A scenario for torus T(2) destruction via a global bifurcation

We show a scenario of a two-frequeney torus breakdown, in which a global bifurcation occurs due to the collision of a quasi-periodic torus T(2) with saddle points, creating a heteroclinic saddle connection. We analyze the geometry of this torus-saddle collision by showing the local dynamics and the invariant manifolds (global dynamics) of the saddle points. Moreover, we present detailed evidences of a heteroclinic saddle-focus orbit responsible for the type-if intermittency induced by this global bifurcation. We also characterize this transition to chaos by measuring the Lyapunov exponents and the scaling laws. (C) 2007 Elsevier Ltd. All rights reserved.

A atividade do capital estrangeiro na Bovespa

Este trabalho discute a recente evolução e a crescente importância do investimento estrangeiro no mercado de capitais brasileiro, observando como a sua presença afeta e é influenciada pela dinâmica local. Como primeiro achado, destaca-se a reatividade desses agentes ao mercado quanto às vendas de ativos; ao investigar se esse comportamento concorreria para um ambiente mais volátil e, em um cenário mais adverso, a própria desestabilização dos preços, constatou-se que suas compras mitigariam o efeito, mas que suas vendas operariam o oposto, sendo que em condições normais de mercado a demanda excessiva dos estrangeiros pressionaria significativamente os preços. Determinou-se também a importância dos mercados externos, das taxas básicas de juros interna e externa, da taxa de câmbio local e da liquidez do mercado à vista como fatores de estímulo a novas compras desses atores, assim como do câmbio, investimento direto líquido, risco país e liquidez para explicar as vendas adicionais. Por fim, surgiram como determinantes à entrada líquida de recursos estrangeiros na Bovespa o desempenho promissor dos mercados externos desenvolvidos e os juros locais em queda, sendo que o desenvolvimento bursátil local e um eventual cenário de crise seriam particularmente significativos na dinâmica de internalização de recursos no país.

Modelos dinâmicos de assembléia

The structure of an ecological community is shaped by several temporally varying mechanisms. Such mechanisms depend in a large extent on species interactions, which are themselves manifestations of the community's own structure. Dynamics and structure are then mutually determined. The assembly models are mathematical or computational models which simulate the dynamics of ecological communities resulting from a historical balance among colonizations and local extinctions, by means of sequential species introductions and their interactions with resident species. They allow analyzing that double relationship between structure and dynamics, recognizing its temporal dependence. It is assumed two spatiotemporal scales: (i) a local scale, where species co-occur and have their dynamics explicitly simulated and (ii) a regional scale without dynamics, representing the external environment which the potential colonizers come from. The mathematical and computational models used to simulate the local dynamics are quite variable, being distinguished according to the complexity mode of population representation, including or not intra or interspecific differences. They determine the community state, in terms of abundances, interactions, and extinctions between two successive colonization attempts. The schedules of species introductions also follow diverse (although arbitrary) rules, which vary qualitatively with respect to species appearance mode, whether by speciation or by immigration, and quantitatively with respect to their rates of introduction into the community. Combining these criteria arises a great range of approaches for assembly models, each with its own limitations and questions, but contributing in a complementary way to elucidate the mechanisms structuring natural communities. To present such approaches, still incipient as research fields in Brazil, to describe some methods of analysis and to discuss the implications of their assumptions for the understanding of ecological patterns are the objectives of the present review.

