19 resultados para interactions plasma-surface

em Universidad Politécnica de Madrid


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Background Most aerial plant parts are covered with a hydrophobic lipid-rich cuticle, which is the interface between the plant organs and the surrounding environment. Plant surfaces may have a high degree of hydrophobicity because of the combined effects of surface chemistry and roughness. The physical and chemical complexity of the plant cuticle limits the development of models that explain its internal structure and interactions with surface-applied agrochemicals. In this article we introduce a thermodynamic method for estimating the solubilities of model plant surface constituents and relating them to the effects of agrochemicals. Results Following the van Krevelen and Hoftyzer method, we calculated the solubility parameters of three model plant species and eight compounds that differ in hydrophobicity and polarity. In addition, intact tissues were examined by scanning electron microscopy and the surface free energy, polarity, solubility parameter and work of adhesion of each were calculated from contact angle measurements of three liquids with different polarities. By comparing the affinities between plant surface constituents and agrochemicals derived from (a) theoretical calculations and (b) contact angle measurements we were able to distinguish the physical effect of surface roughness from the effect of the chemical nature of the epicuticular waxes. A solubility parameter model for plant surfaces is proposed on the basis of an increasing gradient from the cuticular surface towards the underlying cell wall. Conclusions The procedure enabled us to predict the interactions among agrochemicals, plant surfaces, and cuticular and cell wall components, and promises to be a useful tool for improving our understanding of biological surface interactions.

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Background Most aerial plant parts are covered with a hydrophobic lipid-rich cuticle, which is the interface between the plant organs and the surrounding environment. Plant surfaces may have a high degree of hydrophobicity because of the combined effects of surface chemistry and roughness. The physical and chemical complexity of the plant cuticle limits the development of models that explain its internal structure and interactions with surface-applied agrochemicals. In this article we introduce a thermodynamic method for estimating the solubilities of model plant surface constituents and relating them to the effects of agrochemicals. Results Following the van Krevelen and Hoftyzer method, we calculated the solubility parameters of three model plant species and eight compounds that differ in hydrophobicity and polarity. In addition, intact tissues were examined by scanning electron microscopy and the surface free energy, polarity, solubility parameter and work of adhesion of each were calculated from contact angle measurements of three liquids with different polarities. By comparing the affinities between plant surface constituents and agrochemicals derived from (a) theoretical calculations and (b) contact angle measurements we were able to distinguish the physical effect of surface roughness from the effect of the chemical nature of the epicuticular waxes. A solubility parameter model for plant surfaces is proposed on the basis of an increasing gradient from the cuticular surface towards the underlying cell wall. Conclusions The procedure enabled us to predict the interactions among agrochemicals, plant surfaces, and cuticular and cell wall components, and promises to be a useful tool for improving our understanding of biological surface interactions.

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Plant trichomes play important protective functions and may have a major influence on leaf surface wettability. With the aim of gaining insight into trichome structure, composition and function in relation to water-plant surface interactions, we analyzed the adaxial and abaxial leaf surface of Quercus ilex L. (holm oak) as model. By measuring the leaf water potential 24 h after the deposition of water drops on to abaxial and adaxial surfaces, evidence for water penetration through the upper leaf side was gained in young and mature leaves. The structure and chemical composition of the abaxial (always present) and adaxial (occurring only in young leaves) trichomes were analyzed by various microscopic and analytical procedures. The adaxial surfaces were wettable and had a high degree of water drop adhesion in contrast to the highly unwettable and water repellent abaxial holm oak leaf sides. The surface free energy, polarity and solubility parameter decreased with leaf age, with generally higher values determined for the abaxial sides. All holm oak leaf trichomes were covered with a cuticle. The abaxial trichomes were composed of 8% soluble waxes, 49% cutin, and 43% polysaccharides. For the adaxial side, it is concluded that trichomes and the scars after trichome shedding contribute to water uptake, while the abaxial leaf side is highly hydrophobic due to its high degree of pubescence and different trichome structure, composition and density. Results are interpreted in terms of water-plant surface interactions, plant surface physical-chemistry, and plant ecophysiology.

