Relevant bibliographies by topics / MARS-3D

Contents

  1. Journal articles
  2. Dissertations / Theses
  3. Books
  4. Book chapters
  5. Conference papers

Academic literature on the topic 'MARS-3D'

Author: Grafiati
Published: 4 June 2021
Last updated: 1 February 2022

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Journal articles on the topic "MARS-3D"

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Loy, D. Gareth. "Mars in 3D." Computer Music Journal 37, no. 3 (September 2013): 101–3. http://dx.doi.org/10.1162/comj_r_00188.

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Kallio, E., H. Koskinen, S. Barabash, R. Lundin, O. Norberg, and J. G. Luhmann. "3D plasma observations near Mars." Geophysical Research Letters 20, no. 21 (November 5, 1993): 2339–42. http://dx.doi.org/10.1029/93gl02634.

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Courtland, Rachel. "Review: Mars 3D by Jim Bell." New Scientist 200, no. 2686 (December 2008): 47. http://dx.doi.org/10.1016/s0262-4079(08)63167-x.

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O'Neill, Sean. "3D print a home on Mars." New Scientist 226, no. 3023 (May 2015): 27. http://dx.doi.org/10.1016/s0262-4079(15)30462-0.

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Grace, Robert. "Habitats for Humanity - Potentially 3D Printed on Mars." Plastics Engineering 73, no. 8 (September 2017): 16. http://dx.doi.org/10.1002/j.1941-9635.2017.tb01773.x.

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Tao, Yu, Greg Michael, Jan-Peter Muller, Susan J. Conway, and Alfiah R. D. Putri. "Seamless 3D Image Mapping and Mosaicing of Valles Marineris on Mars Using Orbital HRSC Stereo and Panchromatic Images." Remote Sensing 13, no. 7 (April 3, 2021): 1385. http://dx.doi.org/10.3390/rs13071385.

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A seamless mosaic has been constructed including a 3D terrain model at 50 m grid-spacing and a corresponding terrain-corrected orthoimage at 12.5 m using a novel approach applied to ESA Mars Express High Resolution Stereo Camera orbital (HRSC) images of Mars. This method consists of blending and harmonising 3D models and normalising reflectance to a global albedo map. Eleven HRSC image sets were processed to Digital Terrain Models (DTM) based on an opensource stereo photogrammetric package called CASP-GO and merged with 71 published DTMs from the HRSC team. In order to achieve high quality and complete DTM coverage, a new method was developed to combine data derived from different stereo matching approaches to achieve a uniform outcome. This new approach was developed for high-accuracy data fusion of different DTMs at dissimilar grid-spacing and provenance which employs joint 3D and image co-registration, and B-spline fitting against the global Mars Orbiter Laser Altimeter (MOLA) standard reference. Each HRSC strip is normalised against a global albedo map to ensure that the very different lighting conditions could be corrected and resulting in a tiled set of seamless mosaics. The final 3D terrain model is compared against the MOLA height reference and the results shown of this intercomparison both in altitude and planum. Visualisation and access mechanisms to the final open access products are described.
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Domínguez-Pumar, Manuel, Lukasz Kowalski, Vicente Jiménez, Ivette Rodríguez, Manel Soria, Sandra Bermejo, and Joan Pons-Nin. "Analyzing the Performance of a Miniature 3D Wind Sensor for Mars." Sensors 20, no. 20 (October 20, 2020): 5912. http://dx.doi.org/10.3390/s20205912.

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This paper analyzes the behavior of a miniature 3D wind sensor designed for Mars atmosphere. The sensor is a spherical structure of 10 mm diameter divided in four sectors. By setting all the sectors to constant temperature, above that of the air, the 3D wind velocity vector can be measured. Two sets of experiments have been performed. First, an experimental campaign made under typical Mars conditions at the Aarhus Wind Tunnel Simulator is presented. The results demonstrate that both wind speed and angle can be efficiently measured, using a simple inverse algorithm. The effect of sudden wind changes is also analyzed and fast response times in the range of 0.7 s are obtained. The second set of experiments is focused on analyzing the performance of the sensor under extreme Martian wind conditions, reaching and going beyond the Dust Devil scale. To this purpose, both high-fidelity numerical simulations of fluid dynamics and heat transfer and experiments with the sensor have been performed. The results of the experiments, made for winds in the Reynolds number 1000–2000 range, which represent 65–130 m/s of wind speed under typical Mars conditions, further confirm the simulation predictions and show that it will be possible to successfully measure wind speed and direction even under these extreme regimes.
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Basdogan, Cagatay. "From 2D Images to 3D Tangible Models: Autostereoscopic and Haptic Visualization of Martian Rocks in Virtual Environments." Presence: Teleoperators and Virtual Environments 16, no. 1 (February 1, 2007): 1–15. http://dx.doi.org/10.1162/pres.16.1.1.