An analysis of the Hygiea asteroid family orbital region

(10) Hygiea is the fourth largest asteroid of the main belt, by volume and mass, and it is the largest member of its family, that is made mostly by low-albedo, C-type asteroids, typical of the outer main belt. Like many other large families, it is associated with a 'halo' of objects, that extends far beyond the boundary of the core family, as detected by traditional hierarchical clustering methods (HCM) in proper element domains. Numerical simulations of the orbital evolution of family members may help in estimating the family and halo family age, and the original ejection velocity field. But, in order to minimize the errors associated with including too many interlopers, it is important to have good estimates of family membership that include available data on local asteroid taxonomy, geometrical albedo and local dynamics. For this purpose, we obtained synthetic proper elements and frequencies of asteroids in the Hygiea orbital region, with their errors. We revised the current knowledge on asteroid taxonomy, including Sloan Digital Sky Survey-Moving Object Catalog 4th release (SDSS-MOC 4) data, and geometric albedo data from Wide-field Infrared Survey Explorer (WISE) and Near-Earth Object WISE (NEOWISE). We identified asteroid family members using HCM in the domain of proper elements (a, e, sin (i)) and in the domains of proper frequencies most appropriate to study diffusion in the local web of secular resonances, and eliminated possible interlopers based on taxonomic and geometrical albedo considerations. To identify the family halo, we devised a new hierarchical clustering method in an extended domain that includes proper elements, principal components PC1, PC2 obtained based on SDSS photometric data and, for the first time, WISE and NEOWISE geometric albedo. Data on asteroid size distribution, light curves and rotations were also revised for the Hygiea family. The Hygiea family is the largest group in its region, with two smaller families in proper element domain and 18 families in various frequencies domains identified in this work for the first time. Frequency groups tend to extend vertically in the (a, sin (i)) plane and cross not only the Hygiea family but also the near C-type families of Themis and Veritas, causing a mixture of objects all of relatively low albedo in the Hygiea family area. A few high-albedo asteroids, most likely associated with the Eos family, are also present in the region. Finally, the new multidomains hierarchical clustering method allowed us to obtain a good and robust estimate of the membership of the Hygiea family halo, quite separated from other asteroids families halo in the region, and with a very limited (about 3 per cent) presence of likely interlopers. © 2013 The Author Published by Oxford University Press on behalf of the Royal Astronomical Society.

Transformações na estrutura produtiva do aglomerado metropolitano de Curitiba

Pós-graduação em Geografia - IGCE

Modo de vida na várzea: políticas sociais e nova ruralidade: estudo em uma localidade da Reserva de Desenvolvimento Sustentável Mamirauá

Esta dissertação é um estudo sobre as ações em torno do desenvolvimento sustentável e de políticas não agrícolas para as pequenas populações rurais, a partir dos anos 80 e 90. Com a interiorização das políticas, o Estado se torna mais presente nas regiões interioranas redimensionando o mundo rural e suas dinâmicas locais. Neste sentido, um novo rural emerge com as ações políticas que chegam às populações mais distantes expondo o modo de vida a novas situações. Este estudo objetivou analisar as mudanças na organização social e econômica dos moradores da localidade rural de Vila Alencar da Reserva de Desenvolvimento Sustentável Mamirauá (RDSM), no estado do Amazonas, decorrentes da criação de uma reserva de desenvolvimento sustentável (RDS) e das ações institucionalizadas por políticas de Estado. A análise teórica foi fundamentada na noção de habitus e do campo socioambiental da Reserva Mamirauá. Realizaram-se também análises entre as famílias a partir do tempo de união conjugal, com a finalidade de identificar as mudanças ocorridas entre duas gerações familiares. Constatou-se neste estudo que a organização familiar em Vila Alencar se desenvolve levando em consideração as práticas locais e também participam das ações intervencionistas através das políticas sociais por meio do Programa Bolsa Família, das aposentadorias rurais e das atividades em torno do manejo sustentável dos recursos naturais, que estão em sua maioria associadas ao manejo de ecoturismo, a exemplo, da prestação de serviços como guia turístico, auxiliar de cozinha, copeira e carpintaria para a pousada de ecoturismo da RDSM. A combinação de atividades agrícolas, nãoagrícolas e a complementação de renda por benefícios sociais assumem papel importante na composição da renda familiar, o que traz novas perspectivas à reprodução social. O estudo mostrou que as políticas de desenvolvimento sustentável bem como as políticas de benefícios sociais tornam favorável à organização familiar das localidades rurais as características de feições modernizadoras e atrativas do conforto urbano, sobretudo pela expectativa da compra de uma casa na cidade e de melhores condições de qualificação aos filhos para prosperarem em alguma profissão. Aos jovens são delegadas outras responsabilidades que não se inserem exclusivamente no contexto produtivo do trabalho familiar.

