983 resultados para Planetary Exile


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Vilhelm Ekelunds och det litterära fältet 1897-1949 [Vilhelm Ekelund and the literary field 1897-1949] The theoretical background of this study is Pierre Bourdieu’s sociological approach to literature. I use his theory concerning the importance of cultural (and other forms of symbolic) capital for the individual artist – and his description of the literary field as a place characterized by continuous conflict between different categories of participants. In the article, I argue that as a young poet, Ekelund held a position in the field that was with the intellectual group as opposed to the group of commercial authors – and among the young avant-garde as opposed to among the consecrated and well-established writers. However, this position changed somewhat during the years Ekelund spent in exile (1908-1921), and it continued to change after his return to Sweden. His reputation as a thoroughly intellectual writer was accentuated and, as time passed, he himself became a consecrated artist with certain privileges – e.g. grants and awards – to defend.

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Apresentamos fotometria profunda (V ~ 25,5) nas bandas V e I obtidas com a Wide Field and Planetary Camera 2 a bordo do telesc opio espacial Hubble para 7 campos distantes ~5º do centro da Grande Nuvem de Magalhães. Ajustamos isócronas aos diagramas cor-magnitude a fim de identficar diferentes populaões estelares nestes campos. Uma população velha (τ > 10¹º anos) foi encontrada em todos os campos. Alguns eventos de elevada formação estelar, com idades entre 2 x 109 e 4 x 109 anos, foram também encontrados em alguns campos localizados na região N/NO. Funções de luminosidade de estrelas de baixa massa (m ≤ 1; 1msol) foram obtidas para todos os campos. Aparentemente não há diferenças na mistura de populações entre os campos como sugerido através do teste Kolmogorov-Smirnov aplicados as funções de luminosidade. Finalmente, derivamos perfis de densidade para estrelas velhas e de idade intermediária. O primeiro apresenta uma inclinação levemente maior quando comparado com o último.

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Apresentamos a fotometria de 6 campos estelares profundos distribuídos na Grande Nuvem de Magalhães obtidos com a Wide Field and Planetary Camera 2/Hubble Space Telescope em duas bandas fotométricas: F814W (~I) e F555W (~V). Foram selecionadas ao todo 15997 estrelas pela nossa amostra, que somadas às estrelas da amostra de Castro et aI. 2001 [9] contabilizaram 22239 estrelas, dentro de limites de magnitude típicos que estão no intervalo 18.5<-V <-26. Investigamos o comportamento do erro fotométrico através da tarefa PHOT/IRAF, bem como via medidas independentes de magnitude de um mesmo objeto obtidas com diferentes exposições. Implementamos um método de correção para a completeza fotométrica como função da posição no diagrama cor-magnitude, isto é, com função tanto da magnitude como da cor e analisamos a sensibilidade das funções de luminosidade obtidas para diferentes métodos de correção. Foram obtidos os diagramas cor-magnitude, com os quais ajustamos isócronas de Pádova com idades T ;S 16 Gano e metalicidades 0.001 < Z < 0.004 ou -1.3 < [Fe/H] < -0.7. A população mais velha (r~12 Gano) pode ser encontrada através do ponto de turn-off em V~22. Estrelas de idade intermediária (r~1 - 8 Gano) podem ser localizadas pela presença de um clump. Os campos próximos aos aglomerados jovens NGC1805 e NGC1818 são os campos mais populosos, apresentando estrelas com r~1 Gano. Construímos funções de luminosidade para 18.5<-V <-25, utilizando os dados das duas amostras; não foram encontradas diferenças significativas entre os campos Desenvolvemos um método para geração de diagramas cor-magnitude (CMDs) artificiais a partir de um modelo de histórico de formação estelar. Este método incorpora os efeitos de erros fotométricos, binarismo não resolvido, avermelhamento e permite o uso de formas variadas de função de massa inicial e do próprio histórico. Implementamos o Método dos Modelos Parciais para modelamento de CMDs, incluindo experimentos controlados para a comprovação da validade deste método na busca de vínculos ao histórico de formação estelar da Grande Nuvem de Magalhães em dife!entes regiões. Recuperamos SFHs confiáveis para cada um dos 6 campos da LMC. Observamos variações na formação estelar de um campo para outro. Em todos os campos encontramos uma lacuna na formação estelar com 7 rv 700 Mano. Os dois campos próximos à barra (NGC1805 e NGC1818) apresentam alguns pequenos surtos, tendo formado em sua maioria, estrelas velhas ou relativamente jovens. Já os campos próximos a NGC1831 e NGC1868 apresentam formação estelar que se aproxima de um histórico de formação estelar uniforme, com alguns pequenos surtos. Os campos NGC2209 e Hodge 11 apresentam três períodos de formação estelar muitos semelhantes.

