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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Effects of juniper removal and rainfall variation on tree transpiration in a semi‐arid karst: evidence of complex water storage dynamics          下载免费PDF全文

Heather Cardella Dammeyer  Susanne Schwinning  Benjamin F. Schwartz  Georgianne W. Moore 《水文研究》2016,30(24):4568-4581

Brush removal is widely practiced as a tool for increasing groundwater recharge, but its efficacy depends greatly on the way in which the removed species interact with the hydrological system relative to the vegetation replacing it. We examined the effects of Ashe juniper removal in the recharge zone of the Edwards Aquifer, Texas, USA, a karst aquifer. The study was conducted in an Ashe juniper (Juniperus ashei)–live oak (Quercus fusiformis) woodland on a hill slope composed of rocky, shallow soils over fractured limestone bedrock. Ashe juniper is a native species that has been encroaching grasslands and savannas over the past century. In September 2008, a plot was cleared of 90% of its juniper trees. Tree transpiration, predawn water potentials and vegetation cover across the cleared plot and an adjacent reference site were measured from May 2009 to December 2011. Stand‐level tree transpiration from May 2009 to March 2010 was diminished by a severe summer drought in 2009, from which trees were slow to recover. Subsequently, tree transpiration was 5–10× higher in the woodland compared to the clearing. For all of 2011, also a drought year, tree transpiration in the woodland exceeded precipitation inputs, indicating a high capacity for water storage at the study site. However, site differences for oak trees were generally larger than for juniper trees. While juniper removal accounted for a 431 mm year^?1 difference in tree transpiration between sites, vegetation cover in the clearing increased from 42% to 90% over two years, suggesting that understory growth was increasingly compensating for the loss of juniper transpiration. We conclude that the removal of a relatively shallow‐rooted tree, when replaced with herbaceous vegetation and low shrubs, has little effect on deep recharge. By contrast, successive years of precipitation extremes may be more effective increasing recharge by lowering the water transport capacity of trees in the aftermath of severe drought. Copyright © 2016 John Wiley & Sons, Ltd.  相似文献   

Erratum to “Evidence of estuarine nursery origin of five coastal fish species along the Portuguese coast through otolith elemental fingerprints” [Estuar. Coast. Shelf Sci. 79 (2008) 317–327]     

Rita P. Vasconcelos  Patrick Reis-Santos  Susanne Tanner  Anabela Maia  Christopher Latkoczy  Detlef Günther  Maria José Costa  Henrique Cabral 《Estuarine, Coastal and Shelf Science》2009

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Detection of land subsidence in Semarang,Indonesia, using stable points network (SPN) technique   总被引：2，自引：0，他引：2  

Friedrich Kuehn  David Albiol  Geraint Cooksley  Javier Duro  Johanna Granda  Susanne Haas  Arne Hoffmann-Rothe  Dodid Murdohardono 《Environmental Earth Sciences》2010,60(5):909-921

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Large-Eddy Atmosphere–Land-Surface Modelling over Heterogeneous Surfaces: Model Development and Comparison with Measurements     

Yaping Shao  Shaofeng Liu  Jan H. Schween  Susanne Crewell 《Boundary-Layer Meteorology》2013,148(2):333-356

A model is developed for the large-eddy simulation (LES) of heterogeneous atmosphere and land-surface processes. This couples a LES model with a land-surface scheme. New developments are made to the land-surface scheme to ensure the adequate representation of atmosphere–land-surface transfers on the large-eddy scale. These include, (1) a multi-layer canopy scheme; (2) a method for flux estimates consistent with the large-eddy subgrid closure; and (3) an appropriate soil-layer configuration. The model is then applied to a heterogeneous region with 60-m horizontal resolution and the results are compared with ground-based and airborne measurements. The simulated sensible and latent heat fluxes are found to agree well with the eddy-correlation measurements. Good agreement is also found in the modelled and observed net radiation, ground heat flux, soil temperature and moisture. Based on the model results, we study the patterns of the sensible and latent heat fluxes, how such patterns come into existence, and how large eddies propagate and destroy land-surface signals in the atmosphere. Near the surface, the flux and land-use patterns are found to be closely correlated. In the lower boundary layer, small eddies bearing land-surface signals organize and develop into larger eddies, which carry the signals to considerably higher levels. As a result, the instantaneous flux patterns appear to be unrelated to the land-use patterns, but on average, the correlation between them is significant and persistent up to about 650 m. For a given land-surface type, the scatter of the fluxes amounts to several hundred W $\text{ m }^{-2}$ , due to (1) large-eddy randomness; (2) rapid large-eddy and surface feedback; and (3) local advection related to surface heterogeneity.  相似文献   

