928 resultados para Bidirectional power flow


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The energy resource scheduling is becoming increasingly important, as the use of distributed resources is intensified and massive gridable vehicle (V2G) use is envisaged. This paper presents a methodology for day-ahead energy resource scheduling for smart grids considering the intensive use of distributed generation and V2G. The main focus is the comparison of different EV management approaches in the day-ahead energy resources management, namely uncontrolled charging, smart charging, V2G and Demand Response (DR) programs i n the V2G approach. Three different DR programs are designed and tested (trip reduce, shifting reduce and reduce+shifting). Othe r important contribution of the paper is the comparison between deterministic and computational intelligence techniques to reduce the execution time. The proposed scheduling is solved with a modified particle swarm optimization. Mixed integer non-linear programming is also used for comparison purposes. Full ac power flow calculation is included to allow taking into account the network constraints. A case study with a 33-bus distribution network and 2000 V2G resources is used to illustrate the performance of the proposed method.

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The high penetration of distributed energy resources (DER) in distribution networks and the competitiveenvironment of electricity markets impose the use of new approaches in several domains. The networkcost allocation, traditionally used in transmission networks, should be adapted and used in the distribu-tion networks considering the specifications of the connected resources. The main goal is to develop afairer methodology trying to distribute the distribution network use costs to all players which are usingthe network in each period. In this paper, a model considering different type of costs (fixed, losses, andcongestion costs) is proposed comprising the use of a large set of DER, namely distributed generation(DG), demand response (DR) of direct load control type, energy storage systems (ESS), and electric vehi-cles with capability of discharging energy to the network, which is known as vehicle-to-grid (V2G). Theproposed model includes three distinct phases of operation. The first phase of the model consists in aneconomic dispatch based on an AC optimal power flow (AC-OPF); in the second phase Kirschen’s andBialek’s tracing algorithms are used and compared to evaluate the impact of each resource in the net-work. Finally, the MW-mile method is used in the third phase of the proposed model. A distributionnetwork of 33 buses with large penetration of DER is used to illustrate the application of the proposedmodel.

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The use of distribution networks in the current scenario of high penetration of Distributed Generation (DG) is a problem of great importance. In the competitive environment of electricity markets and smart grids, Demand Response (DR) is also gaining notable impact with several benefits for the whole system. The work presented in this paper comprises a methodology able to define the cost allocation in distribution networks considering large integration of DG and DR resources. The proposed methodology is divided into three phases and it is based on an AC Optimal Power Flow (OPF) including the determination of topological distribution factors, and consequent application of the MW-mile method. The application of the proposed tariffs definition methodology is illustrated in a distribution network with 33 buses, 66 DG units, and 32 consumers with DR capacity.

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Energy resource scheduling is becoming increasingly important, such as the use of more distributed generators and electric vehicles connected to the distribution network. This paper proposes a methodology to be used by Virtual Power Players (VPPs), regarding the energy resource scheduling in smart grids and considering day-ahead, hour-ahead and realtime time horizons. This method considers that energy resources are managed by a VPP which establishes contracts with their owners. The full AC power flow calculation included in the model takes into account network constraints. In this paper, distribution function errors are used to simulate variations between time horizons, and to measure the performance of the proposed methodology. A 33-bus distribution network with large number of distributed resources is used.

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Most of distributed generation and smart grid research works are dedicated to network operation parameters studies, reliability, etc. However, many of these works normally uses traditional test systems, for instance, IEEE test systems. This paper proposes voltage magnitude and reliability studies in presence of fault conditions, considering realistic conditions found in countries like Brazil. The methodology considers a hybrid method of fuzzy set and Monte Carlo simulation based on the fuzzy-probabilistic models and a remedial action algorithm which is based on optimal power flow. To illustrate the application of the proposed method, the paper includes a case study that considers a real 12-bus sub-transmission network.

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Energy resource scheduling is becoming increasingly important, as the use of distributed resources is intensified and of massive electric vehicle is envisaged. The present paper proposes a methodology for day-ahead energy resource scheduling for smart grids considering the intensive use of distributed generation and Vehicle-to-Grid (V2G). This method considers that the energy resources are managed by a Virtual Power Player (VPP) which established contracts with their owners. It takes into account these contracts, the users' requirements subjected to the VPP, and several discharge price steps. The full AC power flow calculation included in the model takes into account network constraints. The influence of the successive day requirements on the day-ahead optimal solution is discussed and considered in the proposed model. A case study with a 33-bus distribution network and V2G is used to illustrate the good performance of the proposed method.

