Cette thèse porte sur les effets combinés de l’excentricité et du débit axial sur les propriétés de stabilité linéaire de l’écoulement de Couette circulaire avec cylindre extérieur fixe. Cet écoulement intervient, entre autres, lors du forage de puits de pétrole. Une méthode pseudospectrale est mise en oeuvre pour calculer l’écoulement de base, stationnaire et invariant suivant la direction axiale, ainsi que les modes normaux d’instabilité. L’écoulement est régi par quatre paramètres adimensionnels : rapport de rayons _ et excentricité e pour la géométrie, nombres de Reynolds azimuthal et axial, Re et Rez, pour la dynamique. La première partie de l’étude est consacrée aux propriétés de stabilité temporelle. Il apparaît que l’excentricité repousse le seuil d’instabilité convective vers de plus fortes valeurs de Re. L’effet de l’advection axiale sur le seuil est principalement stabilisant également. L’excentricité a pour conséquence de déformer la structure des modes par rapport au cas concentrique. Le mode au plus fort taux de croissance temporelle est ainsi constitué de tourbillons de Taylor « pseudo-toroïdaux » lorsque le débit axial est nul, et de structures « pseudo-hélicoïdales » d’ordre azimuthal croissant lorsque Rez augmente. Les résultats sont qualitativement similaires lorsque l’on change le rapport de rayons. Les prédictions théoriques sont en bon accord avec les quelques résultats expérimentaux disponibles. Dans une seconde partie, l’instabilité absolue est étudiée par application d’un critère de point selle à la relation de dispersion. Le débit axial a pour effet d’inhiber fortement l’instabilité absolue, d’origine centrifuge, et la valeur de Re au seuil est typiquement supérieure à celle de Rez d’un ordre de grandeur. L’effet de l’excentricité est plus complexe : légère stabilisation aux faibles valeurs de e, puis déstabilisation marquée aux excentricités modérées lorsque Rez est suffisament grand, et enfin stabilisation lorsque e croît davantage. Contrairement au cas de l’instabilité convective, le mode dominant l’instabilité absolue correspond à l’écoulement tourbillonnaire « pseudo-toroïdal » pour toute la gamme de paramètres considérée. / This work is concerned with the combined effects of eccentricity and pressure-driven axial flow on the linear stability properties of circular Couette flow with a fixed outer cylinder. An example of this flow can be found in oil-well drilling operations. A pseudospectral method is implemented to compute the basic flow, steady and homogeneous in the axial direction, as well as the normal modes of instability. There are four non-dimensional parameters: the radius ratio _ and the eccentricity e for the geometry, the azimuthal and axial Reynolds numbers, Re and Rez, for the dynamics. The first part of the study is devoted to the temporal stability properties. It is found that eccentricity pushes the convective instability threshold towards higher values of Re. The effect of axial advection on the threshold also tends to be stabilising. Eccentricity deforms the modes structure compared to the concentric case. As a result, the mode with the largest temporal growth rate takes the form of ‘pseudo-toroidal’ Taylor vortices in the absence of axial flow, and ‘pseudo-helical’ structures with increasing azimuthal order as Rez becomes larger. Results are qualitatively similar for different radius ratios. Agreement with the few available experimental data is good. In a second part, absolute instability is studied by applying the pinch-point criterion to the dispersion relation. Axial flow is found to strongly inhibit absolute instability, the mechanism of which being centrifugal, and the value of Re at the threshold is typically one order of magnitude larger than that of Rez. The effect of eccentricity is more complex: weak stabilisation for low values of e, marked destabilisation for moderate eccentricities and high enough Rez, and finally stabilisation as e is further increased. Unlike temporal instability, the dominant absolutely unstable mode is the ‘pseudo-toroidal’ Taylor vortex flow over the whole range of parameter space considered.

No description available.

Published Article / The paper highlights the design, development and evaluation of a hybrid convective-far-infrared (FIR) dehydrator for the purpose of drying fruit. The methodology followed is based on an experimental and practical approach. The application of the dryer for this study is aimed at the production of apple chips as well as other types of fruit chips and the more common dried fruit. The fruit dryer proposed uses both infrared energy and convective heating to effectively and efficiently dehydrate apple slices to produce dried apple chips. The apple chips are produced in very short time frames and accomplished by using relatively low heater power. These types of apple chip snacks also contribute to the more healthy variety of snacks available on the market.

