Internal waves are generated in the ocean by oscillating tidal flow over bottom topography such as ridges, seamounts, and continental slopes. They are similar to the more familiar surface waves, but not being constrained to move on the surface, propagate throughout the bulk of the world oceans. Internal waves transmit energy over thousands of kilometers, ultimately breaking and releasing their energy into turbulence and mixing. Where these internal waves are generated, as well as where and how they break and cause mixing, has important effects on the general circulation of the ocean, which is in turn a major component in earth's climate. As a first step in a more thorough understanding of the evolution of internal waves in the ocean, it is important to characterize their generation. The two-dimensional generation problem has been studied for four decades, with ample experimental, numerical, and theoretical results. Most of this past work has also been done using linear, inviscid approximations. However, wave generation in the ocean is three-dimensional (3D), and in many locations, nonlinear and viscous effects can be significant. Recent advances in experimental and numerical techniques are only now making the fully nonlinear, 3D generation process accessible. We utilize these new techniques to perform both laboratory experiments and numerical simulations on internal wave generation in 3D. We find that a significant component of the internal wave field generated by tidal flow over 3D topography is radiated in the direction perpendicular to the tidal forcing direction. This could lead to substantial improvements of global internal wave generation models. In addition, we have developed a new method for statistical analysis of ocean data sets, and have found large regions in the deep ocean where internal waves may not propagate. This will also have important effects on the way researchers study the propagation of internal waves, which, when propagating downward, were previously thought to always reflect from the sea floor. / text

A parameterization is presented for turbulence dissipation due to baroclinic tide impacting on abrupt shelf topography that is supercritical with respect to the tide. The parameterization requires knowledge of the topography, stratification, and the remote forcing velocity. Upon impact, the tide cascades to higher vertical modes. Vertical internal modes that are arrested at the crest of the topography in the form of lee waves are assumed to dissipate, while faster modes are assumed to propagate away. The energy flux in each mode is predicted with topography that allows linear numer- ical solutions. The parameterization is tested using high-resolution two-dimensional numerical models of baroclinic tides impinging on an isolated shelf of various heights approximated as a step-function. The recipe is seen to work well compared to numeri- cal simulations of isolated shelves, although it consistently underestimates model flux divergence. Despite low forcing velocities having a more accurate numerical linear solution, the recipe does poorly because it does not accurately predict the modes that become trapped and dissipate. Maximum dissipation occurs when flow is on-shelf and lee waves form, indicating lee waves are the mechanism by which dissipation occurs. / Graduate / 0415

A parameterization is presented for turbulence dissipation due to baroclinic tide impacting on abrupt shelf topography that is supercritical with respect to the tide. The parameterization requires knowledge of the topography, stratification, and the remote forcing velocity. Upon impact, the tide cascades to higher vertical modes. Vertical internal modes that are arrested at the crest of the topography in the form of lee waves are assumed to dissipate, while faster modes are assumed to propagate away. The energy flux in each mode is predicted with topography that allows linear numer- ical solutions. The parameterization is tested using high-resolution two-dimensional numerical models of baroclinic tides impinging on an isolated shelf of various heights approximated as a step-function. The recipe is seen to work well compared to numeri- cal simulations of isolated shelves, although it consistently underestimates model flux divergence. Despite low forcing velocities having a more accurate numerical linear solution, the recipe does poorly because it does not accurately predict the modes that become trapped and dissipate. Maximum dissipation occurs when flow is on-shelf and lee waves form, indicating lee waves are the mechanism by which dissipation occurs. / Graduate / 0415

