Cathodoluminescence of authigenic albite

Authigenic albites in carbonate rocks typically grow in a high-grade diagenetic to low-grade metamorphic environment and often show Roc-Tourné-twinning sensu Füchtbauer. Based on an investigation of four Middle to South European occurrences, they show Mn²⁺- and Fe³⁺-activated cathodoluminescence (CL), as revealed by combined high resolution spectroscopy of cathodoluminescence emission (HRS-CL), electron paramagnetic resonance (EPR), and proton-induced X-ray emission (μPIXE).     

TEM study of a special grain boundary in a synthetic K-feldspar bicrystal: Manebach Twin

 A monoclinic KAlSi₃O₈ feldspar Manebach twin boundary was synthesized by diffusion bonding and examined using high-resolution transmission electron microscopy. The sharp (001) twin boundary is straight and free of strain. The boundary width is smaller than d₀₀₁. There is no rigid body shift observed at the twin boundary, and the feldspar structure is arranged symmetrically across (001). The twin boundary structure consists of bridged tetrahedral crankshafts, which are characteristic of the feldspar lattice. The grain boundary structure is in good agreement with the geometrical model of Taylor et al. (1934). The grain boundary composition of K_1/2H_1/2AlSi₃O₈ differs from their model. Received: 13 February 2002 / Accepted: 24 December 2002 Acknowledgements We thank M. Rühle, S. Hutt, J. Mayer, A. Strecker and U. Salzberger at MPI, Stuttgart, for their support and valuable advice in preparing TEM sections of bicrystals.     

Epikarst hydrology and implications for stalagmite capture of climate changes at Grotta di Ernesto (NE Italy): results from long‐term monitoring

Grotta di Ernesto is a cave site well suited for palaeoclimate studies because it contains annually laminated stalagmites and was monitored from 1995 to the end of 2008 for microclimate, hydrology and hydrochemistry. Long‐term monitoring highlighted that cave drips show three different hydrological responses to rainfall and infiltration: (1) fast seasonal drips in the upper part of the cave, which are mostly fed by fractures, (2) slow seasonal drips, located at mid‐depth in the cave characterized by mixed feeding and (3) slow drips, mostly located in the deeper gallery, which are fed by seepage flow from bulk porosity with a minor fracture‐fed component. The slow drips display daily cycles during spring thaw. Monitoring also indicated that drip waters are only slightly modified by degassing within the soil zone and aquifer and by prior calcite precipitation. Hydrochemical studies show a clear seasonality in calcite saturation index, which results in most cave calcite precipitation occurring during late autumn and winter with similar amounts of precipitated calcite on most stalagmites, regardless of drip rate (discharge) differences. Drip rate, and drip rate variability, therefore, has a minor role in modulating the amount of annual calcite formation. In contrast, drip rate, when associated with moderate reduction in calcite saturation index, clearly influences stalagmite morphology. Increasing drip rate yields a passage from candle‐, to cone‐ to dome‐shaped stalagmites. Very high drip rates feed speleothems with flowstone morphology. In summary, monitoring provides information about the karst aquifer and how hydrology influences those physical and chemical characteristics of speleothems which are commonly used as climate proxies. Copyright © 2010 John Wiley & Sons, Ltd.     

Hydrocarbon distribution in coals and in dispersed organic matter of different maceral compositions and maturities

More than 60 samples from 5 coal seams and adjacent siltstones and sandstones were selected from a well through Westphalian B sediments from Northern Germany in order to study bitumen generation and migration. The cores were drilled between 1200 und 1530 metres depth. In this interval, vitrinite reflectance (Rr) is increasing from 0.70 to 0.92%. Results reveal high hydrocarbon generation potentials for all coal samples, but not for adjacent clastic rocks, although maceral compositions of both are quite similar. Yields and compositions of thermal extracts from the coals depend on maceral compositions and rank. However, the bulk of the already generated bitumen has not been removed during natural coalification and is not easily releasable by thermovaporisation. A mass balance based on elemental composition of dull coals indicates that in the rather narrow rank interval (0.70–0.92% Rr) a total mass loss of 20% may have occurred by migration. This is evidenced by a loss of about 20% of the original hydrogen, the rest being stored in the coals.

