992 resultados para Astronomical chronology


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The work of the Director Plan for the Cathedral of Tarragona has allowed us to make a revision regarding the knowledge, chronology and features of the sacred area of the Concilium Provinciae Hispaniae Citerioris. We present diverse elements of architectural and sculptured decoration recovered from constructive levels of 1st century A.D, and the 6th century A.D levels of re-use and transformation, in contemporary constructions. All these elements ratify the process of imitation of the Forum Augustum made in the capital of the Hispania Citerior.

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Gaia is the most ambitious space astrometry mission currently envisaged and is a technological challenge in all its aspects. We describe a proposal for the payload data handling system of Gaia, as an example of a high-performance, real-time, concurrent, and pipelined data system. This proposal includes the front-end systems for the instrumentation, the data acquisition and management modules, the star data processing modules, and the payload data handling unit. We also review other payload and service module elements and we illustrate a data flux proposal.

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El objetivo de este breve artículo es presentar dos pequeños fragmentos de bronce procedentes de un sepulcro de La Clota (Calaceite, Teruel) que han sido identificados recientemente como pertenecientes a un trípode de tipo chipriota. Pasamos revista sucintamente a las principales cuestiones que plantea el hallazgo: cronología, orígenes, contexto social e influencia en el artesanado local.

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Damos noticia del primer alfarero conocido de terrra sigillata de la antigua Ilerda, -aunque no podemos sino conjeturar su nombre completo- tras los análisis de pasta que indican su condición de local. Se incide asimismo en la estimable fabricación de estas cerámicas (buen número de moldes), así como la cronología de las mismas.

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En el presente trabajo elaboraremos una relación actualizada de las publicaciones periódicas aparecidas en la Cataluña Occidental en el periodo comprendido entre 1808 y 1874. Las razones son dos. Por un lado, esta cronología nos parece correcta desde el punto de vista político, pues durante estos años se desarrolla la Revolución Liberal Burguesa que termina con el Antiguo Régimen absolutista y establece las bases de un Estado monárquico liberal y constitucional. Por otro lado, en Cataluña empieza a desarrollarse la Renaixença, un movimiento político y cultural particular de esta región española que determinará el contenido y las bases sociales del futuro nacionalismo catalán.

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Se ha estudiado un rodal adulto (edad media = 139 años) de Pinus nigra ssp. salzmannii var. pyrenaica en el W de la comarca del Solsonès (Lérida). Se han medido y extraído testigos de madera de 97 árboles adultos, a partir de los cuales se han medido e interdatado 13.340 anillos anuales, construyendo una cronología de crecimientos que abarca desde 1818 a 1996. Se han analizado las relaciones entre diversos parámetros dendrométricos medidos y los crecimientos observados, encontrándose en general muy bajas correlaciones. Se han construido tres series medias de crecimiento (cronología media, estandarizada, y en función de la edad) a partir de las cuales se ha analizado la evolución del rodal. Se ha observado un prolongado período de ralentización y estancamiento del crecimiento que se mantiene cerca de ochenta años, seguido de una fuerte corta a la que la masa reacciona con un notable incremento del crecimiento radial en un momento en que la edad media era ya de 101 años.

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We performed a spatiotemporal analysis of a network of 21 Scots pine (Pinus sylvestris) ring-width chronologies in northern Fennoscandia by means of chronology statistics and multivariate analyses. Chronologies are located on both sides (western and eastern) of the Scandes Mountains (67°N-70°N, 15°E-29°E). Growth relationships with temperature, precipitation, and North Atlantic Oscillation (NAO) indices were calculated for the period 1880-1991. We also assessed their temporal stability. Current July temperature and, to a lesser degree, May precipitation are the main growth limiting factors in the whole area of study. However, Principal Component Analysis (PCA) and mean interseries correlation revealed differences in radial growth between both sides of the Scandes Mountains, attributed to the Oceanic-Continental climatic gradient in the area. The gradient signal is temporally variable and has strengthened during the second half of the 20th century. Northern Fennoscandia Scots pine growth is positively related to early winter NAO indices previous to the growth season and to late spring NAO. NAO/growth relationships are unstable and have dropped in the second half of the 20th century. Moreover, they are noncontinuous through the range of NAO values: for early winter, only positive NAO indices enhance tree growth in the next growing season, while negative NAO does not. For spring, only negative NAO is correlated with radial growth.

