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.

Blooms of the toxic dinoflagellate Karenia brevis are common on the West Florida Shelf (WFS), yet little is known of the relationships between zooplankton and K. brevis. A comprehensive analysis was undertaken to examine 1) perturbations in zooplankton community composition within K. brevis blooms 2) the contribution of zooplankton ammonium and phosphate excretion to K. brevis bloom nutrient requirements, and 3) the role of zooplankton grazing in K. brevis bloom termination. Prior to undertaking the first portion of the study, an examination of the perturbations in the normal zooplankton assemblage within K. brevis blooms, it was first necessary to define the normal zooplankton assemblage on the WFS. To this end, a seasonal analysis of abundance, biomass and community composition of zooplankton was undertaken at 6 stations on the WFS. Monthly sampling was conducted for one year at the 5, 25 and 50- m isobaths. Two major groups in community composition were observed at the near shore (5-m and 25-m) and offshore (50-m) stations. Considerable overlap was seen in community composition between the 5-m to 25-m and 25-m to 50-m isobaths, but little overlap in community composition was observed between the 5-m and 50-m isobaths. Of the 95 species identified, only 25 proved to be important (>90%) contributors to community composition. Near shore, important contributors were Parvocalanus crassirostris, Penilia avirostris, Paracalanus quasimodo, Oithona colcarva, Oikopleura dioica, Centropages velificatus and Pelecypod larvae. As distance offshore increased, important contributors to community composition were Euchonchoichiea chierchiae, Clausocalanus furcatus, Oithona plumifera, Oithona frigida, Oncaea mediteranea, Calaocalanus pavoninius, Oithona similis, and Gastropod larvae. Variations in abundance and biomass between non-bloom and bloom assemblages were evident, including the reduction in abundance of 3 key species within K. brevis blooms. One potential source of nutrients to support K. brevis blooms may be zooplankton regeneration of nutrients. To test this hypothesis, ammonium and phosphate excretion rates of several West Florida Shelf copepods (Labidocera aestiva, Acartia tonsa, Temora turbinata, and Paracalanus quasimodo) were measured and prorated to a 24-hour day. These excretion rates were then extrapolated to other West Florida Shelf zooplankton, combined with available literature excretion rates for some taxa, and applied to zooplankton abundances found for K. brevis blooms on the West Florida Shelf in 1999 and 2001. Ammonium excretion rates were found to be inadequate to support all but 104 cells l-1 of K. brevis, though phosphate excretion rates were adequate to support even 106 cells l-1 of K. brevis. Grazing assessment was conducted for three common zooplankton species that were found within two K. brevis blooms, A. tonsa, P. quasimodo, and L. aestiva, using 14C labeled K. brevis cells. Grazing rates were then applied to the zooplankton community and grazing assessed. Grazing pressure was occasionally heavy, and was capable of reducing K. brevis to background concentrations at stations in the 1999 bloom and at 1 station in the 2001 bloom. Generally, however, grazing pressure proved to be insufficient to reduce K. brevis to background concentrations during the 1999 and 2001 blooms.

