998 resultados para Cores na literatura


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This study was idealized in order to understand the universe of colors in the visual arts and in our lives. The color itself is a mystery even today. Even it has already been explained by several scientists, theorists and experts in our lives, the color is too complex for our understanding and feelings. Every day we see real examples of how colors act in our bodies, in our brains, and our tastes, colors influence us at all. And through this work we can understand a little of the physiological side, and how the color was used in our daily life and the arts

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A realização deste trabalho tem como norte a verificação de questões típicas de países periféricos colonizados, como a busca identitária imbricada num processo de hibridação cultural. Para tanto, trabalhamos com duas obras consagradas da literatura brasileira: Iracema, de José de Alencar, e Macunaíma, de Mário de Andrade, vinculando as mesmas a seus períodos literários correspondentes e, estes, ao meio social e político, numa abordagem que privilegia a sociologia da literatura, em que a obra de Antonio Candido, especialmente, serve de base teórico-prática para a realização desta pesquisa. Nesse contexto, achamos interessante, também, verificar como o indianismo de Alencar, trabalhando numa perspectiva pós-colonial e imbuído de um sentimento patriótico e mitificador do índio e da natureza, faz com que a literatura brasileira integre-se às literaturas européias. E, ainda, com que estratégias Macunaíma consegue inverter esteticamente a visão etnocêntrica tradicional e trabalhar com a capacidade crítica de selecionar o que não é do autóctone mas que nos interessa, tingindo esta ação seletiva e seu produto com as cores locais para torná-los dignos representantes de nosso sincretismo racial e cultural. Assim, através de uma postura crítico-sociológica, damos início a uma caminhada pelo viés literário e verificamos que este revelou a hibridação cultural própria do povo brasileiro, ultrapassando preconceitos etnocêntricos, aparentemente sólidos, e mostrando que o caldeamento de raças e, conseqüentemente de crenças e costumes, não deve ser olhado sob a ótica da anomalia mas, sim, sob a luz da fertilidade. Desse modo, as obras analisadas, apesar de possuírem estéticas singulares e pertencerem a quadros sócio-políticos distintos, apresentam em sua essência um compromisso literário maior: fazer uma ficção representativa da realidade cultural brasileira.

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El carácter pedagógico de la literatura infantil ha servido, por largo tiempo, como factor de desprestigio del género, ya sea por la imposición de paradigmas comportamentales advenidos de una postura autoritaria de los adultos, subyacente al texto, ya sea por haber minimizado la preocupación artística del lenguaje. Este artículo analiza de que manera la narrativa O meu amigo pintor, de Lygia Bojunga, supera ese modelo, al instaurar un equilibrio entre el respeto al universo en formación de los niños y los medios lingüísticos que representan el universo infantil desde la mirada de la propia creatura, facultándole a ella la elaboración de sus significados.

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O estudo remete para uma experiência realizada com crianças em contexto educativo, em estreita colaboração com os seus familiares, abrangendo como eixo temático a Literatura para a infância e espaços educativos. A participação e envolvimento da família na educação das crianças, em contexto de educação pré-escolar, é um dos principais objetivos das instituições de educação ao longo de toda a escolaridade. Salientamos, nesta comunicação, a formação de leitores a partir da participação e envolvimento familiar, visando compreender que importância a leitura de histórias tem no desenvolvimento infantil. Apresenta-se como objetivo geral averiguar de que forma, a participação da família, em atividades de promoção da literatura para a infância, promove um maior envolvimento das crianças. Para tal, descreve-se, a partir de uma grelha de observação retirada do manual Desenvolvendo a Qualidade em Parcerias, o envolvimento das crianças. A partir deste registo, analisa-se a repercussão da participação da família nas práticas de literatura para a infância. A investigação durou três meses e foi estruturada em cinco sessões, durante as quais a investigadora observou um grupo de 20 crianças, analisando os seus comportamentos, tendo em consideração a concentração, energia, complexidade e criatividade, expressão facial e postura, persistência, precisão, tempo de reação, linguagem e satisfação, indicadores indispensáveis para a compreensão dos resultados obtidos em cada sessão. Como resultados salientamos que, ao longo das sessões realizadas, os níveis de envolvimento do grupo mostraram-se mais significativos quando os familiares salientavam as ilustrações das histórias lidas às crianças. As ilustrações frequentemente atraentes, com cores vivas e desenhos elucidativos sobre a história narrada, suscitavam no grupo momentos de grande concentração e questionamento, relacionando a leitura ouvida com as ilustrações observadas em simultâneo. Contudo, crianças de três anos demonstravam níveis de envolvimento mais baixos que as de cinco anos. As ilustrações garantiam ao grupo poder ler as histórias sem saberem ler. Através da investigação, concluiu-se que as crianças se sentiam mais motivadas, interessadas e participativas perante uma atividade associada à literatura infantil, nomeadamente quando os familiares eram solicitados a intervir em contexto escolar.

