971 resultados para Dibujo en 3D


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Despite pattern recognition methods for human behavioral analysis has flourished in the last decade, animal behavioral analysis has been almost neglected. Those few approaches are mostly focused on preserving livestock economic value while attention on the welfare of companion animals, like dogs, is now emerging as a social need. In this work, following the analogy with human behavior recognition, we propose a system for recognizing body parts of dogs kept in pens. We decide to adopt both 2D and 3D features in order to obtain a rich description of the dog model. Images are acquired using the Microsoft Kinect to capture the depth map images of the dog. Upon depth maps a Structural Support Vector Machine (SSVM) is employed to identify the body parts using both 3D features and 2D images. The proposal relies on a kernelized discriminative structural classificator specifically tailored for dogs independently from the size and breed. The classification is performed in an online fashion using the LaRank optimization technique to obtaining real time performances. Promising results have emerged during the experimental evaluation carried out at a dog shelter, managed by IZSAM, in Teramo, Italy.

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Studies have been carried out to recognize individuals from a frontal view using their gait patterns. In previous work, gait sequences were captured using either single or stereo RGB camera systems or the Kinect 1.0 camera system. In this research, we used a new frontal view gait recognition method using a laser based Time of Flight (ToF) camera. In addition to the new gait data set, other contributions include enhancement of the silhouette segmentation, gait cycle estimation and gait image representations. We propose four new gait image representations namely Gait Depth Energy Image (GDE), Partial GDE (PGDE), Discrete Cosine Transform GDE (DGDE) and Partial DGDE (PDGDE). The experimental results show that all the proposed gait image representations produce better accuracy than the previous methods. In addition, we have also developed Fusion GDEs (FGDEs) which achieve better overall accuracy and outperform the previous methods.

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Recent measurements using an X-ray Free Electron Laser (XFEL) and an Electron Beam Ion Trap at the Linac Coherent Light Source facility highlighted large discrepancies between the observed and theoretical values for the Fe XVII 3C/3D line intensity ratio. This result raised the question of whether the theoretical oscillator strengths may be significantly in error, due to insufficiencies in the atomic structure calculations. We present time-dependent spectral modeling of this experiment and show that non-equilibrium effects can dramatically reduce the predicted 3C/3D line intensity ratio, compared with that obtained by simply taking the ratio of oscillator strengths. Once these non-equilibrium effects are accounted for, the measured line intensity ratio can be used to determine a revised value for the 3C/3D oscillator strength ratio, giving a range from 3.0 to 3.5. We also provide a framework to narrow this range further, if more precise information about the pulse parameters can be determined. We discuss the implications of the new results for the use of Fe XVII spectral features as astrophysical diagnostics and investigate the importance of time-dependent effects in interpreting XFEL-excited plasmas.

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When a planet transits its host star, it blocks regions of the stellar surface from view; this causes a distortion of the spectral lines and a change in the line-of-sight (LOS) velocities, known as the Rossiter-McLaughlin (RM) effect. Since the LOS velocities depend, in part, on the stellar rotation, the RM waveform is sensitive to the star-planet alignment (which provides information on the system’s dynamical history). We present a new RM modelling technique that directly measures the spatially-resolved stellar spectrum behind the planet. This is done by scaling the continuum flux of the (HARPS) spectra by the transit light curve, and then subtracting the infrom the out-of-transit spectra to isolate the starlight behind the planet. This technique does not assume any shape for the intrinsic local profiles. In it, we also allow for differential stellar rotation and centre-to-limb variations in the convective blueshift. We apply this technique to HD 189733 and compare to 3D magnetohydrodynamic (MHD) simulations. We reject rigid body rotation with high confidence (>99% probability), which allows us to determine the occulted stellar latitudes and measure the stellar inclination. In turn, we determine both the sky-projected (λ ≈ −0.4 ± 0.2◦) and true 3D obliquity (ψ ≈ 7+12 −4 ◦ ). We also find good agreement with the MHD simulations, with no significant centre-to-limb variations detectable in the local profiles. Hence, this technique provides a new powerful tool that can probe stellar photospheres, differential rotation, determine 3D obliquities, and remove sky-projection biases in planet migration theories. This technique can be implemented with existing instrumentation, but will become even more powerful with the next generation of high-precision radial velocity spectrographs.

