[pt] É notório que a resistência global de uma estrutura composta por várias camadas coladas depende diretamente da qualidade da adesão entre as mesmas. Imperfeições ao longo das interfaces de adesão comprometem significativamente a performance da estrutura. A caracterização não destrutiva destas imperfeições é geralmente tarefa muito difícil. O principal objetivo deste trabalho é apresentar um método analítico-numérico que permite modelar o campo acústico resultante da interação entre ondas ultra-sônicas e interfaces imperfeitas, auxiliando na escolha de parâmetros para o emprego de métodos ultra-sônicos de inspeção. No trabalho, a aproximação quase-estática, proposta por Thompson em meados da década de oitenta,é combinada com o método das perturbações para a modelagem de defeitos localizados ao longo da camada de adesão. O método desenvolvido admite que as camadas sejam feitas de materiais anisotrópicos, e permite a modelagem em altas frequências. Três simulações são apresentadas para exemplificar a aplicação do método. Resultados destas simulações onde feixes ultra-sônicos são incidentes em placas imersas em água revelam frequências e ângulos de incidência para os quais efeitos de espalhamento, que permitem a caracterização de defeitos localizados, são mais significativos. / [en] It is well known that the global strength of multi-layered composite structures strongly depends on the quality of the adhesion between its constituent elements. Imperfections along interfaces of adhesion can strongly compromise structure s performance. The characterization of such defects is a very difficult task. The main goal of this study is the development of an analytic-numerical method to simulate the acoustic field resulting from the interaction between ultrasonic waves and imperfect interfaces, helping in selection of parameters for ultra-sonic inspecting methods. The Quasistatic-approximation (QSA), introduced by Thompson in 1982, is applied together with the perturbation method to allow modelling of interfacial localized aws. A solution algorithm for the problem is developed with the aid of the invariant embedding method. It is applicable to solve wave propagation problems in arbitrarily anisotropic layered plates and it is stable for high frequencies. Three simulations of multi-layered plates immersed in acoustic uid are presented as illustration of the application of the developed method. Results of those simulations indicate the frequencies and angles of incidence where the scattering effects, which allow the characterization of localized defects, are more significant.

When the point under consideration is not near to the source of vibration, the strains developed in the rock mass due to the passage of waves are usually of small magnitude, and within the elastic range. However, the rock mass may be subjected to a wide range of strain levels depending on the source of vibration and the wave frequency, even within the elastic limit. The present study is based on the two general conditions existing at field, long wave length propagation of waves and intermediate wavelength propagation of waves. When the wavelength of propagating wave is much longer than the joint spacing, it is referred to as long wavelength condition and is associated with propagation of low frequency waves across closely spaced joints. When wavelength of propagating wave is nearly equal to joint spacing, it is known as intermediate wavelength condition and is associated with propagation of high frequency waves. Long wave length propagation of waves has been studied by conducting laboratory experiments using Resonant Column Apparatus on developed plaster gypsum samples. The influence of joint types, joint spacing and joint orientation on wave propagation has been analyzed at three confining stresses under various strain levels. The wave velocities and damping ratios at various strain levels have been obtained and presented. Shear wave velocities are more dependent on confining stress than compression wave velocities across frictional joints whereas, compression wave velocities are more dependent on confining stress than shear wave velocities across filled joints. Wave velocities are at minimum and wave damping is at maximum across horizontal joints whereas wave velocities are at maximum and wave damping is at minimum across vertical joints. Shear wave velocity and shear wave damping are more dependent on joint orientations than compression wave velocity and compression wave damping. As Resonant Column Apparatus has some limitations in testing stiff samples, a validated numerical model has been developed using Discrete Element Method (DEM) that can provide resonant frequencies under torsional and flexural vibrations. It has been found from numerical simulations, that reduction of normal and shear stiffness of joint with increasing strain levels leads to wave velocity reduction in jointed rock mass. Intermediate wave length propagation of waves has been studied by conducting tests using Bender/ extender elements and the numerical simulations developed using 3DEC (Three Dimensional Distinct Element Code).Parametric study on energy transmission, wave velocities and wave amplitudes of shear and compression waves, has been carried out using the validated numerical model. The propagation of waves across multiple parallel joints was simulated and the phenomenon of multiple reflections of waves between joints could be observed. The transformations of obliquely incident waves on the joint have been successfully modeled by separating the transmitted transformed P and S waves. The frequency dependent behavior of jointed rocks has been studied by developing a numerical model and by applying a wide range of wave frequencies. It has been found that low frequency shear waves may involve slips of rock blocks depending on the strength of rock joint, leading to less transmission of energy; while low frequency compression waves are well transmitted across the joints. High frequency shear and compression waves experience multiple reflections and absorptions at joints.

