Investigation on Computing Method of Martian Dust Fluid Based on the Energy Dissipation Method
International Journal of Aerospace Engineering, 2020 In this paper, an initiative Martian dust fluid simulating research based on the energy dissipation method was developed to simulate the deposition process of Martian dust fluid which was caused by surface adhesion between particles and Martian rovers ...
Tianxiang Ding +6 more
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The MEDUSA and MicroMED Experiments for the ExoMars Space Programme to Perform In Situ Analysis of Martian Dust [PDF]
, 2011 This thesis describes the work for the PhD in Aerospace, Naval and Total Quality Management of the University of Naples “Federico II” from 2008 to 2011. The work was mostly performed at National Institute of Astrophysics (INAF) - Astronomical Observatory
Ventura, Sergio
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Microbial growth in actual martian regolith in the form of Mars meteorite EETA79001
Communications Earth & Environment, 2023 Studies to understand the growth of organisms on Mars are hampered by the use of simulants to duplicate martian mineralogy and chemistry. Even though such materials are improving, no terrestrial simulant can replace a real martian sample.
Neveda Naz +3 more
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ESGS: A 3D Reconstruction Method for the Martian Surface Based on Optical Remote Sensing Images
Remote SensingMars exploration is an advanced field of global deep space exploration. Accurate three-dimensional reconstruction of the Martian surface topography is very important for autonomous navigation, scientific target recognition, and operation planning.
Qinghe Guan +4 more
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Shear-Induced ringwoodite formation in the Martian shergottite Dar al Gani 670 [PDF]
, 2013 Shock-produced melt veins in the Martian shergottite Dar al Gani 670 crosscut large olivine crystals. The upper part of one of these crystals appears to be sheared off and displaced along the shock vein.
Fritz, Jörg +3 more
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A GRADIENT-REGION CONSTRAINED LEVEL SET METHOD FOR AUTONOMOUS ROCK DETECTION FROM MARS ROVER IMAGE [PDF]
The International Archives of the Photogrammetry, Remote Sensing and Spatial Information Sciences, 2019 Rocks are one of the major Martian surface features and yield significant information about the relevant geology process and the life exploration. However, autonomous Martian rock detection is still a challenging task due to the appearance similar to the
J. Yang, Z. Kang
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Frontiers in Astronomy and Space Sciences, 2022 The detailed Martian Energetic Radiation Environment Model (dMEREM) is a Geant4 based model developed for the European Space Agency, which enables to predict the radiation environment expected at different locations on the Martian orbit, atmosphere and ...
Patrícia Gonçalves +3 more
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The Astrophysical Journal, 1967 Inconsistency in Martian surface pressure as calculated by Gray explained, using Leighton and Murray ...
Ronald A. Schorn, Louise D. Gray
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I. Variability of the Outgoing Thermal IR Spectra and Its Application in GCM Validation. II. The Detection of Cloud/Aerosol in the Outgoing Thermal IR Spectra [PDF]
, 2004 The theme of this thesis is studying the outgoing thermal IR spectra of Earth and Mars. It is divided into two parts: the first part (Chapters 1-4) is focused on the variability seen in the outgoing thermal IR spectra and its application in validating ...
Huang, Xianglei
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Rootless cones on Mars indicating the presence of shallow equatorial ground ice in recent times [PDF]
, 2001 High resolution Mars Orbiter Camera (MOC) images have revealed the existence of clusters of small cones in the Cerberus plains, Marte Valles, and Amazonis Planitia, Mars.
McEwen, A. S. +3 more
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