: Two Earth observation CubeSats (6U, 10 kg each) of Roskosmos, built by Dauria Aerospace.
• NanoACE, a technology demonstrator by Tyvak Nanosatellite Systems, Inc. (Irvine, CA) to validate the Endeavor suite technologies that will be used for future missions and is solely for the purpose of internal Tyvak development as an attitude control experiment. A 3U CubeSat (5.2 kg).
• Mayak: A Russian 3U CubeSat (4kg) developed by a group of young scientists named "Your sector of space" with support of the Moscow State University of Mechanical Engineering (MSUME). In orbit, the 3U CubeSat will deploy four triangular reflectors, 4 m2 each, which form a tetrahedral shape. The reflectors are made from metalized membrane with reflection coefficient of 95%. The reflector will provide a -10 optical magnitude at the beginning of the flight to allow for easy tracking. Mayak will be put into a tumbling motion over all axes, with at least 1 revolution per second.
• Iskra-MAI-85, a CubeSat of the Moscow Aviation Institute. 34)
• Ecuador-UTE-YuZGU, a CubeSat of the Kursk South-Western State University, Russia.
Table 5: Overview of the Kanopus-V-IK timeline (Moscow time, Ref. 26)
• April 3, 2019: First laser transmission tests were carried out with the OSIRIS (Optical Space Infrared Downlink System) instrument on the Flying Laptop mission of the University of Stuttgart and the DLR optical ground station in Oberpfaffenhofen. 35)
- The OSIRIS laser terminal: OSIRIS is extremely compact, with a mass of only 1.3 kg, and is very power efficient. Successful transmission tests have now been carried out using DLR's optical ground station in Oberpfaffenhofen as part of a program of experiments that has been ongoing since the summer of 2018. These results were confirmed during a measurement campaign conducted in March 2019, when the laser beam from the Flying Laptop was received on the ground. The high-precision alignment of the satellite and ground station with one another represents a particular challenge, and has now been demonstrated for the first time.
- "The transmission of satellite data by laser is the future," says Florian David, Deputy Director of the DLR Institute of Communications and Navigation. "The power of optical communications will make it possible to, for example, make far larger amounts of data available to rescue workers on the ground during disaster recovery operations. For this reason, optical communications is a key area of our research." As part of the OSIRIS program, the DLR Institute of Communications and Navigation in Oberpfaffenhofen is developing optical communications systems that are particularly suited to direct downlink from small satellites.
- The University of Stuttgart's ‘Flying Laptop' small satellite is testing new technologies and assisting with scientific Earth observation. In addition to numerous experiments, the satellite is also equipped with a high-resolution camera. The satellite, which was developed and built by students and doctoral candidates as part of the Small Satellite Program at the Institute of Space Systems, was launched from Baikonur in 2017. The operation of the satellite and the scientific evaluation of the data are funded by a grant from the Baden-Württemberg Ministry of Science, Research and the Arts.
- "Although laser data transmission offers huge advantages in terms of achievable data rates, it also poses a tremendous challenge when it comes to accurately aligning the satellite with the ground station. The successful OSIRIS transmission tests demonstrate the high precision of the attitude control system and our satellite's outstanding performance," says Sabine Klinkner, OSIRIS Project Leader at the University of Stuttgart.
- Following the success of the transmission tests, the research teams in Stuttgart and Oberpfaffenhofen are keen to carry out more experiments with OSIRIS on the Flying Laptop. These include the reception of mission data and the characterization of the transmission channel. This should make a vital contribution towards international standardization of the technology and enable the development of even more robust transmission processes for future missions. The experiments will continue in Oberpfaffenhofen from spring 2019.
