Potential vorticity and moisture in extratropical cyclones : climatology and sensitivity experiments

The development of extratropical cyclones can be seen as an interplay of three positive potential vorticity (PV) anomalies: an upper-level stratospheric intrusion, low-tropospheric diabatically produced PV, and a warm anomaly at the surface acting as a surrogate PV anomaly. In the mature stage they become vertically aligned and form a “PV tower” associated with strong cyclonic circulation. This paradigm of extratropical cyclone development provides the basis of this thesis, which will use a climatological dataset and numerical model experiments to investigate the amplitude of the three anomalies and the processes leading in particular to the formation of the diabatically produced low-tropospheric PV anomaly.rnrnThe first part of this study, based on the interim ECMWF Re-Analysis (ERA-Interim) dataset, quantifies the amplitude of the three PV anomalies in mature extratropical cyclones in different regions in the Northern Hemisphere on a climatological basis. A tracking algorithm is applied to sea level pressure (SLP) fields to identify cyclone tracks. Surface potential temperature anomalies ∆θ and vertical profiles of PV anomalies ∆PV are calculated at the time of the cyclones’ minimum SLP and during the intensification phase 24 hours before in a vertical cylinder with a radius of 200 km around the surface cyclone center. To compare the characteristics of the cyclones, they are grouped according to their location (8 regions) and intensity, where the central SLP is used as a measure of intensity. Composites of ∆PV profiles and ∆θ are calculated for each region and intensity class at the time of minimum SLP and during the cyclone intensification phase.rnrnDuring the cyclones’ development stage the amplitudes of all three anomalies increase on average. In the mature stage all three anomalies are typically larger for intense than for weak winter cyclones [e.g., 0.6 versus 0.2 potential vorticity units (PVU) at lower levels, and 1.5 versus 0.5 PVU at upper levels].rnThe regional variability of the cyclones’ vertical structure and the profile evolution is prominent (cyclones in some regions are more sensitive to the amplitude of a particular anomaly than in other regions). Values of ∆θ and low-level ∆PV are on average larger in the western parts of the oceans than in the eastern parts. In addition, a large seasonal variability can be identified, with fewer and weaker cyclones especially in the summer, associated with higher low-tropospheric PV values, but also with a higher tropopause and much weaker surface potential temperature anomalies (compared to winter cyclones).rnrnIn the second part, we were interested in the diabatic low-level part of PV towers. Evaporative sources were identified of moisture that was involved in PV production through condensation. Lagrangian backward trajectories were calculated from the region with high PV values at low-levels in the cyclones. PV production regions were identified along these trajectories and from these regions a new set of backward trajectories was calculated and moisture uptakes were traced along them. The main contribution from surface evaporation to the specific humidity of the trajectories is collected 12-72 hours prior to therntime of PV production. The uptake region for weaker cyclones with less PV in the centre is typically more localized with reduced uptake values compared to intense cyclones. However, in a qualitative sense uptakes and other variables along single trajectories do not vary much between cyclones of different intensity in different regions.rnrnA sensitivity study with the COSMO model comprises the last part of this work. The study aims at investigating the influence of synthetic moisture modification in the cyclone environment in different stages of its development. Moisture was eliminated in three regions, which were identified as important moisture source regions for PV production. Moisture suppression affected the cyclone the most in its early phase. It led to cyclolysis shortly after its genesis. Nevertheles, a new cyclone formed on the other side of a dry box and developed relatively quickly. Also in other experiments, moisture elimination led to strong intensity reduction of the surface cyclone, limited upper-level development, and delayed or missing interaction between the two.rnrnIn summary, this thesis provides novel insight into the structure of different intensity categories of extratropical cyclones from a PV perspective, which corroborates the findings from a series of previous case studies. It reveals that all three PV anomalies are typically enhanced for more intense cyclones, with important regional differences concerning the relative amplitude of the three anomalies. The moisture source analysis is the first of this kind to study the evaporation-condensation cycle related to the intensification of extratropical cyclones. Interestingly, most of the evaporation occurs during the 3 days prior to the time of maximum cyclone intensity and typically extends over fairly large areas along the track of the cyclone. The numerical model case study complements this analysis by analyzing the impact of regionally confined moisture sources for the evolution of the cyclone.

