No description available.

No description available.

This thesis investigates geo-electric fields in the United Kingdom with particular regard to Geomagnetically Induced Currents (GIC) in the Scottish Power electricity transmission network (SPTN). The joint spectral characteristics of Scottish Power GIC and Eskdalemuir magnetic observatory data are analysed, and GIC are shown to be coherent with magnetic field variations over the period range 2-1100s. A bi-variate transfer function model of the physical link between magnetic field variations and GIC demonstrates that long-period (>200s) induction makes a first order contribution to the observed GIC at one SPTN site, and dominates the response at another. Thin-sheet modelling at a period of 750s is used to explore the relative influence of three factors on the size and spatial distribution of the calculated electric field: (i) the contrast in conductance between the sea and the land; (ii) variations in conductance due to sea depth; (iii) lateral variations in conductance representative of those in the geographic area occupied by the SPTN. The modelling suggests that a `coast-only' model (i) will over-predict electric field magnitudes in the SPTN region by a factor of 2-5 in comparison with model (iii). Distortion analysis of Magnetotelluric (MT) data at a period of 750s acquired over numerous field campaigns reveal pervasive galvanic distortion of the electric field in the SPTN region. GIC transfer functions of one site are consistently interpreted as proxy MT responses, and it is shown that galvanic distortion of the electric field modifies significantly the GIC amplitude response. A prototype model of the SPTN developed by the British Geological Survey and the Finnish Meteorological Institute is used to calculate GIC. It is shown that neglect of lateral variations of conductivity may lead to false conclusions about the direction of the external electric field that maximises GIC. Time derivatives of the Eskdalemuir horizontal magnetic field are used as an index of GIC activity, and to select events which may have led to large GIC in the time period (1983-2000) prior to the monitoring of GIC by Scottish Power. Backwards-prediction using the GIC transfer functions and observatory magnetic data suggests that GIC at the Scottish Power monitoring sites have amplitudes less than approximately 30A.

No description available.

There has been a rapid growth of terrestrial and satellite communications in the last few decades of the 20th century. This has resulted in a heavy congestion of low microwave bands and has been a major driving force for exploring the upper microwave and millimeter-wave frequencies. One of the main requirements for a successful shift to the new frequency spectrum is the availability of high power solid-state transmitters. Solid-state devices such as diodes or transistors have been able to meet such demands when their output signals are combined using space-level power combining methods that avoid conduction losses, which become pronounced at millimeter wave frequencies. In this thesis, theoretical and experimental investigations are carried out into the spatial power combiners (SPCs) which employ active planar arrays formed by transistor amplifiers whose input and output ports are equipped with planar radiating elements. The SPC structures include the reflection-type combiner using the tile configuration of planar array and the transmission-type combiner using tile or tray configurations of planar arrays. The frequency bands chosen for the designing and testing of prototypes are X- and Ku-band. The first stage of the investigation concerns the 10 GHz reflection-type power combiner structure formed by a phased planar microstrip reflectarray (MRA) of 37-element dual-feed aperture coupled microstrip patch antennas equipped with open-circuit stubs as phasing components. The experimental tests reveal poor radiation performance and hence poor power combining efficiency of this structure. These results indicated the need for theoretical investigations into the operation of this type of SPC. The study of the unit cell of this power combiner reveals that the phase of an open-circuit stub does not increase linearly as a function of the stub length and its range is limited to less than (about is required for proper functioning). This finding, forms the basis for extending the investigations into alternative phasing mechanisms of a MRA which would offer a phasing range exceeding . A phasing mechanism exploiting variable size stacked patches is chosen. In order to accurately determine the phasing of the reflected wave, a theory based on an equivalent unit cell waveguide approach (WGA) is proposed and developed. The proposed theory is computationally efficient and is proven to be accurate compared with benchmark results published by other researchers. Following the verification, an offset feed 161-element two-layer printed MRA prototype with patches of variable size is designed and developed for operation in Ku-band. The test results aim at verifying the validity of applying a unit cell WGA to designing