No description available.

Neste estudo sao analisados os sistemas convectivos de mesoescala (SCMs) subtropicais, de origem continental e oceanica, observados na America do Sul durante o South American Low Level Experiment (SALLJEX), realizado no verao de 2002/2003. Nesta analise sao avaliadas a distribuicao espacial, variabilidade diurna, ciclo de vida, deslocamento e parametros morfologicos dos SCMs continentais e oceanicos, sendo tambem investigadas as origens das fontes de umidade que contribuem para a genese desses sistemas. Outros aspectos explorados sao a caracterizacao das condicoes sinoticas com atencao a identificacao dos fatores pre-condicionantes e mecanismos de gatilho a conveccao; a avaliacao das condicoes dinamicas e termodinamicas observadas durante a genese do sistema convectivo e sua evolucao ao longo do ciclo de vida. Alem disso, sao realizadas simulacoes numericas dos SCMs com enfoque na verificacao da qualidade da previsao de precipitacao em funcao da capacidade do modelo em reproduzir as condicoes atmosfericas essenciais a geracao da conveccao. Os resultados mostram que os sistemas convectivos continentais sao mais numerosos que os oceanicos, e em ambas as regioes, SCMs com maior duracao apresentam taxas de expansao maiores nas primeiras horas do seu ciclo de vida. O jato de baixos niveis (JBN) afeta a formacao de sistemas continentais, porem, seu efeito sobre os SCMs oceanicos e minimo. O oceano Atlantico tropical, a regiao Amazonica e o oceano Pacifico subtropical, sao as principais regioes de origem da umidade para a genese dos sistemas convectivos, contudo, a atuacao dessas fontes depende da regiao de formacao do sistema e das condicoes sinoticas. O aquecimento diurno da camada limite convectiva, o jato de baixos niveis, o cavado em 500 hPa e a circulacao transversa sao os pre-condicionantes identificados na formacao dos SCMs continentais noturnos. Em relacao aos mecanismos de gatilho, os principais fatores sao os sistemas frontais e o fluxo catabatico dos Andes. Sistemas convectivos que apresentam ciclo de vida mais longo sao gerados em um ambiente em que se identificam mais de um fator pre-condicionante e de gatilho atuando de forma conjunta. Alem disso, o cisalhamento vertical do vento em baixos niveis parece ser um dos diferenciais na fase inicial dos SCMs de maior duracao. Os resultados das simulacoes numericas sugerem que quando as caracteristicas sinoticas e de mesoescala que atuam como pre-condicionantes ou mecanismos de gatilho sao mais bem definidas, o desempenho do modelo melhora sensivelmente, pois a simulacao consegue reproduzir com mais precisao as condicoes ambientais observadas durante a genese do sistema convectivo. Assim, sistemas com maior duracao tendem a ser mais bem simulados. / In this study, we analyze continental and oceanic mesoscale convective systems (MCS\'s) observed in the subtropics of South America during the South American Low Level Experiment (SALLJEX), held in the summer of 2002/2003. This analysis evaluated the spatial distribution, diurnal variability, life cycle, displacement and morphological parameters of the continental and oceanic MCSs, and also investigated the origins of moisture sources that contribute to these systems genesis. Other issues considered are the characterization of the synoptic conditions and the identification of preconditioning and trigger mechanisms, and evaluation of dynamic and thermodynamic conditions observed during the convective system genesis and its evolution over the life cycle. Moreover, MCSs numerical simulations are made focused on the model capability to replicate the essential atmospheric conditions to the convection generation. The results show that the continental convective systems are more numerous than the oceanic ones, and in both regions, MCS\'s with longer duration have higher growth rates in the early hours of their life cycle. The low level jet (LLJ) affects the formation of the continental systems, but its effect on oceanic MCS\'s is minimal. The tropical Atlantic Ocean, the Amazon region and the subtropical Pacific Ocean, are the main moisture source to the genesis of convective systems, however, the incidence of these sources depends on the convective system genesis area and the synoptic conditions. The daytime heating of convective boundary layer, the low level jet, the trough at 500 hPa and transverse circulation are the preconditioning processes identified in the formation of nocturnal MCS\'s with continental origin. For trigger mechanisms, the main factors are the frontal systems and the katabatic flow from the Andes Mountain. Convective systems with longer life cycles are generated in an environment in which several preconditioning and trigger mechanisms act jointly. Moreover, the vertical wind shear at low levels appears to be one of the differences in the initial phase of long living MCSs. The results of numerical simulations suggest that when the characteristics of synoptic and mesoscale that act as pre-conditions or triggering mechanisms are better defined, the model\'s performance improves significantly, because the simulation can more accurately reproduce the environmental conditions observed during the genesis of the convective system. Thus, systems with longer duration tend to be better simulated.

