1,720,971 research outputs found
Paleomagnetismo del Grupo Santa Victoria en la sierra de Mojotoro, Salta: aportes a la reconstrucción paleogeográfica de Pampia en el Paleozoico Temprano
Estudios sedimentológicos, de magnetofábrica y paleomagnéticos fueron realizados en la Formación La Pedrera (Grupo Santa Victoria) de edad ordovícica temprana en la sierra de Mojotoro, provincia de Salta. Estos estudios tienen el objetivo de contribuir al conocimiento de la posición paleogeográfica del bloque de Pampia durante el Paleozoico temprano en relación al supercontinente de Gondwana. Se coleccionaron muestras orientadas en 12 sitios distribuidos en tres localidades. Estos afloramientos consisten en depósitos de plataforma media a proximal de composición principalmente cuarcítica. Los estudios de anisotropía de susceptibilidad magnética (AMS) sugieren una fábrica depositacional en una de las localidades, mientras que en las otras dos no se puede descartar una cierta influencia tectónica en la fábrica. El estudio paleomagnético permitió determinar una componente magnética característica portada por hematita en los 12 sitios. A partir del promedio de los polos geomagnéticos virtuales de cada sitio, se obtuvo un polo paleomagnético para el Grupo Santa Victoria en estas localidades que se ubica en 340,4°E 38,3°N A95=8,8°. La posición de este polo sugiere que ninguna de las tres localidades sufrió rotaciones tectónicas de significación por la orogenia andina o eventos anteriores. Sin embargo, presenta una paleolatitud algo más baja que la esperada según los polos de referencia de similar edad para el Gondwana. Ensayos de magnetizaciones isotérmicas direccionadas sugieren que esta diferencia no se debería a errores de inclinación por compactación. Por su parte, el polo del Grupo Santa Victoria discrepa con los polos obtenidos para el Grupo Mesón (Cámbrico medio a superior) y la Formación Santa Rosita (Ordovícico basal), al norte de la zona de estudio, pero en la misma región. Estas discrepancias se pueden adjudicar a la posible presencia de rotaciones tectónicas andinas según ejes verticales en las localidades ubicadas al norte de la zona de trabajo o bien indicar que el movimiento de Pampia a lo largo del margen del Cratón del Río de la Plata ya habría concluido o estaba próximo a concluir en el Ordovícico Temprano.Fil: Rodriguez Piceda Constanza. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Departamento de Ciencias Geológicas; Argentina. Instituto de Geociencias Básicas, Aplicadas y Ambientales de Buenos Aires; ArgentinaFil: Franceschinis, Pablo Reinaldo. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Geociencias Básicas, Aplicadas y Ambientales de Buenos Aires. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Geociencias Básicas, Aplicadas y Ambientales de Buenos Aires; ArgentinaFil: Escayola Mónica. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Universidad Nacional de Tierra del Fuego; ArgentinaFil: Rapalini Augusto. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Geociencias Básicas, Aplicadas y Ambientales de Buenos Aires. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Geociencias Básicas, Aplicadas y Ambientales de Buenos Aires; Argentin
Lithospheric-scale 3D model of the Southern Central Andes
The Central Andean orogeny is caused by the subduction of the Nazca oceanic plate beneath the South-American continental plate. In Particular, the Southern Central Andes (SCA, 27°-40°S) are characterized by a strong N-S and E-W variation in the crustal deformation style and intensity. Despite being the surface geology relatively well known, the information on the deep structure of the upper plate in terms of its thickness and density configurations is still scarcely constrained. Previous seismic studies have focused on the crustal structure of the northern part of the SCA (~27°-33°S) based upon 2D cross-sections, while 3D crustal models centred on the South-American or the Nazca Plate have been published with lower resolution. To gain insight into the present-day state of the lithosphere in the area, we derived a 3D model that is consistent with both the available geological and seismic data and with the observed gravity field. The model consists on a continental plate with sediments, a two-layer crust and the lithospheric mantle being subducted by an oceanic plate. The model extension covers an area of 700 km x 1100 km, including the orogen, the forearc and the forelandsFil: Rodriguez Piceda, Constanza. German Research Centre for Geosciences; AlemaniaFil: Scheck Wenderoth, Magdalena. German Research Centre for Geosciences; AlemaniaFil: Gómez Dacal, María Laura. German Research Centre for Geosciences; AlemaniaFil: Bott, Judith. German Research Centre for Geosciences; AlemaniaFil: Prezzi, Claudia Beatriz. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Geociencias Básicas, Aplicadas y Ambientales de Buenos Aires. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Geociencias Básicas, Aplicadas y Ambientales de Buenos Aires; ArgentinaFil: Strecker, Manfred. Universitat Potsdam; Alemani
