Solar coronal magnetic fields derived using seismology techniques applied to omnipresent sunspot waves

Sunspots on the surface of the Sun are the observational signatures of intense manifestations of tightly packed magnetic field lines, with near-vertical field strengths exceeding 6,000 G in extreme cases1. It is well accepted that both the plasma density and the magnitude of the magnetic field strength decrease rapidly away from the solar surface, making high-cadence coronal measurements through traditional Zeeman and Hanle effects difficult as the observational signatures are fraught with low-amplitude signals that can become swamped with instrumental noise2, 3. Magneto-hydrodynamic (MHD) techniques have previously been applied to coronal structures, with single and spatially isolated magnetic field strengths estimated as 9–55 G (refs 4,5,6,7). A drawback with previous MHD approaches is that they rely on particular wave modes alongside the detectability of harmonic overtones. Here we show, for the first time, how omnipresent magneto-acoustic waves, originating from within the underlying sunspot and propagating radially outwards, allow the spatial variation of the local coronal magnetic field to be mapped with high precision. We find coronal magnetic field strengths of 32 ± 5 G above the sunspot, which decrease rapidly to values of approximately 1 G over a lateral distance of 7,000 km, consistent with previous isolated and unresolved estimations. Our results demonstrate a new, powerful technique that harnesses the omnipresent nature of sunspot oscillations to provide magnetic field mapping capabilities close to a magnetic source in the solar corona.

Ultraviolet emission lines of Si II in cool star and solar spectra

Recent atomic physics calculations for Si II are employed within the CLOUDY modelling code to analyse Hubble Space Telescope (HST) STIS ultraviolet spectra of three cool stars, β Geminorum, α Centauri A and B, as well as previously published HST/GHRS observations of α Tau, plus solar quiet Sun data from the High Resolution Telescope and Spectrograph. Discrepancies found previously between theory and observation for line intensity ratios involving the 3s²3p ²PJ-3s3p^{2 4}P^J' intercombination multiplet of Si II at ~ 2335 Å are significantly reduced, as are those for ratios containing the 3s²3p ²PJ-3s3p^{2 2}DJ ~ transitions at ~1816 Å. This is primarily due to the effect of the new Si II transition probabilities. However, these atomic data are not only very different from previous calculations, but also show large disagreements with measurements, specifically those of Calamai et al. for the intercombination lines. New measurements of transition probabilities for Si II are hence urgently required to confirm (or otherwise) the accuracy of the recently calculated values. If the new calculations are confirmed, then a long-standing discrepancy between theory and observation will have finally been resolved. However, if the older measurements are found to be correct, then the agreement between theory and observation is simply a coincidence and the existing discrepancies remain.

Chalcogenide thin films for solar cells: growth and properties

Thin film solar cells have in recent years gained market quota against traditional silicon photovoltaic panels. These developments were in a large part due to CdTe solar panels on whose development started earlier than their competitors. Panels based on Cu(In,Ga)Se2 (CIGS), despite being more efficient in a laboratory and industrial scale than the CdTe ones, still need a growth technology cheaper and easier to apply in industry. Although usually presented as a good candidate to make cheap panels, CIGS uses rare and expensive materials as In and Ga. The price evolution of these materials might jeopardize CIGS future. This thesis presents three different studies. The first is the study of different processes for the incorporation of Ga in a hybrid CIGS growth system. This system is based on sputtering and thermal evaporation. This technology is, in principle, easier to be applied in the industry and solar cells with efficiencies around to 7% were fully made in Aveiro. In the second part of this thesis, a new material to replace CIGS in thin film solar cells is studied. The growth conditions and fundamental properties of Cu2ZnSnSe4 (CZTSe) were studied in depth. Suitable conditions of temperature and pressure for the growth of this material are reported. Its band gap energy was estimated at 1.05 eV and the Raman scattering peaks were identified. Solar cells made with this material showed efficiencies lower than 0.1%. Finally, preliminary work regarding the incorporation of selenium in Cu2ZnSnS4 (CZTS) thin films was carried out. The structural and morphological properties of thin films of Cu2ZnSn(S,Se)4 have been studied and the results show that the incorporation of selenium is higher in films with precursors rather with already formed Cu2SnS3 or Cu2ZnSnS4 thin films. A solar cell with 0.9 % of efficiency was prepared.