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Este trabalho considera que o mundo está vivendo uma mudança de paradigma. Neste sentido, procura caminhos de expansão da consciência para esta mudança através da problemática ecológica, da historicidade da ciência e de seus fundamentos na física mecanicista. planetária que a ecologia sugere, a diferentes culturas e tradições de Percebe que a crise física atual e as sabedoria podem contribuir para a construção de uma nova forma de viver. Para tanto, desenvolve o conceito de "expansão da consciência", porque acredita que esta abordagem, resultante da práxis transdisciplinar da autora, pode levar a uma maior percepção da Totalidade da vida e também da sua rica Diversidade, pontos centrais para o novo paradigma. Desta maneira, este trabalho é parte de um movimento de mudança dos conceitos e atitudes presentes no paradigma moderno, a fim de que a Educação comece a vivenciar outras formas de conhecimento do real, diferentes dos rígidos limites científicos.

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Ta-Cu bulk composites combine high mechanical resistance of the Ta with high electrical and thermal conductivity of the Cu. These are important characteristics to electrical contacts, microwave absorber and heat skinks. However, the low wettability of Ta under Cu liquid and insolubility mutual these elements come hard sintering this composite. High-energy milling (HEM) produces composite powders with high homogeneity and refines the grain size. This work focus to study Ta-20wt%Cu composite powders prepared by mechanical mixture and HEM with two different conditions of milling in a planetary ball mill and then their sintering using hydrogen plasma furnace and a resistive vacuum furnace. After milling, the powders were pressed in a steel dye at a pressure of 200 MPa. The cylindrical samples pressed were sintered by resistive vacuum furnace at 10-4torr with a sintering temperature at 1100ºC / 60 minutes and with heat rate at 10ºC/min and were sintered by plasma furnace with sintering temperatures at 550, 660 and 800ºC without isotherm under hydrogen atmosphere with heat rate at 80ºC/min. The characterizations of the powders produced were analyzed by scanning electron microscopy (SEM), x-ray diffraction (XRD) and laser granulometry. After the sintering the samples were analyzed by SEM, XRD and density and mass loss tests. The results had shown that to high intense milling condition produced composite particles with shorter milling time and amorphization of both phases after 50 hours of milling. The composite particles can produce denser structure than mixed powders, if heated above the Cu melting point. After the Cu to arrive in the melting point, liquid copper leaves the composite particles and fills the pores

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Metal powder sintering appears to be promising option to achieve new physical and mechanical properties combining raw material with new processing improvements. It interest over many years and continue to gain wide industrial application. Stainless steel is a widely accepted material because high corrosion resistance. However stainless steels have poor sinterability and poor wear resistance due to their low hardness. Metal matrix composite (MMC) combining soft metallic matrix reinforced with carbides or oxides has attracted considerable attention for researchers to improve density and hardness in the bulk material. This thesis focuses on processing 316L stainless steel by addition of 3% wt niobium carbide to control grain growth and improve densification and hardness. The starting powder were water atomized stainless steel manufactured for Höganäs (D 50 = 95.0 μm) and NbC produced in the UFRN and supplied by Aesar Alpha Johnson Matthey Company with medium crystallite size 16.39 nm and 80.35 nm respectively. Samples with addition up to 3% of each NbC were mixed and mechanically milled by 3 routes. The route1 (R1) milled in planetary by 2 hours. The routes 2 (R2) and 3 (R3) milled in a conventional mill by 24 and 48 hours. Each milled samples and pure sample were cold compacted uniaxially in a cylindrical steel die (Ø 5 .0 mm) at 700 MPa, carried out in a vacuum furnace, heated at 1290°C, heating rate 20°C stand by 30 and 60 minutes. The samples containing NbC present higher densities and hardness than those without reinforcement. The results show that nanosized NbC particles precipitate on grain boundary. Thus, promote densification eliminating pores, control grain growth and increase the hardness values