Ultra Low Frequency (ULF) waves are a ubiquitous feature of Earth's outer atmosphere, known as the magnetosphere, having been observed on the ground for almost two centuries, and in space over the last 50 years. These waves represent small oscillations in Earth's magnetic field, most often as a response to the external influence of the solar wind. They are important for the transfer of energy throughout the magnetosphere and for coupling different regions together. In this thesis, various features of these oscillations are considered. A detailed background on the history and previous study of ULF waves relevant to our work is given in the introductory chapter. In the following chapters, we predominantly use numerical methods to model ULF waves, which are carefully developed and thoroughly tested. We consider the application of these methods to reports on ground and spaced based observations, which allows a more in depth study of the data. In one case, the simulation results provide evidence for an alternative explanation of the data to the original report, which displays the power of theoretical modelling. An analytical model is also constructed, which is tested on simulation data, to identify the incidence and reflection of a class of ULF wave in the flank magnetosphere. This technique is developed with the aim of future applications to satellite data. Further to this, we develop models both in Cartesian and dipole geometries to investigate some of the theoretical aspects of the coupling between various waves modes. New light is shed on the coupling of compressional (fast) and transverse (Alfvén) magnetohydrodynamic (MHD) wave modes in a 3D dipole geometry. Overall, this thesis aims to develop useful numerical models, which can be used to aid in the interpretation of ULF wave observations, as well as probing new aspects of the existing wave theory.

Fifty years after the discovery of the first pulsating neutron star, the field of pulsar science has grown into a multidisciplinary research field, working to address a wide range of problems in astrophysics - from stellar evolution models to high precision tests of General Relativity to analysing the detailed structure of the Interstellar Medium in the Milky Way. Over 2500 Galactic pulsars have been discovered. The next generation telescopes, such as the Square Kilometre Array, promise to discover the complete observable Milky Way population, of several tens of thousands, over the next decade. These point sources in the sky have extreme properties, with matter densities comparable to that of an atomic nucleus, and surface magnetic fields a trillion times stronger than Earth's magnetic field. Observationally, the most valuable property is their rotational stability - allowing us to anticipate and sum their beamed radio emission, as the pulsar spins around its axis, on millisecond to second timescales. The detected radio wave signals carry with them information of the ionised interstellar medium (IISM) paths they traveled along. The imprints reveal that the pulsar signals we detect travel along multiple paths. While the bulk of the emitted signal propagates along a straight line, we also receive delayed emission scattered through small angles, back into our line of sight. This scattering is caused by fluctuations in the free electron densities of the IISM. The impact of these inhomogeneities is exaggerated at low observing frequencies, where averaged pulsar profiles are observed to be broadened, and showcase exponential scattering tails characterised by a scattering timescale г. Simple theoretical models predict a power law dependence of г on frequency, with a spectral index α = 4. Despite these predictions, my analysis of pulsar data in this thesis, reveal a more complex frequency dependence on г. I investigate the scattering characteristics of a set of pulsars observed by the Low Frequency Array (LOFAR), at 110~MHz to 190~MHz. These data are ideal datasets for accurate studies