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A 3D intralaminar continuum damage mechanics based material model, combining damage mode interaction and material nonlinearity, was developed to predict the damage response of composite structures undergoing crush loading. This model captures the structural response without the need for calibration of experimentally determined material parameters. When used in the design of energy absorbing composite structures, it can reduce the dependence on physical testing. This paper validates this model against experimental data obtained from the literature and in-house testing. Results show that the model can predict the force response of the crushed composite structures with good accuracy. The simulated energy absorption in each test case was within 12% of the experimental value. Post-crush deformation and the damage morphologies, such as ply splitting, splaying and breakage, were also accurately reproduced. This study establishes the capability of this damage model for predicting the responses of composite structures under crushing loads.

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Linear aerospike nozzles are envisaged as a possible device able to improve launcher engine performance. One of the most interesting properties of these nozzles is the possibility of a good integration with the vehicle. Tb improve the knowledge of the flow-field and performance of aerospike nozzles, they are studied numerically, with particular attention to the differences between the basic two-dimensional nozzle, usually considered in the design phase, and the more realistic three-dimensional nozzle. The study considers different plug lengths and ambient pressures to assess the role of the linear plug side truncation on the base pressure behavior. Numerical tests are carried out at supersonic flight Mach number. Copyright © 2005 by M. Geron and R. Paciorri.F. Nasuti, F. Sabetta, E. Martelli.

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El presente trabajo consiste en el estudio sobre el diseño de resortes helicoidales circulares a presión. El capítulo I contiene la Hipótesis, Objetivos (generales y específicos), cuestionamientos y alcances del tema de la presente tesis. El capítulo II presenta una información acerca de lsos istemas con miembros elásticos y la variación de la energía potencial elástica. El siguiente capítulo da a conocer las clases de resortes, su representación y acotación según las normas de dibujo técnico. El último capítulo trata sobre el desarrollo de la parte experimental de la tesis con el cálculo de un resorte helicoidal circular aplicado a una matriz de corte; procedimiento para el cálculo de estos elementos; y , el análisis de los valores obtenidos teóricamente con los reales.

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El presente artículo estudia la cartografía de Cacela en el sur de Portugal con el propósito de interpretar su transformación a través del tiempo, considerando la arquitectura, el urbanismo y el paisaje de forma integrada. La lectura de esa transformación se lleva de la mano de las principales cartas de Cacela que coinciden con el inicio del siglo XVII, la aproximación al final del Antiguo Régimen y la transición del siglo XIX al XX, asociando cada uno de estos tiempos a un modo particular de representación. La interpretación de las diferentes cartas está organizada, en términos me- todológicos, a partir del recurso a fuentes escritas de la época, culminando con la elaboración de un dibujo final que contiene la representación del espacio edificado y del paisaje de Cacela a mediados del siglo pasado. Este trabajo se inscribe en una investigación más amplia sobre las aglomeraciones urbanas de pequeña dimensión en las diver- sas subunidades geográficas del sur de Portugal, comprendiendo el paisaje, la morfología urbana y el levantamiento integral de todo el núcleo edificado.

