Central de produção de energia eléctrica a partir de energia solar térmica

Trabalho Final de Mestrado para obtenção do grau de Mestre em Engenharia Mecânica

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

Dissertação para obtenção do grau de Mestre em Engenharia Electrotécnica

Desempenho energético no âmbito do aquecimento solar térmico para as condições de utilização recomendadas pelo RSECE/RCCTE

Trabalho Final de Mestrado para obtenção do grau de Mestre em Engenharia Mecânica

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

Dissertação para obtenção do grau de Mestre em Engenharia Eletrotécnica

Engineering the Properties of Indium Sulfide for Thin Film Solar Cells by Doping

In the present work, structural, optical and electrical properties of indium sulfide are tuned by specific and controlled doping. Silver, tin, copper and chlorine were used as the doping elements. In2S3 thin films for the present study were prepared using a simple and low cost “Chemical Spray Pyrolysis (CSP)” technique. This technique is adaptable for large-area deposition of thin films in any required shape and facilitates easiness of doping and/or variation of atomic ratio. It involves spraying a solution, usually aqueous, containing soluble salts of the constituents of the desired compound onto a heated substrate. Doping process was optimized for different doping concentrations. On optimizing doping conditions, we tuned the structural, optical and electrical properties of indium sulfide thin films making them perform as an ideal buffer layer.

Optimization of Two Stage Process for the Growth of In2S3 , CuInSe2 and CuIn (Sel-xSx)2Thin Films for Solar Cell Application

Two stage processes consisting of precursor preparation by thermal evaporation followed by chalcogenisation in the required atmosphere is found to be a feasible technique for the PV materials such as n-Beta In2S3, p-CulnSe2, p-CulnS2 and p-CuIn(Sel_xSx)2. The growth parameters such as chalcogenisation temperature and duration of chalcogenisation etc have been optimised in the present study.Single phase Beta-In2S3 thin films can be obtained by sulfurising the indium films above 300°C for 45 minutes. Low sulfurisation temperatures required prolonged annealing after the sulfurisation to obtain single phase Beta-1n2S3, which resulted in high material loss. The maximum band gap of 2.58 eV was obtained for the nearly stoichiometric Beta-In2S3 film which was sulfurised at 350°C. This wider band gap, n type Beta-In2S3 can be used as an alternative to toxic CdS as window layer in photovoltaics .The systematic study on the structural optical and electrical properties of CuInSe2 films by varying the process parameters such as the duration of selenization and the selenization temperature led to the conclusion that for the growth of single-phase CuInSe2, the optimum selenization temperature is 350°C and duration is 3 hours. The presence of some binary phases in films for shorter selenization period and lower selenization temperature may be due to the incomplete reaction and indium loss. Optical band gap energy of 1.05 eV obtained for the films under the optimum condition.In order to obtain a closer match to the solar spectrum it is desirable to increase the band gap of the CulnSe2 by a few meV . Further research works were carried out to produce graded band gap CuIn(Se,S)2 absorber films by incorporation of sulfur into CuInSe2. It was observed that when the CulnSe2 prepared by two stage process were post annealed in sulfur atmosphere, the sulfur may be occupying the interstitial positions or forming a CuInS2 phase along with CuInSe2 phase. The sulfur treatment during the selenization process OfCu11 ln9 precursors resulted in Culn (Se,S)2 thin films. A band gap of 1.38 eV was obtained for the CuIn(Se,S)2.The optimised thin films n-beta 1n2S3, p-CulnSe2 and p-Culn(Sel-xSx)2 can be used for fabrication of polycrystalline solar cells.

Projecte per la realització d’ una intal·lació solar fotovoltaica en règim especial als edificis de l’ Escola Politècnica Superior de la UdG

El present projecte té per principal odjectiu dur a terme el disseny d’ una instal·lació solar fotovoltaica de producció d’ energia elèctrica en règim especial sobre teulada instal·lada en un edifici de caràcter oficial de l’ Escola Politècnica Superior de la UdG amb l’ objectiu de generar energia elèctrica

Projecte de la intal·lació de calefacció i ACS amb energia solar i caldera de biomassa en un edifici de quatre vivendes.

Projecte de la instal•lació de calefacció i agua calenta utilitzant energia solar tèrmica i ajudant-se d’ una caldera de biomassa en un edifici en construcció situat a Colera (Alt Empordà). Es tracta d’un bloc de quatre vivendes distribuïdes en dues plantes, soterrani i terrassa superior

Projecte d’instal·lacions d’aigua calenta sanitària per a un hotel de quatre estrelles a Platja d’Aro amb aportació d’energia solar

En el present projecte final de carrera s’han dissenyat i pressupostat les instal·lacions de fontaneria, energia solar i gas natural per abastir d’aigua les dependències d’un hotel. L’hotel es troba situat a municipi de Platja d’Aro, a la província de Girona. La seva categoria és de quatre estrelles i això comporta un nivell alt de qualitat en els serveis oferts, en aquest cas el subministrament d’aigua freda i aigua calenta sanitària (ACS) als seus clients

Avaluació i implantació d’un sistema de climatització amb energia solar a la Facultat de Ciències de la UdG

Estudi de viabilitat de climatització de la Facultat de Ciències de la UdG per energia solar. Estudi de costos i comparació de l’estalvi respecte al sistema actual

