The benefits of the Oceans and Seas have been exploited by societies for many centuries; the marine offshore and naval sectors have been the predominant users of the waters. It has been overlooked until recently, that significant amounts of energy can be harnessed by waves, providing an additional abundant resource for renewable energy generation. The increasing energy needs of current societies have led to the consideration of waves as an exploitable renewable resource. During the past decades, advancements have been made towards commercialising wave energy converters (WECs), though significant knowledge gap exists on the accurate estimation of the potential energy that can be harnessed. In order, to enhance our understanding of opportunities within wave energy highly resolved long-term resource assessment of potential sites are necessary, which will allow for not only a detailed energy estimation methodology but also information on extreme waves that are expected to affect the survivability and reliability of future wave energy converters. This research work aims to contribute the necessary knowledge to the estimation of wave energy resources from both highly energetic and milder sea environment, exhibiting the opportunities that lay within these environments. A numerical model SWAN (Simulating WAves Nearshore), based on spectral wave formulation has been utilised for wave hindcasting which was driven by high resolution temporal and spatially varying wind data. The capabilities of the model, allow a detailed representation of several coastal areas, which are not usually accurately resolved by larger ocean models. The outcome of this research provides long-term data and characterisation of the wave environment and its extremes for the Scottish region. Moreover, investigation on the applicability of wave energy in the Mediterranean Sea, an area which was often overlooked, showed that wave energy is more versatile than expected. The outcomes provide robust estimations of extreme wave values for coastal waters, alongside valuable information about the usage of numerical modelling and WECs to establish energy pattern production. Several key tuning factors and inputs such as boundary wind conditions and computational domain parameters are tested. This was done in a systematic way in order to establish a customized solution and detect parameters that may hinder the process and lead to erroneous results. The uncertainty of power production by WECs is reduced by the introduction of utilization rates based on the long-term data, which include annual and seasonal variability. This will assist to minimize assumptions for energy estimates and financial returns in business plans. Finally, the importance of continuous improvements in resource assessment is stressed in order to enhance our understanding of the wave environment.

In this study, several wave parameters are downloaded or calculated from spectral wave data, and their interdependence is investigated. A literature review is carried out to summarize these dependencies. The literature study is followed by a statistical analysis of the relations between the calculated wave parameters. This statistical analysis is done both for all wave data, resulting in a global expression for the relations, and for the different seas and oceans, resulting in a deeper analysis about local differences and how these differences should be taken into consideration when using wave parameter relations in specific water bodies.