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Em Angola, apenas cerca de 30% da população tem acesso à energia elétrica, nível que decresce para valores inferiores a 10% em zonas rurais mais remotas. Este problema é agravado pelo facto de, na maioria dos casos, as infraestruturas existentes se encontrarem danificadas ou não acompanharem o desenvolvimento da região. Em particular na capital angolana, Luanda que, sendo a menor província de Angola, é a que regista atualmente a maior densidade populacional. Com uma população de cerca de 5 milhões de habitantes, não só há frequentemente problemas relacionados com a falha do fornecimento de energia elétrica como há ainda uma percentagem considerável de municípios onde a rede elétrica ainda nem sequer chegou. O governo de Angola, no seu esforço de crescimento e aproveitamento das suas enormes potencialidades, definiu o setor energético como um dos fatores críticos para o desenvolvimento sustentável do país, tendo assumido que este é um dos eixos prioritários até 2016. Existem objetivos claros quanto à reabilitação e expansão das infraestruturas do setor elétrico, aumentando a capacidade instalada do país e criando uma rede nacional adequada, com o intuito não só de melhorar a qualidade e fiabilidade da rede já existente como de a aumentar. Este trabalho de dissertação consistiu no levantamento de dados reais relativamente à rede de distribuição de energia elétrica de Luanda, na análise e planeamento do que é mais premente fazer relativamente à sua expansão, na escolha dos locais onde é viável localizar novas subestações, na modelação adequada do problema real e na proposta de uma solução ótima para a expansão da rede existente. Depois de analisados diferentes modelos matemáticos aplicados ao problema de expansão de redes de distribuição de energia elétrica encontrados na literatura, optou-se por um modelo de programação linear inteira mista (PLIM) que se mostrou adequado. Desenvolvido o modelo do problema, o mesmo foi resolvido por recurso a software de otimização Analytic Solver e CPLEX. Como forma de validação dos resultados obtidos, foi implementada a solução de rede no simulador PowerWorld 8.0 OPF, software este que permite a simulação da operação do sistema de trânsito de potências.

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Com a alteração da legislação energética em Portugal, nomeadamente a implementação da legislação de Micro e Minigeração, a produção distribuída cresceu de forma exponencial na rede elétrica nacional, diminuindo por um lado as perdas no transporte e distribuição, e por outro aumentando a complexidade na gestão do trânsito de potência ao Distribuidor. No entanto a motivação desta dissertação prende-se com o facto de que as centrais de produção distribuída, em particular as de tecnologia fotovoltaica, pela sua dimensão, serem instaladas nos pontos de consumo, em paralelo com a instalação elétrica de utilização do cliente e como tal, têm sido verificadas diversas anomalias no funcionamento e exploração das mesmas, por influência da má qualidade de energia resultante das más condições de funcionamento e exploração em que se encontram as instalações de consumo. A presente dissertação pretende apresentar uma descrição das anomalias mais frequentes verificadas nas centrais fotovoltaicas de minigeração com origem na qualidade da energia que transita das instalações elétricas de consumo ligadas ao mesmo ponto de interligação com a rede elétrica nacional. Como base de fundamento, foram demonstradas através de três casos práticos reais, algumas das mais frequentes e prejudiciais anomalias descritas na presente dissertação. Foram escolhidos 3 casos reais com diferentes tipos de instalação de consumo sendo que um deles não apresenta qualquer anomalia de forma a comprovar o bom funcionamento em condições normais de ambas as instalações. Foram encontradas e demonstradas várias soluções paras os diferentes tipos de anomalias, no entanto esta dissertação vai permitir não só a resolução deste tipo de anomalias em centrais fotovoltaicas em exploração e já com prejuízos avultados mas também introduzir em futuras instalações a análise da qualidade da energia nas instalações de consumo em fase preliminar de estudo de implementação de centrais fotovoltaicas de minigeração e de autoconsumo, precavendo futuros problemas de rentabilidade técnico-económica. Este estudo, irá certamente servir de motor de impulsão para a preocupação com a Qualidade da Energia essencialmente dentro das instalações elétricas de consumo sensibilizando os seus gestores energéticos. Poderá ainda impulsionar a reformulação do Regulamento de Qualidade de Serviço para exigências ainda mais apertadas de forma a incorporar algumas das anomalias aqui descritas, sendo por isso um elemento de alerta para todos os “Players” do Sistema Elétrico Nacional tendo como limite a melhoria continua da Segurança e da Qualidade da energia na rede elétrica beneficiando da sensibilização de todos os intervenientes.

