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21.
Kobler  Ulrike Gabriele  Wüest  Alfred  Schmid  Martin 《Climatic change》2019,152(3-4):413-429
Climatic Change - The assessment of ecological impacts of pumped-storage (PS) hydropower plants on the two connected water bodies is usually based on present climatic conditions. However,...  相似文献   
22.
This study addresses the influence of landslide dams on surface water drainage and groundwater flow. In the study area of Scanno Lake and Sagittario River (Central Italy), a limestone rockslide‐avalanche formed a lake, which has an outlet that is occasionally active, showing infiltration into the rockslide dam. Several springs are present at the lake's base and are partly fed by seepage through the rockslide debris. Piezometric surveys, discharge measurements, pumping tests and chemical analyses are tools used to build a conceptual model of the groundwater flow and to evaluate the flow through the rockslide debris. Seasonal water isotopic signatures validate the assumed model, showing a mixing of infiltration recharge and groundwater seepage throughout the rockslide debris. Various recharge areas have been found for springs, pointing out those directly fed by the rockslide debris aquifer. Hypotheses about seasonal groundwater mixing between the regional carbonate aquifer and the rockslide debris aquifer are supported by isotope results. Seasonal changes in groundwater table level due to recharge and surface losses from seasonal outlet have been correlated with isotopic groundwater composition from the rockslide debris aquifer and the downstream springs; this relationship highlights the role of the rockslide dam body on the hydrodynamics of the studied area. Relationships between surface waters and groundwater in the area have been completely understood on the basis of water isotopic fingerprinting, finally obtaining a complete evaluation of groundwater renewable resources and its regimen. Copyright © 2010 John Wiley & Sons, Ltd.  相似文献   
23.
Gabriele Bulian 《Ocean Engineering》2010,37(11-12):1007-1026
This paper presents a probabilistic methodology for the analysis of the vulnerability of a ship to the risk of inception of pure loss of stability events. A pure loss of stability failure is modelled as the persistence of the metacentric height below a critical level for a too long time. The metacentric height is modelled as a stationary Gaussian process with a spectrum obtained from the sea elevation spectrum. The time dependent failure index is obtained under the assumption of filtered Poisson process for the occurrence of critical events. The analysis separates cases where the fluctuation of the metacentric height is narrow-band from those where the bandwidth of the spectrum is wide, with an intermediate blending. In case of narrow-band processes appropriate approximate solutions to the problem are provided, while in the wide-band cases an exponential distribution for the persistence time below the critical level is employed. A rational development for the critical persistence time is also provided considering an approximation of the roll dynamics during periods of time where the metacentric height is negative. Monte Carlo simulations are performed to check the developed approximate distributions for the persistence time, and examples of application are provided for a sample ship.  相似文献   
24.
Zusammenfassung Von insgesamt 46 beprobten Profilen aus dem Schilfsandstein (Trias, Km2) Westeuropas wurden bislang 41 Profile mit 343 Einheiten und 870 Handstücken mit 1897 Einzelkernen auf ihren paläomagnetischen Inhalt untersucht.Thermische Entmagnetisierungsversuche an 277 Proben zeigen, daß die natürliche remanente Magnetisierung (NRM) von mehreren, an verschiedene Magnetisierungsträger gebundenen Komponenten getragen wird.Als charakteristische remanente Magnetisierung (CARM), von der angenommen wird, daß sie das zur Ablagerungszeit herrschende Paläofeld abbildet, kristallisiert sich für die Sedimentationsräume Weserbergland und Franken eine Deklination (DR=Deklination rotiert) von 60° und eine Inklination (IR=Inklination rotiert) von 30° (DR/IR 60/30) und für Schwaben und die Nordschweiz DR/IR 240/–30 heraus.Neben der stabilen Paläofeldrichtung werden auch sedimentäre und tektonische Gefüge als weitere stabile Magnetisierungsrichtungen abgebildet. Diese Richtungen liegen der Achse maximaler Suszeptibilität (K1 max) parallel.Unter Annahme einer normalen Polarität des Erdmagnetfeldes zur Zeit der Schilfsandsteinablagerung im Weserbergland und Franken und einer reversen Polarität zur Zeit der Ablagerung in Schwaben und der Nordschweiz errechnet sich ein Paläonordpol bei 111 E 28 N; er fällt damit in die Nähe des Triaspoles der Europäischen Polwanderungskurve (McElhinny, 1973).Für den Ablagerungszeitraum des Raibler Sandsteins in den Südalpen wird ein Paläonordpol bei 128 W 48 N errechnet.Die magnetostratigraphische Zeitskala der Trias (Burek, 1970) kann um die Einstufung des Schilfsandsteins in das höhere obere Karn mit beginnender normaler Polarität und dann reverser Polarität ergänzt werden.
