Caos e fractais na sala de aula

O objectivo deste trabalho é o estudo do tema Caos e Fractais, com o propósito fundamental da sua implementação na sala de aula ou outro ambiente do Ensino Secundário. Com esse fim, é feita uma abordagem teórica dos conteúdos e são apresentadas algumas actividades a desenvolver com os alunos daquele nível de ensino. A introdução dos conceitos é feita de modo a possibilitar a sua leitura por um público mais geral, onde se incluem os alunos mais interessados e curiosos no tema. O estudo é acompanhado, sempre que possível, de exemplos e ilustrações gráficas. Para tal, foi utilizado o software Maxima (software livre) e outras aplicações interactivas disponíveis na Internet. ABSTRACT: The aim of this work is to study the theme of Chaos and Fractals, with the fundamental purpose of its implementation in the classroom, or in other environments of secondary school education. To carry out this aim a theoretical outlook of the contents will be provided alongside some activities to be undergone with students of that school level. The introduction to these concepts is open to the understanding of a larger audience, where we can include the most interested and curious students in this issue. The study is accompanied, whenever possible, with examples and graphics. To do so, the Maxima software (free software) was used, besides other interactive applications available on the Internet.

Temperature-averaged and total free-free Gaunt factors for κ and Maxwellian distributions of electrons

Aims. Optically thin plasmas may deviate from thermal equilibrium and thus, electrons (and ions) are no longer described by the Maxwellian distribution. Instead they can be described by κ-distributions. The free-free spectrum and radiative losses depend on the temperature-averaged (over the electrons distribution) and total Gaunt factors, respectively. Thus, there is a need to calculate and make available these factors to be used by any software that deals with plasma emission. Methods. We recalculated the free-free Gaunt factor for a wide range of energies and frequencies using hypergeometric functions of complex arguments and the Clenshaw recurrence formula technique combined with approximations whenever the difference between the initial and final electron energies is smaller than 10−10 in units of z2Ry. We used double and quadruple precisions. The temperature- averaged and total Gaunt factors calculations make use of the Gauss-Laguerre integration with 128 nodes. Results. The temperature-averaged and total Gaunt factors depend on the κ parameter, which shows increasing deviations (with respect to the results obtained with the use of the Maxwellian distribution) with decreasing κ. Tables of these Gaunt factors are provided.