Learning-Based Fast Iterative Convergence of 3-D MoM via Eigen-AGMRES Method

Three-dimensional (3-D) full-wave electromagnetic simulation using method of moments (MoM) under the framework of fast solver algorithms like fast multipole method (FMM) is often bottlenecked by the speed of convergence of the Krylov-subspace-based iterative process. This is primarily because the electric field integral equation (EFIE) matrix, even with cutting-edge preconditioning techniques, often exhibits bad spectral properties arising from frequency or geometry-based ill-conditioning, which render iterative solvers slow to converge or stagnate occasionally. In this communication, a novel technique to expedite the convergence of MoMmatrix solution at a specific frequency is proposed, by extracting and applying Eigen-vectors from a previously solved neighboring frequency in an augmented generalized minimum residual (AGMRES) iterative framework. This technique can be applied in unison with any preconditioner. Numerical results demonstrate up to 40% speed-up in convergence using the proposed Eigen-AGMRES method.

On the Capacity and Performance of Generalized Spatial Modulation

Generalized spatial modulation (GSM) uses N antenna elements but fewer radio frequency (RF) chains (R) at the transmitter. In GSM, apart from conveying information bits through R modulation symbols, information bits are also conveyed through the indices of the R active transmit antennas. In this letter, we derive lower and upper bounds on the the capacity of a (N, M, R)-GSM MIMO system, where M is the number of receive antennas. Further, we propose a computationally efficient GSM encoding method and a message passing-based low-complexity detection algorithm suited for large-scale GSM-MIMO systems.

Rossby Vortex Simulation on a Paraboloidal Coordinate System Using the Lattice Boltzmann Method

In this paper, we apply our compressible lattice Boltzmann model to a rotating parabolic coordinate system to simulate Rossby vortices emerging in a layer of shallow water flowing zonally in a rotating paraboloidal vessel. By introducing a scaling factor, nonuniform curvilinear mesh can be mapped to a flat uniform mesh and then normal lattice Boltzmann method works. Since the mass per unit area on the two-dimensional (2D) surface varies with the thickness of the water layer, the 2D flow seems to be "compressible" and our compressible model is applied. Simulation solutions meet with the experimental observations qualitatively. Based on this research, quantitative solutions and many natural phenomena simulations in planetary atmospheres, oceans, and magnetized plasma, such as the famous Jovian Giant Red Spot, the Galactic Spiral-vortex, the Gulf Stream, and the Kuroshio Current, etc,, can be expected.

Explorations of electric-current system in solar active regions .1. Empirical inferences of the current flows

In this paper we explore techniques to identify sources of electric current systems and their channels of flow in solar active regions. Measured photospheric vector magnetic fields (VMF) together with high-resolution white-light and H filtergrams provide the data base to derive the current systems in the photosphere and chromosphere. Simple mathematical constructions of fields and currents are also adopted to understand these data. As an example, the techniques are then applied to infer current systems in AR 2372 in early April 1980. The main results are: (i) In unipolar sunspots the current density may reach values of 103 CGSE, and the Lorentz force on it can accelerate the Evershed flow, (ii) Spots exhibiting significant spiral pattrn in the penumbral filaments are the sources of vertical major currents at the photospheric surface, (iii) Magnetic neutral lines where the transverse field was strongly sheared were channels along which strong current system flows, (iv) The inferred current systems produced oppositely-flowing currents in the area of the delta configuration that was the site of flaring in AR 2372.

The permanence of density waves of galaxy and the numerical investigation of waser mechanism

This paper deals with in detail the permanence of the spiral structure of galaxies andthe characters of waser mechanism. A simplified model of galaxy is adopted. Variousdynamical characters of density waves are studied using numerical calculation method. Theresults verify very well the switch character f waser and the tunnel effect of density wavesat the potential barrier of corotation circle as is shown in a previous work of the author.

