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You searched for subject:(MARS 3D). Showing records 1 – 6 of 6 total matches.

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1. Ivan, I. (author). Mars Continuum.

Degree: 2014, Delft University of Technology

The aim of the project is to elaborate upon performance driven design experiments for habitation and production facilities on Mars. The experiments focus on enhancing… (more)

Subjects/Keywords: Mars; Biomimicry; 3D Print

…Multi Material 3D Print 2 Water - Radiation Shielding 2 3 4 5 6 4 Graphene Coating 5… …Greenhouse | Scale 1/50 Neutral Axis Femur porosity Femural stress distribution diagram 3D… …ExploreLab 18 | MARS CONTINUUM 18 19 20 21 One skin - one structure for effective usage of… 

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APA · Chicago · MLA · Vancouver · CSE | Export to Zotero / EndNote / Reference Manager

APA (6th Edition):

Ivan, I. (. (2014). Mars Continuum. (Masters Thesis). Delft University of Technology. Retrieved from http://resolver.tudelft.nl/uuid:06dbbe55-9644-44df-a42f-d7bc10667bec

Chicago Manual of Style (16th Edition):

Ivan, I (author). “Mars Continuum.” 2014. Masters Thesis, Delft University of Technology. Accessed October 22, 2020. http://resolver.tudelft.nl/uuid:06dbbe55-9644-44df-a42f-d7bc10667bec.

MLA Handbook (7th Edition):

Ivan, I (author). “Mars Continuum.” 2014. Web. 22 Oct 2020.

Vancouver:

Ivan I(. Mars Continuum. [Internet] [Masters thesis]. Delft University of Technology; 2014. [cited 2020 Oct 22]. Available from: http://resolver.tudelft.nl/uuid:06dbbe55-9644-44df-a42f-d7bc10667bec.

Council of Science Editors:

Ivan I(. Mars Continuum. [Masters Thesis]. Delft University of Technology; 2014. Available from: http://resolver.tudelft.nl/uuid:06dbbe55-9644-44df-a42f-d7bc10667bec

2. Christoff Vesselinova, Nicole. Détection et caractérisation d'attributs géométriques sur les corps rocheux du système solaire : Detection and characterization of geometric features on rocky surfaces on the solar system.

Degree: Docteur es, Informatique, 2018, Aix-Marseille; Université Technique de Sofia. Faculté Francophone

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… (more)

Subjects/Keywords: Maillages 3D; Extraction automatique de caractéristiques; Courbures discrètes; Réseau de neurones; Détection de cratères; Mars; 3D meshes; Automatic feature extraction; Discrete curvatures; Neural networks; Crater detection; Mars; 510

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APA (6th Edition):

Christoff Vesselinova, N. (2018). Détection et caractérisation d'attributs géométriques sur les corps rocheux du système solaire : Detection and characterization of geometric features on rocky surfaces on the solar system. (Doctoral Dissertation). Aix-Marseille; Université Technique de Sofia. Faculté Francophone. Retrieved from http://www.theses.fr/2018AIXM0565

Chicago Manual of Style (16th Edition):

Christoff Vesselinova, Nicole. “Détection et caractérisation d'attributs géométriques sur les corps rocheux du système solaire : Detection and characterization of geometric features on rocky surfaces on the solar system.” 2018. Doctoral Dissertation, Aix-Marseille; Université Technique de Sofia. Faculté Francophone. Accessed October 22, 2020. http://www.theses.fr/2018AIXM0565.

MLA Handbook (7th Edition):

Christoff Vesselinova, Nicole. “Détection et caractérisation d'attributs géométriques sur les corps rocheux du système solaire : Detection and characterization of geometric features on rocky surfaces on the solar system.” 2018. Web. 22 Oct 2020.

Vancouver:

Christoff Vesselinova N. Détection et caractérisation d'attributs géométriques sur les corps rocheux du système solaire : Detection and characterization of geometric features on rocky surfaces on the solar system. [Internet] [Doctoral dissertation]. Aix-Marseille; Université Technique de Sofia. Faculté Francophone; 2018. [cited 2020 Oct 22]. Available from: http://www.theses.fr/2018AIXM0565.

Council of Science Editors:

Christoff Vesselinova N. Détection et caractérisation d'attributs géométriques sur les corps rocheux du système solaire : Detection and characterization of geometric features on rocky surfaces on the solar system. [Doctoral Dissertation]. Aix-Marseille; Université Technique de Sofia. Faculté Francophone; 2018. Available from: http://www.theses.fr/2018AIXM0565

3. Khojasteh Pour Fard, Iman. Modélisation des échanges dissous entre l'estuaire de la Loire et les baies côtières adjacentes : Modelling of dissolved exchanges between the Loire estuary and the adjacent coastal bays.

