Ergebnisse und Aussichten der Gefügeforschung im pommerschen Diluvium     

Konrad Richter 《International Journal of Earth Sciences》1936,27(2):196-206

Zusammenfassung Die Bewegungsrichtungen der diluvialen, nordischen Inlandeismassen können mit ihren Veränderungen des Nachschubes auf Grund ihres Geschiebeinventars in. Norddeutschland festgestellt werden. Derartige Eisstromstriche im großen stehen mit den lokalen Lagerungsverhältnissen diluvialer Schichtpakete des Jungmoränengebietes sehr oft im Widerspruch. Besonders ist das im küstennahen Gebiet Norddeutschlands der Fall. Selten sind genügend große Aufschlüsse vorhanden, die aus der Art der Schichtenlagerung die bis 90^° betragenden Abweichungen von der normalen Bewegungsrichtung des Inlandeises erkennen lassen. Es wird daher das Kleingefüge der Geschiebemergel zum Erkennen dieser Abweichungen benutzt. Im allgemeinen wurden die Geschiebe im Eis als Stromlinienkörper bewegt, so daß für Pommern eine Karte beigegeben ist, die eine Glazialschrammenkarte ersetzt. Sie läßt die stärkeren lokalen Schwankungen im küstennahen Gebiet deutlich erkennen. Weitere Einregelungsstudien in fluvioglazialen Sedimenten führten besonders bei Osern zur Möglichkeit, ehemalige Stromrichtungen und -stärken festzustellen. Als Darstellungsmethode werden Gefügediagramme empfohlen, wie sieSander, Rüger u. a. vorwiegend bei Schmelztektoniten benutzten. Die Urstromtäler und großen radialen Rinnen in Norddeutschland bergen noch Probleme, die voraussichtlich mit Einregelungsstudien zu lösen sind.  相似文献   

Mondkraterformationen auf der Erde     

Dr. N. Richter 《Pure and Applied Geophysics》1951,20(1):15-23

Zusammenfassung Es wird gezeigt, dass wir einige irdische Vulkankrater kennen, deren morphologischer Aufbau nahezu identisch ist mit den typischen Formen der Mondkrater. Auf die Wichtigkeit dieses Befundes für das Problem der Entstehung der Mondkrater wird hingewiesen. Es ist zu vermuten, dass sich auf der Erde noch weitere Beispiele dieser Art werden finden lassen.

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Summary It is shown, that some terrestrial volcanic craters are known, the morphological structure of which is practically identical with the typical shapes of lunar craters. The importance of this relation for the problem of the origin of lunar craters is pointed out. It may be expected, that some more examples of this kind might be found.

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III. Tektonik Die saxonische Tektonik im Bilde Europas     

Hans Stille  Franz Lotze  Gerhard Richter  A. Kraiß  Otto Heermann  Artur Roll  Fritz Forche 《International Journal of Earth Sciences》1948,35(2):172-175

Ohne Zusammenfassung  相似文献   

Zur Morphologie von Westgriqualand (Südafrika)     

Max Richter 《International Journal of Earth Sciences》1937,28(3-4):243-249

Ohne Zusammenfassung  相似文献   

Bücher- und Zeitschriftenschau     

Bubnoff  L. Rutten  Ernst Habetha  Kienow  Strassl  Konrad Richter  Stickel  Gallwitz  Wilckens 《International Journal of Earth Sciences》1937,28(8):629-641

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Non-destructive porosity determinations of antarctic marine sediments derived from resistivity measurements with an inductive method     

S. Gerland  M. Richter  H. Villinger  G. Kuhn 《Marine Geophysical Researches》1993,15(3):201-218

The fractional porosity of marine sediments is one of the fundamental index properties of rocks. For the determination of porosity a nondestructive, inductive method was used on unsplit sediment cores. The results were compared with galvanically measured resistivities using a miniature Wenner array on split cores. The measurements agree well except for cores with high clay content where measurement frequency related effects cause a resistivity difference of about 10%. Porosities were derived from resistivities using a published resistivity-porosity relationship by Boyce (1968) and compared with sample porosities. A comparison of both data sets shows good agreement.  相似文献   

Crystallization of melilite from CMAS-liquids and the formation of the melilite mantle of Type B1 CAIs: Experimental simulations     

Ruslan A. Mendybaev  Frank M. Richter  Andrew M. Davis 《Geochimica et cosmochimica acta》2006,70(10):2622-2642

Type B CAIs are subdivided into B1s, with well-developed melilite mantles, and B2s, with randomly distributed melilite. Despite intensive study, the origin of the characteristic melilite mantle of the B1s remains unclear. Recently, we proposed that formation of the melilite mantle is caused by depletion of the droplet surface in volatile magnesium and silicon due to higher evaporation rates of volatile species compared to their slow diffusion rates in the melt, thus making possible crystallization of melilite at the edge of the CAI first, followed by its crystallization in the central parts at lower temperatures. Here, we present the results of an experimental study that aimed to reproduce the texture observed in natural Type B CAIs. First, we experimentally determined crystallization temperatures of melilite for three melt compositions, which, combined with literature data, allowed us to find a simple relationship between the melt composition, crystallization temperature, and composition of first crystallizing melilite. Second, we conducted a series of evaporation and cooling experiments exposing CAI-like melts to gas mixtures with different oxygen fugacities (f_O2). Cooling of the molten droplets in gases with logf_O2?IW-4 resulted in crystallization of randomly distributed melilite, while under more reducing conditions, melilite mantles have been formed. Chemical profiles through samples quenched right before melilite started to crystallize showed no chemical gradients in samples exposed to relatively oxidizing gases (logf_O2?IW-4), while the near-surface parts of the samples exposed to very reducing gases (logf_O2?IW-7) were depleted in volatile MgO and SiO₂, and enriched in refractory Al₂O₃. Using these experimental results and the fact that the evaporation rate of magnesium and silicon from CAI-like melts is proportional to , we estimate that Type B1 CAIs could be formed by evaporation of a partially molten precursor in a gas of solar composition with . Type B2 CAIs could form by slower evaporation of the same precursors in the same gas with .  相似文献   

