Uma contribuição ao estudo do transformador com nucleo de metal amorfo para aplicação em sistemas elétricos de potência de alta frequência

Pós-graduação em Engenharia Elétrica - FEIS

Obtenção e caracterização de filmes nanoestruturados de polianilina/látex de borracha natural

Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)

Desenvolvimento e seleção de sensores para avaliação de refrigerantes em língua eletrônica

Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)

Ablação de esmalte e dentina bovinos e humanos com laser de Ti:safira no regime de femtossegundos: análises morfológicas e fisico-químicas comparativas

Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)

Desenvolvimento de um conjunto de modelagem de alta resolução para os métodos eletromagnéticos indutivos

A Modelagem Eletromagnética Analógica tem sido uma poderosa ferramenta no estudo das respostas eletromagnéticas de uma grande variedade das técnicas de levantamentos e de modelos geológicos. Nas aplicações de métodos eletromagnéticos nas investigações de contaminação no subsolo, recentemente em grande demanda, são obtidas anomalias muito baixas (da ordem de 0,01% do campo primário). Com o objetivo de estudar em laboratório os problemas de levantamentos eletromagnéticos para alvos de baixo número de indução, um conjunto de modelagem em escala reduzida de alta sensibilidade, foi projetado e construído. Este conjunto opera na faixa de freqüência de 1 kHz até 1 MHz com excelente linearidade. O transdutor de transmissão gera suficiente densidade de fluxo magnético com corrente de até 3 App (pico a pico) circulando nele. O sistema de recepção, isto é, o conjunto de bobinas receptoras mais o pré-amplificador acoplado apresenta sensibilidade 3 V/A/m na freqüência de 10 kHz com inclinação de 20 dB/dec de freqüência. A alta sensibilidade do sistema de recepção combinada com a boa capacidade de geração do sistema transmissor, permite alcançar a resolução de 0,025% do campo primário. O conjunto dispõe ainda, de um sistema mecânico que permite posicionar o sistema de transdutores (transmissor e receptor) em posições arbitrárias com resolução de 1 mm e precisão de 0,05 mm. A precisão no deslocamento linear do sistema de sonda numa linha de 1715 mm de comprimento é alcançada por meio de um motor de passo controlado por um microcontrolador, que é rigidamente acoplado a um fuso que converte o movimento angular do motor em movimento linear. Com este conjunto, é possível simular uma grande variedade de técnicas de levantamentos eletromagnéticos no formato Slingram, isto é, dipolo-dipolo. Além da boa resolução mecânica e boa resolução de medida eletromagnética do conjunto, todo o processo de controle e aquisição de dados é operacionalizado por meio de um computador mestre.

Methods and results of a search for gravitational waves associated with gamma-ray bursts using the GEO 600, LIGO, and Virgo detectors

In this paper we report on a search for short-duration gravitational wave bursts in the frequency range 64 Hz-1792 Hz associated with gamma-ray bursts (GRBs), using data from GEO 600 and one of the LIGO or Virgo detectors. We introduce the method of a linear search grid to analyze GRB events with large sky localization uncertainties, for example the localizations provided by the Fermi Gamma-ray Burst Monitor (GBM). Coherent searches for gravitational waves (GWs) can be computationally intensive when the GRB sky position is not well localized, due to the corrections required for the difference in arrival time between detectors. Using a linear search grid we are able to reduce the computational cost of the analysis by a factor of O(10) for GBM events. Furthermore, we demonstrate that our analysis pipeline can improve upon the sky localization of GRBs detected by the GBM, if a high-frequency GW signal is observed in coincidence. We use the method of the linear grid in a search for GWs associated with 129 GRBs observed satellite-based gamma-ray experiments between 2006 and 2011. The GRBs in our sample had not been previously analyzed for GW counterparts. A fraction of our GRB events are analyzed using data from GEO 600 while the detector was using squeezed-light states to improve its sensitivity; this is the first search for GWs using data from a squeezed-light interferometric observatory. We find no evidence for GW signals, either with any individual GRB in this sample or with the population as a whole. For each GRB we place lower bounds on the distance to the progenitor, under an assumption of a fixed GW emission energy of 10(-2)M circle dot c(2), with a median exclusion distance of 0.8 Mpc for emission at 500 Hz and 0.3 Mpc at 1 kHz. The reduced computational cost associated with a linear search grid will enable rapid searches for GWs associated with Fermi GBM events once the advanced LIGO and Virgo detectors begin operation.

