The development and improvement of 3-D immersive audio is gaining momentum through the growing interest in virtual reality. Possible applications reach from recreating real world environments to immersive concerts and performances to exploiting big data acoustically. To improve the immersive experience several measures can be taken. The recording of the sound field, the spatialization and the development of the loudspeaker arrays are some of the greatest challenges. In this thesis, these challenges for improving immersive audio will be explored. First, there will be a short introduction about 3D audio and a review about the state of the art technology and research. Next, the thesis will provide an introduction to 3D loudspeaker arrays and describe the systems used during this research. Furthermore, the development of a new 16-element 3rd order sound field microphone will be described. Afterwards, different spatial audio algorithms such as higher order ambisonics, wave field synthesis and vector based amplitude panning will be described, analyzed and compared. For each spatialization algorithm, the quality of soundfield reproduction will be quantified using listener perception tests for clarity and sound source localization. / Master of Science

<div>Near-Field Acoustical Holography (NAH) is an inverse process in which sound pressure measurements made in the near-field of an unknown sound source can be used to reconstruct the sound field so that source locations can be identified. Usually a large number of measurements is required for the usual NAH methods since a large number of parameters in the source or field model need to be determined. However, a large-scale microphone measurement is costly and hard to perform, so the use of NAH is limited by practical experimental conditions. In the present work, with the motivation of decreasing the number of microphone measurements required, and thus facilitating the measurement process, two sparse Equivalent Source Method (ESM) algorithms were studied: i.e., Wideband Acoustical Holography (WBH) and l_1-norm minimization. Based on these two algorithms, a new hybrid NAH procedure was proposed and demonstrated.To study and verify the above mentioned algorithms, simulations of different sources were conducted and then experiments were conducted on different sources: i.e., a loudspeaker cabinet and a diesel engine.</div>

This research presents improvements to the velocity field reconstruction process achieved through computer vision. The first improvement of the velocity reconstruction process is the automation of the scanning laser Doppler vibrometer (SLDV) pose procedure. This automated process results in superior estimates of the position and orientation of the SLDV. The second improvement is the refinement of the formulation for reconstruction of the velocity field. The refined formulation permits faster computation, evaluation, and interpretation of the reconstructed structural velocity field. Taken together, these new procedures significantly improve the overall velocity reconstruction process which results in better, unbiased out-of-plane velocity estimates in the presence of noise. The automation of the SLDV pose procedure is achieved through a computer vision model of the SLDV. The SLDV is modeled as a projective camera, i.e. an imager which preserves projectivities. This projective camera model permits the precise association of object features with image features. Specifically, circular features in the object space are seen by the SLDV as ellipses in the image space. In order to extract object points, the bitangents among the circular features are constructed and the bitangent points selected. The accuracy and precision of the object points are improved through the use of a calibrated object whose circular features are measured with a coordinate measuring machine. The corresponding image points are determined by constructing the bitangents among the ellipses and selecting the tangent points. Taken together, these object/image bitangent point sets are a significantly improved data set for previously developed SLDV pose algorithms. Experimental verification of this automated pose procedure includes demonstrated repeatability, independent validation of the estimated pose parameters, and comparison of the estimated poses with previous methods. The refinement of the velocity reconstruction formulation is a direct result of the computer vision viewpoint adapted for this research. By viewing the velocity data as images of the harmonically excited structure's velocity field, analytical techniques developed for holographic interferometry are extended and applied to SLDV velocity images. Specifically, the "absolute" and "relative" fringe-order methods are used to reconstruct the velocity field with the "best" set of bases. Full and partial least squares solutions with experimental velocity data are calculated. Statistical confidence bounds of the regressed velocity coefficients are analyzed and interpreted to reveal accurate out-of-plane, but poor in-plane velocity estimates. Additionally, the reconstruction process is extended to recover the velocity field of a family of surfaces in the neighborhood of the "real" surface. This refinement relaxes the need for the exact experimental geometry. Finally, the velocity reconstruction procedure is reformulated so that independent least squares solutions are obtained for the two in-plane directions and the out-of plane direction. This formulation divides the original least squares problem into three smaller problems which can be analyzed and interpreted separately. These refinements to the velocity reconstruction process significantly improve the out-of-plane velocity solution and interpretation of the regressed velocity parameters. / Ph. D.