Geología y paleomagnetismo del Grupo Santa Victoria en la Sierra de Mojotoro, provincia de Salta
Fil:Rodriguez Piceda, Constanza. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina
Thermomechanischer Zustand der südlichen Zentral Anden
The Andes are a ~7000 km long N-S trending mountain range developed along the South American western continental margin. Driven by the subduction of the oceanic Nazca plate beneath the continental South American plate, the formation of the northern and central parts of the orogen is a type case for a non-collisional orogeny. In the southern Central Andes (SCA, 29°S-39°S), the oceanic plate changes the subduction angle between 33°S and 35°S from almost horizontal (< 5° dip) in the north to a steeper angle (~30° dip) in the south. This sector of the Andes also displays remarkable along- and across- strike variations of the tectonic deformation patterns. These include a systematic decrease of topographic elevation, of crustal shortening and foreland and orogenic width, as well as an alternation of the foreland deformation style between thick-skinned and thin-skinned recorded along- and across the strike of the subduction zone. Moreover, the SCA are a very seismically active region. The continental plate is characterized by a relatively shallow seismicity (< 30 km depth) which is mainly focussed at the transition from the orogen to the lowland areas of the foreland and the forearc; in contrast, deeper seismicity occurs below the interiors of the northern foreland. Additionally, frequent seismicity is also recorded in the shallow parts of the oceanic plate and in a sector of the flat slab segment between 31°S and 33°S. The observed spatial heterogeneity in tectonic and seismic deformation in the SCA has been attributed to multiple causes, including variations in sediment thickness, the presence of inherited structures and changes in the subduction angle of the oceanic slab. However, there is no study that inquired the relationship between the long-term rheological configuration of the SCA and the spatial deformation patterns. Moreover, the effects of the density and thickness configuration of the continental plate and of variations in the slab dip angle in the rheological state of the lithosphere have been not thoroughly investigated yet. Since rheology depends on composition, pressure and temperature, a detailed characterization of the compositional, structural and thermal fields of the lithosphere is needed. Therefore, by using multiple geophysical approaches and data sources, I constructed the following 3D models of the SCA lithosphere: (i) a seismically-constrained structural and density model that was tested against the gravity field; (ii) a thermal model integrating the conversion of mantle shear-wave velocities to temperature with steady-state conductive calculations in the uppermost lithosphere (< 50 km depth), validated by temperature and heat-flow measurements; and (iii) a rheological model of the long-term lithospheric strength using as input the previously-generated models.
The results of this dissertation indicate that the present-day thermal and rheological fields of the SCA are controlled by different mechanisms at different depths. At shallow depths ( 50 km, largest temperatures variations occur where the descending slab is detected, which implies that the deep thermal field is mainly affected by the slab dip geometry.
The outcomes of this thesis suggests that long-term thermomechanical state of the lithosphere influences the spatial distribution of seismic deformation. Most of the seismicity within the continental plate occurs above the modelled transition from brittle to ductile conditions. Additionally, there is a spatial correlation between the location of these events and the transition from the mechanically strong domains of the forearc and foreland to the weak domain of the orogen. In contrast, seismicity within the oceanic plate is also detected where long-term ductile conditions are expected. I therefore analysed the possible influence of additional mechanisms triggering these earthquakes, including the compaction of sediments in the subduction interface and dehydration reactions in the slab. To that aim, I carried out a qualitative analysis of the state of hydration in the mantle using the ratio between compressional- and shear-wave velocity (vp/vs ratio) from a previous seismic tomography. The results from this analysis indicate that the majority of the seismicity spatially correlates with hydrated areas of the slab and overlying continental mantle, with the exception of the cluster within the flat slab segment. In this region, earthquakes are likely triggered by flexural processes where the slab changes from a flat to a steep subduction angle.
