160 resultados para 220208 Magnetismo
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Programa de doctorado: Tecnología industrial
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UANL
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UANL
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Este vídeo muestra los conceptos básicos del magnetismo, con sencillas experiencias de manipulación de imágenes y brújulas.
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Explicación del magnetismo a través de la utilización de los imanes y de la explicación del porqué de su funcionamiento. Muestra también los diferentes usos del imán que han ido evolucionando en el electromagnetismo o en los generadores de electricidad.
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Se pretende abordar el conjunto de problemas que presenta la enseñanza de la electricidad y el magnetismo como parte fundamental de la Física en educación secundaria. Se proponen soluciones realistas y contrastadas que buscan un aprendizaje significativo y motivador al relacionar la disciplina con el contexto del alumno; en esta obra, se recogen las últimas aportaciones en el campo de la didáctica de las ciencias experimentales, se incluyen ejemplos y actividades para su aplicación en el aula. Se ofrecen diseños curriculares para llevar a cabo en los distintos ciclos de la enseñanza secundaria, incluido Bachillerato, en los que se incluyen criterios de selección de contenidos, propuestas de secuenciación, un desarrollo de la propuesta y orientaciones didácticas y metodológicas.
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Se realiza un breve recorrido por los hitos que jalonaron el descubrimiento del campo magnético, y se proponen sencillos experimentos para estimular en los escolares el razonamiento lógico y la comprensión de lo que observan. Está destinada para la formación técnica del profesor y para la aplicación práctica de lo aprendido mediante recursos accesibles y cercanos a los alumnos.
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Neste trabalho foram estudadas as propriedades morfológicas, estruturais e magnéticas de nanoestruturas de Fe crescidas em Si(111) vicinal. A análise de superfície foi feita usando microscopia de força atômica e microscopia de tunelamento, e as medidas de caracterização estrutural, por espectroscopia de absorção de raios-X. As propriedades magnéticas foram investigadas usando dois métodos distintos: efeito Kerr magneto-óptico e magnetômetro de força de gradiente alternado. Os substratos foram preparados quimicamente com uma solução NH4F e caracterizados por microscopia de força atômica. As análises morfológicas das superfícies permitiram classificá-las em dois grupos: Si(111)- monoatômicos e Si(111)-poliatômicos. Filmes finos de ferro de 1.5, 3, 6 e 12 nm foram crescidos sobre eles. A análise das superfícies indicou dois modos diferentes de crescimento do ferro; o sistema Fe(x)Si(111)-monoatômico resulta em grãos de ferro aleatoriamente distribuídos, e o sistema Fe(x)Si(111)-poliatômico em nanogrãos de ferro alongados na direção perpendicular aos degraus, auto-organizados. Particularmente no filme Fe(3 nm)/Si(111)-poliatômico, ao redor de metade dos grãos estão alinhados ao longo da direção [110] , ou seja, paralelo aos degraus. O padrão de nanogrãos de ferro alongados orientados perpendicular aos degraus foi interpretado com uma conseqüência da anisotropia induzida durante o processo de deposição e a topologia do substrato Si(111)-poliatômico. Uma forte relação entre a morfologia e a resposta magnética dos filmes foi encontrada. Um modelo fenomenológico foi utilizado para interpretar os dados experimentais da magnetização, e uma excelente concordância entre as curvas experimentais e calculadas foi obtida.
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In this thesis we analyze the effects that the presence of a near gas giant planet can cause in its host star. It has been argued that the star planet interaction can cause changes in the coronal and chromospheric stellar activity. With this in mind, we analyze a sample of 53 extrasolar planets orbiting F, G and K main sequence stars, among them three super-Earths. In this analysis, we look for evidence of changes in the chromospheric activity due to the proximity of the giant planet. We show that, so far, there is not enough evidence to support such a hypothesis. Making use of the same sample and also taking in account available data for the Solar System, we revisit the so-called magnetic Bode s law. This law proposes the existence of a direct relationship between magnetism and rotation. By using estimations for the stellar and planetary magnetic momentM and the angular momentumL, we construct a Blackett s diagram (logL logM). In this diagram is evident that the magnetic Bode s law is valid for both the Solar System and the new planetary systems
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The study physical process that control the stellar evolution is strength influenced by several stellar parameters, like as rotational velocity, convective envelope mass deepening, and magnetic field intensity. In this study we analyzed the interconnection of some stellar parameters, as Lithium abundance A(Li), chromospheric activity and magnetic field intensity as well as the variation of these parameters as a function of age, rotational velocity, and the convective envelope mass deepening for a selected sample of solar analogs and twins stars. In particular, we analyzed the convective envelope mass deepening and the dispersion of lithium abundance for these stars. We also studied the evolution of rotation in subgiants stars, because its belong to the following evolutionary stage of solar analogs, and twins stars. For this analyze, we compute evolutionary models with the TGEC code to derive the evolutionary stage, as well as the convective envelope mass deepening, and derive more precisely the stellar mass, and age for this 118 stars. Our Investigation shows a considerable dispersion of lithium abundance for the solar analogs stars. We also realize that this dispersion is not by the convective zone deep, in this way we observed which the scattering of A(Li) can not be explained by classical theories of mixing in the convective zone. In conclusion we have that are necessary extra-mixing process to explain this decrease of Lithium abundance in solar analogs and twins stars. We analyzed the subgiant stars because this are the subsequent evolutionary stage after the solar analogs and twins stars. For this analysis, we compute the rotational period for 30 subgiants stars observed by Co- RoT satellite. For this task we apply two different methods: Lomb-Scargle algorithm, and the Plavchan Periodogram. We apply the TGEC code we compute models with internal distribution of angular momentum to confront the predict results with the models, and the observational results. With this analyze, we showed which solid body rotation models are incompatible with the physical interpretation of observational results. As a result of our study we still concluded that the magnetic field, convective envelope mass deepening, and internal redistribution of angular momentum are essential to explain the evolution of low-mass stars, and its observational characteristics. Based on population synthesis simulation, we concluded that the solar neighborhood presents a considerable quantity of solar twins when compared with the discovered set nowadays. Altogether we foresee the existence around 400 solar analogs in the solar neighborhood (distance of 100 pc). We also study the angular momentum of solar analogs and twins, in this study we concluded that added angular momentum from a Jupiter type planet, putted in the Jupiter position, is not enough to explain the angular momentum predicted by Kraft law (Kraft 1970)
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Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)
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Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)
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Mode of access: Internet.
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Mode of access: Internet.