Baroclinic tides result from the interaction of barotropic tides with topography in stratified oceans. They play an important role in driving deep ocean mixing. In this research, investigations of the dynamics of baroclinic tides and internal solitary waves (ISWs) in the northern South China Sea (SCS) are conducted, mainly by means of the Massachusetts Institute of Technology general circulation model (MITgcm). Firstly, simulations of internal wave generation at the Luzon Strait (LS) are carried out. By conducting three-dimensional (3D), high-resolution experiments, it was found that the generated wave field features a multi-modal structure: large, pronounced ISWs of first mode (amplitude ~120 m) and second mode (amplitude ~120 m) were reproduced. The two north-south aligned ridges in the LS contribute together to the generation of the second mode ISWs, whereas the easternmost ridge of the two is responsible for the first mode ISWs. It was found that multiple generation mechanisms of internal waves could occur in this region, and overall it belongs to a mixed lee wave regime. A specific type of short internal waves arose during the 3D simulation. These ride on a second mode ISW with similar phase speed, trailing a first mode ISW. The short waves possess wavelengths of ~1.5 km and amplitudes of ~20 m, and only show up in the upper layer up to a depth of ~500 m. Scrutiny of the generation process showed that these short waves appear in two distinct regions and are produced due to two mechanisms, namely, the disintegration of an inclined baroclinic bore near the LS, and the overtaking of a second mode ISW in the deep water by a faster first mode ISW. Robust evidence has been sought from satellite imagery and by solving the theoretical Taylor-Goldstein Equation to verify their existence. The effects of superposition of multiple tidal harmonics (diurnal and semidiurnal) on the resultant ISW generation were investigated. It was first found that, by analyzing historical observational data, the occurrence of ISWs in the far-field always follow strong semidiurnal barotropic tidal peaks in the LS, regardless of whether it is the maximum for the diurnal or total tidal strength. However, modelling results of MITgcm and a linear internal tide generation model demonstrate that the diurnal tidal harmonics modulate the arrival time and amplitude of the propagating ISWs. Specifically, it leads to the emergence of the so-called A and B type ISWs and an alternation and transition between the two. Secondly, the shoaling process of ISWs in the northern SCS slope-shelf area is investigated. A series of two-dimensional (2D) experiments are set up to study the shoaling of a large-amplitude second mode concave ISW over a linear slope that resembles the SCS slope. Modelling results show that a strong transformation of the wave profile starts to take place when the wave is approaching the shelf break. A convex type wave is born at the trailing edge of the incident wave and gradually disintegrates into a group of ISWs due to the steepening of the rear wave profile. The frontal face of the wave gets flatter when travelling on the slope, but forms a steep structure right above the shelf break. However, this steep structure shows no tendency to evolve into an ISW: instead, it gets increasingly flat again while evolving on the shelf. The trailing convex wave packet travels faster and merges with the frontal concave wave. Finally, a wave packet with rank-ordered convex ISWs moves forward steadily on the shelf. Energy transfer to the ambient modes is evident, as both first mode and higher modes are clearly seen during and after the shoaling process. First mode ISW evolution is studied too by performing 3D, high-resolution experiments over the wide northern SCS slope and shelf area. It was found that the wave profiles change drastically near the shelf break and the Dongsha Atoll. In agreement with satellite imagery, the wavefront of the leading ISW becomes more spatially oblique with respect to its original orientation as it progresses westward due to the inclination of the slope in the topography. Wave disintegration is prominent in the shallow water zone, and wave polarity reverses near the turning point (at the 130 m isobath), which is consistent with the predictions of weakly nonlinear theory. A series of 2D experiments were set up to inspect the effects of rotation on the shoaling ISW. The results indicate that under the rotation, upon reaching the continental shelf, one shoaling ISW could disintegrate into one ISW packet and one secondary solibore that contains a number of rank-ordered waves with much shorter wavelength than an ISW. The secondary solibore is very pronounced in the northern portion of the northern SCS slope and shelf, but could hardly be discerned in the southern portion, which is consistent with the outcome of 3D simulations.

