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Academic literature on the topic 'ExoMars Rover'

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Published: 10 December 2022
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Journal articles on the topic "ExoMars Rover"

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Barnes, Dave, Enrico Battistelli, Reinhold Bertrand, Francesco Butera, Raja Chatila, Alessandro Del Biancio, Chris Draper, et al. "The ExoMars rover and Pasteur payload Phase A study: an approach to experimental astrobiology." International Journal of Astrobiology 5, no. 3 (July 2006): 221–41. http://dx.doi.org/10.1017/s1473550406003090.

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The Aurora programme is the European Space Agency programme of planetary exploration focused primarily on Mars. Although the long-term goals of Aurora are uncertain, the early phases of the Aurora programme are based on a number of robotic explorer missions – the first of these is the ExoMars rover mission currently scheduled for launch in 2013 (originally 2011). The ExoMars rover – developed during a Phase A study – is a 240 kg Mars rover supporting a 40 kg payload (called Pasteur) of scientific instruments specifically designed for astrobiological prospecting to search for evidence of extant or extinct life. In other words, ExoMars represents a new approach to experimental astrobiology in which scientific instruments are robotically deployed at extraterrestrial environments of astrobiological interest. Presented is an outline of the design of the rover, its robotic technology, its instrument complement and aspects of the design decisions made. ExoMars represents a highly challenging mission, both programmatically and technologically. Some comparisons are made with the highly successful Mars Exploration Rovers, Spirit and Opportunity.
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Li, D., R. Li, and A. Yilmaz. "ESA ExoMars: Pre-launch PanCam Geometric Modeling and Accuracy Assessment." ISPRS - International Archives of the Photogrammetry, Remote Sensing and Spatial Information Sciences XL-3 (August 11, 2014): 177–82. http://dx.doi.org/10.5194/isprsarchives-xl-3-177-2014.

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ExoMars is the flagship mission of the European Space Agency (ESA) Aurora Programme. The mobile scientific platform, or rover, will carry a drill and a suite of instruments dedicated to exobiology and geochemistry research. As the ExoMars rover is designed to travel kilometres over the Martian surface, high-precision rover localization and topographic mapping will be critical for traverse path planning and safe planetary surface operations. For such purposes, the ExoMars rover Panoramic Camera system (PanCam) will acquire images that are processed into an imagery network providing vision information for photogrammetric algorithms to localize the rover and generate 3-D mapping products. Since the design of the ExoMars PanCam will influence localization and mapping accuracy, quantitative error analysis of the PanCam design will improve scientists’ awareness of the achievable level of accuracy, and enable the PanCam design team to optimize its design to achieve the highest possible level of localization and mapping accuracy. Based on photogrammetric principles and uncertainty propagation theory, we have developed a method to theoretically analyze how mapping and localization accuracy would be affected by various factors, such as length of stereo hard-baseline, focal length, and pixel size, etc.
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Patel, Nildeep, Richard Slade, and Jim Clemmet. "The ExoMars rover locomotion subsystem." Journal of Terramechanics 47, no. 4 (August 2010): 227–42. http://dx.doi.org/10.1016/j.jterra.2010.02.004.

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Barrett, Alexander. "Where should the ExoMars rover land?" Astronomy & Geophysics 59, no. 5 (October 1, 2018): 5.12–5.16. http://dx.doi.org/10.1093/astrogeo/aty229.

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Ribes-Pleguezuelo, Pol, Denis Guilhot, Marta Gilaberte Basset, Erik Beckert, Ramona Eberhardt, and Andreas Tünnermann. "Insights of the Qualified ExoMars Laser and Mechanical Considerations of Its Assembly Process." Instruments 3, no. 2 (April 19, 2019): 25. http://dx.doi.org/10.3390/instruments3020025.

