OSIRIS Imaging and Spectroscopy for the GTC     

Jordi Cepa 《Astrophysics and Space Science》1998,263(1-4):369-372

The characteristics of OSIRIS (Optical System for Imaging and low-Resolution Integrated Spectroscopy), an instrument for imaging and low resolution spectroscopy proposed for the GTC 10m telescope, are described. OSIRIS is a multi-purpose instrument that incorporates in a "classical design" several innovations, already tested in 4m-class telescopes, that will provide a powerful first light instrument for the GTC. This revised version was published online in July 2006 with corrections to the Cover Date.  相似文献   

Lower Paleozoic extensional tectonics in the limit between the West Asturian-Leonese and Central Iberian Zones of the Variscan Fold-Belt in NW Spain   总被引：1，自引：1，他引：0  

J. R. Martinez Catalan  M. P. Hacar Rodriguez  P. Villar Alonso  A. Perez-Estaun  F. Gonzalez Lodeiro 《International Journal of Earth Sciences》1992,81(2):545-560

The limit between the West Asturian-Leonese and Central-Iberian Zones in the NW of the Iberian Peninsula is described in the area of Caurel-Truchas (Provinces of Orense and León). From the distribution of the sedimentary formations and the Variscan structures it is inferred that the transition between the two zones was a fault system, which was active during, at least, the Ordovician and Lower Silurian. The faults were supposedly normal, though they had probably some strike-slip component, and gave rise to a half-graben in which a syn-rift sequence was deposited. The latter underwent inversion at the onset of the Variscan tectonism, producing a ramp anticline-syncline pair that forms the more important folds in the area. The varying geometry of these folds is interpreted partly as being due to the existence of previous en échelon folds related to the strike-slip component of the faults and, partly, as a result of the variable intensity of the shear strain undergone during the first variscan phase.

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Zusammenfassung Die Grenze zwischen der West-Asturischen-Leonesischen und Zentral-Iberischen Zone im NW der Iberischen Halbinsel wird aus dem Gebiet von Caurel-Truchas (Provinz Orense und León) beschrieben. Aufgrund der Verteilung der sedimentären Formationen, sowie der variszischen Strukturen wird abgeleitet, daß der Übergang zwischen den beiden Zonen durch ein Störungssystem bedingt wurde, das zumindest zwischen Ordovizium und Untersilur aktiv war. Dabei handelte es sich vermutlich um Abschiebungen mit einer Horizontalverschiebungskomponente. Diese Ausbildung führte zu einem Halbgraben mit darin abgelagerter sedimentärer Syn-Riftsequenz. Letztere wurde während der Anfangsphase der variszischen Tektonik invertiert, so daß es zu einem Rampen-Antiklinal-Synklinal Paar kam, welches die wichtigsten Falten der Gegend bildet. Die variable Geometrie der Falten wird zum einen der Existenz von frühen En-échelon Falten zugeschrieben, die durch die Horizontalverschiebungskomponente der Störungen hervorgerufen wurden; zum anderen sind sie das Resultat der veränderlichen Intensität der Scherspannung während der ersten variszischen Phase.

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Resumen Se describe el límite entre las Zonas Asturoccidental-Leonesa y Centroibérica en el NO de la Península Ibérica en el área del Caurel-Truchas (Provincias de Orense y León). Partiendo de la distribución de las formaciones sedimentarias y de la geometría de las estructuras varíscicas, se deduce que la transición entre las dos zonas fue un sistema de fallas, que fue activo al menos durante el Ordovício y el Silúrico Inferior. Se supone que la principal componente de las fallas fue normal, aunque debió de existir también una componente de desgarre, y su juego originó un semi-graben en el que se acumuló una secuencia sin-rift. Esta última experimentó una inversión al principio de la tectogénesis Varíscica, formándose un par de pliegues de rampa que son los pliegues más importantes del área. La geometría variable de esos pliegues se interpreta como debida, en parte, a la existencia previa de pliegues en escalón relacionados con la componente de desgarre de las fallas y, en parte, como consecuencia de la variable intensidad de la deformación por cizallamiento sufrida durante la primera fase de deformación varíscica.

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How “African” was the early human dispersal out of Africa?     

Jordi Agustí  David Lordkipanidze 《Quaternary Science Reviews》2011,30(11-12):1338-1342

In this paper we review a number of scenarios which have been proposed to explain the first hominin “out of Africa” at the base of the Pleistocene. These are the brain expansion scenario, the cultural exclusion scenario, the migratory wave scenario and the common African home scenario. These scenarios are checked against the current evidence provided by the Georgian site of Dmanisi, which contains the oldest Eurasian hominins. Therefore, it is concluded that none of these scenarios fits with the existing evidence, and that the only real African influence in Dmanisi is restricted to early Homo itself. In order to explain the presence of early Homo at Dmanisi, it is concluded that the expansion out of Africa should have happened before the actual datum of Dmanisi, most probably linked to the spread of Mode 1 tools in Africa.  相似文献   

Organic Pollutants in Coastal Waters,Sediments, and Biota: A Relevant Driver for Ecosystems During the Anthropocene?     

