Bien qu'ayant suscité de nombreuses études sur le sujet, un certain nombre de questions à propos de la formation des vagues sous l'effet du vent restent sans réponse précise. Dans ma thèse, j'aborde ce problème selon une approche peu explorée : l'étude expérimentale de la déformation sous l'effet du vent de la surface d'un liquide fortement visqueux. En effet, contrairement à la majeure partie de la littérature sur le sujet, le liquide que j'utilise n'est pas de l'eau mais un liquide sensiblement plus visqueux. Indépendamment des questions fondamentales sous-jacentes, cela a en pratique l'avantage de simplifier le problème. En effet, du fait de la forte viscosité du liquide, l'écoulement dans le liquide reste laminaire et les perturbations de l'interface qui ne sont pas amplifiées ne peuvent se propager que sur une distance limitée. Pour observer ces déformations de l'interface liquide-air, j'ai développé un nouveau montage expérimental sur lequel a été mise en œuvre la méthode de visualisation Free Surface Synthetic Schlieren. Cette technique non intrusive a permis de mesurer avec une résolution micrométrique les amplitudes de déformations de la surface et d'accéder aux premières déformations à faible vitesse de vent. Dans un premier temps, les expériences furent conduites sur un liquide trente fois plus visqueux que l'eau. Grâce aux données expérimentales obtenues par FS-SS, deux régimes de déformation de l'interface liquide-air ont été mis en évidence. A vitesse de vent faible, l'interface est recouverte de "wrinkles", des perturbations de faible amplitude désorganisées spatialement et globalement alignées dans le sens de l'écoulement. Ces wrinkles peuvent être interprétés comme l'effet sur l'interface des fluctuations de pression de l'écoulement turbulent d'air. A plus forte vitesse, au-dessus d'une vitesse critique, apparaissent des vagues transverses quasi-parallèles entre elles et perpendiculaire à la direction du vent. Les distinctions entre les deux régimes ont été détaillées et les non-linéarités émergeant au-dessus du seuil ont aussi été étudiées. Par la suite, la viscosité du liquide a été changée sur une large gamme. Il ressort des expériences que les deux régimes de déformation de l'interface sous l'effet du vent peuvent être identifiés pour l'ensemble des viscosités parcourues. Suite à ces résultats, un modèle décrivant l'évolution de l'amplitude des wrinkles en fonction du vent et de la viscosité du liquide a été développé. / Despite numerous studies on the subject, the development of waves under the action of wind still retains a certain number of open questions. In my PhD, I approach this problem through a fairly uncommon angle: the experimental study of the deformation by wind of the surface of a highly viscous liquid. Indeed, contrary to the major part of the literature on the matter, the liquid I used is not water but a significantly more viscous liquid. Regardless of the fundamental underlying questions, this has the practical advantage of simplifying the problem. Indeed, due to the high viscosity of the liquid, the flow in the liquid stays laminar and the unamplified perturbations of the interface can only propagate over a limited distance. To observe these deformations at the liquid-air interface, I have developed a new experimental set-up upon which the Free Surface Synthetic Schlieren method of visualization was implemented. This non-intrusive technique allowed to measure with a micrometric accuracy the amplitude of the surface deformation and to access the first deformations at low wind velocity. First, experiments were conducted over a liquid thirty times more viscous than water. The experimental data obtained by FS-SS show two regimes of deformation of the liquid-air interface. At low wind velocity, the interface is populated with ``wrinkles'', small-amplitude streamwise spatially disorganized perturbations. These wrinkles can be interpreted as the effect on the interface of the pressure fluctuations in the turbulent wind. At higher windspeed, above a critical velocity, transverse waves appear with quasi-parallel crests perpendicular to the wind direction. The distinctions between the two regimes have been detailed and the nonlinearities emerging above the threshold have also been studied. Then, the viscosity of the liquid has been changed over a large range. It results from the experiments that the two regimes of surface deformation by wind can be identified for all the viscosities explored. Following these results, a model was developed to account for the evolution of the wrinkles' amplitude both with wind velocity and with viscosity.

Thesis (Ph.D.)--Joint Program in Applied Ocean Science and Engineering (Massachusetts Institute of Technology, Dept. of Ocean Engineering; and the Woods Hole Oceanographic Institution), 2000. / Includes bibliographical references (p. 299-312). / by Sean Patrick McKenna. / Ph.D.

