A full electro-thermal simulation of a three-phase space-vector-modulated (SVM) inverter is performed and validated with measurements. Electrical parameters are extracted over temperature for the insulated gate bipolar transistor (IGBT) and diode electro-thermal models. A thermal network methodology that includes thermal coupling between devices is applied to a six-pack module package containing multiple IGBT and diode chips. The electro-thermal device models and six-pack module thermal model are used to simulate SVM inverter operation at several power levels. Good agreement between model and measurement is obtained for steady state operation of the three-phase inverter. In addition, transient heating of a single IGBT in the six-pack module is modeled and validated, yielding good agreement. / Master of Science

No description available.

A new method for determining the causes of discrepancies between dynamic simulation models and measured data is described. Whilst principally aimed at the validation of building thermal simulation codes, the method may rind application in the validation of simulation models from other disciplines. The new method relies on generating a model of the discrepancies in terms of the variables driving the physical reality which produced the experimental data and the corresponding simulation. Inspection of the resulting error model allows the principal contributors to simulation error to be identified, its dynamic nature to be characterised, and the likely cause of the error to be identified. The method is tested by generating a 'quasi-truth' dataset using the building thermal simulation code SERI-RES. A series of simulations is then prepared with perturbations to selected input parameters. The new tool is found to be capable of recovering details of the perturbations. Finally, the power of the new technique is demonstrated in a series of comparisons between the predictions of the model SERI-RES and data collected in outdoor test rooms. These comparisons reveal that the principal source of error in the predictions is the treatment of the interactions between the heater and the air and fabric of the room. The new technique proves sufficiently sensitive to detect the changing structure of the prediction errors as the position of the heater within the room is changed.

A 3D 8-component thermal compositional simulation study has been performed to evaluate the merits of steam-propane injection and a novel vertical-smart horizontal well system for the Lombardi reservoir in the San Ardo field, California. The novel well system consists of a vertical steam injector and a horizontal producer, whose horizontal section is fully open initially, and after steam breakthrough, only one-third (heel-end) is kept open. A 16x16x20 Cartesian model was used that represented a quarter of a typical 10acre 9-spot inverted steamflood pattern in the field. The prediction cases studied assume prior natural depletion to reservoir pressure of about 415 psia. Main results of the simulation study may be summarized as follows. First, under steam injection, oil recovery is significantly higher with the novel vertical-smart horizontal well system (45.5-58.7% OOIP at 150-300 BPDCWE) compared to the vertical well system (33.6-32.2% OOIP at 150-300 BPDCWE). Second, oil recovery increases with steam injection rate in the vertical-smart horizontal well system but appears to reach a maximum at about 150 BPDCWE in the vertical well system (due to severe bypassing of oil). Third, under steam-propane injection, oil recovery for the vertical-smart horizontal well system increases to 46.1% OOIP at 150 BPDCWE but decreases to 51.6% OOIP at 300 PDCWE due to earlier steam breakthrough that resulted in reduced sweep efficiency. Fourth, for the vertical well system, steam-propane injection results in an increase of oil recovery to 35.4-32.6% OOIP at 150-300 BPDCWE. Fifth, with steam-propane injection, for both well systems, oil production acceleration increases with lower injection rates. Sixth, the second oil production peak in the vertical-smart horizontal well system is accelerated by 24-50% in time for 150-300 BPDCWE compared to that with pure steam injection.

