bluuebunny/crossref_metadata_2025_split huggingface dataset:
La fundamentación zubiriana de la pedagogía de López Quintás
Authors: Esteve Alfredo 
Published: May 2017

Resumen La enseñanza de la filosofía no es únicamente una transmisión de contenidos; incluso probablemente no sea éste el objetivo más importante. Para plantearnos qué es lo más importante en la docencia filosófica deberíamos preguntarnos qué queremos exactamente que aprendan nuestros alumnos. Cuando intentamos responder a esta cuestión se pone de manifiesto la especificidad de la filosofía. La filosofía no es cuestión de contenidos sino de vida; no es cuestión de respuestas, sino de preguntas. En esta comunicación se pretende mostrar la pedagogía de la admiración de Alfonso López Quintás a la luz de la inteligencia sentiente de Xavier Zubiri. Palabras clave: docencia filosofía, Xavier Zubiri, Alfonso López Quintás, capacitación educativa The Zubirian Basis of López Quintás’s Pedagogy Abastract Teaching philosophy is not only about conveying contents; indeed this is probably not the most important goal. In reflecting about what is most important in teaching philosophy we should ask ourselves what we want specifically our students to learn. When we try to answer this question the specificity of philosophy is revealed. Philosophy is not a matter of contents but of life—it is not about answers but about questions. This paper aims to present Alfonso Lopez Quintás’s pedagogy of admiration in the light of Xavier Zubiri’s sentient intelligence. Keywords: teaching philosophy, Xavier Zubiri, Alfonso López Quintás, educational training
Taller de significados inéditos. Redefinición de conceptos siguiendo reglas lógicas
Authors: Calero Morcuende Luis 
Published: May 2017

Resumen: El Taller de significados inéditos está concebido como una práctica filosófica para generar nuevos significados mediante la redefinición, siguiendo reglas lógicas, de conceptos del lenguaje ordinario. A partir de unas simples reglas y de un vocabulario seleccionado, los alumnos son capaces de pensar el lenguaje y recrear la realidad, alumbrando significados originales como expresión de su creatividad e imaginación. Junto a la mejora de la capacidad de definir —una de las operaciones básicas para articular el pensamiento—, el taller también puede servir para aprender a vincular conceptos e imágenes y para ejercitar el sentido crítico, así como para hacer uso del diccionario y las TIC. Palabras clave: definición, reglas, creatividad, significados. English title: Studio of untold meanings. Redefining concepts by following logical rulesAbstract: The Studio of untold meanings has been conceived as a philosophical practise in order to generate new meanings, through redefinition of ordinary language concepts, following logical rules. Starting from simple rules and selected vocabulary, students are able to think the language and recreate reality, lighting up original meanings as expression of their creativity and imagination. Besides improving the ability to define—one of the basic operations of articulate thought—the studio can also help them to learn how to link concepts and images, exercise critical thinking and encourage the use of dictionaries and TIC. Keywords: definition, rules, creativity, meanings.
Educar contra Auschwitz mediante el seminario de lectura
Authors: Batalla Gavaldà Ana Lucía 
Published: May 2017

Resumen: En este escrito defiendo la realización de seminarios de lectura como una experiencia educativa innovadora que permite una mejor comprensión de los textos. En el marco de la educación contra Auschwitz, se propone la lectura conjunta de Si esto es un hombre, obra testimonial de Primo Levi. Mediante este seminario, se busca promover en los estudiantes la deliberación activa, el diálogo, la transmisión de valores y la importancia de escuchar a las víctimas. Palabras clave: seminario de lectura, Primo Levi, Auschwitz, testimonio. English title: Educating against Auschwitz with a reading groupAbstract: In this paper, I argue that reading groups can involve innovative teaching experiences which allow for a better understanding of books. Within the framework of education against Auschwitz, I propose the group reading of If this is a man—a testimonial book by Primo Levi. The aim is to promote in our students active deliberation, dialogue, transmission of values, and the importance of listening to the victims. Keywords: reading group, Primo Levi, Auschwitz, testimony.
Del Homo Ludens a la gamificación
Authors: Carreras Planas Carla 
Published: May 2017

