Aplicação dos Sistemas de Informação Geográfica nas Energias Renováveis: o Potencial da Energia Solar na Ilha de São Vicente – Cabo Verde

A presente dissertação, tem como foco principal a aplicação dos Sistemas de Informação Geográfica (SIG) ao estudo das energias renováveis, tendo como caso avaliar o potencial solar na ilha de São Vicente do arquipélago de Cabo Verde. A energia do sol é a principal fonte de energia renovável, e está disponível em quase todas as regiões do planeta. Quantificar o potencial energético solar de um lugar ou região é indispensável, para avaliar as potencialidades de produção de energia fotovoltaica. Outro fator importante prende-se com ordenamento territorial associado à exploração desses recursos energéticos, pelo que devem ser avaliadas as condições técnicas, ambientais e económicas, quando se pretende instalar parques para a produção de energia fotovoltaica. Assim, neste trabalho foram aplicadas as ferramentas SIG, para quantificar a radiação solar mensal e anual da ilha de São Vicente, arquipélago de Cabo Verde, através do modelo Solar Analyst. Numa segunda fase, aplicou-se a técnica de análise multicritério em combinação com os SIGs para definir as áreas mais favoráveis para a instalação de parques de produção de energia elétrica a partir da energia solar. Para o cálculo da radiação solar na ilha de São de Vicente, utilizou-se o modelo digital de terreno (MDT) e a latitude da ilha como parâmetros de entrada ao modelo. Para a análise multicritério definiram-se um conjunto de critérios que devem ser considerados na implementação de parques solares, nomeadamente, a disponibilidade de radiação solar existente na área, a distância à rede de transporte de energia elétrica e à rede viária, o declive do terreno, o uso e ocupação do solo e a proximidade às linhas de água. Para auxiliar na atribuição dos pesos aos critérios utilizados na análise aplicou-se a método Analytic Hierarchy Process (AHP). As áreas resultantes do processo da análise multicritério, foram confrontadas com a Carta de Condicionantes do esquema regional de ordenamento da ilha de São Vicente, aferindo a conformidade das propostas e reajustes subsequentes, de modo a obter os resultados finais.

Aplicação dos Sistemas de Informação Geográfica nas energias renováveis: o potencial da energia solar na ilha de São Vicente – Cabo Verde

Informação Geográfica (SIG) ao estudo das energias renováveis, tendo como caso avaliar o potencial solar na ilha de São Vicente do arquipélago de Cabo Verde. A energia do sol é a principal fonte de energia renovável, e está disponível em quase todas as regiões do planeta. Quantificar o potencial energético solar de um lugar ou região é indispensável, para avaliar as potencialidades de produção de energia fotovoltaica. Outro fator importante prende-se com ordenamento territorial associado à exploração desses recursos energéticos, pelo que devem ser avaliadas as condições técnicas, ambientais e económicas, quando se pretende instalar parques para a produção de energia fotovoltaica. Assim, neste trabalho foram aplicadas as ferramentas SIG, para quantificar a radiação solar mensal e anual da ilha de São Vicente, arquipélago de Cabo Verde, através do modelo Solar Analyst. Numa segunda fase, aplicou-se a técnica de análise multicritério em combinação com os SIGs para definir as áreas mais favoráveis para a instalação de parques de produção de energia elétrica a partir da energia solar. Para o cálculo da radiação solar na ilha de São de Vicente, utilizou-se o modelo digital de terreno (MDT) e a latitude da ilha como parâmetros de entrada ao modelo. Para a análise multicritério definiram-se um conjunto de critérios que devem ser considerados na implementação de parques solares, nomeadamente, a disponibilidade de radiação solar existente na área, a distância à rede de transporte de energia elétrica e à rede viária, o declive do terreno, o uso e ocupação do solo e a proximidade às linhas de água. Para auxiliar na atribuição dos pesos aos critérios utilizados na análise aplicou-se a método Analytic Hierarchy Process (AHP). As áreas resultantes do processo da análise multicritério, foram confrontadas com a Carta de Condicionantes do esquema regional de ordenamento da ilha de São Vicente, aferindo a conformidade das propostas e reajustes subsequentes, de modo a obter os resultados finais.

Análise de pavimentos de parques infantis feitos com granulados de pneus usados: avaliação do potencial risco para a saúde das crianças

Dissertação apresentada na Faculdade de Ciências e Tecnologia da Universidade Nova de Lisboa para obtenção do grau de Mestre em Engenharia do Ambiente, Perfil Engenharia Sanitária

SIG y Visor Web de energía solar y eólica. Aplicación práctica en el País Vasco.