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Zusammenfassung Um die Entstehung und Migration von Bitumen zu untersuchen wurden in Norddeutschland mehr als 60 Proben aus 5 Kohleflözen und benachbarten Silt- und Sandsteinen aus einer Bohrung durch Westphal B-Sedimente bearbeitet. Die Entnahmetiefe der Bohrkerne liegt zwischen 1200 und 1530 Metern. Innerhalb dieses Intervales steigt die Vitrinit-Reflexion (Rr) von 0,70 auf 0,92%. Für alle Proben aus den Flözen ergeben sich hohe Kohlenwasserstoff-Bildungspotentiale, nicht aber für die benachbarten klastischen Gesteine, obwohl die Mazeral-Zusammensetzungen in beiden ähnlich sind. Die Ausbeute und Zusammensetzung thermaler Extrakte aus den Flözen hängen von Mazeral-Zusammensetzung und Reife ab. Allerdings wurden weder während der Inkohlung größere Mengen des Bitumens abtransportiert, noch ist dieses durch Thermovaporisation leicht freisetzbar. Eine Massenbalanzierung auf der Basis der Elementzusammensetzung ergibt für das relativ schmale Interval von C,70-0,92% Rr ein Massenverlust von 20% durch Migration. Diese Angabe basiert auf einer 20%igen Reduzierung der ursprünglichen Wasserstoffmenge, wobei die restlichen 80% in der Kohle gespeichert bleiben.

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Résumé Dans un forage pratiqué à travers le Westphalien B du nord de l'Allemagne, on a sélectionné plus de 60 échantillons provenant de 5 couches de charbon ainsi que des siltites et grès adjacents, dans le but d'étudier la formation et la migration du bitume. Les carottes proviennent de profondeurs situées entre 1200 et 1530 m. Dans cet intervalle, le pouvoir réflecteur de la vitrinite (Rr) passe de 0,70 à 0,92%. L'étude révèle des potentiels élevés en hydrocarbure pour tous les échantillons de charbon, mais pas pour les roches détritiques voisines, bien que les compositions «macérales» soient analogues dans les deux cas. L'importance et la composition des extrait athermiques des charbons dépendent de la composition «macérale» et du degré d'évolution. Toutefois, la plus grande partie du bitume engendré est restée sur place au cours de la houillification naturelle et elle est difficile à extraire avex la methode de thermovaporisation. Une balance des masses d'éléments indique pour cet intervalle relativement étroit (0,7–0,92% Rr) une perte totale de masse de 20% due à la migration. Ce résultat correspond à une perte d'environ 20% de l'hydrogène originel, les 80% restants étant demeurés dans le charbon.

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60 5 , , . 1200 1530 . /Rr/ 0,7 0,92. , , . , , . , , . , , 20% 0,7 0,92 %. 20%; , 80%, .

     

Validation of the “Lokal-Modell” over heterogeneous land surfaces using aircraft-based measurements of the REEEFA experiment and comparison with micro-scale simulations