First-order variations in the observed tectonic patterns also seem to be influenced by the thermomechanical configuration of the lithosphere. The mechanically strong domains of the forearc and foreland, due to their resistance to deformation, display smaller amounts of shortening than the relatively weak orogenic domain. In addition, the structural and thermomechanical characteristics modelled in this dissertation confirm previous analyses from geodynamic models pointing to the control of the observed heterogeneities in the orogen and foreland deformation style. These characteristics include the lithospheric and crustal thickness, the presence of weak sediments and the variations in gravitational potential energy.
Specific conditions occur in the cold and strong northern foreland, which is characterized by active seismicity and thick-skinned structures, although the modelled crustal strength exceeds the typical values of externally-applied tectonic stresses. The additional mechanisms that could explain the strain localization in a region that should resist deformation are: (i) increased tectonic forces coming from the steepening of the slab and (ii) enhanced weakening along inherited structures from pre-Andean deformation events. Finally, the thermomechanical conditions of this sector of the foreland could be a key factor influencing the preservation of the flat subduction angle at these latitudes of the SCA.Die Anden sind eine ~7000 km lange N-S-verlaufende Hochgebirgskette, die entlang des westlichen südamerikanischen Kontinentalrandes entstanden ist. Aufgrund der Subduktion der ozeanischen Nazca-Platte unter die kontinentale südamerikanische Platte ist die Bildung des nördlichen und zentralen Teils des Gebirges typisch für eine nicht-kollisionale Orogenese. In den südlichen Zentralanden (SZA, 29-39° S) verändert sich der Subduktionswinkel der ozeanischen Platte zwischen 33 ° S und 35 ° S von fast horizontal (< 5° Einfallen) im Norden zu einem steileren Winkel (~ 30 ° Einfallen) im Süden. Begleitet wird dieser Trend von systematischen, Süd-gerichteten Abnahmen der topographischen Erhebung, der Krusteneinengung und der Vorland- und Orogenbreite, sowie von Variationen im Deformationsstil des Vorlandes, wo die Einengung des Deckgebirges in unterschiedlichem Maße von einer entsprechenden Deformation des Grundgebirges begleitet wird. . Darüber hinaus sind die SZA eine seismisch sehr aktive Region. Die Kontinentalplatte zeichnet sich durch eine relativ flache Seismizität (< 30 km Tiefe) aus, die sich hauptsächlich auf die Übergänge vom Orogen zu den Vorlandbereichen konzentriert; im Gegensatz dazu tritt tiefere Seismizität in den zentralen Bereichen des nördlichen Vorlandes auf. Darüber hinaus ist häufig auftretende Seismizität auch in den flachen Teilen der ozeanischen Platte und im Plattensegment mit flach einfallender Subduktion zwischen 31 ° S und 33 ° S festzustellen. Die beobachtete räumliche Heterogenität der tektonischen und seismischen Deformation in den SZA wurde auf mehrere Ursachen zurückgeführt, darunter Schwankungen der Sedimentmächtigkeit, das Vorhandensein vererbter Strukturen und Veränderungen des Subduktionswinkels der ozeanischen Platte. Es gibt jedoch bislang keine Studie, die den Zusammenhang zwischen der langfristigen rheologischen Konfiguration der SZA und den räumlichen Deformationsmustern untersucht hat. Darüber hinaus wurden die Auswirkungen der Dichte- und Mächtigkeitsvariationen in der kontinentalen Oberplatte und der verschiedenen Subduktionswinkel auf den rheologischen Zustand der Lithosphäre noch nicht grundlegend untersucht. Da die Rheologie von der Gesteinsart, dem Druck und der Temperatur abhängt, ist eine detaillierte Charakterisierung der Zusammensetzung, Struktur und des thermischen Feldes der Lithosphäre erforderlich. Daher habe ich unter Verwendung kombinierter Modellierungsansätze und geophysikalischer Daten die folgenden 3D Modelle für die Lithosphäre der SZA konstruiert: (i) ein auf seismischen Daten basierendes Struktur- und Dichtemodell, das anhand des beobachteten Schwerefeldes validiert wurde; (ii) ein thermisches Modell, das die Umwandlung von Mantelscherwellengeschwindigkeiten in Temperaturen mit Berechnungen des konduktiven Wärmetransports für stationäre Bedingungen in der obersten Lithosphäre (<50 km Tiefe) integriert und durch Temperatur- und Wärmeflussmessungen validiert wurde; und (iii) ein rheologisches Modell der langfristig bedingten Lithosphärenfestigkeit, das auf den zuvor erzeugten Modellen gründet.
