Determination of the submerged macrophyte coverage of greifswalder bodden     

Solveig Bartels  Uwe Klüber   《Limnologica》1999,29(3):311

The extent to which a water body can support submerged macrophytic vegetation provides an indicator of its degree of eutrophication. Regular, quantitative assessment of macrophyte populations enables changes in the trophic state of the system to be observed. A combination of aerial photography and underwater videography has proved to be an efficient method for calculating macrophyte coverage of large coastal areas.  相似文献   

The Erbisberg drilling 2011: Implications for the structure and postimpact evolution of the inner ring of the Ries impact crater     

Gernot Arp  Andreas Reimer  Klaus Simon  Sebastian Sturm  Jakob Wilk  Corina Kruppa  Lutz Hecht  Bent T. Hansen  Jean Pohl  Wolf Uwe Reimold  Thomas Kenkmann  Dietmar Jung 《Meteoritics & planetary science》2019,54(10):2448-2482

The 26 km diameter Nördlinger Ries is a complex impact structure with a ring structure that resembles a peak ring. A first research drilling through this “inner crystalline ring” of the Ries was performed at the Erbisberg hill (SW Ries) to better understand the internal structure and lithology of this feature, and possibly reveal impact‐induced hydrothermal alteration. The drill core intersected the slope of a 22 m thick postimpact travertine mound, before entering 42 m of blocks and breccias of crystalline rocks excavated from the Variscan basement at >500 m depth. Weakly shocked gneiss blocks that show that shock pressure did not exceed 5 GPa occur above polymict lithic breccias of shock stage Ia (10–20 GPa), with planar fractures and planar deformation features (PDFs) in quartz. Only a narrow zone at 49.20–50.00 m core depth exhibits strong mosaicism in feldspar and {102} PDFs in quartz, which are indicative of shock stage Ib (20–35 GPa). Finally, 2 m of brecciated Keuper sediments at the base of the section point to an inverse layering of strata. While reverse grading of clast sizes in lithic breccias and gneiss blocks is consistent with lateral transport, the absence of diaplectic glass and melt products argues against dynamic overthrusting of material from a collapsing central peak, as seen in the much larger Chicxulub structure. Indeed, weakly shocked gneiss blocks are rather of local provenance (i.e., the transient crater wall), whereas moderately shocked polymict lithic breccias with geochemical composition and ⁸⁷Sr/⁸⁶Sr signature similar to Ries suevite were derived from a position closer to the impact center. Thus, the inner ring of the Ries is formed by moderately shocked polymict lithic breccias likely injected into the transient crater wall during the excavation stage and weakly shocked gneiss blocks of the collapsing transient crater wall that were emplaced during the modification stage. While the presence of an overturned flap is not evident from the Erbisberg drilling, a survey of all drillings at or near the inner ring point to inverted strata throughout its outer limb. Whether the central ring of the Ries represents remains of a collapsed central peak remains to be shown. Postimpact hydrothermal alteration along the Erbisberg section comprises chloritization, sulfide veinlets, and strong carbonatization. In addition, a narrow zone in the lower parts of the polymict lithic breccia sequence shows a positive Eu anomaly in its carbonate phase. The surface expression of this hydrothermal activity, i.e., the travertine mound, comprises subaerial as well as subaquatic growth phases. Intercalated lake sediments equivalent to the early parts of the evolution of the central crater basin succession confirm a persistent impact‐generated hydrothermal activity, although for less time than previously suggested.  相似文献   

Objektive Analyse ozeanographischer Daten mit orthogonalen Polynomflächen     

Uwe Paul 《Ocean Dynamics》1994,46(1):29-60

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Time-dependent greenhouse warming computations with a coupled ocean-atmosphere model     

Ulrich Cubasch  Klaus Hasselmann  Heinke Höck  Ernst Maier-Reimer  Uwe Mikolajewicz  Benjamin D Santer  Robert Sausen 《Climate Dynamics》1992,8(2):55-69

Climate changes during the next 100 years caused by anthropogenic emissions of greenhouse gases have been simulated for the Intergovernmental Panel on Climate Change Scenarios A (business as usual) and D (accelerated policies) using a coupled ocean-atmosphere general circulation model. In the global average, the near-surface temperature rises by 2.6 K in Scenario A and by 0.6 K in Scenario D. The global patterns of climate change for both IPCC scenarios and for a third step-function 2 x CO₂ experiment were found to be very similar. The warming delay over the oceans is larger than found in simulations with atmospheric general circulation models coupled to mixed-layer models, leading to a more pronounced land-sea contrast and a weaker warming (and in some regions even an initial cooling) in the Southern Ocean. During the first forty years, the global warming and sea level rise due to the thermal expansion of the ocean are significantly slower than estimated previously from box-diffusion-upwelling models, but the major part of this delay can be attributed to the previous warming history prior to the start of present coupled ocean-atmosphere model integration (cold start).  相似文献   

