USE OF SOLAR ENERGY IN THE TREATMENT OF WATER CONTAMINATED WITH PHENOL BY PHOTOCHEMICAL PROCESSES

The solar driven photo-Fenton process for treating water containing phenol as a contaminant has been evaluated by means of pilot-scale experiments with a parabolic trough solar reactor (PTR). The effects of Fe(II) (0.04-1.0 mmol L(-1)), H(2)O(2) (7-270 mmol L(-1)), initial phenol concentration (100 and 500 mg C L(-1)), solar radiation, and operation mode (batch and fed-batch) on the process efficiency were investigated. More than 90% of the dissolved organic carbon (DOC) was removed within 3 hours of irradiation or less, a performance equivalent to that of artificially-irradiated reactors, indicating that solar light can be used either as an effective complementary or as an alternative source of photons for the photo-Fenton degradation process. A non-linear multivariable model based on a neural network was fit to the experimental results of batch-mode experiments in order to evaluate the relative importance of the process variables considered on the DOC removal over the reaction time. This included solar radiation, which is not a controlled variable. The observed behavior of the system in batch-mode was compared with fed-batch experiments carried out under similar conditions. The main contribution of the study consists of the results from experiments under different conditions and the discussion of the system behavior. Both constitute important information for the design and scale-up of solar radiation-based photodegradation processes.

Estimating hourly net radiation for leaf wetness duration using the Penman-Monteith equation

Leaf wetness duration (LWD) is related to plant disease occurrence and is therefore a key parameter in agrometeorology. As LWD is seldom measured at standard weather stations, it must be estimated in order to ensure the effectiveness of warning systems and the scheduling of chemical disease control. Among the models used to estimate LWD, those that use physical principles of dew formation and dew and/or rain evaporation have shown good portability and sufficiently accurate results for operational use. However, the requirement of net radiation (Rn) is a disadvantage foroperational physical models, since this variable is usually not measured over crops or even at standard weather stations. With the objective of proposing a solution for this problem, this study has evaluated the ability of four models to estimate hourly Rn and their impact on LWD estimates using a Penman-Monteith approach. A field experiment was carried out in Elora, Ontario, Canada, with measurements of LWD, Rn and other meteorological variables over mowed turfgrass for a 58 day period during the growing season of 2003. Four models for estimating hourly Rn based on different combinations of incoming solar radiation (Rg), airtemperature (T), relative humidity (RH), cloud cover (CC) and cloud height (CH), were evaluated. Measured and estimated hourly Rn values were applied in a Penman-Monteith model to estimate LWD. Correlating measured and estimated Rn, we observed that all models performed well in terms of estimating hourly Rn. However, when cloud data were used the models overestimated positive Rn and underestimated negative Rn. When only Rg and T were used to estimate hourly Rn, the model underestimated positive Rn and no tendency was observed for negative Rn. The best performance was obtained with Model I, which presented, in general, the smallest mean absolute error (MAE) and the highest C-index. When measured LWD was compared to the Penman-Monteith LWD, calculated with measured and estimated Rn, few differences were observed. Both precision and accuracy were high, with the slopes of the relationships ranging from 0.96 to 1.02 and R-2 from 0.85 to 0.92, resulting in C-indices between 0.87 and 0.93. The LWD mean absolute errors associated with Rn estimates were between 1.0 and 1.5h, which is sufficient for use in plant disease management schemes.

Alterações microclimáticas causadas pelo uso de tela plástica

Com o objetivo de caracterizar as alterações microclimáticas provocadas pelo uso de tela plástica na agricultura, foi desenvolvido um experimento com alface, em área de cultivo agrícola, em Alegre - ES (latitude 20º45 S, longitude 41º28 W e altitude 150 m), no período de setembro a dezembro de 1996. Foram utilizados sombreamentos de 0; 30; 50, e 70%, segundo especificação comercial. Os resultados mostraram que a tela com especificação comercial de 50% de sombreamento provocou uma atenuação média de 41% na radiação solar global, ocorrendo, no entanto, uma flutuação significativa ao longo do dia em função do movimento aparente do sol. A cobertura com a tela plástica não provocou alterações significativas da temperatura e umidade relativa do ar. Em relação à temperatura do solo, foi possível verificar uma atenuação com o aumento do sombreamento.

Estudo morfofisiológico e anatômico de dois genótipos de cacaueiro (Theobroma cacao L.) submetidos a diferentes condições de radiação solar

