4,447 research outputs found

    Leitura de narrativa policial

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    VII Seminário de Extensão Universitária da UNILA (SEUNI); VIII Encontro de Iniciação Científica e IV Encontro de Iniciação em Desenvolvimento Tecnológico e Inovação (EICTI 2019) e Seminário de Atividades Formativas da UNILA (SAFOR)O Curso de Leitura de Narrativa Policial foi pensado a partir do desejo de instigar a comunidade acadêmica e o público externo à universidade a exercitar e desenvolver a leitura, trabalhando-a em grupo, de contos ficcionais da literatura do gênero policial. Desta forma, seu objetivo principal é desenvolver a capacidade crítica dos participantes, tanto da leitura como do pensamento. O curso é realizado a partir de aulas expositivas dialógicas, pautadas na bibliografia básica e complementar sugeridas, assim como em debates, discussões, rodas de leitura e, também, na leitura de obra audiovisual e de imagens. Para melhor aproveitamento, foi dividido em dois módulos, para que cada um fosse realizado em um semestre diferente: “A narrativa policial latino-americana” e “A narrativa policial e as mulheres”. Como resultado parcial, obtivemos a frequência regular de, pelo menos, dez participantes no módulo desenvolvido no primeiro semestre, sendo o maior número deles de pessoas com algum vínculo com a UNILA. Apesar de não ser cobrada avaliação e não haver atribuição de nota e, portanto, não ser quantificada a evolução dos alunos, foi notável o desenvolvimento dos que participavam ativamente, com comentários e envolvimento nas discussões. Estudantes relataram que já recorreram ao que havíamos trabalhado em sala para resolver e/ou compreender situações apresentadas em outra aula, com textos que não são literatura policial, mas que foram bem aproveitados no exercício de ler outros gêneros, a partir do pensamento crítico, “desconfiado”, que desenvolvemos ao longo do semestreEstou grata à UNILA pela oportunidade de fazer parte deste projeto e por vivenciar a experiência da sala de aula por uma outra perspectiv

    Data-driven Radiative Hydrodynamic Modeling of the 2014 March 29 X1.0 Solar Flare

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    Spectroscopic observations of solar flares provide critical diagnostics of the physical conditions in the flaring atmosphere. Some key features in observed spectra have not yet been accounted for in existing flare models. Here we report a data-driven simulation of the well-observed X1.0 flare on 2014 March 29 that can reconcile some well-known spectral discrepancies. We analyzed spectra of the flaring region from the Interface Region Imaging Spectrograph (IRIS) in MgII h&k, the Interferometric BIdimensional Spectropolarimeter at the Dunn Solar Telescope (DST/IBIS) in Hα\alpha 6563 \AA\ and CaII 8542 \AA, and the Reuven Ramaty High Energy Solar Spectroscope Imager (RHESSI) in hard X-rays. We constructed a multi-threaded flare loop model and used the electron flux inferred from RHESSI data as the input to the radiative hydrodynamic code RADYN to simulate the atmospheric response. We then synthesized various chromospheric emission lines and compared them with the IRIS and IBIS observations. In general, the synthetic intensities agree with the observed ones, especially near the northern footpoint of the flare. The simulated MgII line profile has narrower wings than the observed one. This discrepancy can be reduced by using a higher microturbulent velocity (27 km/s) in a narrow chromospheric layer. In addition, we found that an increase of electron density in the upper chromosphere within a narrow height range of \approx800 km below the transition region can turn the simulated MgII line core into emission and thus reproduce the single peaked profile, which is a common feature in all IRIS flares.Comment: 14 pages, 18 figures, accepted in Ap

    Observations of a solar flare and filament eruption in Lyman <span class='mathrm'>α</span> and X-rays

