998 resultados para Aquecimento coronal


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In the present work, we have studied the nature of the physical processes of the coronal heating, considering as basis significant samples of single and binary evolved stars, that have been achieved with the ROSAT satellite. In a total of 191 simple stars were studied, classified in the literature as giants with spectral type F, G and K. The results were compared with those obtained from 106 evolved stars of spectral type F, G and K, which belong to the spectroscopic binary systems. Accurate measurements on rotation and information about binarity were obtained from De Medeiros s catalog. We have analysed the behavior of the coronal activity in function of diverse stellar parameters. With the purpose to better clarify the profile of the stars evolution, the HR diagram was built for the two samples of stars, the single and the binary ones. The evolved traces added in the diagram were obtained from the Toulouse-Geneve code, Nascimento et al. (2000). The stars were segregated in this diagram not only in range of rotational speed but also in range of X-ray flux. Our analysis shows clearly that the single stars and the binary ones have coronal activity controlled by physical process independent on the rotation. Non magnetic processes seem to be strongly influencing the coronal heating. For the binary stars, we have also studied the behavior of the coronal emission as a function of orbital parameters, such as period and eccentricity, in which it was revealed the existence of a discontinuity in the emission of X-rays around an orbital period of 100 days. The study helped to conclude that circular orbits of the binary stars are presented as a necessary property for the existence of a higher level ofX-rays emission, suggesting that the effect of the gravitational tide has an important role in the coronal activity level. When applied the Kolmogorov-Smirnov test (KS test ) for the Vsini and FX parameters to the samples of single and binary stars, we could evidence very relevant aspects for the understanding of the mechanisms inherent to the coronal activity. For the Vsini parameter, the differences between the single stars and the binary ones for rotation over 6.3 km/s were really remarkable. We believe, therefore, that the existence of gravitational tide is, at least, one of the factors that most contribute for this behavior. About the X-rays flux, the KS test showed that the behavior of the single and the binary stars, regarding the coronal activity, comes from the same origin

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In the present work we study the processes of heating in the high stellar atmosphere, with base in an analysis of behavior of the cromospheric and coronal emission for a sample of single stars classified as giant in the literature. The evolutionary status of the stars of the sample was determined from HIPPARCOS satellite trigonometric parallax measurements and from the Toulouse Genéve code. In this study we show the form of behavior of the CaII emission flux in spectral lines H and K F(CaII) and the X-ray emission flux in function of the rotation, number of Rossby Ro and depth in mass of the convective envelope. In this analysis we show that while the cromospheric activity is dominated clearly by a physical process of heating associated with the rotation, like a magnetic field produced by dynamo effect, the coronal activity seems to be influenced for a mechanism independent of the rotation. We show also that the effective role of the depth in massa of the convective envelope on the stellar activity has an important effect in the responsible physical process for the behavior of the activity in the atmosphere of the stars.

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In this dissertation we propose a Teaching Unit of Physics to teach content through environmental discussions of the greenhouse effect and global warming. This teaching unit is based on a problem-methodological intervention from the application of the method of the Arch of Charles Maguerez. The methodological foundations of the thesis are embedded in action research and this is structured in five chapters: the first chapter deals with the Physical Environment (FMA) as a subject in Degree Courses in Physics in Brazil, bringing the concern of how this discipline has been taught. We started the first chapter explaining the reasons behind the inclusion of the discipline of Physical Environment in a Physics Degree Courses. Then we did a search on the websites of Institutions of Higher Education, to know of the existence or not of this discipline on curricular. We then analyzed the menus to see what bibliographies are being adopted and what content of Physics are being worked, and how it has been done. The courses surveyed were those of Federal and Federal Institutes Universities. Thus ended the first chapter. Given the inseparability between studies in Physics Teaching and studies on competencies, skills and significant learning, wrote the second chapter. In this chapter we discuss the challenge of converting information into knowledge. Initially on initial teacher training, because even if this is not our focus, the study is a discipline on the upper reaches, therefore, offered to future teachers. Then we talked about the culture of knowledge, where we emphasize the use of a teaching approach that promotes meanings taught by content and make sense to the student. We finished the third chapter, making some considerations on skills and abilities, in order to identify what skills and competencies were developed and worked during and after the implementation of Curriculum Unit. The third chapter is the result of a literature review and study of the radioactive EarthSun interaction. The subjects researched approach from the generation of energy in the sun to topics stain solar coronal mass ejections, solar wind, black body radiation, Wien displacement law, Stefan-Boltzmann Law, greenhouse effect and global warming. This chapter deals with material support for the teacher of the aforementioned discipline. The fourth chapter talks about the arc method of Charles Maguerez; Here we explain the structure of each of the five steps of the Arc and how to use them in teaching. We also show another version of this method adapted by Bordenave. In the fifth and final chapter brought a description of how the method of Arc was used in physics classes of Environment, with students majoring in Physics IFRN Campus Santa Cruz. Here, in this chapter, a transcript of classes to show how was the application of a problem-based methodology in the teaching of content proposed for Physics Teaching Unit from the environmental discussion about the greenhouse effect and global warming phenomena