Implementation of an F-statistic all-sky search for continuous gravitational waves in Virgo VSR1 data

We present an implementation of the F-statistic to carry out the first search in data from the Virgo laser interferometric gravitational wave detector for periodic gravitational waves from a priori unknown, isolated rotating neutron stars. We searched a frequency f(0) range from 100 Hz to 1 kHz and the frequency dependent spindown f(1) range from -1.6(f(0)/100 Hz) x 10(-9) Hz s(-1) to zero. A large part of this frequency-spindown space was unexplored by any of the all-sky searches published so far. Our method consisted of a coherent search over two-day periods using the F-statistic, followed by a search for coincidences among the candidates from the two-day segments. We have introduced a number of novel techniques and algorithms that allow the use of the fast Fourier transform (FFT) algorithm in the coherent part of the search resulting in a fifty-fold speed-up in computation of the F-statistic with respect to the algorithm used in the other pipelines. No significant gravitational wave signal was found. The sensitivity of the search was estimated by injecting signals into the data. In the most sensitive parts of the detector band more than 90% of signals would have been detected with dimensionless gravitational-wave amplitude greater than 5 x 10(-24).

Surface morphology and structural modification induced by femtosecond pulses in hydrogenated amorphous silicon films

Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)

Audiological findings in patients treated with radio- and concomitant chemotherapy for head and neck tumors

Abstract Objective To evaluate the functionality of the auditory system in patients who underwent radiotherapy and chemotherapy treatment with cisplatin to treat head and neck tumors. Study Design Case series with planned data collection. Setting From May 2007 to May 2008 by the Department of Otorhinolaryngology and the Department of Oncology/Radiotherapy at Faculdade de Medicina de Marília. Subjects and Methods Audiological evaluation (Pure Tone Audiometry (air and bone conduction), Speech Audiometry, Tympanometry, Acoustic Reflex testing and Distortion Product Otoacoustic Emissions) was performed in 17 patients diagnosed with head and neck neoplasia and treated with chemotherapy, using cisplatin, and radiotherapy. Results 12 left ears (70.5%) and 11 right ears (64.7%) presented bilateral decreased hearing soon after the treatment for the frequency 1 kHz (mild auditory damage) and for the frequency 8 kHz (more significant auditory damage). Conclusion Patients with head and neck cancer submitted to the conventional radiotherapy treatment, combined with the chemotherapy with cisplatin, presented a high incidence of decreased hearing by the end of treatment. Strong evidence was observed linking auditory alteration to the amount of radiotherapy treatment.

Dielectric properties of cobalt ferrite nanoparticles in ultrathin nanocomposite films

Multilayered nanocomposite films (thickness 50-90 nm) of cobalt ferrite nanoparticles (np-CoFe2O4, 18 nm) were deposited on top of interdigitated microelectrodes by the layer-by-layer technique in order to study their dielectric properties. For that purpose, two different types of nanocomposite films were prepared by assembling np-CoFe2O4 either with poly(3,4-ethylenedioxy thiophene):poly(styrene sulfonic acid) or with polyaniline and sulfonated lignin. Despite the different film architectures, the morphology of both was dominated by densely-packed layers of nanoparticles surrounded by polyelectrolytes. The dominant effect of np-CoFe2O4 was also observed after impedance spectroscopy measurements, which revealed that dielectric behavior of the nanocomposites was largely influenced by the charge transport across nanoparticle-polyelectrolyte interfaces. For example, nanocomposites containing np-CoFe2O4 exhibited a single low-frequency relaxation process, with time constants exceeding 15 ms. At 1 kHz, the dielectric constant and the dissipation factor (tan ᵟ) of these nanocomposites were 15 and 0.15, respectively. These values are substantially inferior to those reported for pressed pellets made exclusively of similar nanoparticles. Impedance data were further fitted with equivalent circuit models from which individual contributions of particle's bulk and interfaces to the charge transport within the nanocomposites could be evaluated. The present study evidences that such nanocomposites display a dielectric behavior dissimilar from that exhibited by their individual counterparts much likely due to enlarged nanoparticle- polyelectrolyte interfaces.