OSIRIS (Optical Space Infrared Downlink System) communication experiment:
Flying Laptop is is the first mission of University of Stuttgart's small satellite program to demonstrate new optical communication technologies in space. For high data rate transmission of the mission data to ground, FLP is equipped with the first generation of OSIRIS terminals (Figure 19). The payload consists of a power supply unit as well as a laser unit with two independent laser sources. In this configuration, the payload consumes 26 W and adds 1.3 kg to the satellite mass while transmitting data with up to 1 W of optical output power, at a data rate of up to 200 Mbit/s. The transmission laser divergence is therefore adapted to the pointing accuracy of the satellite, using the body pointing with the star cameras as reference. Therefore, no beacon laser is required to operate OSIRISv1. 36)
Figure 19: OSIRIS payload for the FLP (Flying Laptop), image credit: University of Stuttgart
Table 6: Key performance data of OSIRISv1
Figure 20: Photo of OSIRISv1 installed in Flying Laptop (image credit: University of Stuttgart)
Successful downlinks with OSIRISv1 could be demonstrated in late summer and fall of 2018. After a calibration campaign with the first reception of light on 17 August and a subsequent optimization of the offset between OSIRISv1 and Flying Laptop, a stable conduction of experiments is possible and ongoing. Figure 21 shows the first received flash as seen on the tracking camera of Optical Ground Station Oberpfaffenhofen, as well as exemplary telemetry data of the EDFA (Erbium Dopen Fiber Amplifier) operated in orbit. All systems onboard the satellite behave as expected.
Figure 21: First flash from OSIRISv1 on Flying Laptop received on Optical Ground Station Oberpfaffenhofen's tracking camera during calibration campaign (left); Telemetry of EDFA on Flying Laptop during initial testing (right), image credit: DLR, University of Stuttgart
Figure 22: Photo of the DLR Laser ground station in Oberpfaffenhofen (image credit: DLR)
Identification of the collimator orientation: The exact knowledge of the collimator orientation is mandatory because FLP uses an open-loop approach for the pointing of OSIRIS. The collimator is mounted on the payload optical bench of the FLP. The Panoramic Camera (PamCam) is mounted on the same bench in close proximity. PamCam images can therefore be used to determine the orientation of the collimator. Images in the integration room with active laser diodes and detector cards were taken with the PamCam before launch. Since the camera was used outside it's nominal focal parameters in the small integration room the test images were slightly blurred resulting in an estimated deviation between the boresight of the PamCam and the OSIRIS EDFA of -0.27° to -0.25° in horizontal and 0.40° to 0.48° in vertical direction.
After successful commissioning of the satellite bus, the payloads were taken into operation and the deviation of the PamCam boresight from the satellite's z-axis could be determined. Combined with the deviation of the OSIRIS lasers to the PamCam, the collimator orientation w.r.t. to the satellites body coordinate system could be calculated. The PamCam orientation was obtained by taking nadir images and a comparison with the location of the satellites subpoint as well as the boresight location on ground. Due to the low spatial resolution of the PamCam and other uncertainties in the collimator orientation, e.g. mechanical stress during launch and thermal effects in orbit, a comparably large uncertainty area of 36 x 36 mrad around the theoretical collimator orientation was assumed. A meander pointing pattern as shown in Figure 23 was used to examine this area. The pattern was achieved by commanding corresponding angle offsets of the pointing axis to the optical ground station while the satellite performed a target pointing maneuver. During target pointing rotational rates of up to 1.8°/s with the satellite are necessary to maintain its orientation to the ground station. Therefore, additional slews for the pattern were limited to 0.03°/s to maintain a stable pointing. This limited the area that could be covered during a pass with a typical duration of 8.5 minutes. Hence, it was decided to divide the area into 9 sectors with 17 individual points each. Figure 23 shows exemplary patterns for three passes.
Figure 23: Search area with three exemplary sectors. Each sector was searched with a meander pattern (image credit: University of Stuttgart)
• October 2018: Mission Results: With the payload request handling package, the project was able to drastically increase the number of observations made. More than 300 observations have successfully been executed within the last 4 months with more than 12,000 images received (Ref. 40).
Figure 24: Part of a PamCam linescan image of the Persian Golf acquired on 5 November 2017 (image credit: IRS Stuttgart)
Figure 25: MICS NIR image of a portion of Glacier Bay National Park, located in Southeast Alaska west of Juneau. The image was acquired on 3 May 2018 (image credit: IRS Stuttgart)
Figure 26 shows all recorded AIS messages during a 24 h data take in nadir mode, regarding its power budget the Flying Laptop would be able to perform constant payload operations in nadir mode. 48 h continuous AIS data takes were also conducted.