No description available.

the presented work demonstrates the fabrication process of the master for nano-imprint lithography (NIL) stamp for multi-mode waveguide (MM-WG) with μ-mirror using hybrid-lithography, which includes a 2-photon-polymerization direct laser writing process (2PP-DLW) for μ-mirror surface and UV-photo lithography for MM-WGs. For the definition of the mirror surface at either end of waveguides in the master stamp, the 2PP-DLW process was used. It offers a lower surface roughness (< 0.1 λ) with fewer processing steps, alignment accuracy of ± 1 μm, prints fine and sharp contours, and relatively faster scanning for a specific material, which makes it the foremost technology over the traditional micro-mirror processes such as the dicing process, moving mask lithography, laser ablation, wet etching, and dry etching. For the fabrication of the waveguide core with rectangular cross-sections in the master stamp, UV mask exposure with SU-8 was used. It is a mass-production and low-cost technique. It gives a smooth structure with 90-degree sidewalls compared to other processes like dry etching, wet etching, mosquito method, and E-beam writing. We demonstrated the design and process of a master pattern with a density range from 0.04 to 0.2 to maintain equal pressure over the stamp in the NIL step for an almost uniform residual thickness layer.:Abstract Introduction Design of Experiments Experimental Results and Discussions Conclusion

In this study the description and development of intensity-based laser interferometric techniques for the detection and measurement of ultrasonic stress waves and their small displacement amplitudes is presented. The dynamic displacement sensitive interferometers described in the following chapters allow the quantitative point-by-point measurement of both in-plane and out-of-plane components of surface displacement motion. These uniquely developed interferometric sensors are: 1) an optical system design for the detection of the surface acoustic wave (Rayleigh wave). The technique is based on the Fourier analysis of coherent light and diffraction imaging properties of an illuminated grating; 2) the design and construction of a two-beam unequal-path laser interferometer for the measurement of out-of-plane surface displacement of ultrasonic waves; 3) extension of a flexible fiber optic probing device which is optically coupled to the test arm of the above two-beam interferometer. This permits scanning of the test surface which may be at some distance from the main optical system components; 4) the design and construction of a laser speckle interferometer for retro-reflective diffusing surfaces in which the in-plane displacements of the ultrasonic wave are interrogated. The inherent advantages of these newly designed optical configurations in terms of their greater simplicity, feasibility, and sensitivity over the conventional counterparts (classical/speckle laser interferometers) are explained. The function-response limitations of these interferometric sensors on lateral displacement resolution, on upper and lower-bound displacement sensitivity (dynamic range), on high-frequency bandwidth probing capability, on low-frequency environmentally associated noise disturbance, and on specularly reflective or diffusively retro-reflective specimen surface preparation are also mentioned. Finally, in a series of experimental observations, the application of a couple of these acoustic sensors in pulsed-excitation ultrasonic Specifically, the optically testing methods is cited. detected ultrasonic signals revealing the true nature of the various surface displacement modes of vibration are presented. / Ph. D.

Master of Science / Department of Geology / Abdelmoneam Raef / Geotechnical site characteristics are a function of the subsurface elastic moduli and the geologic structures. This study integrates borehole, surface and laboratory measurements for a geotechnical investigation that is focused on investigating shear-wave velocity (Vs) variation and its implication to geotechnical aspects of the Ogden test site in eastern Kansas. The area has a potential of seismicity due to the seismic zone associated with the Nemaha formation where earthquakes pose a moderate hazard. This study is in response to recent design standards for bridge structures require integrating comprehensive geotechnical site characterization. Furthermore, evaluation of dynamic soil properties is important for proper seismic response analysis and soil modeling programs. In this study, near surface geophysical site characterization in the form of 2D shear-wave velocity (Vs) structure that is compared with laboratory measurements of elastic moduli and earth properties at simulated in situ overburden pressure conditions and synergy with downhole Acoustic Televiewer time and amplitude logs, proved very robust “validated” workflow in site characterization for geotechnical purposes. An important component of a geotechnical site characterization is the evaluation of in-situ shear modulus, Poisson’s ratio and reliable and accurate elastic modulus ([lambda]) and shear modulus ([mu]) estimates are important in a good geotechnical site characterization. The geophysical site characterization, undertaken in this study, will complement and help in extrapolating drilling and core-based properties deduced by the geotechnical engineers interested at the test site.