In this thesis, we present the generation and studies of a 87Rb Bose-Einstein condensate (BEC) perturbed by an oscillatory excitation. The atoms are trapped in a harmonic magnetic trap where, after an evaporative cooling process, we produce the BEC. In order to study the effect caused by oscillatory excitations, a quadrupole magnetic field time oscillatory is superimposed to the trapping potential. Through this perturbation, collective modes were observed. The dipole mode is excited even for low excitation amplitudes. However, a minimum excitation energy is needed to excite the condensate quadrupole mode. Observing the excited cloud in TOF expansion, we note that for excitation amplitude in which the quadrupole mode is excited, the cloud expands without invert its aspect ratio. By looking these clouds, after long time-of-flight, it was possible to see vortices and, sometimes, a turbulent state in the condensed cloud. We calculated the momentum distribution of the perturbed BECs and a power law behavior, like the law to Kolmogorov turbulence, was observed. Furthermore, we show that using the method that we have developed to calculate the momentum distribution, the distribution curve (including the power law exponent) exhibits a dependence on the quadrupole mode oscillation of the cloud. The randomness distribution of peaks and depletions in density distribution image of an expanded turbulent BEC, remind us to the intensity profile of a speckle light beam. The analogy between matter-wave speckle and light speckle is justified by showing the similarities in the spatial propagation (or time expansion) of the waves. In addition, the second order correlation function is evaluated and the same dependence with distance was observed for the both waves. This creates the possibility to understand the properties of quantum matter in a disordered state. The propagation of a three-dimensional speckle field (as the matter-wave speckle described here) creates an opportunity to investigate the speckle phenomenon existing in dimensions higher than 2D (the case of light speckle). / Nesta tese, descrevemos a produção e os estudos de condensados de Bose-Einstein, em átomos de 87Rb, perturbados através de excitações oscilatórias. Os átomos aprisionados são aprisionados em uma armadilha magnética harmônica onde produzimos o condensado de Bose-Einstein após o processo de resfriamento evaporativo. Com o objetivo de estudar o efeito de excitações oscilatórias, um campo magnético quadrupolar temporalmente oscilanteé superposto ao campo de aprisionamento. Através dessa perturbação, podemos observar a excitação de modos coletivos no condensado. Mesmo para baixas amplitudes de excitação, o modo dipolar é facilmente excitado. Porém, observamos que para excitar o modo quadrupolar no condensado é necessária uma energia mínima. Através da expansão em tempo de voo da nuvem excitada, identificamos que, para amplitude de excitação na quail o modo quadrupolar é excitado, a nuvem expande sem inverter o aspect ratio. Analisando essas nuvens por longos tempos de voo, foi possível observar alguns vórtices e, às vezes, um estado turbulento na nuvem condensada. Calculamos a distribuição de momento dessas nuvens e notamos que ela exibe um comportamento de lei de potência, parecido com a lei de Kolmogorov para turbulência. Além disso, mostramos que pelo nosso método que desenvolvemos para calcular a distribuição de momento, a forma da curva dessa distribuição (inclusive o expoente da lei de potência) exibe uma dependência com o modo quadrupolar de oscilação da nuvem. A distribuição desordenada de picos e depleções, na imagem da distribuição de densidade do condensado turbulento expandido, assemelha-se ao perfil de intensidade de um feixe de luz com speckle. A analogia entre speckle de onda de matéria e de luz é fundamentada através das semelhanças entre a propagação (ou expansão) dessas duas ondas. Além disso, a função de correlação de segunda ordem foi calculada e a mesma dependência com a distância foi observada para as duas ondas. Isto cria a possibilidade de entender melhor as propriedades da matéria quântica em um estado de desordem. A propagação de um campo de speckle tridimensional (como é o caso do speckle de onda de matéria aqui descrito) cria uma oportunidade de investigar o fenômeno de speckle em dimensões maiores que 2D (o caso do speckle de luz).

There are some empirical formulas used in the design of rubble mound breakwaters to find the weight of armour layer stone. The effect of wave grouping and spectral shape could not put into these design formulas since their effects are still under question. The influences of wave groups and spectral shape on the stability of rubble mound breakwaters have been investigated by several researchers up to now. However, results were not conclusive in these researches, where different wave grouping and spectral shape parameters were used. This study aims to investigate the influences of wave groups and spectral shape on the stability of rubble mound breakwaters by means of hydraulic model experiments. According to the result of the experiments, the damage to breakwater armour layer is almost same for different spectrum shapes and pronounced wave grouping, under the condition of similar wave statistics. Experiments also indicated that the wave trains with same significant wave height, H1/3, but with different distribution of the heights of extreme waves which were defined as wave heights higher than H1/3 in this study, cause different damage levels. Based on these results, extended experiments were conducted to observe the effect of heights of extreme waves in a wave train on the stability of rubble mound breakwaters. Results of the experiments showed that the higher the extreme waves are, the more destructive the wave train is. By carrying experimental results into design conditions, it was shown that a wave train with high extreme waves may affect the design weight of armour stone. Finally, in order to achieve more practical tools for engineering applications, occurrence probabilities of extreme waves under different spectral shapes were obtained by a numerical simulation. As a result, for different occurrence probabilities of extreme waves under the most widely used spectrums of PM and JONSWAP, necessary weight of armour stone was given in a range comparing with the formula of Meer. Moreover, it was noted that the spectral shape indirectly affects the stability not due to the wave grouping but due to the extreme waves in a wave train since the occurrence probability of the high extreme waves becomes higher as the spectral shape becomes narrower under same significant wave height condition.