A luminosidade desponta como um dos fatores abióticos de maior importância no estabelecimento das plantas, podendo ocasionar alterações a nível fisiológico e anatômico, interferindo diretamente no desenvolvimento das mesmas e consequentemente, sua produtividade. O cacaueiro (Theobroma cacao – Malvaceae) possui grande interesse econômico devido à utilização de suas sementes para produção de manteiga de cacau e chocolate. Neste sentido, o objetivo deste trabalho foi comparar características fisiológicas e anatômicas de dois genótipos de cacaueiro (PH 16 e IPIRANGA 01), submetidos a diferentes condições de radiação solar de modo a inferir a respeito das condições de luminosidade mais favoráveis ao desenvolvimento dos mesmos. Foram realizadas análises de crescimento, teor de pigmentos, trocas gasosas e anatômicas caulinares e foliares. O delineamento experimental foi em Blocos casualizados (DBC), com 4 repetições em arranjo fatorial 2 x 5, constituído de dois genótipos e 5 níveis de luminosidade (0% - pleno sol -, 18%, 30%, 50% e 80% de sombreamento), totalizando 40 parcelas com 10 plantas cada. Os dados obtidos foram submetidos à análise de variância e regressão. Os resultados de crescimento indicam maior adaptação, de ambos os genótipos, em condições de irradiância alta a moderada. O índice de qualidade de Dickson demonstrou maior capacidade de sobrevivência em condições de campo a níveis altos de irradiância para o genótipo PH 16 e a níveis de irradiância moderada para IPIRANGA 01. Os teores de pigmentos fotossintetizantes de IPIRANGA 01 mostram-se mais elevados na condição de 30% de sombreamento, enquanto que, para PH 16 os maiores teores foram observados em 50% de sombreamento. Ambos os genótipos demonstraram altas taxas de A, Ci, E, A/E, A/Gs e A/Ci, sob elevadas irradiâncias, assim como adaptações anatômicas caulinares e foliares a maiores luminosidades, tais como, maior espessamento do limbo foliar, parênquima paliçádico, esponjoso, limbo foliar, epiderme adaxial e densidade estomática, além de maior densidade e frequência de elementos de vaso e espessura do xilema secundário. Os genótipos PH 16 e IPIRANGA 01 apresentaram uma grande plasticidade em relação aos diferentes níveis de irradiância, no entanto, constatou-se que PH 16 apresentou melhor desempenho sob condições de alta irradiância, como as obtidas nos tratamentos a pleno sol e 18% de sombreamento, enquanto que, IPIRANGA 01 mostrou-se mais adaptado sob sombreamento moderado, a 30% de sombra.

Torre solar: estudo do rendimento e viabilidade de centrais térmicas solares para produção de energia eléctrica de pequena e média dimensão

O aproveitamento da radiação solar representa um recurso energético extremamente benéfico, quer no âmbito energético, quer no ambiental, contribuindo para a redução das emissões de gases nocivos para a atmosfera. Portugal apresenta uma radiação solar total média anual bastante elevada, colocando-se entre um dos países que apresentam melhores potencialidades para o aproveitamento da energia solar. A torre solar consiste numa estufa com uma determinada extensão com uma chaminé no seu centro e o seu funcionamento baseia-se no aquecimento do ar que circula por baixo da estufa, sendo expelido pela chaminé. Nesta tese é abordado o tema da torre solar e os princípios físicos inerentes ao seu funcionamento. Foi estudado e descrito o método de cálculo de diversos parâmetros e resultados associados ao funcionamento da torre solar. Elaborou-se uma folha de cálculo para obtenção dos valores de simulações de torres com diversas dimensões, tecendo-se conclusões quanto aos resultados e às variações dos mesmos, consoante as alterações de dimensão dos elementos que a constituem. Foram descritos os vários elementos que constituem uma torre solar, bem como as suas características e tipologias. Efectuou-se um estudo com aplicação a um caso real, para se tecer algumas conclusões e comentários relativamente à viabilidade de uma torre solar para a situação em causa. Por fim, com base em todo o trabalho desenvolvido e abordado, foi possível tecer-se algumas conclusões quanto à viabilidade das torres solares.

Planeamento de curto prazo de sistemas de energia solar usando técnicas de otimização robusta

Dissertação para obtenção do grau de Mestre em Engenharia Electrotécnica

Otimização estocástica para a exploração de centrais de concentração solar considerando incerteza e risco

Dissertação para obtenção do grau de Mestre em Engenharia Eletrotécnica

Desenvolvimento de um concentrador solar com sistema de seguimento

Dissertação de mestrado em Engenharia Mecânica

Seguidor do ponto de máxima potência multi-conversor para sistemas solares fotovoltaicos

Dissertação de mestrado integrado em Engenharia Eletrónica Industrial e de Computadores

Desenvolvimento de microcápsulas ativadas por radiação solar para aplicação em painéis cerâmicos exteriores

Dissertação de mestrado integrado em Engenharia de Materiais

Desenvolvimento de materiais para isolamento térmico com base em biomimética

Dissertação de mestrado Internacional em Sustentabilidade do Ambiente Construído

Radiação solar em superfieies horizontal e vertical com exposição norte

In the field of agrometeorological studies we are in need of the estimation of the solar radiation frequently. At the present study the authors have worked out some dat:t regarding the hours of sunshine during the months of August, September, October, November, December and January of 1957, 1958 and 1959. Based on such hours of sunshine in the Agrometeorological Station, located at the Escola Superior de Agricultura "Luiz de Queiroz" - U.S. P., in Piracicaba, the authors calculated the solar radiation received on a plane and horizontal surface, from the method proposed by Glover and Mc Culloch. With those results the authors estimated the percentual part of radiation that would be received on vertical wall facing north.