Les phonons polaritons de surface (SPhPs) sont des ondes électromagnétiques de surface évanescentes générées par le couplage phonon-photon et se propageant le long d’une interface entre un milieu polaire (tel que SiO2 et SiC) et un diélectrique. Dans ce mémoire, nous nous intéressons à de possibles applications des SPhPs pour améliorer les performances thermiques des nanosystèmes, en focalisant leur énergie thermique avec des micro- et nanostructures, en réduisant leurs angles de diffraction à travers des ouvertures sub-longueur d’onde, et en démontrant leur émission thermique cohérente large-bande. Nous avons aussi effectué des mesures par microscopie spectrophotométrique infrarouge de micro-objets et démontré l’excitation thermique de modes de grandes longueurs de propagation dans un large domaine spectral. Nos résultats sont obtenus sur des bases à la fois théoriques, de simulations numériques et expérimentales. Ces travaux sont pertinents dans les domaines liés au transfert thermique, à l’optique infrarouge, au rayonnement thermique de champ proche, à la microscopie infrarouge, et à la polaritonique. / Surface phonon-polaritons (SPhPs) are evanescent electromagnetic surface waves generated by the phononphoton coupling and that propagate along the interface of a polar medium (such as SiO2 and SiC) and a dielectric one. In this work, we investigate possible applications of SPhPs for enhancing the thermal performance of micro- and nanoscale devices, focusing of thermal energy with micro-structures, decreasing the diffraction angles of infrared radiation on subwavelength apertures, and demonstrating broadband coherent thermal emission. We also perform infrared spectroscopy microscopy measurements of microscale objects and demonstrate long-range thermally excited surface modes in a broad frequency range. The results presented in this thesis can have possible applications in fields related to heat transfer, infrared optics, near-field thermal radiation, infrared microscopy, and polaritonics.

The United States Navy (USN) currently utilizes a Rapid Penetration Test (RPT) on both land and in water as the means to determine whether sufficient soil bearing capacity exists for piles in axial compression, prior to construction of the Elevated Causeway System (Modular) [ELCAS(M)] pile-supported pier system. The USN desires a replacement for the RPT because of issues with the method incorrectly classifying soils as well as the need to have a less labor-and-equipment-intensive method for geotechnical investigation. The Multichannel Analysis of Surface Waves (MASW) method is selected herein as the potential replacement for the RPT. The MASW method is an existing, geophysical method for determining soil properties based upon the acquisition and analysis of seismic surface waves used to develop shear wave velocity profiles for the soils at specific sites. Correlations between shear wave velocity and Cone Penetration Testing are utilized to classify soils, develop pile blow count estimates, and calculate soil bearing capacity. This researcher found that the MASW method was feasible and reliable in predicting the required properties for terrestrial sites. However, it was not successful in predicting those properties for underwater marine sites due to issues with equipment and field setup. Future areas of improvement are recommended to address these issues and, due to the success of the method on land, it is expected that once the issues are addressed the MASW method will be a reliable replacement for the RPT method across the entire subaerial and subaqueous profile.

Ma thèse est consacrée aux nouveaux phénomènes nano-optiques et aux dispositifs basés sur l'interaction spin-orbite de la lumière (SOI). Tout d'abord, il a été démontré un SOI uniquement piloté par le champ magnétique de la lumière permettant de diriger avec précision les ondes de surface de Bloch, offrant ainsi une nouvelle manifestation du champ magnétique optique. Ensuite, nous avons proposé et démontré le concept de nano-antenne plasmonique hélicoïdale à ondes progressives (TW-HPA), c’est-à-dire un fil hélicoïdal en or étroit alimenté optiquement par une nano-antenne dipolaire dans une configuration « end-firing ». Une telle nano-antenne a été démontrée comme la première optique de polarisation sublongueur d’onde. L’agencement de TW-HPAs à l’échelle de quelques microns a permis de convertir « à la carte » un faisceau polarisé linéairement en une distribution de faisceaux directifs présentant des polarisations différentes définies de façon déterministe par la géométrie et les dimensions des nano-antennes. Par le biais d’un couplage en champ proche de quatre nano-antennes à hélicités opposées, nous avons obtenus une optique sublongueur d’onde permettant un degré de liberté dans le contrôle de la polarisation qui est interdit avec les composants et méthodes classiques basées sur l’exploitation de matériaux biréfringents ou dichroïques, ou de métamatériaux imitant ces propriétés. / My thesis is devoted to novel nano-optical phenomena and devices based on spin-orbit interaction (SOI) of light. First, magnetic spin-locking, i.e., an SOI solely driven by the magnetic field of light, is demonstrated with Bloch surface waves. It provides a new manifestation of the magnetic light field. Then, we propose and demonstrate the concept of traveling-wave plasmonic helical antenna (TW-HPA), consisting of a narrow helical gold-coated wire non-radiatively fed with a dipolar nano-antenna. By swirling surface plasmons, the TW-HPA combines subwavelength illumination and polarization transformation. The TW-HPA is demonstrated to radiate on the subwavelength scale almost perfectly circularly polarized optical waves upon illumination with linearly polarized light. With this subwavelength plasmonic antenna, we developed strongly integrated arrays of point-light emissions of opposite handedness and tunable intensities. Finally, by coupling two couples of TW-HPAs of opposite handedness, we obtained new polarization properties so far unattainable.