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Tipicamente as redes elétricas de distribuição apresentam uma topologia parcialmente malhada e são exploradas radialmente. A topologia radial é obtida através da abertura das malhas nos locais que otimizam o ponto de operação da rede, através da instalação de aparelhos de corte que operam normalmente abertos. Para além de manterem a topologia radial, estes equipamentos possibilitam também a transferência de cargas entre saídas, aquando da ocorrência de defeitos. As saídas radiais são ainda dotadas de aparelhos de corte que operam normalmente fechados, estes têm como objetivo maximizar a fiabilidade e isolar defeitos, minimizando a área afetada pelos mesmos. Assim, na presente dissertação são desenvolvidos dois algoritmos determinísticos para a localização ótima de aparelhos de corte normalmente abertos e fechados, minimizando a potência ativa de perdas e o custo da energia não distribuída. O algoritmo de localização de aparelhos de corte normalmente abertos visa encontrar a topologia radial ótima que minimiza a potência ativa de perdas. O método é desenvolvido em ambiente Matlab – Tomlab, e é formulado como um problema de programação quadrática inteira mista. A topologia radial ótima é garantida através do cálculo de um trânsito de potências ótimo baseado no modelo DC. A função objetivo é dada pelas perdas por efeito de Joule. Por outro lado o problema é restringido pela primeira lei de Kirchhoff, limites de geração das subestações, limites térmicos dos condutores, trânsito de potência unidirecional e pela condição de radialidade. Os aparelhos de corte normalmente fechados são localizados ao longo das saídas radiais obtidas pelo anterior algoritmo, e permite minimizar o custo da energia não distribuída. No limite é possível localizar um aparelho de corte normalmente fechado em todas as linhas de uma rede de distribuição, sendo esta a solução que minimiza a energia não distribuída. No entanto, tendo em conta que a cada aparelho de corte está associado um investimento, é fundamental encontrar um equilíbrio entre a melhoria de fiabilidade e o investimento. Desta forma, o algoritmo desenvolvido avalia os benefícios obtidos com a instalação de aparelhos de corte normalmente fechados, e retorna o número e a localização dos mesmo que minimiza o custo da energia não distribuída. Os métodos apresentados são testados em duas redes de distribuição reais, exploradas com um nível de tensão de 15 kV e 30 kV, respetivamente. A primeira rede é localizada no distrito do Porto e é caraterizada por uma topologia mista e urbana. A segunda rede é localizada no distrito de Bragança e é caracterizada por uma topologia maioritariamente aérea e rural.

