The structure of the eastern border of the Andes in north-western Argentina     

Dr. Ricardo Mon 《International Journal of Earth Sciences》1976,65(1):211-222

In the eastern border area of the Andes of north-western Argentina two structural units are represented: the Cordillera Oriental and the Sierras Subandinas.The Cordillera Oriental represents a structural unit of faulted blocks strongly uplifted in relation to the Sierras Subandinas. In the Cordillera Oriental, the metamorphic basement has been partially folded together with the sedimentary cover. In some cases the cover has been detached away from its substratum and folded independently of it.It was generally accepted that the Sierras Subandinas coincide with big asymmetrical anticlines produced in the cover rocks by tilting of rigid basement blocks. The detailed geological mapping of the region situated between the parallels 24° 45 and 26° latitude south and the meridians 64° 30 and 66° west has provided data that permit to modify considerably this scheme.The existence of important strike-slip faults running highly oblique to the main regional structural pattern and controlling the shape of the Sierras Subandinas folds has been verified. These highly oblique faults with strike-slip movements, that affect the whole region, are probably ancient lineaments reactivated during Andean diastrophism in Upper Pliocene to Early Pleistocene time.

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Zusammenfassung Im östlichen Grenzgebiet der Anden im nordwestlichen Argentinien liegen zwei strukturell unterschiedliche Einheiten vor, die Cordillera Oriental und die subandinen Sierren (Sierras Subandinas).Die Cordillera Oriental besteht aus Leistenschollen eines leicht metamorphisierten Sockels. Sie ist als Ganzes im Verhältnis zu den subandinen Sierren stark herausgehoben worden. In der Cordillera Oriental wurde dieser Sockel zum Teil zusammen mit seinen sedimentären Deckschichten verfaltet, zum Teil wurden sie aber auch von ihrem Unterlager abgeschert und unabhängig von ihm gefaltet.Bisher wurde allgemein angenommen, daß die subandinen Sierren aus großen assymmetrischen Falten aufgebaut werden, die in den Deckschichten durch Kippung starrer Blöcke im tieferen Untergrund hervorgerufen wurden. Die genaue geokartographische Aufnahme eines Gebietes zwischen den Breitenkreisen 24° 45 und 26° südl. Breite und den Längenkreisen 64° 30 und 66° westl. Länge erbrachte Daten, die es erlauben, diese Vorstellung erheblich zu modifizieren.Weit durchhaltende Seitenverschiebungen, die die übergeordneten Strukturen des gesamten Gebietes schräg durchziehen und die Gestalt der Falten in den Sierren erheblich beeinflussen, wurden nachgewiesen. Sie stellen wahrscheinlich alte, präandine Lineamente dar, die während der Anden-Orogenese im Jungtertiär bis Altpleistozän reaktiviert Wurden.

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Resumen En el borde oriental de los Andes del Noroeste Argentino están representadas dos unidades estructurales: la Cordillera Oriental y las Sierras Subandinas.La Cordillera Oriental es una unidad constituida por bloques fallados y, en conjunto, elevada con respecto a las Sierras Subandinas. En la Cordillera Oriental el basamento metamórfico ha sido parcialmente plegado junto con la cobertura sedimentaria. En algunos casos lo cobertura ha sido despegada de su substrato y plegada independientemente.En general se aceptaba que las Sierras Subandinas coincidian con grandes anticlinales asimétricos producidos en la cobertura sedimentaria por el basculamiento de bloques rígidos de basamento situados en el subsuelo. La cartografía geológica-estructural detallada de la región comprendida por los paralelos 24° 45 y 26° S y los meridianos 64° 30 y 66° W ha proporcionado datos que permiten modificar considerablemente este esquema.Se ha comprobado la existencia de importantes fallas transcurrentes, fuertemente oblicuas con respecto a la estructura regional, que han tenido profunda influencia sobre la forma de los pliegues subandinos. Estas fallas oblicuas son probablemente lineamientos antiguos en los que el diastrofismo Andico (Plioceno-Pleistoceno) ha producido considerables desplazamientos paralelos al rumbo de los mismos.