L'estiu de 2005, es varen instal·lar un sismòmetre de fons marí (OBS, sigles en anglès d'Ocean Bottom Seimometer) permanent, de tres components i banda ampla, i un sensor diferencial de pressió, a les immediacions de la plataforma petrolífera Casablanca (Repsol Investigaciones Petrolíferas S.A.), a uns 150 m de fondària i 50 km de la costa de Tarragona. Aquesta iniciativa, pionera a l'Estat espanyol, es va portar a terme en el marc del projecte Casablanca (REN2003-06577), concedit pel Ministerio de Educación y Ciencia a l'Institut Geològic de Catalunya (IGC) i l'Observatori de l'Ebre, amb l'objectiu de caracteritzar la detectabilitat de l'OBS i millorar el coneixement de la sismicitat i el risc sísmic a la zona. L'any 2007, després d'una reinstal·lació dels sensors en què es varen introduir millores, la transmissió satèl·lit en temps real del senyal al centre de recepció de dades sísmiques a l'IGC de Barcelona va possibilitar la integració de l'OBS a la xarxa sísmica de Catalunya.L'anàlisi de soroll sísmic ambiental a l'emplaçament de l'OBS Casablanca mostra nivells alts als tres components, especialment a baixes freqüències i a la banda microsísmica. Així mateix, s'observen variacions estacionals i la influència de les condicions meteorològiques i oceanogràfiques. La comparació dels nivells de soroll a l'OBS Casablanca amb el d'un altre OBS situat a la mar de Ligúria, amb una instrumentació semblant, però instal·lat a una fondària de 2500 m, mostra un comportament més sorollós a Casablanca, probablement a causa de la menor profunditat a què està situat.Tot i el seu comportament sorollós, l'OBS Casablanca ha enregistrat diversos sismes locals, regionals i telesismes. Malgrat la petita magnitud i l'escassesa de terratrèmols locals succeïts durant el període de funcionament de l'OBS, l'estació ha mostrat la seva utilitat de cara a la millora de les localitzacions hipocentrals dels sismes propers amb epicentre a la mar. Noves dades permetran la validació d'aquest resultat.El senyal de l'OBS Casablanca, juntament amb el d'estacions situades a la Península Ibèrica, el nord d'Àfrica i les Illes Balears, s'ha pogut utilitzar amb èxit en un estudi de tomografia d'ones superficials amb soroll sísmic ambiental realitzat al NE de la Península. El procediment de l'estudi tomogràfic ha inclòs un tractament del senyal a fi de minimitzar l'energia aportada pels terratrèmols i normalitzar les amplituds a totes les freqüències. Mitjançant el càlcul de la correlació creuada per a tots els parells d'estacions disponibles durant un període de més d'un any, s'ha trobat un senyal equivalent a la funció de Green del medi, que ha possibilitat la mesura de la velocitat de grup i de fase. La representació dels resultats en forma de mapes de dispersió mostra zones d'altes i baixes velocitats, coherents amb les principals estructures geològiques de l'escorça i part del mantell superior. / Durante el verano de 2005, se instalaron un sismómetro de fondo marino (OBS, siglas en inglés de Ocean Bottom Seismometer) permanente, de tres componentes y banda ancha, y un sensor diferencial de presión, en las inmediaciones de la plataforma petrolífera Casablanca (Repsol Investigaciones Petrolíferas S.A.), a unos 150 m de profundidad y 50 km de la costa de Tarragona. Esta iniciativa, pionera en España, se llevó a cabo en el marco del proyecto Casablanca (REN2003-06577), concedido por el Ministerio de Educación y Ciencia al Institut Geològic de Catalunya (IGC) y al Observatori de l'Ebre, con el objetivo de caracterizar la detectabilidad del OBS y mejorar el conocimiento de la sismicidad y el riesgo sísmico en la zona. En el año 2007, después de una reinstalación en la que se introdujeron mejoras, la transmisión satélite en tiempo real de la señal al centro de recepción de datos sísmicos del IGC en Barcelona posibilitó la integración del OBS a la red sísmica de Cataluña.El análisis del ruido sísmico ambiental en el emplazamiento del OBS Casablanca muestra niveles altos en las tres componentes, especialmente a bajas frecuencias y en la banda microsísmica. También se observan variaciones estacionales y la influencia de las condiciones meteorológicas