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    &lt;p&gt;&lt;b&gt;Context&lt;/b&gt;: L&#945; is a strong chromospheric emission line, which has been relatively rarely observed in flares. The Transition Region and Coronal Explorer (TRACE) has a broad “Lyman &#945;” channel centered at 1216 Å used primarily at the beginning of the mission. A small number of flares were observed in this channel.&lt;/p&gt; &lt;p&gt;&lt;b&gt;Aims&lt;/b&gt;: We aim to characterise the appearance and behaviour of a flare and filament ejection which occurred on 8th September 1999 and was observed by TRACE in L&#945;, as well as by the Yohkoh Soft and Hard X-ray telescopes. We explore the flare energetics and its spatial and temporal evolution. We have in mind the fact that the L&#945; line is a target for the Extreme Ultraviolet Imaging telescope (EUI) which has been selected for the Solar Orbiter mission, as well as the LYOT telescope on the proposed SMESE mission.&lt;/p&gt; &lt;p&gt;&lt;b&gt;Methods&lt;/b&gt;: We use imaging data from the TRACE 1216 Å, 1600 Å and 171 Å channels, and the Yohkoh hard and soft X-ray telescopes. A correction is applied to the TRACE data to obtain a better estimate of the pure L&#945; signature. The L&#945;  power is obtained from a knowledge of the TRACE response function, and the flare electron energy budget is estimated by interpreting Yohkoh/HXT emission in the context of the collisional thick target model.&lt;/p&gt; &lt;p&gt;&lt;b&gt;Results&lt;/b&gt;: We find that the L&#945;  flare is characterised by strong, compact footpoints (smaller than the UV ribbons) which correlate well with HXR footpoints. The L&#945; power radiated by the flare footpoints can be estimated, and is found to be on the order of 1026 erg s-1 at the peak. This is less than 10% of the power inferred for the electrons which generate the co-spatial HXR emission, and can thus readily be provided by them. The early stages of the filament eruption that accompany the flare are also visible, and show a diffuse, roughly circular spreading sheet-like morphology, with embedded denser blobs.&lt;/p&gt; &lt;p&gt;&lt;b&gt;Conclusions&lt;/b&gt;: On the basis of this observation, we conclude that flare and filament observations in the L&#945; line with the planned EUI and LYOT telescopes will provide valuable insight into solar flare evolution and energetics, especially when accompanied by HXR imaging and spectroscopy.&lt;/p&gt

    Uncovered stent does not provoke reactions in renal arteries and renal parenchyma in swines

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    OBJECTIVE: To assess the histological changes of the aorta, the renal arteries and the renal parenchyma in swine, induced by a metalic uncovered stent implanted in transrenal position in the abdominal aorta. METHODS: Ten pigs with a mean weight of 86.6 kg and mean age of 6 months underwent implantation of metal stent graft placed in the aorta at the level of the renal arteries after 100 days of implantation. The self-expanding stents were released by laparotomy. Anatomic and histological analyses of the abdominal aorta, the renal arteries and the renal parenchyma were performed. Histological slices were performed in the following sites: 1) transitional zone between the aorta with and without stent graft; 2) portion of the renal arteries ostia; 3) renal parenchyma. The slices were stained through the hematoxylin and eosin stain technique and analyzed according the protocol of histological analyses applied in the clinical practice of pathology labs. RESULTS: The macroscopic findings showed thickening of the aortic wall; patent renal arteries; and normal anatomic renal structures. Microscopic analyses, close to the stents, showed thickening of the vascular wall, renal arteries without changes, and preserved renal parenchyma. CONCLUSION: The uncovered stainless steel stent caused a significant inflammatory reaction with thickening of the aortic wall. However, the renal arteries remained patent and the renal parenchyma did not present embolic or ischemic changes.OBJETIVO: Avaliar as alterações histológicas da aorta, artéria renal e parênquima renal, em suínos, induzidos pelo stent metálico descoberto implantado em localização transrenal na aorta abdominal. MÉTODOS: Foram utilizados 10 suínos com peso médio de 86,6 quilos e idade média de 6 meses, submetidos a implante de stent metálico posicionado na aorta, no nível das artérias renais, após 100 dias do implante. Os stents foram liberados por auto-expansão com laparotomia. Foram realizadas análises anatômicas e histológicas da aorta abdominal, artérias renais e parênquima renal. Os cortes histológicos foram realizados nos seguintes locais: 1) transição entre a aorta normal e aorta contendo stent; 2) porção contendo os óstios das artérias renais, 3) parênquima renal. As lâminas foram coradas pela técnica da hematoxilina e eosina e analisadas conforme protocolo de análise histológica aplicada na prática clínica dos laboratórios de patologia. RESULTADOS: Os achados macroscópicos revelaram espessamento da parede aórtica; artérias renais pérvias; estrutura anatômica renal normal. Análises microscópicas, próximas aos stents, evidenciaram espessamento da parede vascular, artérias renais sem alterações e parênquima renal preservado. CONCLUSÃO: O stent de aço inoxidável descoberto produziu importante reação inflamatória com espessamento da parede da aorta. No entanto, as artérias renais permaneceram pérvias e o parênquima renal sem alterações isquêmicas ou embólicas.INCOR Hospital Maternidade Marieta Konder BonhausemUNIFESPUNIFESP - Escola Paulista de Medicina São PauloUniversidade do Estado de Santa Catarina Hospital VeterinárioLaboratório RochaHospital São JoséSanta CasaUNIFESP, EPMSciEL
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