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  • Applied geophysics
  • LUNAR AND PLANETARY EXPLORATION
  • 1965-1969  (6)
  • 1935-1939  (7)
  • 1
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    In:  Geophysics, Milano, Gustav Fischer, vol. 1, no. 3, pp. 252-256, pp. L24306, (ISBN: 0534351875, 2nd edition)
    Publication Date: 1936
    Keywords: Applied geophysics ; Amplitude ; Seismics (controlled source seismology)
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  • 2
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    In:  Beiträge zur angewandten Geophysik, Milano, Gustav Fischer, vol. 6, no. 3, pp. 125-140, pp. L24306, (ISBN: 0534351875, 2nd edition)
    Publication Date: 1936
    Keywords: Applied geophysics ; Seismics (controlled source seismology)
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  • 3
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    In:  Geol. Soc. Am. Proc., Milano, Gustav Fischer, vol. 27, no. 6, pp. 240, pp. L24306, (ISBN: 0534351875, 2nd edition)
    Publication Date: 1937
    Keywords: Applied geophysics
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  • 4
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    In:  Trans., Am. Geophys. Union, Milano, Gustav Fischer, vol. 19, no. 6, pp. 156, pp. L24306, (ISBN: 0534351875, 2nd edition)
    Publication Date: 1938
    Keywords: Velocity analysis ; Applied geophysics ; NOISE ; Acoustics ; EOS
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  • 5
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    In:  Petroleum World, Annual Review, Milano, Gustav Fischer, vol. 34, no. 6, pp. 12-13, pp. L24306, (ISBN: 0534351875, 2nd edition)
    Publication Date: 1937
    Keywords: Applied geophysics
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  • 6
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    In:  Ergebnisse der kosmischen Physik, Milano, Gustav Fischer, vol. 4, no. 6, pp. 169-218, pp. L24306, (ISBN: 0534351875, 2nd edition)
    Publication Date: 1939
    Keywords: Applied geophysics ; Seismics (controlled source seismology)
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  • 7
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    Inst. f. Geophysik und Meteorologie
    In:  Geophysikalische Arbeiten sowie Mitteilungen aus Meteorologie und Astrophysik (GAMMA), TU Braunschweig, Inst. f. Geophysik und Meteorologie, vol. 10, no. 3, pp. 341-343, (ISBN 0 08 042822 3)
    Publication Date: 1968
    Keywords: Applied geophysics ; Electromagnetic methods/phenomena
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  • 8
    Publication Date: 2011-08-19
    Description: A global array of 20 radio observatories was used to measure the three-dimensional position and velocity of the two meteorological balloons that were injected into the equatorial region of the Venus atmosphere near Venus midnight by the VEGA spacecraft on June 11 and 15, 1985. Initial analysis of only radial velocities indicates that each balloon was blown westward about 11,500 kilometers (8,000 kilometers on the night side) by zonal winds with a mean speed of about 70 meters per second. Excursions of the data from a model of constant zonal velocity were generally less than 3 meters per second; however, a much larger variation was evident near the end of the flight of the second balloon. Consistent systematic trends in the residuals for both balloons indicate the possibility of a solar-fixed atmospheric feature. Rapid variations in balloon velocity were often detected within a single transmission (330 seconds); however, they may represent not only atmospheric motions but also self-induced aerodynamic motions of the balloon.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: Science (ISSN 0036-8075); 231; 1414-141
    Format: text
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  • 9
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    In:  CASI
    Publication Date: 2019-06-28
    Description: This project is based on designing a small lunar probe which will conduct research relating to future manned missions to the moon. The basic design calls for two experiments to be run. The first of these experiments is an enclosed environment section which will be exposed to solar radiation while on the moon. The purpose of this experiment is to determine the effect of radiation on an enclosed environment and how different shielding materials can be used to moderate this effect. The eight compartments will have the following covering materials: glass, polarized glass, plexiglass, polyurethane, and boron impregnated versions of the polyurethane and plexiglass. The enclosed atmosphere will be sampled by a mass spectrometer to determine elemental breakdown of its primary constituents. This is needed so that an accurate atmospheric processing system can be designed for a manned mission. The second experiment is a seismic study of the moon. A small penetrating probe will be shot into the lunar surface and data will be collected onboard the lander by an electronic seismograph which will store the data in the data storage unit for retrieval and transmission once every twenty-three hours. The project is designed to last ten years with possible extended life for an additional nine years at which point power requirements prevent proper functioning of the various systems.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: NASA-CR-197177 , NAS 1.26:197177
    Format: application/pdf
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  • 10
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    In:  CASI
    Publication Date: 2019-06-27
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: NASA-EP-39
    Format: application/pdf
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