X ray attenuation coefficients from 10 kev to 100 mev.

Mode of access: Internet.

Protection against Roentgen and gamma-rays. USSR.

Translation of p. 94-226 and p. 233-237 of Zashchita ot rentgenovykh i gamma lucheĭ.

The fundamentals of X-ray and radium physics.

Mode of access: Internet.

Röntgen rays;

Bibliography: p. 74.

Assembler's guide to diagnostic x-ray equipment under the Federal Performance Standard.

Mode of access: Internet.

The Roentgen rays, their production and use.

Plates printed on both sides.

Fundamentals of X-ray; physics and technique.

Loose-leaf; reproduced from type-written copy.

American National Standard N537 : radiological safety standard for the design of radiographic and fluoroscopic industrial x-ray equipment /

"ANSI N537-1976."

ESTUDO COMPARATIVO ENTRE A ANÁLISE FACIAL SUBJETIVA E ANÁLISE CEFALOMÉTRICA DE TECIDOS MOLES NO DIAGNÓSTICO ORTODÔNTICO

O propósito deste estudo foi avaliar a concordância entre a Análise facial subjetiva, proposta por CAPELOZZA FILHO e a Análise Cefalométrica de Tecidos Moles, de ARNETT; McLAUGHLIN. Fotografias de frente e de perfil e telerradiografias em norma lateral padronizadas, de 50 indivíduos, com média de idade de 24 anos e 1 mês foram utilizadas para a avaliação. Verificou-se também nos indivíduos classificados como Padrão I, a correspondência dos valores médios e dos desvios-padrão das medidas obtidas, com os valores normativos da Análise Cefalométrica dos Tecidos Moles para os indivíd uos com harmonia facial. Constatou-se em indivíduos do Padrão I que os lábios sempre se encontram à frente da Linha Vertical Verdadeira, e que apesar de grandes variações do ponto pogônio, ainda é mantido o equilíbrio facial. Os resultados demonstraram que a Análise facial subjetiva eficiente na classificação do padrão facial.

DETERMINAÇÃO DA POSIÇÃO DE REPOUSO DA LÍNGUA EM INDIVÍDUOS COM OCLUSÃO DENTÁRIA NORMAL

O propósito neste estudo foi determinar a posição de repouso da língua em indivíduos com oclusão dentária normal e respiração nasal, por meio de telerradiografias em norma lateral realizadas após a ingestão de bário. A amostra foi composta por 66 radiografias de indivíduos brancos com oclusão dentária normal, sendo 26 do sexo masculino e 40 do sexo feminino, na faixa etária de 12 a 21 anos de idade, procedentes de escolas da região do Grande ABC Paulista. O critério utilizado para diagnóstico da oclusão normal foi As Seis Chaves para a Oclusão Normal preconizadas por Andrews (1972), devendo estar presentes no mínimo quatro das seis chaves, sendo obrigatória a presença da primeira chave de oclusão que é a da relação interarcos. As radiografias foram obtidas com o indivíduo em posição natural da cabeça após a ingestão de contraste de sulfato de bário para evidenciar o controle da língua. Posteriormente foi feito o desenho anatômico das estruturas pesquisadas, marcados os pontos cefalométricos, traçadas as linhas e os planos, e por último obtidas as seguintes medidas lineares: comprimento e altura da língua, distância do dorso da língua na sua porção média até o palato duro e a distância entre a ponta da língua e a incisal do incisivo inferior. Por meio dos resultados encontrados verificou-se que não existe um padrão único de posicionamento de repouso da língua dentro da cavidade oral, em pacientes respiradores nasais, variando muito sua distância até a incisal dos incisivos inferiores, bem como até o palato duro, havendo uniformidade apenas no fato da língua tocar o palato mole em todos os indivíduos da amostra. Não houve relação estatisticamente significante entre a posição de repouso da língua e os biotipos faciais e nem dimorfismo sexual.