Ambientes de confluência no contexto da rede de drenagem: exemplo da bacia hidrográfica do rio Ivaí - estado do Paraná

Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)

Ambientes de confluência no contexto da rede de drenagem: exemplo da bacia hidrográfica do rio Ivaí - estado do Paraná

Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)

Solvatationsdynamik: lokales Relaxationsverhalten glasbildender Systeme

In dieser Arbeit wurde das lokale Relaxationsverhalten niedermolekularer glasbildender Materialien mit der Methode der Solvatationsdynamik untersucht. Bei dieser Methode werden phosphoreszente Farbstoffe als molekulare Sonden für die lokale Dynamik im Glasbildner eingesetzt. Je nach verwendeter Sonde sind unterschiedliche Eigenschaften zugänglich:Mit Farbstoffen, die ihr Dipolmoment bei optischer Anregung nicht ändern, wird eine mechanische Solvatation gemessen, die die lokale viskoelastische Antwort des Materials widerspiegelt. Mit Farbstoffen, die eine Änderung des Dipolmoments bei optischer Anregung aufweisen,sind zusätzlich lokale dielektrische Eigenschaften des Materials zugänglich, die bei endlicher Polarität des Lösungsmittels dominieren. Das heterogene Relaxationsverhalten des Glasbildners 2-Methyltetrahydrofuran wurde quantitativ untersucht.Auf einem Temperaturbereich, auf dem die mittlere Relaxationszeit um mehr als 4 Dekaden variiert, konnte gezeigt werden, daß die Relaxation lokal rein exponentiell verläuft. Zur Abschätzung von Reichweiteneffekten wurden Solvatationsmessungen in einschränkenden Geometrien in Form von porösen Sol-Gel Gläsern mit Porendurchmessern zwischen 7,5-2,5 nm durchgeführt. Der Einfluß der Beschaffenheit der Porenoberfläche wurde durch Vergleichzwischen der Solvatation in nativen und in silanisierten Gläsern untersucht. Es wurde gezeigt, daß auch in den kleinsten verwendeten silanisierten Poren alle Charakteristika des jeweiligen Bulk-Systems erhalten bleiben.In den nativen porösen Gläsern dagegen führt der Einfluß der stark polaren Oberfläche zu einer Änderung der Dynamik.

Genetic structure and connectivity between populations of two common Mediterranean sessile invertebrates

Population genetic and phylogeography of two common mediterranean species were studied in 10 localities located on the coasts of Toscana, Puglia and Calabria. The aim of the study was to verify the extent of genetic breaks, in areas recognized as boundaries between Mediterranean biogeographic sectors. From about 100 sequences obtained from the mitochondrial Cytochrome Oxidase subunit I (COI) gene of Halocynthia papillosa and Hexaplex trunculus genetic diversity, genetic structure at small and large distances and demographic history of both specieswere analyzed. No evidences of genetic breaks were found for the two species in Toscana and Puglia. The genetic structure of H. trunculus evidences the extent of a barrier to gene flow localized in Calabria, which could be represented by the Siculo-Tunisian Strait and the Strait of Messina. The observed patterns showed similar level of gene flow at small distances in both species, although the two species have different larval ecology. These results suggest that other factors, such as currents, local dynamics and seasonal temperatures, influence the connectivity along the Italian peninsula. The geographic distribution of the haplotypes shows that H. papillosacould represent a single genetic pool in expansion, whereas H. trunculus has two distinct genetic pools in expansion. The demographic pattern of the two species suggests that Pleistocene sea level oscillations, in particular of the LGM, may have played a key role in shaping genetic structure of the two species. This knowledge provides basic information, useful for the definition of management plans, or for the design of a network of marine protected areas along the Italian peninsula.

