Corona effect in frequency dependent transmission line models

The inclusion of the corona effect in a frequency dependent transmission line model is proposed in this paper. The transmission line is represented through a cascade of π circuits and the frequency dependence of the longitudinal parameters is synthesized with series and parallel resistors and inductors. The corona effect will be represented using the Gary and Skilling-Umoto models. The currents and voltages along the line are calculated by using state-space technique. To demonstrate the accuracy and validity of the proposed frequency dependent line model, time domain simulations of a 10 km length single-phase line response under energization procedure will be presented. ©2008 IEEE.

A distributed-parameters transmission line model developed directly in the phase domain

This article shows a transmission line model developed directly in the phase domain. The proposed model is based on the relationships between the phase currents and voltages at both the sending and receiving ends of a single-phase line. These relationships, established using an ABCD matrix, were extended to multi-phase lines. The proposed model was validated by using it to represent a transmission line during short-and open-circuit tests. The results obtained with the proposed model were compared with results obtained with a classical model based on modal decomposition. These comparisons show that proposed model was correctly developed. © 2013 Taylor and Francis Group, LLC.

Modelamento da permissividade dielétrica de rochas saturadas de óleo e água e suas aplicações em perfilagem de poço

A ferramenta de propagação eletromagnética (EPT) fornece o tempo de propagação (T_pl) e a atenuação (A) de uma onda eletromagnética que se propaga num meio com perdas. Estas respostas da EPT são funções da permissividade dielétrica do meio. Existem vários modelos e fórmulas de misturas sobre a permissividade dielétrica de rochas reservatório que podem ser utilizados na interpretação da ferramenta de alta frequência. No entanto, as fórmulas de mistura não consideram a distribuição e a geometria do espaço poroso, e estes parâmetros são essenciais para que sejam obtidas respostas dielétricas mais próximas de uma rocha real. Foi selecionado um modelo baseado nos parâmetros descritos acima e este foi aplicado à dados dielétricos disponíveis na literatura. Foi obtida uma boa concordância entre as curvas teóricas e os dados experimentais, comprovando assim que a distribuição e a geometria dos poros têm que ser levadas em conta no desenvolvimento de um modelo realista. Foram conseguidas também funções de distribuição de razão de aspecto de poros, através das quais geramos várias curvas relacionando as respostas da EPT com diversas saturações de óleo/gás. Estas curvas foram aplicadas na análise de perfis. Como o modelo selecionado ajusta-se bem aos dados dielétricos disponíveis na literatura, torna-se atraente aplicá-lo à dados experimentais obtidos em rochas de campos brasileiros produtores de hidrocarbonetos para interpretação da EPT corrida em poços destes campos petrolíferos.

Bulk plasmon polariton-gap soliton-induced transparency in one-dimensional Kerr-metamaterial superlattices

Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)

Differential cross sections for elastic and inelastic positronium-hydrogen-atom scattering

A time reversal symmetric regularized electron exchange model was used to elastic scattering, target elastic Ps excitations and target inelastic excitation of hydrogen in a five state coupled model. A singlet Ps-H-S-wave resonance at 4.01 eV of width 0.15 eV and a P-wave resonance at 5.08 eV of width 0.004 eV were obtained using this model. The effect on the convergence of the coupled-channel scheme due to the inclusion of the excited Ps and H states was also analyzed.

Comparative study on the far-field spectra and near-field amplitudes for silver and gold nanocubes irradiated at 514, 633 and 785 nm as a function of the edge length

We describe a systematic investigation by the discrete dipole approximation on the optical properties of silver (Ag) and gold (Au) nanocubes as a function of the edge length in the 20-100 nm range. Our results showed that, as the nanocube size increased, the plasmon resonance modes shifted to higher wavelengths, the contribution from scattering to the extinction increased, and the quadrupole modes became more intense in the spectra. The electric field amplitudes at the surface of the nanocubes were calculated considering 514, 633 and 785 nm as the excitation wavelengths. While Ag nanocubes displayed the highest electric field amplitudes (vertical bar E vertical bar(max)) when excited at 514 nm, the Au nanocubes displayed higher vertical bar E vertical bar(max) values than Ag, for all sizes investigated, when the excitation wavelength was either 633 or 785 nm. The variations in vertical bar E vertical bar(max) as a function of size for both Ag and Au nanocubes could be explained based on the relative position of the surface plasmon resonance peak relative to the wavelength of the incoming electromagnetic wave. Our results show that not only size and composition, but also the excitation wavelength, can play an important role over the maximum near-field amplitudes values generated at the surface of the nanocubes.