In this thesis, we present the generation and studies of a 87Rb Bose-Einstein condensate (BEC) perturbed by an oscillatory excitation. The atoms are trapped in a harmonic magnetic trap where, after an evaporative cooling process, we produce the BEC. In order to study the effect caused by oscillatory excitations, a quadrupole magnetic field time oscillatory is superimposed to the trapping potential. Through this perturbation, collective modes were observed. The dipole mode is excited even for low excitation amplitudes. However, a minimum excitation energy is needed to excite the condensate quadrupole mode. Observing the excited cloud in TOF expansion, we note that for excitation amplitude in which the quadrupole mode is excited, the cloud expands without invert its aspect ratio. By looking these clouds, after long time-of-flight, it was possible to see vortices and, sometimes, a turbulent state in the condensed cloud. We calculated the momentum distribution of the perturbed BECs and a power law behavior, like the law to Kolmogorov turbulence, was observed. Furthermore, we show that using the method that we have developed to calculate the momentum distribution, the distribution curve (including the power law exponent) exhibits a dependence on the quadrupole mode oscillation of the cloud. The randomness distribution of peaks and depletions in density distribution image of an expanded turbulent BEC, remind us to the intensity profile of a speckle light beam. The analogy between matter-wave speckle and light speckle is justified by showing the similarities in the spatial propagation (or time expansion) of the waves. In addition, the second order correlation function is evaluated and the same dependence with distance was observed for the both waves. This creates the possibility to understand the properties of quantum matter in a disordered state. The propagation of a three-dimensional speckle field (as the matter-wave speckle described here) creates an opportunity to investigate the speckle phenomenon existing in dimensions higher than 2D (the case of light speckle). / Nesta tese, descrevemos a produção e os estudos de condensados de Bose-Einstein, em átomos de 87Rb, perturbados através de excitações oscilatórias. Os átomos aprisionados são aprisionados em uma armadilha magnética harmônica onde produzimos o condensado de Bose-Einstein após o processo de resfriamento evaporativo. Com o objetivo de estudar o efeito de excitações oscilatórias, um campo magnético quadrupolar temporalmente oscilanteé superposto ao campo de aprisionamento. Através dessa perturbação, podemos observar a excitação de modos coletivos no condensado. Mesmo para baixas amplitudes de excitação, o modo dipolar é facilmente excitado. Porém, observamos que para excitar o modo quadrupolar no condensado é necessária uma energia mínima. Através da expansão em tempo de voo da nuvem excitada, identificamos que, para amplitude de excitação na quail o modo quadrupolar é excitado, a nuvem expande sem inverter o aspect ratio. Analisando essas nuvens por longos tempos de voo, foi possível observar alguns vórtices e, às vezes, um estado turbulento na nuvem condensada. Calculamos a distribuição de momento dessas nuvens e notamos que ela exibe um comportamento de lei de potência, parecido com a lei de Kolmogorov para turbulência. Além disso, mostramos que pelo nosso método que desenvolvemos para calcular a distribuição de momento, a forma da curva dessa distribuição (inclusive o expoente da lei de potência) exibe uma dependência com o modo quadrupolar de oscilação da nuvem. A distribuição desordenada de picos e depleções, na imagem da distribuição de densidade do condensado turbulento expandido, assemelha-se ao perfil de intensidade de um feixe de luz com speckle. A analogia entre speckle de onda de matéria e de luz é fundamentada através das semelhanças entre a propagação (ou expansão) dessas duas ondas. Além disso, a função de correlação de segunda ordem foi calculada e a mesma dependência com a distância foi observada para as duas ondas. Isto cria a possibilidade de entender melhor as propriedades da matéria quântica em um estado de desordem. A propagação de um campo de speckle tridimensional (como é o caso do speckle de onda de matéria aqui descrito) cria uma oportunidade de investigar o fenômeno de speckle em dimensões maiores que 2D (o caso do speckle de luz).

The wind and wave (wind wave/swell wave) climate has an important role in the design and operation of coastal and marine structures, harbors and ports. The objective of this study is to identify the statistical characteristics of the winds, wind waves and swell waves in Eastern Mediterranean, and coastline of T&uuml / rkiye. For this purpose, the data of wind speed and direction, swell and wind wave height, period and direction for a certain duration with the six hours time intervals are obtained from ECMWF for the wind and wave climate computations. The data covers the area of eastern Mediterranean region. In order to compute the wind and wave climate at any selected coastal location, a software is developed by Serhan Aldogan in his MSc thesis. For every location, the wind wave roses, significant height of wind wave and swell wave versus mean period of primary wind directions, extreme probability analysis and distribution, and log-linear cumulative probability analysis and distributions is presented, compared and discussed. By the help of the specifically developed software, it is possible and convenient to analyze the wind and wave climate using ECMWF data at any coordinate.