40Ar-39Ar dating and isotopic composition of groundmass and felspar samples from core AND-2A

The AND-2A drillcore (Antarctic Drilling Program-ANDRILL) was successfully completed in late 2007 on the Antarctic continental margin (Southern McMurdo Sound, Ross Sea) with the aim of tracking ice proximal to shallow marine environmental fluctuations and to document the 20-Ma evolution of the Erebus Volcanic Province. Lava clasts and tephra layers from the AND-2A drillcore were investigated from a petrographic and stratigraphic point of view and analyzed by the 40Ar-39Ar laser technique in order to constrain the age model of the core and to gain information on the style and nature of sediment deposition in the Victoria Land Basin since Early Miocene. Ten out of 17 samples yielded statistically robust 40Ar-39Ar ages, indicating that the AND-2A drillcore recovered <230 m of Middle Miocene (~128-358 m below sea floor, ~11.5-16.0 Ma) and >780 m of Early Miocene (~358-1093 m below sea floor, ~16.0-20.1 Ma). Results also highlight a nearly continuous stratigraphic record from at least 358 m below sea floor down hole, characterized by a mean sedimentation rate of ~19 cm/ka, possible oscillations of no more than a few hundreds of ka and a break within ~17.5-18.1 Ma. Comparison with available data from volcanic deposits on land, suggests that volcanic rocks within the AND-2A core were supplied from the south, possibly with source areas closer to the drill site for the upper core levels, and from 358 m below sea floor down hole, with the 'proto-Mount Morning' as the main source.

Stable carbon isotope ratios of Cibicidoides wuellerstorfi of MIS 2 time slices

The interval of time represented by marine isotope stages 11 and 12 (~360-470 ka) contains what may be the most extreme glacial and interglacial climate conditions of the Late Pleistocene. It has been suggested that sea level rose by ~160 m at the termination of glacial stage 12. This is 30% greater than the sea level rise that followed the most recent glacial maximum. There have been few detailed studies of the unique conditions that existed during the stage 11-12 time period because of the lack of high-quality core material. This problem has been addressed by the collection of high deposition rate cores from sediment drifts in the western North Atlantic during Ocean Drilling Project Leg 172. Benthic foraminiferal d13C data from cores collected between ~4600 and 1800 m were used to reconstruct bathymetric gradients in deep and intermediate water properties for selected time slices during this glacial-interglacial cycle. During glacial stage 12, the deep western North Atlantic was filled by a water mass that was more nutrient-enriched than modern Antarctic Bottom Water. Above 2000 m, a more nutrient-depleted water mass existed during this glacial stage. Such an intermediate water mass has been described for more recent glacial periods and presumably forms in a more proximate region of the North Atlantic. Interglacial stage 11 water mass properties closely resemble those of the present-day western North Atlantic. A nutrient-depleted water mass (d13C of 0.75-1.0 per mil), similar to modern North Atlantic Deep Water existed between 3500 and 2000 m. This was underlain by a water mass with lower d13C values (<0.75 per mil) that probably was derived from a southern source. Using Leg 172 data, along with previously published results from the Atlantic and Pacific oceans, we estimate a mean global d13C change of 0.95 per mil from stage 12 to stage 11. This is twice the whole ocean ?13C change reported for the transition from the last glacial maximum to the Holocene.

Geochemical studies of the Cretaceous-Tertiary boundary in ODP Holes 113-689B and 113-690C

In a study of ODP Hole 689B no iridium (Ir) anomaly was found in Sections 1 through 6 of Core 25X or in Core 26X from the top down to section 2, 3-12 cm. The background Ir abundance averaged 11 parts per trillion (ppt) and a clay-enriched region had nearly the same average, 26 ± 12 ppt. If the Cretaceous-Tertiary (K-T) contact is in the region studied, then sedimentation was not continuous, and the K-T boundary was probably either not deposited or it was eroded away. In a study of Cores 15X and 16X of ODP Hole 690C, an iridium peak with a maximum abundance of 1566 ± 222 ppt was found in Section 4 of Core 15X at 39-40 cm with a half-width of 6.6 cm. Background abundances were ~15 ppt and distinctly higher Ir abundances were observed from 119 cm below to 72 cm above the main peak. The Ir distribution below the main peak is attributed to bioturbation by organisms with burrows extending at least 0.4 m. The Ir distribution above the main peak may be due to the same cause but other explanations may be significant. There are variable enrichments of clay in the mainly CaCO3 sediment of Core 15X, and the stratigraphically lowest part of the most abundant clay deposits is found (within 2 cm) in the same position as the main Ir peak. The clay deposit, which is estimated to be about 50% of the sediment, extends upward ~19 cm and then slowly decreases to a background level of 10% over 1 m. The degree of homogeneity of the clay-rich interval suggests it was not due to episodic volcanism but may have been due to a decrease of the CaCO3 deposition rate which was possibly triggered by the impact of a large asteroid or comet on the Earth.

An Intercomparison of Modelling Approaches for Simulating the Atmospheric Dispersion of Ammonia Emitted by Agricultural Sources

