Ce sujet de thèse s'intéresse à l'étude des effets des charges aérodynamiques sur le comportement dynamique non linéaire d'une éolienne à axe vertical de type Darrieus. Cette dernière présente, comparativement aux autres éoliennes, des profits très importants à exploiter, notamment dans les milieux urbains. Il s'agit d'une technologie fiable caractérisée surtout par son fonctionnement omnidirectionnel ainsi que son adaptation à tout type de vent. Généralement, ces éoliennes, ayant des phénomènes aérodynamiques complexes, sont affectées par des vibrations au niveau de leur système de transmission de puissance. En fait, ces vibrations commencent à se manifester à partir des pales du rotor jusqu'au génératrice. L'écoulement autour de ses pales présente également un fort caractère instationnaire. Cette caractéristique augmente d'avantage les vibrations aérodynamiques, qui sont automatiquement transmise au système d'engrenage d'éolienne. À ce niveau, nous avons développé un code de calcul numérique permettant de simuler la complexité des aspects aérodynamiques instationnaires tout en gardant un compromis entre la fiabilité des prédictions et la rapidité de calcul. Les simulations sont réalisées suivant une méthode de mécanique des fluides numérique (CFD) instationnaire bidimensionnel. Les résultats de simulation comparés avec ceux disponibles dans la littérature sont en bonne concordance, le rendement aérodynamique étant optimisé, qui présente un apport scientifique notable. Cette étude numérique a été l'objectif de l'analyse de l'impact des charges aérodynamiques vis-à-vis le comportement dynamique du système d'engrenage de l'éolienne en régime non-stationnaire. Dans ce contexte, une étude paramétrique a été développée afin d'établir le fonctionnement optimal de l'éolienne, caractérisé par un couple aérodynamique plus performant associé à des niveaux de vibrations dynamiques acceptables. En général, il est difficile d'identifier précisément la réponse dynamique des éoliennes à cause du caractère turbulent et stochastique des charges aérodynamiques. Par conséquent, il est indispensable de tenir en compte la variabilité des paramètres d'entrée pour assurer la robustesse du système étudié. Adoptons l'objectif de dimensionnement robuste. Une méthode d'évaluation basée sur des approches stochastiques, particulièrement la méthode du Chaos Polynomial, est utilisée pour simuler le comportement dynamique non-linéaire du système d'engrenage d'éolienne, en tenant compte des incertitudes. Ces dernières sont au niveau des charges aérodynamiques, inhérentes au calcul des niveaux vibratoires du système d'engrenage. Ce qui implique un apport scientifique important. Les résultats obtenus par l'approximation par Chaos Polynomial démontrent une forte dispersion des charges aérodynamiques aléatoires dans la réponse dynamique du système d'engrenage, contrairement aux études déterministes. Ce qui prouve l'insuffisance de telles études pour une analyse de robustesse. Les résultats mettent également en évidence la forte corrélation entre les phénomènes aérodynamiques complexes et les vibrations dynamiques. Le couplage établi constitue l'originalité de notre travail. / This thesis focuses on the study of the aerodynamic loads effects on the nonlinear dynamic behavior of Darrieus--type vertical axis wind turbine. The latter has received more attention due to its efficiency in urban regions compared to other wind turbines. In fact, the wind flow speed in urban regions continuously changes direction and is extremely turbulent. The inherent characteristics of its omni-directionality make it more suitable to harnessing this kind of flow. It is known that Darrieus wind turbine is characterized by an inherently unsteady aerodynamic behavior and a complex flow around rotor blades. The non-stationary behavior of the mentioned turbine increases vibration. These aerodynamic vibrations are transmitted to the gearing mechanism. We have, firstly, developed a numerical simulation, allowing to simulate the complexity of the unsteady aerodynamic phenomena keeping a compromise between the reliability of prediction and the rapidity of calculation. This numerical simulation has been carried out using a two-dimensional unsteady Computational Fluid Dynamics (CFD) method. Simulation results compared to those available in the literature are in good agreement. The Darrieus turbine efficiency is also optimized; thus introducing a significant scientific contribution. The latter is the objective of analyzing the aerodynamic load impact in the dynamic behavior of the Darrieus turbine in non-stationary regime. In this context, a parametric study has been developed in order to find optimal functioning of the studied turbine, which is