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The premature fusion of unilateral coronal suture can cause a significant asymmetry of the craniofacial skeleton, with an oblique deviation of the cranial base that negatively impacts soft tissue facial symmetry. The purpose of this study was to assess facial symmetry obtained in patients with unilateral coronal synostosis (UCS) surgically treated by 2 different techniques. We hypothesized that nasal deviation should not be addressed in a primary surgical correction of UCS. Consecutive UCS patients were enrolled in a prospective study and randomly divided into 2 groups. In group 1, the patients underwent total frontal reconstruction and transferring of onlay bone grafts to the recessive superior orbital rim (n = 7), and in group 2, the patients underwent total frontal reconstruction and unilateral fronto-orbital advancement (n = 5). Computerized photogrammetric analysis measured vertical and horizontal axis of the nose and the orbital globe in the preoperative and postoperative periods. Intragroup and intergroup comparisons were performed. Intragroup preoperative and postoperative comparisons showed a significant (all P < 0.05) reduction of the nasal axis and the orbital-globe axis in the postoperative period in the 2 groups. Intergroup comparisons showed no significant difference (all P > 0.05). Facial symmetry was achieved in the patients with UCS who underwent surgery regardless of surgical approach evaluated here. Our data showed a significant improvement in nasal and orbital-globe deviation, leading us to question the necessity of primary nasal correction in these patients.

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This study evaluated the sealing ability of different lengths of remaining root canal filling and post space preparation against coronal leakage of Enterococcus faecalis. Forty-one roots of maxillary incisors were biomechanically prepared, maintaining standardized canal diameter at the middle and coronal thirds. The roots were autoclaved and all subsequent steps were undertaken in a laminar flow chamber. The canals of 33 roots were obturated with AH Plus sealer and gutta-percha. The root canal fillings were reduced to 3 predetermined lengths (n=11): G1=6 mm, G2=4 mm and G3=2 mm. The remaining roots served as positive and negative controls. Bacterial leakage test apparatuses were fabricated with the roots attached to Eppendorf tubes keeping 2 mm of apex submerged in BHI in glass flasks. The specimens received an E. faecalis inoculum of 1 x 107 cfu/mL every 3 days and were observed for bacterial leakage daily during 60 days. Data were submitted to ANOVA, Tukey's test and Fisher's test. At 60 days, G1 (6 mm) and G2 (4 mm) presented statistically similar results (p>0.05) (54.4% of specimens with bacterial leakage) and both groups differed significantly (p<0.01) from G3 (2 mm), which presented 100% of specimens with E. faecalis leakage. It may be concluded that the shortest endodontic obturation remnant leaked considerably more than the other lengths, although none of the tested conditions avoids coronal leakage of E. faecalis.

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This study compared the coronal and apical leakage of AH Plus with gutta-percha to that of Epiphany with Resilon. Twenty-four single rooted teeth were instrumented and divided into 2 groups according to the solutions for smear layer removal and the obturation materials employed: Group A - 17% EDTA-T and AH Plus with gutta-percha; Group B - primer and Epiphany with Resilon. The Group B specimens were light-cured in the coronal area for 20 s. The external root surfaces were covered with a double layer of ethyl cyanoacrylate, except for the apical foramen and the cavity access. The teeth were immersed in 0.5% methylene blue for 48 h. The specimens were rinsed, dried and axially split for dye penetration measurement with the ImageLab 2.3 software. The t-test showed no significant differences for coronal leakage between the groups, but there were significant differences for apical leakage between the groups (P < 0.05). AH Plus with gutta-percha and Epiphany with Resilon provided the same coronal seal, whereas Epiphany with Resilon provided the best apical seal.

