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  • 1
    Electronic Resource
    Electronic Resource
    Rotating lunar globules (1980)
    [s.l.] : Nature Publishing Group
    Nature 283 (1980), S. 108-108 
    Details
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] SEVERAL theories have been proposed for the origin of the shapes of lunar dumbbell and ellipsoidal glass globules. The rotational theory1 assumes that they solidify while rotating in free fall above the lunar surface, the rotation giving the elongation in form. A second theory imagines ...
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1038/283108a0
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    Paper (German National Licenses)
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  • 2
    Electronic Resource
    Electronic Resource
    Continuous Spectrum of Taurus A at 1.2 mm Wavelength (1969)
    [s.l.] : Nature Publishing Group
    Nature 221 (1969), S. 944-945 
    Details
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] The optical quality of the telescope was used for a preliminary determination of the pointing accuracy of the infrared system to within 1' of arc during a brief cloud-free interlude, but the observations themselves were made on the night of November 30December 1 through cloud, relying on the ...
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1038/221944a0
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  • 3
    Electronic Resource
    Electronic Resource
    A Corrugated Model for the Lunar Surface (1962)
    [s.l.] : Nature Publishing Group
    Nature 196 (1962), S. 1305-1305 
    Details
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] Fig. 1 It is clear from radiation considerations that during an eclipse the temperature 2\ of the bases of the indentations of our model vary very much less than will the temperature T2 of the upper surfaces. Eclipse measurements1'2 show a greater variation of effective temperature for regions ...
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1038/1961305a0
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    Paper (German National Licenses)
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  • 4
    Electronic Resource
    Electronic Resource
    Interpretation of Cosmology (1960)
    [s.l.] : Nature Publishing Group
    Nature 188 (1960), S. 923-924 
    Details
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] Gravitational formulations of Mach's Principle4 5 assume that the dynamical properties of a body are due to the gravitational interaction of the body with the matter composing the rest of the universe. The resulting gravitational potential of the body becomes a function of its velocity, so that the ...
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1038/188923a0
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    Paper (German National Licenses)
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  • 5
    Electronic Resource
    Electronic Resource
    Localisation of lunar acoustic energy (1970)
    Springer
    Earth, moon and planets 1 (1970), S. 449-450 
    Details
    ISSN: 1573-0794
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geosciences , Physics
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1007/BF00561915
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  • 6
    Electronic Resource
    Electronic Resource
    Infrared observations of the moon and their interpretation (1972)
    Springer
    Earth, moon and planets 5 (1972), S. 16-30 
    Details
    ISSN: 1573-0794
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geosciences , Physics
    Notes: Abstract The lunar spectrum, resulting from both the directly scattered solar radiation and the Moon's intrinsic thermal radiation, is described. The variations of the thermal component with latitude and phase, and during eclipse conditions, are described and compared with a plane homogeneous model of temperature-independent thermal constants. A review is given of that data appropriate to the lunar crust which may be obtained, both from comparison of this model with observation and from those modifications of the model, which explain otherwise anomalous measurements. Finally, a discussion of the various methods of determining the vertical temperature gradient at the surface leads to a mean value of about 2Km−1, although the heat flux associated with these results is much less than the recent direct measurement.
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1007/BF00562102
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  • 7
    Electronic Resource
    Electronic Resource
    The origin of the shapes of lunar globules (1979)
    Springer
    Earth, moon and planets 21 (1979), S. 283-288 
    Details
    ISSN: 1573-0794
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geosciences , Physics
    Notes: Abstract This paper considers three hypotheses for the origin of the shapes of the regular elongated prolate and dumbbell-shaped lunar glass globules. These are the break-up of a jet, the vibration-freezing hypothesis and the rotational hypothesis. It is concluded that there are many results favouring the latter hypothesis so that its validity now appears conclusive. Applications of the hypothesis as a tool in lunar science are briefly discussed.
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1007/BF00897356
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  • 8
    Electronic Resource
    Electronic Resource
    Planetary relaxation with spatially- and temporarily-dependent viscosity (1983)
    Springer
    Earth, moon and planets 28 (1983), S. 1-9 
    Details
    ISSN: 1573-0794
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geosciences , Physics
    Notes: Abstract This paper examines the relaxation of planetary surface features in the size range from one to several hundred kilometers. For this purpose a new type of computational method is used. This involves the assumption of axial symmetry and supposes also that motion takes place in a vertical direction only. Although this later assumption may seem restrictive, comparison with results computed by other techniques show that it produces relatively exact results. Furthermore, the method may be easily applied to a wide variety of situations in which for example the viscosity is a function of position time, shear-gradient, and even previous history, as well as cases in which inertial terms are important. In this paper the results of applying the method to two particular problems are briefly described — relaxation under a highly depth-dependent viscosity condition, and the relaxation of lunar mascons.
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1007/BF01371665
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  • 9
    Electronic Resource
    Electronic Resource
    Thermal instabilities and the formation of lunar maria (1973)
    Springer
    Earth, moon and planets 8 (1973), S. 335-339 
    Details
    ISSN: 1573-0794
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geosciences , Physics
    Notes: Abstract A model is discussed for a possible type of thermal instability in the outer layers of the Moon. An estimate is made for the temperature differential driving the instability. It is suggested that such an instability may have been involved in the formation of the lunar maria.
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1007/BF00581727
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  • 10
    Electronic Resource
    Electronic Resource
    Note on the rings of Saturn (1981)
    Springer
    Earth, moon and planets 24 (1981), S. 467-467 
    Details
    ISSN: 1573-0794
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geosciences , Physics
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1007/BF00896913
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