Influence of Training Set Selection in Artificial Neural Network-Based Propagation Path Loss Predictions

This paper analyzes the use of artificial neural networks (ANNs) for predicting the received power/path loss in both outdoor and indoor links. The approach followed has been a combined use of ANNs and ray-tracing, the latter allowing the identification and parameterization of the so-called dominant path. A complete description of the process for creating and training an ANN-based model is presented with special emphasis on the training process. More specifically, we will be discussing various techniques to arrive at valid predictions focusing on an optimum selection of the training set. A quantitative analysis based on results from two narrowband measurement campaigns, one outdoors and the other indoors, is also presented.

Empirical Doppler Characterization of Signals Scattered by Wind Turbines in the UHF Band under Near Field Condition

Time variability of the scattering signals from wind turbines may lead to degradation problems on the communication systems provided in the UHF band, especially under near field condition. In order to analyze the variability due to the rotation of the blades, this paper characterizes empirical Doppler spectra obtained from real samples of signals scattered by wind turbines with rotating blades under near field condition. A new Doppler spectrum model is proposed to fit the spectral characteristics of these signals, providing notable goodness of fit. Finally, the effect of this kind of time variability on the degradation of OFDM signals is studied.

New technologies driving decade-bandwidth radio astronomy : quad-ridged flared horn and compound-semiconductor LNAs

Among the branches of astronomy, radio astronomy is unique in that it spans the largest portion of the electromagnetic spectrum, e.g., from about 10 MHz to 300 GHz. On the other hand, due to scientific priorities as well as technological limitations, radio astronomy receivers have traditionally covered only about an octave bandwidth. This approach of "one specialized receiver for one primary science goal" is, however, not only becoming too expensive for next-generation radio telescopes comprising thousands of small antennas, but also is inadequate to answer some of the scientific questions of today which require simultaneous coverage of very large bandwidths.

This thesis presents significant improvements on the state of the art of two key receiver components in pursuit of decade-bandwidth radio astronomy: 1) reflector feed antennas; 2) low-noise amplifiers on compound-semiconductor technologies. The first part of this thesis introduces the quadruple-ridged flared horn, a flexible, dual linear-polarization reflector feed antenna that achieves 5:1-7:1 frequency bandwidths while maintaining near-constant beamwidth. The horn is unique in that it is the only wideband feed antenna suitable for radio astronomy that: 1) can be designed to have nominal 10 dB beamwidth between 30 and 150 degrees; 2) requires one single-ended 50 Ohm low-noise amplifier per polarization. Design, analysis, and measurements of several quad-ridged horns are presented to demonstrate its feasibility and flexibility.

The second part of the thesis focuses on modeling and measurements of discrete high-electron mobility transistors (HEMTs) and their applications in wideband, extremely low-noise amplifiers. The transistors and microwave monolithic integrated circuit low-noise amplifiers described herein have been fabricated on two state-of-the-art HEMT processes: 1) 35 nm indium phosphide; 2) 70 nm gallium arsenide. DC and microwave performance of transistors from both processes at room and cryogenic temperatures are included, as well as first-reported measurements of detailed noise characterization of the sub-micron HEMTs at both temperatures. Design and measurements of two low-noise amplifiers covering 1--20 and 8—50 GHz fabricated on both processes are also provided, which show that the 1--20 GHz amplifier improves the state of the art in cryogenic noise and bandwidth, while the 8--50 GHz amplifier achieves noise performance only slightly worse than the best published results but does so with nearly a decade bandwidth.

Parylene-C as a new piezoelectric material

The goal of this thesis is to develop a proper microelectromechanical systems (MEMS) process to manufacture piezoelectric Parylene-C (PA-C), which is famous for its chemical inertness, mechanical and thermal properties and electrical insulation. Furthermore, piezoelectric PA-C is used to build miniature, inexpensive, non-biased piezoelectric microphones.

These piezoelectric PA-C MEMS microphones are to be used in any application where a conventional piezoelectric and electret microphone can be used, such as in cell phones and hearing aids. However, they have the advantage of a simplified fabrication process compared with existing technology. In addition, as a piezoelectric polymer, PA-C has varieties of applications due to its low dielectric constant, low elastic stiffness, low density, high voltage sensitivity, high temperature stability and low acoustic and mechanical impedance. Furthermore, PA-C is an FDA approved biocompatible material and is able to maintain operate at a high temperature.