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Sylvia Orthof (1932-1997) consagrou-se como uma das mais importantes escritoras da literatura infantil brasileira. Entre suas temáticas recorrentes, os animais não humanos figuram em profusão, assim sendo, este estudo objetiva verificar a destacada presença dos gatos na obra da autora arrolada, e mais especificamente os bichanos não domésticos vivenciando momentos de especial cumplicidade com outros seres não humanos. Para tanto, realiza a análise dos seguintes textos zooliterários - o conto de animais História engatada e da fábula poética Gato pra cá, rato pra lá. As formulações críticas e teóricas, nomeadamente, de Jacques Derrida (2011) e (2003), Nelly Novaes Coelho (1991) e Fanny Abramovich (1999) fundamentam a leitura.

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Dynamic light scattering (DLS) has become a primary nanoparticle characterization technique with applications from materials characterization to biological and environmental detection. With the expansion in DLS use from homogeneous spheres to more complicated nanostructures, comes a decrease in accuracy. Much research has been performed to develop different diffusion models that account for the vastly different structures but little attention has been given to the effect on the light scattering properties in relation to DLS. In this work, small (core size < 5 nm) core-shell nanoparticles were used as a case study to measure the capping thickness of a layer of dodecanethiol (DDT) on Au and ZnO nanoparticles by DLS. We find that the DDT shell has very little effect on the scattering properties of the inorganic core and hence can be ignored to a first approximation. However, this results in conventional DLS analysis overestimating the hydrodynamic size in the volume and number weighted distributions. By introducing a simple correction formula that more accurately yields hydrodynamic size distributions a more precise determination of the molecular shell thickness is obtained. With this correction, the measured thickness of the DDT shell was found to be 7.3 ± 0.3 Å, much less than the extended chain length of 16 Å. This organic layer thickness suggests that on small nanoparticles, the DDT monolayer adopts a compact disordered structure rather than an open ordered structure on both ZnO and Au nanoparticle surfaces. These observations are in agreement with published molecular dynamics results.

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A combined experimental and numerical program was conducted to study the in-plane shear behaviour of hollow concrete masonry panels containing reinforced grout cores. This paper is focused on the numerical program. A two dimensional macromodelling strategy was used to simulate the behaviour of the confined masonry (CM) shear panels. Both the unreinforced masonry and the confining element were modelled using macromasonry properties and the steel reinforcement was modelled as an embedded truss element located within the grout using perfectly bonded constraint. The FE model reproduced key behaviours observed in the experiments, including the shear strength, the deformation and the crack patterns of the unconfined and confined masonry panels. The predictions of the validated model were used to evaluate the existing in-plane shear expressions available in the national masonry standards and research publications.

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We present new evidence for sector collapses of the South Soufrière Hills (SSH) edifice, Montserrat during the mid-Pleistocene. High-resolution geophysical data provide evidence for sector collapse, producing an approximately 1 km3 submarine collapse deposit to the south of SSH. Sedimentological and geochemical analyses of submarine deposits sampled by sediment cores suggest that they were formed by large multi-stage flank failures of the subaerial SSH edifice into the sea. This work identifies two distinct geochemical suites within the SSH succession on the basis of trace-element and Pb-isotope compositions. Volcaniclastic turbidites in the cores preserve these chemically heterogeneous rock suites. However, the subaerial chemostratigraphy is reversed within the submarine sediment cores. Sedimentological analysis suggests that the edifice failures produced high-concentration turbidites and that the collapses occurred in multiple stages, with an interval of at least 2 ka between the first and second failure. Detailed field and petrographical observations, coupled with SEM image analysis, shows that the SSH volcanic products preserve a complex record of magmatic activity. This activity consisted of episodic explosive eruptions of andesitic pumice, probably triggered by mafic magmatic pulses and followed by eruptions of poorly vesiculated basaltic scoria, and basaltic lava flows.