Summary An aircraft-based experimental investigation of the atmospheric boundary layer (ABL) structure and of the energy exchange processes over heterogeneous land surfaces is presented. The measurements are used for the validation of the mesoscale atmospheric model “Lokal-Modell” (LM) of the German Weather Service with 2.8 km resolution. In addition, high-resolution simulations using the non-hydrostatic model FOOT3DK with 250 m resolution are performed in order to resolve detailed surface heterogeneities. Two special observation periods in May 1999 show comparable convective boundary layer (CBL) conditions. For one case study vertical profiles and area averages of meteorological quantities and energy fluxes are investigated in detail. The measured net radiation is highly dependent on surface albedo, and the latent heat flux exhibits a strong temporal variability in the investigation area. A reduction of this variability is possible by aggregation of multiple flight patterns. To calculate surface fluxes from aircraft measurements at low altitude, turbulent energy fluxes were extrapolated to the ground by the budget method, which turned out to be well applicable for the sensible heat flux, but not for the latent flux. The development of the ABL is well captured by the LM simulation. The comparison of spatiotemporal averages shows an underestimation of the observed net radiation, which is mainly caused by thin low-level clouds in the LM compared to observed scattered CBL clouds. The sensible heat flux is reproduced very well, while the latent flux is highly overestimated especially above forests. The realistic representation of surface heterogeneities in the investigation area in the FOOT3DK simulations leads to improvements for the energy fluxes, but an overestimation of the latent heat flux still persists. A study of upscaling effects yields more structures than the LM fields when averaged to the same scale, which are partly caused by the non-linear effects of parameter aggregation on the LM scale.     

Pétrographie des „Permoskyth“ der Jaggl-Plawen-Einheit (Südtirol) und Diskussion der Detritusherkunft mit Hilfe von Kathoden-Lumineszenz-Untersuchungen

The Permo-Scythian deposits E of Lake Reschen (North-Italy) are composed of a sequence of terrestrial sediments in Verrucanofacies and of a series of detrital carbonate and lagoonal-evaporitic rocks (“Wechselschichten”) overlaid by Anisian fossiliferous dolomites. Examinations by cathodo-luminescence give reference to the source area of the detrius and to the diagenesis of the sediments. Further statements can be made by X-ray (triclinity of K-feldspars; inclusions in authigenic minerals) and chemical examinations (composition of dolomites). The detritus of the slightly metamorphic rocks, indicated by the crystallinity of illite, does not originate from the underlying “Plawenkristallin” and from the adjacent “ötztalkristallin”, respectively, but by 70% from a porphyritic source area that is supposed to be located in the region of Lugano.     

Rain rate estimation from a synergetic use of SSM/I, AVHRR and meso-scale numerical model data

Summary In this paper a retrieval technique for estimating rainfall rates is introduced. The novel feature of this technique is the combination of two satellite radiometers — the Special Sensor Microwave/Imager (SSM/I) and the Advanced Very High-Resolution Radiometer (AVHRR) — with mesoscale weather prediction model data. This offers an adjustment of the model atmospheres to reality which is necessary for calculating brightness temperatures that can be compared with microwave satellite measurements.In sensitivity studies it was found that the estimation of precipitation is determined to a high degree by the particle size distribution of rain and snow, especially by the size distribution of solid hydrometeors. These studies also reveal the influence of the knowledge of the correct cloud coverage inside a SSM/I pixel and the importance of using a realistic temperature profile instead of using standard atmospheres.The retrieval technique is based on radiative transfer calculations using the model of Kummerow et al. (1989). The algorithm consists of two parts: First Guess (FG) brightness temperatures for the SSM/I frequencies are generated as a function of the cloud top height and the cloud coverage, derived from AVHRR data and predictions from a meso-scale model. The rainfall rate of different types of clouds containing raindrops, ice particles and coexisting ice and water hydrometeors is then calculated as a function of the cloud top height. As an example, a strong convective rain event over the western part of Europe and over the Alps is taken to evaluate the performance of this technique. Good agreement with radar data from the German Weather Service was achieved. Compared to statistical rainfall algorithms, the current algorithm shows a better performance of detecting rainfall areas.With 12 Figures     

Binary stellar winds

Stellar winds from a binary star pair will interact with each other along a contact discontinuity. We discuss qualitatively the geometry of the flow and field resulting from this interaction in the simplest case where the stars and winds are identical. We consider the shape of the critical surface (defined as the surface where the flow speed is equal to the sound speed) as a function of stellar separation and the role of shock waves in the flow field. The effect of stellar spin and magnetic sectors on the field configuration is given. The relative roles of mass loss and magnetic torque in the evolution of orbital parameters are discussed.