RESUMEN La dispersión del amoniaco (NH3) emitido por fuentes agrícolas en medias distancias, y su posterior deposición en el suelo y la vegetación, pueden llevar a la degradación de ecosistemas vulnerables y a la acidificación de los suelos. La deposición de NH3 suele ser mayor junto a la fuente emisora, por lo que los impactos negativos de dichas emisiones son generalmente mayores en esas zonas. Bajo la legislación comunitaria, varios estados miembros emplean modelos de dispersión inversa para estimar los impactos de las emisiones en las proximidades de las zonas naturales de especial conservación. Una revisión reciente de métodos para evaluar impactos de NH3 en distancias medias recomendaba la comparación de diferentes modelos para identificar diferencias importantes entre los métodos empleados por los distintos países de la UE. En base a esta recomendación, esta tesis doctoral compara y evalúa las predicciones de las concentraciones atmosféricas de NH3 de varios modelos bajo condiciones, tanto reales como hipotéticas, que plantean un potencial impacto sobre ecosistemas (incluidos aquellos bajo condiciones de clima Mediterráneo). En este sentido, se procedió además a la comparación y evaluación de varias técnicas de modelización inversa para inferir emisiones de NH3. Finalmente, se ha desarrollado un modelo matemático simple para calcular las concentraciones de NH3 y la velocidad de deposición de NH3 en ecosistemas vulnerables cercanos a una fuente emisora. La comparativa de modelos supuso la evaluación de cuatro modelos de dispersión (ADMS 4.1; AERMOD v07026; OPS-st v3.0.3 y LADD v2010) en un amplio rango de casos hipotéticos (dispersión de NH3 procedente de distintos tipos de fuentes agrícolas de emisión). La menor diferencia entre las concentraciones medias estimadas por los distintos modelos se obtuvo para escenarios simples. La convergencia entre las predicciones de los modelos fue mínima para el escenario relativo a la dispersión de NH3 procedente de un establo ventilado mecánicamente. En este caso, el modelo ADMS predijo concentraciones significativamente menores que los otros modelos. Una explicación de estas diferencias podríamos encontrarla en la interacción de diferentes “penachos” y “capas límite” durante el proceso de parametrización. Los cuatro modelos de dispersión fueron empleados para dos casos reales de dispersión de NH3: una granja de cerdos en Falster (Dinamarca) y otra en Carolina del Norte (EEUU). Las concentraciones medias anuales estimadas por los modelos fueron similares para el caso americano (emisión de granjas ventiladas de forma natural y balsa de purines). La comparación de las predicciones de los modelos con concentraciones medias anuales medidas in situ, así como la aplicación de los criterios establecidos para la aceptación estadística de los modelos, permitió concluir que los cuatro modelos se comportaron aceptablemente para este escenario. No ocurrió lo mismo en el caso danés (nave ventilada mecánicamente), en donde el modelo LADD no dio buenos resultados debido a la ausencia de procesos de “sobreelevacion de penacho” (plume-rise). Los modelos de dispersión dan a menudo pobres resultados en condiciones de baja velocidad de viento debido a que la teoría de dispersión en la que se basan no es aplicable en estas condiciones. En situaciones de frecuente descenso en la velocidad del viento, la actual guía de modelización propone usar un modelo que sea eficaz bajo dichas condiciones, máxime cuando se realice una valoración que tenga como objeto establecer una política de regularización. Esto puede no ser siempre posible debido a datos meteorológicos insuficientes, en cuyo caso la única opción sería utilizar un modelo más común, como la versión avanzada de los modelos Gausianos ADMS o AERMOD. Con el objetivo de evaluar la idoneidad de estos modelos para condiciones de bajas velocidades de viento, ambos modelos fueron utilizados en un caso con condiciones Mediterráneas. Lo que supone sucesivos periodos de baja velocidad del viento. El estudio se centró en la dispersión de NH3 procedente de una granja de cerdos en Segovia (España central). Para ello la concentración de NH3 media mensual fue medida en 21 localizaciones en torno a la granja. Se realizaron también medidas de concentración de alta resolución en una única localización durante una campaña de una semana. En este caso, se evaluaron dos estrategias para mejorar la respuesta del modelo ante bajas velocidades del viento. La primera se basó en “no zero wind” (NZW), que sustituyó periodos de calma con el mínimo límite de velocidad del viento y “accumulated calm emissions” (ACE), que forzaban al modelo a calcular las emisiones totales en un periodo de calma y la siguiente hora de no-calma. Debido a las importantes incertidumbres en los datos de entrada del modelo (inputs) (tasa de emisión de NH3, velocidad de salida de la fuente, parámetros de la capa límite, etc.), se utilizó el mismo caso para evaluar la incertidumbre en la predicción del modelo y valorar como dicha incertidumbre puede ser considerada en evaluaciones del modelo. Un modelo dinámico de emisión, modificado para el caso de clima Mediterráneo, fue empleado para estimar la variabilidad temporal en las emisiones de NH3. Así mismo, se realizó una comparativa utilizando las emisiones dinámicas y la tasa constante de emisión. La incertidumbre predicha asociada a la incertidumbre de los inputs fue de 67-98% del valor medio para el modelo ADMS y entre 53-83% del valor medio para AERMOD. La mayoría de esta incertidumbre se debió a la incertidumbre del ratio de emisión en la fuente (50%), seguida por la de las condiciones meteorológicas (10-20%) y aquella asociada a las velocidades de salida (5-10%). El modelo AERMOD predijo mayores concentraciones que ADMS y existieron más simulaciones que alcanzaron los criterios de aceptabilidad cuando se compararon las predicciones con las concentraciones medias anuales medidas. Sin embargo, las predicciones del modelo ADMS se correlacionaron espacialmente mejor con las mediciones. El uso de valores dinámicos de emisión estimados mejoró el comportamiento de ADMS, haciendo empeorar el de AERMOD. La aplicación de estrategias destinadas a mejorar el comportamiento de este último tuvo efectos contradictorios similares. Con el objeto de comparar distintas técnicas de modelización inversa, varios modelos (ADMS, LADD y WindTrax) fueron empleados para un caso no agrícola, una colonia de pingüinos en la Antártida. Este caso fue empleado para el estudio debido a que suponía la oportunidad de obtener el primer factor de emisión experimental para una colonia de pingüinos antárticos. Además las condiciones eran propicias desde el punto de vista de la casi total ausencia de concentraciones ambiente (background). Tras el trabajo de modelización existió una concordancia suficiente entre las estimaciones obtenidas por los tres modelos. De este modo se pudo definir un factor de emisión de para la colonia de 1.23 g NH3 por pareja criadora por día (con un rango de incertidumbre de 0.8-2.54 g NH3 por pareja criadora por día). Posteriores aplicaciones de técnicas de modelización inversa para casos agrícolas mostraron también un buen compromiso estadístico entre las emisiones estimadas por los distintos modelos. Con todo ello, es posible concluir que la modelización inversa es una técnica robusta para estimar tasas de emisión de NH3. Modelos de selección (screening) permiten obtener una rápida y aproximada estimación de los impactos medioambientales, siendo una herramienta útil para evaluaciones de impactos en tanto que permite eliminar casos que presentan un riesgo potencial de daño bajo. De esta forma, lo recursos del modelo pueden Resumen (Castellano) destinarse a casos en donde la posibilidad de daño es mayor. El modelo de Cálculo Simple de los Límites de Impacto de Amoniaco (SCAIL) se desarrolló para obtener una estimación de la concentración media de NH3 y de la tasa de deposición seca asociadas a una fuente agrícola. Está técnica de selección, basada en el modelo LADD, fue evaluada y calibrada con diferentes bases de datos y, finalmente, validada utilizando medidas independientes de concentraciones realizadas cerca de las fuentes. En general SCAIL dio buenos resultados de acuerdo a los criterios estadísticos establecidos. Este trabajo ha permitido definir situaciones en las que las concentraciones predichas por modelos de dispersión son similares, frente a otras en las que las predicciones difieren notablemente entre modelos. Algunos modelos nos están diseñados para simular determinados escenarios en tanto que no incluyen procesos relevantes o están más allá de los límites de su aplicabilidad. Un ejemplo es el modelo LADD que no es aplicable en fuentes con velocidad de salida significativa debido a que no incluye una parametrización de sobreelevacion del penacho. La evaluación de un esquema simple combinando la sobreelevacion del penacho y una turbulencia aumentada en la fuente mejoró el comportamiento del modelo. Sin embargo más pruebas son necesarias para avanzar en este sentido. Incluso modelos que son aplicables y que incluyen los procesos relevantes no siempre dan similares predicciones. Siendo las razones de esto aún desconocidas. Por ejemplo, AERMOD predice mayores concentraciones que ADMS para dispersión de NH3 procedente de naves de ganado ventiladas mecánicamente. Existe evidencia que sugiere que el modelo ADMS infraestima concentraciones en estas situaciones debido a un elevado límite de velocidad de viento. Por el contrario, existen evidencias de que AERMOD sobreestima concentraciones debido a