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  • 1
    Call number: SR 90.0924(33)
    In: Nordwestdeutsches Oberkarbon
    In: Fortschritte in der Geologie von Rheinland und Westfalen
    Type of Medium: Series available for loan
    Pages: 323 S. + 3 Beil.
    Series Statement: 33
    Language: German
    Location: Lower compact magazine
    Branch Library: GFZ Library
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  • 2
    Electronic Resource
    Electronic Resource
    Oxford, UK : Blackwell Publishing Ltd
    Geophysical journal international 104 (1991), S. 0 
    ISSN: 1365-246X
    Source: Blackwell Publishing Journal Backfiles 1879-2005
    Topics: Geosciences
    Notes: The coalification data (vitrinite reflectance, percentage Rm) from 49 boreholes located in the Czechoslovak part of the Upper Silesian Basin were processed and the palaeotemperature gradient which prevailed during the Namurian and the Early Westphalian was estimated. Very high gradients (mean: 95 Km-1) are calculated at least in the western part of the basin during the Namurian A. At that time, the Ostrava Formation (FM) was deposited with a high subsidence rate. The corresponding heat flow density of 200 mW m-2 may not reflect the characteristic heat flow density of the region, but may represent a subsurface value within the uppermost 2–3 km thick layer, probably sustained by the convective system inside the basin. The gradient during the Namurian B, C and Westphalian A is lower (mean: 77 K km-1 in the Karviná FM). It is suggested that the decrease in the gradient coincides with changes in the basin development. An intra Namurian hiatus occurred at the turn of the Namurian A and B. The lower thermal regime which governed during the sedimentation of the Karviná FM, results also from the Rm data of the Ostrava FM at the southern rim and in the Karviná part of the basin (mean gradient 60–65 K km-1). Due to the relatively small thickness of the Ostrava FM and/or the big thickness of the Karviná FM in these areas, the sediments of the Ostrava FM reached the maximum temperature during the deposition of the Karviná FM. Thus, the Rm data must reflect the lower gradient. By applying palaeogradients estimated in both formations together with present mean thermal conductivities within them, a heat flow density of 115–130 mWm-2 was computed. This value agrees well with the heat flow of 125 mWm-2 estimated for the Westphalian A in the Ruhr Basin by the same method.
    Type of Medium: Electronic Resource
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  • 3
    Electronic Resource
    Electronic Resource
    Amsterdam : Elsevier
    Earth and Planetary Science Letters 83 (1987), S. 175-177 
    ISSN: 0012-821X
    Source: Elsevier Journal Backfiles on ScienceDirect 1907 - 2002
    Topics: Geosciences , Physics
    Type of Medium: Electronic Resource
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  • 4
    Electronic Resource
    Electronic Resource
    Amsterdam : Elsevier
    Earth and Planetary Science Letters 99 (1990), S. 48-57 
    ISSN: 0012-821X
    Source: Elsevier Journal Backfiles on ScienceDirect 1907 - 2002
    Topics: Geosciences , Physics
    Type of Medium: Electronic Resource
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  • 5
    Electronic Resource
    Electronic Resource
    Amsterdam : Elsevier
    Earth and Planetary Science Letters 32 (1976), S. 84-90 
    ISSN: 0012-821X
    Source: Elsevier Journal Backfiles on ScienceDirect 1907 - 2002
    Topics: Geosciences , Physics
    Type of Medium: Electronic Resource
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  • 6
    Electronic Resource
    Electronic Resource
    Springer
    International journal of earth sciences 65 (1976), S. 809-819 
    ISSN: 1437-3262
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geosciences
    Description / Table of Contents: Abstract The heat flow, measured at the surface can be reduced with the help of various methods, so that conclusions are possible about the quantity from the upper mantle. The linear relationship between heat generation and heat flow within a heat flow province yields directly the reduced heat flow without models of the structure of the crust. The heat generation can also be estimated from the structure of the crust for small areals with the assumption of its exponential depletion with depth. The integral of the distribution of the radiogen heat sources and the thickness of the crust yields the heat flow generated in the crust, so that the heat flow from the upper mantle is deducable from the value at the surface by substraction the value generated in the crust. Another method is deduced from correlations between heat generation as well with the density as with the longitudinal velocity. A model of the distribution of heat generation in the crust results directly from gravity and seismic models by using those correlations. The integral of the distribution of the heat sources in the crust yields the heat flow from the upper mantle by subtraction the value of the integral from the surface value of the heat flow.
