937 resultados para Organ masses.


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En aquesta part del tema, intentarem donar resposta a les qüestions següents: - Quins són els principals impactes ambientals que pot generar l’activitat turística? - Quines diferències podem establir considerant les diverses modalitats turístiques i l’escala d’estudi, segons el punt de vista local o global? - Quines mesures poden prendre’s des de la gestió i planificació turística per a minimitzar i evitar impactes? - Què és el turisme sostenible?

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Within the European water framework directive (WFD), the status assessment of littoral waters is based both on the chemical quality and on the ecological quality of each water body. Quality elements enabling to assess the ecological status of a water body are, among other things, biological quality elements (phytoplankton, macroalgae, angiosperms, benthic invertebrates, fish), for each of which the member states have developed quantitative indicators. This document is one of the deliverables of a multi-annual study intended to characterize the sensitivity of these biological indicators towards the various anthropogenic pressures exerted on the French Atlantic and Channel coast: ultimately, the goal is to establish a quantitative and predictive relationship, statistically robust, between the WFD indicators used along the French channel and Atlantic coastline, and various anthropogenic pressures acting on these coasts. The aim of the WFD is indeed to restore or maintain a good chemical and biological quality of coastal waters, and thus to limit the impact of human activities potentially responsible for the degradation of ecosystems. This understanding of the linkages and interactions existing between anthropogenic pressures and ecological status of water bodies is therefore essential to identify priorities for action (challenges, substances ...), prioritize actions to implement within restoration programs (technical, fiscal, financial), but also to be able to communicate constructively and persuasively in talks between managers and the various stakeholders of coastal regions. Using the DPSIR methodology, this literature analysis has permitted to identify, for each WFD biological quality element (except fish), which pressures (or pressure types) are potentially relevant in the light of their impact on the indicators of the ecological status of water bodies. Some metrics and indicators of anthropogenic pressures used in the literature to characterize the sensitivity of the biological quality elements, within quantitative approaches, were also identified. It is also clear from this review that the biological quality elements can be particularly sensitive to intrinsic environmental conditions, and therefore to certain changes related to natural phenomena occurring at large scales (e.g. climate change, paroxysmal climate episode...). Therefore, when one is interested in the sensitivity of biological indicators to different anthropogenic pressures, two factors can complicate the analysis and are likely to weaken the resulting statistical relationships: on the one hand, the variability of biological responses depending on the natural context and, on the other hand, interactions (so called synergistic effects) between different types of anthropogenic pressures and the alterations they can generate.

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Within the European water framework directive (WFD), the status assessment of littoral waters is based both on the chemical quality and on the ecological quality of each water body. Quality elements enabling to assess the ecological status of a water body are, among other things, biological quality elements (phytoplankton, macroalgae, angiosperms, benthic invertebrates, fish), for each of which member states have developed quantitative indicators. This document compiles three deliverables of a multi-annual study intended to characterize the sensitivity of these biological indicators regarding the various anthropogenic pressures exerted on the French Atlantic and Channel coast: ultimately, the goal is to establish a quantitative and predictive relationship, statistically robust, between the WFD indicators used along the French channel and Atlantic coastline, and various anthropogenic pressures acting on these coasts. These three deliverables are the following : - The reports of various interviews performed with French national referents for the biological quality elements used within the littoral part of the WFD in Channel and Atlantic (phytoplankton, subtidal and intertidal macroalgae, opportunistic blooming macroalgae, angiosperms and benthic invertebrates). These interviews aimed to specify, for each metric constitutive of the BQE indicator (if multi-metric), the "relevant" pressures, as well as the trend of this impact, - Sheets describing the "pressure" and "environment" data available, in order to characterize spatially and quantitatively these "relevant" anthropogenic pressures acting on French Channel and Atlantic coast, - A progress report dealing with the development of a database tool, for archiving quantitative data characterizing "relevant" littoral anthropogenic pressures.

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In the context of ƒ (R) gravity theories, we show that the apparent mass of a neutron star as seen from an observer at infinity is numerically calculable but requires careful matching, first at the star’s edge, between interior and exterior solutions, none of them being totally Schwarzschild-like but presenting instead small oscillations of the curvature scalar R; and second at large radii, where the Newtonian potential is used to identify the mass of the neutron star. We find that for the same equation of state, this mass definition is always larger than its general relativistic counterpart. We exemplify this with quadratic R^2 and Hu-Sawicki-like modifications of the standard General Relativity action. Therefore, the finding of two-solar mass neutron stars basically imposes no constraint on stable ƒ (R) theories. However, star radii are in general smaller than in General Relativity, which can give an observational handle on such classes of models at the astrophysical level. Both larger masses and smaller matter radii are due to much of the apparent effective energy residing in the outer metric for scalar-tensor theories. Finally, because the ƒ (R) neutron star masses can be much larger than General Relativity counterparts, the total energy available for radiating gravitational waves could be of order several solar masses, and thus a merger of these stars constitutes an interesting wave source.