Neste estudo sao analisados os sistemas convectivos de mesoescala (SCMs) subtropicais, de origem continental e oceanica, observados na America do Sul durante o South American Low Level Experiment (SALLJEX), realizado no verao de 2002/2003. Nesta analise sao avaliadas a distribuicao espacial, variabilidade diurna, ciclo de vida, deslocamento e parametros morfologicos dos SCMs continentais e oceanicos, sendo tambem investigadas as origens das fontes de umidade que contribuem para a genese desses sistemas. Outros aspectos explorados sao a caracterizacao das condicoes sinoticas com atencao a identificacao dos fatores pre-condicionantes e mecanismos de gatilho a conveccao; a avaliacao das condicoes dinamicas e termodinamicas observadas durante a genese do sistema convectivo e sua evolucao ao longo do ciclo de vida. Alem disso, sao realizadas simulacoes numericas dos SCMs com enfoque na verificacao da qualidade da previsao de precipitacao em funcao da capacidade do modelo em reproduzir as condicoes atmosfericas essenciais a geracao da conveccao. Os resultados mostram que os sistemas convectivos continentais sao mais numerosos que os oceanicos, e em ambas as regioes, SCMs com maior duracao apresentam taxas de expansao maiores nas primeiras horas do seu ciclo de vida. O jato de baixos niveis (JBN) afeta a formacao de sistemas continentais, porem, seu efeito sobre os SCMs oceanicos e minimo. O oceano Atlantico tropical, a regiao Amazonica e o oceano Pacifico subtropical, sao as principais regioes de origem da umidade para a genese dos sistemas convectivos, contudo, a atuacao dessas fontes depende da regiao de formacao do sistema e das condicoes sinoticas. O aquecimento diurno da camada limite convectiva, o jato de baixos niveis, o cavado em 500 hPa e a circulacao transversa sao os pre-condicionantes identificados na formacao dos SCMs continentais noturnos. Em relacao aos mecanismos de gatilho, os principais fatores sao os sistemas frontais e o fluxo catabatico dos Andes. Sistemas convectivos que apresentam ciclo de vida mais longo sao gerados em um ambiente em que se identificam mais de um fator pre-condicionante e de gatilho atuando de forma conjunta. Alem disso, o cisalhamento vertical do vento em baixos niveis parece ser um dos diferenciais na fase inicial dos SCMs de maior duracao. Os resultados das simulacoes numericas sugerem que quando as caracteristicas sinoticas e de mesoescala que atuam como pre-condicionantes ou mecanismos de gatilho sao mais bem definidas, o desempenho do modelo melhora sensivelmente, pois a simulacao consegue reproduzir com mais precisao as condicoes ambientais observadas durante a genese do sistema convectivo. Assim, sistemas com maior duracao tendem a ser mais bem simulados. / In this study, we analyze continental and oceanic mesoscale convective systems (MCS\'s) observed in the subtropics of South America during the South American Low Level Experiment (SALLJEX), held in the summer of 2002/2003. This analysis evaluated the spatial distribution, diurnal variability, life cycle, displacement and morphological parameters of the continental and oceanic MCSs, and also investigated the origins of moisture sources that contribute to these systems genesis. Other issues considered are the characterization of the synoptic conditions and the identification of preconditioning and trigger mechanisms, and evaluation of dynamic and thermodynamic conditions observed during the convective system genesis and its evolution over the life cycle. Moreover, MCSs numerical simulations are made focused on the model capability to replicate the essential atmospheric conditions to the convection generation. The results show that the continental convective systems are more numerous than the oceanic ones, and in both regions, MCS\'s with longer duration have higher growth rates in the early hours of their life cycle. The low level jet (LLJ) affects the formation of the continental systems, but its effect on oceanic MCS\'s is minimal. The tropical Atlantic Ocean, the Amazon region and the subtropical Pacific Ocean, are the main moisture source to the genesis of convective systems, however, the incidence of these sources depends on the convective system genesis area and the synoptic conditions. The daytime heating of convective boundary layer, the low level jet, the trough at 500 hPa and transverse circulation are the preconditioning processes identified in the formation of nocturnal MCS\'s with continental origin. For trigger mechanisms, the main factors are the frontal systems and the katabatic flow from the Andes Mountain. Convective systems with longer life cycles are generated in an environment in which several preconditioning and trigger mechanisms act jointly. Moreover, the vertical wind shear at low levels appears to be one of the differences in the initial phase of long living MCSs. The results of numerical simulations suggest that when the characteristics of synoptic and mesoscale that act as pre-conditions or triggering mechanisms are better defined, the model\'s performance improves significantly, because the simulation can more accurately reproduce the environmental conditions observed during the genesis of the convective system. Thus, systems with longer duration tend to be better simulated.

