1000 resultados para textural evolution


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Context. The understanding of Galaxy evolution can be facilitated by the use of population synthesis models, which allow to test hypotheses on the star formation history, star evolution, as well as chemical and dynamical evolution of the Galaxy. Aims. The new version of the Besanc¸on Galaxy Model (hereafter BGM) aims to provide a more flexible and powerful tool to investigate the Initial Mass Function (IMF) and Star Formation Rate (SFR) of the Galactic disc. Methods. We present a new strategy for the generation of thin disc stars which assumes the IMF, SFR and evolutionary tracks as free parameters. We have updated most of the ingredients for the star count production and, for the first time, binary stars are generated in a consistent way. We keep in this new scheme the local dynamical self-consistency as in Bienayme et al (1987). We then compare simulations from the new model with Tycho-2 data and the local luminosity function, as a first test to verify and constrain the new ingredients. The effects of changing thirteen different ingredients of the model are systematically studied. Results. For the first time, a full sky comparison is performed between BGM and data. This strategy allows to constrain the IMF slope at high masses which is found to be close to 3.0, excluding a shallower slope such as Salpeter"s one. The SFR is found decreasing whatever IMF is assumed. The model is compatible with a local dark matter density of 0.011 M pc−3 implying that there is no compelling evidence for significant amount of dark matter in the disc. While the model is fitted to Tycho2 data, a magnitude limited sample with V<11, we check that it is still consistent with fainter stars. Conclusions. The new model constitutes a new basis for further comparisons with large scale surveys and is being prepared to become a powerful tool for the analysis of the Gaia mission data.

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OBJETIVO: Possibilitar a distinção entre tecidos sãos e patológicos em pacientes da faixa etária pediátrica portadores de tumores da fossa posterior, por meio da análise de parâmetros texturais calculados a partir de imagens de ressonância magnética. MATERIAIS E MÉTODOS: Foram analisados 14 pacientes da faixa etária pediátrica, portadores de tumores da fossa posterior, através da definição dos valores texturais das regiões de interesse representando tecidos sãos e patológicos, com base em imagens de ressonância magnética pesadas em T2 pelo "software" MaZda. RESULTADOS: Houve diferença estatisticamente significativa entre os tecidos normal e tumoral, bem como entre os tecidos presumidamente normais adjacentes e distantes da lesão. Não foi possível a distinção entre edema e tumor. CONCLUSÃO: A avaliação textural por ressonância magnética é uma técnica útil para a determinação de diferenças entre diversos tipos de tecidos, inclusive entre áreas de tecidos presumidamente normais à análise visual.

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In this paper we focus our attention on a particle that follows a unidirectional quantum walk, an alternative version of the currently widespread discrete-time quantum walk on a line. Here the walker at each time step can either remain in place or move in a fixed direction, e.g., rightward or upward. While both formulations are essentially equivalent, the present approach leads us to consider discrete Fourier transforms, which eventually results in obtaining explicit expressions for the wave functions in terms of finite sums and allows the use of efficient algorithms based on the fast Fourier transform. The wave functions here obtained govern the probability of finding the particle at any given location but determine as well the exit-time probability of the walker from a fixed interval, which is also analyzed.

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Understanding the birth and diversification of multigene families is a fundamental evolutionary problem. I argue for the insect chemoreceptor superfamily as an outstanding model. Although these receptors are currently the preserve of neuroscientists, putative homologous genes exist in diverse animal and plant genomes, implying an ancient origin. Moreover, functional studies suggest that they act as ligand-gated ion channels in both chemosensory and non-chemosensory processes. This family permits synergism of investigations into its structural and regulatory evolution with ecological studies of the selective pressures driving these changes. In addition, sequence divergence in these receptors can be exploited through co-evolutionary and comparative genomics analyses to help to elucidate their 3D structure and signaling mechanisms, and to reveal experimentally-accessible candidate loci to explore the genetic basis of adaptation.

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Snow cover is an important control in mountain environments and a shift of the snow-free period triggered by climate warming can strongly impact ecosystem dynamics. Changing snow patterns can have severe effects on alpine plant distribution and diversity. It thus becomes urgent to provide spatially explicit assessments of snow cover changes that can be incorporated into correlative or empirical species distribution models (SDMs). Here, we provide for the first time a with a lower overestimation comparison of two physically based snow distribution models (PREVAH and SnowModel) to produce snow cover maps (SCMs) at a fine spatial resolution in a mountain landscape in Austria. SCMs have been evaluated with SPOT-HRVIR images and predictions of snow water equivalent from the two models with ground measurements. Finally, SCMs of the two models have been compared under a climate warming scenario for the end of the century. The predictive performances of PREVAH and SnowModel were similar when validated with the SPOT images. However, the tendency to overestimate snow cover was slightly lower with SnowModel during the accumulation period, whereas it was lower with PREVAH during the melting period. The rate of true positives during the melting period was two times higher on average with SnowModel with a lower overestimation of snow water equivalent. Our results allow for recommending the use of SnowModel in SDMs because it better captures persisting snow patches at the end of the snow season, which is important when modelling the response of species to long-lasting snow cover and evaluating whether they might survive under climate change.