passive and active MRAs. The next investigations, which are presented in the thesis concern increasing operational bandwidth of the transmission-type SPC in tile configuration. The designs presented so far in the open literatures were based on edge-feed microstrip patch antennas as radiating elements of individual active stages and featured a narrow-band performance. In order to overcome this shortcoming, stacked patch (SP) microstrip antennas as receiving and transmitting elements in an active transmitarray (TXA) are proposed. For the aim of testing the proposed concept, a 16-element SP TXA is designed for operation in X-band. Two identical hard horn antennas with an approximately uniform field across the aperture for signal launching and collecting complete the design and development of this space-level power combiner. The performance of the developed device is assessed experimentally and an increased operational bandwidth is demonstrated. The final structure being investigated in the thesis project is the transmission-type SPC in tray configuration. This power combining structure employs a travelling wave antenna of uniplanar quasi-Yagi type as a radiating element to achieve broad-band operation. The investigated SPC is formed by seven trays of uniplanar quasi-Yagi antenna. In order to achieve uniform and in-phase excitation of individual trays, which is required to obtain high power combining efficiency, hard horn antennas and Schiffman phase shifters are employed in the design of this space-level combiner. The proposed device is developed and its performance is assessed through experiments. The work performed as part of this Ph.D. thesis project has resulted in 5 journal papers and 11 refereed conference papers. This acceptance rate supports the claim of the originality and significance of the research undertaken as part of the thesis project.

Prolongement central de la sclère, la cornée est la couche la plus externe de l'œil. Elle laisser pénétrer la lumière dans le globe oculaire grâce à sa propriété de transparence. Cette transparence repose sur une structure très organisée du tissu, maintenue en équilibre physiologique. Lorsque cet équilibre est rompu, notamment suite à une augmentation anormale de son taux d'hydratation et au développement d'un œdème, l'épaisseur du tissu augmente et il tend à s'opacifier. Lorsque l'œdème devient trop important, il est nécessaire de procéder à une greffe. Les cornées destinées à la greffe sont triées dans des banques de tissus, et sont en particulier soumises à une évaluation qualitative de leur transparence. Cette thèse s'inscrit dans le cadre d'un projet visant à étudier les propriétés de diffusion de greffons cornéens humains, afin d'améliorer l'évaluation quantitative de leur transparence en banque des tissus ou de mieux paramétrer les lasers de découpe lors des greffes de cornées, dont les performances sont altérées à cause du phénomène de diffusion. Le comportement diffusant de la cornée est mesuré dans l'espace réfléchi, afin d'évaluer à terme la possibilité d'une caractérisation in vivo. Conjointement à la mesure de diffusion, une imagerie du volume de la cornée est réalisée grâce à un dispositif de tomographie de cohérence optique apportant une caractérisation de la structure microscopique du tissu. L'œdème et son développement sont ainsi caractérisés par l'analyse de la diffusion du tissu, de sa transparence et des hétérogénéités à l'échelle du micron. / Along with the crystalline lens, the cornea is the unique tissue being transparent in the human body. With a transmission coefficient over 90% in the visible spectrum, the main function of the cornea is to transmit the light inside the eye. This property is due to an absence of blood vessels and a very regular organization of the corneal bulk. In the case of an edema development, the cornea swells because of an abnormally high hydration. This involves a disorganization of its internal structure and an increase of the light scattering, leading to cornea haziness. When the edema is too critical, a graft is then required. In tissue banks, several criteria, such as the evaluation of the transparency, are considered in order to choose only the tissues eligible for corneal transplantation. This thesis aims to study the scattering properties of human corneal grafts in order to improve transparency evaluation in tissue banks or to lead to a better calibration of laser cuts during surgery procedure. A characterization of the scattering properties of the tissues is performed in the reflective half-space. Indeed, backscattering characterization could be used in in-situ conditions. Moreover, 3D images of the bulk of the cornea are performed using a Optical Coherence Tomography set-up. Edema developement is studied through the analysis of the scattering behaviour and of the microscopic structure of the graft. Scattering properties and microstructure are linked together through the use of an electromagnetic modelling. Maxwell's equations are solved using Born approximation, and a numerical method was adapted to perform those calculations in the case of the cornea.

