957 resultados para Fondazioni Pozzo Terreno Interazione Ponte


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This work studies the major sports overload injuries of the lower extremities from the biomechanical point of view. At the same time, the main paradigms of podiatric biomechanics and the application of new biomechanical theories in the study of these lesions are reviewed. With current legislation, clinical gait biomechanical studies should be carried out in health centres and the only health professionals who can perform them are podiatrists and doctors (because they both can diagnose). Graduates in physical education can carry out studies in the field or in the sports court for the sole purpose of improving athletic performance, but never intended to treat a pathology overload.

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Three different worlds, sometimes concentric and often intersecting —society, theatre and the art of performance— and social work. Diverse worlds that live, reflect and self-reflect and interact, and can also afford an opportunity for meeting, misunderstanding and confrontation, and above all offer the possibility of profound change.This article considers the experience of a theatre company that has spent more than three years moving at the limits of these three universes. To these three worlds can be added an infinite number of words that fill them with meaning and significance: territory, meeting, diversity and search. An artistic experience that has chosen to focus on creating scenarios for debate and to examine the difficulties, the human contradictions and the constant and inexhaustible confrontation with human experience. At the heart of this theatrical activity is all of this, seeking the balance between narration, meeting, investigation and the artistic dimension. This meeting between society, theatre and social work also contains the search for sustainability of this cultural business, in an Italy that has been destroyed by a crisis that is not merely economic, but also of values and, above all, of role models. The guiding theme, though not always made explicit, is always present and essential: the search for beauty.

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El rol desempeñado por la opinión pública en el desarrollo de la política criminal actual justifica el incremento de investigaciones destinadas a evaluar las actitudes de los ciudadanos hacia el castigo. No obstante, los avances en este ámbito han sido limitados debido a la utilización de rudimentarios instrumentos de medida. Por ello, el presente trabajo tiene como propósito explorar el efecto que generan en la opinión ciudadana ciertas variables referidas al hecho delictivo y al infractor, precisando su contribución relativa y la interacción existente entre ellas. Para satisfacer este objetivo se recurrió a un diseño factorial de la encuesta, creando una población de 256 casos-escenario fruto de la combinación de cuatro factores: la edad del joven, su historial delictivo, el grado de implicación en el hecho y el tipo de delito cometido. Los mismos fueron distribuidos en grupos de ocho casos ordenados aleatoriamente y fueron suministrados a 32 sujetos. Posteriormente se aplicaron análisis de regresión logística binaria. Los resultados obtenidos revelan que la naturaleza violenta de los hechos, la implicación activa de los jóvenes y el historial delictivo son predictores importantes de las condenas punitivas. Sin embargo la edad, una variable fundamental en la configuración de la justicia juvenil, no resulta significativa. De este modo, el trabajo muestra el potencial explicativo de este conjunto de factores y debate sus implicaciones teóricas y metodológicas para la investigación futura en este terreno.

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We tried to extend the notion of truth, from the rational concept towards the subjective one. We not only exist by the thought, but also by the feeling. If we apply the scientific method to everything, we remain without art. We want to adhere ourselves to the intimate experience of the subjective thing. In art, the eye introduces the perspective and eliminates the interpretation possibility. Something similar happens with the matter: verb is to matter as name is to form. The Academy has given importance to the form, and it has forgotten the poetical qualities of the matter; it has focused on the figure and it has forgotten the background. However, we have to pay attention to the accidental thing, to the rupture of the protocol, to the frenzy of everything that is alive. For this reason, we pay attention to our intuition, to the sleepy subsoil of our ordinary experience whose inertia has lost the disruptive value of the action. At the end of this article we offer practical exercises, with which we wish to revitalize our centres of attention.

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We present mid-infrared (MIR) observations of the Type II-plateau supernova (SN) 2004et, obtained with the Spitzer Space Telescope between 64 and 1406 days past explosion. Late-time optical spectra are also presented. For the period 300-795 days past explosion, we argue that the spectral energy distribution (SED) of SN 2004et comprises (1) a hot component due to emission from optically thick gas, as well as free-bound radiation; (2) a warm component due to newly formed, radioactively heated dust in the ejecta; and (3) a cold component due to an IR echo from the interstellar-medium dust of the host galaxy, NGC 6946. There may also have been a small contribution to the IR SED due to free-free emission from ionized gas in the ejecta. We reveal the first-ever spectroscopic evidence for silicate dust formed in the ejecta of a supernova. This is supported by our detection of a large, but progressively declining, mass of SiO. However, we conclude that the mass of directly detected ejecta dust grew to no more than a few times 10(-4) M-circle dot. We also provide evidence that the ejecta dust formed in comoving clumps of fixed size. We argue that, after about two years past explosion, the appearance of wide, box-shaped optical line profiles was due to the impact of the ejecta on the progenitor circumstellar medium and that the subsequent formation of a cool, dense shell was responsible for a later rise in the MIR flux. This study demonstrates the rich, multifaceted ways in which a typical core-collapse supernova and its progenitor can produce and/or interact with dust grains. The work presented here adds to the growing number of studies that do not support the contention that SNe are responsible for the large mass of observed dust in high-redshift galaxies.

