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  • 1
    facet.materialart.00 | 00 |
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    Cambridge : Cambridge Univ. Press
    Signatur: M 15.89483
    Materialart: 00 | 00 |
    Seiten: viii, 381 S.
    Ausgabe: 3rd ed.
    Sprache: Englisch
    Standort: Lesesaal
    Zweigbibliothek: GFZ Bibliothek
    Standort Signatur Erwartet Verfügbarkeit
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  • 2
    Digitale Medien
    Digitale Medien
    Palo Alto, Calif. : Annual Reviews
    Annual Review of Astronomy and Astrophysics 7 (1969), S. 177-200 
    ISSN: 0066-4146
    Quelle: Annual Reviews Electronic Back Volume Collection 1932-2001ff
    Thema: Physik
    Materialart: Digitale Medien
    Standort Signatur Erwartet Verfügbarkeit
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  • 3
    Digitale Medien
    Digitale Medien
    Oxford, UK : Blackwell Publishing Ltd
    Geophysical journal international 5 (1945), S. 0 
    ISSN: 1365-246X
    Quelle: Blackwell Publishing Journal Backfiles 1879-2005
    Thema: Geologie und Paläontologie
    Notizen: A method is given of deriving the main features of the seismological travel-time tables from various assumed forms of the ray velocity variation. Attention is drawn to the utility of the functions dΔ/dp/dΔ and Σ in this connection. Attention is also drawn to the utility of the approximate formula v = arb which is both simple in application and gives very accurate results in parts of the Earth's interior, notably the region between the crustal layers and the level reached by rays for which Δ= 20°.
    Materialart: Digitale Medien
    Standort Signatur Erwartet Verfügbarkeit
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  • 4
    Digitale Medien
    Digitale Medien
    Oxford, UK : Blackwell Publishing Ltd
    Geophysical journal international 16 (1968), S. 0 
    ISSN: 1365-246X
    Quelle: Blackwell Publishing Journal Backfiles 1879-2005
    Thema: Geologie und Paläontologie
    Notizen: Using Birch's development of finite-strain theory for the Earth, a simple formula is derived expressing the compression f in terms of the pressure and incompressibility at internal points of the Earth. The formula is free from certain limitations in an earlier formula used by Birch, and is not restricted to the mantle. The formula is applied to determining values of f for six representative Earth models, and preferred estimates of f are set down for the Earth. The results are compared with Birch's earlier estimates of f for the mantle. The computed values of f do not significantly exceed 0·13 in the mantle or 0·20 in the core. Across the mantle-core boundary, f is likely to be nearly continuous; any sudden change is likely to be less than about 5 per cent. The results are subject to the reliability of Birch's form of equation of state for the internal regions of the Earth and, as in Birch's method, neglect possible effects of phase changes.
    Materialart: Digitale Medien
    Standort Signatur Erwartet Verfügbarkeit
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  • 5
    Digitale Medien
    Digitale Medien
    Oxford, UK : Blackwell Publishing Ltd
    Geophysical journal international 6 (1951), S. 0 
    ISSN: 1365-246X
    Quelle: Blackwell Publishing Journal Backfiles 1879-2005
    Thema: Geologie und Paläontologie
    Notizen: Calculations have been made of the partitioning of energy of P waves incident from above against the boundary of the Earth's inner core, and of P and SV waves incident against this boundary from below. In these calculations the inner core has been assumed to have rigidity as in an Earth model based on compressibility theory. The calculations have been applied to estimating the relative amplitudes of the phases PKJKP and PKIKP at various epicentral distances for a given earthquake. It is shown that, on the assumptions made, the phase PKJKP is most likely to be observed over a range 130°≫Δ≫ 155° of epicentral distance, the amplitude in this range being about one-fifth of that for PKIKP. It is suggested that readers of seismograms who find PKIKP strongly recorded in this range might also look for the phase PKJKP; the writer of this paper would much appreciate it if observational evidence supporting the existence of the phase PKJKP could be communicated to him for purposes of collation.