La problématique de l'imagerie radar pose comme objectif de caractériser la cible observée. Dans le contexte de la télédétection appliquée aux milieux forestiers, il s'agit d'extraire les paramètres physiques constitutifs de la végétation.Ce manuscrit traite donc de la problématique de l'inversion de données électromagnétiques pour les basses fréquences radar, de la bande VHF à la bande P. Dans ces bandes de fréquences la canopée (feuilles et petites branches) n'interagit quasiment pas avec l'onde radar et la forêt peut donc, en première approximation, être représentée par des cylindres verticaux (troncs) et inclinés (branches primaires).Dans ce contexte, les méthodes d'inversion numériques s'appuient sur des modèles qui calculent, à de multiples reprises, les champs rayonnés par ce type de diffuseurs. Il faut alors choisir un modèle physique dont le compromis rapidité/précision penche en faveur de la rapidité, donc un modèle "approché". La précision du modèle choisi est ensuite étudié puis validé par comparaison à un modèle dont le compromis rapidité/précision est inversé, donc un modèle "exact". Parmi les nombreuses méthodes d'inversion, celle de l'algorithme génétique (AG) a été choisie. Cet algorithme bien connu est ici analysé puis amélioré pour répondre aux exigences du problème électromagnétique posé. Il est ensuite validé sur des données simulées et mesurées. Cette validation est aussi l'occasion d'étudier l'impact du jeu de données utilisé sur la rapidité et la précision de l'inversion, en fonction des configurations d'antenne (fréquences, positions, polarisations). / The objective of radar imaging is to characterize the observed target. In the case of forest remote sensing, the objective is to extract the component of the vegetation physical parameters.This manuscript addresses the problem of the inversion of electromagnetic data for low frequency wave, VHF band to the P band. In these frequency bands, the canopy (leaves and small branches) does not almost interact with the radar wave and the forest can thus, in first approximation, be represented by vertical cylinders (trunks) and tilted (primary branches).In this context, the numerical electromagnetic methods of inversion lean on models which calculate, many times, the scattered fields radiated by such broadcasters. It is then necessary to choose a physical model which compromise speed/accuracy tilts in favor of the speed, thus a "approached" model. The exactness of the chosen model is then studied and then validated by comparison to a model which the compromise speed/accuracy is inverted, thus a "exact" model. Among the many numerical methods of inversion, that of the genetic algorithm (AG) was chosen. This algorithm, well known, is analyzed here then improved to meet the requirements of the composed electromagnetic problem. It is then validated on simulated and measured data. This validation is also an opportunity to study the impact of the set of data used on the speed and the precision of the inversion, according to the configurations of antenna (frequencies, positions, polarizations).

In the past few years, intensive research efforts have been devoted to studying new approaches to controlling the photon emission of quantum emitters (QEs), especially for telecommunication applications. These approaches rely on tailoring the QE\'s radiation, usually assessed via well-known figures-of-merit such as lifetime (τ) and quantum efficiency (η). Controlling the QE\'s photon emission is important because the faster its photons are emitted, the greater is the number of times it returns to the excited state per second. Therefore, it is crucial to create additional decay channels to reduce τ, which necessarily requires increasing the Purcell factor (P). One of the most promising approaches to increase P involves a new class of metamaterials, known as hyperbolic metamaterials (HMM). This class of materials exhibits pronounced anisotropy, with the parallel and perpendicular permittivity tensor elements (with respect to the anisotropy