sobreestimaciones a bajas Resumen (Castellano) velocidades de viento. Sin embrago, una modificación simple del pre-procesador meteorológico parece mejorar notablemente el comportamiento del modelo. Es de gran importancia que estas diferencias entre las predicciones de los modelos sean consideradas en los procesos de evaluación regulada por los organismos competentes. Esto puede ser realizado mediante la aplicación del modelo más útil para cada caso o, mejor aún, mediante modelos múltiples o híbridos. ABSTRACT Short-range atmospheric dispersion of ammonia (NH3) emitted by agricultural sources and its subsequent deposition to soil and vegetation can lead to the degradation of sensitive ecosystems and acidification of the soil. Atmospheric concentrations and dry deposition rates of NH3 are generally highest near the emission source and so environmental impacts to sensitive ecosystems are often largest at these locations. Under European legislation, several member states use short-range atmospheric dispersion models to estimate the impact of ammonia emissions on nearby designated nature conservation sites. A recent review of assessment methods for short-range impacts of NH3 recommended an intercomparison of the different models to identify whether there are notable differences to the assessment approaches used in different European countries. Based on this recommendation, this thesis compares and evaluates the atmospheric concentration predictions of several models used in these impact assessments for various real and hypothetical scenarios, including Mediterranean meteorological conditions. In addition, various inverse dispersion modelling techniques for the estimation of NH3 emissions rates are also compared and evaluated and a simple screening model to calculate the NH3 concentration and dry deposition rate at a sensitive ecosystem located close to an NH3 source was developed. The model intercomparison evaluated four atmospheric dispersion models (ADMS 4.1; AERMOD v07026; OPS-st v3.0.3 and LADD v2010) for a range of hypothetical case studies representing the atmospheric dispersion from several agricultural NH3 source types. The best agreement between the mean annual concentration predictions of the models was found for simple scenarios with area and volume sources. The agreement between the predictions of the models was worst for the scenario representing the dispersion from a mechanically ventilated livestock house, for which ADMS predicted significantly smaller concentrations than the other models. The reason for these differences appears to be due to the interaction of different plume-rise and boundary layer parameterisations. All four dispersion models were applied to two real case studies of dispersion of NH3 from pig farms in Falster (Denmark) and North Carolina (USA). The mean annual concentration predictions of the models were similar for the USA case study (emissions from naturally ventilated pig houses and a slurry lagoon). The comparison of model predictions with mean annual measured concentrations and the application of established statistical model acceptability criteria concluded that all four models performed acceptably for this case study. This was not the case for the Danish case study (mechanically ventilated pig house) for which the LADD model did not perform acceptably due to the lack of plume-rise processes in the model. Regulatory dispersion models often perform poorly in low wind speed conditions due to the model dispersion theory being inapplicable at low wind speeds. For situations with frequent low wind speed periods, current modelling guidance for regulatory assessments is to use a model that can handle these conditions in an acceptable way. This may not always be possible due to insufficient meteorological data and so the only option may be to carry out the assessment using a more common regulatory model, such as the advanced Gaussian models ADMS or AERMOD. In order to assess the suitability of these models for low wind conditions, they were applied to a Mediterranean case study that included many periods of low wind speed. The case study was the dispersion of NH3 emitted by a pig farm in Segovia, Central Spain, for which mean monthly atmospheric NH3 concentration measurements were made at 21 locations surrounding the farm as well as high-temporal-resolution concentration measurements at one location during a one-week campaign. Two strategies to improve the model performance for low wind speed conditions were tested. These were ‘no zero wind’ (NZW), which replaced calm periods with the minimum threshold wind speed of the model and ‘accumulated calm emissions’ (ACE), which forced the model to emit the total emissions during a calm period during the first subsequent non-calm hour. Due to large uncertainties in the model input data (NH3 emission rates, source exit velocities, boundary layer parameters), the case study was also used to assess model prediction uncertainty and assess how this uncertainty can be taken into account in model evaluations. A dynamic emission model modified for the Mediterranean climate was used to estimate the temporal variability in NH3 emission rates and a comparison was made between the simulations using the dynamic emissions and a constant emission rate. Prediction uncertainty due to model input uncertainty was 67-98% of the mean value for ADMS and between 53-83% of the mean value for AERMOD. Most of this uncertainty was due to source emission rate uncertainty (~50%), followed by uncertainty in the meteorological conditions (~10-20%) and uncertainty in exit velocities (~5-10%). AERMOD predicted higher concentrations than ADMS and more of the simulations met the model acceptability criteria when compared with the annual mean measured concentrations. However, the ADMS predictions were better correlated spatially with the measurements. The use of dynamic emission estimates improved the performance of ADMS but worsened the performance of AERMOD and the application of strategies to improved model performance had similar contradictory effects. In order to compare different inverse modelling techniques, several models (ADMS, LADD and WindTrax) were applied to a non-agricultural case study of a penguin colony in Antarctica. This case study was used since it gave the opportunity to provide the first experimentally-derived emission factor for an Antarctic penguin colony and also had the advantage of negligible background concentrations. There was sufficient agreement between the emission estimates obtained from the three models to define an emission factor for the penguin colony (1.23 g NH3 per breeding pair per day with an uncertainty range of 0.8-2.54 g NH3 per breeding pair per day). This emission estimate compared favourably to the value obtained using a simple micrometeorological technique (aerodynamic gradient) of 0.98 g ammonia per breeding pair per day (95% confidence interval: 0.2-2.4 g ammonia per breeding pair per day). Further application of the inverse modelling techniques for a range of agricultural case studies also demonstrated good agreement between the emission estimates. It is concluded, therefore, that inverse dispersion modelling is a robust technique for estimating NH3 emission rates. Screening models that can provide a quick and approximate estimate of environmental impacts are a useful tool for impact assessments because they can be used to filter out cases that potentially have a minimal environmental impact allowing resources to be focussed on more potentially damaging cases. The Simple Calculation of Ammonia Impact Limits (SCAIL) model was developed as a screening model to provide an estimate of the mean NH3 concentration and dry deposition rate downwind of an agricultural source. This screening tool, based on the LADD model, was evaluated and calibrated with several experimental datasets and then validated using independent concentration measurements made near sources. Overall SCAIL performed acceptably according to established statistical criteria. This work has identified situations where the concentration predictions of dispersion models are similar and other situations where the predictions are significantly different. Some models are simply not designed to simulate certain scenarios since they do not include the relevant processes or are beyond the limits of their applicability. An example is the LADD model that is not applicable to sources with significant exit velocity since the model does not include a plume-rise parameterisation. The testing of a simple scheme combining a momentum-driven plume rise and increased turbulence at the source improved model performance, but more testing is required. Even models that are applicable and include the relevant process do not always give similar predictions and the reasons for this need to be investigated. AERMOD for example predicts higher concentrations than ADMS for dispersion from mechanically ventilated livestock housing. There is evidence to suggest that ADMS underestimates concentrations in these situations due to a high wind speed threshold. Conversely, there is also evidence that AERMOD overestimates concentrations in these situations due to overestimation at low wind speeds. However, a simple modification to the meteorological pre-processor appears to improve the performance of the model. It is important that these differences between the predictions of these models are taken into account in regulatory assessments. This can be done by applying the most suitable model for the assessment in question or, better still, using multiple or hybrid models.