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The coherent three-wave interaction, with linear growth in the higher frequency wave and damping in the two other waves, is reconsidered; for equal dampings, the resulting three-dimensional (3-D) flow of a relative phase and just two amplitudes behaved chaotically, no matter how small the growth of the unstable wave. The general case of different dampings is studied here to test whether, and how, that hard scenario for chaos is preserved in passing from 3-D to four-dimensional flows. It is found that the wave with higher damping is partially slaved to the other damped wave; this retains a feature of the original problem an invariant surface that meets an unstable fixed point, at zero growth rate! that gave rise to the chaotic attractor and determined its structure, and suggests that the sudden transition to chaos should appear in more complex wave interactions.

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En esta tesis se investiga la interacción entre un fluido viscoso y un cuerpo sólido en presencia de una superficie libre. El problema se expresa teóricamente poniendo especial atención a los aspectos de conservación de energía y de la interacción del fluido con el cuerpo. El problema se considera 2D y monofásico, y un desarrollo matemático permite una descomposición de los términos disipativos en términos relacionados con la superficie libre y términos relacionados con la enstrofía. El modelo numérico utilizado en la tesis se basa en el método sin malla Smoothed Particle Hydrodynamics (SPH). De manera análoga a lo que se hace a nivel continuo, las propiedades de conservación se estudian en la tesis con el sistema discreto de partículas. Se tratan también las condiciones de contorno de un cuerpo que se mueve en un flujo viscoso, implementadas con el método ghost-fluid. Se ha desarrollado un algoritmo explícito de interacción fluido / cuerpo. Se han documentado algunos casos de modo detallado con el objetivo de comprobar la capacidad del modelo para reproducir correctamente la disipación de energía y el movimiento del cuerpo. En particular se ha investigado la atenuación de una onda estacionaria, comparando la simulación numérica con predicciones teóricas. Se han realizado otras pruebas para monitorizar la disipación de energía para flujos más violentos que implican la fragmentación de la superficie libre. La cantidad de energía disipada con los diferentes términos se ha evaluado en los casos estudiados con el modelo numérico. Se han realizado otras pruebas numéricas para verificar la técnica de modelización de la interacción fluido / cuerpo, concretamente las fuerzas ejercidas por las olas en cuerpos con formas simples, y el equilibrio de un cuerpo flotante con una forma compleja. Una vez que el modelo numérico ha sido validado, se han realizado simulaciones numéricas para obtener una comprensión más completa de la física implicada en casos (casi) realistas sobre los había aspectos que no se conocían suficientemente. En primer lugar se ha estudiado el el flujo alrededor de un cilindro bajo la superficie libre. El estudio se ha realizado con un número de Reynolds moderado, para un rango de inmersiones del cilindro y números de Froude. La solución numérica permite una investigación de los patrones complejos que se producen. La estela del cilindro interactúa con la superficie libre. Se han identificado algunos inestabilidades características. El segundo estudio se ha realizado sobre el problema de sloshing, tanto experimentalmente como numéricamente. El análisis se restringe a aguas poco profundas y con oscilación horizontal, pero se ha estudiado un gran número de condiciones, lo que lleva a una comprensión bastante completa de los sistemas de onda involucradas. La última parte de la tesis trata también sobre un problema de sloshing pero esta vez el tanque está oscilando con rotación y hay acoplamiento con un sistema mecánico. El sistema se llama pendulum-TLD (Tuned Liquid Damper - con líquido amortiguador). Este tipo de sistema se utiliza normalmente para la amortiguación de las estructuras civiles. El análisis se ha realizado analíticamente, numéricamente y experimentalmente utilizando líquidos con viscosidades diferentes, centrándose en características no lineales y mecanismos de disipación. ABSTRA C T The subject of the present thesis is the interaction between a viscous fluid and a solid body in the presence of a free surface. The problem is expressed first theoretically with a particular focus on the energy conservation and the fluid-body interaction. The problem is considered 2D and monophasic, and some mathematical development allows for a decomposition of the energy dissipation into terms related to the Free Surface and others related to the enstrophy. The numerical model used on the thesis is based on Smoothed Particle Hydrodynamics (SPH): a computational method that works by dividing the fluid into particles. Analogously to what is done at continuum level, the conservation properties are studied on the discrete system of particles. Additionally the boundary conditions for a moving body in a viscous flow are treated and discussed using the ghost-fluid method. An explicit algorithm for handling fluid-body coupling is also developed. Following these theoretical developments on the numerical model, some test cases are devised in order to test the ability of the model to correctly reproduce the energy dissipation and the motion of the body. The attenuation of a standing wave is used to compare what is numerically simulated to what is theoretically predicted. Further tests are done in order to monitor the energy dissipation in case of more violent flows involving the fragmentation of the free-surface. The amount of energy dissipated with the different terms is assessed with the numerical model. Other numerical tests are performed in order to test the fluid/body interaction method: forces exerted by waves on simple shapes, and equilibrium of a floating body with a complex shape. Once the numerical model has been validated, numerical tests are performed in order to get a more complete understanding of the physics involved in (almost) realistic cases. First a study is performed on the flow passing a cylinder under the free surface. The study is performed at moderate Reynolds numbers, for various cylinder submergences, and various Froude numbers. The capacity of the numerical solver allows for an investigation of the complex patterns which occur. The wake from the cylinder interacts with the free surface, and some characteristical flow mechanisms are identified. The second study is done on the sloshing problem, both experimentally and numerically. The analysis is restrained to shallow water and horizontal excitation, but a large number of conditions are studied, leading to quite a complete understanding of the wave systems involved. The last part of the thesis still involves a sloshing problem but this time the tank is rolling and there is coupling with a mechanical system. The system is named pendulum-TLD (Tuned Liquid Damper). This kind of system is normally used for damping of civil structures. The analysis is then performed analytically, numerically and experimentally for using liquids with different viscosities, focusing on non-linear features and dissipation mechanisms.