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Résumé Dans la bordure orientale des Andes du Nord-ouest de l'Argentine, deux unités structurales différentes sont présentes: les Sierras subandines et la Cordillère orientale.La Cordillère orientale est composée d'un socle faiblement métamorphique faillé en blocs fortement surélevés par rapport aux Sierras subandines. Dans la Cordillère orientale, ce socle métamorphique a été en partie plissé avec sa couverture sédimentaire; mais parfois celle-ci a été décolée de son substratum et plissé indépendentement.Jusqu'à présent, on admettait que les Sierras subandines sont constituées de grands anticlinaux assymétriques produits dans la couverture par l'ascension de blocs faillés du socle. La cartographie géologico-structurale detaillée de la région comprise entre les parallèles 24° 45 et 26° de latitude sud et les méridiens 64° 30 et 60° ouest conduit à modifier considérablement ce schéma.D'importants décrochements très obliques par rapport à la direction de la structure régionale et qui ont fortement influencé la forme des plis subandins sont probablement des accidents anciens rajeunis pendant le diastrophisme andin au cours du Pliocène supérieur et du Pléistocène inférieur.

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The continental record of Ediacaran volcano‐sedimentary successions in southern Brazil and their global implications     

Liliane Janikian  Renato Paes De Almeida  Ricardo Ivan Ferreira Da Trindade  Antonio Romalino Santos Fragoso‐Cesar  Manoel Souza D′Agrella‐Filho  Elton Luis Dantas  Eric Tohver 《地学学报》2008,20(4):259-266

The Ediacaran is one of the most important periods on Earth evolution, including the first appearance of soft‐bodied macrofossils, major climatic changes and a supposed rise in free oxygen. In southernmost Brazil, this period is represented by Camaquã Supergroup, including the Bom Jardim Group and the Acampamento Velho Formation, both of which record continental palaeoenvironmental changes in a more than 5000 m thick stratigraphic succession. Age constraints are given by seven Ar‐Ar and U‐Pb determinations on volcanic rocks, which bracket these units between c. 605 and 574 Ma, revealing the best dated and most continuous documented Ediacaran continental succession to date. Depositional systems evolution supports a Phanerozoic‐type glacial context during the last Neoproterozoic glacial event and presents the Picada das Graças Formation (580 ± 3.6 Ma) as the first dated non‐glacial unit coeval to the Gaskiers Formation.  相似文献   

Direct dating of the Sete Lagoas cap carbonate (Bambuí Group,Brazil) and implications for the Neoproterozoic glacial events     

Marly Babinski  Lucieth Cruz Vieira  Ricardo I. F. Trindade 《地学学报》2007,19(6):401-406

The end of the Neoproterozoic is punctuated by glacial deposition, but the chronology of these deposits is hindered presently by the paucity of geochronological data. Here, we present new radiometric dating for the basal Sete Lagoas cap carbonate deposits that overlie glacial units in the São Francisco craton. Six samples from aragonite‐pseudomorph crystal‐rich facies, showing pristine textures and constant ⁸⁷Sr/⁸⁶Sr ratios around 0.7075, yielded a Pb–Pb isochron age of 740 ± 22 Ma, which is interpreted as the depositional age for these remarkably preserved rocks. This age can be used to infer a low‐to‐moderate palaeolatitude of 20–30° for carbonate (and glacial) deposition. In addition, as it overlaps the ages obtained for the oldest Neoproterozoic glacial successions, our result reinforces the idea of a long‐standing ‘Sturtian’ interval, suggesting that this event represents either different discrete glaciations or a protracted event encompassing almost 80 Ma.  相似文献   

Concurrent imaging of chlorophyll fluorescence,Chlorophyll a content and green fluorescent proteins‐like proteins of symbiotic cnidarians          下载免费PDF全文

Miguel Costa Leal  Bruno Jesus  João Ezequiel  Ricardo Calado  Rui Jorge Miranda Rocha  Paulo Cartaxana  João Serôdio 《Marine Ecology》2015,36(3):572-584

Research on photosynthetic cnidarians has been mainly focused on the symbiosis established between the cnidarian host and its dinoflagellates endosymbionts from genus Symbiodinium. Despite the potential of imaging techniques for assessing the spatial distribution of key parameters of cnidarian photobiology, such as photochemical activity, chlorophyll a content or green fluorescent proteins (GFPs), to our best knowledge, no study has ever attempted to simultaneous map these three features. In this study, we developed a modified imaging pulse amplitude fluorometer by applying excitation light of different wavelengths and selectively detecting short spectral bands through bandpass filters. The imaging system was used to sequentially excite and quantify chlorophyll variable fluorescence (maximum quantum yield of photosystem II, F_v/F_m), Chl a content (normalized difference vegetation index) and relative content of GFPs. The spatial distribution of these photophysiological parameters was mapped both horizontally, across the surface of the soft corals Sarcophyton cf. glaucum and Sinularia flexibilis and the zoanthid Protopalythoa sp., and vertically, throughout a vertical section of S. cf. glaucum. Results showed bleached areas within each individual coral colony and registered photophysiological changes with S. cf. glaucum tissue depth. Analysis of Protopalythoa sp. polyps’ expansion revealed differential surface patterns of NDVI and GFP concentration, and a negative relation between these latter parameters within each polyp. This novel non‐invasive approach allowed a high‐resolution characterization of the spatial relationship between these key parameters through the analysis of image information on a pixel‐by‐pixel basis, which has great potential for investigating the physiological state of symbiotic associations.  相似文献   

