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  • Lunar and Planetary Science and Exploration  (27)
  • Communications and Radar  (1)
  • PACS. 47.54.+r Pattern selection; pattern formation – 61.30.-v Liquid crystals – 47.20.Ky Nonlinearity (including bifurcation theory)  (1)
  • cables  (1)
  • nonlinear dynamics  (1)
  • 2000-2004  (31)
Collection
Keywords
Publisher
Years
Year
  • 1
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    Mars Odyssey Science: The First Year and Beyond (2003)
    In:  CASI
    Details
    Publication Date: 2017-10-02
    Description: The 2001 Mars Odyssey orbital science mission officially began in late February, 2002. The spacecraft carries three science instrument packages: the Gamma Ray Spectrometer suite (GRS), the Thermal Emission Imaging System (THEMIS), and the Martian Radiation Environment Experiment (MARIE). The GRS suite of three instruments includes the Gamma Sensor Subsystem (GSS), the Neutron Spectrometer (NS) and the High Energy Neutron Detector (HEND). THEMIS consists of two cameras sharing a single set of telescopic optics: a 5-band visible imager and a 10-band thermal infrared imager. Spacecraft and instrument performance have been nominal to this point in the science mission.
    Keywords: Lunar and Planetary Science and Exploration
    Type: Lunar and Planetary Science XXXIV; LPI-Contrib-1156
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    NASA TECHNICAL REPORTS
  • 2
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    Small Crater Populations on Mars: Studies of MOC Images (2000)
    In:  Other Sources
    Details
    Publication Date: 2017-10-02
    Description: Populations of small martian craters can now be studied using MOC images. The smallest craters record aspects of the crater production and resurfacing history that could not be observed previously. Examples from a number of terrains are shown.
    Keywords: Lunar and Planetary Science and Exploration
    Type: Lunar and Planetary Science XXXI; LPI-Contrib-1000
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  • 3
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    Topographic and Roughness Characteristics of the Vastitas Borealis Formation on Mars Described by Fractal Statistics (2000)
    In:  Other Sources
    Details
    Publication Date: 2017-10-02
    Description: The surface roughness of the Vastitas Borealis Formation on Mars was analyzed with fractal statistics. Root mean square slopes and fractal dimensions were calculated for 74 topographic profiles. Results have implications for radar scattering models.
    Keywords: Lunar and Planetary Science and Exploration
    Type: Lunar and Planetary Science XXXI; LPI-Contrib-1000
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  • 4
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    The Tellus Region of Venus: Processes in the Formation and Modification of Tessera Terrain (2000)
    In:  Other Sources
    Details
    Publication Date: 2017-10-02
    Description: A study using structural and stereo analysis of early and late stage geologic events within the Tellus region is performed. Evidence is presented that suggests that some tessera material may consist of layered volcanics.
    Keywords: Lunar and Planetary Science and Exploration
    Type: Lunar and Planetary Science XXXI; LPI-Contrib-1000
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  • 5
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    Orbital Synthetic Aperture Radar (SAR) for Mars Post Sample Return Exploration (2000)
    In:  Other Sources
    Details
    Publication Date: 2017-10-02
    Description: A Mars orbital radar mission would use two frequencies to map the planet at 50 m resolution, penetrating 5-10 m. Some areas will be imaged at 5-m resolution. A 50-m resolution topographic map will be acquired, and surface changes detected.
    Keywords: Lunar and Planetary Science and Exploration
    Type: Lunar and Planetary Science XXXI; LPI-Contrib-1000
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  • 6
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    2001 Mars Odyssey Project report (2002)
    In:  Other Sources
    Details
    Publication Date: 2018-06-11
    Description: The Mars Odyssey orbiter was launched on April 7, 2001, and arrived at Mars on October 24, 2001. The orbiter carries scientific instruments that will determine surface elemental composition, mineralogy and morphology, and measure the Mars radiation environment from orbit. In addition, the orbiter will serve as a data relay for future surface missions. This paper will present an overview of the Odyssey project, including the key elements of the spacecraft design, mission design and navigation, mission operations, and the science approach. The project's risk management process will be described. Initial findings of the science team will be summarized.
