Nous enfocaments per a la didàctica de la literatura grega: observacions sobre experiències en el treball col•laboratiu i semipresencial

Arran de les experiències tant a la Universitat Oberta de Catalunya com a la Universitat de València, els autors comenten els aspectes més innovadors per a un nou enfocament en la docència de la Literatura grega. Aquest nou enfocament combina una nova programació de continguts amb nous plantejament dels procediments didàctics. Pel que fa als continguts, s'ha fet una adaptació que respon als interessos que la matèria desvetlla en el món contemporani. Quant als procediments didàctics comptem sobretot amb el treball col•laboratiu amb alumnat de diversa procedència -i amb interessos també diversos- juntament amb noves estratègies a partir de l'ús de les eines virtuals

Actividade física, desporto e lazer na adolescência

RESUMO: Os estilos de vida pessoais evoluíram notavelmente com o passar dos anos como consequência das mudanças verificadas nas sociedades modernas. As condições da vida urbana, os horários das actividades escolares, a televisão, os videojogos e a Internet estão a potenciar um maior sedentarismo dos adolescentes (Redondo, Gross, Moreno & García-Fuentes, 2010), que usam cada vez menos as suas potencialidades físicas, embora se saiba que os indivíduos que praticam regularmente uma actividade física percepcionam ter um estado de saúde mais positivo (Mota & Duarte, 1999). Nesta perspectiva, o interesse em conceitos como actividade física, estilo de vida, qualidade de vida, promoção da saúde, têm vindo a adquirir uma relevância crescente para a determinação das variáveis que contribuem para a melhoria do bem-estar dos indivíduos, por meio do incremento do nível de actividade física habitual. Porque sabemos que a promoção da actividade física na infância e na adolescência significa o estabelecimento de uma base sólida para a redução do sedentarismo na idade adulta, contribuindo desta forma para uma melhor qualidade de vida (Lazzoli et al.,1998), e porque são reconhecidos os efeitos benéficos da actividade física na saúde, (bem-estar físico, social e psicológico) (Diniz,1998), pretende-se, com o presente trabalho, analisar os estilos de vida dos adolescentes dos 8º e 9º anos de escolaridade do Agrupamento de Escolas Sophia de Mello Breyner Andresen ao nível da actividade física, prática desportiva e ocupação de tempos livres, relacionando-os com os padrões sustentados nos estudos da HBSC/OMS (Health Behaviour in School-aged Children/Organização Mundial de Saúde), ou mais concretamente com os dados do Relatório preliminar do estudo HBSC 2006 - “A Saúde dos Adolescentes Portugueses - Hoje e em 8 Anos”, levado a cabo pela ASS (Aventura Social e Saúde).

Le musee local de la nouvelle generation au Portugal, un pas en avant dans la gestion communautaire qualitative : essai d'interprétation épistémologique

Le musée local, au Portugal, tel qu’il apparaît dans la perspective de la révolution socio-cultureile de 74, puis projeté à l’avant-scène de la muséologie portugaise renaissante, lors du IIe Atelier international de Nouvelle muséologie (Lisbonne/Seixal/Monte Redondo — Musées locaux/Nouvelle musólogie, novembre 85), se perpétue jusqu’à nos jours, tout au moins dans le discours de ses promoteurs, préoccupé par le rapport aux pouvoirs et aux populations. Fortement enraciné dans la structure municipale et associative, utilisé à ses débuts, à des degrés divers, comme un outil de militance communautaire, le musée local présente un modèle muséographique de type ethnographique diffusé à travers le pays. Celui-ci est fondé sur la participation de donateurs d’objets utiles de la vie courante, mis à contribution dans le programme, de même que sur l’apport des savoir-faire populaires et artisanaux, évitant de tomber dans le folklorisme par une réflexion alimentée par les universitaires. Ce mouvement naissant correspond à la mode de l’écomusée dont il épouse certains contours, tout en demeurant enraciné dans la tradition ethnographique du pays.