Photoinactivation of viruses by porphyrins

A inativação fotodinâmica tem sido usada com sucesso na inativação de microorganismos. Diversos aspetos da inativação fotodinâmica foram já estudados para diferentes microrganismos, contudo, existe ainda pouca informação disponível no que diz respeito à inativação de bacteriófagos por processos fotodinâmicos. Este trabalho pretendeu elucidar e avaliar vários aspetos da fotoinativação de vírus, em particular de bacteriófagos, incluindo (i) o efeito de diversos parâmetros de luz utilizados na fotoinativação de bacteriófagos; (ii) a eficiência da inativação fotodinâmica de diferentes tipos de bacteriófagos (fagos do tipo DNA e RNA); (iii) o principal mecanismo através do qual a inativação fotodinâmica tem lugar; (iv) o efeito da fotoinativação nas proteínas do bacteriófago; e (v) o possível desenvolvimento de resistência e recuperação da viabilidade após vários tratamentos fotodinâmicos consecutivos. Para avaliar o efeito dos diferentes parâmetros de luz, suspensões fágicas com 107 UFP mL-1 foram irradiadas com diferentes fontes e doses de luz, intensidades luminosas e tempos de irradiação (30,90 e 270 min) na presença de 0,5; 1,0 e 5,0 μM dos derivados porfirínicos catiónicos Tri- Py+-Me-PF e Tetra-Py+-Me. A eficiência da fotoinativação de diferentes fagos do tipo DNA e RNA, foi avaliada através da irradiação da suspensão fágica com luz branca (40 W m-2) durante 270 min na presença de 0,5 e 5,0 μM do derivado porfirínico Tri-Py+-Me-PF, respetivamente para os fagos do tipo RNA e DNA. O mecanismo através do qual a fotoinativação de fagos de DNA (fago do tipo T4) e de RNA (fago Qb) tem lugar foi avaliado por exposição da suspensão fágica à luz branca com uma potência de 40 W m-2, na presença de fotossensibilizador (Tri-Py+-Me-PF e Tetra-Py+-Me) e inibidores, quer do oxigénio singuleto (azida de sódio e L-histidina) quer de radicais livres (Dmanitol e L-cisteína). Os danos nas proteínas do fago do tipo T4, induzidos pelas espécies reativas de oxigénio geradas por 5,0 μM Tri-Py+-Me-PF, foram avaliados pelo método convencional de SDS-PAGE e por espectroscopia de infravermelho. O possível desenvolvimento de resistência e recuperação da viabilidade após a inativação fotodinâmica dos bacteriófagos foi avaliado após dez ciclos consecutivos de tratamento fotodinâmico incompletos (120 min sob irradiação de luz branca a uma potência de 40 W m-2) na presença de 5,0 μM do derivado porfirínico Tri-Py+-Me-PF. Os resultados deste trabalho mostraram que (i) quando uma quantidade de energia (dose de luz) determinada foi aplicada numa suspensão fágica, a partir de uma mesma fonte irradiação, a fotoinactivação do fago foi tanto mais eficiente quanto mais baixa foi a potência luminosa aplicada; (ii) os bacteriófagos foram eficientemente inativados até ao limite de deteção (redução de 6-7 log); (ii) os fagos do tipo RNA foram inativados mais facilmente do que os fagos do tipo DNA (tempos de exposição mais curtos e com concentração de fotossensibilizador dez vezes menor do que a usada para inativar os fagos do tipo DNA); (iii) o mecanismo do tipo II (via produção de oxigénio singuleto) foi o principal mecanismo através do qual a fotoinativação dos bacteriófagos teve lugar; (iv) foi possível detectar danos no perfil proteico após tratamento fotodinâmico e a espectroscopia de infravermelho apresentou-se como uma metodologia promissora de screening para avaliação dos danos induzidos pela inativação fotodinâmica em proteínas; e (v) após dez ciclos consecutivos de tratamento fotodinâmico, o fago do tipo T4 não revelou nenhum tipo de resistência ao tratamento fotodinâmico nem recuperou a sua viabilidade. Como conclusão, a inativação fotodinâmica microbiana é uma tecnologia bastante eficaz para a fotoinativação de bacteriófagos do tipo DNA e RNA sem invólucro, a qual pode ser considerada como uma alternativa ao tratamento convencional com agentes antivíricos, mesmo com intensidades luminosas baixas, sem o risco associado de desenvolvimento de mecanismos de resistência.