axis) presenting opposite signs, resulting in an open hyperboloidal isofrequency surface (IS). This unusual IS shape leads to the most outstanding feature of HMMs, namely, the existence of photonic modes with wavenumber (k) much larger than those in free-space (k0), known as high-k modes. By engineering these modes, it is possible to manipulate the HMM photonic density of states (PDoS), thus controlling the QE\'s radiation parameters. The simplest approach to designing HMM is by means of a planar stack of alternating thin metal and dielectric layers. However, the finite thickness of these layers induces spatial dispersion, making the extraction of effective parameters (homogenization) of these media a challenging task. In this context, we propose in this thesis a new constitutive parameter retrieval approach that takes spatial dispersion into account for all electromagnetic parameters of the medium. We demonstrate that the real part of the dispersion curve flattens out (correspondingly with a large imaginary part) because of the absence of propagating modes inside the metamaterial. This flat region is strongly dependent on the layer thicknesses and is a direct manifestation of spatial dispersion. Moreover, we demonstrate that the QE\'s lifetime calculation is overestimated if this effect is not taken into account in the homogenization procedure, which is detrimental for telecommunication applications. Moreover, we demonstrate how to enhance P by a factor greater than 100 with the use of HMMs. However, most of the QE dissipated power couples into the HMM as high-k modes (which do not propagate in free-space). Therefore, the energy is thermally dissipated inside the HMM with a consequent reduction of η . Some authors have resorted to nano-patterned HMMs (NPHM) to convert the high-k modes into free-space modes (k≤k0) aiming at increasing η. However, much of the NPHMs designs still rely on computationally costly three dimensional (3D) numerical simulations. Thus, we also propose in this thesis a new semi-analytical method to model, both in two- and three-dimensions (2D and 3D, respectively), the radiation emission of QEs interacting with nano-patterned structures. The low computational cost of this method makes it attractive for mapping P and η as function of the QE and NPHM relative position. This mapping is a helpful tool to understand the decay behavior of the whole system since QEs are arbitrarily distributed and oriented inside the NPHM. The analytically calculated decay curve allows the systems effective quantum efficiency (ηeff) and Purcell factor (Peff) to be directly obtained assuming multiple arbitrarily distributed electromagnetic sources. In this sense, we propose here a new procedure to optimize the NPHM geometrical parameters to maximize ηeff while achieving the desired Peff. We apply the proposed model to an NPHM composed of nine Ag/SiO2 layers, with the polymer host layer embedded with Rhodamine 6G, to maximize ηeff for a specified tenfold increase of Peff. This procedure allowed ηeff to be increased by 69% and 170% for one- and two-dimensional nano-patterning, respectively. Moreover, the time required to build the P and η maps (used in the calculation of the decay behavior) is reduced by approximately 96% when compared to those numerically calculated via FDTD. This procedure paves the way to the realization of new high-speed and efficient light sources for telecommunication applications. / Nos últimos anos, intensivo esforço tem sido devotado para o estudo de novas método para o controla da missão de fótons de emissores quânticos (EQs), especialmente para aplicações em telecomunicações. Estes métodos dependem da adaptação da radiação dos EQs, geralmente avaliadas por meio das bem conhecidas figuras de mérito, como o tempo de meia vida (τ) e a eficiência quântica (η). O controle da emissão de fótons é importante pois quanto mais rápido os fótons são emitidos, maior é o número de vezes que o EQ retorna ao seu estado excitado por segundo. Portanto, é crucial criar canais de decaimento