A Zona de Convergência do Atlântico Sul (ZCAS) é um fenômeno meteorológico que exerce um papel preponderante no regime de chuvas na região onde atua, acarretando altos índices pluviométricos na América do Sul. Este estudo mostra que, em uma análise de mesoescala, um Vórtice Ciclônico de Mesoescala (VCM) está associado à ZCAS através de um processo de retroalimentação. Este sistema é gerado dentro de um ambiente estratiforme na região da ZCAS, suga a umidade, acelera os ventos na vertical provocando intensa precipitação e, como conseqüência, pode afetar drasticamente as regiões atingidas provocando sérios danos sócio-econômicos. Este trabalho enfoca a atuação destes VCMs que se formam associados à ZCAS, identificando as propriedades termodinâmicas durante os diversos estágios de seu ciclo de vida. O trabalho é desenvolvido em três fases: (a) documentação da representação da precipitação e do transporte de umidade para a região da ZCAS através de conjuntos de reanálises de nova geração; (b) avaliação da importância da atuação dos VCMs embebidos na ZCAS, através do desenvolvimento de um sistema de detecção para determinação de estatística de ocorrência e (c) realização de simulações com o modelo de mesoescala BRAMS (Brazilian Regional Atmospheric Modeling System) para compreensão do comportamento de episódios específicos destes sistemas de mesoescala e sua relação com a ZCAS. A primeira parte do trabalho evidencia o avanço das novas reanálises da tentativa de representar de forma mais adequada à variável precipitação acumulada na região da ZCAS. A documentação é baseada em seis conjuntos de reanálises atmosféricas (MERRA, ERA-Interim, ERA-40, NCEP 1, NCEP 2 e NCEP CFSR) e cinco conjuntos de produtos observados de precipitação (SALDAS, CPC, CMAP, GPCP e GLDAS). Através das reanálises também foi avaliado o transporte de umidade sobre a região da ZCAS, para os anos de 1979 a 2007. Os diagramas de Taylor mostram que os produtos de precipitação estão bem correlacionados com o ponto de referência (CPC), com coeficientes entre 0,6 e 0,9. Somente a reanálise do NCEP CFSR possui correlações próximas as dos produtos de precipitação. Os VCMs, embebidos na banda de nebulosidade da ZCAS, são selecionados através de um critério objetivo de detecção, baseado na vorticidade e circulação do sistema, aplicado ao período de 2000 a 2009. Um total de 300 VCMs úmidos foram detectados na baixa troposfera, enquanto que na média e alta troposfera foram detectados 277 VCMs. Na baixa troposfera a maioria dos VCMs úmidos se localiza mais para SW na região continental costeira (ZCC) da ZCAS. Verifica-se também uma concordância entre os vórtices destas regiões de máxima vorticidade ciclônica e os extremos de precipitação. O estudo de dois casos específicos nas regiões da Continental Amazônica (ZCA) e ZOC, simulados através do modelo BRAMS, enfoca a relação entre a formação de mesovórtices e a atividade convectiva presente próximo à região de formação. Em ambas as regiões, os VCMs apresentam características similares, que podem ser consideradas como uma assinatura do sistema. Nos dois casos simulados estes sistemas apresentam o ciclo de vida inferior a 24 horas, escala espacial de aproximadamente 200 x 200 km2, intensa precipitação, deslocamento no mesmo sentido do escoamento na baixa troposfera, vorticidade relativa da mesma ordem de magnitude do parâmetro de Coriolis (10-4 s-1), núcleo quente acima do nível de máxima intensidade e um rápido crescimento do centro de vorticidade ciclônica principalmente nos baixos níveis. O balanço de vorticidade e o ciclo de energia desses sistemas são analisados. Pela comparação da chuva simulada com o produto Hidroestimador, sugere-se que o modelo BRAMS, com uma alta resolução espacial e temporal, melhora a representação do VCM, comparado com os dados da reanálise