Troposphere Calibration Techniques for Deep Space Probe Tracking

Ground-based Earth troposphere calibration systems play an important role in planetary exploration, especially to carry out radio science experiments aimed at the estimation of planetary gravity fields. In these experiments, the main observable is the spacecraft (S/C) range rate, measured from the Doppler shift of an electromagnetic wave transmitted from ground, received by the spacecraft and coherently retransmitted back to ground. If the solar corona and interplanetary plasma noise is already removed from Doppler data, the Earth troposphere remains one of the main error sources in tracking observables. Current Earth media calibration systems at NASA’s Deep Space Network (DSN) stations are based upon a combination of weather data and multidirectional, dual frequency GPS measurements acquired at each station complex. In order to support Cassini’s cruise radio science experiments, a new generation of media calibration systems were developed, driven by the need to achieve the goal of an end-to-end Allan deviation of the radio link in the order of 3×〖10〗^(-15) at 1000 s integration time. The future ESA’s Bepi Colombo mission to Mercury carries scientific instrumentation for radio science experiments (a Ka-band transponder and a three-axis accelerometer) which, in combination with the S/C telecommunication system (a X/X/Ka transponder) will provide the most advanced tracking system ever flown on an interplanetary probe. Current error budget for MORE (Mercury Orbiter Radioscience Experiment) allows the residual uncalibrated troposphere to contribute with a value of 8×〖10〗^(-15) to the two-way Allan deviation at 1000 s integration time. The current standard ESA/ESTRACK calibration system is based on a combination of surface meteorological measurements and mathematical algorithms, capable to reconstruct the Earth troposphere path delay, leaving an uncalibrated component of about 1-2% of the total delay. In order to satisfy the stringent MORE requirements, the short time-scale variations of the Earth troposphere water vapor content must be calibrated at ESA deep space antennas (DSA) with more precise and stable instruments (microwave radiometers). In parallel to this high performance instruments, ESA ground stations should be upgraded to media calibration systems at least capable to calibrate both troposphere path delay components (dry and wet) at sub-centimetre level, in order to reduce S/C navigation uncertainties. The natural choice is to provide a continuous troposphere calibration by processing GNSS data acquired at each complex by dual frequency receivers already installed for station location purposes. The work presented here outlines the troposphere calibration technique to support both Deep Space probe navigation and radio science experiments. After an introduction to deep space tracking techniques, observables and error sources, in Chapter 2 the troposphere path delay is widely investigated, reporting the estimation techniques and the state of the art of the ESA and NASA troposphere calibrations. Chapter 3 deals with an analysis of the status and the performances of the NASA Advanced Media Calibration (AMC) system referred to the Cassini data analysis. Chapter 4 describes the current release of a developed GNSS software (S/W) to estimate the troposphere calibration to be used for ESA S/C navigation purposes. During the development phase of the S/W a test campaign has been undertaken in order to evaluate the S/W performances. A description of the campaign and the main results are reported in Chapter 5. Chapter 6 presents a preliminary analysis of microwave radiometers to be used to support radio science experiments. The analysis has been carried out considering radiometric measurements of the ESA/ESTEC instruments installed in Cabauw (NL) and compared with the requirements of MORE. Finally, Chapter 7 summarizes the results obtained and defines some key technical aspects to be evaluated and taken into account for the development phase of future instrumentation.