adicionais para reduzir τ, o que necessariamente requer o aumento do fator de Purcell (P). Uma das abordagens mais promissoras para aumentar P envolve uma nova classe de metamateriais, conhecida como metamateriais hiperbólicos (MHs). Esta classe de materiais apresenta pronunciada anisotropia, onde os elementos paralelo e perpendicular do tensor de permissividade (em relação ao eixo de anisotropia) apresentam sinais opostos, resultando em uma superfície de isofrequência (SI) hiperboloidal aberta (IS). Essa forma incomum de SI leva à característica mais marcante dos MHs, a existência de modos fotônicos com número de onda (k) muito maior do que aqueles no espaço livre (k0), conhecidos como modos alto-k. Ao manipular esses modos, é possível manipular a densidade de estados fotônicos (DES) dos MHs, controlando assim os parâmetros de radiação do QE. A abordagem mais simples para a criação de MHs é por meio de uma pilha plana de camadas metálicas e dielétricas alternadas. Entretanto, a espessura finita dessas camadas induz a dispersão espacial, tornando a extração de parâmetros efetivos (homogeneização) destes meios uma tarefa desafiadora. Neste contexto, propomos nesta tese uma nova abordagem de recuperação de parâmetros constitutivos a dispersão espacial de todos os parâmetros eletromagnéticos do meio é levada em consideração. Nós demonstramos que a parte real da curva de dispersão se aplaina (correspondentemente com uma grande parte imaginária) devido à ausência de modos propagantes dentro do metamaterial. Esta região plana é fortemente dependente das espessuras das camadas e é uma manifestação direta da dispersão espacial Além disso, nós mostramos que se a dispersão espacial não for corretamente considerada no processo de homogeneização, o tempo de meia vida do EQ pode ser superestimado, o que é prejudicial para aplicações de telecomunicações. Além disso, demonstramos como melhorar P por um fator maior que 100 com o uso de MHs. a maior parte da potência dissipada pelos EQs são acopladas nos MHs como modos de alto-k (que não se propagam no espaço livre). Portanto, a energia é dissipada termicamente no interior do MH, resultando em uma redução de η. Alguns autores recorreram a MHs nano-estruturados (MHNE) para converter os modos alto-k em modos de espaço livre (k≤k0) visando o aumento de η. No entanto, muitos dos projetos do NPHM ainda dependem de simulações numéricas tridimensionais (3D) computacionalmente dispendiosas. Assim, também propomos nesta tese um novo método semi-analítico para modelar, tanto em duas como em três dimensões (2D e 3D, respectivamente), a emissão de radiação de EQs interagindo com estruturas nano-estruturadas. O baixo custo computacional deste método faz com que seja atrativo para o mapeamento de P e η em função da posição relativa do EQ e do MHNE. Esse mapeamento é uma ferramenta útil para entender o comportamento de decaimento de todo o sistema, já que os EQs são arbitrariamente distribuídos e orientados dentro do MHNE. A curva de decaimento calculada analiticamente permite que a eficiência quântica efetiva do sistema (ηeff) e o fator de Purcell (Peff) sejam obtidos diretamente, assumindo múltiplas fontes eletromagnéticas arbitrariamente distribuídas. Neste sentido, propomos aqui um novo procedimento para otimizar os parâmetros geométricos do MHNE visando a maximização de ηeff enquanto Peff é aumentado à um valor desejado. Aplicamos o modelo proposto a um MHNE composto por nove camadas de Ag/SiO2, com a camada de polímero embutida com Rodamina 6G, visando maximizar ηeff para um aumento de dez vezes de Peff. Este procedimento permitiu que o ηeff fosse incrementado em 69% e 170% para nano-estruturas uni e bidimensionais, respectivamente. Além disso, o tempo necessário para construir os mapas P e η (utilizados no cálculo da curva de decaimento) é reduzido em aproximadamente 96% quando comparado com os calculados numericamente via FDTD. Este procedimento abre caminho para o desenvolvimento de novas fontes de luz de alta velocidade e eficiência para aplicações de telecomunicações.