Resumen: Parece que las últimas tendencias en educación pasan por introducir la gamificación en las aulas y en todas las actividades educativas. La idea de que los contenidos deben interesar a nuestros estudiantes combinada con el convencimiento de que “se aprende mejor jugando”, han llevado a pensar que debemos dar a esos contenidos una forma lúdica o, mejor todavía, convertirlos en juegos. ¿Es la gamificación una moda o una oportunidad? Y en el caso concreto de la educación, ¿se trata sólo de un recurso metodológico para aprender más eficazmente o es una característica que debería tener toda actividad que pretenda ser educativa? ¿Cómo gamificar las clases (de filosofía, en nuestro caso)? Palabras clave: gamificación, Huizinga, Homo ludens. English title: From Homo Ludens to gamificationAbstract: Latest trends in education go through introducing gamification in classrooms and in all educational activities. The idea that contents should interest our students combined with the conviction that “they learn better by playing” have led us to think that we should give these contents a playful form or, even better, turn them into games. Is gamification a trend or an opportunity? And in the specific case of education, is it only a methodological resource to learn more effectively or is it a characteristic that should have all activity that pretends to be educational? How to gamify courses (philosophy courses, more concretely)? Keywords: gamification, Huizinga, Homo ludens.
Juno observations of energetic charged particles over Jupiter's polar regions: Analysis of monodirectional and bidirectional electron beams
Authors: Mauk B. H. , Haggerty D. K. , Paranicas C. , Clark G. , Kollmann P. , Rymer A. M. , Mitchell D. G. , Bolton S. J. , Levin S. M. , Adriani A. , Allegrini F. , Bagenal F. , Connerney J. E. P. , Gladstone G. R. , Kurth W. S. , McComas D. J. , Ranquist D. , Szalay J. R. , Valek P. 
Published: May 2017

AbstractJuno obtained unique low‐altitude space environment measurements over Jupiter's poles on 27 August 2016. Here Jupiter Energetic‐particle Detector Instrument observations are presented for electrons (25–800 keV) and protons (10–1500 keV). We analyze magnetic field‐aligned electron angular beams over expected auroral regions that were sometimes symmetric (bidirectional) but more often strongly asymmetric. Included are variable but surprisingly persistent upward, monodirectional electron angular beams emerging from what we term the “polar cap,” poleward of the nominal auroral ovals. The energy spectra of all beams were monotonic and hard (not structured in energy), showing power law‐like distributions often extending beyond ~800 keV. Given highly variable downward energy fluxes (below 1 RJ altitudes within the loss cone) as high as 280 mW/m2, we suggest that mechanisms generating these beams are among the primary processes generating Jupiter's uniquely intense auroral emissions, distinct from what is typically observed at Earth.
Latitudinal beaming of Jovian decametric radio emissions as viewed from Juno and the Nançay Decameter Array
Authors: Imai Masafumi , Kurth William S. , Hospodarsky George B. , Bolton Scott J. , Connerney John E. P. , Levin Steven M. , Lecacheux Alain , Lamy Laurent , Zarka Philippe 
Published: May 2017

AbstractTwo well‐defined Jovian decametric radio arcs were observed at latitudinal separations of 11°–16° from the Juno spacecraft near Jupiter and the Nançay Decameter Array (NDA) at Earth on 17 May and 25 August 2016. These discrete arcs are from the so‐called A source covering both Io‐related and non‐Io‐related emissions. By measuring the wave arrival time at two distant observers with propagation time correction, the remaining delay times are 92.8 ± 1.3 min for the first arc and 116.0 ± 1.2 min for the second arc. This implies that both radio sources are not controlled by the orbital motion of Io but Jupiter's rotation itself. The geometrical information for Juno and NDA and the loss cone‐driven electron cyclotron maser instability theory provide these radio sources that are located at about 173° ± 10° in system III longitude projected onto Jupiter's north surface and imply resonant electron energy ranges from 0.5 to 11 keV.
Increased sediment oxygen flux in lakes and reservoirs: The impact of hypolimnetic oxygenation
Authors: Bierlein Kevin A. , Rezvani Maryam , Socolofsky Scott A. , Bryant Lee D. , Wüest Alfred , Little John C. 
Published: May 2017