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We present results based on mid-infrared (3.6-30 mm) observations with the Spitzer Space Telescope of the nearby Type IIP supernova 2005af. We report the first ever detection of the SiO molecule in a Type IIP supernova. Together with the detection of the CO fundamental, this is an exciting finding as it may signal the onset of dust condensation in the ejecta. From a wealth of fine-structure lines we provide abundance estimates for stable Ni, Ar, and Ne that, via spectral synthesis, may be used to constrain nucleosynthesis models.

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We present mid-infrared (MIR) spectroscopy of a Type II-plateau supernova, SN 2004dj, obtained with the Spitzer Space Telescope, spanning 106--1393d after explosion. MIR photometry plus optical/near-IR observations are also reported. An early-time MIR excess is attributed to emission from non-silicate dust formed within a cool dense shell (CDS). Most of the CDS dust condensed between 50d and 165d, reaching a mass of $0.3x^(-5)Msun. Throughout the observations much of the longer wavelength (>10microns) part of the continuum is explained as an IR echo from interstellar dust. The MIR excess strengthened at later times. We show that this was due to thermal emission from warm, non-silicate dust formed in the ejecta. Using optical/near-IR line-profiles and the MIR continua, we show that the dust was distributed as a disk whose radius appeared to be slowly shrinking. The disk radius may correspond to a grain destruction zone caused by a reverse shock which also heated the dust. The dust-disk lay nearly face-on, had high opacities in the optical/near-IR regions, but remained optically thin in the MIR over much of the period studied. Assuming a uniform dust density, the ejecta dust mass by 996d was 0.5+/-0.1 x 10^(-4)Msun, and exceeded 10^(-4)Msun by 1393d. For a dust density rising toward the center the limit is higher. Nevertheless, this study suggests that the amount of freshly-synthesized dust in the SN 2004dj ejecta is consistent with that found from previous studies, and adds further weight to the claim that such events could not have been major contributors to the cosmic dust budget.

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We present mid-infrared (5.2-15.2 mu m) spectra of the Type Ia supernovae (SNe Ia) 2003hv and 2005df observed with the Spitzer Space Telescope. These are the first observed mid-infrared spectra of thermonuclear supernovae, and show strong emission from fine-structure lines of Ni, Co, S, and Ar. The detection of Ni emission in SN 2005df 135 days after the explosion provides direct observational evidence of high-density nuclear burning forming a significant amount of stable Ni in a SN Ia. The SN 2005df Ar lines also exhibit a two-pronged emission profile, implying that the Ar emission deviates significantly from spherical symmetry. The spectrum of SN 2003hv also shows signs of asymmetry, exhibiting blueshifted [Co (III)], which matches the blueshift of [Fe (II)] lines in nearly coeval near-infrared spectra. Finally, local thermodynamic equilibrium abundance estimates for the yield of radioactive Ni-56 give M-56Ni approximate to 0.5 M-circle dot, for SN 2003hv, but only M-56Ni approximate to 0.13-0.22 M-circle dot for the apparently subluminous SN 2005df, supporting the notion that the luminosity of SNe Ia is primarily a function of the radioactive 56Ni yield. The observed emission-line profiles in the SN 2005df spectrum indicate a chemically stratified ejecta structure, which matches the predictions of delayed detonation (DD) models, but is entirely incompatible with current three-dimensional deflagration models. Furthermore, the degree that this layering persists to the innermost regions of the supernova is difficult to explain even in a DD scenario, where the innermost ejecta are still the product of deflagration burning. Thus, while these results are roughly consistent with a delayed detonation, it is clear that a key piece of physics is still missing from our understanding of the earliest phases of SN Ia explosions.