    Materialart: Digitale Medien
    Standort Signatur Erwartet Verfügbarkeit
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  • 6
    Digitale Medien
    Digitale Medien
    Oxford, UK : Blackwell Publishing Ltd
    Geophysical journal international 7 (1957), S. 0 
    ISSN: 1365-246X
    Quelle: Blackwell Publishing Journal Backfiles 1879-2005
    Thema: Geologie und Paläontologie
    Notizen: A re-examination of the internal structure of Mars has been made in the light of revised observational data on the radius R. Taking the reduced value R=3330 km, and the mass of Mars as 6.442 ± 1026 g, the hypotheses (a) that the Earth and Mars have the same overall composition and (b) that Model B gives a satisfactory representation of the Earth's mantle, are examined. It is confirmed that the reduced value of the radius implies the presence of a significant proportion of uncombined iron in the mantle of Mars. The assumptions would also require the interior of Mars to deviate from a hydrostatic state, and if correct lend support to the view of Jeffreys that the material of Mars has finite strength. It is still possible for Mars to have a small iron (and/or nickel) core, the radius of which most probably does not exceed 700–900 km; the smaller the radius of the core, however, the less the deviation from a hydrostatic state.On hypothesis (a), the reduced radius further implies that the Earth contains uncombined iron outside the inner core. A provisional view was that this uncombined iron was located mainly in the outer core. Further calculation, however, gives rise to the speculation that it is the mantle of the Earth which contains this uncombined iron and not the outer core. A coherent picture can be derived by assuming that Mars and the mantle of the Earth both consist broadly of a mixture of uncombined iron with silicates or FeO, MgO, SiO2 phases. The Earth's outer core on this view would contain no uncombined iron, the latter having gravitated toward the centre to form the inner core. In this way, the hypothesis (a) can be reconciled with the reduced Mars radius and with a hydrostatic state. The corresponding density distribution (p g/cm3) in Mars is given approximately by p=4–68 -0.86x2, where x=r/R, r being the distance from the centre.
    Materialart: Digitale Medien
    Standort Signatur Erwartet Verfügbarkeit
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  • 7
    Digitale Medien
    Digitale Medien
    Oxford, UK : Blackwell Publishing Ltd
    Geophysical journal international 6 (1952), S. 0 
    ISSN: 1365-246X
    Quelle: Blackwell Publishing Journal Backfiles 1879-2005
    Thema: Geologie und Paläontologie
    Notizen: A critical examination is made of curves presented by W. M. Elsasser on the density and compressibility of materials at zero temperatures and pressures up to 30 million atmospheres, and of Elsasser's inference that the Earth's core consists of iron or nickel-iron. An argument leading Elsasser to suggest that the writer's Earth Models A and B may require adjustments because of discrepancies with Elsasser's results is shown to be invalid.New tables are presented which fit the data used by Elsasser at 30 million atmospheres and are also consistent with geophysical data. The calculations leading to these tables imply that the atomic number to be associated with the material of the outer central core should be at least six units less than the value derived using simple extrapolations from quantummechanical calculations for high pressures. If the reduction in the atomic number is no more than six units, the most probable composition of the material in question would still be nickel-iron, and to this extent Elsasser's main conclusion is supported. But there are other aspects of the new calculations which suggest that the needed reduction may be greater than six units; these aspects raise the probability that the outer central core consists of a modification of ultra-basic rock. A caution is issued against forming too definite conclusions on either of the two opposing theories on the whole evidence so far available.Some support is found for the view that the Earth's present inner core is more likely to consist of an accumulation of iron and denser materials than of ultra-basic rock that has undergone a second pressure transformation. Support is also found for the view that the density gradients of Model B require a progressive change of composition with increase of depth in the inner core. The hypothesis that the inner core is solid is strengthened. Strong support is given to Elsasser's argument against the presence of large amounts of compressed hydrogen in the central core.The new tables suggest that the density of uranium (Z=92) may be a fairly smooth function of pressure from zero pressure right through to 30 million atmospheres, but that, for elements of smaller atomic numbers, there are likely to be significant density jumps at specific intermediate pressures. Tables are presented which give newly computed densities of uranium from 0.1 to 30 million atmospheres, and may serve as a useful basis of discussion in other contexts.As an incidental to discussing Elsasser's arguments, an Earth model (Model X) has been constructed with the property that the density in the central core near its outer boundary is 6.5 g/cm3. The model has a density gradient in the mantle only a little steeper than that in Models A and B, and has somewhat greater densities in the inner core. The outer part of the central core (between depths of 2900 and 4980km), however, differs radically from that of Models A and B through having a far steeper density gradient. The new model has to be regarded as implausible inasmuch as the last property implies far greater changes of composition with depth in the fluid part of the core than anywhere in the mantle.