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A planetary rover acquires a large collection of images while exploring its surrounding environment. For example, 2D stereo images of the Martian surface captured by the lander and the Sojourner rover during the Mars Pathfinder mission in 1997 were transmitted to Earth for scientific analysis and navigation planning. Due to the limited memory and computational power of the Sojourner rover, most of the images were captured by the lander and then transmitted to Earth directly for processing. If these images were merged together at the rover site to reconstruct a 3D representation of the rover's environment using its on-board resources, more information could potentially be transmitted to Earth in a compact manner. However, construction of a 3D model from multiple views is a highly challenging task to accomplish even for the new generation rovers (Spirit and Opportunity) running on the Mars surface at the time this article was written. Moreover, low transmission rates and communication intervals between Earth and Mars make the transmission of any data more difficult. We propose a robust and computationally efficient method for progressive transmission of multi-resolution 3D models of Martian rocks and soil reconstructed from a series of stereo images. For visualization of these models on Earth, we have developed a new multimodal visualization setup that integrates vision and touch. Our scheme for 3D reconstruction of Martian rocks from 2D images for visualization on Earth involves four main steps: a) acquisition of scans: depth maps are generated from stereo images, b) integration of scans: the scans are correctly positioned and oriented with respect to each other and fused to construct a 3D volumetric representation of the rocks using an octree, c) transmission: the volumetric data is encoded and progressively transmitted to Earth, d) visualization: a surface model is reconstructed from the transmitted data on Earth and displayed to a user through a new autostereoscopic visualization table and a haptic device for providing touch feedback. To test the practical utility of our approach, we first captured a sequence of stereo images of a rock surface from various viewpoints in JPL MarsYard using a mobile cart and then performed a series of 3D reconstruction experiments. In this paper, we discuss the steps of our reconstruction process, our multimodal visualization system, and the tradeoffs that have to be made to transmit multiresolution 3D models to Earth in an efficient manner under the constraints of limited computational resources, low transmission rate, and communication interval between Earth and Mars.
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Coughlin, Natalie, Bradley Drake, Mikala Fjerstad, Easton Schuster, Tyler Waege, Adrian Weerakkody, and Todd Letcher. "Development and Mechanical Properties of Basalt Fiber-Reinforced Acrylonitrile Butadiene Styrene for In-Space Manufacturing Applications." Journal of Composites Science 3, no. 3 (September 5, 2019): 89. http://dx.doi.org/10.3390/jcs3030089.

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A new basalt fiber reinforced acrylonitrile butadiene styrene (ABS) filament has been developed for fused filament fabrication (FFF, 3D printing) to be used in Mars habitat construction. Building habitats on Mars will be expensive, especially if all material must be shipped from earth. However, if some materials can be used from Mars, costs will dramatically decrease. Basalt is easily mined from the surface of Mars. This study details the production process of the material, experimental results from mechanical testing, and preliminary X-ray shielding characteristics. The addition of chopped 3 mm basalt fibers to standard FFF material, ABS, increased strength and stiffness of the composite material. By adding 25% (by weight) basalt fiber to ABS, tensile strength improved nearly 40% by increasing from 36.55 MPa to 50.58 MPa, while Modulus of Elasticity increased about 120% from 2.15 GPa to 4.79 GPa. Flexural strength increased by about 20% from 56.94 MPa to 68.51 MPa, while Flexural Modulus increased by about 70% from 1.81 GPa to 3.05 GPa. While compression results did not see much strength improvements, the addition of fibers also did not decrease compressive strength. This is important when considering that basalt fibers provide radiation shielding and the cost of adding basalt fibers to construction materials on Mars will be negligible compared to the cost of shipping other materials from earth. In preliminary digital radiography testing, it was shown that 77% of X-rays were shielded with 25% basalt fiber added (as compared to neat ABS). In small-scale 3D printing applications, the 25% fiber ratio seems to be the highest ratio that provides reliable FFF printing.
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Basak, Arnab, and Dibyendu Nandy. "Modelling the imposed magnetospheres of Mars-like exoplanets: star–planet interactions and atmospheric losses." Monthly Notices of the Royal Astronomical Society 502, no. 3 (January 28, 2021): 3569–81. http://dx.doi.org/10.1093/mnras/stab225.