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1960 is the birth year of both the laser and the Mars exploration missions. Eleven years passed before the first successful landing on Mars, and another six before the first rover could explore the planet’s surface. In 2011, both technologies were reunited with the first laser landing on Mars as part of the ChemCam instrument, integrated inside the Curiosity Rover. In 2020, two more rovers with integrated lasers are expected to land on Mars: one through the National Aeronautics and Space Administration (NASA) Mars 2020 mission and another through the European Space Agency (ESA) ExoMars mission. The ExoMars mission laser is one of the components of the Raman Spectrometer instrument, which the Aerospace Technology National Institute of Spain (INTA) is responsible for. It uses as its excitation source a laser designed by Monocrom and manufactured in collaboration with the Fraunhofer Institute for Applied Optics and Precision Engineering (IOF). In this paper, we present for the first time the final flight module laser that has been installed in the rover’s onboard laboratory and validated to be shipped to Mars in 2020. Particular emphasis is given to mechanical considerations and assembly procedures, as the ExoMars laser assembly has required soldering techniques in contrast to the standard adhesive technologies used for most laser assembly processes in order to fulfill the environmental and optical requirements of the mission.
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Coates, A. J., R. Jaumann, A. D. Griffiths, C. E. Leff, N. Schmitz, J. L. Josset, G. Paar, et al. "The PanCam Instrument for the ExoMars Rover." Astrobiology 17, no. 6-7 (July 2017): 511–41. http://dx.doi.org/10.1089/ast.2016.1548.

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Pérez del Pulgar Mancebo, Carlos Jesús Pérez del Pulgar, Pablo Romeo Manrique, Gonzalo Jesús Paz Delgado, José Ricardo Sánchez Ibáñez, and Martin Azkarate. "Choosing the Best Locomotion Mode in Reconfigurable Rovers." Electronics 8, no. 7 (July 22, 2019): 818. http://dx.doi.org/10.3390/electronics8070818.

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The use of autonomous rovers for planetary exploration is crucial to traverse long distances and perform new discoveries on other planets. One of the most important issues is related to the interaction between the rover wheel and terrain, which would help to save energy and even avoid getting entrapped. The use of reconfigurable rovers with different locomotion modes has demonstrated improvement of traction and energy consumption. Therefore, the objective of this paper is to determine the best locomotion mode during the rover traverse, based on simple parameters, which would be obtained from propioceptive sensors. For this purpose, interaction of different terrains have been modelled and analysed with the ExoTeR, a scale prototype rover of the European ExoMars 2020 mission. This rover is able to perform, among others, the wheel walking locomotion mode, which has been demonstrated to improve traction in different situations. Currently, it is difficult to decide the instant time the rover has to switch from this locomotion mode to another. This paper also proposes a novel method to estimate the slip ratio, useful for deciding the best locomotion mode. Finally, results are obtained from an immersive simulation environment. It shows how each locomotion mode is suitable for different terrains and slopes and the proposed method is able to estimate the slip ratio.
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Ellery, Alex, Lutz Richter, and Reinhold Bertrand. "CHASSIS DESIGN & PERFORMANCE ANALYSIS FOR THE EUROPEAN EXOMARS ROVER." Transactions of the Canadian Society for Mechanical Engineering 29, no. 4 (December 2005): 507–17. http://dx.doi.org/10.1139/tcsme-2005-0031.

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The European Space Agency’s (ESA) ExoMars rover has recently been subject to a Phase A study led by EADS Astrium, UK. This rover mission represents a highly ambitious venture in that the rover is of considerable size ~200+kg with high mobility carrying a highly complex scientific instrument suite (Pasteur) of up to 40 kg in mass devoted to exobiological investigation of the Martian surface and sub-surface. The chassis design has been a particular challenge given the inhospitable terrain on Mars and the need to traverse such terrain robustly in order to deliver the scientific instruments to science targets of exobiological interest, We present some of the results and design issues encountered during the Phase A study related to the chassis. In particular, we have focussed on the overall tractive performance of a number of candidate chassis designs and selected the RCL (Science & Technology Rover Company Ltd in Russian) concept C design as the baseline option in terms of high performance with minimal mechanical complexity overhead. This design is a six-wheeled double-rocker bogie design to provide springless suspension and maintain approximately equal weight distribution across each wheel.
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Barthelmes, Stefan, and Ulrich Konigorski. "Model-based chassis control system for an over-actuated planetary exploration rover." at - Automatisierungstechnik 68, no. 1 (January 28, 2020): 58–71. http://dx.doi.org/10.1515/auto-2019-0090.