Jordi Dachs  Laurence Méjanelle 《Estuaries and Coasts》2010,33(1):1-14

The total number of synthetic organic chemicals introduced to the environment by humans has never been quantified, but it is not lower than thousands. A fraction of these chemicals have toxic effects to coastal organisms and presumably affect ecosystems structure and function. During the last decades, some of the processes affecting the transport, degradation, and fate of a limited number of chemicals have been studied, and the rising concern for environmental risk of organic chemical has lead to the regulation of a few of them by national and international organisms. However, the environmental inventory of organic pollutants is far from being quantified, and current methodologies used in most toxicological tests only allow to determine effects of individual chemicals to organisms. There are major limitations on appropriate methodologies to assess the effects of organic pollutants at population and ecosystem levels and the effects induced by complex mixtures of organic pollutants present in natural environments. The modification of the composition of the biosphere by a myriad of organic pollutants at ultra-trace levels is not yet regarded as another vector of environmental change which is irreversible due to the persistent character of many of these chemicals and due to its global coverage. Here, we claim that the modification of the atmosphere, water, sediments, and biota composition is a factor to be taken into account in coastal ecosystems, and that its pressure on the environment has been exponentially increasing during the last six decades of the anthropocene.  相似文献   

Pseudo-nitzschia spp. (Bacillariophyceae) and dissolved organic matter (DOM) dynamics in the Ebro Delta (Alfacs Bay, NW Mediterranean Sea)     

Sofia Loureiro  Esther Garcs  Margarita Fernndez-Tejedor  Dolors Vaqu  Jordi Camp 《Estuarine, Coastal and Shelf Science》2009,83(4):539-549

Samples were collected during one annual cycle (April 2007–March 2008) at Alfacs Bay (NW Mediterranean Sea) central station in order to assess the influence of organic nutrients in the growth of the microalgae assemblage, with special reference to Pseudo-nitzschia spp. This potentially toxic diatom forms natural and recurrent blooms in the study area. To assess further the relationship between Pseudo-nitzschia spp. and nutrients an enrichment experiment with high molecular weight dissolved organic matter (HMWDOM) was performed with field samples obtained during a Pseudo-nitzschia spp. bloom. HMWDOM was extracted from water collected at Alfacs Bay. Five bioassays were prepared: N + P (seawater with addition of nitrate and phosphate), DOM (addition of HMWDOM), (−N + P) + DOM (nitrogen deficient, with addition of phosphate and HMWDOM), (N + P) + DOM (addition of nitrate, phosphate and HMWDOM), seawater control (without added nutrients), and B + DOM (control of bacteria, without microalgae). The experiment was run in batch mode over 4 days. Results from the field study revealed that the concentrations of organic nutrients mostly surpassed the inorganic pool. Pseudo-nitzschia spp. was the most frequent and abundant taxa of the microalgae community. The micro-planktonic assemblage was arranged according to a seasonal factor (ANOSIM and cluster analysis). DON, nitrate and silicate were the most important abiotic parameters contributing to the dissimilarities between seasons (SIMPER analysis) and thereby potentially influencing the seasonal distribution of microalgae in the representative station. In the experimental investigation, Pseudo-nitzschia cells increased by the end of the experiment in the DOM bioassay but no respective increase was observed for chlorophyll a. This could point to an acquisition of nutrients through the DOM fraction that would conjointly reduce the need of chlorophyll a. The data obtained suggest that organic nutrients may exert an important role in the development of microalgae, including Pseudo-nitzschia spp., in the selected location.  相似文献   

The impact of a merger episode in the galactic disc white dwarf population     

Santiago Torres  Enrique García-Berro  reas Burkert  Jordi Isern 《Monthly notices of the Royal Astronomical Society》2001,328(2):492-500

In this paper we analyse the consequences in the white dwarf population of a hypothetical merger episode in our Galactic disc. We have studied several different merging scenarios with our Monte Carlo simulator. For each one of these scenarios we have derived the main characteristics of the resulting white dwarf population and we have compared them with the available observational data, namely the white dwarf luminosity function and the kinematic properties of the white dwarf population. Our results indicate that very recent (less than ∼6 Gyr ago) and massive (∼16 per cent of the mass of our Galaxy) merger episodes are quite unlikely in view of the available kinematical properties of the disc white dwarf population. Smaller merger episodes (of the order of ∼4 per cent of the mass of our Galaxy) are, however, compatible with our current knowledge of those kinematical properties. Finally, we prove that the white dwarf luminosity function is quite insensitive to such a merger episode.  相似文献   

The Ardón L6 ordinary chondrite: A long‐hidden Spanish meteorite fall     

Josep M. Trigo‐Rodríguez  Jordi Llorca  Mona Weyrauch  Addi Bischoff  Carles E. Moyano‐Cambero  Klaus Keil  Matthias Laubenstein  Andreas Pack  José María Madiedo  Jacinto Alonso‐Azcárate  My Riebe  Rainer Wieler  Uli Ott  Mar Tapia  Narcís Mestres 《Meteoritics & planetary science》2014,49(8):1475-1484

