Buffered high charge spectrally-peaked proton beams in the relativistic-transparency regime

Spectrally-peaked proton beams of high charge (E_p ≈ 8 MeV, ΔE ≈ 4 MeV, N ≈ 50 nC ) have been observed from the interaction of an intense laser (>10¹⁹Wcm^-2) with ultrathinCHfoils, as measured by spectrally-resolved full beam profiles. These beams are reproducibly generated for foil thicknesses 5-100 nm, and exhibit narrowing divergence with decreasing target thickness down to ≈8° for 5 nm. Simulations demonstrate that the narrow energy spread feature is a result of buffered acceleration of protons. The radiation pressure at the front of the target results in asymmetric sheath fields which permeate throughout the target, causing preferential forward acceleration. Due to their higher chargeto-mass ratio, the protons outrun a carbon plasma driven in the relativistic transparency regime.

Parametric scans of HB and LS-RPA regimes employing Petawatt laser

By contrast to the Target Normal Sheath acceleration (TNSA) mechanism [1], Radiation Pressure Acceleration (RPA) is currently attracting a substantial amount of experimental [2,3] and theoretical [4-6] attention worldwide due to its superior scaling in terms of ion energy and laser-ion conversion efficiency. Employing Vulcan Petawatt lasers of the Rutherford Appleton Laboratory, UK, both the Hole-boring (HB) and the Light-Sail (LS) regimes of the RPA have been extensively explored. When the target thickness is of the order of hole-boring velocity times the laser pulse duration, highly collimated plasma jets of near solid density are ejected from the foil, lasting up to ns after the laser interaction. By changing the linear polarisation of the laser to circular, improved homogeneity in the jet's spatial density profile is achieved which suggests more uniform and sustained radiation pressure drive on target ions. By decreasing the target areal density or increasing irradiance on the target, the LS regime of the RPA is accessed where relatively high flux (~ 1012 particles/MeV/Sr) of ions are accelerated to ~ 10 MeV/nucleon energies in a narrow energy bandwidth. The ion energy scaling obtained from the parametric scans agrees well with theoretical estimation based on RPA mechanism and the narrow bandwidth feature in the ion spectra is studied by 2D particle-in-simulations.

Ion acceleration and plasma jet formation in ultra-thin foils undergoing expansion and relativistic transparency

At sufficiently high laser intensities, the rapid heating to relativistic velocities and resulting decompression of plasma electrons in an ultra-thin target foil can result in the target becoming relativistically transparent to the laser light during the interaction. Ion acceleration in this regime is strongly affected by the transition from an opaque to a relativistically transparent plasma. By spatially resolving the laser-accelerated proton beam at near-normal laser incidence and at an incidence angle of 30°, we identify characteristic features both experimentally and in particle-in-cell simulations which are consistent with the onset of three distinct ion acceleration mechanisms: sheath acceleration; radiation pressure acceleration; and transparency-enhanced acceleration. The latter mechanism occurs late in the interaction and is mediated by the formation of a plasma jet extending into the expanding ion population. The effect of laser incident angle on the plasma jet is explored.

Scaling of Ion Spectral Peaks in the Hybrid RPA-TNSA Region

The role of the radiation pressure of an intense laser beam in the formation of proton and carbon spectra from thin foils is discussed. The data presented suggests that, in competition with the Target Normal Sheath Acceleration mechanism, the onset of the Light Sail (LS) region of Radiation Pressure Acceleration can be obtained for suitably thin targets at currently available laser intensities,. The spectral features and their scaling with the laser and target parameters are consistent with the scenario of Light Sail (LS) acceleration.