Nocturnal isoprene declines in a semi-urban environment     

David Doughty  Jose D. Fuentes  Ricardo Sakai  Xiao-Ming Hu  Kevin Sanchez 《Journal of Atmospheric Chemistry》2015,72(3-4):215-234

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Trends and correlations in annual extreme precipitation indices for mainland Portugal, 1941–2007     

M. Isabel P. de Lima  Fátima Espírito Santo  Alexandre M. Ramos  Ricardo M. Trigo 《Theoretical and Applied Climatology》2015,119(1-2):55-75

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Meteorites at Meridiani Planum provide evidence for significant amounts of surface and near‐surface water on early Mars     

Alberto G. FAIRÉN  James M. DOHM  Victor R. BAKER  Shane D. THOMPSON  William C. MAHANEY  Kenneth E. HERKENHOFF  J. Alexis P. RODRÍGUEZ  Alfonso F. DAVILA  Dirk SCHULZE‐MAKUCH  M. Ramy EL MAARRY  Esther R. UCEDA  Ricardo AMILS  Hirdy MIYAMOTO  Kyeong J. KIM  Robert C. ANDERSON  Christopher P. McKAY 《Meteoritics & planetary science》2011,46(12):1832-1841

Abstract– Six large iron meteorites have been discovered in the Meridiani Planum region of Mars by the Mars Exploration Rover Opportunity in a nearly 25 km‐long traverse. Herein, we review and synthesize the available data to propose that the discovery and characteristics of the six meteorites could be explained as the result of their impact into a soft and wet surface, sometime during the Noachian or the Hesperian, subsequently to be exposed at the Martian surface through differential erosion. As recorded by its sediments and chemical deposits, Meridiani has been interpreted to have undergone a watery past, including a shallow sea, a playa, an environment of fluctuating ground water, and/or an icy landscape. Meteorites could have been encased upon impact and/or subsequently buried, and kept underground for a long time, shielded from the atmosphere. The meteorites apparently underwent significant chemical weathering due to aqueous alteration, as indicated by cavernous features that suggest differential acidic corrosion removing less resistant material and softer inclusions. During the Amazonian, the almost complete disappearance of surface water and desiccation of the landscape, followed by induration of the sediments and subsequent differential erosion and degradation of Meridiani sediments, including at least 10–80 m of deflation in the last 3–3.5 Gy, would have exposed the buried meteorites. We conclude that the iron meteorites support the hypothesis that Mars once had a denser atmosphere and considerable amounts of water and/or water ice at and/or near the surface.  相似文献   

Comparisons of ocean scatterometer and anemometer winds off the southwestern Iberian Peninsula     

Ricardo F. Sánchez  Paulo Relvas  Henrique O. Pires 《Continental Shelf Research》2007

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Stramonita haemastoma as a bioindicator for organotin contamination in coastal environments     

Limaverde AM  Wagener Ade L  Fernandez MA  Scofield Ade L  Coutinho R 《Marine environmental research》2007,64(3):384-398

Stramonita haemastoma was investigated as a suitable bioindicator of TBT and TPhT contamination in the tropical Atlantic Ocean by: 1. Imposex induction in healthy females after inoculation with TBT and TPhT in the laboratory; and 2. Determining incidence of imposex in S. haemastoma collected from areas with various levels of tributyltin (TBT) and triphenyltin (TPhT) and determining the concentrations of these chemical in its tissues and that of its prey, the mussell Perna pernas. Imposex intensities and organotin concentrations in tissues showed good correlation, indicating S. haemastoma as a reliable bioindicator of TBT and TPhT contamination in coastal waters. Body burden threshold of TBT and TPhT for imposex induction was estimated to be 10-20 ng g(-1).  相似文献   

Miscible transfer of solute in different model fractures: From random to multiscale wall roughness     

Harold Auradou  Alejandro Boschan  Ricardo Chertcoff  Maria-Veronica D’Angelo  Jean-Pierre Hulin  Irene Ippolito 《Comptes Rendus Geoscience》2010,342(7-8):644-652

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