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La présence de disques circumstellaires signale la formation actuelle ou passée de systèmes planétaires, pour lesquels les processus de formation sont encore mal compris. Ce mémoire porte sur la détection et la caractérisation de disques circumstellaires autour d’étoiles de faibles masses (types spectraux > K5) et de naines brunes qui sont candidates ou membres d’associations cinématiques jeunes. Nous présentons ici les résultats de cette recherche ainsi que son implication pour la compréhension des processus de formation et d’évolution des systèmes planétaires. De l’échantillon initial composé de ∼ 1600 objets provenant des relevés BANYAN de Malo et al. ainsi que Gagné et al., dont seulement 600 satisfont nos critères de qualité sur les données, quatre nouveaux candidats de disque ont été découverts en détectant leur excès d’émission infrarouge dans les données d’archive de la mission WISE. Les données du relevé 2MASS ainsi que les spectres synthétiques BT-Settl ont été conjointement utilisés pour modéliser l’émission des étoiles. Les nouveaux candidats, dont les types spectraux sont tardifs (M4.5 à L0) et les masses se situent entre ∼ 13 et 120 M_Jup, ont des températures de disque de ∼ 135–520 K et des luminosités fractionnaires de 0,021–0,15. Pour deux des cibles, nous avons obtenu des spectres dans les longueurs d’onde visibles et infrarouges proches. Ces nouveaux spectres montrent respectivement des signes d’émission en Hα et Paβ, indiquant la présence d’accrétion, et ainsi de gaz, et renforçant l’hypothèse que ces objets sont réellement jeunes. Ces deux objets, vraisemblablement âgés de 40 Ma, pourraient représenter la première détection et caractérisation de disques porteurs de gaz plus vieux que 20 Ma.

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La présence de disques circumstellaires signale la formation actuelle ou passée de systèmes planétaires, pour lesquels les processus de formation sont encore mal compris. Ce mémoire porte sur la détection et la caractérisation de disques circumstellaires autour d’étoiles de faibles masses (types spectraux > K5) et de naines brunes qui sont candidates ou membres d’associations cinématiques jeunes. Nous présentons ici les résultats de cette recherche ainsi que son implication pour la compréhension des processus de formation et d’évolution des systèmes planétaires. De l’échantillon initial composé de ∼ 1600 objets provenant des relevés BANYAN de Malo et al. ainsi que Gagné et al., dont seulement 600 satisfont nos critères de qualité sur les données, quatre nouveaux candidats de disque ont été découverts en détectant leur excès d’émission infrarouge dans les données d’archive de la mission WISE. Les données du relevé 2MASS ainsi que les spectres synthétiques BT-Settl ont été conjointement utilisés pour modéliser l’émission des étoiles. Les nouveaux candidats, dont les types spectraux sont tardifs (M4.5 à L0) et les masses se situent entre ∼ 13 et 120 M_Jup, ont des températures de disque de ∼ 135–520 K et des luminosités fractionnaires de 0,021–0,15. Pour deux des cibles, nous avons obtenu des spectres dans les longueurs d’onde visibles et infrarouges proches. Ces nouveaux spectres montrent respectivement des signes d’émission en Hα et Paβ, indiquant la présence d’accrétion, et ainsi de gaz, et renforçant l’hypothèse que ces objets sont réellement jeunes. Ces deux objets, vraisemblablement âgés de 40 Ma, pourraient représenter la première détection et caractérisation de disques porteurs de gaz plus vieux que 20 Ma.

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Aims The objective of the 5th International Consultation on Incontinence (ICI) chapter on Adult Conservative Management was to review and summarize the new evidence on conservative management of urinary incontinence (UI) and pelvic organ prolapse (POP) in order to compile a current reference source for clinicians, health researchers, and service planners. In this paper, we present the review highlights and new evidence on female conservative management. Methods Revision and updates of the 4th ICI Report using systematic review covering years 2008–2012. Results Each section begins with a brief definition and description of the intervention followed by a summary, where possible, of both the state and level of evidence for prevention and treatment, and ends with a “grade of recommendation.” The paper concludes with areas identified as requiring further research. Conclusions For UI, there are no prevention trials on lifestyle interventions. There are, however, few new intervention trials of lifestyle interventions involving weight loss and fluid intake with improved levels of evidence and grade of recommendation. Outside of pre- and post-natal pelvic floor muscle training (PFMT) trials for the prevention of female UI, there is a dearth of PFMT prevention trials for women with UI. PFMT remains the first-line treatment for female UI with high levels of evidence and grades of recommendation. Bladder training levels of evidence and grades of recommendation are maintained. For POP, new evidence supports the effectiveness of physiotherapy in the treatment of POP and there are now improved levels of evidence and grades of recommendation.

