La Guerra de las Galaxias como metodología innovadora para mejorar la motivación

Numerosos estudiantes ven el estudio como algo aburrido, se sienten desmotivados. El docente no puede limitarse a aceptar la situación como un espectador. Es nuestra realidad y de la misma forma que cada estudiante debe responsabilizarse de su propia educación, los profesores tenemos que responsabilizarnos de cambiar ese sentimiento. Para ello se analizará en primer lugar el significado del término motivación y cuáles son los factores en los que los profesores podemos influir. Se verá que una de las formas de intervención es la innovación, por lo que también se analizará el vocablo y se discutirá qué constituye innovación y qué no. Por tanto, el docente se enfrenta a diario con la necesidad de encontrar nuevas formas de enseñar, que capten la atención de los alumnos. Se dice que no hay nada nuevo bajo el sol; sin embargo, hay que ser capaz de encontrar nuevos usos a con recursos que ya existen. Con el presente trabajo se pretende dar respuesta a esa necesidad. Se plantea el uso de una metodología que propone una innovación continua que consiste en establecer un paralelismo entre un relato o una historia y una unidad didáctica de la asignatura de Tecnología. Como historia se ha escogido la conocida película “La Guerra de las Galaxias” y el curso de referencia será el primer curso de Educación Secundaria Obligatoria (1º E.S.O.). En concreto se presenta un material adaptado con fotografías de la película, ejemplos inspirados en la saga y otras adaptaciones educativas. Con ello se consigue una sorpresa continua para el estudiante y así mantener su atención, facilitando su aprendizaje. Se tiene hecho parte del camino, aunque no todo. En este punto, se hace necesario introducir algunas medidas suplementarias, que refuercen y complementen esta metodología y que nos impidan apartarnos del objetivo pretendido: que los alumnos aprendan de manera significativa. ¿Quién dijo que estudiar es aburrido? A number of students see studying as something boring. The teacher cannot be a spectator. It is our reality and, so on one hand, the student has the responsibility of building his education and on the other, the teacher must change that feeling. In order to this, the term motivation will be analysed, and also which are the related aspects in which we have some influence. One of those ways of intervention is motivation. It is for that word, innovation will be analysed as well, discussing what innovation is and what is not. Therefore, teachers face, day by day, the need of finding new ways of teaching for students to pay attention in classes. As people say, there is nothing new under the sun; however, new uses for existing resources are required. This paper pretends to solve that problem. A continuous innovating methodology is set, consisting in establishing a parallelism between a story or tale and a didactic unit in Technology subject. As a story, the well-known film “Star Wars” is chosen, and as a reference course, the first course of Educación Secundaria Obligatoria (1st E.S.O.). Specifically, we introduce an adapted material with pictures from the movie, saga inspired examples and, some other educational adaptations. With it, students are continuously surprised and their attention grabbed, making his learning easier. Part of the problem is solved, but there is a long way to go. At this point, some supplementary steps are needed, in order to enforce and complement this methodology, and to avoid getting far away from the attempted objective: students learning in a significant way. Who said studying is annoying?

Discovery of a low-mass brown dwarf companion of the young nearby star G196-3.

A substellar-mass object in orbit at about 300 astronomical units from the young low-mass star G 196-3 was detected by direct imaging. Optical and infrared photometry and low- and intermediate-resolution spectroscopy of the faint companion, hereafter referred to as G 196-3B, confirm its cool atmosphere ?15 Jupiter masses. The separation and allow its mass to be estimated at 25?10 between the objects and their mass ratio suggest the fragmentation of a collapsing cloud as the most likely origin for G 196-3B, but alternatively it could have originated from a protoplanetary disc that has been dissipated. Whatever the formation process was, the young age of the primary star (about 100 million years) demonstrates that substellar companions can form on short time scales.

Let's Gain More Confidence Of Clinicians With Our Colorful Contours: Blood Flow Simulation In Arteries Using Abaqus & STAR-CCM+

The objective of the current work is to present the results of several numerical simulations of pulsatile blood flow in healthy and diseased arteries and compare with clinical expectations. Different realistic and physiological aspects such as blood flow interaction with arterial walls, effect of heart movement, cardiovascular autoregulation, arterial walls' hyperelasticity and cardiovascular disorders have been incorporated in the models thanks to a direct coupling of Abaqus and STAR-CCM+. Comparisons of implicit and explicit coupling methods in cardiovascular simulations have been discussed. An in-house methodology combined with explicit FSI coupling has reduced considerably calculation time while the simulations stay realistic and reliable for clinicians

Optimización del análisis best-estimate de un elemento combustible BWR con el código STAR-CCM+

The objective of the project is the evaluation of the code STAR-CCM +, as well as the establishment of guidelines and standardized procedures for the discretization of the area of study and the selection of physical models suitable for the simulation of BWR fuel. For this purpose several of BFBT experiments have simulated provide a data base for the development of experiments for measuring distribution of fractions of holes to changes in power in order to find the most appropriate models for the simulation of the problem.

Star dust memories, or how to detect allergen traces in powder foods

Allergies and food intolerances are at the forefront of institutional interest (European Regulation No 1169/2011) for their impact on consumer health. Allergies to peanuts and other nuts and gluten intolerance, makes production processes involving mixtures of powders a great concern for the industry, given the need to indicate the existence of traces of any of them. The food industry requires non-destructive and non-invasive methods of quantification that meet sensitivity requirements but also specificity levels. Optical methods such as NIR spectrophotometry or hyper-spectral image are currently some of the technologies that show potential success. This is the context of this paper that evaluates how to use NIR spectroscopy (900-1600nm) to detect traces of 15 different kinds of nuts and 20 other flours.