IRAS 00183-7111: ALMA and X-ray view of an ultra luminous infrared galaxy

The aim of this Thesis work is to study the multi-frequency properties of the Ultra Luminous Infrared Galaxy (ULIRG) IRAS 00183-7111 (I00183) at z = 0.327, connecting ALMA sub-mm/mm observations with those at high energies in order to place constraints on the properties of its central power source and verify whether the gas traced by the CO may be responsible for the obscuration observed in X-rays. I00183 was selected from the so-called Spoon diagnostic diagram (Spoon et al. 2007) for mid-infrared spectra of infrared galaxies based on the equivalent width of the 6.2 μm Polycyclic Aromatic Hydrocarbon (PAH) emission feature versus the 9.7 μm silicate strength. Such features are a powerful tool to investigate the contribution of star formation and AGN activity in this class of objects. I00183 was selected from the top-left region of the plot where the most obscured sources, characterized by a strong Si absorption feature, are located. To link the sub-mm/mm to the X-ray properties of I00183, ALMA archival Cycle 0 data in Band 3 (87 GHz) and Band 6 (270 GHz) have been calibrated and analyzed, using CASA software. ALMA Cycle 0 was the Early Science program for which data reprocessing is strongly suggested. The main work of this Thesis consisted in reprocessing raw data to provide an improvement with respect to the available archival products and results, which were obtained using standard procedures. The high-energy data consists of Chandra, XMM-Newton and NuSTAR observations which provide a broad coverage of the spectrum in the energy range 0.5 − 30 keV. Chandra and XMM archival data were used, with an exposure time of 22 and 22.2 ks, respectively; their reduction was carried out using CIAO and SAS software. The 100 ks NuSTAR are still private and the spectra were obtained by courtesy of the PI (K. Iwasawa). A detailed spectral analysis was done using XSPEC software; the spectral shape was reproduced starting from simple phenomenological models, and then more physical models were introduced to account for the complex mechanisms that involve this source. In Chapter 1, an overview of the scientific background is discussed, with a focus on the target, I00183, and the Spoon diagnostic diagram, from which it was originally selected. In Chapter 2, the basic principles of interferometry are briefly introduced, with a description of the calibration theory applied to interferometric observations. In Chapter 3, ALMA and its capabilities, both current and future, are shown, explaining also the complex structure of the ALMA archive. In Chapter 4, the calibration of ALMA data is presented and discussed, showing also the obtained imaging products. In Chapter 5, the analysis and discussion of the main results obtained from ALMA data is presented. In Chapter 6, the X-ray observations, data reduction and spectral analysis are reported, with a brief introduction to the basic principle of X-ray astronomy and the instruments from which the observations were carried out. Finally, the overall work is summarized, with particular emphasis on the main obtained results and the possible future perspectives.

Determinação do estado fundamental de compostos antiferromagnéticos da série Tb(1-x)Y(x)RhIn(5): aproximação teórico experimental

We present the results of electrical resistivity, magnetic susceptibility, specific heat and x-ray absorption spectroscopy measurements in Tb1−xYxRhIn5 (x = 0.00, 0.15, 0.4.0, 0.50 e 0.70) single crystals. Tb1−xYxRhIn5 is an antiferromagnetic AFM compound with ordering temperature TN ≈ 46 K, the higher TN within the RRhIn5 serie (R : rare earth). We evaluate the physical properties evolution and the supression of the AFM state considering doping and Crystalline Electric Field (CEF) effects on magnetic exchange interaction between Tb3+ magnetic ions. CEF acts like a perturbation potential, breaking the (2J + 1) multiplet s degeneracy. Also, we studied linear-polarization-dependent soft x-ray absorption at Tb M4 and M5 edges to validate X-ray Absorption Spectroscopy as a complementary technique in determining the rare earth CEF ground state. Samples were grown by the indium excess flux and the experimental data (magnetic susceptibility and specific heat) were adjusted with a mean field model that takes account magnetic exchange interaction between first neighbors and CEF effects. XAS experiments were carried on Total Electron Yield mode at Laborat´onio Nacional de Luz S´ıncrotron, Campinas. We measured X-ray absorption at Tb M4,5 edges with incident polarized X-ray beam parallel and perpendicular to c-axis (E || c e E ⊥ c). The mean field model simulates the mean behavior of the whole system and, due to many independent parameters, gives a non unique CEF scheme. XAS is site- and elemental- specific technique and gained the scientific community s attention as complementary technique in determining CEF ground state in rare earth based compounds. In this work we wil discuss the non conclusive results of XAS technique in TbRhIn5 compounds.

Preparation of Excitation Sources to Portable X-Ray Spectrometer by Recovering 241am from Radioactive Lightning Conductor

With the prohibition of the use of radioactive lightning conductor in Brazil, this material passed to be collected and stored as radioactive waste in the waste deposits of The Brazilian National Nuclear Energy Commission (CNEN). The majority of these lightning conductor used as radioactive source 241Am with activity varying of 1 the 5 mCi. In this work are presented preliminary studies by recovering of 241Am through the electroplating technique, in order to posterior use as sources to portable X-rays fluorescence spectrometer. The 241Am sources have been removed from lightning conductor and dissolved in acid solution. The solution presented an activity of 0,6 Ci L-1. Small amounts of this solution were added to some electrolytes and tested in order to evaluate optimum electrolyte for deposition of 241Am. It was studied as electrolytes: HNO3 (0,2 mol L-1), NH4Cl (5,0 mol L-1) and a mixture of KCN and K2CO3 (in the rate of 2,0 g of each per liter). Yields of up to 90% were obtained applied a current density of 50 mA cm-2.

Probabilistic Evaluation of Three-Dimensional Reconstructions from X-Ray Images Spanning a Limited Angle

An important part of computed tomography is the calculation of a three-dimensional reconstruction of an object from series of X-ray images. Unfortunately, some applications do not provide sufficient X-ray images. Then, the reconstructed objects no longer truly represent the original. Inside of the volumes, the accuracy seems to vary unpredictably. In this paper, we introduce a novel method to evaluate any reconstruction, voxel by voxel. The evaluation is based on a sophisticated probabilistic handling of the measured X-rays, as well as the inclusion of a priori knowledge about the materials that the object receiving the X-ray examination consists of. For each voxel, the proposed method outputs a numerical value that represents the probability of existence of a predefined material at the position of the voxel while doing X-ray. Such a probabilistic quality measure was lacking so far. In our experiment, false reconstructed areas get detected by their low probability. In exact reconstructed areas, a high probability predominates. Receiver Operating Characteristics not only confirm the reliability of our quality measure but also demonstrate that existing methods are less suitable for evaluating a reconstruction.