Photodegradation of sertraline by solar radiation and influencing factors

Photodegradation is considered to be one of the most important processes of elimination of pharmaceutical drugs from natural water matrices. The high consumption and discharge of these substances, in particular antidepressants, to the aquatic environment supports the need to study degradation processes. This dissertation aimed at studying the direct and indirect photodegradation of sertraline, an antidepressant known for its persistence in the environment, and the evaluation of the influence of environmentally relevant factors in its photodegradation. The photodegradation experiments were developed under simulated solar light and the irradiation times converted to summer sunny days (SSD), an equivalent time in natural environmental conditions. The direct photodegradation was evaluated in solutions of sertraline prepared in ultrapure water and the indirect photodegradation was studied through the addition of photosensitizers (humic substances, Fe(III), nitrates and oxygen). Further irradiation studies were perfomed in aqueous samples collected from two wastewater treatment plants, Vouga river and Ria de Aveiro. The samples were chemically characterized (dissolved organic carbon, nitrates and nitrites and iron determination and UV/Vis spectroscopy). The quantification of sertraline was done by HPLC-UV and photoproducts from direct photodegradation were identified by electrospray mass spectrometry. An observed direct photodegradation rate of sertraline of 0.0062 h-1 was determined, corresponding to a half-life time of 111 h (equivalent to 29 SSD). A significant influence of photosensitizers was observed, the best results being achieved in irradiations of sertraline with humic acids, obtaining a half-life time of 12 h. This was attributed to the hydrophobicity of this substance and higher absortivity in the UV/Vis wavelength, which promote processes of indirect photodegradation. The degradation of sertraline in natural samples was also enhanced comparatively to the direct photodegradation, achieving half-life times between 10 and 25h; the best results were achieved in samples from the primary treatment of a wastewater treatment plant and Ria de Aveiro, with half-life times of 10 and 16 h, respectively. A total of six photoproducts formed during the direct photodegradation of sertraline were identified, three of which were not yet identified in the literature. The main factors contributing to the degradation of sertraline were analysed but this was not fully accomplished, requiring further studies of the composition of the natural matrices and the combined influence of distinct photosensitizers during the irradiation. Nevertheless, it was concluded that the photodegradation of sertraline is greatly influenced by indirect photodegradation processes, promoted by the presence of photosensitizers.

Prediction of the solar radiation using RBF neural networks and ground-to-sky images

In this study, Artificial Neural Networks are applied to multistep long term solar radiation prediction. The networks are trained as one-step-ahead predictors and iterated over time to obtain multi-step longer term predictions. Auto-regressive and Auto-regressive with exogenous inputs solar radiationmodels are compared, considering cloudiness indices as inputs in the latter case. These indices are obtained through pixel classification of ground-to-sky images. The input-output structure of the neural network models is selected using evolutionary computation methods.

Estudo da utilização de energia solar nas escolas básicas e secundárias da região do Algarve

Utilização da energia solar nas escolas e.b. 2/3 do Algarve.

Tele-experimentação de técnicas de monitorização via internet com aplicações em agricultura e energia solar (TeleAgriSol)

Tele-experimentação detécnicas de monitorização via Internet com aplicações em agricultura e energia solar.

Dessalinização da água do mar através da energia solar: caso de estudo: Salamansa - Cabo Verde

Dissertação de mest., Engenharia do Ambiente, Faculdade de Ciências e Tecnologia, Univ. do Algarve, 2012

Estudo da aplicação de um sistema frigorífico de absorção movido a energia solar na Ilha do Príncipe

Dissertação de mest., Energias Renováveis e Gestão de Energia (Tecnológica), Faculdade de Ciências e Tecnologia, Univ. do Algarve, 2012

