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  • 1
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    Contributions of Space Geodesy to Geodynamics: Earth Dynamics (1993)
    Am. Geophys. Un.
    In:  Malden, MA, Am. Geophys. Un., vol. 24, no. Publ. No. 12, pp. 95-104, (ISBN: 0-08-043930-6)
    Details
    Publication Date: 1993
    Keywords: Geodesy ; GeodesyY ; Plate tectonics ; Textbook of geophysics ; Textbook of geodesy
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    BIBLIOGRAPHY SEISMOLOGY
  • 2
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    Nonlinear Dynamics and Predictability of Geophysical Phenomena (1994)
    American Geophysical Union
    In:  Washington, 107 pp., American Geophysical Union, vol. IUGG Volume 18, no. 85, pp. 799-804, (ISBN 3-540-23219-2)
    Details
    Publication Date: 1994
    Keywords: Non-linear effects ; FractureT ; Chaotic behaviour ; SOC ; criticality ; Textbook of geophysics ; Dynamic ; Earthquake precursor: prediction research
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    BIBLIOGRAPHY SEISMOLOGY
  • 3
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    Contributions of Space Geodesy to Geodynamics: Crustal Dynamics (1993)
    Am. Geophys. Un.
    In:  Malden, MA, Am. Geophys. Un., vol. 23, no. Publ. No. 12, pp. 95-104, (ISBN: 0-08-043930-6)
    Details
    Publication Date: 1993
    Keywords: Geodesy ; GeodesyY ; Plate tectonics ; Textbook of geophysics ; Textbook of geodesy
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    BIBLIOGRAPHY SEISMOLOGY
  • 4
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    Contributions of Space Geodesy to Geodynamics: Technology (1993)
    Am. Geophys. Un.
    In:  Malden, MA, Am. Geophys. Un., vol. 25, no. Publ. No. 12, pp. 95-104, (ISBN: 0-08-043930-6)
    Details
    Publication Date: 1993
    Keywords: Geodesy ; Handbook of geophysics ; Handbook of geodesy ; Instruments
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    BIBLIOGRAPHY SEISMOLOGY
  • 5
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    Evidence for chaotic fault interactions in the seismicity of the San Andreas fault and Nankai trough (1990)
    In:  Other Sources
    Details
    Publication Date: 2011-08-19
    Description: The dynamical behavior introduced by fault interactions is examined here using a simple spring-loaded, slider-block model with velocity-weakening friction. The model consists of two slider blocks coupled to each other and to a constant-velocity driver by elastic springs. For an asymmetric system in which the frictional forces on the two blocks are not equal, the solutions exhibit chaotic behavior. The system's behavior over a range of parameter values seems to be generally analogous to that of weakly coupled segments of an active fault. Similarities between the model simulations and observed patterns of seismicity on the south central San Andreas fault in California and in the Nankai trough along the coast of southwestern Japan.
    Keywords: GEOPHYSICS
    Type: Nature (ISSN 0028-0836); 348; 234-236
    Format: text
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    NASA TECHNICAL REPORTS
  • 6
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    Coupled evolution of the atmospheres and interiors of planets and satellites (1989)
    In:  Other Sources
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    Publication Date: 2011-08-19
    Description: The evolution of a planetary atmosphere can be powerfully influenced by the planetary interior's function as both a source and a sink of atmospheric constituents; the interior can in turn be strongly influenced by the atmosphere because the mechanism of interior heat loss depends on a volatile content for which the atmosphere can serve both as sink and source. The dependence of mantle rheology on volatile content could furnish a feedback mechanism tending to keep regassing/degassing in balance, thereby maintaining a relatively constant atmospheric mass. Consideration of the abundances of radiogenic and nonradiogenic noble gases in the earth's atmosphere, and of the fluxes of these gases from the mantle, support a large degassing event early on, followed by a decrease in degassing efficiency with time and relatively inefficient outgassing over most of geologic time.