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JUSTIFICATIVA E OBJETIVOS: Hipotermia intra-operatória é complicação frequente, favorecida por operação abdominal. A eficácia da associação dos métodos de aquecimento por condução e convecção na prevenção de hipotermia e seus efeitos no período de recuperação pós-operatória foram os objetivos deste estudo. MÉTODO: Quarenta e três pacientes de ambos os sexos de 18 a 88 anos de idade, submetidos à laparotomia xifopúbica sob anestesia geral e monitorização da temperatura esofágica, foram distribuídos de modo aleatório em dois grupos de aquecimento: COND (n = 24), com colchão de circulação de água a 37°C no dorso e COND + CONV (n = 19), com a mesma condição associada à manta de ar aquecido a 42°C sobre o tórax e membros superiores. Analisados peso, sexo, idade, duração da operação e anestesia, temperaturas na indução anestésica (Mi), horas consecutiva (M1, M2), final da operação (Mfo) e anestesia (Mfa), entrada (Me-REC) e saída (Ms-REC) da recuperação pós-anestésica (SRPA), além das incidências de tremores e queixas de frio no pós-operatório. RESULTADOS: Os grupos foram semelhantes em todas as variáveis analisadas, exceto nas temperaturas em M2, M3, M4, Mfo e Mfa. O grupo COND reduziu a temperatura a partir da segunda hora da indução anestésica, mas o grupo COND + CONV só na quarta hora. Em COND, observou-se hipotermia na entrada e saída da SRPA. CONCLUSÕES: Associar métodos de aquecimento retardou a instalação e diminui a intensidade da hipotermia intra-operatória, mas não reduziu a incidência das queixas de frio e tremores.

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This work discusses the determination of the breathing patterns in time sequence of images obtained from magnetic resonance (MR) and their use in the temporal registration of coronal and sagittal images. The registration is made without the use of any triggering information and any special gas to enhance the contrast. The temporal sequences of images are acquired in free breathing. The real movement of the lung has never been seen directly, as it is totally dependent on its surrounding muscles and collapses without them. The visualization of the lung in motion is an actual topic of research in medicine. The lung movement is not periodic and it is susceptible to variations in the degree of respiration. Compared to computerized tomography (CT), MR imaging involves longer acquisition times and it is preferable because it does not involve radiation. As coronal and sagittal sequences of images are orthogonal to each other, their intersection corresponds to a segment in the three-dimensional space. The registration is based on the analysis of this intersection segment. A time sequence of this intersection segment can be stacked, defining a two-dimension spatio-temporal (2DST) image. The algorithm proposed in this work can detect asynchronous movements of the internal lung structures and lung surrounding organs. It is assumed that the diaphragmatic movement is the principal movement and all the lung structures move almost synchronously. The synchronization is performed through a pattern named respiratory function. This pattern is obtained by processing a 2DST image. An interval Hough transform algorithm searches for synchronized movements with the respiratory function. A greedy active contour algorithm adjusts small discrepancies originated by asynchronous movements in the respiratory patterns. The output is a set of respiratory patterns. Finally, the composition of coronal and sagittal image pairs that are in the same breathing phase is realized by comparing of respiratory patterns originated from diaphragmatic and upper boundary surfaces. When available, the respiratory patterns associated to lung internal structures are also used. The results of the proposed method are compared with the pixel-by-pixel comparison method. The proposed method increases the number of registered pairs representing composed images and allows an easy check of the breathing phase. (C) 2010 Elsevier Ltd. All rights reserved.

