Bücher- und Zeitschriftenschau

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Farbmessungen im Mittleren und Oberen Buntsandstein Süddeutschlands

Zusammenfassung Die große Variationsbreite der rotbraunen Farben im Buntsandstein bieten bei geeignetem Meßgerät und spezieller Methode eine wichtige Anwendungsmöglichkeit für stratigraphisches Arbeiten. Ein Farbprofil der Röttone (so 3 T, so 4 T) über 120 km Distanz, sowie die Auswertung der Farben von Kernbohrungen im Mittleren Buntsandstein (sm) zeigen den großen Wert exakter Farbmessungen.

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Colour measurements in the Middle and Upper Buntsandstein of Southern Germany prove that the method used here is a simple instrument for the correlation of strata series. A colour section of the Röttone (so 3 T, so 4 T) along a distance of 120 km and the interpretation of drill cores of the Middle Buntsandstein (sm) show the value of the exact colour measurements for stratigraphical research.

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Résumé Des mensurations de la couleur, à l'aide d'un Lovibond-Schofield-Tintometer, du Buntsandstein moyen et supérieur en Allemagne du Sud sont aptes à l'établissement de corrélations stratigraphiques. Des mesures dans les Röttone (so3T,so4T) sur une distance de 120 km et des interprétations des couleurs du Buntsandstein moyen (sm) — obtenues par carottage — témoignent de l'importance de tels mesures pour les recherches stratigraphiques.

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, (sm).

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Poster anläßlich der 72. Jahrestagung der Geologischen Vereinigung am 25.-27. 2. 1982 in Würzburg.     

Sublimation coefficient of water ice under simulated cometary-like conditions

In papers dealing with evolution of cometary nuclei it is commonly assumed that the coefficients of sublimation _s and condensation _c of vapour are both equal to one. The experimental investigation of ice samples under simulated cometary-like conditions (Kossacki, K.J., Kömle, N.I., Leliwa-Kopysty ski, J., Kargl, G., 1997. Thermal and structural evolution of cometary subsurface layer: selfconsistent model and experimental verification. Icarus 128, 127–144) suggests, however, that the sublimation flux calculated with the Hertz–Knudsen formula and the above assumption is nearly an order of magnitude too high. This may imply that actual values of _s for the ice/dust sample used in these experiments are of the order of 0.1. A similar conclusion can be drawn for _c from the results of various experiments concerning growth of ice crystals from the vapour phase and their sublimation (Lamb, D., Scott, W.D., 1972. Linear growth rates of ice crystals grown from the vapor phase. Journal of Crystal Growth 12, 21–31; Beckmann, W., Lacmann, R., 1982. Interface kinetics of growth and evaporation of ice II. Journal of Crystal Growth 58, 433–442; Sei, T., Gonda, T., 1989. The growth mechanism and the habit change of ice crystals growing from the vapour phase. Journal of Crystal Growth 94, 697–707). The exact values of both of these coefficients depend on various parameters such as temperature, concentration of surface impurities and deviation of the vapour pressure from that of the phase equilibrium. In this work the temperature dependence of the sublimation and condensation coefficients is discussed and an appropriate formula is proposed to fit the experimental results. This new formulation is then used to analyse the implications for the thermal conductivity of a porous cometary-like ice and the rate of vapour flux from a cometary nucleus.