    Keywords: ASTROPHYSICS
    Format: text
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    NASA TECHNICAL REPORTS
  • 7
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    The spatial distribution of coronae on Venus (1992)
    In:  CASI
    Details
    Publication Date: 2013-08-31
    Description: Coronae on Venus are large, generally circular surface features that have distinctive tectonic, volcanic, and topographic expressions. They range in diameter from less than 200 km to at least 1000 km. Data from the Magellan spacecraft have now allowed complete global mapping of the spatial distribution of coronae on the planet. Unlike impact craters, which show a random (i.e., Poisson) spatial distribution, the distribution of coronae appears to be nonrandom. We investigate the distribution here in detail, and explore its implications in terms of mantle convection and surface modification processes.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: Lunar and Planetary Inst., Papers Presented to the International Colloquium on Venus; p 119-120
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    NASA TECHNICAL REPORTS
  • 8
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    Spectral study of Venus global topography and geoid from Magellan and PVO data (1993)
    In:  CASI
    Details
    Publication Date: 2013-08-31
    Description: An analysis of newly available global harmonic models for topography and geoid on Venus was conducted. It was found that the power spectral density for Venus topography has a power law dependence on wave-number characteristic of Brown Noise, similar to what is found for the Earth. However, the Venus topography spectrum presents a rollover at lower degree (l = 3) than is observed for the Earth spectrum and has smaller amplitudes than that of the Earth's. The Venus geoid also obeys a power law relationship, at least for small values of l, but with a smaller slope and more power (for l greater than 3) than the Earth geoid.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: Lunar and Planetary Inst., Twenty-Fourth Lunar and Planetary Science Conference. Part 2: G-M; p 831-832
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    NASA TECHNICAL REPORTS
  • 9
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    Properties of the lithosphere and asthenosphere deduced from geoid observations (1985)
    In:  CASI
    Details
    Publication Date: 2016-06-07
    Description: Data from the GEOS-3 and SEASAT Satellites provided a very accurate geoid map over the oceans. Broad bathymetric features in the oceans such as oceanic swells and plateaus are fully compensated. It is shown that the geoid anomalies due to the density structures of the lithosphere are proportional to the first moment of the density distribution. The deepening of the ocean basins is attributed to thermal isostasy. The thickness of the oceanic lithosphere increases with age due to the loss of heat to the sea floor. Bathymetry and the geoid provide constraints on the extent of this heat loss. Offsets in the geoid across major fracture zones can also be used to constrain this problem. Geoid bathymetry correlations show that the Hawaiian and Bermuda swells and the Cape Verde Rise are probably due to lithospheric thinning.
    Keywords: GEOPHYSICS
    Type: NASA, Washington Geopotential Res. Mission (GRM); p 44-45
    Format: application/pdf
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    NASA TECHNICAL REPORTS
  • 10
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    Implications of Convection in the Moon and the Terrestrial Planets (1985)
    In:  CASI
    Details
    Publication Date: 2014-10-08
    Description: The early evolution of the Moon and its implications for the early evolution of the Earth was studied. The study is divided into two parts: (1) studies of core formation. Cosmochemical studies strongly favor a near-homogeneous accretion of the Earth. It is shown that core segregation probably occurred within the first 10,000 years of Earth history. It is found that dissipative heating may be a viable mechanism for core segregation if sufficiently large bodies of liquid iron can form; (2) early thermal evolution of the Earth and Moon. The energy associated with the accretion of the Earth and the segregation of the core is more than sufficient to melt the entire Earth. The increase in the mantle liquidus with depth (pressure) is the dominant effect influencing heat transfer through the magma ocean. It is found that a magma ocean with a depth of 100 km would have existed as the Earth accreted. It is concluded that this magma ocean zone refined the earth resulting in the simultaneous formation of the core and the atmosphere during accretion. The resulting mantle was a well-mixed solid with a near pyrolite composition.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: NASA, Washington Repts. of Planetary Geol. and Geophys. Program, 1984; p 211
    Format: text
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