Assessing climate persistence from climatic ‘noise’     

Uwe Radok 《Climatic change》1992,20(2):155-167

Changes in climate are generally defined as differences between means. The autocorrelation usually encountered in geophysical series and the implied persistence, or reduced number of independent observations, tend to render significance tests of mean differences inconclusive until a considerable amount of data has accumulated, by which time a climatic change could be well under way. A more efficient alternative approach is provided by small-sample variances. Under slightly idealized conditions their frequency distribution is of the chi-square type with a number of degrees of freedom that measures the persistence in the series and can be monitored on a short time scale with a sequential sampling procedure.Also at homein CIRES, Campus Box 449, University of Colorado, Boulder, CO 80309, U.S.A.  相似文献   

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

Uwe Ring  Lothar Ratschbacher  Wolfgang Frisch  Sören DÜrr  Susanne Borchert 《International Journal of Earth Sciences》1990,79(3):725-739

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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Secular variation of calcium carbonate mineralogy; an evaluation of ooid and micrite chemistries     

Nicholas R. Bates  Uwe Brand 《International Journal of Earth Sciences》1990,79(1):27-46

Three ooid types are recognized from the Lower Tournaisian »Kohlenkalk« shelf facies at Velbert, Germany. Ooids from this unit have a predominantly concentric laminae fabric. Radial-concentric and small radial fibrous ooids are minor components to this oolite. The diagenetic response of Kohlenkalk ooid chemistry is significantly different from that observed in contemporaneous crinoid and brachiopod material. Fabric evidence suggests that radial-concentric and radial-fibrous ooids were probably originally aragonite/high-Mg calcite and high-Mg calcite respectively. Fabric and trace elemental chemistries of the concentric fabric ooids suggests that they were originally precipitated as aragonite and subsequently altered to low-Mg calcite.Recent papers have proposed temporal shifts in the dominant mineralogy of shallow marine non-skeletal carbonates between calcite and aragonite. Changing Phanerozoic atmospheric pCO₂ levels and oceanic Mg/Ca ratios may have been factors controlling the dominant mineralogy. The chemistries of the Kohlenkalk ooids in conjunction with other ooid and micrite data spanning the Mid-Paleozoic to Recent are evaluated in context with these temporal shifts between »calcite« and »aragonite seas«. The strontium chemistries of the ooids (¯x = 1010 ppm, range 145–3010 ppm) and micrites (¯x = 841 ppm, range 3–8800 ppm) suggests they had an aragonite precursor mineralogy. No statistical correlation was observed between ooid/micrite chemistries, their mineralogies and the proposed secular trend. Therefore, we suggest that aragonitic ooids and micrites were dominant components of shallow-marine carbonate environments throughout the Phanerozoic. The distribution and abundance of aragonitic and calcitic ooids in the geologic past was probably dependant on local hydraulic, physicochemical, and environmental conditions, areally constrained by global tectonics, eustatic, climatic and atmospheric effects, with significant diagenetic overprinting of the original geochemical and fabric information.

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Zusammenfassung In der Kohlenkalk-Schelffazies des Untertournais bei Velbert (Bundesrepublik Deutschland) lassen sich drei Ooidtypen unterscheiden. Gemeinsam ist diesen Ooiden ein vorwiegend konzentrischer Lagenbau. Dagegen ist das Vorkommen radial-konzentrischer und radial-fibröser Ooide minimal. Die diagenetische Entwicklung der Kohlenkalkooide ist hinsichtlich ihrer chemischen Zusammensetzung deutlich von gleichalten Crinoiden- oder Brachiopodenmaterial zu unterscheiden. Strukturelle Beobachtungen lassen darauf schließen, daß radial-konzentrische und radial-fibröse Ooide ursprünglich aus Aragonit/Hoch-Mg-Calcit bzw. Hoch-Mg-Calcit bestanden. Die Zusammensetzung der Spurenelemente und die Struktur der konzentrisch aufgebauten Ooide hingegen deutet auf eine Fällung von Aragonit, der im Laufe der Diagenese zu Niedrig-Mg-Calcit umgewandelt wurde.In letzter Zeit wurde in einigen Veröffentlichungen die These vertreten, daß die Mineralogie von nicht-skelett Karbonaten zwischen Calcit und Aragonit in unbekannten Intervallen wechselt. Wechsel des atmosphärischen CO₂ Drucks und des Mg/Ca Verhältnisses in den Ozeanen während des Phanerozoikums könnten Vorgänge sein, die die vorherrschende Mineralogie dieser Karbonate beeinflussen. In dieser Arbeit wird der Chemismus der Kohlenkalkooide in Verbindung mit anderen Ooiden und Daten über Mikrite des Mittelpaläozoikums bis heute in bezug auf den Wechsel zwischen »Calcit«- und »Aragonit-Ozeanen« diskutiert. Der Strontiumgehalt der Ooide (¯x = 1010 ppm, Spannbreite: 145–3010 ppm) und der Mikrite (¯x = 841 ppm, Spannbreite: 3–8800 ppm) spricht für eine primäre Aragonitfällung. Zwischen der Ooid/Mikrit Chemie und ihrer Mineralogie gab es keine mögliche statistische Korrelation. Daraus schließen wir, daß während des ganzen Phanerozoikums aragonitische Ooide und mikrite große Bedeutung in flachmarinen Schelfregionen mit Karbonatsedimentation hatten und haben. Das Vorkommen aragonitischer und calcitischer Ooide ist wahrscheinlich an hydraulische und physiko-chemische Vorgänge gebunden, die auf globale Tektonik, eustatische-, klimatische- und atmosphärische Veränderungen zurückzuführen sind. Diese führten dazu, daß die ursprüngliche Geochemie und Struktur diagenetisch verändert wurde.

