999 resultados para SI-29
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In der vorliegenden Dissertation werden die Kernreaktionen 25Mg(alpha,n)28Si, 26Mg(alpha,n)29Si und 18O(alpha,n)21Ne im astrophysikalisch interessanten Energiebereich von E alpha = 1000 keV bis E alpha = 2450 keV untersucht.rnrnDie Experimente wurden am Nuclear Structure Laboratory der University of Notre Dame (USA) mit dem vor Ort befindlichen Van-de-Graaff Beschleuniger KN durchgeführt. Hierbei wurden Festkörpertargets mit evaporiertem Magnesium oder anodisiertem Sauerstoff mit alpha-Teilchen beschossen und die freigesetzten Neutronen untersucht. Zum Nachweis der freigesetzten Neutronen wurde mit Hilfe von Computersimulationen ein Neutrondetektor basierend auf rn3He-Zählrohren konstruiert. Weiterhin wurden aufgrund des verstärkten Auftretens von Hintergrundreaktionen verschiedene Methoden zur Datenanalyse angewendet.rnrnAbschliessend wird mit Hilfe von Netzwerkrechnungen der Einfluss der Reaktionen 25Mg(alpha,n)28Si, 26Mg(alpha,n)29Si und 18O(alpha,n)21Ne auf die stellare Nukleosynthese untersucht.rn
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The aim of this work was to verify the stability of the beta Co(2)Si phase in the Co-Si system. The samples were produced via arc-melting and characterized through Scanning Electron Microscopy (SEM) and Differential Thermal Analysis (DTA). The results have confirmed the stability of the beta Co(2)Si phase, however, a modification of the shape of beta CoSi phase field is proposed in order to fully explain the results.
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Context. The formation and evolution of the Galactic bulge and its relationship with the other Galactic populations is still poorly understood. Aims. To establish the chemical differences and similarities between the bulge and other stellar populations, we performed an elemental abundance analysis of alpha- (O, Mg, Si, Ca, and Ti) and Z-odd (Na and Al) elements of red giant stars in the bulge as well as of local thin disk, thick disk and halo giants. Methods. We use high-resolution optical spectra of 25 bulge giants in Baade's window and 55 comparison giants (4 halo, 29 thin disk and 22 thick disk giants) in the solar neighborhood. All stars have similar stellar parameters but cover a broad range in metallicity (-1.5 < [Fe/H] < +0.5). A standard 1D local thermodynamic equilibrium analysis using both Kurucz and MARCS models yielded the abundances of O, Na, Mg, Al, Si, Ca, Ti and Fe. Our homogeneous and differential analysis of the Galactic stellar populations ensured that systematic errors were minimized. Results. We confirm the well-established differences for [alpha/Fe] at a given metallicity between the local thin and thick disks. For all the elements investigated, we find no chemical distinction between the bulge and the local thick disk, in agreement with our previous study of C, N and O but in contrast to other groups relying on literature values for nearby disk dwarf stars. For -1.5 < [Fe/H] < -0.3 exactly the same trend is followed by both the bulge and thick disk stars, with a star-to-star scatter of only 0.03 dex. Furthermore, both populations share the location of the knee in the [alpha/Fe] vs. [Fe/H] diagram. It still remains to be confirmed that the local thick disk extends to super-solar metallicities as is the case for the bulge. These are the most stringent constraints to date on the chemical similarity of these stellar populations. Conclusions. Our findings suggest that the bulge and local thick disk stars experienced similar formation timescales, star formation rates and initial mass functions, confirming thus the main outcomes of our previous homogeneous analysis of [O/Fe] from infrared spectra for nearly the same sample. The identical a-enhancements of thick disk and bulge stars may reflect a rapid chemical evolution taking place before the bulge and thick disk structures we see today were formed, or it may reflect Galactic orbital migration of inner disk/bulge stars resulting in stars in the solar neighborhood with thick-disk kinematics.
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Partially solid commercial Al-Si and Mg-Al alloys have been deformed in shear during solidification using vane rheometry. The dendritic mush was deformed for a short period at 29% solid and allowed to cool naturally after deformation. Both alloys exhibited yield point behaviour and deformation was highly localised at the surface of maximum shear stress. The short period of deformation was found to have a distinct impact on the as-cast microstructure leading to fragmented dendrites in the deformation region of both alloys. In the case of the Mg-Al alloy, a concentrated region of interdendritic porosity was also observed in the deformation region. Concentrated porosity was not observed in the Al-Si alloy. (c) 2005 Elsevier B.V. All rights reserved.