In the past few years, intensive research efforts have been devoted to studying new approaches to controlling the photon emission of quantum emitters (QEs), especially for telecommunication applications. These approaches rely on tailoring the QE\'s radiation, usually assessed via well-known figures-of-merit such as lifetime (τ) and quantum efficiency (η). Controlling the QE\'s photon emission is important because the faster its photons are emitted, the greater is the number of times it returns to the excited state per second. Therefore, it is crucial to create additional decay channels to reduce τ, which necessarily requires increasing the Purcell factor (P). One of the most promising approaches to increase P involves a new class of metamaterials, known as hyperbolic metamaterials (HMM). This class of materials exhibits pronounced anisotropy, with the parallel and perpendicular permittivity tensor elements (with respect to the anisotropy axis) presenting opposite signs, resulting in an open hyperboloidal isofrequency surface (IS). This unusual IS shape leads to the most outstanding feature of HMMs, namely, the existence of photonic modes with wavenumber (k) much larger than those in free-space (k0), known as high-k modes. By engineering these modes, it is possible to manipulate the HMM photonic density of states (PDoS), thus controlling the QE\'s radiation parameters. The simplest approach to designing HMM is by means of a planar stack of alternating thin metal and dielectric layers. However, the finite thickness of these layers induces spatial dispersion, making the extraction of effective parameters (homogenization) of these media a challenging task. In this context, we propose in this thesis a new constitutive parameter retrieval approach that takes spatial dispersion into account for all electromagnetic parameters of the medium. We demonstrate that the real part of the dispersion curve flattens out (correspondingly with a large imaginary part) because of the absence of propagating modes inside the metamaterial. This flat region is strongly dependent on the layer thicknesses and is a direct manifestation of spatial dispersion. Moreover, we demonstrate that the QE\'s lifetime calculation is overestimated if this effect is not taken into account in the homogenization procedure, which is detrimental for telecommunication applications. Moreover, we demonstrate how to enhance P by a factor greater than 100 with the use of HMMs. However, most of the QE dissipated power couples into the HMM as high-k modes (which do not propagate in free-space). Therefore, the energy is thermally dissipated inside the HMM with a consequent reduction of η . Some authors have resorted to nano-patterned HMMs (NPHM) to convert the high-k modes into free-space modes (k≤k0) aiming at increasing η. However, much of the NPHMs designs still rely on computationally costly three dimensional (3D) numerical simulations. Thus, we also propose in this thesis a new semi-analytical method to model, both in two- and three-dimensions (2D and 3D, respectively), the radiation emission of QEs interacting with nano-patterned structures. The low computational cost of this method makes it attractive for mapping P and η as function of the QE and NPHM relative position. This mapping is a helpful tool to understand the decay behavior of the whole system since QEs are arbitrarily distributed and oriented inside the NPHM. The analytically calculated decay curve allows the systems effective quantum efficiency (ηeff) and Purcell factor (Peff) to be directly obtained assuming multiple arbitrarily distributed electromagnetic sources. In this sense, we propose here a new procedure to optimize the NPHM geometrical parameters to maximize ηeff while achieving the desired Peff. We apply the proposed model to an NPHM composed of nine Ag/SiO2 layers, with the polymer host layer embedded with Rhodamine 6G, to maximize ηeff for a specified tenfold increase of Peff. This procedure allowed ηeff to be increased by 69% and 170% for one- and two-dimensional nano-patterning, respectively. Moreover, the time required to build the P and η maps (used in the calculation of the decay behavior) is reduced by approximately 96% when compared to those numerically calculated via FDTD. This procedure paves the way to the realization of new high-speed and efficient light sources for telecommunication applications. / Nos últimos anos, intensivo esforço tem sido devotado para o estudo de novas método para o controla da missão de fótons de emissores quânticos (EQs), especialmente para aplicações em telecomunicações. Estes métodos dependem da adaptação da radiação dos EQs, geralmente avaliadas por meio das bem conhecidas figuras de mérito, como o tempo de meia vida (τ) e a eficiência quântica (η). O controle da emissão de fótons é importante pois quanto mais rápido os fótons são emitidos, maior é o número de vezes que o EQ retorna ao seu estado excitado por segundo. Portanto, é crucial criar canais de decaimento adicionais para reduzir τ, o que necessariamente requer o aumento do fator de Purcell (P). Uma das abordagens mais promissoras