In the equatorial Pacific Ocean, earthquakes are used as an indicator of tectonic stress for normal faults in the Galapagos Spreading Center, transform faults along the East Pacific Rise and thrust faults in the Middle American subduction zone. Linkages between seafloor tectonic processes and oceanographic and lunar conditions were explored using time-series cross-correlation analyses on two different time scales. Data for earthquakes in the eastern tropical Pacific study area are obtained using the hydrophone arrays of the NOAA-VENTS Program. Hydroacoustic monitoring (listening to underwater sounds) provides scientists with a detailed dataset that includes even small earthquakes, starting as low as magnitude 0.6, that are not perceived by land-based seismographs. Data for sea surface heights (SSH) consist of two different datasets. On a moon's quarter time scale, SSH data used to investigate the influence of the earth tide and changes in oceanic conditions were remotely acquired by the altimeter on board the TOPEX/Poseidon (T/P) satellite. SSH data used to investigate the influence of the ocean tides were obtained from the Tidal Model Driver (Padman and Erofeeva 2003), that predicts SSH for locations every hour. The Geographic Information System (GIS) was used for the visual display of the data and to compute basic descriptive statistics. A lab-book was created for the educational-outreach section of this work, explaining step by step how GIS has been used. Significant results show correlations between normal faults and ocean tides and between the thrust fault and earth tides. Also, the Quebrada and the Discovery transform faults show high correlation of earthquake events, suggesting that at such temporal and spatial resolution, the plate moves as a rigid block. / Graduation date: 2006

The history of Newfoundland is intimately tied to its relationship with the sea, to its island status and its consequent cultural isolation, to its reliance on fishing and more recently oil. But it is also one of tides - of prosperity and loss, migration and resettlement, of occupation and erasure. This research is an investigation into the nature of mutable landscapes – shifting settlements, resources and infrastructures. It is recognized that the needs of each community and the resources of each environment are diverse in type and supply. The spatialization of an energy infrastructure has the opportunity to link, in a dynamic system, the ecological, political, cultural, and historical constituents atomized communities. It has the potential to be a dynamic system that forces a presence in the everyday lives of a cultural habitat. This investigation tests the possibility for a contemporary energy infrastructure, usually hidden from the cultural landscape, to become a physically and culturally pronounced manifestation of a layered historical narrative. This work exhumes histories of Newfoundland and uncovers omnipresent themes of mutability, shifting, movement, and transience, presenting the history of Newfoundland as a fluctuating story of the sea. These stories not only frame the historical spatializations of Newfoundland’s population, its infrastructures, and economies through various media, but they also simultaneously outline the social and economic deficiencies of modern approaches to developing the island. Structured chronologically, the research forms the basis for an investigation into new ideas for an infrastructure off the southern coast of Newfoundland. This design project exemplifies themes of shifting and movement through a mobile, water-based energy, research, and cultural infrastructure. It is situated off the southern coast of Newfoundland and engages both the land and the sea. This thesis does not try to tame, resolve, or control the sea. The sea is always itself, ordered by its own cycles of tides, currents and ecologies. One can really only synchronize the relationships between land and sea.

Confined coasts in general, and pocket beach environments in particular, are under huge development pressures worldwide, not least due to their sheltered nature and perceived shoreline stability. However, understanding of their physical functioning is poor in comparison to that of open coast beaches. This study aims to improve understanding in terms of the existing gaps in knowledge of wave processes and nearshore currents, and also to examine the importance of local wind and tide factors in generating nearshore currents, in micro-tidal pocket beaches. The boundaries of embayments are generally recognized as important controls of their beach processes and responses, yet little detailed knowledge exists of how the exact embayment dimensions and characteristics influences these processes. One key embayment feature the influence of which is poorly understood is the downcoast headland. In this thesis, field observations plus Zanuttigh and Van der Meer’s (2008) approach, and the SWAN wave model were used to evaluate the downcoast headland effects on wave processes within Okains Bay, an example pocket beach environment. The results showed that incident wave heights and directions were significantly influenced by wave reflection processes from the downcoast headland inside the bay. The intensity of reflection effects on wave characteristics inside the pocket beach varied according to approaching wave direction. Reflection effects reduced when waves approached from angles close to parallel to the headlands, increasing towards headland-perpendicular wave approaches. Field observations and the XBeach model were used to examine whether or not tides can significantly influence nearshore currents within example and model pocket beach environments. Results indicated that tides can be the primary driver of nearshore currents close to the bed inside micro-tidal pocket beaches, depending on incident wave conditions. In areas of micro-tidal pocket beaches exposed to direct approaching waves, currents were wave driven, while in areas further into the bay that experienced headland filtering of their wave environment, currents were mainly tide generated. The results of this study demonstrated how the current circulation system within micro-tidal pocket beaches is related to the incoming directions of offshore waves. If high energy waves approach oblique or normal to the shoreline (with the assumption that the shoreline is at 90° to the headlands), the current system was found to consist of longshore currents influenced by headlands, plus a rip current in the center of the shoreline or a toporip in proximity to headlands. The location of the rip current or toporip was determined by the direction of approaching incident waves. This study also examined the behavior of local winds in a pocket beach environment and their consequent effects on nearshore currents. Results for Okains Bay show that local winds tended to blow in offshore and onshore directions, as the bay is located in a valley, so orographic effects channel and shift the wind directions to angles close to offshore and onshore directions inside the bay. Results also indicated that local winds influence the hydrodynamic currents of pocket beaches that are confined by elevated topography, producing semi-cross shore influences since the winds are topographically channelled to blow in predominantly offshore and onshore directions. This research significantly refines our understanding of micro-tidal pocket beach wave and current processes, including quantification of the filtering effects of headlands on their wave environments, revealing the various and variable influences of tides and winds compared to in open coast beaches; and, significantly, highlighting the role of downcoast headland wave reflection effects. With regard to the latter, this research elucidates some key process differences between pocket and embayed beaches and clarifies reasons why the application of embayed beach models that include refraction and diffraction but exclude reflection effects to the study of pocket beaches is inappropriate for studying pocket beaches. This research also provides methodological and topic suggestions for future research on pocket beach environments, including how to use the improved hydrodynamic knowledge of this study in future studies seeking to better understand pocket beach sediment systems, a topic that was beyond the scope of the current research.