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AbstractIn planetary exploration, wheeled mobile robots (rovers) are popular for extending action range compared to a lander. Despite their success, they continue to struggle with soft grounds which shows in high sinkage and can lead to an immobilization in the worst case. Rovers usually are over-actuated due to individual wheel drives and steering, which is rarely made use of in current missions. Some work optimizing the resulting degrees of freedom exists but often does not use all available model knowledge. In this work, the rover is consequently modeled with the subsystems rigid body dynamics, kinematics and wheel/ground dynamics. Feedback linearization is used for the rigid body and the underlying wheel/ground controllers on individual wheel level. The control allocation of the forces is done via the pseudo-inverse and a base of the null-space to extract the available degrees of freedom. A verification of the approach is shown in a co-simulation with a high-fidelity model of the ExoMars rover.
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Amos, Steve, and Paul Brochard. "Battery for Extended Temperature Range Exomars Rover Mission." E3S Web of Conferences 16 (2017): 06001. http://dx.doi.org/10.1051/e3sconf/20171606001.

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Dissertations / Theses on the topic "ExoMars Rover"

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Li, Ding. "ESA ExoMars Rover PanCam System Geometric Modeling and Evaluation." The Ohio State University, 2015. http://rave.ohiolink.edu/etdc/view?acc_num=osu1420788556.

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Jördening, Jendrik. "Scheduling Strategies for Relay of Mars Rover Data via Mars Orbiter and Earth Stations." Thesis, Luleå tekniska universitet, Institutionen för system- och rymdteknik, 2016. http://urn.kb.se/resolve?urn=urn:nbn:se:ltu:diva-340.

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In this thesis, the relay communication between landed assets on the surface of Mars via a relay orbiter to Earth is studied for its latencies and the times which can be provided for the landed asset to work and for the ground to plan depending on the operational margins, the available ground station network and the available relay orbiters. In this context, an automated solver is developed to evaluate a locally optimal strategy of relay pass assignment respecting the different constraints and is proven to provide a solution close to the globally optimal one. The solver is determining the link opportunities and reasons on them, by minimising a cost function for each relay pass and choosing the cheapest ones in an iterative process. With this solver, it is shown that the best operational approach is to await commands confirmation and to provide the possibility of resending corrupted files. Moreover, it is shown that a 24/7 ground station coverage should be ideally provided, on which priority for booking should be given to relay missions since they depend on the actual timing of the orbiter overflights over the lander. Further- more, it is shown that adding additional relay orbiters increases the solution space drastically, making it desirable to use them. The possibility to restrict cross-agency support is assessed, showing that cross-support is still eligible. Finally, the data volume is shown to be sufficient to fulfil the ExoMars Rover and Surface Platform mission requirements, when using multiple orbiters, even though the solver itself would need extra capabilities to cope with allocating appropriate relay passes.
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Harris, Liam Vincent. "Raman spectroscopy using miniaturised spectrometers in preparation for the 2020 ExoMars rover mission." Thesis, University of Leicester, 2018. http://hdl.handle.net/2381/42619.