Figure 26: AIS messages received during a 24h data take (image credit: IRS Stuttgart)
• September 2018: The small satellite Flying Laptop, launched in July 2017, was developed and built by PhD, graduate and undergraduate students at the Institute of Space Systems (IRS) of the University of Stuttgart with assistance by industry and research institutions. The project goals include technology demonstration, earth observation and improving the education of students at the University of Stuttgart in the fields of satellite development, integration, test, and operations. 37)
• Nominal Satellite Operations: During the nominal satellite operations phase more and more requests for payload data takes and experiments slots were received. The available software tools to handle these requests required significant manual work and appeared to be not practical for nominal satellite operations. Parts of the operations team and the on-board software development team share the same personal, however their expertise was needed for necessary onboard software updates addressing the bespoken bugs, as well as to optimize the on-board store handling and to improve the pointing performance. Staffing and pass execution was therefore reduced drastically. Only one uplink pass on each working day is used with a single person attending this pass in the control room sending a pre-defined command stack and monitoring live TM (Ref. 40).
- To reduce the amount of manual work for the command controller and mission planner ground-based automation tools were developed. The aim of this development was to automate the generation of command stacks and to provide them for each uplink pass without human interaction. All of these tools are written in Python and are interacting with Redmine via its REST API. An overview of the ground-based automation tools is shown in Figure 27, they are divided into modules accessing the different data sources.
Figure 27: Overview: Ground-based automation tools (image credit: IRS Stuttgart)
• July 2018: The Flying Laptop has been in orbit for one year. After all the systems were commissioned during the first week after the project launch, the Flying Laptop began regular operations. Project manager Sabine Klinkner, Professor for Satellite Technology at the IRS sums up: "All components were successfully commissioned, the satellite system was stable from the beginning and is undergoing continuous optimization. The project, carried out by doctoral students and students at our institute, is a great success for research and teaching in the field of Stuttgart's space flight research." The communication via the university's ground station is functioning flawlessly with over 2200 ground contacts. 38)
• June 2018: Object-oriented programming is widely used in the software development branch but is not as popular for flight software of spacecraft. Flying Laptop uses a component-based object-oriented software and is compatible with ECSS-PUS (European Cooperation for Space Standards-Packet Utilization Standard). 39)
- The first half year of operations showed that an object oriented flight software is able to provide a reliable platform for a small satellite. From an operator's perspective the mode management and the FDIR concepts show that hiding complexity in encapsulated components can simplify daily work without hiding important information.
- Nominal operation is simplified due to the automatisms implemented building on the FSFW(Flight Software Framework) component model. As a result, operations can be performed with a crew of usually 2 operators during weekdays and no operator during weekends with experiments and other tasks running 24/7. Telemetry checks can be performed quickly as failure types and the device specific attribution is clearly visible to the operator.
- Further development is ongoing at the University of Stuttgart. For the mode management, another decrease in needed commands will be established with adding the activation of mode specific housekeeping telemetry into the components. Also, further missions with the FSFW are planed, which will benefit from the in-flight experience with Flying Laptop.
• Commissioning: During commissioning all payload devices were taken into operation and further redundant bus components were checked, including a switch to the redundant transmitter and OBC. The first image taken by the PamCam (Panoramic Camera) was received 5 days after launch. The commissioning phase was executed successfully as all payloads were working fine and returning data. All passes were executed in target pointing mode for stable TM/TC and DDS links. The duration of the day and night shifts were reduced by using only passes over Germany with an operations team consisting of four positions. The amount of activities for the mission planner increased as more and more time-tagged operations were planned. Another bug in the on-board software was found during the commissioning, a full housekeeping store did not allow for simultaneous read and write operations (Ref. 40).
Figure 28: First light image of the PanCam camera, acquired on 19 July 2018, showing south-west Germany with Stuttgart in the center (image credit: IRS Stuttgart)
• The first successful contact with the satellite was at 9:48:32 UTC on 14 July 2017 with the WHM (Weilheim) ground station. A total of 60 passes within 4 days followed and were mostly executed successfully, with some minor ground related issues. Operations were performed 20 hours a day in two shifts with 9 positions each. The operations team consists of a Flight Director (FD), a Command Controller (CC), four Spacecraft Controllers (SC), a Ground Controller (GC), a Antenna Controller (AC) and a Mission Planner (MP). 40)
- Solar panels were deployed on the second day and check outs of several functions, the higher ACS devices and modes and some redundancies were performed. A bug in the on-board software was discovered that prevented the usage of both star trackers at the same time. Thus, initially only one star tracker was used. All remaining subsystems worked as expected and LEOP (Launch and Early Operations Phase) was finished ahead of schedule. Battery state of charge remained above 95% throughout the LEOP, communication links were stable and temperatures remained between 5° and 20°C, the OBC (On-Board Computer) did not reboot. All ACS modes worked with pointing accuracies below 1°, which could be improved significantly throughout the following phase.