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We present a new, detailed analysis of late-time mid-infrared observations of the Type II-P supernova (SN) 2003gd. At about 16 months after the explosion, the mid-IR flux is consistent with emission from 4 x 10(-5) M. of newly condensed dust in the ejecta. At 22 months emission from pointlike sources close to the SN position was detected at 8 and 24 mu m. By 42 months the 24 mu m flux had faded. Considerations of luminosity and source size rule out the ejecta of SN 2003gd as the main origin of the emission at 22 months. A possible alternative explanation for the emission at this later epoch is an IR echo from preexisting circumstellar or interstellar dust. We conclude that, contrary to the claim of Sugerman and coworkers, the mid-IR emission from SN 2003gd does not support the presence of 0.02 M. of newly formed dust in the ejecta. There is, as yet, no direct evidence that core-collapse supernovae are major dust factories.

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We present late-time ( 590 - 994 days) mid-IR photometry of the normal but highly reddened Type IIP supernova SN 2002hh. Bright, cool, slowly fading emission is detected from the direction of the supernova. Most of this flux appears not to be driven by the supernova event but instead probably originates in a cool, obscured star formation region or molecular cloud along the line of sight. We also show, however, that the declining component of the flux is consistent with an SN-powered IR echo from a dusty progenitor CSM. Mid-IR emission could also be coming from newly condensed dust and/or an ejecta/CSM impact, but their contributions are likely to be small. For the case of a CSM-IR echo, we infer a dust mass of as little as 0.036 M-. with a corresponding CSM mass of 3.6(0.01/ r(dg)) M-., where rdg is the dust-to-gas mass ratio. Such a CSM would have resulted from episodic mass loss whose rate declined significantly about 28,000 years ago. Alternatively, an IR echo from a surrounding, dense, dusty molecular cloud might also have been responsible for the fading component. Either way, this is the first time that an IR echo has been clearly identified in a Type IIP supernova. We find no evidence for or against the proposal that Type IIP supernovae produce large amounts of dust via grain condensation in the ejecta. However, within the CSM-IR echo scenario, the mass of dust derived implies that the progenitors of the most common of core-collapse supernovae may make an important contribution to the universal dust content.

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As práticas educativas e os procedimentos pedagógicos, no plano do ensino pré-escolar, podem ser classificados mediante variadas propostas presentes na literatura e passíveis de serem observadas no terreno. Nesta perspetiva, e de modo introdutório ao tema, pergunto-me acerca dos modos pelos quais o agente educativo pode acompanhar e intervir pedagogicamente no âmbito da expressão plástica. Questão que surgiu por ter tido oportunidade de observar práticas de Expressão Plástica que parecem configurar num quadro marcado ora por um método de ensino muito condicionado pelas intenções do educador, ora por um método completamente aleatório, onde não se faz qualquer preparação prévia dando lugar ao que se entende por expressão livre. Face a este quadro questionei-me sobre qual deverá ser a minha atuação em termos de práticas e dinâmicas de expressão plástica no ensino pré-escolar. Neste relatório, reuni algumas respostas para a questão anterior, utilizando a revisão de literatura. Destaco, também, alguns dados empíricos recolhidos de maneira não sistemática pela observação direta e por entrevistas realizadas no âmbito desta investigação.

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O objectivo do estudo centrou-se na avaliação da dinâmica de nemátodes fitoparasitas, e relação com alguns parâmetros físico-químicos, num terreno utilizado para produção de beterraba sacarina, na zona de Coruche. Com o intuito de acompanhar o processo de crescimento da cultura, o estudo foi efectuado de Janeiro a Junho de 2003. Recorreu-se a métodos standard para a amostragem, extracção e observação dos nemátodes. Empregaram-se comparações estatísticas entre a sua presença e distribuição. As relações entre fitoparasitas e vários parâmetros físico-químicos do seu habitat foram verificadas por análise de componentes principais (PCA), análise canónica de correspondência (CCA) e correlações. Em virtude das acções causadas pelas práticas agrícolas, a comunidade decresceu de Janeiro a Abril, aumentando até Junho com o início do processo de rega. O número de nemátodes do género Meloidogyne foi significativamente superior, secundado por Helicotylenchus e Tylenchus. As correlações entre indivíduos e parâmetros ambientais indicam que, aparte a influência directa do hospedeiro, o cálcio, o potássio e o azoto influenciaram as relações de abundância entre os géneros.