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ABSTRACT Based on 3D compressible magnetohydrodynamic simulations, we explore the interactions between the magnetized wind from a solar-like star and a Mars-like planet – with a gravitionally stratified atmosphere – that is either non-magnetized or hosts a weak intrinsic dipolar field. The primary mechanism for the induction of a magnetosphere around a non-magnetized conducting planet is the pile-up of stellar magnetic fields in the day-side region. The magnetopause stand-off distance decreases as the strength of the planetary dipole field is lowered and saturates to a minimum value for the case of a planet with no magnetic field. Global features such as bow shock, magnetosheath, magnetotail, and strong current sheets are observed in the imposed magnetosphere. We explore variations in atmospheric mass loss rates for different stellar wind strengths to understand the impact of stellar magnetic activity and plasma winds – and their evolution – on (exo)planetary habitability. In order to simulate a case analogous to the present-day Mars, a planet without atmosphere is considered. Our simulations are found to be in good agreement with observational data from Mars Global Surveyor and Mars Atmosphere and Volatile EvolutioN missions and is expected to complement observations from the Emirates (Hope) Mars Mission, China's Tianwen-1 and NASA's Mars 2020 Perseverance mission.
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Dissertations / Theses on the topic "MARS-3D"

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Christoff, Vesselinova Nicole. "Détection et caractérisation d'attributs géométriques sur les corps rocheux du système solaire." Thesis, Aix-Marseille, 2018. http://www.theses.fr/2018AIXM0565/document.

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L’un des défis de la science planétaire est la détermination de l’âge des surfaces des différents corps célestes du système solaire, pour comprendre leurs processus de formation et d’évolution. Une approche repose sur l’analyse de la densité et de la taille des cratères d’impact. En raison de l’énorme quantité de données à traiter, des approches automatiques ont été proposées pour détecter les cratères d’impact afin de faciliter ce processus de datation. Ils utilisent généralement les valeurs de couleur des images ou les valeurs d’altitude de "modèles numériques d’élévation" (DEM). Dans cette thèse, nous proposons une nouvelle approche pour détecter les bords des cratères. L’idée principale est de combiner l’analyse de la courbure avec une classification basée sur un réseau de neurones. Cette approche comporte deux étapes principales : premièrement, chaque sommet du maillage est étiqueté avec la valeur de la courbure minimale; deuxièmement, cette carte de courbure est injectée dans un réseau de neurones pour détecter automatiquement les formes d’intérêt. Les résultats montrent que la détection des formes est plus efficace en utilisant une carte en deux dimensions s’appuyant sur le calcul d’estimateurs différentiels discrets, plutôt qu’en utilisant la valeur de l’élévation en chaque sommet. Cette approche réduit significativement le nombre de faux négatifs par rapport aux approches précédentes basées uniquement sur une information topographique. La validation de la méthode est effectuée sur des DEM de Mars, acquis par un altimètre laser à bord de la sonde spatiale "Mars Global Surveyor" de la NASA et combinés avec une base de données de cratères identifiés manuellement
One of the challenges of planetary science is the age determination of the surfaces of the different celestial bodies in the solar system, to understand their formation and evolution processes. An approach relies on the analysis of the crater impact density and size. Due to the huge quantity of data to process, automatic approaches have been proposed for automatically detecting impact craters in order to facilitate this dating process. They generally use the color values from images or the elevation values from Digital Elevation Model (DEM). In this PhD thesis, we propose a new approach for detecting craters rims. The main idea is to combine curvature analysis with Neural Network based classification. This approach contains two main steps: first, each vertex of the mesh is labeled with the value of the minimal curvature; second, this curvature map is injected into a neural network to automatically detect the shapes of interest. The results show that detecting forms are more efficient using a two-dimensional map based on the computation of discrete differential estimators, than by the value of the elevation at each vertex. This approach significantly reduces the number of false negatives compared to previous approaches based on topographic information only. The validation of the method is performed on DEMs of Mars, acquired by a laser altimeter aboard NASA’s Mars Global Surveyor spacecraft and combined with a database of manually identified craters
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Tessier, Caroline. "Caractérisation et dynamique des turbidités en zone côtière : l'exemple de la région marine Bretagne Sud." Bordeaux 1, 2006. http://www.theses.fr/2006BOR13307.