of pulsar scattering, providing broad frequency bands at low frequencies. I find anomalously low power law spectral indices, α, describing the frequency dependence of г. These indices are likely due to anisotropic scattering mechanisms or small scattering clouds in the IISM. To conduct effective data analysis, I develop scattering fitting techniques by first analysing IISM effects on simulated pulsar data. I investigate the effects of two different types of scattering mechanisms, isotropic and anisotropic scattering, and consider each of their particular frequency-dependent impacts on pulsar data. The work on simulated data provides a robust fitting technique for extracting scattering parameters and a framework for the interpretation of the LOFAR data used in this study. The fitting technique simultaneously models scattering effects and standard frequency-dependent pulse profile evolution. I present results for 13 pulsars with simple pulse shapes, and find that г, associated with scattering by a single thin screen, has a power law dependence on frequency with α ranging from 1.50 to 4.0. My results show that extremely anisotropic scattering can cause low α measurements. The anomalous scattering properties can also be caused by the presence of small scattering clumps in the IISM, as opposed to the conventionally modelled large scattering screens. Evidence for both anisotropic scattering and small scattering clouds with high electron densities come from other areas of research. Indications of the anisotropic nature of the local IISM mostly come from high resolution pulsar scintillation analyses, while evidence for high density scattering clouds is often based on extreme scattering events measured through quasar observations. My results suggest that these anomalous scattering properties are more prevalent than formerly thought, prompting us to reconsider the physical conditions of the IISM, where traditionally high electron densities are reserved for H_II regions and anisotropy is not modelled. High quality, low frequency pulsar data, where anomalous propagation effects become measurable, are a valuable addition in assisting us to distinguish between the different physical mechanisms that can be at play. The more complex these IISM characteristics reveal themselves to be, the harder it will be to disentangle intrinsic profile emission from IISM propagation imprints. Successfully separating these effects, however, promises to improve our understanding of the intrinsic pulsar radio emission - a process that is still poorly understood.

In 1865 Maxwell outlined the theoretical framework for electromagnetic field propagation. Since then many important developments have been made in the field, with an emphasis on systems using high frequencies for long-range interactions. It was not until recent years that applications based on short-range inductive coupling demonstrated the advantages of using low frequency transmissions with magnetic fields to transfer power and information. This thesis investigates magnetic transmissions in the near-field and the possibility of producing induced voltages in printed circuit boards. A near-field magnetic induction system is designed to generate a magnetic flux in the very low frequency region, and used experimentally to evaluate circuit board induction in several interesting environments. The resulting voltages are measured with digital signal processing techniques, using Welch’s method to estimate the spectrum of the received voltage signal. The results show that the amount of induced voltage is proportional to the inverse cube of the transmission distance, and that the system is able to achieve a maximum induced voltage of 65 \micro V at a distance of 2.5 m and under line-of-sight conditions. It is also concluded that conductive obstructions, electromagnetic shielding and background noise all have a large impact on the obtained voltage, either cancelling the signal or causing it to fluctuate.