Ondas internas são movimentos ondulatórios que ocorrem no interior da coluna de água, associadas à estratificação de densidade. Ondas internas cuja frequência de oscilação se assemelha à das marés são chamadas marés internas. Estas ocasionam escoamentos intensos que influenciam a dinâmica de sedimentos, os processos de mistura e a produtividade primária. Em um ambiente energético como a Plataforma Continental Amazônica (PCA), localizada na costa norte brasileira, a estratificação varia consideravelmente, tanto espacial quanto temporalmente, de acordo com o balanço entre as diversas forçantes presentes. Na região da PCA alguns autores sugerem a presença de marés internas, entretanto, estudos específicos acerca do tema não figuram na literatura. Dessa forma, desenvolvemos neste trabalho um estudo da maré interna na região da PCA. Como objetivo, procuramos comprovar a ocorrência de marés internas na PCA, caracterizar seu comportamento e verificar sua intermitência. Para tal foram realizadas análises de dados provenientes do programa AMASSedS (A Multidisciplinary Amazon Shelf Sediment Study). Para caracterizar as marés internas, aplicamos dois métodos distintos para obtenção do campo baroclínico. O primeiro foi fundamentado no estabelecimento de uma corrente barotrópica préviamente obtida atráves de simulações numéricas. O segundo método empregado embasou-se na aplicação das funções empíricas ortogonais para a separação em modos estatísticos. Verificamos que as ondas internas na PCA estão ligadas à vazão do Rio Amazonas e são observadas, principalmente, na frequência semi-diurna. Aparentemente, as marés internas semi-diurnas influenciam não somente a hidrodinâmica da PCA como também são responsáveis por parte da variabilidade da salinidade próximo à superfície. / Internal waves are oscillatory motions that occur within the density stratified ocean. The ones with tidal frequency are then called internal tides or baroclinic tides, and are, on several locations around the planet, responsible for strong fluxes that affect several processes, like sediment transport, mixing processes and primary production. In such a strong environment as the Amazon Continental Shelf (ACS), located at the northern brazilian coast, it\'s stratification changes considerably with time and space, accordingly with the balance between the several forcing variables present. In this region, some authors suggest that internal tides occur, however, none research have been made about it on the ACS. That being said, we propose a study on internal tides on the ACS. As we hypothesize that internal tides occur, we look forward to characterize it\'s behavior and verify it\'s intermittency on the ACS. To do so, the data collected during the AMASSedS project (A Multidisciplinary Amazon Shelf Sediment Study) is going to be analyzed. In order to characterize it, two different method were applied to obtain the baroclinic field. The first method was the definition of a modeled-based barotropic current of the ACS obtained on the literature. The second method was the application of Empirical Orthogonal Functions in order to split the field on statistical modes of variability and analyze them separately. Our results indicate that internal tides on the ACS occur preferentially on the semi-diurnal frequency and it\'s generation is intimately connected to river discharge. Also, the analysis of the salinity anomaly field indicates that internal tides are responsible for part of the variability of the later on the surface on mid-shelf.

Ondas internas são movimentos ondulatórios que ocorrem no interior da coluna de água, associadas à estratificação de densidade. Ondas internas cuja frequência de oscilação se assemelha à das marés são chamadas marés internas. Estas ocasionam escoamentos intensos que influenciam a dinâmica de sedimentos, os processos de mistura e a produtividade primária. Em um ambiente energético como a Plataforma Continental Amazônica (PCA), localizada na costa norte brasileira, a estratificação varia consideravelmente, tanto espacial quanto temporalmente, de acordo com o balanço entre as diversas forçantes presentes. Na região da PCA alguns autores sugerem a presença de marés internas, entretanto, estudos específicos acerca do tema não figuram na literatura. Dessa forma, desenvolvemos neste trabalho um estudo da maré interna na região da PCA. Como objetivo, procuramos comprovar a ocorrência de marés internas na PCA, caracterizar seu comportamento e verificar sua intermitência. Para tal foram realizadas análises de dados provenientes do programa AMASSedS (A Multidisciplinary Amazon Shelf Sediment Study). Para caracterizar as marés internas, aplicamos dois métodos distintos para obtenção do campo baroclínico. O primeiro foi fundamentado no estabelecimento de uma corrente barotrópica préviamente obtida atráves de simulações numéricas. O segundo método empregado embasou-se na aplicação das funções empíricas ortogonais para a separação em modos estatísticos. Verificamos que as ondas internas na PCA estão ligadas à vazão do Rio Amazonas e são observadas, principalmente, na frequência semi-diurna. Aparentemente, as marés internas semi-diurnas influenciam não somente a hidrodinâmica da PCA como também são responsáveis por parte da variabilidade da salinidade próximo à superfície. / Internal waves are oscillatory motions that occur within the density stratified ocean. The ones with tidal frequency are then called internal tides or baroclinic tides, and are, on several locations around the planet, responsible for strong fluxes that affect several processes, like sediment transport, mixing processes and primary production. In such a strong environment as the Amazon Continental Shelf (ACS), located at the northern brazilian coast, it\'s stratification changes considerably with time and space, accordingly with the balance between the several forcing variables present. In this region, some authors suggest that internal tides occur, however, none research have been made about it on the ACS. That being said, we propose a study on internal tides on the ACS. As we hypothesize that internal tides occur, we look forward to characterize it\'s behavior and verify it\'s intermittency on the ACS. To do so, the data collected during the AMASSedS project (A Multidisciplinary Amazon Shelf Sediment Study) is going to be analyzed. In order to characterize it, two different method were applied to obtain the baroclinic field. The first method was the definition of a modeled-based barotropic current of the ACS obtained on the literature. The second method was the application of Empirical Orthogonal Functions in order to split the field on statistical modes of variability and analyze them separately. Our results indicate that internal tides on the ACS occur preferentially on the semi-diurnal frequency and it\'s generation is intimately connected to river discharge. Also, the analysis of the salinity anomaly field indicates that internal tides are responsible for part of the variability of the later on the surface on mid-shelf.