    Materialart: Digitale Medien
    Standort Signatur Erwartet Verfügbarkeit
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  • 8
    Digitale Medien
    Digitale Medien
    Oxford, UK : Blackwell Publishing Ltd
    Geophysical journal international 7 (1956), S. 0 
    ISSN: 1365-246X
    Quelle: Blackwell Publishing Journal Backfiles 1879-2005
    Thema: Geologie und Paläontologie
    Notizen: iThe effect of errors in the expression for dp/dr used in constructing the Earth Model A is examined. It is shown that, for a 10 per cent error in dp/dr arising from possible deviations from adiabatic gradients and uniform chemical composition in the regions B and D, the maximum error in the density ρ in the mantle of Model A would be only 0.07 g/cm3. This is less than one-quarter of the error that would be entailed if a 10 per cent correction to dp/dr were applied throughout the mantle. Thus temperature deviations to any likely extent cannot be considered as serious sources of error in the density distribution of Model A.
    Materialart: Digitale Medien
    Standort Signatur Erwartet Verfügbarkeit
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  • 9
    Digitale Medien
    Digitale Medien
    Oxford, UK : Blackwell Publishing Ltd
    Geophysical journal international 7 (1955), S. 0 
    ISSN: 1365-246X
    Quelle: Blackwell Publishing Journal Backfiles 1879-2005
    Thema: Geologie und Paläontologie
    Notizen: Previous theoretical work on features of seismic rays has been extended to the case of pP and PP rays. It is shown that, for a wide class of velocity variations in the Earth's outer mantle, there is a cusp in the pP travel-time curve which corresponds to a ray which leaves a focus at finite depth in a direction inclined at a finite angle above the horizontal through the focus. It is also shown that the cusp is in general theoretically similar to the cusp in the PKP case. A method is given for locating this cusp for particular focal depths and is illustrated in an application to the Jeffreys-Bullen travel-time data. The general influence of the 20° discontinuity is discussed. Comment is made on conventions in naming pP and PP rays.
    Materialart: Digitale Medien
    Standort Signatur Erwartet Verfügbarkeit
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  • 10
    Digitale Medien
    Digitale Medien
    Oxford, UK : Blackwell Publishing Ltd
    Geophysical journal international 5 (1949), S. 0 
    ISSN: 1365-246X
    Quelle: Blackwell Publishing Journal Backfiles 1879-2005
    Thema: Geologie und Paläontologie
    Notizen: The hypothesis has been set down that at pressures ranging from 0.4 × 1012 to at least 3.6 × 1012 dynes/cm.2 (the latter being the pressure at the Earth's centre) the compressibility K−1 of a substance at temperatures of the order of those in the Earth's deep interior is essentially independent of its chemical composition. A simple form of the hypothesis to the effect that K and dk/dp (where p denotes pressure) change continuously and smoothly throughout the Earth below a depth of 1000 km. has been discussed in relation to seismic data. The hypothesis entails an abnormally large density gradient in the lowest 200 km. of the Earth's mantle, and in the Earth's inner core, and that these two regions are not chemically homogeneous. It entails that the density near the Earth's centre lies between about 16 g./cm.3 and 20 g./cm.3 (apart from a possible accumulation of even denser material very close to the centre). The hypothesis in its simplest form would require the Earth's density to be a little higher in the region above the 1000-km. level than the figures given in a previous model. The hypothesis would entail that the inner core is solid, capable of transmitting S waves at a speed not less than about 4.9 km./sec. and probably less than 6.0 km./sec.
    Materialart: Digitale Medien
    Standort Signatur Erwartet Verfügbarkeit
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