In the Schilfsandstein (Triassic, Km2) of Western Europe 41 sections with 343 units and 1897 cores were sampled for palaeomagnetic investigations. By thermal demagnetization experiments different magnetic minerals were determined as carriers of the natural rémanent magnetization (NRM).The characteristic remanent magnetization (CARM) reflecting the palaeofield direction is described in the Weserbergland and Franken by DR/IR 60/30 (DR = declination after tectonic correction/IR=inclination after tectonic correction) and in Schwaben and Northern Switzerland by DR/IR 240/–30.In addition stable directions are reported which are related to sedimentary and tectonic fabric. These directions are parallel to the axis of maximum susceptibility (Klmax).Assuming normal polarity for the magnetic field during deposition of the Schilfsandstein in the Weserbergland and Franken and assuming reversed polarity in Schwaben and Northern Switzerland a palaeonorthpole is estimated at 111 E 28 N. This poleposition fits near the Triassic poleposition of the European polar wandering curve (McElhinny, 1973).The poleposition of the Bergamasker Alps (Raibler Sandstein, Southern Alps) is figured out at 128 W 48 N.The triassic magnetostratigraphic time scale ofBurek (1970) can be completed as far as the Schilfsandstein is to arrange into the highest Upper Carnian starting with normal polarity going on with reversed polarity.

Résumé Dans le Grès à roseaux (Trias, Km 2) de l'Europe occidentale, 343 prélèvements provenant de 41 profils et 1897 carrottes extraites de 870 échantillons ont fait l'objet de recherches paléomagnétiques. — Des essais de démagnétisation thermique sur 277 échantillons ont révélé différents minéraux magnétiques comme étant les porteurs de l'aimantation rémanente naturelle (NRM). — L'aimentation rémanente caractéristique (CARM) reflétant la direction du paléochamp magnétique au moment de la sédimentation donne des valeurs de 60/30 pour DR/IR (DR=déclinaison après correction tectonique, — IR=inclinaison après correction tectonique) dans le Weserbergland et en Franconie et 240/– 30 pour DR/IR en Souabe et dans la Suisse septentrionale. — En plus de la direction stable du paléo champ, on a trouvé d'autres directions d'aimentation stables reliées aux structures sédimentaires et tectoniques. Ces directions sont parallèles à l'axe de la susceptibilité magnétique maximale (K1 max). — En supposant une polarité normale du champ magnétique terrestre au moment de la sédimentation du Grès à roseaux dans le Weserbergland et la Franconie, et une polarité inversée pendant sa formation en Souabe et en Suisse septentrionale, il en résulte une position géographique de 111 E et 28° N pour le paléopôle Nord, ce qui coïncide à peu près avec la position du pôle triasique sur la courbe polaire de l'Europe (McElhinny, 1973). Pendant la sédimentation du Grès de Raibler dans les Alpes bergamasques, le paléopôle Nord se trouvait à 128° O 48° N. — L'echelle magnétostratigraphique pour le Trias (Burek, 1970) peut maintenant être complétée en datant le Grès à roseaux dans la partie supérieure du Carnien supérieur, débutant par une aimantation normale et continuant par une aimantation inversée.

343 41 ( ) 1897 870 . 277 , — NRM — . — CARM —, , , , , (DR = Deklination rotiert) 60°, (IR = Inklination rotiert) 30° (DR/IR 60/30), DR/IR 240/-30. , . /1makc. , 111 E 28 N, . ., . 128 W 48 N. (Burek, 1970) . . , .
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25.
26.
Synthetic orthopyroxenes free of trivalent cations Mg x Fe 2-x Si2O6 (x=0; 1; 1.6) were investigated using both Mössbauer spectroscopy (MS) and single-crystal X-ray diffraction (XRD) in order to compare the results obtained on the same samples by the two techniques. The Mg-Fe distribution over M1 and M2 octahedral sites was determined on compounds with x = 1 and x=1.6, unheated and annealed at 650, 850 and 1040° C for 29 to 42 hours to obtain different degrees of order. The data obtained by the two techniques are in very good agreement, thus suggesting, for these compositions, the absence of systematic errors. The investigation of a synthetic compound with x=0 (ferrosilite) confirmed that the accuracy of both methods is very good. The observed small discrepancies between the results are not significant if compared with the relevant standard deviations which, for both methods, were derived by leastsquares calculations. The best fit is obtained for Fe(M1)/ Fe(tot) parameters that, in both methods, are directly calculated without using data from chemical analysis. For the unheated samples the values by MS and XRD are respectively: 0.185(9) and 0.180(4) for x = 1.6; 0.282(8) and 0.285(2) for x=1; 0.503(7) and 0.502(1) for x=0. For all the investigated samples the correlation between the geometrical distortion parameters, calculated by X-ray refinement, and the quadrupole splitting values, measured by Mössbauer spectroscopy, agrees with the theoretical model of Ingalls (1964).  相似文献   
27.