To accomplish piezoelectric PA-C, a MEMS-compatible poling technology has been developed. The PA-C film is poled by applying electrical field during heating. The piezoelectric coefficient, -3.75pC/N, is obtained without film stretching.

The millimeter-scale piezoelectric PA-C microphone is fabricated with an in-plane spiral arrangement of two electrodes. The dynamic range is from less than 30 dB to above 110 dB SPL (referenced 20 µPa) and the open-circuit sensitivities are from 0.001 – 0.11 mV/Pa over a frequency range of 1 - 10 kHz. The total harmonic distortion of the device is less than 20% at 110 dB SPL and 1 kHz.

Métodos de desacoplo de antenas PIFA en terminales móviles

[ES]Hoy en día, los sistemas de comunicación inalámbricos soportan un amplio número de servicios como la voz, datos y vídeos que requieren unas grandes tasas de transmisión. Por ello la mejora de la calidad del enlace que ofrecen los sistemas MIMO es clave. El problema surge al colocar varias antenas en un terminal móvil sin que aparezca un acoplamiento entre las distintas antenas que evite el correcto funcionamiento de estas. En este documento se realizará un estudio de los diferentes métodos de desacoplo entre antenas PIFA (Planar Inverted-F antenna) en un terminal móvil.

SIW teknologiadun antena simulazioa

[EU]Lan honetan, lehenik eta behin, SIW teknologiaren funtzionamendua ikasi dugu. Ondoren, eta gaur egun ezagunagoak diren antzeko mikrouhinetako teknologiei (microstrip, uhin gida edo antzerako transmisio lerroak) buruzko jakintza handitu ostean, hauen eta SIW teknologiaren arteko baliokidetasuna nola lortu ikasi dugu. HFSS simulazio-tresnarekin SIW teknologiadun antena ezberdinak diseinatu eta simulatu ditugu (propietate nahiz tamaina ezberdinekoak) eta hauen emaitzak aztertu, besteak beste bere erradiazio diagrama eta S parametroak. Azkenik emaitza hauek interpretatu, eta ondorio bat lortu dugu. SIW teknologiak besteekiko dituen abantailaz gain, diseinu hauek aurrera eramateko bete ditugun pausuak eta simulazio emaitzetatik lortutako interpretazioak ondorengo memoria honetan azalduko ditugu, baita lan honek izan dituen fase ezberdinak eta lan hau aurrera ateratzearen aurrekontua ere.

A Multiwavelength Study of the Intracluster Medium and the Characterization of the Multiwavelength Sub/millimeter Inductance Camera

The first part of this thesis combines Bolocam observations of the thermal Sunyaev-Zel’dovich (SZ) effect at 140 GHz with X-ray observations from Chandra, strong lensing data from the Hubble Space Telescope (HST), and weak lensing data from HST and Subaru to constrain parametric models for the distribution of dark and baryonic matter in a sample of six massive, dynamically relaxed galaxy clusters. For five of the six clusters, the full multiwavelength dataset is well described by a relatively simple model that assumes spherical symmetry, hydrostatic equilibrium, and entirely thermal pressure support. The multiwavelength analysis yields considerably better constraints on the total mass and concentration compared to analysis of any one dataset individually. The subsample of five galaxy clusters is used to place an upper limit on the fraction of pressure support in the intracluster medium (ICM) due to nonthermal processes, such as turbulent and bulk flow of the gas. We constrain the nonthermal pressure fraction at r500c to be less than 0.11 at 95% confidence, where r500c refers to radius at which the average enclosed density is 500 times the critical density of the Universe. This is in tension with state-of-the-art hydrodynamical simulations, which predict a nonthermal pressure fraction of approximately 0.25 at r500c for the clusters in this sample.