O início da construção de estruturas para reserva de água no mundo é conhecido há milhares de anos, e, desde então, as barragens são consideradas alternativas viáveis não apenas para reserva de água para consumo, mas também para as finalidades de geração de energia hidrelétrica, contenção de rejeitos, entre outras. Entretanto, mesmo com os contínuos avanços nas técnicas construtivas e na fiscalização da segurança destas estruturas, a possibilidade de rompimento de barragens é uma realidade constante. Nesta perspectiva, o presente texto objetiva analisar os aspectos hidráulicos de metodologias simplificadas para estimativa de parâmetros de inundação proveniente do rompimento de barragens, a saber, as vazões e respectivas profundidades atingidas no vale a jusante, em um evento de rompimento hipotético. Para tal, analisaram-se os resultados de três metodologias simplificadas existentes, aplicadas em três barragens estudo de caso, com características estruturais e geometria do vale a jusante distintas. Os resultados das metodologias simplificadas foram comparados com os estudos de Dam Break das três barragens estudo de caso, obtidos com o uso do software HEC-RAS unidimensional e cedidos por empreendedores. O presente texto também sugere uma nova equação empírica para previsão da vazão máxima resultante do rompimento de barragens por galgamento, e propõe uma nova metodologia simplificada para análise preliminar de rompimento de barragens, com base nos métodos analisados e nas respectivas conclusões obtidas. Os resultados indicam que o uso de metodologias simplificadas na análise preliminar de rompimento de barragens é uma alternativa viável em vales cuja declividade do talvegue é acentuada e cujas características geométricas são aproximadamente constantes. Identificou-se que pequenas alterações no coeficiente de rugosidade do terreno e na declividade da linha de energia refletiram em diferenças nos resultados de profundidades e larguras máximas de 20%, em média. A proposta de nova equação empírica para previsão de vazão máxima na seção da barragem baseou-se na análise de 39 casos reais envolvendo ruptura de barragens por galgamento e resultou em um coeficiente de determinação (R²) de 0,79. Quando comparada com as principais equações semelhantes indicadas na bibliografia, a equação proposta obteve vazões máximas próximas ou superiores às dos demais pesquisadores analisados sempre que a altura da barragem foi inferior a 30 m. Evidencia-se a importância na estimativa cautelosa da vazão máxima na seção da barragem, uma vez que essa reflete em diferenças significativas nas vazões e respectivas profundidades alcançadas ao longo do vale a jusante da estrutura. Nos casos analisados, diferentes vazões máximas na seção da barragem refletiram em distinções de até 50%, em média, nas profundidades e larguras máximas a jusante. A nova metodologia proposta para definição de características de inundação provenientes do rompimento de barragens pode contribuir em estudos preliminares para tal, especialmente aos empreendedores que possuem número expressivo de barragens. Nesses casos, a metodologia poderá nortear a prioridade a ser dada em estudos detalhados de Dam Break. / For thousands of years, water reservoir structures have been built worldwide. Since then, dams have been considered viable alternatives not only for reserving water for consumption but also for the purposes of hydroelectric power generation and sediment retention, among others. Despite the continuous advances in the construction techniques and in the safety inspection of these structures, the possibility of breaking of dams remains a constant reality. Hence, this paper aims to analyze the hydraulic aspects of simplified methodologies for estimating flood parameters on dam ruptures, namely, the flows and respective depths reached in the downstream valley in a hypothetical breach event. Results of three existing simplified methodologies were studied applied in three dams with different structural characteristics and downstream valley geometry. The results of simplified methodologies were compared with dam break studies of three study case dams, obtained with one-dimensional HEC-RAS and provided by entrepreneurs. The present paper suggests also a new empirical equation for predicting the maximum flow resulting from the overtopping dam failure and proposes a new simplified methodology for preliminary analysis of dam rupture, based on the analyzed methods and respective obtained conclusions. The results indicate that the use of simplified methodologies in the preliminary dam break analysis is a viable alternative in valleys with high thalweg declivities and close to constant geometric characteristics. It was identified that small changes in the coefficient of rough terrain and in the energy line slope reflected in differences in the results of depths and maximum widths of 20%, on average. The proposed new empirical equation for maximum flow prediction in the dam section was based on the analysis of 39 actual cases involving overtopping dam failure and resulted in a coefficient of determination (R²) of 0.79. When compared to similar main equations indicated in the bibliography, the proposed equation obtained maximum flows near or higher than those of other researchers analyzed whenever the height of the dam did not exceed 30 m. The importance of a cautious estimation of the maximum flow rate in the dam section is to be highlighted, since it results in significant variations of flow and respective depths along the valley and downstream of the structure. Different maximum flows were found in the dam section, which reflected in distinctions of up to 50%, in average, in the maximum depths and widths downstream. The new proposed methodology for defining dam break characteristics caused by dam rupture may contribute to preliminary studies, especially to entrepreneurs who own a significant number of dams. In these cases, the methodology may guide the priority to be given in detailed studies of dam break.