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La mise en registre 3D (opération parfois appelée alignement) est un processus de transformation d’ensembles de données 3D dans un même système de coordonnées afin d’en aligner les éléments communs. Deux ensembles de données alignés ensemble peuvent être les scans partiels des deux vues différentes d’un même objet. Ils peuvent aussi être deux modèles complets, générés à des moments différents, d’un même objet ou de deux objets distincts. En fonction des ensembles de données à traiter, les méthodes d’alignement sont classées en mise en registre rigide ou non-rigide. Dans le cas de la mise en registre rigide, les données sont généralement acquises à partir d’objets rigides. Le processus de mise en registre peut être accompli en trouvant une seule transformation rigide globale (rotation, translation) pour aligner l’ensemble de données source avec l’ensemble de données cible. Toutefois, dans le cas non-rigide, où les données sont acquises à partir d’objets déformables, le processus de mise en registre est plus difficile parce qu’il est important de trouver à la fois une transformation globale et des déformations locales. Dans cette thèse, trois méthodes sont proposées pour résoudre le problème de mise en registre non-rigide entre deux ensembles de données (représentées par des maillages triangulaires) acquises à partir d’objets déformables. La première méthode permet de mettre en registre deux surfaces se chevauchant partiellement. La méthode surmonte les limitations des méthodes antérieures pour trouver une grande déformation globale entre deux surfaces. Cependant, cette méthode est limitée aux petites déformations locales sur la surface afin de valider le descripteur utilisé. La seconde méthode est s’appuie sur le cadre de la première et est appliquée à des données pour lesquelles la déformation entre les deux surfaces est composée à la fois d’une grande déformation globale et de petites déformations locales. La troisième méthode, qui se base sur les deux autres méthodes, est proposée pour la mise en registre d’ensembles de données qui sont plus complexes. Bien que la qualité que elle fournit n’est pas aussi bonne que la seconde méthode, son temps de calcul est accéléré d’environ quatre fois parce que le nombre de paramètres optimisés est réduit de moitié. L’efficacité des trois méthodes repose sur des stratégies via lesquelles les correspondances sont déterminées correctement et le modèle de déformation est exploité judicieusement. Ces méthodes sont mises en oeuvre et comparées avec d’autres méthodes sur diverses données afin d’évaluer leur robustesse pour résoudre le problème de mise en registre non-rigide. Les méthodes proposées sont des solutions prometteuses qui peuvent être appliquées dans des applications telles que la mise en registre non-rigide de vues multiples, la reconstruction 3D dynamique, l’animation 3D ou la recherche de modèles 3D dans des banques de données.

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In this study, we utilise a novel approach to segment out the ventricular system in a series of high resolution T1-weighted MR images. We present a brain ventricles fast reconstruction method. The method is based on the processing of brain sections and establishing a fixed number of landmarks onto those sections to reconstruct the ventricles 3D surface. Automated landmark extraction is accomplished through the use of the self-organising network, the growing neural gas (GNG), which is able to topographically map the low dimensionality of the network to the high dimensionality of the contour manifold without requiring a priori knowledge of the input space structure. Moreover, our GNG landmark method is tolerant to noise and eliminates outliers. Our method accelerates the classical surface reconstruction and filtering processes. The proposed method offers higher accuracy compared to methods with similar efficiency as Voxel Grid.

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The aim of this study was to evaluate the combination of abdominoplasty with liposuction of both flanks with regards to length of scar, complications, and patient's satisfaction. A retrospective analysis of 35 patients who underwent esthetic abdominoplasty at our institution between 2002 and 2004 was performed. Thirteen patients underwent abdominoplasty with liposuction of both flanks, 22 patients underwent conventional abdominoplasty. Liposuction of the flanks did not increase the rate of complications of the abdominoplasty procedures. We found a tendency toward shorter scars in patients who underwent abdominoplasty combined with liposuction of the flanks. Implementation of 3-dimensional laser surface scanning to objectify the postoperative outcomes, documented a comparable degree of flatness of the achieved body contouring in both procedures. 3-dimensional laser surface scanning can be a valuable tool to objectify assessment of postoperative results.

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The goal of this study was to investigate the performance of 3D synchrotron differential phase contrast (DPC) imaging for the visualization of both macroscopic and microscopic aspects of atherosclerosis in the mouse vasculature ex vivo. The hearts and aortas of 2 atherosclerotic and 2 wild-type control mice were scanned with DPC imaging with an isotropic resolution of 15 μm. The coronary artery vessel walls were segmented in the DPC datasets to assess their thickness, and histological staining was performed at the level of atherosclerotic plaques. The DPC imaging allowed for the visualization of complex structures such as the coronary arteries and their branches, the thin fibrous cap of atherosclerotic plaques as well as the chordae tendineae. The coronary vessel wall thickness ranged from 37.4 ± 5.6 μm in proximal coronary arteries to 13.6 ± 3.3 μm in distal branches. No consistent differences in coronary vessel wall thickness were detected between the wild-type and atherosclerotic hearts in this proof-of-concept study, although the standard deviation in the atherosclerotic mice was higher in most segments, consistent with the observation of occasional focal vessel wall thickening. Overall, DPC imaging of the cardiovascular system of the mice allowed for a simultaneous detailed 3D morphological assessment of both large structures and microscopic details.