U–Pb zircon ages and structural development of metagranitoids of the Teplá crystalline complex: evidence for pervasive Cambrian plutonism within the Bohemian massif (Czech Republic)

U–Pb zircon dating of three metagranitoids, situated within a tilted crustal section at the northwestern border of the Teplá Barrandian unit (Teplá crystalline complex, TCC), yields similar Cambrian ages. The U–Pb data of zircons of the Teplá orthogneiss define an upper intercept age of 513 +7/–6?Ma. The ²⁰⁷Pb/²⁰⁶Pb ages of 516±10 and 511±10?Ma of nearly concordant zircons of the Hanov orthogneiss and the Lestkov granite are interpreted to be close to the formation age of the granitoid protolith. Similar to the Cambrian granitoids of the southwestern part of the Teplá Barrandian unit (Doma?lice crystalline complex, DCC) the Middle Cambrian emplacement of the TCC granitoids postdates Cadomian deformation and metamorphism of the Upper Proterozoic country rocks, but predates Variscan tectonometamorphic imprints. Structural data as well as sedimentological criteria suggest a dextral transtensional setting during the Cambrian plutonism, related to the Early Paleozoic break-up of northern Gondwana. Due to strong Variscan crustal tilting, the degree of Variscan tectonometamorphic overprint is strikingly different in the dated granitoids. It is lowest in the weakly or undeformed Lestkov granite, located in the greenschist-facies domain. The Teplá orthogneiss in the north underwent pervasive top-to-NW mylonitic shearing under amphibolite-facies conditions. There is no indication for a resetting of the U–Pb isotopic system of the Teplá orthogneiss zircons that could be attributed to this imprint. Radiation damages accumulated until recent have probably caused lead loss.     

The internal structure of the Arosa Zone (Swiss-Austrian Alps)

The Arosa Zone, part of the main Alpine suture zone between the Austroalpine and the Penninic realms, forms a heterogeneous unit composed of rocks of oceanic and continental origin. It exhibits mélange character due to minor sedimentary mixing and local penetrative tectonic deformation during Cretaceous and Early Tertiary imbrication. Competent blocks of both Austroalpine and Penninic origin, covering up to 2.5 km², are embedded in incompetent serpentinitic or shaly-calcareous matrix. On a mesoscale, disrupted strata occur in and adjacent to thrust and shear zones. Contrasting competence between blocks and matrix partitioned deformation into brittle and ductile processes. Extension veins and shear fractures affected the competent strata whereas the matrix developed a penetrative foliation during ductile flow and accommodated high strain. Flow was mainly non-coaxial in the matrix, and coaxial extension prevailed in the blocks.In a regional tectonic setting, we define the Arosa Zone as the tectonostratigraphic unit sandwiched between the Austroalpine and Penninic units. It forms a narrow and highly imbricated zone containing both South Penninic ophiolitic and sedimentary rocks as well as blocks and slices of Austroalpine origin.

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Zusammenfassung Die Arosa Zone ist Teil der Alpinen Suturzone zwischen Ostalpin und Pennimkum und bildet eine lithologisch heterogene Einheit aus kontinentalen und ozeanischen Gesteinen. Sie zeigt den Charakter einer Melange, die aus, untergeordnet, sedimentärer Durchmischung und lokaler, aber penetrativer tektonischer Deformation während kretazisch und alttertiärer Tektonik resultiert. Kompetente Blöcke ostalpiner und penninischer Herkunft, die bis zu 3 km im Streichen verfolgbar sind, schwimmen in einer inkompetenten serpentinitischen oder tonig-karbonatischen Matrix. Im Mesobereich treten zerbrochene Gesteinsabfolgen in oder direkt an Überschiebungs- und Scherzonen auf. Unterschiedliche Kompetenz zwischen Blöcken und Matrix teilt die Deformation in spröde und duktile Prozesse auf. Die kompetenten Gesteine zeigen Extensionsspalten und Scherbrüche, in der Matrix entwickelte sich durch duktiles Fließen eine penetrative Schieferung bei hoher Strainintensität. Die Deformation in der Matrix war hauptsächlich nicht-koaxial, koaxiale Extension herrschte in den Blöcken.Im regionalen tektonischen Rahmen definieren wir die Arosa Zone als tektonostratigraphische Einheit zwischen Ostalpin und Penninikum. Sie bildet eine schmale, stark imbrikierte Zone die, aus südpenninischen ophiolithischen und sedimentären Gesteinen, sowie aus Blöcken und Spänen ostalpiner Herkunft aufgebaut wird.