O objetivo deste trabalho é tratar da simulação do fenômeno de propagação de ondas em uma haste heterogênea elástico, composta por dois materiais distintos (um linear e um não-linear), cada um deles com a sua própria velocidade de propagação da onda. Na interface entre estes materiais existe uma descontinuidade, um choque estacionário, devido ao salto das propriedades físicas. Empregando uma abordagem na configuração de referência, um sistema não-linear hiperbólico de equações diferenciais parciais, cujas incógnitas são a velocidade e a deformação, descrevendo a resposta dinâmica da haste heterogénea. A solução analítica completa do problema de Riemann associado são apresentados e discutidos. / The objective of this work is the simulation of the wave propagation phenomenon in a heterogeneous elastic rod, composed by two distinct materials (a linear and a non-linear one), each of them with its own wave propagation speed. At the interface between these materials there is a discontinuity, a stationary shock, due to the jump of the physical properties. Employing a reference configuration approach, a nonlinear hyperbolic system of partial differential equations, whose unknowns are the velocity and the strain, describing the dynamical response of the heterogeneous rod. The complete analytical solution of the associated Riemann problem is presented and discussed.

Nous analysons les propriétés dynamiques de milieux architecturés périodiques et de réseaux fibreux aléatoires en petites et grandes déformations, à partie de méthodes d’homogénéisation afin de calculer leurs propriétés statiques et dynamiques. Des modèles effectifs de type micropolaire et du second gradient sont élaborés afin de prendre en compte l’impact de la microstructure sur le comportement effectif. L’influence des degrés de liberté en rotation additionnels et des gradients d’ordre supérieur du déplacement sur les relations de dispersion sont analysés pour des comportements élastique et viscoélastique du matériau constitutif. Les milieux continus généralisés ainsi construits conduisent à des effets dispersifs, en accord avec les observations. Dans la seconde partie du travail, nous analysons l’influence des grandes déformations sur la propagation des ondes élastiques dans des milieux architecturés périodiques. Des méthodes théoriques assortis de schémas numériques sont développés afin de prédire l’influence des déformations finies générées au sein des structures sur l’évolution de leur diagramme de bande. Un schéma incrémental d’évolution de la fréquence et de la vitesse de phase du milieu continu homogénéisé est établi, à partir d’une méthode de perturbation établie pour des structures 1D, 2D et 3D, en considérant plus particulièrement des structures auxétiques. Ce schéma montre un effet important de l’état de déformation appliquée et de la densité effective sur l’évolution de la fréquence et de la vitesse de phase des ondes. Une méthode de perturbation spécifique aux structures périodiques nonlinéaires est développée afin de généraliser le théorème de Bloch pour couvrir les non linéarités tant géométriques que matérielles. Des modèles hyperélastiques du premier et du second gradient de différentes structures sont identifiés par des tests virtuels reposant sur une méthode d’homogénéisation dédiée, qui permettent de formuler des équations d’onde spécifiques – équations de Burgers et de Boussinesq – dont les propriétés dispersives sont analysées / Micropolar and second gradient effective continua are constructed as two different strategies to account for microstructural effects. The influence of additional degrees of freedom or higher order displacement gradients on the dispersion relations is analyzed in both situations of elastic and viscoelastic behaviors of the material. Generalized effective continua lead to dispersive waves, as observed in experiments. In the second part of the thesis, we analyze the influence of large deformations on the propagation of acoustic waves in repetitive network materials. Both theoretical and numerical methods are developed in order to assess the influence of finite strains developing within the networks on the evolution of their band diagrams. An incremental scheme for the update of frequency and phase velocity of the computed homogenized medium is developed based on a perturbation method for 1D, 2D and 3D structures, considering with a special emphasis auxetic networks. This scheme shows an important effect of the applied finite deformation on the frequency and phase velocity of the propagating waves. A perturbation method for nonlinear periodic structures is developed to extend Bloch’s theorem to cover both geometrical and material nonlinearities. Hyperelastic first and second order gradient constitutive models of different network materials are identified based on dedicated homogenization methods, from which specific wave equations are formulated - Burgers and Boussinesq equations - the dispersion properties of which are analyzed

