Projecte d'energia solar tèrmica

El proyecto consiste en el diseño de una instalación solar térmica para producción de agua caliente sanitaria (ACS) en un edificio de nueva construcción en la localidad de Mollerussa (Lleida). Se han estudiado las necesidades térmicas de ACS en atención a las características constructivas y funcionales del edificio, dando cumplimiento a la normativa vigente. Conocida la demanda energética esperada, se han analizado los datos climatológicos y de temperatura de red de agua fría propios del emplazamiento, y se ha propuesto un campo de captación compuesto por captadores planos y los distintos subconjuntos que componen la instalación: acumulación, transferencia térmica, trazado hidráulico, regulación y control, y energía auxiliar. Con ello se ha llevado a cabo una simulación energética mediante la herramienta TSOL, software de simulación solar recomendado por entidades de reconocido prestigio, para comprobar que se han alcanzado los objetivos del sistema propuesto. Por último, se ha realizado un estudio del beneficio medioambiental que supone la instalación proyectada, indicando el ahorro energético para el usuario y las toneladas equivalentes de dióxido de carbono evitadas.

Anàlisi i disseny d'un programari de Gestió Remota d'un Parc Modular d'Energia Solar

Anàlisi i disseny d'una aplicació per gestionar de manera remota l'activitat d'un parc d'energia solar fotovoltaica.

Projecte d’una instal•lació solar fotovoltaica per a un sistema de bombes de reg

Instal.lació d’una explotació agrícola amb funcionament per energia solar fotovoltaica a Torregrossa (Tarragona). Disseny i definició de les parts necessàries que conformaran la instal•lació solar fotovoltaica que subministrarà energia elèctrica a les bombes de reg

Projecte d'implantació d'energia solar fotovoltaica al municipi d'Albanyà

Disseny d’una instal·lació d’energia solar fotovoltaica per als edificis públics del municipi d’Albanyà (Alt Empordà) per connectar-la a la xarxa i amb un estudi sobre la substitució dels actuals fanals de l’enllumenat públic per fanals alimentats amb energia solar fotovoltaica

Seguidor solar controlat per microcontrolador

L’objectiu d’aquest projecte és la realització d’un seguidor solar, i per poder tenir la màxima precisió en el control de moviment utilitzarem un microcontrolador (PIC 16F877) per controlar el seu estat en tot moment. Volem aconseguir que aquesta placa electrònica pugui controlar un seguidor i posteriorment ampliar-ho a un camp de seguidor solars per una vivenda estàndard. Quan parlem de controlar els seguidor ens referim a fer la orientació adient a cada moment del dia, aquesta orientació tindrà dos graus de llibertat. També aprofitarem les hores vall per poder fer el reposicionament de totes les plaques solarsAquest sistema microprocessat tindrà el suport d’un sistema d’actualització de calendari solar, per saber en quin moment del dia s’ha de posar en marxa i en quina direcció s’ha de posicionar

Temporal variability and trends of the downward solar radiation over Europe during the 20th century, with regional focus in the dimming/brightening phenomena on the Iberian Peninsula

