907 resultados para camera link
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We will prove that, for a 2 or 3 component L-space link, HFL- is completely determined by the multi-variable Alexander polynomial of all the sub-links of L, as well as the pairwise linking numbers of all the components of L. We will also give some restrictions on the multi-variable Alexander polynomial of an L-space link. Finally, we use the methods in this paper to prove a conjecture of Yajing Liu classifying all 2-bridge L-space links.
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[ES]Mediante este trabajo se va a diseñar un mecanismo para crear un sistema de suspensión progresiva para la suspensión trasera de una motocicleta a partir de un muelle lineal. El muelle introducido en la suspensión será lineal, por lo tanto, tendrá una sola rigidez, constante y la cual delimita el muelle, pero gracias a un mecanismo diseñado especialmente para la suspensión trasera de una moto, se va conseguir que la rigidez varíe. El mecanismo utilizado para este trabajo se llama Pro-Link y la empresa que lo emplea es Honda. Para ello, se creará un esquema del mecanismo en sí y tras un análisis cinemático mediante el programa Creo Parametric, y haciendo varios cambios en el sistema para ajustarlo a la mejor progresividad posible, se obtendrá la gráfica en la que se observará la curva que marca la rigidez progresiva. Esto es, se verá la evolución de la nueva rigidez dependiendo de la oscilación vertical de la rueda. Por otra parte, gracias a un análisis dinámico del mismo programa se conseguirán las reacciones del sistema y se calcularán los elementos auxiliares de éste para el buen funcionamiento del mismo. Finalmente, se creará el diseño del triángulo y un diseño preliminar del basculante mediante el método de elementos finitos del programa.
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The first part of this thesis combines Bolocam observations of the thermal Sunyaev-Zel’dovich (SZ) effect at 140 GHz with X-ray observations from Chandra, strong lensing data from the Hubble Space Telescope (HST), and weak lensing data from HST and Subaru to constrain parametric models for the distribution of dark and baryonic matter in a sample of six massive, dynamically relaxed galaxy clusters. For five of the six clusters, the full multiwavelength dataset is well described by a relatively simple model that assumes spherical symmetry, hydrostatic equilibrium, and entirely thermal pressure support. The multiwavelength analysis yields considerably better constraints on the total mass and concentration compared to analysis of any one dataset individually. The subsample of five galaxy clusters is used to place an upper limit on the fraction of pressure support in the intracluster medium (ICM) due to nonthermal processes, such as turbulent and bulk flow of the gas. We constrain the nonthermal pressure fraction at r500c to be less than 0.11 at 95% confidence, where r500c refers to radius at which the average enclosed density is 500 times the critical density of the Universe. This is in tension with state-of-the-art hydrodynamical simulations, which predict a nonthermal pressure fraction of approximately 0.25 at r500c for the clusters in this sample.
The second part of this thesis focuses on the characterization of the Multiwavelength Sub/millimeter Inductance Camera (MUSIC), a photometric imaging camera that was commissioned at the Caltech Submillimeter Observatory (CSO) in 2012. MUSIC is designed to have a 14 arcminute, diffraction-limited field of view populated with 576 spatial pixels that are simultaneously sensitive to four bands at 150, 220, 290, and 350 GHz. It is well-suited for studies of dusty star forming galaxies, galaxy clusters via the SZ Effect, and galactic star formation. MUSIC employs a number of novel detector technologies: broadband phased-arrays of slot dipole antennas for beam formation, on-chip lumped element filters for band definition, and Microwave Kinetic Inductance Detectors (MKIDs) for transduction of incoming light to electric signal. MKIDs are superconducting micro-resonators coupled to a feedline. Incoming light breaks apart Cooper pairs in the superconductor, causing a change in the quality factor and frequency of the resonator. This is read out as amplitude and phase modulation of a microwave probe signal centered on the resonant frequency. By tuning each resonator to a slightly different frequency and sending out a superposition of probe signals, hundreds of detectors can be read out on a single feedline. This natural capability for large scale, frequency domain multiplexing combined with relatively simple fabrication makes MKIDs a promising low temperature detector for future kilopixel sub/millimeter instruments. There is also considerable interest in using MKIDs for optical through near-infrared spectrophotometry due to their fast microsecond response time and modest energy resolution. In order to optimize the MKID design to obtain suitable performance for any particular application, it is critical to have a well-understood physical model for the detectors and the sources of noise to which they are susceptible. MUSIC has collected many hours of on-sky data with over 1000 MKIDs. This work studies the performance of the detectors in the context of one such physical model. Chapter 2 describes the theoretical model for the responsivity and noise of MKIDs. Chapter 3 outlines the set of measurements used to calibrate this model for the MUSIC detectors. Chapter 4 presents the resulting estimates of the spectral response, optical efficiency, and on-sky loading. The measured detector response to Uranus is compared to the calibrated model prediction in order to determine how well the model describes the propagation of signal through the full instrument. Chapter 5 examines the noise present in the detector timestreams during recent science observations. Noise due to fluctuations in atmospheric emission dominate at long timescales (less than 0.5 Hz). Fluctuations in the amplitude and phase of the microwave probe signal due to the readout electronics contribute significant 1/f and drift-type noise at shorter timescales. The atmospheric noise is removed by creating a template for the fluctuations in atmospheric emission from weighted averages of the detector timestreams. The electronics noise is removed by using probe signals centered off-resonance to construct templates for the amplitude and phase fluctuations. The algorithms that perform the atmospheric and electronic noise removal are described. After removal, we find good agreement between the observed residual noise and our expectation for intrinsic detector noise over a significant fraction of the signal bandwidth.