Este trabalho apresenta os resultados obtidos no processo de otimização realizado nas câmeras astronômicas do instrumento BTFI (Brazilan Tunable Filter Imager) instalado no telescópio SOAR, no Chile, para reduzir o ruído nos sinais. O instrumento BTFI opera com duas câmeras astronômicas de alto desempenho que utilizam detectores de imagens denominados EMCCDs. Esses detectores são sensores de imagem baseados em dispositivos de carga acoplada (CCDs) otimizados por um estágio integrado de multiplicação de elétrons por avalanche. Essa característica permite atingir ao mesmo tempo altas taxas de leitura (10 MHz) e níveis de ruído muito baixos (<1 elétron/pixel). Detectores CCD exigem temperaturas de operação da ordem de -100oC para operar com baixo ruído, o que demanda uma série de especificações técnicas quanto ao projeto da câmera. O trabalho aqui exposto fundamentou-se na otimização de aspectos mecânicos e eletrônicos de câmeras astronômicas com o intuito de se obter a melhor relação sinal-ruído, mostrando a importância do correto desenho mecânico (do ponto de vista térmico) e sua influência no comportamento eletrônico da câmera. São expostos os resultados obtidos com as duas câmeras em laboratório, os métodos e processos de caracterização utilizados, bem como as simulações térmicas e experimentos realizados em laboratório. Com as técnicas empregadas alcançou-se níveis de ruído total menores que 0,18 elétrons/pixel/segundo para exposições de 10 segundos. Os resultados atingidos foram observados nas duas câmeras do instrumento BTFI e foram validados em laboratório, onde demonstraram estabilidade durante 71 dias consecutivos. Por fim, é mostrada uma caracterização comparativa entre as duas câmeras quanto aos níveis de ruídos, ganho, estabilidade, eficiência quântica, linearidade e relação sinal-ruído. / This work presents results of the optimization performed in the astronomical cameras from the Brazilian Tunable Filter Imager (BTFI), instrument for the SOAR Telescope in Chile, in order to reduce the signals noise. The BTFI instrument has two highperformance cameras equipped with detectors named EMCCDs, which are image sensors based on charge-coupled devices (CCDs) optimized by an electron multiplication integrated stage. This feature enables to achieve high readout rates (10 MHz) and very low noise levels (<1 electron/pixel) at the same time. CCD detectors demand running temperatures of about -100,sup>oC for very low noise operation, which requires a series of technical specifications for the camera design. The work shown here is based in the optimization of the mechanical and electronic aspects for the astronomical cameras, in order to obtain the best signal to noise ratio, showing the importance of the correct mechanical design (from the thermal point of view) and its influence on the camera electronic behavior. The laboratory results obtained with the two cameras, the characterization procedures, as well as the thermal simulations and laboratory ratification experiments that allowed achieve the results presented are exposed. Using such techniques it was possible to achieve total noise levels lower than 0.18 electron/pixel/second for 10 seconds of exposure time. The results achieved were observed in both BTFI cameras and were validated in laboratory showing 71 consecutive days of stability. Finally it is shown a comparative characterization between both cameras in: noise and gain levels, stability, quantum efficiency, linearity and signal to noise ratio.

Este trabalho apresenta os resultados obtidos no processo de otimização realizado nas câmeras astronômicas do instrumento BTFI (Brazilan Tunable Filter Imager) instalado no telescópio SOAR, no Chile, para reduzir o ruído nos sinais. O instrumento BTFI opera com duas câmeras astronômicas de alto desempenho que utilizam detectores de imagens denominados EMCCDs. Esses detectores são sensores de imagem baseados em dispositivos de carga acoplada (CCDs) otimizados por um estágio integrado de multiplicação de elétrons por avalanche. Essa característica permite atingir ao mesmo tempo altas taxas de leitura (10 MHz) e níveis de ruído muito baixos (<1 elétron/pixel). Detectores CCD exigem temperaturas de operação da ordem de -100oC para operar com baixo ruído, o que demanda uma série de especificações técnicas quanto ao projeto da câmera. O trabalho aqui exposto fundamentou-se na otimização de aspectos mecânicos e eletrônicos de câmeras astronômicas com o intuito de se obter a melhor relação sinal-ruído, mostrando a importância do correto desenho mecânico (do ponto de vista térmico) e sua influência no comportamento eletrônico da câmera. São expostos os resultados obtidos com as duas câmeras em laboratório, os métodos e processos de caracterização utilizados, bem como as simulações térmicas e experimentos realizados em laboratório. Com as técnicas empregadas alcançou-se níveis de ruído total menores que 0,18 elétrons/pixel/segundo para exposições de 10 segundos. Os resultados atingidos foram observados nas duas câmeras do instrumento BTFI e foram validados em laboratório, onde demonstraram estabilidade durante 71 dias consecutivos. Por fim, é mostrada uma caracterização comparativa entre as duas câmeras quanto aos níveis de ruídos, ganho, estabilidade, eficiência quântica, linearidade e relação sinal-ruído. / This work presents results of the optimization performed in the astronomical cameras from the Brazilian Tunable Filter Imager (BTFI), instrument for the SOAR Telescope in Chile, in order to reduce the signals noise. The BTFI instrument has two highperformance cameras equipped with detectors named EMCCDs, which are image sensors based on charge-coupled devices (CCDs) optimized by an electron multiplication integrated stage. This feature enables to achieve high readout rates (10 MHz) and very low noise levels (<1 electron/pixel) at the same time. CCD detectors demand running temperatures of about -100,sup>oC for very low noise operation, which requires a series of technical specifications for the camera design. The work shown here is based in the optimization of the mechanical and electronic aspects for the astronomical cameras, in order to obtain the best signal to noise ratio, showing the importance of the correct mechanical design (from the thermal point of view) and its influence on the camera electronic behavior. The laboratory results obtained with the two cameras, the characterization procedures, as well as the thermal simulations and laboratory ratification experiments that allowed achieve the results presented are exposed. Using such techniques it was possible to achieve total noise levels lower than 0.18 electron/pixel/second for 10 seconds of exposure time. The results achieved were observed in both BTFI cameras and were validated in laboratory showing 71 consecutive days of stability. Finally it is shown a comparative characterization between both cameras in: noise and gain levels, stability, quantum efficiency, linearity and signal to noise ratio.