Kipus: revista andina de letras. 15 (Reseñas)

Presenta las reseñas de los siguientes libros: Susana Zanetti, LA DORADA GARRA DE LA LECTURA. LECTORAS y LECTORES DE NOVELA EN AMÉRICA LATINA, Rosario: Beatriz Viterbo, 2002, 448 pp. -- Orlando Pérez, LA CELEBRACiÓN DE LA LIBERTAD, Quito: Libresa, Colección Crónica de sueños, 2002. -- Martha Rodríguez, PERO ES DESPUÉS, BAJO EL SOL, Quito: Libresa, Colección Crónica de sueños, 2002, 95 pp. -- Tomás Eloy Martínez, EL VUELO DE LA REINA, Madrid: Alfaguara, 2002, 295 pp. -- Gabriela Alemán, FUGA PERMANENTE, Quito: Eskeletra, 2a. ed., 2002, 113 pp. -- Alfonso Monsalve, CUENTOS DE PELÍCULA, Quito: Eskeletra, 2002, 182 pp. -- Galo Mora W. UN PÁJARO REDONDO PARA JUGAR, Quito: Eskeletra, 2002,289 pp. -- Sonia Navarro, SABOR A OLVIDO (BIOGRAFÍA DE LA SRA. RENÉ), Guayaquil: Centro de Difusión y Publicaciones Espol, 165 pp. -- Margarito Cuéllar, LOS RIESGOS DEL PLACER, Carolina Andrade Monterrey, Nuevo León: Ediciones Castillo S. A.de C. V., 2002, 78 pp.

Patterns of diversification in two species of short-tailed bats (Carollia Gray, 1838): the effects of historical fragmentation of Brazilian rainforests

The small-sized frugivorous bat Carollia perspicillata is an understory specialist and occurs in a wide range of lowland habitats, tending to be more common in tropical dry or moist forests of South and Central America. Its sister species, Carollia brevicauda, occurs almost exclusively in the Amazon rainforest. A recent phylogeographic study proposed a hypothesis of origin and subsequent diversification for C. perspicillata along the Atlantic coastal forest of Brazil. Additionally, it also found two allopatric clades for C. brevicauda separated by the Amazon Basin. We used cytochrome b gene sequences and a more extensive sampling to test hypotheses related to the origin and diversification of C. perspicillata plus C. brevicauda clade in South America. The results obtained indicate that there are two sympatric evolutionary lineages within each species. In C. perspicillata, one lineage is limited to the Southern Atlantic Forest, whereas the other is widely distributed. Coalescent analysis points to a simultaneous origin for C. perspicillata and C. brevicauda, although no place for the diversification of each species can be firmly suggested. The phylogeographic pattern shown by C. perspicillata is also congruent with the Pleistocene refugia hypothesis as a likely vicariant phenomenon shaping the present distribution of its intraspecific lineages. (C) 2011 The Linnean Society of London, Biological Journal of the Linnean Society, 2011, 102, 527-539.

Upper limit on the cosmic-ray photon flux above 10(19) eV using the surface detector of the Pierre Auger Observatory

A method is developed to search for air showers initiated by photons using data recorded by the surface detector of the Auger Observatory. The approach is based on observables sensitive to the longitudinal shower development, the signal risetime and the curvature of the shower front. Applying this method to the data, tipper limits on the flux of photons of 3.8 x 10(-3), 2.5 x 10(-3), and 2.2 x 10(-3) km(-2) sr(-1) yr(-1) above 10(19) eV, 2 x 10(19) eV, and 4 x 10(19) eV are derived, with corresponding limits on the fraction of photons being 2.0%, 5.1%, and 31% (all limits at 95% c.l.). These photon limits disfavor certain exotic models of sources of cosmic rays. The results also show that the approach adopted by the Auger Observatory to calibrate the shower energy is not strongly biased by a contamination from photons. (C) 2008 Elsevier B.V. All rights reserved.

Correlation of the highest-energy cosmic rays with the positions of nearby active galactic nuclei

Data collected by the Pierre Auger Observatory provide evidence for anisotropy in the arrival directions of the cosmic rays with the highest-energies, which are correlated with the positions of relatively nearby active galactic nuclei (AGN) [Pierre Auger Collaboration, Science 318 (2007) 938]. The correlation has maximum significance for cosmic rays with energy greater than similar to 6 x 10(19) eV and AGN at a distance less than similar to 75 Mpc. We have confirmed the anisotropy at a confidence level of more than 99% through a test with parameters specified a priori, using an independent data set. The observed correlation is compatible with the hypothesis that cosmic rays with the highest-energies originate from extra-galactic sources close enough so that their flux is not significantly attenuated by interaction with the cosmic background radiation (the Greisen-Zatsepin-Kuz`min effect). The angular scale of the correlation observed is a few degrees, which suggests a predominantly light composition unless the magnetic fields are very weak outside the thin disk of our galaxy. Our present data do not identify AGN as the sources of cosmic rays unambiguously, and other candidate sources which are distributed as nearby AGN are not ruled out. We discuss the prospect of unequivocal identification of individual sources of the highest-energy cosmic rays within a few years of continued operation of the Pierre Auger Observatory. (C) 2008 Elsevier B.V. All rights reserved.