Surface InGaAs nanostructures for sensing applications

El desarrollo de sensores está ganando cada vez mayor importancia debido a la concienciación ciudadana sobre el medio ambiente haciendo que su desarrollo sea muy elevado en todas las disciplinas, entre las que cabe destacar, la medicina, la biología y la química. A pesar de la existencia de estos dispositivos, este área está aún por mejorar, ya que muchos de los materiales propuestos hasta el momento e incluso los ya comercializados muestran importantes carencias de funcionamiento, eficiencia e integrabilidad entre otros. Para la mejora de estos dispositivos, se han propuesto diversas aproximaciones basadas en nanosistemas. Quizá, uno de las más prometedoras son las nanoestructuras de punto cuántico, y en particular los semiconductores III-V basados en la consolidada tecnología de los arseniuros, las cuáles ofrecen excelentes propiedades para su uso como sensores. Además, estudios recientes demuestran su gran carácter sensitivo al medio ambiente, la posibilidad de funcionalizar la superficie para la fabricación de sensores interdisciplinares y posibilididad de mejorar notablemente su eficiencia. A lo largo de esta tesis, nos centramos en la investigación de SQD de In0.5Ga0.5As sobre substratos de GaAs(001) para el desarrollo de sensores de humedad. La tesis abarca desde el diseño, crecimiento y caracterización de las muestras hasta la el posterior procesado y caracterización de los dispositivos finales. La optimización de los parámetros de crecimiento es fundamental para conseguir una nanoestructura con las propiedades operacionales idóneas para un fin determinado. Como es bien sabido en la literatura, los parámetros de crecimiento (temperatura de crecimiento, relación de flujos del elemento del grupo V y del grupo I II (V/III), velocidad de crecimiento y tratamiento térmico después de la formación de la capa activa) afectan directamente a las propiedades estructurales, y por tanto, operacionales de los puntos cuánticos (QD). En esta tesis, se realiza un estudio de las condiciones de crecimiento para el uso de In0.5Ga0.5As SQDs como sensores. Para los parámetros relacionados con la temperatura de crecimiento de los QDs y la relación de flujos V / I I I se utilizan los estudios previamente realizados por el grupo. Mientras que este estudio se centrará en la importancia de la velocidad de crecimiento y en el tratamiento térmico justo después de la nucleación de los QDs. Para ello, se establece la temperatura de creciemiento de los QDs en 430°C y la relación de flujos V/III en 20. Como resultado, los valores más adecuados que se obtienen para la velocidad de crecimiento y el tratamiento térmico posterior a la formación de los puntos son, respectivamente, 0.07ML/s y la realización de una bajada y subida brusca de la temperatura del substrato de 100°C con respecto a la temperatura de crecimiento de los QDs. El crecimiento a una velocidad lo suficientemente alta que permita la migración de los átomos por la superficie, pero a su vez lo suficientemente baja para que se lleve a cabo la nucleación de los QDs; en combinación con el tratamiento brusco de temperatura que hace que se conserve la forma y composición de los QDs, da lugar a unos SQDs con un alto grado de homogeneidad y alta densidad superficial. Además, la caracterización posterior indica que estas nanoestructuras de gran calidad cristalina presentan unas propiedades ópticas excelentes incluso a temperatura ambiente. Una de las características por la cual los SQD de Ino.5Gao.5As se consideran candidatos prometedores para el desarrollo de sensores es el papel decisivo que juega la superficie por el mero hecho de estar en contacto directo con las partículas del ambiente y, por tanto, por ser capaces de interactuar con sus moléculas. Así pues, con el fin de demostrar la idoneidad de este sistema para dicha finalidad, se evalúa el impacto ambiental en las propiedades ópticas y eléctricas de las muestras. En un primer lugar, se analiza el efecto que tiene el medio en las propiedades ópticas. Para dicha evaluación se compara la variación de las propiedades de emisión de una capa de puntos enterrada y una superficial en distintas condiciones externas. El resultado que se obtiene es muy claro, los puntos enterrados no experimentan un cambio óptico apreciable cuando se varían las condiciones del entorno; mientras que, la emisión de los SQDs se modifica significativamente con las condiciones del medio. Por una parte, la intensidad de emisión de los puntos superficiales desaparece en condiciones de vacío y decrece notablemente en atmósferas secas de gases puros (N2, O2). Por otra parte, la fotoluminiscencia se conserva en ambientes húmedos. Adicionalmente, se observa que la anchura a media altura y la longitud de onda de emisión no se ven afectadas por los cambios en el medio, lo que indica, que las propiedades estructurales de los puntos se conservan al variar la atmósfera. Estos resultados apuntan directamente a los procesos que tienen lugar en la superficie entre estados confinados y superficiales como responsables principales de este comportamiento. Así mismo, se ha llevado a cabo un análisis más detallado de la influencia de la calidad y composición de la atmósfera en las propiedades ópticas de los puntos cuánticos superficiales. Para ello, se utilizan distintas sustancias con diferente polaridad, composición atómica y masa molecular. Como resultado se observa que las moléculas de menor polaridad y más pesadas causan una mayor variación en la intensidad de emisión. Además, se demuestra que el oxígeno juega un papel decisivo en las propiedades ópticas. En presencia de moléculas que contienen oxígeno, la intensidad de fotoluminiscencia disminuye menos que en atmósferas constituidas por especies que no contienen oxígeno. Las emisión que se observa respecto a la señal en aire es del 90% y del 77%, respectivamente, en atmósferas con presencia o ausencia de moléculas de oxígeno. El deterioro de la señal de emisión se atribuye a la presencia de defectos, enlaces insaturados y, en general, estados localizados en la superficie. Estos estados actúan como centros de recombinación no radiativa y, consecuentemente, se produce un empeoramiento de las propiedades ópticas de los SQDs. Por tanto, la eliminación o reducción de la densidad de estos estados superficiales haría posible una mejora de la intensidad de emisión. De estos experimentos de fotoluminiscencia, se deduce que las interacciones entre las moléculas presentes en la atmósfera y la superficie de la muestra modifican la superficie. Esta alteración superficial se traduce en un cambio significativo en las propiedades de emisión. Este comportamiento se atribuye a la posible adsorción de moléculas sobre la superficie pasivando los centros no radiativos, y como consecuencia, mejorando las propiedades ópticas. Además, los resultados demuestran que las moléculas que contienen oxígeno con mayor polaridad y más ligeras son adsorbidas con mayor facilidad, lo que hace que la intensidad óptica sufra variaciones despreciables con respecto a la emisión en aire. Con el fin de desarrollar sensores, las muestras se procesan y los dispositivos se caracterizan eléctricamente. El procesado consiste en dos contactos cuadrados de una aleación de Ti/Au. Durante el procesado, lo más importante a tener en cuenta es no realizar ningún ataque o limpieza que pueda dañar la superficie y deteriorar las propiedades de las nanostructuras. En este apartado, se realiza un análisis completo de una serie de tres muestras: GaAs (bulk), un pozo cuántico superficial (SQW) de Ino.5Gao.5As y SQDs de Ino.5Gao.5As. Para ello, a cada una de las muestras se le realizan medidas de I-V en distintas condiciones ambientales. En primer lugar, siguiendo los resultados obtenidos ópticamente, se lleva a cabo una comparación de la respuesta eléctrica en vacío y aire. A pesar de que todas las muestras presentan un carácter más resistivo en vacío que en aire, se observa una mayor influencia sobre la muestra de SQD. En vacío, la resistencia de los SQDs decrece un 99% respecto de su valor en aire, mientras que la variación de la muestras de GaAs e Ino.5Gao.5As SQW muestran una reducción, respectivamente, del 31% y del 20%. En segundo lugar, se realiza una evaluación aproximada del posible efecto de la humedad en la resistencia superficial de las muestras mediante la exhalación humana. Como resultado se obtiene, que tras la exhalación, la resistencia disminuye bruscamente y recupera su valor inicial cuando dicho proceso concluye. Este resultado preliminar indica que la humedad es un factor crítico en las propiedades eléctricas de los puntos cuánticos superficiales. Para la determinación del papel de la humedad en la respuesta eléctrica, se somete a las muestras de SQD y SQW a ambientes con humedad relativa (RH, de la siglas del inglés) controlada y se analiza el efecto sobre la conductividad superficial. Tras la variación de la RH desde 0% hasta el 70%, se observa que la muestra SQW no cambia su comportamiento eléctrico al variar la humedad del ambiente. Sin embargo, la respuesta de la muestra SQD define dos regiones bien diferenciadas, una de alta sensibilidad para valores por debajo del 50% de RH, en la que la resistencia disminuye hasta en un orden de magnitud y otra, de baja sensibilidad (>50%), donde el cambio de la resistencia es menor. Este resultado resalta la especial relevancia no sólo de la composición sino también de la morfología de la nanostructura superficial en el carácter sensitivo de la muestra. Por último, se analiza la influencia de la iluminación en la sensibilidad de la muestra. Nuevamente, se somete a las muestras SQD y SQW a una irradiación de luz de distinta energía y potencia a la vez que se varía controladamente la humedad ambiental. Una vez más, se observa que la muestra SQW no presenta ninguna variación apreciable con las alteraciones del entorno. Su resistencia superficial permanece prácticamente inalterable tanto al modificar la potencia de la luz incidente como al variar la energía de la irradiación. Por el contrario, en la muestra de SQD se obtiene una reducción la resistencia superficial de un orden de magnitud al pasar de condiciones de oscuridad a iluminación. Con