El proyecto es un Sistema de Información Geográfica y Visor web centrado en las energías renovables solar y eólica, contiene funcionalidad dirigida a facilitar elacceso de los ciudadanos y de las empresas del sector a la información de estas dos energías. Incorpora una herramienta de edición que pretende tener una base de datos actualizada de los parques solares y eólicos de España. Otra orientada al entorno urbano que permite saber la electricidad aproximada que se generaría en la cubierta de un edificio de Vitoria en función del panel solar que se instale en dicha cubierta. También se ha realizado un análisis espacial para encontrar los lugares óptimos para la instalación de paneles solares y eólicos en el País Vasco, se han publicado las capas resultado en el visor para que puedan acceder a ellas cualquier sociedad o empresa que le interese conocer este tipo de información. Para estos análisis se han tenido en cuenta estudios de diferentes universidades e informes de organizaciones como Greenpeace. No obstante, no deja de ser una propuesta objeto de posibles mejoras.

Aerodinámica experimental de elementos de parques energéticos

La creciente demanda de energía eléctrica y la necesidad de implementar energías no contaminantes hace que las llamadas tecnologías verdes sean cada día más solicitadas. Entre estas tecnologías encontramos la energía solar y la energía eólica; ambas tienen una trayectoria de uso e investigación bastante amplia, sin embargo aún presentan problemas de fondo que impiden dar mayor impulso a su uso. El objetivo de la presente tesis es presentar soluciones a problemas de optimización en campos conversores de energía. Para ello se analizan y resuelven dos problemas por medio de técnicas de aerodinámica experimental: el primero sobre campos de colectores solares y el segundo sobre campos eólicos. Las técnicas de medición utilizadas en aerodinámica, y en el presente trabajo, son: medición de cargas, anemometría de hilo caliente, velocimetría por imagen de partículas y escaneo de presiones; además de un análisis estadístico de los datos. En el primer caso se ensayan experimentalmente colectores solares parabólicos en donde, por cuestiones de seguridad o por protección contra el viento, se utilizan cercas. Éstas modifican el comportamiento del flujo corriente abajo y se ha encontrado que la distancia a la cual se colocan, así como el tipo de cercas (sólida o permeable), modifican las cargas estructurales a las que los colectores están expuestos. Los resultados demuestran que existe una distancia crítica en la cual la presencia de la cerca aumenta la carga en lugar de disminuirla, por lo cual la selección adecuada del parapeto y la distancia a la cual se coloca son de suma importancia para la optimización de la estructura. En el segundo caso se ensaya experimentalmente y simula numéricamente la estela de turbinas eólicas por medio de discos porosos. En donde un disco permeable simula el rotor de una turbina. El disco es capaz de semejar la estela y los efectos que ésta puede causar corriente abajo. Los resultados muestran que seleccionando adecuadamente la porosidad, es posible simular coeficientes de empuje similares a los desarrollados por los aerogeneradores, además la estela y sus efectos son semejantes a los medidos en campo. ABSTRACT The called green energy technologies are increasingly required because of the growing demand for electricity and the need to implement nonpolluting energy. Among the green energy technologies it is found the solar and the wind energy, both have a history of use and fairly extensive research; however they still have problems which limit to give them further impetus to its use. The aim of this thesis is to present solutions to optimization problems in energy harvesting. To this end it is analysed, and solved, two problems by means of techniques in experimental aerodynamics: the first issue with regard to parabolic troughs and the second about wind farms. The measurement techniques commonly used in aerodynamics, and used in this research work, are: measurement of loads, hot wire anemometry, particle image velocimetry and scanning of pressures; where data are collected and then an statistical analysis is done. In the first case it is tested parabolic troughs where, either for security reasons or protection against the wind actions, fences are used. These fences modify the behaviour of flow downstream and it was found that the distance at which they are placed, and the type of fences (solid or permeable) modify the structural loads to which the parabolic troughs are exposed. The results show that there is a critical distance at which the presence of the fence increases the load instead of protecting the parabolic trough, hence making the proper selection of the parapet and the distance at which it stands are paramount for the optimization of the structure. In the second case it is tested, experimentally and numerically, the wake of wind turbines by means of porous disks; where the permeable disc simulates a turbine rotor. The disc is able to mimic the wake and the effects that it can cause downstream. The results show that by properly selecting the porosity, it is possible to simulate drag coefficients similar to those developed by wind turbines; moreover the porous disk wake and its effects are similar to those measured on field.

Propuesta para la iluminación adecuada con energías renovables en parques de deportes urbanos y nuevas tendencias (DUNT)

74 p.