Harmful Algal Blooms (HABs) in the Gulf of Mexico (GOM) are natural phenomena that can have negative impacts on marine ecosystems on which human health and the economy of some Gulf States depends. Many of the HABs in the GOM are dominated by the toxic dinoflagellate Karenia brevis. Non-toxic phytoplankton taxa such as Scrippsiella sp. also form intense blooms off the Mexican coast that result in massive fish mortality and economic losses, particularly as they may lead to anoxia. The main objectives of this dissertation were to (1) evaluate and improve the techniques developed for detection of Karenia spp. blooms on the West Florida Shelf (WFS) using satellite remote sensing methods, (2) test the use of these methods for waters in the GOM, and (3) use the output of these techniques to better understand the dynamics and evolution of Karenia spp. blooms in the WFS and off Mexico. The first chapter of this dissertation examines the performance of several Karenia HABs detection techniques using Moderate Resolution Imaging Spectroradiometer (MODIS) satellite images and historical ground truth observations collected on the WFS from August 2002 to December 2011. A total of 2323 in situ samples collected by the Florida Fish and Wildlife Research Institute to test for Karenia spp. matched pixels with valid ocean color satellite observations over this period. This dataset was used to systematically optimize variables and coefficients used in five published HAB detection methods. Each technique was tested using a set of metrics that included the F-Measure (FM). Before optimization, the average FM for all techniques was 0.47. After optimization, the average FM increased to 0.59, and false positives decreased ~50%. The addition of a Fluorescence Line Height (FLH) criterion improved the performance of every method. A new practical method was developed using a combination of FLH and Remote Sensing Reflectance at 555 nm (Rrs555-FLH). The new method resulted in an FM of 0.62 and 3% false negatives, similar to those from more complex techniques. The first chapter concludes with a series of recommendations on how to improve the detection techniques and how to take these results a step further into a Gulf wide observing systems for HABs. In chapter two, ocean color techniques were used to examine the extension, evolution and displacement of four Karenia spp. events that occurred in the WFS between 2004 and 2011. Blooms were identified in the imagery using the new Rrs-FLH method and validated using in situ phytoplankton cell counts. The spatial extension of each event was followed in time by delineating the blooms. In 2004 and 2005, the WFS was affected by a series of hurricanes that led to high river discharge and intense sediment resuspension events. Both processes had an impact on HAB occurrence. For example, I tracked a Karenia spp. bloom found in late December 2004 approximately 40-80 km offshore Saint Petersburg, which then expanded reaching an extension of >8000 km2 in February 2005. The bloom weakened in spring 2005 and intensified again in summer reaching >42,000 km2 after the passage of hurricane Katrina in August 2005. This bloom covered the WFS from Charlotte Harbor to the Florida Panhandle. Two other cases were studied in the WFS. The results of the Hybrid Coordinate Ocean Model from the U.S. Navy aid understanding the dispersal of the blooms. During fall 2011, three field campaigns to study HABs in Mexico were conducted to do an analysis of optical properties and explore the possibility of using ocean color techniques to distinguish between the main phytoplankton blooms in that region. Three main bloom scenarios were observed in the Campeche Bank region: massive diatom blooms, blooms dominated by Scrippsiella spp., and Karenia spp. blooms. The normalized specific phytoplankton absorption spectra were found to be different for Karenia spp. and Scrippsiella sp. blooms. A new technique that combines phytoplankton absorption derived from MODIS data and the new technique developed in Chapter One showed potential for a detection technique that can distinguish between Karenia and Scrippsiella blooms. Additional work is needed to improve the new technique developed for Mexican waters, but results show potential for detection techniques that can be used Gulf-wide. This will help better understand the dynamic and possible connectivity of phytoplankton blooms in the GOM.