y oceanográficas. La comparación de los niveles de ruido en el OBS Casablanca con los de otro OBS situado en el mar de Liguria, de instrumentación similar, pero instalado a 2500 m de profundidad, muestra un comportamiento más ruidoso en Casablanca, probablemente a causa de la menor profundidad a la que está situado.Aunque de comportamiento ruidoso, el OBS Casablanca ha registrado numerosos seísmos locales, regionales y teleseísmos. A pesar de la pequeña magnitud y la escasez de terremotos locales durante el periodo de funcionamiento del OBS, la estación ha mostrado su utilidad de cara a la mejora de las localizaciones hipocentrales de los seísmos cercanos con epicentro en el mar. Nuevos datos permitirán la validación de este resultado.La señal del OBS Casablanca, junto con la de estaciones situadas en la Península Ibérica, el norte de África y las Islas Baleares, se ha podido utilizar con éxito en un estudio de tomografía de ondas superficiales con ruido sísmico ambiental realizado al NE de la Península. El procedimiento del estudio tomográfico ha incluido el tratamiento de la señal para minimizar la energía aportada por los terremotos y normalizar las amplitudes para todas las frecuencias. Mediante el cálculo de la correlación cruzada para todos los pares de estaciones disponibles durante un periodo de más de un año, se ha obtenido una señal equivalente a la función de Green del medio, que ha posibilitado la medida de la velocidad de grupo y de fase. La representación de los resultados en forma de mapas de dispersión muestra zonas de altas y bajas velocidades, coherentes con las principales estructuras geológicas de la corteza y parte del manto superior. / During the summer of 2005, a three-component broad-band permanent ocean bottom seismometer (OBS) and a differential pressure gauge were deployed near the Casablanca oil platform (Repsol Investigaciones Petrolíferas S.A.) at a depth of about 150 m and 50 km away from the Tarragona coast (NE Iberian Peninsula). This initiative, pioneer in Spain, was carried out within the framework of the Casablanca project (RES2003-06577), given by the Ministerio de Educación y Ciencia to the Institut Geològic de Catalunya (IGC) and to the Observatori de l'Ebre. The aim of this project was to characterize the OBS detection threshold and to improve the knowledge of the seismicity and seismic risk in the area around. In 2007 satellite transmission was implemented to have continuous and real time data, which allowed integrating the OBS into the Catalan Seismic Network.A seismic ambient noise analysis at the Casablanca OBS site shows high levels on the three components, especially at low frequencies and at the microseismic band. Seasonal variations and the meteorological and oceanographic conditions influence are also observed. The comparison between Casablanca OBS noise levels and those from another OBS placed at the Ligurian Sea, equipped with similar instrumentation but installed at a depth of 2500 m, shows that the Casablanca site is noisier, probably due to its shallower deployment.Despite its noisy behaviour, the Casablanca OBS has recorded a number of local and regional earthquakes and teleseisms. Only few close small events have occurred during the OBS running period. Nevertheless, the station has shown its utility to improve hipocentral locations of close earthquakes with the epicentre offshore.The Casablanca OBS signal, together with that from stations placed at the Iberian Peninsula, northern Africa and Balearic Islands, has been successfully used in a surface wave tomographic study from ambient noise in the NE Iberian Peninsula. The tomographic study includes a signal processing to minimize the energy from earthquakes and to normalize the amplitudes for all frequencies. A signal equivalent to the Green function has been obtained through the cross-correlation between all the possible station pairs during a period longer than one year, allowing the measurement of group and phase velocities. The results, which are presented as dispersion maps, show areas of high and low velocities that are coherent with the main crust and upper mantle geological structures.