In this study, vertical profiles of velocity and hydrographic properties measured by the Lowered ADCP and CTD, respectively are used to calculate the vertical eddy diffusivity K based on small-scale turbulence theory. Two methods are used to estimate K, that is, the Thorpe scale analysis method (designated as Kz) and vertical wave number shear spectral method (designated as Ksh). Four different experiments with different flow conditions and bathymetry, i.e., internal tides, deep open-ocean, nonlinear internal waves and Kuroshio, are conducted and their K values are estimated and discussed. The internal tides at the mouth of Kao-Ping Submarine Canyon (KPSC) are observed during July and December (spring tide) of 2008. In each cruise the LADCP/CTD casts are repeated every two hours and last 27 and 40 hours, respectively. The results indicate the existence of strong, semi-diurnal internal tides with vertical displacement of 50~100 m and the nature of first baroclinic mode. Turbulent mixing during flood is significantly stronger than that during ebb. Note that in the winter experiments the Kz can reach 0.01 m2 s-1, which is even larger than the reported Kz values in other submarine canyons of the world, suggesting strong mixing processes are taking place in the KPSC. From the LADCP/CTD data of the joint hydrographic survey on May 2008 at SEATS station of the South China Sea, the estimated average values of Kz and Ksh in the upper 3000 m are about 3¡Ñ10-4 m2 s-1 and 1.8¡Ñ10-4 m2 s-1, respectively. The average value of Kz near the ocean bottom increases to 2.5¡Ñ10-3 m2 s-1. These estimated Kz are somewhat larger than the reported values in the open ocean. On the other hand, Kz values between 300 and 700 m deep are almost zero, indicating that turbulent mixing is inhibited in the stratified layer. Nonlinear internal waves are tracked in the South China Sea during May 2007. Our results show that after the internal solitons passed in the deep waters, the Kz profiles change significantly, surface mixing is weak, and Kz increases gradually from 400 m deep to the ocean bottom. In the shallow water region, shoaling effect of the nonlinear internal waves lead to enhanced energy dissipation and higher values of Kz, with the maximum value reaches 1 m2 s-1 near 180m depth. The flow structure of Kuroshio current between Taiwan and Lanyu is observed in October 2007. The results show that Kz in the surface layer is high (~10-2 m2 s-1), obviously due to strong Kuroshio flows there. At the 3000 m deep submarine trench near Lanyu, the Kz in the bottom layer is also very high (~ 1 m2 s-1 ), indicating that effective turbulent mixing in the bottom layer is mainly due to topography, which has similar level as the nonlinear internal waves.

Submarine canyons incising the continental shelf and slope are hot spots for topography-internal wave interactions, with elevated dissipation and mixing contributing to regional transport and biological productivity. At two Barkley Canyon sites (the continental slope below the shelf-break, and deep within the canyon), four overlapping years of horizontal velocity time-series data are used to examine the effects of irregular topography on the internal wave field. Mean currents are topographically guided at both sites, and in the canyon there is an inter-annually consistent, periodic (about a week) up-canyon flow (-700 to -900 m) above a near-bottom down-canyon layer. There is elevation of internal wave energy near topography, up to a factor of 10, 130 m above the slope, and up to a factor of 100, 230 m above the canyon bottom. All bands display weak inter-annual variability, but significant seasonality. Sub-diurnal and diurnal flows are presumably sub-inertially trapped along topography, and the diurnal band appears to be forced locally (barotropically). Both sites have high near-inertial energy. At the slope site, near-inertial energy is attenuated with depth, while in the canyon it is amplified near the bottom. Both sites show intermittent near-inertial forcing associated with wind events, downward propagation of high-mode internal waves, and the seasonal mixed-layer depth, though fewer events are observed in the canyon. Free semidiurnal internal tides are focused and reflected near critical shelf-break and canyon floor topography, and appear to experience both local and remote (baroclinic) forcing. The high-frequency internal wave continuum has enhanced energy near bottom at both sites (up to 7 times the open-ocean Garrett-Munk spectrum), and inferred dissipation rates increasing from a background of less than 10^-9 W kg^-1 and reaching 10^-7 W kg^-1 near topography. Dissipation is most strongly correlated with the semidiurnal (M2) constituent at both sites, with secondary contributions from the sub-diurnal (Sub_K1) band on the slope, and the near-inertial (NI) band in the canyon. Power laws for these dependencies are dissipation ~ M2^0.83 + Sub_K1^0.59 at the slope, and dissipation ~ M2^1.47 + NI^0.24 in the canyon. There is evidence in spectra of a near-buoyancy frequency build-up of energy correlated with high-frequency continuum variability, with a power law fit of 'shoulder' power ~ dissipation^0.34 that is independent of site topography. Though some general results are expected from observations at other slope and canyon sites, the greater temporal extent of these data provide a uniquely long-term evaluation of such processes. / Graduate