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Over the past two decades, the potential of Raman spectroscopy as a tool for planetary exploration has been explored in detail and greatly advocated. It is ideally suited for in situ measurement as it provides rapid, non-destructive, unambiguous molecular identification, without any need for mechanical or chemical sample preparation. Developments in the miniaturisation of lasers, charge-coupled device detectors and other instrument components has, for the first time, enabled the development of Raman instruments for space missions. The first to be deployed on another planet will be the Raman Laser Spectrometer instrument onboard the ExoMars rover, a joint mission between the European Space Agency and the Roscosmos State Corporation for Space Activities, which will be launched in 2020. Two further Raman instruments, SuperCam and SHERLOC, will be included in the payload of NASA’s Mars 2020 rover. Prior to the deployment of these instruments, it is necessary to conduct analogue studies using flight-representative hardware in order to optimise instrument configuration, mode of operation, data extraction and analysis protocols. The programme of research presented in this thesis constitutes a series of such studies. The capabilities of two flight-representative, portable Raman spectrometers, one using 532 nm excitation and the other 785 nm, have been evaluated through a series of Mars analogue studies. Spectra have been acquired from a range of relevant target materials, including silica, haematite and calcium sulphate of varying levels of hydration. Caution is urged in the interpretation of spectra from portable Raman systems, since limitations introduced by their miniaturisation make band misassignment possible. As a result of this research, it is recommended that instruments are designed with a minimum spectral range from 100 to 4000 cm-1 and a spectral resolution of at least 3 cm-1, in order to avoid the misinterpretation of spectra. Several sets of analogue samples that are rich in reduced carbon have also been studied. It has been demonstrated that reduced carbon can not only be detected in concentrations as low as 0.08%, but distinct carbon populations can be differentiated by the measurement of certain spectral parameters. Furthermore, this analysis enables the qualitative comparison of the thermal maturity of different samples containing reduced carbon. These analytical techniques will be highly valuable when analysing spectra returned by planetary instruments.
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Rusu, Alexandru. "Planification de chemin et navigation autonome pour un rover d’exploration planétaire." Thesis, Toulouse, ISAE, 2014. http://www.theses.fr/2014ESAE0049/document.

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Dans le cadre du programme ExoMars, l’ESA va déployer un rover sur Mars dont la mission sera de réaliser des prélèvements d’échantillons par forage souterrain et les analyser à l’aide des instruments scientifiques embarqués. Pour atteindre en toute sécurité les différents points d’intérêt où seront effectués ces prélèvements, le rover devra être capable de parcourir plus de 70 mètres par sol (jour martien) tout en respectant les limitations des communications interplanétaires. Les performances des algorithmes de navigation autonome embarqués impacteront directement la réussite scientifique de cette mission. Le premier objectif de cette thèse est d’améliorer les performances de l’architecture de planification de chemin local itératif proposée par le CNES. Tout d’abord, l’utilisation d’un planificateur incrémental de chemin local ”Fringe Retrieving A∗” permettant de réduire la charge de calcul est proposée. Il est complété par l’introduction de tas binaires dans les structures de gestion de la liste de priorité du planificateur de chemin.Ensuite, les manœuvres de rotation sur place pendant l’exécution des trajectoires sont réduites à l’aide d’un planificateur de chemins non-holonomes. Ce planificateur utilise un ensemble de chemins pré-calculés en tenant compte des capacités de braquage du rover. Le second axe de recherche concerne la planification de chemin global d’un rover d’exploration planétaire. Dans un premier temps, la contrainte de mémoire embarquée est détendue et une étude statistique évalue la pertinence d’un planificateur de chemin de type D∗ lite. Dans un deuxième temps, une nouvelle représentation multi-résolution de la carte de navigation est proposée pour stocker de plus grandes zones explorées par le rover sans augmenter l’utilisation de la mémoire embarquée. Cette représentation est utilisée par la suite par un planificateur de chemin global qui réduit automatiquement la charge de calcul en adaptant le sens de recherche en fonction de la forme et de la distribution des obstacles dans l’espace de navigation
ESA’s ExoMars mission will deploy a 300kg class rover on Mars, which will serveas a mobile platform for the onboard scientific instruments to reach safely desired locations where subsurface drilling and scientific measurements are scheduled. Due to the limited inter-planetary communication constraints, full autonomous on board navigation capabilities are crucial as the rover has to drive over 70 meters per sol(Martian day) to reach designated scientific sites. The core of the navigation softwareto be deployed on the ExoMars rover uses as baseline the autonomous navigation architecture developed by CNES during the last 20 years. Such algorithms are designed to meet the mission-specific constraints imposed by the available spatial technology such as energy consumption, memory, computation power and time costs.The first objective of this thesis is to improve the performance of the successive localpath planning architecture proposed by CNES. First, the use of an increment allocal path planner, Fringe Retrieving A∗, is proposed to reduce the path planning computation load. This is complemented by the introduction of binary heaps in the management structures of the path planner. In-place-turn maneuvers during trajectory execution are further reduced by using a state lattice path planner which encodes the steering capabilities of the rover.The second research direction concerns global path planning capabilities for roboticplanetary exploration. First the onboard memory constraints are relaxed and a studyevaluating the use of a global D∗ lite path planner is performed. Second, a novel multi-resolution representation of the navigation map which covers larger areas atno memory cost increase is proposed. It is further used by a global path planner which automatically reduces the computational load by selecting its search direction based on obstacle shapes and distribution in the navigation space
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Herve, Yann. "Le radar WISDOM à bord du Rover de la mission ExoMars : Caractérisation et préparation du retour scientifique." Thesis, Université Paris-Saclay (ComUE), 2018. http://www.theses.fr/2018SACLV071/document.