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Aims The objective of the 5th International Consultation on Incontinence (ICI) chapter on Adult Conservative Management was to review and summarize the new evidence on conservative management of urinary incontinence (UI) and pelvic organ prolapse (POP) in order to compile a current reference source for clinicians, health researchers, and service planners. In this paper, we present the review highlights and new evidence on female conservative management. Methods Revision and updates of the 4th ICI Report using systematic review covering years 2008–2012. Results Each section begins with a brief definition and description of the intervention followed by a summary, where possible, of both the state and level of evidence for prevention and treatment, and ends with a “grade of recommendation.” The paper concludes with areas identified as requiring further research. Conclusions For UI, there are no prevention trials on lifestyle interventions. There are, however, few new intervention trials of lifestyle interventions involving weight loss and fluid intake with improved levels of evidence and grade of recommendation. Outside of pre- and post-natal pelvic floor muscle training (PFMT) trials for the prevention of female UI, there is a dearth of PFMT prevention trials for women with UI. PFMT remains the first-line treatment for female UI with high levels of evidence and grades of recommendation. Bladder training levels of evidence and grades of recommendation are maintained. For POP, new evidence supports the effectiveness of physiotherapy in the treatment of POP and there are now improved levels of evidence and grades of recommendation.

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Concert Program

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A month-long intensive measurement campaign was conducted in March/April 2007 at Agnes Water, a remote coastal site just south of the Great Barrier Reef on the east coast of Australia. Particle and ion size distributions were continuously measured during the campaign. Coastal nucleation events were observed in clean, marine air masses coming from the south-east on 65% of the days. The events usually began at ~10:00 local time and lasted for 1-4 hrs. They were characterised by the appearance of a nucleation mode with a peak diameter of ~10 nm. The freshly nucleated particles grew within 1-4 hrs up to sizes of 20-50 nm. The events occurred when solar intensity was high (~1000 W m-2) and RH was low (~60%). Interestingly, the events were not related to tide height. The volatile and hygroscopic properties of freshly nucleated particles (17-22.5 nm), simultaneously measured with a volatility-hygroscopicity-tandem differential mobility analyser (VH-TDMA), were used to infer chemical composition. The majority of the volume of these particles was attributed to internally mixed sulphate and organic components. After ruling out coagulation as a source of significant particle growth, we conclude that the condensation of sulphate and/or organic vapours was most likely responsible for driving particle growth during the nucleation events. We cannot make any direct conclusions regarding the chemical species that participated in the initial particle nucleation. However, we suggest that nucleation may have resulted from the photo-oxidation products of unknown sulphur or organic vapours emitted from the waters of Hervey Bay, or from the formation of DMS-derived sulphate clusters over the open ocean that were activated to observable particles by condensable vapours emitted from the nutrient rich waters around Fraser Island or Hervey Bay. Furthermore, a unique and particularly strong nucleation event was observed during northerly wind. The event began early one morning (08:00) and lasted almost the entire day resulting in the production of a large number of ~80 nm particles (average modal concentration during the event was 3200 cm-3). The Great Barrier Reef was the most likely source of precursor vapours responsible for this event.

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here/there/then/now was a practice-led research project that brought together 10 independent artists in dance, music, theatre and visual/media arts to create a site-specific program within the walls of the Brisbane Powerhouse. The purpose was to explore how to best conceive flexible performance platforms, theatricalise site-specific work and engage new audiences through forms of promenade experience that could provide open choices on how and where to view it. The sold out season of 6 performances, which took place 14-19 May 2002, presented three discrete performance installations set in intimate parts of the building, each with their own aesthetic and communicative intention, culminating in a fourth in-theatre installation, where memories of the first three coalesced and were reinterrogated. Each site thereby investigated meaning-making via the moving body and its critical relationship with space and objects, in a dramatic re-contextualisation of traditional solo dance forms, now re-articulated through interdisciplinary practices. The benefit of this approach was the creation of a layered and multimodal experience that could be both shared and subsequently critiqued by performers and audience alike.