981 resultados para 110-676
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"October 1985."
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"10 September 1985."
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(Garrels is at far right.)
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German words.
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Mode of access: Internet.
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Chemical turbulence in the oscillatory catalytic CO oxidation on Pt(110) is suppressed by means of focused laser light. The laser locally heats the platinum surface which leads to a local increase of the oscillation frequency, and to the formation of a pacemaker which emits target waves. These waves slowly entrain the medium and suppress the spatiotemporal chaos present in the absence of laser light. Our experimental results are confirmed by a detailed numerical analysis of one- and two-dimensional media using the Krischer-Eiswirth-Ertl model for CO oxidation on Pt110. Different control regimes are identified and the dispersion relation of the system is determined using the pacemaker as an externally tunable wave source.
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The genesis of a catalytically active model Pt/Al2O3/NiAl{110} oxidation catalyst is described. An ultrathin, crystalline γ-Al2O3 film was prepared via direct oxidation of a NiAl{110} single-crystal substrate. The room-temperature deposition of Pt clusters over the γ-Al2O3 film was characterised by LEED, AES and CO titration and follows a Stranski–Krastanov growth mode. Surface sulfation was attempted via SO2/O2 adsorption and thermal processing over bare and Pt promoted Al2O3/NiAl{110}. Platinum greatly enhances the saturation SOx coverage over that of bare alumina. Over clean Pt/γ-Al2O3 surfaces some adsorbed propene desorbs molecularly [similar]250 K while the remainder decomposes liberating hydrogen. Coadsorbed oxygen or sulfate promote propene combustion, with adsorbed sulfoxy species the most efficient oxidant. The chemistry of these alumina-supported Pt clusters shows a general evolution from small polycrystalline clusters to larger clusters with properties akin to low-index, Pt single-crystal surfaces.
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The exponential growth of studies on the biological response to ocean acidification over the last few decades has generated a large amount of data. To facilitate data comparison, a data compilation hosted at the data publisher PANGAEA was initiated in 2008 and is updated on a regular basis (doi:10.1594/PANGAEA.149999). By January 2015, a total of 581 data sets (over 4 000 000 data points) from 539 papers had been archived. Here we present the developments of this data compilation five years since its first description by Nisumaa et al. (2010). Most of study sites from which data archived are still in the Northern Hemisphere and the number of archived data from studies from the Southern Hemisphere and polar oceans are still relatively low. Data from 60 studies that investigated the response of a mix of organisms or natural communities were all added after 2010, indicating a welcomed shift from the study of individual organisms to communities and ecosystems. The initial imbalance of considerably more data archived on calcification and primary production than on other processes has improved. There is also a clear tendency towards more data archived from multifactorial studies after 2010. For easier and more effective access to ocean acidification data, the ocean acidification community is strongly encouraged to contribute to the data archiving effort, and help develop standard vocabularies describing the variables and define best practices for archiving ocean acidification data.
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El uso de fuentes de Zn (orgánicas e inorgánicas) en el pienso de cerdos prepúberes se ha mostrado indispensable, ya que este mineral ha evidenciado beneficios relacionados con aspectos reproductivos, respuesta inmunitaria, estado de salud, ganancia de peso, consumo de pienso. Los primeros estudios que identificaron al Zn como componente fundamental en la reproducción fueron en la década de los 40´s, en donde se estableció la importancia de este mineral en el desarrollo de las células de Leydig, a partir de estos descubrimientos se recomienda la utilización del mineral en el pienso de los cerdos. Sin embargo, las recomendaciones que se han hecho para apoyar el efecto del Zn en la reproducción, fueron identificadas hace 30 años, y poco se ha estudiado desde entonces con respecto al nivel de Zn que habría que incluir en el pienso. Por otra parte, la industria alimenticia animal ha desarrollado fuentes minerales con mayor biodisponibilidad, por un lado para que el organismo pueda utilizarlo más rápida y eficientemente (>biodisponibilidad) y por otra parte para evitar que el mineral consumido por el animal, se pierda a través de las deyecciones, asegurando con ello no solo la reducción de las pérdidas económicas, sino la minimización del impacto ambiental que el Zn ejerce negativamente. De esta manera, se decidió realizar una investigación que proporcionara información sobre el efecto de las fuentes y niveles de Zn, en la eficiencia de crecimiento y desarrollo de cerdos prepúberes y verracos jóvenes, en el desarrollo de los testículos y sus estructuras celulares, así como en el comportamiento sexual de los verracos jóvenes. Para lo anterior se utilizaron 50 cerdos de la línea genética York x Landrace, con un peso medio inicial de 35±1.25, estos animales se distribuyeron en siete tratamientos, los cuales correspondieron a dietas formuladas con y sin la adición de fuente de Zn (ZnSO4, ZnO, ZnMet) , y a dos niveles (150ppm y 200ppm de Zn). La dieta base fue formulada utilizando la tabla de necesidades nutritivas del FEDNA (2006). Todos los cerdos fueron colocados en jaulas individuales, con comedero y bebedero individual. Se les dio un periodo de adaptación de 15 días, posteriormente se inició la fase experimental en la que se midió el consumo de pienso (CDP), conversión alimenticia (CA), ganancia de peso (GDP), al finalizar el periodo de crianza (Crecimiento, Desarrollo y Finalización) y los cerdos llegaron a un peso mayor a 100Kg, se sacrificaron tres cerdos, de los cuales se obtuvieron los testículos, epidídimos, bazo, páncreas, hueso (fémur), hígado y riñones, para analizar a través de Espectrofotometría de Absorción Atómica la concentración de Zn...