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La recherche de trace de vie, passée ou présente, sur Mars est l’objectif principal de la mission martienne européenne ExoMars (ESA-Roscosmos), dont le lancement est prévu pour l’été 2020. Cette mission déposera à la surface de Mars un Rover équipé d'instruments dédiés notamment à l’étude du sous-sol de la planète dont une foreuse collectera des échantillons. Le travail de thèse présenté dans ce manuscrit porte sur la préparation du retour scientifique de l’expérience du radar WISDOM (Water Ice and Subsurface Deposits Observation on Mars) embarqué à bord du Rover d’ExoMars 2020 et dont l’objectif principal est la caractérisation, avant forage, du sous-sol proche de Mars.Les données recueillies par WISDOM permettront d’identifier les formations géologiques du sous-sol et de comprendre les processus qui en sont à l’origine. Elles guideront également les opérations de prélèvement d'échantillons en profondeur. L'objectif de cette thèse était de préparer les outils de traitements et d'interprétation de ces données. Les résultats obtenus doivent permettre d'exploiter au mieux les possibilités de l'instrument et d’atteindre les ambitieux objectifs technologiques (en termes notamment de résolution et de sensibilité) et scientifiques fixés. Plus précisément, il s’agissait de mettre en place des outils pour aboutir à une description des premiers mètres du sous-sol via l’interprétation des radargrammes de WISDOM en termes d’épaisseur de couche(s), de rugosité des interfaces, de distribution en taille d’éventuelles roches enfouies, d’orientation des strates et de constantes géo-électriques pour les unités géologiques détectées.Ce travail de thèse a permis la mise en place d’une chaîne de traitement de données ainsi que d’outils d’interprétation (traitement automatique et modélisation du radar).L’approche a été d’aborder le problème à la fois du point de vue théorique et du point de vue pratique. En conséquence, ce travail s’est appuyé sur deux aspects indissociables que sont, d’une part, la modélisation (analytique et numérique) du fonctionnement de l’instrument dans son environnement et, d’autre part, le traitement des données simulées et/ou expérimentales obtenues en milieu contrôlé ou lors de campagnes de mesures organisées dans le cadre de cette thèse
The main objective of European ExoMars (ESA-Roscosmos) mission is to search for signs of past or present life on Mars. The mission, to be launched in summer 2020, will deliver a rover on the surface of Mars. This rover accommodates instruments designed to investigate the close subsurface and, in particular, a drill that will collect samples at depth ranging from 0.5 m to 2 m. This thesis manuscript relates the preparation of the scientific return of the WISDOM (Water Ice and Subsurface Deposits Observation on Mars) radar experiment whose main objective is to characterize, before drilling, the shallow subsurface of Mars.Data obtained by WISDOM will shed the light on geological structures in the subsurface and therefore help trace back the history of the investigated Martian sites. Furthermore, they will help to identify the most promising locations to collect samples without jeopardizing the drill. The objective of this thesis was to efficiently pave the way to data interpretation and appraise WISDOM’s potentiality.In order to reach the ambitious scientific and technologic objectives (especially in terms of resolution and sensitivity) of WISDOM, we have developed tools that rely on a deep understanding of the instrument. The ultimate goal of these tools is to provide a reliable representation of the shallow subsurface and quantitative interpretation in terms of thickness and orientation of underground layers, roughness at interfaces, distribution of buried rocks and geoelectrical constant for each geological unit detected.This thesis manuscript describes the signal processing chain and tools developed in order to prepare WISDOM’s scientific return. When possible, approaches based on automatic detection were preferred. This work relies both on theoretical and practical investigations, including an accurate (analytical and numerical) modeling of the instrument operations and test on experimental data acquired during field campaigns on potential Martian analogs
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Barthelmes, Stefan [Verfasser]. "Model-Based Chassis Control of a Wheeled Mobile Robot on Soft Ground Using the Example of the ExoMars Planetary Exploration Rover / Stefan Barthelmes." München : Verlag Dr. Hut, 2020. http://d-nb.info/1222353156/34.