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L’étude des variabilités spatio-temporelles des turbidités en Bretagne Sud a été entreprise en associant les résultats des campagnes hydrologiques, des suivis in situ au point fixe, des observations satellitales et une modélisation numérique 3D déterministe. La synthèse des observations antérieures montre un gradient côte-large des concentrations qui ne dépassent guère les 30 mg/l au delà de la zone littorale. Des profileurs acoustiques (ADCP) ont été mouillés pour mesurer les courants, les vagues et la dynamique des particules fines associée à ces forçages. A partir du signal rétrodiffusé, les séries temporelles de concentration massique sur toute la colonne d’eau ont été déduites, les valeurs peuvent atteindre 100 mg/l à 1. 50 m du fond pendant les événements de houles, à l’entrée de la baie de Vilaine. La calibration empirique du signal rétrodiffusé avec des mesures indépendantes de turbidité s’est révélée très satisfaisante et plus efficace que l’inversion d’un modèle de rétrodiffusion, du fait des incertitudes instrumentales et environnementales. Ces mesures au point fixe ont permis de calibrer un modèle hydro-sédimentaire (MARS-3D/SiAM) en configuration quasi-réaliste (marée, vent, apports par les fleuves, couverture sédimentaire), avec une paramétrisation simple des processus sédimentaires (érosion, dépôt). Le forçage des vagues est issu du modèle SWAN. Les résultats de 5 mois de simulation montrent l’importance des circulations liées au vent et de la structure hydrologique dans la répartition spatiale des turbidités, qui restent principalement générées par les houles. Les concentrations moyennes par secteurs et les flux de matière sont aussi estimés.
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Khojasteh, Pour Fard Iman. "Modélisation des échanges dissous entre l'estuaire de la Loire et les baies côtières adjacentes." Thesis, Bordeaux, 2015. http://www.theses.fr/2015BORD0300/document.

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Les estuaires sont des zones à l’interface terre-mer au coeur de la question du devenir des apports continentaux drainés par les grands bassins versants. L’objet de cette étude est focalisé sur l’estuaire de la Loire et ses zones adjacentes (i.e. baie de Bourgneuf et le Mor-Bras) situés dans le nord-est du Golfe de Gascogne. C’est un environnement soumis à l’influence significative de la marée qui se propage en amont de l’embouchure à plus de 100 km, de forçages météorologiques de moyennes latitudes donc hautement variables qui induisent en particulier des débits fluviaux pouvant varier d’un facteur dix. Cette variabilité est étudiée à l’aide d’un modèle numérique et des outils de description de la circulation qui permettent de mieux cerner les temps de séjours et de transits des eaux continentales dans l’estuaire et vers les baies riveraines. L’approche s’appuie sur un modèle en grille structurée mais dont la malléabilité pour décrire la complexité du domaine à simuler est donnée par le caractère non orthogonal des mailles employées pour la discrétisation. Le choix d’un système de coordonnées optimale (covariantes ou contravariantes) est discuté puis implémenté dans le code MARS-3D. Ce nouvel outil est qualifié et validé sur des cas-test puis implémenté en conditions réelles sur un domaine à la géométrie particulièrement accidentée. Les simulations reproduisent très finement la dynamique du grand panache de la Loire et confirment sa très grande variabilité spatiale et temporelle que décrivent partiellement des observations à haute fréquence et ponctuelles ; elles permettent de décrire les chemins privilégiés des masses d’eau à travers les sections de références choisies
Estuaries are key areas in between land and ocean which play a major role in the spreading ofcontinental runoff drained by large watershed. This study focused on the Loire Estuary and its adjacentbays (i.e. Bourgneuf bay and Mor-Braz sea) all located in the north-east side of the bay of Biscay. It isinfluenced by the large tidal wave that propagates upstream the mouth on more than a 100 km, by highlymid-latitude meteorological forcing that may not only induced High variability in the circulation driversbut also on the river runoffs that may vary from 1 to 10 from early spring to late summer. This Highvariability is studied thanks to numerical simulation and tools dedicated to describe the circulation withsynthetic index such as transit time and mean age of water. The approach lies on a numerical modeldiscretized on a structure grid which constraints have been relaxed to better fit the fractal coastal lineusing non orthogonal grid cells. The optimal coordinate framework (co or contra-variant) have beendiscussed, and implemented within a pre-existing code (i.e. MARS-3D). This tools was validated withtest cases and implemented on a domain with a particular complex geometry. The numerical simulationscatch very accurately the dynamic of this large plume at least as it is described by available in situobservations. This numerical solution allowed to exhibit the main path of water masses through the areaand from place to place and their variability according to the main forcings
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Böttger, Henning M. "Modelling the water cycle on Mars." Thesis, University of Oxford, 2003. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.289340.

