Magmatismo paleozoico en el Macizo del Roc de Frausa (Pirineos Orientales)

En el Macizo del Roc de Frausa se han diferenciado mediante criterios geoquímicos dos tipos diferentes de anfibolitas. El primer tipo lo forman metabasitas de afinidad toleitica y composición próxima a los E-MOIIB. Proceden de magmas poco evolucionados moderadamente bajos en potasio. Forman sills intercalados entre los metasedimentos cambro-ordovícicos y están asociadas a porfiroides gneísicos. Los porfiroides gneisicos representan términos ácidos subaluminicos de carácter explosivo y afinidad calcoalcalina con un contenido medio en potasio. Su relación genética con las metabasitas es poco clara; se interpretan como diferenciados ácidos de estas con una importante mezcla de material cortical. Se sugiere para este magmatismo un ámbito geodinámico continental fini-compresivo en relación con cucncas marginales.

A well-posedness theory in measures for some kinetic models of collective motion

We present existence, uniqueness and continuous dependence results for some kinetic equations motivated by models for the collective behavior of large groups of individuals. Models of this kind have been recently proposed to study the behavior of large groups of animals, such as flocks of birds, swarms, or schools of fish. Our aim is to give a well-posedness theory for general models which possibly include a variety of effects: an interaction through a potential, such as a short-range repulsion and long-range attraction; a velocity-averaging effect where individuals try to adapt their own velocity to that of other individuals in their surroundings; and self-propulsion effects, which take into account effects on one individual that are independent of the others. We develop our theory in a space of measures, using mass transportation distances. As consequences of our theory we show also the convergence of particle systems to their corresponding kinetic equations, and the local-in-time convergence to the hydrodynamic limit for one of the models.

Estudio de la alineación rotacional en la artroplastia total de rodilla mediante tomografía computarizada

L'alineació rotacional a l'astroplàstia total de genoll es refereix a la posició dels implants en el pla axial. Un mínim desplaçament afectarà la distribució de la càrrega y variarà l'estabilitat, l'alineació i la cinemàtica de l'articulació. Tot i que hi ha un consens pel que fa als efectes adversos d'una alineació rotacional incorrecta, encara no està clar quines són les referències anatòmiques que cal utilitzar. Les mesures de l'alineació rotacional requereixen un estudi d'alta qualitat. La TC és la modalitat d'imatge d'elecció per a l'estudi postoperatori de l'artroplàstia total de genoll. L'objectiu d'aquest treball es avaluar la capacitat diagnòstica de la TC per a l'estudi de l'alineació rotacional postoperatòria en l'artroplàstia total de genoll i presentar les variacions en el protocol de TC que minimitzen l'artefacte metàl•lic. Aquest estudi avalua la reproductibilitat de l'angle condili posterior, format per l'eix epicondili quirúrgic i la línia bicondilia posterior, mesurant la correlació entre dos observadors. El coeficient de correlació de Pearson mostra una forta correlació positiva (R=0.84) entre els dos observadors. La mitja d'error de les mesures adquirides és de -0.14º amb una desviació estàndar de 2.06º (-0.14 ± 2.06), per la qual cosa la modificació dels paràmetres tècnics de la TC per a la minimització dels artefactes metàl•lics és eficaç per l'avaluació rotacional. No obstant, l'alta magnitud de l'error indica que el radiòleg ha de ser prudent en el diagnòstic de mínimes variacions angulars que impliquin canvis en l'actitud mèdica i terapèutica.

Conception mécanique d'un chien robot : GIPO

La conceció de GIPO té com a areferència el gos AIBO, desenvolupat per Sony. L'estudi per a la seva realització comprèn el desenvolupament de la part tecnològica. S'assumeix que la cinemàtica d'AIBO ha estat àmpliament provada i que és òptima.