This thesis describes methods for using spectral interferometry for the complete space-time characterisation of few-cycle near-infrared femtosecond pulses and extreme ultraviolet (XUV) attosecond pulses produced via high harmonic generation (HHG). Few-cycle pulses tend to exhibit one or more of the following: (1) an octave-spanning bandwidth, (2) a highly modulated spectrum and (3) space-time coupling. These characteristics, coupled with the desire to measure them in a single-shot (to characterise shot-to-shot fluctuations) and in real-time (for online optimisation and control) causes problems for conventional characterisation techniques. The first half of this thesis describes a method, based on a spatially encoded arrangement for spectral phase interferometry for direct electric-field reconstruction (SEA-SPIDER). SEA-SPIDER is demonstrated for sub-10fs pulses with a central wavelength near 800nm, a bandwidth over 350nm, and a pulse energy of several nano-Joules. In addition, the pulses exhibit a modulated spectrum and space-time coupling. The spatially-dependent temporal intensity of the pulse is reconstructed and compared to other techniques: interferometric frequency-resolved optical gating (IFROG) and spectral phase interferometry for direct electric field reconstruction (SPIDER). SEA-SPIDER will prove useful in both femtoscience, which requires accurate knowledge of the space-time character of few-cycle pulses, and in HHG, which requires the precise knowledge of the driving pulse for seeding into simulations and controlling the generation process itself. Pulses arising from HHG are known to exhibit significant space-time coupling. The second half of this thesis describes how spectral interferometry may be performed to obtain the complete space-time nature of these fields via the use of lateral shearing interferometry. Finally, it is shown, via numerical simulations, how to extend the SPIDER technique for temporal characterisation of XUV pulses from HHG by driving the process with two spectrally-sheared driving pulses. Different experimental configurations and their applicability to different laser systems are discussed. This method recovers the space-time nature of the harmonics in a single shot, thus reducing the stability constraint currently required for photoelectron based techniques and may serve as a complimentary method for studying interactions of XUV attosecond pulses with matter.

Ce manuscrit traite de la problématique de la surveillance des structures depuis la mesure en service jusqu'à la caractérisation des champs mécaniques. La technologie des systèmes de mesure est étudiée dans la première partie. Les spécifications d'un système de mesure embarqué sont identifiées à partir d'essais en service sur des structures et à partir des applications envisagées. Ces spécifications définissent les hypothèses de résolution du problème inverse lié à l'interprétation des mesures.La deuxième partie présente la formulation du problème inverse de surveillance des structures à partir des hypothèses précédemment énoncées. Le principe est de reconstruire les champs mécaniques à partir de l'identification des conditions aux limites. Seul le chargement est considéré et le principe de Saint-Venant permet de restreindre le nombre de paramètres nécessaires à sa modélisation. La difficulté réside alors dans le choix des bonnes bases de chargement et dans le positionnement des capteurs. Cette méthode est appliquée aux structures poutres dans la troisième partie. Les bases de chargement sont obtenues à partir d'une projection des solutions analytiques du problème de poutre sur les bords des structures. Le positionnement des capteurs est ensuite étudié sur des structures poutres élémentaires qui réduisent le problème inverse à une identification polynomiale. La décomposition des structures poutres complexes en structures élémentaires simplifie alors la définition des bases de chargement et le positionnement des capteurs. La dernière partie présente les résultats obtenus sur des structures plaques. Les bases de chargement sont construites par projection des solutions analytiques pour les domaines étoilés. L'extension à des domaines quelconques est faite en considérant seulement les bords chargés des structures pour se ramener à des domaines étoilés équivalents. Bien que ces bases ne soient plus complètes, les résultats obtenus sur des plaques trouées montrent leur intérêt. Ces résultats servent ensuite à la construction des bases de chargement et au positionnement des capteurs pour les structures complexes modélisées par des assemblages de plaques. / This thesis tackles the problem of structural monitoring from integrated measurements to full-field reconstruction.In a first part, the technology of measurement systems is studied. An integrated measurement system is specified from some structural tests in-service and its future applications. These specifications define the mechanical framework of structural monitoring.The inverse problem associated with structural monitoring is expressed in a second part. The mechanical hypothesis result from the previously defined framework. The boundary conditions are identified in order to reconstruct the mechanical fields. The loads are considered only and the Saint-Venant's principle allows to limit the number of the loading parameters. The main issue is then to find the right loading basis and then to optimize the sensor locations.This method for structural monitoring is applied to beams in the third part. The analytical solutions of the mechanical equations for beams are projected on the boundary of the structures in order to obtain the loading basis. The optimal sensor locations are then estimate from elementary structures, what reduces the inverse problem to a polynomial identification. The complex beam structures are then decomposed into elementary ones, what drastically simplifies the construction of the loading bases and the sensor locations.In a last part, plate structures are considered. The loading basis are firstly defined by the projection of the analytical solutions of star-shaped domain. These basis are then extended to any plate structures using some loaded boundaries only in order to design an equivalent star-shaped domain. Even if these loading basis are incomplete sets, the results are in good agreement. The same principle is used to obtain the loading basis for complex structures modeled by plate assemblies.

