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  • 1980-1984  (4)
  • 1984  (4)
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  • 1980-1984  (4)
Year
  • 1984  (4)
Subjects(RVK)
  • 1
    Online Resource
    Online Resource
    Elsevier BV ; 1984
    In:  Earth and Planetary Science Letters Vol. 70, No. 2 ( 1984-10), p. 395-406
    In: Earth and Planetary Science Letters, Elsevier BV, Vol. 70, No. 2 ( 1984-10), p. 395-406
    Type of Medium: Online Resource
    ISSN: 0012-821X
    RVK:
    Language: English
    Publisher: Elsevier BV
    Publication Date: 1984
    detail.hit.zdb_id: 300203-2
    detail.hit.zdb_id: 1466659-5
    SSG: 16,13
    Location Call Number Limitation Availability
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  • 2
    Online Resource
    Online Resource
    Springer Science and Business Media LLC ; 1984
    In:  Nature Vol. 310, No. 5976 ( 1984-8), p. 401-403
    In: Nature, Springer Science and Business Media LLC, Vol. 310, No. 5976 ( 1984-8), p. 401-403
    Type of Medium: Online Resource
    ISSN: 0028-0836 , 1476-4687
    RVK:
    RVK:
    RVK:
    Language: English
    Publisher: Springer Science and Business Media LLC
    Publication Date: 1984
    detail.hit.zdb_id: 120714-3
    detail.hit.zdb_id: 1413423-8
    SSG: 11
    Location Call Number Limitation Availability
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  • 3
    Online Resource
    Online Resource
    Cambridge University Press (CUP) ; 1984
    In:  International Astronomical Union Colloquium Vol. 75 ( 1984), p. 675-676
    In: International Astronomical Union Colloquium, Cambridge University Press (CUP), Vol. 75 ( 1984), p. 675-676
    Abstract: A three-dimensional numerical model has been developed with the goal of studying limited dynamical problems relevant to the latest stage of planet growth in the accretion theory. A small number of large protoplanets (~ moon-size) of different masses, moving around the Sun, are considered. The dynamical evolution and growth of the population is studied under mutual gravitational perturbations, accretion and collisional fragmentation processes. Gravitational encounters are treated exactly by numerical integration of the N-body problem. Outcomes of collisional fragmentation are modeled according to the results of Greenberg et al. (1978).
    Type of Medium: Online Resource
    ISSN: 0252-9211
    Language: English
    Publisher: Cambridge University Press (CUP)
    Publication Date: 1984
    Location Call Number Limitation Availability
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  • 4
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 1984
    In:  Journal of Geophysical Research: Solid Earth Vol. 89, No. B13 ( 1984-12-10), p. 11171-11179
    In: Journal of Geophysical Research: Solid Earth, American Geophysical Union (AGU), Vol. 89, No. B13 ( 1984-12-10), p. 11171-11179
    Abstract: Geoid heights over the Louisville Ridge seamount chain, deduced from the Seasat satellite altimeter data, have been analyzed and interpreted. Two uncharted seamounts belonging to the chain have been detected. The elastic thickness of the oceanic lithosphere has been determined along the chain. This was done rigorously using the three‐dimensional geoid and bathymetry maps and was also computed approximately using spectral methods on geoid and bathymetry profiles. A slightly increasing elastic thickness from the southeast to the northwest, in the range 15.5–22.5 km has been estimated.
    Type of Medium: Online Resource
    ISSN: 0148-0227
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 1984
    detail.hit.zdb_id: 2033040-6
    detail.hit.zdb_id: 3094104-0
    detail.hit.zdb_id: 2130824-X
    detail.hit.zdb_id: 2016813-5
    detail.hit.zdb_id: 2016810-X
    detail.hit.zdb_id: 2403298-0
    detail.hit.zdb_id: 2016800-7
    detail.hit.zdb_id: 161666-3
    detail.hit.zdb_id: 161667-5
    detail.hit.zdb_id: 2969341-X
    detail.hit.zdb_id: 161665-1
    detail.hit.zdb_id: 3094268-8
    detail.hit.zdb_id: 710256-2
    detail.hit.zdb_id: 2016804-4
    detail.hit.zdb_id: 3094181-7
    detail.hit.zdb_id: 3094219-6
    detail.hit.zdb_id: 3094167-2
    detail.hit.zdb_id: 2220777-6
    detail.hit.zdb_id: 3094197-0
    SSG: 16,13
    Location Call Number Limitation Availability
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