Trigger and aperture of the surface detector array of the Pierre Auger Observatory

The surface detector array of the Pierre Auger Observatory consists of 1600 water-Cherenkov detectors, for the study of extensive air showers (EAS) generated by ultra-high-energy cosmic rays. We describe the trigger hierarchy, from the identification of candidate showers at the level of a single detector, amongst a large background (mainly random single cosmic ray muons), up to the selection of real events and the rejection of random coincidences. Such trigger makes the surface detector array fully efficient for the detection of EAS with energy above 3 x 10(18) eV, for all zenith angles between 0 degrees and 60 degrees, independently of the position of the impact point and of the mass of the primary particle. In these range of energies and angles, the exposure of the surface array can be determined purely on the basis of the geometrical acceptance. (C) 2009 Elsevier B.V. All rights reserved.

Atmospheric effects on extensive air showers observed with the surface detector of the Pierre Auger observatory

Atmospheric parameters, Such as pressure (P), temperature (T) and density (rho proportional to P/T), affect the development of extensive air showers initiated by energetic cosmic rays. We have Studied the impact of atmospheric variations on extensive air showers by means of the surface detector of the Pierre Auger Observatory. The rate of events shows a similar to 10% seasonal modulation and similar to 2% diurnal one. We find that the observed behaviour is explained by a model including the effects associated with the variations of P and rho. The former affects the longitudinal development of air showers while the latter influences the Moliere radius and hence the lateral distribution of the shower particles. The model is validated with full simulations of extensive air showers using atmospheric profiles measured at the site of the Pierre Auger Observatory. (C) 2009 Elsevier B.V. All rights reserved.

Upper limit on the cosmic-ray photon fraction at EeV energies from the Pierre Auger Observatory

From direct observations of the longitudinal development of ultra-high energy air showers performed with the Pierre Auger Observatory, upper limits of 3.8%, 2.4%, 3.5% and 11.7% (at 95% c.l.) are obtained on the fraction of cosmic-ray photons above 2, 3, 5 and 10 EeV (1 EeV equivalent to 10(18) eV), respectively. These are the first experimental limits on ultra-high energy photons at energies below 10 EeV. The results complement previous constraints on top-down models from array data and they reduce systematic uncertainties in the interpretation of shower data in terms of primary flux, nuclear composition and proton-air cross-section. (C) 2009 Elsevier B.V. All rights reserved.

The fluorescence detector of the Pierre Auger Observatory

The Pierre Auger Observatory is a hybrid detector for ultra-high energy cosmic rays. It combines a surface array to measure secondary particles at ground level together with a fluorescence detector to measure the development of air showers in the atmosphere above the array. The fluorescence detector comprises 24 large telescopes specialized for measuring the nitrogen fluorescence caused by charged particles of cosmic ray air showers. In this paper we describe the components of the fluorescence detector including its optical system, the design of the camera, the electronics, and the systems for relative and absolute calibration. We also discuss the operation and the monitoring of the detector. Finally, we evaluate the detector performance and precision of shower reconstructions. (C) 2010 Elsevier B.V All rights reserved.

Measurement of the energy spectrum of cosmic rays above 10(18) eV using the Pierre Auger Observatory

We report a measurement of the flux of cosmic rays with unprecedented precision and Statistics using the Pierre Auger Observatory Based on fluorescence observations in coincidence with at least one Surface detector we derive a spectrum for energies above 10(18) eV We also update the previously published energy spectrum obtained with the surface detector array The two spectra are combined addressing the systematic uncertainties and, in particular. the influence of the energy resolution on the spectral shape The spectrum can be described by a broken power law E(-gamma) with index gamma = 3 3 below the ankle which is measured at log(10)(E(ankle)/eV) = 18 6 Above the ankle the spectrum is described by a power law with index 2 6 followed by a flux suppression, above about log(10)(E/eV) = 19 5, detected with high statistical significance (C) 2010 Elsevier B V All rights reserved

A study of the effect of molecular and aerosol conditions in the atmosphere on air fluorescence measurements at the Pierre Auger Observatory