We propose a new formal definition of discovery for a Solar System object. It is based on an objective and mathematically rigorous algorithm to assess when a set of observations is enough to constitute a discovery. When this definition is satisfied, in almost all cases the orbit is defined well enough to establish the nature of the object discovered (Main Belt vs. Near Earth Asteroid, Trans-Neptunian vs. long period comet). The frequency of occurrence of exceptions is estimated by a set of numerical experiments. The availability of a non-subjective definition of discovery allows some rules to be adopted for the assignment of discovery credit with a minimum risk of dispute. Such rules should be fair, encourage good practice by the observers and acknowledge the contribution of the orbit computers providing the identifications and the orbits, as well as the one of all the contributing observers.  相似文献   
28.
We investigated microphytobenthic photosynthesis at four stations in the coral reef sediments at Heron Reef, Australia. The microphytobenthos was dominated by diatoms, dinoflagellates and cyanobacteria, as indicated by biomarker pigment analysis. Conspicuous algae firmly attached to the sand grains (ca. 100 μm in diameter, surrounded by a hard transparent wall) were rich in peridinin, a marker pigment for dinoflagellates, but also showed a high diversity based on cyanobacterial 16S rDNA gene sequence analysis. Specimens of these algae that were buried below the photic zone exhibited an unexpected stimulation of respiration by light, resulting in an increase of local oxygen concentrations upon darkening. Net photosynthesis of the sediments varied between 1.9 and 8.5 mmol O2 m−2 h−1 and was strongly correlated with Chl a content, which lay between 31 and 84 mg m−2. An estimate based on our spatially limited dataset indicates that the microphytobenthic production for the entire reef is in the order of magnitude of the production estimated for corals. Photosynthesis stimulated calcification at all investigated sites (0.2–1.0 mmol Ca2+ m−2 h−1). The sediments of at least three stations were net calcifying. Sedimentary N2-fixation rates (measured by acetylene reduction assays at two sites) ranged between 0.9 to 3.9 mmol N2 m−2 h−1 and were highest in the light, indicating the importance of heterocystous cyanobacteria. In coral fingers no N2-fixation was measurable, which stresses the importance of the sediment compartment for reef nitrogen cycling.  相似文献   
29.
Understanding the factors that cause population divergence has long been of interest to marine biologists in their attempts to interpret the effect of human‐mediated vectors. Broadcast‐spawning species with limited dispersal capability are excellent candidates to measure the present‐day patterns of genetic diversity. The tunicate Ciona intestinalis (Ascidiacea) is comprised of a complex of morphologically cryptic species that form vigorous aggregates in eutrophic habitats (harbors, gulfs and lagoons) where they can compete with the epibenthic community and cause biofouling problems. This study investigated biogeographic variability and migration patterns of C. intestinalis sp. A along Northeast Atlantic and Mediterranean coasts using microsatellite markers. Data presented here on 371 specimens collected from 17 populations reveal high genetic polymorphism, but with a deficit of heterozygote deficiency. Absence of evidence for isolation by distance suggests that the genetic patterns do not reflect the geographic distribution of sampled populations. Substantial gene flow and artificial potential for dispersal boost high levels of within‐population genetic variability and prevent genetic differentiation within and between seas. A predominant eastward migration pattern was revealed by the data set, with very limited opportunity for C. intestinalis sp. A to travel westward. This directional movement indicates that other properties (e.g. habitat quality, genetic traits, mating system, life cycle) may cause adaptive divergence at a large biogeographic scale.  相似文献   
30.
The Radio Science Experiment is one of the on board experiments of the Mercury ESA mission BepiColombo that will be launched in 2014. The goals of the experiment are to determine the gravity field of Mercury and its rotation state, to determine the orbit of Mercury, to constrain the possible theories of gravitation (for example by determining the post-Newtonian parameters), to provide the spacecraft position for geodesy experiments and to contribute to planetary ephemerides improvement. This is possible thanks to a new technology which allows to reach great accuracies in the observables range and range rate; it is well known that a similar level of accuracy requires studying a suitable model taking into account numerous relativistic effects. In this paper we deal with the modelling of the space-time coordinate transformations needed for the light-time computations and the numerical methods adopted to avoid rounding-off errors in such computations.  相似文献   
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