Die Ergebnisse dieser Dissertation zeigen, dass die thermischen und rheologischen Bedingungen in den heutigen SZA durch verschiedene Mechanismen in unterschiedlichen Tiefen gesteuert werden. In flachen Tiefen ( 50 km treten die größten Temperaturschwankungen dort auf, wo die subduzierten Platte nachgewiesen wurde, was bedeutet, dass das tiefe thermische Feld den Subduktionswinkel gesteuert wird.
Die Ergebnisse dieser Doktorarbeit legen nahe, dass der langfristige thermomechanische Zustand der Lithosphäre die räumliche Verteilung rezenter Seismizität beeinflusst. Der größte Anteil innerhalb der Kontinentalplatte registrierter Erdbebentätigkeit tritt oberhalb des modellierten Übergangs von spröden zu duktilen Bedingungen auf. Außerdem besteht eine räumliche Korrelation zwischen Erdbebenclustern und den Übergängen von den mechanisch rigideren Vorlandbereichen (Forearc und Foreland) zum mechanisch schwächeren Orogen. Demgegenüber wird vermehrte Seismizität innerhalb der ozeanischen Platte auch dort nachgewiesen, wo entsprechend der Modellierung langfristig duktile Bedingungen erwartet werden. Ich habe daher den möglichen Einfluss zusätzlicher Mechanismen untersucht, die ein Auslösen dieser Erdbeben begünstigen könnten, darunter die Kompaktion von Sedimenten an der Subduktionsgrenzfläche und Dehydrationsreaktionen innerhalb der Platte. Dazu habe ich eine qualitative Analyse des Hydratationszustandes des Mantels unter Verwendung des Verhältnisses zwischen Kompressions- und Scherwellengeschwindigkeit (Vp/Vs-Verhältnis aus einemseismischen Tomographiemodell) durchgeführt. Die Ergebnisse dieser Analyse zeigen, dass der Großteil der Seismizität räumlich mit hydratisierten Bereichen in der subduzierten Platte und im darüber liegenden kontinentalen Mantel korreliert, mit Ausnahme eines Erdbebenclusters, das innerhalb des flachen Plattensegments auftritt. In diesem Bereich wechselt die subduzierte Platte von einem flachen in einen steilen Subduktionswinkel und Erdbeben werden wahrscheinlich durch Biegevorgänge in der Platte ausgelöst.
Auch die wichtigsten Variationen in den beobachteten tektonischen Mustern scheinen durch die thermomechanische Konfiguration der Lithosphäre beeinflusst zu sein. Die mechanisch starken Bereiche von Forearc und Foreland zeigen aufgrund ihrer Verformungsbeständigkeit geringere Verkürzungsraten als der relativ schwache Bereich des Orogens. Darüber hinaus bestätigen die in dieser Dissertation modellierten strukturellen und thermomechanischen Eigenschaften der Lithosphäre auch frühere Analysen geodynamischer Simulationen, denen zufolge der Deformationsstil im Orogen- und Vorlandbereich jeweils von Variationen in der Lithosphären- und Krustendicke, im Vorhandensein schwacher Sedimente und in der gravitativen potentiellen Energie kontrolliert wird.