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Objectives: The aim of this study was to assess the fracture resistance of endodontically treated teeth submitted to bleaching with 38% hydrogen peroxide activated by light-emitting diode (LED)-laser system. Methods: Fifty maxillary incisors were endodontically treated, received a zinc phosphate barrier and were embedded in acrylic resin until cemento-enamel junction. The specimens were distributed into five groups (n = 10) according to the number of bleaching sessions: GI, no treatment (control); GII, one session; GIII, two sessions; GIV, three sessions and GV, four sessions. The whitening gel was applied to the buccal surface of the tooth and inside the pulp chamber for three times in each session, followed by LED-laser activation. Specimens were submitted to the fracture resistance test (kN) and data were submitted to the Tukey-Kramer multiple comparisons test. Results: No significant difference (p > 0.05) was found between GI (0.71 +/- 0.30) and GII (0.65 +/- 0.13), which presented the highest strength values to fracture. Groups III (0.35 +/- 0.17), IV (0.23 +/- 0.13) and V (0.38 +/- 0.15) showed lower resistance to fracture (p < 0.01) when compared to GI and GII. Conclusions: The fracture resistance of endodontically treated teeth decreased after two sessions of bleaching with 38% hydrogen peroxide activated by LED-laser system. (c) 2008 Elsevier Ltd. All rights reserved.

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O conhecimento da localização da artéria etmoidal anterior (AEA) constitui etapa importante na cirurgia do recesso do seio frontal e do etmóide anterior. A tomografia computadorizada (TC), em especial no plano coronal pode fornecer reparos anatômicos que identificam o trajeto da AEA. OBJETIVO: Identificar os reparos anatômicos que caracterizam o trajeto da AEA na parede medial da órbita e na parede lateral da fossa olfatória. Verificar a correlação entre a presença de pneumatização supra-orbitária e a visualização do etmoidal anterior (canal da AEA). CASUÍSTICA E MÉTODOS: Estudo retrospectivo de 198 tomografias computadorizadas dos seios paranasais no plano coronal do período de agosto a dezembro de 2006. RESULTADOS: Pneumatização supra-orbitária foi identificada em 35% (70 exames). O canal da AEA foi caracterizado em 41% (81 exames). O sulco etmoidal anterior foi visualizado em 98% (194 dos exames) e o forame etmoidal anterior foi identificado em todos os exames (100%). CONCLUSÃO: O forame etmoidal anterior e o sulco etmoidal anterior foram referências anatômicas presentes em quase 100% dos exames avaliados. Houve correlação entre a presença de pneumatização supra-orbitária e a caracterização do canal da AEA.

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O ambiente da criação intensiva de suínos influencia diretamente as condições de conforto e bem-estar animal; ambiente estressante provoca várias respostas, dependendo da capacidade de adaptação do animal, e as instalações têm como finalidade minimizar esses problemas. Objetivou-se, com este trabalho, avaliar o comportamento fisiológico e os índices zootécnicos das matrizes e dos leitões, com a utilização dos sistemas de aquecimento e resfriamento do piso. O delineamento experimental utilizado foi o inteiramente casualizado, no esquema fatorial em parcelas subdivididas, com cinco repetições para os tratamentos: piso aquecido para os leitões e resfriado para as matrizes (PCARA), piso sem aquecimento para os leitões e resfriado para as matrizes (PRCA) e piso sem modificação (PSMCA). Foram avaliados os parâmetros térmicos e fisiológicos das matrizes dos tratamentos PRCA e PCARA. O tratamento PRCA apresentou o melhor resultado, proporcionando maior conforto térmico para os animais, que atingiram em média um ganho 233 gramas por dia.

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O presente trabalho é constituído por dois temas principais: as máquinas de absorção LiBr/H2O e NH3/H2O, e os sistemas solares capazes de fornecer calor aos geradores das máquinas. Na primeira parte são referidos os diferentes sistemas de absorção, tendo sido descrito o seu funcionamento com os respectivos esquemas de princípio tendo sempre em atenção a sua optimização energética. Fez-se um estudo sobre os processos termodinâmicos associados ao funcionamento do ciclo NH3/H2O, para as temperaturas nos diferentes componentes aplicados num sistema de climatização Após esta análise termodinâmica foi realizado um estudo concreto para uma máquina, com a potência frigorífica de 16,9 kW, valor real da máquina de absorção ROBUR Modelo GAHP-AR, que servirá de base para a implementação de um sistema de fornecimento de calor, obtido com um conjunto de painéis solares. A segunda parte deste trabalho é dedicada aos sistemas solares, com uma análise dos diversos tipos de painéis, e respectivo funcionamento. Procurámos realizar o dimensionamento e optimização dessa instalação de captação de energia solar, de modo a captar cargas térmicas para um circuito de água, e assim fornecer a energia necessária ao correcto funcionamento do gerador do sistema de absorção.