CFSR do NCEP. / The South Atlantic Convergence Zone (SACZ) is a meteorological phenomena that plays an important role in the precipitation regime over the region it covers, resulting in a high pluviometric indices in South America. This study shows, from the mesoscale analysis prospective that Mesoscale Cyclonic Vortex (MCV) is associated to the SACZ through a feedback process. This system is generated embedded in a stratiform environment within the SACZ region, taking moisture up, increasing vertical winds resulting in intense precipitation and consequently can affect drastically susceptible regions prone to natural disasters causing serious social and economic problems. This study highlights the MCVs associated to the SACZ, identifying the thermodynamic properties of the various stages during its lifetime cycle. This study is separated in 3 distinct parts as follows: (a) document the representation of the precipitation and moisture transport into the SACZ new generation reanalysis; (b) develop a detection system to compute the frequency statistics to assess the importance of the embedded MCVs to the SACZ and (c) use of the BRAMS (Brazilian Regional Atmospheric Modeling System) mesoscale model to understand specific MCVs episodes and its relationship with SACZ. In its first part, this work clearly shows the progresses made by the new reanalysis on the correct representation of the accumulated precipitation over the SACZ region. The documentation is based upon six atmospheric reanalysis datasets namely MERRA, ERA-Interim, ERA-40, NCEP 1, NCEP 2 and NCEP CFSR in addition to five precipitation products namely SALDAS, CPC, CMAP, GPCP and GLDAS. The reanalysis were also used to assess the moisture transport over the SACZ region from 1979 through 2007. Taylor plots show that the precipitation products are well associated to the reference dataset (CPC) with correlation coefficients varying between 0,6 and 0,9. Furthermore, only the NCEP CFSR reanalysis present precipitation correlation close to the abovementioned products. The MCVs embedded within the SACZ cloud bands are selected through an objective detection criteria based on the vorticity and circulation of the system, performed from 2000 to 2009. A total of 300 moist MCVs were detected in the lower troposphere whereas in the medium and high troposphere 277 were detected. Most of the MCVs in the lower troposphere were located in the Southwestern region of the continental coastal line of the SACZ and are possibly associated to topographic effects and local instability caused by incursion of transient systems into the SACZ region. Moreover, the vortices in this region match very well the regions of maximum cyclonic vorticity and maximum precipitation intensity. Two case studies were conducted over the Continental Amazonia Zone, simulated using the BRAMS model, showing the relationship between the mesovortices formation and the convective activity near its formation region. In both regions the MCVs present similar characteristics which could be considered as a \"signature\" for such systems. The case studies also present a lifetime shorter than 24 hours and spatial scale of approximately 200 km2 in addition to intense precipitation, shifting in the flow direction in the lower troposphere, relative vorticity of the same order as the Coriolis parameter (10-4 s-1), warm core above the level of maximum intensity and rapid growth of the cyclonic vorticity center mostly in the lower levels. The vorticity balance and the energy cycle of these systems is then analyzed. The simulated precipitation is compared against the Hidroestimador precipitation product. The results suggest that the BRAMS model, configured with high spatial and temporal resolutions improves the representation of the MCVs when compared to the NCEP CFSR reanalysis.