Lake Vostok, der größte der über 70 subglazialen Seen in der Antarktis, ist derzeit einer der Forschungsschwerpunkte der geowissenschaftlichen Polarforschung. Der See erstreckt sich unter einer 4 000 m dicken Eisschicht auf über 250 km Länge mit einer Wassertiefe von bis zu 1 000 m. Ziel der hier vorliegenden Arbeit ist die Untersuchung des Einflusses der Gezeiten auf den Wasserstand des Sees, die eine bisher nicht betrachtete Komponente in der Zirkulation im See darstellen. Auf Grund seiner Ausdehnung ist das Gezeitenpotential an verschiedenen Punkten auf dem See nicht gleich, sondern weist differentielle Unterschiede auf. Unter der Annahme, dass sich die Seeoberfläche entlang einer Äquipotentialfläche ausrichtet, ergeben sich Gleichgewichtsgezeiten des Sees mit Amplituden von bis zu 4,6 mm für die größte ganztägige Tide K1 und 1,8 mm für die größte halbtägige Tide M2. Differenzen des Luftdruckes zwischen Nord- und Südteil des Sees rufen zusätzlich einen differentiellen inversen Barometer-Effekt hervor. Der inverse Barometer-Effekt besitzt im wesentlichen die spektralen Eigenschaften eines roten Rauschens. Die Variationen erreichen bis zu +/- 20 mm. Zum messtechnischen Nachweis derartiger Höhenänderungen an der Eisoberfläche über dem See wurden drei unterschiedliche Verfahren herangezogen. Differentielle GPS-Messungen zwischen einem Punkt auf aufliegendem Eis und einem zweiten in der südlichen Seemitte bestätigen die Modellvorstellungen und zeigen sowohl mit der Luftdruckdifferenz korrelierte Höhenänderungen als auch Höhenänderungen mit ganz- und halbtägigen Perioden. Die SAR-Interferometrie als flächenhaft arbeitende Methode zur Bestimmung von Höhenänderungen lässt den räumlichen Verlauf der Deformation erkennen. Dabei zeigt sich, dass sich die Aufsetzzone auf dem etwa 50 km breiten See bis in die Seemitte ersteckt. Erdgezeitenregistrierungen, die im Jahr 1969 in der Station Vostok durchgeführt wurden, zeigen zwar Auffälligkeiten wie etwa einen stark erhöhten Luftdruckregressionskoeffzienten und einen Phasenvorlauf der K1-Tide, diese können jedoch nicht eindeutig als Resultat von Höhenänderungen der Seeoberfläche identifiziert werden. Auf Grund der Lage der Station Vostok nahe dem Ufer des Sees ist die Deformation dort schon stark gedämpft. Die zu erwartenden Effekte liegen daher unterhalb der Auflösung der damaligen Messungen. Damit sind die theoretischen Grundvorstellungen über die Reaktion des subglazialen Sees auf Gezeiten- und Luftdruckanregungen herausgearbeitet, sowie diese Effekte mit zwei unabhängigen und komplementären Messverfahren nachgewiesen. / Lake Vostok, the largest of more than 70 subglacial lakes in the Antarctic, is one of the prominent topics of recent geoscientific polar research. The lake extends beneath the 4,000 m thick ice sheet to a length of more than 250 km with a water depth of up to 1,000 m. This thesis aims to investigate the influence of tides on the lake level which has not been considered so far in the discussion of water circulation within the lake. Due to the extent of the lake the tidal potential at different positions on its surface is not equal but exhibits a differential effect. Under the assumption of the lake level to be parallel to an equipotential surface the equilibrium tides of the lake yield amplitudes of up to 4.6 mm for the largest diurnal tidal constituent K1 and 1.8 mm for the largest semi-diurnal wave M2. In addition, differences in air pressure between the northern and the southern part of the lake result in a differential inverse barometric effect. This effect shows red noise characteristics with variations of up to +/- 20 mm. Three different types of measurements were used to verify corresponding height changes of the ice surface above the lake. Differential GPS measurements between one station on grounded ice and one in the southern centre of the lake confirm the concept and show height changes correlated to air pressure differences as well as changes with diurnal and semi-diurnal periods. SAR interferometry as a spatial method to determine height changes reveals the areal extent of the deformation with a grounding zone extending to the centre of the about 50 km wide lake. Gravimetric earth tide data recorded at Vostok Station in 1969 show pecularities such as an increased regression with air pressure and a phase lead of the K1 tide. However, these effects cannot be explicitly attributed to height changes of the lake surface. Due to the position of the station near the edge of the lake the effect is highly attenuated and below the noise level of these measurements. This work introduces the concept of the response of the subglacial lake to the tidal potential and to air pressure forcings and presents evidence for the effect by two different techniques proving the validity of the model.