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Resumo O trabalho de investigação que está a decorrer, tem como objeto de estudo as questões da identidade e da memória de uma aldeia alentejana, enquanto território de partilha de uma comunidade rural, tendo em conta a participação estratégica dos atores locais. Estudaremos a partir daí, a sua relação com a terra, o quotidiano, a mudança, a organização social, a ruralidade, os fatores portadores de futuro e novas propostas de desenvolvimento local, para territórios de baixa densidade. Pretende-se encontrar formas contributivas para preservar a identidade da aldeia e concomitantemente encontrar conjuntamente com os atores locais territorializados, alternativas de desenvolvimento local, capazes de contrariar a tendência de despovoamento e empobrecimento territorial. Com este trabalho de investigação, que se insere no âmbito da Sociologia da Ação, será utilizada metodologicamente o MACTOR e a sua aplicabilidade na determinação da estratégia de atores e respetivas relações de forças com o território e o que a ele diz respeito e ainda a observação participante/método de pesquisa de terreno e consequentemente o inquérito por entrevista. Pretendendo-se aprofundar e conhecer os problemas da interioridade e abandono populacional, designadamente na aldeia de Penedos que se situa na margem direita do rio Guadiana, freguesia de S. Miguel do Pinheiro e concelho de Mértola, no Baixo Alentejo. Abstract The research that is taking place, has as its object of study the issues of identity and memory of an Alentejo village, while sharing the territory of a rural community, taking into account the strategic participation of local actors. We'll look from there, his relationship with the earth, the everyday, change, social organization, rurality, the factors bearing on the future and new proposals for local development to areas of low density. The aim is to find ways contributory to preserve the identity of the village and found concomitantly in conjunction with local stakeholders territorialized, alternative local development, able to counteract the trend of depopulation and impoverishment territorial. With this research work, which falls within the Sociology of Action, will be used to methodologically MACTOR and its applicability in determining the strategy of respective actors and power relations with the territory and that he has concerns and participant observation / method of field research and thus the survey interview. Intending to go deeper and understand the problems of interiority and abandoned population, particularly in the village of Penedos which lies on the right bank of the Guadiana River, parish of S. Miguel do Pinheiro, county of Mértola, in the Baixo Alentejo.

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This article details how the primary studies are specified to establish the flow of energy power generation and principally the turbines design flow, starting from the analysis of how determine the flow of a basin and also the methods to define the runoff flow which generates the rainfalls in the basins, analyzing the kind of grounds. When the flow of the river (basin) and design flow are specified, the type of turbine to be used is determined and also define the best efficiency possible, taking into consideration the geography of the zone of the hydroelectric, the abacus help to choose the turbine in agreed to parameters like electricity potency, voltage drops and voltage. By using the above software previously, for the design house Sarapullo and Alluriquín Hydroelectric Project Toachi machines - Pilatón, it was determined that each generating station will have three turbines type Francis of vertical axis with their complementary systems for its operation which are designed to generate 254.4 megawatts (MW) using a flow of 33.33 m3/s. Keywords: flow, basin, electric power, runoff, hydroelectric, turbine.

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El diseño de una empresa agrícola productora de frutilla en la ciudad de Quito, fue creado con el fin de implementar un proyecto atractivo con ventajas competitivas que permitan obtener resultados positivos, dentro del cual se realizan cuatro estudios que son: de mercado, técnico, financiero y de impacto. Por tanto, para observar la viabilidad del mismo se investigó utilizando una muestra poblacional de 384 familias del sector norte de la ciudad de Quito y mediante la colaboración de otras fuentes, con lo cual se pudo obtener resultados confiables sobre la oferta y demanda de frutilla existente en la ciudad de Quito, con lo cual se obtuvo que la oferta de frutilla para el presente año, en la ciudad de Quito, es de 3`564.074 kilos y la demanda es de 4´455.093 kilos, resultando una demanda insatisfecha de 891.018 kilos de frutilla, cuya demanda puede ser satisfecha con la implementación de proyectos como éste. Esta empresa estará ubicada en el sector norte de Quito, en San Juan de Calderón, donde se realizará el cultivo de frutilla con la utilización de un terreno de 1080 metros cuadrados, distribuidos eficiente y adecuadamente para obtener la productividad esperada, constando de 12 platabandas con tres hileras cada una, que medirán 47 metros de largo y 1 metro de ancho, cuyo cultivo, producirá la cantidad de 18360 kilos de frutilla al año. Contando con las respectivas contingencias, este cultivo se desarrolla en un ciclo de producción de tres meses, momento en el cual ya está lista la fruta para su distribución, realizando para esto tres siembras de cuatro platabandas cada una de ellas, las cuales se sembrarán cuatro en enero, cuatro en febrero y las últimas cuatro platabandas en marzo, obteniendo con esto una producción secuencial mensual a partir del mes de abril del primer año, puesto que la cantidad de equilibrio de la distribución de frutilla en la ciudad de Quito es de 8.098 kilos al año, lo que representa que la producción a obtener es superior, también es necesario expresar que aunque es un cultivo muy fácil de implementar se deben tener los conocimientos necesarios para ello, cuya información se encuentra en el presente trabajo.