L’analyse de la performance énergétique des bâtiments neufs repose massivement sur des outils logiciels de simulation. La valeur ajoutée de ces derniers est indéniable : ils permettent d’optimiser la conception en facilitant l’évaluation des performances énergétiques du bâtiment durant la phase de conception. Leur impact est cependant limité par plusieurs obstacles, dont les principaux sont le niveau d’expertise requis pour leur utilisation et l’absence de connexion aux outils de Conception Assistée par Ordinateur (CAO). Ce dernier point devient particulièrement critique au moment où l’utilisation de la maquette numérique BIM (Building Information Model) se généralise et où les modèles issus d’outils de CAO sont de plus en plus riches.Cette thèse repose sur cette observation et propose, afin de profiter pleinement du potentiel du BIM et des outils en lien, de contribuer à l’émergence d’approches permettant une transformation fiable et transparente des informations du bâtiment numérique BIM vers les fichiers d'entrée des environnements de simulation. Cela se traduirait par des avantages significatifs, tant sur le rapport coût-efficacité (l’analyse est effectuée plus efficacement), qu’au niveau de la fiabilité (les modèles de simulation sont conformes aux modèles de conception). Toutefois, pour mettre en œuvre de telles approches, plusieurs obstacles doivent être pris en compte : le premier est la nécessité de disposer d’un langage normalisé commun pour le BIM, le deuxième est la définition de mécanismes méthodologiques efficaces et normalisés afin d’enrichir le BIM pour la simulation, le troisième est la mise à disposition d'outils logiciels fiables pour la transformation automatisée du BIM vers les modèles de simulation thermique.Le premier obstacle est en passe d’être levé grâce aux standards issus du consortium international buildingSMART, en particulier les « Industry Foundation Classes » (IFC) qui sont désormais largement reconnus comme un format d'échange standard du BIM dans le domaine de la construction. Le deuxième verrou reste actuel : l’IFC, même dans sa dernière version IFC4, laisse entier de nombreux problèmes de formulation de concepts propres aux domaines métiers, en particulier celui de la simulation énergétique. Cependant, des environnements méthodologiques ont vu le jour permettant d’étendre et d’enrichir de façon structurée les formats de données BIM. C’est par exemple le cas de l’IDM (Information Delivery Manual) et du MVD (Model View Définition) de buildingSMART, pour les IFC.L’objectif de nos travaux est triple. En premier lieu, il s’agit de mettre en œuvre et évaluer l’environnement IDM/ MVD de buildingSMART pour l’interconnexion entre le BIM (format IFC) et la simulation énergétique. Cette étude nous a amenés à proposer un modèle pivot (BSM pour « Building Simulation Model ») basé sur une analogie avec les approches prônées par l’ingénierie dirigée par les modèles. Nous avons également développé un outil logiciel, qui inclut une base de règles de mapping, afin d’automatiser la traduction de l’information entre le modèle IFC et le modèle de simulation. Cette approche a été évaluée sur la base de l’outil COMETH (moteur de simulation de la régulation thermique française RT2012) mais elle est généralisable. / Energy performance analysis of new buildings strongly relies on simulation tools. They optimize the design by facilitating building performance analysis during the design phase. However, there are several limitations, among which one of the main is the lack of reliable connections between Computer Aided Design (CAD) and simulation tools. This is particularly critical at a time when the concept of Building Information Model (BIM) is widely applied and the CAD models are becoming richer.This thesis proposes to take advantage of the potential of BIM in order to contribute to emerging approaches for a reliable and seamless interconnection between building information models and simulation environment input files. This would result into significant benefits, both from the cost-effectiveness (analysis is performed more effectively) and the reliability (simulation models strictly comply with design models) points of view. However, to implement such approaches, several barriers have to be considered. The first is the need for a common, standardized BIM language. The second is the definition of adequate and standardized extension mechanisms, to customize BIM for simulation-specific purposes. The third is the provision of software tools, for effective and reliable BIM to simulation models transformation.The first barrier is likely to be overcome through the advent of the buildingSMART Industry Foundation Classes (IFC), which is widely recognized as a standard BIM exchange format in the construction industry. However, with respect to the second barrier, the IFC remains a wide-purpose modelling language and as such, fails to address many domain-specific issues, like e.g. energy simulation. This limitation has been acknowledged by buildingSMART, who have delivered novel methodological tools to allow for domain-specific customization of IFC. The main one is called the Information Delivery Manual (IDM). The aim of our work is the implementation and evaluation the BuildingSMART framework IDM/MVD to interconnect BIM (IFC) and energy simulation. This study led us to propose a pivotal model (BSM for « Building Simulation Model») based on an analogy with model driven engineering approaches. We also have developed a software prototype, which includes a set of mapping rules that automates the translation process between the IFC model and the simulation tool. In the scope of this study, we targeted the COMETH simulation tool (a simulation engine based on the French thermal regulation RT2012) but our results can easily be extended to additional tools.