In the summer of 2007, the number of people living in the world’s urban areas exceeded that of those living in the countryside. Such urbanisation tends to modify the climates of towns and cities as a result of a number of factors which together form the ‘urban heat island’ effect. In order to better design buildings and urban areas to cope with these effects, it is first necessary to understand the heat transfer mechanisms which are taking place. The aim of the current research has therefore been to provide convective heat transfer data appropriate for low-rise urban environments by investigating the effects of wind speed, direction and street geometry. The research has employed the naphthalene sublimation technique which has been extended in several fundamental areas including development of a novel approach to measure the rate of sublimation from wind tunnel models. This technique has permitted measurements to be made over an array of discrete locations, revealing the variation across building surfaces. The uncertainty in the convective heat transfer coefficients obtained was calculated to be approximately ±6%. Tests were conducted in the BRE wind tunnel with an atmospheric boundary layer simulation appropriate to inner city areas. Cube models were arranged so as to form long rows of flat-roofed buildings referred to as ‘street canyons’. A series of correlations have been derived from the experimental results from which the rate of convection occurring from each building surface may be obtained with respect to wind speed. The greatest rates of convective heat transfer have been shown to occur at the top of the windward wall and leading edge of the roof, the lowest rates from the leeward wall of a building. Convection was found to be reduced in narrow street canyons. In wider street canyons, the convective coefficients on the exposed windward and roof surfaces of buildings were higher, but the values on the leeward wall are lessened due to the distancing of the downstream windward vortex. The effect of wind direction was found to be relatively small and therefore it is proposed that the convective heat transfer relationships presented may be applied irrespective of wind direction.

The Great Basin is a region of the Basin and Range Physiographic Province, which is completely isolated hydrologically from the sea. All precipitation that falls within the Great Basin is lost from the land surface or from the surf ace of closed inland lakes through evapotranspiration. Playas are often found at the base of these undrained basins. This study focuses on subsurface groundwater flow patterns in closed basins. Because all discharge from the basins occurs via evapotranspiration on and near the playa, the water table of the aquifer beneath the playa is often just below the ground surface. Fluctuations of the water table due to climatic events cause the water table to rise and dissolve the salts on the playa surface. This mass transfer can produce density gradients that in turn cause flow. This study is an extension of the work performed by Duffy and Al-Hassan (Duffy and Al-Hassan 1988) in which numerical experiments were used to show that the free convection, caused by the variation in density of the bulk fluid propenies, appears to play an important role in determining the patterns of groundwater flow beneath the playa. Their work considered only homogeneous, isotropic porous media in symmetric basins. The effects of anisotropy, periodic stratification, and asymmetric basins on the groundwater flow and transport patterns was studied here. Dimensionless parameters, the Rayleigh number and the salt nose length, L0*, were defined for each of the systems incorporated and were shown to be linearly related. The implication of this relationship is that the Rayleigh number can be used to predict basin-scale circulation patterns in the hypothetical closed basins studied. It was also determined that an equivalent anisotropic system could be defined for a horizontally stratified aquifer in order to predict basin-scale circulation patterns. An equivalent isotropic system was defined for each anisotropic system in a similar manner.

Data from the GARP Atlantic Tropical Experiment (GATE) was analysed in an exploratory manner to discover the characteristics of mesoscale organization of convection and it's relationship to large-scale wind profiles. Automated methods were developed to identify the convective cells and their linear organization. These automated methods use a median high-pass filter to identify enhanced cells and a simple pattern recognition technique to ascertain the linear organization between them. Due to the simplified nature of the algorithm, the whole data set of the 21 day period from the phase 3 of GATE was processed in an economical manner obtaining a large data base which was used in the investigation of clusters and other associated phenomena. The mesoscale organization of convective cells and the widespread areas of lighter precipitation associated with them showed expected characteristics and compared satisfactorily with previous results. A large fraction of the rainfall (64%) fell from the widespread area. The total precipitation had a correlation of 0.94 with the fractional area of the widespread and a correlation of 0.89 with the fractional area of the clusters. The widespread precipitation had a correlation index of 0.97 with it's fractional area and the cluster precipitation had a strong linear relationship to it's area with a correlation of 0.99. These factors argue well for the parameterization of rainfall rate in tropical regions to a high accuracy by the area covered by organized convective cells and widespread areas. It was also seen that there was a good correlation with the number of clusters and number of cores with the total precipitation rate in a given area. These factors create a strong argument for identifying mesoscale systems consisting of convective cells and widespread precipitation as basic units of precipitation in tropical regions, having a characteristic life cycle of their own. The widespread and total precipitation showed very good correlation with upper-level vertical motion. Clusters tended to align parallel with the horizontal low-level wind shear and the degree of alignment appears to depend on the strength of the wind shear. / Graduation date: 1991