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Reinhardt, Manuel [Verfasser], Volker [Akademischer Betreuer] Thiel, Volker [Gutachter] Thiel, Walter [Gutachter] Goetz, and Lorenz [Gutachter] Schwark. "Assessing the formation and preservation of organic signatures in extreme environments in the context of the ExoMars 2020 rover mission / Manuel Reinhardt ; Gutachter: Volker Thiel, Walter Goetz, Lorenz Schwark ; Betreuer: Volker Thiel." Göttingen : Niedersächsische Staats- und Universitätsbibliothek Göttingen, 2019. http://d-nb.info/1195777140/34.

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Vijayan, Ria. "Wheel-terrain contact angle estimation for planetary exploration rovers." Thesis, Luleå tekniska universitet, Rymdteknik, 2018. http://urn.kb.se/resolve?urn=urn:nbn:se:ltu:diva-70676.

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During space missions, real time tele-operation of a rover is not practical because of significant signal latencies associated with inter planetary distances, making some degree of autonomy in rover control desirable. One of the challenges to achieving autonomy is the determination of terrain traversability. As part of this field, the determination of motion state of a rover on rough terrain via the estimation of wheel-terrain contact angles is proposed. This thesis investigates the feasibility of estimating the contact angles from the kinematics of the rover system and measurements from the onboard inertial measurement unit (IMU), joint angle sensors and wheel encoders. This approach does not rely on any knowledge of the terrain geometry or terrain mechanical properties. An existing framework of rover velocity and wheel slip estimation for flat terrain has been extended to additionally estimate the wheel-terrain contact angle along with a side slip angle for each individual wheel, for rough terrain drive. A random walk and a damped model are used to describe the evolution of the contact angle and side slip angle over an unknown terrain. A standard strapdown algorithm for the estimation of attitude and velocity from IMU measurements, is modified to incorporate the 3D kinematics of the rover in the implementation of a nonlinear Kalman filter to estimate the motion states. The estimation results from the filter are verified using tests performed on the ExoMars BB2. The obtained contact angle estimates are found to be consistent with the reference values.
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Reinhardt, Manuel. "Assessing the formation and preservation of organic signatures in extreme environments in the context of the ExoMars 2020 rover mission." Doctoral thesis, 2019. http://hdl.handle.net/21.11130/00-1735-0000-0003-C1C2-7.

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Book chapters on the topic "ExoMars Rover"

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Vago, Jorge L., Andrew J. Coates, Ralf Jaumann, Oleg Korablev, Valérie Ciarletti, Igor Mitrofanov, Jean-Luc Josset, et al. "Searching for Traces of Life With the ExoMars Rover." In From Habitability to Life on Mars, 309–47. Elsevier, 2018. http://dx.doi.org/10.1016/b978-0-12-809935-3.00011-6.