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[spa]Los bozales y las muserolas en bronce para caballo constituyen unos excepcionales complementos ecuestres cuyo conocimiento se encuentra disperso en una extensa bibliografía. De muchos ejemplares apenas se ha publicado una breve descripción y nunca hasta el presente han sido objeto de un estudio monográfico, quizás por el desaliento que produce el desconocimiento de su procedencia en unos casos, o la superficial noticia del contexto de aparición en la mayoría de ellos, hecho que ha limitado las consideraciones cronológicas y de asociación. La identificación de nuevos ejemplares inéditos en los museos de Barcelona y Lleida ha animado a los autores a emprender un trabajo que por primera vez reúne y revisa los ejemplares conocidos de la Península Ibérica, para los que se propone una descripción normalizada, una clasificación tipológica y, en determinadas piezas, una sustancial revisión de las escenas decorativas y cronologías comúnmente admitidas. La seriación formal y la propuesta de datación implican la referencia de los ejemlares aparecidos en Grecia e Italia. Esa ampliación espacial conduce a replantear los agentes sociales que pueden estar detrás de la propagación de ese complemento ecuestre hasta la peninsua más occidental del Mediterráneo. [eng] Horse muzzles and Bronze muzzles are unique equestrian tools that have been referred to in scattered accounts throughout history. Nevertheless, the majority of these objects have received short descriptions and an overall study is still missing. The lack of a comprehensive study hinges on the over looked importance of these items and the superficial manner that have characterized their documentation. Both these reasons have limited observations on chronology and archaeological investigation. The recent identification of new unpublished exemplars among the Museums" collections in Barcelona and Lleida has encouraged the authors of this paper to start a new study dedicated to these objects. Starting from a catalogue inclusive of all muzzles and muzzles currently known in the Iberian Peninsula, an attempt will be made to propose an accurate description, typological classification and, for some of the items, a revision of the decorative scenes that have marked their place in bronze horse muzzle and muzzle chronology. The formal development and the chronological framework here proposed refer to those of the exemplars found in Greece and in Italy. The broadening of the geographical area will allow reconsideration of those social phenomena that have in the past determined the diffusion of elements in horse tack throughout most of the western Peninsula in the Mediterranean.

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The infilling of the river Ter Plain was produced by alluvial systems under the control of sea-level changes during the Quaternary. This paper describes the sedimentary evolution of the plain, and attemps to present a chronology of the recent geological events based on eustatic curves

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We use interplanetary transport simulations to compute a database of electron Green's functions, i.e., differential intensities resulting at the spacecraft position from an impulsive injection of energetic (>20 keV) electrons close to the Sun, for a large number of values of two standard interplanetary transport parameters: the scattering mean free path and the solar wind speed. The nominal energy channels of the ACE, STEREO, and Wind spacecraft have been used in the interplanetary transport simulations to conceive a unique tool for the study of near-relativistic electron events observed at 1 AU. In this paper, we quantify the characteristic times of the Green's functions (onset and peak time, rise and decay phase duration) as a function of the interplanetary transport conditions. We use the database to calculate the FWHM of the pitch-angle distributions at different times of the event and under different scattering conditions. This allows us to provide a first quantitative result that can be compared with observations, and to assess the validity of the frequently used term beam-like pitch-angle distribution.

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Context. White dwarfs can be used to study the structure and evolution of the Galaxy by analysing their luminosity function and initial mass function. Among them, the very cool white dwarfs provide the information for the early ages of each population. Because white dwarfs are intrinsically faint only the nearby (~ 20 pc) sample is reasonably complete. The Gaia space mission will drastically increase the sample of known white dwarfs through its 5-6 years survey of the whole sky up to magnitude V = 20-25. Aims. We provide a characterisation of Gaia photometry for white dwarfs to better prepare for the analysis of the scientific output of the mission. Transformations between some of the most common photometric systems and Gaia passbands are derived. We also give estimates of the number of white dwarfs of the different galactic populations that will be observed. Methods. Using synthetic spectral energy distributions and the most recent Gaia transmission curves, we computed colours of three different types of white dwarfs (pure hydrogen, pure helium, and mixed composition with H/He = 0.1). With these colours we derived transformations to other common photometric systems (Johnson-Cousins, Sloan Digital Sky Survey, and 2MASS). We also present numbers of white dwarfs predicted to be observed by Gaia. Results. We provide relationships and colour-colour diagrams among different photometric systems to allow the prediction and/or study of the Gaia white dwarf colours. We also include estimates of the number of sources expected in every galactic population and with a maximum parallax error. Gaia will increase the sample of known white dwarfs tenfold to about 200 000. Gaia will be able to observe thousands of very cool white dwarfs for the first time, which will greatly improve our understanding of these stars and early phases of star formation in our Galaxy.

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In this paper we design and develop several filtering strategies for the analysis of data generated by a resonant bar gravitational wave (GW) antenna, with the goal of assessing the presence (or absence) therein of long-duration monochromatic GW signals, as well as the eventual amplitude and frequency of the signals, within the sensitivity band of the detector. Such signals are most likely generated in the fast rotation of slightly asymmetric spinning stars. We develop practical procedures, together with a study of their statistical properties, which will provide us with useful information on the performance of each technique. The selection of candidate events will then be established according to threshold-crossing probabilities, based on the Neyman-Pearson criterion. In particular, it will be shown that our approach, based on phase estimation, presents a better signal-to-noise ratio than does pure spectral analysis, the most common approach.