A rapid growth in the national electricity demand is placing an ever-increasing demand on the national electricity supply utility, Eskom. Projections show that the load demand in South Africa may exceed the installed capacity by as early as 2007. This is mainly due to the increase in demand in the residential sector as a result of the electrification of rural and previously disadvantaged communities. However, the industrial and commercial sectors also have a role in this increase. In an attempt to reduce the demand for electricity Eskom has adopted its Demand Side Management (DSM) initiative. This initiative is aimed at lowering the electricity demand in peak times through energy efficiency (EE) or load shift, out of peak demand times. Eskom is implementing the DSM strategy by financing Energy Service Companies (ESCOs) to reduce the demand load of major electricity end-users during peak times. Buildings consume a large percentage of the total energy supply in the world. Most of the energy consumed in buildings is used by the heating, ventilation and air-conditioning (HVAC) systems, as well as lighting. However, a large potential for energy savings exists in buildings. Studies have shown that up to 70% of the electricity consumption of a building can be saved through retrofit studies. However, to capitalise on these opportunities, the ESCOs require tools and procedures that would enable them to accomplish energy savings studies quickly and efficiently. It should be a holistic approach to the typical ESCO building audit. A study of current available software programs showed the lack of holistic tools aimed specifically at retrofit audits, and therefore also the need for such a program. The building simulation program most suited to the retrofit study was chosen and it was used in a retrofit audit. By emulating a retrofit audit with this software, its performance in the field, both positive and negative, could be established. With the experience gained from the retrofit study, as well as input from ESCOs in the industry, a need for such a retrofit tool was established. The simulation program that was tested in the retrofit study is the tool Quickcontrol, as well as the newer version of the program, entitled QEC. The case study showed that even though these packages are well suited to ESCO work, they have certain drawbacks in view of the holistic project approach. The ESCOs require a simple, fast, and integrated procedure for energy audits. This procedure should be embodied in a software program. This study proposes a new integrated procedure for energy audits and the analyses of buildings, in the form of a software tool. This new tool is geared towards the ESCO building audit, in both South A6ica and internationally. It is designed to enable a diplomate engineer to accomplish a building energy and retrofit analysis in two weeks, leading the user through all the main project steps, from data acquisition to writing of the final project report. This is a significant improvement, since it normally takes 50 man-days for an experienced and trained engineering team to complete a full building audit. This tool was used in a case study to test its validity and accuracy. It was found that certain situations would arise in which the criteria that were set for the program would not be adequate. The results from the case study were favourable and satisfied the criteria that were set for the procedure. / Thesis (Ph.D. (Mechanical Engineering))--North-West University, Potchefstroom Campus, 2004.