characterized by the most performing aerodynamic torque associated with acceptable levels of dynamic vibration. In general, it is difficult to predict the dynamic response of the wind turbine with a good level of accuracy due to the aerodynamic loads turbulence and uncertain characteristics. It becomes necessary to take into account the uncertainty in the input parameters to ensure the robustness of the Darrieus turbine geared system. In a robustness study objective, the Polynomial Chaos method is adopted to predict the nonlinear dynamic behavior of the gearing system taking into account uncertainties which are associated to the performance coefficient of the input aerodynamic torque. This leads to an important scientific research contribution. The results have shown a large dispersion of the random parameter in the dynamic response of the gearing system compared to the deterministic study. That proves the insufficiency of that study for a robustness analyses. They have also proved that the Polynomial Chaos method is an efficient probabilistic tool for uncertainty propagation. Finally, the new proposed robust mechanical analysis indicates a good capacity to investigate the dynamic behavior of the Darrieus turbine thanks to its superior predictive capabilities in coupling complex aerodynamic phenomena with a mechanical gearing system vibration. Where the originality of such correlation in our work.

Made available in DSpace on 2014-06-11T19:25:29Z (GMT). No. of bitstreams: 0 Previous issue date: 2011-07-13Bitstream added on 2014-06-13T19:32:38Z : No. of bitstreams: 1 pereira_aj_me_guara.pdf: 1147049 bytes, checksum: 5c149bbd658e37d0e33085f764c18b50 (MD5) / Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES) / Uma abordagem analítica para o movimento rotacional de satélites artificiais estabilizados por rotação é apresentada, considerando os satélites em órbita elíptica e a influência conjunta do torque aerodinâmico, o torque de gradiente de gravidade, o torque magnético residual e o torque magnético devido às correntes de Foucault. Modelos matemáticos são apresentados para todos os torques e os componentes médios de cada torque são determinados para um período orbital. O torque médio já inclui os principais efeitos de cada torque sobre o movimento rotacional e são necessários nas equações do movimento. As equações do movimento são descritas em termos do módulo da velocidade angular de rotação do satélite, da declinação e da ascensão reta do eixo de rotação do satélite. Uma solução analítica para as equações do movimento rotacional é determinada, considerando os valores do torques externos médios em um período orbital, sendo válida para um período orbital. Por esta solução observa-se que o torque gradiente de gravidade e torque magnético devido às correntes de Foucault afetam o módulo da velocidade angular de rotação, contribuindo também para as variações temporais da ascensão reta e declinação do eixo de rotação, associadas com a precessão e deriva do eixo de rotação do satélite. O torque magnético residual e o torque aerodinâmico afetam apenas a ascensão reta e declinação do eixo de rotação, pois seu componente no eixo z são nulo. Aplicações são realizadas para os Satélites de Coleta de Dados Brasileiros SCD1 e SCD2, através de uma primeira abordagem com atualização diária dos dados de atitude e órbita e uma segunda abordagem sem a atualização diária destes dados. Os resultados mostram uma boa concordância entre os resultados obtidos pela teoria e os dados fornecidos pelo Centro de Controle de... / An analytical approach for the rotational motion of artificial satellites stabilized by rotation is presented, considering the satellites in elliptical orbit and the influence of the aerodynamic torque, gravity gradient torque, residual magnetic torque and magnetic torque due to the Foucault currents. Mathematical models for all the torques are shown and average components of each torque are determined for an orbital period. These components are needed in the equations of rotational motion. The average torque already included the main effects of each torque upon the rotational motion. The equations of rotational motion are described in terms of the satellite’s spin velocity, the declination and right ascension of the spin axis of the satellite. An analytical solution for the equations of the rotational motion is determined, considering mean values in an orbital period for the external torques. This solution is valid for an orbital period. Through this solution, it is noticed that the gravity gradient torque and the magnetic torques affects the spin velocity and the spin axis. The temporal variations of right ascension and declination of the spin axis causes the precession and drift