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  • 1
    Monograph available for loan
    Monograph available for loan
    Bristol : Hilger
    Call number: FHD 152
    Type of Medium: Monograph available for loan
    Pages: XIV, 208 S. : graph. Darst.
    ISBN: 0852744455
    Location: Upper compact magazine
    Branch Library: GFZ Library
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  • 2
    Electronic Resource
    Electronic Resource
    Oxford, UK : Blackwell Publishing Ltd
    Geophysical journal international 115 (1993), S. 0 
    ISSN: 1365-246X
    Source: Blackwell Publishing Journal Backfiles 1879-2005
    Topics: Geosciences
    Type of Medium: Electronic Resource
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  • 3
    Electronic Resource
    Electronic Resource
    [s.l.] : Nature Publishing Group
    Nature 186 (1960), S. 301-301 
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] According to ndrade, the viscosity, rj, thermal conductivity, k, and specific heat at constant volume, Cp, for a non-metallic monatomic liquid at the melting point, are related according to the expression: T, _ Aff1 i\\ A/ ./x jv-"y \ * / Here A, a constant, is approximately unity: for ...
    Type of Medium: Electronic Resource
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  • 4
    Electronic Resource
    Electronic Resource
    [s.l.] : Nature Publishing Group
    Nature 194 (1962), S. 564-565 
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] For forced convection, let the fluid be caused to move past the surface with steady speed v. The boundary temperature will be sssumed to be greater than that of the main fluid by an amount AT(4= 0); but the opposite situation could equally well apply. Difficulties over the detailed specification of ...
    Type of Medium: Electronic Resource
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  • 5
    Electronic Resource
    Electronic Resource
    Springer
    Earth, moon and planets 36 (1986), S. 97-102 
    ISSN: 1573-0794
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geosciences , Physics
    Notes: Abstract It is widely accepted that Mars holds a quantity of water in its surface crustal region but the amount is unknown. The present arguments quantify this suspicion, offering an estimate of the quantity on the basis of certain consequences of the comparison between the present observed compositions of the atmospheres of the planets Earth, Venus, and Mars, and the inferred compositions of the mantles of the icy satellites. The results are consistent with alternative estimates such as they are but offer possibilities of regarding the problems of the crustal region of Mars in a different way.
    Type of Medium: Electronic Resource
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  • 6
    Electronic Resource
    Electronic Resource
    Springer
    Surveys in geophysics 5 (1982), S. 89-139 
    ISSN: 1573-0956
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geosciences , Physics
    Notes: Abstract A deeper understanding of the constituents of the Solar System has been obtained over the last decade due primarily to the success of a variety of space missions which have provided a wealth of data to augment that obtained from Earth based observatories. Although the measurements refer directly to both the surface and atmospheric conditions, inferences can be made about conditions within the main bodies of the planets. This has been achieved through the closest collaboration between physicists, chemists and geologists in the study of these problems. In the present review we explore in a general way some of the types of problem involved with the physics of the interiors of planetary bodies. Concern will be with elucidating the structure of these bodies on the basis of the properties observed now. The arguments will be made in general terms and will not be concerned with any one planet in close detail.
    Type of Medium: Electronic Resource
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  • 7
    Electronic Resource
    Electronic Resource
    Springer
    Surveys in geophysics 8 (1986), S. 439-457 
    ISSN: 1573-0956
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geosciences , Physics
    Notes: Abstract The study of the cosmic chemical abundance of the elements suggests that water (which is a combination of the first and second most abundant chemically active elements) is likely to be the most abundant chemical compound in the solar system. It is found that water indeed appears to be a common constituent of planetary bodies even though its presence is not always directly detectable. The amount involved, and the form it takes, varies from one object to another. The Earth has surface liquid water and crustal hydrate materials and only Mars of the terrestrial planets is also likely to have non-atmospheric water and that in frozen form near the surface. The mantles of the icy satellites, and particularly those of Jupiter and Saturn, are the most extended locations of water in the solar system although Uranus and Neptune are likely to have substantial mid-mantle internal water components. Only Mercury and Moon appear to be devoid of water. The smaller bodies such as comets are excluded from the discussion even though they are now known to be composed largely of water-ice.
    Type of Medium: Electronic Resource
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  • 8
    Electronic Resource
    Electronic Resource
    Springer
    Earth, moon and planets 35 (1986), S. 213-218 
    ISSN: 1573-0794
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geosciences , Physics
    Notes: Abstract An argument is given, based on considerations of moments of inertia and the equatorial location of the large crater Herschel, which implies that Mimas (one of the smallest satellites of the major planets) shows a high degree of internal differentiation (with a silicate-type core but a mantle with a density rather greater than for water-ice alone). Some consequences of these arguments are adduced and possible compositions of the mantle considered.
    Type of Medium: Electronic Resource
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  • 9
    Electronic Resource
    Electronic Resource
    Springer
    Surveys in geophysics 11 (1990), S. 1-54 
    ISSN: 1573-0956
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geosciences , Physics
    Notes: Abstract An understanding of the origin of the Solar System is proving hard to achieve and there is still no finally accepted account. A wider range of reliable data, and especially for the outer Solar System, has become available over the last decade due to the use of space vehicles, and particularly the two Voyager probes which are now passing out of the Solar System. The planetary and satellite systems can, therefore, be viewed now more nearly as a whole than previously and consequences for the theory of the origin of the System should follow. The subject is here reviewed again but emphasis is placed on the relative planetology of the whole System. The only reliable data available to us are associated with the System as it is now and this will be the starting point for our discussion.
    Type of Medium: Electronic Resource
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  • 10
    Publication Date: 1986-07-01
    Print ISSN: 0031-9228
    Electronic ISSN: 1945-0699
    Topics: Physics
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