750 resultados para Fachadas solares


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Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)

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Solar heaters are an appropriate technology in tropical and sub-tropical climates to heat bath water by solar energy. Low-cost solar heaters meet the demand of low-income rural communities which currently do not have access to this technology. Current research analyzes the economic viability of solar heaters, built with recyclable materials, to reduce electric energy bill. A solar heating system was built consisting of recyclable materials in accordance with the manuals provided by the Secretariat of Environment of the state of Paraná (SEMA). Duration of use of electric showers by families of rural properties was determined to calculate expenses and billing of electricity. Simulation and material costs showed that the system was feasible. Commercial solar heaters could be replaced at a cost of R$ 22.61 per month during 13 months.

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Since ancient times, it has been a huge challenge to all people around the world to manage to get their fresh water, keeping it clean and providing it to every human being, so that it can be used for their daily needs. This is especially true for small properties in the countryside and in isolated areas with low demographic density. Pumping the water in those regions is a solution that rationalizes its use in domestic chores, in animal rearing and in the irrigation systems of cultivated areas. Making feasible local, renewable and non-polluted energetic alternatives is the aim for those areas that are usually far away from the public electric network. Using photovoltaic solar energy is the alternative now proposed. For this objective was built a system with two monocrystalline panels, one pump, two water tanks, two level sensors and a solenoid valve to pump water, using a pump powered an array of monocrystalline solar panels. The main goal was to compare their rate of water flow and their energy consumption. The use of one data acquisition equipment allowed collecting meteorological, electrical and hydraulic values, and also serving for the control and activation of the pumping system. During four months in a row as from April 2009, arrangements with one or two panels were tested. Mathematics correlations and adjustment lines were used to interpret the behavior of obtained dataset. During the analyzed period the system followed the linear equations with great accuracy. The daily average amount of water pumped by the several tested arrays stayed between 1,100 and 2,500 liters, and that is enough to supply a small rural property. The pumping system with two panels effectively showed the major amount of water, but a system with one panel can be an economical solution until 1,500 liters on day. It did not characterize a direct relationship between power or quantity of photovoltaic panels and daily outflow of water pumping.

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Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)

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Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)

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Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)

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Pós-graduação em Física - IFT

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Pós-graduação em Engenharia Elétrica - FEIS

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A radiação ultravioleta emitida pela radiação solar pode causar sérios danos à pele humana, sendo essa estratificada em três regiões do espectro de luz: UVA (315-400nm), UVB (280-315nm) e UVC (200-280nm). A incidência da radiação UVA sobre a pele induz a formação de espécies reativas de oxigênio (EROS), afetando indiretamente o DNA humano, podendo provocar câncer de pele. Além disso, a radiação UVB afeta diretamente as bases pirimidínicas das moléculas de DNA, aumentando sua produção e favorecendo processos mutagênicos, produzindo novas células tumorigênicas também. Entre os filtros solares químicos conhecidos estão as benzofenonas e os cinamatos. O objetivo deste trabalho foi sintetizar pró-fármacos derivados de filtros solares químicos baseados nas estruturas das benzofenonas ligadas à derivados do ácido cinâmico, com propriedades antioxidantes para, desta maneira, obter um composto que prevenisse a carcinogênese cutânea por diferentes vertentes. Foram obtidos dois compostos, os quais foram caracterizados estruturalmente por Ressonância Magnética Nuclear de Hidrogênio e sua capacidade fotoprotetora através do método Optometrics, indicando atividade promissora.

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This work is consideration of an analysis of second-order (nonlinear analysis) applied to e metal towers and flares. The analysis is mainly done using the wind efforts and the weight of the structure. The analysis itself is carried out with the aid of a structural analysis software, SAP2000 where two proposes modeling. The first for the linear effects and the second for the nonlinear effects

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A radiação ultravioleta emitida pela radiação solar pode causar sérios danos à pele humana, sendo essa estratificada em três regiões do espectro de luz: UVA (315-400nm), UVB (280-315nm) e UVC (200-280nm). A incidência da radiação UVA sobre a pele induz a formação de espécies reativas de oxigênio (EROS), afetando indiretamente o DNA humano, podendo provocar câncer de pele. Além disso, a radiação UVB afeta diretamente as bases pirimidínicas das moléculas de DNA, aumentando sua produção e favorecendo processos mutagênicos, produzindo novas células tumorigênicas também. Entre os filtros solares químicos conhecidos estão as benzofenonas e os cinamatos. O objetivo deste trabalho foi sintetizar pró-fármacos derivados de filtros solares químicos baseados nas estruturas das benzofenonas ligadas à derivados do ácido cinâmico, com propriedades antioxidantes para, desta maneira, obter um composto que prevenisse a carcinogênese cutânea por diferentes vertentes. Foram obtidos dois compostos, os quais foram caracterizados estruturalmente por Ressonância Magnética Nuclear de Hidrogênio e sua capacidade fotoprotetora através do método Optometrics, indicando atividade promissora.

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This work is consideration of an analysis of second-order (nonlinear analysis) applied to e metal towers and flares. The analysis is mainly done using the wind efforts and the weight of the structure. The analysis itself is carried out with the aid of a structural analysis software, SAP2000 where two proposes modeling. The first for the linear effects and the second for the nonlinear effects

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Context. The ESO public survey VISTA variables in the Via Lactea (VVV) started in 2010. VVV targets 562 sq. deg in the Galactic bulge and an adjacent plane region and is expected to run for about five years. Aims. We describe the progress of the survey observations in the first observing season, the observing strategy, and quality of the data obtained. Methods. The observations are carried out on the 4-m VISTA telescope in the ZYJHK(s) filters. In addition to the multi-band imaging the variability monitoring campaign in the K-s filter has started. Data reduction is carried out using the pipeline at the Cambridge Astronomical Survey Unit. The photometric and astrometric calibration is performed via the numerous 2MASS sources observed in each pointing. Results. The first data release contains the aperture photometry and astrometric catalogues for 348 individual pointings in the ZYJHK(s) filters taken in the 2010 observing season. The typical image quality is similar to 0 ''.9-1 ''.0. The stringent photometric and image quality requirements of the survey are satisfied in 100% of the JHK(s) images in the disk area and 90% of the JHK(s) images in the bulge area. The completeness in the Z and Y images is 84% in the disk, and 40% in the bulge. The first season catalogues contain 1.28 x 10(8) stellar sources in the bulge and 1.68 x 10(8) in the disk area detected in at least one of the photometric bands. The combined, multi-band catalogues contain more than 1.63 x 10(8) stellar sources. About 10% of these are double detections because of overlapping adjacent pointings. These overlapping multiple detections are used to characterise the quality of the data. The images in the JHK(s) bands extend typically similar to 4 mag deeper than 2MASS. The magnitude limit and photometric quality depend strongly on crowding in the inner Galactic regions. The astrometry for K-s = 15-18 mag has rms similar to 35-175 mas. Conclusions. The VVV Survey data products offer a unique dataset to map the stellar populations in the Galactic bulge and the adjacent plane and provide an exciting new tool for the study of the structure, content, and star-formation history of our Galaxy, as well as for investigations of the newly discovered star clusters, star-forming regions in the disk, high proper motion stars, asteroids, planetary nebulae, and other interesting objects.