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Résumé Parmi les facies de plate-forme du Tournaisien inférieur, dans le calcaire carbonifère de Velbert (RFA), on distingue trois types d'ooïdes: les plus abondantes présentent une structure lamellaire concentrique; d'autres, en quantité subordonnée, sont radiaires-concentriques et fibro-radiées. En réponse à leur chimisme, les ooïdes du calcaire carbonifère ont connu une évolution diagénétique nettement différente de celle des sédiments à crinoïdes et à brachiopodes de même âge. L'organisation structurale des ooides radiaires-concentriques et fibro-radiées indique que'elles étaient constituées respectivement d'aragonite + calcite magnésienne et de calcite magnésienne. Par contre, la structure et le chimisme des éléments en traces des ooïdes concentriques suggèrent qu'elles ont été d'abord précipitées en aragonite et transformées ensuite en calcite pauvre en Mg.Selon certains travaux récents, la composition minéralogique des sédiments carbonatés non organo-détritiques aurait fluctué au cours du temps entre l'aragonite et la calcite. Des factures déterminants de ce processus auraient pû être les changements, au cours du Phanérozoïque, de pCO₂ dans l'atmosphère et du rapport Mg/Ca dans les océans. Le chimisme des ooïdes du calcaire carbonifère, comparé à celui de micrites et d'autres ooïdes d'âges phanérozoïque moyen à récent est examiné en relation avec ces passages de «mers à calcite» à «mer à aragonite» au cours du temps. Le chimisme du Sr des ooïdes (x = 1010 ppm; intervalle 145–3010 ppm) et des micrites (x = 841 ppm; intervalle 3–8800 ppm) suggère une précipitation primaire d'aragonite. Il n'apparaît aucune corrélation statistique entre le chimisme des ooïdes et micrites, leur minéralogie, et les fluctuations temporelles suggérées. Pour ces raisons, nous pensons que les ooïdes et micrites aragonitiques ont été les composants dominants des milieux carbonatés peu profonds pendant tout le Phanérozoïque. L'abondance et la répartition des ooïdes aragonitiques et calcitiques dans la nature ancienne ont vraisemblablement résulté de conditions locales hydrauliques, physico-chimiques et d'environnement, déterminées par la tectonique globale, et par les changements eustatiques, climatiques ou atmosphériques, qui ont surimposé leur empreinte diagénetique aux caractères structuraux et géochimiques primaires.

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Temperature dependence of the water-ice spectrum between 1 and 4 microns: Application to Europa,Ganymede and Saturn's rings     

Uwe Fink  Harold P. Larson 《Icarus》1975,24(4):411-420

Reflection spectra of water ice from 1 to 4 μm are presented as a function of temperature. It is found that a feature at 6056 cm^?1 changes its intensity sufficiently that it can be used as a spectroscopic measure of the ice temperature. A temperature calibration curve of this feature down to 55 K is developed and is used to determine ice temperatures for the Galilean satellites Europa (95±10 K), Ganymede (103±10 K), and the rings of Saturn (80±5 K). The ice temperatures for the Galilean satellites are lower than their measured brightness temperatures, which can be explained by a higher albedo of the ice covered regions relative to the rest of the satellite and possibly a concentration of the ice near the polar caps.  相似文献   

Vertical gradient of nutrients in two dimictic lakes – influence of phototrophic sulfur bacteria on nutrient balance     

Uwe?SeligEmail author  Thomas?Hübener  Reinhard?Heerkloss  Hendrik?Schubert 《Aquatic Sciences - Research Across Boundaries》2004,66(3):247-256

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Nesseltalgraben,a new reference section of the last glacial period in southern Germany     

Christoph Mayr  Birgit Brandlmeier  Volker Diersche  Philipp Stojakowits  Uwe Kirscher  Renate Matzke-Karasz  Valerian Bachtadse  Michael Eigler  Ulrich Haas  Bernhard Lempe  Paula J. Reimer  Christoph Spötl 《Journal of Paleolimnology》2017,57(2):213-219

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