para aumentar P envolve uma nova classe de metamateriais, conhecida como metamateriais hiperbólicos (MHs). Esta classe de materiais apresenta pronunciada anisotropia, onde os elementos paralelo e perpendicular do tensor de permissividade (em relação ao eixo de anisotropia) apresentam sinais opostos, resultando em uma superfície de isofrequência (SI) hiperboloidal aberta (IS). Essa forma incomum de SI leva à característica mais marcante dos MHs, a existência de modos fotônicos com número de onda (k) muito maior do que aqueles no espaço livre (k0), conhecidos como modos alto-k. Ao manipular esses modos, é possível manipular a densidade de estados fotônicos (DES) dos MHs, controlando assim os parâmetros de radiação do QE. A abordagem mais simples para a criação de MHs é por meio de uma pilha plana de camadas metálicas e dielétricas alternadas. Entretanto, a espessura finita dessas camadas induz a dispersão espacial, tornando a extração de parâmetros efetivos (homogeneização) destes meios uma tarefa desafiadora. Neste contexto, propomos nesta tese uma nova abordagem de recuperação de parâmetros constitutivos a dispersão espacial de todos os parâmetros eletromagnéticos do meio é levada em consideração. Nós demonstramos que a parte real da curva de dispersão se aplaina (correspondentemente com uma grande parte imaginária) devido à ausência de modos propagantes dentro do metamaterial. Esta região plana é fortemente dependente das espessuras das camadas e é uma manifestação direta da dispersão espacial Além disso, nós mostramos que se a dispersão espacial não for corretamente considerada no processo de homogeneização, o tempo de meia vida do EQ pode ser superestimado, o que é prejudicial para aplicações de telecomunicações. Além disso, demonstramos como melhorar P por um fator maior que 100 com o uso de MHs. a maior parte da potência dissipada pelos EQs são acopladas nos MHs como modos de alto-k (que não se propagam no espaço livre). Portanto, a energia é dissipada termicamente no interior do MH, resultando em uma redução de η. Alguns autores recorreram a MHs nano-estruturados (MHNE) para converter os modos alto-k em modos de espaço livre (k≤k0) visando o aumento de η. No entanto, muitos dos projetos do NPHM ainda dependem de simulações numéricas tridimensionais (3D) computacionalmente dispendiosas. Assim, também propomos nesta tese um novo método semi-analítico para modelar, tanto em duas como em três dimensões (2D e 3D, respectivamente), a emissão de radiação de EQs interagindo com estruturas nano-estruturadas. O baixo custo computacional deste método faz com que seja atrativo para o mapeamento de P e η em função da posição relativa do EQ e do MHNE. Esse mapeamento é uma ferramenta útil para entender o comportamento de decaimento de todo o sistema, já que os EQs são arbitrariamente distribuídos e orientados dentro do MHNE. A curva de decaimento calculada analiticamente permite que a eficiência quântica efetiva do sistema (ηeff) e o fator de Purcell (Peff) sejam obtidos diretamente, assumindo múltiplas fontes eletromagnéticas arbitrariamente distribuídas. Neste sentido, propomos aqui um novo procedimento para otimizar os parâmetros geométricos do MHNE visando a maximização de ηeff enquanto Peff é aumentado à um valor desejado. Aplicamos o modelo proposto a um MHNE composto por nove camadas de Ag/SiO2, com a camada de polímero embutida com Rodamina 6G, visando maximizar ηeff para um aumento de dez vezes de Peff. Este procedimento permitiu que o ηeff fosse incrementado em 69% e 170% para nano-estruturas uni e bidimensionais, respectivamente. Além disso, o tempo necessário para construir os mapas P e η (utilizados no cálculo da curva de decaimento) é reduzido em aproximadamente 96% quando comparado com os calculados numericamente via FDTD. Este procedimento abre caminho para o desenvolvimento de novas fontes de luz de alta velocidade e eficiência para aplicações de telecomunicações.

L’objectif de cette thèse est d’explorer de nouvelles technologies permettant de faciliter l’intégration des isolateurs dans les chaînes radiofréquences de satellites. Ces composants sont utilisés pour contrôler l’adaptation des amplificateurs dans les sections d’entrée et de sortie des équipements RF bas niveaux. Nous proposons deux voies de réalisation de ces isolateurs. Une première voie basée sur l’utilisation de matériaux ferricomposites est étudiée pour concevoir des composants en bande Ku. Une deuxième voie, basée sur l’utilisation d’hexaferrites de strontium et de baryum préorientés, a été étudiée pour concevoir des composants auto-polarisés (sans aimants) en bandes Q et Ka. / The goal of this PhD thesis is to explore new technologies that make possible to improve the integration of isolators in radiofrequency chain of satellites. These components are especially used to control matching of amplifiers.We propose two ways of producing these isolators. At first, ferricomposite materials are studied to design low-cost isolators at Kuband.Then, we studied pre-oriented strontium or barium hexaferrites to design self-biased components (without magnets) for Q and Ka band frequencies.