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O objeto da presente tese é o estudo comparativo do desempenho de soluções de aquecimento de águas quentes sanitárias (AQS) de dois sistemas solares alternativos, um sistema do tipo Termossifão “versus” um sistema de Circulação Forçada. Foi realizada uma campanha de medições durante um ano, que permitiu avaliar o desempenho dos dois sistemas e as poupanças que resultaram da utilização de um sistema solar, em comparação com um sistema convencional de aquecimento de águas quentes com recurso a gás natural. Estes dados experimentais foram confrontados com os resultados de simulação fornecidos por software dedicado ao cálculo de energia em sistemas solares, conhecido como SolTerm. Concluiu-se que, para o perfil de consumo estabelecido, os sistemas de Circulação Forçada e de Termossifão Reais, tiveram um desempenho equivalente. Na simulação realizada no SolTerm, o sistema Termossifão foi mais eficiente, com um fração solar de 69,7%. Já para o sistema de Circulação Forçada a fração solar foi de 63,3%, com uma diferença de produtividade anual de 67 kWh/m2 de coletor. Contrariamente ao que era previsto pelo SolTerm, ambos os sistemas Reais tiveram desempenhos inferiores, obtendo frações solares de 55,8% e 58,5% para o Termossifão e Circulação Forçado respetivamente. Para o Termossifão esta diferença foi mais acentuada, ao passo que no Circulação Forçada se aproximou do comportamento previsto na simulação.

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Trabalho Final de Mestrado para obtenção do grau de Mestre em Engenharia Mecânica

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O presente trabalho tem como principal objectivo o estudo da possibilidade de recuperação de calor de um efluente proveniente do tratamento primário da fábrica do grupo Portucel Soporcel (fábrica produtora de pasta de papel), para o aquecimento da corrente de lamas do digestor anaeróbio da SimRia S.A. – ETAR Norte, (ambas localizadas em Cacia, distrito de Aveiro). A solução consiste na implementação de um sistema de permuta térmica entre estas duas correntes, constituído fundamentalmente por dois permutadores de placas em espiral, montados em paralelo que operam em contra-corrente. Segundo este novo sistema de aquecimento, as lamas abandonam o digestor anaeróbio da mesma ETAR a um caudal de 110 m3/h, que se dividirá em duas linhas, sendo admitidas em cada permutador a 55 m3/h e a uma temperatura de 32 ºC regressando ao digestor a uma temperatura de 37 ºC (temperatura óptima a que ocorre a digestão anaeróbia das lamas). O efluente disponível, abandona o tratamento primário da Portucel, a 45 ºC e é encaminhado até aos permutadores da SimRia S.A., onde vai trocar calor com as lamas e regressa à Portucel a 40ºC, sendo admitido nas torres de arrefecimento da fábrica de papel. A nova instalação proposta pretende substituir a actual existente na ETAR em causa, em que a corrente de água que aquece as lamas, circula num circuito fechado entre um único permutador e uma caldeira, alimentada com o biogás que se produz no digestor anaeróbio, e que é responsável pelo controlo da temperatura da corrente de água. Pretende-se que a implementação deste novo método de aquecimento de lamas seja uma alternativa económica relativamente ao actual sistema, uma vez que vai substituir a corrente de biogás alimentada à caldeira podendo este recurso ser transformado em energia eléctrica e posteriormente comercializada. A análise financeira realizada ao projecto demonstrou que o projecto é rentável, uma vez que, a diferença entre todos ganhos e custos ao fim dos 10 anos de vida útil estimados é de cerca de 150 000,0 €. O período de retorno do investimento é alcançado no final dos primeiros 6 anos e a taxa interna de rentabilidade obtida foi de 36 %. Posteriormente incluiu-se neste estudo a possibilidade de tratamento das lamas geradas na fábrica da Portucel na ETAR da SimRia recorrendo a um terceiro digestor. Conclui-se que se trata duma opção vantajosa, uma vez que permite obter um caudal de biogás 44 m3/h, que convertido em potência permite obter 150 kW que poderá ser aproveitado para produção de energia ou comercializado gerando uma receita adicional de 130 000,0 €/ano para as entidades envolvidas.