Sensor complement: (MICS, AIS)
The scientific payload of the satellite is a triple imaging system, a VNIR (Visible Near-Infrared) system called MICS, the PamCam, and AIS Receiver, as well as the star tracker of the Attitude Control System of the Flying Laptop.
MICS (Multispectral Imaging Camera System):
The objective is to observe in the VNIR range of the spectrum in three bands at medium resolution (GSD of 20 m). MICS consists of three single cameras, each with an area array CCD detector for snapshot observations.
Table 7: Key parameters of the MICS instrument
The optical system uses a double Gauss telescope with interference filters placed in front of the system. The use of an area array detector has advantages for multi-angular measurements. The multi-angular measurements will be done in the target-pointing mode, where the satellite is focused on the target site during the whole passage.
In order to accomplish reliable scientific measurements, periodic calibration of the instrument is mandatory, not only on ground, but also in space. A particular LED (Light Emitting Diode) device is being used to verify the following items:
• Pixel-to-pixel shift (flat-field calibration)
• Spectral shift of interference filters
• Radiometric performance.
Figure 29: Schematic sectional drawing of MICS (image credit: IRS Stuttgart)
Pointing modes for image acquisition:
Three attitude control modes have been defined for image acquisition:
1) Inertial pointing mode: In this mode, the star sensor is being used to provide high accuracy pointing knowledge of 7.5 arcseconds. The satellite will be and will also remain inertially stabilized, i.e. the coordinate system of the satellite will maintain in the same orientation with respect to stars. Note: This mode is not useful for taking Earth imagery. Other observations (e.g. stars, moon) are possible.
2) Nadir pointing mode: In this mode the satellite is being aligned in the direction of the Earth, i.e. the z-vector of the satellite's coordinate system is perpendicular to the Earth's surface; hence, the angular rate remains constant. This mode is also called the "Earth-pointing mode," being used for image acquisition, attenuation measurements and trace gas detection.
3) Target-pointing mode (or spotlight mode): This mode is being used to achieve the required coverage/resolution of the planned scientific observations. In this mode, the S/C points at fixed target (spot an Earth's surface) during an extended period of time thereby achieving a TDI (Time Delay Integration) effect. The spotlight service requires a slewing of the S/C to keep the instruments pointed. The maximum slew rate for this maneuver is 1º/s. This is the most demanding support mode of the satellite in terms of control algorithms.
Figure 30: Imaging modes: A) Inertial-, B) Nadir- and C) Target-pointing mode (image credit: IRS Stuttgart)
Research experiments and technology demonstrations:
• FPGAs: The introduction and reliance of onboard computing with an FPGA system represents a new approach to conventional system architectures. It provides the capability to directly generate the logical configuration of FPGA gates from a C-like high level language without producing the machine code for a processor (hence, massive parallel processing is possible). Using an onboard computer architecture with several reciprocative checking FPGAs, a safe system is obtained that even exceeds the performance of current PCs through its ability of parallel real-time processing. An inherent advantage of FPGA architectures is the capability of reconfiguration within milliseconds.
To make the system fault-tolerant and to address radiation issues, a cold redundant computer system is used.
• NEO (Near Earth Object) detection. Aside from delivering attitude information, the star tracker in use possesses a built-in feature to automatically detect, identify and track any other faint luminous object, not being a star, as long as the object is brighter than the visual (or apparent) magnitude Mv 11.
The Technical University of Denmark (DTU) has proposed an interplanetary mission to search for Near Earth Asteroids (NEA), based on their star tracker, µASC. Observation time for these science experiments of the Flying Laptop will be made available to test and verify this concept, in the eclipse phase of the LEO orbit (for further information see reference 6).