Molekulardynamik-Simulationen supramolekularer Komplexe unter Einfluss einer externen Kraft

Supramolekulare Komplexe werden durch nichtkovalente Bindungen stabilisiert. Legt man eine externe Kraft an einen solchen Komplex an, ist es möglich, diese Bindungen zu öffnen. Anhand der dafür benötigten Kraft läßt sich die Stabilität des Komplexes bestimmen. Im Rahmen dieser Arbeit wurden zwei supramolekulare Komplexe, die unterschiedliche Arten von nichtkovalenten Bindungen enthalten, mit Hilfe von Molekulardynamik (MD) Simulationen untersucht. In beiden Fällen wurden die relevanten Bindungsstrukturen und deren Stabilität ermittelt.rnZum einen wurden zwei synthetische Calix[4]aren-Catenan-Dimersysteme betrachtet, in denen die beiden Monomere über Wasserstoffbrückenbindungen aneinander gebunden sind. Die Besonderheit dieser Komplexe ist, dass die Monomere aufgrund von verschlauften Alkylketten (Catenan-Struktur) nicht vollständig voneinander getrennt werden können. In Abhängigkeit der Länge derrnAlkylketten findet man für die beiden Komplexe eine unterschiedliche Zahl von relevanten Bindungsstrukturen (Zustände). Für ein System mit relativ kurzen Alkylketten findet man zwei Zustände, eine kompakte Struktur, die auch im Gleichgewicht beobachtet wird und eine gestreckte Struktur, die nur unter dem Einfluss der externen Kraft stabil ist. Verlängert man die Alkylketten,rnbeobachtet man einen weiteren Zustand, in dem das Dimer vollständig gestreckt ist und die Monomere eine größere Separation aufweisen.rnBei dem zweiten System, das untersucht wurde, handelte es sich um einen Carbohydrat-Kation-Carbohydrat Komplex, der für die Selbstadhäsion von Meeresschwämmen eine wichtige Rolle spielt. Experimentell ist bekannt, dass sich dieser Komplex zwar mit Calciumionen, nicht aber mit Magnesiumionen bildet. Im Rahmen dieser Arbeit wurde gezeigt, dass die wesentlichen Unterschiede der beiden Kationarten in Bezug auf die Komplexbildung auf den kleineren Ionenradius des Magnesiumions zurückzuführen sind. Aufgrund des kleineren Radius bindet ein solvatisiertes Magnesiumion die Hydrathülle stärker und die Komplexbindung wird kinetisch gehemmt. Zum anderen bindet im Magnesiumkomplex nur eines der beiden Carbohydrate direkt an das Kation.rnDas andere Carbohydrat bindet nur indirekt über ein Wassermolekül an das Kation. Da diese indirekte Bindung gegenüber einer direkten Bindung schwächer ist, weist der Magensiumkomplex eine geringere Stabilität auf als ein vergleichbarer Calciumkomplex.rnDes Weiteren wurde untersucht, inwieweit die Ergebnisse von MD Simulationen vom verwendeten Modell (Kraftfeld) abhängen. Allgemein ist bekannt, dass die Ergebnisse von Gleichgewichtssimulationen kraftfeldabhängig sind. Im Rahmen diese Arbeit konnte gezeigt werden, dass sich für Zugsimulationen, in denen eine externe Kraft an das System angelegt wird, eine ähnliche Kraftfeldabhängigkeit ergibt. Da sich die Unterschiede der Ergebnisse auf Unterschiede in den Gleichgewichtssimulationen zurückführen lassen, kann man annehmen, dass die externe Kraft keine zusätzliche Einschränkung in Bezug auf die Zuverlässigkeit der Kraftfelder darstellt.rnAbgesehen von den MD Simulationen wurde eine in der Literatur beschriebene Methode zur Analyse von Zweizustandssystemen unter dem Einfluss einer konstanten externen Kraft erweitert. Ein Komplex läßt sich als Zweizustandssystem beschreiben, wenn dieser zwei relevante Bindungsstrukturen aufweist. Wird an solch einen Komplex eine konstante Kraft angelegt, lassen sich Übergänge zwischen den beiden Zuständen beobachten. Ist das System weit entfernt vom Gleichgewicht, kann es problematisch sein, einen der beiden Übergänge vollständig aufzulösen. In diesen Fällen wird nun vorgeschlagen, die beiden Übergänge zu einem sogenannten Kreisübergang zusammen zu fassen und diese zu zählen. Bestimmt man die Zahl der Übergänge pro Zeit in Abhängigkeit der angelegten Kraft, können die Übergangsraten bestimmt werden. Um die Methode zu validieren wurden kinetische Monte-Carlo Simulationen durchgeführt. Es zeigt sich, dass schon mit relativ kleinen Datensätzen gute Ergebnisse erzielt werden können.