Instal•lació solar tèrmica i fotovoltaica per a una vivenda aïllada

Aquest projecte va destinat a una família que disposa d’una vivenda aïllada del nucli urbà d’Arenys de Munt, comarca del Maresme, la qual no té al seu abast la connexió del gas ni la de la xarxa elèctrica. S’ha decidit dimensionar la instal•lació per energia solar tèrmica i energia solar fotovoltaica, ja que són energies més constants que l’energia eòlica per a l’indret on ens trobem i a més a més hi ha un mercat que ofereix molts més productes i prestacions

Estudi comparatiu entre un sistema de climatització solar amb planta d’absorció geotèrmica i un sistema de climatització amb bomba de calor geotèrmica

Disseny i dimensionat d’una instal•lació de climatització, durant tot l'any, i comparació entre un sistema de climatització solar amb una planta d’absorció geotèrmica i un sistema de climatització mitjançant una bomba de calor geotèrmica, per al despatx de professors i becaris del nou laboratori d’ energia de l’EPS, mitjançant la utilització d’un sistema d’energia solar tèrmica de baixa temperatura, com a medi d’aportació de calor, i per energia geotèrmica per a la climatització integral

Instal•lació solar tèrmica per la producció d’ACS i climatització de 10 H.P.O. a Quart

Aquesta instal•lació solar tèrmica s’ha dissenyat per cobrir part de les necessitats energètiques d’un edifici que consta de 10 habitatges de protecció oficial construïts en 2 plantes a la localitat de Quart. L’objectiu d’aquest projecte és arribar a una cobertura solar aproximada del 50% de les necessitats d’ aigua calenta sanitària (ACS) i climatització

Solar influences on dynamical coupling between the stratosphere and troposphere

We use a simplified atmospheric general circulation model (AGCM) to investigate the response of the lower atmosphere to thermal perturbations in the lower stratosphere. The results show that generic heating of the lower stratosphere tends to weaken the sub-tropical jets and the tropospheric mean meridional circulations. The positions of the jets, and the extent of the Hadley cells, respond to the distribution of the stratospheric heating, with low latitude heating displacing them poleward, and uniform heating displacing them equatorward. The patterns of response to the low latitude heating are similar to those found to be associated with solar variability in previous observational data analysis, and to the effects of varying solar UV radiation in sophisticated AGCMs. In order to investigate the chain of causality involved in converting the stratospheric thermal forcing to a tropospheric climate signal we conduct an experiment which uses an ensemble of model spin-ups to analyse the time development of the response to an applied stratospheric perturbation. We find that the initial effect of the change in static stability at the tropopause is to reduce the eddy momentum flux convergence in this region. This is followed by a vertical transfer of the momentum forcing anomaly by an anomalous mean circulation to the surface, where it is partly balanced by surface stress anomalies. The unbalanced part drives the evolution of the vertically integrated zonal flow. We conclude that solar heating of the stratosphere may produce changes in the circulation of the troposphere even without any direct forcing below the tropopause. We suggest that the impact of the stratospheric changes on wave propagation is key to the mechanisms involved.

Solar induced climate effects

Solar electromagnetic radiation powers Earth’s climate system and, consequently, it is often naively assumed that changes in this solar output must be responsible for changes in Earth’s climate. However, the Sun is close to a blackbody radiator and so emits according to its surface temperature and the huge thermal time constant of the outer part of the Sun limits the variability in surface temperature and hence output. As a result, on all timescales of interest, changes in total power output are limited to small changes in effective surface temperature (associated with magnetic fields) and potential, although as yet undetected, solar radius variations. Larger variations are seen in the UV part of the spectrum which is emitted from the lower solar atmosphere (the chromosphere) and which influences Earth’s stratosphere. There is interest in“top-down” mechanisms whereby solar UV irradiance modulates stratospheric temperatures and winds which, in turn, may influence the underlying troposphere where Earth’s climate and weather reside. This contrasts with “bottom-up” effects in which the small total solar irradiance (dominated by the visible and near-IR) variations cause surface temperature changes which drive atmospheric circulations. In addition to these electromagnetic outputs, the Sun modulates energetic particle fluxes incident on the Earth. Solar Energetic Particles (SEP) are emitted by solar flares and from the shock fronts ahead of supersonic (and super-Alfvenic) ejections of material from the solar atmosphere. These SEPs enhance the destruction of polar stratospheric ozone which could be an additional form of top-down climate forcing. Even more energetic are Galactic Cosmic Rays (GCRs). These particles are not generated by the Sun, rather they originate at the shock fronts emanating from violent galactic events such as supernovae explosions; however, the expansion of the solar magnetic field into interplanetary space means that the Sun modulates the number of GCRs reaching Earth. These play a key role in enabling Earth’s global electric (thunderstorm) circuit and it has been proposed that they also modulate the formation of clouds. Both electromagnetic and corpuscular solar effects are known to vary over the solar magnetic cycle which is typically between 10 and 14 yrs in length (with an average close to 11 yrs). The solar magnetic field polarity at any one phase of one of these activity cycles is opposite to that at the same phase of the next cycle and this influences some phenomena, for example GCRs, which therefore show a 22 yr (“Hale”) cycle on average. Other phenomena, such as irradiance modulation, do not depend on the polarity of the magnetic field and so show only the basic 11-yr activity cycle. However, any effects on climate are much more significant for solar drifts over centennial timescales. This chapter discusses and evaluates potential effects on Earth’s climate system of variations in these solar inputs. Because of the great variety of proposed mechanisms, the wide range of timescales studied (from days to millennia) and the many debates (often triggered by the application of inadequate statistical methods), the literature on this subject is vast, complex, divergent and rapidly changing: consequently the number of references cited in this review is very large (yet still only a small fraction of the total).