Phylogenetic and functional diversity of estuarine bacterioneuston

A micro-camada superficial da água (SML) é caracterizada pela ocorrência de grandes quantidades de compostos orgânicos, pela acumulação de contaminantes antropogênicos e é submetida a uma intensa radiação solar, extrema mudança de temperatura e, no caso dos estuários, flutuação de salinidade. Estas propriedades físico-químicas estão, provavelmente, a modular a comunidade bacteriana (bacterioneuston) com propriedades filogenéticas e funcionais específicas. Neste estudo, as abordagens dependentes e independentes do cultivo foram aplicadas para avaliar a estrutura e dinâmica das comunidades bacterioneuston e bacterioplâncton em três localizações geográficas ao longo do estuário da Ria de Aveiro. Além disso, comparámos a diversidade filogenética de grupos específicos (Aeromonas, Pseudomonas e Psychrobacter) presentes em bacterioneuston e bacterioplâncton. Finalmente, as duas comunidades foram comparadas em termos de prevalência e diversidade de bactérias resistentes aos antibióticos e respetivos genes de resistência. Bactérias heterotróficas cultiváveis foram enriquecidas em SML. Eletroforese em gel de gradiente desnaturante (DGGE) permitiu a identificação de filotipos específicos em SML. Além disso, a análise de agrupamento dos perfis de DGGE de ambas as comunidades revelou uma ligeira tendência de agrupamento de acordo com a camada amostrada. As diferenças entre as duas comunidades variaram de acordo com factores espaciais e temporais. Em termos de diversidade filogenética de grupos específicos, não foram identificadas diferenças consistentes entre SML e UW com relação às comunidades de Aeromonas. Com relação ao género Pseudomonas, uma unidade operacional taxonómica cultivável foi consistentemente hiper-representada nas amostras de SML. Metodologias dependentes e independentes do cultivo revelaram a presença de populações de Psychrobacter complexas e muito estáveis em todos os sítios e datas de amostragens, com diferenças significativas entre as comunidades de Psychrobacter presentes em SML e UW. Estirpes representativas de prováveis novas espécies também foram cultivadas. Em termos de resistência aos antibióticos, a prevalência de bactérias resistentes em SML foi alta sugerindo selecção pelas condições presentes em SML. É preciso enfatizar que a resistência aos antibióticos foi incomum entre as bactérias estuarinas e os mecanismos de resistência foram, predominantemente, intrínsecos. Pela combinação de abordagens inovadoras dependentes e independentes do cultivo, este estudo forneceu novas e consistentes informações com relação às diferenças em ambas as comunidades bacterianas e em relação a alguns dos fatores que contribuem para a sua formação.

Primary production in systems subject to natural and anthropogenic eutrophication

Tese dout., Química, Universidade do Algarve, 2005

Application of radial basis function neural networks to a greenhouse inside air temperature model

The problem with the adequacy of radial basis function neural networks to model the inside air temperature as a function of the outside air temperature and solar radiation, and the inside relative humidity in an hydroponic greenhouse is addressed.

Comparison of on-line learning algorithms for RBF models in greenhouse environmental control problems

The problem with the adequacy of radial basis function neural networks to model the inside air temperature as a function of the outside air temperature and solar radiation, and the inside relative humidity in an hydroponic greenhouse is addressed.

Identification of greenhouse climate dynamic models

In this paper climate discrete-time dynamic models for the inside air temperature of two different greenhouses are identified, using data acquired during two different periods of the year. These models employ data from air temperature and relative humidity (both outside and inside the greenhouse), solar radiation, wind speed, and control inputs (ventialtion, etc.).

Predicting the greenhouse inside air temperature with RBF neural networks

The application of the Radial Basis Function (RBF) Neural Network (NN) to greenhouse inside air temperature modelling has been previously investigated (Ferreira et al., 2000a). In those studies, the inside air temperature is modelled as a function of the inside relative humidity and of the outside temperature and solar radiation. A second-order model structure previously selected (Cunha et al., 1996) in the context of dynamic temperature models identification, is used.