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Soares, Filipa Freitas. "Going Mars, the beginning of a printed living machine Development of 3D printed structures with in-situ resources." Dissertação, 2018. https://hdl.handle.net/10216/117622.

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Soares, Filipa Freitas. "Going Mars, the beginning of a printed living machine Development of 3D printed structures with in-situ resources." Master's thesis, 2018. https://hdl.handle.net/10216/117622.

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Books on the topic "MARS-3D"

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Vacation Bible School To Mars and Beyond 3D Planet Scene Craft Kit: Explore Where God's Power Can Take You! Cokesbury, 2020.

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Book chapters on the topic "MARS-3D"

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Müller, M., S. Gruber, M. D. Coen, R. Campbell, D. Kim, and B. Morrell. "Operational Benefit of a 3D Printer in Future Human Mars Missions—Results from Analog Simulation Testing." In Space Operations: Inspiring Humankind's Future, 747–77. Cham: Springer International Publishing, 2019. http://dx.doi.org/10.1007/978-3-030-11536-4_29.

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Christoff, Nicole, Agata Manolova, Laurent Jorda, Sophie Viseur, Sylvain Bouley, and Jean-Luc Mari. "Level-Set Based Algorithm for Automatic Feature Extraction on 3D Meshes: Application to Crater Detection on Mars." In Computer Vision and Graphics, 103–14. Cham: Springer International Publishing, 2018. http://dx.doi.org/10.1007/978-3-030-00692-1_10.

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Stricker, Andrew G., Cynthia Calongne, Barbara Truman, David J. Lyle, and J. J. Jacobson. "AI-Augmented Developmental Instruction for Improving Contemplative Practices in the Face of Complexity." In Recent Advances in Applying Identity and Society Awareness to Virtual Learning, 343–67. IGI Global, 2019. http://dx.doi.org/10.4018/978-1-5225-9679-0.ch017.

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A simulation design is introduced for using artificial intelligence (AI)-augmented developmental instruction for improving contemplative practices in the face of complexity. The focus of the design is on developmental instruction in the use of contemplative cognitive and moral reasoning practices to improve self-awareness and means to better discern and address complicated and complex challenges. Developmental instruction is supported by an AI-augmented tutoring aid provided during a simulated mission to Mars within an immersive 3D-world. A set of tasks are introduced during the Mars simulation to assist with the development of contemplative practices. The AI-augmented tutoring aid assists participants in the simulation to better understand and apply contemplative practices involving cognitive and moral reasoning meta-thinking suitable for each task. High levels of fidelity, involving visual, auditory, and interactive model-based reasoning (MBR) tools help to embed the senses, thoughts, and actions of participants in the feeling of traveling and being on Mars.
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Shih, Ya-Chun, and Molly Leonard. "Immersion and Interaction via Avatars within Google Street View." In Packaging Digital Information for Enhanced Learning and Analysis, 266–81. IGI Global, 2014. http://dx.doi.org/10.4018/978-1-4666-4462-5.ch012.

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The optimal approach to learning a target culture is to experience it in its real-life context through interaction. The new 3D virtual world platform under consideration, Blue Mars Lite, enables users to be immersed in existing Google Maps Street View panorama, globally. Google Maps with Street View contains a massive collection of 360-degree street-level images of the most popular places worldwide. The authors explore the possibility of integrating these global panoramas, in which multiple users can explore, discuss, and role-play, into the classroom. The goal of this chapter is to shed new light on merging Google Street View with the 3D virtual world for cultural learning purposes. This approach shows itself to be a promising teaching method that can help EFL learners to develop positive attitudes toward the target culture and cultural learning in this new cultural setting.
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Shih, Ya-Chun, and Molly Leonard. "Immersion and Interaction via Avatars within Google Street View." In Cross-Cultural Interaction, 660–75. IGI Global, 2014. http://dx.doi.org/10.4018/978-1-4666-4979-8.ch037.