The second part of this thesis focuses on the characterization of the Multiwavelength Sub/millimeter Inductance Camera (MUSIC), a photometric imaging camera that was commissioned at the Caltech Submillimeter Observatory (CSO) in 2012. MUSIC is designed to have a 14 arcminute, diffraction-limited field of view populated with 576 spatial pixels that are simultaneously sensitive to four bands at 150, 220, 290, and 350 GHz. It is well-suited for studies of dusty star forming galaxies, galaxy clusters via the SZ Effect, and galactic star formation. MUSIC employs a number of novel detector technologies: broadband phased-arrays of slot dipole antennas for beam formation, on-chip lumped element filters for band definition, and Microwave Kinetic Inductance Detectors (MKIDs) for transduction of incoming light to electric signal. MKIDs are superconducting micro-resonators coupled to a feedline. Incoming light breaks apart Cooper pairs in the superconductor, causing a change in the quality factor and frequency of the resonator. This is read out as amplitude and phase modulation of a microwave probe signal centered on the resonant frequency. By tuning each resonator to a slightly different frequency and sending out a superposition of probe signals, hundreds of detectors can be read out on a single feedline. This natural capability for large scale, frequency domain multiplexing combined with relatively simple fabrication makes MKIDs a promising low temperature detector for future kilopixel sub/millimeter instruments. There is also considerable interest in using MKIDs for optical through near-infrared spectrophotometry due to their fast microsecond response time and modest energy resolution. In order to optimize the MKID design to obtain suitable performance for any particular application, it is critical to have a well-understood physical model for the detectors and the sources of noise to which they are susceptible. MUSIC has collected many hours of on-sky data with over 1000 MKIDs. This work studies the performance of the detectors in the context of one such physical model. Chapter 2 describes the theoretical model for the responsivity and noise of MKIDs. Chapter 3 outlines the set of measurements used to calibrate this model for the MUSIC detectors. Chapter 4 presents the resulting estimates of the spectral response, optical efficiency, and on-sky loading. The measured detector response to Uranus is compared to the calibrated model prediction in order to determine how well the model describes the propagation of signal through the full instrument. Chapter 5 examines the noise present in the detector timestreams during recent science observations. Noise due to fluctuations in atmospheric emission dominate at long timescales (less than 0.5 Hz). Fluctuations in the amplitude and phase of the microwave probe signal due to the readout electronics contribute significant 1/f and drift-type noise at shorter timescales. The atmospheric noise is removed by creating a template for the fluctuations in atmospheric emission from weighted averages of the detector timestreams. The electronics noise is removed by using probe signals centered off-resonance to construct templates for the amplitude and phase fluctuations. The algorithms that perform the atmospheric and electronic noise removal are described. After removal, we find good agreement between the observed residual noise and our expectation for intrinsic detector noise over a significant fraction of the signal bandwidth.

Desarrollo de técnicas de fresado en cinco ejes de engranajes espiro cónicos y posterior metrología.

[ES]El presente Trabajo Fin de Grado tiene como objetivo contribuir al desarrollo de diferentes técnicas de fresado de engranajes espiro cónicos mediante fresadoras genéricas de cinco ejes. El proyecto estará dividido en varias partes que incluirán: el diseño de la geometría de las piezas a mecanizar, el propio proceso de manufactura y su posterior metrología. Durante el transcurso del curso 2014-2015 se documentará y participará activamente en el desarrollo de dichas técnicas de fresado. Proceso que será dirigido por Álvaro Álvarez, doctorando del departamento de Mecánica de la Escuela Superior de Ingeniería de Bilbao. El objetivo principal es llegar a ser capaz de obtener piezas de gran complejidad en su diseño y proceso de fabricación, dentro de los márgenes de calidad exigidos por las normas pertinentes y mediante un proceso novedoso y competitivo a nivel internacional.