Numerical study of Anderson localization of terahertz waves in disordered waveguides

We present a numerical study of electromagnetic wave transport in disordered quasi-one-dimensional waveguides at terahertz frequencies. Finite element method calculations of terahertz wave propagation within LiNbO3 waveguides with randomly arranged air-filled circular scatterers exhibit an onset of Anderson localization at experimentally accessible length scales. Results for the average transmission as a function of waveguide length and scatterer density demonstrate a clear crossover from diffusive to localized transport regime. In addition, we find that transmission fluctuations grow dramatically when crossing into the localized regime. Our numerical results are in good quantitative agreement with theory over a wide range of experimentally accessible parameters both in the diffusive and localized regime opening the path towards experimental observation of terahertz wave localization.

Influence of Atmospheric Conditions on mmWave CATR Facilities: Formulation and Compensation Scheme

The performance of a CATR relies on the planarity of the synthesized test wave, which is generated within a bounded volume for which specifications are drawn. Millimetre-wave facilities deal with the classical limitations of this frequency band, among which two become critical in our analysis: time-extensive acquisition campaigns and impact of environmental variables. Both features become more evident when increasing the frequency of operation. The variation in atmospheric variables, such as humidity, temperature and pressure has an influence over the performance of all the elements of the facility. The instrumentation behavior is influenced both by the warming up process, and the ambience conditions that surround the equipment. On the changes of the atmosphere itself, they affect the electromagnetic wave propagation, given the physical link between the conditions of the atmosphere and its electric properties as an electromagnetic waves propagation medium

Ion-Ion correlations effect on nonlinear high-frequency plasma conductivity. AT(30-1)-1238-MATT-675

On the basis of the BBGKY hierarchy of equations an expression is derived for the response of a fully ionized plasma to a strong, high-frequency electric field in the limit of infinite ion mass. It is found that even in this limit the ionion correlation function is substantially affected by the field. The corrections to earlier nonlinear results for the current density appear to be quite ssential. The validity of the model introduced by Dawson and Oberman to study the response to a vanishingly small field is confirmed for larger values of the field when the eorrect expression for the ion-ion correlations i s introduced; the model by itself does not yield such an expression. The results have interest for the heating of the plasma and for the propagation of a strong electromagnetic wave through the plasma. The theory seems to be valid for any field intensity for which the plasma is stable.

Estudio de modelos de propagación en bandas milimétricas para su futura utilización en redes de comunicaciones móviles 5G