AbstractHypolimnetic oxygenation is an increasingly common lake management strategy for mitigating hypoxia/anoxia and associated deleterious effects on water quality. A common effect of oxygenation is increased oxygen consumption in the hypolimnion and predicting the magnitude of this increase is the crux of effective oxygenation system design. Simultaneous measurements of sediment oxygen flux (JO2) and turbulence in the bottom boundary layer of two oxygenated lakes were used to investigate the impact of oxygenation on JO2. Oxygenation increased JO2 in both lakes by increasing the bulk oxygen concentration, which in turn steepens the diffusive gradient across the diffusive boundary layer. At high flow rates, the diffusive boundary layer thickness decreased as well. A transect along one of the lakes showed JO2 to be spatially quite variable, with near‐field and far‐field JO2 differing by a factor of 4. Using these in situ measurements, physical models of interfacial flux were compared to microprofile‐derived JO2 to determine which models adequately predict JO2 in oxygenated lakes. Models based on friction velocity, turbulence dissipation rate, and the integral scale of turbulence agreed with microprofile‐derived JO2 in both lakes. These models could potentially be used to predict oxygenation‐induced oxygen flux and improve oxygenation system design methods for a broad range of reservoir systems.
Evapotranspiration of urban landscapes in Los Angeles, California at the municipal scale
Authors: Litvak E. , Manago K. F. , Hogue T. S. , Pataki D. E. 
Published: May 2017

AbstractEvapotranspiration (ET), an essential process in biosphere‐atmosphere interactions, is highly uncertain in cities that maintain cultivated and irrigated landscapes. We estimated ET of irrigated landscapes in Los Angeles by combining empirical models of turfgrass ET and tree transpiration derived from in situ measurements with previously developed remotely sensed estimates of vegetation cover and ground‐based vegetation surveys. We modeled irrigated landscapes as a two‐component system comprised of trees and turfgrass to assess annual and spatial patterns of ET. Annual ET from vegetated landscapes (ETveg) was 1110 ± 53 mm/yr and ET from the whole city (vegetated and nonvegetated areas, ETland) was three times smaller, reflecting the fractional vegetation cover. With the exception of May and June, monthly ETland was significantly higher than predicted by the North American Land Data Assimilation System. ETveg was close to potential ET, indicating abundant irrigation inputs. Monthly averaged ETveg varied from 1.5 ± 0.1 mm/d (December) to 4.3 ± 0.2 mm/d (June). Turfgrass was responsible for ∼70% of ETveg. For trees, angiosperm species (71% of all trees) contributed over 90% to total tree transpiration, while coniferous and palm species made very small contributions. ETland was linearly correlated with median household income across the city, confirming the importance of social factors in determining spatial distribution of urban vegetation. These estimates have important implications for constraining the municipal water budget of Los Angeles and improving regional‐scale hydrologic models, as well as for developing water‐saving practices. The methodology used in this study is also transferable to other semiarid regions for quantification of urban landscape ET.
Plasma environment at the dawn flank of Jupiter's magnetosphere: Juno arrives at Jupiter
Authors: McComas D. J. , Szalay J. R. , Allegrini F. , Bagenal F. , Connerney J. , Ebert R. W. , Kurth W. S. , Louarn P. , Mauk B. , Reno M. , Thomsen M. F. , Valek P. , Weidner S. , Wilson R. J. , Bolton S. 
Published: May 2017

AbstractThis study examines the first observations from the Jovian Auroral Distributions Experiment (JADE) as the Juno spacecraft arrived at Jupiter. JADE observations show that Juno crossed the bow shock at 08:16 UT on 2016 day of year (DOY) 176 and magnetopause at 21:20 on DOY 177, with additional magnetopause encounters until 23:39 on DOY 181. JADE made the first detailed observations of the plasma environment just inside the dawn flank of the magnetopause. We find subcorotational ions and variable electron beaming, with multiple flux tubes of varying plasma properties. Ion composition shows a dearth of heavy ions; protons dominate the plasma, with only intermittent, low fluxes of O+/S++, along with traces of O++ and S+++. We also find very little
or He+, which are expected for an ionospheric plasma source. A few heavy ion bursts occur when the radial field nears reversal, but many other such reversals are not accompanied by heavy ions.
Plasma measurements in the Jovian polar region with Juno/JADE
Authors: Szalay J. R. , Allegrini F. , Bagenal F. , Bolton S. , Clark G. , Connerney J. E. P. , Dougherty L. P. , Ebert R. W. , Gershman D. J. , Kurth W. S. , Levin S. , Louarn P. , Mauk B. , McComas D. J. , Paranicas C. , Ranquist D. , Reno M. , Thomsen M. F. , Valek P. W. , Weidner S. , Wilson R. J. 
Published: May 2017

