Magnetic properties and cation ordering of nanopowders of the synthetic analogue of kuramite, Cu3SnS4

An extensive characterisation of the magnetic properties of synthetic powders of kuramite, with formal composition Cu₃SnS₄, was performed. Powders were investigated through superconducting quantum interference device (SQUID) magnetometry, electron paramagnetic resonance (EPR) spectroscopy, X-ray powder diffraction (XRPD), scanning and transmission electron microscopies (SEM and TEM) and microanalysis. SEM and TEM reveal the presence of nanodimensioned particles. XRPD clearly shows that Cu₃SnS₄ crystallised in a cubic sphalerite-type structural model, in spite of the stannite-type tetragonal structure described for the natural phase. This difference arises from a full random distribution of cations. Synthetic kuramite nanopowders exhibit a marked paramagnetism, originated by the presence of Cu(II), definitely assessed by EPR measurements. Moreover, the overall magnetic behaviour of the sample cannot be simply ascribed to diluted paramagnetism, and this suggests the presence of strong superexchange interactions among Cu(II) ions even at room temperature. The main consequences of these results are the definitive assessment of the chemical formula Cu(I)₂Cu(II)SnS₄ and of a random distribution of Cu(II), Cu(I) and Sn(IV) ions within the available tetrahedral sites.     

Empirically-based modeling of spatial sampling uncertainties associated with rainfall measurements by rain gauges

In the quantitative evaluation of radar-rainfall products (maps), rain gauge data are generally used as a good approximation of the true ground rainfall. However, rain gauges provide accurate measurements for a specific location, while radar estimates represent areal averages. Because these sampling discrepancies could introduce noise into the comparisons between these two sensors, they need to be accounted for. In this study, the spatial sampling error is defined as the ratio between the measurements by a single rain gauge and the true areal rainfall, defined as the value obtained by averaging the measurements by an adequate number of gauges within a pixel. Using a non-parametric scheme, the authors characterize its full statistical distribution for several spatial (4, 16 and 36 km²) and temporal (15 min and hourly) scales.     

A seismic reconnaissance survey of the northern Congo Fan

To study the time-varying influence of the Congo River and the Benguela Current on the deposition at the Angola Continental Margin, a high-resolution reflection seismic survey was carried out on the northern Congo Fan. Four seismostratigraphic units have been defined for the upper 800 m (1000 ms TWT) of the data. The units record different depositional environments, ranging from pre-establishment of the Congo River drainage system to the influence of the Benguela Current. An indication of a general change in the turbidite system is provided by a shift in channel distribution and a relocation of the depocentre of coarse material. The ascent of salt is recorded up to the Pliocene. Gas that has migrated out of Lower Cretaceous shales and that was produced from large quantities of organic matter in the younger sediments can be found on the flanks and on top of the salt domes. In a few places, this gas even ascends to the ocean floor along structural pathways through the topmost unit.     

Lateral variations in tectonic style across cross-strike discontinuities: an example from the Central Apennines belt (Italy)

In foreland thrust belts, abrupt lateral changes in tectonic style, structural–stratigraphic features, and topography usually occur across cross-strike faults. The Central Apennines of Italy offer an exceptional scenario of lateral variations in tectonic setting. Here, the Sangro Volturno oblique thrust ramp (SVOTR) represents the outer thrust front of the Pliocene–Quaternary foreland thrust system, confining southward the axial culmination of the orogen that occurs in the Central Apennines. We present an interpretation of the Pliocene–Quaternary evolution of this cross-strike fault through an integrated dataset including structural-geological mapping and subsurface onshore seismic reflection profiles. The interpretation of the structural framework is augmented by the analysis of low-temperature thermochronometers from 32 new sites extending across the subsurface transverse structure. As evidenced by seismic line interpretation, the localization and development of the SVOTR have been influenced by inherited extensional faults within a positive inversion tectonics context. The regional distribution of the maximum paleotemperature values across the SVOTR constrains the original extent of the allochthonous thrust sheet over all its hanging-wall and footwall blocks. The Pliocene–Quaternary thrusting and inversion of SVOTR caused the strong hanging-wall uplift, which brought to the complete erosion of the allochthonous units and the exhumation of the Adria units. The integrated analysis of low-temperature thermochronometers and structural evidence as applied in the study case can define the role of major cross-strike discontinuities in foreland thrust belts, by constraining and verifying their tectonics inversion significance and the amount of related exhumation.     

Biomarkers of Exposure and Effects for Assessing Toxicological Risk of Endocrine Disrupters in Top Predators of the Mediterranean Sea

Abstract. Endocrine Disrupting Chemicals (EDCs) have the potential to alter hormone pathways that regulate reproductive processes in wildlife and fisheries. In this research the unexplored hypothesis that Mediterranean top predator species (such as large pelagic fish and marine mammals) are potentially at risk due to EDCs is investigated. In the Mediterranean environment, top predators accumulate high concentrations of polyhalogenated aromatic hydrocarbons (PHAHs) and toxic metals, incurring high toxicological risk. Here we illustrate the need to develop sensitive biomarkers for evaluation of toxicological risk in top marine predators (Xiphias gladius, Thunnus thynnus thynnus) and non-lethal techniques, such as non-destructive biomarkers, for the hazard assessment of threatened species exposed to EDCs, such as marine mammals ( Stenella coeruleoalba, Tursiops truncatus, Delphinus delphis and Balaenoptera physalus ).     

Paläomagnetische Untersuchungen im Schilfsandstein (Trias,Km2) Westeuropas

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.

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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.

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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.

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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) . . , .

     

Integration error over very long time spans

The main limit to the time span of a numerical integration of the planetary orbits is no longer set by the availability of computer resources, but rather by the accumulation of the integration error. By the latter we mean the difference between the computed orbit and the dynamical behaviour of the real physical system, whatever the causes. The analysis of these causes requires an interdisciplinary effort: there are physical model and parameters errors, algorithm and discretisation errors, rounding off errors and reliability problems in the computer hardware and system software, as well as instabilities in the dynamical system. We list all the sources of integration error we are aware of and discuss their relevance in determining the present limit to the time span of a meaningful integration of the orbit of the planets. At present this limit is of the order of 10⁸ years for the outer planets. We discuss in more detail the truncation error of multistep algorithms (when applied to eccentric orbits), the coefficient error, the method of Encke and the associated coordinate change error, the procedures used to test the numerical integration software and their limitations. Many problems remain open, including the one of a realistic statistical model of the rounding off error; at present, the latter can only be described by a semiempirical model based upon the simpleN ² formula (N=number of steps, =machine accuracy), with an unknown numerical coefficient which is determined only a posteriori.