50 resultados para archive virtuelle


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L"objectiu de la contribució que presentem és força senzill d"entendre: hem volgut donar forma a una activitat viscuda per recordar-la i per aprofitar-la quan l"haguem de menester. Com ho hem fet?, doncs materialitzant uns fets, uns pensaments i unes idees en forma de document, el qual a hores d"ara ja forma part del nostre fons personal. La finalitat del document, però, va més enllà: volem donar a conèixer la vàlua dels fons personals com a recurs estratègic per a l"aprenentatge de l"Arxivística. Hem volgut compartir la nostra experiència en aquest canal de comunicació professional perquè pensem, modestament, que treballs com aquest poden ser noves formes d"avançar en el progrés teòric de l"Arxivística.

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An annual-resolved precipitation reconstruction for the last 800 yr in Southern Spain has been performed using stable carbon isotope (δ13C) of Pinus nigra tree rings. The reconstruction exhibits high- to low-frequency variability and distinguishes a Little Ice Age (LIA, AD 13501850) characterized by lower averaged rainfall than both in the transition from the Medieval Climate Anomaly to the LIA and in the 20th century. The driest conditions are recorded during the Maunder solar Minimum (mid 17thearly 18th centuries), in good agreement with the Spanish documentary archive. Similar linkage between solar activity (maximum/minimum) and precipitation (increase/decrease) is observed throughout the entire LIA. Additionally, the relationship between the hydrological pattern in the Iberian Peninsula and Morocco during the LIA suggests different spatial distribution of precipitation in the south-eastern sector of the North Atlantic region such as it is known currently. Whereas in the instrumental record the precipitation evolves similarly in both regions and opposite to the North Atlantic oscillation (NAO) index, the coldest periods of the LIA shows a contrasting pattern with drier conditions in the South of Spain and wetter in Northern Africa. We suggest an extreme negative NAO conditions, accompanied by a southward excursion of the winter rainfall band beyond that observed in the last century, can explain this contrast. The sustained NAO conditions could have been triggered by solar minima and higher volcanic activity during the LIA.

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Poeta, autor de narracions i memòries, Miquel Martí i Pol també fou un prolífic traductor del francès, amb petites incursions en les literatures anglesa, italiana i llatinoamericana. S’estrenà a la segona meitat dels anys seixanta, quan la tènue obertura del Ministeri d’Informació i Turisme aportà aires de modernitat a la indústria editorial catalana, que volgué introduir i difondre nous corrents. En vuit anys, entre 1965 i 1973, traduí al català, majoritàriament del francès, vuit obres de la literatura i del pensament contemporanis. Contextualitzades les traduccions de Miquel Martí i Pol, l’article se centra en l’estudi dels expedients de censura dels vuit títols que traduí al català entre 1965 i 1973, dipositats a l’Archivo General de la Administración d’Alcalá de Henares.

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A short duration burst reminiscent of a soft gamma-ray repeater/anomalous X-ray pulsar behaviour was detected in the direction of LS I +61 303 by the Swift satellite. While the association with this well known gamma-ray binary is likely, a different origin cannot be excluded. Aims. We explore the error box of this unexpected flaring event and establish the radio, near-infrared and X-ray sources in our search for any peculiar alternative counterpart. Methods. We carried out a combined analysis of archive Very Large Array radio data of LS I +61 303 sensitive to both compact and extended emission. We also reanalysed previous near infrared observations with the 3.5 m telescope of the Centro Astronómico Hispano Alemán and X-ray observations with the Chandra satellite. Results. Our deep radio maps of the LS I +61 303 environment represent a significant advancement on previous work and 16 compact radio sources in the LS I +61 303 vicinity are detected. For some detections, we also identify near infrared and X-ray counterparts. Extended emission features in the field are also detected and confirmed. The possible connection of some of these sources with the observed flaring event is considered. Based on these data, we are unable to claim a clear association between the Swift-BAT flare and any of the sources reported here. However, this study represents the most sophisticated attempt to determine possible alternative counterparts other than LS I +61 303.

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Postprint (author’s final draft)