Gedenktage     

Walter Stein 《Ocean Dynamics》1965,18(3):130-132

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Geochemistry, tectonic setting and geodynamic significance of late orogenic dikes in the Melibocus Massif, Bergsträsser Odenwald     

U. Altenberger  R. Oberhänsli  E. Stein  M. Moghni 《Mineralogy and Petrology》2001,72(1-3):209-228

Summary The Melibocus Massif forms a tonalite pluton in the W’ Bergstr?sser Odenwald, which is interpreted as part of a magmatic arc of Devonian to Carboniferous age. Dikes of various compositions intrude frequently this tonalite. Different dike-lithologies are associated with different strike directions. Most dikes show evidence of high-temperature shearing. A probable maximum paleostress direction of ca. 060° can be estimated, i.e. nearly parallel to the known Variscan subduction zone in the Northwest. Due to their ductile deformation under conditions around the Ar-closing temperature of amphibole, intrusion likely occurred during the Carboniferous (Mississippian). The gabbroic to dioritic dikes (malchites) have calc-alkaline composition. Comparison with modern analogues suggests subduction-related arc magmatism. Rare earth element distributions indicate more than 5% partial melting of the mantle source with limited amounts of residual garnet. In contrast to the tonalite pluton the granitoid dikes (alsbachites) are of S-type origin, as indicated by primary muscovite and chemical composition. This requires involvement of continental material in the dike’s source rather than in the tonalite host rock’s source. The trace element chemistry of these dikes indicates magma formation in a convergent plate tectonic situation, i.e. a magmatic arc regime. Therefore, the dikes are probably the late part of the same subduction-related magmatism, which produced the tonalitic and other plutons of the Bergstr?sser Odenwald. In contrast to the large pluton-forming magmas, formation of the dikes during late or post-collisional extension or transtension followed by a phase of compression or transpression is probable.

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Zusammenfassung Geochemie, tektonische Stellung und geodynamische Signifikanz sp?torogener G?nge im Melibocus Massiv, Bergstr?sser Odenwald Der Melibokus Tonalit-Pluton geh?rt zum Bergstr?sser Odenwald, der als Teil eines devonisch-karbonischen magmatischen Bogens interpretiert wird. In diesem Pluton treten sehr h?ufig magmatische G?nge unterschiedlicher Zusammensetzung auf. Die Arbeit zeigt, dass die G?nge unterschiedlicher Zusammensetzung unterschiedliche Streichrichtungen haben. Die meisten der untersuchten G?nge zeigen Hochtemperatur-Schergefüge. Aus der Lage der zerscherten G?nge l?sst sich eine Pal?ostressrichtung mit 060° für Sigma 1 ableiten. Diese Richtung weicht nur unwesentlich von der bekannten variskischen Subduktionszone im Nordwesten ab. Aufgrund ihrer Hochtemperatur-Gefüge, die im Bereich der Schlie?ungstemperatur von Ar in Hornblenden gebildet wurden, ist das Alter der G?nge wahrscheinlich ebenfalls als Karbon (Mississippian) einzustufen. Die gabbroiden bis dioritischen G?nge (Malchite) haben eine kalkalkaline Zusammensetzung. Der Vergleich mit rezenten Magmatiten deutet auf eine Entstehung in einem magmatischen Bogen (Kontinentalrand) hin. Die Seltenerdelementverteilung der G?nge zeigt einen wahrscheinlichen Aufschmelzungsgrad der Mantelquellregion von über 5% bei einem geringen Anteil von residualem Granat an. Im Gegensatz zu den tonalitischen Nebengesteinen zeigen die granitoiden G?nge anhand ihrer modalen (Muskovit) als auch chemischen Zusammensetzung S-Typ-Charakter. Dies bedeutet eine h?here Beteiligung krustaler Komponente in der Magmenquelle als dies für den Tonalit angenommen werden darf. Die Spurenelementchemie der granitoiden G?nge zeigt ebenfalls eine Bildung in einem konvergenten plattentektonischen Regime, d.h. innerhalb eines magmatischen Bogens. Die G?nge stellen somit vermutlich das Produkt eines sp?ten Abschnittes des subduktionsbezogenen Magmatismus, der auch die Tonalite und andere Plutone im zentralen Bergstr?sser Odenwald geschaffen hat, dar. Im Gegensatz zu dem Magmatismus der die Plutone erzeugt hat, sind die G?nge wahrscheinlich gegen Ende der Kollision oder nachfolgend auf diese in eine sich dehnende Kruste intrudiert und in einem nachfolgenden kompressiven Regime deformiert worden.