Aerosol-cloud interactions studied with a chemistry-climate model

This study aims at a comprehensive understanding of the effects of aerosol-cloud interactions and their effects on cloud properties and climate using the chemistry-climate model EMAC. In this study, CCN activation is regarded as the dominant driver in aerosol-cloud feedback loops in warm clouds. The CCN activation is calculated prognostically using two different cloud droplet nucleation parameterizations, the STN and HYB CDN schemes. Both CDN schemes account for size and chemistry effects on the droplet formation based on the same aerosol properties. The calculation of the solute effect (hygroscopicity) is the main difference between the CDN schemes. The kappa-method is for the first time incorporated into Abdul-Razzak and Ghan activation scheme (ARG) to calculate hygroscopicity and critical supersaturation of aerosols (HYB), and the performance of the modied scheme is compared with the osmotic coefficient model (STN), which is the standard in the ARG scheme. Reference simulations (REF) with the prescribed cloud droplet number concentration have also been carried out in order to understand the effects of aerosol-cloud feedbacks. In addition, since the calculated cloud coverage is an important determinant of cloud radiative effects and is influencing the nucleation process two cloud cover parameterizations (i.e., a relative humidity threshold; RH-CLC and a statistical cloud cover scheme; ST-CLC) have been examined together with the CDN schemes, and their effects on the simulated cloud properties and relevant climate parameters have been investigated. The distinct cloud droplet spectra show strong sensitivity to aerosol composition effects on cloud droplet formation in all particle sizes, especially for the Aitken mode. As Aitken particles are the major component of the total aerosol number concentration and CCN, and are most sensitive to aerosol chemical composition effect (solute effect) on droplet formation, the activation of Aitken particles strongly contribute to total cloud droplet formation and thereby providing different cloud droplet spectra. These different spectra influence cloud structure, cloud properties, and climate, and show regionally varying sensitivity to meteorological and geographical condition as well as the spatiotemporal aerosol properties (i.e., particle size, number, and composition). The changes responding to different CDN schemes are more pronounced at lower altitudes than higher altitudes. Among regions, the subarctic regions show the strongest changes, as the lower surface temperature amplifies the effects of the activated aerosols; in contrast, the Sahara desert, where is an extremely dry area, is less influenced by changes in CCN number concentration. The aerosol-cloud coupling effects have been examined by comparing the prognostic CDN simulations (STN, HYB) with the reference simulation (REF). Most pronounced effects are found in the cloud droplet number concentration, cloud water distribution, and cloud radiative effect. The aerosol-cloud coupling generally increases cloud droplet number concentration; this decreases the efficiency of the formation of weak stratiform precipitation, and increases the cloud water loading. These large-scale changes lead to larger cloud cover and longer cloud lifetime, and contribute to high optical thickness and strong cloud cooling effects. This cools the Earth's surface, increases atmospheric stability, and reduces convective activity. These changes corresponding to aerosol-cloud feedbacks are also differently simulated depending on the cloud cover scheme. The ST-CLC scheme is more sensitive to aerosol-cloud coupling, since this scheme uses a tighter linkage of local dynamics and cloud water distributions in cloud formation process than the RH-CLC scheme. For the calculated total cloud cover, the RH-CLC scheme simulates relatively similar pattern to observations than the ST-CLC scheme does, but the overall properties (e.g., total cloud cover, cloud water content) in the RH simulations are overestimated, particularly over ocean. This is mainly originated from the difference in simulated skewness in each scheme: the RH simulations calculate negatively skewed distributions of cloud cover and relevant cloud water, which is similar to that of the observations, while the ST simulations yield positively skewed distributions resulting in lower mean values than the RH-CLC scheme does. The underestimation of total cloud cover over ocean, particularly over the intertropical convergence zone (ITCZ) relates to systematic defficiency of the prognostic calculation of skewness in the current set-ups of the ST-CLC scheme.rnOverall, the current EMAC model set-ups perform better over continents for all combinations of the cloud droplet nucleation and cloud cover schemes. To consider aerosol-cloud feedbacks, the HYB scheme is a better method for predicting cloud and climate parameters for both cloud cover schemes than the STN scheme. The RH-CLC scheme offers a better simulation of total cloud cover and the relevant parameters with the HYB scheme and single-moment microphysics (REF) than the ST-CLC does, but is not very sensitive to aerosol-cloud interactions.