Les mers Indonésiennes sont le siège de très fort courants de marée qui interagissent avec la topographie pour créer des ondes internes à la fréquence de la marée que l'on appelle marée interne. Certaines d'entres elles, vont se propager et se dissiper dans l'océan intérieur. Le mélange associé provoque la remontée d'eau plus froide et plus riche en nutriments en surface qui influence le climat tropical et toute la chaine des écosystèmes marins. Surveiller les ressources marines est l'objectif du projet INDESO, dont cette thèse fait partie. Prendre en compte le mélange induit par la marée interne n'est pas facile. En effet, le résoudre entièrement n'est pas possible car les échelles concernées par les différents processus des ondes internes varient de plusieurs milliers de kilomètres (propagation) à quelques centimètres/millimètres (dissipation). De plus en plus de scientifiques introduisent le forçage de la marée dans leur modèle mais sans savoir où va l'énergie et comment les ondes sont dissipées. Dans cette thèse nous cherchons à proposer des outils et des débuts de réponses pour participer à cette meilleure compréhension de la dissipation des ondes internes dans le modèle numérique d'océan NEMO. Nous proposons certaines quantifications que nous comparons aux anciennes paramétrisations. J'ai, tout d'abord, contribué à une étude d'INDESO sur la validation de NEMO grâce à de nombreux jeu de données. Ensuite, j'ai cherché à quantifier et à qualifier le mélange induit par l'introduction de la marée explicite dans le modèle, ainsi que son impact sur les masses d'eau. (c'est redit plus loin)Il produit un refroidissement de surface de 0.3°C avec des maxima atteignant 0.8°C au niveau des sites de génération des ondes internes. Le modèle reproduit 75% de l'énergie attendue de génération des ondes internes, en bon accord avec des études précédentes. L'essentiel de la dissipation a lieu horizontalement (19GW) est proche de celle induite par la paramétrisation couramment utilisée (16GW), alors que, dans la réalité, on s'attend principalement à une dissipation réalisée grâce à des processus verticaux. Le modèle, au dessus des zones de génération, est de façon surprenante en très bon accord avec les mesures in situ de dissipation obtenues lors de la campagne INDOMIX. Par contre, dans les régions distantes des sources de génération, le modèle surestime le mélange par rapport aux observations d'INDOMIX. Dans la dernière partie de cette thèse j'ai commencé à apporter des éléments de réponse à la quantification des puits d'énergie dans NEMO. J'ai pour cela travaillé avec le cas test COMODO, qui est une section d'un fluide stratifié constituée d'une plaine abyssale, d'un talus et d'un plateau, forcée par la marée et sans friction de fond. Le modèle T-UGOm, un modèle hydrodynamique de marée, est comparé au modèle NEMO. Dans ce cadre, nous avons développé une méthode originale pour séparer la marée barotrope de la marée barocline. Elle repose sur la projection en modes normaux. Cette méthode donne, à première vue, des résultats similaires à ceux obtenus grâce à la méthode plus classique de soustraction par la moyenne verticale. Cependant, lorsque l'on regarde plus en détail les diagnostiques d'énergie on trouve que la méthode de projection en modes normaux offre une plus grande précision et un plus grand réalisme pour séparer la marée barotrope de la marée barocline. Plus on monte dans des modes élevés plus les longueurs ondes se raccourcissent dans NEMO par rapport à T-UGOm. Par ailleurs, NEMO dissipe la marée barotrope dans la plaine abyssale, alors qu'il n'y a explicitement pas de friction. Ce ne peut pas être la diffusion verticael ou horizontale qui est à l'œuvre ici, car il n'y a pas de raison physique pour une diffusion sur un fond plat. Le meilleur candidat pour expliquer cette diffusion serait le couplage 2D/3D du time splitting de NEMO. Un travail est en cours pour appliquer cette méthode sur l'ensemble de l'archipel Indonésien. / In the Indonesian seas, large tidal currents interact with the rough topography and create strong internal waves at the tidal frequency, called internal tides. Part of them will eventually propagate and dissipate far away from generation sites. Their associated mixing upwells cold and nutrient-rich water that prove to be critical for climate system and for marine resources. This thesis uses the physical ocean general circulation model, NEMO, as