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Received August 31, 1999; revised version accepted October 9, 2000  相似文献   

The magnetic effects of brecciation and shock in meteorites: III. The achondrites     

Aviva Brecher  Miriam Fuhrman  Judy Stein 《Earth, Moon, and Planets》1979,20(3):265-279

We present results of a magnetic survey of achondritic meteorites, representing the aubrites (A), diogenites (D), Irowardites (H), and eucrites (E) groups and relate their magnetic behavior to respective class characteristics and models of origin.Magnetic susceptibility (x) values cluster well within each group and decrease systematically between groups (from 2 to 0.1×10^–3GOe^–1 cm^–3), with the average metal contents, (from 1 to <0.1 wt%) in the above order. The natural remanent magnetization (NRM) values range broadly within each group, but group averages decrease roughly as above. However, the considerable within-sample and intra-group variability in NRM level and its demagnetization characteristics attest to inhomogeneous and localized brecciation effects. Although petrological-chemical studies resolve a primary component of magmatic differentiation on the planetoid of origin, no clear magnetic record of such event has been preserved. The magnetization of achondrites is mainly the product of their complex, multi-stage impact brecciation and metamorphism history, in accord with other lines of evidence.The magnetic behavior of achondrites is remarkably similar to that characteristic of lunar breccias and impact-melt rocks and reinforces their analogous mode of genesis, as brought out by chemical and petrographic analyses.  相似文献   

Postglacial uplift and relative sea level changes in Finnmark,northern Norway     

Anders Romundset  Stein Bondevik  Ole Bennike 《Quaternary Science Reviews》2011,30(19-20):2398-2421

The outer coast of Finnmark in northern Norway is where the former Fennoscandian and Barents Sea ice sheets coalesced. This key area for isostatic modelling and deglaciation history of the ice sheets has abundant raised shorelines, but only a few existing radiocarbon dates constrain their chronology. Here we present three Holocene sea level curves based on radiocarbon dated deposits from isolation basins at the outermost coast of Finnmark; located at the islands Sørøya and Rolvsøya and at the Nordkinn peninsula. We analysed animal and plant remains in the basin deposits to identify the transitions between marine and lacustrine sediments. Terrestrial plant fragments from these transitions were then radiocarbon dated. Radiocarbon dated mollusk shells and marine macroalgae from the lowermost deposits in several basins suggest that the first land at the outer coast became ice free around 14,600 cal yr BP. We find that the gradients of the shorelines are much lower than elsewhere along the Norwegian coast because of substantial uplift of the Barents Sea. Also, the anomalously high elevation of the marine limit in the region can be attributed to uplift of the adjacent seafloor. After the Younger Dryas the coast emerged 1.6–1.0 cm per year until about 9500–9000 cal yr BP. Between 9000 and 7000 cal yr BP relative sea level rose 2–4 m and several of the studied lakes became submerged. At the outermost locality Rolvsøya, relative sea level was stable at the transgression highstand for more than 3000 years, between ca 8000 and 5000 cal yr BP. Deposits in five of the studied lakes were disturbed by the Storegga tsunami ca 8200–8100 cal yr BP.  相似文献   

Three‐dimensional modeling of problems in poro‐elasticity via a mixed least‐squares method using linear tetrahedral elements     

Maria Tchonkova  John Peters  Stein Sture 《国际地质力学数值与分析法杂志》2011,35(15):1656-1681

In a previous publication we developed a new mixed least‐squares method for poro‐elasticity. The approximate solution was obtained via a minimization of a least‐squares functional, based upon the equations of equilibrium, the equations of continuity and weak forms of the constitutive relationships for elasticity and Darcy flow. The formulation involved four independent types of variables: displacements, stresses, pore pressures and velocities. All of them were approximated by linear continuous triangles. Encouraged by the computational results, obtained from the two‐dimensional implementation of the method, we extended our formulation to three dimensions. In this paper we present numerical examples for the performance of continuous linear tetrahedra within the context of the mixed least‐squares method. The initial results suggest that the method works well in the nearly and entirely incompressible limits for elasticity. For poro‐elasticity, the obtained pore pressures are stable without exhibiting the oscillations, which are observed when the standard Galerkin formulation is used. Copyright © 2010 John Wiley & Sons, Ltd.  相似文献   

Nonlinear output constraints handling for production optimization of oil reservoirs     

Eka Suwartadi  Stein Krogstad  Bjarne Foss 《Computational Geosciences》2012,16(2):499-517

Adjoint-based gradient computations for oil reservoirs have been increasingly used in closed-loop reservoir management optimizations. Most constraints in the optimizations are for the control input, which may either be bound constraints or equality constraints. This paper addresses output constraints for both state and control variables. We propose to use a (interior) barrier function approach, where the output constraints are added as a barrier term to the objective function. As we assume there always exist feasible initial control inputs, the method maintains the feasibility of the constraints. Three case examples are presented. The results show that the proposed method is able to preserve the computational efficiency of the adjoint methods.  相似文献   

Paired uraninite and molybdenite dating of the K?nigshain granite: implications for the onset of late-Variscan magmatism in the Lausitz Block     

Hans-Jürgen F?rster  Dieter Rhede  Holly J. Stein  Rolf L. Romer  Gerhard Tischendorf 《International Journal of Earth Sciences》2012,101(1):57-67