• PamCam (Panoramic Camera) is an additional COTS camera on Flying Laptop to provide context color video imagery of Earth . PamCam is required because the narrow FOVs of the two science imagers (MICS and TICS) are insufficient for context information imagery to increase public outreach of the Small Satellite Program. PamCam uses CMOS technology with a pixel pitch of 6.7 µm. It has 1280 x 1024 pixels and can capture up to 27 images per second in full resolution. Using a focal length of approximately 25 mm, the sensor can cover a FOV of 20º x 16º. This results in a swath width of approximately 250 km and a ground sample distance of around 200 m from a 700 km orbit. The video link of PamCam employs a lossy video compression technique to be able to handle the large source data volume. 41)
AIS (Automatic Identification System):
In Q3 of 2012, an AIS receiver inclusive antenna was implemented as a new payload on Flying Laptop. This payload was developed, build and tested by the DLR Institute of Space System in Bremen. The objective of the AIS instrumentation is to receive AIS signals from ships in the ground segment. 42)
Since January 1, 2004, it is mandatory to run an AIS transmitter for all ships bigger than 300 GRT (Gross Register Tonnage) in international waters. Since July 1, 2008, all ships in national waters bigger than 500 GRT also need to run an AIS transmitter. AIS, is a system to supervise marine traffic. In times of increasing ship traffic, a system like this is indispensable. AIS shall be used or the following:
- preventing collisions
- information for adjoining coastal states considering ships and their cargo
- appliance for landward surveillance.
The system works as follows: Ships will send a message in regular time intervals. These messages contain, among other information the position, route, and velocity of the ship, the ship name and the call sign. If a ship has an AIS receiver on board, it can use the signals for better planning and decision making.
The AIS signals can also be received from a spacecraft. In a last-minute cooperation, between DLR and the IRS (Institute of Space Systems) of the University of Stuttgart, an AIS receiver incl. antenna could be accommodated within the satellite. According to the slogan, form follow function, the unusual form of the AIS receiver housing was created.
Figure 31: Photo of the AIS instrumentation (image credit: IRS Stuttgart)
To communicate with the Institute's own satellite, the IRS has its own ground station. The objective of the installation of the system is to automate operations as much as possible. Thus, the usage time of the satellite is to be maximized without providing an expensive and complex 24‐hour manual operation. The main tasks of this station are sending commands to the satellite (telecommanding, TC), the reception of Housekeeping data (telemetry, TM), as well as the download of the scientific payload data from the satellite [downlink payload, DDS (Data Downlink System)].
The antenna system with a reflector diameter of 2.5 m is capable to transmit within the commercial space research S‐band (2075 MHz ‐ 2090 MHz) with an equivalent output power of up to 20 kW and simultaneously, also within the commercial space research S‐band (2257 MHz ‐ 2278 MHz) to receive telemetry. Both are done in the right‐hand circular polarization oriented (RHCP). Simultaneously, the antenna system is able to receive the payload data in the left‐hand circular polarization LHCP with up to 10 Mbit/s in the amateur radio S‐band (2400 MHz ‐ 2428 MHz). The transceiver is the commercial satellite transceiver CORTEX CRT of Zodiac Aerospace.
In order to increase the contact time and to auxiliary ground stations in the fault case of the IRS station, a network of ground stations was established.
In LEOP (Launch and Early Orbit Phase), three DLR Ground are being used, all of which allow TM downlink and TC uplink on a live data ling using SLE through GSOC (German Space Operations Center):
• Weilheim (WHM) station in Bavaria, Germany
• Inuvik (INU) station in the Northwest Territories, Canada
• O'Higgins (OHG) station in Antarctica.
The Weilheim ground station was used during the commissioning phase. The IRS ground station shall be taken into operation during this phase and shall support more and more passes. At the end of commissioning the IRS ground station shall be the main operational ground and Weilheim shall only be used in emergencies as well. Also the ground station of GFZ (German Research Center for Geosciences) in Ny Alesund, Svalbard, Norway (NYA) shall be started to be used for automated TM downlink during this phase. This ground station only provides offline TM reception and no uplink.
For the data downlink, two additional ham radio stations at the University Putra Malaysia in Kuala Lumpur (MAL) and a private one in Kiel, Germany (KIE) may be used.