Progettazione e sviluppo di un'unità di acquisizione ed elaborazione dati provenienti da giroscopi mems triassiali per lo studio della cinematica cardiaca

La rotazione dell’apice del cuore è una delle espressioni della complessa cinematica del miocardio e rappresenta un importante indice di funzionalità cardiaca. Disporre di un sensore impiantabile che permetta un monitoraggio continuo di tale parametro consentirebbe di individuare precocemente un deterioramento della performance cardiaca e di adattare tempestivamente la terapia. L’obiettivo del lavoro di tesi è la realizzazione di un sistema di acquisizione dati per segnali provenienti da un giroscopio MEMS triassiale da utilizzarsi per lo studio della cinematica cardiaca, in particolare della rotazione del cuore. Per leggere e decodificare i segnali digitali in uscita dal giroscopio MEMS triassiale utilizzato (CMR3100, VTI Technologies) è stata progettata e sviluppata un’unità di condizionamento composta da una board Arduino ADK, associata ad un adattatore di tensione PCA9306 e a 3 convertitori digitali/analogici MCP4921, che ha richiesto lo sviluppo di software per la gestione del protocollo di comunicazione e della decodifica del segnale digitale proveniente dal sensore. Per caratterizzare e validare il sistema realizzato sono state effettuate prove di laboratorio, che hanno permesso di individuare i parametri di lavoro ottimali del sensore. Una prima serie di prove ha dimostrato come l’unità di condizionamento realizzata consenta di acquisire i segnali con una velocità di processo elevata (1 kHz) che non comporta perdita di dati in uscita dal sensore. Successivamente, attraverso un banco prova di simulazione appositamente assemblato allo scopo di riprodurre rotazioni cicliche nel range dei valori fisio-patologici, è stato quantificato lo sfasamento temporale (St) tra il segnale rilevato dal CMR3100 e decodificato dall'unità di condizionamento e un segnale analogico in uscita da un giroscopio analogico, ottenendo un valore medio St=4 ms. Attraverso lo stesso banco di simulazione, è stata infine dimostrata una buona accuratezza (errore percentuale <10%) nella misura dell'angolo di rotazione derivato dal segnale di velocità angolare rilevato direttamente dal sensore CRM300.

Coupling of LMS with a fs-laser ablation ion source: elemental and isotope composition measurements

Mass spectrometric analysis of elemental and isotopic compositions of several NIST standards is performed by a miniature laser ablation/ionisation reflectron-type time-of-flight mass spectrometer (LMS) using a fs-laser ablation ion source (775 nm, 190 fs, 1 kHz). The results of the mass spectrometric studies indicate that in a defined range of laser irradiance (fluence) and for a certain number of accumulations of single laser shot spectra, the measurements of isotope abundances can be conducted with a measurement accuracy at the per mill level and at the per cent level for isotope concentrations higher and lower than 100 ppm, respectively. Also the elemental analysis can be performed with a good accuracy. The LMS instrument combined with a fs-laser ablation ion source exhibits similar detection efficiency for both metallic and non-metallic elements. Relative sensitivity coefficients were determined and found to be close to one, which is of considerable importance for the development of standard-less instruments. Negligible thermal effects, sample damage and excellent characteristics of the fs-laser beam are thought to be the main reason for substantial improvement of the instrumental performance compared to other laser ablation mass spectrometers.

