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Universal slow plasmons and giant field enhancement in atomically thin quasi-two-dimensional metals
Plasmons depend strongly on dimensionality: while plasmons in three-dimensional systems start with finite energy at wavevector q = 0, plasmons in traditional two-dimensional (2D) electron gas disperse as ωp∼q√. However, besides graphene, plasmons in real, atomically thin quasi-2D materials were heretofore not well understood. Here we show that the plasmons in real quasi-2D metals are qualitatively different, being virtually dispersionless for wavevectors of typical experimental interest. This stems from a broken continuous translational symmetry which leads to interband screening; so, dispersionless plasmons are a universal intrinsic phenomenon in quasi-2D metals. Moreover, our ab initio calculations reveal that plasmons of monolayer metallic transition metal dichalcogenides are tunable, long lived, able to sustain field intensity enhancement exceeding 107, and localizable in real space (within ~20 nm) with little spreading over practical measurement time. This opens the possibility of tracking plasmon wave packets in real time for novel imaging techniques in atomically thin materials
Leitura de narrativa policial
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
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 H 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 800 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
<p><b>Context</b>: Lα 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 α” channel centered at 1216 Å used primarily at the beginning of the mission. A small number of flares were observed in this channel.</p>
<p><b>Aims</b>: 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 Lα, 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 Lα 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.</p>
<p><b>Methods</b>: 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 Lα signature. The Lα 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.</p>
<p><b>Results</b>: We find that the Lα flare is characterised by strong, compact footpoints (smaller than the UV ribbons) which correlate well with HXR footpoints. The Lα 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.</p>
<p><b>Conclusions</b>: On the basis of this observation, we conclude that flare and filament observations in the Lα 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.</p>
Uncovered stent does not provoke reactions in renal arteries and renal parenchyma in swines
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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