Remediation Of 17-α-ethinylestradiol Aqueous Solution By Photocatalysis And Electrochemically-assisted Photocatalysis Using Tio2 And Tio2/wo3 Electrodes Irradiated By A Solar Simulator.

TiO2 and TiO2/WO3 electrodes, irradiated by a solar simulator in configurations for heterogeneous photocatalysis (HP) and electrochemically-assisted HP (EHP), were used to remediate aqueous solutions containing 10 mg L(-1) (34 μmol L(-1)) of 17-α-ethinylestradiol (EE2), active component of most oral contraceptives. The photocatalysts consisted of 4.5 μm thick porous films of TiO2 and TiO2/WO3 (molar ratio W/Ti of 12%) deposited on transparent electrodes from aqueous suspensions of TiO2 particles and WO3 precursors, followed by thermal treatment at 450 (°)C. First, an energy diagram was organized with photoelectrochemical and UV-Vis absorption spectroscopy data and revealed that EE2 could be directly oxidized by the photogenerated holes at the semiconductor surfaces, considering the relative HOMO level for EE2 and the semiconductor valence band edges. Also, for the irradiated hybrid photocatalyst, electrons in TiO2 should be transferred to WO3 conduction band, while holes move toward TiO2 valence band, improving charge separation. The remediated EE2 solutions were analyzed by fluorescence, HPLC and total organic carbon measurements. As expected from the energy diagram, both photocatalysts promoted the EE2 oxidation in HP configuration; after 4 h, the EE2 concentration decayed to 6.2 mg L(-1) (35% of EE2 removal) with irradiated TiO2 while TiO2/WO3 electrode resulted in 45% EE2 removal. A higher performance was achieved in EHP systems, when a Pt wire was introduced as a counter-electrode and the photoelectrodes were biased at +0.7 V; then, the EE2 removal corresponded to 48 and 54% for the TiO2 and TiO2/WO3, respectively. The hybrid TiO2/WO3, when compared to TiO2 electrode, exhibited enhanced sunlight harvesting and improved separation of photogenerated charge carriers, resulting in higher performance for removing this contaminant of emerging concern from aqueous solution.

Recreação, lazer e educação física na cidade de Campinas : um olhar acerca dos parques e recantos infantis (1940-1960)

Universidade Estadual de Campinas . Faculdade de Educação Física

Parques publicos de Curitiba

Universidade Estadual de Campinas. Faculdade de Educação Física

Dosimetria esporular: Bacillus subtilis TKJ6312 como biossensor de radiação solar biologicamente ativa

Since 2000, spore dosimetry and spectral photometry have been performed in parallel at the Southern Space Observatory, São Martinho da Serra (Southern Brazil). A comparative study involving data from Punta Arenas - Chile (53.2º S), São Martinho da Serra (29.5º S), Padang - Indonesia (0.9ºS), Brussels - Belgium (50.9º N) and Kiyotake - Japan (31.9º N) from 2000 to 2006 is presented. The Spore Inactivation Doses presented the higher values in summer (973 ± 73 for Punta Arenas and 4,369 ± 202 for São Martinho da Serra, as well 1,402 ± 170 and 3,400 ± 1,674 for Brussels and Kiyotake, respectively). The simplicity, robustness and high resistance of bacterial spores makes the biosensor an potential biological tool for UV-B monitoring.

Turbulent magnetic pumping in a Babcock-Leighton solar dynamo model

Context. The turbulent pumping effect corresponds to the transport of magnetic flux due to the presence of density and turbulence gradients in convectively unstable layers. In the induction equation it appears as an advective term and for this reason it is expected to be important in the solar and stellar dynamo processes. Aims. We explore the effects of turbulent pumping in a flux-dominated Babcock-Leighton solar dynamo model with a solar-like rotation law. Methods. As a first step, only vertical pumping has been considered through the inclusion of a radial diamagnetic term in the induction equation. In the second step, a latitudinal pumping term was included and then, a near-surface shear was included. Results. The results reveal the importance of the pumping mechanism in solving current limitations in mean field dynamo modeling, such as the storage of the magnetic flux and the latitudinal distribution of the sunspots. If a meridional flow is assumed to be present only in the upper part of the convective zone, it is the full turbulent pumping that regulates both the period of the solar cycle and the latitudinal distribution of the sunspot activity. In models that consider shear near the surface, a second shell of toroidal field is generated above r = 0.95 R(circle dot) at all latitudes. If the full pumping is also included, the polar toroidal fields are efficiently advected inwards, and the toroidal magnetic activity survives only at the observed latitudes near the equator. With regard to the parity of the magnetic field, only models that combine turbulent pumping with near-surface shear always converge to the dipolar parity. Conclusions. This result suggests that, under the Babcock-Leighton approach, the equartorward motion of the observed magnetic activity is governed by the latitudinal pumping of the toroidal magnetic field rather than by a large scale coherent meridional flow. Our results support the idea that the parity problem is related to the quadrupolar imprint of the meridional flow on the poloidal component of the magnetic field and the turbulent pumping positively contributes to wash out this imprint.