Identificación de tensiones iniciales en un macizo rocoso a partir de medidas de presión de agua en excavación de túneles

En las últimas décadas, dentro del mundo de la ingeniería civil, así como en otras disciplinas, se han desarrollado los métodos de identificación de parámetros. Esta técnica de estudio se basa en realizar un análisis inverso, el cual se lleva a cabo mediante técnicas probabilísticas normalmente, aunque existen otras técnicas para abordar el problema inverso. El objetivo final de la identificación de parámetros es a través de una serie de medidas realizar el análisis inverso y finalmente conocer que valor de un parámetro se ajusta mejor a las medidas realizadas.La mayoría de los trabajos asociados a la construcción de túneles han utilizado las medidas correspondientes a los desplazamientos para formular el problema de identificación. Dentro del presente trabajo se quiere profundizar en una vía de investigación poco desarrollada, la cual esta asociada a las medidas de presión de agua en la construcción de túneles. Las medidas de desplazamientos pueden presentar mayores desviaciones que las medidas de presión de agua, ya que las técnicas de auscultación causan una mayor distorsión de las condiciones iniciales en el caso de los

Variació del nivell del mar a la Península Ibèrica durant l'últim segle

Segons l'IPCC en valor mitjà mundial del nivell del mar augmenta a raó de 3.1 ± 0.7 mm·a-1. Aquest estudi ha calculat que a la Península Ibèrica, en nivell mitjà del mar ha augmentat a raó de 3.01 ± 0.45 mm·a-1, per tant, a un ritme similar del valor mundial. No obstant, es mostra un comportament diferent entre el conjunt Atlàntic - Cantàbric i el Mediterrani, que podria ser explicat pel efecte baromètric invertit i l'expansió tèrmica. En l'últim període estudiat, 1997-2009, les tendències mostren un augment dels ritmes de pujada en totes les zones amb resultats estadísticament significatius. En un futur, es preveu que en el conjunt de la Península Ibèrica el nivell mitjà del mar augmenti per a l'any 2050, 104 ± 30 mm i per a l'any 2100, 174 ± 60 mm. Aquest fet podria tenir un impacte important sobre les costes ibèriques, i per tant, catalanes.

A new maximum likelihood method for luminosity calibrations

A new statistical parallax method using the Maximum Likelihood principle is presented, allowing the simultaneous determination of a luminosity calibration, kinematic characteristics and spatial distribution of a given sample. This method has been developed for the exploitation of the Hipparcos data and presents several improvements with respect to the previous ones: the effects of the selection of the sample, the observational errors, the galactic rotation and the interstellar absorption are taken into account as an intrinsic part of the formulation (as opposed to external corrections). Furthermore, the method is able to identify and characterize physically distinct groups in inhomogeneous samples, thus avoiding biases due to unidentified components. Moreover, the implementation used by the authors is based on the extensive use of numerical methods, so avoiding the need for simplification of the equations and thus the bias they could introduce. Several examples of application using simulated samples are presented, to be followed by applications to real samples in forthcoming articles.

uvbyHbeta photometry of main sequence A type stars.

We present Stroemgren uvby and Hbeta_ photometry for a set of 575 northern main sequence A type stars, most of them belonging to the Hipparcos Input Catalogue, with V from 5mag to 10mag and with known radial velocities. These observations enlarge the catalogue we began to compile some years ago to more than 1500 stars. Our catalogue includes kinematic and astrophysical data for each star. Our future goal is to perform an accurate analysis of the kinematical behaviour of these stars in the solar neighbourhood.

Period-Luminosity-Colour distribution and classification of Galactic oxygen-rich LPVs I. Luminosity calibrations

The absolute K magnitudes and kinematic parameters of about 350 oxygen-rich Long-Period Variable stars are calibrated, by means of an up-to-date maximum-likelihood method, using HIPPARCOS parallaxes and proper motions together with radial velocities and, as additional data, periods and V-K colour indices. Four groups, differing by their kinematics and mean magnitudes, are found. For each of them, we also obtain the distributions of magnitude, period and de-reddened colour of the base population, as well as de-biased period-luminosity-colour relations and their two-dimensional projections. The SRa semiregulars do not seem to constitute a separate class of LPVs. The SRb appear to belong to two populations of different ages. In a PL diagram, they constitute two evolutionary sequences towards the Mira stage. The Miras of the disk appear to pulsate on a lower-order mode. The slopes of their de-biased PL and PC relations are found to be very different from the ones of the Oxygen Miras of the LMC. This suggests that a significant number of so-called Miras of the LMC are misclassified. This also suggests that the Miras of the LMC do not constitute a homogeneous group, but include a significant proportion of metal-deficient stars, suggesting a relatively smooth star formation history. As a consequence, one may not trivially transpose the LMC period-luminosity relation from one galaxy to the other.