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Cette thèse analyse la co-évolution de deux secteurs dans la politique de la santé: santé publique (public health) et soins aux malades (health care). En d'autres termes, la relation entre les dimensions curative et préventive de la politique de la santé et leur développement dans la durée. Une telle recherche est nécessaire car les problèmes de la santé sont complexes et ont besoin de solutions coordonnées. De plus, les dépenses de la santé ont augmenté sans arrt durant les dernières décennies. Un moyen de réduire une future augmentation des dépenses pourrait consister en davantage d'investissement dans des mesures préventives. En relation avec cette idée, ma recherche analyse les politiques de la santé publique et les soins aux malades de cinq pays: Allemagne, Angleterre, Australie, Etats-Unis et Suisse. En m'appuyant sur la littérature secondaire, des statistiques descriptives et des entretiens avec des experts et des politiciens, j'analyse la relation entre les deux secteurs depuis la fin du dix-neuvième siècle. En particulier, je me focalise sur la relation des deux champs sur trois niveaux: institutions, acteurs et politiques. Mes résultats montrent les similitudes et les différences d'évolution entre les cinq pays. D'un c^oté, lorsque la profession médicale est politiquement active et que le pays consiste en une fédération centralisée ou en un gouvernement unitaire, les deux secteurs sont intégrés au niveau institutionnel, ralliant les professions et groupes d'intérêt des deux secteurs la cause commune dans une activité politique. Par contre, dans tous les pays, les deux secteurs ont co-évolué vers une complémentarité malgré de la politisation des professions et la centralisation du gouvernement. Ces résultats sont intéressants pour la science politique en général car ils soulignent l'importance des professions pour le développement institutionnel et proposent un cadre pour l'analyse de la co-évolution des politiques publiques en général. -- This Ph.D. thesis analyzes the co-evolution of the health care and the public health sectors. In other words, the relation between preventive and curative health policy and its evolution over time. Such research is necessary, because current health problems are complex and might need coordinated solutions. What is more, health expenditures have increased continuously in the last decades. One way to slow down further increase in health spending could be to invest more in preventative health policies. Therefore, I am connecting individual health care and public health into a common analysis, taking Australia, Germany, Switzerland, the UK and the U.S. as examples. Based on secondary literature, descriptive statistics and interviews with experts and policymakers, I am analyzing how the two sectors' relations co-evolved between the late nineteenth and the early twenty-first century. Specifically, I am researching how health care and public health were related on the levels of institutions, actors and policies. My results show that there are differences and similarities in the co-evolution of policy sectors between these countries. On the one hand, when the medical profession was politically active and the country a centralized federation or a unitary state, there was institutional integration and common political advocacy of the sectors' interest groups and professions. On the other hand, in all countries, both sectors co-evolved towards complementarity, irrespectively of the politicization of professions and centralization of government. These findings are interesting for the political science literature at large, because they underline the importance of professions for institutional development and propose an analytical framework for analyzing the co-evolution of policy sectors in general.

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Iberia underwent intraplate deformation during the Mesozoic and Cenozoic. In eastem Ibena, compression took place during the Palaeogene and early Miocene, giving rise to the Iberian Chain, and extension started during the early Miocene in the coastal areas and the Valencia trough; during early Miocene compression continued in the western Iberian Chain whereas extension had started in the eastern Iberian Chain. From the kinematic data obtained from the major compressional and extensional structures formed dunng the Cenozoic, a simple dynamic model using Bott's (1959) formula is presented. The results show that both extension and compression may have been produced assuming a main horizontal stress-axis approximately N-S, in a similar direction that the convergence between Europe, Ibena and Afnca dunng the Cenozoic.