New constraints on the chemical evolution of the solar neighbourhood and Galactic disc(s) Improved astrophysical parameters for the Geneva-Copenhagen Survey

We present a re-analysis of the Geneva-Copenhagen survey, which benefits from the infrared flux method to improve the accuracy of the derived stellar effective temperatures and uses the latter to build a consistent and improved metallicity scale. Metallicities are calibrated on high-resolution spectroscopy and checked against four open clusters and a moving group, showing excellent consistency. The new temperature and metallicity scales provide a better match to theoretical isochrones, which are used for a Bayesian analysis of stellar ages. With respect to previous analyses, our stars are on average 100 K hotter and 0.1 dex more metal rich, which shift the peak of the metallicity distribution function around the solar value. From Stromgren photometry we are able to derive for the first time a proxy for [alpha/Fe] abundances, which enables us to perform a tentative dissection of the chemical thin and thick disc. We find evidence for the latter being composed of an old, mildly but systematically alpha-enhanced population that extends to super solar metallicities, in agreement with spectroscopic studies. Our revision offers the largest existing kinematically unbiased sample of the solar neighbourhood that contains full information on kinematics, metallicities, and ages and thus provides better constraints on the physical processes relevant in the build-up of the Milky Way disc, enabling a better understanding of the Sun in a Galactic context.

The radius and mass of the close solar twin 18 Scorpii derived from asteroseismology and interferometry

The growing interest in solar twins is motivated by the possibility of comparing them directly to the Sun. To carry on this kind of analysis, we need to know their physical characteristics with precision. Our first objective is to use asteroseismology and interferometry on the brightest of them: 18 Sco. We observed the star during 12 nights with HARPS for seismology and used the PAVO beam-combiner at CHARA for interferometry. An average large frequency separation 134.4+/-0.3 mu Hz and angular and linear radiuses of 0.6759 +/- 0.0062 mas and 1.010 +/- 0.009 R(circle dot) were estimated. We used these values to derive the mass of the star, 1.02 +/- 0.03 M(circle dot).

Solar twins in M 67: evolutionary status and lithium abundance

Aims. We determine the age and mass of the three best solar twin candidates in open cluster M 67 through lithium evolutionary models. Methods. We computed a grid of evolutionary models with non-standard mixing at metallicity [Fe/H] = 0.01 with the Toulouse-Geneva evolution code for a range of stellar masses. We estimated the mass and age of 10 solar analogs belonging to the open cluster M 67. We made a detailed study of the three solar twins of the sample, YPB637, YPB1194, and YPB1787. Results. We obtained a very accurate estimation of the mass of our solar analogs in M 67 by interpolating in the grid of evolutionary models. The three solar twins allowed us to estimate the age of the open cluster, which is 3.87(-0.66)(+0.55) Gyr, which is better constrained than former estimates. Conclusions. Our results show that the 3 solar twin candidates have one solar mass within the errors and that M 67 has a solar age within the errors, validating its use as a solar proxy. M 67 is an important cluster when searching for solar twins.

Transiting exoplanets from the CoRoT space mission XIII. CoRoT-13b: a dense hot Jupiter in transit around a star with solar metallicity and super-solar lithium content

We announce the discovery of the transiting planet CoRoT-13b. Ground-based follow-up in CFHT and IAC80 confirmed CoRoT's observations. The mass of the planet was measured with the HARPS spectrograph and the properties of the host star were obtained analyzing HIRES spectra from the Keck telescope. It is a hot Jupiter-like planet with an orbital period of 4.04 days, 1.3 Jupiter masses, 0.9 Jupiter radii, and a density of 2.34 g cm(-3). It orbits a G0V star with T(eff) = 5 945 K, M(*) = 1.09 M(circle dot), R(*) = 1.01 R(circle dot), solar metallicity, a lithium content of +1.45 dex, and an estimated age of between 0.12 and 3.15 Gyr. The lithium abundance of the star is consistent with its effective temperature, activity level, and age range derived from the stellar analysis. The density of the planet is extreme for its mass, implies that heavy elements are present with a mass of between about 140 and 300 M(circle plus).