    Abstract: Resume La densité du flux géothermique mesurée à la surface, peut être réduite à l'aide de différentes méthodes, de manière à pouvoir en déduire la grandeur du flux thermique du manteau supérieur. La relation linéaire entre la production thermique et le flux thermique, donne directement la valeur réduite, sans qu'il y ait besoin d'utiliser des modèles de structuraux de la croûte. Dans les régions locales, la production thermique, en admettant qu'elle diminue exponentiellement avec la profondeur, peut être évaluée approximativement à l'aide de la structure de la croûte; l'intégrale de la distribution en profondeur des producteurs de chaleur radiogènes y donne la densité du flux thermique engendré dans la croûte, qui, soustraite de la valeur à la surface, donne la densité du flux thermique du manteau supérieur. Une autre méthode s'obtient à l'aide de corrélations entre la production thermique due à la densité et celle due à la vitesse des ondes de compression. Les corrélations, obtenues à l'aide de modèles gravimétriques et sismiques, donnent un modèle de la distribution de la production thermique dans la croûte, dont l'intégrale d'une part et la densité du flux thermique à la surface d'autre part, permettent d'évaluer approximativement la valeur relative au manteau supérieur.
    Notes: Zusammenfassung Die an der Erdoberfläche gemessene Wärmeflußdichte kann mit Hilfe verschiedener Methoden soweit reduziert werden, daß Aussagen über die Größe der Wärmeflußdichte aus dem oberen Mantel möglich sind. Die lineare Beziehung zwischen Wärmeproduktion und Wärmeflußdichte innerhalb einer Wärmeflußprovinz ergibt den reduzierten Wert direkt, ohne Modelle zum Aufbau der Erdkruste benutzen zu müssen. Für kleinere Gebiete kann die Wärmeproduktion unter der Annahme ihrer exponentiellen Abnahme mit der Tiefe aus der Struktur der Erdkruste abgeschätzt werden, und das Integral der Verteilung der radiogenen Wärmeproduzenten über die Tiefe ergibt die in der Kruste generierte Wärmeflußdichte, die, vom Oberfläcbenwert subtrahiert, die Wärmeflußdichte aus dem oberen Mantel ergibt. Eine weitere Methode wird aus Korrelationen zwischen der Wärmeproduktion sowohl mit der Dichte als auch mit der Kompressionswellengeschwindigkeit abgeleitet. Die Korrelationen ergeben aus gravimetrischen und seismischen Modellen ein Modell der Wärmeproduktionsverteilung in der Kruste, aus deren Integral und der Oberflächen-Wärmeflußdichte der Wert aus dem oberen Mantel abgeschätzt wird.
    Type of Medium: Electronic Resource
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  • 7
    Electronic Resource
    Electronic Resource
    Springer
    Studia geophysica et geodaetica 34 (1990), S. 208-219 
    ISSN: 1573-1626
    Source: Springer Online Journal Archives 1860-2000
    Topics: Architecture, Civil Engineering, Surveying , Geosciences , Physics
    Notes: Summary The coalification data of 12 boreholes in the Central Bohemian Basin are used to evaluate the paleotemperature gradients for the Upper Carboniferous period of the basin's development. Two versions of the burial history considered are supposed to yield an upper and a lower estimate. According to the more probable “lower” version, the average values of the paleogradient suggest an increasing tendency from west to east in the interval of 45–53K/km. The current geothermal gradients vary in the range of 28–35K/km. By combining the present thermal conductivity and the paleogradients, we have tried to estimate the Upper Carboniferous heat flow. Its values range from 96mW/m 2 to 117mW/m 2 . The results obtained can be compared with the paleogradient estimates in the Saar-Nahe Basin (F. R. of Germany). This region, which is similar with respect to the time of origin and tectonic pattern to the Central Bohemian Basin, displays on the average a slightly higher Permo-Carboniferous geothermal gradient of 60K/km.
    Type of Medium: Electronic Resource
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  • 8
    Publication Date: 1981-07-01
    Print ISSN: 0377-0273
    Electronic ISSN: 1872-6097
    Topics: Geosciences
    Published by Elsevier
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  • 9
    Publication Date: 1981-05-01
    Print ISSN: 0040-1951
    Electronic ISSN: 1879-3266
    Topics: Geosciences , Physics
    Published by Elsevier
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  • 10
    Publication Date: 1990-07-01
    Print ISSN: 0039-3169
    Electronic ISSN: 1573-1626
    Topics: Architecture, Civil Engineering, Surveying , Geosciences , Physics
    Published by Springer
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