Zeeman effect in atmospheric O₂ measured by ground-based microwave radiometry

In this work we study the Zeeman effect on stratospheric O₂ using ground-based microwave radiometer measurements. The interaction of the Earth magnetic field with the oxygen dipole leads to a splitting of O₂ energy states, which polarizes the emission spectra. A special campaign was carried out in order to measure this effect in the oxygen emission line centered at 53.07 GHz. Both a fixed and a rotating mirror were incorporated into the TEMPERA (TEMPERature RAdiometer) in order to be able to measure under different observational angles. This new configuration allowed us to change the angle between the observational path and the Earth magnetic field direction. Moreover, a high-resolution spectrometer (1 kHz) was used in order to measure for the first time the polarization state of the radiation due to the Zeeman effect in the main isotopologue of oxygen from ground-based microwave measurements. The measured spectra showed a clear polarized signature when the observational angles were changed, evidencing the Zeeman effect in the oxygen molecule. In addition, simulations carried out with the Atmospheric Radiative Transfer Simulator (ARTS) allowed us to verify the microwave measurements showing a very good agreement between model and measurements. The results suggest some interesting new aspects for research of the upper atmosphere.

Bone conduction responses of middle ear structures in Thiel embalmed heads

Thiel-embalmed human whole-head specimens offer a promising alternative model for bone conduction (BC) studies of middle ear structures. In this work we present the Thiel model’s linearity and stability over time as well as its possible use in the study of a fixed ossicle chain. Using laser Doppler vibrometry (LDV), the motion of the retroauricular skull, the promontory, the stapes footplate and the round window (RW) were measured. A bone-anchored hearing aid stimulated the ears with step sinus tones logarithmically spread between 0.1 and 10 kHz. Linearity of the model was verified using input levels in steps of 10 dBV. The stability of the Thiel model over time was examined with measurements repeated after hours and weeks. The influence of a cement-fixed stapes was assessed. The middle ear elements measured responded linearly in amplitude for the applied input levels (100, 32.6, and 10 mV). The variability of measurements for both short- (2 h) and long-term (4-16 weeks) repetitions in the same ear was lower than the interindividual difference. The fixation of the stapes induced a lowered RW displacement for frequencies near 750 Hz (-4 dB) and an increased displacement for frequencies above 1 kHz (max. +3.7 dB at 4 kHz). LDV assessment of BC-induced middle ear motion in Thiel heads can be performed with stable results. The vibratory RW response is affected by the fixation of the stapes, indicating a measurable effect of ossicle chain inertia on BC response in Thiel embalmed heads.

Petrophysical investigation on sediment core CRP-3 from the Ross Sea, Antarctica

A suite of petrophysical properties - velocity, resistivity, bulk density, porosity, and matrix density - was measured on 88 core plugs from the CRP-3 drillhole. Core-plug bulk densities were used to recalibrate both whole-core and downhole bulk density logs. Core-plug measurements of matrix density permit conversion of the whole-core and downhole bulk density logs to porosity. Both velocity and formation factor (a normalized measure of resistivity) are strongly correlated with porosity. The velocity/porosity pattern is similar to that for the lower part of CRP-2A and is consistent with the empirical relationship for sandstones. Core-plug and whole-core measurements of P-wave velocity at atmospheric pressure exhibit excellent agreement. Measurements of velocity as a function of pressure indicate a significantly higher velocity sensitivity to pressure than has been observed at CRP-1 and CRP-2A; rebound or presence of microcracks at CRP-3 may be responsible. The percentage difference between velocities at in situ pressures and atmospheric pressures increases downhole from 0% at the seafloor to 9% at the bottom. This pattern can be used to correct whole-core velocity data, measured at atmospheric pressure, to in situ velocities for depth-to-time conversion and associated comparison to the seismic profile across the drillsite