Dr. Ralph Garber (Canada), President 1988 - 1996

A fully revealing portrait of Ralph Garber would require a latter-day Boswell. As ordained, however, an attempt must be made to create a recognizable word picture. And it must give initial attention to the range of influences and factors in Ralph Garber's inheritance and environment that, throughout his life, he experienced, absorbed and utilized in his remarkably creative career.

Planet formation models: the interplay with the planetesimal disc

Context. According to the sequential accretion model (or core-nucleated accretion model), giant planet formation is based first on the formation of a solid core which, when massive enough, can gravitationally bind gas from the nebula to form the envelope. The most critical part of the model is the formation time of the core: to trigger the accretion of gas, the core has to grow up to several Earth masses before the gas component of the protoplanetary disc dissipates. Aims: We calculate planetary formation models including a detailed description of the dynamics of the planetesimal disc, taking into account both gas drag and excitation of forming planets. Methods: We computed the formation of planets, considering the oligarchic regime for the growth of the solid core. Embryos growing in the disc stir their neighbour planetesimals, exciting their relative velocities, which makes accretion more difficult. Here we introduce a more realistic treatment for the evolution of planetesimals' relative velocities, which directly impact on the formation timescale. For this, we computed the excitation state of planetesimals, as a result of stirring by forming planets, and gas-solid interactions. Results: We find that the formation of giant planets is favoured by the accretion of small planetesimals, as their random velocities are more easily damped by the gas drag of the nebula. Moreover, the capture radius of a protoplanet with a (tiny) envelope is also larger for small planetesimals. However, planets migrate as a result of disc-planet angular momentum exchange, with important consequences for their survival: due to the slow growth of a protoplanet in the oligarchic regime, rapid inward type I migration has important implications on intermediate-mass planets that have not yet started their runaway accretion phase of gas. Most of these planets are lost in the central star. Surviving planets have masses either below 10 M⊕ or above several Jupiter masses. Conclusions: To form giant planets before the dissipation of the disc, small planetesimals (~0.1 km) have to be the major contributors of the solid accretion process. However, the combination of oligarchic growth and fast inward migration leads to the absence of intermediate-mass planets. Other processes must therefore be at work to explain the population of extrasolar planets that are presently known.

A Compensating Anastigmatic Submillimeter Array Imaging System for STEAMR

In this paper, we present a novel technique for the removal of astigmatism in submillimeter-wave optical systems through employment of a specific combination of so-called astigmatic off-axis reflectors. This technique treats an orthogonally astigmatic beam using skew Gaussian beam analysis, from which an anastigmatic imaging network is derived. The resultant beam is considered truly stigmatic, with all Gaussian beam parameters in the orthogonal directions being matched. This is thus considered an improvement over previous techniques wherein a beam corrected for astigmatism has only the orthogonal beam amplitude radii matched, with phase shift and phase radius of curvature not considered. This technique is computationally efficient, negating the requirement for computationally intensive numerical analysis of shaped reflector surfaces. The required optical surfaces are also relatively simple to implement compared to such numerically optimized shaped surfaces. This technique is implemented in this work as part of the complete optics train for the STEAMR antenna. The STEAMR instrument is envisaged as a mutli-beam limb sounding instrument operating at submillimeter wavelengths. The antenna optics arrangement for this instrument uses multiple off-axis reflectors to control the incident radiation and couple them to their corresponding receiver feeds. An anastigmatic imaging network is successfully implemented into an optical model of this antenna, and the resultant design ensures optimal imaging of the beams to the corresponding feed horns. This example also addresses the challenges of imaging in multi-beam antenna systems.