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Conference papers on the topic "ExoMars Rover"

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Riva, Stefano, Pietro Zanella, Romano Romani, Raffaella Contini, Jose Maria Arroyo, Juan Carlos Bahillo, Cristina Borque, et al. "The ExoMars Rover Solar Array Assembly." In 2019 European Space Power Conference (ESPC). IEEE, 2019. http://dx.doi.org/10.1109/espc.2019.8932077.

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Joudrier, Luc, A. Elfving, and Nuno Silva. "Challenges of the ExoMars Rover Control." In AIAA Infotech@Aerospace Conference. Reston, Virigina: American Institute of Aeronautics and Astronautics, 2009. http://dx.doi.org/10.2514/6.2009-1807.

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Tosi, Maria Cristina, Sergio Mannu, Gwyn Jones, Andrew Quinn, and Jim Clemmet. "EXOMARS ROVER MODULE Thermal Control System." In International Conference On Environmental Systems. 400 Commonwealth Drive, Warrendale, PA, United States: SAE International, 2008. http://dx.doi.org/10.4271/2008-01-2003.

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Alary, Coralie, and Stéphane Lapensée. "Thermal Design of the ExoMars Rover Module." In 40th International Conference on Environmental Systems. Reston, Virigina: American Institute of Aeronautics and Astronautics, 2010. http://dx.doi.org/10.2514/6.2010-6188.

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Tricot, Helene, and Paul Brochard. "EXOMARS 2020 mission Descent module & Rover batteries." In 2019 European Space Power Conference (ESPC). IEEE, 2019. http://dx.doi.org/10.1109/espc.2019.8931994.

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Nikiforov, S. Y., I. G. Mitrofanov, M. L. Litvak, A. A. Anikin, D. V. Golovin, M. V. Djachkova, A. S. Kozyrev, et al. "The ADRON-RM Instrument Onboard the ExoMars Rover." In XVI Young Scientists Conference “Fundamental and Applied Space Researches”. Space Research Institute, 2019. http://dx.doi.org/10.21046/kmu-2019-114-120.

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John Faber Archila-Diaz, Ingrid Lorena Argote-Pedraza, Luiz Alves Neto, Ataulfo Vizotto, Tiberon Petrus, Marcelo Becker, and Mario Luiz Tronco. "SIMULATION OF CURIOSITY AND EXOMARS ROVER ON AGRICULTURETERRAIN." In IX Congresso Nacional de Engenharia Mecânica. Rio de Janeiro, Brazil: ABCM Associação Brasileira de Engenharia e Ciências Mecânicas, 2016. http://dx.doi.org/10.20906/cps/con-2016-1283.

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Plettemeier, Dirk, Valerie Ciarletti, Svein-Erik Hamran, Charlotte Corbel, Philippe Cais, Wolf-Stefan Benedix, Klaus Wolf, Stefan Linke, and Susanne Roddecke. "Full polarimetric GPR antenna system aboard the ExoMars rover." In 2009 IEEE Radar Conference. IEEE, 2009. http://dx.doi.org/10.1109/radar.2009.4977120.

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Balme, Matt, Elena Favaro, Stephen Lewis, and Alexander Barrett. "AEOLIAN BEDFORMS AT THE EXOMARS ROSALIND FRANKLIN ROVER LANDING SITE." In GSA 2020 Connects Online. Geological Society of America, 2020. http://dx.doi.org/10.1130/abs/2020am-358731.

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Martinez Fadrique, Fran, Rafael Sánchez-Beato Fernández, Marco Barrera, Paola Franceschetti, and Luc Joudrier. "ExoMars 2020: Rover Operations Control System Design as part of the Rover Operations Control Center (ROCC)." In 15th International Conference on Space Operations. Reston, Virginia: American Institute of Aeronautics and Astronautics, 2018. http://dx.doi.org/10.2514/6.2018-2405.

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