La generalización del uso de dispositivos móviles, con su consiguiente aumento del tráfico de datos, está generando una demanda cada vez mayor de bandas de frecuencia para el despliegue de sistemas de comunicación inalámbrica, así como una creciente congestión en las bandas bajas del espectro (hasta 3 GHz). Entre las posibles soluciones a este problema, se ha propuesto que la próxima generación de sistemas celulares, 5G, hagan uso de la banda milimétrica, entre 30 GHz y 300 GHz, donde hay anchos de banda contiguos disponibles con tamaños muy difíciles de encontrar en las frecuencias en uso en la generación actual. Este Proyecto de Fin de Grado tiene como finalidad estudiar la viabilidad del despliegue de sistemas celulares en dicha banda, basándose en los estudios tanto empíricos como teóricos ya publicados, así como en las recomendaciones de la UIT donde se estudian las características de propagación en estas bandas. En un siguiente apartado, se han analizado los documentos disponibles de los distintos proyectos y grupos, como pueden ser METIS-2020, impulsado por la Comisión Europea o IMT-2020 promovido por la UIT, dedicados a definir los futuros estándares de comunicación y sus características, así como la evolución de los actuales. Aparte del trabajo de documentación, se han realizado una serie de simulaciones. En primer lugar, se ha utilizado MATLAB para estudiar el comportamiento y la atenuación de la onda electromagnética a las frecuencias de interés en diferentes ubicaciones y climas, tanto en ubicaciones habituales como extremas, estudiándose los efectos de los gases atmosféricos y los hidrometeoros. También se ha utilizado software de planificación radioeléctrica profesional para hacer estudios de cobertura en entornos tanto urbanos, entre ellos Madrid o Barcelona, suburbanos, como Tres Cantos (Madrid) y O Barco de Valdeorras (Orense), y rurales como Valdefuentes (Cáceres) y Quiruelas de Vidriales (Zamora). Por último se han recogido todos los resultados, tanto los provenientes de los estudios como los obtenidos de nuestras propias simulaciones, y se ha realizado un breve comentario, comparando estos y analizando su impacto para posibles despliegues futuros de redes 5G. ABSTRACT. The generalization of mobile device use, with its associated data traffic growth, is generating a growing demand of spectrum for its use in the deployment of wireless telecommunication systems, and a growing congestion in the lower end of the spectrum (until 3 GHz). Among the possible solutions for this problem, it has been proposed that the next generation of cellular systems, 5G, makes use of the millimeter band, between 30 GHz and 300 GHz, where there are contiguous bandwidths with sizes hardly available in the bands used in the present. This Project aims to study the feasibility of cellular system deployments in said band, based on published empirical and theoretical studies and papers, and the ITU recommendations, where the propagation characteristics in those bands are studied. In the next section, available documentation coming from the different study groups and projects like METIS 2020 promoted by the European Commission, or IMT-2020, promoted by the ITU has been studied. In the documentation, future telecommunication standards and its characteristics and the evolution of the current ones are defined. Besides the documentation work, a series of simulations have been carried out. First, MATLAB has been used to study the behavior and attenuation of the electromagnetic wave at the frequencies of interest in different locations and climates, studying the effects of atmospheric gasses and hydrometeors in conventional and extreme locations. Industry standard radioelectric planning software has been used to study the coverage in different environments, such as urban locations like Madrid and Barcelona, both in Spain, suburban locations like Tres Cantos (Madrid, Spain) and O Barco de Valdeorras (Orense, Spain) and rural locations such as Valdefuentes (Cáreces, Spain) and Quiruelas de Vidriales (Zamora, Spain). Finally, all the results, both from the documentation and our own simulations, have been collected, and a brief commentary has been made, comparing those results and their possible impact in the future deployment of 5G networks.

A distributed equivalent magnetic current based FDTD method for the calculation of E-fields induced by gradient coils

This paper evaluates a new, low-frequency finite-difference time-domain method applied to the problem of induced E-fields/eddy currents in the human body resulting from the pulsed magnetic field gradients in MRI. In this algorithm, a distributed equivalent magnetic current is proposed as the electromagnetic source and is obtained by quasistatic calculation of the empty coil's vector potential or measurements therein. This technique circumvents the discretization of complicated gradient coil geometries into a mesh of Yee cells, and thereby enables any type of gradient coil modelling or other complex low frequency sources. The proposed method has been verified against an example with an analytical solution. Results are presented showing the spatial distribution of gradient-induced electric fields in a multi-layered spherical phantom model and a complete body model. (C) 2004 Elsevier Inc. All rights reserved.

Design of complementary UWB printed monopole antennas using simple formulas

Simple design formulas for designing ultra wideband (UWB) antennas in the form of complementary planar monopoles are described and their validity is tested using full electromagnetic wave simulations and measurements. Assuming dielectric substrate with relative permittivity of 10.2, the designed antennas feature a small size of 13 mmtimes26 mm. They exhibit a 10 dB return loss bandwidth from 3 to more than 15 GHz accompanied by near omnidirectional characteristics and good radiation efficiency throughout this band

Decelerating Airy pulses

It is shown that an electromagnetic wave equation in time domain is reduced in paraxial approximation to an equation similar to the Schrodinger equation but in which the time and space variables play opposite roles. This equation has solutions in form of time-varying pulses with the Airy function as an envelope. The pulses are generated by a source point with an Airy time varying field and propagate in vacuum preserving their shape and magnitude. The motion is according to a quadratic law with the velocity changing from infinity at the source point to zero in infinity. These one-dimensional results are extended to the 3D+time case when a similar Airy-Bessel pulse is excited by the field at a plane aperture. The same behaviour of the pulses, the non-diffractive preservation and their deceleration, is found. © 2011 IEEE.