The history of Newfoundland is intimately tied to its relationship with the sea, to its island status and its consequent cultural isolation, to its reliance on fishing and more recently oil. But it is also one of tides - of prosperity and loss, migration and resettlement, of occupation and erasure. This research is an investigation into the nature of mutable landscapes – shifting settlements, resources and infrastructures. It is recognized that the needs of each community and the resources of each environment are diverse in type and supply. The spatialization of an energy infrastructure has the opportunity to link, in a dynamic system, the ecological, political, cultural, and historical constituents atomized communities. It has the potential to be a dynamic system that forces a presence in the everyday lives of a cultural habitat. This investigation tests the possibility for a contemporary energy infrastructure, usually hidden from the cultural landscape, to become a physically and culturally pronounced manifestation of a layered historical narrative. This work exhumes histories of Newfoundland and uncovers omnipresent themes of mutability, shifting, movement, and transience, presenting the history of Newfoundland as a fluctuating story of the sea. These stories not only frame the historical spatializations of Newfoundland’s population, its infrastructures, and economies through various media, but they also simultaneously outline the social and economic deficiencies of modern approaches to developing the island. Structured chronologically, the research forms the basis for an investigation into new ideas for an infrastructure off the southern coast of Newfoundland. This design project exemplifies themes of shifting and movement through a mobile, water-based energy, research, and cultural infrastructure. It is situated off the southern coast of Newfoundland and engages both the land and the sea. This thesis does not try to tame, resolve, or control the sea. The sea is always itself, ordered by its own cycles of tides, currents and ecologies. One can really only synchronize the relationships between land and sea.

Pour cette thèse, nous avons été intéressé par les effets de la cavité magnétique et les effets de marées stellaires sur nos modèles de populations de synthèses planétaires. La cavité magnétique a été proposé comme un mécanisme important de la formation planétaire, en cela qu'elle peut stopper la migration radiale de la planète vers l'étoile (Lin et al. 1995). Dans ce travail on a modifié l'équation de diffusion pour l'évolution radiale de la densité de surface du disque de gas (1D), afin de tenir compte de l'effet du couple magnétique sur le disque (Armitage et al. 1999). D'autre part les effets de marées ont été inclus par un modèle analytique (Benitez-Llambay et al. 2011). Pour ce travail, on a utilisé le modèle de formation planétaire de Bern (Mordasini et al 2009a), auquel nous avons inclus ces deux effets. Enfin, nous avons comparé la distribution orbitale synthétique à la distribution orbitale observée par Kepler (Howard et al. 2012).Finalement, un dernier chapitre traite un sujet différent du reste de la thèse. Nous avons testé l'accrétion de pebbles (ou "pebble mechanism") dans le modèle de formation de Bern. Ce chapitre, est en fait un premier pas vers un modèle plus complet. Cependant, nous avons montré que l'implémentation numérique fonctionne bien. / In this thesis, we have been interested on the effects of the magnetic cavity and the stellar tides in synthetic planet population. The magnetic cavity is thought be important at the formation phase since it can truncates the gaseous disk and potentially stops the inward migration of planets (Lin et al. 1995). In this work we modified the standard radial viscous equation in order to take into account the effect of the magnetic torque on the gaseous disk (Armitage et al. 1999). Moreover, the stellar tides have been included in an analytical way as in (Bénitez-Llambay et al. 2011). For this work, we used the planetary model of Bern (Mordasini et al. 2012) at which we included both effects. The end of the thesis compare the synthetic orbital distribution with the orbital distribution observed by Kepler (Howard et al. 2012).Finally, a last chapter treats a topic different than the rest of the thesis. We tested the so called pebble mechanism (Ormel&Klahr2010) in the planetary formation model of Bern. So far, this chapter is a first step to a more complete model. However, we show that the numerical implementation is working well.