AbstractJupiter's main auroral oval provides a window into the complex magnetospheric dynamics of the Jovian system. The Juno spacecraft entered orbit about Jupiter on 5 July 2016 and carries on board the Auroral Distributions Experiment (JADE) that can directly sample the auroral plasma structures. Here we identify five distinct regimes in the JADE data based on composition/energy boundaries and magnetic field mappings, which exhibit considerable symmetry between the northern and southern passes. These intervals correspond to periods when Juno was connected to the Io torus, inner plasma sheet, middle plasma sheet, outer plasma sheet, and the polar region. When connected to the torus and inner plasma sheet, the heavy ions are consistent with a corotating pickup population. For Juno's first perijove, we do not find evidence for a broad auroral acceleration region at Jupiter's main auroral oval for energies below 100 keV.
Preliminary results on the composition of Jupiter's troposphere in hot spot regions from the JIRAM/Juno instrument
Authors: Grassi D. , Adriani A. , Mura A. , Dinelli B. M. , Sindoni G. , Turrini D. , Filacchione G. , Migliorini A. , Moriconi M. L. , Tosi F. , Noschese R. , Cicchetti A. , Altieri F. , Fabiano F. , Piccioni G. , Stefani S. , Atreya S. , Lunine J. , Orton G. , Ingersoll A. , Bolton S. , Levin S. , Connerney J. , Olivieri A. , Amoroso M. 
Published: May 2017

AbstractThe Jupiter InfraRed Auroral Mapper (JIRAM) instrument on board the Juno spacecraft performed observations of two bright Jupiter hot spots around the time of the first Juno pericenter passage on 27 August 2016. The spectra acquired in the 4–5 µm spectral range were analyzed to infer the residual opacities of the uppermost cloud deck as well as the mean mixing ratios of water, ammonia, and phosphine at the approximate level of few bars. Our results support the current view of hot spots as regions of prevailing descending vertical motions in the atmosphere but extend this view suggesting that upwelling may occur at the southern boundaries of these structures. Comparison with the global ammonia abundance measured by Juno Microwave Radiometer suggests also that hot spots may represent sites of local enrichment of this gas. JIRAM also identifies similar spatial patterns in water and phosphine contents in the two hot spots.
Searching for low‐altitude magnetic field anomalies by using observations of the energetic particle loss cone on JUNO
Authors: Zhang X.‐J. , Thorne R. M. , Ma Q. , Li W. , Mauk B. H. , Paranicas C. , Haggerty D. K. , Connerney J. E. P. , Bolton S. J. 
Published: May 2017

AbstractIn inner planetary magnetospheres, pitch angle distributions of charged particles are shaped by the global magnetic field topology when they bounce fast along magnetic field lines. Therefore, one can estimate the magnetic field intensity at the top of the atmosphere from the loss cone size, inferred from particle pitch angle distributions at higher altitudes. We propose such a technique to estimate the magnetic field intensity near the top of Jovian atmosphere based on Jupiter Energetic Particle Detector Instruments particle distributions captured by JUNO and verify the algorithm by using plasma measurements from Van Allen Probes in the Earth's inner magnetosphere. Our results demonstrate that the low‐altitude magnetic field can be significantly larger than the expected field from present models, which supports recent reports on the anomaly of Jovian internal magnetic field from in situ JUNO measurements. We also discuss possible modifications and applications of the proposed technique to future investigations of the global Jovian magnetic field configuration.
Generation of the Jovian hectometric radiation: First lessons from Juno
Authors: Louarn P. , Allegrini F. , McComas D. J. , Valek P. W. , Kurth W. S. , André N. , Bagenal F. , Bolton S. , Connerney J. , Ebert R. W. , Imai M. , Levin S. , Szalay J. R. , Weidner S. , Wilson R. J. , Zink J. L. 
Published: May 2017