Figure 32: Ground segment overview for Flying Laptop (image credit: IRS Stuttgart, Ref. 37)
Routine Operations Phase Network: After the LEOP, the main ground station used for TM, TC, and DDS links was the IRS ground station at the University of Stuttgart. It features a 2.5 m parabolic dish with a custom designed feed to cover both the commercial and ham radio S-band. A Cortex-CRT unit manufactured by ZODIAC Aerospace is used as the baseband unit together with other COTS equipment for radio signal processing. A custom developed Java software is used to control the IRS ground station.
Furthermore, a ground station in Ny-Ålesund (NYA) on Svalbard, Norway, operated by the German Research Center for Geosciences (GFZ), is used for additional TM and payload data downlink twice a day during routine operations. Received data are transferred to the IRS network after each pass though file exchange servers.
MCS (Mission Control System): ESA's SCOS-2000 (Spacecraft Control & Operation System-2000) MCS was chosen early in the project as the main control software. It is a generic MCS software with extensive manual and automatic commanding as well as TM packet and parameter display functionalities. It requires the application of the ECSS Packet Utilization Standard (PUS) for TM and TC definitions.
FDS (Flight Dynamics System): The FDS is an in-house developed Python software which can process Two Line Elements (TLE) and GPS data measured on-board from the TM Archive to propagate the orbit. For orbit propagation, the commercial Analysis, Simulation and Trajectory Optimization Software (ASTOS) tool is used, whose execution is automated by the Python software. 43)The FDS generates information on ground station passes and earth observation target visibility as well as eclipse times, which it writes to a MySQL database. This flight dynamics database is further used for pass and earth observation planning. Furthermore, the FDS generates a file containing a CCSDS standardized set of orbit parameters from the filtered on-board GPS measurements. This file is forwarded to DLR flight dynamics at GSOC, where it is converted to a TLE file. This TLE file is of higher accuracy than those provided online by NORAD and is used for antenna control at all ground stations.
Mission Planning System: For mission planning, the MOIS (Manufacturing and Operations Information System) Scheduler tool is used, which takes information on orbital events from the FDS as well as predefined FOPs as input. A human operator can plan the execution of offline FOPs (Flight Operations Procedures) based on the orbital events and check the resulting plan for conflicts based on configurable rules. From the plan, a command stack file for import into SCOS-2000 can then be exported.
Payload Data Processing: Separately from the TM/TC processing, a payload data processing chain was implemented with custom developed Java software. The reception software extracts payload data from the data stream, determines its source (camera system, AIS receiver), and handles incomplete or duplicate data by generating complete images from multiple downlinks of the same image. It then performs additional image processing and saves the data to a MongoDB database. It can then be viewed by an operator using the web frontend.
Control Room: A control room was set-up at the IRS to perform in-orbit operations as well as operational simulations for operator training and educational purposes. Two large screens show the main SCOS-2000 windows for commanding, the orbit ground track as well as a live video feed of the IRS ground station antenna (Figure 33).
It features a total of nine standard desktop computer consoles, one for each operator position. Most of these consoles feature a modern Linux installation with a virtual machine for the older SCOS-2000 version in use. At the command console, two physical machines run two SCOS-2000 servers for redundancy, whereas all other consoles have SCOS-2000 client installations, which can connect to either server as needed.
Figure 33: The IRS mission control room (image credit: IRS)
Network Infrastructure: The operational infrastructure is mainly deployed within an operational network that has very limited interfaces to other networks, including the public Internet, for security reasons. The only interfaces allowing data in- and output are the SLE connection to the DLR ground station, which has its own dedicated firewall, and a file exchange network drive that can also be reached from the IRS office network. Other interfaces only allow data to be transferred from the operational to the office network, e.g. to send notification emails and duplicate the databases to allow access via the web frontend from outside.
1) Information provided by Jens Eickhoff, Astrium GmbH, Friedrichshafen, Germany
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The information compiled and edited in this article was provided by Herbert J. Kramer from his documentation of: "Observation of the Earth and Its Environment: Survey of Missions and Sensors" (Springer Verlag) as well as many other sources after the publication of the 4th edition in 2002. - Comments and corrections to this article are always welcome for further updates (email@example.com).