The air fluorescence detector of the Pierre Auger Observatory is designed to perforin calorimetric measurements of extensive air showers created by Cosmic rays of above 10(18) eV. To correct these measurements for the effects introduced by atmospheric fluctuations, the Observatory contains a group Of monitoring instruments to record atmospheric conditions across the detector site, ail area exceeding 3000 km(2). The atmospheric data are used extensively in the reconstruction of air showers, and are particularly important for the correct determination of shower energies and the depths of shower maxima. This paper contains a summary of the molecular and aerosol conditions measured at the Pierre Auger Observatory since the start of regular operations in 2004, and includes a discussion of the impact of these measurements oil air shower reconstructions. Between 10(18) and 10(20) eV, the systematic Uncertainties due to all atmospheric effects increase from 4% to 8% in measurements of shower energy, and 4 g cm(-2) to 8 g cm(-2) in measurements of the shower maximum. (C) 2010 Elsevier B.V. All rights reserved.

The Cariris Velhos tectonic event in Northeast Brazil

The Borborema Province in northeastern South America is a typical Brasiliano-Pan-African branching system of Neoproterozoic orogens that forms part of the Western Gondwana assembly. The province is positioned between the Sao Luis-West Africa craton to the north and the Sao Francisco (Congo-Kasai) craton to the south. For this province the main characteristics are (a) its subdivision into five major tectonic domains, bounded mostly by long shear zones, as follows: Medio Coreau, Ceara Central, Rio Grande do Norte, Transversal, and Southern; (b) the alternation of supracrustal belts with reworked basement inliers (Archean nuclei + Paleoproterozoic belts); and (c) the diversity of granitic plutonism, from Neoproterozoic to Early Cambrian ages, that affect supracrustal rocks as well as basement inliers. Recently, orogenic rock assemblages of early Tonian (1000-920 Ma) orogenic evolution have been recognized, which are restricted to the Transversal and Southern domains of the Province. Within the Transversal Zone, the Alto Pajeu terrane locally includes some remnants of oceanic crust along with island arc and continental arc rock assemblages, but the dominant supracrustal rocks are mature and immature pelitic metasedimentary and metavolcaniclastic rocks. Contiguous and parallel to the Alto Pajeu terrane, the Riacho Gravata subterrane consists mainly of low-grade metamorphic successions of metarhythmites, some of which are clearly turbiditic in origin, metaconglomerates, and sporadic marbles, along with interbedded metarhyolitic and metadacitic volcanic or metavolcaniclastic rocks. Both terrane and subterrane are cut by syn-contractional intrusive sheets of dominantly peraluminous high-K calc-alkaline, granititic to granodioritic metaplutonic rocks. The geochemical patterns of both supracrustal and intrusive rocks show similarities with associations of mature continental arc volcano-sedimentary sequences, but some subordinate intra-plate characteristics are also found. In both the Alto Pajeu and Riacho Gravata terranes, TIMS and SHRIMP U-Pb isotopic data from zircons from both metavolcanic and metaplutonic rocks yield ages between 1.0 and 0.92 Ga, which define the time span for an event of orogenic character, the Cariris Velhos event. Less extensive occurrences of rocks of Cariris Velhos age are recognized mainly in the southernmost domains of the Province, as for example in the Polo Redondo-Maranco terrane, where arc-affinity migmatite-granitic and meta-volcano-sedimentary rocks show U-Pb ages (SHRIMP data) around 0.98-0.97 Ga. For all these domains, Sm-Nd data exhibit Tom model ages between 1.9 and 1.1 Ga with corresponding slightly negative to slightly positive epsilon(Nd)(t) values. These domains, along with the Borborema Province as a whole, were significantly affected by tectonic and magmatic events of the Brasiliano Cycle (0.7-0.5 Ga), so that it is possible that there are some other early Tonian rock assemblages which were completely masked and hidden by these later Brasiliano events. Cariris Velhos processes are younger than the majority of orogenic systems at the end of Mesoproterozoic Era and beginning of Neoproterozoic throughout the world, e.g. Irumide belt, Kibaride belt and Namaqua-Natal belt, and considerably younger than those of the youngest orogenic process (Ottawan) in the Grenvillian System. Therefore, they were probably not associated with the proposed assembly of Rodinia. We suggest, instead, that Cariris Velhos magmatism and tectonism could have been related to a continental margin magmatic arc, with possible back-arc associations, and that this margin may have been a short-lived (<100 m.y.) leading edge of the newly assembled Rodinia supercontinent. (C) 2009 Elsevier Ltd. All rights reserved.