EChO

A dedicated mission to investigate exoplanetary atmospheres represents a major milestone in our quest to understand our place in the universe by placing our Solar System in context and by addressing the suitability of planets for the presence of life. EChO—the Exoplanet Characterisation Observatory—is a mission concept specifically geared for this purpose. EChO will provide simultaneous, multi-wavelength spectroscopic observations on a stable platform that will allow very long exposures. The use of passive cooling, few moving parts and well established technology gives a low-risk and potentially long-lived mission. EChO will build on observations by Hubble, Spitzer and ground-based telescopes, which discovered the first molecules and atoms in exoplanetary atmospheres. However, EChO’s configuration and specifications are designed to study a number of systems in a consistent manner that will eliminate the ambiguities affecting prior observations. EChO will simultaneously observe a broad enough spectral region—from the visible to the mid-infrared—to constrain from one single spectrum the temperature structure of the atmosphere, the abundances of the major carbon and oxygen bearing species, the expected photochemically-produced species and magnetospheric signatures. The spectral range and resolution are tailored to separate bands belonging to up to 30 molecules and retrieve the composition and temperature structure of planetary atmospheres. The target list for EChO includes planets ranging from Jupiter-sized with equilibrium temperatures T eq up to 2,000 K, to those of a few Earth masses, with T eq \u223c 300 K. The list will include planets with no Solar System analog, such as the recently discovered planets GJ1214b, whose density lies between that of terrestrial and gaseous planets, or the rocky-iron planet 55 Cnc e, with day-side temperature close to 3,000 K. As the number of detected exoplanets is growing rapidly each year, and the mass and radius of those detected steadily decreases, the target list will be constantly adjusted to include the most interesting systems. We have baselined a dispersive spectrograph design covering continuously the 0.4–16 μm spectral range in 6 channels (1 in the visible, 5 in the InfraRed), which allows the spectral resolution to be adapted from several tens to several hundreds, depending on the target brightness. The instrument will be mounted behind a 1.5 m class telescope, passively cooled to 50 K, with the instrument structure and optics passively cooled to \u223c45 K. EChO will be placed in a grand halo orbit around L2. This orbit, in combination with an optimised thermal shield design, provides a highly stable thermal environment and a high degree of visibility of the sky to observe repeatedly several tens of targets over the year. Both the baseline and alternative designs have been evaluated and no critical items with Technology Readiness Level (TRL) less than 4–5 have been identified. We have also undertaken a first-order cost and development plan analysis and find that EChO is easily compatible with the ESA M-class mission framework.

High-density metallic nano-emitter arrays and their field emission characteristics

We report the fabrication and field emission properties of high-density nano-emitter arrays with on-chip electron extraction gate electrodes and up to 106 metallic nanotips that have an apex curvature radius of a few nanometers and a the tip density exceeding 108 cm−2. The gate electrode was fabricated on top of the nano-emitter arrays using a self-aligned polymer mask method. By applying a hot-press step for the polymer planarization, gate–nanotip alignment precision below 10 nm was achieved. Fabricated devices exhibited stable field electron emission with a current density of 0.1 A cm−2, indicating that these are promising for applications that require a miniature high-brightness electron source.

AIV procedure for a CHEOPS demonstration model

The CHaracterizing ExOPlanet Satellite (CHEOPS) is an ESA Small Mission whose launch is planned for the end of 2017. It is a Ritchey-Chretien telescope with a 320 mm aperture providing a FoV of 0.32 degrees, which will target nearby bright stars already known to host planets, and measure, through ultrahigh precision photometry, the radius of exo-planets, allowing to determine their composition. This paper will present the details of the AIV plan for a demonstration model of the CHEOPS Telescope with equivalent structure but different CTEs. Alignment procedures, needed GSEs and devised verification tests will be described and a path for the AIV of the flight model, which will take place at industries premises, will be sketched. © (2014) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE).

Natural and anthropogenic methane fluxes in Eurasia: a mesoscale quantification by generalized atmospheric inversion