Bio-synthesis of nanosized semiconductors using mine wastes as material sources

This work describes the synthesis of nanosized metal sulfides and respective SiO2 and/or TiO2 composites in high yield via a straightforward process, under ambient conditions (temperature and pressure), by adding to aqueous metals a nutrient solution containing biologically generated sulfide from sulfate-reducing bacteria (SRB). The nanoparticles‘ (NPs) morphological properties were shown not to be markedly altered by the SRB growth media composition neither by the presence of bacterial cells. We further extended the work carried out, using the effluent of a bioremediation system previously established. The process results in the synthesis of added value products obtained from metal rich effluents, such as Acid Mine Drainage (AMD), when associated with the bioremediation process. Precipitation of metals using sulfide allows for the possibility of selective recovery, as different metal sulfides possess different solubilities. We have evaluated the selective precipitation of CuS, ZnS and FeS as nanosized metal sulfides. Again, we have also tested the precipitation of these metal sulfides in the presence of support structures, such as SiO2. Studies were carried out using both artificial and real solutions in a continuous bioremediation system. We found that this method allowed for a highly selective precipitation of copper and a lower selectivity in the precipitation of zinc and iron, though all metals were efficiently removed (>93% removal). This research has also demonstrated the potential of ZnS-TiO2 nanocomposites as catalysts in the photodegradation of organic pollutants using the cationic dye, Safranin-T, as a model contaminant. The influence of the catalyst amount, initial pH and dye concentration were also evaluated. Finally, the efficiency of the precipitates as catalysts in sunlight mediated photodegradation was investigated, using different volumes of dye-contaminated water (150 mL and 10 L). This work demonstrates that all tested composites have the potential to be used as photocatalysts for the degradation of Safranin-T.

Cartografia solar: estimativa do potencial solar no município de Albufeira

A dependência energética dos combustíveis fósseis é, reconhecidamente, uma das principiais inquietações das economias mundiais. Questões como a concentração de gases de efeito de estufa, poluição atmosférica e o facto de estes combustíveis serem esgotáveis estão cada vez mais no centro das atenções globais, ao que se associa um aumento significativo da população mundial e por conseguinte, dos consumos. Contudo, começa a ser notório um empenho na procura de soluções viáveis que possam contornar esta dependência, nomeadamente no desenvolvimento de tecnologia que permita o aproveitamento de fontes de energias renováveis. Neste sentido, Portugal encontra-se numa posição privilegiada sendo, dos países da europa, o que apresenta índices mais elevados de radiação solar por unidade de superfície, em média cerca de 1500kWh/m2/ano. O sucesso do aproveitamento de fontes de energia renováveis vai depender, em muito, da análise e compreensão do potencial determinado pelas realidades locais, pelos dados meteorológicos, pelas tecnologias existentes e por fatores económicos. (WITTMAN et al., 1997). O processo para estimativa o potencial não é simples e implica uma interação disciplinar; no entanto tendem a aparecer modelos que, a montante do processo, simplificam a análise espacial da energia solar. Neste campo, o contributo dos Sistemas de Informação Geográfica tem sido fundamental, oferecendo um conjunto de ferramentas de processamento de dados bastantes úteis para a modelação solar. A presente dissertação combina a utilização dos SIG com a análise do potencial solar, apresentando como objetivos principais: i) a estimativa do potencial solar no Município de Albufeira e ii) a criação de uma aplicação que disponibilize os resultados através da web, facilitando a consulta e análise espacial dos mesmos.

Comparação energética de sistemas de aquecimento a energia solar para o conforto térmico dos ocupantes de um edifício residencial

Dissertação de mestrado, Energia e Climatização de Edifícios, Instituto Superior de Engenharia, Universidade do Algarve, 2015

Enabling solar electricity with electric vehicles in future energy systems

Tese de doutoramento, Sistemas Sustentáveis de Energia, Universidade de Lisboa, Faculdade de Ciências, 2015

Modelling real solar cell using PSCAD/MATLAB

This paper presents the development of a solar photovoltaic (PV) model based on PSCAD/EMTDC - Power System Computer Aided Design – including a mathematical model study. An additional algorithm has been implemented in MATLAB software in order to calculate several parameters required by the PSCAD developed model. All the simulation study has been performed in PSCAD/MATLAB software simulation tool. A real data base concerning irradiance, cell temperature and PV power generation was used in order to support the evaluation of the implemented PV model.