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Electric probes are objects immersed in the plasma with sharp boundaries which collect of emit charged particles. Consequently, the nearby plasma evolves under abrupt imposed and/or naturally emerging conditions. There could be localized currents, different time scales for plasma species evolution, charge separation and absorbing-emitting walls. The traditional numerical schemes based on differences often transform these disparate boundary conditions into computational singularities. This is the case of models using advection-diffusion differential equations with source-sink terms (also called Fokker-Planck equations). These equations are used in both, fluid and kinetic descriptions, to obtain the distribution functions or the density for each plasma species close to the boundaries. We present a resolution method grounded on an integral advancing scheme by using approximate Green's functions, also called short-time propagators. All the integrals, as a path integration process, are numerically calculated, what states a robust grid-free computational integral method, which is unconditionally stable for any time step. Hence, the sharp boundary conditions, as the current emission from a wall, can be treated during the short-time regime providing solutions that works as if they were known for each time step analytically. The form of the propagator (typically a multivariate Gaussian) is not unique and it can be adjusted during the advancing scheme to preserve the conserved quantities of the problem. The effects of the electric or magnetic fields can be incorporated into the iterative algorithm. The method allows smooth transitions of the evolving solutions even when abrupt discontinuities are present. In this work it is proposed a procedure to incorporate, for the very first time, the boundary conditions in the numerical integral scheme. This numerical scheme is applied to model the plasma bulk interaction with a charge-emitting electrode, dealing with fluid diffusion equations combined with Poisson equation self-consistently. It has been checked the stability of this computational method under any number of iterations, even for advancing in time electrons and ions having different time scales. This work establishes the basis to deal in future work with problems related to plasma thrusters or emissive probes in electromagnetic fields.