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Study on variable stars is an important topic of modern astrophysics. After the invention of powerful telescopes and high resolving powered CCD’s, the variable star data is accumulating in the order of peta-bytes. The huge amount of data need lot of automated methods as well as human experts. This thesis is devoted to the data analysis on variable star’s astronomical time series data and hence belong to the inter-disciplinary topic, Astrostatistics. For an observer on earth, stars that have a change in apparent brightness over time are called variable stars. The variation in brightness may be regular (periodic), quasi periodic (semi-periodic) or irregular manner (aperiodic) and are caused by various reasons. In some cases, the variation is due to some internal thermo-nuclear processes, which are generally known as intrinsic vari- ables and in some other cases, it is due to some external processes, like eclipse or rotation, which are known as extrinsic variables. Intrinsic variables can be further grouped into pulsating variables, eruptive variables and flare stars. Extrinsic variables are grouped into eclipsing binary stars and chromospheri- cal stars. Pulsating variables can again classified into Cepheid, RR Lyrae, RV Tauri, Delta Scuti, Mira etc. The eruptive or cataclysmic variables are novae, supernovae, etc., which rarely occurs and are not periodic phenomena. Most of the other variations are periodic in nature. Variable stars can be observed through many ways such as photometry, spectrophotometry and spectroscopy. The sequence of photometric observa- xiv tions on variable stars produces time series data, which contains time, magni- tude and error. The plot between variable star’s apparent magnitude and time are known as light curve. If the time series data is folded on a period, the plot between apparent magnitude and phase is known as phased light curve. The unique shape of phased light curve is a characteristic of each type of variable star. One way to identify the type of variable star and to classify them is by visually looking at the phased light curve by an expert. For last several years, automated algorithms are used to classify a group of variable stars, with the help of computers. Research on variable stars can be divided into different stages like observa- tion, data reduction, data analysis, modeling and classification. The modeling on variable stars helps to determine the short-term and long-term behaviour and to construct theoretical models (for eg:- Wilson-Devinney model for eclips- ing binaries) and to derive stellar properties like mass, radius, luminosity, tem- perature, internal and external structure, chemical composition and evolution. The classification requires the determination of the basic parameters like pe- riod, amplitude and phase and also some other derived parameters. Out of these, period is the most important parameter since the wrong periods can lead to sparse light curves and misleading information. Time series analysis is a method of applying mathematical and statistical tests to data, to quantify the variation, understand the nature of time-varying phenomena, to gain physical understanding of the system and to predict future behavior of the system. Astronomical time series usually suffer from unevenly spaced time instants, varying error conditions and possibility of big gaps. This is due to daily varying daylight and the weather conditions for ground based observations and observations from space may suffer from the impact of cosmic ray particles. Many large scale astronomical surveys such as MACHO, OGLE, EROS, xv ROTSE, PLANET, Hipparcos, MISAO, NSVS, ASAS, Pan-STARRS, Ke- pler,ESA, Gaia, LSST, CRTS provide variable star’s time series data, even though their primary intention is not variable star observation. Center for Astrostatistics, Pennsylvania State University is established to help the astro- nomical community with the aid of statistical tools for harvesting and analysing archival data. Most of these surveys releases the data to the public for further analysis. There exist many period search algorithms through astronomical time se- ries analysis, which can be classified into parametric (assume some underlying distribution for data) and non-parametric (do not assume any statistical model like Gaussian etc.,) methods. Many of the parametric methods are based on variations of discrete Fourier transforms like Generalised Lomb-Scargle peri- odogram (GLSP) by Zechmeister(2009), Significant Spectrum (SigSpec) by Reegen(2007) etc. Non-parametric methods include Phase Dispersion Minimi- sation (PDM) by Stellingwerf(1978) and Cubic spline method by Akerlof(1994) etc. Even though most of the methods can be brought under automation, any of the method stated above could not fully recover the true periods. The wrong detection of period can be due to several reasons such as power leakage to other frequencies which is due to finite total interval, finite sampling interval and finite amount of data. Another problem is aliasing, which is due to the influence of regular sampling. Also spurious periods appear due to long gaps and power flow to harmonic frequencies is an inherent problem of Fourier methods. Hence obtaining the exact period of variable star from it’s time series data is still a difficult problem, in case of huge databases, when subjected to automation. As Matthew Templeton, AAVSO, states “Variable star data analysis is not always straightforward; large-scale, automated analysis design is non-trivial”. Derekas et al. 2007, Deb et.al. 2010 states “The processing of xvi huge amount of data in these databases is quite challenging, even when looking at seemingly small issues such as period determination and classification”. It will be beneficial for the variable star astronomical community, if basic parameters, such as period, amplitude and phase are obtained more accurately, when huge time series databases are subjected to automation. In the present thesis work, the theories of four popular period search methods are studied, the strength and weakness of these methods are evaluated by applying it on two survey databases and finally a modified form of cubic spline method is intro- duced to confirm the exact period of variable star. For the classification of new variable stars discovered and entering them in the “General Catalogue of Vari- able Stars” or other databases like “Variable Star Index“, the characteristics of the variability has to be quantified in term of variable star parameters.