O Porto de Santos está localizado no litoral Paulista, na costa Sudeste do Brasil e é o maior e mais importante porto do país. Desde 1859 vem sofrendo adaptações e modernizações tanto em suas instalações físicas quanto em sua estrutura administrativa. As variáveis com as quais a Engenharia Civil deve lidar podem ser resumidas basicamente aos fenômenos naturais, pois estes determinam como serão projetadas e construídas as estruturas e instalações. Em projetos portuários, diversas características naturais devem ser mensuradas como, por exemplo, ventos, correntes marítimas, incidência de ondas, tipo de solo em que se encontra o porto, as temperaturas médias do local e, sobretudo, o nível do mar. Os mares e oceanos não possuem superfícies estáveis e apresentam cotas que estão em movimentos constantes. Estas variações se dão basicamente por ondas de curto ou longo período. A maré é uma onda de longo período que causa a variação diária do nível do mar. Atualmente é cada vez maior o interesse da comunidade científica pela temática relacionada às variações do nível do mar. Buscando contribuir com o tema, o presente estudo tem como objetivo principal a análise das variações do nível do mar no Porto de Santos ao longo dos últimos 60 anos, utilizando-se de dados coletados nos três marégrafos da região. Foi elaborada a média móvel desta série com a finalidade de detectar alguma variação significativa. A análise dos dados implicou que fossem considerados períodos de 18,61 anos, correspondentes ao intervalo do ciclo de precessão lunar, de modo a eliminar o efeito da variação astronômica no nível do mar. A elevação do nível máximo, médio e mínimo do mar no período de 1953 a 2008, apresentou uma elevação média de 2,5 mm/ano, resultado semelhante a outros estudos. Foram avaliados também o impacto da variação do nível do mar sobre as estruturas portuárias, indicando os efeitos da elevação nas estruturas, nos cais, nos aparelhos de defensa e ancoragem, nos equipamentos de descarga e outros. / Santos Harbor is at São Paulo\'s coast, in Brazil\'s southeast coast and it is the biggest and the most important port of the country. Since 1859 had been suffering adaptations and modernizations in its installations such as in its administrative structure. The variables that Civil Engineering has to deal with can be resumed basically to the natural phenomena because its determines how projected and built the structures will be. In docks projects, several natural characteristics must be measured, as example, winds, ocean currents, waves incidence, kind of soil that supports the harbor\'s structures, the local medium temperatures and, mainly the sea level. The seas and oceans doesn\'t have stables surfaces and shows levels that are in constant movements. These variations are products of short and long period waves. The tide is a long period wave that causes the daily sea level variation. Actually, the interest of the scientific community in sea level variation is increasing. Aiming to contribute with this theme, the present study has as main objective analyzing the sea level variations at Santos Harbor above the last 60 years, using data collected from three tidal gauges in the region. It was applied the moving average of the series to detect some significant variation. The data analysis demanded that the periods of 18,61 years, which corresponds to the interval of the moon precession cycles, was considered to purge the astronomic variation over the sea level. The maximum sea level, average and minimum sea level, in the period of 1953 and 2008 showed an average increase of 2.5 mm/year, which is similar to other studies. It was evaluated the impact of this sea level rise over the port\'s structures, showing the structural effects, over the docks; in the defense and anchorage equipment, unload equipment and others.