La concentration de plus en plus importante de la population dans les milieux urbains exposés à une forte sismicité peut générer de plus en plus de dommages et de pertes. La réponse sismique en milieu urbain dépend des effets du site (direct amplification et non-linéarité du sol) et du couplage entre le sol et les structures (interaction sol-structure et site-ville). Par conséquent, la compréhension de la sismologie urbaine, c'est-à-dire le mouvement du sol intégrant l'environnement urbain, est critique pour réduire les dommages. Cela passe par la prédiction du mouvement du sol dans le milieu urbain, ingrédient fondamental à l'évaluation de l'aléa sismique. La prise en compte de l'amplification provoquée par la présence de sédiments est largement étudiée. Au contraire, la réponse non-linéarité du sol et du couplage entre le sol et la structure est rarement intégrée à la prédiction du mouvement du sol. A cause de leur complexité, ces problèmes ont toujours été abordés séparément. Dans ce contexte, cette thèse analyse la réponse non-linéaire du système sol-structure en intégrant la non-linéarité du sol et de l'interaction sol-structure. Deux travaux expérimentaux ont été conduits, avec comme but de proposer un proxy, rendant compte de la non-linéarité du sol. Le premier est l'essai en centrifugeuse qui reproduit à échelle réduite la réponse du sol et des structures. L'état de contrainte et de déformation est conservé en appliquant une accélération artificielle au modèle. Cet essai a été effectué à IFSTTAR Nantes dans le cadre de l'ANR ARVISE. Différentes configurations ont été testées, avec et sans bâtiments, sous différents niveaux de sollicitation, pour analyser la réponse du sol et des structures. Le deuxième utilise les enregistrements des réseaux accélérométriques verticaux de deux sites tests californiens : Garner Valley Downhole Arrat (GVDA) et Wildlife Liquefaction Array (WLA), gérés tout deux par l'Université de Californie, Santa Barbara (UCSB), Etats-Unis. La réponse in-situ est importante car elle décrit le comportement réel du site. Plusieurs informations décrivant les conditions de sites sont disponibles et les séismes enregistrés ont permis de tester plusieurs niveaux de déformations pour reconstruire la réponse globale de chaque site. De plus, le site GVDA est équipé d'une structure Soil-Foundation-Structure-Interaction (SFSI) qui a comme objectif d'étudier les problèmes d'interaction sol-structure. Dans les deux expériences, grace au réseau accélérométrique vertical dans le sol et la structure, on peut appliquer la méthode de propagation d'ondes 1D pour extraire la réponse de ces systèmes. Les ondes sont considérées comme des ondes SH qui se propage horizontalement dans une couche 1D. La méthode interférométrie sismique par déconvolution est appliquée pour extraire l'Impulse Response Function (IRF) du système 1D. On analyse ainsi la variation de Vs en fonction de la solliictation et à différente position dans le sol ainsi que la variation des éléments expliquant la réponse dynamique du système sol-structure. On propose au final un proxy de déformation permettant de rendre compte mais aussi de prédire la nonlinéarité des sols en fonction des niveaux sismiques subits. / The concentration of population in urban areas in seismic-prone regions can generate more and more damages and losses. Seismic response in urban areas depends on site effects (direct amplification and nonlinearity of the soil) and the coupling between the soil and structures (soil-structure and site-city interaction). Therefore, the understanding of urban seismology, that is the ground motion incorporating the urban environment, is critical to reduce the damage. This requires the prediction of ground motion in urban areas, a fundamental element in the evaluation of the seismic hazard. Taking into account the amplification caused by the presence of sediment has been widely studied. However, the non-linearity of the soil and the coupling between the ground and the structure is seldom integrated to the prediction of the ground motion. Because of their complexity, these