Identifying genetic signatures of selection in a non-model species, alpine gentian (Gentiana nivalis L.), using a landscape genetic approach

It is generally accepted that most plant populations are locally adapted. Yet, understanding how environmental forces give rise to adaptive genetic variation is a challenge in conservation genetics and crucial to the preservation of species under rapidly changing climatic conditions. Environmental variation, phylogeographic history, and population demographic processes all contribute to spatially structured genetic variation, however few current models attempt to separate these confounding effects. To illustrate the benefits of using a spatially-explicit model for identifying potentially adaptive loci, we compared outlier locus detection methods with a recently-developed landscape genetic approach. We analyzed 157 loci from samples of the alpine herb Gentiana nivalis collected across the European Alps. Principle coordinates of neighbor matrices (PCNM), eigenvectors that quantify multi-scale spatial variation present in a data set, were incorporated into a landscape genetic approach relating AFLP frequencies with 23 environmental variables. Four major findings emerged. 1) Fifteen loci were significantly correlated with at least one predictor variable (R (adj) (2) > 0.5). 2) Models including PCNM variables identified eight more potentially adaptive loci than models run without spatial variables. 3) When compared to outlier detection methods, the landscape genetic approach detected four of the same loci plus 11 additional loci. 4) Temperature, precipitation, and solar radiation were the three major environmental factors driving potentially adaptive genetic variation in G. nivalis. Techniques presented in this paper offer an efficient method for identifying potentially adaptive genetic variation and associated environmental forces of selection, providing an important step forward for the conservation of non-model species under global change.

Melanin-based colour polymorphism responding to climate change.

Climate warming leads to a decrease in biodiversity. Organisms can deal with the new prevailing environmental conditions by one of two main routes, namely evolving new genetic adaptations or through phenotypic plasticity to modify behaviour and physiology. Melanin-based colouration has important functions in animals including a role in camouflage and thermoregulation, protection against UV-radiation and pathogens and, furthermore, genes involved in melanogenesis can pleiotropically regulate behaviour and physiology. In this article, I review the current evidence that differently coloured individuals are differentially sensitive to climate change. Predicting which of dark or pale colour variants (or morphs) will be more penalized by climate change will depend on the adaptive function of melanism in each species as well as how the degree of colouration covaries with behaviour and physiology. For instance, because climate change leads to a rise in temperature and UV-radiation and dark colouration plays a role in UV-protection, dark individuals may be less affected from global warming, if this phenomenon implies more solar radiation particularly in habitats of pale individuals. In contrast, as desertification increases, pale colouration may expand in those regions, whereas dark colourations may expand in regions where humidity is predicted to increase. Dark colouration may be also indirectly selected by climate warming because genes involved in the production of melanin pigments confer resistance to a number of stressful factors including those associated with climate warming. Furthermore, darker melanic individuals are commonly more aggressive than paler conspecifics, and hence they may better cope with competitive interactions due to invading species that expand their range in northern latitudes and at higher altitudes. To conclude, melanin may be a major component involved in adaptation to climate warming, and hence in animal populations melanin-based colouration is likely to change as an evolutionary or plastic response to climate warming.

Empirical studies of cloud effects on UV radiation: A review

The interest in solar ultraviolet (UV) radiation from the scientific community and the general population has risen significantly in recent years because of the link between increased UV levels at the Earth's surface and depletion of ozone in the stratosphere. As a consequence of recent research, UV radiation climatologies have been developed, and effects of some atmospheric constituents (such as ozone or aerosols) have been studied broadly. Correspondingly, there are well-established relationships between, for example, total ozone column and UV radiation levels at the Earth's surface. Effects of clouds, however, are not so well described, given the intrinsic difficulties in properly describing cloud characteristics. Nevertheless, the effect of clouds cannot be neglected, and the variability that clouds induce on UV radiation is particularly significant when short timescales are involved. In this review we show, summarize, and compare several works that deal with the effect of clouds on UV radiation. Specifically, works reviewed here approach the issue from the empirical point of view: Some relationship between measured UV radiation in cloudy conditions and cloud-related information is given in each work. Basically, there are two groups of methods: techniques that are based on observations of cloudiness (either from human observers or by using devices such as sky cameras) and techniques that use measurements of broadband solar radiation as a surrogate for cloud observations. Some techniques combine both types of information. Comparison of results from different works is addressed through using the cloud modification factor (CMF) defined as the ratio between measured UV radiation in a cloudy sky and calculated radiation for a cloudless sky. Typical CMF values for overcast skies range from 0.3 to 0.7, depending both on cloud type and characteristics. Despite this large dispersion of values corresponding to the same cloud cover, it is clear that the cloud effect on UV radiation is 15–45% lower than the cloud effect on total solar radiation. The cloud effect is usually a reducing effect, but a significant number of works report an enhancement effect (that is increased UV radiation levels at the surface) due to the presence of clouds. The review concludes with some recommendations for future studies aimed to further analyze the cloud effects on UV radiation