Monitoria na Disciplina “Técnica Cirúrgica e Cirurgia Experimental”

Na monitoria da disciplina Técnica Cirúrgica e Cirurgia Experimental, alunos que foram aprovados no curso participam do ensino dos atuais discentes em atividades práticas. Um questionário de resposta voluntária inquiriu a motivação para o exercício da monitoria e a avaliação dos monitores sobre a atividade. Aceitaram participar dezenove monitores, de 2014 a 2015. Para 94,7% dos que responderam ao questionário, a monitoria atingiu o esperado ou o além do esperado, e todos indicam a monitoria a outros alunos da faculdade. Isso a caracteriza como fator positivo na formação dos participantes dessa atividade acadêmica. Essa boa avaliação associa-se ao maior aprendizado do aluno monitor sobre o conteúdo da disciplina, à melhoria da comunicação interpessoal e à maior vivência com a cirurgia que a monitoria proporciona. Aos alunos da disciplina, o ganho ao utilizar essa estratégia didática consiste na maior empatia que os monitores têm com aqueles que cursam a disciplina em comparação com os docentesIn the monitoring of the discipline Surgical Technique and Experimental Surgery, students that were previously approved in the course take part in the teaching of the current students in practical activities. A questionnaire with voluntary answer asked the motivation to participate in the monitoring and the evaluation of the activity by the monitors. Nineteen monitors accepted to participate, from 2014 and 2015. For 94.7% of the answers, monitoring reached the expected or better than expected and all the participants indicate monitoring to other college students. This fact shows that this academic activity is a positive factor in the formation of the participants. A positive evaluation associates with the enhanced learning of the discipline content by the monitor, the improving of interpersonal communication and the greater experience in surgery that the monitoring provides. To the students of the discipline, adopting this didactical strategy is better due to the greater empathy that monitors have with the students comparing with the professor

O que está subjacente à escolha do estudante pela profissão médica?

PURPOSE: To determine the reasons for choosing the medical profession by interviewing freshmen medical students from the Faculty of Medicine, University of São Paulo and investigating their socio-economic and psychological profiles, as well as to determine whether there are gender differences. METHOD: One hundred and sixty three freshmen medical students answered a questionnaire regarding their socio-economical profile. Of those, 30 female and 30 male students underwent a face-to-face interview regarding the career choice, the Thematic Apperception Test (TAT) and the 16 Personality Factor Questionnaire (16 PF). The results were analyzed qualitatively and by Mann-Whitney, chi2, Fisher's Exact, and r p coefficient tests. RESULTS: Most students were middle class, catholic, and had physicians in their families. Students of both genders had made an: early choice of the medical career and a persistence in taking exams many times, even after being discouraged. They also showed an awareness of the difficulties and limitations in developing their careers. The study revealed a strong valuation of the humanistic aspects of medicine; openness to new experiences; a deep personal identification with the choice of profession; a critical need for fulfillment in their careers; and conscious and unconscious desires to help people and be recognized for their usefulness, without being narcissistic. Female students were more sensitive (POBJETIVO: Determinar as razões da escolha da profissão médica em um grupo de alunos do primeiro ano de medicina da Faculdade de Medicina da Universidade de São Paulo, investigando o perfil sócio-econômico e psicológico, e as diferenças com relação ao gênero dos alunos. MÉTODO: Cento e sessenta e três alunos responderam a um questionário para avaliar seu perfil sócio-econômico. Destes, 30 mulheres e 30 homens submeteram-se a uma entrevista face a face sobre a escolha da profissão, ao Teste de Apercepção Temática (TAT) e ao teste 16 PF. Os resultados foram analisados qualitativamente e pelos testes de Mann-Whitney, chi2, Fisher's Exact e coeficiente r p. RESULTADOS: A maioria dos estudantes pertence à classe média, são católicos e possuem médicos na família. Estudantes de ambos os gêneros haviam escolhido precocemente a profissão e mostraram persistência para prestar o vestibular, mesmo quando desencorajados por terceiros. O estudo revelou consciência das dificuldades e limitações da carreira médica, bem como grande valorização dos aspectos humanísticos da medicina e espírito aberto a novas experiências. Verificou-se que a profissão ocupa um papel central em suas identidades, a relevância dada à satisfação profissional, o desejo consciente e inconsciente de ajudar os semelhantes e de serem reconhecidos por isso, sem a busca exclusiva de uma gratificação narcísica. As alunas apresentaram maior Brandura (