Kinetic isotopic fractionation during diffusion of ionic species in water     

Frank M. Richter  Ruslan A. Mendybaev  Ian D. Hutcheon  Neil C. Sturchio 《Geochimica et cosmochimica acta》2006,70(2):277-289

Experiments specifically designed to measure the ratio of the diffusivities of ions dissolved in water were used to determine . The measured ratio of the diffusion coefficients for Li and K in water (D_Li/D_K = 0.6) is in good agreement with published data, providing evidence that the experimental design being used resolves the relative mobility of ions with adequate precision to also be used for determining the fractionation of isotopes by diffusion in water. In the case of Li, we found measurable isotopic fractionation associated with the diffusion of dissolved LiCl (D_⁷Li/D_⁶Li=0.99772±0.00026). This difference in the diffusion coefficient of ⁷Li compared to ⁶Li is significantly less than that reported in an earlier study, a difference we attribute to the fact that in the earlier study Li diffused through a membrane separating the water reservoirs. Our experiments involving Mg diffusing in water found no measurable isotopic fractionation (D_²⁵Mg/D_²⁴Mg=1.00003±0.00006). Cl isotopes were fractionated during diffusion in water (D_³⁷Cl/D_³⁵Cl=0.99857±0.00080) whether or not the co-diffuser (Li or Mg) was isotopically fractionated. The isotopic fractionation associated with the diffusion of ions in water is much smaller than values we found previously for the isotopic fractionation of Li and Ca isotopes by diffusion in molten silicate liquids. A major distinction between water and silicate liquids is that water surrounds dissolved ions with hydration shells, which very likely play an important but still poorly understood role in limiting the isotopic fractionation associated with diffusion.  相似文献   

The first detection of propane on Saturn     

Thomas K. Greathouse  John H. Lacy  Bruno Bézard  Matthew J. Richter  Claudia Knez 《Icarus》2006,181(1):266-271

We report the first detection of propane, C₃H₈, in Saturn's stratosphere. Observations taken on September 8, 2002 UT at NASA's IRTF using TEXES, show multiple emission lines due to the 748 cm⁻¹ν₂₁ band of C₃H₈. Using a line-by-line radiative transfer code, we are able to fit the data by scaling the propane vertical mixing ratio profile from the photochemical model of Moses et al. [2000. Icarus 143, 244-298]. Multiplicative factors of 0.7 and 0.65 are required to fit the −20° and −80° planetocentric latitude spectra. The resultant profiles are characterized by a 5 mbar mixing ratio of 2.7±0.8×¹⁰⁻⁸ at −20° and at −80° latitude. These results suggest that the time scale for meridional circulation lies between the net photochemical lifetimes of C₂H₂ and C₃H₈, ≈30-600 years.  相似文献   

Moisture transport from the Atlantic to the Pacific basin and its response to North Atlantic cooling and global warming     

Ingo Richter  Shang-Ping Xie 《Climate Dynamics》2010,35(2-3):551-566

Atmospheric moisture transport from the Atlantic to the Pacific basin plays an important role in regulating North Atlantic salinity and thus the strength of the thermohaline circulation. Potential changes in the strength of this moisture transport are investigated for two different climate-change scenarios: North Atlantic cooling representative of Heinrich events, and increased greenhouse gas (GHG) forcing. The effect of North Atlantic cooling is studied using a coupled regional model with comparatively high resolution that successfully simulates Central American gap winds and other important aspects of the region. Cooler North Atlantic sea surface temperature (SST) in this model leads to a regional decrease of atmospheric moisture but also to an increase in wind speed across Central America via an anomalous pressure gradient. The latter effect dominates, resulting in a 0.13 Sv (1 Sv = 10⁶ m³ s^?1) increase in overall moisture transport to the Pacific basin. In fresh water forcing simulations with four different general circulation models, the wind speed effect is also present but not strong enough to completely offset the effect of moisture decrease except in one model. The influence of GHG forcing is studied using simulations from the Intergovernmental Panel on Climate Change archive. In these simulations atmospheric moisture increases globally, resulting in an increase of moisture transport by 0.25 Sv from the Atlantic to Pacific. Thus, in both scenarios, moisture transport changes act to stabilize the thermohaline circulation. The notion that the Andes effectively block moisture transport from the Atlantic to the Pacific basin is not supported by the simulations and atmospheric reanalyses examined here. This indicates that such a blocking effect does not exist or else that higher resolution is needed to adequately represent the steep orography of the Andes.  相似文献