respecto a la potencia y energía de la luz incidente, se observa que a pesar de que la muestra no experimenta variaciones notables con la potencia de la irradiación, esta sufre cambios significativos con la energía de la luz incidente. Cuando se ilumina con energías por encima de la energía de la banda prohibida (gap) del GaAs (Eg ~1.42 eV ) se produce una reducción de la resistencia de un orden de magnitud en atmósferas húmedas, mientras que en atmósferas secas la conductividad superficial permanece prácticamente constante. Sin embargo, al inicidir con luz de energía menor que Eg, el efecto que se produce en la respuesta eléctrica es despreciable. Esto se atribuye principalmente a la densidad de portadores fotoactivados durante la irradiación. El volumen de portadores excita dos depende de la energía de la luz incidente. De este modo, cuando la luz que incide tiene energía menor que el gap, el volumen de portadores generados es pequeño y no contribuye a la conductividad superficial. Por el contrario, cuando la energía de la luz incidente es alta (Eg), el volumen de portadores activados es elevado y éstos contribuyen significantemente a la conductividad superficial. La combinación de ambos agentes, luz y humedad, favorece el proceso de adsorción de moléculas y, por tanto, contribuye a la reducción de la densidad de estados superficiales, dando lugar a una modificación de la estructura electrónica y consecuentemente favoreciendo o dificultando el transporte de portadores. ABSTRACT Uncapped three-dimensional (3D) nanostructures have been generally grown to assess their structural quality. However, the tremendous growing importance of the impact of the environment on life has become such nanosystems in very promising candidates for the development of sensing devices. Their direct exposure to changes in the local surrounding may influence their physical properties being a perfect sign of the atmosphere quality. The goal of this thesis is the research of Ino.5Gao.5As surface quantum dots (SQDs) on GaAs(001), covering from their growth to device fabrication, for sensing applications. The achievement of this goal relies on the design, growth and sample characterization, along with device fabrication and characterization. The first issue of the thesis is devoted to analyze the main growth parameters affecting the physical properties of the Ino.5Gao.5As SQDs. It is well known that the growing conditions (growth temperature , deposition rate, V/III flux ratio and treatment after active layer growth) directly affect the physical properties of the epilayer. In this part, taking advantage of the previous results in the group regarding Ino.5Gao.5As QD growth temperature and V/III ratio, the effect of the growth rate and the temperature treatment after QDs growth nucleation is evaluated. Setting the QDs growth temperature at 430°C and the V/III flux ratio to ~20, it is found that the most appropriate conditions rely on growing the QDs at 0.07ML/s and just after QD nucleation, rapidly dropping and again raising 100°C the substrate temperature with respect to the temperature of QD growth. The combination of growing at a fast enough growth rate to promote molecule migration but sufficiently slow to allow QD nucleation, together with the sharp variation of the temperature preserving their shape and composition yield to high density, homogeneous Ino.5Gao.5As SQDs. Besides, it is also demonstrated that this high quality SQDs show excellent optical properties even at room temperature (RT). One of the characteristics by which In0.5Ga0.5As/GaAs SQDs are considered promising candidates for sensing applications is the crucial role that surface plays when interacting with the gases constituting the atmosphere. Therefore, in an attempt to develop sensing devices, the influence of the environment on the physical properties of the samples is evaluated. By comparing the resulting photoluminescence (PL) of SQDs with buried QDs (BQDs), it is found that BQDs do not exhibit any significant variation when changing the environmental conditions whereas, the external conditions greatly act on the SQDs optical properties. On one hand, it is evidenced that PL intensity of SQDs sharply quenches under vacuum and clearly decreases under dry-pure gases atmospheres (N2, O2). On the other hand, it is shown that, in water containing atmospheres, the SQDs PL intensity is maintained with respect to that in air. Moreover, it is found that neither the full width at half maximun nor the emission wavelength manifest any noticeable change indicating that the QDs are not structurally altered by the external atmosphere. These results decisively point to the processes taking place at the surface such as coupling between confined and surface states, to be responsible of this extraordinary behavior. A further analysis of the impact of the atmosphere composition on the optical characteristics is conducted. A sample containing one uncapped In0.5Ga0.5As QDs layer is exposed to different environments. Several solvents presenting different polarity, atomic composition and molecular mass, are used to change the atmosphere composition. It is revealed that low polarity and heavy molecules cause a greater variation on the PL intensity. Besides, oxygen is demonstrated to play a decisive role on the PL response. Results indicate that in presence of oxygen-containing molecules, the PL intensity experiments a less reduction than that suffered in presence of nonoxygen-containing molecules, 90% compared to 77% signal respect to the emission in air. In agreement with these results, it is demonstrated that high polarity and lighter molecules containing oxygen are more easily adsorbed, and consequently, PL intensity is less affected. The presence of defects, unsaturated bonds and in general localized states in the surface are proposed to act as nonradiative recombination centers deteriorating the PL emission of the sample. Therefore, suppression or reduction of the density of such states may lead to an increase or, at least, conservation of the PL signal. This research denotes that the interaction between sample surface and molecules in the atmosphere modifies the surface characteristics altering thus the optical properties. This is attributed to the likely adsoption of some molecules onto the surface passivating the nonradiative recombination centers, and consequently, not deteriorating the PL emission. Aiming for sensors development, samples are processed and electrically characterized under different external conditions. Samples are processed with two square (Ti/Au) contacts. During the processing, especial attention must be paid to the surface treatment. Any process that may damage the surface such as plasma etching or annealing must be avoided to preserve the features of the surface nanostructures. A set of three samples: a GaAs (bulk), In0.5Ga0.5As SQDs and In0.5Ga0.5As surface quantum well (SQW) are subjected to a throughout evaluation. I-V characteristics are measured following the results from the optical characterization. Firstly, the three samples are exposed to vacuum and air. Despite the three samples exhibit a more resistive character in vacuum than in air, it is revealed a much more clear influence of the pressure atmosphere in the SQDs sample. The sheet resistance (Rsh) of SQDs decreases a 99% from its response value under vacuum to its value in air, whereas Rsh of GaAs and In0.5Ga0.5As SQW reduces its value a 31% and a 20%, respectively. Secondly, a rough analysis of the effect of the human breath on the electrical response evidences the enormous influence of moisture (human breath is composed by several components but the one that overwhelms all the rest is the high concentration of water vapor) on the I-V characteristics. Following this result, In0.5Ga0.5As SQDs and In0.5Ga0.5As SQW are subjected to different controlled relative humidity (RH) environments (from 0% to 70%) and electrically characterized. It is found that SQW shows a nearly negligible Rsh variation when increasing the RH in the surroundings. However, the response of SQDs to changes in the RH defines two regions. Below 50%, high sensitive zone, Rsh of SQD decreases by more than one order of magnitude, while above 50% the dependence of Rsh on the RH becomes weaker. These results remark the role of the surface and denote the existence of a finite number of surface states. Nevertheless, most significantly, they highlight the importance not only of the material but also of the morphology. Finally, the impact of the illumination is determined by means of irradiating the In0.5Ga0.5As SQDs and In0.5Ga0.5As SQW samples with different energy and power sources. Once again, SQW does not exhibit any correlation between the surface conductivity and the external conditions. Rsh remains nearly unalterable independently of the energy and power of the incident light. Conversely, Rsh of SQD experiences a decay of one order of magnitude from dark-to-photo conditions. This is attributed to the less density of surface states of SQW compared to that of SQDs. Additionally, a different response of Rsh of SQD with the energy of the impinging light is found. Illuminating with high energy light results in a Rsh reduction of one order of mag nitude under humid atmospheres, whereas it remains nearly unchanged under dry environments. On the contrary, light with energy below the bulk energy bandgap (Eg), shows a negligible effect on the electrical properties regardless the local moisture. This is related to the density of photocarriers generated while lighting up. Illuminating with excitation energy below Eg affects a small absorption volume and thus, a low density of photocarriers may be activated leading to an insignificant contribution to the conductivity. Nonetheless, irradiating with energy above the Eg can excite a high density of photocarriers and greatly improve the surface conductivity. These results demonstrate that both illumination and humidity are therefore needed for sensing. The combination of these two agents improves the surface passivation by means of molecule adsorption reducing the density of surface states, thus modifying the electronic structures, and consequently, promoting the carrier motion.