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This work a studied the high energy milling effect in microstructure and magnetic properties of the WC-10wt.%Co composite. The composite powders were prepared by mechanical mixed and milled at 2 hours, 100 hours, 200 hours and 300 hours in planetary milling. After this process the composite were compacted in stainless steel die with cylindrical county of 10 mm of diameter, at pressure 200 Mpa and sintered in a resistive furnace in argon atmosphere at 1400 oC for 5 min. The sintered composite were cutted, inlaid, sandpapered, and polished. The microestrutural parameters of the composite was analyzed by X-ray diffraction, scanning electronic microscopy, optical microscopy, hardness, magnetic propriety and Rietveld method analyze. The results shows, with milling time increase the particle size decrease, it possibility minor temperature of sintering. The increase of milling time caused allotropic transformation in cobalt phase and cold welding between particles. The cold welding caused the formation of the particle composite. The X-ray diffraction pattern of composite powders shows the WC peaks intensity decrease with the milling time increase. The X-ray diffraction pattern of the composite sintered samples shows the other phases. The magnetic measurements detected a significant increase in the coercitive field and a decrease in the saturation magnetization with milling time increase. The increase coercitive field it was also verified with decrease grain size with milling time increase. For the composite powders the increase coercitive field it was verified with particle size reduction and saturation magnetization variation is relate with the variation of free cobalt. The Rietveld method analyze shows at milling time increase the mean crystalline size of WC, and Co-cfc phases in composite sintered sample are higher than in composite powders. The mean crystallite size of Co-hc phase in composite powders is higher than in composite sintered sample. The mean lattice strains of WC, Co-hc and Co-cfc phases in composite powders are higher than in composite sintered samples. The cells parameters of the composite powder decrease at milling time increase this effect came from the particle size reduction at milling time increase. In sintered composite the cells parameters is constant with milling time increase

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In this work, was studied the formation of a composite of the refractory metal niobium with copper, through the process of high-energy milling and liquid phase sintering. The HEM can be used to synthesize composite powders with high homogeneity and fine size particle distribution. It may also produce the solid solubility in immiscible systems such as Nb-Cu, or extend the solubility of systems with limited solubility. Therefore, in the immiscible system Cu-Nb, the high-energy milling was successfully used to obtain the composite powder particles. Initially, the formation of composite particles during the HEM and the effect of preparation technique on the microstructure of the material was evaluated. Four loads of Nb and Cu powders containing 20%wt Cu were synthesized by MAE in a planetary type ball mill under different periods of grinding. The influence of grinding time on the metal particles is evaluated during the process by the withdrawal of samples at intermediate times of milling. After compaction under different forces, the samples were sintered in a vacuum furnace. The liquid phase sintering of these samples prepared by HEM produced a homogeneous and fine grained. The composite particles forming the sintered samples are the addition of a hard phase (Nb) with a high melting point, and a ductile phase (Cu) with low melting point and high thermal and electrical conductivities. Based on these properties, the Nb-Cu system is a potential material for many applications, such as electrical contacts, welding electrodes, coils for generating high magnetic fields, heat sinks and microwave absorbers, which are coupled to electronic devices. The characterization techniques used in this study, were laser granulometry, used to evaluate the homogeneity and particle size, and the X-ray diffraction, in the phase identification and to analyze the crystalline structure of the powders during milling. The morphology and dispersion of the phases in the composite powder particles, as well the microstructures of the sintered samples, were observed by scanning electron microscopy (SEM). Subsequently, the sintered samples are evaluated for density and densification. And finally, they were characterized by techniques of measuring the electrical conductivity and microhardness, whose properties are analyzed as a function of the parameters for obtaining the composite