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The Ivrea and the Strona-Ceneri zones, NW italy and S Switzerland, offer the possibility to study the continental crust of the Southern Alps. Because of its high metamorphic degree and the abundant Permo- Carboniferous mafic intrusions, the Ivrea Zone is classically interpreted an exposed section trough the Permian lower crust. The present work is focused here on metasedimentary slices (septa) intercalated within Permian gabbro (mafic complex). In particular I studied the evolution of accessory phases such as rutile and zircon and the chemistry of the metasediments. The septa build an irregular and discontinuous band that cut obliquely the mafic complex from its deepest part (N) to its roof (S). The chemistry of the metasediments evolves along the band and the chemical evolution can be compared with that observed in the country-rock surrounding the mafic intrusion to the NE and overprinted by a main regional metamorphic event. This suggests that the degree of chemical depletion of the septa was mainly established during the same regional metamorphic event. Moreover it suggests that incorporation of the septa within the gabbro did not modify their original stratigraphie distribution within the crust. It implies that the mafic complex has been emplaced following a dynamic substantially different from the classic model of « gabbro glacier » (Quick et al., 1992; Quick et al., 1994). It is more likely that it has been emplaced by repeated injections of sills at different depths during a protracted period of time. Zircon trace elements and U-Pb ages suggest that regional metamorphism occurred 330-320Ma, the first sills in the deepest part of the Mafic Complex are injected at ~300Ma, the mafic magmas reached higher levels in the crust at 285Ma and the magmatic activity continued locally until 275Ma. The ages of detrital cores in zircons fix the maximal sedimentation age at ~370Ma, this age corresponds therefore with the maximal age of the incorporation of the Ivrea zone within the lower crust. I propose that the Ivrea zone has been accreted to the lower crust during the Hercynian orogeny sensu lato. The analysis of detrital ages suggests that the source terrains for the Ivrea zone and those for the Strona-Ceneri zone have a completely different Palaeozoic history. The systematic analysis of rutile in partially molten metasediments of the Ivrea zone reveals the occurrence of two generations. The two generations are characterized by a different chemistry and textural distribution. A first generation is formed during pro-grade metamorphism in the restitic counterpart. The second generation is formed in the melts during cooling at the same time that part of the first generation re-equilibrate. Re-equilibration of the first generation seems to be spatially controlled by the presence of fluids. Locally the second generation forms overgrowths on the first generation. Considered the different diffusivity of U and Pb in rutile, U heterogeneities have important implication for U-Pb dating of rutile. ID-TIMS and LA-ICPMS dating coupled with a careful textural investigation (SEM) suggest that rutile grains are characterized by multiple path along which Pb diffusion can occur: volume diffusion is an important process, but intragrain and subgrain boundaries provide additional high diffusivity pathways for Pb escape and reduce drastically the effective diffusion length. -- La zone d'Ivrea et la zone de Strona-Ceneri, en Italie nord-occidentale et Suisse méridionale, offrent la possibilité d'étudier la croûte continentale des Alpes du Sud. En raison du haut degré métamorphique et l'abondance d'intrusions mafiques d'âge Permo-Carbonifère [complexe mafique), la zone d'Ivrea est interprétée classiquement comme de la croûte inférieure permienne. Ce travail ce concentre sur des bandes metasédimentaires (septa) incorporées dans les magmas mafiques lors de l'intrusion. Les septa forment une bande irrégulière qui coupe obliquement le complexe mafique du bas (N) vers le haut (S). La chimie des septa évolue du bas vers le haut et l'évolution chimique se rapproche de l'évolution observé dans la roche encaissante l'intrusion affecté par un événement métamorphique régionale. Cette relation suggère que le degré d'appauvrissement chimique des septa a été établit principalement lors de l'événement métamorphique régional. De plus l'incorporation dans les gabbros n'a pas perturbée la distribution stratigraphique originelle des septa. Ces deux observations impliquent que le métamorphisme dans la roche encaissante précède la mise en place du gabbro et que cette dernière ne se fait pas selon le modèle classique (« gabbro glacier » de Quick et al., 1992, 1994), mais se fait plutôt par injections répétées de sills a différentes profondeurs. Les âges U-Pb et les éléments traces des zircons suggèrent que le métamorphisme régionale a eu lieu 330-320Ma, alors que les premiers sills dans la partie profonde du Mafic Complex s'injectent à ~300Ma, le magmatisme mafique atteigne des niveaux supérieurs à 285Ma et continue localement jusqu'à 270Ma. Les âges des coeurs détritiques des zircons permettent de fixer l'âge maximale de sédimentation à ~370Ma ce qui correspond donc à l'âge maximale de l'incorporation de la zone d'Ivrea dans la croûte inférieur. L'analyse systématique des rutiles, nous a permit de montrer l'existence de plusieurs générations qui ont une répartition texturale et une chimie différente. Une génération se forme lors de l'événement UHT dans les restites, une autre génération se forme dans les liquides lors du refroidissement, au même temps qu'une partie de la première génération se rééquilibre au niveau du Zr. Localement la deuxième génération peut former des surcroissances autour de la première génération. Dans ces cas, des fortes différences en uranium entre les deux générations ont des importantes implications pour la datation U-Pb sur rutile. Classiquement les ratios Pb/U dans le rutile sont interprétés comme indiquant l'âges du refroidissement du minéral sous une température à la quelle la diffusion du Pb dans le minéral n'est plus détectable et la diffusion à plus hautes températures est assumée se faire par «volume diffusion» dans le grain (Mezger et al., 1989). Par des datations ID-TIMS (sur grain entier) et LA-ICPMS (in-situ) et une analyse texturale (MEB) approfondie nous montrons que cette supposition est trop simpliste et que le rutile est repartie en sous-domaines. Chacun de ces domaines a ça propre longueur ou chemin de diffusion spécifique. Nous proposons donc une nouvelle approche plus cohérente pour l'interprétation des âges U-Pb sur rutile.