Identifier et caractériser les effets du réchauffement climatique est un des grands enjeux scientifiques de ce début de siècle. Élévation du niveau des mers, bouleversements hydrologiques sont autant de conséquences de ce phénomène qui conditionnent l’existence de toutes les formes de vie présentes sur Terre. Dû à sa capacité thermique élevée, on estime que 84% de l’énergie développée par le réchauffement climatique est stockée dans les premières couches de l’océan. Il est cependant assez difficile d’évaluer son impact global au cours des 50 dernières années car l’océan ne se réchauffe pas de manière uniforme et l’échantillonnage in-homogène (spatial et temporel) des mesures océanographiques, des erreurs instrumentales (XBT) et des biais relatifs aux processus d’estimation des indicateurs globaux peuvent altérer notre appréciation de l’évolution des paramètres océaniques. Afin de pallier ces difficultés inhérentes à l’exploitation des mesures in situ, nous proposons dans cette thèse une correction empirique des données XBT basée sur l’analyse de profils colocalisés, caractérisée par une fonction parabolique sur l’immersion de la sonde et un terme d’offset thermique. À partir de la base de données corrigée, nous présentons ensuite une méthode originale de création de champs grillés grande échelle s’articulant autour de la reconstruction des modes propres de variabilité (DINEOF). Enfin, nous présentons les principaux résultats issus de ces reconstructions en termes de tendances globales et de variabilité du contenu thermique et contenu d’eau douce. Ces travaux contribuent ainsi à mieux documenter la variabilité océanique dans la couche 0-700m. / To identify and characterize the effects of global warming is one of the major scientific challenges of this new century. The rise of sea level, the hydrological changes are some consequences of this phenomenon which will influence all forms of life on Earth. Due to its high thermal capacity, it is estimated that 84% of the energy developed by global warming is stored in the first layers of the ocean. However, it is rather difficult to assess its overall impact over the last 50 years because the ocean is not warming uniformly and the inhomogeneous sampling (spatial and temporal) of oceanographic observations, instrumental errors (XBT) and biases related to the estimation process of global indicators can affect our assessment of the evolution of ocean parameters. To overcome these difficulties of in situ measurements analysis, we propose here an empirical correction of XBT data based on the analysis of collocated profiles, characterized by a parabolic function of the immersion of the probe and a thermal offset. From the corrected database, we present a new method for creating large-scale gridded fields based on the reconstruction of the natural modes of variability (DINEOF). Finally, we present the main results from these reconstructions in terms of global trends and variability of heat content and freshwater content. This work contributes to better document the oceanic variability in the 0-700m layer.