High Resolution Simulation of the Variability of Surface Energy Balance Fluxes Across Central London with Urban Zones for Energy Partitioning     

Thomas Loridan  Fredrik Lindberg  Oriol Jorba  Simone Kotthaus  Susanne Grossman-Clarke  C. S. B. Grimmond 《Boundary-Layer Meteorology》2013,147(3):493-523

The parameterization of surface heat-flux variability in urban areas relies on adequate representation of surface characteristics. Given the horizontal resolutions (e.g. $\approx $ 0.1–1 km) currently used in numerical weather prediction (NWP) models, properties of the urban surface (e.g. vegetated/built surfaces, street-canyon geometries) often have large spatial variability. Here, a new approach based on Urban Zones to characterize Energy partitioning (UZE) is tested within a NWP model (Weather Research and Forecasting model; WRF v3.2.1) for Greater London. The urban land-surface scheme is the Noah/Single-Layer Urban Canopy Model (SLUCM). Detailed surface information (horizontal resolution 1 km) in central London shows that the UZE offers better characterization of surface properties and their variability compared to default WRF-SLUCM input parameters. In situ observations of the surface energy fluxes and near-surface meteorological variables are used to select the radiation and turbulence parameterization schemes and to evaluate the land-surface scheme and choice of surface parameters. For radiative fluxes, improved performance (e.g. $>$ 25 W m $^{-2}$ root-mean-square error reduction for the net radiation) is attained with UZE parameters compared to the WRF v3.2.1 default for all three methods from the simplest to the most detailed. The UZE-based spatial fluxes reproduce a priori expectations of greater energy storage and less evaporation in the dense city centre compared to the residential surroundings. Problems in Noah/SLUCM partitioning of energy between the daytime turbulent fluxes are identified with the overestimation of the turbulent sensible heat and underestimation of the turbulent latent heat fluxes.  相似文献   

Igneous and shock processes affecting chassignite amphibole evaluated using chlorine/water partitioning and hydrogen isotopes          下载免费PDF全文

Paul A. Giesting  Susanne P. Schwenzer  Justin Filiberto  Natalie A. Starkey  Ian A. Franchi  Allan H. Treiman  Andy G. Tindle  Monica M. Grady 《Meteoritics & planetary science》2015,50(3):433-460

Amphibole in chassignite melt inclusions provides valuable information about the volatile content of the original interstitial magma, but also shock and postshock processes. We have analyzed amphibole and other phases from NWA 2737 melt inclusions, and we evaluate these data along with published values to constrain the crystallization Cl and H₂O content of phases in chassignite melt inclusions and the effects of shock on these amphibole grains. Using a model for the Cl/OH exchange between amphibole and melt, we estimate primary crystallization OH contents of chassignite amphiboles. SIMS analysis shows that amphibole from NWA 2737 currently has 0.15 wt% H₂O. It has lost ~0.6 wt% H₂O from an initial 0.7–0.8 wt% H₂O due to intense shock. Chassigny amphibole had on average 0.3–0.4 wt% H₂O and suffered little net loss of H₂O due to shock. NWA 2737 amphibole has δD ≈ +3700‰; it absorbed Martian atmosphere‐derived heavy H in the aftermath of shock. Chassigny amphibole, with δD ≤ +1900‰, incorporated less heavy H. Low H₂O/Cl ratios are inferred for the primitive chassignite magma, which had significant effects on melting and crystallization. Volatiles released by the degassing of Martian magma were more Cl‐rich than on Earth, resulting in the high Cl content of Martian surface materials.  相似文献   

Clay mineralogy of a red clay–loess sequence from Lingtai, the Chinese Loess Plateau     