AbstractUsing Juno plasma and wave and magnetic observations (JADE and Waves and MAG instruments), the generation mechanism of the Jovian hectometric radio emission is analyzed. It is shown that suitable conditions for the cyclotron maser instability (CMI) are observed in the regions of the radio sources. Pronounced loss cone in the electron distributions are likely the source of free energy for the instability. The theory reveals that sufficient growth rates are obtained from the distribution functions that are measured by the JADE‐Electron instrument. The CMI would be driven by upgoing electron populations at 5–10 keV and 10–30° pitch angle, the amplified waves propagating at 82°–87° from the B field, a fraction of a percent above the gyrofrequency. Typical e‐folding times of 10−4 s are obtained, leading to an amplification path of ~1000 km. Overall, this scenario for generation of the Jovian hectometric waves differs significantly from the case of the auroral kilometric radiation at Earth.
Characterization of the white ovals on Jupiter's southern hemisphere using the first data by the Juno/JIRAM instrument
Authors: Sindoni G. , Grassi D. , Adriani A. , Mura A. , Moriconi M. L. , Dinelli B. M. , Filacchione G. , Tosi F. , Piccioni G. , Migliorini A. , Altieri F. , Fabiano F. , Turrini D. , Noschese R. , Cicchetti A. , Stefani S. , Bolton S. J. , Connerney J. E. P. , Atreya S. K. , Bagenal F. , Hansen C. , Ingersoll A. , Janssen M. , Levin S. M. , Lunine J. I. , Orton G. , Olivieri A. , Amoroso M. 
Published: May 2017

AbstractDuring the first perijove passage of the Juno mission, the Jovian InfraRed Auroral Mapper (JIRAM) observed a line of closely spaced oval features in Jupiter's southern hemisphere, between 30°S and 45°S. In this work, we focused on the longitudinal region covering the three ovals having higher contrast at 5 μm, i.e., between 120°W and 60°W in System III coordinates. We used the JIRAM's full spectral capability in the range 2.4–3 μm together with a Bayesian data inversion approach to retrieve maps of column densities and altitudes for an NH3 cloud and an N2H4 haze. The deep (under the saturation level) volume mixing ratio and the relative humidity for gaseous ammonia were also retrieved. Our results suggest different vortex activity for the three ovals. Updraft and downdraft together with considerations about the ammonia condensation could explain our maps providing evidences of cyclonic and anticyclonic structures.
Multiple‐wavelength sensing of Jupiter during the Juno mission's first perijove passage
Authors: Orton G. S. , Momary T. , Ingersoll A. P. , Adriani A. , Hansen C. J. , Janssen M. , Arballo J. , Atreya S. K. , Bolton S. , Brown S. , Caplinger M. , Grassi D. , Li C. , Levin S. , Moriconi M. L. , Mura A. , Sindoni G. 
Published: May 2017

AbstractWe compare Jupiter observations made around 27 August 2016 by Juno's JunoCam, Jovian Infrared Auroral Mapper (JIRAM), MicroWave Radiometer (MWR) instruments, and NASA's Infrared Telescope Facility. Visibly dark regions are highly correlated with bright areas at 5 µm, a wavelength sensitive to gaseous NH3 gas and particulate opacity at p ≤5 bars. A general correlation between 5‐µm and microwave radiances arises from a similar dependence on NH3 opacity. Significant exceptions are present and probably arise from additional particulate opacity at 5 µm. JIRAM spectroscopy and the MWR derive consistent 5‐bar NH3 abundances that are within the lower bounds of Galileo measurement uncertainties. Vigorous upward vertical transport near the equator is likely responsible for high NH3 abundances and with enhanced abundances of some disequilibrium species used as indirect indicators of vertical motions.
Io‐Jupiter decametric arcs observed by Juno/Waves compared to ExPRES simulations
Authors: Louis C. K. , Lamy L. , Zarka P. , Cecconi B. , Imai M. , Kurth W. S. , Hospodarsky G. , Hess S. L. G. , Bonnin X. , Bolton S. , Connerney J. E. P. , Levin S. M. 
Published: May 2017

AbstractWe compare observations from the Juno/Waves radio experiment with simulations of radio «arcs» in the time‐frequency plane resulting from the Io‐Jupiter interaction, performed with the ExPRES code. We identify the hemisphere of origin of the observed arcs directly from simulations and confirm this identification through comparison with Juno, Nançay, and Wind observations. The occurrence and shape of observed arcs are well modeled, at low latitudes with their usual shapes as seen from Earth, as well as at high latitudes with longer, bowl‐shaped, arcs observed for the first time. Predicted emission is actually observed only when the radio beaming angle θ = (k,B) ≥ 70° ± 5°, providing new constraints on the generation of the decameter emission by the Cyclotron Maser Instability. Further improvements of ExPRES are outlined, which will then be applied to Juno and Earth‐based observations of radio emissions induced by other Galilean satellites or associated to the main auroral oval.