We report and describe an L6 ordinary chondrite fall that occurred in Ardón, León province, Spain (longitude 5.5605°W, latitude 42.4364°N) on July 9th, 1931. The 5.5 g single stone was kept hidden for 83 yr by Rosa González Pérez, at the time an 11 yr old who had observed the fall and had recovered the meteorite. According to various newspaper reports, the event was widely observed in Northern Spain. Ardón is a very well‐preserved, fresh, strongly metamorphosed (petrologic type 6), and weakly shocked (S3) ordinary chondrite with well‐equilibrated and recrystallized minerals. The mineral compositions (olivine Fa_23.7±0.3, low‐Ca pyroxene Fs_20.4±0.2Wo_1.5±0.2, plagioclase An_10.3±0.5Ab_84.3±1.2), magnetic susceptibility (log χ = 4.95 ± 0.05 × 10^?9 m³ kg^?1), bulk density (3.49 ± 0.05 g   cm^?3), grain density (3.58 ± 0.05 g   cm^?3), and porosity (2.5 vol%) are typical for L6 chondrites. Short‐lived radionuclides confirm that the meteorite constitutes a recent fall. The ²¹Ne and ³⁸Ar cosmic ray exposure ages are both about 20–30 Ma, similar to values for many other L chondrites. The cosmogenic ²²Ne/²¹Ne ratio indicates that preatmospheric Ardón was a relatively large body. The fact that the meteorite was hidden in private hands for 83 yr makes one wonder if other meteorite falls may have experienced the same fate, thus possibly explaining the anomalously low number of falls reported in continental Spain in the 20th century.  相似文献   

Nocturnal offshore precipitation near the Mediterranean coast of the Iberian Peninsula     

Jordi Mazon  David Pino 《Meteorology and Atmospheric Physics》2013,120(1-2):11-28

While nocturnal offshore precipitation, which produces rain cells and bands, has been studied in tropical areas, few studies have analyzed the occurrence of this phenomenon at higher latitudes. Using radar reflectivity, nocturnal rainfall in the western Mediterranean area has been detected near the coast of the Iberian Peninsula and North Africa. More than 50 events have been recorded since 2009. MM5 mesoscale simulations of some of the recorded events allow us to establish that the most likely causes for these precipitation events are: (1) the interaction between cold air masses conducted by drainage and katabatic winds, and (2) a wetter and warmer synoptic wind. Two different episodes are presented: one in the northeastern Iberian Peninsula, caused by stratiform clouds, which occurred at the mouths of three rivers; the other case, produced by convective clouds, occurred at the southern Iberian Peninsula and was caused by the drainage winds flowing down from some mountain ranges located close to the coast.  相似文献   

Coastal inshore waters in the NW Mediterranean: Physicochemical and biological characterization and management implications     

Eva Flo  Esther Garcés  Marta Manzanera  Jordi Camp 《Estuarine, Coastal and Shelf Science》2011

The physicochemical and biological characteristics of coastal waters form a gradient extending from land to ocean. In the Mediterranean this gradient is particularly large, due to the sea’s weak tides. Within coastal waters, those waters in contact with land are called coastal inshore waters (CIW), defined herein as between 0 and 200 m from the shoreline. Here we present the first physicochemical and biological characterization of CIW of the NW Mediterranean Sea. This case study is based on 19 years of data collected from coastal inshore (CIW; 0–200 m), nearshore (CNW; 200–1500 m), and offshore (COW; >1500 m) waters of the Catalan coast. Analyses of these data showed that the physicochemical and biological characteristics of CIW differ significantly from those of CNW and COW due to: (1) significantly higher concentrations of dissolved inorganic nutrients (nitrate = 11.07 μM, nitrite = 0.52 μM, ammonium = 6.43 μM, phosphate = 0.92 μM, silicates = 5.99 μM) and chlorophyll-a (=2.42 μg/L) in CIW than in either CNW or COW (in some cases up to one order of magnitude); (2) a greater variability of dissolved inorganic nutrients and chlorophyll-a in CIW than in CNW and COW, and (3) the presence of a mostly urban population and the effects of river inflows as a primary source of CIW variability but with minimal impact on CNW or COW. In addition, the risk of eutrophication was found to be highest in CIW, placing human and environmental interests at greater risk than in the outermost coastal waters. The results highlight the importance of considering the distinctive physicochemical and biological properties of CIW in future coastal waters studies. This is of major importance in assessments of eutrophication and coastal water quality, not only to identify the pressure–impact relationships but also to allow the timely detection of local environmental problems and thus avoid endangering the unique communities of CIW and ensuring the sustainability of human activities. In conclusion, CIW characterization is essential to integrate coastal zone management.  相似文献   

The strength of cometary meteoroids: clues to the structure and evolution of comets   总被引：3，自引：0，他引：3  

Josep M. Trigo-Rodríguez  Jordi Llorca 《Monthly notices of the Royal Astronomical Society》2006,372(2):655-660

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