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Résumé La Zone d'Arosa, partie de la zone de suture alpine entre l'Austro-alpin et le Pennique, forme une unité hétérogène composée de roches d'origines océanique et continentale. Elle présente le caractère d'un mélange qui résulte d'un brassage sédimentaire mineur, et de déformations tectoniques, locales mais pénétratives, au cours du Crétacé et du Tertiaire ancien. Des blocs compétents de l'Austro-alpin et du Pennique qui couvrent jusqu'à 2.5 km², sont enrobés dans une matrice incompétente serpentineuse ou argilo-calcaire. A moyenne échelle, les couches disloquées se rencontrent dans les zones charriées et cisaillées, ou y sont adjacentes. La différence de compétence entre les blocs et la matrice répartit la déformation en processus cassants et ductiles. Les roches compétentes montrent des fentes d'extension et des fractures de cisaillement, alors que dans la matrice, sous l'action d'un flux ductile et d'une intensité de contrainte élevée, se développe une foliation pénétrative. La déformation fut principalement non coaxiale dans la matrice et coaxiale dans les blocs d'extension.Dans un cadre tectonique régional, nous définissons la Zone d'Arosa comme une unité tectonostratigraphique prise entre l'Austro-alpin et le Pennique. Elle constitue une zone étroite et fortement imbriquée composée aussi bien de roches ophiolitiques du Sud-Pennique et de roches sédimentaires, que de blocs et d'écaillés de l'Austro-alpin.

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A stabilization procedure for the differential equations of the symmetric gyroscope including perturbing torques

This paper shows that for the free symmetric top a formulation of the equations of motion is possible, which is Liapunov stable. The formalism applied is equivalent to the conservative stabilization of the Keplerian problem. The perturbed problem appears in -stable form. This stabilization procedure could be useful in celestial mechanics, if the gyroscopic motion of a satellite is considered and one is interested in the exact position of the angles.     

Origin of phlogopite-orthopyroxene inclusions in chromites from the Merensky Reef of the Bushveld Complex,South Africa

About 30% of the chromite grains of variable sizes in a chromitite seam at the base of the Merensky Reef of the Bushveld Complex on the farm Vlakfontein contain abundant composite mineral inclusions. The inclusions are polygonal to circular with radial cracks that protrude into the enclosing chromite. They vary from a few microns to several millimeters in diameter and are concentrated in the cores and mantles of chromite crystals. Electron backscattered patterns indicate that the host chromites are single crystals and not amalgamations of multiple grains. Na-phlogopite and orthopyroxene are most abundant in the inclusions. Edenitic hornblende, K-phlogopite, oligoclase and quartz are less abundant. Cl-rich apatite, rutile, zircon and chalcopyrite are present at trace levels. Na-phlogopite is unique to the inclusions; it has not been found elsewhere in the Bushveld Complex. Other minerals in the inclusions are also present in the matrix of the chromitite seam, but their compositions are different. The Mg/(Mg+Fe²⁺) ratios of orthopyroxene in the inclusions are slightly higher than those of orthopyroxene in the matrix. K-phlogopite in the inclusions contains more Na than in the matrix. The average compositions of the inclusions are characterized by high MgO (26 wt%), Na₂O (2.4 wt%) and H₂O (2.6 wt%), and low CaO (1.1 wt%) and FeO (4.4 wt%). The δ¹⁸O value of the trapped melt, estimated by analysis of inclusion-rich and inclusion-poor chromites, is ∼7‰. This value is consistent with the previous estimates for the Bushveld magma and with the δ¹⁸O values of silicate minerals throughout the reef. The textural features and peculiar chemical compositions are consistent with entrapment of orthopyroxene with variable amounts of volatile-rich melts during chromite crystallization. The volatile-rich melts are thought to have resulted from variable degrees of mixing between the magma on the floor of the chamber and Na-K-rich fluids expelled from the underlying crystal pile. The addition of fluid to the magma is thought to have caused dissolution of orthpyroxene, leaving the system saturated only in chromite. Both oxygen and hydrogen isotopic values are consistent with the involvement of a magmatic fluid in the process of fluid addition and orthopyroxene dissolution. Most of the Cr and Al in the inclusions was contributed through wall dissolution of the host chromite. Dissolution of minor rutile trapped along with orthopyroxene provided most of the Ti in the inclusions. The Na- and K-rich hydrous silicate minerals in the inclusions were formed during cooling by reaction between pyroxene and the trapped volatile-rich melts.     

Synergy of satellite remote sensing and numerical modeling for monitoring of suspended particulate matter

Monitoring and modeling of the distribution of suspended particulate matter (SPM) is an important task, especially in coastal environments. Several SPM models have been developed for the North Sea. However, due to waves in shallow water and strong tidal currents in the southern part of the North Sea, this is still a challenging task. In general there is a lack of measurements to determine initial distributions of SPM in the bottom sediment and essential model parameters, e.g., appropriate exchange coefficients. In many satellite-borne ocean color images of the North Sea a plume is visible, which is caused by the scattering of light at SPM in the upper ocean layer. The intensity and length of the plume depends on the wave and current climate. It is well known that the SPM plume is especially obvious shortly after strong storm events. In this paper a quasi-3-D and a 3-D SPM transport model are presented. Utilizing the synergy of satellite-borne ocean color data with numerical models, the vertical exchange coefficients due to currents and waves are derived. This results in models that for the first time are able to reproduce the temporal and spatial evolution of the plume intensity. The SPM models consist of several modules to compute ocean dynamics, the vertical and horizontal exchange of SPM in the water column, and exchange processes with the seabed such as erosion, sedimentation, and resuspension. In the bottom layer, bioturbation via benthos and diffusion processes is taken into account.Responsible Editor: Jörg-Olaf Wolff     