Degree: Docteur es, Physique de l'environnement, 2015, Bordeaux

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… (more)

Subjects/Keywords: Hydrodynamique côtière; Golfe de Gascogne; Simulations Numériques; Estuaire de la Loire; MARS-3D; Non-Orthogonal; Maillage Curviligne; Coastal Hydrodynamics; River Plume; Loire Estuary (France); Biscay Bay; Flushing Time; MARS-3D; Non-Orthogonal; Curvilinear grid

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APA (6th Edition):

Khojasteh Pour Fard, I. (2015). Modélisation des échanges dissous entre l'estuaire de la Loire et les baies côtières adjacentes : Modelling of dissolved exchanges between the Loire estuary and the adjacent coastal bays. (Doctoral Dissertation). Bordeaux. Retrieved from http://www.theses.fr/2015BORD0300

Chicago Manual of Style (16th Edition):

Khojasteh Pour Fard, Iman. “Modélisation des échanges dissous entre l'estuaire de la Loire et les baies côtières adjacentes : Modelling of dissolved exchanges between the Loire estuary and the adjacent coastal bays.” 2015. Doctoral Dissertation, Bordeaux. Accessed October 22, 2020. http://www.theses.fr/2015BORD0300.

MLA Handbook (7th Edition):

Khojasteh Pour Fard, Iman. “Modélisation des échanges dissous entre l'estuaire de la Loire et les baies côtières adjacentes : Modelling of dissolved exchanges between the Loire estuary and the adjacent coastal bays.” 2015. Web. 22 Oct 2020.

Vancouver:

Khojasteh Pour Fard I. Modélisation des échanges dissous entre l'estuaire de la Loire et les baies côtières adjacentes : Modelling of dissolved exchanges between the Loire estuary and the adjacent coastal bays. [Internet] [Doctoral dissertation]. Bordeaux; 2015. [cited 2020 Oct 22]. Available from: http://www.theses.fr/2015BORD0300.

Council of Science Editors:

Khojasteh Pour Fard I. Modélisation des échanges dissous entre l'estuaire de la Loire et les baies côtières adjacentes : Modelling of dissolved exchanges between the Loire estuary and the adjacent coastal bays. [Doctoral Dissertation]. Bordeaux; 2015. Available from: http://www.theses.fr/2015BORD0300


University of Michigan

4. Ma, Yingjuan. Three-dimensional multispecies global MHD studies of the solar wind interaction with Mars and Saturn's magnetospheric plasma flow with Titan.

Degree: PhD, Pure Sciences, 2006, University of Michigan

 This dissertation presents numerical simulation results of the interaction of the solar wind/magnetospheric plasma flow with weakly magnetized/unmagnetized solar system bodies (Mars and Titan) using… (more)

Subjects/Keywords: 3d; Dimensional; Flow; Global; Interaction; Magnetohydrodynamics; Magnetospheric Plasma; Mars; Mhd; Multi; Multispecies; Saturn; Solar Wind; Species; Studies; Three; Titan

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APA (6th Edition):

Ma, Y. (2006). Three-dimensional multispecies global MHD studies of the solar wind interaction with Mars and Saturn's magnetospheric plasma flow with Titan. (Doctoral Dissertation). University of Michigan. Retrieved from http://hdl.handle.net/2027.42/125701

Chicago Manual of Style (16th Edition):

Ma, Yingjuan. “Three-dimensional multispecies global MHD studies of the solar wind interaction with Mars and Saturn's magnetospheric plasma flow with Titan.” 2006. Doctoral Dissertation, University of Michigan. Accessed October 22, 2020. http://hdl.handle.net/2027.42/125701.

MLA Handbook (7th Edition):

Ma, Yingjuan. “Three-dimensional multispecies global MHD studies of the solar wind interaction with Mars and Saturn's magnetospheric plasma flow with Titan.” 2006. Web. 22 Oct 2020.

Vancouver:

Ma Y. Three-dimensional multispecies global MHD studies of the solar wind interaction with Mars and Saturn's magnetospheric plasma flow with Titan. [Internet] [Doctoral dissertation]. University of Michigan; 2006. [cited 2020 Oct 22]. Available from: http://hdl.handle.net/2027.42/125701.

Council of Science Editors:

Ma Y. Three-dimensional multispecies global MHD studies of the solar wind interaction with Mars and Saturn's magnetospheric plasma flow with Titan. [Doctoral Dissertation]. University of Michigan; 2006. Available from: http://hdl.handle.net/2027.42/125701


University of Michigan

5. Liu, Yifan. 3D multispecies MHD studies of the interaction of the ionospheres of unmagnetized solar system bodies with the solar wind or magnetospheric plasma flows.