Eine Sonderstellung nimmt der nordöstliche Vorlandbereich der SZA ein, wo eine verstärkte Seismizität und eine das Deck-und Grundgebirge erfassende Deformation zu beobachten sind, obwohl die modellierte Krustenfestigkeit dort Werte übersteigt, die für die in diesem Gebiet anzunehmenden tektonischen Spannungen typisch wären. . Mechanismen zur Lokalisierung verstärkter Deformation in einem Gebiet beitragen können, das nach den vorliegenden Modellen einer tektonischen Verformung widerstehen sollte, sind: (i) erhöhte tektonische Kräfte durch ein steileres Abtauchen der Platte und (ii) Schwächezonen in der Kruste, die auf prä-andine Deformationsereignisse zurückgehen. Schließlich könnten die thermomechanischen Bedingungen in diesem Teil des Vorlands einchlüsselfaktor für die Erhaltung des flachen Subduktionswinkels in diesen Breiten der SZA sein
Controls of the Lithospheric Thermal Field of an OceanContinent Subduction Zone: The Southern Central Andes
In an ocean-continent subduction zone, the assessment of the lithospheric thermal state is essential to determine the controls of the deformation within the upper plate and the dip angle of the subducting lithosphere. In this study, we evaluate the degree of influence of both the configuration of the upper plate (i.e., thickness and composition of the rock units) and variations of the subduction angle on the lithospheric thermal field of the southern Central Andes (29°–39°S). Here, the subduction angle increases from subhorizontal (5°) north of 33°S to steep (~30°) in the south. We derived the 3D temperature and heat flow distribution of the lithosphere in the southern Central Andes considering conversion of S wave tomography to temperatures together with steady-state conductive thermal modeling. We found that the orogen is overall warmer than the forearc and the foreland and that the lithosphere of the northern part of the foreland appears colder than its southern counterpart. Sedimentary blanketing and the thickness of the radiogenic crust exert the main control on the shallow thermal field (50 km, the temperatures of the overriding plate are mainly controlled by the mantle heat input and the subduction angle. The thermal field of the upper plate likely preserves the flat subduction angle and influences the spatial distribution of shortening.Fil: Rodriguez Piceda, Constanza. German Research Centre for Geosciences; AlemaniaFil: Scheck Wenderoth, Magdalena. German Research Centre for Geosciences; AlemaniaFil: Bott, Judith. German Research Centre for Geosciences; AlemaniaFil: Gómez Dacal, María Laura. German Research Centre for Geosciences; Alemania. Consejo Nacional de Investigaciones Científicas y Técnicas; ArgentinaFil: Cacace, M.. German Research Centre for Geosciences; AlemaniaFil: Pons, Michaël. German Research Centre for Geosciences; AlemaniaFil: Prezzi, Claudia Beatriz. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Geociencias Básicas, Aplicadas y Ambientales de Buenos Aires. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Geociencias Básicas, Aplicadas y Ambientales de Buenos Aires; ArgentinaFil: Strecker, Manfred. German Research Centre for Geosciences; Alemani
Lithospheric density structure of the southern Central Andes constrained by 3D data-integrative gravity modelling
The southern Central Andes (SCA) (between 27° S and 40° S) is bordered to the west by the convergent margin between the continental South American Plate and the oceanic Nazca Plate. The subduction angle along this margin is variable, as is the deformation of the upper plate. Between 33° S and 35° S, the subduction angle of the Nazca plate increases from sub-horizontal (< 5°) in the north to relatively steep (~ 30°) in the south. The SCA contain inherited lithological and structural heterogeneities within the crust that have been reactivated and overprinted since the onset of subduction and associated Cenozoic deformation within the Andean orogen. The distribution of the deformation within the SCA has often been attributed to the variations in the subduction angle and the reactivation of these inherited heterogeneities. However, the possible influence that the thickness and composition of the continental crust have had on both short-term and long-term deformation of the SCA is yet to be thoroughly investigated. For our investigations, we have derived density distributions and thicknesses for various layers that make up the lithosphere and evaluated their relationships with tectonic events that occurred over the history of the Andean orogeny and, in particular, investigated the short- and long-term nature of the present-day deformation processes. We established a 3D model of lithosphere beneath the orogen and its foreland (29° S–39° S) that is consistent with currently available geological and geophysical data, including the gravity data. The modelled crustal configuration and density distribution reveal spatial relationships with different tectonic domains: the crystalline crust in the orogen (the magmatic arc and the main orogenic wedge) is thicker (~ 55 km) and less dense (~ 2900 kg/m3) than in the forearc (~ 35 km, ~ 2975 kg/m3) and foreland (~ 30 km, ~ 3000 kg/m3). Crustal thickening in the orogen probably occurred as a result of stacking of low-density domains, while density and thickness variations beneath the forearc and foreland most likely reflect differences in the tectonic evolution of each area following crustal accretion. No clear spatial relationship exists between the density distribution within the lithosphere and previously proposed boundaries of crustal terranes accreted during the early Paleozoic. Areas with ongoing deformation show a spatial correlation with those areas that have the highest topographic gradients and where there are abrupt changes in the average crustal-density contrast. This suggests that the short-term deformation within the interior of the Andean orogen and its foreland is fundamentally influenced by the crustal composition and the relative thickness of different crustal layers. A thicker, denser, and potentially stronger lithosphere beneath the northern part of the SCA foreland is interpreted to have favoured a strong coupling between the Nazca and South American plates, facilitating the development of a sub-horizontal slab.Fil: Rodriguez Piceda, Constanza. German Research Centre for Geosciences; Alemania. Universitat Potsdam; AlemaniaFil: Scheck Wenderoth, Magdalena. German Research Centre for Geosciences; Alemania. RWTH Aachen University; AlemaniaFil: Gómez Dacal, María Laura. German Research Centre for Geosciences; Alemania. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata; ArgentinaFil: Bott, Judith. German Research Centre for Geosciences; AlemaniaFil: Prezzi, Claudia Beatriz. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Geociencias Básicas, Aplicadas y Ambientales de Buenos Aires. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Geociencias Básicas, Aplicadas y Ambientales de Buenos Aires; ArgentinaFil: Strecker, Manfred R.. German Research Centre for Geosciences; Alemania. Universitat Potsdam; Alemani
3D thermal model of the southern Central Andes
The Central Andean orogen formed as a result of the subduction of the oceanic Nazca plate beneath the continental South-American plate. In the southern segment of the Central Andes (SCA, 29°S-39°S), the oceanic plate subducts beneath the continental plate with distinct dip angles from north to south. Subduction geometry, tectonic deformation, and seismicity at this plate boundary are closely related to lithospheric temperature distribution in the upper plate. Previous studies provided insights into the present-day thermal field with focus on the surface heat flow distribution in the orogen or through modelling of the seismic velocity distribution in restricted regions of the SCA as indirect proxy of the deep thermal field. Despite these recent advances, the information on the temperature distribution at depth of the SCA lithosphere remains scarcely constrained.
To gain insight into the present-day thermal state of the lithosphere in the region, we derived the 3D lithospheric temperature distribution from inversion of S-wave velocity to temperature and calculations of the steady state thermal field. The configuration of the region – concerning both, the heterogeneity of the lithosphere and the slab dip – was accounted for by incorporating a 3D data-constrained structural and density model of the SCA into the workflow (Rodriguez Piceda et al. 2020a-b). The model consists on a continental plate with sediments, a two-layer crust and the lithospheric mantle being subducted by an oceanic plate. The model extension covers an area of 700 km x 1100 km, including the orogen (i.e. magmatic arc, main orogenic wedge), the forearc and the foreland, and it extents down to 200 km depth.Fil: Rodriguez Piceda, Constanza. German Research Centre for Geosciences; AlemaniaFil: Sheck Wenderoth, Magdalena. German Research Centre for Geosciences; AlemaniaFil: Bott, Judith. German Research Centre for Geosciences; AlemaniaFil: Gómez Dacal, María Laura. German Research Centre for Geosciences; AlemaniaFil: Pons, Michael. German Research Centre for Geosciences; AlemaniaFil: Prezzi, Claudia Beatriz. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Geociencias Básicas, Aplicadas y Ambientales de Buenos Aires. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Geociencias Básicas, Aplicadas y Ambientales de Buenos Aires; ArgentinaFil: Strecker, Manfred Reinhard Karl. Universitat Potsdam; Alemani
Going Beyond Counting First Authors in Author Co-citation Analysis
The present study examines one of the fundamental aspects of author co-citation analysis (ACA) - the way co-citation
counts are defined. Co-citation counting provides the data on which all subsequent statistical analyses and mappings
are based, and we compare ACA results based on two different types of co-citation counting - the traditional type that
only counts the first one among a cited work's authors on the one hand and a non-traditional type that takes into
account the first 5 authors of a cited work on the other hand. Results indicate that the picture produced through this non-traditional author co-citation counting contains more coherent author groups and is therefore considerably clearer. However, this picture represents fewer specialties in the research field being studied than that produced through the traditional first-author co-citation counting when the same number of top-ranked authors is selected and analyzed. Reasons for these effects are discussed
Variations on the Author
“Variations on the Author” discusses two of Eduardo Coutinho’s recent films (Um Dia na Vida, from 2010, and Últimas Conversas, posthumously released in 2015) and their contribution to the general question of documentary authorship. The director’s filmography is characterized by a consistent yet self-effacing form of authorial self-inscription: Coutinho often features as an interviewer that rather than express opinions propels discourses; an interviewer that is good at listening. This mode of self-inscription characterizes him as an author who is not expressive but who is nonetheless markedly present on the screen. In Um Dia na Vida, however, Coutinho is completely absent form the image, while Últimas Conversas, on the contrary, includes a confessional prologue that moves the director from the margins to the center of his films. This article examines the ways in which these works stand out in the filmography of a director who offers new insights into the notion of cinematic authorship
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