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Nach einem einleitenden ersten Kapitel wird im zweiten Kapitel der Stand der Technik für Regelungs- und Monitoringsysteme mit vernetzten Systemen dargestellt. Daraus wird die Motivation zur Entwicklung neuer, kostengünstiger Systeme abgeleitet. Im dritten Kapitel folgt eine Darstellung der verschiedenen Arten marktverfügbarer Embedded Systems und dafür geeigneter Betriebs­systeme. Anforderungen an verteilte Regelungssysteme, unterschiedliche Strukturen dieser Systeme und deren Vor- und Nachteile sind Gegenstand des vierten Kapitels. Anhand von Beispielen aus den Bereichen Erzeugungsmanagement für den Betrieb von KWK-Anlagen, Energieverbrauchsmonitoring und Smart-Metering wird der Einsatz von verteilten Regelungs- und Monitoringsystemen im fünften Kapitel dargestellt. Im folgenden sechsten Kapitel wird die Bedeutung normierter Kommunikation für den Einsatz in verteilten Systemen sowie dafür vorhandene Standards aus der elektrischen Energieversorgungstechnik und der Automatisierungstechnik behandelt. Der Stand der Internet-Technik für verteilte Systeme ist Gegenstand des siebten Kapitels. Dabei werden zunächst die verschiedenen drahtlosen und drahtgebundenen Kommunikationsmedien vorgestellt und ihre Eigenschaften und die Rand­bedingungen für ihren Einsatz erörtert. Ebenso werden technische Probleme beim Einsatz der Internet-Technik aufgezeigt und Lösungsmöglichkeiten für diese Probleme dargestellt. Es folgt eine Übersicht von Netzwerkdiensten, die für den Betrieb von verteilten Systemen notwendig sind. Außerdem werden Techniken zur Überwachung von verteilten Systemen behandelt. Kapitel acht zeigt Sicherheitsrisiken bei der Nutzung des Internets auf und bewertet verschiedene Techniken zur Absicherung des Netzwerkverkehrs. Kapitel neun stellt ein Internet-basiertes Client-Server-System zur Online-Visualisierung von Anlagendaten im Webbrowser mit Hilfe von Java-Applets und XML-RPC vor. Die Visualisierung von Anlagendaten auf Mobiltelefonen mit Hilfe des Wireless Application Protocol sowie die dafür notwendige Software und Infrastruktur ist Gegenstand des zehnten Kapitels. Im elften Kapitel wird eine neuartige Software für die Simulation von dezentralen Energiesystemen und deren Regelungs­systemen auf Basis von virtuellen Maschinen, virtuellen Netzwerken und einer thermischen Simulationsumgebung vorgestellt sowie deren Anwendung für die Reglerentwicklung erklärt. Verschiedene Techniken für die Installation von Betriebssystemen und Software für die Embedded Systems eines verteilten Systems werden im Kapitel zwölf untersucht. Im Kapitel 13 werden verschiedene Technologien zur Konfiguration und Parametrierung von Regelungssystemen in der industriellen Prozess- und Fertigungs­automatisierung hinsichtlich ihrer Eignung für dezentrale Energiesysteme analysiert. Anschließend wird eine Software zur Installation und Parametrierung von Monitoringsystemen sowie der dazugehörigen Infrastruktur vorgestellt. Kapitel 14 beschäftigt sich mit Anforderungen an die Hardware für verteilte Systeme und mit Maßnahmen zur Erhöhung der Betriebs- und der Datensicherheit. Im 15. Kapitel werden die in den bisherigen Kapiteln vorgestellten Techniken anhand eines großen verteilten Monitoringsystems und anhand eines Power Flow and Power Quality Management Systems auf Basis von verteilten Embedded Systems evaluiert. Kapitel 16 fasst die Ergebnisse der Arbeit zusammen und enthält einen Ausblick auf zukünftige Entwicklungen.

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The stability of stationary flow of a two-dimensional ice sheet is studied when the ice obeys a power flow law (Glen's flow law). The mass accumulation rate at the top is assumed to depend on elevation and span and the bed supporting the ice sheet consists of an elastic layer lying on a rigid surface. The normal perturbation of the free surface of the ice sheet is a singular eigenvalue problem. The singularity of the perturbation at the front of the ice sheet is considered using matched asymptotic expansions, and the eigenvalue problem is seen to reduce to that with fixed ice front. Numerical solution of the perturbation eigenvalue problem shows that the dependence of accumulation rate on elevation permits the existence of unstable solutions when the equilibrium line is higher than the bed at the ice divide. Alternatively, when the equilibrium line is lower than the bed, there are only stable solutions. Softening of the bed, expressed through a decrease of its elastic modulus, has a stabilising effect on the ice sheet.

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Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)