Susanne Gylesj  Eve Arnold 《Global and Planetary Change》2006,51(3-4):181-194

The Chinese Loess Plateau (CLP) comprises an extensive record of eolian deposition that contains important information about climate change. The objective of this study is to investigate if mineralogy can provide more insight into the long-term evolution of the East Asian monsoon. Comparisons between mineralogy and other paleoclimatic records (grain size and magnetic susceptibility) from the CLP have been made to evaluate the efficacy of mineralogy as a paleoclimatic tool.Here we present data from a mineralogical study of a red clay–loess sequence at Lingtai, central Chinese Loess Plateau. Changes related to source area(s), transport processes and weathering regime over time are recorded in mineral variation.Higher average concentrations of kaolinite, chlorite and quartz in the red clay, together with abrupt changes in relative mineral abundances across the red clay–loess boundary suggest a change of source area at 2.6 Ma. From 2.6 Ma to about 1.7 Ma the summer monsoon influence increases, destroying chlorite and contributing fine illite particles to the sediment. At around 1.7 Ma the mineralogy becomes relatively constant, suggesting that the monsoon was fairly stable during this period. At 0.7–0.5 Ma an increase of both summer monsoon and winter monsoon activity is inferred from illite, kaolinite, chlorite and plagioclase concentrations. Over the last 0.5 Ma mineralogy suggests an aridification of source area(s) as chlorite and plagioclase concentrations increase where illite concentration decreases. The last major change occurred around 0.07 Ma and indicates reducing summer monsoon influence as chlorite and quartz concentrations increase and illite concentration, as well as the < 2 μm size fraction, decreases. The mineralogical trends and differences between loess and paleosols units suggest different source areas in the last 0.5 Ma.  相似文献   

Clues to starburst evolution: The tale of dense gas     

Susanne Hüttemeister  Susanne Aalto 《Astrophysics and Space Science》2003,284(2):877-880

The dense gas tracers HNC and CN prove to be detectable in sensitive single dish studies of infrared luminous starburst galaxies. Their line intensity with respect to both the standard tracer of molecular gas, CO, and the dense, starforming component, HCN, varies significantly. This opens a new, extinction-free window into the investigation of the properties and the evolutionary stage of starbursts. This revised version was published online in August 2006 with corrections to the Cover Date.  相似文献   

Tectonic and climate control of oil shale deposition in the Upper Cretaceous Qingshankou Formation (Songliao Basin, NE China)   总被引：4，自引：0，他引：4  

Jianliang Jia  Zhaojun Liu  Achim Bechtel  Susanne A. I. Strobl  Pingchang Sun 《International Journal of Earth Sciences》2013,102(6):1717-1734

Oil shales were deposited in the Songliao Basin (NE China) during the Upper Cretaceous period, representing excellent hydrocarbon source rocks. High organic matter (OM) contents, a predominance of type-I kerogen, and a low maturity of OM in the oil shales are indicated by bulk geochemical parameters and biomarker data. A major contribution of aquatic organisms and minor inputs from terrigenous land plants to OM input are indicated by n-alkane distribution patterns, composition of steroids, and organic macerals. Strongly reducing bottom water conditions during the deposition of the oil shale sequences are indicated by low pristane/phytane ratios, high C₁₄-aryl-isoprenoid contents, homohopane distribution patterns, and high V/Ni ratios. Enhanced salinity stratification with mesosaline and alkaline bottom waters during deposition of the oil shales are indicated by high gammacerane index values, low MTTC ratios, high β-carotene contents, low TOC/S ratios, and high Sr/Ba ratios. The stratified water column with anoxic conditions in the bottom water enhanced preservation of OM. Moderate input of detrital minerals during the deposition of the oil shale sequences is reflected by titanium concentrations. In this study, environmental conditions in the paleo-lake leading to OM accumulation in the sediments are related to sequence stratigraphy governed by climate and tectonics. The first Member of the Qingshankou Formation (K₂qn₁) in the Songliao Basin, containing the oil shale sequence, encompasses a third-order sequence that can be divided into three system tracts (transgressive system tract—TST, highstand system tract—HST, and regressive system tract—RST). Enrichment of OM changed from low values during TST-I to high-moderate values during TST-II/III and HST-I/II. Low OM enrichment occurs during RST-I and RST-II. Therefore, the highest enrichment of OM in the sediments is related to stages of mid-late TST and early HST.  相似文献