part of the INDESO project that aims at monitoring the Indonesian marine living resources. Models not taking into account tidal missing are unable to correctly reproduce the vertical structure of watermasses in Indonesian seas. However, taking into account this mixing is no simple task as the phenomena involved in tidal mixing cover a wide spectrum of spatial scales. Internal tides indeed propagate over thousands of kilometres while dissipation and mixing occurs at centimetric to millimetric scales. A model capable of resolving all these processes at the same time does not exist. Until now scientists either parameterised the tidal mixing or used models which only partly resolve internal tides. More and more scientists introduce explicit tidal forcing in their models but without knowing where the energy is going and how the internal tides are dissipated. This thesis intends to quantify energy dissipation in NEMO forced with explicit tidal forcing and compares it to the dissipation induced by the currently used parameterization. This thesis also provides new results about the quantification of the tidal energy budget in NEMO. I first contributed to an INDESO study that aimed at validating the model against several observation data sets. In a second and third study, I investigated the mixing produced in the model by explicit tidal forcing and its impact on water mass. Explicit tides forcing proves to produce a mixing comparable to the one produced by the parameterization. It also produces a significant cooling of 0.3 °C with maxima reaching 0.8°C in the areas of internal tide generation. The cooling is stronger on austral winter. The spring tides and neap tides modulate this impact by 0.1°C to 0.3°C. The model generates 75% of the expected internal tides energy, in good agreement with other previous studies. In the ocean interior, most of it is dissipated by horizontal momentum dissipation (19 GW), while in reality one would expect dissipation through vertical possesses. This value is close to the dissipation induced by the parameterization (16 GW). The mixing is strong over generation sites, and only 20% remains for far field dissipation mainly in the Banda and Sulawesi Seas. The model and the recent INDOMIX cruise [Koch-Larrouy et al. (2015)], which provided direct estimates of the mixing, are surprisingly in good agreement mainly above straits. However, in regions far away from the energy generation sites where INDOMIX found NO evidence of intensified mixing, the model produces too strong mixing. The bias comes from the lack of specific set up of internal tides in the model. More work is thus needed to improve the modeled dissipation, which is a theme of active research for the scientific community. I dedicated the last part of my thesis to the quantification of tidal energy sinks in NEMO. I first worked on a simple academic case: the COMODO internal tides test case, which analyses the behaviour of a vertically stratified fluid forced by a barotropic flow interacting over an idealized abyssal plain/slope/shelf topography without bottom friction. The results of the finite element T-UGOm hydrodynamic model are compared with those of NEMO. The central issue in calculating tidal energy budget is the separation of barotropic and baroclinic precesses.

Tide-topography coupling is important for understanding surface-tide energy loss, the intermittency of internal tides, and the cascade of internal-tide energy from large to small scales. Although tide-topography coupling has been observed and modeled for 50 years, the identification of surface and internal tides over arbitrary topography has not been standardized. Here, we begin by examining five surface/internal-tide decompositions and find that only one is (i) consistent with the normal-mode description of tides over a flat bottom, (ii) produces a physically meaningful depth-structure of internal-tide energy flux, and (iii) results in an established expression for internal-tide generation. Next, we examine the expression for internal-tide generation and identify how it is influenced by remotely-generated shoaling internal tides. We show that internal-tide generation is subject to both resonance and intermittency, and can not always be predicted from isolated regional models. Lastly, we quantify internal-tide generation and scattering on the Oregon Continental slope. First, we derive a previously unpublished expression for inter-modal energy conversion. Then we evaluate it using observations and numerical simulations. We find that the surface tide generates internal tides, which propagate offshore; while at the same time, low-mode internal tides shoal on the slope, scatter, and drive turbulent mixing. These results suggest that internal tides are unlikely to survive reflection from continental slopes, and that continental margins play an important role in deep-ocean tidal-energy dissipation. / Graduation date: 2011