(Table 1) Age determination of western North Atlantic sediment cores

Foraminiferal abundance, 14C ventilation ages, and stable isotope ratios in cores from high deposition rate locations in the western subtropical North Atlantic are used to infer changes in ocean and climate during the Younger Dryas (YD) and Last Glacial Maximum (LGM). The d18O of the surface dwelling planktonic foram Globigerinoides ruber records the present-day decrease in surface temperature (SST) of ~4°C from Gulf Stream waters to the northeastern Bermuda Rise. If during the LGM the modern d18O/salinity relationship was maintained, this SST contrast was reduced to 2°C. With LGM to interglacial d18O changes of at least 2.2 per mil, SSTs in the western subtropical gyre may have been as much as 5°C colder. Above ~2.3 km, glacial d13C was higher than today, consistent with nutrient-depleted (younger) bottom waters, as identified previously. Below that, d13C decreased continually to -0.5 per mil, about equal to the lowest LGM d13C in the North Pacific Ocean. Seven pairs of benthic and planktonic foraminiferal 14C dates from cores >2.5 km deep differ by 1100 ± 340 years, with a maximum apparent ventilation age of ~1500 years at 4250 m and at ~4700 m. Apparent ventilation ages are presently unavailable for the LGM < 2.5 km because of problems with reworking on the continental slope when sea level was low. Because LGM d13C is about the same in the deep North Atlantic and the deep North Pacific, and because the oldest apparent ventilation ages in the LGM North Atlantic are the same as the North Pacific today, it is possible that the same water mass, probably of southern origin, flowed deep within each basin during the LGM. Very early in the YD, dated here at 11.25 ± 0.25 (n = 10) conventional 14C kyr BP (equal to 12.9 calendar kyr BP), apparent ventilation ages <2.3 km water depth were about the same as North Atlantic Deep Water today. Below ~2.3 km, four YD pairs average 1030 ± 400 years. The oldest apparent ventilation age for the YD is 1600 years at 4250 m. This strong contrast in ventilation, which indicates a front between water masses of very different origin, is similar to glacial profiles of nutrient-like proxies. This suggests that the LGM and YD modes of ocean circulation were the same.

Protein utilisation and turnover in lines of chickens selected for different aspects of body composition

1. Protein utilisation and turnover were measured in male chickens sampled from a line selected for high breast yield and a randombred control line (lines QL and CL, experiment 1) and in male chickens sampled from lines selected for either high or low abdominal fatness (lines FL and LL, experiment 2). In each experiment, 18 birds per line were given iso-energetic (12.9 MJ ME/kg) diets containing either 120 or 220 g CP/kg from 21 to 29 d (experiment 1) and 33 to 43 d (experiment 2). 2. Measurements were made of growth rate, food intake, body composition, excreta production and N-tau-methylhistidine excretion as a measure of myofibrillar protein breakdown, and fractional rates (%/d) of protein deposition, breakdown and synthesis were calculated. 3. In experiment 1, there were no significant differences between the line means for the fractional measures of protein turnover, but there was marked differential response in the two lines in the fractional rates of protein deposition, breakdown and synthesis, to increase in protein intake. The positive slope of the regressions of fractional (%/d) protein deposition and synthesis rates on protein intake (g/d/kg BW) were approximately 1.4- and 2.0-fold higher respectively in the QL than the CL line birds, and the negative slope of the regression of fractional breakdown rate on protein intake was approximately threefold greater in the CL than the QL line birds. 4. In experiment 2, fractional deposition rate was 6.2% lower, but fractional breakdown rate 9.4% higher in the LL than the FL birds, whilst there was essentially no difference in response of the FL and LL birds in the components of protein turnover to increase in protein intake. Line differences in deposition and breakdown rates were thus a reflection of the considerably higher (20%) food and hence protein intake in the FL than the LL birds. 5. The differential line responses in protein turnover in the two experiments suggest that selection for increased breast muscle yield and for reduced body fatness manipulate different physiological pathways in relation to protein turnover, but neither selection strategy results in an improvement in net protein utilisation at typical levels of protein intake by birds on commercial broiler diets, through a reduction in protein breakdown rate.