Crystallization behaviour of some melt spun Nd-Fe-B alloys

The kinetics of crystallization of four amorphous (or partially amorphous) melt spun Nd-Fe-B alloys induced by thermal treatment is studied by means of differential scanning calorimetry and scanning electron microscopy, In the range of temperatures explored experimentally, the crystallization process is thermally activated and generally proceeds in various stages. The Curie temperature and the crystallization behavior have been measured. The apparent activation energy of crystallization of most of the crystallization stages has been determined for each melt spun alloy. The explicit form of the kinetic equation that best describes the first stage of crystallization has been found. It follows in general the Johnson-Mehl-Avrami-Erofe'ev model, but clear deviations to that model occur for one alloy. Scanning electron microscopy demonstrates that preferentially hetereogeneous nucleation occurs at the ribbon surface which was in contact with the wheel. From crystallization kinetics results the lower part of the experimental time-temperature-transformation curves for all studied alloys are deduced and extrapolated to the high temperature limit of their range of validity, also deduced.

Accuracy in the experimental calorimetric study of the crystallization kinetics and predicitve transformation diagrams: Application to a Ga-Te amorphous alloy

The uncertainties inherent to experimental differential scanning calorimetric data are evaluated. A new procedure is developed to perform the kinetic analysis of continuous heating calorimetric data when the heat capacity of the sample changes during the crystallization. The accuracy of isothermal calorimetric data is analyzed in terms of the peak-to-peak noise of the calorimetric signal and base line drift typical of differential scanning calorimetry equipment. Their influence in the evaluation of the kinetic parameters is discussed. An empirical construction of the time-temperature and temperature heating rate transformation diagrams, grounded on the kinetic parameters, is presented. The method is applied to the kinetic study of the primary crystallization of Te in an amorphous alloy of nominal composition Ga20Te80, obtained by rapid solidification.

Fusion of the extended modified liquid drop model for nucleation and dynamical nucleation theory

We present a new phenomenological approach to nucleation, based on the combination of the extended modified liquid drop model and dynamical nucleation theory. The new model proposes a new cluster definition, which properly includes the effect of fluctuations, and it is consistent both thermodynamically and kinetically. The model is able to predict successfully the free energy of formation of the critical nucleus, using only macroscopic thermodynamic properties. It also accounts for the spinodal and provides excellent agreement with the result of recent simulations.

The Besançon Galaxy Model renewed. I. Constraints on the Galactic thin disc evolution from Tycho data

Context. The understanding of Galaxy evolution can be facilitated by the use of population synthesis models, which allow to test hypotheses on the star formation history, star evolution, as well as chemical and dynamical evolution of the Galaxy. Aims. The new version of the Besanc¸on Galaxy Model (hereafter BGM) aims to provide a more flexible and powerful tool to investigate the Initial Mass Function (IMF) and Star Formation Rate (SFR) of the Galactic disc. Methods. We present a new strategy for the generation of thin disc stars which assumes the IMF, SFR and evolutionary tracks as free parameters. We have updated most of the ingredients for the star count production and, for the first time, binary stars are generated in a consistent way. We keep in this new scheme the local dynamical self-consistency as in Bienayme et al (1987). We then compare simulations from the new model with Tycho-2 data and the local luminosity function, as a first test to verify and constrain the new ingredients. The effects of changing thirteen different ingredients of the model are systematically studied. Results. For the first time, a full sky comparison is performed between BGM and data. This strategy allows to constrain the IMF slope at high masses which is found to be close to 3.0, excluding a shallower slope such as Salpeter"s one. The SFR is found decreasing whatever IMF is assumed. The model is compatible with a local dark matter density of 0.011 M pc−3 implying that there is no compelling evidence for significant amount of dark matter in the disc. While the model is fitted to Tycho2 data, a magnitude limited sample with V<11, we check that it is still consistent with fainter stars. Conclusions. The new model constitutes a new basis for further comparisons with large scale surveys and is being prepared to become a powerful tool for the analysis of the Gaia mission data.

Concepcions i raonaments en l'ús de sistemes de referència galileans

Durant la darrera dècada s'han multiplicat les investigacions sobre les idees que tenen els nens i els estudiants en general de diversos aspectes que s'estudien a les classes de Ciències i de !'impacte que les classes de Ciències fan 'Sobre aquestes idees ( Driver i Erickson, 1983, Gilbert i Watts, 1983, Osborne i Freyberg, 1985, etc. )...