Évaluation du potentiel de croissance et de rendement d’une culture de tomates biologiques cultivées dans une serre climatisée à l’aide d’un système géothermique

Ce projet visait à comparer les effets agronomiques d’une serre de tomates biologiques semi-fermée utilisant un système de climatisation par géothermie comparativement à une serre ouverte. Deux serres de 228 et 230 m2 ont été équipées d’un système d’échangeur d’air avec géothermie qui refroidissait et déshumidifiait l’air (serre semi-fermée) et d’un système de ventilation naturelle (serre témoin). Ces dernières ont été comparées au cours des années 2012 et 2013 entre lesquels les traitements ont été permutés. Les variables mesurées étaient les paramètres de croissance des plants ainsi que le rendement, le calibre des fruits et les propriétés physico-chimiques des tomates. Les résultats ont démontré que le système de climatisation n’a pas eu d’effets significatifs sur la croissance des plants, la qualité des fruits ainsi que le rendement. Les deux serres avaient des cibles de concentration en CO2 comprises entre 450 µL L-1 et 1000 µL L-1 selon l’ensoleillement. Les quantités de CO2 injectées ont été de 11 kg/m2 et 15 kg/m2 respectivement en 2012 et 2013 dans la serre semi-fermée alors qu’elles ont été de 24 kg/m2 et 25 kg/m2 dans la serre témoin. Bien qu’ayant nécessité moins d’injection, la serre semi-fermée a permis de conserver des concentrations en CO2 de 638 µL L-1 en 2012 et de 593 µL L-1 en 2013. Ces concentrations sont plus élevées que celles obtenues dans la serre témoin qui étaient respectivement de 385 µL L-1 et 486 µL L-1 en 2012 et 2013. De ce fait, le coût monétaire associé à l’enrichissement carboné a été de 1,6 à 2,0 fois plus élevé dans la serre témoin que dans la serre semi-fermée.

Do Urban Canyons Influence Street Level Grass Pollen Concentrations

In epidemiological studies, outdoor exposure to pollen is typically estimated using rooftop monitoring station data, whilst exposure overwhelmingly occurs at street level. In this study the relationship between street level and roof level grass pollen concentrations was investigated for city centre street canyon environments in Aarhus, Denmark, and London, UK, during the grass pollen seasons of 2010 and 2011 respectively. For the period mid-day to late evening, street level concentrations in both cities tended to be lower than roof-level concentrations, though this difference was found to be statistically significant only in London. The ratio of street/roof level concentrations was compared with temperature, relative humidity, wind speed and direction, and solar radiation. Results indicated that the concentration ratio responds to wind direction with respect to relative canyon orientation and local source distribution. In the London study, an increase in relative humidity was linked to a significant decrease in street/roof level concentration ratio, and a possible causative mechanism involving moisture mediated pollen grain buoyancy is proposed. Relationships with the other weather variables were not found to be significant in either location. These results suggest a tendency for monitoring station data to overestimate exposure in the canyon environment.

Mesoscale Atmospheric Transport of Ragweed Pollen Allergens from Infected to Uninfected Areas

Allergenic ragweed (Ambrosia spp.) pollen grains, after being released from anthers, can be dispersed by air masses far from their source. However, the action of air temperature,humidity and solar radiation on pollen grains in the atmosphere could impact on the ability of long distance transported (LDT) pollen to maintain allergenic potency. Here, we report that the major allergen of Ambrosia artemisiifolia pollen (Amb a 1) collected in ambient air during episodes of LDT still have immunoreactive properties. The amount of Amb a 1 found in LDT ragweed pollen grains was not constant and varied between episodes. In addition to allergens in pollen sized particles, we detected reactive Amb a 1 in subpollen sized respirable particles. These findings suggest that ragweed pollen grains have the potential to cause allergic reactions, not only in the heavily infested areas but, due to LDT episodes, also in the regions unaffected by ragweed populations.

Tarefas de investigação na aprendizagem do tema energia : do sol para a terra

Relatório da Prática de Ensino Supervisionada, Mestrado em Ensino de Física e Química no 3º ciclo do Ensino Básico e no Ensino Secundário, Universidade de Lisboa, 2015