Eight surface observation sites providing quasi-continuous measurements of atmospheric methane mixingratios have been operated since the mid-2000’s in Siberia. For the first time in a single work, we assimilate 1 year of these in situ observations in an atmospheric inversion. Our objective is to quantify methane surface fluxes from anthropogenic and wetland sources at the mesoscale in the Siberian lowlands for the year 2010. To do so, we first inquire about the way the inversion uses the observations and the way the fluxes are constrained by the observation sites. As atmospheric inver- sions at the mesoscale suffer from mis-quantified sources of uncertainties, we follow recent innovations in inversion techniques and use a new inversion approach which quantifies the uncertainties more objectively than the previous inversion systems. We find that, due to errors in the representation of the atmospheric transport and redundant pieces of information, only one observation every few days is found valuable by the inversion. The remaining high-resolution quasi-continuous signal is representative of very local emission patterns difficult to analyse with a mesoscale system. An analysis of the use of information by the inversion also reveals that the observation sites constrain methane emissions within a radius of 500 km. More observation sites than the ones currently in operation are then necessary to constrain the whole Siberian lowlands. Still, the fluxes within the constrained areas are quantified with objectified uncertainties. Finally, the tolerance intervals for posterior methane fluxes are of roughly 20 % (resp. 50 %) of the fluxes for anthropogenic (resp. wetland) sources. About 50–70 % of Siberian lowlands emissions are constrained by the inversion on average on an annual basis. Extrapolating the figures on the constrained areas to the whole Siberian lowlands, we find a regional methane budget of 5–28 TgCH4 for the year 2010, i.e. 1–5 % of the global methane emissions. As very few in situ observations are available in the region of interest, observations of methane total columns from the Greenhouse Gas Observing SATellite (GOSAT) are tentatively used for the evaluation of the inversion results, but they exhibit only a marginal signal from the fluxes within the region of interest.

Pollen and charcoal in lake sediments compared with historically documented forest fires in southern Switzerland since AD 1920

Charcoal in unlaminated sediments dated by 210Pb was analysed by the pollen-slide and thin-section methods. The results were compared with the number and area of forest fires on different spatial scales in the area around Lago di Origlio as listed in the wildfire database of southern Switzerland since AD 1920. The influx of the number of charcoal particles > 75 µm2 in pollen slides correlates well with the number of annual forest fires recorded within a distance of 20-50 km from the coring site. Hence a size-class distinction or an area measurement by image analysis may not be absolutely necessary for the reconstruction of regional fire history. A regression equation was computed and tested against an independent data set. Its use makes it possible to estimate the charcoal area influx (or concentration) from the particle number influx (or concentration). Local fires within a radius of 2 km around the coring site correlate well with the area influx of charcoal particles estimated by the thin-section method measuring the area of charcoal particles larger than 20 000 µm2 or longer than 50 µm. Pollen percentages and influx values suggest that intensive agriculture and Castanea sativa cultivation were reduced 30-40 years ago, followed by an increase of forest area and a development to more natural woodlands. The traditional Castanea sativa cultivation was characterized by a complete use of the biomass produced, so abandonment of chestnut led to an increasing accumulation of dead biomass, thereby raising the fire risk. On the other hand, the pollen record of the regional vegetation does not show any clear response to the increase of fire frequency during the last three decades in this area.

Los promotores en la metodología de intervención del programa Pro-Huerta Córdoba, Argentina

El Pro-Huerta (PPH) es un programa estatal nacional que aborda la seguridad alimentaria, dirigido a la población pobre. La zona Gran Córdoba comprende la ciudad de Córdoba y un amplio territorio que involucra los pueblos cercanos en un radio aproximado de unos 50 km de la capital, donde se trabaja con más de 120 promotores y 14.500 huerteros. Debido a que los promotores son los actores que los técnicos destacan como fundamentales en el funcionamiento del programa, las principales preguntas que este estudio se formula son: ¿quiénes son los actores que participan como promotores en el PPH de la provincia de Córdoba? y ¿cómo perciben los promotores los beneficios y limitaciones del componente de capacitación? La metodología utilizada combina procedimientos cuanti y cualitativos en el tratamiento de los datos. El universo de promotores fue clasificado contemplando las funciones que desempeñan en el programa y sus demandas de capacitación. Se observó una relación significativa entre el subtipo que cumple una función de promoción más integral y el subtipo que demanda capacitación en aspectos sociales. Asimismo es importante la relación entre el subtipo que limita su función sólo a convocar reuniones para repartir semillas con el que manifiesta una menor demanda de capacitación en general.