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In this study it was used two metallic oxides, Ta2O5 and TiO2, in order to obtain metallic powders of Ta and Ti through aluminothermic reduction ignited by plasma. Ta2O5 and TiO2 powders were mixed with Al in a planetary mill, using different milling times. A thermal analysis study (DTA and TG) was carried out, in order to know the temperature to react both the mixtures. Then, these mixtures were submitted to a hollow cathode discharge, where they were reacted using aluminothermic reduction ignited by plasma. The product obtained was characterized by XRD and SEM, where it was proven the possibility of producing these metallic particles, different from the conventional process, where metallic ingots are obtained. It was verified that the aluminothermic reduction ignited by plasma is able to produce metallic powders of Ta and Ti, and a higher efficiency was observed to the process with Ta2O5-Al mixtures. Among different microstructural aspects observed, it can be noted the presence of metallic nanoparticles trapped into an Al2O3 matrix, besides acicular structures (titanium) and dendritic structures (tantalum), which are a product characteristic from a fast cooling

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Steel is an alloy EUROFER promising for use in nuclear reactors, or in applications where the material is subjected to temperatures up to 550 ° C due to their lower creep resistance under. One way to increase this property, so that the steel work at higher temperatures it is necessary to prevent sliding of its grain boundaries. Factors that influence this slip contours are the morphology of the grains, the angle and speed of the grain boundaries. This speed can be decreased in the presence of a dispersed phase in the material, provided it is fine and homogeneously distributed. In this context, this paper presents the development of a new material metal matrix composite (MMC) which has as starting materials as stainless steel EUROFER 97, and two different kinds of tantalum carbide - TaC, one with average crystallite sizes 13.78 nm synthesized in UFRN and another with 40.66 nm supplied by Aldrich. In order to improve the mechanical properties of metal matrix was added by powder metallurgy, nano-sized particles of the two types of TaC. This paper discusses the effect of dispersion of carbides in the microstructure of sintered parts. Pure steel powders with the addition of 3% TaC UFRN and 3% TaC commercial respectively, were ground in grinding times following: a) 5 hours in the planetary mill for all post b) 8 hours of grinding in the mill Planetary only for steel TaC powders of commercial and c) 24 hours in the conventional ball mill mixing the pure steel milled for 5 hours in the planetary mill with 3% TaC commercial. Each of the resulting particulate samples were cold compacted under a uniaxial pressure of 600MPa, on a cylindrical matrix of 5 mm diameter. Subsequently, the compressed were sintered in a vacuum furnace at temperatures of 1150 to 1250 ° C with an increment of 20 ° C and 10 ° C per minute and maintained at these isotherms for 30, 60 and 120 minutes and cooled to room temperature. The distribution, size and dispersion of steel and composite particles were determined by x-ray diffraction, scanning electron microscopy followed by chemical analysis (EDS). The structures of the sintered bodies were observed by optical microscopy and scanning electron accompanied by EDS beyond the x-ray diffraction. Initial studies sintering the obtained steel EUROFER 97 a positive reply in relation to improvement of the mechanical properties independent of the processing, because it is obtained with sintered microhardness values close to and even greater than 100% of the value obtained for the HV 333.2 pure steel as received in the form of a bar

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The thesis aims at discussing and analyzing the Principle of Human Dignity in its multidimensionality, in a way not exclusively individual and anthropocentrical, but rather intersubjective and planetary, which implies to say that such understanding transcends the human itself, in order to contemplate the dignity of an individual connected to the world. In this context, the thesis proposes stretching the disciplinarity of the Law, unfolding the Legal Science to a more thorough perception of the human condition, encompassing the individual, social, anthropolitical and anthropoetical dimensions. It is not about, however, resorting to an abstract idea, but rather undertaking the construction of the concrete universality of such understanding, which translates into contextualizing the face of a planetary identity of the man, also taking into account its triunic nature which encompasses the dialogical and complementary relations amongst individual, society and species