Studies of the mass composition of cosmic rays and proton-proton interaction cross-sections at ultra-high energies with the Pierre Auger Observatory

In this work, we present an estimate of the cosmic-ray mass composition from the distributions of the depth of the shower maximum (Xmax) measured by the fluorescence detector of the Pierre Auger Observatory. We discuss the sensitivity of the mass composition measurements to the uncertainties in the properties of the hadronic interactions, particularly in the predictions of the particle interaction cross-sections. For this purpose, we adjust the fractions of cosmic-ray mass groups to fit the data with Xmax distributions from air shower simulations. We modify the proton-proton cross-sections at ultra-high energies, and the corresponding air shower simulations with rescaled nucleus-air cross-sections are obtained via Glauber theory. We compare the energy-dependent composition of ultra-high-energy cosmic rays obtained for the different extrapolations of the proton-proton cross-sections from low-energy accelerator data

Study of downward Terrestrial Gamma-ray Flashes with the surface detector of the Pierre Auger Observatory

The surface detector (SD) of the Pierre Auger Observatory, consisting of 1660 water-Cherenkov detectors (WCDs), covers 3000 km2 in the Argentinian pampa. Thanks to the high efficiency of WCDs in detecting gamma rays, it represents a unique instrument for studying downward Terrestrial Gamma-ray Flashes (TGFs) over a large area. Peculiar events, likely related to downward TGFs, were detected at the Auger Observatory. Their experimental signature and time evolution are very different from those of a shower produced by an ultrahigh-energy cosmic ray. They happen in coincidence with low thunderclouds and lightning, and their large deposited energy at the ground is compatible with that of a standard downward TGF with the source a few kilometers above the ground. A new trigger algorithm to increase the TGF-like event statistics was installed in the whole array. The study of the performance of the new trigger system during the lightning season is ongoing and will provide a handle to develop improved algorithms to implement in the Auger upgraded electronic boards. The available data sample, even if small, can give important clues about the TGF production models, in particular, the shape of WCD signals. Moreover, the SD allows us to observe more than one point in the TGF beam, providing information on the emission angle

Combined fit to the spectrum and composition data measured by the Pierre Auger Observatory including magnetic horizon effects

The measurements by the Pierre Auger Observatory of the energy spectrum and mass composition of cosmic rays can be interpreted assuming the presence of two extragalactic source populations, one dominating the flux at energies above a few EeV and the other below. To fit the data ignoring magnetic field effects, the high-energy population needs to accelerate a mixture of nuclei with very hard spectra, at odds with the approximate E$^{-2}$ shape expected from diffusive shock acceleration. The presence of turbulent extragalactic magnetic fields in the region between the closest sources and the Earth can significantly modify the observed CR spectrum with respect to that emitted by the sources, reducing the flux of low-rigidity particles that reach the Earth. We here take into account this magnetic horizon effect in the combined fit of the spectrum and shower depth distributions, exploring the possibility that a spectrum for the high-energy population sources with a shape closer to E$^{-2}$ be able to explain the observations

The dynamic range of the upgraded surface-detector stations of AugerPrime

The detection of ultra-high-energy cosmic rays by means of giant detector arrays is often limited by the saturation of the recorded signals near the impact point of the shower core at the ground, where the particle density dramatically increases. The saturation affects in particular the highest energy events, worsening the systematic uncertainties in the reconstruction of the shower characteristics. The upgrade of the Pierre Auger Observatory, called AugerPrime, includes the installation of an 1-inch Small PhotoMultiplier Tube (SPMT) inside each water-Cherenkov station (WCD) of the surface detector array. The SPMT allows an unambiguous measurement of signals down to about 250m from the shower core, thus reducing the number of events featuring a saturated station to a negligible level. In addition, a 3.8m2 plastic scintillator (Scintillator Surface Detector, SSD) is installed on top of each WCD. The SSD is designed to match the WCD (with SPMT) dynamic range, providing a complementary measurement of the shower components up to the highest energies. In this work, the design and performances of the upgraded AugerPrime surface-detector stations in the extended dynamic range are described, highlighting the accuracy of the measurements. A first analysis employing the unsaturated signals in the event reconstruction is also presented