Modulation of tissue transglutaminase in tubular epithelial cells alters extracellular matrix levels: a potential mechanism of tissue scarring

The up-regulation and trafficking of tissue transglutaminase (TG2) by tubular epithelial cells (TEC) has been implicated in the development of kidney scarring. TG2 catalyses the crosslinking of proteins via the formation of highly stable e(?-glutamyl) lysine bonds. We have proposed that TG2 may contribute to kidney scarring by accelerating extracellular matrix (ECM) deposition and by stabilising the ECM against proteolytic decay. To investigate this, we have studied ECM metabolism in Opossum kidney (OK) TEC induced to over-express TG2 by stable transfection and in tubular cells isolated from TG2 knockout mice. Increasing the expression of TG2 led to increased extracellular TG2 activity (p < 0.05), elevated e(?-glutamyl) lysine crosslinking in the ECM and higher levels of ECM collagen per cell by 3H-proline labelling. Immunofluorescence demonstrated that this was attributable to increased collagen III and IV levels. Higher TG2 levels were associated with an accelerated collagen deposition rate and a reduced ECM breakdown by matrix metalloproteinases (MMPs). In contrast, a lack of TG2 was associated with reduced e(?-glutamyl) lysine crosslinking in the ECM, causing reduced ECM collagen levels and lower ECM per cell. We report that TG2 contributes to ECM accumulation primarily by accelerating collagen deposition, but also by altering the susceptibility of the tubular ECM to decay. These findings support a role for TG2 in the expansion of the ECM associated with kidney scarring.

Chemical studies of plasma etchants used in integrated circuit manufacture

Plasma or "dry" etching is an essential process for the production of modern microelectronic circuits. However, despite intensive research, many aspects of the etch process are not fully understood. The results of studies of the plasma etching of Si and Si02 in fluorine-containing discharges, and the complementary technique of plasma polymerisation are presented in this thesis. Optical emission spectroscopy with argon actinometry was used as the principle plasma diagnostic. Statistical experimental design was used to model and compare Si and Si02 etch rates in CF4 and SF6 discharges as a function of flow, pressure and power. Etch mechanisms m both systems, including the potential reduction of Si etch rates in CF4 due to fluorocarbon polymer formation, are discussed. Si etch rates in CF4 /SF6 mixtures were successfully accounted for by the models produced. Si etch rates in CF4/C2F6 and CHF3 as a function of the addition of oxygen-containing additives (02, N20 and CO2) are shown to be consistent with a simple competition between F, 0 and CFx species for Si surface sites. For the range of conditions studied, Si02 etch rates were not dependent on F-atom concentration, but the presence of fluorine was essential in order to achieve significant etch rates. The influence of a wide range of electrode materials on the etch rate of Si and Si02 in CF4 and CF4 /02 plasmas was studied. It was found that the Si etch rate in a CF4 plasma was considerably enhanced, relative to an anodised aluminium electrode, in the presence of soda glass or sodium or potassium "doped" quartz. The effect was even more pronounced in a CF4 /02 discharge. In the latter system lead and copper electrodes also enhanced the Si etch rate. These results could not be accounted for by a corresponding rise in atomic fluorine concentration. Three possible etch enhancement mechanisms are discussed. Fluorocarbon polymer deposition was studied, both because of its relevance to etch mechanisms and its intrinsic interest, as a function of fluorocarbon source gas (CF4, C2F6, C3F8 and CHF3), process time, RF power and percentage hydrogen addition. Gas phase concentrations of F, H and CF2 were measured by optical emission spectroscopy, and the resultant polymer structure determined by X-ray photoelectron spectroscopy and infrared spectroscopy. Thermal and electrical properties were measured also. Hydrogen additions are shown to have a dominant role in determining deposition rate and polymer composition. A qualitative description of the polymer growth mechanism is presented which accounts for both changes in growth rate and structure, and leads to an empirical deposition rate model.

Ion plating

Under ideal conditions ion plating produces finely grained dense coatings with excellent adhesion. The ion bombardment induced damage initiates a large number of small nuclei. Simultaneous coating and sputtering stimulates high rates of diffusion and forms an interfacial region of graded composition responsible for good adhesion. To obtain such coatings on components far industrial applications, the design and construction Of an ion plater with a 24" (O.6rn) diameter chamber were investigated and modifications of the electron beam gun were proposed. A 12" (O.3m) diameter ion plater was designed and constructed. The equipment was used to develop surfaces for solar energy applications. The conditions to give extended surfaces by sputter etching were studied. Austenitic stainless steel was sputter etched at 20 and 30 mTorr working pressure and at 3, 4 and 5 kV. Uniform etching was achieved by redesigning the specimen holder to give a uniform electrostatic field over the surfaces of the specimens. Surface protrusions were observed after sputter etching. They were caused by the sputter process and were independent of grain boundaries, surface contaminants and inclusions. The sputtering rate of stainless steel was highly dependent on the background pressure which should be kept below 10-5 Torr. Sputter etching improved the performance of stainless steel used as a solar selective surface. A twofold improvement was achieved on sputter etching bright annealed stainless steel. However, there was only slight improvement after sputter etching stainless steel which had been mechanically polished to a mirror finish. Cooling curves Were used to measure the thermal emittance of specimens.The deposition rate of copper was measured at different levels of power input and was found to be a maximum at 9.5 kW. The diameter of the copper feed rod was found to be critical for the maintenance of a uniform evaporation rate.

Coke formation in the oxidative dehydrogenation of ethylbenzene to styrene by TEOM

A packed bed microbalance reactor setup (TEOM-GC) is used to investigate the formation of coke as a function of time-on-stream on γ-Al2O3 and 3P/SiO2 catalyst samples under different conditions for the ODH reaction of ethylbenzene to styrene. All samples show a linear correlation of the styrene selectivity and yield with the initial coverage of coke. The COX production increases with the coverage of coke. On the 3 wt% P/SiO2 sample, the initial coke build-up is slow and the coke deposition rate increases with time. On alumina-based catalyst samples, a fast initial coke build-up takes place, decreasing with time-on-stream, but the amount of coke does not stabilize. A higher O2 : EB feed ratio results in more coke, and a higher temperature results in less coke. This coking behaviour of Al2O3 can be described by existing "monolayer-multilayer" models. Further, the coverage of coke on the catalyst varies with the position in the bed. For maximal styrene selectivity, the optimal coverage of coke should be sufficient to convert all O2, but as low as possible to prevent selectivity loss by COX production. This is in favour of high temperature and low O2 : EB feed ratios. The optimal coke coverage depends in a complex way on all the parameters: temperature, the O2 : EB feed ratio, reactant concentrations, and the type of starting material. This journal is