Resumo:
El objetivo de este proyecto ha sido el de diseñar un sistema de suspensión englobado en el ámbito de la competición interuniversitaria MotoStudent. Además de la normativa de la competición, dicha suspensión debe cumplir una serie de requisitos extra impuestos por el equipo de MotoStudent de la ETSI de Bilbao. Las características principales de la suspensión en cuestión deben ser las siguientes: La rigidez del sistema de suspensión debe ser progresiva, de forma que se comporte como una suspensión blanda a bajas solicitaciones, y como una suspensión dura a altas solicitaciones. A fin de poder adaptar la suspensión de la moto a diferentes circuitos, el esta deberá estar dotada de un sistema de regulación. Para ello el sistema de suspensión elegido es el sistema por bieletas tipo Pro- Link, cuya principal característica es que, en dicha solución, el balancín no solo tiene movimiento angular, sino que tiene también movimiento lineal, de forma que es mucho más versátil a la hora de diseñar. Figura[
Resumo:
A stereo-video baited camera system (BotCam) has been developed as a fishery-independent tool to monitor and study deepwater fish species and their habitat. During testing, BotCam was deployed primarily in water depths between 100 and 300 m for an assessment of its use in monitoring and studying Hawaiian bottomfish species. Details of the video analyses and data from the pilot study with BotCam in Hawai`i are presented. Multibeam bathymetry and backscatter data were used to delineate bottomfish habitat strata, and a stratified random sampling design was used for BotCam deployment locations. Video data were analyzed to assess relative fish abundance and to measure f ish size composition. Results corroborate published depth ranges and zones of the target species, as well as their habitat preferences. The results indicate that BotCam is a promising tool for monitoring and studying demersal fish populations associated with deepwater habitats to a depth of 300 m, at mesohabitat scales. BotCam is a flexible, nonextractive, and economical means to better understand deepwater ecosystems and improve science-based ecosystem approaches to management.
Resumo:
We describe the application of two types of stereo camera systems in fisheries research, including the design, calibration, analysis techniques, and precision of the data obtained with these systems. The first is a stereo video system deployed by using a quick-responding winch with a live feed to provide species- and size- composition data adequate to produce acoustically based biomass estimates of rockfish. This system was tested on the eastern Bering Sea slope where rockfish were measured. Rockfish sizes were similar to those sampled with a bottom trawl and the relative error in multiple measurements of the same rockfish in multiple still-frame images was small. Measurement errors of up to 5.5% were found on a calibration target of known size. The second system consisted of a pair of still-image digital cameras mounted inside a midwater trawl. Processing of the stereo images allowed fish length, fish orientation in relation to the camera platform, and relative distance of the fish to the trawl netting to be determined. The video system was useful for surveying fish in Alaska, but it could also be used broadly in other situations where it is difficult to obtain species-composition or size-composition information. Likewise, the still-image system could be used for fisheries research to obtain data on size, position, and orientation of fish.
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É apresentado como problema atual na área de Publicidade e Propaganda a exibição de conteúdo personalizado para nichos específicos. A propaganda acaba se concentrando nos produtos de maior sucesso, tendo como foco alguns públicos-alvo previamente determinados. Assim, o estudo pretende avaliar um novo canal para exibição de propaganda em nível individual, através das perspectivas da Cauda Longa e da Realidade Aumentada (R.A.). O ponto principal desse trabalho é, portanto, mostrar a quantidade de nichos existentes e sugerir uma personalização da propaganda a um nível praticamente individual, como uma ligação direta entre produto e consumidor, usando como suporte tecnológico a R.A. A partir da análise de trabalhos de Romero Tori, Paul Milgram, Ronald Azuma, Cláudio Kirner, Robson Siscouto, Lúcia Santaella, entre outros autores, foi feita uma avaliação dos principais pontos de interesse da tecnologia de Realidade Aumentada para profissionais da área do Design. Discorrendo não só sobre suas características como também identificando problemas e questionamentos atuais, tanto para esses profissionais como para o consumidor final. A tese se enquadra na linha de pesquisa de Design e Tecnologia ao passo que os profissionais desta área de conhecimento são responsáveis diretos por pensar as formas de interação de modo que sejam mais orgânicas e intuitivas para os usuários. Existe muito trabalho a ser realizado, no tocante à Ergonomia e Usabilidade, nas soluções que usam a Realidade Aumentada, principalmente na forma como se dá a sobreposição da informação digital ao ambiente real capturado pela câmera e sua manipulação pelo indivíduo.