Stratigraphie rezenter Tiefseesedimente auf Grund der Foraminiferenfauna

Ohne ZusammenfassungKurzer Bericht über den Vortrag auf der Versammlung der Geologischen Vereinigung in Frankfurt a. M. am 8. Jan. 1938.     

Time-series of surface water CO2 and oxygen measurements on a platform in the central Arkona Sea (Baltic Sea): Seasonality of uptake and release

High resolution measurements of carbon dioxide and oxygen were made in surface waters of the central Arkona Sea (Baltic Sea) from May 2003 to September 2004. Sensors for CO₂ partial pressure (pCO₂^w) and oxygen (O₂) concentration were mounted in 7 m depth on a moored platform which is used for hydrographic and meteorological monitoring. The pCO₂^w data were obtained in half hour intervals and O₂ was measured each hour as an average of a 10 min measurement. To check the performance of the sensors, pCO₂^w and O₂ were determined by shipboard measurements on a research vessel which visited the site in 1–2 month intervals. In addition, pCO₂^w was measured on a “volunteer observing ship” (VOS) passing the platform each second day at a distance of about 25 km. Minima of 220 to 250 μatm of pCO₂^w were observed at the time of the spring bloom and a cyanobacteria bloom in mid-summer. During winter the pCO₂^w was mostly close to equilibrium with the atmosphere but maxima of 430 to 530 μatm were also observed. The seasonality of oxygen and pCO₂^w showed an opposing pattern. From a multiple regression analysis, we concluded that two processes primarily controlled pCO₂^w during our study: biological turnover and mixing. A parameterization, based on apparent oxygen utilisation (AOU) and salinity (S) only (pCO₂^w = 1.23 AOU + 43 S), reproduced the seasonality of pCO₂^w in surface water reasonably well. Based on our pCO₂, salinity, and temperature data set, we attempted to separate processes changing total inorganic carbon concentrations (C_T) by using an alkalinity–salinity relation for the area. The contribution of CO₂ gas exchange and mixing were calculated and from this the biological turnover was deduced to reveal the calculated C_T changes.The net annual uptake of CO₂ in the central Arkona Sea was estimated to be about 1.5 Tg (1.5·10¹² g) which was approximately balanced by a net oxygen release considering the uncertainties of the flux calculations. Near-coast CO₂ emission due to episodic upwelling partly compensated the uptake of the central part of the Arkona Sea reducing the overall magnitude of the CO₂ uptake.     

Der Einfluß von Entmischung und Oxydation auf die magnetischen Eigenschaften der Titanomagnetite in Basalten bei 250° und 350 °C

Zusammenfassung An zwei typischen Basalten der Göttinger Umgebung wird untersucht, wie sich die magnetischen Größen nach Erhitzung verändert haben. Die magnetischen Materialeigenschaften: Sättigungsmagnetisierung, Curie-Punkt und magnetische Anfangssuszeptibilität zeigen systematische Veränderungen. Aus licht- und elektronenoptischen Untersuchungen folgt, daß Entmischungsstrukturen allein nicht als Erklärung hierfür angesehen werden können. Der entscheidende Prozeß scheint die Tieftemperaturoxydation von Fe²⁺ zu sein, die bei den gewählten Temperaturen 250 und 350° C eine Folge der Abgabe von Kristallwasser ist.Eine bei denselben Temperaturen erzeugte isothermale Remanenz zeigt starke Abhängigkeit von der Dauer der Erhitzung. In einzelnen Fällen ergab sich eine inverse Magnetisierung, die allerdings nicht stabil war.Teilzusammenfassungen, die mehr ins einzelne gehen, finden sich auf den S. 334 und 345.

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The magnetic behaviour of two typical basalts of the Göttingen area after heat treatment is studied. The magnetic characteristic properties: saturation magnetization, Curie Point and magnetic susceptibility change systematically. Application of light — and electronoptical methods shows that exsolution structures alone cannot be responsible for these changes. The most important process seems to be the low-temperature-oxidation of Fe²⁺ which (at the chosen temperatures of 250 °C and 350 °C) is caused by loss of crystal water.An isothermal remanent magnetization (IRM), which is produced at the same temperature, shows a pronounced dependance on the duration of heating. A few experiments produced an inverse IRM which, however, was not stable.More detailed, partial summaries will be found on pages 334 and 345.