Proyecto de investigación elaborado a partir de una estancia en el Institute for Atmospheric and Climate Science, a Alemanya, entre 2010 y 2012. La radiación solar que alcanza la superficie terrestre es un factor clave entre los procesos que controlan el clima de la Tierra, dado el papel que desempeñan en el balance energético y el ciclo hidrológico. Establecer su contribución al cambio climático reciente supone una gran dificultad debido a la complejidad de los procesos implicados, la gran cantidad de información requerida, y la incertidumbre de las bases de datos disponibles en la actualidad. Así, el objetivo principal del proyecto ha consistido en generar una base de datos de insolación incluyendo las series más largas (desde finales del siglo XIX) disponibles en toda Europa. Esta base de datos complementa para nuestro continente el Global Energy Balance Archive (GEBA) que mantiene y gestiona el grupo que ha acogido al receptor de la ayuda postdoctoral, y permite extender espacial (especialmente en países del sur de Europa) y temporalmente las series climáticas disponibles de mediciones de irradiancia solar. Como la insolación es un proxy de la irradiancia solar, el proyecto actual también ha tratado de calibrar de forma exhaustiva ambas variables, a fin de generar una nueva base de datos reconstruida de esta segunda variable que esté disponible desde finales del siglo XIX en Europa. Un segundo objetivo del proyecto ha consistido en continuar trabajando a escala de mayor detalle sobre la Península Ibérica, con el fin de proporcionar una mejor comprensión del fenómeno del “global dimming/brightening” y su impacto en el ciclo hidrológico y balance energético. Finalmente, un tercer objetivo del presente proyecto postdoctoral ha consistido en continuar estudiando los posibles ciclos semanales a gran escala de diferentes variables climáticas, línea de investigación de interés para la detección de posibles efectos de los aerosoles antrópicos en el clima a escalas temporales breves, y consecuentemente estrechamente vinculado al fenómeno del “global dimming/brightening”.

Dessalinização da Água do Mar Através da Energia Solar - Caso de Estudo Salamansa – Cabo Verde

principal objectivo deste trabalho é o estudo da viabilidade técnica e económica da dessalinização da água do mar, utilizando a energia solar, tomando como caso de aplicação uma pequena comunidade rural de Cabo Verde, a vila piscatória de Salamansa, local onde há graves problemas com a disponibilidade de água potável. No entanto, a proximidade do mar e a disponibilidade de energia solar sugerem a dessalinização como processo para mitigar a falta de água. A dessalinização da água do mar pode ser obtida através de diversas técnicas que podem ser agrupadas de acordo com os princípios em que estes processos se baseiam: processos de dessalinização térmica (destilação solar, destilação multi-estágio, destilação multi-efeito, etc.) e processos de dessalinização por membranas (electrodiálise e osmose inversa). A destilação solar passiva foi a tecnologia de dessalinização estudada neste trabalho e que se pode vir a tornar uma alternativa promissora para um fornecimento regular de água. Por outro lado, o uso de fontes alternativas de energia, como a solar, apresenta-se como uma solução para viabilizar a dessalinização em meios semi-áridos como o deste caso de estudo. Fez-se uma modelação matemática da unidade de destilação solar proposta utilizando o Engineering Equation Solver (EES) como ferramenta para ajudar a resolver as equações de balanço térmico. O projecto do destilador solar proposto poderá atender às necessidades de água doce para consumo de 18 famílias constituídas por 5 agregados (92 pessoas) e apresenta uma eficiência média diária de aproximadamente 78% no Verão e 77% no Inverno.

Energy Management for Stand-Alone Renewable Energy Systems (E-MAN-RES). Simulacions de sistemes.

L’objecte del present informe és la descripció dels treballs duts a terme en l’Activitat 2 del projecte E-MAN-RES: models de simulació i càlcul per optimització i anàlisi de sensibilitat de la gestió de la demanda, per part de la Universitat Politècnica de Catalunya.

Characterization and discrimination of soils by their reflected electromagnetic energy

The objective of this work was to verify if reflected energy of soils can characterize and discriminate them. A spectroradiometer (Spectral reflectance between: 400-2,500 nm) was utilized in laboratory. The soils evaluated are located in Bauru region, SP, Brazil, and are classified as Typic Argiudoll (TR), Typic Eutrorthox (LR), Typic Argiudoll (PE), Typic Haplortox (LE), Typic Paleudalf (PV) and Typic Quartzipsamment (AQ). They were characterized by their spectral reflectance as for descriptive conventional methods (Brazilian and International) according to the types of spectral curves. A method for the spectral descriptive evaluation of soils was established. It was possible to characterize and discriminate the soils by their spectral reflectance, with exception for LR and TR. The spectral differences were better identified by the general shape of spectral curves, by the intensity of band absorption and angle tendencies. These characteristics were mainly influenced by organic matter, iron, granulometry and mineralogy constituents. A reduction of iron and clay contents, which influenced higher reflectance intensity and shape variations, occurred on the soils LR/TR, PE, LE, PV and AQ, on that sequence. Soils of the same group with different clay textures could be discriminated. The conventional descriptive evaluation of spectral curves was less efficient on discriminating soils. Simulated orbital data discriminated soils mainly by bands 5 and 7.