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This paper is about a PV system connected to the electric grid by power electronic converters, using classical PI controller. The modelling for the converters emulates the association of a DC-DC boost with a two-level power inverter (TwLI) or three-level power inverter (ThLI) in order to follow the performance of a testing experimental system. Pulse width modulation (PWMo) by sliding mode control (SMCo) associated with space vector modulation (SVMo) is applied to the boost and the inverter. The PV system is described by the five parameters equivalent circuit. Parameter identification and simulation studies are performed for comparison with the testing experimental system.
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Treball de recerca realitzat per un alumne d'ensenyament secundari i guardonat amb un Premi CIRIT per fomentar l'esperit científic del Jovent l'any 2009. L’objectiu d’aquest treball ha estat donar pautes de reflexió sobre la crisi i el moment econòmic actual. Es volia valorar si era certa la idea que la situació econòmica dels nostres dies té certs paral•lelismes amb la crisi que va patir el món occidental el 1929. Per tal d’establir la veracitat de la hipòtesi plantejada es va dissenyar un model d’investigació basat en les entrevistes i en el recull i buidatge d’articles de premsa relacionats amb el tema, durant un període de temps no gaire extens, període que correspon als tres mesos a partir dels quals s’evidencia la situació de crisi. Al mateix temps era interessant copsar l’opinió de dos grans mestres en l’estudi de l’economia del nostre país, el Dr. Fabià Estapé i el Dr. Anton Costas, mestre i deixeble respectivament.. Sense esperar massa sorpreses, la crisi actual presenta molts punts de similitud amb el procés inciat l’any 1929. Ambdós esdeveniments econòmics tenen molts punts de connexió i les mesures proposades per solucionar o per pal•liar les conseqüències són també similars. En tots dos casos la figura de l’economista britànic John Maynard Keynes és cabdal per part dels diversos governs a l’hora de reconduir i adreçar la situació econòmica.
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[Acte. 1726-10-29. Les Thuilleries]
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A tensão de cisalhamento e a coesão do solo constituem importantes propriedades físicas do solo, podendo ser influenciadas pelo sistema de manejo e óxidos de Fe, Si e Al do solo. Os efeitos de diferentes sistemas de manejo de solo cultivado com cana-de-açúcar na tensão de cisalhamento, ângulo de atrito interno, coesão do solo e nos teores de óxidos de Fe, Si e Al de um Argissolo Amarelo Coeso foram estudados em quatro áreas da Usina Triunfo, no Estado de Alagoas. Os tratamentos abrangeram: uma área irrigada, uma área não irrigada, uma com aplicação de vinhaça e uma sob floresta nativa, como condição original. Amostras foram tiradas de cada área a 0,2-0,4 m e 0,4-0,8 m de profundidade. Os sistemas sequeiro e irrigado promoveram os maiores aumentos na coesão, ângulo de atrito interno e resistência ao cisalhamento do solo. Os teores de água e de óxidos no solo influíram nos valores de coesão do solo, tendo sido os maiores valores deste atributo obtidos em solos com teores de água mais baixos e solos com maiores teores de óxidos.
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En 2008 y en dos ocasiones, la Sala Primera del Tribunal Supremo ha resuelto la cuestión relativa a si el propietario de una finca, la cual había contaminado como consecuencia del desarrollo de su actividad industrial y había vendido ocultando esta circunstancia, es responsable extracontractualmente frente al tercer adquirente por los daños económicos sufridos. En la primera Sentencia, de 29.10.2008, el Tribunal Supremo condena al contaminador por responsabilidad extracontractual. En la segunda, de 22.12.2008, el Tribunal Supremo absuelve a éste de la responsabilidad extracontracual porqué los daños fueron causados a una finca propia.