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urface treatments have been recently shown to play an active role in electrical characteristics in AlGaN/GaN HEMTs, in particular during the passivation processing [1-4]. However, the responsible mechanisms are partially unknown and further studies are demanding. The effects of power and time N2 plasma pre-treatment prior to SiN deposition using PE-CVD (plasma enhanced chemical vapour deposition) on GaN and AlGaN/GaN HEMT have been investigated. The low power (60 W) plasma pre-treatment was found to improve the electronic characteristics in GaN based HEMT devices, independently of the time duration up to 20 min. In contrast, high power (150 and 210 W) plasma pretreatment showed detrimental effects in the electronic properties (Fig. 1), increasing the sheet resistance of the 2DEG, decreasing the 2DEG charge density in AlGaN/GaN HEMTs, transconductance reduction and decreasing the fT and fmax values up to 40% respect to the case using 60 W N2 plasma power. Although AFM (atomic force microscopy) results showed AlGaN and GaN surface roughness is not strongly affected by the N2-plasma, KFM (Kelvin force microscopy) surface analysis shows significant changes in the surface potential, trending to increase its values as the plasma power is higher. The whole results point at energetic ions inducing polarization-charge changes that affect dramatically to the 2-DEG charge density and the final characteristics of the HEMT devices. Therefore, we conclude that AlGaN surface is strongly sensitive to N2 plasma power conditions, which turn to be a key factor to achieve a good surface preparation prior to SiN passivation.