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The optimal approach to learning a target culture is to experience it in its real-life context through interaction. The new 3D virtual world platform under consideration, Blue Mars Lite, enables users to be immersed in existing Google Maps Street View panorama, globally. Google Maps with Street View contains a massive collection of 360-degree street-level images of the most popular places worldwide. The authors explore the possibility of integrating these global panoramas, in which multiple users can explore, discuss, and role-play, into the classroom. The goal of this chapter is to shed new light on merging Google Street View with the 3D virtual world for cultural learning purposes. This approach shows itself to be a promising teaching method that can help EFL learners to develop positive attitudes toward the target culture and cultural learning in this new cultural setting.
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Conference papers on the topic "MARS-3D"

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Nakazato, M., and T. S. Huang. "3D MARS: immersive virtual reality for content-based image retrieval." In IEEE International Conference on Multimedia and Expo, 2001. ICME 2001. IEEE, 2001. http://dx.doi.org/10.1109/icme.2001.1237651.

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Zhang, Tingting, Zhichun Mu, Yihang Li, Qing Liu, and Yi Zhang. "3D Face and Ear Recognition based on Partial MARS Map." In 6th International Conference on Pattern Recognition Applications and Methods. SCITEPRESS - Science and Technology Publications, 2017. http://dx.doi.org/10.5220/0006244206330637.

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Cottin, Pierre, François Babin, Daniel Cantin, Adam Deslauriers, and Bruno Sylvestre. "Active 3D camera design for target capture on Mars orbit." In SPIE Defense, Security, and Sensing, edited by Monte D. Turner and Gary W. Kamerman. SPIE, 2010. http://dx.doi.org/10.1117/12.850169.

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Bonafini, Stefano, and Claudio Sacchi. "3D Ray-tracing Analysis of Radio Propagation on Mars Surface." In 2021 IEEE Aerospace Conference. IEEE, 2021. http://dx.doi.org/10.1109/aero50100.2021.9438180.

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"An Output and 3D Visualization Concept for the MSAAS System Mars." In 2017 Spring Simulation Multi-Conference. Society for Modeling and Simulation International (SCS), 2017. http://dx.doi.org/10.22360/springsim.2017.ads.004.

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Ge, Jian, Deqing Ren, Jonathan I. Lunine, Robert H. Brown, Roger V. Yelle, and Laurence A. Soderblom. "Compact high-resolution 3D imaging spectrometer for discovering oases on Mars." In Astronomical Telescopes and Instrumentation, edited by Richard B. Hoover, Alexei Y. Rozanov, and Roland R. Paepe. SPIE, 2003. http://dx.doi.org/10.1117/12.457334.

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Carrato, Peter J. "Use of BIM and 3D Printing in Mars Habitat Design Challenge." In 17th Biennial International Conference on Engineering, Science, Construction, and Operations in Challenging Environments. Reston, VA: American Society of Civil Engineers, 2021. http://dx.doi.org/10.1061/9780784483374.072.

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Tsagkaris, Christos, Andrea Camera, Ana Sofia Mota, and Maria Lydakaki. "3D Printing for medicinal chemistry in space: Crafting our way to Mars." In 5th International Electronic Conference on Medicinal Chemistry. Basel, Switzerland: MDPI, 2019. http://dx.doi.org/10.3390/ecmc2019-06355.

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Weast, A. B., J. M. Ota, C. A. Kitts, C. A. Bulich, A. M. Laurence, C. M. Lwin, T. D. Wigle, W. B. Perkins, and J. F. Cook. "Integrating digital stereo cameras with Mars Pathfinder technology for 3D regional mapping underwater." In 1999 IEEE Aerospace Conference. Proceedings (Cat. No.99TH8403). IEEE, 1999. http://dx.doi.org/10.1109/aero.1999.790206.

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Dickensheets, David L., Phillip A. Himmer, Robert A. Friholm, and B. Jeffrey Lutzenberger. "Miniature high-resolution imaging system with 3D MOEMS beam scanning for Mars exploration." In Micromachining and Microfabrication, edited by M. Edward Motamedi and Rolf Goering. SPIE, 2000. http://dx.doi.org/10.1117/12.396518.

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