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  • LUNAR AND PLANETARY EXPLORATION  (5)
  • Stress  (4)
  • Plate tectonics  (3)
  • Earthquake precursor: prediction research  (1)
  • Textbook of geophysics  (1)
  • FractureT
  • 1980-1984  (11)
Collection
Keywords
Publisher
Years
Year
  • 1
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    The role of an intracrustal asthenosphere on the behavior of major strike-slip faults (1984)
    In:  J. Geophys. Res., Taipei, EGS, vol. 89, no. 2, pp. 5801-5816, pp. 8039, (ISSN: 1340-4202)
    Details
    Publication Date: 1984
    Keywords: Fault zone ; Crustal deformation (cf. Earthquake precursor: deformation or strain) ; Plate tectonics ; Asthenosphere ; JGR
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    BIBLIOGRAPHY SEISMOLOGY
  • 2
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    Geodynamics: Application of Continuum Physics to Geological Problems (1982)
    John Wiley and Sons, 449 pp.
    In:  New York, John Wiley and Sons, 449 pp., vol. 271, no. ALEX(01)-FR-77-01, AFTAC Contract F08606-76-C-0025, pp. 329, (ISBN: 0-08-043649-8)
    Details
    Publication Date: 1982
    Keywords: Textbook of geophysics
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    BIBLIOGRAPHY SEISMOLOGY
  • 3
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    Stress accumulated mechanisms on strike-slip faults (1982)
    Vieweg
    In:  Professional Paper, Open-File Rept., Multidisciplinary Approach to Earthquake Prediction, Braunschweig, Vieweg, vol. 1, no. 16, pp. 471-485, (ISBN 0080419208)
    Details
    Publication Date: 1982
    Keywords: Review article ; Earthquake precursor: prediction research ; Stress ; Strike-slip ; Fault zone ; Modelling
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    BIBLIOGRAPHY SEISMOLOGY
  • 4
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    A steady state model for the distribution of stress and temperature on the San Andreas fault (1980)
    In:  J. Geophys. Res., Taipei, EGS, vol. 85, no. 2, pp. 6224-6230, pp. 8039, (ISSN: 1340-4202)
    Details
    Publication Date: 1980
    Keywords: Stress ; Geothermics ; Friction
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    BIBLIOGRAPHY SEISMOLOGY
  • 5
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    Mechanism of active and passive rifting (1983)
    In:  Tectonophys., Taipei, EGS, vol. 94, no. 2, pp. 39-50, pp. 8039, (ISSN: 1340-4202)
    Details
    Publication Date: 1983
    Keywords: Fault plane solution, focal mechanism ; Plate tectonics ; Structural geology ; Stress
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    BIBLIOGRAPHY SEISMOLOGY
  • 6
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    The state of stress at passive continental margins (1982)
    Am. Geophys. Union & Geol. Soc. Am.
    In:  Professional Paper, Open-File Rept., Dynamics of Passive Margins, Boulder, Am. Geophys. Union & Geol. Soc. Am., vol. 1, no. 16, pp. 141-146, (ISBN 0080419208)
    Details
    Publication Date: 1982
    Keywords: Stress ; Plate tectonics ; Tectonics
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    BIBLIOGRAPHY SEISMOLOGY
  • 7
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    Geophysical and geochemical constraints favoring the capture hypothesis (1984)
    In:  Other Sources
    Details
    Publication Date: 2019-01-25
    Description: The early fractionation of the Moon as a result of melting the outer layer of the Moon is discussed. This melting can be attributed to the accretional heating of the moon. Computations of the early thermal evolution of the Earth and Moon based on the assumption that these bodies accreted independently were carried out. The results are consistent with many observations. The concept of geochemical reservoirs was also applied to the Moon.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: Lunar Planetary Inst. Conf. on the Origin of the Moon; p 3
    Format: text
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    NASA TECHNICAL REPORTS
  • 8
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    Role of membrane stresses in the support of planetary topography (1981)
    In:  Other Sources
    Details
    Publication Date: 2019-06-28
    Description: The role of membrane stresses and bending stresses in supporting topographic loads on planetary elastic lithospheres is examined. A dimensionless parameter is introduced in order to determine the ability of a spherical shell to support loads through membrane stresses. It is determined that when this parameter is large, membrane stresses can fully support topographic loads with flexure, and when it is small the influence of the membrane stresses can be neglected. Equations governing the behavior of a spherical shell are solved for a topographic load expressed in terms of spherical harmonics, and spherical harmonic expansions of the measured gravity and topography for Mars and the moon are compared with the theory. It is concluded that membrane stresses play an important role in the support of topographic loads on the moon and Mars. The correlation of observed gravitational potential anomalies with the topography on Mars is explained by membrane stresses in the elastic lithosphere.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: Journal of Geophysical Research; 86; May 10
    Format: text
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  • 9
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    Support of topographic and other loads on the moon and on the terrestrial planets (1982)
    In:  Other Sources
    Details
    Publication Date: 2019-07-13
    Description: The existence of mascons on the moon indicates that the lunar elastic lithosphere can support substantial loads for about three billion years. Lunar topography also appears to be uncompensated. Observations of gravity on Mars show that the Tharsis uplift is only partially compensated. A number of authors have attributed this support to lithospheric flexure. In this paper it is shown that membrane stresses play an important role in the support of loads on the moon, Mars, and Mercury. For loads that have been expressed in terms of spherical harmonics analytical expressions for the degree of compensation are obtained as a function of the degree of the load. The results are compared with the observed dependence of the ratio of gravitational potential to topography on degree. It is also concluded that membrane stresses can support a significant ellipticity for a tidally despun planetary body.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: Lunar and Planetary Science Conference; Mar 16, 1981 - Mar 20, 1981; Houston, TX
    Format: text
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    NASA TECHNICAL REPORTS
  • 10
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    Thermal stresses in planetary elastic lithospheres (1983)
    In:  Other Sources
    Details
    Publication Date: 2019-07-13
    Description: The role of thermal stresses in the tectonics of the moon is reexamined in this paper. A model is used that considers a spherical elastic shell overlying a fluid core. It is shown that the thermal stresses generated by temperature changes within the shell usually dominate over the thermal contraction or expansion of the core. During the entire evolution of the moon the cooling of the lithosphere is likely to have dominated the cooling of the interior and the result would be tensional lithospheric thermal stresses. However, during the recent evolution of the moon the change in the near surface thermal stresses is compressional. It is argued that the surface compressional features on Mercury are not due to the thermal contraction of the interior
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: Lunar and Planetary Science Conference; Mar 15, 1982 - Mar 19, 1982; Houston, TX
    Format: text
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