We present geochronological data for late-Variscan magmatism in the Lausitz Block of the Saxo-Thuringian Zone, Germany. The Th–U–total Pb age of uraninite and the Re–Os age of molybdenite from the composite biotite–monzogranite pluton of K?nigshain overlap at the 2σ confidence limit: 328.6 ± 1.9 Ma (uraninite), and 327.0 ± 1.3 Ma and 327.6 ± 1.3 Ma (molybdenite), indicating that crystallization of magmatic uraninite and deposition of molybdenite were nearly contemporaneous. These data imply that magmatic processes in this part of the Variscan orogen already started in latest Visean time, about 10 Ma earlier than previously assumed (315–320 Ma). The new ages correspond to ages for plutonic rocks in the Elbe Zone immediately west of the Lausitz (around 335–325 Ma) and the bulk of late-Variscan igneous rocks in the Saxo-Thuringian Zone (335–320 Ma).  相似文献   

Grid adaptation for the Dirichlet–Neumann representation method and the multiscale mixed finite-element method     

Knut-Andreas Lie  Jostein R. Natvig  Stein Krogstad  Yahan Yang  Xiao-Hui Wu 《Computational Geosciences》2014,18(3-4):357-372

A Dirichlet–Neumann representation method was recently proposed for upscaling and simulating flow in reservoirs. The DNR method expresses coarse fluxes as linear functions of multiple pressure values along the boundary and at the center of each coarse block. The number of flux and pressure values at the boundary can be adjusted to improve the accuracy of simulation results and, in particular, to resolve important fine-scale details. Improvement over existing approaches is substantial especially for reservoirs that contain high-permeability streaks or channels. As an alternative, the multiscale mixed finite-element (MsMFE) method was designed to obtain fine-scale fluxes at the cost of solving a coarsened problem, but can also be used as upscaling methods that are flexible with respect to geometry and topology of the coarsened grid. Both methods can be expressed in mixed-hybrid form, with local stiffness matrices obtained as “inner products” of numerically computed basis functions with fine-scale sub-resolution. These basis functions are determined by solving local flow problems with piecewise linear Dirichlet boundary conditions for the DNR method and piecewise constant Neumann conditions for MsMFE. Adding discrete pressure points in the DNR method corresponds to subdividing faces in the coarse grid and hence increasing the number of basis functions in the MsMFE method. The methods show similar accuracy for 2D Cartesian cases, but the MsMFE method is more straightforward to formulate in 3D and implement for general grids.  相似文献   

Excitation of solar-like oscillations: From PMS to MS stellar models     

R. Samadi  M. -J. Goupil  E. Alecian  F. Baudin  D. Georgobiani  R. Trampedach  R. Stein  å. Nordlund 《Journal of Astrophysics and Astronomy》2005,26(2-3):171-184

The amplitude of solar-like oscillations results from a balance between excitation and damping. As in the sun, the excitation is attributed to turbulent motions that stochastically excite thep modes in the uppermost part of the convective zone. We present here a model for the excitation mechanism. Comparisons between modeled amplitudes and helio and stellar seismic constraints are presented and the discrepancies discussed. Finally the possibility and the interest of detecting such stochastically excited modes in pre-main sequence stars are also discussed.  相似文献   

Accumulation of particulate organic carbon at the Eurasian continental margin during late Quaternary times: controlling mechanisms and paleoenvironmental significance     

R. Stein  B. Boucsein  K. Fahl  T. Garcia de Oteyza  J. Knies  F. Niessen 《Global and Planetary Change》2001,31(1-4)

Data on the amount and composition of organic carbon were determined in sediment cores from the Kara and Laptev Sea continental margin, representing oxygen isotope stages 1–6. The characterization of organic matter is based on hydrogen index (HI) values, n-alkanes and maceral composition, indicating the predominance of terrigenous organic matter through space and time. The variations in the amount and composition of organic carbon are mainly influenced by changes in fluvial sediment supply, Atlantic water inflow, and continental ice sheets. During oxygen isotope stage (OIS) 6, high organic carbon contents in sediments from the Laptev Sea and western East Siberian Sea continental margin were probably caused by the increased glacial erosion and further transport in the eastward-flowing boundary current along the continental margin. During OIS 5 and early OIS 3, some increased amounts of marine organic matter were preserved in sediments east of the Lomonosov Ridge, suggesting an influence of nutrient-rich Pacific waters. During OIS 2, terrigenous organic carbon supply was increased along the Barents and western Kara Sea continental margin caused by extended continental ice sheets in the Barents Sea (Svalbard to Franz Josef Land) area and increased glacial erosion. Along the Laptev Sea continental margin, on the other hand, the supply of terrigenous (organic) matter was significantly reduced due to the lack of major ice sheets and reduced river discharge. Towards the Holocene, the amount of total organic carbon (TOC) increased along the Kara and Laptev Sea continental margin, reaching average values of up to 0.5 g C cm⁻² ky⁻¹. Between about 8 and 10 ka (9 and 11 Cal ka), i.e., during times when the inner shallow Kara and Laptev seas became largely flooded for the first time after the Last Glacial Maximum, maximum supply of terrigenous organic carbon occurred, which is related to an increase in coastal erosion and Siberian river discharge. During the last 8000 years, the increased amount of marine organic carbon preserved in the sediments from the Kara and Laptev Sea continental margin is interpreted as a result of the intensification of Atlantic water inflow along the Eurasian continental margin.  相似文献