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Crassulacean acid metabolism (CAM) photosynthesis is an adaptation to water and atmospheric CO2 deficits that has been linked to diversification in dry-adapted plants. We investigated whether CAM evolution can be associated with the availability of new or alternative niches, using Eulophiinae orchids as a case study. Carbon isotope ratios, geographical and climate data, fossil records and DNA sequences were used to: assess the prevalence of CAM in Eulophiinae orchids; characterize the ecological niche of extant taxa; infer divergence times; and estimate whether CAM is associated with niche shifts. CAM evolved in four terrestrial lineages during the late Miocene/Pliocene, which have uneven diversification patterns. These lineages originated in humid habitats and colonized dry/seasonally dry environments in Africa and Madagascar. Additional key features (variegation, heterophylly) evolved in the most species-rich CAM lineages. Dry habitats were also colonized by a lineage that includes putative mycoheterotrophic taxa. These findings indicate that the switch to CAM is associated with environmental change. With its suite of adaptive traits, this group of orchids represents a unique opportunity to study the adaptations to dry environments, especially in the face of projected global aridification.

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The mutualistic versus antagonistic nature of an interaction is defined by costs and benefits of each partner, which may vary depending on the environment. Contrasting with this dynamic view, several pollination interactions are considered as strictly obligate and mutualistic. Here, we focus on the interaction between Trollius europaeus and Chiastocheta flies, considered as a specialized and obligate nursery pollination system - the flies are thought to be exclusive pollinators of the plant and their larvae develop only in T.europaeus fruits. In this system, features such as the globelike flower shape are claimed to have evolved in a coevolutionary context. We examine the specificity of this pollination system and measure traits related to offspring fitness in isolated T.europaeus populations, in some of which Chiastocheta flies have gone extinct. We hypothesize that if this interaction is specific and obligate, the plant should experience dramatic drop in its relative fitness in the absence of Chiastocheta. Contrasting with this hypothesis, T.europaeus populations without flies demonstrate a similar relative fitness to those with the flies present, contradicting the putative obligatory nature of this pollination system. It also agrees with our observation that many other insects also visit and carry pollen among T.europaeus flowers. We propose that the interaction could have evolved through maximization of by-product benefits of the Chiastocheta visits, through the male flower function, and selection on floral traits by the most effective pollinator. We argue this mechanism is also central in the evolution of other nursery pollination systems.

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BACKGROUND: Major factors influencing the phenotypic diversity of a lineage can be recognized by characterizing the extent and mode of trait evolution between related species. Here, we compared the evolutionary dynamics of traits associated with floral morphology and climatic preferences in a clade composed of the genera Codonanthopsis, Codonanthe and Nematanthus (Gesneriaceae). To test the mode and specific components that lead to phenotypic diversity in this group, we performed a Bayesian phylogenetic analysis of combined nuclear and plastid DNA sequences and modeled the evolution of quantitative traits related to flower shape and size and to climatic preferences. We propose an alternative approach to display graphically the complex dynamics of trait evolution along a phylogenetic tree using a wide range of evolutionary scenarios. RESULTS: Our results demonstrated heterogeneous trait evolution. Floral shapes displaced into separate regimes selected by the different pollinator types (hummingbirds versus insects), while floral size underwent a clade-specific evolution. Rates of evolution were higher for the clade that is hummingbird pollinated and experienced flower resupination, compared with species pollinated by bees, suggesting a relevant role of plant-pollinator interactions in lowland rainforest. The evolution of temperature preferences is best explained by a model with distinct selective regimes between the Brazilian Atlantic Forest and the other biomes, whereas differentiation along the precipitation axis was characterized by higher rates, compared with temperature, and no regime or clade-specific patterns. CONCLUSIONS: Our study shows different selective regimes and clade-specific patterns in the evolution of morphological and climatic components during the diversification of Neotropical species. Our new graphical visualization tool allows the representation of trait trajectories under parameter-rich models, thus contributing to a better understanding of complex evolutionary dynamics.