Formation and investigation of nanostructured thin films

Small devices, in the range of nanometers, are playing a major role in today's technology. The field of nanotechnology is concerned with materials and systems whose structures and components exhibit novel and significantly improved physical, chemical and biological properties, phenomena and processes due to their small nanoscale size. Researches more and more are finding that structural features in the range of about 1 to 100 nanometers behave quite differently than isolated molecules (1 nanometer) or bulk materials. For comparison, a 10 nanometer structure is 1000 times smaller than the diameter of a human hair. The virtues of working in the nanodomain are increasingly recognized by the scientific community and discussed in the popular press. The use of such devices is expected to revolutionize our industries and lives. ^ This work mainly focuses on the fabrication, characterization and discovery of new nanostructured thin films. This research consists of the design of a new high-deposition rate nanoparticle machine for depositing nanostructured films from beams of nanoparticles and investigation film's unique optical and physical properties.^ A high-deposition rate nanoparticle machine was designed, built and successfully tested. Different nanostructured thin films were deposited from Copper, Gold, Iron and Zirconium targets with the grain size of between 1 to 20 nm under different conditions. Transmission Electron Microscopy (TEM), Atomic Force Microscopy (AFM), and x-ray diffraction (XRD) confirmed nanoscale grain size structures of deposited films. The optical properties of the nanostructured films deposited from copper, Iron and Zirconium targets were significantly different from optical properties of bulk and thin films. Zr, Cu and Fe films were transparent. Gold films revealed an epitaxial contact with the silicon substrate with interesting crystal structures. ^ The new high-deposition rate nanoparticle machine was able to deposit new nanostructured films with different properties from bulk and thin films reported in the literatures. ^

Description of manganese deposits collected by R/V Nothwind during the 1963 expedition in the Laptev sea

The 400-km-wide, low gradient Laptev Sea continental shelf consists of flat terrace-like features at regular depth intervals from 10 to 40 m below present sea level. The five large submarine valleys traversing the shelf do not continuously grade seaward, but contain elongated, closed basins. These terraces and closed basins plus deltaic sediments associated with the submarine valleys quite possibly mark sea level Stillstands, and enable reconstruction of the paleogeography of the Laptev Sea shore line at five periods during post-Wisconsin (Holocene) time. Radiocarbon dates on the silty-clay to clayey-silt sediments from cores of the northeastern Laptev Sea indicate average sedimentation intensity of 2 to 15 mg/cm2/yr. The presence of manganese nodules and crusts in surface samples from less than 55 m depths and a general decrease in total foraminiferal abundances with depth in the cores suggest that the present deposition rate is less than when sea level was lower. The main components of the shelf deposits are near- shore sediments which were spread over the shelf as Holocene sea level fluctuated and marine currents distributed modern fine sediment. Rare silty-sand layers and the coarser nuclei of the manganese crusts and nodules indicate ice rafting. However, this mechanism is probably only locally important as a significant transporting agent.

Prioritizing tropical habitats for long-distance migratory songbirds: an assessment of habitat quality at a stopover site in Colombia

Long-distance migratory birds are declining globally and migration has been identified as the primary source of mortality in this group. Despite this, our lack of knowledge of habitat use and quality at stopovers, i.e., sites where the energy for migration is accumulated, remains a barrier to designing appropriate conservation measures, especially in tropical regions. There is therefore an urgent need to assess stopover habitat quality and concurrently identify efficient and cost-effective methods for doing so. Given that fuel deposition rates directly influence stopover duration, departure fuel load, and subsequent speed of migration, they are expected to provide a direct measure of habitat quality and have the advantage of being measurable through body-mass changes. Here, we examined seven potential indicators of quality, including body-mass change, for two ecologically distinct Neotropical migratory landbirds on stopover in shade-coffee plantations and tropical humid premontane forest during spring migration in Colombia: (1) rate of body-mass change; (2) foraging rate; (3) recapture rate; (4) density; (5) flock size; (6) age and sex ratios; and (7) body-mass distribution. We found higher rates of mass change in premontane forest than in shade-coffee in Tennessee Warbler Oreothlypis peregrina, a difference that was mirrored in higher densities and body masses in forest. In Gray-cheeked Thrush Catharus minimus, a lack of recaptures in shade-coffee and higher densities in forest, also suggested that forest provided superior fueling conditions. For a reliable assessment of habitat quality, we therefore recommend using a suite of indicators, taking into account each species’ ecology and methodological considerations. Our results also imply that birds stopping over in lower quality habitats may spend a longer time migrating and require more stopovers, potentially leading to important carryover effects on reproductive fitness. Evaluating habitat quality is therefore imperative prior to defining the conservation value of newly identified stopover regions.

Percentages of sand-sized material and biogenic components in sediment core GIK12392-1

The paleo-oceanography of the southeastern North Atlantic Ocean during the last 150,000 yr has been studied using biogenous and terrigenous components of hemipelagic sediments sampled close to the northwest African continental margin. Variations of oxygen isotope ratios in shells of benthic calcareous foraminifers in two cores allow the assignment of absolute ages to these cores (in the best case at 1000 yr increments). The uncorrected bulk sedimentation rates of the longest core range from 3.4 to 7.6 cm/ 1000 yr during Interglacial conditions, and from 6.5 to 9.9 cm/1000 yr during Glacial conditions; all other cores have given results of the same order of magnitude, but with generally increasing values towards the continental edge. The distribution of sediment components allow us to make inferences about paleo-oceanographic changes in this region. Frequencies of biogenic components from benthic organisms, oxygen isotope ratios measured in benthic calcareous foraminiferal shells, the total carbonate contents of the sediment and distributions of biogenic components from planktonic organisms often fluctuate in concert. However, all fluctuations which can be attributed to changes of the bottom water masses (North Atlantic Deep Water) seem to precede by several thousand years those which can be linked to changes of the surface water mass distributions or to changes of the climate over the neighboring land masses. Late Quaternary planktonic foraminiferal assemblages in the cores from the northwest African continental margin can be defined satisfactorily in the way that distributions of assemblages found in sediment surface samples from the northeast Atlantic Ocean have been explained. The distributions of assemblages in the northwest African cores can also be used to estimate past sea surface temperatures and salinities. The downcore record of these estimates reveals two warm periods during the last 150,000 yr, the lower one corresponding to the oxygen isotope stage 5 e (equivalent to the Eemian proper in Europe), the upper one to the younger half of the Holocene. Winter surface water temperatures during oxygen isotope stages 6, 4, 3, and 2 are remarkably constant in most cores, while summer sea surface temperatures during stage 3 reach values comparable to those of the warm periods during the Late Holocene and Eemian. Estimated winter sea surface temperatures range from > 16 °C to < 11°C, the summer sea surface temperatures from > 22 °C to < 15 °C during the last 150,000 yr. Estimates of the winter sea surface salinities fluctuate between 36.6? and 35.5?, the higher values being restricted to the warm periods since the penultimate Glacial. Estimates for sea surface temperatures and salinities for two cores from the center of today's coastal upwelling region show less pronounced fluctuations than the record of the open ocean cores in the case of the station 12379 off Cape Barbas, more pronounced in the case of station 12328 off Cape Blanc. Seasonal differences between winter and summer sea surface temperatures derived from the estimated temperatures are today more pronounced in the boundary region of the ocean to the continent than further away from the continent. The differences are generally higher during warm climatic periods of the last 150,000 yr than during cooler ones. The abundance of terrigenous grains in the coarse fractions generally decreases with increasing distance from the continental edge, and also from south to north. The dominant portion of the terrigenous detritus is carried out into the ocean during the relatively cool climatic periods (stage 6, 4, later part of stage 3, stage 2 and oldest part of stage 1). The enhanced precision of dating combined with the stratigraphic resolution of these high deposition rate cores make it clear that the peaks of the terrigenous input off this part of the northwest African continental margin occur simultaneously with times of rapid sea level fluctuations resulting from large volume changes of the large Glacial ice sheets.