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  • About
  • The Global ETD Search service is a free service for researchers to find electronic theses and dissertations. This service is provided by the Networked Digital Library of Theses and Dissertations.
    Our metadata is collected from universities around the world. If you manage a university/consortium/country archive and want to be added, details can be found on the NDLTD website.
41

Geophysical investigations of the crustal structure and evolution of Mars

Leftwich, 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).
42

Influence of mechanical stratigraphy and strain on the displacement-length scaling of normal faults on Mars

Polit, 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.
43

Remote sensing of shallow-marine impact craters on Mars

De Villiers, Germari Marzen, Luke J. King, David T. January 2007 (has links)
Thesis--Auburn University, 2007. / Abstract. Vita. Includes bibliographic references (p.133-142)
44

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).
45

VOLCANO-ICE INTERACTIONS ON THE EARTH AND MARS

Allen, Carlton January 1979 (has links)
No description available.
46

The Influence of Dust Devils on Martian Water Vapour Transport

Chen, Kuan-Chih Unknown Date
No description available.
47

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.
48

Thermal analysis and thermal control system requirements for a solar sail Mars mission

Tiedemann, Maik 16 February 2010 (has links)
Master of Engineering
49

Mechanical design of a Stewart platform-based crawling vehicle

Mele, 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
50

Baroclinic eddies in the Martian atmosphere : a general circulation model study

Matheson, 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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