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This thesis deals with the intellectual itinerary of the humanist, lawyer and educator RN Helio Vasconcelos in building a more cohesive society, just and egalitarian, less marked by inequality, by poverty, ignorance and lack of freedom of his people suffered and loved. It also shows, as after suffering the hardships caused by the political persecution and imprisonment, exile faced with dignity, developing an exemplary job of defending the rights of children and adolescents. For this, redo the way that intellectual humanist, simple man who never gave up their way of thinking, of viewing the world, to love and respect all that surrounds him, thinking globally and acting locally, always holding the defense Rights human. Helium shows how solidarity exercised intensely and as bothered with the real interests of the community to hold public office. It seeks to demonstrate the need for reformulation of Legal Education in order to stimulate the formation of a lawyer gifted humanist profile

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The networks terminology has been growing in different meanings, in which emergent structures coming from one not so recently typology aquired, in the 90 s, fluid shapes impelled by waves without borders of the New Information and Communication Technologies. Ever since, the pattern and the morphology are being multiply and strengthen. With this backdrop, this study deals with the Education for Environment Networks, as a political and social, educative and cultural alternative intervention, as an answer for some contemporary demands. But what are these networks? In wich way they organize themselves to germinate political actions? Where is the core of these actions? What are their limits or potentialities? These are some of the questions that are presented along the study proposed. Therefore, we have in view to unveil the network social and environmental pedagogic dimension, as an alternative proposal towards to the planetary cintzenship formation for persons and coletivity. The study employs the exploration reasearch as the analysis of the organizational reference basis and the dinamics of conections that support the dialogue among the groups that belong to the Education for Environment Networks. We conclude that the networks overcome themselves as a powerfull tool to articulate and moblize people. They establish a potential pedagogic act for political and social intervention, as an alternative proposal for the citizen formation and his world vision. We sinalize that the networks are sometimes limited by the poorness of knowledge that still remains on those who find themselves twisted on them, and on the decreasing optics by those who are absent.

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O segundo satélite da Missão Espacial Completa Brasileira (SCD2/MECB) foi colocado em órbita em 23 de Outubro de 1998 e carrega a bordo um experimento de células solares. Célula solar de silício é um dispositivo semicondutor, que pode medir a intensidade da radiação visível e parte da radiação infravermelha (400-1100 nm). O experimento permite medir simultaneamente a insolação direta e parte da radiação solar que é refletida pela Terra para o espaço. Os dados do experimento célula solar são transmitidos em tempo real pela telemetria do satélite e recebidos pela estação terrestre em Cuiabá, MT-Brasil (16°S; 56°W). Este fato limita a cobertura espacial para um círculo sobre a América do Sul. O albedo planetário é obtido dentro desta cobertura e seus valores podem ser agrupados em períodos temporais (anual, sazonal ou mensal), ou podem ser estudados para várias localizações (latitude e longitude) durante a vida do satélite. O coeficiente de transmissão atmosférica ou índice de claridade (Kt), medido em estações meteorológicas na superfície da Terra, junto com o valor medido simultaneamente do albedo planetário, permite calcular o coeficiente de absorção atmosférica (Ka). O método desenvolvido neste trabalho para avaliar Ka considera que o albedo planetário é composto por duas partes: uma refletividade local e uma refletividade não local. Considerando este novo conceito, é definida uma taxa de absorção atmosférica (denominada Ra) que é a razão entre Ka e a potência de irradiância solar líquida, que não atravessou a atmosfera (100%-Kt). A taxa de absorção atmosférica assim definida é independente da cobertura de nuvens. O histograma de freqüência de Ra mostra os valores de 0,86±0,07 e 0,88±0,09 sobre as cidades de Botucatu-SP e do Rio de Janeiro-RJ, durante os anos de 1999 até 2006, respectivamente.