66 research outputs found

    Restauración Del Arte Pictórico y La Química Analítica : Diseño De Una Asignatura Electiva

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    Este trabajo de investigación se diseñó fundamentado en el trabajo de grado titulado “Restauración del arte pictórico: estrategia en la enseñanza de la química para estudiantes de formación inicial de la licenciatura en química” (Marquez,B.2018) , como continuación de este proyecto investigativo, donde se da un indicio acerca de la restauración de arte pictórico y la química, su relación con la estequiometria química y los procesos de oxido reducción en una obra pictórica, todo esto con el fin de diseñar una asignatura electiva, que unifique postulados, conceptos, teorías, entre otros de la química analítica y de la restauración de una obra pictórica.This research work was designed based on the degree work entitled "Restoration of pictorial art: strategy in the teaching of chemistry for initial training students of the bachelor of chemistry" (Marquez, B. 2018), as a continuation of this project research, where an indication is given about the restoration of pictorial art and chemistry and its relationship with chemical stoichiometry and the processes of oxide reduction in a pictorial work and from this, an elective subject is designed, which unifies postulates, concepts, theories, among others of analytical chemistry and the restoration of a pictorial work. At the beginning, a state of the art of the chemical processes that occur in the restoration of paintings of pictorial art is proposed and to determine how said restoration includes analytical chemistry as a basis in the restoration, based on the model of conceptual pedagogy proposed by Zubiría (2007) takes the hexagon model as a tool, which reveals 2 dimensions, the didactic and the pedagogical, which focus on the why, and the other on the how, in this way the design is based on this model which focuses on student motivation and thus raises the entire sequential process of elective design, presenting different strategies to gather important information for the design, such as the number of credits, total hours, thematic axes, motivating activities for the students, the themes, and how they relate (analytical chemistry one directly to the other (pictorial art)

    Amor, empatía y conductas prosociales: una reflexión interdisciplinaria

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    This book presents, through reflection, the relevance, timeliness and necessity of love, empathy and prosocial behaviors within the framework of the professional and disciplinary work of the authors. The reader will be able to find here what these professionals, academics and intellectuals think and feel about it. Let the reader know that it was not a simple writing project, maybe because of the invitation to think about oneself, maybe because of the presence of the concept of "love" in the academy, or maybe, because we are not so accustomed to putting in the first person the reflection turned from what we relate to day by day. May this text be the excuse to continue to reflect on the role of love, empathy and prosocial behavior in a world that sometimes shows great desolation. May these unknotted reflections allow us to understand and resignify, learn and continue.PublishedEste libro expone, por la vía de la reflexión, la pertinencia, actualidad y necesidad del amor, la empatía y las conductas prosociales en el marco del quehacer profesional y disciplinar de los autores. El lector podrá encontrar aquí lo que esos profesionales, académicos e intelectuales piensan y sienten al respecto. Sepa el lector que no fue un proyecto de escritura sencillo, quizá por la invitación a pensar sobre sí, quizá por la presencia del concepto “amor” en la academia, o quizá, simplemente, porque no estamos tan acostumbrados a poner en primera persona la reflexión devenida de aquello con lo que día a día nos relacionamos. Que sea este texto la excusa para continuar reflexionando sobre el papel del amor, la empatía y las conductas prosociales en un mundo que a veces muestra gran desolación. Que estas reflexiones des-anudadas permitan comprender y resignificar, aprender y continuar

    A search for ultra-high-energy photons at the Pierre Auger Observatory exploiting air-shower universality

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    The Pierre Auger Observatory is the most sensitive detector to primary photons with energies above ∼0.2 EeV. It measures extensive air showers using a hybrid technique that combines a fluorescence detector (FD) with a ground array of particle detectors (SD). The signatures of a photon-induced air shower are a larger atmospheric depth at the shower maximum (Xmax_{max}) and a steeper lateral distribution function, along with a lower number of muons with respect to the bulk of hadron-induced background. Using observables measured by the FD and SD, three photon searches in different energy bands are performed. In particular, between threshold energies of 1-10 EeV, a new analysis technique has been developed by combining the FD-based measurement of Xmax_{max} with the SD signal through a parameter related to its muon content, derived from the universality of the air showers. This technique has led to a better photon/hadron separation and, consequently, to a higher search sensitivity, resulting in a tighter upper limit than before. The outcome of this new analysis is presented here, along with previous results in the energy ranges below 1 EeV and above 10 EeV. From the data collected by the Pierre Auger Observatory in about 15 years of operation, the most stringent constraints on the fraction of photons in the cosmic flux are set over almost three decades in energy

    Study on multi-ELVES in the Pierre Auger Observatory

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    Since 2013, the four sites of the Fluorescence Detector (FD) of the Pierre Auger Observatory record ELVES with a dedicated trigger. These UV light emissions are correlated to distant lightning strikes. The length of recorded traces has been increased from 100 μs (2013), to 300 μs (2014-16), to 900 μs (2017-present), to progressively extend the observation of the light emission towards the vertical of the causative lightning and beyond. A large fraction of the observed events shows double ELVES within the time window, and, in some cases, even more complex structures are observed. The nature of the multi-ELVES is not completely understood but may be related to the different types of lightning in which they are originated. For example, it is known that Narrow Bipolar Events can produce double ELVES, and Energetic In-cloud Pulses, occurring between the main negative and upper positive charge layer of clouds, can induce double and even quadruple ELVES in the ionosphere. This report shows the seasonal and daily dependence of the time gap, amplitude ratio, and correlation between the pulse widths of the peaks in a sample of 1000+ multi-ELVES events recorded during the period 2014-20. The events have been compared with data from other satellite and ground-based sensing devices to study the correlation of their properties with lightning observables such as altitude and polarity

    Outreach activities at the Pierre Auger Observatory

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    The ultra-high-energy cosmic-ray sky above 32 EeV viewed from the Pierre Auger Observatory

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    First results from the AugerPrime Radio Detector

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    Update of the Offline Framework for AugerPrime

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    Extraction of the Muon Signals Recorded with the Surface Detector of the Pierre Auger Observatory Using Recurrent Neural Networks

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    We present a method based on the use of Recurrent Neural Networks to extract the muon component from the time traces registered with water-Cherenkov detector (WCD) stations of the Surface Detector of the Pierre Auger Observatory. The design of the WCDs does not allow to separate the contribution of muons to the time traces obtained from the WCDs from those of photons, electrons and positrons for all events. Separating the muon and electromagnetic components is crucial for the determination of the nature of the primary cosmic rays and properties of the hadronic interactions at ultra-high energies. We trained a neural network to extract the muon and the electromagnetic components from the WCD traces using a large set of simulated air showers, with around 450 000 simulated events. For training and evaluating the performance of the neural network, simulated events with energies between 1018.5, eV and 1020 eV and zenith angles below 60 degrees were used. We also study the performance of this method on experimental data of the Pierre Auger Observatory and show that our predicted muon lateral distributions agree with the parameterizations obtained by the AGASA collaboration

    Large-scale and multipolar anisotropies of cosmic rays detected at the Pierre Auger Observatory with energies above 4 EeV

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