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  • FID-GEO-DE-7
  • Geoelektrik
  • Lunar and Planetary Science and Exploration
  • Magnetismus
  • People
  • 2015-2019
  • 1990-1994  (6)
  • 1990  (6)
Collection
Years
  • 2015-2019
  • 1990-1994  (6)
Year
  • 1
    Publication Date: 2011-08-24
    Description: No abstract available
    Keywords: Lunar and Planetary Science and Exploration
    Type: Scientific American (ISSN 0036-8733); Volume 263; 4; 78-84
    Format: text
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  • 2
    Publication Date: 2011-08-24
    Description: Selective thermal modulation (STM) is a technique which produces a concentration-dependent pulse by selectively modulating a sample in a gas stream. Several types of modulation techniques, both chemical and physical, using adsorption, decomposition, and catalytic and mechanical methods have been developed for use with multiplex gas chromatography. Two of these applications involve selective modulation of the components present in the sample gas stream. The selective modulation of the concentration of specific sample molecules or classes of molecules provides additional analytical selectivity which can lead to selective detection. For some specific applications, the column may even be eliminated. Chemical modulation by absorption of a substance from the sample stream by a stationary phase will also produce a change in the signal intensity. Removal of a substance from the sample stream results in a signal containing a vacancy peak. In the work reported here, a selective thermal modulation technique has been developed as a method for determination of water vapor for possible use in Mars' atmosphere.
    Keywords: Lunar and Planetary Science and Exploration
    Type: Journal of high resolution chromatography : HRC (ISSN 0935-6304); Volume 13; 835-7
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  • 3
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    In:  CASI
    Publication Date: 2018-06-12
    Description: The Center for Space Construction is a major element of the University of Colorado's initiative to upgrade space-related research and education on its Boulder campus. With the support of NASA's University Space Engineering Research Centers Program, the Center provides a mechanism for interdisciplinary and system-level space engineering research and training. This document contains the conference proceedings for the Center's second annual symposium. The primary topic is the construction of lunar bases.
    Keywords: Lunar and Planetary Science and Exploration
    Type: NASA-CR-193010 , HQ-E-DAA-TN30899 , Colorado Univ. Annual Symposium; 17-19 Oct. 1990; Boulder, CO; United States
    Format: application/pdf
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  • 4
    Publication Date: 2019-07-12
    Description: A manufacturing plant and process for production of oxygen on the moon uses lunar minerals as feed and a minimum of earth-imported, process materials. Lunar feed stocks are hydrogen-reducible minerals, ilmenite and lunar agglutinates occurring in numerous, explored locations mixed with other minerals in the pulverized surface layer of lunar soil known as regolith. Ilmenite (FeTiO.sub.3) and agglutinates contain ferrous (Fe.sup.+2) iron reducible by hydrogen to yield H.sub.2 O and metallic Fe at about 700.degree.-1,200.degree. C. The H.sub.2 O is electrolyzed in gas phase to yield H.sub.2 for recycle and O.sub.2 for storage and use. Hydrogen losses to lunar vacuum are minimized, with no net hydrogen (or any other earth-derived reagent) consumption except for small leaks. Feed minerals are surface-mined by front shovels and transported in trucks to the processing area. The machines are manned or robotic. Ilmenite and agglutinates occur mixed with silicate minerals which are not hydrogen-reducible at 700.degree.-1,200.degree. C. and consequently are separated and concentrated before feeding to the oxygen generation process. Solids rejected from the separation step and reduced solids from the oxygen process are returned to the mine area. The plant is powered by nuclear or solar power generators. Vapor-phase water electrolysis, a staged, countercurrent, fluidized bed reduction reactor and a radio-frequency-driven ceramic gas heater are used to improve thermal efficiency.
    Keywords: Lunar and Planetary Science and Exploration
    Format: application/pdf
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  • 5
    Publication Date: 2019-08-13
    Description: Dust elevated in local or global dust storms on the Martian surface could settle on photovoltaic (PV) surfaces and seriously hamper their performance. Using a recently developed technique to apply a uniform dust layer, PV surface materials were subjected to simulated Martian winds in an attempt to determine whether natural Aeolian processes on Mars would sweep off the settled dust. Three different types of dust were used; an optical polishing powder, basaltic "trap rock", and iron (III) oxide crystals. The effects of wind velocity, angle of attack, height above the Martian surface, and surface coating material were investigated. It was found that arrays mounted with an angle of attack approaching 45 degrees show the most efficient clearing. Although the angular dependence is not sharp, horizontally mounted arrays required significantly higher wind velocities to clear off the dust. From this test it appears that the arrays may be erected quite near the ground, but previous studies have suggested that saltation effects can be expected to cause such arrays to be covered by soil if they are set up less than about a meter from the ground. Particle size effects appear to dominate over surface chemistry in these experiments, but additional tests are required to confirm this. Providing that the surface chemistry of Martian dusts is not drastically different from simulated dust and that gravity differences have only minor effects, the materials used for protective coatings for photovoltaic arrays may be optimized for other considerations such as transparency, and chemical or abrasion resistance. The static threshold velocity is low enough that there are regions on Mars which experience winds strong enough to clear off a photovoltaic array if it is properly oriented. Turbulence fences proved to be an ineffective strategy to keep dust cleared from the photovoltaic surfaces.
    Keywords: Lunar and Planetary Science and Exploration
    Type: E-5600 , Space Simulation Conference; Nov 05, 1990 - Nov 08, 1990; Albuquerque, NM; United States
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  • 6
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    In:  Other Sources
    Publication Date: 2019-07-10
    Description: Live footage shows several speakers participating in the Magellan Press Conference. Speakers include the Director of Solar System Exploration Division West Huntress, Magellan Project Manager Tony Spear, Spacecraft Team Chief W. Ledbetter, Radar System Chief Engineer T. Johnson, and Magellan Project Manager from Hughes Aircraft Co. T. McCarthy. The speakers discuss the Venus Orbiting Insertion (VOI), radar system components, spacecraft development, mission objectives, and the flight plans. This is tape 1 of 2; tape 2 has a report number NONP-NASA-VT-2000036566.
    Keywords: Lunar and Planetary Science and Exploration
    Type: NONP-NASA-VT-2000036552
    Format: text
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