A influência da espessura óssea na medição da altura da borda alveolar em imagens de tomografia computadorizada de feixe cônico e espiral

Imagens de tomografia computadorizada (TC) permitem a visualização, sem distorções ou sobreposições, do complexo maxilo-facial, principalmente do osso alveolar. Estudos demonstraram boa reprodutibilidade e precisão da mensuração da altura da borda alveolar, todavia a influência da espessura óssea ainda é pouco descrita. Através da comparação com a mensuração direta, o objetivo deste estudo foi avaliar a precisão, reprodutibilidade e a influência da espessura óssea, na mensuração da altura da borda alveolar em imagens volumétricas e imagens bidimensionais multiplanares em TC de feixe cônico (TCFC) e em TC espiral (TCE). Utilizando 10 mandíbulas secas de humanos, 57 dentes anteriores foram tomografados em equipamentos iCAT (Imaging Science International, Hatfield, PA, EUA) e Brilliance 64 canais (Philips Eletronics, Eindhoven, Holanda), ambos utilizando voxels de 0,25 mm. Através de imagens volumétricas (3D) e imagens bidimensionais (2D) de cortes multiplanares, foi comparada a mensuração da altura da borda alveolar dessas imagens com a mensuração direta nas mandíbulas, feita por vestibular e lingual, por três avaliadores, com o auxílio de um paquímetro, totalizando 114 bordas alveolares medidas. Alta reprodutibilidade intra-avaliador (0,999 a 0,902) e interavaliador (0,998 e 0,868) foi observada através do índice de correlação intraclasse (ICC). Observou-se alta correlação entre a mensuração direta e indireta da altura da borda alveolar em imagens 2D, sendo r=0,923** e 0,916**, e em imagens 3D, com r=0,929** e 0,954*, em TCFC e TCE, respectivamente. Imagens 2D superestimam a altura da borda alveolar em 0,32 e 0,49 mm e imagens 3D em 0,34 e 0,30 mm, em TCFC e TCE respectivamente. Quando o osso alveolar apresenta espessura de no mínimo 0,6 mm a média da diferença entre medidas diretas e indiretas é de 0,16 e 0,28 mm em imagens 2D e de 0,12 e 0,03 mm em imagens 3D para TCFC e TCE respectivamente, sendo que 95% do limite de concordância varia de -0,46 a 0,79 mm e -0,32 a 0,88 mm em imagens 2D, e de -0,64 a 0,67 mm e -0,57 a 0,62 mm em imagens 3D, para TCFC e TCE respectivamente. Quando o osso alveolar é mais fino do que 0,6 mm a TC é imprecisa, pois 95% do limite de concordância variou de -1,74 a 5,42 mm e -1,64 a 5,42 mm em imagens 2D, e de -3,70 a 4,28 mm e -3,49 a 4,25 mm em imagens 3D, para TCFC e TCE respectivamente. Conclui-se que a mensuração da altura da borda alveolar através de imagens tomográficas apresenta alta reprodutibilidade, sendo que quando a borda alveolar apresenta pelo menos 0,6 mm, a precisão da mensuração é alta, todavia quando esta espessura é menor do que 0,6 mm a técnica é imprecisa.

A fábrica de peles: Hundertwasser e o caminhar contemporâneo

Por convergência teórica, esta tese de dissertação é estruturada em quatro capítulos, retomando a teoria das cinco peles de Hundertwaser. O artista austríaco, filho de mãe judia e pai ariano, realizou em Paris sua primeira exposição no ano de 1954 e desde então, não cessou mais de trabalhar, aglutinando os exercícios de arquiteto, ambientalista, naturista e higienista moral, assim como as atividades de pintor e gravador, todos efetivados nos múltiplos diálogos estabelecidos por cada pele. As cinco peles de Hundertwasser acredita o homem como um ser de camadas, que se desenrolam por uma espiral concêntrica, que parte do eu-profundo para o mundo exterior, operada por osmose, nas cadeias sucessivas dos níveis de consciência do indivíduo. as cinco peles de Hundertwasser são um plano de vida - e mais: uma reflexão profunda do ser e estar sobre a terra, colocado em prática ao longo de sua jornada artística. A abordagem pretende desdobrar tal teoria - o que cada pele me suscita - no corpo fabril da minha produção em relação a de outros artistas e teóricos. A transmissão das cinco peles de Hunderwasser desenvolve-se em situações de alargamento das peles. Uma apropriação que re contextualiza, revela novos posicionamentos no caminhar da arte contemporânea