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Analysis of river flow using hydraulic modelling and its implications in derived environ-mental applications are inextricably connected with the way in which the river boundary shape is represented. This relationship is scale-dependent upon the modelling resolution which in turn determines the importance of a subscale performance of the model and the way subscale (surface and flow) processes are parameterised. Commonly, the subscale behaviour of the model relies upon a roughness parameterisation whose meaning depends on the dimensionality of the hydraulic model and the resolution of the topographic represen¬tation scale. This latter is, in turn, dependent on the resolution of the computational mesh as well as on the detail of measured topographic data. Flow results are affected by this interactions between scale and subscale parameterisation according to the dimensionality approach. The aim of this dissertation is the evaluation of these interactions upon hy¬draulic modelling results. Current high resolution topographic source availability induce this research which is tackled using a suitable roughness approach according to each di¬mensionality with the purpose of the interaction assessment. A 1D HEC-RAS model, a 2D raster-based diffusion-wave model with a scale-dependent distributed roughness parame-terisation and a 3D finite volume scheme with a porosity algorithm approach to incorporate complex topography have been used. Different topographic sources are assessed using a 1D scheme. LiDAR data are used to isolate the mesh resolution from the topographic content of the DEM effects upon 2D and 3D flow results. A distributed roughness parameterisation, using a roughness height approach dependent upon both mesh resolution and topographic content is developed and evaluated for the 2D scheme. Grain-size data and fractal methods are used for the reconstruction of topography with microscale information, required for some applications but not easily available. Sensitivity of hydraulic parameters to this topographic parameterisation is evaluated in a 3D scheme at different mesh resolu¬tions. Finally, the structural variability of simulated flow is analysed and related to scale interactions. Model simulations demonstrate (i) the importance of the topographic source in a 1D models; (ii) the mesh resolution approach is dominant in 2D and 3D simulations whereas in a 1D model the topographic source and even the roughness parameterisation impacts are more critical; (iii) the increment of the sensitivity to roughness parameterisa-tion in 1D and 2D schemes with detailed topographic sources and finer mesh resolutions; and (iv) the topographic content and microtopography impact throughout the vertical profile of computed 3D velocity in a depth-dependent way, whereas 2D results are not affected by topographic content variations. Finally, the spatial analysis shows that the mesh resolution controls high resolution model scale results, roughness parameterisation control 2D simulation results for a constant mesh resolution; and topographic content and micro-topography variations impacts upon the organisation of flow results depth-dependently in a 3D scheme. Resumen La topografía juega un papel fundamental en la distribución del agua y la energía en los paisajes naturales (Beven and Kirkby 1979; Wood et al. 1997). La simulación hidráulica combinada con métodos de medición del terreno por teledetección constituyen una poderosa herramienta de investigación en la comprensión del comportamiento de los flujos de agua debido a la variabilidad de la superficie sobre la que fluye. La representación e incorporación de la topografía en el esquema hidráulico tiene una importancia crucial en los resultados y determinan el desarrollo de sus aplicaciones al campo medioambiental. Cualquier simulación es una simplificación de un proceso del mundo real, y por tanto el grado de simplificación determinará el significado de los resultados simulados. Este razonamiento es particularmente difícil de trasladar a la simulación hidráulica donde aspectos de la escala tan diferentes como la escala de los procesos de flujo y de representación del contorno son considerados conjuntamente incluso en fases de parametrización (e.g. parametrización de la rugosidad). Por una parte, esto es debido a que las decisiones de escala vienen condicionadas entre ellas (e.g. la dimensionalidad del modelo condiciona la escala de representación del contorno) y por tanto interaccionan en sus resultados estrechamente. Y por otra parte, debido a los altos requerimientos numéricos y computacionales de una representación explícita de alta resolución de los procesos de flujo y discretización de la malla. Además, previo a la modelización hidráulica, la superficie del terreno sobre la que el agua fluye debe ser modelizada y por tanto presenta su propia escala de representación, que a su vez dependerá de la escala de los datos topográficos medidos con que se elabora el modelo. En última instancia, esta topografía es la que determina el comportamiento espacial del flujo. Por tanto, la escala de la topografía en sus fases de medición y modelización (resolución de los datos y representación topográfica) previas a su incorporación en el modelo hidráulico producirá a su vez un impacto que se acumulará al impacto global resultante debido a la escala computacional del modelo hidráulico y su dimensión. La comprensión de las interacciones entre las complejas geometrías del contorno y la estructura del flujo utilizando la modelización hidráulica depende de las escalas consideradas en la simplificación de los procesos hidráulicos y del terreno (dimensión del modelo, tamaño de escala computacional y escala de los datos topográficos). La naturaleza de la aplicación del modelo hidráulico (e.g. habitat físico, análisis de riesgo de inundaciones, transporte de sedimentos) determina en primer lugar la escala del estudio y por tanto el detalle de los procesos a simular en el modelo (i.e. la dimensionalidad) y, en consecuencia, la escala computacional a la que se realizarán los cálculos (i.e. resolución computacional). Esta última a su vez determina, el detalle geográfico con que deberá representarse el contorno acorde con la resolución de la malla computacional. La parametrización persigue incorporar en el modelo hidráulico la cuantificación de los procesos y condiciones físicas del sistema natural y por tanto debe incluir no solo aquellos procesos que tienen lugar a la escala de modelización, sino también aquellos que tienen lugar a un nivel subescalar y que deben ser definidos mediante relaciones de escalado con las variables modeladas explícitamente. Dicha parametrización se implementa en la práctica mediante la provisión de datos al modelo, por tanto la escala de los datos geográficos utilizados para parametrizar el modelo no sólo influirá en los resultados, sino también determinará la importancia del comportamiento subescalar del modelo y el modo en que estos procesos deban ser parametrizados (e.g. la variabilidad natural del terreno dentro de la celda de discretización o el flujo en las direcciones laterales y verticales en un modelo unidimensional). En esta tesis, se han utilizado el modelo unidimensional HEC-RAS, (HEC 1998b), un modelo ráster bidimensional de propagación de onda, (Yu 2005) y un esquema tridimensional de volúmenes finitos con un algoritmo de porosidad para incorporar la topografía, (Lane et al. 2004; Hardy et al. 2005). La geometría del contorno viene definida por la escala de representación topográfica (resolución de malla y contenido topográfico), la cual a su vez depende de la escala de la fuente cartográfica. Todos estos factores de escala interaccionan en la respuesta del modelo hidráulico a la topografía. En los últimos años, métodos como el análisis fractal y las técnicas geoestadísticas utilizadas para representar y analizar elementos geográficos (e.g. en la caracterización de superficies (Herzfeld and Overbeck 1999; Butler et al. 2001)), están promoviendo nuevos enfoques en la cuantificación de los efectos de escala (Lam et al. 2004; Atkinson and Tate 2000; Lam et al. 2006) por medio del análisis de la estructura espacial de la variable (e.g. Bishop et al. 2006; Ju et al. 2005; Myint et al. 2004; Weng 2002; Bian and Xie 2004; Southworth et al. 2006; Pozd-nyakova et al. 2005; Kyriakidis and Goodchild 2006). Estos métodos cuantifican tanto el rango de valores de la variable presentes a diferentes escalas como la homogeneidad o heterogeneidad de la variable espacialmente distribuida (Lam et al. 2004). En esta tesis, estas técnicas se han utilizado para analizar el impacto de la topografía sobre la estructura de los resultados hidráulicos simulados. Los datos de teledetección de alta resolución y técnicas GIS también están siendo utilizados para la mejor compresión de los efectos de escala en modelos medioambientales (Marceau 1999; Skidmore 2002; Goodchild 2003) y se utilizan en esta tesis. Esta tesis como corpus de investigación aborda las interacciones de esas escalas en la modelización hidráulica desde un punto de vista global e interrelacionado. Sin embargo, la estructura y el foco principal de los experimentos están relacionados con las nociones espaciales de la escala de representación en relación con una visión global de las interacciones entre escalas. En teoría, la representación topográfica debe caracterizar la superficie sobre la que corre el agua a una adecuada (conforme a la finalidad y dimensión del modelo) escala de discretización, de modo que refleje los procesos de interés. La parametrización de la rugosidad debe de reflejar los efectos de la variabilidad de la superficie a escalas de más detalle que aquellas representadas explícitamente en la malla topográfica (i.e. escala de discretización). Claramente, ambos conceptos están físicamente relacionados por un