Radicalización política y sectores populares en la Argentina de los '70 : La juventud peronista [JP] y su articulación con Montoneros en los barrios periféricos de la ciudad de La Plata

La Tesis, a través de un estudio de caso, se propone aportar una descripción empírica sobre los nexos que las organizaciones armadas establecieron con los sectores populares durante los '70 en la Argentina. Con ese propósito, reconstruye el sistema de unidades básicas organizado por la Juventud Peronista platense articulada con Montoneros en los barrios de la periferia platense entre 1972/74. Para el abordaje y comprensión de este conjunto, la investigación se ocupa previamente de la reconstrucción de aspectos de la larga trayectoria de la JP platense, previa a su articulación con Montoneros, durante los años '60, cuando delineo una estrategia de expansión política centrada en los ámbitos barriales, asimilando también una serie de influencias y prácticas producto de los procesos de radicalización en curso. Luego la tesis analiza el universo de las unidades básicas montoneras atendiendo a tres grandes componentes. Primero, los actores barriales más representativos: los militantes y las unidades básicas. Segundo, las prácticas sobre las que se sostuvo toda la experiencia: las de tipo reivindicativas y las más propiamente políticas. Por ultimo, el conjunto de representaciones que guiaron el debate y circulación de ideas: la recepción que tuvieron en el seno de las unidades básicas las concepciones criticas de los jóvenes montoneros en tomo a Perón y al peronismo y las nociones de socialismo y la lucha armada. La tesis permite apreciar la complejidad y variedad de lazos e intercambios que tuvieron lugar en el ámbito barrial montonero de la ciudad de La Plata y, a la vez, Ios límites y la dinámica que llevó a su disolución

En zaga de tantos otros : Paul Groussac y la angustia de las influencias en el Río de la Plata

En este artículo analizo las opiniones de Paul Groussac sobre la cultura americana (tanto norte como latinoamericana), condenada en tanto copia falsa y defectuosa de un único original: el canon europeo en el que el francés autoriza su escritura y se autolegitima como crítico literario en el Río de la Plata. Me concentro en algunos textos clave en relación con el problema de los comienzos de la literatura latinoamericana y con la angustia de influencias que caracteriza al propio Groussac: su lectura de La tempestad de Shakespeare, sus escritos en Del Plata al Niágara y sus notas sobre Los raros y Prosas profanas de Rubén Darío

Radicalización política y sectores populares en la Argentina de los '70 : La juventud peronista [JP] y su articulación con Montoneros en los barrios periféricos de la ciudad de La Plata

La Tesis, a través de un estudio de caso, se propone aportar una descripción empírica sobre los nexos que las organizaciones armadas establecieron con los sectores populares durante los '70 en la Argentina. Con ese propósito, reconstruye el sistema de unidades básicas organizado por la Juventud Peronista platense articulada con Montoneros en los barrios de la periferia platense entre 1972/74. Para el abordaje y comprensión de este conjunto, la investigación se ocupa previamente de la reconstrucción de aspectos de la larga trayectoria de la JP platense, previa a su articulación con Montoneros, durante los años '60, cuando delineo una estrategia de expansión política centrada en los ámbitos barriales, asimilando también una serie de influencias y prácticas producto de los procesos de radicalización en curso. Luego la tesis analiza el universo de las unidades básicas montoneras atendiendo a tres grandes componentes. Primero, los actores barriales más representativos: los militantes y las unidades básicas. Segundo, las prácticas sobre las que se sostuvo toda la experiencia: las de tipo reivindicativas y las más propiamente políticas. Por ultimo, el conjunto de representaciones que guiaron el debate y circulación de ideas: la recepción que tuvieron en el seno de las unidades básicas las concepciones criticas de los jóvenes montoneros en tomo a Perón y al peronismo y las nociones de socialismo y la lucha armada. La tesis permite apreciar la complejidad y variedad de lazos e intercambios que tuvieron lugar en el ámbito barrial montonero de la ciudad de La Plata y, a la vez, Ios límites y la dinámica que llevó a su disolución

En zaga de tantos otros : Paul Groussac y la angustia de las influencias en el Río de la Plata

En este artículo analizo las opiniones de Paul Groussac sobre la cultura americana (tanto norte como latinoamericana), condenada en tanto copia falsa y defectuosa de un único original: el canon europeo en el que el francés autoriza su escritura y se autolegitima como crítico literario en el Río de la Plata. Me concentro en algunos textos clave en relación con el problema de los comienzos de la literatura latinoamericana y con la angustia de influencias que caracteriza al propio Groussac: su lectura de La tempestad de Shakespeare, sus escritos en Del Plata al Niágara y sus notas sobre Los raros y Prosas profanas de Rubén Darío