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Detailed knowledge of the past history of an active volcano is crucial for the prediction of the timing, frequency and style of future eruptions, and for the identification of potentially at-risk areas. Subaerial volcanic stratigraphies are often incomplete, due to a lack of exposure, or burial and erosion from subsequent eruptions. However, many volcanic eruptions produce widely-dispersed explosive products that are frequently deposited as tephra layers in the sea. Cores of marine sediment therefore have the potential to provide more complete volcanic stratigraphies, at least for explosive eruptions. Nevertheless, problems such as bioturbation and dispersal by currents affect the preservation and subsequent detection of marine tephra deposits. Consequently, cryptotephras, in which tephra grains are not sufficiently concentrated to form layers that are visible to the naked eye, may be the only record of many explosive eruptions. Additionally, thin, reworked deposits of volcanic clasts transported by floods and landslides, or during pyroclastic density currents may be incorrectly interpreted as tephra fallout layers, leading to the construction of inaccurate records of volcanism. This work uses samples from the volcanic island of Montserrat as a case study to test different techniques for generating volcanic eruption records from marine sediment cores, with a particular relevance to cores sampled in relatively proximal settings (i.e. tens of kilometres from the volcanic source) where volcaniclastic material may form a pervasive component of the sedimentary sequence. Visible volcaniclastic deposits identified by sedimentological logging were used to test the effectiveness of potential alternative volcaniclastic-deposit detection techniques, including point counting of grain types (component analysis), glass or mineral chemistry, colour spectrophotometry, grain size measurements, XRF core scanning, magnetic susceptibility and X-radiography. This study demonstrates that a set of time-efficient, non-destructive and high-spatial-resolution analyses (e.g. XRF core-scanning and magnetic susceptibility) can be used effectively to detect potential cryptotephra horizons in marine sediment cores. Once these horizons have been sampled, microscope image analysis of volcaniclastic grains can be used successfully to discriminate between tephra fallout deposits and other volcaniclastic deposits, by using specific criteria related to clast morphology and sorting. Standard practice should be employed when analysing marine sediment cores to accurately identify both visible tephra and cryptotephra deposits, and to distinguish fallout deposits from other volcaniclastic deposits.

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The ability of E coli recA protein to promote homologous pairing with linear duplex DNA bound to HU protein (Nucleosome cores) was found to be differentially affected. The formation of paranemic joint molecules was not affected whereas the formation of plectomic joint molecules was inhibited from the start of the reaction. The formation of paranemic joint molecules between nucleoprotein filaments of recA protein-circular single stranded DNA and closed circular duplex DNA is believed to generate positive supercoiling in the duplex DNA. We found that the positively superhelical duplex DNA was inert in the formation of joint molecules but could be converted into an active substrate, in situ, by the action of wheat germ topoisomerase I. These observations initiate an understanding of the structural features of E coli chromosome such as DNA supercoiling and nucleosome-like structures in homologous recombination.