Forecasting the Earth"s radiation belts and modeling solar energetic particle events: Recent results from SPACECAST

High-energy charged particles in the van Allen radiation belts and in solar energetic particle events can damage satellites on orbit leading to malfunctions and loss of satellite service. Here we describe some recent results from the SPACECAST project on modelling and forecasting the radiation belts, and modelling solar energetic particle events. We describe the SPACECAST forecasting system that uses physical models that include wave-particle interactions to forecast the electron radiation belts up to 3 h ahead. We show that the forecasts were able to reproduce the >2 MeV electron flux at GOES 13 during the moderate storm of 7-8 October 2012, and the period following a fast solar wind stream on 25-26 October 2012 to within a factor of 5 or so. At lower energies of 10- a few 100 keV we show that the electron flux at geostationary orbit depends sensitively on the high-energy tail of the source distribution near 10 RE on the nightside of the Earth, and that the source is best represented by a kappa distribution. We present a new model of whistler mode chorus determined from multiple satellite measurements which shows that the effects of wave-particle interactions beyond geostationary orbit are likely to be very significant. We also present radial diffusion coefficients calculated from satellite data at geostationary orbit which vary with Kp by over four orders of magnitude. We describe a new automated method to determine the position at the shock that is magnetically connected to the Earth for modelling solar energetic particle events and which takes into account entropy, and predict the form of the mean free path in the foreshock, and particle injection efficiency at the shock from analytical theory which can be tested in simulations.

A numeric model to simulate solar individual ultraviolet exposure.

Exposure to solar ultraviolet (UV) light is the main causative factor for skin cancer. UV exposure depends on environmental and individual factors. Individual exposure data remain scarce and development of alternative assessment methods is greatly needed. We developed a model simulating human exposure to solar UV. The model predicts the dose and distribution of UV exposure received on the basis of ground irradiation and morphological data. Standard 3D computer graphics techniques were adapted to develop a rendering engine that estimates the solar exposure of a virtual manikin depicted as a triangle mesh surface. The amount of solar energy received by each triangle was calculated, taking into account reflected, direct and diffuse radiation, and shading from other body parts. Dosimetric measurements (n = 54) were conducted in field conditions using a foam manikin as surrogate for an exposed individual. Dosimetric results were compared to the model predictions. The model predicted exposure to solar UV adequately. The symmetric mean absolute percentage error was 13%. Half of the predictions were within 17% range of the measurements. This model provides a tool to assess outdoor occupational and recreational UV exposures, without necessitating time-consuming individual dosimetry, with numerous potential uses in skin cancer prevention and research.

Forecasting the Earth"s radiation belts and modeling solar energetic particle events: Recent results from SPACECAST

High-energy charged particles in the van Allen radiation belts and in solar energetic particle events can damage satellites on orbit leading to malfunctions and loss of satellite service. Here we describe some recent results from the SPACECAST project on modelling and forecasting the radiation belts, and modelling solar energetic particle events. We describe the SPACECAST forecasting system that uses physical models that include wave-particle interactions to forecast the electron radiation belts up to 3 h ahead. We show that the forecasts were able to reproduce the >2 MeV electron flux at GOES 13 during the moderate storm of 7-8 October 2012, and the period following a fast solar wind stream on 25-26 October 2012 to within a factor of 5 or so. At lower energies of 10- a few 100 keV we show that the electron flux at geostationary orbit depends sensitively on the high-energy tail of the source distribution near 10 RE on the nightside of the Earth, and that the source is best represented by a kappa distribution. We present a new model of whistler mode chorus determined from multiple satellite measurements which shows that the effects of wave-particle interactions beyond geostationary orbit are likely to be very significant. We also present radial diffusion coefficients calculated from satellite data at geostationary orbit which vary with Kp by over four orders of magnitude. We describe a new automated method to determine the position at the shock that is magnetically connected to the Earth for modelling solar energetic particle events and which takes into account entropy, and predict the form of the mean free path in the foreshock, and particle injection efficiency at the shock from analytical theory which can be tested in simulations.