    Keywords: Lunar and Planetary Science and Exploration
    Type: 53rd International Astronautical Congress; Houston, TX; United States
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  • 7
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    Impact Crater Abundance of the Martian South Polar Layered Deposits from THEMIS Visible Imaging (2004)
    In:  CASI
    Details
    Publication Date: 2018-06-11
    Description: The polar layered deposits (PLD) of Mars have attracted considerable attention since their identification in Mariner 9 images, largely due to the possibility that these finely layered, volatile-rich deposits hold a record of recent eras in Martian climate history. The PLD have been a target of imaging and other sensors in the last several decades, but only recently has it been possible to obtain a moderately high resolution image map, using the visible sensor on 2001 Mars Odyssey's Thermal Emission Imaging System (THEMIS). THEMIS has acquired a 36 meter/pixel contiguous single-band visible image data set of the south polar layered deposits (SPLD), during the southern spring in 2003. The data will undoubtedly be applied to many problems in Mars polar studies. We use these images to further characterize the population of impact craters on the SPLD, and the implications of the observed population for the age and evolution of the SPLD.
    Keywords: Lunar and Planetary Science and Exploration
    Type: Lunar and Planetary Science XXXV: Mars Polar Science and Exploration; LPI-Contrib-1197
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  • 8
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    South Polar Cryptic Region Revisited: THEMIS Observations (2003)
    In:  CASI
    Details
    Publication Date: 2017-10-02
    Description: The early part of the Mars Global Surveyor mission provided good TES coverage of the Mars south polar region. These data allow mapping of the polar cap recession, surface and atmospheric temperatures, and albedo features found within the seasonal cap itself over Ls = 180 - 270 deg. During this period, the seasonal south polar cap retreated continuously and asymmetrically around the geographic pole, similar to the observations of Viking in 1976- 1977 [3]. A prominent albedo feature on the seasonal cap is a region that appears almost as dark as bare ground, yet remains cold. We refer to this region, generally located between latitudes 85 deg. S and 75 deg. S and longitudes 150 deg. W and 310 deg. W, as the Cryptic region.
    Keywords: Lunar and Planetary Science and Exploration
    Type: Third International Conference on Mars Polar Science and Exploration; LPI-Contrib-1184
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  • 9
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    The Mars Express/NASA Project at JPL (2003)
    In:  CASI
    Details
    Publication Date: 2017-10-02
    Description: ESA's Mars Express Mission is an international collaboration between the European Space Agency (ESA) and the European space agencies with the National Aeronautics and Space Administration (NASA) as a junior partner. The primary objective of the mission is to conduct a search for potential hydrologic resources from orbit and on the surface of Mars. Launch will be from Baikonur, Kazakhstan in late May 2003; arrival at Mars will be in late December 2003.
    Keywords: Lunar and Planetary Science and Exploration
    Type: Lunar and Planetary Science XXXIV; LPI-Contrib-1156
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  • 10
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    Probing the Subsurface of the Martian Polar Regions with MARSIS on Mars Express (2003)
    In:  CASI
    Details
    Publication Date: 2017-10-02
    Description: The European Space Agency (ESA) is currently conducting a mission to Mars known as Mars Express. The orbiter carries an instrument called the Mars Advanced Radar for Subsurface and Ionospheric Sounding (MARSIS). The MARSIS experiment is a joint project between NASA and the Italian Space Agency, and is being carried out by the University of Rome, the Jet Propulsion Laboratory, Alenia Aerospazio, and the University of Iowa. This paper describes the science objectives of the experiment, the instrument characteristics, and applications of the MARSIS investigation to studies of the martian polar regions.
    Keywords: Lunar and Planetary Science and Exploration
    Type: Third International Conference on Mars Polar Science and Exploration; LPI-Contrib-1184
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