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This thesis presents experimental studies of rare earth (RE) metal induced structures on Si(100) surfaces. Two divalent RE metal adsorbates, Eu and Yb, are investigated on nominally flat Si(100) and on vicinal, stepped Si(100) substrates. Several experimental methods have been applied, including scanning tunneling microscopy/spectroscopy (STM/STS), low energy electron diffraction (LEED), synchrotron radiation photoelectron spectroscopy (SR-PES), Auger electron spectroscopy (AES), thermal desorption spectroscopy (TDS), and work function change measurements (Δφ). Two stages can be distinguished in the initial growth of the RE/Si interface: the formation of a two-dimensional (2D) adsorbed layer at submonolayer coverage and the growth of a three-dimensional (3D) silicide phase at higher coverage. The 2D phase is studied for both adsorbates in order to discover whether they produce common reconstructions or reconstructions common to the other RE metals. For studies of the 3D phase Yb is chosen due to its ability to crystallize in a hexagonal AlB2 type lattice, which is the structure of RE silicide nanowires, therefore allowing for the possibility of the growth of one-dimensional (1D) wires. It is found that despite their similar electronic configuration, Eu and Yb do not form similar 2D reconstructions on Si(100). Instead, a wealth of 2D structures is observed and atomic models are proposed for the 2×3-type reconstructions. In addition, adsorbate induced modifications on surface morphology and orientational symmetry are observed. The formation of the Yb silicide phase follows the Stranski-Krastanov growth mode. Nanowires with the hexagonal lattice are observed on the flat Si(100) substrate, and moreover, an unexpectedly large variety of growth directions are revealed. On the vicinal substrate the growth of the silicide phase as 3D islands and wires depends drastically on the growth conditions. The conditions under which wires with high aspect ratio and single orientation parallel to the step edges can be formed are demonstrated.
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A seleção de genótipos com resistência quantitativa à ferrugem da folha da aveia (Avena sativa), baseada nos componentes que a condicionam, necessita do conhecimento da associação destes componentes entre si e deles com a quantidade de doença no campo, representada pela área abaixo da curva de progresso da doença (AACPD). Este trabalho objetivou determinar estas correlações, a partir de resultados de ensaios realizados previamente, em que 31 genótipos de aveia branca tiveram sua reação à ferrugem determinada no campo e seus componentes de resistência quantificados. As correlações encontradas foram geralmente baixas, tanto dos componentes entre si, como deles com a intensidade da doença no campo. As correlações mais altas, e consistentes entre os anos, com a AACPD foram da eficiência de infecção em plântulas, do período de latência e do comprimento de pústulas em plantas adultas. Estes dados sugerem que os componentes citados podem ter uma influência um pouco maior que os demais sobre a expressão da resistência parcial a campo. Entretanto, a baixa correlação entre os componentes medidos, indica que a seleção de genótipos, nesta interação patógeno-hospedeiro, não deve ser realizada com base em apenas um componente de resistência. Os resultados sugerem que a expressão da resistência parcial à ferrugem da folha da aveia não é condicionada apenas por um componente de resistência, mas sim pelo efeito conjunto de todos eles. Além disto, é possível que mecanismos diferenciados estejam atuando em cada genótipo, de forma que os componentes de resistência mais importantes para um não sejam os mesmos para outro.
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L’objectif de cette étude consiste à déterminer si les conventions de l’Organisation internationale du travail (OIT) sont effectives en ce qui concerne l’éradication du travail des enfants en Mauritanie. Cette effectivité est appréciée en mesurant la réception juridique et la réception sociale en Mauritanie de la Convention 29 sur le travail forcé, de la Convention 138 sur l’âge minimum d’admission à l’emploi et de la Convention 182 sur les pires formes de travail des enfants. La réception juridique des conventions est mesurée par un examen de l’intégration de leurs dispositions dans le droit national mauritanien. La réception juridique comprend également l’appréciation du contrôle du respect des conventions en territoire mauritanien. La réception sociale fait référence, quant à elle, aux stratégies de mise en œuvre des conventions de l’OIT par le Gouvernement mauritanien à travers ses programmes et ses politiques. Notre analyse démontre que l’effectivité des Conventions 29, 138 et 182 de l’OIT en ce qui concerne l’éradication du travail des enfants en Mauritanie est, selon nous, partielle. Dans l’ensemble, la situation tend à s’améliorer et le Gouvernement mauritanien tente de respecter l’esprit de ces conventions et de leur faire écho dans le droit national. Toutefois, il n’existe pas beaucoup d’information sur l’impact des programmes mis en place pour éradiquer le travail des enfants.
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Resumen tomado de la revista. Ponencia presentada en las Jornadas La normalització lingüística a l'ensenyament i a l'àmbit sindical, que tuvieron lugar en la sala de actos del edificio Anselm Turmeda del campus de la Universitat de les Illes Balears los días 3 y 4 de octubre de 2002