Distributed Energy Production in the North-West Region of Russia

The energy system of Russia is the world's fourth largest measured by installed power. The largest are that of the the United States of America, China and Japan. After 1990, the electricity consumption decreased as a result of the Russian industry crisis. The vivid economic growth during the latest few years explains the new increase in the demand for energy resources within the State. In 2005 the consumption of electricity achieved the maximum level of 1990 and continues to growth. In the 1980's, the renewal of power facilities was already very slow and practically stopped in the 1990's. At present, the energy system can be very much characterized as outdated, inefficient and uneconomic because of the old equipment, non-effective structure and large losses in the transmission lines. The aim of Russia's energy reform, which was started in 2001, is to achieve a market based energy policy by 2011. This would thus remove the significantly state-controlled monopoly in Russia's energy policy. The reform will stimulateto decrease losses, improve the energy system and employ energy-saving technologies. The Russian energy system today is still based on the use of fossil fuels, and it almost totally ignores the efficient use of renewable sources such as wind, solar, small hydro and biomass, despite of their significant resources in Russia. The main target of this project is to consider opportunities to apply renewable energy production in the North-West Federal Region of Russia to partly solve the above mentioned problems in the energy system.

The first SEPServer event catalogue 68-MeV solar proton events observed at 1 AU in 1996-2010

SEPServer is a three-year collaborative project funded by the seventh framework programme (FP7-SPACE) of the European Union. The objective of the project is to provide access to state-of-the-art observations and analysis tools for the scientific community on solar energetic particle (SEP) events and related electromagnetic (EM) emissions. The project will eventually lead to better understanding of the particle acceleration and transport processes at the Sun and in the inner heliosphere. These processes lead to SEP events that form one of the key elements of space weather. In this paper we present the first results from the systematic analysis work performed on the following datasets: SOHO/ERNE, SOHO/EPHIN, ACE/EPAM, Wind/WAVES and GOES X-rays. A catalogue of SEP events at 1 AU, with complete coverage over solar cycle 23, based on high-energy (~68-MeV) protons from SOHO/ERNE and electron recordings of the events by SOHO/EPHIN and ACE/EPAM are presented. A total of 115 energetic particle events have been identified and analysed using velocity dispersion analysis (VDA) for protons and time-shifting analysis (TSA) for electrons and protons in order to infer the SEP release times at the Sun. EM observations during the times of the SEP event onset have been gathered and compared to the release time estimates of particles. Data from those events that occurred during the European day-time, i.e., those that also have observations from ground-based observatories included in SEPServer, are listed and a preliminary analysis of their associations is presented. We find that VDA results for protons can be a useful tool for the analysis of proton release times, but if the derived proton path length is out of a range of 1 AU < s[3 AU, the result of the analysis may be compromised, as indicated by the anti-correlation of the derived path length and release time delay from the asso ciated X-ray flare. The average path length derived from VDA is about 1.9 times the nominal length of the spiral magnetic field line. This implies that the path length of first-arriving MeV to deka-MeV protons is affected by interplanetary scattering. TSA of near-relativistic electrons results in a release time that shows significant scatter with respect to the EM emissions but with a trend of being delayed more with increasing distance between the flare and the nominal footpoint of the Earth-connected field line.