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In this paper, we use density functional theory corrected for on-site Coulomb interactions (DFT + U) and hybrid DFT (HSE06 functional) to study the defects formed when the ceria (110) surface is doped with a series of trivalent dopants, namely, Al3+, Sc3+, Y3+, and In 3+. Using the hybrid DFT HSE06 exchange-correlation functional as a benchmark, we show that doping the (110) surface with a single trivalent ion leads to formation of a localized MCe / + O O • (M = the 3+ dopant), O- hole state, confirming the description found with DFT + U. We use DFT + U to investigate the energetics of dopant compensation through formation of the 2MCe ′ +VO ̈ defect, that is, compensation of two dopants with an oxygen vacancy. In conjunction with earlier work on La-doped CeO2, we find that the stability of the compensating anion vacancy depends on the dopant ionic radius. For Al3+, which has the smallest ionic radius, and Sc3+ and In3+, with intermediate ionic radii, formation of a compensating oxygen vacancy is stable. On the other hand, the Y3+ dopant, with an ionic radius close to that of Ce4+, shows a positive anion vacancy formation energy, as does La3+, which is larger than Ce4+ (J. Phys.: Condens. Matter 2010, 20, 135004). When considering the resulting electronic structure, in Al3+ doping, oxygen hole compensation is found. However, Sc 3+, In3+, and Y3+ show the formation of a reduced Ce3+ cation and an uncompensated oxygen hole, similar to La3+. These results suggest that the ionic radius of trivalent dopants strongly influences the final defect formed when doping ceria with 3+ cations. In light of these findings, experimental investigations of these systems will be welcome.
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Thirty-four sediment and mudline temperatures were collected from six drill holes on ODP Leg 110 near the toe of the Barbados accretionary complex. When combined with thermal conductivity measurements these data delineate the complicated thermal structure on the edge of this convergent margin. Surface heat-flow values from Leg 110 (calculated from geothermal gradients forced through the bottom-water temperature at mudline) of 92 to 192 mW/m**2 are 80% to 300% higher than values predicted by standard heat flow vs. age models for oceanic crust, but are compatible with earlier surface measurements made at the same latitude. Measured heat flow tends to decrease downhole at four sites, suggesting the presence of heat sources within the sediments. These results are consistent with the flow of warm fluid through the complex along sub-horizontal, high-permeability conduits, including thrust faults, the major decollement zone, and sandy intervals. Simple calculations suggest that this flow is transient, occurring on time scales of tens to tens of thousands of years. High heat flow in the vicinity of 15°30'N and not elsewhere along the deformation front suggests that the Leg 110 drill sites may be situated over a fluid discharge zone, with dewatering more active here than elsewhere along the accretionary complex.
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Previous studies about the strength of the lithosphere in the Iberia centre fail to resolve the depth of earthquakes because of the rheological uncertainties. Therefore, new contributions are considered (the crustal structure from a density model) and several parameters (tectonic regime, mantle rheology, strain rate) are checked in this paper to properly examine the role of lithospheric strength in the intraplate seismicity and the Cenozoic evolution. The strength distribution with depth, the integrated strength, the effective elastic thickness and the seismogenic thickness have been calculated by a finite element modelling of the lithosphere across the Central System mountain range and the bordering Duero and Madrid sedimentary basins. Only a dry mantle under strike-slip/extension and a strain rate of 10-15 s-1, or under extension and 10-16 s-1, causes a strong lithosphere. The integrated strength and the elastic thickness are lower in the mountain chain than in the basins. These anisotropies have been maintained since the Cenozoic and determine the mountain uplift and the biharmonic folding of the Iberian lithosphere during the Alpine deformations. The seismogenic thickness bounds the seismic activity in the upper–middle crust, and the decreasing crustal strength from the Duero Basin towards the Madrid Basin is related to a parallel increase in Plio–Quaternary deformations and seismicity. However, elasto–plastic modelling shows that current African–Eurasian convergence is resolved elastically or ductilely, which accounts for the low seismicity recorded in this region.