of the spin. The residual magnetic torque and the aerodynamic torque, doesn´t affect the spin velocity because its component at z-axis is null. Applications are made for the Brazilian Data Collection Satellites SCD1 and SCD2, through a first approach with daily updates of the attitude and orbit data, and a second approach without the daily update of these data. The results show a good agreement between the results obtained by theory and data supplied by the Satellite Control Center of INPE in the first approach during 10 days. For the approach without updates, the results prove to be suitable only for 3 days of simulation. To validate the analytical solution, the pointing error (deviation from the rotational... (Complete abstract click electronic access below)

Orientadora: Maria Cecília F. P. S. Zanardi / Banca: Ana Paula Marins Chiaradia / Banca: Sandro da Silva Fernandes / Resumo: Uma abordagem analítica para o movimento rotacional de satélites artificiais estabilizados por rotação é apresentada, considerando os satélites em órbita elíptica e a influência conjunta do torque aerodinâmico, o torque de gradiente de gravidade, o torque magnético residual e o torque magnético devido às correntes de Foucault. Modelos matemáticos são apresentados para todos os torques e os componentes médios de cada torque são determinados para um período orbital. O torque médio já inclui os principais efeitos de cada torque sobre o movimento rotacional e são necessários nas equações do movimento. As equações do movimento são descritas em termos do módulo da velocidade angular de rotação do satélite, da declinação e da ascensão reta do eixo de rotação do satélite. Uma solução analítica para as equações do movimento rotacional é determinada, considerando os valores do torques externos médios em um período orbital, sendo válida para um período orbital. Por esta solução observa-se que o torque gradiente de gravidade e torque magnético devido às correntes de Foucault afetam o módulo da velocidade angular de rotação, contribuindo também para as variações temporais da ascensão reta e declinação do eixo de rotação, associadas com a precessão e deriva do eixo de rotação do satélite. O torque magnético residual e o torque aerodinâmico afetam apenas a ascensão reta e declinação do eixo de rotação, pois seu componente no eixo z são nulo. Aplicações são realizadas para os Satélites de Coleta de Dados Brasileiros SCD1 e SCD2, através de uma primeira abordagem com atualização diária dos dados de atitude e órbita e uma segunda abordagem sem a atualização diária destes dados. Os resultados mostram uma boa concordância entre os resultados obtidos pela teoria e os dados fornecidos pelo Centro de Controle de... (Resumo completo, clicar acesso eletrônico abaixo) / Abstract: An analytical approach for the rotational motion of artificial satellites stabilized by rotation is presented, considering the satellites in elliptical orbit and the influence of the aerodynamic torque, gravity gradient torque, residual magnetic torque and magnetic torque due to the Foucault currents. Mathematical models for all the torques are shown and average components of each torque are determined for an orbital period. These components are needed in the equations of rotational motion. The average torque already included the main effects of each torque upon the rotational motion. The equations of rotational motion are described in terms of the satellite's spin velocity, the declination and right ascension of the spin axis of the satellite. An analytical solution for the equations of the rotational motion is determined, considering mean values in an orbital period for the external torques. This solution is valid for an orbital period. Through this solution, it is noticed that the gravity gradient torque and the magnetic torques affects the spin velocity and the spin axis. The temporal variations of right ascension and declination of the spin axis causes the precession and drift of the spin. The residual magnetic torque and the aerodynamic torque, doesn't affect the spin velocity because its component at z-axis is null. Applications are made for the Brazilian Data Collection Satellites SCD1 and SCD2, through a first approach with daily updates of the attitude and orbit data, and a second approach without the daily update of these data. The results show a good agreement between the results obtained by theory and data supplied by the Satellite Control Center of INPE in the first approach during 10 days. For the approach without updates, the results prove to be suitable only for 3 days of simulation. To validate the analytical solution, the pointing error (deviation from the rotational... (Complete abstract click electronic access below) / Mestre