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To understand how tree growth has responded to recent climate warming, an understanding of the tree-climate-site complex is necessary. To achieve this, radial growth variability among 204 trees established before 1850 was studied in relation to both climatic and site factors. Seventeen forest stands were sampled in the Spanish Central Pyrenees. Three species were studied: Pinus uncinata, Abies alba, and Pinus sylvestris. For each tree, a ring-width residual chronology was built. All trees cross-dated well, indicating a common influence of the regional climate. For the 1952-1993 period, the radial growth of all species, especially P. uncinata, was positively correlated with warm Novembers during the year before ring formation and warm Mays of the year the annual ring formed. Differences in species-stand elevation modulated the growth-climate associations. Radial growth in P. uncinata at high elevation sites was reduced when May temperatures were colder and May precipitation more abundant. In the 20th century, two contrasting periods in radial growth were observed: one (1900-1949) with low frequency of narrow and wide rings, low mean annual sensitivity, and low common growth variation; and another (1950-1994) with the reverse characteristics. The increased variability in radial growth since the 1950s was observed for all species and sites, which suggests a climatic cause. The low shared variance among tree chronologies during the first half of the 20th century may result from a"relaxation" of the elevation gradient, allowing local site conditions to dominate macroclimatic influence. These temporal trends may be related to the recently reported increase of climatic variability and warmer conditions. This study emphasizes the need to carefully assess the relationships between radial growth and site conditions along ecological gradients to improve dendroclimatic reconstructions.

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In 2009, Cygnus X-3 (Cyg X-3) became the first microquasar to be detected in the GeV γ-ray regime, via the satellites Fermi and AGILE. The addition of this new band to the observational toolbox holds promise for building a more detailed understanding of the relativistic jets of this and other systems. We present a rich data set of radio, hard and soft X-ray, and γ-ray observations of Cyg X-3 made during a flaring episode in 2010 May. We detect a ~3 day softening and recovery of the X-ray emission, followed almost immediately by a ~1 Jy radio flare at 15 GHz, followed by a 4.3σ γ-ray flare (E > 100 MeV) ~1.5 days later. The radio sampling is sparse, but we use archival data to argue that it is unlikely the γ-ray flare was followed by any significant unobserved radio flares. In this case, the sequencing of the observed events is difficult to explain in a model in which the γ-ray emission is due to inverse Compton scattering of the companion star's radiation field. Our observations suggest that other mechanisms may also be responsible for γ-ray emission from Cyg X-3.

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[cat]Els treballs arqueològics duts a terme al solar localitzat entre la plaça de Pau Vila i els carrers del Dr. Aiguader i de la Marquesa, al peu del baluard del Migdia, han permès descriure l'evolució geoarqueològica d'un tram del front marítim de Barcelona i generar dades fiables de la configuració de la façana litoral. Sota una potent capa de sorres, s'identificà un paquet de llims i argiles orgàniques característiques d'un medi de baixa energia; és a dir, protegit de l'onatge marí probablement per barres sorrenques. Aquesta seqüència presenta una cronologia entre finals del segle IX i ca. 1440, moment en què es realitzaren els primers intents de construcció d'estructures portuàries. En aquest nivell llimoargilós s'han dut a terme analítiques paleoambientals consistents en l'estudi pol·línic, sedimentològic i geoquímic dels sediments que han posat en evidència els canvis ambientals del front marítim barceloní, del paisatge vegetal del pla, com també de les activitats agrícoles i productives urbanes en època medieval i inicis de l'edat moderna. La informació així obtinguda ha estat contrastada amb la informació històrica. [eng]The archaeological work conducted at the site located at the foot of the Baluard del Migdia bastion between Plaça Pau Vila and Carrer Dr. Aiguader and Carrer Marquesa has provided the opportunity to describe the geoarchaeological evolution of a stretch of the seafront of Barcelona and to generate reliable data on the configuration of the coastline. A layer of silt and organic clays typical of a low-energy environment was found below a thick layer of sands. In other words, this packet was protected from the swell of the sea, probably by sandbars. This sequence presents a chronology spanning from the late 9th century BC to around 1440, the time when the first attempts were made to build port structures. This layer of silt and clay has been subjected to palaeoenvironmental analyses consisting of the study of the pollen, sediment and the geochemistry of the sediments. The results of this analysis provide evidence of the environmental changes in the seafront of Barcelona and the landscape in the plain, as well as the urban agricultural and production activities in medieval times and the early modern age. The information obtained has been compared with historical information.