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Geophysical investigations of the crustal structure and evolution of MarsLeftwich, Timothy E., January 2006 (has links)
Thesis (Ph. D.)--Ohio State University, 2006. / Title from first page of PDF file. Includes bibliographical references (p. 191-205).
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Influence of mechanical stratigraphy and strain on the displacement-length scaling of normal faults on MarsPolit, Anjani T. January 2005 (has links)
Thesis (M.S.)--University of Nevada, Reno, 2005. / "December, 2005." Includes bibliographical references (leaves 43-48). Online version available on the World Wide Web.
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Remote sensing of shallow-marine impact craters on MarsDe Villiers, Germari Marzen, Luke J. King, David T. January 2007 (has links)
Thesis--Auburn University, 2007. / Abstract. Vita. Includes bibliographic references (p.133-142)
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Fluid and particle simulations of the interaction of the solar wind with magnetic anomalies on the surface of the Moon and Mars /Harnett, Erika Megan. January 2003 (has links)
Thesis (Ph. D.)--University of Washington, 2003. / Vita. Includes bibliographical references (p. 133-140).
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VOLCANO-ICE INTERACTIONS ON THE EARTH AND MARSAllen, Carlton January 1979 (has links)
No description available.
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The Influence of Dust Devils on Martian Water Vapour TransportChen, Kuan-Chih Unknown Date
No description available.
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Properties of water ice clouds over major Martian volcanoes observed by MOC /Benson, Jennifer L. January 2006 (has links)
Dissertation (Ph.D.)--University of Toledo, 2006. / Typescript. "Submitted as partial fulfillment of the requirements for the Doctor of Philosophy Degree in Physics." Bibliography: leaves 103-113.
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Thermal analysis and thermal control system requirements for a solar sail Mars missionTiedemann, Maik 16 February 2010 (has links)
Master of Engineering
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Mechanical design of a Stewart platform-based crawling vehicleMele, Paul A. 17 March 2010 (has links)
It is well established that a vast majority of the Earth's surface is inaccessible to conventional vehicles. Furthernore, projects alluding to the exploration of Mar's conclude that its surface is too rough for conventional wheeled vehicles. Man and cursorial animals, however, are capable of traversing virtually all types of terrain. These reasons, among others, have focused almost all development on walking vehicles having fixed torsos and articulated legs which emulate the locomotion of man and animals. Insects such as the caterpillar move with fixed legs and an articulated torso. They too can traverse rough terrain but do so with greater stability than bipeds or quadrupeds.
This thesis presents a design for a caterpillar-like crawling vehicle. An overview of the effort to develop walking vehicles is included to show the depth of interest in developing a vehicle capable of traversing rough terrain. A general overview of crawling vehicle objectives and the control problems hampering the realization of a crawling vehicle are then described. Finally, this thesis provides a detailed mechanical design with the kinematic and mechanical considerations governing that design. / Master of Science
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Baroclinic eddies in the Martian atmosphere : a general circulation model studyMatheson, Mark 14 November 2000 (has links)
A variety of general circulation model experiments are performed to
investigate the influence of seasonality and topography on the strength of baroclinic
eddies in the Martian atmosphere. Three different models are used: a full physics
model, a simplified physics model, and a zonally symmetric simplified physics
model. All three models are sigma coordinate, finite difference global atmospheric
circulation models that have been adapted to the Martian regime. The full physics
model has previously been tested extensively by researchers at the NASA Ames
Research Center. The simplified physics model replaces many of the atmospheric
physics routines with simple parameterizations; most importantly, the radiation
code is replaced by Newtonian cooling. A Newtonian cooling code with a radiative
time constant that varies in height and latitude produces superior results to one with
a radiative time constant that is the same everywhere throughout the atmosphere.
It is found that baroclinic eddy activity is extremely sensitive to the mean
meridional temperature gradient in the simplified model. A power law fit gives an
exponent of approximately six. The baroclinic eddy activity is also sensitive to the
maximum growth rate in the Eady model of baroclinic activity. This is due to the
close connection between the meridional temperature gradient and the maximum
growth rate. Baroclinic adjustment theory, which predicts how baroclinic eddies
will react to changes in the mean circulation, does not appear to be valid in the
Martian regime, according to the simplified model. This finding may be related to
the differences in the relative strengths of the baroclinic eddies and the mean
circulation on Earth and Mars.
The simplified model indicates that seasonality is more important than
topography in creating stronger eddies in the northern hemisphere winter than in
the southern hemisphere winter. However, the effects of topography in the
simplified model may not be adequately matching the effects of topography in the
full physics model, particularly in the southern hemisphere. / Graduation date: 2001
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