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Physical properties provide valuable information about the nature and behavior of rocks and minerals. The changes in rock physical properties generate petrophysical contrasts between various lithologies, for example, between shocked and unshocked rocks in meteorite impact structures or between various lithologies in the crust. These contrasts may cause distinct geophysical anomalies, which are often diagnostic to their primary cause (impact, tectonism, etc). This information is vital to understand the fundamental Earth processes, such as impact cratering and associated crustal deformations. However, most of the present day knowledge of changes in rock physical properties is limited due to a lack of petrophysical data of subsurface samples, especially for meteorite impact structures, since they are often buried under post-impact lithologies or eroded. In order to explore the uppermost crust, deep drillings are required. This dissertation is based on the deep drill core data from three impact structures: (i) the Bosumtwi impact structure (diameter 10.5 km, 1.07 Ma age; Ghana), (ii) the Chesapeake Bay impact structure (85 km, 35 Ma; Virginia, U.S.A.), and (iii) the Chicxulub impact structure (180 km, 65 Ma; Mexico). These drill cores have yielded all basic lithologies associated with impact craters such as post-impact lithologies, impact rocks including suevites and breccias, as well as fractured and unfractured target rocks. The fourth study case of this dissertation deals with the data of the Paleoproterozoic Outokumpu area (Finland), as a non-impact crustal case, where a deep drilling through an economically important ophiolite complex was carried out. The focus in all four cases was to combine results of basic petrophysical studies of relevant rocks of these crustal structures in order to identify and characterize various lithologies by their physical properties and, in this way, to provide new input data for geophysical modellings. Furthermore, the rock magnetic and paleomagnetic properties of three impact structures, combined with basic petrophysics, were used to acquire insight into the impact generated changes in rocks and their magnetic minerals, in order to better understand the influence of impact. The obtained petrophysical data outline the various lithologies and divide rocks into four domains. Based on target lithology the physical properties of the unshocked target rocks are controlled by mineral composition or fabric, particularly porosity in sedimentary rocks, while sediments result from diverse sedimentation and diagenesis processes. The impact rocks, such as breccias and suevites, strongly reflect the impact formation mechanism and are distinguishable from the other lithologies by their density, porosity and magnetic properties. The numerous shock features resulting from melting, brecciation and fracturing of the target rocks, can be seen in the changes of physical properties. These features include an increase in porosity and subsequent decrease in density in impact derived units, either an increase or a decrease in magnetic properties (depending on a specific case), as well as large heterogeneity in physical properties. In few cases a slight gradual downward decrease in porosity, as a shock-induced fracturing, was observed. Coupled with rock magnetic studies, the impact generated changes in magnetic fraction the shock-induced magnetic grain size reduction, hydrothermal- or melting-related magnetic mineral alteration, shock demagnetization and shock- or temperature-related remagnetization can be seen. The Outokumpu drill core shows varying velocities throughout the drill core depending on the microcracking and sample conditions. This is similar to observations by Kern et al., (2009), who also reported the velocity dependence on anisotropy. The physical properties are also used to explain the distinct crustal reflectors as observed in seismic reflection studies in the Outokumpu area. According to the seismic velocity data, the interfaces between the diopside-tremolite skarn layer and either serpentinite, mica schist or black schist are causing the strong seismic reflectivities.

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The spectral index-luminosity relationship for steep-spectrum cores in galaxies and quasars has been investigated, and it is found that the sample of galaxies supports earlier suggestions of a strong correlation, while there is weak evidence for a similar relationship for the quasars. It is shown that a strong spectral index-luminosity correlation can be used to set an upper limit to the velocities of the radio-emitting material which is expelled from the nucleus in the form of collimated beams or jets having relativistic bulk velocities. The data on cores in galaxies indicate that the Lorentz factors of the radiating material are less than about 2.

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Multiwavelength data indicate that the X-ray-emitting plasma in the cores of galaxy clusters is not cooling catastrophically. To a large extent, cooling is offset by heating due to active galactic nuclei (AGNs) via jets. The cool-core clusters, with cooler/denser plasmas, show multiphase gas and signs of some cooling in their cores. These observations suggest that the cool core is locally thermally unstable while maintaining global thermal equilibrium. Using high-resolution, three-dimensional simulations we study the formation of multiphase gas in cluster cores heated by collimated bipolar AGN jets. Our key conclusion is that spatially extended multiphase filaments form only when the instantaneous ratio of the thermal instability and free-fall timescales (t(TI)/t(ff)) falls below a critical threshold of approximate to 10. When this happens, dense cold gas decouples from the hot intracluster medium (ICM) phase and generates inhomogeneous and spatially extended Ha filaments. These cold gas clumps and filaments ``rain'' down onto the central regions of the core, forming a cold rotating torus and in part feeding the supermassive black hole. Consequently, the self-regulated feedback enhances AGN heating and the core returns to a higher entropy level with t(TI)/t(ff) > 10. Eventually, the core reaches quasi-stable global thermal equilibrium, and cold filaments condense out of the hot ICM whenever t(TI)/t(ff) less than or similar to 10. This occurs despite the fact that the energy from AGN jets is supplied to the core in a highly anisotropic fashion. The effective spatial redistribution of heat is enabled in part by the turbulent motions in the wake of freely falling cold filaments. Increased AGN activity can locally reverse the cold gas flow, launching cold filamentary gas away from the cluster center. Our criterion for the condensation of spatially extended cold gas is in agreement with observations and previous idealized simulations.