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The influence of nanosecond laser pulses applied by laser shock peening without absorbent coating (LSPwC) with a Q-switched Nd:YAG laser operating at a wavelength of λ = 1064 nm on 6082-T651 Al alloy has been investigated. The first portion of the present study assesses laser shock peening effect at two pulse densities on three-dimensional (3D) surface topography characteristics. In the second part of the study, the peening effect on surface texture orientation and micro-structure modification, i.e. the effect of surface craters due to plasma and shock waves, were investigated in both longitudinal (L) and transverse (T) directions of the laser-beam movement. In the final portion of the study, the changes of mechanical properties were evaluated with a residual stress profile and Vickers micro-hardness through depth variation in the near surface layer, whereas factorial design with a response surface methodology (RSM) was applied. The surface topographic and micro-structural effect of laser shock peening were characterised with optical microscopy, InfiniteFocus® microscopy and scanning electron microscopy (SEM). Residual stress evaluation based on a hole-drilling integral method confirmed higher compression at the near surface layer (33 μm) in the transverse direction (σmin) of laser-beam movement, i.e. − 407 ± 81 MPa and − 346 ± 124 MPa, after 900 and 2500 pulses/cm2, respectively. Moreover, RSM analysis of micro-hardness through depth distribution confirmed an increase at both pulse densities, whereas LSPwC-generated shock waves showed the impact effect of up to 800 μm below the surface. Furthermore, ANOVA results confirmed the insignificant influence of LSPwC treatment direction on micro-hardness distribution indicating essentially homogeneous conditions, in both L and T directions.

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A novel concept for active space debris removal known as Ion Beam Shepherd (IBS) which has been recently presented by our group is investigated. The concept makes use of a highly collimated ion beam to exert the necessary force on a generic debris to modify its orbit and/or attitude from a safe distance in a controlled manner, without the need of docking. After describing the main characteristics of the IBS system, some of the key aspects of thruster plasma and its interaction with the debris are studied, namely, (1) the modeling of the expansion of an plasma beam, based on the quasi-selfsimilarity exhibited by hypersonic plumes, (2) the characterization of the force and torque exerted upon the target debris, and (3) a preliminary evaluation of other plasma-body interactions.

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A study supported by the European Space Agency (ESA), in the context of its General Studies Programme, performed an investigation of the possible use of space for studies in pure and applied plasma physics, in areas not traditionally covered by ‘space plasma physics’. A set of experiments have been identified that can potentially provide access to new phenomena and to allow advances in several fields of plasma science. These experiments concern phenomena on a spatial scale (101–104 m) intermediate between what is achievable on the ground and the usual solar system plasma observations. Detailed feasibility studies have been performed for three experiments: active magnetic experiments, largescale discharges and long tether–plasma interactions. The perspectives opened by these experiments are discussed for magnetic reconnection, instabilities, MHD turbulence, atomic excited states kinetics, weakly ionized plasmas,plasma diagnostics, artificial auroras and atmospheric studies. The discussion is also supported by results of numerical simulations and estimates.