problems have been addressed separately. In this context, this dissertation analyzes the non-linear response of the soil-structure by integrating the non-linearity of the soil and the soil-structure interaction. Two experimental studies were performed, with the aim of providing a proxy that reflects the non-linearity of the soil. The first is the centrifuge test that reproduces the response of soil and structures at reduced scale. The state of stress and strain is conserved by applying an artificial acceleration model. This test was performed at IFSTTAR Nantes in the framework of the ANR ARVISE. Different configurations were tested with and without buildings, under different stress levels, to analyze the response of the soil and structures. The second uses the vertical accelerometric networks of two sites in California: Garner Valley Downhole (GVDA) and the Wildlife Liquefaction Array (WLA), both managed by the University of California, Santa Barbara (UCSB), USA. In-situ response is important since it describes the actual behavior of the site. Information describing the conditions of sites is widely available and the earthquakes recorded were used to test several levels of shaking to reconstruct the overall response of each site. In addition, the GVDA site is equipped with a Soil-Foundation-Structure-Interaction structure (SFSI) which aims to study the problems of soil-structure interaction. In both experiments, thanks to the vertical accelerometer network in the ground and the structure we are able to apply the 1D wave propagation method to extract the response of these systems. The waves are considered as an SH wave which propagates in a 1D horizontal layer. Seismic interferometry by deconvolution method is applied to extract the Impulse Response Function (IRF) of the 1D system. Thus the analysis of the variation in function of elastic properties of the soil and the structure is done under several magnitude of shaking, including variation in depth and the elements of the total response of the structure including the soil-structure interaction. At the end, a deformation proxy to evaluate and also to predict the nonlinear response of the soil, the structure and the soil-structure interaction is proposed.

As ondas geradas por tempestades causam as alterações mais significativas na costa arenosa. Este trabalho avaliou a influência da variabilidade interanual do clima de ondas nos processos costeiros do litoral Sudeste e Sul do Brasil. O clima de ondas foi determinado a partir de resultados entre 1997 e 2010 do modelo numérico NOAA WAVEWATCH III (NWW3) com seis pontos de água profunda. O modelo numérico MIKE 21 SW foi utilizado para verificar o efeito destas ondas na Enseada de Massaguaçu (SP) e no trecho Sul de Imbituba (SC). Foram simuladas as direções de ondas mais frequentes e foi calculado o transporte longitudinal de sedimentos gerado por elas. As ondas do quadrante Sul foram mais energéticas e não foi identificado um padrão na variação interanual do clima de ondas. Em São Paulo, as direções de onda mais frequentes (Sul e Sul-Sudoeste) não geraram quantidade efetiva de transporte de sedimentos, e foram as ondas de Leste-Sudeste a Sudeste-Sul que geraram a maior quantidade de transporte longitudinal de sedimentos. Em Santa Catarina foram as ondas de Leste a Sul que geraram maior transporte longitudinal de sedimentos. / The coastal dynamics is mainly controlled by waves, being the energetic storm waves the most influential. This study aims to assess the wave climate influence on coastal processes in the South and Southeastern coast of Brazil. The wave climate was defined through NOAA WAVEWATCH III (NWW3) numerical model results for six offshore points, from 1997 to 2010. In order to propagate the waves onshore the Spectral Wave FM from MIKE 21 numerical model has been applied on Massaguaçu bay (SP) and Imbituba (SC). Most frequent storm waves have been simulated for each year and sector and sediment longshore transport along each sector was calculated. Waves from the South are the most energetic. There is no clear interanual pattern in the time-series. For SP, the most frequent directions (South and South-Southwest) do not generate considerable longshore sediment transport, with East-Southeast to Southeast-South waves generating most sediment transport, which was northwards for all beaches. In SC the sediment transport was northwards in Vila and Vila Nova beaches and southwards on Itapirubá beach, with waves from Eastern and Southern quadrants generating more longshore sediment transport.