Degree: PhD, Pure Sciences, 2000, University of Michigan

 We used 3D multi-species MHD models to study the solar wind interaction with the ionosphere of Mars and the magnetospheric interaction with the ionospheres of… (more)

Subjects/Keywords: 3d; Europa; Interaction; Ionosphere; Ionospheres; Magnetohydrodynamics; Magnetospheric; Mars; Mhd; Multispecies; Plasma Flows; Solar Wind; Studies; Titan; Unmagnetized Solar System Bodies

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APA · Chicago · MLA · Vancouver · CSE | Export to Zotero / EndNote / Reference Manager

APA (6th Edition):

Liu, Y. (2000). 3D multispecies MHD studies of the interaction of the ionospheres of unmagnetized solar system bodies with the solar wind or magnetospheric plasma flows. (Doctoral Dissertation). University of Michigan. Retrieved from http://hdl.handle.net/2027.42/132825

Chicago Manual of Style (16th Edition):

Liu, Yifan. “3D multispecies MHD studies of the interaction of the ionospheres of unmagnetized solar system bodies with the solar wind or magnetospheric plasma flows.” 2000. Doctoral Dissertation, University of Michigan. Accessed October 22, 2020. http://hdl.handle.net/2027.42/132825.

MLA Handbook (7th Edition):

Liu, Yifan. “3D multispecies MHD studies of the interaction of the ionospheres of unmagnetized solar system bodies with the solar wind or magnetospheric plasma flows.” 2000. Web. 22 Oct 2020.

Vancouver:

Liu Y. 3D multispecies MHD studies of the interaction of the ionospheres of unmagnetized solar system bodies with the solar wind or magnetospheric plasma flows. [Internet] [Doctoral dissertation]. University of Michigan; 2000. [cited 2020 Oct 22]. Available from: http://hdl.handle.net/2027.42/132825.

Council of Science Editors:

Liu Y. 3D multispecies MHD studies of the interaction of the ionospheres of unmagnetized solar system bodies with the solar wind or magnetospheric plasma flows. [Doctoral Dissertation]. University of Michigan; 2000. Available from: http://hdl.handle.net/2027.42/132825

6. Najib, Dalal. The Interaction of Fast Flowing Plasma with Non-Magnetized Solar System Bodies: A New 3D Multi-fluid MHD Model of Mars and its Applications.

Degree: PhD, Atmospheric and Space Sciences, 2011, University of Michigan

 This dissertation presents numerical simulation results of the interaction of Mars ionosphere with the solar wind plasma using our new multi-fluid model, and the application… (more)

Subjects/Keywords: The Interaction of Fast Flowing Plasma With Non-Magnetized Solar System Bodies: a New 3D Multi-fluid MHD Model of Mars and Its Applications; Atmospheric, Oceanic and Space Sciences; Science

3D Multi-fluid MHD Model of Mars and its Applications by Dalal Najib Co-Chairs: Andrew F… …x28;1999) developed a 2-species, 3D, MHD model of Mars by considering solar wind protons and… …IV. Multi-fluid model of Mars’ interaction with the solar wind . 54 3.6 3.7 3.8 4.1 4.2… …gas densities at Mars (Chen et al., 1978). . . 5 1.4 Interaction of the solar… …Mars simulations showing the two-refinement levels… 

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APA (6th Edition):

Najib, D. (2011). The Interaction of Fast Flowing Plasma with Non-Magnetized Solar System Bodies: A New 3D Multi-fluid MHD Model of Mars and its Applications. (Doctoral Dissertation). University of Michigan. Retrieved from http://hdl.handle.net/2027.42/84512

Chicago Manual of Style (16th Edition):

Najib, Dalal. “The Interaction of Fast Flowing Plasma with Non-Magnetized Solar System Bodies: A New 3D Multi-fluid MHD Model of Mars and its Applications.” 2011. Doctoral Dissertation, University of Michigan. Accessed October 22, 2020. http://hdl.handle.net/2027.42/84512.

MLA Handbook (7th Edition):

Najib, Dalal. “The Interaction of Fast Flowing Plasma with Non-Magnetized Solar System Bodies: A New 3D Multi-fluid MHD Model of Mars and its Applications.” 2011. Web. 22 Oct 2020.

Vancouver:

Najib D. The Interaction of Fast Flowing Plasma with Non-Magnetized Solar System Bodies: A New 3D Multi-fluid MHD Model of Mars and its Applications. [Internet] [Doctoral dissertation]. University of Michigan; 2011. [cited 2020 Oct 22]. Available from: http://hdl.handle.net/2027.42/84512.

Council of Science Editors:

Najib D. The Interaction of Fast Flowing Plasma with Non-Magnetized Solar System Bodies: A New 3D Multi-fluid MHD Model of Mars and its Applications. [Doctoral Dissertation]. University of Michigan; 2011. Available from: http://hdl.handle.net/2027.42/84512

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