A rapid growth in the national electricity demand is placing an ever-increasing demand on the national electricity supply utility, Eskom. Projections show that the load demand in South Africa may exceed the installed capacity by as early as 2007. This is mainly due to the increase in demand in the residential sector as a result of the electrification of rural and previously disadvantaged communities. However, the industrial and commercial sectors also have a role in this increase. In an attempt to reduce the demand for electricity Eskom has adopted its Demand Side Management (DSM) initiative. This initiative is aimed at lowering the electricity demand in peak times through energy efficiency (EE) or load shift, out of peak demand times. Eskom is implementing the DSM strategy by financing Energy Service Companies (ESCOs) to reduce the demand load of major electricity end-users during peak times. Buildings consume a large percentage of the total energy supply in the world. Most of the energy consumed in buildings is used by the heating, ventilation and air-conditioning (HVAC) systems, as well as lighting. However, a large potential for energy savings exists in buildings. Studies have shown that up to 70% of the electricity consumption of a building can be saved through retrofit studies. However, to capitalise on these opportunities, the ESCOs require tools and procedures that would enable them to accomplish energy savings studies quickly and efficiently. It should be a holistic approach to the typical ESCO building audit. A study of current available software programs showed the lack of holistic tools aimed specifically at retrofit audits, and therefore also the need for such a program. The building simulation program most suited to the retrofit study was chosen and it was used in a retrofit audit. By emulating a retrofit audit with this software, its performance in the field, both positive and negative, could be established. With the experience gained from the retrofit study, as well as input from ESCOs in the industry, a need for such a retrofit tool was established. The simulation program that was tested in the retrofit study is the tool Quickcontrol, as well as the newer version of the program, entitled QEC. The case study showed that even though these packages are well suited to ESCO work, they have certain drawbacks in view of the holistic project approach. The ESCOs require a simple, fast, and integrated procedure for energy audits. This procedure should be embodied in a software program. This study proposes a new integrated procedure for energy audits and the analyses of buildings, in the form of a software tool. This new tool is geared towards the ESCO building audit, in both South A6ica and internationally. It is designed to enable a diplomate engineer to accomplish a building energy and retrofit analysis in two weeks, leading the user through all the main project steps, from data acquisition to writing of the final project report. This is a significant improvement, since it normally takes 50 man-days for an experienced and trained engineering team to complete a full building audit. This tool was used in a case study to test its validity and accuracy. It was found that certain situations would arise in which the criteria that were set for the program would not be adequate. The results from the case study were favourable and satisfied the criteria that were set for the procedure. / Thesis (Ph.D. (Mechanical Engineering))--North-West University, Potchefstroom Campus, 2004.

Neste trabalho é apresentado o desenvolvimento de um programa computacional que simula o desempenho térmico de um sistema de aquecimento solar de água com circulação forçada, adequado para uso em edificações. O programa trabalha realizando o balanço de massa e de energia no reservatório térmico a cada hora, tendo como valores de entrada dados do ano meteorológico típico da localidade selecionada e a vazão de água quente de consumo. Os componentes do sistema são o reservatório térmico de água quente com aquecedor auxiliar interno, o coletor solar e a bomba de circulação. A base de dados meteorológicos escolhida foi a do projeto SWERA, que contém arquivos no formato padrão TMY disponíveis na internet para um número considerável de cidades, incluindo diversas localidades brasileiras. Foi proposto um modelo de temperatura de água da rede de abastecimento relacionado com a temperatura do solo, dado disponível nos arquivos de entrada utilizados. O programa utilizou como referência para a validação dos modelos de cálculo resultados obtidos pelo programa comercial de simulação TRNSYS. Foram comparados resultados para os modelos de irradiação incidente em superfície inclinada, do coletor solar e do sistema completo. Para isto foram simulados sistemas localizados em quatro cidades distintas com climas diferentes. O tempo total usado nas simulações foi de um ano e os resultados das comparações dos valores resultantes foram considerados satisfatórios. / This paper presents the development of a software that simulates the thermal performance of a solar water heating system with forced circulation, suitable for buildings. The implemented model computes the mass and energy balance in the thermal tank every hour. Its input data are values from a typical meteorological year of a chosen location and the hot water load. The system components are the thermal tank, the solar collector and the circulation pump. The Swera project was used as the meteorological database, which contains files in the standard TMY format. Those are available on the internet for a number of cities, including several Brazilian locations. A model for the network water supply temperature was proposed. It is related with the ground temperature, available in the data input files. The validation of the models used results obtained by the commercial simulation software TRNSYS. Results for the incident radiation on tilted surface, the solar collector and the complete system models were compared. For that, systems were simulated in four cities with different climates. The total time used in the simulations was one year and the results obtained from this comparison were satisfactory.