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The effects of power and time conditions of in situ N2 plasma treatment, prior to silicon nitride (SiN) passivation, were investigated on an AlGaN/GaN high-electron mobility transistor (HEMT). These studies reveal that N2 plasma power is a critical parameter to control the SiN/AlGaN interface quality, which directly affects the 2-D electron gas density. Significant enhancement in the HEMT characteristics was observed by using a low power N2 plasma pretreatment. In contrast, a marked gradual reduction in the maximum drain-source current density (IDS max) and maximum transconductance (gm max), as well as in fT and fmax, was observed as the N2 plasma power increases (up to 40% decrease for 210 W). Different mechanisms were proposed to be dominant as a function of the discharge power range. A good correlation was observed between the device electrical characteristics and the surface assessment by atomic force microscopy and Kelvin force microscopy techniques.

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On 22nd February '96, the space mission STS 75 started ,from the NASA facilities at Cape Canaveral. Such a mission consists in the launch of the shuttle Columbia in order to carry out two experiments in the space: the TSS 1R (Tethered Satellite Sistem 1 Refliight) and the USMP (United States Microgravity Payload). The TSS 1R is a replica of a similar mission TSS 1 '92. The TSS space programme is a bilateral scientific cooperation between the USA space agency NASA (National Aeronautics and Space Agency) and the ASI (Italian Space Agency. The TSS 1R system consists on the shuttle Columbia which deploys, up-ward, by means a conducting tether 20 km long, a spherical satellite (1.5 mt diameter) containing scientific instrumentation. This system, orbiting at about 300 km from the Earth's surface, represents, presently, the largest experimental space structure, Due to its dimensions, flexibility and conducting properties of the tether, the system interacts, in a quite complex manner, wih the earth magnetic field and the ionospheric plasma, in a way that the total system behaves as an electromagnetic radiating antenna as well as an electric power generator. Twelve scientific experiments have been assessed by US and Italian scientists in order to study the electro dynamic behaviour of the structure orbiting in the ionos phere. Two experiments have been prepared in the attempt to receive on the Earth's surface possible electromagnetic events radiated by the TSS 1R. The project EMET (Electro Magnetic Emissions from Tether),USA and the project OESEE (Observations on the Earth Surface of Electromagnetic Emissions) Italy, consist in a coordinated programme of passive detection of such possible EM emissions. This detection will supply the verification of some thoretical hypotheses on the electrodynamic interactions between the orbiting system, the Earth's magnetic field and the ionospheric plasma with two principal aims as the technological assesment of the system concept as well as a deeper knowledge of the ionosphere properties for future space applications. A theoretical model that keeps the peculiarities of tether emissionsis being developed for signal prediction at constant tether current. As a step previous to the calculation of the expected ground signal , the Alfven-wave signature left by the tether far back in the ionosphere has been determined. The scientific expectations from the combined effort to measure the entity of those perturbations will be outlined taking in to account the used ground track sensor systems.

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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.

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We investigate the dynamics of localized solutions of the relativistic cold-fluid plasma model in the small but finite amplitude limit, for slightly overcritical plasma density. Adopting a multiple scale analysis, we derive a perturbed nonlinear Schrödinger equation that describes the evolution of the envelope of circularly polarized electromagnetic field. Retaining terms up to fifth order in the small perturbation parameter, we derive a self-consistent framework for the description of the plasma response in the presence of localized electromagnetic field. The formalism is applied to standing electromagnetic soliton interactions and the results are validated by simulations of the full cold-fluid model. To lowest order, a cubic nonlinear Schrödinger equation with a focusing nonlinearity is recovered. Classical quasiparticle theory is used to obtain analytical estimates for the collision time and minimum distance of approach between solitons. For larger soliton amplitudes the inclusion of the fifth-order terms is essential for a qualitatively correct description of soliton interactions. The defocusing quintic nonlinearity leads to inelastic soliton collisions, while bound states of solitons do not persist under perturbations in the initial phase or amplitude